Sample records for observed decadal variability

  1. Robustness of observation-based decadal sea level variability in the Indo-Pacific Ocean

    NASA Astrophysics Data System (ADS)

    Nidheesh, A. G.; Lengaigne, M.; Vialard, J.; Izumo, T.; Unnikrishnan, A. S.; Meyssignac, B.; Hamlington, B.; de Boyer Montegut, C.

    2017-07-01

    We examine the consistency of Indo-Pacific decadal sea level variability in 10 gridded, observation-based sea level products for the 1960-2010 period. Decadal sea level variations are robust in the Pacific, with more than 50% of variance explained by decadal modulation of two flavors of El Niño-Southern Oscillation (classical ENSO and Modoki). Amplitude of decadal sea level variability is weaker in the Indian Ocean than in the Pacific. All data sets indicate a transmission of decadal sea level signals from the western Pacific to the northwest Australian coast through the Indonesian throughflow. The southern tropical Indian Ocean sea level variability is associated with decadal modulations of ENSO in reconstructions but not in reanalyses or in situ data set. The Pacific-independent Indian Ocean decadal sea level variability is not robust but tends to be maximum in the southwestern tropical Indian Ocean. The inconsistency of Indian Ocean decadal variability across the sea level products calls for caution in making definitive conclusions on decadal sea level variability in this basin.

  2. Decadal variability of surface incident solar radiation over China: Observations, satellite retrievals, and reanalyses

    NASA Astrophysics Data System (ADS)

    Wang, Kaicun; Ma, Qian; Li, Zhijun; Wang, Jiankai

    2015-07-01

    Existing studies have shown that observed surface incident solar radiation (Rs) over China may have important inhomogeneity issues. This study provides metadata and reference data to homogenize observed Rs, from which the decadal variability of Rs over China can be accurately derived. From 1958 to 1990, diffuse solar radiation (Rsdif) and direct solar radiation (Rsdir) were measured separately, and Rs was calculated as their sum. The pyranometers used to measure Rsdif had a strong sensitivity drift problem, which introduced a spurious decreasing trend into the observed Rsdif and Rs data, whereas the observed Rsdir did not suffer from this sensitivity drift problem. From 1990 to 1993, instruments and measurement methods were replaced and measuring stations were restructured in China, which introduced an abrupt increase in the observed Rs. Intercomparisons between observation-based and model-based Rs performed in this research show that sunshine duration (SunDu)-derived Rs is of high quality and can be used as reference data to homogenize observed Rs data. The homogenized and adjusted data of observed Rs combines the advantages of observed Rs in quantifying hourly to monthly variability and SunDu-derived Rs in depicting decadal variability and trend. Rs averaged over 105 stations in China decreased at -2.9 W m-2 per decade from 1961 to 1990 and remained stable afterward. This decadal variability is confirmed by the observed Rsdir and diurnal temperature ranges, and can be reproduced by high-quality Earth System Models. However, neither satellite retrievals nor reanalyses can accurately reproduce such decadal variability over China.

  3. Intensification of decadal and multi-decadal sea level variability in the western tropical Pacific during recent decades

    NASA Astrophysics Data System (ADS)

    Han, Weiqing; Meehl, Gerald A.; Hu, Aixue; Alexander, Michael A.; Yamagata, Toshio; Yuan, Dongliang; Ishii, Masayoshi; Pegion, Philip; Zheng, Jian; Hamlington, Benjamin D.; Quan, Xiao-Wei; Leben, Robert R.

    2014-09-01

    Previous studies have linked the rapid sea level rise (SLR) in the western tropical Pacific (WTP) since the early 1990s to the Pacific decadal climate modes, notably the Pacific Decadal Oscillation in the north Pacific or Interdecadal Pacific Oscillation (IPO) considering its basin wide signature. Here, the authors investigate the changing patterns of decadal (10-20 years) and multidecadal (>20 years) sea level variability (global mean SLR removed) in the Pacific associated with the IPO, by analyzing satellite and in situ observations, together with reconstructed and reanalysis products, and performing ocean and atmosphere model experiments. Robust intensification is detected for both decadal and multidecadal sea level variability in the WTP since the early 1990s. The IPO intensity, however, did not increase and thus cannot explain the faster SLR. The observed, accelerated WTP SLR results from the combined effects of Indian Ocean and WTP warming and central-eastern tropical Pacific cooling associated with the IPO cold transition. The warm Indian Ocean acts in concert with the warm WTP and cold central-eastern tropical Pacific to drive intensified easterlies and negative Ekman pumping velocity in western-central tropical Pacific, thereby enhancing the western tropical Pacific SLR. On decadal timescales, the intensified sea level variability since the late 1980s or early 1990s results from the "out of phase" relationship of sea surface temperature anomalies between the Indian and central-eastern tropical Pacific since 1985, which produces "in phase" effects on the WTP sea level variability.

  4. A further assessment of vegetation feedback on decadal Sahel rainfall variability

    NASA Astrophysics Data System (ADS)

    Kucharski, Fred; Zeng, Ning; Kalnay, Eugenia

    2013-03-01

    The effect of vegetation feedback on decadal-scale Sahel rainfall variability is analyzed using an ensemble of climate model simulations in which the atmospheric general circulation model ICTPAGCM ("SPEEDY") is coupled to the dynamic vegetation model VEGAS to represent feedbacks from surface albedo change and evapotranspiration, forced externally by observed sea surface temperature (SST) changes. In the control experiment, where the full vegetation feedback is included, the ensemble is consistent with the observed decadal rainfall variability, with a forced component 60 % of the observed variability. In a sensitivity experiment where climatological vegetation cover and albedo are prescribed from the control experiment, the ensemble of simulations is not consistent with the observations because of strongly reduced amplitude of decadal rainfall variability, and the forced component drops to 35 % of the observed variability. The decadal rainfall variability is driven by SST forcing, but significantly enhanced by land-surface feedbacks. Both, local evaporation and moisture flux convergence changes are important for the total rainfall response. Also the internal decadal variability across the ensemble members (not SST-forced) is much stronger in the control experiment compared with the one where vegetation cover and albedo are prescribed. It is further shown that this positive vegetation feedback is physically related to the albedo feedback, supporting the Charney hypothesis.

  5. Ocean impact on decadal Atlantic climate variability revealed by sea-level observations.

    PubMed

    McCarthy, Gerard D; Haigh, Ivan D; Hirschi, Joël J-M; Grist, Jeremy P; Smeed, David A

    2015-05-28

    Decadal variability is a notable feature of the Atlantic Ocean and the climate of the regions it influences. Prominently, this is manifested in the Atlantic Multidecadal Oscillation (AMO) in sea surface temperatures. Positive (negative) phases of the AMO coincide with warmer (colder) North Atlantic sea surface temperatures. The AMO is linked with decadal climate fluctuations, such as Indian and Sahel rainfall, European summer precipitation, Atlantic hurricanes and variations in global temperatures. It is widely believed that ocean circulation drives the phase changes of the AMO by controlling ocean heat content. However, there are no direct observations of ocean circulation of sufficient length to support this, leading to questions about whether the AMO is controlled from another source. Here we provide observational evidence of the widely hypothesized link between ocean circulation and the AMO. We take a new approach, using sea level along the east coast of the United States to estimate ocean circulation on decadal timescales. We show that ocean circulation responds to the first mode of Atlantic atmospheric forcing, the North Atlantic Oscillation, through circulation changes between the subtropical and subpolar gyres--the intergyre region. These circulation changes affect the decadal evolution of North Atlantic heat content and, consequently, the phases of the AMO. The Atlantic overturning circulation is declining and the AMO is moving to a negative phase. This may offer a brief respite from the persistent rise of global temperatures, but in the coupled system we describe, there are compensating effects. In this case, the negative AMO is associated with a continued acceleration of sea-level rise along the northeast coast of the United States.

  6. Tides and Decadal Variability

    NASA Technical Reports Server (NTRS)

    Ray, Richard D.

    2003-01-01

    This paper reviews the mechanisms by which oceanic tides and decadal variability in the oceans are connected. We distinguish between variability caused by tides and variability observed in the tides themselves. Both effects have been detected at some level. The most obvious connection with decadal timescales is through the 18.6-year precession of the moon's orbit plane. This precession gives rise to a small tide of the same period and to 18.6-year modulations in the phase and amplitudes of short-period tides. The 18.6-year "node tide" is very small, no more than 2 cm anywhere, and in sea level data it is dominated by the ocean's natural Variability. Some authors have naively attributed climate variations with periods near 19 years directly to the node tide, but the amplitude of the tide is too small for this mechanism to be operative. The more likely explanation (Loder and Garrett, JGR, 83, 1967-70, 1978) is that the 18.6-y modulations in short-period tides, especially h e principal tide M2, cause variations in ocean mixing, which is then observed in temperature and other climatic indicators. Tidally forced variability has also been proposed by some authors, either in response to occasional (and highly predictable) tidal extremes or as a nonlinear low-frequency oscillation caused by interactions between short-period tides. The former mechanism can produce only short-duration events hardly more significant than normal tidal ranges, but the latter mechanism can in principle induce low-frequency oscillations. The most recent proposal of this type is by Keeling and Whorf, who highlight the 1800-year spectral peak discovered by Bond et al. (1997). But the proposal appears contrived and should be considered, in the words of Munk et al. (2002), "as the most likely among unlikely candidates."

  7. North Atlantic sub-decadal variability in climate models

    NASA Astrophysics Data System (ADS)

    Reintges, Annika; Martin, Thomas; Latif, Mojib; Park, Wonsun

    2017-04-01

    The North Atlantic Oscillation (NAO) is the dominant variability mode for the winter climate of the North Atlantic sector. During a positive (negative) NAO phase, the sea level pressure (SLP) difference between the subtropical Azores high and the subpolar Icelandic low is anomalously strong (weak). This affects, for example, temperature, precipitation, wind, and surface heat flux over the North Atlantic, and over large parts of Europe. In observations we find enhanced sub-decadal variability of the NAO index that goes along with a dipolar sea surface temperature (SST) pattern. The corresponding SLP and SST patterns are reproduced in a control experiment of the Kiel Climate Model (KCM). Large-scale air-sea interaction is suggested to be essential for the North Atlantic sub-decadal variability in the KCM. The Atlantic Meridional Overturning Circulation (AMOC) plays a key role, setting the timescale of the variability by providing a delayed negative feedback to the NAO. The interplay of the NAO and the AMOC on the sub-decadal timescale is further investigated in the CMIP5 model ensemble. For example, the average CMIP5 model AMOC pattern associated with sub-decadal variability is characterized by a deep-reaching dipolar structure, similar to the KCM's sub-decadal AMOC variability pattern. The results suggest that dynamical air-sea interactions are crucial to generate enhanced sub-decadal variability in the North Atlantic climate.

  8. Solar forcing synchronizes decadal North Atlantic climate variability.

    PubMed

    Thiéblemont, Rémi; Matthes, Katja; Omrani, Nour-Eddine; Kodera, Kunihiko; Hansen, Felicitas

    2015-09-15

    Quasi-decadal variability in solar irradiance has been suggested to exert a substantial effect on Earth's regional climate. In the North Atlantic sector, the 11-year solar signal has been proposed to project onto a pattern resembling the North Atlantic Oscillation (NAO), with a lag of a few years due to ocean-atmosphere interactions. The solar/NAO relationship is, however, highly misrepresented in climate model simulations with realistic observed forcings. In addition, its detection is particularly complicated since NAO quasi-decadal fluctuations can be intrinsically generated by the coupled ocean-atmosphere system. Here we compare two multi-decadal ocean-atmosphere chemistry-climate simulations with and without solar forcing variability. While the experiment including solar variability simulates a 1-2-year lagged solar/NAO relationship, comparison of both experiments suggests that the 11-year solar cycle synchronizes quasi-decadal NAO variability intrinsic to the model. The synchronization is consistent with the downward propagation of the solar signal from the stratosphere to the surface.

  9. Decadal Variability of Surface Incident Solar Radiation over China

    NASA Astrophysics Data System (ADS)

    Wang, Kaicun

    2015-04-01

    Observations have reported a widespread dimming of surface incident solar radiation (Rs) from the 1950s to the 1980s and a brightening afterwards. However, none of the state-of-the-art earth system models, including those from the Coupled Model Intercomparison Project phase 5 (CMIP5), could successfully reproduce the dimming/brightening rates over China. This study provides metadata and reference data to investigate the observed variability of Rs in China. From 1958 to 1990, diffuse solar radiation (Rsdif) and direct solar radiation (Rsdir) was measured separately in China, from which Rs was calculated a sum. However, pyranometers used to measure Rsdif had a strong sensitivity drift problem, which introduced a spurious decreasing trend to Rsdif and Rs measurements. The observed Rsdir did not suffer from such sensitivity drift problem. From 1990 to 1993, the old instruments were replaced and measuring stations were relocated in China, which introduced an abrupt increase in the observed Rs. After 1993, Rs was measured by solid black thermopile pyranometers. Comprehensive comparisons between observation-based and model-based Rs performed in this research have shown that sunshine duration (SunDu)-derived Rs is of high quality and provide accurate estimate of decadal variability of Rs over China. SunDu-derived Rs averaged over 105 stations in China decreased at -2.9 W m-2 per decade from 1961 to 1990 and remained stable afterward. This decadal variability has been confirmed by the observed Rsdir, independent studies on aerosols and diurnal temperature range, and can be reproduced by certain high-quality earth system models. However, neither satellite retrievals (the Global Energy and Water Exchanges Project Surface Radiation Budget (GEWEX SRB)) nor reanalyses (ERA-Interim and Modern-Era Retrospective analysis for Research and Applications (MERRA)) can accurately reproduce such decadal variability of Rs over China for their exclusion of annual variability of tropospheric

  10. Improved spectral comparisons of paleoclimate models and observations via proxy system modeling: Implications for multi-decadal variability

    NASA Astrophysics Data System (ADS)

    Dee, S. G.; Parsons, L. A.; Loope, G. R.; Overpeck, J. T.; Ault, T. R.; Emile-Geay, J.

    2017-10-01

    The spectral characteristics of paleoclimate observations spanning the last millennium suggest the presence of significant low-frequency (multi-decadal to centennial scale) variability in the climate system. Since this low-frequency climate variability is critical for climate predictions on societally-relevant scales, it is essential to establish whether General Circulation models (GCMs) are able to simulate it faithfully. Recent studies find large discrepancies between models and paleoclimate data at low frequencies, prompting concerns surrounding the ability of GCMs to predict long-term, high-magnitude variability under greenhouse forcing (Laepple and Huybers, 2014a, 2014b). However, efforts to ground climate model simulations directly in paleoclimate observations are impeded by fundamental differences between models and the proxy data: proxy systems often record a multivariate and/or nonlinear response to climate, precluding a direct comparison to GCM output. In this paper we bridge this gap via a forward proxy modeling approach, coupled to an isotope-enabled GCM. This allows us to disentangle the various contributions to signals embedded in ice cores, speleothem calcite, coral aragonite, tree-ring width, and tree-ring cellulose. The paper addresses the following questions: (1) do forward-modeled ;pseudoproxies; exhibit variability comparable to proxy data? (2) if not, which processes alter the shape of the spectrum of simulated climate variability, and are these processes broadly distinguishable from climate? We apply our method to representative case studies, and broaden these insights with an analysis of the PAGES2k database (PAGES2K Consortium, 2013). We find that current proxy system models (PSMs) can help resolve model-data discrepancies on interannual to decadal timescales, but cannot account for the mismatch in variance on multi-decadal to centennial timescales. We conclude that, specific to this set of PSMs and isotope-enabled model, the paleoclimate

  11. Simulated decadal modes of the NH atmospheric circulation arising from intra-decadal variability, external forcing and slow-decadal climate processes

    NASA Astrophysics Data System (ADS)

    Lou, Jiale; Zheng, Xiaogu; Frederiksen, Carsten S.; Liu, Haibo; Grainger, Simon; Ying, Kairan

    2017-04-01

    A decadal variance decomposition method is applied to the Northern Hemisphere (NH) 500-hPa geopotential height (GPH) and the sea level pressure (SLP) taken from the last millennium (850-1850 AD) experiment with the coupled climate model CCSM4, to estimate the contribution of the intra-decadal variability to the inter-decadal variability. By removing the intra-decadal variability from the total inter-decadal variability, the residual variability is more likely to be associated with slowly varying external forcings and slow-decadal climate processes, and therefore is referred to as slow-decadal variability. The results show that the (multi-)decadal changes of the NH 500-hPa GPH are primarily dominated by slow-decadal variability, whereas the NH SLP field is primarily dominated by the intra-decadal variability. At both pressure levels, the leading intra-decadal modes each have features related to the El Niño-southern oscillation, the intra-decadal variability of the Pacific decadal oscillation (PDO) and the Arctic oscillation (AO); while the leading slow-decadal modes are associated with external radiative forcing (mostly with volcanic aerosol loadings), the Atlantic multi-decadal oscillation and the slow-decadal variability of AO and PDO. Moreover, the radiative forcing has much weaker effect to the SLP than that to the 500-hPa GPH.

  12. The Oceanic Contribution to Atlantic Multi-Decadal Variability

    NASA Astrophysics Data System (ADS)

    Wills, R. C.; Armour, K.; Battisti, D. S.; Hartmann, D. L.

    2017-12-01

    Atlantic multi-decadal variability (AMV) is typically associated with variability in ocean heat transport (OHT) by the Atlantic Meridional Overturning Circulation (AMOC). However, recent work has cast doubt on this connection by showing that slab-ocean climate models, in which OHT cannot vary, exhibit similar variability. Here, we apply low-frequency component analysis to isolate the variability of Atlantic sea-surface temperatures (SSTs) that occurs on decadal and longer time scales. In observations and in pre-industrial control simulations of comprehensive climate models, we find that AMV is confined to the extratropics, with the strongest temperature anomalies in the North Atlantic subpolar gyre. We show that warm subpolar temperatures are associated with a strengthened AMOC, increased poleward OHT, and local heat fluxes from the ocean into the atmosphere. In contrast, the traditional index of AMV based on the basin-averaged SST anomaly shows warm temperatures preceded by heat fluxes from the atmosphere into the ocean, consistent with the atmosphere driving this variability, and shows a weak relationship with AMOC. The autocorrelation time of the basin-averaged SST index is 1 year compared to an autocorrelation time of 5 years for the variability of subpolar temperatures. This shows that multi-decadal variability of Atlantic SSTs is sustained by OHT variability associated with AMOC, while atmosphere-driven SST variability, such as exists in slab-ocean models, contributes primarily on interannual time scales.

  13. Multi-decadal and seasonal variability of dust observations in West Greenland.

    NASA Astrophysics Data System (ADS)

    Bullard, Joanna E.; Mockford, Tom

    2017-04-01

    Since the early 1900s expedition records from west Greenland have reported local dust storms. The Kangerlussuaq region, near the inland ice, is dry (mean annual precipitation <160 mm) with, on average, 150 snow-free days per year. The main local dust sources are active, proglacial outwash plains although reworking of loess deposits may also be important. This paper presents an analysis of 70-years of dust storm observations (1945-2015) based on WMO weather codes 6 (dust haze), 7 (raised dust or sand) and 9 (distant or past dust storm) and associated wind data. The 70-year average number of dust observations days is 5 per year but variable ranging from 0 observations to 23 observations in 1985. Over the past 7 decades the number of dust days has increased from <30 in 1945-54 to >75 in 1995-2004 and 2005-2015. The seasonality of dust observations has remained consistent throughout most of the period. Dust days occur all year round but are most frequent in May-June and September-October and are associated with minimum snow cover and glacial meltwater-driven sediment supply to the outwash plains during spring and fall flood events. Wind regime is bimodal dominated by katabatic winds from the northeast, which are strongest and most frequent during winter months (Nov-Jan), with less frequent, southwesterly winds generated by Atlantic storms mostly confined to spring (May, June). The southwesterly winds are those most likely to transport dust onto the Greenland ice sheet.

  14. Re-Examination of the Observed Decadal Variability of Earth Radiation Budget Using Altitude-Corrected ERBE/ERBS Nonscanner WFOV Data

    NASA Technical Reports Server (NTRS)

    Wong, Takmeng; Wielicki, Bruce A.; Lee, Robert B.; Smith, G. Louis; Bush, Kathryn A.

    2005-01-01

    This paper gives an update on the observed decadal variability of Earth Radiation Budget using the latest altitude-corrected Earth Radiation Budget Experiment (ERBE)/Earth Radiation Budget Satellite (ERBS) Nonscanner Wide Field of View (WFOV) instrument Edition3 dataset. The effects of the altitude correction are to modify the original reported decadal changes in tropical mean (20N to 20S) longwave (LW), shortwave (SW), and net radiation between the 1980s and the 1990s from 3.1/-2.4/-0.7 to 1.6/-3.0/1.4 Wm(sup -2) respectively. In addition, a small SW instrument drift over the 15-year period was discovered during the validation of the WFOV Edition3 dataset. A correction was developed and applied to the Edition3 dataset at the data user level to produce the WFOV Edition3_Rev1 dataset. With this final correction, the ERBS Nonscanner observed decadal changes in tropical mean LW, SW, and net radiation between the 1980s and the 1990s now stand at 0.7/-2.1/1.4 Wm(sup -2), respectively, which are similar to the observed decadal changes in the HIRS Pathfinder OLR and the ISCCP FD record; but disagree with the AVHRR Pathfinder ERB record. Furthermore, the observed interannual variability of near-global ERBS WFOV Edition3_Rev1 net radiation is found to be remarkably consistent with the latest ocean heat storage record for the overlapping time period of 1993 to 1999. Both data sets show variations of roughly 1.5 Wm(sup -2) in planetary net heat balance during the 1990s.

  15. Agulhas leakage dynamics affects decadal variability in Atlantic overturning circulation.

    PubMed

    Biastoch, A; Böning, C W; Lutjeharms, J R E

    2008-11-27

    Predicting the evolution of climate over decadal timescales requires a quantitative understanding of the dynamics that govern the meridional overturning circulation (MOC). Comprehensive ocean measurement programmes aiming to monitor MOC variations have been established in the subtropical North Atlantic (RAPID, at latitude 26.5 degrees N, and MOVE, at latitude 16 degrees N) and show strong variability on intraseasonal to interannual timescales. Observational evidence of longer-term changes in MOC transport remains scarce, owing to infrequent sampling of transoceanic sections over past decades. Inferences based on long-term sea surface temperature records, however, supported by model simulations, suggest a variability with an amplitude of +/-1.5-3 Sv (1 Sv = 10(6) m(3) s(-1)) on decadal timescales in the subtropics. Such variability has been attributed to variations of deep water formation in the sub-arctic Atlantic, particularly the renewal rate of Labrador Sea Water. Here we present results from a model simulation that suggest an additional influence on decadal MOC variability having a Southern Hemisphere origin: dynamic signals originating in the Agulhas leakage region at the southern tip of Africa. These contribute a MOC signal in the tropical and subtropical North Atlantic that is of the same order of magnitude as the northern source. A complete rationalization of observed MOC changes therefore also requires consideration of signals arriving from the south.

  16. Processes Understanding of Decadal Climate Variability

    NASA Astrophysics Data System (ADS)

    Prömmel, Kerstin; Cubasch, Ulrich

    2016-04-01

    The realistic representation of decadal climate variability in the models is essential for the quality of decadal climate predictions. Therefore, the understanding of those processes leading to decadal climate variability needs to be improved. Several of these processes are already included in climate models but their importance has not yet completely been clarified. The simulation of other processes requires sometimes a higher resolution of the model or an extension by additional subsystems. This is addressed within one module of the German research program "MiKlip II - Decadal Climate Predictions" (http://www.fona-miklip.de/en/) with a focus on the following processes. Stratospheric processes and their impact on the troposphere are analysed regarding the climate response to aerosol perturbations caused by volcanic eruptions and the stratospheric decadal variability due to solar forcing, climate change and ozone recovery. To account for the interaction between changing ozone concentrations and climate a computationally efficient ozone chemistry module is developed and implemented in the MiKlip prediction system. The ocean variability and air-sea interaction are analysed with a special focus on the reduction of the North Atlantic cold bias. In addition, the predictability of the oceanic carbon uptake with a special emphasis on the underlying mechanism is investigated. This addresses a combination of physical, biological and chemical processes.

  17. Meridional Modes and Increasing Pacific Decadal Variability Under Anthropogenic Forcing

    NASA Astrophysics Data System (ADS)

    Liguori, Giovanni; Di Lorenzo, Emanuele

    2018-01-01

    Pacific decadal variability has strong impacts on the statistics of weather, atmosphere extremes, droughts, hurricanes, marine heatwaves, and marine ecosystems. Sea surface temperature (SST) observations show that the variance of the El Niño-like decadal variability has increased by 30% (1920-2015) with a stronger coupling between the major Pacific climate modes. Although we cannot attribute these trends to global climate change, the examination of 30 members of the Community Earth System Model Large Ensemble (LENS) forced with the RCP8.5 radiative forcing scenario (1920-2100) suggests that significant anthropogenic trends in Pacific decadal variance will emerge by 2020 in response to a more energetic North Pacific Meridional Mode (PMM)—a well-known El Niño precursor. The PMM is a key mechanism for energizing and coupling tropical and extratropical decadal variability. In the LENS, the increase in PMM variance is consistent with an intensification of the winds-evaporation-SST thermodynamic feedback that results from a warmer mean climate.

  18. Enceladus Plumes: Causes of Decadal Variability

    NASA Astrophysics Data System (ADS)

    Ingersoll, Andrew P.; Ewald, Shawn P.

    2016-10-01

    The Enceladus plumes have decreased over the decade that Cassini has been observing them. This long-term variation is superposed on the much shorter-term variation tied to the position of Enceladus in its orbit around Saturn. The observations are ISS and VIMS images, which reveal the particles in the plumes but not the gas. The decadal variability largely consists of a 2-fold decline in the mass of plume material, but there is a hint of a recent turnaround. Here we offer three hypotheses, each with its strengths and weaknesses, to explain the long-term variability. The first is seasonal change, from summer to fall in the southern hemisphere. The loss of sunlight could increase the build-up of ice around the tiger stripes. The weakness is that the sunlight is likely to have a small effect, e.g., decreasing the sublimation rate of the ice by only ~1 cm/year. The second hypothesis is a statistical fluctuation in the number of active plumes, which tend to turn themselves off due to build-up of ice at the throat of the vent. The weakness is that the plumes are likely to fluctuate independently, and if there are ~100 plumes, their sum will only fluctuate by 10%. The third hypothesis is that the variation is part of a well-known decadal cycle of orbital eccentricity, which varies by ±2.5% around a mean of 0.0047. The peak eccentricity occurred in 2009-2010, and the minimum occurred in 2015. Since eccentricity controls the short-term orbital cycle variations, it could also control the longer-term decadal variations. The weakness is that the eccentricity variation is small, from 0.0046 to 0.0048. It is not certain that such a small variation could cause a 2-fold variation in the strength of the plumes. An independent study, still in its infancy, is the possibility that liquid water reaches the surface during part of the orbital cycle.

  19. Anatomy of North Pacific Decadal Variability.

    NASA Astrophysics Data System (ADS)

    Schneider, Niklas; Miller, Arthur J.; Pierce, David W.

    2002-03-01

    rain in the KOE region.The preponderance of variance at decadal timescales in the KOE results from the integration of stochastic Ekman pumping along Rossby wave trajectories. The Ekman pumping is primarily due to atmospheric variability that expresses itself worldwide including in the tropical Pacific. A positive feedback between the coupled model KOE SST (driven by the ocean streamfunction) and North Pacific Ekman pumping is consistent with the enhanced variance of the coupled model at 20-30-yr periods. However, the time series are too short to unambiguously distinguish this positive feedback hypothesis from sampling variability. No evidence is found for a midlatitude gyre ocean-atmosphere delayed negative feedback loop.Comparisons with available observations confirm the seasonality of the forcing, the up to 5-yr time lag between like-signed central North Pacific and KOE SST anomalies, and the associated damping of SST in the KOE region by the latent heat flux. The coupled model results also suggest that observed SST anomalies in the KOE region may be predictable from the history of the wind-stress curl over the North Pacific.

  20. Role of internal variability in recent decadal to multidecadal tropical Pacific climate changes

    NASA Astrophysics Data System (ADS)

    Bordbar, Mohammad Hadi; Martin, Thomas; Latif, Mojib; Park, Wonsun

    2017-05-01

    While the Earth's surface has considerably warmed over the past two decades, the tropical Pacific has featured a cooling of sea surface temperatures in its eastern and central parts, which went along with an unprecedented strengthening of the equatorial trade winds, the surface component of the Pacific Walker Circulation (PWC). Previous studies show that this decadal trend in the trade winds is generally beyond the range of decadal trends simulated by climate models when forced by historical radiative forcing. There is still a debate on the origin of and the potential role that internal variability may have played in the recent decadal surface wind trend. Using a number of long control (unforced) integrations of global climate models and several observational data sets, we address the question as to whether the recent decadal to multidecadal trends are robustly classified as an unusual event or the persistent response to external forcing. The observed trends in the tropical Pacific surface climate are still within the range of the long-term internal variability spanned by the models but represent an extreme realization of this variability. Thus, the recent observed decadal trends in the tropical Pacific, though highly unusual, could be of natural origin. We note that the long-term trends in the selected PWC indices exhibit a large observational uncertainty, even hindering definitive statements about the sign of the trends.Plain Language SummaryWhile the Earth's surface has considerably warmed over the past two <span class="hlt">decades</span>, the tropical Pacific has featured a cooling of sea surface temperatures in its eastern and central parts, which went along with an unprecedented strengthening of the equatorial trade winds. Here we show that climate models simulate a high level of internal <span class="hlt">variability</span>, so that the recent changes in the tropical Pacific could still be due to natural processes.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li class="active"><span>1</span></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_1 --> <div id="page_2" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="21"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC33H..08M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC33H..08M"><span>Societal Impacts of Natural <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span> - The Pacemakers of Civilizations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mehta, V. M.</p> <p>2017-12-01</p> <p>Natural <span class="hlt">decadal</span> climate <span class="hlt">variability</span> (DCV) is one of the oldest areas of climate research. Building on centuries-long literature, a substantial body of research has emerged in the last two to three <span class="hlt">decades</span>, focused on understanding causes, mechanisms, and impacts of DCV. Several DCV phenomena - the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) or the Interdecadal Pacific Oscillation (IPO), tropical Atlantic sea-surface temperature gradient <span class="hlt">variability</span> (TAG for brevity), West Pacific Warm Pool <span class="hlt">variability</span>, and <span class="hlt">decadal</span> <span class="hlt">variability</span> of El Niño-La Niña events - have been identified in <span class="hlt">observational</span> records; and are associated with <span class="hlt">variability</span> of worldwide atmospheric circulations, water vapor transport, precipitation, and temperatures; and oceanic circulations, salinity, and temperatures. Tree-ring based drought index data going back more than 700 years show presence of <span class="hlt">decadal</span> hydrologic cycles (DHCs) in North America, Europe, and South Asia. Some of these cycles were associated with the rise and fall of civilizations, large-scale famines which killed millions of people, and acted as catalysts for socio-political revolutions. Instrument-measured data confirm presence of such worldwide DHCs associated with DCV phenomena; and show these DCV phenomena's worldwide impacts on river flows, crop productions, inland water-borne transportation, hydro-electricity generation, and agricultural irrigation. Fish catch data also show multiyear to <span class="hlt">decadal</span> catch <span class="hlt">variability</span> associated with these DCV phenomena in all oceans. This talk, drawn from my recently-published book (Mehta, V.M., 2017: Natural <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span>: Societal Impacts. CRC Press, Boca Raton, Florida, 326 pp.), will give an overview of worldwide impacts of DCV phenomena, with specific examples of socio-economic-political impacts. This talk will also describe national and international security implications of such societal impacts, and worldwide food security implications. The talk will end with an outline of needed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS23D..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS23D..01H"><span>Multi-<span class="hlt">decadal</span> trend and space-time <span class="hlt">variability</span> of sea level over the Indian Ocean since the 1950s: impact of <span class="hlt">decadal</span> climate modes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, W.; Stammer, D.; Meehl, G. A.; Hu, A.; Sienz, F.</p> <p>2016-12-01</p> <p>Sea level varies on <span class="hlt">decadal</span> and multi-<span class="hlt">decadal</span> timescales over the Indian Ocean. The variations are not spatially uniform, and can deviate considerably from the global mean sea level rise (SLR) due to various geophysical processes. One of these processes is the change of ocean circulation, which can be partly attributed to natural internal modes of climate <span class="hlt">variability</span>. Over the Indian Ocean, the most influential climate modes on <span class="hlt">decadal</span> and multi-<span class="hlt">decadal</span> timescales are the Interdecadal Pacific Oscillation (IPO) and <span class="hlt">decadal</span> <span class="hlt">variability</span> of the Indian Ocean dipole (IOD). Here, we first analyze <span class="hlt">observational</span> datasets to investigate the impacts of IPO and IOD on spatial patterns of <span class="hlt">decadal</span> and interdecadal (hereafter decal) sea level <span class="hlt">variability</span> & multi-<span class="hlt">decadal</span> trend over the Indian Ocean since the 1950s, using a new statistical approach of Bayesian Dynamical Linear regression Model (DLM). The Bayesian DLM overcomes the limitation of "time-constant (static)" regression coefficients in conventional multiple linear regression model, by allowing the coefficients to vary with time and therefore measuring "time-evolving (dynamical)" relationship between climate modes and sea level. For the multi-<span class="hlt">decadal</span> sea level trend since the 1950s, our results show that climate modes and non-climate modes (the part that cannot be explained by climate modes) have comparable contributions in magnitudes but with different spatial patterns, with each dominating different regions of the Indian Ocean. For <span class="hlt">decadal</span> <span class="hlt">variability</span>, climate modes are the major contributors for sea level variations over most region of the tropical Indian Ocean. The relative importance of IPO and <span class="hlt">decadal</span> <span class="hlt">variability</span> of IOD, however, varies spatially. For example, while IOD <span class="hlt">decadal</span> <span class="hlt">variability</span> dominates IPO in the eastern equatorial basin (85E-100E, 5S-5N), IPO dominates IOD in causing sea level variations in the tropical southwest Indian Ocean (45E-65E, 12S-2S). To help decipher the possible contribution of external</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS31B2016S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS31B2016S"><span>Identifying <span class="hlt">Decadal</span> to Multi-<span class="hlt">decadal</span> <span class="hlt">Variability</span> in the Pacific by Empirical Mode Decomposition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sommers, L. A.; Hamlington, B.; Cheon, S. H.</p> <p>2016-12-01</p> <p>Large scale climate <span class="hlt">variability</span> in the Pacific Ocean like that associated with ENSO and the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) has been shown to have a significant impact on climate and sea level across a range of timescales. The changes related to these climate signals have worldwide impacts on fisheries, weather, and precipitation patterns among others. Understanding these inter-annual to multi-<span class="hlt">decadal</span> oscillations is imperative to longer term climate forecasts and understanding how climate will behave, and its effect on changes in sea level. With a 110-year reconstruction of sea level, we examine <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> seen in the sea level fluctuations in the Pacific Ocean. Using empirical mode decomposition (EMD), we break down regional sea level into a series of intrinsic mode functions (IMFs) and attempt attribution of these IMFs to specific climate modes of <span class="hlt">variability</span>. In particular, and not unexpectedly, we identify IMFs associated with the PDO, finding correlations between the PDO Index and IMFs in the Pacific Ocean upwards of 0.6-0.8 over the 110-year reconstructed record. Perhaps more significantly, we also find evidence of a longer multi-<span class="hlt">decadal</span> signal ( 50-60 years) in the higher order IMFs. This lower frequency <span class="hlt">variability</span> has been suggested in previous literature as influencing GMSL, but here we find a regional pattern associated with this multi-<span class="hlt">decadal</span> signal. By identifying and separating these periodic climate signals, we can gain a better understanding of how the sea level <span class="hlt">variability</span> associated with these modes can impact sea level on short timescales and serve to exacerbate the effects of long-term sea level change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PrOce.161..131J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PrOce.161..131J"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> on the Northwest European continental shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, Sam; Cottier, Finlo; Inall, Mark; Griffiths, Colin</p> <p>2018-02-01</p> <p><span class="hlt">Decadal</span> scale time series of the shelf seas are important for understanding both climate and process studies. Despite numerous investigations of long-term temperature <span class="hlt">variability</span> in the shelf seas, studies of salinity <span class="hlt">variability</span> are few. Salt is a more conservative tracer than temperature in shallow seas, and it can reveal changes in local hydrographic conditions as well as transmitted basin-scale changes. Here, new inter-annual salinity time series on the northwest European shelf are developed and a 13 year high resolution salinity record from a coastal mooring in western Scotland is presented and analysed. We find strong temporal <span class="hlt">variability</span> in coastal salinity on timescales ranging from tidal to inter-annual, with the magnitude of <span class="hlt">variability</span> greatest during winter months. There is little seasonality and no significant <span class="hlt">decadal</span> trend in the coastal time series of salinity. We propose 4 hydrographic states to explain salinity variance in the shelf area west of Scotland based on the interaction between a baroclinic coastal current and wind-forced barotropic flow: while wind forcing is important, we find that changes in the buoyancy-driven flow are more likely to influence long-term salinity <span class="hlt">observations</span>. We calculate that during prevailing westerly wind conditions, surface waters in the Sea of the Hebrides receive a mix of 62% Atlantic origin water to 38% coastal sources. This contrasts with easterly wind conditions, during which the mix is 6% Atlantic to 94% coastal sources on average. This 'switching' between hydrographic states is expected to impact nutrient transport and therefore modify the level of primary productivity on the shelf. This strong local <span class="hlt">variability</span> in salinity is roughly an order of magnitude greater than changes in the adjacent ocean basin, and we infer from this that Scottish coastal waters are likely to be resilient to <span class="hlt">decadal</span> changes in ocean climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC41A1006Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC41A1006Z"><span>Tropical rainforests dominate multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of the global carbon cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, X.; Wang, Y. P.; Peng, S.; Rayner, P. J.; Silver, J.; Ciais, P.; Piao, S.; Zhu, Z.; Lu, X.; Zheng, X.</p> <p>2017-12-01</p> <p>Recent studies find that inter-annual <span class="hlt">variability</span> of global atmosphere-to-land CO2 uptake (NBP) is dominated by semi-arid ecosystems. However, the NBP variations at <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> timescales are still not known. By developing a basic theory for the role of net primary production (NPP) and heterotrophic respiration (Rh) on NBP and applying it to 100-year simulations of terrestrial ecosystem models forced by <span class="hlt">observational</span> climate, we find that tropical rainforests dominate the multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of global NBP (48%) rather than the semi-arid lands (35%). The NBP variation at inter-annual timescales is almost 90% contributed by NPP, but across longer timescales is progressively controlled by Rh that constitutes the response from the NPP-derived soil carbon input (40%) and the response of soil carbon turnover rates to climate <span class="hlt">variability</span> (60%). The NBP variations of tropical rainforests is modulated by the ENSO and the PDO through their significant influences on temperature and precipitation at timescales of 2.5-7 and 25-50 years, respectively. This study highlights the importance of tropical rainforests on the multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of global carbon cycle, suggesting that we need to carefully differentiate the effect of NBP long-term fluctuations associated with ocean-related climate modes on the long-term trend in land sink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A23K..08W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A23K..08W"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of surface solar radiation over China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, K.</p> <p>2015-12-01</p> <p><span class="hlt">Observations</span> show that national average surface solar radiation (Rs) decreased by -8.0 W m-2 per <span class="hlt">decade</span> from 1960 to 1990 and sharply increased from 1990 to 1993. However, none of the state-of-the-art climate models can reproduce such decrease/increase of Rs. This study shows that Rs <span class="hlt">observations</span> over China have significant inhomogeneity. Before 1989, Rs was calculated as a sum of direct (Rsdir) and diffuse (Rsdif) solar radiation <span class="hlt">observations</span> measured by pyrheliometers and shaded pyranometers separately. Due to technical limitations and irregular calibration, pyranometers before 1990 had a strong sensitivity drift problem, which introduced crucial spurious decreasing trends into Rsdif and Rs data. From 1990 to 1993, instruments and measurement methods were replaced and measuring stations were restructured in China, which resulted in an abrupt increase in the <span class="hlt">observed</span> Rs. Rs calculated from Sunshine duration (SunDu) provide a reliable reference in assessing <span class="hlt">decadal</span> <span class="hlt">variability</span> of Rs. SunDu derived Rs have no sensitivity drift problem because of its daily changed recording material. SunDu-derived Rs averaged over China decreased by -2.9 W m-2 per <span class="hlt">decade</span> from 1961 to 1990, and had a negligible trend afterward. During the period of 1994-2012 when Rs <span class="hlt">observations</span> were free of inhomogeneity mentioned above, the <span class="hlt">observed</span> and SunDu-derived Rs consistently show a negligible trend, being less than 0.1 W m-2 per <span class="hlt">decade</span>. These trends can be reproduced by high-quality CMIP5 Earth System Models (ESM). This level of agreement is due to the incorporation of a near real emission inventory of atmospheric aerosols by CMIP5 ESMs. Rs from ERA-Interim has a good agreement with SunDu-derived Rs. However, ERA-interim does not allow aerosol loading to change annually. ERA-Interim Rs shows an unreliable increasing trend of 1.9 W m-2 per <span class="hlt">decade</span> from 1990 to 2013 because it does not include the impact of recent increased atmospheric aerosols over China. GEWEX Rs calculated from ISCCP cloud</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45..916L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45..916L"><span>Current and Future <span class="hlt">Decadal</span> Trends in the Oceanic Carbon Uptake Are Dominated by Internal <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Hongmei; Ilyina, Tatiana</p> <p>2018-01-01</p> <p>We investigate the internal <span class="hlt">decadal</span> <span class="hlt">variability</span> of the ocean carbon uptake using 100 ensemble simulations based on the Max Planck Institute Earth system model (MPI-ESM). We find that on <span class="hlt">decadal</span> time scales, internal <span class="hlt">variability</span> (ensemble spread) is as large as the forced temporal <span class="hlt">variability</span> (ensemble mean), and the largest internal <span class="hlt">variability</span> is found in major carbon sink regions, that is, the 50-65°S band of the Southern Ocean, the North Pacific, and the North Atlantic. The MPI-ESM ensemble produces both positive and negative 10 year trends in the ocean carbon uptake in agreement with <span class="hlt">observational</span> estimates. Negative <span class="hlt">decadal</span> trends are projected to occur in the future under RCP4.5 scenario. Due to the large internal <span class="hlt">variability</span>, the Southern Ocean and the North Pacific require the most ensemble members (more than 53 and 46, respectively) to reproduce the forced <span class="hlt">decadal</span> trends. This number increases up to 79 in future <span class="hlt">decades</span> as CO2 emission trajectory changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28428539','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28428539"><span>Separating <span class="hlt">decadal</span> global water cycle <span class="hlt">variability</span> from sea level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hamlington, B D; Reager, J T; Lo, M-H; Karnauskas, K B; Leben, R R</p> <p>2017-04-20</p> <p>Under a warming climate, amplification of the water cycle and changes in precipitation patterns over land are expected to occur, subsequently impacting the terrestrial water balance. On global scales, such changes in terrestrial water storage (TWS) will be reflected in the water contained in the ocean and can manifest as global sea level variations. Naturally occurring climate-driven TWS <span class="hlt">variability</span> can temporarily obscure the long-term trend in sea level rise, in addition to modulating the impacts of sea level rise through natural periodic undulation in regional and global sea level. The internal <span class="hlt">variability</span> of the global water cycle, therefore, confounds both the detection and attribution of sea level rise. Here, we use a suite of <span class="hlt">observations</span> to quantify and map the contribution of TWS <span class="hlt">variability</span> to sea level <span class="hlt">variability</span> on <span class="hlt">decadal</span> timescales. In particular, we find that <span class="hlt">decadal</span> sea level <span class="hlt">variability</span> centered in the Pacific Ocean is closely tied to low frequency <span class="hlt">variability</span> of TWS in key areas across the globe. The unambiguous identification and clean separation of this component of <span class="hlt">variability</span> is the missing step in uncovering the anthropogenic trend in sea level and understanding the potential for low-frequency modulation of future TWS impacts including flooding and drought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160003531','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160003531"><span>Interannual to <span class="hlt">Decadal</span> <span class="hlt">Variability</span> of Ocean Evaporation as Viewed from Climate Reanalyses</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robertson, Franklin R.; Bosilovich, Michael G.; Roberts, Jason B.; Wang, Hailan</p> <p>2015-01-01</p> <p>Questions we'll address: Given the uncoupled framework of "AMIP" (Atmosphere Model Inter-comparison Project) experiments, what can they tell us regarding evaporation <span class="hlt">variability</span>? Do Reduced <span class="hlt">Observations</span> Reanalyses (RedObs) using Surface Fluxes and Clouds (SFC) pressure (and wind) provide a more realistic picture of evaporation <span class="hlt">variability</span>? What signals of interannual <span class="hlt">variability</span> (e.g. El Nino/Southern Oscillation (ENSO)) and <span class="hlt">decadal</span> <span class="hlt">variability</span> (Interdecadal Pacific Oscillation (IPO)) are detectable with this hierarchy of evaporation estimates?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70185082','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70185082"><span>North Pacific <span class="hlt">decadal</span> climate <span class="hlt">variability</span> since 1661</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Biondi, Franco; Gershunov, Alexander; Cayan, Daniel R.</p> <p>2001-01-01</p> <p>Climate in the North Pacific and North American sectors has experienced interdecadal shifts during the twentieth century. A network of recently developed tree-ring chronologies for Southern and Baja California extends the instrumental record and reveals <span class="hlt">decadal</span>-scale <span class="hlt">variability</span> back to 1661. The Pacific <span class="hlt">decadal</span> oscillation (PDO) is closely matched by the dominant mode of tree-ring <span class="hlt">variability</span> that provides a preliminary view of multiannual climate fluctuations spanning the past four centuries. The reconstructed PDO index features a prominent bidecadal oscillation, whose amplitude weakened in the late l700s to mid-1800s. A comparison with proxy records of ENSO suggests that the greatest <span class="hlt">decadal</span>-scale oscillations in Pacific climate between 1706 and 1977 occurred around 1750, 1905, and 1947.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGC42B..01C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGC42B..01C"><span>The role of clouds in driving North Atlantic multi-<span class="hlt">decadal</span> climate <span class="hlt">variability</span> in <span class="hlt">observations</span> and models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clement, A. C.; Bellomo, K.; Murphy, L.</p> <p>2013-12-01</p> <p>Large scale warming and cooling periods of the North Atlantic is known as the Atlantic Multidecadal Oscillation (AMO). The pattern of warming and cooling in the North Atlantic Ocean over the 20th century that has a characteristic spatial structure with maximum warming in the mid-latitudes and subtropics. This has been most often attributed to changes in the strength of the Atlantic Meridional Overturning Circulation (AMOC), which in turn affects poleward heat transport. A recent modeling study by Booth et al. (2012), however, suggested that aerosols can explain both the spatial pattern and temporal history of Atlantic SST through indirect effects of aerosols on cloud cover; although this idea is controversial (Zhang et al., 2013). We have found <span class="hlt">observational</span> evidence that changes in cloud amount can drive SST changes on multi-<span class="hlt">decadal</span> timescale. We hypothesize that a positive local feedback between SST and cloud radiative effect amplifies SST and gives rise to the <span class="hlt">observed</span> pattern of SST change. During cool North Atlantic periods, a southward shift of the ITCZ strengthens the trade winds in the tropical North Atlantic and increases low-level cloud cover, which acts to amplify the SST cooling in the North Atlantic. During warm periods in the North Atlantic, the opposite response occurs. We are testing whether the amplitude of this feedback is realistically simulated in the CMIP5 models, and whether inter-model differences in the amplitude of the feedback can explain differences in model simulations of Atlantic multi-<span class="hlt">decadal</span> <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS11A1449E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS11A1449E"><span>Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> in the view of linear equatorial wave theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Emile-Geay, J. B.; Cane, M. A.</p> <p>2006-12-01</p> <p>It has recently been proposed, within the framework of the linear shallow water equations, that tropical Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> can be accounted for by basin modes with eigenperiods of 10 to 20 years, amplifying a mid- latitude wind forcing with an essentially white spectrum (Cessi and Louazel 2001; Liu 2003). We question this idea here, using a different formalism of linear equatorial wave theory. We compute the Green's function for the wind forced response of a linear equatorial shallow water ocean, and use the results of Cane and Moore (1981) to obtain a compact, closed form expression for the motion of the equatorial thermocline, which applies to all frequencies lower than seasonal. At very low frequencies (<span class="hlt">decadal</span> timescales), we recover the planetary geostrophic solution used by Cessi and Louazel (2001), as well as the equatorial wave solution of Liu (2003), and give a formal explanation for this convergence. Using this more general solution to explore more realistic wind forcings, we come to a different interpretation of the results. We find that the equatorial thermocline is inherently more sensitive to local than to remote wind forcing, and that planetary Rossby modes only weakly alter the spectral characteristics of the response. Tropical winds are able to generate a strong equatorial response with periods of 10 to 20 years, while midlatitude winds can only do so for periods longer than about 50 years. Since the <span class="hlt">decadal</span> pattern of <span class="hlt">observed</span> winds shows similar amplitude for tropical and midlatitude winds, we conclude that the latter are unlikely to be responsible for the <span class="hlt">observed</span> <span class="hlt">decadal</span> tropical Pacific SST <span class="hlt">variability</span>. References : Cane, M. A., and Moore, D. W., 1981: A note on low-frequency equatorial basin modes. J. Phys. Oceanogr., 11(11), 1578 1584. Cessi, P., and Louazel, S., 2001: <span class="hlt">Decadal</span> oceanic response to stochastic wind forcing. J. Phys. Oceanogr., 31, 3020 3029. Liu, Z., 2003: Tropical ocean <span class="hlt">decadal</span> <span class="hlt">variability</span> and resonance of planetary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1275738-frontiers-decadal-climate-variability-proceedings-workshop','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1275738-frontiers-decadal-climate-variability-proceedings-workshop"><span>Frontiers in <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span>: Proceedings of a Workshop</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Purcell, Amanda</p> <p></p> <p>A number of studies indicate an apparent slowdown in the overall rise in global average surface temperature between roughly 1998 and 2014. Most models did not predict such a slowdown--a fact that stimulated a lot of new research on <span class="hlt">variability</span> of Earth's climate system. At a September 2015 workshop, leading scientists gathered to discuss current understanding of climate <span class="hlt">variability</span> on <span class="hlt">decadal</span> timescales (10 to 30 years) and whether and how prediction of it might be improved. Many researchers have focused their attention on the climate system itself, which is known to vary across seasons, <span class="hlt">decades</span>, and other timescales. Several naturalmore » <span class="hlt">variables</span> produce "ups and downs" in the climate system, which are superimposed on the long-term warming trend due to human influence. Understanding <span class="hlt">decadal</span> climate <span class="hlt">variability</span> is important not only for assessing global climate change but also for improving decision making related to infrastructure, water resources, agriculture, energy, and other realms. Like the well-studied El Nino and La Nina interannual variations, <span class="hlt">decadal</span> climate <span class="hlt">variability</span> is associated with specific regional patterns of temperature and precipitation, such as heat waves, cold spells, and droughts. Several participants shared research that assesses <span class="hlt">decadal</span> predictive capability of current models.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020587','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020587"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of precipitation over Western North America</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cayan, D.R.; Dettinger, M.D.; Diaz, Henry F.; Graham, N.E.</p> <p>1998-01-01</p> <p><span class="hlt">Decadal</span> (>7- yr period) variations of precipitation over western North America account for 20%-50% of the variance of annual precipitation. Spatially, the <span class="hlt">decadal</span> <span class="hlt">variability</span> is broken into several regional [O(1000 km)] components. These <span class="hlt">decadal</span> variations are contributed by fluctuations in precipitation from seasons of the year that vary from region to region and that are not necessarily concentrated in the wettest season(s) alone. The precipitation variations are linked to various <span class="hlt">decadal</span> atmospheric circulation and SST anomaly patterns where scales range from regional to global scales and that emphasize tropical or extratropical connections, depending upon which precipitation region is considered. Further, wet or dry <span class="hlt">decades</span> are associated with changes in frequency of at least a few short-period circulation 'modes' such as the Pacific-North American pattern. Precipitation fluctuations over the southwestern United States and the Saskatchewan region of western Canada are associated with extensive shifts of sea level pressure and SST anomalies, suggesting that they are components of low-frequency precipitation <span class="hlt">variability</span> from global-scale climate proceses. Consistent with the global scale of its pressure and SST connection, the Southwest <span class="hlt">decadal</span> precipitation is aligned with opposing precipitation fluctuations in northern Africa.<span class="hlt">Decadal</span> (>7-yr period) variations of precipitation over western North America account for 20%-50% of the variance of annual precipitation. Spatially, the <span class="hlt">decadal</span> <span class="hlt">variability</span> is broken into several regional [O(1000 km)] components. These <span class="hlt">decadal</span> variations are contributed by fluctuations in precipitation from seasons of the year that vary from region to region and that are not necessarily concentrated in the wettest season(s) alone. The precipitation variations are linked to various <span class="hlt">decadal</span> atmospheric circulation and SST anomaly patterns where scales range from regional to global scales and that emphasize tropical or extratropical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P23D..07D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P23D..07D"><span>Two <span class="hlt">Decades</span> (almost) of Keck <span class="hlt">Observations</span> of Io</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Pater, I.; Davies, A. G.; de Kleer, K.</p> <p>2015-12-01</p> <p>We have regularly <span class="hlt">observed</span> Io with the 10-m Keck Telescope since 1998, initially using the speckle imaging technique, and switching to Adaptive Optics techniques when this became available in 2001. In this talk we will discuss several eruptions that we witnessed, and present 20-30 year timelines of thermal emission from Pele, Pillan, Janus Patera, Kanehekili Fluctus, and Loki Patera, updating timelines in recent publications [1, 2] with additional Keck adaptive optics data obtained between 2002 and 2015. These new timelines are the most comprehensive plots ever produced of the volcanic thermal emission <span class="hlt">variability</span> for these or any other locations on Io, utilizing data from multiple ground- and space-based assets. Our continuing multi-<span class="hlt">decadal</span> <span class="hlt">observing</span> program forms the basis for charting the <span class="hlt">variability</span> of Io's volcanic activity, of great importance for understanding the evolution of the Galilean satellite system, and with the expectation of new missions to the jovian system in the next <span class="hlt">decade</span>. Acknowledgements: This research is in part supported by NSF grant AST-1313485 to UC Berkeley. AGD is supported by a grant from the NASA OPR Program. References: [1] Davies et al. (2012) Icarus, 221, 466-470. [2] Rathbun and Spencer (2010) Icarus, 209, 625-630.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914547S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914547S"><span>The role of internal <span class="hlt">variability</span> for <span class="hlt">decadal</span> carbon uptake anomalies in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spring, Aaron; Hi, Hongmei; Ilyina, Tatiana</p> <p>2017-04-01</p> <p>The Southern Ocean is a major sink for anthropogenic CO2 emissions and hence it plays an essential role in modulating global carbon cycle and climate change. Previous studies based on <span class="hlt">observations</span> (e.g., Landschützer et al. 2015) show pronounced <span class="hlt">decadal</span> variations of carbon uptake in the Southern Ocean in recent <span class="hlt">decades</span> and this <span class="hlt">variability</span> is largely driven by internal climate <span class="hlt">variability</span>. However, due to limited ensemble size of simulations, the <span class="hlt">variability</span> of this important ocean sink is still poorly assessed by the state-of-the-art earth system models (ESMs). To assess the internal <span class="hlt">variability</span> of carbon sink in the Southern Ocean, we use a large ensemble of 100 member simulations based on the Max Planck Institute-ESM (MPI-ESM). The large ensemble of simulations is generated via perturbed initial conditions in the ocean and atmosphere. Each ensemble member includes a historical simulation from 1850 to 2005 with an extension until 2100 under Representative Concentration Pathway (RCP) 4.5 future projections. Here we use model simulations from 1980-2015 to compare with available <span class="hlt">observation</span>-based dataset. We found several ensemble members showing <span class="hlt">decadal</span> decreasing trends in the carbon sink, which are similar to the trend shown in <span class="hlt">observations</span>. This result suggests that MPI-ESM large ensemble simulations are able to reproduce <span class="hlt">decadal</span> variation of carbon sink in the Southern Ocean. Moreover, the decreasing trends of Southern Ocean carbon sink in MPI-ESM are mainly contributed by region between 50-60°S. To understand the internal <span class="hlt">variability</span> of the air-sea carbon fluxes in the Southern Ocean, we further investigate the <span class="hlt">variability</span> of underlying processes, such as physical climate <span class="hlt">variability</span> and ocean biological processes. Our results indicate two main drivers for the <span class="hlt">decadal</span> decreasing trend of carbon sink: i) Intensified winds enhance upwelling of old carbon-rich waters, this leads to increase of the ocean surface pCO2; ii) Primary production is reduced in area</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC54A..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC54A..08F"><span><span class="hlt">Variability</span> of western Amazon dry-season precipitation extremes: importance of <span class="hlt">decadal</span> fluctuations and implications for predictability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernandes, K.; Baethgen, W.; Verchot, L. V.; Giannini, A.; Pinedo-Vasquez, M.</p> <p>2014-12-01</p> <p>A complete assessment of climate change projections requires understanding the combined effects of <span class="hlt">decadal</span> <span class="hlt">variability</span> and long-term trends and evaluating the ability of models to simulate them. The western Amazon severe droughts of the 2000s were the result of a modest drying trend enhanced by reduced moisture transport from the tropical Atlantic. Most of the WA dry-season precipitation <span class="hlt">decadal</span> <span class="hlt">variability</span> is attributable to <span class="hlt">decadal</span> fluctuations of the north-south gradient (NSG) in Atlantic sea surface temperature (SST). The <span class="hlt">observed</span> WA and NSG <span class="hlt">decadal</span> co-<span class="hlt">variability</span> is well reproduced in Global Climate Models (GCMs) pre-industrial control (PIC) and historical (HIST) experiments that were part of the Intergovernmental Panel on Climate Change fifth assessment report (IPCC-AR5). This suggests that unforced or natural climate <span class="hlt">variability</span>, characteristic of the PIC simulations, determines the nature of this coupling, as the results from HIST simulations (forced with greenhouse gases (GHG) and natural and anthropogenic aerosols) are comparable in magnitude and spatial distribution. <span class="hlt">Decadal</span> fluctuation in the NSG also determines shifts in the probability of repeated droughts and pluvials in WA, as there is a 65% chance of 3 or more years of droughts per <span class="hlt">decade</span> when NSG>0 compared to 18% when NSG<0. The HIST and PIC model simulations also reproduce the <span class="hlt">observed</span> shifts in probability distribution of droughts and pluvials as a function of the NSG <span class="hlt">decadal</span> phase, suggesting there is great potential for <span class="hlt">decadal</span> predictability based on GCMs. Persistence of the current NSG positive phase may lead to continuing above normal frequencies of western Amazon dry-season droughts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020022509&hterms=climate+change+evidence&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclimate%2Bchange%2Bevidence','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020022509&hterms=climate+change+evidence&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclimate%2Bchange%2Bevidence"><span>Evidence for Large <span class="hlt">Decadal</span> <span class="hlt">Variability</span> in the Tropical Mean Radiative Energy Budget</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wielicki, Bruce A.; Wong, Takmeng; Allan, Richard; Slingo, Anthony; Kiehl, Jeffrey T.; Soden, Brian J.; Gordon, C. T.; Miller, Alvin J.; Yang, Shi-Keng; Randall, David R.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20020022509'); toggleEditAbsImage('author_20020022509_show'); toggleEditAbsImage('author_20020022509_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20020022509_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20020022509_hide"></p> <p>2001-01-01</p> <p>It is widely assumed that variations in the radiative energy budget at large time and space scales are very small. We present new evidence from a compilation of over two <span class="hlt">decades</span> of accurate satellite data that the top-of-atmosphere (TOA) tropical radiative energy budget is much more dynamic and <span class="hlt">variable</span> than previously thought. We demonstrate that the radiation budget changes are caused by changes In tropical mean cloudiness. The results of several current climate model simulations fall to predict this large <span class="hlt">observed</span> variation In tropical energy budget. The missing <span class="hlt">variability</span> in the models highlights the critical need to Improve cloud modeling in the tropics to support Improved prediction of tropical climate on Inter-annual and <span class="hlt">decadal</span> time scales. We believe that these data are the first rigorous demonstration of <span class="hlt">decadal</span> time scale changes In the Earth's tropical cloudiness, and that they represent a new and necessary test of climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NatCC...8..493M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NatCC...8..493M"><span>Model tropical Atlantic biases underpin diminished Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McGregor, Shayne; Stuecker, Malte F.; Kajtar, Jules B.; England, Matthew H.; Collins, Mat</p> <p>2018-06-01</p> <p>Pacific trade winds have displayed unprecedented strengthening in recent <span class="hlt">decades</span>1. This strengthening has been associated with east Pacific sea surface cooling2 and the early twenty-first-century slowdown in global surface warming2,3, amongst a host of other substantial impacts4-9. Although some climate models produce the timing of these recently <span class="hlt">observed</span> trends10, they all fail to produce the trend magnitude2,11,12. This may in part be related to the apparent model underrepresentation of low-frequency Pacific Ocean <span class="hlt">variability</span> and <span class="hlt">decadal</span> wind trends2,11-13 or be due to a misrepresentation of a forced response1,14-16 or a combination of both. An increasingly prominent connection between the Pacific and Atlantic basins has been identified as a key driver of this strengthening of the Pacific trade winds12,17-20. Here we use targeted climate model experiments to show that combining the recent Atlantic warming trend with the typical climate model bias leads to a substantially underestimated response for the Pacific Ocean wind and surface temperature. The underestimation largely stems from a reduction and eastward shift of the atmospheric heating response to the tropical Atlantic warming trend. This result suggests that the recent Pacific trends and model <span class="hlt">decadal</span> <span class="hlt">variability</span> may be better captured by models with improved mean-state climatologies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC33H..05L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC33H..05L"><span>The summer North Atlantic Oscillation (SNAO) <span class="hlt">variability</span> on <span class="hlt">decadal</span> to paleoclimate time scales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Linderholm, H. W.; Folland, C. K.; Zhang, P.; Gunnarson, B. E.; Jeong, J. H.; Ren, H.</p> <p>2017-12-01</p> <p>The summer North Atlantic Oscillation (SNAO), strongly related to the latitude of the North Atlantic and European summer storm tracks, exerts a considerable influence on European summer climate <span class="hlt">variability</span> and extremes. Here we extend the period covered by the SNAO from July and August to June, July and August (JJA). As well as marked interannual <span class="hlt">variability</span>, the JJA SNAO has shown a large inter-<span class="hlt">decadal</span> change since the 1970s. <span class="hlt">Decadally</span> averaged, there has been a change from a very positive to a rather negative SNAO phase. This change in SNAO phase is opposite in sign from that expected by a number of climate models under enhanced greenhouse forcing by the late twenty first century. It has led to noticeably wetter summers in North West Europe in the last <span class="hlt">decade</span>. On interannual to multidecadal timescales, SNAO <span class="hlt">variability</span> is linked to variations in North Atlantic sea surface temperature (SST): <span class="hlt">observations</span> and models indicate an association between the Atlantic Multi-<span class="hlt">decadal</span> Oscillation (AMO) where the cold (warm) phase of the AMO corresponds a positive (negative) phase of the SNAO. <span class="hlt">Observations</span> also indicate a link with SST in the Gulf Stream region of the North Atlantic where, particularly on <span class="hlt">decadal</span> time scales, SST warming may favour a more positive phase of the SNAO. Influences of Arctic climate change on North Atlantic and European atmospheric circulation may also exist, particularly reduced sea ice coverage, perhaps favouring the negative phase of the SNAO. A new tree-ring data based JJA SNAO reconstruction extending over the last millennium, as well as climate model output for the same period, enables us to examine the influence of North Atlantic SST and Arctic sea-ice coverage, as well as SNAO impacts on European summer climate, in a long-term, pre-industrial context.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_2 --> <div id="page_3" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="41"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H53K..04L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H53K..04L"><span>Sustainability or Collapse: Interplay Between <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span> and Human Activities Matters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Y.; Hu, H.; Tian, F.</p> <p>2016-12-01</p> <p>The Aral Sea Crisis and the deterioration of Tarim River Basin are representative cases of emergent water deficit problems in arid areas. Comparing cases of water deficit problems in different regions and considering the in the perspective of socio-hydrology is helpful to obtain guidance on integrated management of arid area basins. Analyzing the interplay between <span class="hlt">decadal</span> climate <span class="hlt">variability</span> and human activities in both basins, the important role of human activities is <span class="hlt">observed</span>. <span class="hlt">Decadal</span> climate <span class="hlt">variability</span> tempts people to adapt fast to increasing water resources and slowly to decreasing water resources, while using unsustainable technical measures to offset water shortage. Due to this asymmetry the situation deteriorates with technically enhanced capabilities of societies to exploit water resources, and more integrated long-term management capacity is in high demand.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110023617','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110023617"><span>Atmospheric Blocking and Atlantic Multi-<span class="hlt">Decadal</span> Ocean <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Haekkinen, Sirpa; Rhines, Peter B.; Worthlen, Denise L.</p> <p>2011-01-01</p> <p>Based on the 20th century atmospheric reanalysis, winters with more frequent blocking, in a band of blocked latitudes from Greenland to Western Europe, are found to persist over several <span class="hlt">decades</span> and correspond to a warm North Atlantic Ocean, in-phase with Atlantic multi-<span class="hlt">decadal</span> ocean <span class="hlt">variability</span>. Atmospheric blocking over the northern North Atlantic, which involves isolation of large regions of air from the westerly circulation for 5 days or more, influences fundamentally the ocean circulation and upper ocean properties by impacting wind patterns. Winters with clusters of more frequent blocking between Greenland and western Europe correspond to a warmer, more saline subpolar ocean. The correspondence between blocked westerly winds and warm ocean holds in recent <span class="hlt">decadal</span> episodes (especially, 1996-2010). It also describes much longer-timescale Atlantic multidecadal ocean <span class="hlt">variability</span> (AMV), including the extreme, pre-greenhouse-gas, northern warming of the 1930s-1960s. The space-time structure of the wind forcing associated with a blocked regime leads to weaker ocean gyres and weaker heat-exchange, both of which contribute to the warm phase of AMV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ERL....12j4005B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ERL....12j4005B"><span><span class="hlt">Decadal</span> climate <span class="hlt">variability</span> and the spatial organization of deep hydrological drought</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barros, Ana P.; Hodes, Jared L.; Arulraj, Malarvizhi</p> <p>2017-10-01</p> <p>Empirical Orthogonal Function (EOF), wavelet, and wavelet coherence analysis of baseflow time-series from 126 streamgauges (record-length > 50 years; small and mid-size watersheds) in the US South Atlantic (USSA) region reveal three principal modes of space-time <span class="hlt">variability</span>: (1) a region-wide dominant mode tied to annual precipitation that exhibits non-stationary <span class="hlt">decadal</span> <span class="hlt">variability</span> after the mid 1990s concurrent with the warming of the AMO (Atlantic Multidecadal Oscillation); (2) two spatial modes, east and west of the Blue Ridge, exhibiting nonstationary seasonal to sub-<span class="hlt">decadal</span> <span class="hlt">variability</span> before and after 1990 attributed to complex nonlinear interactions between ENSO and AMO impacting precipitation and recharge; and (3) deep (<span class="hlt">decadal</span>) and shallow (< 6 years) space-time modes of groundwater <span class="hlt">variability</span> separating basins with high and low annual mean baseflow fraction (MBF) by physiographic region. The results explain the propagation of multiscale climate <span class="hlt">variability</span> into the regional groundwater system through recharge modulated by topography, geomorphology, and geology to determine the spatial organization of baseflow <span class="hlt">variability</span> at <span class="hlt">decadal</span> (and longer) time-scales, that is, deep hydrologic drought. Further, these findings suggest potential for long-range predictability of hydrological drought in small and mid-size watersheds, where baseflow is a robust indicator of nonstationary yield capacity of the underlying groundwater basins. Predictive associations between climate mode indices and deep baseflow (e.g. persistent decreases of the <span class="hlt">decadal</span>-scale components of baseflow during the cold phase of the AMO in the USSA) can be instrumental toward improving forecast lead-times and long-range mitigation of severe drought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4411201W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4411201W"><span>A Census of Atmospheric <span class="hlt">Variability</span> From Seconds to <span class="hlt">Decades</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, Paul D.; Alexander, M. Joan; Barnes, Elizabeth A.; Butler, Amy H.; Davies, Huw C.; Garfinkel, Chaim I.; Kushnir, Yochanan; Lane, Todd P.; Lundquist, Julie K.; Martius, Olivia; Maue, Ryan N.; Peltier, W. Richard; Sato, Kaoru; Scaife, Adam A.; Zhang, Chidong</p> <p>2017-11-01</p> <p>This paper synthesizes and summarizes atmospheric <span class="hlt">variability</span> on time scales from seconds to <span class="hlt">decades</span> through a phenomenological census. We focus mainly on unforced <span class="hlt">variability</span> in the troposphere, stratosphere, and mesosphere. In addition to atmosphere-only modes, our scope also includes coupled modes, in which the atmosphere interacts with the other components of the Earth system, such as the ocean, hydrosphere, and cryosphere. The topics covered include turbulence on time scales of seconds and minutes, gravity waves on time scales of hours, weather systems on time scales of days, atmospheric blocking on time scales of weeks, the Madden-Julian Oscillation on time scales of months, the Quasi-Biennial Oscillation and El Niño-Southern Oscillation on time scales of years, and the North Atlantic, Arctic, Antarctic, Pacific <span class="hlt">Decadal</span>, and Atlantic Multidecadal Oscillations on time scales of <span class="hlt">decades</span>. The paper serves as an introduction to a special collection of Geophysical Research Letters on atmospheric <span class="hlt">variability</span>. We hope that both this paper and the collection will serve as a useful resource for the atmospheric science community and will act as inspiration for setting future research directions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1378474','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1378474"><span>AMOC <span class="hlt">decadal</span> <span class="hlt">variability</span> in Earth system models: Mechanisms and climate impacts</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Fedorov, Alexey</p> <p></p> <p>This is the final report for the project titled "AMOC <span class="hlt">decadal</span> <span class="hlt">variability</span> in Earth system models: Mechanisms and climate impacts". The central goal of this one-year research project was to understand the mechanisms of <span class="hlt">decadal</span> and multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of the Atlantic Meridional Overturning Circulation (AMOC) within a hierarchy of climate models ranging from realistic ocean GCMs to Earth system models. The AMOC is a key element of ocean circulation responsible for oceanic transport of heat from low to high latitudes and controlling, to a large extent, climate variations in the North Atlantic. The questions of the AMOC stability, <span class="hlt">variability</span> andmore » predictability, directly relevant to the questions of climate predictability, were at the center of the research work.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A41P..04D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41P..04D"><span>Atmospheric River Characteristics under <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Done, J.; Ge, M.</p> <p>2017-12-01</p> <p>How does <span class="hlt">decadal</span> climate <span class="hlt">variability</span> change the nature and predictability of atmospheric river events? <span class="hlt">Decadal</span> swings in atmospheric river frequency, or shifts in the proportion of precipitation falling as rain, could challenge current water resource and flood risk management practice. Physical multi-scale processes operating between Pacific sea surface temperatures (SSTs) and atmospheric rivers over the Western U.S. are explored using the global Model for Prediction Across Scales (MPAS). A 45km global mesh is refined over the Western U.S. to 12km to capture the major terrain effects on precipitation. The performance of the MPAS is first evaluated for a case study atmospheric river event over California. Atmospheric river characteristics are then compared in a pair of idealized simulations, each driven by Pacific SST patterns characteristic of opposite phases of the Interdecadal Pacific Oscillation (IPO). Given recent evidence that we have entered a positive phase of the IPO, implications for current reservoir management practice over the next <span class="hlt">decade</span> will be discussed. This work contributes to the NSF-funded project UDECIDE (Understanding Decision-Climate Interactions on <span class="hlt">Decadal</span> Scales). UDECIDE brings together practitioners, engineers, statisticians, and climate scientists to understand the role of <span class="hlt">decadal</span> climate information for water management and decisions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/588604-greenhouse-warming-decadal-variability-el-nino-attempt-understand-anomalous','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/588604-greenhouse-warming-decadal-variability-el-nino-attempt-understand-anomalous"><span>Greenhouse warming, <span class="hlt">decadal</span> <span class="hlt">variability</span>, or El Nino? An attempt to understand the anomalous 1990s</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Latif, M.; Eckert, C.; Kleeman, R.</p> <p></p> <p>The dominant <span class="hlt">variability</span> modes in the Tropics are investigated and contrasted with the anomalous situation <span class="hlt">observed</span> during the last few years. The prime quantity analyzed is anomalous sea surface temperature (SST) in the region 30{degrees}S-60{degrees}N. Additionally, <span class="hlt">observed</span> tropical surface wind stress fields were investigated. Further tropical atmospheric information was derived from a multidecadal run with an atmospheric general circulation model that was forced by the same SSTs. The tropical SST <span class="hlt">variability</span> can be characterized by three modes: an interannual mode [the El Nino-Southern Oscillation (ENSO)], a <span class="hlt">decadal</span> mode, and a trend or unresolved ultra-low-frequency <span class="hlt">variability</span>. 48 refs., 20 figs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoRL..3921705A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoRL..3921705A"><span>The amplitude of <span class="hlt">decadal</span> to multidecadal <span class="hlt">variability</span> in precipitation simulated by state-of-the-art climate models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ault, T. R.; Cole, J. E.; St. George, S.</p> <p>2012-11-01</p> <p>We assess the magnitude of <span class="hlt">decadal</span> to multidecadal (D2M) <span class="hlt">variability</span> in Climate Model Intercomparison Project 5 (CMIP5) simulations that will be used to understand, and plan for, climate change as part of the Intergovernmental Panel on Climate Change's 5th Assessment Report. Model performance on D2M timescales is evaluated using metrics designed to characterize the relative and absolute magnitude of <span class="hlt">variability</span> at these frequencies. In <span class="hlt">observational</span> data, we find that between 10% and 35% of the total variance occurs on D2M timescales. Regions characterized by the high end of this range include Africa, Australia, western North America, and the Amazon region of South America. In these areas D2M fluctuations are especially prominent and linked to prolonged drought. D2M fluctuations account for considerably less of the total variance (between 5% and 15%) in the CMIP5 archive of historical (1850-2005) simulations. The discrepancy between <span class="hlt">observation</span> and model based estimates of D2M prominence reflects two features of the CMIP5 archive. First, interannual components of <span class="hlt">variability</span> are generally too energetic. Second, <span class="hlt">decadal</span> components are too weak in several key regions. Our findings imply that projections of the future lack sufficient <span class="hlt">decadal</span> <span class="hlt">variability</span>, presenting a limited view of prolonged drought and pluvial risk.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27404090','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27404090"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of tropical tropopause temperature and its relationship to the Pacific <span class="hlt">Decadal</span> Oscillation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Wuke; Matthes, Katja; Omrani, Nour-Eddine; Latif, Mojib</p> <p>2016-07-12</p> <p>Tropopause temperatures (TPTs) control the amount of stratospheric water vapour, which influences chemistry, radiation and circulation in the stratosphere, and is also an important driver of surface climate. <span class="hlt">Decadal</span> <span class="hlt">variability</span> and long-term trends in tropical TPTs as well as stratospheric water vapour are largely unknown. Here, we present for the first time evidence, from reanalysis and state-of-the-art climate model simulations, of a link between <span class="hlt">decadal</span> <span class="hlt">variability</span> in tropical TPTs and the Pacific <span class="hlt">Decadal</span> Oscillation (PDO). The negative phase of the PDO is associated with anomalously cold sea surface temperatures (SSTs) in the tropical east and central Pacific, which enhance the zonal SST gradient across the equatorial Pacific. The latter drives a stronger Walker Circulation and a weaker Hadley Circulation, which leads to less convection and subsequently a warmer tropopause over the central equatorial Pacific. Over the North Pacific, positive sea level pressure anomalies occur, which damp vertical wave propagation into the stratosphere. This in turn slows the Brewer-Dobson circulation, and hence warms the tropical tropopause, enabling more water vapour to enter the stratosphere. The reverse chain of events holds for the positive phase of the PDO. Such ocean-troposphere-stratosphere interactions may provide an important feedback on the Earth's global surface temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4941568','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4941568"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of tropical tropopause temperature and its relationship to the Pacific <span class="hlt">Decadal</span> Oscillation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Wuke; Matthes, Katja; Omrani, Nour-Eddine; Latif, Mojib</p> <p>2016-01-01</p> <p>Tropopause temperatures (TPTs) control the amount of stratospheric water vapour, which influences chemistry, radiation and circulation in the stratosphere, and is also an important driver of surface climate. <span class="hlt">Decadal</span> <span class="hlt">variability</span> and long-term trends in tropical TPTs as well as stratospheric water vapour are largely unknown. Here, we present for the first time evidence, from reanalysis and state-of-the-art climate model simulations, of a link between <span class="hlt">decadal</span> <span class="hlt">variability</span> in tropical TPTs and the Pacific <span class="hlt">Decadal</span> Oscillation (PDO). The negative phase of the PDO is associated with anomalously cold sea surface temperatures (SSTs) in the tropical east and central Pacific, which enhance the zonal SST gradient across the equatorial Pacific. The latter drives a stronger Walker Circulation and a weaker Hadley Circulation, which leads to less convection and subsequently a warmer tropopause over the central equatorial Pacific. Over the North Pacific, positive sea level pressure anomalies occur, which damp vertical wave propagation into the stratosphere. This in turn slows the Brewer-Dobson circulation, and hence warms the tropical tropopause, enabling more water vapour to enter the stratosphere. The reverse chain of events holds for the positive phase of the PDO. Such ocean-troposphere-stratosphere interactions may provide an important feedback on the Earth’s global surface temperature. PMID:27404090</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7710S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7710S"><span>Interannual to <span class="hlt">decadal</span> <span class="hlt">variability</span> of circulation in the northern Japan/East Sea, 1958-2006</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stepanov, Dmitry; Stepanova, Victoriia; Gusev, Anatoly</p> <p>2015-04-01</p> <p>We use a numerical ocean model INMOM (Institute of Numerical Mathematics Ocean Model) and atmospheric forcing data extracted from the CORE (Coordinated Ocean Reference Experiments) dataset and reconstruct a circulation in the Japan/East Sea (JES) from 1958 to 2006 and its interannual and <span class="hlt">decadal</span> <span class="hlt">variability</span> in the intermediate and abyssal layers in the northern JES. It is founded that the circulation is cyclonic over the course of a climatological year. The circulation increases in spring and decreases in autumn. We analyzes the relative vorticity (RV) averaged over the Japan Basin (JB) and show that the <span class="hlt">variability</span> is characterized by the interannual oscillations (2.3, 3.7 and 4.7 years) and <span class="hlt">decadal</span> <span class="hlt">variability</span> (9.5 and 14.3 years). The spectrum structure of the average RV <span class="hlt">variability</span> does not change with depth; however, the energy of the <span class="hlt">decadal</span> oscillations decreases in contrast to that of the interannual oscillations. We analyze monthly anomalies of the wind stress curl and sensible heat flux and reveal that interannual <span class="hlt">variability</span> (3-4 years) of the circulation over the JB result from 4-year <span class="hlt">variability</span> of the wind stress curl. In contrast, the <span class="hlt">decadal</span> <span class="hlt">variability</span> (period of 9.5 years) of the circulation over the JB is generated by both the wind stress curl and the <span class="hlt">decadal</span> <span class="hlt">variability</span> in deep convection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990017735','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990017735"><span>Interannual and <span class="hlt">Decadal</span> <span class="hlt">Variability</span> of Summer Rainfall over South America</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zhou, Jiayu; Lau, K.-M.</p> <p>1999-01-01</p> <p>Using the CPC (Climate Prediction Center) Merged Analysis of Precipitation product along with the Goddard Earth <span class="hlt">Observing</span> System reanalysis and the Climate Analysis Center sea surface temperature (SST) data, we conduct a diagnostic study of the interannual and <span class="hlt">decadal</span> scale <span class="hlt">variability</span> of summer rainfall over South America. Results show three leading modes of rainfall variation identified with interannual, <span class="hlt">decadal</span>, and long-term trend <span class="hlt">variability</span>. Together, these modes explain more than half the total variance. The first mode is highly correlated with El Nino/southern oscillation (ENSO), showing severe drought over Northeast Brazil and copious rainfall over the Ecuador coast and the area of Uruguay-Southern Brazil in El Nino years. This pattern is attributed to the large scale zonal shift of the Walker circulation and local Hadley cell anomaly induced by positive (negative) SST anomaly over the eastern (western) equatorial Pacific. In El Nino years, two convective belts indicated by upper tropospheric velocity potential trough and mid-tropospheric rising motion, which are somewhat symmetric about the equator, extend toward the northeast and the southeast into the tropical North and South Atlantic respectively. Sandwiched between the ascent is a region of descending motion over Northeast Brazil. The southern branch of the anomalous Hadley cell is dynamically linked to the increase of rainfall over Uruguay-Southern Brazil. The regional response of anomalous circulation shows a stronger South American summer monsoon and an enhanced (weakened) subtropical high over the South Atlantic (South Pacific) Ocean. The <span class="hlt">decadal</span> variation displays a meridional shift of the Intertropical Convergence Zone (ITCZ), which is tie to the anomalous cross-equatorial SST gradient over the Atlantic and the eastern Pacific. In conjunction with this mode is a large scale mass swing between the polar regions and midlatitudes in both hemispheres. Over the South Atlantic and the South Pacific</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS13A1795Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS13A1795Y"><span>Indo-Pacific sea level <span class="hlt">variability</span> during recent <span class="hlt">decades</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamanaka, G.; Tsujino, H.; Nakano, H.; Urakawa, S. L.; Sakamoto, K.</p> <p>2016-12-01</p> <p><span class="hlt">Decadal</span> <span class="hlt">variability</span> of sea level in the Indo-Pacific region is investigated using a historical OGCM simulation. The OGCM driven by the atmospheric forcing removing long-term trends clearly exhibits <span class="hlt">decadal</span> sea level <span class="hlt">variability</span> in the Pacific Ocean, which is associated with eastern tropical Pacific thermal anomalies. During the period of 1977-1987, the sea level anomalies are positive in the eastern equatorial Pacific and show deviations from a north-south symmetric distribution, with strongly negative anomalies in the western tropical South Pacific. During the period of 1996-2006, in contrast, the sea level anomalies are negative in the eastern equatorial Pacific and show a nearly north-south symmetric pattern, with positive anomalies in both hemispheres. Concurrently, sea level anomalies in the south-eastern Indian Ocean vary with those in the western tropical Pacific. These sea level variations are closely related to large-scale wind fields. Indo-Pacific sea level distributions are basically determined by wind anomalies over the equatorial region as well as wind stress curl anomalies over the off-equatorial region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC14E2102M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC14E2102M"><span>Global <span class="hlt">decadal</span> climate <span class="hlt">variability</span> driven by Southern Ocean convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marinov, I.; Cabre, A.</p> <p>2016-02-01</p> <p>Here we suggest a set of new "teleconnections" by which the Southern Ocean (SO) can induce anomalies in the tropical oceans and atmosphere. A 5000-year long control simulation in a coupled atmosphere-ocean model (CM2Mc, a low-resolution GFDL model) shows a natural, highly regular multi-<span class="hlt">decadal</span> oscillation between periods of SO open sea convection and non-convective periods. This process happens naturally, with different frequencies and durations of convection across the majority of CMIP5 under preindustrial forcing (deLavergne et al., 2014). In our model, oscillations in Weddell Sea convection drive multidecadal <span class="hlt">variability</span> in SO and global SSTs, as well as SO heat storage, with convective <span class="hlt">decades</span> warm due to the heat released from the Circumpolar Deep Water and non-convective <span class="hlt">decades</span> cold due to subsurface heat storage. Convective pulses drive local SST and sea ice variations south of 60S, immediately triggering changes in the Ferrell and Hadley cells, atmospheric energy budget and cross-equatorial heat exchange, ultimately influencing the position of the Intertropical Convergence Zone and rain patterns in the tropics. Additionally, the SO convection pulse is propagated to the tropics and the North Atlantic MOC via oceanic pathways on relatively fast (<span class="hlt">decadal</span>) timescales, in agreement with recent <span class="hlt">observational</span> constraints. Open sea convection is the major mode of Antarctic Bottom Water (AABW) formation in the CMIP5 models. Future improvements in the representation of shelf convection and sea-ice interaction in the SO are a clear necessity. These model improvements should render the AABW representation more realistic, and might influence (a) the connectivity of the SO with the rest of the planet, as described above and (b) the oceanic and global carbon cycle, of which the AABW is a fundamental conduit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26089521','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26089521"><span>OCEAN CIRCULATION. <span class="hlt">Observing</span> the Atlantic Meridional Overturning Circulation yields a <span class="hlt">decade</span> of inevitable surprises.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Srokosz, M A; Bryden, H L</p> <p>2015-06-19</p> <p>The importance of the Atlantic Meridional Overturning Circulation (AMOC) heat transport for climate is well acknowledged. Climate models predict that the AMOC will slow down under global warming, with substantial impacts, but measurements of ocean circulation have been inadequate to evaluate these predictions. <span class="hlt">Observations</span> over the past <span class="hlt">decade</span> have changed that situation, providing a detailed picture of variations in the AMOC. These <span class="hlt">observations</span> reveal a surprising degree of AMOC <span class="hlt">variability</span> in terms of the intraannual range, the amplitude and phase of the seasonal cycle, the interannual changes in strength affecting the ocean heat content, and the decline of the AMOC over the <span class="hlt">decade</span>, both of the latter two exceeding the variations seen in climate models. Copyright © 2015, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC21E0980P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21E0980P"><span>An '<span class="hlt">Observational</span> Large Ensemble' to compare <span class="hlt">observed</span> and modeled temperature trend uncertainty due to internal <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poppick, A. N.; McKinnon, K. A.; Dunn-Sigouin, E.; Deser, C.</p> <p>2017-12-01</p> <p>Initial condition climate model ensembles suggest that regional temperature trends can be highly <span class="hlt">variable</span> on <span class="hlt">decadal</span> timescales due to characteristics of internal climate <span class="hlt">variability</span>. Accounting for trend uncertainty due to internal <span class="hlt">variability</span> is therefore necessary to contextualize recent <span class="hlt">observed</span> temperature changes. However, while the <span class="hlt">variability</span> of trends in a climate model ensemble can be evaluated directly (as the spread across ensemble members), internal <span class="hlt">variability</span> simulated by a climate model may be inconsistent with <span class="hlt">observations</span>. <span class="hlt">Observation</span>-based methods for assessing the role of internal <span class="hlt">variability</span> on trend uncertainty are therefore required. Here, we use a statistical resampling approach to assess trend uncertainty due to internal <span class="hlt">variability</span> in historical 50-year (1966-2015) winter near-surface air temperature trends over North America. We compare this estimate of trend uncertainty to simulated trend <span class="hlt">variability</span> in the NCAR CESM1 Large Ensemble (LENS), finding that uncertainty in wintertime temperature trends over North America due to internal <span class="hlt">variability</span> is largely overestimated by CESM1, on average by a factor of 32%. Our <span class="hlt">observation</span>-based resampling approach is combined with the forced signal from LENS to produce an '<span class="hlt">Observational</span> Large Ensemble' (OLENS). The members of OLENS indicate a range of spatially coherent fields of temperature trends resulting from different sequences of internal <span class="hlt">variability</span> consistent with <span class="hlt">observations</span>. The smaller trend <span class="hlt">variability</span> in OLENS suggests that uncertainty in the historical climate change signal in <span class="hlt">observations</span> due to internal <span class="hlt">variability</span> is less than suggested by LENS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp...24Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp...24Y"><span><span class="hlt">Variability</span> and predictability of <span class="hlt">decadal</span> mean temperature and precipitation over China in the CCSM4 last millennium simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ying, Kairan; Frederiksen, Carsten S.; Zheng, Xiaogu; Lou, Jiale; Zhao, Tianbao</p> <p>2018-02-01</p> <p>The modes of <span class="hlt">variability</span> that arise from the slow-<span class="hlt">decadal</span> (potentially predictable) and intra-<span class="hlt">decadal</span> (unpredictable) components of <span class="hlt">decadal</span> mean temperature and precipitation over China are examined, in a 1000 year (850-1850 AD) experiment using the CCSM4 model. Solar variations, volcanic aerosols, orbital forcing, land use, and greenhouse gas concentrations provide the main forcing and boundary conditions. The analysis is done using a <span class="hlt">decadal</span> variance decomposition method that identifies sources of potential <span class="hlt">decadal</span> predictability and uncertainty. The average potential <span class="hlt">decadal</span> predictabilities (ratio of slow-to-total <span class="hlt">decadal</span> variance) are 0.62 and 0.37 for the temperature and rainfall over China, respectively, indicating that the (multi-)<span class="hlt">decadal</span> variations of temperature are dominated by slow-<span class="hlt">decadal</span> <span class="hlt">variability</span>, while precipitation is dominated by unpredictable <span class="hlt">decadal</span> noise. Possible sources of <span class="hlt">decadal</span> predictability for the two leading predictable modes of temperature are the external radiative forcing, and the combined effects of slow-<span class="hlt">decadal</span> <span class="hlt">variability</span> of the Arctic oscillation (AO) and the Pacific <span class="hlt">decadal</span> oscillation (PDO), respectively. Combined AO and PDO slow-<span class="hlt">decadal</span> <span class="hlt">variability</span> is associated also with the leading predictable mode of precipitation. External radiative forcing as well as the slow-<span class="hlt">decadal</span> <span class="hlt">variability</span> of PDO are associated with the second predictable rainfall mode; the slow-<span class="hlt">decadal</span> <span class="hlt">variability</span> of Atlantic multi-<span class="hlt">decadal</span> oscillation (AMO) is associated with the third predictable precipitation mode. The dominant unpredictable <span class="hlt">decadal</span> modes are associated with intra-<span class="hlt">decadal</span>/inter-annual phenomena. In particular, the El Niño-Southern Oscillation and the intra-<span class="hlt">decadal</span> <span class="hlt">variability</span> of the AMO, PDO and AO are the most important sources of prediction uncertainty.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC41B1015W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC41B1015W"><span>Interannual to <span class="hlt">Decadal</span> SST <span class="hlt">Variability</span> in the Tropical Indian Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, G.; Newman, M.; Han, W.</p> <p>2017-12-01</p> <p>The Indian Ocean has received increasing attention in recent years for its large impacts on regional and global climate. However, due mainly to the close interdependence of the climate variation within the Tropical Pacific and the Indian Ocean, the internal sea surface temperature (SST) <span class="hlt">variability</span> within the Indian Ocean has not been studied extensively on longer time scales. In this presentation we will show analysis of the interannual to <span class="hlt">decadal</span> SST <span class="hlt">variability</span> in the Tropical Indian Ocean in <span class="hlt">observations</span> and Linear Inverse Model (LIM) results. We also compare the decoupled Indian Ocean SST <span class="hlt">variability</span> from the Pacific against fully coupled one based on LIM integrations, to test the factors influence the features of the leading SST modes in the Indian Ocean. The result shows the Indian Ocean Basin (IOB) mode, which is strongly related to global averaged SST <span class="hlt">variability</span>, passively responses to the Pacific variation. Without tropical Indo-Pacific coupling interaction, the intensity of IOB significantly decreases by 80%. The Indian Ocean Dipole (IOD) mode demonstrates its independence from the Pacific SST <span class="hlt">variability</span> since the IOD does not change its long-term characteristics at all without inter-basin interactions. The overall SSTA variance decreases significantly in the Tropical Indian Ocean in the coupling restricted LIM runs, especially when the one-way impact from the Pacific to the Indian Ocean is turned off, suggesting that most of the <span class="hlt">variability</span> in the Indian Ocean comes from the Pacific influence. On the other hand, the Indian Ocean could also transport anomalies to the Pacific, making the interaction a complete two-way process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME21C..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME21C..02M"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> in the oxygen inventory of North Atlantic Subtropical Underwater captured by sustained, long-term oceanographic time-series <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montes, E.; Muller-Karger, F. E.; Cianca, A.; Lomas, M. W.; Lorenzoni, L.; Habtes, S. Y.</p> <p>2016-02-01</p> <p>Historical <span class="hlt">observations</span> of potential temperature (θ), salinity (S), and dissolved oxygen concentrations (O2) in the subtropical North Atlantic (0-500 m; 0-40°N, 10-80°W) were examined to understand <span class="hlt">decadal</span>-scale changes in O2 in Subtropical Underwater (STUW). STUW is <span class="hlt">observed</span> at four of the longest, sustained ocean biogeochemical and ecological time-series stations, namely the CARIACO Ocean Time-Series Program (10.5°N, 64.7°W), the Bermuda Atlantic Time-series Study (BATS; 31.7°N, 64.2°W), Hydrostation "S" (32.1°N, 64.4°W), and the European Station for Time-series in the Ocean, Canary Islands (ESTOC; 29.2°N, 15.5°W). Data archived by NOAA NODC show that, between 1980 and 2013, STUW O2 (upper 300 m) has declined 0.58 μmol kg-1 yr-1 in the southeastern Caribbean Sea (10-15°N, 60-70°W), and 0.68 μmol kg-1 yr-1 in the western subtropical North Atlantic, respectively (30-35°N, 60-65°W). <span class="hlt">Observations</span> at CARIACO (1995-2013) and BATS (1988-2012), specifically, show that STUW O2 has decreased approximately 0.61 and 0.21 μmol kg-1 yr-1, respectively. No apparent change in STUW O2 was <span class="hlt">observed</span> at ESTOC over the course of the time series (1994-2013). Most of the <span class="hlt">observed</span> O2 loss seems to result from shifts in ventilation associated with wind-driven mixing and slow down of STUW formation rates, rather than changes in diffusive air-sea O2 gas exchange. <span class="hlt">Variability</span> of STUW O2 showed a strong relationship with the Atlantic Multidecadal Oscillation (AMO; R2=0.32, p < 0.001) index phase. During negative AMO years trade winds are stronger between 10°N and 30°N. These conditions stimulate the formation and ventilation of STUW. The decreasing trend in STUW O2 in the three <span class="hlt">decades</span> spanning 1980 through 2013 thus reflects a shift from a strongly negative AMO between mid-1980's and mid-1990's to a positive AMO <span class="hlt">observed</span> between the mid-1990's and 2013. These changes in STUW O2 were captured by the CARIACO, BATS, and Hydrostation "S" time series stations. Sustained</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110008410','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110008410"><span>Atmospheric Blocking and Atlantic Multi-<span class="hlt">Decadal</span> Ocean <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hakkinen, Sirpa; Rhines, Peter B.; Worthen, Denise L.</p> <p>2011-01-01</p> <p>Atmospheric blocking over the northern North Atlantic involves isolation of large regions of air from the westerly circulation for 5-14 days or more. From a recent 20th century atmospheric reanalysis (1,2) winters with more frequent blocking persist over several <span class="hlt">decades</span> and correspond to a warm North Atlantic Ocean, in-phase with Atlantic multi-<span class="hlt">decadal</span> ocean <span class="hlt">variability</span> (AMV). Ocean circulation is forced by wind-stress curl and related air/sea heat exchange, and we find that their space-time structure is associated with dominant blocking patterns: weaker ocean gyres and weaker heat exchange contribute to the warm phase of AMV. Increased blocking activity extending from Greenland to British Isles is evident when winter blocking days of the cold years (1900-1929) are subtracted from those of the warm years (1939-1968).</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990116067&hterms=regional+impacts+climate+change&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dregional%2Bimpacts%2Bclimate%2Bchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990116067&hterms=regional+impacts+climate+change&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dregional%2Bimpacts%2Bclimate%2Bchange"><span>Advances in Understanding <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Busalaacchi, Antonio J.</p> <p>1998-01-01</p> <p>Recently, a joint Brazil-France-U.S. program, known as PIRATA (Pilot Research moored Array in the Tropical Atlantic), was proposed to begin the deployment of moored measurement platforms in the tropical Atlantic in order to enhance the existing <span class="hlt">observational</span> data base and subsequent understanding of the processes by which the ocean and atmosphere couple in key regions of the tropical Atlantic Ocean. Empirical studies have suggested that there are strong relationships between tropical Atlantic upper ocean <span class="hlt">variability</span>, SST, ocean-atmosphere coupling and regional climate <span class="hlt">variability</span>. During the early 1980's a coordinated set of surface wind, subsurface thermal structure, and subsurface current <span class="hlt">observations</span> were obtained as part of the U.S.-France SEQUAL- FOCAL process experiment designed to <span class="hlt">observe</span> the seasonal response of the tropical Atlantic Ocean to surface forcing. Since that time, however, the <span class="hlt">observational</span> data base for the tropical Atlantic Ocean has disintegrated to a few shiptracks measuring ocean temperatures and a small collection of tide gauge stations measuring sea level. A more comprehensive set of <span class="hlt">observations</span>, modeling and empirical studies is now in order to make progress on understanding the regional climate <span class="hlt">variability</span>. The proposed PIRATA program will use mooring platforms similar to the tropical Pacific Ocean TAO array to measure surface fluxes of momentum and heat and the corresponding changes in the upper ocean thermal structure. It is anticipated that the oceanic data from this monitoring array will also be used in a predictive mode for initialization studies of regional coupled climate models. Of particular interest are zonal and meridional modes of ocean-atmosphere <span class="hlt">variability</span> within the tropical Atlantic basin that have significant impacts on the regional climate of the bordering continents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990064457&hterms=climate+change+temperature&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dclimate%2Bchange%2Btemperature','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990064457&hterms=climate+change+temperature&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dclimate%2Bchange%2Btemperature"><span>Advances in Understanding <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Busalacchi, Antonio J.</p> <p>1999-01-01</p> <p>Recently, a joint Brazil-France-U.S. program, known as PIRATA (Pilot Research moored Array in the Tropical Atlantic), was proposed to begin the deployment of moored measurement platforms in the tropical Atlantic in order to enhance the existing <span class="hlt">observational</span> data base and subsequent understanding of the processes by which the ocean and atmosphere couple in key regions of the tropical Atlantic Ocean. Empirical studies have suggested that there are strong relationships between tropical Atlantic upper ocean <span class="hlt">variability</span>, SST, ocean-atmosphere coupling and regional climate <span class="hlt">variability</span>. During the early 1980's a coordinated set of surface wind, subsurface thermal structure, and subsurface current <span class="hlt">observations</span> were obtained as part of the U.S.-France SEQUAL-FOCAL process experiment designed to <span class="hlt">observe</span> the seasonal response of the tropical Atlantic Ocean to surface forcing. Since that time, however, the <span class="hlt">observational</span> data base for the tropical Atlantic Ocean has disintegrated to a few ship-tracks measuring ocean temperatures and a small collection of tide gauge stations measuring sea level. A more comprehensive set of <span class="hlt">observations</span>, modeling and empirical studies is now in order to make progress on understanding the regional climate <span class="hlt">variability</span>. The proposed PIRATA program will use mooring platforms similar to the tropical Pacific Ocean TAO array to measure surface fluxes of momentum and heat and the corresponding changes in the upper ocean thermal structure. It is anticipated that the oceanic data from this monitoring array will also be used in a predictive mode for initialization studies of regional coupled climate models. Of particular interest are zonal and meridional modes of ocean-atmosphere <span class="hlt">variability</span> within the tropical Atlantic basin that have significant impacts on the regional climate of the bordering continents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29867150','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29867150"><span>Role of subsurface ocean in <span class="hlt">decadal</span> climate predictability over the South Atlantic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Morioka, Yushi; Doi, Takeshi; Storto, Andrea; Masina, Simona; Behera, Swadhin K</p> <p>2018-06-04</p> <p><span class="hlt">Decadal</span> climate predictability in the South Atlantic is explored by performing reforecast experiments using a coupled general circulation model with two initialization schemes; one is assimilated with <span class="hlt">observed</span> sea surface temperature (SST) only, and the other is additionally assimilated with <span class="hlt">observed</span> subsurface ocean temperature and salinity. The South Atlantic is known to undergo <span class="hlt">decadal</span> <span class="hlt">variability</span> exhibiting a meridional dipole of SST anomalies through variations in the subtropical high and ocean heat transport. <span class="hlt">Decadal</span> reforecast experiments in which only the model SST is initialized with the <span class="hlt">observation</span> do not predict well the <span class="hlt">observed</span> <span class="hlt">decadal</span> SST <span class="hlt">variability</span> in the South Atlantic, while the other experiments in which the model SST and subsurface ocean are initialized with the <span class="hlt">observation</span> skillfully predict the <span class="hlt">observed</span> <span class="hlt">decadal</span> SST <span class="hlt">variability</span>, particularly in the Southeast Atlantic. In-depth analysis of upper-ocean heat content reveals that a significant improvement of zonal heat transport in the Southeast Atlantic leads to skillful prediction of <span class="hlt">decadal</span> SST <span class="hlt">variability</span> there. These results demonstrate potential roles of subsurface ocean assimilation in the skillful prediction of <span class="hlt">decadal</span> climate <span class="hlt">variability</span> over the South Atlantic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC21A..06O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC21A..06O"><span>Wintertime atmospheric response to <span class="hlt">decadal</span> SST anomalies in the North Pacific frontal zone and its relationship to dominant atmospheric internal <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Okajima, S.; Nakamura, H.; Nishii, K.; Miyasaka, T.; Kuwano-Yoshida, A.; Taguchi, B.</p> <p>2016-02-01</p> <p>A <span class="hlt">decadal</span>-scale warm SST anomaly <span class="hlt">observed</span> in the North Pacific subarctic frontal zone (SAFZ) tends to accompany a basin-scale anticyclonic anomaly in the troposphere that peaks in January. A set of sensitivity experiments conducted with an AGCM simulates an anticyclonic ensemble response over the North Pacific in January. As <span class="hlt">observed</span>, the simulated anticyclonic response is in equivalent barotropic structure and maintained mainly through energy conversion from the ensemble mean circulation realized under the climatological SST, suggesting that the anomaly may have a characteristic of a dynamical mode. Conversion of both available potential energy (APE) and kinetic energy (KE) from the mean flow is important for the <span class="hlt">observed</span> anomaly, while only the former is important for the model response. This is because the model response is located to the north of the jet core region whereas the <span class="hlt">observed</span> anomaly is straddling the jet exit region, which appears to be in correspondence to the northwestward displacement of the center of the dominant atmospheric internal <span class="hlt">variability</span> in our model relative to the <span class="hlt">observed</span> center. Transient eddy feedback forcing also acts to maintain the <span class="hlt">observed</span> anomaly rather efficiently, while its efficiency is much lower for the simulated response, which seems to be consistent with the poleward displacement of the anticyclonic response from the jet and stormtrack axes. A multi-<span class="hlt">decadal</span> integration of our coupled GCM also suggests that atmospheric internal <span class="hlt">variability</span> may be important for determining atmospheric response to the <span class="hlt">decadal</span> SST <span class="hlt">variability</span> of the SAFZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGC14B..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGC14B..04B"><span>Food Price Volatility and <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brown, M. E.</p> <p>2013-12-01</p> <p>The agriculture system is under pressure to increase production every year as global population expands and more people move from a diet mostly made up of grains, to one with more meat, dairy and processed foods. Weather shocks and large changes in international commodity prices in the last <span class="hlt">decade</span> have increased pressure on local food prices. This paper will review several studies that link climate <span class="hlt">variability</span> as measured with satellite remote sensing to food price dynamics in 36 developing countries where local monthly food price data is available. The focus of the research is to understand how weather and climate, as measured by variations in the growing season using satellite remote sensing, has affected agricultural production, food prices and access to food in agricultural societies. Economies are vulnerable to extreme weather at multiple levels. Subsistence small holders who hold livestock and consume much of the food they produce are vulnerable to food production <span class="hlt">variability</span>. The broader society, however, is also vulnerable to extreme weather because of the secondary effects on market functioning, resource availability, and large-scale impacts on employment in trading, trucking and wage labor that are caused by weather-related shocks. Food price <span class="hlt">variability</span> captures many of these broad impacts and can be used to diagnose weather-related vulnerability across multiple sectors. The paper will trace these connections using market-level data and analysis. The context of the analysis is the humanitarian aid community, using the guidance of the USAID Famine Early Warning Systems Network and the United Nation's World Food Program in their response to food security crises. These organizations have worked over the past three <span class="hlt">decades</span> to provide baseline information on food production through satellite remote sensing data and agricultural yield models, as well as assessments of food access through a food price database. Econometric models and spatial analysis are used</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50.2971U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50.2971U"><span>Extremes in East African hydroclimate and links to Indo-Pacific <span class="hlt">variability</span> on interannual to <span class="hlt">decadal</span> timescales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ummenhofer, Caroline C.; Kulüke, Marco; Tierney, Jessica E.</p> <p>2018-04-01</p> <p>East African hydroclimate exhibits considerable <span class="hlt">variability</span> across a range of timescales, with implications for its population that depends on the region's two rainy seasons. Recent work demonstrated that current state-of-the-art climate models consistently underestimate the long rains in boreal spring over the Horn of Africa while overestimating the short rains in autumn. This inability to represent the seasonal cycle makes it problematic for climate models to project changes in East African precipitation. Here we consider whether this bias also has implications for understanding interannual and <span class="hlt">decadal</span> <span class="hlt">variability</span> in the East African long and short rains. Using a consistent framework with an unforced multi-century global coupled climate model simulation, the role of Indo-Pacific <span class="hlt">variability</span> for East African rainfall is compared across timescales and related to <span class="hlt">observations</span>. The dominant driver of East African rainfall anomalies critically depends on the timescale under consideration: Interannual variations in East African hydroclimate coincide with significant sea surface temperature (SST) anomalies across the Indo-Pacific, including those associated with the El Niño-Southern Oscillation (ENSO) in the eastern Pacific, and are linked to changes in the Walker circulation, regional winds and vertical velocities over East Africa. Prolonged drought/pluvial periods in contrast exhibit anomalous SST predominantly in the Indian Ocean and Indo-Pacific warm pool (IPWP) region, while eastern Pacific anomalies are insignificant. We assessed dominant frequencies in Indo-Pacific SST and found the eastern equatorial Pacific dominated by higher-frequency <span class="hlt">variability</span> in the ENSO band, while the tropical Indian Ocean and IPWP exhibit lower-frequency <span class="hlt">variability</span> beyond 10 years. This is consistent with the different contribution to regional precipitation anomalies for the eastern Pacific versus Indian Ocean and IPWP on interannual and <span class="hlt">decadal</span> timescales, respectively. In the model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC43A1174R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC43A1174R"><span><span class="hlt">Observed</span> Decrease of North American Winter Temperature <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rhines, A. N.; Tingley, M.; McKinnon, K. A.; Huybers, P. J.</p> <p>2015-12-01</p> <p>There is considerable interest in determining whether temperature <span class="hlt">variability</span> has changed in recent <span class="hlt">decades</span>. Model ensembles project that extratropical land temperature variance will detectably decrease by 2070. We use quantile regression of station <span class="hlt">observations</span> to show that decreasing <span class="hlt">variability</span> is already robustly detectable for North American winter during 1979--2014. Pointwise trends from GHCND stations are mapped into a continuous spatial field using thin-plate spline regression, resolving small-scales while providing uncertainties accounting for spatial covariance and varying station density. We find that <span class="hlt">variability</span> of daily temperatures, as measured by the difference between the 95th and 5th percentiles, has decreased markedly in winter for both daily minima and maxima. Composites indicate that the reduced spread of winter temperatures primarily results from Arctic amplification decreasing the meridional temperature gradient. Greater <span class="hlt">observed</span> warming in the 5th relative to the 95th percentile stems from asymmetric effects of advection during cold versus warm days; cold air advection is generally from northerly regions that have experienced greater warming than western or southwestern regions that are generally sourced during warm days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.3458S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.3458S"><span>Two centuries of <span class="hlt">observed</span> atmospheric <span class="hlt">variability</span> and change over the North Sea region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stendel, Martin; van den Besselaar, Else; Hannachi, Abdel; Kent, Elizabeth; Lefebvre, Christiana; van Oldenborgh, Geert Jan; Rosenhagen, Gudrun; Schenk, Frederik; van der Schrier, Gerard</p> <p>2015-04-01</p> <p>Situated in northwestern Europe, the North Sea region is under influence of air masses from subtropical to arctic origin, and thus exhibits significant natural climate <span class="hlt">variability</span>. As the land areas surrounding the North Sea are densely populated, climate change is an important issue in terms of e.g. coastal protection, fishery and trade. This study is part of the NOSCCA initiative (North Sea Region Climate Change Assessment) and presents <span class="hlt">observed</span> <span class="hlt">variability</span> and changes in atmospheric parameters during the last roughly 200 years. Circulation patterns show considerable <span class="hlt">decadal</span> <span class="hlt">variability</span>. In recent <span class="hlt">decades</span>, a northward shift of storm tracks and increased cyclonic activity has been <span class="hlt">observed</span>. There is also an indication of increased persistence of weather types. The wind climate is dominated by large multidecadal <span class="hlt">variability</span>, and no robust long-term trends can be identified in the available datasets. There is a clear positive trend in near-surface temperatures, in particular during spring and winter. Over the region as a whole, no clear long-term precipitation trends are visible, although regional indications exist for an increased risk of extreme precipitation events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53D2282M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53D2282M"><span><span class="hlt">Decadal</span> <span class="hlt">Variability</span> of Temperature and Salinity in the Northwest Atlantic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mishonov, A. V.; Seidov, D.; Reagan, J. R.; Boyer, T.; Parsons, A. R.</p> <p>2017-12-01</p> <p>There are only a few regions in the World Ocean where the density of <span class="hlt">observations</span> collected over the past 60 years is sufficient for reliable data mapping with spatial resolutions finer than one-degree. The Northwest Atlantic basin is one such regions where a spatial resolution of gridded temperature and salinity fields, comparable to those generated by eddy-resolving numerical models of ocean circulation, has recently becomes available. Using the new high-resolution Northwest Atlantic Regional Climatology, built on quarter-degree and one-tenth-degree resolution fields, we analyzed <span class="hlt">decadal</span> <span class="hlt">variability</span> and trends of temperature and salinity over 60 years in the Northwest Atlantic, and two 30-year ocean climates of 1955-1984 and 1985-2012 to evaluate the oceanic climate shift in this region. The 30-year climate shift is demonstrated using an innovative 3-D visualization of temperature and salinity. Spatial and temporal <span class="hlt">variability</span> of heat accumulation found in previous research of the entire North Atlantic Ocean persists in the Northwest Atlantic Ocean. Salinity changes between two 30-year climates were also computed and are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30..460M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30..460M"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> in the oxygen inventory of North Atlantic subtropical underwater captured by sustained, long-term oceanographic time series <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montes, Enrique; Muller-Karger, Frank E.; Cianca, Andrés.; Lomas, Michael W.; Lorenzoni, Laura; Habtes, Sennai</p> <p>2016-03-01</p> <p>Historical <span class="hlt">observations</span> of potential temperature (θ), salinity (S), and dissolved oxygen concentrations (O2) in the tropical and subtropical North Atlantic (0-500 m; 0-40°N, 10-90°W) were examined to understand <span class="hlt">decadal</span>-scale changes in O2 in subtropical underwater (STUW). STUW is <span class="hlt">observed</span> at four of the longest, sustained ocean biogeochemical and ecological time series stations, namely, the CArbon Retention In A Colored Ocean (CARIACO) Ocean Time Series Program (10.5°N, 64.7°W), the Bermuda Atlantic Time-series Study (BATS; 31.7°N, 64.2°W), Hydrostation "S" (32.1°N, 64.4°W), and the European Station for Time-series in the Ocean, Canary Islands (ESTOC; 29.2°N, 15.5°W). <span class="hlt">Observations</span> over similar time periods at CARIACO (1996-2013), BATS (1988-2011), and Hydrostation S (1980-2013) show that STUW O2 has decreased approximately 0.71, 0.28, and 0.37 µmol kg-1 yr-1, respectively. No apparent change in STUW O2 was <span class="hlt">observed</span> at ESTOC over the course of the time series (1994-2013). Ship <span class="hlt">observation</span> data for the tropical and subtropical North Atlantic archived at NOAA National Oceanographic Data Center show that between 1980 and 2013, STUW O2 (upper ~300 m) declined 0.58 µmol kg-1 yr-1 in the southeastern Caribbean Sea (10-15°N, 60-70°W) and 0.68 µmol kg-1 yr-1 in the western subtropical North Atlantic (30-35°N, 60-65°W). A declining O2 trend was not <span class="hlt">observed</span> in the eastern subtropical North Atlantic (25-30°N, 15-20°W) over the same period. Most of the <span class="hlt">observed</span> O2 loss seems to result from shifts in ventilation associated with decreased wind-driven mixing and a slowing down of STUW formation rates, rather than changes in diffusive air-sea O2 gas exchange or changes in the biological oceanography of the North Atlantic. <span class="hlt">Variability</span> of STUW O2 showed a significant relationship with the wintertime (January-March) Atlantic Multidecadal Oscillation index (AMO, R2 = 0.32). During negative wintertime AMO years trade winds are typically stronger between 10°N and 30</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110012422','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110012422"><span>CLARREO Cornerstone of the Earth <span class="hlt">Observing</span> System: Measuring <span class="hlt">Decadal</span> Change Through Accurate Emitted Infrared and Reflected Solar Spectra and Radio Occultation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sandford, Stephen P.</p> <p>2010-01-01</p> <p>The Climate Absolute Radiance and Refractivity Observatory (CLARREO) is one of four Tier 1 missions recommended by the recent NRC <span class="hlt">Decadal</span> Survey report on Earth Science and Applications from Space (NRC, 2007). The CLARREO mission addresses the need to provide accurate, broadly acknowledged climate records that are used to enable validated long-term climate projections that become the foundation for informed decisions on mitigation and adaptation policies that address the effects of climate change on society. The CLARREO mission accomplishes this critical objective through rigorous SI traceable <span class="hlt">decadal</span> change <span class="hlt">observations</span> that are sensitive to many of the key uncertainties in climate radiative forcings, responses, and feedbacks that in turn drive uncertainty in current climate model projections. These same uncertainties also lead to uncertainty in attribution of climate change to anthropogenic forcing. For the first time CLARREO will make highly accurate, global, SI-traceable <span class="hlt">decadal</span> change <span class="hlt">observations</span> sensitive to the most critical, but least understood, climate forcings, responses, and feedbacks. The CLARREO breakthrough is to achieve the required levels of accuracy and traceability to SI standards for a set of <span class="hlt">observations</span> sensitive to a wide range of key <span class="hlt">decadal</span> change <span class="hlt">variables</span>. The required accuracy levels are determined so that climate trend signals can be detected against a background of naturally occurring <span class="hlt">variability</span>. Climate system natural <span class="hlt">variability</span> therefore determines what level of accuracy is overkill, and what level is critical to obtain. In this sense, the CLARREO mission requirements are considered optimal from a science value perspective. The accuracy for <span class="hlt">decadal</span> change traceability to SI standards includes uncertainties associated with instrument calibration, satellite orbit sampling, and analysis methods. Unlike most space missions, the CLARREO requirements are driven not by the instantaneous accuracy of the measurements, but by accuracy in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1171388','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1171388"><span>Pacific <span class="hlt">Decadal</span> <span class="hlt">Variability</span> and Central Pacific Warming El Niño in a Changing Climate</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Di Lorenzo, Emanuele</p> <p></p> <p>This research aimed at understanding the dynamics controlling <span class="hlt">decadal</span> <span class="hlt">variability</span> in the Pacific Ocean and its interactions with global-scale climate change. The first goal was to assess how the dynamics and statistics of the El Niño Southern Oscillation and the modes of Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> are represented in global climate models used in the IPCC. The second goal was to quantify how <span class="hlt">decadal</span> dynamics are projected to change under continued greenhouse forcing, and determine their significance in the context of paleo-proxy reconstruction of long-term climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040075030&hterms=TOM&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DTOM','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040075030&hterms=TOM&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DTOM"><span>Evaluation of a Multi-<span class="hlt">Decadal</span> Simulation of Stratospheric Ozone by Comparison with Total Ozone Mapping Spectrometer (TOMS) <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Douglass, Anne R.; Stolarski, Richard S.; Steenrod, Steven; Pawson, Steven</p> <p>2003-01-01</p> <p>One key application of atmospheric chemistry and transport models is prediction of the response of ozone and other constituents to various natural and anthropogenic perturbations. These include changes in composition, such as the previous rise and recent decline in emission of man-made chlorofluorcarbons, changes in aerosol loading due to volcanic eruption, and changes in solar forcing. Comparisons of hindcast model results for the past few <span class="hlt">decades</span> with <span class="hlt">observations</span> are a key element of model evaluation and provide a sense of the reliability of model predictions. The 25 year data set from Total Ozone Mapping Spectrometers is a cornerstone of such model evaluation. Here we report evaluation of three-dimensional multi-<span class="hlt">decadal</span> simulation of stratospheric composition. Meteorological fields for this off-line calculation are taken from a 50 year simulation of a general circulation model. Model fields are compared with <span class="hlt">observations</span> from TOMS and also with <span class="hlt">observations</span> from the Stratospheric Aerosol and Gas Experiment (SAGE), Microwave Limb Sounder (MLS), Cryogenic Limb Array Etalon Spectrometer (CLAES), and the Halogen Occultation Experiment (HALOE). This overall evaluation will emphasize the spatial, seasonal, and interannual <span class="hlt">variability</span> of the simulation compared with <span class="hlt">observed</span> atmospheric <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H23G1311L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H23G1311L"><span>Drivers of annual to <span class="hlt">decadal</span> streamflow <span class="hlt">variability</span> in the lower Colorado River Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lambeth-Beagles, R. S.; Troch, P. A.</p> <p>2010-12-01</p> <p>The Colorado River is the main water supply to the southwest region. As demand reaches the limit of supply in the southwest it becomes increasingly important to understand the dynamics of streamflow in the Colorado River and in particular the tributaries to the lower Colorado River. Climate change may pose an additional threat to the already-scarce water supply in the southwest. Due to the narrowing margin for error, water managers are keen on extending their ability to predict streamflow volumes on a mid-range to <span class="hlt">decadal</span> scale. Before a predictive streamflow model can be developed, an understanding of the physical drivers of annual to <span class="hlt">decadal</span> streamflow <span class="hlt">variability</span> in the lower Colorado River Basin is needed. This research addresses this need by applying multiple statistical methods to identify trends, patterns and relationships present in streamflow, precipitation and temperature over the past century in four contributing watersheds to the lower Colorado River. The four watersheds selected were the Paria, Little Colorado, Virgin/Muddy, and Bill Williams. Time series data over a common period from 1906-2007 for streamflow, precipitation and temperature were used for the initial analysis. Through statistical analysis the following questions were addressed: 1) are there <span class="hlt">observable</span> trends and patterns in these <span class="hlt">variables</span> during the past century and 2) if there are trends or patterns, how are they related to each other? The Mann-Kendall test was used to identify trends in the three <span class="hlt">variables</span>. Assumptions regarding autocorrelation and persistence in the data were taken into consideration. Kendall’s tau-b test was used to establish association between any found trends in the data. Initial results suggest there are two primary processes occurring. First, statistical analysis reveals significant upward trends in temperatures and downward trends in streamflow. However, there appears to be no trend in precipitation data. These trends in streamflow and temperature speak to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PrOce.156...41M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PrOce.156...41M"><span>The impact of the ocean <span class="hlt">observing</span> system on estimates of the California current circulation spanning three <span class="hlt">decades</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, Andrew M.; Jacox, Michael G.; Crawford, William J.; Laughlin, Bruce; Edwards, Christopher A.; Fiechter, Jérôme</p> <p>2017-08-01</p> <p>Data assimilation is now used routinely in oceanography on both regional and global scales for computing ocean circulation estimates and for making ocean forecasts. Regional ocean <span class="hlt">observing</span> systems are also expanding rapidly, and <span class="hlt">observations</span> from a wide array of different platforms and sensor types are now available. Evaluation of the impact of the <span class="hlt">observing</span> system on ocean circulation estimates (and forecasts) is therefore of considerable interest to the oceanographic community. In this paper, we quantify the impact of different <span class="hlt">observing</span> platforms on estimates of the California Current System (CCS) spanning a three <span class="hlt">decade</span> period (1980-2010). Specifically, we focus attention on several dynamically related aspects of the circulation (coastal upwelling, the transport of the California Current and the California Undercurrent, thermocline depth and eddy kinetic energy) which in many ways describe defining characteristics of the CCS. The circulation estimates were computed using a 4-dimensional variational (4D-Var) data assimilation system, and our analyses also focus on the impact of the different elements of the control vector (i.e. the initial conditions, surface forcing, and open boundary conditions) on the circulation. While the influence of each component of the control vector varies between different metrics of the circulation, the impact of each <span class="hlt">observing</span> system across metrics is very robust. In addition, the mean amplitude of the circulation increments (i.e. the difference between the analysis and background) remains relatively stable throughout the three <span class="hlt">decade</span> period despite the addition of new <span class="hlt">observing</span> platforms whose impact is redistributed according to the relative uncertainty of <span class="hlt">observations</span> from each platform. We also consider the impact of each <span class="hlt">observing</span> platform on CCS circulation <span class="hlt">variability</span> associated with low-frequency climate <span class="hlt">variability</span>. The low-frequency nature of the dominant climate modes in this region allows us to track through time the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ERL....11l5008W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ERL....11l5008W"><span><span class="hlt">Variability</span> of fire emissions on interannual to multi-<span class="hlt">decadal</span> timescales in two Earth System models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ward, D. S.; Shevliakova, E.; Malyshev, S.; Lamarque, J.-F.; Wittenberg, A. T.</p> <p>2016-12-01</p> <p>Connections between wildfires and modes of <span class="hlt">variability</span> in climate are sought as a means for predicting fire activity on interannual to multi-<span class="hlt">decadal</span> timescales. Several fire drivers, such as temperature and local drought index, have been shown to vary on these timescales, and analysis of tree-ring data suggests covariance between fires and climate oscillation indices in some regions. However, the shortness of the satellite record of global fire events limits investigations on larger spatial scales. Here we explore the interplay between climate <span class="hlt">variability</span> and wildfire emissions with the preindustrial long control numerical experiments and historical ensembles of CESM1 and the NOAA/GFDL ESM2Mb. We find that interannual <span class="hlt">variability</span> in fires is underpredicted in both Earth System models (ESMs) compared to present day fire emission inventories. Modeled fire emissions respond to the El Niño/southern oscillation (ENSO) and Pacific <span class="hlt">decadal</span> oscillation (PDO) with increases in southeast Asia and boreal North America emissions, and decreases in southern North America and Sahel emissions, during the ENSO warm phase in both ESMs, and the PDO warm phase in CESM1. Additionally, CESM1 produces decreases in boreal northern hemisphere fire emissions for the warm phase of the Atlantic Meridional Oscillation. Through analysis of the long control simulations, we show that the 20th century trends in both ESMs are statistically significant, meaning that the signal of anthropogenic activity on fire emissions over this time period is detectable above the annual to <span class="hlt">decadal</span> timescale noise. However, the trends simulated by the two ESMs are of opposite sign (CESM1 decreasing, ESM2Mb increasing), highlighting the need for improved understanding, proxy <span class="hlt">observations</span>, and modeling to resolve this discrepancy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18..785J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18..785J"><span><span class="hlt">Decadal</span> trend of precipitation and temperature patterns and impacts on snow-related <span class="hlt">variables</span> in a semiarid region, Sierra Nevada, Spain.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>José Pérez-Palazón, María; Pimentel, Rafael; Herrero, Javier; José Polo, María</p> <p>2016-04-01</p> <p>, with the exception of the average annual mean and maximum daily temperature. In the case of the snow-related <span class="hlt">variables</span>, no significant trends are <span class="hlt">observed</span> at this time scale; nonetheless, a global decreasing rate is predominant in most of the <span class="hlt">variables</span>. The torrential events are more frequent in the last <span class="hlt">decades</span> of the study period, with an apparently increasing associated dispersion. This study constitutes a first sound analysis of the long-term <span class="hlt">observed</span> trends of the snow regime in this area under the context of increasing temperature and decreasing precipitation regimes. The results highlight the complexity of non-linearity in environmental processes in Mediterranean regions, and point out to a significant shift in the precipitation and temperature regime, and thus on the snow-affected hydrological <span class="hlt">variables</span> in the study area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMPP53A..08R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMPP53A..08R"><span>D/H Ratios From Sierra Nevada Varved Lake Sediments Record <span class="hlt">Decadal</span> Hydroclimate <span class="hlt">Variability</span> During The Medieval Period</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roach, L. D.; Cayan, D. R.; Sessions, A. L.; Charles, C. D.; Anderson, R. S.</p> <p>2009-12-01</p> <p> in the Swamp Lake watershed, depending on the extent to which these reservoirs are replenished seasonally by wintertime precipitation. Throughout the Medieval period, we <span class="hlt">observe</span> significant (>30‰), reproducible D/H <span class="hlt">variability</span> that also fluctuates on multi-year to <span class="hlt">decadal</span> time scales, with mean values falling within the same range as those recorded over the 20th century. Strong covariance among the aquatic and terrestrial plant fatty acids analyzed, along with the mean values, lends confidence that primary isotopic signatures have been retained. These results can therefore be compared directly to other measures of hydroclimate <span class="hlt">variability</span> throughout the last millennium, offering a unique new perspective on the mega-drought intervals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1393921','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1393921"><span><span class="hlt">Variability</span> of fire emissions on interannual to multi-<span class="hlt">decadal</span> timescales in two Earth System models</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Ward, D. S.; Shevliakova, E.; Malyshev, S.</p> <p></p> <p>Connections between wildfires and modes of <span class="hlt">variability</span> in climate are sought as a means for predicting fire activity on interannual to multi-<span class="hlt">decadal</span> timescales. Several fire drivers, such as temperature and local drought index, have been shown to vary on these timescales, and analysis of tree-ring data suggests covariance between fires and climate oscillation indices in some regions. HBut, the shortness of the satellite record of global fire events limits investigations on larger spatial scales. Here we explore the interplay between climate <span class="hlt">variability</span> and wildfire emissions with the preindustrial long control numerical experiments and historical ensembles of CESM1 and the NOAA/GFDLmore » ESM2Mb. We find that interannual <span class="hlt">variability</span> in fires is underpredicted in both Earth System models (ESMs) compared to present day fire emission inventories. Modeled fire emissions respond to the El Niño/southern oscillation (ENSO) and Pacific <span class="hlt">decadal</span> oscillation (PDO) with increases in southeast Asia and boreal North America emissions, and decreases in southern North America and Sahel emissions, during the ENSO warm phase in both ESMs, and the PDO warm phase in CESM1. In addition, CESM1 produces decreases in boreal northern hemisphere fire emissions for the warm phase of the Atlantic Meridional Oscillation. Through analysis of the long control simulations, we show that the 20th century trends in both ESMs are statistically significant, meaning that the signal of anthropogenic activity on fire emissions over this time period is detectable above the annual to <span class="hlt">decadal</span> timescale noise. However, the trends simulated by the two ESMs are of opposite sign (CESM1 decreasing, ESM2Mb increasing), highlighting the need for improved understanding, proxy <span class="hlt">observations</span>, and modeling to resolve this discrepancy.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1393921-variability-fire-emissions-interannual-multi-decadal-timescales-two-earth-system-models','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1393921-variability-fire-emissions-interannual-multi-decadal-timescales-two-earth-system-models"><span><span class="hlt">Variability</span> of fire emissions on interannual to multi-<span class="hlt">decadal</span> timescales in two Earth System models</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ward, D. S.; Shevliakova, E.; Malyshev, S.; ...</p> <p>2016-12-02</p> <p>Connections between wildfires and modes of <span class="hlt">variability</span> in climate are sought as a means for predicting fire activity on interannual to multi-<span class="hlt">decadal</span> timescales. Several fire drivers, such as temperature and local drought index, have been shown to vary on these timescales, and analysis of tree-ring data suggests covariance between fires and climate oscillation indices in some regions. HBut, the shortness of the satellite record of global fire events limits investigations on larger spatial scales. Here we explore the interplay between climate <span class="hlt">variability</span> and wildfire emissions with the preindustrial long control numerical experiments and historical ensembles of CESM1 and the NOAA/GFDLmore » ESM2Mb. We find that interannual <span class="hlt">variability</span> in fires is underpredicted in both Earth System models (ESMs) compared to present day fire emission inventories. Modeled fire emissions respond to the El Niño/southern oscillation (ENSO) and Pacific <span class="hlt">decadal</span> oscillation (PDO) with increases in southeast Asia and boreal North America emissions, and decreases in southern North America and Sahel emissions, during the ENSO warm phase in both ESMs, and the PDO warm phase in CESM1. In addition, CESM1 produces decreases in boreal northern hemisphere fire emissions for the warm phase of the Atlantic Meridional Oscillation. Through analysis of the long control simulations, we show that the 20th century trends in both ESMs are statistically significant, meaning that the signal of anthropogenic activity on fire emissions over this time period is detectable above the annual to <span class="hlt">decadal</span> timescale noise. However, the trends simulated by the two ESMs are of opposite sign (CESM1 decreasing, ESM2Mb increasing), highlighting the need for improved understanding, proxy <span class="hlt">observations</span>, and modeling to resolve this discrepancy.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613612K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613612K"><span>Multi-<span class="hlt">decadal</span> <span class="hlt">Variability</span> of the Wind Power Output</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kirchner Bossi, Nicolas; García-Herrera, Ricardo; Prieto, Luis; Trigo, Ricardo M.</p> <p>2014-05-01</p> <p>The knowledge of the long-term wind power <span class="hlt">variability</span> is essential to provide a realistic outlook on the power output during the lifetime of a planned wind power project. In this work, the Power Output (Po) of a market wind turbine is simulated with a daily resolution for the period 1871-2009 at two different locations in Spain, one at the Central Iberian Plateau and another at the Gibraltar Strait Area. This is attained through a statistical downscaling of the daily wind conditions. It implements a Greedy Algorithm as classificator of a geostrophic-based wind predictor, which is derived by considering the SLP daily field from the 56 ensemble members of the longest homogeneous reanalysis available (20CR, 1871-2009). For calibration and validation purposes we use 10 years of wind <span class="hlt">observations</span> (the predictand) at both sites. As a result, a series of 139 annual wind speed Probability Density Functions (PDF) are obtained, with a good performance in terms of wind speed uncertainty reduction (average daily wind speed MAE=1.48 m/s). The obtained centennial series allow to investigate the multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of wind power from different points of view. Significant periodicities around the 25-yr frequency band, as well as long-term linear trends are detected at both locations. In addition, a negative correlation is found between annual Po at both locations, evidencing the differences in the dynamical mechanisms ruling them (and possible complementary behavior). Furthermore, the impact that the three leading large-scale circulation patterns over Iberia (NAO, EA and SCAND) exert over wind power output is evaluated. Results show distinct (and non-stationary) couplings to these forcings depending on the geographical position and season or month. Moreover, significant non-stationary correlations are <span class="hlt">observed</span> with the slow varying Atlantic Multidecadal Oscillation (AMO) index for both case studies. Finally, an empirical relationship is explored between the annual Po and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.H13I1695T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.H13I1695T"><span>Stochastically-forced <span class="hlt">Decadal</span> <span class="hlt">Variability</span> in Australian Rainfall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taschetto, A.</p> <p>2015-12-01</p> <p>Iconic Australian dry and wet periods were driven by anomalous conditions in the tropical oceans, such as the worst short-term drought in the southeast in 1982 associated with the strong El Niño and the widespread "Big Wet" in 1974 linked with a La Niña event. The association with oceanic conditions makes droughts predictable to some extent. However, prediction can be difficult when there is no clear external forcing such as El Niños. Can dry spells be triggered and maintained with no ocean memory? In this study, we investigate the potential role of internal multi-century atmospheric <span class="hlt">variability</span> in controlling the frequency, duration and intensity of long-term dry and wet spells over Australia. Two multi-century-scale simulations were performed with the NCAR CESM: (1) a fully-coupled simulation (CPLD) and (2) an atmospheric simulation forced by a seasonal SST climatology derived from the coupled experiment (ACGM). Results reveal that droughts and wet spells can indeed be generated by internal <span class="hlt">variability</span> of the atmosphere. Those internally generated events are less severe than those forced by oceanic <span class="hlt">variability</span>, however the duration of dry and wet spells longer than 3 years is comparable with and without the ocean memory. Large-scale ocean modes of <span class="hlt">variability</span> seem to play an important role in producing continental-scale rainfall impacts over Australia. While the Pacific <span class="hlt">Decadal</span> Oscillation plays an important role in generating droughts in the fully coupled model, perturbations of monsoonal winds seem to be the main trigger of dry spells in the AGCM case. Droughts in the mid-latitude regions such as Tasmania can be driven by perturbations in the Southern Annular Mode, not necessarily linked to oceanic conditions even in the fully-coupled model. The mechanisms behind internally-driven mega-droughts and mega-wets will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMGC23C..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMGC23C..03F"><span>Holocene Multi-<span class="hlt">Decadal</span> to Millennial-Scale Hydrologic <span class="hlt">Variability</span> on the South American Altiplano</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fritz, S. C.; Baker, P. A.; Ekdahl, E.; Burns, S.</p> <p>2006-12-01</p> <p>On orbital timescales, lacustrine sediment records in the tropical central Andes show massive changes in lake level due to mechanisms related to global-scale drivers, varying at precessional timescales. Here we use stable isotopic and diatom records from two lakes in the Lake Titicaca drainage basin to reconstruct multi- <span class="hlt">decadal</span> to millennial scale precipitation <span class="hlt">variability</span> during the last 7000 to 8000 years. The records are tightly coupled at multi-<span class="hlt">decadal</span> to millennial scales with each other and with lake-level fluctuations in Lake Titicaca, indicating that the lakes are recording a regional climate signal. A quantitative reconstruction of precipitation from stable isotopic data indicates that the central Andes underwent significant wet to dry alternations at multi- centennial frequencies with an amplitude of 30 to 40% of total precipitation. A strong millennial-scale component, similar in duration to periods of increased ice rafted debris flux in the North Atlantic, is <span class="hlt">observed</span> in both lake records, suggesting that tropical North Atlantic sea-surface temperature (SST) <span class="hlt">variability</span> may partly control regional precipitation. No clear relationship is evident between these records and the inferred ENSO history from Lago Pallcacocha in the northern tropical Andes. In the instrumental period, regional precipitation <span class="hlt">variability</span> on inter-annual timescales is clearly influenced by Pacific modes; for example, most El Ninos produce dry and warm conditions in this part of the central Andes. However, on longer timescales, the control of tropical Pacific modes is less clear. Our reconstructions suggest that the cold intervals of the Holocene Bond events are periods of increased precipitation in the central Andes, thus indicating an anti-phasing of precipitation variation in the southern tropics of South America relative to the Northern Hemisphere monsoon region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150022507','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150022507"><span>Global Ocean Evaporation: How Well Can We Estimate Interannual to <span class="hlt">Decadal</span> <span class="hlt">Variability</span>?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robertson, Franklin R.; Bosilovich, Michael G.; Roberts, Jason B.; Wang, Hailan</p> <p>2015-01-01</p> <p>Evaporation from the world's oceans constitutes the largest component of the global water balance. It is important not only as the ultimate source of moisture that is tied to the radiative processes determining Earth's energy balance but also to freshwater availability over land, governing habitability of the planet. Here we focus on <span class="hlt">variability</span> of ocean evaporation on scales from interannual to <span class="hlt">decadal</span> by appealing to three sources of data: the new MERRA-2 (Modern-Era Retrospective analysis for Research and Applications -2); climate models run with historical sea-surface temperatures, ice and atmospheric constituents (so-called AMIP experiments); and state-of-the-art satellite retrievals from the Seaflux and HOAPS (Hamburg Ocean-Atmosphere Parameters and Fluxes from Satellite) projects. Each of these sources has distinct advantages as well as drawbacks. MERRA-2, like other reanalyses, synthesizes evaporation estimates consistent with <span class="hlt">observationally</span> constrained physical and dynamical models-but data stream discontinuities are a major problem for interpreting multi-<span class="hlt">decadal</span> records. The climate models used in data assimilation can also be run with lesser constraints such as with SSTs and sea-ice (i.e. AMIPs) or with additional, minimal <span class="hlt">observations</span> of surface pressure and marine <span class="hlt">observations</span> that have longer and less fragmentary <span class="hlt">observational</span> records. We use the new ERA-20C reanalysis produced by ECMWF embodying the latter methodology. Still, the model physics biases in climate models and the lack of a predicted surface energy balance are of concern. Satellite retrievals and comparisons to ship-based measurements offer the most <span class="hlt">observationally</span>-based estimates, but sensor inter-calibration, algorithm retrieval assumptions, and short records are dominant issues. Our strategy depends on maximizing the advantages of these combined records. The primary diagnostic tool used here is an analysis of bulk aerodynamic computations produced by these sources and uses a first</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080045519','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080045519"><span>The Spatiotemporal Structure of 20th Century Climate Variations in <span class="hlt">Observations</span> and Reanalyses. Part 2; Pacific Pan-<span class="hlt">Decadal</span> <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chen, Junye; DelGenio, Anthony D.; Carlson, Barbara E.; Bosilovich, Michael G.</p> <p>2007-01-01</p> <p>The dominant interannual El Nino-Southern Oscillation phenomenon (ENSO) and the short length of climate <span class="hlt">observation</span> records make it difficult to study long-term climate variations in the spatiotemporal domain. Based on the fact that the ENS0 signal spreads to remote regions and induces delayed climate variation through atmospheric teleconnections, we develop an ENSO-removal method through which the ENS0 signal can be approximately removed at the grid box level from the spatiotemporal field of a climate parameter. After this signal is removed, long-term climate variations, namely, the global warming trend (GW) and the Pacific pan-<span class="hlt">decadal</span> <span class="hlt">variability</span> (PDV), are isolated at middle and low latitudes in the climate parameter fields from <span class="hlt">observed</span> and reanalyses datasets. In this study, we show that one of several PDV interdecadal regime shifts occurred during the 1990s. This significant change in the Pacific basin is comparable but opposite in phase to the 1976 climate regime shift, which results persisting warming in the central-eastern Pacific, and cooling in the North and South Pacific. The 1990s PDV regime shift is consistent with <span class="hlt">observed</span> changes in ocean biosphere and ocean circulation. A comprehensive picture of PDV as manifested in the troposphere and at the surface is described. In general, the PDV spatial patterns in different parameter fields share some similarities with the patterns associated with ENSO, but important differences exist. First, the PDV atmospheric circulation pattern is shifted westward by about 20deg and its zonal extent is limited to approx.60deg compared to approx.110deg for ENS0 pattern. The westward shift of the PDV wave train produces a different, more west-east oriented, North American teleconnection pattern. The lack of a strong PDV surface temperature (ST) signal in the western equatorial Pacific and the relatively strong ST signal in the subtropical regions are consistent with an atmospheric overturning circulation response that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70000159','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70000159"><span>Associations of multi-<span class="hlt">decadal</span> sea-surface temperature <span class="hlt">variability</span> with US drought</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McCabe, G.J.; Betancourt, J.L.; Gray, S.T.; Palecki, M.A.; Hidalgo, H.G.</p> <p>2008-01-01</p> <p>Recent research suggests a link between drought occurrence in the conterminous United States (US) and sea surface temperature (SST) <span class="hlt">variability</span> in both the tropical Pacific and North Atlantic Oceans on <span class="hlt">decadal</span> to multidecadal (D2M) time scales. Results show that the Atlantic Multidecadal Oscillation (AMO) is the most consistent indicator of D2M drought <span class="hlt">variability</span> in the conterminous US during the 20th century, but during the 19th century the tropical Pacific is a more consistent indicator of D2 M drought. The interaction between El Nin??o-Southern Oscillation (ENSO) and the AMO explain a large part of the D2M drought <span class="hlt">variability</span> in the conterminous US. More modeling studies are needed to reveal possible mechanisms linking low-frequency ENSO <span class="hlt">variability</span> and the AMO with drought in the conterminous US. ?? 2007 Elsevier Ltd and INQUA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1821V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1821V"><span>Missing pieces of the puzzle: understanding <span class="hlt">decadal</span> <span class="hlt">variability</span> of Sahel Rainfall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vellinga, Michael; Roberts, Malcolm; Vidale, Pier-Luigi; Mizielinski, Matthew; Demory, Marie-Estelle; Schiemann, Reinhard; Strachan, Jane; Bain, Caroline</p> <p>2015-04-01</p> <p>The instrumental record shows that substantial <span class="hlt">decadal</span> fluctuations affected Sahel rainfall from the West African monsoon throughout the 20th century. Climate models generally underestimate the magnitude of <span class="hlt">decadal</span> Sahel rainfall changes compared to <span class="hlt">observations</span>. This shows that the processes that control low-frequency Sahel rainfall change are misrepresented in most CMIP5-era climate models. Reliable climate information of future low-frequency rainfall changes thus remains elusive. Here we identify key processes that control the magnitude of the <span class="hlt">decadal</span> rainfall recovery in the Sahel since the mid-1980s. We show its sensitivity to model resolution and physics in a suite of experiments with global HadGEM3 model configurations at resolutions between 130-25 km. The <span class="hlt">decadal</span> rainfall trend increases with resolution and at 60-25 km falls within the <span class="hlt">observed</span> range. Higher resolution models have stronger increases of moisture supply and of African Easterly wave activity. Easterly waves control the occurrence of strong organised rainfall events which carry most of the <span class="hlt">decadal</span> trend. Weak rainfall events occur too frequently at all resolutions and at low resolution contribute substantially to the <span class="hlt">decadal</span> trend. All of this behaviour is seen across CMIP5, including future scenarios. Additional simulations with a global 12km version of HadGEM3 show that treating convection explicitly dramatically improves the properties of Sahel rainfall systems. We conclude that interaction between convective scale and global scale processes is key to <span class="hlt">decadal</span> rainfall changes in the Sahel. This work is distributed under the Creative Commons Attribution 3.0 Unported License together with an author copyright. This license does not conflict with the regulations of the Crown Copyright.Crown Copyright</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.1379A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.1379A"><span>North Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span>: insights from a biennial ENSO environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Achuthavarier, Deepthi; Schubert, Siegfried D.; Vikhliaev, Yury V.</p> <p>2017-08-01</p> <p>This study examines the mechanisms of the Pacific <span class="hlt">decadal</span> oscillation (PDO) in the NASA GEOS-5 general circulation model (GCM). Similar to several other state-of-the-art GCMs, the El Niño-Southern Oscillation (ENSO) simulated by the GEOS-5 has a strong biennial periodicity. Since this is a model bias that precludes a strong role of ENSO, it provides a unique environment to assess the other leading mechanisms of North Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span>. Despite the biennial ENSO periodicity, the model simulates a realistic PDO pattern in the North Pacific that is resolved as the first empirical orthogonal function (EOF) of winter mean sea surface temperature (SST). The spectrum of the PDO indicates no preferred periodicity. The SST anomalies associated with the PDO, particularly its basin wide structure, are primarily forced by the Aleutian low through Ekman transport. The slow geostrophic transport in association with the meridional adjustment of the subtropical gyre is limited to a narrow region in the Kuroshio-Oyashio extension, north of 40°N. The atmosphere's response to the PDO, while weak, projects onto the North Pacific Oscillation (NPO), a meridional dipole in sea level pressure. Both the lack of preferred periodicity and the weak atmospheric response indicate an air-sea coupled oscillation is an unlikely mechanism in this model. In agreement with recent studies, the NPO is correlated with the North Pacific Gyre Oscillation, which is another leading EOF of North Pacific SST <span class="hlt">variability</span>. The results emphasize the role of atmospheric <span class="hlt">variability</span> in the North Pacific SST modes, thereby bringing into question the potential for their predictability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160013299&hterms=insight&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinsight','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160013299&hterms=insight&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinsight"><span>North Pacific <span class="hlt">Decadal</span> <span class="hlt">Variability</span>: Insights from a Biennial ENSO Environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Achuthavarier, Deepthi; Schubert, Siegfried D.; Vikhliaev, Yury V.</p> <p>2016-01-01</p> <p>This study examines the mechanisms of the Pacific <span class="hlt">decadal</span> oscillation (PDO) in the NASA GEOS-5 general circulation model (GCM). Similar to several other state-of-the-art GCMs, the El Niño-Southern Oscillation (ENSO) simulated by the GEOS-5 has a strong biennial periodicity. Since this is a model bias that precludes a strong role of ENSO, it provides a unique environment to assess the other leading mechanisms of North Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span>. Despite the biennial ENSO periodicity, the model simulates a realistic PDO pattern in the North Pacific that is resolved as the first empirical orthogonal function (EOF) of winter mean sea surface temperature (SST). The spectrum of the PDO indicates no preferred periodicity. The SST anomalies associated with the PDO, particularly its basin wide structure, are primarily forced by the Aleutian low through Ekman transport. The slow geostrophic transport in association with the meridional adjustment of the subtropical gyre is limited to a narrow region in the Kuroshio-Oyashio extension, north of 40degN. The atmosphere's response to the PDO, while weak, projects onto the North Pacific Oscillation (NPO), a meridional dipole in sea level pressure. Both the lack of preferred periodicity and the weak atmospheric response indicate an air-sea coupled oscillation is an unlikely mechanism in this model. In agreement with recent studies, the NPO is correlated with the North Pacific Gyre Oscillation, which is another leading EOF of North Pacific SST <span class="hlt">variability</span>. The results emphasize the role of atmospheric <span class="hlt">variability</span> in the North Pacific SST modes, thereby bringing into question the potential for their predictability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT........34K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT........34K"><span>Influence of <span class="hlt">Decadal</span> <span class="hlt">Variability</span> of Global Oceans on South Asian Monsoon and ENSO-Monsoon Relation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krishnamurthy, Lakshmi</p> <p></p> <p>This study has investigated the influence of the <span class="hlt">decadal</span> <span class="hlt">variability</span> associated with global oceans on South Asian monsoon and El Nino-Southern Oscillation (ENSO)-monsoon relation. The results are based on <span class="hlt">observational</span> analysis using long records of monsoon rainfall and circulation and coupled general circulation model experiments using the National Center for Atmospheric Research (NCAR) Community Climate System Model (CCSM) version 4 model. The multi-channel singular spectrum analysis (MSSA) of the <span class="hlt">observed</span> rainfall over India yields three <span class="hlt">decadal</span> modes. The first mode (52 year period) is associated with the Atlantic Multidecadal Oscillation (AMO), the second one (21 year) with the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) and the third mode (13 year) with the Atlantic tripole. The existence of these <span class="hlt">decadal</span> modes in the monsoon was also found in the control simulation of NCAR CCSM4. The regionally de-coupled model experiments performed to isolate the influence of North Pacific and North Atlantic also substantiate the above results. The relation between the <span class="hlt">decadal</span> modes in the monsoon rainfall with the known <span class="hlt">decadal</span> modes in global SST is examined. The PDO has significant negative correlation with the Indian Monsoon Rainfall (IMR). The mechanism for PDO-monsoon relation is hypothesized through the seasonal footprinting mechanism and further through Walker and Hadley circulations. The model results also confirm the negative correlation between PDO and IMR and the mechanism through which PDO influences monsoon. Both <span class="hlt">observational</span> and model analysis show that droughts (floods) are more likely over India than floods (droughts) when ENSO and PDO are in their warm (cold) phase. This study emphasizes the importance of carefully distinguishing the different <span class="hlt">decadal</span> modes in the SST in the North Atlantic Ocean as they have different impacts on the monsoon. The AMO exhibits significant positive correlation with the IMR while the Atlantic tripole has significant negative</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950047289&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtemperature%2Bvariability','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950047289&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtemperature%2Bvariability"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of the Tropical Atlantic Ocean Surface Temperature in shipboard measurements and in a Global Ocean-Atmosphere model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mehta, Vikram M.; Delworth, Thomas</p> <p>1995-01-01</p> <p>Sea surface temperature (SST) <span class="hlt">variability</span> was investigated in a 200-yr integration of a global model of the coupled oceanic and atmospheric general circulations developed at the Geophysical Fluid Dynamics Laboratory (GFDL). The second 100 yr of SST in the coupled model's tropical Atlantic region were analyzed with a variety of techniques. Analyses of SST time series, averaged over approximately the same subregions as the Global Ocean Surface Temperature Atlas (GOSTA) time series, showed that the GFDL SST anomalies also undergo pronounced quasi-oscillatory <span class="hlt">decadal</span> and multidecadal <span class="hlt">variability</span> but at somewhat shorter timescales than the GOSTA SST anomalies. Further analyses of the horizontal structures of the <span class="hlt">decadal</span> timescale <span class="hlt">variability</span> in the GFDL coupled model showed the existence of two types of <span class="hlt">variability</span> in general agreement with results of the GOSTA SST time series analyses. One type, characterized by timescales between 8 and 11 yr, has high spatial coherence within each hemisphere but not between the two hemispheres of the tropical Atlantic. A second type, characterized by timescales between 12 and 20 yr, has high spatial coherence between the two hemispheres. The second type of <span class="hlt">variability</span> is considerably weaker than the first. As in the GOSTA time series, the multidecadal <span class="hlt">variability</span> in the GFDL SST time series has approximately opposite phases between the tropical North and South Atlantic Oceans. Empirical orthogonal function analyses of the tropical Atlantic SST anomalies revealed a north-south bipolar pattern as the dominant pattern of <span class="hlt">decadal</span> <span class="hlt">variability</span>. It is suggested that the bipolar pattern can be interpreted as <span class="hlt">decadal</span> <span class="hlt">variability</span> of the interhemispheric gradient of SST anomalies. The <span class="hlt">decadal</span> and multidecadal timescale <span class="hlt">variability</span> of the tropical Atlantic SST, both in the actual and in the GFDL model, stands out significantly above the background 'red noise' and is coherent within each of the time series, suggesting that specific sets of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...143..278M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...143..278M"><span><span class="hlt">Decadal</span> sea level <span class="hlt">variability</span> in the East China Sea linked to the North Pacific Gyre Oscillation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moon, Jae-Hong; Song, Y. Tony</p> <p>2017-07-01</p> <p>In view of coastal community's need for adapting to sea level rise (SLR), understanding and predicting regional <span class="hlt">variability</span> on <span class="hlt">decadal</span> to longer time scales still remain a challenging issue in SLR research. Here, we have examined the low-frequency sea level signals in the East China Sea (ECS) from the 50-year hindcast of a non-Boussinesq ocean model in comparison with data sets from altimeters, tide-gauges, and steric sea level produced by in-situ profiles. It is shown that the mean sea levels in the ECS represent significant <span class="hlt">decadal</span> fluctuations over the past 50 years, with a multi-<span class="hlt">decadal</span> trend shift since the mid-1980s compared to the preceding 30 years. The <span class="hlt">decadal</span> fluctuations in sea level are more closely linked to the North Pacific Gyre Oscillation (NPGO) rather than the Pacific <span class="hlt">Decadal</span> Oscillation, which reflects the multi-<span class="hlt">decadal</span> trend shift. A composite analysis indicates that wind patterns associated with the NPGO is shown to control the <span class="hlt">decadal</span> <span class="hlt">variability</span> of the western subtropical North Pacific. A positive NPGO corresponds to cyclonic wind stress curl anomaly in the western subtropical regions that results in a higher sea level in the ECS, particularly along the continental shelf, and lower sea levels off the ECS. The reverse occurs in years of negative NPGO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130000599','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130000599"><span>Temporal <span class="hlt">Variability</span> of <span class="hlt">Observed</span> and Simulated Hyperspectral Earth Reflectance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roberts, Yolanda; Pilewskie, Peter; Kindel, Bruce; Feldman, Daniel; Collins, William D.</p> <p>2012-01-01</p> <p> series analysis of the PC scores using techniques such as Singular Spectrum Analysis (SSA) and Multichannel SSA will provide information about the temporal <span class="hlt">variability</span> of the dominant <span class="hlt">variables</span>. Quantitative comparison techniques can evaluate how well the OSSE reproduces the temporal <span class="hlt">variability</span> <span class="hlt">observed</span> by SCIAMACHY spectral reflectance measurements during the first <span class="hlt">decade</span> of the 21st century. PCA of OSSE-simulated reflectance can also be used to study how the dominant spectral <span class="hlt">variables</span> change on centennial scales for forced and unforced climate change scenarios. To have confidence in OSSE predictions of the spectral <span class="hlt">variability</span> of hyperspectral reflectance, it is first necessary for us to evaluate the degree to which the OSSE simulations are able to reproduce the Earth?s present-day spectral <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy..tmp..897G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy..tmp..897G"><span>The impacts of oceanic deep temperature perturbations in the North Atlantic on <span class="hlt">decadal</span> climate <span class="hlt">variability</span> and predictability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Germe, Agathe; Sévellec, Florian; Mignot, Juliette; Fedorov, Alexey; Nguyen, Sébastien; Swingedouw, Didier</p> <p>2017-12-01</p> <p><span class="hlt">Decadal</span> climate predictability in the North Atlantic is largely related to ocean low frequency <span class="hlt">variability</span>, whose sensitivity to initial conditions is not very well understood. Recently, three-dimensional oceanic temperature anomalies optimally perturbing the North Atlantic Mean Temperature (NAMT) have been computed via an optimization procedure using a linear adjoint to a realistic ocean general circulation model. The spatial pattern of the identified perturbations, localized in the North Atlantic, has the largest magnitude between 1000 and 4000 m depth. In the present study, the impacts of these perturbations on NAMT, on the Atlantic meridional overturning circulation (AMOC), and on climate in general are investigated in a global coupled model that uses the same ocean model as was used to compute the three-dimensional optimal perturbations. In the coupled model, these perturbations induce AMOC and NAMT anomalies peaking after 5 and 10 years, respectively, generally consistent with the ocean-only linear predictions. To further understand their impact, their magnitude was varied in a broad range. For initial perturbations with a magnitude comparable to the internal <span class="hlt">variability</span> of the coupled model, the model response exhibits a strong signature in sea surface temperature and precipitation over North America and the Sahel region. The existence and impacts of these ocean perturbations have important implications for <span class="hlt">decadal</span> prediction: they can be seen either as a source of predictability or uncertainty, depending on whether the current <span class="hlt">observing</span> system can detect them or not. In fact, comparing the magnitude of the imposed perturbations with the uncertainty of available ocean <span class="hlt">observations</span> such as Argo data or ocean state estimates suggests that only the largest perturbations used in this study could be detectable. This highlights the importance for <span class="hlt">decadal</span> climate prediction of accurate ocean density initialisation in the North Atlantic at intermediate and greater</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1415029','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1415029"><span>Collaborative Research: Improving <span class="hlt">Decadal</span> Prediction of Arctic Climate <span class="hlt">Variability</span> and Change Using a Regional Arctic</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gutowski, William J.</p> <p></p> <p>This project developed and applied a regional Arctic System model for enhanced <span class="hlt">decadal</span> predictions. It built on successful research by four of the current PIs with support from the DOE Climate Change Prediction Program, which has resulted in the development of a fully coupled Regional Arctic Climate Model (RACM) consisting of atmosphere, land-hydrology, ocean and sea ice components. An expanded RACM, a Regional Arctic System Model (RASM), has been set up to include ice sheets, ice caps, mountain glaciers, and dynamic vegetation to allow investigation of coupled physical processes responsible for <span class="hlt">decadal</span>-scale climate change and <span class="hlt">variability</span> in the Arctic. RASMmore » can have high spatial resolution (~4-20 times higher than currently practical in global models) to advance modeling of critical processes and determine the need for their explicit representation in Global Earth System Models (GESMs). The pan-Arctic region is a key indicator of the state of global climate through polar amplification. However, a system-level understanding of critical arctic processes and feedbacks needs further development. Rapid climate change has occurred in a number of Arctic System components during the past few <span class="hlt">decades</span>, including retreat of the perennial sea ice cover, increased surface melting of the Greenland ice sheet, acceleration and thinning of outlet glaciers, reduced snow cover, thawing permafrost, and shifts in vegetation. Such changes could have significant ramifications for global sea level, the ocean thermohaline circulation and heat budget, ecosystems, native communities, natural resource exploration, and commercial transportation. The overarching goal of the RASM project has been to advance understanding of past and present states of arctic climate and to improve seasonal to <span class="hlt">decadal</span> predictions. To do this the project has focused on <span class="hlt">variability</span> and long-term change of energy and freshwater flows through the arctic climate system. The three foci of this research are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1986JAVSO..15..148M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1986JAVSO..15..148M"><span><span class="hlt">Variable</span> Star <span class="hlt">Observing</span> in Hungary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mizser, Attila</p> <p>1986-12-01</p> <p>Astronomy and <span class="hlt">variable</span> star <span class="hlt">observing</span> has a long history in Hungary, dating back to the private observatories erected by the Hungarian nobility in the late 19th Century. The first organized network of amateur <span class="hlt">variable</span> star <span class="hlt">observers</span>, the <span class="hlt">Variable</span> Star Section of the new Hungarian Astronomical Association, was organized around the Urania Observatory in Budapest in 1948. Other groups, dedicated to various types of <span class="hlt">variables</span>, have since been organized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ERL....13b4016F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ERL....13b4016F"><span>Synchronous multi-<span class="hlt">decadal</span> climate <span class="hlt">variability</span> of the whole Pacific areas revealed in tree rings since 1567</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fang, Keyan; Cook, Edward; Guo, Zhengtang; Chen, Deliang; Ou, Tinghai; Zhao, Yan</p> <p>2018-02-01</p> <p>Oceanic and atmospheric patterns play a crucial role in modulating climate <span class="hlt">variability</span> from interannual to multi-<span class="hlt">decadal</span> timescales by causing large-scale co-varying climate changes. The brevity of the existing instrumental records hinders the ability to recognize climate patterns before the industrial era, which can be alleviated using proxies. Unfortunately, proxy based reconstructions of oceanic and atmospheric modes of the past millennia often have modest agreements with each other before the instrumental period, raising questions about the robustness of the reconstructions. To ensure the stability of climate signals in proxy data through time, we first identified tree-ring datasets from distant regions containing coherent variations in Asia and North America, and then interpreted their climate information. We found that the multi-<span class="hlt">decadal</span> covarying climate patterns of the middle and high latitudinal regions around the northern Pacific Ocean agreed quite well with the climate reconstructions of the tropical and southern Pacific areas. This indicates a synchronous <span class="hlt">variability</span> at the multi-<span class="hlt">decadal</span> timescale of the past 430 years for the entire Pacific Ocean. This pattern is closely linked to the dominant mode of the Pacific sea surface temperature (SST) after removing the warming trend. This Pacific multi-<span class="hlt">decadal</span> SST <span class="hlt">variability</span> resembles the Interdecadal Pacific Oscillation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9994K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9994K"><span>New <span class="hlt">Observations</span> of the Martian Ionosphere and its <span class="hlt">Variability</span> - An Overview</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kopf, Andrew J.</p> <p>2017-04-01</p> <p>The Martian ionosphere is a highly <span class="hlt">variable</span> system, owed to the strong influence of the Sun on its properties and behavior, particularly at higher altitudes. Recent measurements from the MAVEN and Mars Express spacecraft have allowed for a more complete understanding of the ionosphere and its <span class="hlt">variability</span> from two different perspectives. Due to the low-altitude periapsis of its orbit, MAVEN has allowed for the first in-situ ionospheric studies since Viking, yielding detailed direct measurements of the ionosphere's structure, composition, and dynamics, as well as its rate of loss to space. Mars Express has over a <span class="hlt">decade</span> of continuous ionospheric <span class="hlt">observation</span> of the red planet, with the unique ability to remotely sound the ionosphere. These features enable Mars Express to make long-period ionospheric measurements on each orbit, at all local times and solar zenith angles. Utilized together, these two spacecraft form a powerful <span class="hlt">observational</span> suite that has provided new insights into this dynamic environment. This talk will highlight several important recent results in the study of the Martian ionosphere and its <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP54B..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP54B..02B"><span>Multi-Proxy Reconstructions of Northeast Pacific <span class="hlt">Decadal</span> <span class="hlt">Variability</span> from Bivalve Mollusks and Trees</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Black, B.; Griffin, D.</p> <p>2017-12-01</p> <p><span class="hlt">Decadal</span>-scale climate <span class="hlt">variability</span> in the Northeast Pacific Ocean profoundly influences fisheries production, forest growth, wildfire, drought, and snowpack in western North America. However, there remains considerable and long-standing uncertainly in its behavior prior to AD 1900 and the extent to which 20th century dynamics are atypical in a multi-centennial context. Here, we target the leading EOF of SST in the northeastern Pacific (ARCSST) as an index of Pacific <span class="hlt">Decadal</span> <span class="hlt">Variability</span>, which has been dynamically linked to sea level pressure and unlike the Pacific <span class="hlt">Decadal</span> Oscillation Index, retains a linear warming trend. The ARCSST reconstruction is generated from a broad network of target-sensitive North American tree-ring data standardized using signal-free detrending to preserve lower frequency signals common to the original data. In a preliminary analysis, the mean of the approximately 50 chronologies that significantly (p < 0.01) correlate to the target <span class="hlt">variable</span> explain 60% of the variance in cool-season ARCSST. Reconstruction skill is independently verified by three marine bivalve (Pacific geoduck; Panopea generosa) chronologies, the mean of which accounts for over 50% of the reconstruction variance over the common 1870-1900 interval. The nested reconstruction spans over 500 years and indicates that i) PDV is dominated by pentadecadal cycles, ii) century-long quiescent periods can occur, iii) 20th century regime shifts are typical, but iv) late 20th century warming is atypical in the longer-term context. Moreover, the reconstruction closely tracks paleofisheries datasets, particularly northern anchovy (Engraulis mordax) abundance inferred from scale deposition rates in the Santa Barbara Basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..12210560N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..12210560N"><span>Exploring the Links in Monthly to <span class="hlt">Decadal</span> <span class="hlt">Variability</span> of the Atmospheric Water Balance Over the Wettest Regions in ERA-20C</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nogueira, M.</p> <p>2017-10-01</p> <p>Monthly-to-<span class="hlt">decadal</span> <span class="hlt">variability</span> of the regional precipitation over Intertropical Convergence Zone and north-Atlantic and north-Pacific storm tracks was investigated using ERA-20C reanalysis. Satellite-based precipitation (<fi>P</fi>) and evaporation (<fi>E</fi>) climatological patterns were well reproduced by ERA-20C. Regional <fi>P</fi> and <fi>E</fi> monthly time series displayed 20% differences, but these decreased rapidly with time scale ( 10% at yearly time scales). Spectral analysis showed good scale-by-scale statistical agreement between ERA-20C and <span class="hlt">observations</span>. Using ERA-Interim showed no improvement despite the much wider range of information assimilated (including satellites). Remarkably high Detrended Cross-Correlation Analysis coefficients (<fi>ρ</fi>DCCA > 0.7 and often <fi>ρ</fi>DCCA > 0.9) revealed tight links between the nonperiodic <span class="hlt">variability</span> of <fi>P</fi>, moisture divergence (DIV), and pressure velocity (<fi>ω</fi>) at monthly-to-<span class="hlt">decadal</span> time scales over all the wet regions. In contrast, <fi>ρ</fi>DCCA was essentially nonsignificant between nonperiodic <fi>P</fi> and <fi>E</fi> or sea surface temperature (SST). Thus, the nonperiodic monthly-to-<span class="hlt">decadal</span> <span class="hlt">variability</span> of precipitation in these regions is almost fully controlled by dynamics and not by local <fi>E</fi> or SST (suggested by Clausius-Clapeyron relation). Analysis of regional nonperiodic standard deviations and power spectra (and respective spectral exponents, <fi>β</fi>) provided further robustness to this conclusion. Finally, clear transitions in <fi>β</fi> for <fi>P</fi>, DIV, and <fi>ω</fi> between tropical and storm track regions were found. The latter is dominated by transient storms, with energy accumulation at synoptic scales and <fi>β</fi> < 0.1 at monthly-to-<span class="hlt">decadal</span> time scales, implying that <span class="hlt">variability</span> and information creation decrease rapidly with time scale. Larger <fi>β</fi> values (0.2 to 0.4) were found in the tropics, implying longer-range autocorrelations and</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27713662','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27713662"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of extreme wave height representing storm severity in the northeast Atlantic and North Sea since the foundation of the Royal Society.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Santo, H; Taylor, P H; Gibson, R</p> <p>2016-09-01</p> <p>Long-term estimation of extreme wave height remains a key challenge because of the short duration of available wave data, and also because of the possible impact of climate <span class="hlt">variability</span> on ocean waves. Here, we analyse storm-based statistics to obtain estimates of extreme wave height at locations in the northeast Atlantic and North Sea using the NORA10 wave hindcast (1958-2011), and use a 5 year sliding window to examine temporal <span class="hlt">variability</span>. The <span class="hlt">decadal</span> <span class="hlt">variability</span> is correlated to the North Atlantic oscillation and other atmospheric modes, using a six-term predictor model incorporating the climate indices and their Hilbert transforms. This allows reconstruction of the historic extreme climate back to 1661, using a combination of known and proxy climate indices. Significant <span class="hlt">decadal</span> <span class="hlt">variability</span> primarily driven by the North Atlantic oscillation is <span class="hlt">observed</span>, and this should be considered for the long-term survivability of offshore structures and marine renewable energy devices. The analysis on wave climate reconstruction reveals that the variation of the mean, 99th percentile and extreme wave climates over <span class="hlt">decadal</span> time scales for locations close to the dominant storm tracks in the open North Atlantic are comparable, whereas the wave climates for the rest of the locations including the North Sea are rather different.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5046986','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5046986"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of extreme wave height representing storm severity in the northeast Atlantic and North Sea since the foundation of the Royal Society</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Taylor, P. H.; Gibson, R.</p> <p>2016-01-01</p> <p>Long-term estimation of extreme wave height remains a key challenge because of the short duration of available wave data, and also because of the possible impact of climate <span class="hlt">variability</span> on ocean waves. Here, we analyse storm-based statistics to obtain estimates of extreme wave height at locations in the northeast Atlantic and North Sea using the NORA10 wave hindcast (1958–2011), and use a 5 year sliding window to examine temporal <span class="hlt">variability</span>. The <span class="hlt">decadal</span> <span class="hlt">variability</span> is correlated to the North Atlantic oscillation and other atmospheric modes, using a six-term predictor model incorporating the climate indices and their Hilbert transforms. This allows reconstruction of the historic extreme climate back to 1661, using a combination of known and proxy climate indices. Significant <span class="hlt">decadal</span> <span class="hlt">variability</span> primarily driven by the North Atlantic oscillation is <span class="hlt">observed</span>, and this should be considered for the long-term survivability of offshore structures and marine renewable energy devices. The analysis on wave climate reconstruction reveals that the variation of the mean, 99th percentile and extreme wave climates over <span class="hlt">decadal</span> time scales for locations close to the dominant storm tracks in the open North Atlantic are comparable, whereas the wave climates for the rest of the locations including the North Sea are rather different. PMID:27713662</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016RSPSA.47260376S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016RSPSA.47260376S"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of extreme wave height representing storm severity in the northeast Atlantic and North Sea since the foundation of the Royal Society</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santo, H.; Taylor, P. H.; Gibson, R.</p> <p>2016-09-01</p> <p>Long-term estimation of extreme wave height remains a key challenge because of the short duration of available wave data, and also because of the possible impact of climate <span class="hlt">variability</span> on ocean waves. Here, we analyse storm-based statistics to obtain estimates of extreme wave height at locations in the northeast Atlantic and North Sea using the NORA10 wave hindcast (1958-2011), and use a 5 year sliding window to examine temporal <span class="hlt">variability</span>. The <span class="hlt">decadal</span> <span class="hlt">variability</span> is correlated to the North Atlantic oscillation and other atmospheric modes, using a six-term predictor model incorporating the climate indices and their Hilbert transforms. This allows reconstruction of the historic extreme climate back to 1661, using a combination of known and proxy climate indices. Significant <span class="hlt">decadal</span> <span class="hlt">variability</span> primarily driven by the North Atlantic oscillation is <span class="hlt">observed</span>, and this should be considered for the long-term survivability of offshore structures and marine renewable energy devices. The analysis on wave climate reconstruction reveals that the variation of the mean, 99th percentile and extreme wave climates over <span class="hlt">decadal</span> time scales for locations close to the dominant storm tracks in the open North Atlantic are comparable, whereas the wave climates for the rest of the locations including the North Sea are rather different.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6747L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6747L"><span>Effect of climate <span class="hlt">variability</span> and change on winter haze over eastern China in recent <span class="hlt">decades</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liao, Hong; Yang, Yang</p> <p>2017-04-01</p> <p>In recent years, eastern China has frequently experienced persistent and severe winter haze pollution episodes with high aerosol concentrations, which have affected half of the 1.3 billion people in China. In this work, the increases in wintertime aerosol concentrations and severe haze events in eastern China over 1985-2015 were quantified by using <span class="hlt">observed</span> atmospheric visibility from the National Climatic Data Center Global Summary of Day database, <span class="hlt">observed</span> PM2.5 concentrations from the network of China National Environmental Monitoring Centre (CNEMC), and simulated PM2.5 concentrations from the Goddard Earth-<span class="hlt">Observing</span> System (GEOS) chemical transport model (GEOS-Chem). <span class="hlt">Observed</span> winter haze days (defined as days with atmospheric visibility less than 10 km and relative humidity less than 80%) averaged over eastern China (105-122.5°E, 20-45°N) increased from 21 days in 1980 to 42 days in 2014. <span class="hlt">Observed</span> severe haze days (defined as days with PM2.5 >150 μg m-3) occurred mainly over Northern China. Considering variations in both anthropogenic emissions and meteorological parameters, the GEOS-Chem model simulated an increasing trend in wintertime surface-layer PM2.5 concentrations of 10.5 (±6.2) μg m-3 <span class="hlt">decade</span>-1 over eastern China in the past <span class="hlt">decades</span>. Sensitivity studies showed that changes in anthropogenic emissions and in climate contributed 87% and 17% to this increasing trend, respectively. Wintertime severe haze events over eastern China showed large interannual variations, driven by climate <span class="hlt">variability</span>. Process analyses were performed to identify the key meteorological parameters that determined the interannual variations of wintertime severe haze events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A13M..04G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A13M..04G"><span>Analyzing nearly four <span class="hlt">decades</span> of historical radiosonde <span class="hlt">observations</span> of tropical tropopause layer and cold-point temperatures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gilford, D.; Randel, W. J.</p> <p>2017-12-01</p> <p>An understanding of historical trends and <span class="hlt">variability</span> in the thermal structure of the tropical tropopause layer (TTL) is important for assessing climate and investigating TTL processes. In particular, the cold-point tropopause (CPT) plays an important role in stratospheric dehydration, the potential intensities of tropical cyclones, and other forms of stratospheric-tropospheric coupling. Uncertainties and biases of in-situ <span class="hlt">observations</span>, however, make long-term estimation of TTL temperatures challenging, especially in the early <span class="hlt">decades</span> of the satellite era. The goal of this study is to construct and analyze a long-term record of radiosondes temperatures with minimal biases. Temperature <span class="hlt">observations</span> from 1979-present are drawn from the Integrated Global Radiosonde Archive version 2 (IGRA2). Vertically integrated radiosonde temperatures are compared with brightness temperatures from the Microwave Sounding Units (MSU) Lower Stratosphere channel to identify the radiosonde stations with the smallest temporal discontinuities. Insights from this comparison highlight the importance of independent measurements when evaluating TTL temperatures. The 38-year dataset constructed from IGRA2 stations with the smallest biases spans the tropics and has high vertical resolution, permitting reasonable estimates of the CPT temperature. Radiosonde temperatures show good agreement with GPS radio occultation measurements over the past <span class="hlt">decade</span>. A multivariate regression model incorporating the Quasi-Biennial Oscillation and the El Nino Southern Oscillation is fit to the deseasonalized data to evaluate the spatial and temporal structures in its <span class="hlt">variability</span>. Long-term trends in CPT temperatures are considered in the context of historical estimates from climate models. Correlations with TTL water vapor concentrations from the Stratospheric Water and OzOne Satellite Homogenized (SWOOSH) data set suggest a strong relationship between the historically <span class="hlt">observed</span> CPT temperatures and dehydration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010037382','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010037382"><span>Surface Salinity <span class="hlt">Variability</span> in the North Atlantic During Recent <span class="hlt">Decades</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Haekkinen, Sirpa</p> <p>2001-01-01</p> <p>The sea surface salinity (SSS) <span class="hlt">variability</span> in the North Atlantic is investigated using numerical model simulations for the last 50 years based on atmospheric forcing <span class="hlt">variability</span> from Comprehensive Atmosphere Ocean Data Set (COADS) and National Center for Environmental Prediction / National Center for Atmospheric Research (NCEP/NCAR) Reanalysis. The largest interannual and longer term <span class="hlt">variability</span> occurs in two regions: the Labrador Sea and the North Equatorial Countercurrent (NECC) region. In both regions the seasonality of the surface salinity <span class="hlt">variability</span> is prominent with the maximum standard deviation occurring in the summer/fall period. In the Labrador Sea the summer SSS anomalies far exceed those of wintertime in amplitude. The interannual SSS <span class="hlt">variability</span> in the subpolar gyre can be attributed to two factors: excess ice melt and heat flux (i.e. deep mixing) variations. On the other hand, heat flux <span class="hlt">variability</span> can also lead to meridional overturning changes on <span class="hlt">decadal</span> time scales such that weak overturning is manifested in fresh surface conditions in the subpolar gyre. The overturning changes also influence the NECC region SSS <span class="hlt">variability</span>. Moreover, the subpolar freshening events are expected to occur during the negative phase of North Atlantic Oscillation which is associated with a weak wintertime surface heat loss in the subpolar gyre. No excess sea ice melt or precipitation is necessary for the formation of the fresh anomalies, because with the lack of wide-spread deep mixing, the fresh water that would be expected based on climatology, would accumulate at the surface. Thus, the fresh water 'conveyor' in the Atlantic operates via the overturning circulation such that deep mixing inserts fresh water while removing heat from the water column.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H42H..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H42H..04B"><span>Hydrologic impacts of land cover <span class="hlt">variability</span> and change at seasonal to <span class="hlt">decadal</span> time scales over North America, 1992-2016</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bohn, T. J.; Vivoni, E. R.</p> <p>2017-12-01</p> <p>Land cover <span class="hlt">variability</span> and change have been shown to influence the terrestrial hydrologic cycle by altering the partitioning of moisture and energy fluxes. However, the magnitude and directionality of the relationship between land cover and surface hydrology has been shown to vary substantially across regions. Here, we provide an assessment of the impacts of land cover change on hydrologic processes at seasonal (vegetation phenology) to <span class="hlt">decadal</span> scales (land cover conversion) in the United States and Mexico. To this end, we combine time series of remotely-sensed land surface characteristics with land cover maps for different <span class="hlt">decades</span> as input to the <span class="hlt">Variable</span> Infiltration Capacity hydrologic model. Land surface characteristics (leaf area index, surface albedo, and canopy fraction derived from normalized difference vegetation index) were obtained from the Moderate Resolution Imaging Spectrometer (MODIS) at 8-day intervals over the period 2000-2016. Land cover maps representing conditions in 1992, 2001, and 2011 were derived by homogenizing the National Land Cover Database over the US and the INEGI Series I through V maps over Mexico. An additional map covering all of North America was derived from the most frequent land cover class <span class="hlt">observed</span> in each pixel of the MODIS MOD12Q1 product during 2001-2013. Land surface characteristics were summarized over land cover fractions at 1/16 degree (6 km) resolution. For each land cover map, hydrologic simulations were conducted that covered the period 1980-2013, using the best-available, hourly meteorological forcings at a similar spatial resolution. Based on these simulations, we present a comparison of the contributions of land cover change and climate <span class="hlt">variability</span> at seasonal to <span class="hlt">decadal</span> scales on the hydrologic and energy budgets, identifying the dominant components through time and space. This work also offers a valuable dataset on land cover <span class="hlt">variability</span> and its hydrologic response for continental-scale assessments and modeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...621251D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...621251D"><span>The Footprint of the Inter-<span class="hlt">decadal</span> Pacific Oscillation in Indian Ocean Sea Surface Temperatures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dong, Lu; Zhou, Tianjun; Dai, Aiguo; Song, Fengfei; Wu, Bo; Chen, Xiaolong</p> <p>2016-02-01</p> <p>Superimposed on a pronounced warming trend, the Indian Ocean (IO) sea surface temperatures (SSTs) also show considerable <span class="hlt">decadal</span> variations that can cause regional climate oscillations around the IO. However, the mechanisms of the IO <span class="hlt">decadal</span> <span class="hlt">variability</span> remain unclear. Here we perform numerical experiments using a state-of-the-art, fully coupled climate model in which the external forcings with or without the <span class="hlt">observed</span> SSTs in the tropical eastern Pacific Ocean (TEP) are applied for 1871-2012. Both the <span class="hlt">observed</span> timing and magnitude of the IO <span class="hlt">decadal</span> variations are well reproduced in those experiments with the TEP SSTs prescribed to <span class="hlt">observations</span>. Although the external forcings account for most of the warming trend, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is dominated by internal <span class="hlt">variability</span> that is induced by the TEP SSTs, especially the Inter-<span class="hlt">decadal</span> Pacific Oscillation (IPO). The IPO weakens (enhances) the warming of the external forcings by about 50% over the IO during IPO’s cold (warm) phase, which contributes about 10% to the recent global warming hiatus since 1999. The <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is modulated by the IPO-induced atmospheric adjustment through changing surface heat fluxes, sea surface height and thermocline depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26884089','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26884089"><span>The Footprint of the Inter-<span class="hlt">decadal</span> Pacific Oscillation in Indian Ocean Sea Surface Temperatures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dong, Lu; Zhou, Tianjun; Dai, Aiguo; Song, Fengfei; Wu, Bo; Chen, Xiaolong</p> <p>2016-02-17</p> <p>Superimposed on a pronounced warming trend, the Indian Ocean (IO) sea surface temperatures (SSTs) also show considerable <span class="hlt">decadal</span> variations that can cause regional climate oscillations around the IO. However, the mechanisms of the IO <span class="hlt">decadal</span> <span class="hlt">variability</span> remain unclear. Here we perform numerical experiments using a state-of-the-art, fully coupled climate model in which the external forcings with or without the <span class="hlt">observed</span> SSTs in the tropical eastern Pacific Ocean (TEP) are applied for 1871-2012. Both the <span class="hlt">observed</span> timing and magnitude of the IO <span class="hlt">decadal</span> variations are well reproduced in those experiments with the TEP SSTs prescribed to <span class="hlt">observations</span>. Although the external forcings account for most of the warming trend, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is dominated by internal <span class="hlt">variability</span> that is induced by the TEP SSTs, especially the Inter-<span class="hlt">decadal</span> Pacific Oscillation (IPO). The IPO weakens (enhances) the warming of the external forcings by about 50% over the IO during IPO's cold (warm) phase, which contributes about 10% to the recent global warming hiatus since 1999. The <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is modulated by the IPO-induced atmospheric adjustment through changing surface heat fluxes, sea surface height and thermocline depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PrOce..74..329F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PrOce..74..329F"><span>Zooplankton time-series in the Balearic Sea (Western Mediterranean): <span class="hlt">Variability</span> during the <span class="hlt">decade</span> 1994 2003</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernández de Puelles, Maria Luz; Alemany, Francisco; Jansá, Javier</p> <p>2007-08-01</p> <p>Studies of plankton time-series from the Balearic islands waters are presented for the past <span class="hlt">decade</span>, with main emphasis on the <span class="hlt">variability</span> of zooplankton and how it relates to the environment. The seasonal and interannual patterns of temperature, salinity, nutrients, chlorophyll concentration and zooplankton abundance are described with data obtained between 1994 and 2003. Samples were collected every 10 days at a monitoring station in the Mallorca channel, an area with marked hydrographic <span class="hlt">variability</span> in the Western Mediterranean. Mesoscale <span class="hlt">variability</span> was also assessed using data from monthly sampling survey carried out between 1994 and 1999 in a three station transect located in the same study area. The copepods were the most abundant group with three higher peaks (March, May and September) distinguished during the annual cycle and a clear coastal-offshore decreasing gradient. Analysis of the zooplankton community revealed two distinct periods: the mixing period during winter and early spring, where copepods, siphonophores and ostracods were most abundant and, the stratified period characterised by an increase of cladocerans and meroplankton abundances. Remarkable interannual zooplankton <span class="hlt">variability</span> was <span class="hlt">observed</span> in relation to hydrographic regime with higher abundances of main groups during cool years, when northern Mediterranean waters prevailed in the area. The warmer years showed the lowest zooplankton abundances, associated with the inflow of less saline and nutrient-depleted Atlantic Waters. Moreover, the correlation found between copepod abundance and large scale climatic factors (e.g., NAO) suggested that they act as main driver of the zooplankton <span class="hlt">variability</span>. Therefore, the seasonal but particularly the interannual variation <span class="hlt">observed</span> in plankton abundance and structure patterns of the Balearic Sea seems to be highly modulated by large-scale forcing and can be considered an ideal place where to investigate potential consequences of global climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.B23C0442S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.B23C0442S"><span>Response of Tropical Forests to Intense Climate <span class="hlt">Variability</span> and Rainfall Anomaly of Last <span class="hlt">Decade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saatchi, S. S.; Asefi Najafabady, S.</p> <p>2011-12-01</p> <p>During the last <span class="hlt">decade</span>, strong precipitation anomalies resulted from increased sea surface temperature in the tropical Atlantic, have caused extensive drying trends in rainforests of western Amazonia, exerting water stress, tree mortality, biomass loss, and large-scale fire disturbance. In contrast, there have been no reports on large-scale disturbance in rainforests of west and central Africa, though being exposed to similar intensity of climate <span class="hlt">variability</span>. Using data from Tropical Rainfall Mapping Mission (TRMM) (1999-2010), and time series of rainfall <span class="hlt">observations</span> from meteorological stations (1971-2000), we show that both Amazonian and African rainforest experienced strong precipitation anomalies from 2005-2010. We monitored the response of forest to the climate <span class="hlt">variability</span> by analyzing the canopy water content <span class="hlt">observed</span> by SeaWinds Ku-band Scatterometer (QSCAT) (1999-2009) and found that more than 70 million ha of forests in western Amazonia experienced a strong water deficit during the dry season of 2005 and a closely corresponding decline in canopy backscatter that persisted until the next major drought in 2010. This decline in backscatter has been attributed to loss of canopy water content and large-scale tree mortality corroborated by ground and airborne <span class="hlt">observations</span>. However, no strong impacts was <span class="hlt">observed</span> on tropical forests of Africa, suggesting that the African rainforest may have more resilience to droughts. We tested this hypothesis by examining the seasonal rainfall patterns, maximum water deficit, and the surface temperature variations. Results show that there is a complex pattern of low annual rainfall, moderate seasonality, and lower surface temperature in Central Africa compared to Amazonia, indicating potentially a lower evapotranspiration circumventing strong water deficits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA522335','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA522335"><span><span class="hlt">Decadal</span> <span class="hlt">Variability</span> of the Tropical Stratosphere: Secondary Influence of the El Nino-Southern Oscillation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-02-04</p> <p>the QBO [McCormack et al., 2007, and references therein]. However, it is also possible that “feedbacks from below” are a significant contributing cause...<span class="hlt">DECADAL</span> <span class="hlt">VARIABILITY</span> OF THE TROPICAL STRATOSPHERE ozone <span class="hlt">variability</span> from other sources (notably from the equatorial quasi-biennial wind oscillation, or QBO ...work (SH06 and references therein), but with the addition of an ENSO term and including a more complete representation of the QBO : X(t) = µ(i) + βtrendt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990006015','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990006015"><span><span class="hlt">Decadal</span> Air-Sea Interaction in the North Atlantic Based on <span class="hlt">Observations</span> and Modeling Results</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hakkinen, Sirpa</p> <p>1998-01-01</p> <p>The <span class="hlt">decadal</span>, 12-14 year, cycle <span class="hlt">observed</span> in the North Atlantic SST and tide gauge data was examined using the NCEP/NCAR reanalyses, COADS data and an ocean model simulation. Besides this <span class="hlt">decadal</span> mode, a shorter, subdecadal period of about 8 years exists in tide gauge data north of 40N, in the subpolar SST and in the winter North Atlantic Oscillation (NAO) index and in subpolar winter heat flux values. The <span class="hlt">decadal</span> cycle is a well separated mode in a singular spectrum analysis (SSA) for a time series of SST EOF mode 1 with a center over the Gulf Stream extension. Tide gauge and SST data are consistent in that both show a significant subdecadal periodicity exclusively in the subpolar gyre, but in subtropics the 12-14 year period is the prominent, but nonstationary, <span class="hlt">decadal</span> signal. The main finding of this study is that this 12-14 year cycle can be constructed based on the leading mode of the surface heat flux. This connection to the surface heat flux implicates the participation of the thermohaline circulation in the <span class="hlt">decadal</span> cycle. During the cycle starting from the positive index phase of NAO, SST and oceanic heat content anomalies are created in subtropics due to local heat flux and intensification of the thermohaline circulation. The anomalies advect to the subpolar gyre where they are amplified by local heat flux and are part of the negative feedback of thermohaline circulation on itself. Consequently the oceanic thermohaline circulation slows down and the opposite cycle starts. The oscillatory nature would not be possible without the active atmospheric participation in the cycle, because it provides the unstable interaction through heat flux, without it, the oceanic mode would be damped. This analysis suggests that the two principal modes of heat flux <span class="hlt">variability</span>, corresponding to patterns similar to North Atlantic Oscillation (NAO) and Western Atlantic (WA), are part of the same <span class="hlt">decadal</span> cycle and an indirect measure of the north-south movement of the storm tracks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC32B..01O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC32B..01O"><span>Increasing Megadrought Risk at the Intersection of <span class="hlt">Decadal</span> to Centennial <span class="hlt">Variability</span> and Climate Change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Overpeck, J. T.; Parsons, L. A.; Loope, G. R.; Ault, T.; Cole, J. E.; Otto-Bliesner, B. L.; Buckle, N.; Stevenson, S.; Fasullo, J.</p> <p>2016-12-01</p> <p>Even more than the 1930's U.S. Dust Bowl Drought, the 20th century Sahel drought stands out as the most unprecedented drought of the instrumental era, in part because it extended over multiple <span class="hlt">decades</span>. Paleoclimatic evidence makes it clear that this Sahel drought was nonetheless not really unprecedented - droughts many <span class="hlt">decades</span> long have occurred in sub-Saharan Africa regularly over the last several thousand years, and these constitute what is now increasingly referred to as "megadrought." Paleoclimatic evidence also makes it clear that all drought-prone semi-arid and arid regions of the globe, including southwestern North America, southeastern Australia, and the Mediterranean/Middle Eastern region likely experienced multiple such multidecadal megadroughts in recent pre-Anthropocene Earth history. In other regions of the globe, including parts of South Asia and Amazonia, short but devastating droughts of the last 50-150 years, were also eclipsed in recent Earth history by much more serious megadrought, although these megadroughts were shorter than the multidecadal droughts of Africa or SW North America. In the past, megadroughts have occurred for reasons that are increasingly well understood in terms of ocean-atmosphere dynamics that led to unusually persistent precipitation deficits. Many of these same dynamics are well simulated in state-of-the-art Earth System Models, and yet comparisons between simulated and <span class="hlt">observed</span> paleohydroclimatic <span class="hlt">variability</span> suggests the models generally underestimate the risk of megadrought. Paleohydroclimatic records in some cases overestimate drought persistence, but there appear to be other issues at play that need to be better understood and simulated: positive land-atmosphere feedbacks, overly energetic interannual (i.e., ENSO) modes of <span class="hlt">variability</span>, and insufficient internal multidecadal to centennial coupled climate system <span class="hlt">variability</span>. Taking these issues and the impact of anthropogenic climate change into account means that the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H42G..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H42G..02S"><span>Examining the last few <span class="hlt">decades</span> of global hydroclimate for evidence of anthropogenic change amidst natural <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seager, R.; Naik, N.; Ting, M.; Kushnir, Y.; Kelley, C. P.</p> <p>2011-12-01</p> <p>Climate models robustly predict that the deep tropics and mid-latitude-to-subpolar regions will moisten, and the subtropical dry zones both dry and expand, as a consequence of global warming driven by rising greenhouse gases. The models also predict that this transition to a more extreme climatological mean global hydroclimate should already be underway. Given the importance of these predictions it is an imperative that the climate science community assess whether there is evidence within the <span class="hlt">observational</span> record that they are correct. This task is made difficult by the tremendous natural <span class="hlt">variability</span> of the hydrological cycle on seasonal to multidecadal timescales. Here we will use instrumental <span class="hlt">observations</span>, reanalyses, sea surface temperature forced atmosphere models and coupled model simulations, and a variety of methodologies, to attempt to separate global radiatively-forced hydroclimate change from ongoing natural <span class="hlt">variability</span>. The results will be applied to explain trends and recent events in key regions such as Mexico, the United States and the Mediterranean. It is concluded that the signal of anthropogenic change is small compared to the amplitude of natural <span class="hlt">variability</span> but that it is a discernible contributor. Globally the evidence reveals that radiatively-forced hydroclimate change is occurring with an amplitude and spatial pattern largely consistent with the predictions by IPCC AR4 models of hydroclimate change to date. However it will also be shown that the radiatively-forced component does not in and of itself provide a useful prediction of near term hydroclimate change because for many regions the amplitude of natural <span class="hlt">decadal</span> <span class="hlt">variability</span> is as large or larger. Useful predictions need to account for how natural <span class="hlt">variability</span> may evolve as well as forced change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110006943','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110006943"><span>A <span class="hlt">Decade</span> of Satellite Ocean Color <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McClain, Charles R.</p> <p>2009-01-01</p> <p>After the successful Coastal Zone Color Scanner (CZCS, 1978-1986), demonstration that quantitative estimations of geophysical <span class="hlt">variables</span> such as chlorophyll a and diffuse attenuation coefficient could be derived from top of the atmosphere radiances, a number of international missions with ocean color capabilities were launched beginning in the late 1990s. Most notable were those with global data acquisition capabilities, i.e., the Ocean Color and Temperature Sensor (OCTS 1996-1997), the Sea-viewing Wide Field-of-view Sensor (SeaWiFS, United States, 1997-present), two Moderate Resolution Imaging Spectroradiometers, (MODIS, United States, Terra/2000-present and Aqua/2002-present), the Global Imager (GLI, Japan, 2002-2003), and the Medium Resolution Imaging Spectrometer (MERIS, European Space Agency, 2002-present). These missions have provided data of exceptional quality and continuity, allowing for scientific inquiries into a wide variety of marine research topics not possible with the CZCS. This review focuses on the scientific advances made over the past <span class="hlt">decade</span> using these data sets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSOD14B2420L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSOD14B2420L"><span>The CARIACO Ocean Time-Series: two <span class="hlt">decades</span> of oceanographic <span class="hlt">observations</span> to understand linkages between biogeochemistry, ecology, and long-term environmental <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lorenzoni, L.; Muller-Karger, F. E.; Rueda-Roa, D. T.; Thunell, R.; Scranton, M. I.; Taylor, G. T.; benitez-Nelson, C. R.; Montes, E.; Astor, Y. M.; Rojas, J.</p> <p>2016-02-01</p> <p>The CARIACO Ocean Time-Series project, located in the Cariaco Basin off the coast of Venezuela, seeks to understand relationships between hydrography, primary production, community composition, microbial activity, particle fluxes, and element cycling in the water column, and how variations in these processes are preserved in sediments accumulating in this anoxic basin. CARIACO uses autonomous and shipboard measurements to understand ecological and biogeochemical changes and how these relate to regional and global climatic/ocean <span class="hlt">variability</span>. CARIACO is a model for national ocean <span class="hlt">observing</span> programs in Central/South America, and has been developed as a community facility platform with open access to all data (http://imars.marine.usf.edu/cariaco). Research resulting from this program has contributed to knowledge about the decomposition and cycling of particles, the biological pump, and to our understanding of the ecology and oceanography of oxygen minimum zones. Despite this basin being anoxic below 250m, remineralization rates of organic matter are comparable to those in well oxygenated waters. A dynamic microbial community significantly influences carbon and nutrient biogeochemical cycling throughout the water column. Since 1995, declining particulate organic carbon fluxes have been measured throughout the water column using sediment traps, likely in response to declining Chl-a concentrations and smaller phytoplankton which have replaced the larger taxa over the past <span class="hlt">decade</span>. This community shift appears to be caused by regional changes in the physical regime. CARIACO also recorded marked long-term changes in surface and deep DIC in response to a combination of factors including surface water warming. The <span class="hlt">observations</span> of CARIACO highlight the importance of a sustained, holistic approach to studying biodiversity, ecology and the marine carbon cycle to predict potential impacts of climate change on the ocean's ecosystem services and carbon sequestration efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2381G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2381G"><span><span class="hlt">Decadal</span> modulation of the relationship between intraseasonal tropical <span class="hlt">variability</span> and ENSO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gushchina, Daria; Dewitte, Boris</p> <p>2018-05-01</p> <p>The El Niño Southern Oscillation (ENSO) amplitude is modulated at <span class="hlt">decadal</span> timescales, which, over the last <span class="hlt">decades</span>, has been related to the low-frequency changes in the frequency of occurrence of the two types of El Niño events, that is the Eastern Pacific (EP) and Central Pacific (CP) El Niños. Meanwhile ENSO is tightly linked to the intraseasonal tropical <span class="hlt">variability</span> (ITV) that is generally enhanced prior to El Niño development and can act as a trigger of the event. Here we revisit the ITV/ENSO relationship taking into account changes in ENSO properties over the last six <span class="hlt">decades</span>. The focus is on two main components of ITV, the Madden-Julian Oscillation (MJO) and convectively coupled equatorial Rossby waves (ER). We show that the ITV/ENSO relationship exhibits a <span class="hlt">decadal</span> modulation that is not related in a straight-forward manner to the change in occurrence of El Niño types and Pacific <span class="hlt">decadal</span> modes. While enhanced MJO activity associated to EP El Niño development mostly took place over the period 1985-2000, the ER activity is enhanced prior to El Niño development over the whole period with a tendency to relate more to CP El Niño than to EP El Niño. In particular the relationship between ER activity and ENSO was particularly strong for the period 2000-2015, which results in a significant positive long-term trend of the predictive value of ER activity. The statistics of the MJO and ER activity is consistent with the hypothesis that they can be considered a state-dependent noise for ENSO linked to distinct lower frequency climate modes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1253370','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1253370"><span>The footprint of the inter-<span class="hlt">decadal</span> Pacific oscillation in Indian Ocean sea surface temperatures</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Dong, Lu; Zhou, Tianjun; Dai, Aiguo</p> <p></p> <p>Superimposed on a pronounced warming trend, the Indian Ocean (IO) sea surface temperatures (SSTs) also show considerable <span class="hlt">decadal</span> variations that can cause regional climate oscillations around the IO. However, the mechanisms of the IO <span class="hlt">decadal</span> <span class="hlt">variability</span> remain unclear. Here we perform numerical experiments using a state-of-the-art, fully coupled climate model in which the external forcings with or without the <span class="hlt">observed</span> SSTs in the tropical eastern Pacific Ocean (TEP) are applied for 1871–2012. Both the <span class="hlt">observed</span> timing and magnitude of the IO <span class="hlt">decadal</span> variations are well reproduced in those experiments with the TEP SSTs prescribed to <span class="hlt">observations</span>. Although the external forcingsmore » account for most of the warming trend, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is dominated by internal <span class="hlt">variability</span> that is induced by the TEP SSTs, especially the Inter-<span class="hlt">decadal</span> Pacific Oscillation (IPO). The IPO weakens (enhances) the warming of the external forcings by about 50% over the IO during IPO’s cold (warm) phase, which contributes about 10% to the recent global warming hiatus since 1999. As a result, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is modulated by the IPO-induced atmospheric adjustment through changing surface heat fluxes, sea surface height and thermocline depth.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1253370-footprint-inter-decadal-pacific-oscillation-indian-ocean-sea-surface-temperatures','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1253370-footprint-inter-decadal-pacific-oscillation-indian-ocean-sea-surface-temperatures"><span>The footprint of the inter-<span class="hlt">decadal</span> Pacific oscillation in Indian Ocean sea surface temperatures</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Dong, Lu; Zhou, Tianjun; Dai, Aiguo; ...</p> <p>2016-02-17</p> <p>Superimposed on a pronounced warming trend, the Indian Ocean (IO) sea surface temperatures (SSTs) also show considerable <span class="hlt">decadal</span> variations that can cause regional climate oscillations around the IO. However, the mechanisms of the IO <span class="hlt">decadal</span> <span class="hlt">variability</span> remain unclear. Here we perform numerical experiments using a state-of-the-art, fully coupled climate model in which the external forcings with or without the <span class="hlt">observed</span> SSTs in the tropical eastern Pacific Ocean (TEP) are applied for 1871–2012. Both the <span class="hlt">observed</span> timing and magnitude of the IO <span class="hlt">decadal</span> variations are well reproduced in those experiments with the TEP SSTs prescribed to <span class="hlt">observations</span>. Although the external forcingsmore » account for most of the warming trend, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is dominated by internal <span class="hlt">variability</span> that is induced by the TEP SSTs, especially the Inter-<span class="hlt">decadal</span> Pacific Oscillation (IPO). The IPO weakens (enhances) the warming of the external forcings by about 50% over the IO during IPO’s cold (warm) phase, which contributes about 10% to the recent global warming hiatus since 1999. As a result, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in IO SSTs is modulated by the IPO-induced atmospheric adjustment through changing surface heat fluxes, sea surface height and thermocline depth.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..297..265D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..297..265D"><span>Three <span class="hlt">decades</span> of Loki Patera <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Pater, Imke; de Kleer, Katherine; Davies, Ashley G.; Ádámkovics, Máté</p> <p>2017-11-01</p> <p>We present <span class="hlt">observations</span> of Io's Loki Patera taken with the 10-m Keck telescopes between 1998 and 2016. Adding these data to those published by Rathbun and Spencer (2006) and the Gemini data of de Kleer and de Pater (2016a, 2017) results in a database of 3.5-3.8 μm emission from Loki Patera over almost 3 <span class="hlt">decades</span>. Data presented here contain adaptive optics (AO) <span class="hlt">observations</span> of Io's sunlit hemisphere at wavelengths between 1.6 and 5 μm, AO <span class="hlt">observations</span> of Io in eclipse at 2-5 μm, and non-AO <span class="hlt">observations</span> of Io in eclipse at 1.6-12 μm. The non-AO data were taken in September of 1999, during the early phase of a brightening event that was documented by Howell et al. (2001). Dual-component Io Flow model (IFM) fits to our 1999 <span class="hlt">observations</span> show a mostly cool lava crust over almost the entire patera floor, with a relatively small hotter component making up less than 1% of the total area, consistent with previous <span class="hlt">observations</span>. The 30-year timeline of Loki Patera revealed that, after an apparent cessation of, or change in, brightening events in 2002, Loki Patera became active again in 2009. The more recent activity may have a slightly shorter periodicity than <span class="hlt">observed</span> by Rathbun et al. (2002), and the direction of flow propagation appears to have reversed. Since 2009 the flow direction is in the clockwise direction, starting in the north or north-east corner and propagating along the patera towards the south-west. During the Galileo era the propagation was in the counter-clockwise direction, starting in the south-west and propagating towards the east. Both the 30-year timeline and the 1.6-12 μm spectrum that was obtained during the brightening event in 1999 agree well with Matson et al.'s (2006) overturning lava lake model, as modified by de Kleer and de Pater (2017).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1167250','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1167250"><span>A Generalized Stability Analysis of the AMOC in Earth System Models: Implication for <span class="hlt">Decadal</span> <span class="hlt">Variability</span> and Abrupt Climate Change</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Fedorov, Alexey V.</p> <p>2015-01-14</p> <p>The central goal of this research project was to understand the mechanisms of <span class="hlt">decadal</span> and multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of the Atlantic Meridional Overturning Circulation (AMOC) as related to climate <span class="hlt">variability</span> and abrupt climate change within a hierarchy of climate models ranging from realistic ocean models to comprehensive Earth system models. Generalized Stability Analysis, a method that quantifies the transient and asymptotic growth of perturbations in the system, is one of the main approaches used throughout this project. The topics we have explored range from physical mechanisms that control AMOC <span class="hlt">variability</span> to the factors that determine AMOC predictability in the Earth systemmore » models, to the stability and <span class="hlt">variability</span> of the AMOC in past climates.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AdWR..109..236K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AdWR..109..236K"><span>Four <span class="hlt">decades</span> of microwave satellite soil moisture <span class="hlt">observations</span>: Part 2. Product validation and inter-satellite comparisons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karthikeyan, L.; Pan, Ming; Wanders, Niko; Kumar, D. Nagesh; Wood, Eric F.</p> <p>2017-11-01</p> <p>Soil moisture is widely recognized as an important land surface <span class="hlt">variable</span> that provides a deeper knowledge of land-atmosphere interactions and climate change. Space-borne passive and active microwave sensors have become valuable and essential sources of soil moisture <span class="hlt">observations</span> at global scales. Over the past four <span class="hlt">decades</span>, several active and passive microwave sensors have been deployed, along with the recent launch of two fully dedicated missions (SMOS and SMAP). Signifying the four <span class="hlt">decades</span> of microwave remote sensing of soil moisture, this Part 2 of the two-part review series aims to present an overview of how our knowledge in this field has improved in terms of the design of sensors and their accuracy for retrieving soil moisture. The first part discusses the developments made in active and passive microwave soil moisture retrieval algorithms. We assess the evolution of the products of various sensors over the last four <span class="hlt">decades</span>, in terms of daily coverage, temporal performance, and spatial performance, by comparing the products of eight passive sensors (SMMR, SSM/I, TMI, AMSR-E, WindSAT, AMSR2, SMOS and SMAP), two active sensors (ERS-Scatterometer, MetOp-ASCAT), and one active/passive merged soil moisture product (ESA-CCI combined product) with the International Soil Moisture Network (ISMN) in-situ stations and the <span class="hlt">Variable</span> Infiltration Capacity (VIC) land surface model simulations over the Contiguous United States (CONUS). In the process, the regional impacts of vegetation conditions on the spatial and temporal performance of soil moisture products are investigated. We also carried out inter-satellite comparisons to study the roles of sensor design and algorithms on the retrieval accuracy. We find that substantial improvements have been made over recent years in this field in terms of daily coverage, retrieval accuracy, and temporal dynamics. We conclude that the microwave soil moisture products have significantly evolved in the last four <span class="hlt">decades</span> and will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1304704-role-atlantic-multi-decadal-oscillation-global-mean-temperature-variability','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1304704-role-atlantic-multi-decadal-oscillation-global-mean-temperature-variability"><span>The role of Atlantic Multi-<span class="hlt">decadal</span> Oscillation in the global mean temperature <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Chylek, Petr; Klett, James D.; Dubey, Manvendra K.; ...</p> <p>2016-11-01</p> <p>We simulated the global mean 1900–2015 warming by 42 Coupled Models Inter-comparison Project, phase 5 (CMIP5) climate models varies between 0.58 and 1.70 °C. The <span class="hlt">observed</span> warming according to the NASA GISS temperature analysis is 0.95 °C with a 1200 km smoothing radius, or 0.86 °C with a 250 km smoothing radius. The projection of the future 2015–2100 global warming under a moderate increase of anthropogenic radiative forcing (RCP4.5 scenario) by individual models is between 0.7 and 2.3 °C. The CMIP5 climate models agree that the future climate will be warmer; however, there is little consensus as to how largemore » the warming will be (reflected by an uncertainty of over a factor of three). Moreover, a parsimonious statistical regression model with just three explanatory <span class="hlt">variables</span> [anthropogenic radiative forcing due to greenhouse gases and aerosols (GHGA), solar <span class="hlt">variability</span>, and the Atlantic Multi-<span class="hlt">decadal</span> Oscillation (AMO) index] accounts for over 95 % of the <span class="hlt">observed</span> 1900–2015 temperature variance. This statistical regression model reproduces very accurately the past warming (0.96 °C compared to the <span class="hlt">observed</span> 0.95 °C) and projects the future 2015–2100 warming to be around 0.95 °C (with the IPCC 2013 suggested RCP4.5 radiative forcing and an assumed cyclic AMO behavior). The AMO contribution to the 1970–2005 warming was between 0.13 and 0.20 °C (depending on which AMO index is used) compared to the GHGA contribution of 0.49–0.58 °C. During the twenty-first century AMO cycle the AMO contribution is projected to remain the same (0.13–0.20 °C), while the GHGA contribution is expected to decrease to 0.21–0.25 °C due to the levelling off of the GHGA radiative forcing that is assumed according to the RCP4.5 scenario. Therefore, the anthropogenic contribution and natural <span class="hlt">variability</span> are expected to contribute about equally to the anticipated global warming during the second half of the twenty-first century for the RCP4.5 trajectory.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1304704','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1304704"><span>The role of Atlantic Multi-<span class="hlt">decadal</span> Oscillation in the global mean temperature <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Chylek, Petr; Klett, James D.; Dubey, Manvendra K.</p> <p></p> <p>We simulated the global mean 1900–2015 warming by 42 Coupled Models Inter-comparison Project, phase 5 (CMIP5) climate models varies between 0.58 and 1.70 °C. The <span class="hlt">observed</span> warming according to the NASA GISS temperature analysis is 0.95 °C with a 1200 km smoothing radius, or 0.86 °C with a 250 km smoothing radius. The projection of the future 2015–2100 global warming under a moderate increase of anthropogenic radiative forcing (RCP4.5 scenario) by individual models is between 0.7 and 2.3 °C. The CMIP5 climate models agree that the future climate will be warmer; however, there is little consensus as to how largemore » the warming will be (reflected by an uncertainty of over a factor of three). Moreover, a parsimonious statistical regression model with just three explanatory <span class="hlt">variables</span> [anthropogenic radiative forcing due to greenhouse gases and aerosols (GHGA), solar <span class="hlt">variability</span>, and the Atlantic Multi-<span class="hlt">decadal</span> Oscillation (AMO) index] accounts for over 95 % of the <span class="hlt">observed</span> 1900–2015 temperature variance. This statistical regression model reproduces very accurately the past warming (0.96 °C compared to the <span class="hlt">observed</span> 0.95 °C) and projects the future 2015–2100 warming to be around 0.95 °C (with the IPCC 2013 suggested RCP4.5 radiative forcing and an assumed cyclic AMO behavior). The AMO contribution to the 1970–2005 warming was between 0.13 and 0.20 °C (depending on which AMO index is used) compared to the GHGA contribution of 0.49–0.58 °C. During the twenty-first century AMO cycle the AMO contribution is projected to remain the same (0.13–0.20 °C), while the GHGA contribution is expected to decrease to 0.21–0.25 °C due to the levelling off of the GHGA radiative forcing that is assumed according to the RCP4.5 scenario. Therefore, the anthropogenic contribution and natural <span class="hlt">variability</span> are expected to contribute about equally to the anticipated global warming during the second half of the twenty-first century for the RCP4.5 trajectory.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413778S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413778S"><span>Response of Tropical Forests to Intense Climate <span class="hlt">Variability</span> and Rainfall Anomaly over the Last <span class="hlt">Decade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saatchi, S.; Asefi, S.</p> <p>2012-04-01</p> <p>During the last <span class="hlt">decade</span>, strong precipitation anomalies resulted from increased sea surface temperature in the tropical Atlantic, have caused extensive drying trends in rainforests of western Amazonia, exerting water stress, tree mortality, biomass loss, and large-scale fire disturbance. In contrast, there have been no reports on large-scale disturbance in rainforests of west and central Africa, though being exposed to similar intensity of climate <span class="hlt">variability</span>. Using data from Tropical Rainfall Mapping Mission (TRMM) (1999-2010), and time series of rainfall <span class="hlt">observations</span> from meteorological stations (1971-2000), we show that both Amazonian and African rainforest experienced strong precipitation anomalies from 2005-2010. We monitored the response of forest to the climate <span class="hlt">variability</span> by analyzing the canopy water content <span class="hlt">observed</span> by SeaWinds Ku-band Scatterometer (QSCAT) (1999-2009) and found that more than 70 million ha of forests in western Amazonia experienced a strong water deficit during the dry season of 2005 and a closely corresponding decline in canopy backscatter that persisted until the next major drought in 2010. This decline in backscatter has been attributed to loss of canopy water content and large-scale tree mortality corroborated by ground and airborne <span class="hlt">observations</span>. However, no strong impacts was <span class="hlt">observed</span> on tropical forests of Africa, suggesting that the African rainforest may have more resilience to droughts. We tested this hypothesis by examining the seasonal rainfall patterns, maximum water deficit, and the surface temperature variations. Results show that there is a complex pattern of low annual rainfall, moderate seasonality, and lower surface temperature in Central Africa compared to Amazonia, indicating potentially a lower evapotranspiration circumventing strong water deficits</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AcMeS..26..289C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AcMeS..26..289C"><span><span class="hlt">Decadal</span> features of heavy rainfall events in eastern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Huopo; Sun, Jianqi; Fan, Ke</p> <p>2012-06-01</p> <p>Based on daily precipitation data, the spatial-temporal features of heavy rainfall events (HREs) during 1960-2009 are investigated. The results indicate that the HREs experienced strong <span class="hlt">decadal</span> <span class="hlt">variability</span> in the past 50 years, and the <span class="hlt">decadal</span> features varied across regions. More HRE days are <span class="hlt">observed</span> in the 1960s, 1980s, and 1990s over Northeast China (NEC); in the 1960s, 1970s, and 1990s over North China (NC); in the early 1960s, 1980s, and 2000s over the Huaihe River basin (HR); in the 1970s-1990s over the mid-lower reaches of the Yangtze River valley (YR); and in the 1970s and 1990s over South China (SC). These <span class="hlt">decadal</span> changes of HRE days in eastern China are closely associated with the <span class="hlt">decadal</span> variations of water content and stratification stability of the local atmosphere. The intensity of HREs in each sub-region is also characterized by strong <span class="hlt">decadal</span> <span class="hlt">variability</span>. The HRE intensity and frequency co-vary on the long-term trend, and show consistent <span class="hlt">variability</span> over NEC, NC, and YR, but inconsistent <span class="hlt">variability</span> over SC and HR. Further analysis of the relationships between the annual rainfall and HRE frequency as well as intensity indicates that the HRE frequency is the major contributor to the total rainfall <span class="hlt">variability</span> in eastern China, while the HRE intensity shows only relative weak contribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.B52C..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.B52C..03B"><span>Can we reconcile our understanding of the atmospheric methane budget over the past <span class="hlt">decades</span> with atmospheric <span class="hlt">observations</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bruhwiler, L. M.; Matthews, E.</p> <p>2007-12-01</p> <p>The balance of methane in the atmosphere is determined by surface emission, and losses due to uptake in soils and reaction with the hydroxyl radical. The atmospheric abundance of methane has risen by about a factor of three since pre-industrial times, but the growth rate has decreased substantially since the 1990's. Thus, global atmospheric methane appears to have equilibrated to around 1780 ppb subject to considerable interannual <span class="hlt">variability</span>, the causes of which are not well-understood. Methane emissions are expected to increase in the future due to increases in fossil fuel use and possible changes in wetlands at high-latitudes, and it is therefore important to test our understanding of the methane budget over the last two <span class="hlt">decades</span> against network <span class="hlt">observations</span> of atmospheric methane. Issues of interest are whether we can match the rise in methane over the 1980's, whether we can explain the decrease in growth rate during the 1990's, and whether we are able to simulate the <span class="hlt">observed</span> interannual <span class="hlt">variability</span> in the <span class="hlt">observations</span>. We will show results from a multi-<span class="hlt">decade</span> model simulation using analyzed meteorology from the ERA-40 reanalysis over this period. New times series of methane sources for 1980 through the early 2000's are used in the simulation. Anthropogenic sources include fossil fuels with a total of 7 fuel-process emission combinations associated with mining, processing, transport and distribution of coal, natural gas and oil; ruminant animals and manure based on regionally-representative profiles of bovine populations ; landfills including the impact of on- site methane capture; and irrigated rice cultivation based on seasonal rice-cropping calendars. Natural sources we include are biomass burning from the GFED emission data base, oceans, termites, and natural wetlands using a multiple-regression model derived from a process-based model. If time permits, we will also show preliminary results of a methane data assimilation using the Cooperative Air</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC11C0752P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC11C0752P"><span>Defining Essential Biodiversity <span class="hlt">Variables</span> (EBVs) as a contribution to Essential Ocean <span class="hlt">Variables</span> (EOVs): A Core Task of the Marine Biodiversity <span class="hlt">Observation</span> Network (MBON) to Accelerate Integration of Biological <span class="hlt">Observations</span> in the Global Ocean <span class="hlt">Observing</span> System (GOOS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pearlman, J.; Muller-Karger, F. E.; Sousa Pinto, I.; Costello, M. J.; Duffy, J. E.; Appeltans, W.; Fischer, A. S.; Canonico, G.; Klein, E.; Obura, D.; Montes, E.; Miloslavich, P.; Howard, M.</p> <p>2017-12-01</p> <p>The Marine Biodiversity <span class="hlt">Observation</span> Network (MBON) is a networking effort under the umbrella of the Group on Earth <span class="hlt">Observations</span> Biodiversity <span class="hlt">Observation</span> Network (GEO BON). The objective of the MBON is to link existing groups engaged in ocean <span class="hlt">observation</span> and help define practical indices to deploy in an operational manner to track changes in the number of marine species, the abundance and biomass of marine organisms, the diverse interactions between organisms and the environment, and the <span class="hlt">variability</span> and change of specific habitats of interest. MBON serves as the biodiversity arm of Blue Planet, the initiative of the Group on Earth <span class="hlt">Observations</span> (GEO) for the benefit of society. The Global Ocean <span class="hlt">Observing</span> System (GOOS) was established under the auspices of the Intergovernmental Oceanographic Commission (IOC) in 1991 to organize international ocean <span class="hlt">observing</span> efforts. The mission of the GOOS is to support monitoring to improve the management of marine and coastal ecosystems and resources, and to enable scientific research. GOOS is engaged in a continuing, rigorous process of identifying Essential Ocean <span class="hlt">Variables</span> (EOVs). MBON is working with GOOS and the Ocean Biogeographic Information System (OBIS, also under the IOC) to define Essential Biodiversity <span class="hlt">Variables</span> (EBVs) as those Essential Ocean <span class="hlt">Variables</span> (EOVs) that have explicit taxonomic records associated with them. For practical purposes, EBVs are a subset of the EOVs. The focus is to promote the integration of biological EOVs including EBVs into the existing and planned national and international ocean <span class="hlt">observing</span> systems. The definition avoids a proliferation of 'essential' <span class="hlt">variables</span> across multiple organizations. MBON will continue to advance practical and wide use of EBVs and related EOV. This is an effective way to contribute to several UN assessments (e.g., from IPBES, IPCC, and the World Ocean Assessment under the UN Regular Process), UN Sustainable Development Goals, and to address targets and goals defined under</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014HydJ...22.1825H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014HydJ...22.1825H"><span>Watershed-scale response of groundwater recharge to inter-annual and inter-<span class="hlt">decadal</span> <span class="hlt">variability</span> in precipitation (Alberta, Canada)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hayashi, Masaki; Farrow, Christopher R.</p> <p>2014-12-01</p> <p>Groundwater recharge sets a constraint on aquifer water balance in the context of water management. Historical data on groundwater and other relevant hydrological processes can be used to understand the effects of climatic <span class="hlt">variability</span> on recharge, but such data sets are rare. The climate of the Canadian prairies is characterized by large inter-annual and inter-<span class="hlt">decadal</span> <span class="hlt">variability</span> in precipitation, which provides opportunities to examine the response of groundwater recharge to changes in meteorological conditions. A <span class="hlt">decadal</span> study was conducted in a small (250 km2) prairie watershed in Alberta, Canada. Relative magnitude of annual recharge, indicated by water-level rise, was significantly correlated with a combination of growing-season precipitation and snowmelt runoff, which drives depression-focussed infiltration of meltwater. Annual precipitation was greater than vapour flux at an experimental site in some years and smaller in other years. On average precipitation minus vapour flux was 10 mm y-1, which was comparable to the magnitude of watershed-scale groundwater recharge estimated from creek baseflow. Average baseflow showed a distinct shift from a low value (4 mm y-1) in 1982-1995 to a high value (15 mm y-1) in 2003-2013, indicating the sensitivity of groundwater recharge to a <span class="hlt">decadal</span>-scale <span class="hlt">variability</span> of meteorological conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1030607','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1030607"><span>Towards the Prediction of <span class="hlt">Decadal</span> to Centennial Climate Processes in the Coupled Earth System Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Liu, Zhengyu; Kutzbach, J.; Jacob, R.</p> <p>2011-12-05</p> <p>In this proposal, we have made major advances in the understanding of <span class="hlt">decadal</span> and long term climate <span class="hlt">variability</span>. (a) We performed a systematic study of multidecadal climate <span class="hlt">variability</span> in FOAM-LPJ and CCSM-T31, and are starting exploring <span class="hlt">decadal</span> <span class="hlt">variability</span> in the IPCC AR4 models. (b) We develop several novel methods for the assessment of climate feedbacks in the <span class="hlt">observation</span>. (c) We also developed a new initialization scheme DAI (Dynamical Analogue Initialization) for ensemble <span class="hlt">decadal</span> prediction. (d) We also studied climate-vegetation feedback in the <span class="hlt">observation</span> and models. (e) Finally, we started a pilot program using Ensemble Kalman Filter in CGCM for decadalmore » climate prediction.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170005493','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170005493"><span>Reconciling Land-Ocean Moisture Transport <span class="hlt">Variability</span> in Reanalyses with P-ET in <span class="hlt">Observationally</span>-Driven Land Surface Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robertson, Franklin R.; Bosilovich, Michael G.; Roberts, Jason B.</p> <p>2016-01-01</p> <p>Vertically integrated atmospheric moisture transport from ocean to land [vertically integrated atmospheric moisture flux convergence (VMFC)] is a dynamic component of the global climate system but remains problematic in atmospheric reanalyses, with current estimates having significant multidecadal global trends differing even in sign. Continual evolution of the global <span class="hlt">observing</span> system, particularly stepwise improvements in satellite <span class="hlt">observations</span>, has introduced discrete changes in the ability of data assimilation to correct systematic model biases, manifesting as nonphysical <span class="hlt">variability</span>. Land surface models (LSMs) forced with <span class="hlt">observed</span> precipitation P and near-surface meteorology and radiation provide estimates of evapotranspiration (ET). Since <span class="hlt">variability</span> of atmospheric moisture storage is small on interannual and longer time scales, VMFC equals P minus ET is a good approximation and LSMs can provide an alternative estimate. However, heterogeneous density of rain gauge coverage, especially the sparse coverage over tropical continents, remains a serious concern. Rotated principal component analysis (RPCA) with prefiltering of VMFC to isolate the artificial <span class="hlt">variability</span> is used to investigate artifacts in five reanalysis systems. This procedure, although ad hoc, enables useful VMFC corrections over global land. The P minus ET estimates from seven different LSMs are evaluated and subsequently used to confirm the efficacy of the RPCA-based adjustments. Global VMFC trends over the period 1979-2012 ranging from 0.07 to minus 0.03 millimeters per day per <span class="hlt">decade</span> are reduced by the adjustments to 0.016 millimeters per day per <span class="hlt">decade</span>, much closer to the LSM P minus ET estimate (0.007 millimeters per day per <span class="hlt">decade</span>). Neither is significant at the 90 percent level. ENSO (El Nino-Southern Oscillation)-related modulation of VMFC and P minus ET remains the largest global interannual signal, with mean LSM and adjusted reanalysis time series correlating at 0.86.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.H32F..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.H32F..02H"><span>Climate-informed stochastic hydrological modeling: Incorporating <span class="hlt">decadal</span>-scale <span class="hlt">variability</span> using paleoclimate data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Henley, B. J.; Thyer, M. A.; Kuczera, G. A.</p> <p>2012-12-01</p> <p>A hierarchical framework for incorporating modes of climate <span class="hlt">variability</span> into stochastic simulations of hydrological data is developed, termed the climate-informed multi-time scale stochastic (CIMSS) framework. To characterize long-term <span class="hlt">variability</span> for the first level of the hierarchy, paleoclimate and instrumental data describing the Interdecadal Pacific Oscillation (IPO) and the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) are analyzed. A new paleo IPO-PDO time series dating back 440 yrs is produced, combining seven IPO-PDO paleo sources using an objective smoothing procedure to fit low-pass filters to individual records. The paleo data analysis indicates that wet/dry IPO-PDO states have a broad range of run-lengths, with 90% between 3 and 33 yr and a mean of 15 yr. Model selection techniques were used to determine a suitable stochastic model to simulate these run-lengths. The Markov chain model, previously used to simulate oscillating wet/dry climate states, was found to underestimate the probability of wet/dry periods >5 yr, and was rejected in favor of a gamma distribution. For the second level of the hierarchy, a seasonal rainfall model is conditioned on the simulated IPO-PDO state. Application to two high-quality rainfall sites close to water supply reservoirs found that mean seasonal rainfall in the IPO-PDO dry state was 15%-28% lower than the wet state. The model was able to replicate <span class="hlt">observed</span> statistics such as seasonal and multi-year accumulated rainfall distributions and interannual autocorrelations for the case study sites. In comparison, an annual lag-one autoregressive AR(1) model was unable to adequately capture the <span class="hlt">observed</span> rainfall distribution within separate IPO-PDO states. Furthermore, analysis of the impact of the CIMSS framework on drought risk analysis found that short-term drought risks conditional on IPO/PDO state were considerably higher than the traditional AR(1) model.hort-term conditional water supply drought risks for the CIMSS and AR(1) models</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28376345','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28376345"><span>The effect of modeled absolute timing <span class="hlt">variability</span> and relative timing <span class="hlt">variability</span> on <span class="hlt">observational</span> learning.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grierson, Lawrence E M; Roberts, James W; Welsher, Arthur M</p> <p>2017-05-01</p> <p>There is much evidence to suggest that skill learning is enhanced by skill <span class="hlt">observation</span>. Recent research on this phenomenon indicates a benefit of <span class="hlt">observing</span> <span class="hlt">variable/erred</span> demonstrations. In this study, we explore whether it is <span class="hlt">variability</span> within the relative organization or absolute parameterization of a movement that facilitates skill learning through <span class="hlt">observation</span>. To do so, participants were randomly allocated into groups that <span class="hlt">observed</span> a model with no <span class="hlt">variability</span>, absolute timing <span class="hlt">variability</span>, relative timing <span class="hlt">variability</span>, or <span class="hlt">variability</span> in both absolute and relative timing. All participants performed a four-segment movement pattern with specific absolute and relative timing goals prior to and following the <span class="hlt">observational</span> intervention, as well as in a 24h retention test and transfers tests that featured new relative and absolute timing goals. Absolute timing error indicated that all groups initially acquired the absolute timing, maintained their performance at 24h retention, and exhibited performance deterioration in both transfer tests. Relative timing error revealed that the <span class="hlt">observation</span> of no <span class="hlt">variability</span> and relative timing <span class="hlt">variability</span> produced greater performance at the post-test, 24h retention and relative timing transfer tests, but for the no <span class="hlt">variability</span> group, deteriorated at absolute timing transfer test. The results suggest that the learning of absolute timing following <span class="hlt">observation</span> unfolds irrespective of model <span class="hlt">variability</span>. However, the learning of relative timing benefits from holding the absolute features constant, while the <span class="hlt">observation</span> of no <span class="hlt">variability</span> partially fails in transfer. We suggest learning by <span class="hlt">observing</span> no <span class="hlt">variability</span> and <span class="hlt">variable/erred</span> models unfolds via similar neural mechanisms, although the latter benefits from the additional coding of information pertaining to movements that require a correction. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........45D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........45D"><span>On the <span class="hlt">variability</span> of Pacific Ocean tides at seasonal to <span class="hlt">decadal</span> time scales: <span class="hlt">Observed</span> vs modelled</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Devlin, Adam Thomas</p> <p></p> <p> forward in time to the predicted sea level in 2100. Results suggest that stations with large positive combined A-TATs produce total water levels that are greater than those predicted by an increase in MSL alone, increasing the chances of high-water events. Part II examines the mechanisms behind the yearly (TAT) <span class="hlt">variability</span> in the Western Tropical Pacific Ocean. Significant amplitude TATs are found at more than half of 26 gauges for each of the two strongest tidal constituents, K1 (diurnal) and M2 (semidiurnal). For the lesser constituents analyzed (O1 and S2), significant trends are <span class="hlt">observed</span> at ten gauges. Part III analyzes the seasonal behavior of tides (STATs) at twenty tide gauges in the Southeast Asian waters, which exhibit variation by 10 -- 30% of mean tidal amplitudes. A barotropic ocean tide model that considers the seasonal effects of MSL, stratification, and geostrophic and Ekman velocity is used to explain the <span class="hlt">observed</span> seasonal <span class="hlt">variability</span> in tides due to variations in monsoon-influenced climate forcing, with successful results at about half of all gauges. The <span class="hlt">observed</span> changes in tides are best explained by the influence of non-tidal velocities (geostrophic and Ekman), though the effect of changing stratification is also an important secondary causative mechanism. From the results of these surveys and investigations, it is concluded that short-term fluctuations in MSL and tidal properties at multiple time scales may be as important in determining the state of future water levels as the long-term trends. Global explanations for the <span class="hlt">observed</span> tidal behavior have not been found in this study; however, significant regional explanations are found at the yearly time scale in the Solomon Sea, and at the seasonal time scale in Southeast Asia. It is likely that tidal sensitivity to annual and seasonal variations in MSL at other locations also are driven by locally specific processes, rather than factors with basin-wide coherence. (Abstract shortened by ProQuest.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GPC...162..252M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GPC...162..252M"><span><span class="hlt">Observed</span> climate <span class="hlt">variability</span> over Chad using multiple <span class="hlt">observational</span> and reanalysis datasets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maharana, Pyarimohan; Abdel-Lathif, Ahmat Younous; Pattnayak, Kanhu Charan</p> <p>2018-03-01</p> <p>Chad is the largest of Africa's landlocked countries and one of the least studied region of the African continent. The major portion of Chad lies in the Sahel region, which is known for its rapid climate change. In this study, multiple <span class="hlt">observational</span> datasets are analyzed from 1950 to 2014, in order to examine the trend of precipitation and temperature along with their <span class="hlt">variability</span> over Chad to understand possible impacts of climate change over this region. Trend analysis of the climatic fields has been carried out using Mann-Kendall test. The precipitation over Chad is mostly contributed during summer by West African Monsoon, with maximum northward limit of 18° N. The Atlantic Ocean as well as the Mediterranean Sea are the major source of moisture for the summer rainfall over Chad. Based on the rainfall time series, the entire study period has been divided in to wet (1950 to 1965), dry (1966 to 1990) and recovery period (1991 to 2014). The rainfall has decreased drastically for almost 3 <span class="hlt">decades</span> during the dry period resulted into various drought years. The temperature increases at a rate of 0.15 °C/<span class="hlt">decade</span> during the entire period of analysis. The seasonal rainfall as well as temperature plays a major role in the change of land use/cover. The decrease of monsoon rainfall during the dry period reduces the C4 cover drastically; this reduction of C4 grass cover leads to increase of C3 grass cover. The slow revival of rainfall is still not good enough for the increase of shrub cover but it favors the gradual reduction of bare land over Chad.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50.1129S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50.1129S"><span><span class="hlt">Observed</span> modes of sea surface temperature <span class="hlt">variability</span> in the South Pacific region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saurral, Ramiro I.; Doblas-Reyes, Francisco J.; García-Serrano, Javier</p> <p>2018-02-01</p> <p>The South Pacific (SP) region exerts large control on the climate of the Southern Hemisphere at many times scales. This paper identifies the main modes of interannual sea surface temperature (SST) <span class="hlt">variability</span> in the SP which consist of a tropical-driven mode related to a horseshoe structure of positive/negative SST anomalies within midlatitudes and highly correlated to ENSO and Interdecadal Pacific Oscillation (IPO) <span class="hlt">variability</span>, and another mode mostly confined to extratropical latitudes which is characterized by zonal propagation of SST anomalies within the South Pacific Gyre. Both modes are associated with temperature and rainfall anomalies over the continental regions of the Southern Hemisphere. Besides the leading mode which is related to well known warmer/cooler and drier/moister conditions due to its relationship with ENSO and the IPO, an inspection of the extratropical mode indicates that it is associated with distinct patterns of sea level pressure and surface temperature advection. These relationships are used here as plausible and partial explanations to the <span class="hlt">observed</span> warming trend <span class="hlt">observed</span> within the Southern Hemisphere during the last <span class="hlt">decades</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC32B..07J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC32B..07J"><span>A preindustrial to present record of SST from Darwin Island, Galápagos: constraining Eastern Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jimenez, G.; Cole, J. E.; Vetter, L.; Thompson, D. M.; Tudhope, A. W.</p> <p>2017-12-01</p> <p>Climate reconstructions from sub-seasonally resolved corals have greatly enhanced our understanding of climate <span class="hlt">variability</span> related to the El Niño-Southern Oscillation (ENSO). However, few such records exist from the Eastern Pacific, which experiences the greatest ENSO-related variance in sea surface temperature (SST). Therefore, climate patterns and mechanisms in the region remain unclear, particularly on <span class="hlt">decadal</span> to multidecadal timescales. Here, we present a new, bimonthly-resolved δ18O-SST reconstruction from a Darwin Island coral, in the northern Galápagos archipelago. Comparison with Sr/Ca data from the same coral demonstrates that δ18O values in the core dominantly track SST, as is expected in areas with low-magnitude sea surface salinity changes such as the Galápagos. Spanning 2015 to approximately 1800 CE, our record thus represents the longest sub-seasonally resolved SST reconstruction bridging the pre-industrial era to the present day in the Eastern Pacific. This time span and resolution is ideal for identifying climatic processes on a range of timescales: the presence of modern data allows us to calibrate the record using satellite datasets, while several <span class="hlt">decades</span> of data preceding the onset of greenhouse warming enables comparison between natural and anthropogenic climate forcings. Together with other reconstructions from the region, we use the record to establish a baseline of (ENSO-related) Eastern Pacific interannual and <span class="hlt">decadal</span> <span class="hlt">variability</span> and assess evidence for climate emergence and trends. Preliminary evidence suggests increased <span class="hlt">decadal</span> <span class="hlt">variability</span> during the latter half of the twentieth century, as well as a secular warming trend of approximately 0.1°C/<span class="hlt">decade</span>, in agreement with other Eastern Pacific coral records. Finally, we explore the applications of coral δ13C values in reconstructing regional upwelling. Our record contributes to constraining the pre- to post-industrial climate history of the Eastern Pacific and provides insight into</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H52G..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H52G..07C"><span>A Robust Decision-Making Technique for Water Management under <span class="hlt">Decadal</span> Scale Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Callihan, L.; Zagona, E. A.; Rajagopalan, B.</p> <p>2013-12-01</p> <p>Robust decision making, a flexible and dynamic approach to managing water resources in light of deep uncertainties associated with climate <span class="hlt">variability</span> at inter-annual to <span class="hlt">decadal</span> time scales, is an analytical framework that detects when a system is in or approaching a vulnerable state. It provides decision makers the opportunity to implement strategies that both address the vulnerabilities and perform well over a wide range of plausible future scenarios. A strategy that performs acceptably over a wide range of possible future states is not likely to be optimal with respect to the actual future state. The degree of success--the ability to avoid vulnerable states and operate efficiently--thus depends on the skill in projecting future states and the ability to select the most efficient strategies to address vulnerabilities. This research develops a robust decision making framework that incorporates new methods of <span class="hlt">decadal</span> scale projections with selection of efficient strategies. Previous approaches to water resources planning under inter-annual climate <span class="hlt">variability</span> combining skillful seasonal flow forecasts with climatology for subsequent years are not skillful for medium term (i.e. <span class="hlt">decadal</span> scale) projections as decision makers are not able to plan adequately to avoid vulnerabilities. We address this need by integrating skillful <span class="hlt">decadal</span> scale streamflow projections into the robust decision making framework and making the probability distribution of this projection available to the decision making logic. The range of possible future hydrologic scenarios can be defined using a variety of nonparametric methods. Once defined, an ensemble projection of <span class="hlt">decadal</span> flow scenarios are generated from a wavelet-based spectral K-nearest-neighbor resampling approach using historical and paleo-reconstructed data. This method has been shown to generate skillful medium term projections with a rich variety of natural <span class="hlt">variability</span>. The current state of the system in combination with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMPP23C1424M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMPP23C1424M"><span>Holocene <span class="hlt">Decadal</span> to Multidecadal Hydrologic <span class="hlt">Variability</span> in the Everglades: Climate and Implications for Ecosystem Management</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moses, C. S.; Anderson, W. T.; Saunders, C.; Rebenack, C.</p> <p>2009-12-01</p> <p>The Florida Everglades are a complex, unique ecosystem. Adding to the complexity, a system of canals and gates control the flow of waters from central Florida southward into the Everglades, and ultimately Florida Bay and the Gulf of Mexico. With south Florida’s distinct wet and dry seasons, the hydrology has driven ecosystem evolution over the last 4-5 kya. However, since the 1920s the water content of the Everglades has largely been anthropogenically modulated, with the exception of the natural <span class="hlt">variability</span> of evaporation and precipitation over the large area south of the Tamiami Trail. Because of the incredibly flat nature of the Everglades, small changes in the freshwater balance have substantial impacts on the diversity and distribution of organisms. <span class="hlt">Decadal</span> and multidecadal <span class="hlt">variability</span> in precipitation, hurricane incidence, and sea level rise all have important effects on the ecosystem. During the instrumental record, the natural precipitation across south Florida has been strongly influenced by combinations of the Atlantic Multidecadal Oscillation, Pacific <span class="hlt">Decadal</span> Oscillation, and ENSO. Here we discuss evidence of natural climate <span class="hlt">variability</span> impacts on the ecosystem beyond the anthropogenic hydrological controls. Proxy environmental data from seeds, charcoal, and trees, plus the sparse, but available, instrumental records provide evidence of changes in the ecosystem over the Holocene, and suggest considerations for future management.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020194','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020194"><span>Mesoscale disturbance and ecological response to <span class="hlt">decadal</span> climatic <span class="hlt">variability</span> in the American Southwest</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Swetnam, T.W.; Betancourt, J.L.</p> <p>1998-01-01</p> <p>Ecological responses to climatic <span class="hlt">variability</span> in the Southwest include regionally synchronized fires, insect outbreaks, and pulses in tree demography (births and deaths). Multicentury, tree-ring reconstructions of drought, disturbance history, and tree demography reveal climatic effects across scales, from annual to <span class="hlt">decadal</span>, and from local (<102 km2) to mesoscale (104-106 km2). Climate-disturbance relations are more <span class="hlt">variable</span> and complex than previously assumed. During the past three centuries, mesoscale outbreaks of the western spruce budworm (Choristoneura occidentalis) were associated with wet, not dry episodes, contrary to conventional wisdom. Regional fires occur during extreme droughts but, in some ecosystems, antecedent wet conditions play a secondary role by regulating accumulation of fuels. Interdecadal changes in fire-climate associations parallel other evidence for shifts in the frequency or amplitude of the Southern Oscillation (SO) during the past three centuries. High interannual, fire-climate correlations (r = 0.7 to 0.9) during specific <span class="hlt">decades</span> (i.e., circa 1740-80 and 1830-60) reflect periods of high amplitude in the SO and rapid switching from extreme wet to dry years in the Southwest, thereby entraining fire occurrence across the region. Weak correlations from 1780 to 1830 correspond with a decrease in SO frequency or amplitude inferred from independent tree-ring width, ice core, and coral isotope reconstructions. Episodic dry and wet episodes have altered age structures and species composition of woodland and conifer forests. The scarcity of old, living conifers established before circa 1600 suggests that the extreme drought of 1575-95 had pervasive effects on tree populations. The most extreme drought of the past 400 years occurred in the mid-twentieth century (1942-57). This drought resulted in broadscale plant dieoffs in shrublands, woodlands, and forests and accelerated shrub invasion of grasslands. Drought conditions were broken by the post</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913099B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913099B"><span><span class="hlt">Observing</span> atmospheric blocking with GPS radio occultation - one <span class="hlt">decade</span> of measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunner, Lukas; Steiner, Andrea</p> <p>2017-04-01</p> <p>Atmospheric blocking has received a lot of attention in recent years due to its impact on mid-latitude circulation and subsequently on weather extremes such as cold and warm spells. So far blocking studies have been based mainly on re-analysis data or model output. However, it has been shown that blocking frequency exhibits considerable inter-model spread in current climate models. Here we use one <span class="hlt">decade</span> (2006 to 2016) of satellite-based <span class="hlt">observations</span> from GPS radio occultation (RO) to analyze blocking in RO data building on work by Brunner et al. (2016). Daily fields on a 2.5°×2.5° longitude-latitude grid are calculated by applying an adequate gridding strategy to the RO measurements. For blocking detection we use a standard blocking detection algorithm based on 500 hPa geopotential height (GPH) gradients. We investigate vertically resolved atmospheric <span class="hlt">variables</span> such as GPH, temperature, and water vapor before, during, and after blocking events to increase process understanding. Moreover, utilizing the coverage of the RO data set, we investigate global blocking frequencies. The main blocking regions in the northern and southern hemisphere are identified and the (vertical) atmospheric structure linked to blocking events is compared. Finally, an inter-comparison of results from RO data to different re-analyses, such as ERA-Interim, MERRA 2, and JRA-55, is presented. Brunner, L., A. K. Steiner, B. Scherllin-Pirscher, and M. W. Jury (2016): Exploring atmospheric blocking with GPS radio occultation <span class="hlt">observations</span>. Atmos. Chem. Phys., 16, 4593-4604, doi:10.5194/acp-16-4593-2016.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.6793F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.6793F"><span><span class="hlt">Decadal</span> covariability of Atlantic SSTs and western Amazon dry-season hydroclimate in <span class="hlt">observations</span> and CMIP5 simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernandes, Katia; Giannini, Alessandra; Verchot, Louis; Baethgen, Walter; Pinedo-Vasquez, Miguel</p> <p>2015-08-01</p> <p>The unusual severity and return time of the 2005 and 2010 dry-season droughts in western Amazon is attributed partly to <span class="hlt">decadal</span> climate fluctuations and a modest drying trend. <span class="hlt">Decadal</span> <span class="hlt">variability</span> of western Amazon hydroclimate is highly correlated to the Atlantic sea surface temperature (SST) north-south gradient (NSG). Shifts of dry and wet events frequencies are also related to the NSG phase, with a 66% chance of 3+ years of dry events per <span class="hlt">decade</span> when NSG > 0 and 19% when NSG < 0. The western Amazon and NSG <span class="hlt">decadal</span> covariability is well reproduced in general circulation models (GCMs) historical (HIST) and preindustrial control (PIC) experiments of the Coupled Model Intercomparison Project Phase 5 (CMIP5). The HIST and PIC also reproduce the shifts in dry and wet events probabilities, indicating potential for <span class="hlt">decadal</span> predictability based on GCMs. Persistence of the current NSG positive phase favors above normal frequency of western Amazon dry events in coming <span class="hlt">decades</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3885547','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3885547"><span>Coral Luminescence Identifies the Pacific <span class="hlt">Decadal</span> Oscillation as a Primary Driver of River Runoff <span class="hlt">Variability</span> Impacting the Southern Great Barrier Reef</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rodriguez-Ramirez, Alberto; Grove, Craig A.; Zinke, Jens; Pandolfi, John M.; Zhao, Jian-xin</p> <p>2014-01-01</p> <p>The Pacific <span class="hlt">Decadal</span> Oscillation (PDO) is a large-scale climatic phenomenon modulating ocean-atmosphere <span class="hlt">variability</span> on <span class="hlt">decadal</span> time scales. While precipitation and river flow <span class="hlt">variability</span> in the Great Barrier Reef (GBR) catchments are sensitive to PDO phases, the extent to which the PDO influences coral reefs is poorly understood. Here, six Porites coral cores were used to produce a composite record of coral luminescence <span class="hlt">variability</span> (runoff proxy) and identify drivers of terrestrial influence on the Keppel reefs, southern GBR. We found that coral skeletal luminescence effectively captured seasonal, inter-annual and <span class="hlt">decadal</span> <span class="hlt">variability</span> of river discharge and rainfall from the Fitzroy River catchment. Most importantly, although the influence of El Niño-Southern Oscillation (ENSO) events was evident in the luminescence records, the <span class="hlt">variability</span> in the coral luminescence composite record was significantly explained by the PDO. Negative luminescence anomalies (reduced runoff) were associated with El Niño years during positive PDO phases while positive luminescence anomalies (increased runoff) coincided with strong/moderate La Niña years during negative PDO phases. This study provides clear evidence that not only ENSO but also the PDO have significantly affected runoff regimes at the Keppel reefs for at least a century, and suggests that upcoming hydrological disturbances and ecological responses in the southern GBR region will be mediated by the future evolution of these sources of climate <span class="hlt">variability</span>. PMID:24416214</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24416214','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24416214"><span>Coral luminescence identifies the Pacific <span class="hlt">Decadal</span> Oscillation as a primary driver of river runoff <span class="hlt">variability</span> impacting the southern Great Barrier Reef.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rodriguez-Ramirez, Alberto; Grove, Craig A; Zinke, Jens; Pandolfi, John M; Zhao, Jian-xin</p> <p>2014-01-01</p> <p>The Pacific <span class="hlt">Decadal</span> Oscillation (PDO) is a large-scale climatic phenomenon modulating ocean-atmosphere <span class="hlt">variability</span> on <span class="hlt">decadal</span> time scales. While precipitation and river flow <span class="hlt">variability</span> in the Great Barrier Reef (GBR) catchments are sensitive to PDO phases, the extent to which the PDO influences coral reefs is poorly understood. Here, six Porites coral cores were used to produce a composite record of coral luminescence <span class="hlt">variability</span> (runoff proxy) and identify drivers of terrestrial influence on the Keppel reefs, southern GBR. We found that coral skeletal luminescence effectively captured seasonal, inter-annual and <span class="hlt">decadal</span> <span class="hlt">variability</span> of river discharge and rainfall from the Fitzroy River catchment. Most importantly, although the influence of El Niño-Southern Oscillation (ENSO) events was evident in the luminescence records, the <span class="hlt">variability</span> in the coral luminescence composite record was significantly explained by the PDO. Negative luminescence anomalies (reduced runoff) were associated with El Niño years during positive PDO phases while positive luminescence anomalies (increased runoff) coincided with strong/moderate La Niña years during negative PDO phases. This study provides clear evidence that not only ENSO but also the PDO have significantly affected runoff regimes at the Keppel reefs for at least a century, and suggests that upcoming hydrological disturbances and ecological responses in the southern GBR region will be mediated by the future evolution of these sources of climate <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThApC.tmp..444I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThApC.tmp..444I"><span><span class="hlt">Variability</span>, trends, and teleconnections of <span class="hlt">observed</span> precipitation over Pakistan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iqbal, Muhammad Farooq; Athar, H.</p> <p>2017-10-01</p> <p>The precipitation <span class="hlt">variability</span>, trends, and teleconnections are studied over six administrative regions of Pakistan (Gilgit-Baltistan or GB, Azad Jammu and Kashmir or AJK, Khyber Pakhtoonkhawa or KPK, Punjab, Sindh, and Balochistan) on multiple timescales for the period of recent 38 years (1976-2013) using precipitation data of 42 stations and circulation indices datasets (Indian Ocean Dipole [IOD], North Atlantic Oscillation [NAO], Arctic Oscillation [AO], El Niño Southern Oscillation [ENSO], Pacific <span class="hlt">Decadal</span> Oscillation [PDO], Atlantic Multidecadal Oscillation [AMO], and Quasi-Biennial Oscillation [QBO]). The summer monsoon season received the highest precipitation, amounting to 45%, whereas the winter and pre-monsoon (post-monsoon) seasons contributed 30 and 20% (5%), respectively, of the annual total precipitation. Positive percentile changes were <span class="hlt">observed</span> in GB, KPK, Punjab, and Balochistan regions during pre-monsoon season and in Balochistan region during post-monsoon season in second half as compared to first half of 38-year period. The Mann-Kendall test revealed increasing trends for the period of 1995-2013 as compared to period of 1976-1994 for entire Pakistan during monsoon season and on annual timescale. A significant influence of ENSO was <span class="hlt">observed</span> in all the four seasons in Balochistan, KPK, Punjab, and AJK regions during monsoon and post-monsoon seasons. This study not only offers an understanding of precipitation <span class="hlt">variability</span> linkages with large-scale circulations and trends, but also it contributes as a resource document for policy makers to take measures for adaptation and mitigation of climate change and its impacts with special focus on precipitation over different administrative regions of Pakistan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A41N..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A41N..04H"><span><span class="hlt">Observed</span> and simulated changes in Antarctic sea ice and sea level pressure: anthropogenic or natural <span class="hlt">variability</span>? (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hobbs, W. R.</p> <p>2013-12-01</p> <p>Statistically-significant changes in Antarctic sea ice cover and the overlying atmosphere have been <span class="hlt">observed</span> over the last 30 years, but there is an open question of whether these changes are due to multi-<span class="hlt">decadal</span> natural <span class="hlt">variability</span> or an anthropogenically-forced response. A number of recent papers have shown that the slight increase in total sea ice cover is within the bounds of internal <span class="hlt">variability</span> exhibited by coupled climate models in the CMIP5 suite. Modelled changes for the same time period generally show a decrease, but again with a magnitude that is within internal <span class="hlt">variability</span>. However, in contrast to the Arctic, sea ice tends in the Antarctic are spatially highly heterogeneous, and consideration of the total ice cover may mask important regional signals. In this work, a robust ';fingerprinting' approach is used to show that the <span class="hlt">observed</span> spatial pattern of sea ice trends is in fact outside simulated natural <span class="hlt">variability</span> in west Antarctic, and furthermore that the CMIP5 models consistently show decreased ice cover in the Ross and Weddell Seas, sectors which in fact have an <span class="hlt">observed</span> increase in cover. As a first step towards understanding the disagreement between models and <span class="hlt">observations</span>, modelled sea level pressure trends are analysed using and optimal fingerprinting approach, to identify whether atmospheric deficiencies in the models can explain the model-<span class="hlt">observation</span> discrepancy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41E..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41E..05D"><span>Multi-<span class="hlt">Decadal</span> Averages of Basal Melt for Ross Ice Shelf, Antarctica Using Airborne <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, I.; Bell, R. E.; Tinto, K. J.; Frearson, N.; Kingslake, J.; Padman, L.; Siddoway, C. S.; Fricker, H. A.</p> <p>2017-12-01</p> <p>Changes in ice shelf mass balance are key to the long term stability of the Antarctic Ice Sheet. Although the most extensive ice shelf mass loss currently is occurring in the Amundsen Sea sector of West Antarctica, many other ice shelves experience changes in thickness on time scales from annual to ice age cycles. Here, we focus on the Ross Ice Shelf. An 18-year record (1994-2012) of satellite radar altimetry shows substantial <span class="hlt">variability</span> in Ross Ice Shelf height on interannual time scales, complicating detection of potential long-term climate-change signals in the mass budget of this ice shelf. <span class="hlt">Variability</span> of radar signal penetration into the ice-shelf surface snow and firn layers further complicates assessment of mass changes. We investigate Ross Ice Shelf mass balance using aerogeophysical data from the ROSETTA-Ice surveys using IcePod. We use two ice-penetrating radars; a 2 GHz unit that images fine-structure in the upper 400 m of the ice surface and a 360 MHz radar to identify the ice shelf base. We have identified internal layers that are continuous along flow from the grounding line to the ice shelf front. Based on layer continuity, we conclude that these layers must be the horizons between the continental ice of the outlet glaciers and snow accumulation once the ice is afloat. We use the Lagrangian change in thickness of these layers, after correcting for strain rates derived using modern day InSAR velocities, to estimate multidecadal averaged basal melt rates. This method provides a novel way to quantify basal melt, avoiding the confounding impacts of spatial and short-timescale <span class="hlt">variability</span> in surface accumulation and firn densification processes. Our estimates show elevated basal melt rates (> -1m/yr) around Byrd and Mullock glaciers within 100 km from the ice shelf front. We also compare modern InSAR velocity derived strain rates with estimates from the comprehensive ground-based RIGGS <span class="hlt">observations</span> during 1973-1978 to estimate the potential magnitude of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A41C2287C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41C2287C"><span>Long-term <span class="hlt">Observations</span> of Intense Precipitation Small-scale Spatial <span class="hlt">Variability</span> in a Semi-arid Catchment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cropp, E. L.; Hazenberg, P.; Castro, C. L.; Demaria, E. M.</p> <p>2017-12-01</p> <p>In the southwestern US, the summertime North American Monsoon (NAM) provides about 60% of the region's annual precipitation. Recent research using high-resolution atmospheric model simulations and retrospective predictions has shown that since the 1950's, and more specifically in the last few <span class="hlt">decades</span>, the mean daily precipitation in the southwestern U.S. during the NAM has followed a decreasing trend. Furthermore, days with more extreme precipitation have intensified. The current work focuses the impact of these long-term changes on the <span class="hlt">observed</span> small-scale spatial <span class="hlt">variability</span> of intense precipitation. Since limited long-term high-resolution <span class="hlt">observational</span> data exist to support such climatological-induced spatial changes in precipitation frequency and intensity, the current work utilizes <span class="hlt">observations</span> from the USDA-ARS Walnut Gulch Experimental Watershed (WGEW) in southeastern Arizona. Within this 150 km^2 catchment over 90 rain gauges have been installed since the 1950s, measuring at sub-hourly resolution. We have applied geospatial analyses and the kriging interpolation technique to identify long-term changes in the spatial and temporal correlation and anisotropy of intense precipitation. The <span class="hlt">observed</span> results will be compared with the previously model simulated results, as well as related to large-scale variations in climate patterns, such as the El Niño Southern Oscillation (ENSO) and the Pacific <span class="hlt">Decadal</span> Oscillation (PDO).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.5749K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.5749K"><span>Pronounced differences between <span class="hlt">observed</span> and CMIP5-simulated multidecadal climate <span class="hlt">variability</span> in the twentieth century</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kravtsov, Sergey</p> <p>2017-06-01</p> <p>Identification and dynamical attribution of multidecadal climate undulations to either variations in external forcings or to internal sources is one of the most important topics of modern climate science, especially in conjunction with the issue of human-induced global warming. Here we utilize ensembles of twentieth century climate simulations to isolate the forced signal and residual internal <span class="hlt">variability</span> in a network of <span class="hlt">observed</span> and modeled climate indices. The <span class="hlt">observed</span> internal <span class="hlt">variability</span> so estimated exhibits a pronounced multidecadal mode with a distinctive spatiotemporal signature, which is altogether absent in model simulations. This single mode explains a major fraction of model-data differences over the entire climate index network considered; it may reflect either biases in the models' forced response or models' lack of requisite internal dynamics, or a combination of both.<abstract type="synopsis"><title type="main">Plain Language SummaryGlobal and regional warming trends over the course of the twentieth century have been nonuniform, with <span class="hlt">decadal</span> and longer periods of faster or slower warming, or even cooling. Here we show that state-of-the-art global models used to predict climate fail to adequately reproduce such multidecadal climate variations. In particular, the models underestimate the magnitude of the <span class="hlt">observed</span> <span class="hlt">variability</span> and misrepresent its spatial pattern. Therefore, our ability to interpret the <span class="hlt">observed</span> climate change using these models is limited.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC32B..01P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC32B..01P"><span>Inability of CMIP5 Climate Models to Simulate Recent Multi-<span class="hlt">decadal</span> Climate Change in the Tropical Pacific.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Power, S.; Delage, F.; Kociuba, G.; Wang, G.; Smith, I.</p> <p>2017-12-01</p> <p><span class="hlt">Observed</span> 15-year surface temperature trends beginning 1998 or later have attracted a great deal of interest because of an apparent slowdown in the rate of global warming, and contrasts between climate model simulations and <span class="hlt">observations</span> of such trends. Many studies have addressed the statistical significance of these relatively short trends, whether they indicate a possible bias in models and the implications for global warming generally. Here we analyse historical and projected changes in 38 CMIP5 climate models. All of the models simulate multi-<span class="hlt">decadal</span> warming in the Pacific over the past half-century that exceeds <span class="hlt">observed</span> values. This stark difference cannot be fully explained by <span class="hlt">observed</span>, internal multi-<span class="hlt">decadal</span> climate <span class="hlt">variability</span>, even if allowance is made for an apparent tendency for models to underestimate internal multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> in the Pacific. We also show that CMIP5 models are not able to simulate the magnitude of the strengthening of the Walker Circulation over the past thirty years. Some of the reasons for these major shortcomings in the ability of models to simulate multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> in the Pacific, and the impact these findings have on our confidence in global 21st century projections, will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A41G0148Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A41G0148Y"><span>Climatic controls of the interannual to <span class="hlt">decadal</span> <span class="hlt">variability</span> in Saudi Arabian dust activity: Towards the development of a seasonal prediction tool</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Y.; Notaro, M.; Liu, Z.; Alkolibi, F.; Fadda, E.; Bakhrjy, F.</p> <p>2013-12-01</p> <p>Atmospheric dust significantly influences the climate system, as well as human life in Saudi Arabia. Skillful seasonal prediction of dust activity with climatic <span class="hlt">variables</span> will help prevent some negative social impacts of dust storms. Yet, the climatic regulators on Saudi Arabian dust activity remain largely unaddressed. Remote sensing and station <span class="hlt">observations</span> show consistent seasonal cycles in Saudi Arabian dust activity, which peaks in spring and summer. The climatic controls on springtime and summertime Saudi Arabian dust activity during 1975-2010 are studied using <span class="hlt">observational</span> and reanalysis data. Empirical Orthogonal Function (EOF) of the <span class="hlt">observed</span> Saudi Arabian dust storm frequency shows a dominant homogeneous pattern across the country, which has distinct interannual and <span class="hlt">decadal</span> variations, as revealed by the power spectrum. Regression and correlation analyses reveal that Saudi Arabian dust activity is largely tied to precipitation on the Arabian Peninsula in spring and northwesterly (Shamal) wind in summer. On the seasonal-interannual time scale, warm El Niño-Southern Oscillation (ENSO) phase (El Niño) in winter-to-spring inhibits spring dust activity by increasing the precipitation over the Rub'al Khali Desert, a major dust source region on the southern Arabian Peninsula; warm ENSO and warm Indian Ocean Basin Mode (IOBM) in winter-to-spring favor less summer dust activity by producing anomalously low sea-level pressure over eastern north Africa and Arabian Peninsula, which leads to the reduced Shamal wind speed. The <span class="hlt">decadal</span> variation in dust activity is likely associated with the Atlantic Multidecadal Oscillation (AMO), which impacts Sahel rainfall and North African dust, and likely dust transport to Saudi Arabia. The Pacific <span class="hlt">Decadal</span> Oscillation (PDO) and tropical Indian Ocean SST also have influence on the <span class="hlt">decadal</span> variation in Saudi Arabian dust activity, by altering precipitation over the Arabian Peninsula and summer Shamal wind speed. Using eastern</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8581O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8581O"><span>Mechanisms of <span class="hlt">decadal</span> <span class="hlt">variability</span> in the Labrador Sea and the wider North Atlantic in a high-resolution climate model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortega, Pablo; Robson, Jon; Sutton, Rowan; Andrews, Martin</p> <p>2017-04-01</p> <p>A necessary step before assessing the performance of <span class="hlt">decadal</span> predictions is the evaluation of the processes that bring memory to the climate system, both in climate models and <span class="hlt">observations</span>. These mechanisms are particularly relevant in the North Atlantic, where the ocean circulation, related to both the Subpolar Gyre and the Meridional Overturning Circulation (AMOC), is thought to be important for driving significant heat content anomalies. Recently, a rapid decline in <span class="hlt">observed</span> densities in the deep Labrador Sea has pointed to an ongoing slowdown of the AMOC strength taking place since the mid 90s, a decline also hinted by in-situ <span class="hlt">observations</span> from the RAPID array. This study explores the use of Labrador Sea densities as a precursor of the ocean circulation changes, by analysing a 300-year long simulation with the state-of-the-art coupled model HadGEM3-GC2. The major drivers of Labrador density <span class="hlt">variability</span> are investigated, and are characterised by three major contributions. First, the integrated effect of local surface heat fluxes, mainly driven by year-to-year changes in the North Atlantic Oscillation, which accounts for 62% of the total variance. Additionally, two multidecadal-to-centennial contributions from the Arctic are quantified; the first associated with freshwater exports via the East Greenland Current, and the second with changes in the Denmark Strait Overflow. Finally, evidence is shown that <span class="hlt">decadal</span> trends in Labrador Sea densities are followed by important atmospheric impacts. In particular, a delayed winter NAO response appears to be at play, providing a phase reversal mechanism for the Labrador Sea density changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThApC.tmp..262O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThApC.tmp..262O"><span><span class="hlt">Variability</span> of temperature properties over Kenya based on <span class="hlt">observed</span> and reanalyzed datasets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ongoma, Victor; Chen, Haishan; Gao, Chujie; Sagero, Phillip Obaigwa</p> <p>2017-08-01</p> <p>Updated information on trends of climate extremes is central in the assessment of climate change impacts. This work examines the trends in mean, diurnal temperature range (DTR), maximum and minimum temperatures, 1951-2012 and the recent (1981-2010) extreme temperature events over Kenya. The study utilized daily <span class="hlt">observed</span> and reanalyzed monthly mean, minimum, and maximum temperature datasets. The analysis was carried out based on a set of nine indices recommended by the Expert Team on Climate Change Detection and Indices (ETCCDI). The trend of the mean and the extreme temperature was determined using Mann-Kendall rank test, linear regression analysis, and Sen's slope estimator. December-February (DJF) season records high temperature while June-August (JJA) experiences the least temperature. The <span class="hlt">observed</span> rate of warming is + 0.15 °C/<span class="hlt">decade</span>. However, DTR does not show notable annual trend. Both seasons show an overall warming trend since the early 1970s with abrupt and significant changes happening around the early 1990s. The warming is more significant in the highland regions as compared to their lowland counterparts. There is increase variance in temperature. The percentage of warm days and warm nights is <span class="hlt">observed</span> to increase, a further affirmation of warming. This work is a synoptic scale study that exemplifies how seasonal and <span class="hlt">decadal</span> analyses, together with the annual assessments, are important in the understanding of the temperature <span class="hlt">variability</span> which is vital in vulnerability and adaptation studies at a local/regional scale. However, following the quality of <span class="hlt">observed</span> data used herein, there remains need for further studies on the subject using longer and more data to avoid generalizations made in this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010015246&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dtemperature%2Bvariability','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010015246&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dtemperature%2Bvariability"><span>Satellite <span class="hlt">Observed</span> <span class="hlt">Variability</span> in Antarctic and Arctic Surface Temperatures and Their Correlation to Open Water Areas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, Josefino C.; Zukor, Dorothy (Technical Monitor)</p> <p>2000-01-01</p> <p>Recent studies using meterological station data have indicated that global surface air temperature has been increasing at a rate of 0.05 K/<span class="hlt">decade</span>. Using the same set of data but for stations in the Antarctic and Arctic regions (>50 N) only, the increases in temperature were 0.08, and 0.22 K/<span class="hlt">decade</span>, when record lengths of 100 and 50 years, respectively, were used. To gain insights into the increasing rate of warming, satellite infrared and passive microwave <span class="hlt">observations</span> over the Arctic region during the last 20 years were processed and analyzed. The results show that during this period, the ice extent in the Antarctic has been increasing at the rate of 1.2% per <span class="hlt">decade</span> while the surface temperature has been decreasing at about 0.08 K per <span class="hlt">decade</span>. Conversely, in the Northern Hemisphere, the ice extent has been decreasing at a rate of 2.8% per <span class="hlt">decade</span>, while the surface temperatures have been increasing at the rate of 0.38 K per <span class="hlt">decade</span>. In the Antarctic, it is surprising that there is a short term trend of cooling during a global period of warming. Very large anomalies in open water areas in the Arctic were <span class="hlt">observed</span> especially in the western region, that includes the Beaufort Sea, where the <span class="hlt">observed</span> open water area was about 1x10(exp 6) sq km, about twice the average for the region, during the summer of 1998. In the eastern region, that includes the Laptev Sea, the area of open water was also abnormally large in the summer of 1995. Note that globally, the warmest and second warmest years in this century, were 1998 and 1995, respectively. The data, however, show large spatial <span class="hlt">variability</span> with the open water area distribution showing a cyclic periodicity of about ten years, which is akin to the North Atlantic and Arctic Oscillations. This was <span class="hlt">observed</span> in both western and eastern regions but with the phase of one lagging the other by about two years. This makes it difficult to interpret what the trends really mean. But although the record length of satellite data is still</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JSR....93..118F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JSR....93..118F"><span>High marsh foraminiferal assemblages' response to intra-<span class="hlt">decadal</span> and multi-<span class="hlt">decadal</span> precipitation <span class="hlt">variability</span>, between 1934 and 2010 (Minho, NW Portugal)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fatela, Francisco; Moreno, João; Leorri, Eduardo; Corbett, Reide</p> <p>2014-10-01</p> <p>Foraminiferal assemblages of Caminha tidal marshes have been studied since 2002 revealing a peculiar dominance of brackish species, such as Haplophragmoides manilaensis, Haplophragmoides wilberti, Haplophragmoides sp., Pseudothurammina limnetis and Trochamminita salsa/irregularis in the high marshes of the Minho and the Coura lower estuaries. The assemblage composition reflects low salinity conditions, despite the short distance to the estuarine mouth (~ 4 km). However, in May 2010, the presence of salt marsh species Trochammina inflata and Jadammina macrescens became very significant, likely a result of 5 consecutive dry years and a corresponding salinity rise in sediment pore water. Correspondence analysis (CA) groups the surface samples according to their marsh zone, showing a positive correlation with the submersion time of each sampling point. The brackish and normal salinity foraminiferal species appear separated in the CA. This <span class="hlt">observation</span> was applied to the top 10 cm of a high marsh sediment core that corresponds to the period of instrumental record of precipitation and river flow in the Minho region. We found that river flow strongly correlates with precipitation in the Lima and Minho basins. The longer precipitation record was, therefore, used to interpret the foraminiferal assemblages' <span class="hlt">variability</span>. Three main phases were distinguished along ca. 80 years of precipitation data: 1) negative anomalies from 1934 to 1957; 2) positive anomalies from 1958 to 1983; and 3) negative anomalies from 1984 to 2010. This last dryer period exhibits the precipitation maximum and the greatest amplitude of rainfall values. High marsh foraminifera reveals a fast response to these short-term shifts; low salinity species relative abundance increases when precipitation increases over several <span class="hlt">decades</span>, as well as in the same <span class="hlt">decade</span>, in the years of heavy rainfall of dryer periods. High marsh foraminifera records the increase of freshwater flooding and seepage by 1) decreasing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP51A1059P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP51A1059P"><span>Multi-<span class="hlt">decadal</span> <span class="hlt">Variability</span> of the Indian Monsoon Rainfall for the last 14 kyr</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panmei, C.; Pothuri, D.</p> <p>2017-12-01</p> <p>Precise reconstruction of Indian monsoon fluctuation events and <span class="hlt">variability</span> trends over the last 14 kyr has great implications for understanding the dynamics and possible forcing/feedback mechanisms associated with it. We have carried out high-resolution Indian monsoon <span class="hlt">variability</span> studies of multi-<span class="hlt">decadal</span> to sub-centennial timescales for the past 14 kyr through oxygen isotopes and Mg/Ca-derived sea surface temperatures (SST) from a western Bay of Bengal sediment core MD 161/17, using planktonic foraminifera Globigerinoides ruber. Indian summer monsoon (ISM) intensity was low during the Younger Dryas (YD) as evidenced by enriched δ18Osw coincides with a striking warming of 1.5°C. We <span class="hlt">observed</span> ISM intensification from 12-9 kyr, followed by a milder period from 9-7.2 kyr. ISM gradually weakened from 7.2-2.5 kyr, after which there were two very prominent shifts in both ISM and SST; abrupt decrease at 2.4 kyr and increase at 1.4 kyr for ISM, while SST exhibited opposite trend. The contrasting trend continued from 1.4 kyr to the present wherein ISM precipitation has been decreasing and SST has been increasing. In addition, spectral analysis was done using Redfit and the ISM precipitation records reveal statistically significant periodicities at 2118, 411, 344, 144, 101 and 90 yrs. Furthermore, we compared our results with other existing records from the Northern Indian Ocean and adjacent regions, and found that the records share similarities suggesting regional dynamics being expressed coherently. Our results suggest that ISM precipitation and warming/cooling of the Northern Indian Ocean is directly associated with the southward/northward shift of the Intertropical Convergence Zone, which in turn is influenced by Atlantic Meridional Overturning Circulation, North Atlantic climate, and solar insolation interplaying differently at different timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A11L0169S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A11L0169S"><span>Evidence of the Atlantic Multidecadal Oscillation driving multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of summertime surface air quality in the eastern United States: Implications for air quality management in the coming <span class="hlt">decades</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shen, L.; Mickley, L. J.</p> <p>2016-12-01</p> <p>Atlantic sea surface temperatures have a significant influence on the summertime meteorology and air quality in the eastern United States. In this study, we investigate the effect of the Atlantic Multidecadal Oscillation (AMO) on two key air pollutants, surface ozone and PM2.5, over the eastern United States. The shift of AMO from cold to warm phase increases surface air temperatures by 0.5 K across the East and reduces precipitation, resulting in a warmer and drier summer. By applying <span class="hlt">observed</span>, present-day relationships between these pollutants and meteorological <span class="hlt">variables</span> to a variety of <span class="hlt">observations</span> and historical reanalysis datasets, we calculate the impacts of AMO on U.S. air quality. Our study reveals a multidecadal <span class="hlt">variability</span> in mean summertime (JJA) maximum daily 8-hour (MDA8) ozone and surface PM2.5 concentrations in the eastern United States. In one-half cycle ( 30 years) of the AMO from negative to positive phase with constant anthropogenic emissions, JJA MDA8 ozone concentrations increase by 1-3 ppbv in the Northeast and 2-5 ppbv in the Great Plains; JJA PM2.5 concentrations increase by 0.8-1.2 μg m-3 in the Northeast and Southeast. The resulting impact on mortality rates is 4000 excess deaths per half cycle of AMO. We suggest that a complete picture of air quality management in coming <span class="hlt">decades</span> requires consideration of the AMO influence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.3214A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.3214A"><span>Tracking the Pacific <span class="hlt">Decadal</span> Precession</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anderson, Bruce T.; Furtado, Jason C.; Di Lorenzo, Emanuele; Short Gianotti, Daniel J.</p> <p>2017-03-01</p> <p>Events of recent years—including extended droughts across California, record fires across western Canada, and destabilization of marine ecosystems—highlight the profound impact of multiannual to <span class="hlt">decadal</span>-scale climate shifts upon physical, biological, and socioeconomic systems. While previous research has focused on the influence of <span class="hlt">decadal</span>-scale climate oscillations such as the Atlantic Multidecadal Oscillation and the Pacific <span class="hlt">Decadal</span> Oscillation/Interdecadal Pacific Oscillation, recent research has revealed the presence of a quasi-<span class="hlt">decadal</span> mode of climate <span class="hlt">variability</span> that, unlike the quasi-stationary standing wave-like structure of the oscillatory modes, involves a progression of atmospheric pressure anomalies around the North Pacific, which has been termed the Pacific <span class="hlt">Decadal</span> Precession (PDP). In this paper we develop a set of methods to track the spatial and temporal evolutions of the PDP within historical <span class="hlt">observations</span> as well as numerical model simulations. In addition, we provide a method that approximates the time evolution of the PDP across the full period of available data for real-time monitoring of the PDP. Through the development of these tracking methods, we hope to provide the community with a consistent framework for future analysis and diagnosis of the PDP's characteristics and underlying processes, thereby avoiding the use of different, and disparate, phenomenological- and mathematical-based indices that can confound our understanding of the PDP and its evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23996901','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23996901"><span>Reassessing regime shifts in the North Pacific: incremental climate change and commercial fishing are necessary for explaining <span class="hlt">decadal</span>-scale biological <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Litzow, Michael A; Mueter, Franz J; Hobday, Alistair J</p> <p>2014-01-01</p> <p>In areas of the North Pacific that are largely free of overfishing, climate regime shifts - abrupt changes in modes of low-frequency climate <span class="hlt">variability</span> - are seen as the dominant drivers of <span class="hlt">decadal</span>-scale ecological <span class="hlt">variability</span>. We assessed the ability of leading modes of climate <span class="hlt">variability</span> [Pacific <span class="hlt">Decadal</span> Oscillation (PDO), North Pacific Gyre Oscillation (NPGO), Arctic Oscillation (AO), Pacific-North American Pattern (PNA), North Pacific Index (NPI), El Niño-Southern Oscillation (ENSO)] to explain <span class="hlt">decadal</span>-scale (1965-2008) patterns of climatic and biological <span class="hlt">variability</span> across two North Pacific ecosystems (Gulf of Alaska and Bering Sea). Our response <span class="hlt">variables</span> were the first principle component (PC1) of four regional climate parameters [sea surface temperature (SST), sea level pressure (SLP), freshwater input, ice cover], and PCs 1-2 of 36 biological time series [production or abundance for populations of salmon (Oncorhynchus spp.), groundfish, herring (Clupea pallasii), shrimp, and jellyfish]. We found that the climate modes alone could not explain ecological <span class="hlt">variability</span> in the study region. Both linear models (for climate PC1) and generalized additive models (for biology PC1-2) invoking only the climate modes produced residuals with significant temporal trends, indicating that the models failed to capture coherent patterns of ecological <span class="hlt">variability</span>. However, when the residual climate trend and a time series of commercial fishery catches were used as additional candidate <span class="hlt">variables</span>, resulting models of biology PC1-2 satisfied assumptions of independent residuals and out-performed models constructed from the climate modes alone in terms of predictive power. As measured by effect size and Akaike weights, the residual climate trend was the most important <span class="hlt">variable</span> for explaining biology PC1 <span class="hlt">variability</span>, and commercial catch the most important <span class="hlt">variable</span> for biology PC2. Patterns of climate sensitivity and exploitation history for taxa strongly associated with biology</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.3637W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.3637W"><span><span class="hlt">Decadal</span> Record of Satellite Carbon Monoxide <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Worden, Helen; Deeter, Merritt; Frankenberg, Christian; George, Maya; Nichitiu, Florian; Worden, John; Aben, Ilse; Bowman, Kevin; Clerbaux, Cathy; Coheur, Pierre-Francois; de Laat, Jos; Warner, Juying; Drummond, James; Edwards, David; Gille, John; Hurtmans, Daniel; Ming, Luo; Martinez-Alonso, Sara; Massie, Steven; Pfister, Gabriele</p> <p>2013-04-01</p> <p>Atmospheric carbon monoxide (CO) distributions are controlled by anthropogenic emissions, biomass burning, chemical production, transport and oxidation by reaction with the hydroxyl radical (OH). Quantifying trends in CO is therefore important for understanding changes related to all of these contributions. Here we present a comprehensive record of satellite <span class="hlt">observations</span> from 2000 through 2011 of total column CO using the available measurements from nadir-viewing thermal infrared instruments: MOPITT, AIRS, TES and IASI. We examine trends for CO in the Northern and Southern hemispheres along with regional trends for E. China, E. USA, Europe and India. Measurement and sampling methods for each of the instruments are discussed, and we show diagnostics for systematic errors in MOPITT trends. We find that all the satellite <span class="hlt">observations</span> are consistent with a modest decreasing trend around -1%/year in total column CO over the Northern hemisphere for this time period. Decreasing trends in total CO column are <span class="hlt">observed</span> for the United States, Europe and E. China with more than 2σ significance. For India, the trend is also decreasing, but smaller in magnitude and less significant. Decreasing trends in surface CO have also been <span class="hlt">observed</span> from measurements in the U.S. and Europe. Although less information is available for surface CO in China, there is a decreasing trend reported for Beijing. Some of the interannual <span class="hlt">variability</span> in the <span class="hlt">observations</span> can be explained by global fire emissions, and there may be some evidence of the global financial crisis in late 2008 to early 2009. But the overall decrease needs further study to understand the implications for changes in anthropogenic emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.2625O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.2625O"><span>Mechanisms of <span class="hlt">decadal</span> <span class="hlt">variability</span> in the Labrador Sea and the wider North Atlantic in a high-resolution climate model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortega, Pablo; Robson, Jon; Sutton, Rowan T.; Andrews, Martin B.</p> <p>2017-10-01</p> <p>A necessary step before assessing the performance of <span class="hlt">decadal</span> predictions is the evaluation of the processes that bring memory to the climate system, both in climate models and <span class="hlt">observations</span>. These mechanisms are particularly relevant in the North Atlantic, where the ocean circulation, related to both the Subpolar Gyre and the Meridional Overturning Circulation (AMOC), is thought to be important for driving significant heat content anomalies. Recently, a rapid decline in <span class="hlt">observed</span> densities in the deep Labrador Sea has pointed to an ongoing slowdown of the AMOC strength taking place since the mid 90s, a decline also hinted by in-situ <span class="hlt">observations</span> from the RAPID array. This study explores the use of Labrador Sea densities as a precursor of the ocean circulation changes, by analysing a 300-year long simulation with the state-of-the-art coupled model HadGEM3-GC2. The major drivers of Labrador Sea density <span class="hlt">variability</span> are investigated, and are characterised by three major contributions. First, the integrated effect of local surface heat fluxes, mainly driven by year-to-year changes in the North Atlantic Oscillation, which accounts for 62% of the total variance. Additionally, two multidecadal-to-centennial contributions from the Greenland-Scotland Ridge outflows are quantified; the first associated with freshwater exports via the East Greenland Current, and the second with density changes in the Denmark Strait Overflow. Finally, evidence is shown that <span class="hlt">decadal</span> trends in Labrador Sea densities are followed by important atmospheric impacts. In particular, a positive winter NAO response appears to follow the negative Labrador Sea density trends, and provides a phase reversal mechanism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51L..03T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51L..03T"><span>Forced and Internal Multi-<span class="hlt">Decadal</span> <span class="hlt">Variability</span> in the North Atlantic and their Climate Impacts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ting, M.</p> <p>2017-12-01</p> <p>Atlantic Multidecadal <span class="hlt">Variability</span> (AMV), a basin-wide North Atlantic sea surface temperature warming or cooling pattern varying on <span class="hlt">decadal</span> and longer time scales, is one of the most important climate variations in the Atlantic basin. The AMV has shown to be associated with significant climate impacts regionally and globally, from Atlantic hurricane activities, frequency and severity of droughts across North America, as well as rainfall anomalies across the African Sahel and northeast Brazil. Despite the important impacts of the AMV, its mechanisms are not completely understood. In particular, it is not clear how much of the historical Atlantic SST fluctuations were forced by anthropogenic sources such as greenhouse warming and aerosol cooling, versus driven internally by changes in the coupled ocean-atmosphere processes in the Atlantic. Using climate models such as the NCAR large ensemble simulations, we were able to successfully separate the forced and internally generated North Atlantic sea surface temperature anomalies through a signal-to-noise maximizing Empirical Orthogonal Function (S/N EOF) analysis method. Two forced modes were identified with one representing a hemispherical symmetric mode and one asymmetric mode. The symmetric mode largely represents the greenhouse forced component while the asymmetric mode resembles the anthropogenic aerosol forcing. When statistically removing both of the forced modes, the residual multidecadal Atlantic SST <span class="hlt">variability</span> shows a very similar structure as the AMV in the preindustrial simulation. The distinct climate impacts of each of these modes are also identified and the implications and challenges for <span class="hlt">decadal</span> climate prediction will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JMS...148..249C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JMS...148..249C"><span>Regional circulation around New Caledonia from two <span class="hlt">decades</span> of <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cravatte, Sophie; Kestenare, Elodie; Eldin, Gérard; Ganachaud, Alexandre; Lefèvre, Jérôme; Marin, Frédéric; Menkes, Christophe; Aucan, Jérôme</p> <p>2015-08-01</p> <p>The regional and near-coastal circulation around New Caledonia is investigated using a compilation of more than 20 years of <span class="hlt">observations</span>. Velocity profiles acquired by Shipboard Acoustic Doppler Current Profiler (SADCP) during 109 research cruises and ship transits since 1991 are analyzed and compared with absolute geostrophic currents inferred from hydrographic profiles and Argo floats drifts. In addition, altimetric surface currents are used to explore the <span class="hlt">variability</span> of the circulation at various timescales. By making the best use of the strength of these various <span class="hlt">observations</span>, this study provides an unprecedented detailed picture of the mean circulation around New Caledonia and of its <span class="hlt">variability</span> in the upper layers. New Caledonia, together with the Vanuatu Archipelago and the Fiji Islands, acts as a 750-km long obstacle to the westward South Equatorial Current (SEC) entering the Coral Sea. On average, the SEC bifurcates against New Caledonia's east coast into a northwestward boundary current, the East Caledonian Current, beginning east of the Loyalty Islands and extending to at least 1000 m depth, and into a weak southeastward current. The latter, the Vauban Current, flows into the Loyalty channel against the mean trade winds where it extends to at least 500 m depth. It is highly <span class="hlt">variable</span> at intraseasonal timescales; it often reverses and its <span class="hlt">variability</span> is mainly driven by incoming mesoscale eddies east and south of New Caledonia. West of the Island, the southeastward Alis Current of New Caledonia (ACNC) flows along the reef slope in the 0-150 m layer. It overlays a weaker northwestward current, creating an unusual coastal circulation reminiscent of the current system along the Australian west coast. The ACNC is a persistent feature of the <span class="hlt">observations</span>, even if its transport is also strongly modulated by the presence of offshore eddies. This study highlights the fact, if needed, that a snapshot view of the currents provided by a single transect can be strongly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPA11C..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPA11C..07S"><span>Linking the <span class="hlt">Observation</span> of Essential <span class="hlt">Variables</span> to Societal Benefits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sylak-Glassman, E.</p> <p>2017-12-01</p> <p>Different scientific communities have established sets of commonly agreed upon essential <span class="hlt">variables</span> to help coordinate data collection in a variety of Earth <span class="hlt">observation</span> areas. As an example, the World Meteorological Organization Global Climate <span class="hlt">Observing</span> System has identified 50 Essential Climate <span class="hlt">Variables</span> (ECVs), such as sea-surface temperature and carbon dioxide, which are required to monitoring the climate and detect and attribute climate change. In addition to supporting climate science, measuring these ECVs deliver many types of societal benefits, ranging from disaster mitigation to agricultural productivity to human health. While communicating the value in maintaining and improving <span class="hlt">observational</span> records for these <span class="hlt">variables</span> has been a challenge, quantifying how the measurement of these ECVs results in the delivery of many different societal benefits may help support their continued measurement. The 2016 National Earth <span class="hlt">Observation</span> Assessment (EOA 2016) quantified the impact of individual Earth <span class="hlt">observation</span> systems, sensors, networks, and surveys (or Earth <span class="hlt">observation</span> systems, for short) on the achievement of 217 Federal objectives in 13 societal benefit areas (SBAs). This study will demonstrate the use of the EOA 2016 dataset to show the different Federal objectives and SBAs that are impacted by the Earth <span class="hlt">observation</span> systems used to measure ECVs. Describing how the measurements from these Earth <span class="hlt">observation</span> systems are used not only to maintain the climate record but also to meet additional Federal objectives may help articulate the continued measurement of the ECVs. This study will act as a pilot for the use of the EOA 2016 dataset to map between the measurements required to <span class="hlt">observe</span> additional sets of <span class="hlt">variables</span>, such as the Essential Ocean <span class="hlt">Variables</span> and Essential Biodiversity <span class="hlt">Variables</span>, and the ability to achieve a variety of societal benefits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OcSci..14..205E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OcSci..14..205E"><span>Orbit-related sea level errors for TOPEX altimetry at seasonal to <span class="hlt">decadal</span> timescales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esselborn, Saskia; Rudenko, Sergei; Schöne, Tilo</p> <p>2018-03-01</p> <p>Interannual to <span class="hlt">decadal</span> sea level trends are indicators of climate <span class="hlt">variability</span> and change. A major source of global and regional sea level data is satellite radar altimetry, which relies on precise knowledge of the satellite's orbit. Here, we assess the error budget of the radial orbit component for the TOPEX/Poseidon mission for the period 1993 to 2004 from a set of different orbit solutions. The errors for seasonal, interannual (5-year), and <span class="hlt">decadal</span> periods are estimated on global and regional scales based on radial orbit differences from three state-of-the-art orbit solutions provided by different research teams: the German Research Centre for Geosciences (GFZ), the Groupe de Recherche de Géodésie Spatiale (GRGS), and the Goddard Space Flight Center (GSFC). The global mean sea level error related to orbit uncertainties is of the order of 1 mm (8 % of the global mean sea level <span class="hlt">variability</span>) with negligible contributions on the annual and <span class="hlt">decadal</span> timescales. In contrast, the orbit-related error of the interannual trend is 0.1 mm yr-1 (27 % of the corresponding sea level <span class="hlt">variability</span>) and might hamper the estimation of an acceleration of the global mean sea level rise. For regional scales, the gridded orbit-related error is up to 11 mm, and for about half the ocean the orbit error accounts for at least 10 % of the <span class="hlt">observed</span> sea level <span class="hlt">variability</span>. The seasonal orbit error amounts to 10 % of the <span class="hlt">observed</span> seasonal sea level signal in the Southern Ocean. At interannual and <span class="hlt">decadal</span> timescales, the orbit-related trend uncertainties reach regionally more than 1 mm yr-1. The interannual trend errors account for 10 % of the <span class="hlt">observed</span> sea level signal in the tropical Atlantic and the south-eastern Pacific. For <span class="hlt">decadal</span> scales, the orbit-related trend errors are prominent in a several regions including the South Atlantic, western North Atlantic, central Pacific, South Australian Basin, and the Mediterranean Sea. Based on a set of test orbits calculated at GFZ, the sources of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........71P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........71P"><span>Sources and Impacts of Modeled and <span class="hlt">Observed</span> Low-Frequency Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parsons, Luke Alexander</p> <p></p> <p> structure of the variance spectrum has important consequences for the probability of multi-year drought. Our lake record suggests there is a significant background threat of multi-year, and even <span class="hlt">decade</span>-length, drought in western Amazonia, whereas climate model simulations indicate most droughts likely last no longer than one to three years. These findings suggest climate models may underestimate the future risk of extended drought in this important region. In Appendix C, we expand our analysis of climate <span class="hlt">variability</span> beyond South America. We use <span class="hlt">observations</span>, well-constrained tropical paleoclimate, and Earth system model data to examine the overall shape of the climate spectrum across interannual to century frequencies. We find a general agreement among <span class="hlt">observations</span> and models that temperature <span class="hlt">variability</span> increases with timescale across most of the globe outside the tropics. However, as compared to paleoclimate records, climate models generate too little low-frequency <span class="hlt">variability</span> in the tropics (e.g., Laepple and Huybers, 2014). When we compare the shape of the simulated climate spectrum to the spectrum of a simple autoregressive process, we find much of the modeled surface temperature <span class="hlt">variability</span> in the tropics could be explained by ocean smoothing of weather noise. Importantly, modeled precipitation tends to be similar to white noise across much of the globe. By contrast, paleoclimate records of various types from around the globe indicate that both temperature and precipitation <span class="hlt">variability</span> should experience much more low-frequency <span class="hlt">variability</span> than a simple autoregressive or white-noise process. In summary, state-of-the-art climate models generate some degree of dynamically driven low-frequency climate <span class="hlt">variability</span>, especially at high latitudes. However, the latest climate models, <span class="hlt">observations</span>, and paleoclimate data provide us with drastically different pictures of the background climate system and its associated risks. This research has important consequences for improving</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JCli...11..831G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JCli...11..831G"><span>A <span class="hlt">Decadal</span> Climate Cycle in the North Atlantic Ocean as Simulated by the ECHO Coupled GCM.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grötzner, A.; Latif, M.; Barnett, T. P.</p> <p>1998-05-01</p> <p>In this paper a <span class="hlt">decadal</span> climate cycle in the North Atlantic that was derived from an extended-range integration with a coupled ocean-atmosphere general circulation model is described. The <span class="hlt">decadal</span> mode shares many features with the <span class="hlt">observed</span> <span class="hlt">decadal</span> <span class="hlt">variability</span> in the North Atlantic. The period of the simulated oscillation, however, is somewhat longer than that estimated from <span class="hlt">observations</span>. While the <span class="hlt">observations</span> indicate a period of about 12 yr, the coupled model simulation yields a period of about 17 yr. The cyclic nature of the <span class="hlt">decadal</span> <span class="hlt">variability</span> implies some inherent predictability at these timescales.The <span class="hlt">decadal</span> mode is based on unstable air-sea interactions and must be therefore regarded as an inherently coupled mode. It involves the subtropical gyre and the North Atlantic oscillation. The memory of the coupled system, however, resides in the ocean and is related to horizontal advection and to the oceanic adjustment to low-frequency wind stress curl variations. In particular, it is found that variations in the intensity of the Gulf Stream and its extension are crucial to the oscillation. Although differing in details, the North Atlantic <span class="hlt">decadal</span> mode and the North Pacific mode described by M. Latif and T. P. Barnett are based on the same fundamental mechanism: a feedback loop between the wind driven subtropical gyre and the extratropical atmospheric circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRA..119.5800P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRA..119.5800P"><span><span class="hlt">Observations</span> and simulations of the ionospheric lunar tide: Seasonal <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pedatella, N. M.</p> <p>2014-07-01</p> <p>The seasonal <span class="hlt">variability</span> of the ionospheric lunar tide is investigated using a combination of Constellation <span class="hlt">Observing</span> System for Meteorology, Ionosphere, and Climate (COSMIC) <span class="hlt">observations</span> and thermosphere-ionosphere-mesosphere electrodynamics general circulation model (TIME-GCM) simulations. The present study focuses on the seasonal <span class="hlt">variability</span> of the lunar tide in the ionosphere and its potential connection to the occurrence of stratosphere sudden warmings (SSWs). COSMIC maximum F region electron density (NmF2) and total electron content <span class="hlt">observations</span> reveal a primarily annual variation of the ionospheric lunar tide, with maximum amplitudes occurring at low latitudes during December-February. Simulations of the lunar tide climatology in TIME-GCM display a similar annual <span class="hlt">variability</span> as the COSMIC <span class="hlt">observations</span>. This leads to the conclusion that the annual <span class="hlt">variability</span> of the lunar tide in the ionosphere is not solely due to the occurrence of SSWs. Rather, the annual <span class="hlt">variability</span> of the lunar tide in the ionosphere is generated by the seasonal <span class="hlt">variability</span> of the lunar tide at E region altitudes. However, compared to the <span class="hlt">observations</span>, the ionospheric lunar tide annual <span class="hlt">variability</span> is weaker in the climatological simulations which is attributed to the occurrence of SSWs during the majority of the years included in the <span class="hlt">observations</span>. Introducing a SSW into the TIME-GCM simulation leads to an additional enhancement of the lunar tide during Northern Hemisphere winter, increasing the lunar tide annual <span class="hlt">variability</span> and resulting in an annual <span class="hlt">variability</span> that is more consistent with the <span class="hlt">observations</span>. The occurrence of SSWs can therefore potentially bias lunar tide climatologies, and it is important to consider these effects in studies of the lunar tide in the atmosphere and ionosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006cosp...36.2610Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006cosp...36.2610Y"><span>Near-infrared <span class="hlt">observations</span> of the <span class="hlt">variable</span> crab nebula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamamoto, M.; Mori, K.; Shibata, S.; Tsujimoto, M.; Misawa, T.; Burrows, D.; Kawai, N.</p> <p></p> <p>We present three near-infrared NIR <span class="hlt">observations</span> of the Crab Nebula obtained with CISCO on the Subaru Telescope and Quick Infrared Camera on the University of HAWAII 88 inch Telescope The <span class="hlt">observations</span> were performed on 2004 September 2005 February and 2005 October and were coordinated with X-ray <span class="hlt">observations</span> obtained with the Chandra X-ray observatory within 10 days As shown in previous optical and X-ray monitoring <span class="hlt">observations</span> outward-moving wisps and <span class="hlt">variable</span> knots are detected also in our NIR <span class="hlt">observations</span> The NIR variations are closely correlated with variations in the X-ray <span class="hlt">observations</span> indicating that both variations are driven by the same physical process We discuss the origin of NIR-emitting particles based on the temporal variations as well as the spectral energy distributions of each <span class="hlt">variable</span> component</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29374176','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29374176"><span><span class="hlt">Decadal</span> climate predictability in the southern Indian Ocean captured by SINTEX-F using a simple SST-nudging scheme.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Morioka, Yushi; Doi, Takeshi; Behera, Swadhin K</p> <p>2018-01-26</p> <p><span class="hlt">Decadal</span> climate <span class="hlt">variability</span> in the southern Indian Ocean has great influences on southern African climate through modulation of atmospheric circulation. Although many efforts have been made to understanding physical mechanisms, predictability of the <span class="hlt">decadal</span> climate <span class="hlt">variability</span>, in particular, the internally generated <span class="hlt">variability</span> independent from external atmospheric forcing, remains poorly understood. This study investigates predictability of the <span class="hlt">decadal</span> climate <span class="hlt">variability</span> in the southern Indian Ocean using a coupled general circulation model, called SINTEX-F. The ensemble members of the <span class="hlt">decadal</span> reforecast experiments were initialized with a simple sea surface temperature (SST) nudging scheme. The <span class="hlt">observed</span> positive and negative peaks during late 1990s and late 2000s are well reproduced in the reforecast experiments initiated from 1994 and 1999, respectively. The experiments initiated from 1994 successfully capture warm SST and high sea level pressure anomalies propagating from the South Atlantic to the southern Indian Ocean. Also, the other experiments initiated from 1999 skillfully predict phase change from a positive to negative peak. These results suggest that the SST-nudging initialization has the essence to capture the predictability of the internally generated <span class="hlt">decadal</span> climate <span class="hlt">variability</span> in the southern Indian Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040081225&hterms=chlorophyll&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dchlorophyll','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040081225&hterms=chlorophyll&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dchlorophyll"><span>Patterns and <span class="hlt">Variability</span> in Global Ocean Chlorophyll: Satellite <span class="hlt">Observations</span> and Modeling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregg, Watson</p> <p>2004-01-01</p> <p>Recent analyses of SeaWiFS data have shown that global ocean chlorophyll has increased more than 4% since 1998. The North Pacific ocean basin has increased nearly 19%. These trend analyses follow earlier results showing <span class="hlt">decadal</span> declines in global ocean chlorophyll and primary production. To understand the causes of these changes and trends we have applied the newly developed NASA Ocean Biogeochemical Assimilation Model (OBAM), which is driven in mechanistic fashion by surface winds, sea surface temperature, atmospheric iron deposition, sea ice, and surface irradiance. The model utilizes chlorophyll from SeaWiFS in a daily assimilation. The model has in place many of the climatic <span class="hlt">variables</span> that can be expected to produce the changes <span class="hlt">observed</span> in SeaWiFS data. This enables us to diagnose the model performance, the assimilation performance, and possible causes for the increase in chlorophyll. A full discussion of the changes and trends, possible causes, modeling approaches, and data assimilation will be the focus of the seminar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.A51A0082S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.A51A0082S"><span>Atmospheric <span class="hlt">Variability</span> of CO2 impact on space <span class="hlt">observation</span> Requirements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swanson, A. L.; Sen, B.; Newhart, L.; Segal, G.</p> <p>2009-12-01</p> <p>If International governments are to reduce GHG levels by 80% by 2050, as recommended by most scientific bodies concerned with avoiding the most hazardous changes in climate, then massive investments in infrastructure and new technology will be required over the coming <span class="hlt">decades</span>. Such an investment will be a huge commitment by governments and corporations, and while it will offer long-term dividends in lower energy costs, a healthier environment and averted additional global warming, the shear magnitude of upfront costs will drive a call for a monitoring and verification system. Such a system will be required to offer accountability to signatories of governing bodies, as well as, for the global public. Measuring the average global distribution of CO2 is straight forward, as exemplified by the long running station measurements managed by NOAA’s Global Monitoring Division that includes the longterm Keeling record. However, quantifying anthropogenic and natural source/sink distributions and atmospheric mixing have been much more difficult to constrain. And, yet, an accurate accounting of all anthropogenic source strengths is required for Global Treaty verification. The only way to accurately assess Global GHG emissions is to construct an integrated system of ground, air and space based <span class="hlt">observations</span> with extensive chemical modeling capabilities. We look at the measurement requirements for the space based component of the solutions. To determine what space sensor performance requirements for ground resolution, coverage, and revisit, we have analyzed regional CO2 distributions and <span class="hlt">variability</span> using NASA and NOAA aircraft flight campaigns. The results of our analysis are presented as variograms showing average spatial <span class="hlt">variability</span> over several Northern Hemispheric regions. There are distinct regional differences with the starkest contrast between urban versus rural and Coastal Asia versus Coastal US. The results suggest specific consequences on what spatial and temporal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810017372','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810017372"><span>IUE <span class="hlt">observations</span> of <span class="hlt">variability</span> in winds from hot stars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Grady, C. A.; Snow, T. P., Jr.</p> <p>1981-01-01</p> <p><span class="hlt">Observations</span> of <span class="hlt">variability</span> in stellar winds or envelopes provide an important probe of their dynamics. For this purpose a number of O, B, Be, and Wolf-Rayet stars were repeatedly <span class="hlt">observed</span> with the IUE satellite in high resolution mode. In the course of analysis, instrumental and data handling effects were found to introduce spurious <span class="hlt">variability</span> in many of the spectra. software was developed to partially compensate for these effects, but limitations remain on the type of <span class="hlt">variability</span> that can be identified from IUE spectra. With these contraints, preliminary results of multiple <span class="hlt">observations</span> of two OB stars, one Wolf-Rayet star, and a Be star are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....1711135S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....1711135S"><span><span class="hlt">Variability</span> and quasi-<span class="hlt">decadal</span> changes in the methane budget over the period 2000-2012</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saunois, Marielle; Bousquet, Philippe; Poulter, Ben; Peregon, Anna; Ciais, Philippe; Canadell, Josep G.; Dlugokencky, Edward J.; Etiope, Giuseppe; Bastviken, David; Houweling, Sander; Janssens-Maenhout, Greet; Tubiello, Francesco N.; Castaldi, Simona; Jackson, Robert B.; Alexe, Mihai; Arora, Vivek K.; Beerling, David J.; Bergamaschi, Peter; Blake, Donald R.; Brailsford, Gordon; Bruhwiler, Lori; Crevoisier, Cyril; Crill, Patrick; Covey, Kristofer; Frankenberg, Christian; Gedney, Nicola; Höglund-Isaksson, Lena; Ishizawa, Misa; Ito, Akihiko; Joos, Fortunat; Kim, Heon-Sook; Kleinen, Thomas; Krummel, Paul; Lamarque, Jean-François; Langenfelds, Ray; Locatelli, Robin; Machida, Toshinobu; Maksyutov, Shamil; Melton, Joe R.; Morino, Isamu; Naik, Vaishali; O'Doherty, Simon; Parmentier, Frans-Jan W.; Patra, Prabir K.; Peng, Changhui; Peng, Shushi; Peters, Glen P.; Pison, Isabelle; Prinn, Ronald; Ramonet, Michel; Riley, William J.; Saito, Makoto; Santini, Monia; Schroeder, Ronny; Simpson, Isobel J.; Spahni, Renato; Takizawa, Atsushi; Thornton, Brett F.; Tian, Hanqin; Tohjima, Yasunori; Viovy, Nicolas; Voulgarakis, Apostolos; Weiss, Ray; Wilton, David J.; Wiltshire, Andy; Worthy, Doug; Wunch, Debra; Xu, Xiyan; Yoshida, Yukio; Zhang, Bowen; Zhang, Zhen; Zhu, Qiuan</p> <p>2017-09-01</p> <p>Following the recent Global Carbon Project (GCP) synthesis of the <span class="hlt">decadal</span> methane (CH4) budget over 2000-2012 (Saunois et al., 2016), we analyse here the same dataset with a focus on quasi-<span class="hlt">decadal</span> and inter-annual <span class="hlt">variability</span> in CH4 emissions. The GCP dataset integrates results from top-down studies (exploiting atmospheric <span class="hlt">observations</span> within an atmospheric inverse-modelling framework) and bottom-up models (including process-based models for estimating land surface emissions and atmospheric chemistry), inventories of anthropogenic emissions, and data-driven approaches. The annual global methane emissions from top-down studies, which by construction match the <span class="hlt">observed</span> methane growth rate within their uncertainties, all show an increase in total methane emissions over the period 2000-2012, but this increase is not linear over the 13 years. Despite differences between individual studies, the mean emission anomaly of the top-down ensemble shows no significant trend in total methane emissions over the period 2000-2006, during the plateau of atmospheric methane mole fractions, and also over the period 2008-2012, during the renewed atmospheric methane increase. However, the top-down ensemble mean produces an emission shift between 2006 and 2008, leading to 22 [16-32] Tg CH4 yr-1 higher methane emissions over the period 2008-2012 compared to 2002-2006. This emission increase mostly originated from the tropics, with a smaller contribution from mid-latitudes and no significant change from boreal regions. The regional contributions remain uncertain in top-down studies. Tropical South America and South and East Asia seem to contribute the most to the emission increase in the tropics. However, these two regions have only limited atmospheric measurements and remain therefore poorly constrained. The sectorial partitioning of this emission increase between the periods 2002-2006 and 2008-2012 differs from one atmospheric inversion study to another. However, all top-down studies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20180002887&hterms=methane&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmethane','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20180002887&hterms=methane&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmethane"><span><span class="hlt">Variability</span> and Quasi-<span class="hlt">Decadal</span> Changes in the Methane Budget over the Period 2000-2012</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Saunois, Marielle; Bousquet, Philippe; Poulter, Ben; Peregon, Anna; Ciais, Philippe; Canadell, Josep G.; Dlugokencky, Edward J.; Etiope, Giuseppe; Bastviken, David; Houweling, Sander; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20180002887'); toggleEditAbsImage('author_20180002887_show'); toggleEditAbsImage('author_20180002887_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20180002887_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20180002887_hide"></p> <p>2017-01-01</p> <p>Following the recent Global Carbon Project (GCP) synthesis of the <span class="hlt">decadal</span> methane (CH4) budget over 2000- 2012, we analyse here the same dataset with a focus on quasi-<span class="hlt">decadal</span> and inter-annual <span class="hlt">variability</span> in CH4 emissions. The GCP dataset integrates results from top-down studies (exploiting atmospheric <span class="hlt">observations</span> within an atmospheric inverse-modelling framework) and bottom-up models (including process-based models for estimating land surface emissions and atmospheric chemistry), inventories of anthropogenic emissions, and data-driven approaches. The annual global methane emissions from top-down studies, which by construction match the <span class="hlt">observed</span> methane growth rate within their uncertainties, all show an increase in total methane emissions over the period 2000-2012, but this increase is not linear over the 13 years. Despite differences between individual studies, the mean emission anomaly of the top-down ensemble shows no significant trend in total methane emissions over the period 2000-2006, during the plateau of atmospheric methane mole fractions, and also over the period 2008-2012, during the renewed atmospheric methane increase. However, the top-down ensemble mean produces an emission shift between 2006 and 2008, leading to 22 [16-32] Tg CH4 yr(exp -1) higher methane emissions over the period 2008-2012 compared to 2002-2006. This emission increase mostly originated from the tropics, with a smaller contribution from mid-latitudes and no significant change from boreal regions. The regional contributions remain uncertain in top-down studies. Tropical South America and South and East Asia seem to contribute the most to the emission increase in the tropics. However, these two regions have only limited atmospheric measurements and remain therefore poorly constrained. The sectorial partitioning of this emission increase between the periods 2002-2006 and 2008-2012 differs from one atmospheric inversion study to another. However, all top-down studies suggest smaller</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...48.1841V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...48.1841V"><span><span class="hlt">Decadal</span> climate prediction with a refined anomaly initialisation approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volpi, Danila; Guemas, Virginie; Doblas-Reyes, Francisco J.; Hawkins, Ed; Nichols, Nancy K.</p> <p>2017-03-01</p> <p>In <span class="hlt">decadal</span> prediction, the objective is to exploit both the sources of predictability from the external radiative forcings and from the internal <span class="hlt">variability</span> to provide the best possible climate information for the next <span class="hlt">decade</span>. Predicting the climate system internal <span class="hlt">variability</span> relies on initialising the climate model from <span class="hlt">observational</span> estimates. We present a refined method of anomaly initialisation (AI) applied to the ocean and sea ice components of the global climate forecast model EC-Earth, with the following key innovations: (1) the use of a weight applied to the <span class="hlt">observed</span> anomalies, in order to avoid the risk of introducing anomalies recorded in the <span class="hlt">observed</span> climate, whose amplitude does not fit in the range of the internal <span class="hlt">variability</span> generated by the model; (2) the AI of the ocean density, instead of calculating it from the anomaly initialised state of temperature and salinity. An experiment initialised with this refined AI method has been compared with a full field and standard AI experiment. Results show that the use of such refinements enhances the surface temperature skill over part of the North and South Atlantic, part of the South Pacific and the Mediterranean Sea for the first forecast year. However, part of such improvement is lost in the following forecast years. For the tropical Pacific surface temperature, the full field initialised experiment performs the best. The prediction of the Arctic sea-ice volume is improved by the refined AI method for the first three forecast years and the skill of the Atlantic multidecadal oscillation is significantly increased compared to a non-initialised forecast, along the whole forecast time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1330744','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1330744"><span>Collaborative Proposal: Improving <span class="hlt">Decadal</span> Prediction of Arctic Climate <span class="hlt">Variability</span> and Change Using a Regional Arctic System Model (RASM)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Maslowski, Wieslaw</p> <p></p> <p>This project aims to develop, apply and evaluate a regional Arctic System model (RASM) for enhanced <span class="hlt">decadal</span> predictions. Its overarching goal is to advance understanding of the past and present states of arctic climate and to facilitate improvements in seasonal to <span class="hlt">decadal</span> predictions. In particular, it will focus on <span class="hlt">variability</span> and long-term change of energy and freshwater flows through the arctic climate system. The project will also address modes of natural climate <span class="hlt">variability</span> as well as extreme and rapid climate change in a region of the Earth that is: (i) a key indicator of the state of global climate throughmore » polar amplification and (ii) which is undergoing environmental transitions not seen in instrumental records. RASM will readily allow the addition of other earth system components, such as ecosystem or biochemistry models, thus allowing it to facilitate studies of climate impacts (e.g., droughts and fires) and of ecosystem adaptations to these impacts. As such, RASM is expected to become a foundation for more complete Arctic System models and part of a model hierarchy important for improving climate modeling and predictions.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcMod..97...65D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcMod..97...65D"><span>North Atlantic simulations in Coordinated Ocean-ice Reference Experiments phase II (CORE-II). Part II: Inter-annual to <span class="hlt">decadal</span> <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Danabasoglu, Gokhan; Yeager, Steve G.; Kim, Who M.; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; Bleck, Rainer; Böning, Claus; Bozec, Alexandra; Canuto, Vittorio M.; Cassou, Christophe; Chassignet, Eric; Coward, Andrew C.; Danilov, Sergey; Diansky, Nikolay; Drange, Helge; Farneti, Riccardo; Fernandez, Elodie; Fogli, Pier Giuseppe; Forget, Gael; Fujii, Yosuke; Griffies, Stephen M.; Gusev, Anatoly; Heimbach, Patrick; Howard, Armando; Ilicak, Mehmet; Jung, Thomas; Karspeck, Alicia R.; Kelley, Maxwell; Large, William G.; Leboissetier, Anthony; Lu, Jianhua; Madec, Gurvan; Marsland, Simon J.; Masina, Simona; Navarra, Antonio; Nurser, A. J. George; Pirani, Anna; Romanou, Anastasia; Salas y Mélia, David; Samuels, Bonita L.; Scheinert, Markus; Sidorenko, Dmitry; Sun, Shan; Treguier, Anne-Marie; Tsujino, Hiroyuki; Uotila, Petteri; Valcke, Sophie; Voldoire, Aurore; Wang, Qiang; Yashayaev, Igor</p> <p>2016-01-01</p> <p>Simulated inter-annual to <span class="hlt">decadal</span> <span class="hlt">variability</span> and trends in the North Atlantic for the 1958-2007 period from twenty global ocean - sea-ice coupled models are presented. These simulations are performed as contributions to the second phase of the Coordinated Ocean-ice Reference Experiments (CORE-II). The study is Part II of our companion paper (Danabasoglu et al., 2014) which documented the mean states in the North Atlantic from the same models. A major focus of the present study is the representation of Atlantic meridional overturning circulation (AMOC) <span class="hlt">variability</span> in the participating models. Relationships between AMOC <span class="hlt">variability</span> and those of some other related <span class="hlt">variables</span>, such as subpolar mixed layer depths, the North Atlantic Oscillation (NAO), and the Labrador Sea upper-ocean hydrographic properties, are also investigated. In general, AMOC <span class="hlt">variability</span> shows three distinct stages. During the first stage that lasts until the mid- to late-1970s, AMOC is relatively steady, remaining lower than its long-term (1958-2007) mean. Thereafter, AMOC intensifies with maximum transports achieved in the mid- to late-1990s. This enhancement is then followed by a weakening trend until the end of our integration period. This sequence of low frequency AMOC <span class="hlt">variability</span> is consistent with previous studies. Regarding strengthening of AMOC between about the mid-1970s and the mid-1990s, our results support a previously identified <span class="hlt">variability</span> mechanism where AMOC intensification is connected to increased deep water formation in the subpolar North Atlantic, driven by NAO-related surface fluxes. The simulations tend to show general agreement in their temporal representations of, for example, AMOC, sea surface temperature (SST), and subpolar mixed layer depth <span class="hlt">variabilities</span>. In particular, the <span class="hlt">observed</span> <span class="hlt">variability</span> of the North Atlantic SSTs is captured well by all models. These findings indicate that simulated <span class="hlt">variability</span> and trends are primarily dictated by the atmospheric datasets which</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160008690','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160008690"><span>North Atlantic Simulations in Coordinated Ocean-Ice Reference Experiments Phase II (CORE-II) . Part II; Inter-Annual to <span class="hlt">Decadal</span> <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Danabasoglu, Gokhan; Yeager, Steve G.; Kim, Who M.; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; Bleck, Rainer; Boening, Claus; Bozec, Alexandra; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160008690'); toggleEditAbsImage('author_20160008690_show'); toggleEditAbsImage('author_20160008690_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160008690_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160008690_hide"></p> <p>2015-01-01</p> <p>Simulated inter-annual to <span class="hlt">decadal</span> <span class="hlt">variability</span> and trends in the North Atlantic for the 1958-2007 period from twenty global ocean - sea-ice coupled models are presented. These simulations are performed as contributions to the second phase of the Coordinated Ocean-ice Reference Experiments (CORE-II). The study is Part II of our companion paper (Danabasoglu et al., 2014) which documented the mean states in the North Atlantic from the same models. A major focus of the present study is the representation of Atlantic meridional overturning circulation (AMOC) <span class="hlt">variability</span> in the participating models. Relationships between AMOC <span class="hlt">variability</span> and those of some other related <span class="hlt">variables</span>, such as subpolar mixed layer depths, the North Atlantic Oscillation (NAO), and the Labrador Sea upper-ocean hydrographic properties, are also investigated. In general, AMOC <span class="hlt">variability</span> shows three distinct stages. During the first stage that lasts until the mid- to late-1970s, AMOC is relatively steady, remaining lower than its long-term (1958-2007) mean. Thereafter, AMOC intensifies with maximum transports achieved in the mid- to late-1990s. This enhancement is then followed by a weakening trend until the end of our integration period. This sequence of low frequency AMOC <span class="hlt">variability</span> is consistent with previous studies. Regarding strengthening of AMOC between about the mid-1970s and the mid-1990s, our results support a previously identified <span class="hlt">variability</span> mechanism where AMOC intensification is connected to increased deep water formation in the subpolar North Atlantic, driven by NAO-related surface fluxes. The simulations tend to show general agreement in their representations of, for example, AMOC, sea surface temperature (SST), and subpolar mixed layer depth <span class="hlt">variabilities</span>. In particular, the <span class="hlt">observed</span> <span class="hlt">variability</span> of the North Atlantic SSTs is captured well by all models. These findings indicate that simulated <span class="hlt">variability</span> and trends are primarily dictated by the atmospheric datasets which include</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70162171','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70162171"><span>Lake oxygen isotopes as recorders of North American Rocky Mountain hydroclimate: Holocene patterns and <span class="hlt">variability</span> at multi-<span class="hlt">decadal</span> to millennial time scales</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Anderson, Lesleigh; Max Berkelhammer,; Barron, John A.; Steinman, Byron A.; Finney, Bruce P.; Abbott, Mark B.</p> <p>2016-01-01</p> <p>Lake sediment oxygen isotope records (calcium carbonate-δ18O) in the western North American Cordillera developed during the past <span class="hlt">decade</span> provide substantial evidence of Pacific ocean–atmosphere forcing of hydroclimatic <span class="hlt">variability</span> during the Holocene. Here we present an overview of 18 lake sediment δ18O records along with a new compilation of lake water δ18O and δ2H that are used to characterize lake sediment sensitivity to precipitation-δ18O in contrast to fractionation by evaporation. Of the 18 records, 14 have substantial sensitivity to evaporation. Two records reflect precipitation-δ18O since the middle Holocene, Jellybean and Bison Lakes, and are geographically positioned in the northern and southern regions of the study area. Their comparative analysis indicates a sequence of time-varying north–south precipitation-δ18O patterns that is evidence for a highly non-stationary influence by Pacific ocean–atmosphere processes on the hydroclimate of western North America. These <span class="hlt">observations</span> are discussed within the context of previous research on North Pacific precipitation-δ18O based on empirical and modeling methods. The Jellybean and Bison Lake records indicate that a prominent precipitation-δ18O dipole (enriched-north and depleted-south) was sustained between ~ 3.5 and 1.5 ka, which contrasts with earlier Holocene patterns, and appears to indicate the onset of a dominant tropical control on North Pacific ocean–atmosphere dynamics. This remains the state of the system today. Higher frequency reversals of the north–south precipitation-δ18O dipole between ~ 2.5 and 1.5 ka, and during the Medieval Climate Anomaly and the Little Ice Age, also suggest more varieties of Pacific ocean–atmosphere modes than a single Pacific <span class="hlt">Decadal</span> Oscillation (PDO) type analogue. Results indicate that further investigation of precipitation-δ18O patterns on short (<span class="hlt">observational</span>) and long (Holocene) time scales is needed to improve our understanding of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A32G..03G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A32G..03G"><span>Santa Ana Winds of Southern California: Their Climatology and <span class="hlt">Variability</span> Spanning 6.5 <span class="hlt">Decades</span> from Regional Dynamical Modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guzman-Morales, J.; Gershunov, A.</p> <p>2015-12-01</p> <p>Santa Ana Winds (SAWs) are an integral feature of the regional climate of Southern California/Northern Baja California region. In spite of their tremendous episodic impacts on the health, economy and mood of the region, climate-scale behavior of SAW is poorly understood. In the present work, we identify SAWs in mesoscale dynamical downscaling of a global reanalysis product and construct an hourly SAW catalogue spanning 65 years. We describe the long-term SAW climatology at relevant time-space resolutions, i.e, we developed local and regional SAW indices and analyse their <span class="hlt">variability</span> on hourly, daily, annual, and multi-<span class="hlt">decadal</span> timescales. Local and regional SAW indices are validated with available anemometer <span class="hlt">observations</span>. Characteristic behaviors are revealed, e.g. the SAW intensity-duration relationship. At interdecadal time scales, we find that seasonal SAW activity is sensitive to prominent large-scale low-frequency modes of climate <span class="hlt">variability</span> rooted in the tropical and north Pacific ocean-atmosphere system that are also known to affect the hydroclimate of this region. Lastly, we do not find any long-term trend in SAW frequency and intensity as previously reported. Instead, we identify a significant long-term trend in SAW behavior whereby contribution of extreme SAW events to total seasonal SAW activity has been increasing at the expense of moderate events. These findings motivate further investigation on SAW evolution in future climate and its impact on wildfires.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JSR....86...97T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JSR....86...97T"><span>Impact of the river nutrient load <span class="hlt">variability</span> on the North Aegean ecosystem functioning over the last <span class="hlt">decades</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsiaras, K. P.; Petihakis, G.; Kourafalou, V. H.; Triantafyllou, G.</p> <p>2014-02-01</p> <p>The impact of river load <span class="hlt">variability</span> on the North Aegean ecosystem functioning over the last <span class="hlt">decades</span> (1980-2000) was investigated by means of a coupled hydrodynamic/biogeochemical model simulation. Model results were validated against available SeaWiFS Chl-a and in situ data. The simulated food web was found dominated by small cells, in agreement with <span class="hlt">observations</span>, with most of the carbon channelled through the microbial loop. Diatoms and dinoflagellates presented a higher relative abundance in the more productive coastal areas. The increased phosphate river loads in the early 80s resulted in nitrogen and silicate deficiency in coastal, river-influenced regions. Primary production presented a decreasing trend for most areas. During periods of increased phosphate/nitrate inputs, silicate deficiency resulted in a relative decrease of diatoms, triggering an increase of dinoflagellates. Such an increase was simulated in the late 90s in the Thermaikos Gulf, in agreement with the <span class="hlt">observed</span> increased occurrence of Harmful Algal Blooms. Microzooplankton was found to closely follow the relative increase of dinoflagellates under higher nutrient availability, showing a faster response than mesozooplankton. Sensitivity simulations with varying nutrient river inputs revealed a linear response of net primary production and plankton biomass. A stronger effect of river inputs was simulated in the enclosed Thermaikos Gulf, in terms of productivity and plankton composition, showing a significant increase of dinoflagellates relative abundance under increased nutrient loads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/20765','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/20765"><span>On measuring bird habitat: influence of <span class="hlt">observer</span> <span class="hlt">variability</span> and sample size</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>William M. Block; Kimberly A. With; Michael L. Morrison</p> <p>1987-01-01</p> <p>We studied the effects of <span class="hlt">observer</span> <span class="hlt">variability</span> when estimating vegetation characteristics at 75 0.04-ha bird plots. <span class="hlt">Observer</span> estimates were significantly different for 31 of 49 <span class="hlt">variables</span>. Multivariate analyses showed significant interobserver differences for five of the seven classes of <span class="hlt">variables</span> studied. <span class="hlt">Variable</span> classes included the height, number, and diameter of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19344309','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19344309"><span>Photometric <span class="hlt">variability</span> in earthshine <span class="hlt">observations</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Langford, Sally V; Wyithe, J Stuart B; Turner, Edwin L</p> <p>2009-04-01</p> <p>The identification of an extrasolar planet as Earth-like will depend on the detection of atmospheric signatures or surface non-uniformities. In this paper we present spatially unresolved flux light curves of Earth for the purpose of studying a prototype extrasolar terrestrial planet. Our monitoring of the photometric <span class="hlt">variability</span> of earthshine revealed changes of up to 23% per hour in the brightness of Earth's scattered light at around 600 nm, due to the removal of specular reflection from the view of the Moon. This <span class="hlt">variability</span> is accompanied by reddening of the spectrum and results from a change in surface properties across the continental boundary between the Indian Ocean and Africa's east coast. Our results based on earthshine monitoring indicate that specular reflection should provide a useful tool in determining the presence of liquid water on extrasolar planets via photometric <span class="hlt">observations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810017411','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810017411"><span><span class="hlt">Observations</span> of cataclysmic <span class="hlt">variables</span> with IUE</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hartmann, L.; Raymond, J.</p> <p>1981-01-01</p> <p><span class="hlt">Observations</span> are reported of the cataclysmic <span class="hlt">variables</span> AN UMa, 2AO311-227, VV Pup, DQ Her, and GK Per. Continuum emission was detected in the short wavelength region in DQ Her. This object exhibits a quasi-blackbody spectrum at short wavelengths, such blackbody components are a common property of the <span class="hlt">variables</span> AM Her, SS Cyg, and U Gem, suggesting an underlying similarity in the activity of these diverse systems. Flat continuum components at longer wavelengths in general are not compatible with standard disk models. The emission line ratios in AE Aqr are anomalous in that C IV is absent to a very low level relative to N V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50.1597H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50.1597H"><span><span class="hlt">Decadal</span> fluctuations in the western Pacific recorded by long precipitation records in Taiwan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Wan-Ru; Wang, S.-Y. Simon; Guan, Biing T.</p> <p>2018-03-01</p> <p>A 110-year precipitation record in Taiwan, located at the western edge of the subtropical North Pacific, depicts a pronounced quasi-<span class="hlt">decadal</span> oscillation (QDO). The QDO in Taiwan exhibits a fluctuating relationship with the similar <span class="hlt">decadal</span> variations of sea surface temperature (SST) anomalies in the central equatorial Pacific, known as the Pacific QDO. A regime change was <span class="hlt">observed</span> around 1960, such that the <span class="hlt">decadal</span> variation of Taiwan's precipitation became more synchronized with the Pacific QDO's coupled evolutions of SST and atmospheric circulation than before, while the underlying pattern of the Pacific QOD did not change. Using long-term reanalysis data and CMIP5 single-forcing experiments, the presented analysis suggests that increased SST in the subtropical western Pacific and the strengthened western extension of the North Pacific subtropical anticyclone may have collectively enhanced the relationship between the Taiwan precipitation and the Pacific QDO. This finding provides possible clues to similar regime changes in quasi-<span class="hlt">decadal</span> <span class="hlt">variability</span> <span class="hlt">observed</span> around the western Pacific rim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JOL....36..193Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JOL....36..193Z"><span>An aftereffect of global warming on tropical Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zheng, Jian; Liu, Qinyu; Wang, Chuanyang</p> <p>2018-03-01</p> <p>Studies have shown that global warming over the past six <span class="hlt">decades</span> can weaken the tropical Pacific Walker circulation and maintain the positive phase of the Interdecadal Pacific Oscillation (IPO). Based on <span class="hlt">observations</span> and model simulations, another aftereffect of global warming on IPO is found. After removing linear trends (global warming signals) from <span class="hlt">observations</span>, however, the tropical Pacific climate still exhibited some obvious differences between two IPO negative phases. The boreal winter (DJF) equatorial central-eastern Pacific sea surface temperature (SST) was colder during the 1999-2014 period (P2) than that during 1961-1976 (P1). This difference may have been a result of global warming nonlinear modulation of precipitation; i.e., in the climatological rainy region, the core area of the tropical Indo-western Pacific warm pool receives more precipitation through the "wet-get-wetter" mechanism. Positive precipitation anomalies in the warm pool during P2 are much stronger than those during P1, even after subtracting the linear trend. Corresponding to the differences of precipitation, the Pacific Walker circulation is stronger in P2 than in P1. Consequent easterly winds over the equatorial Pacific led to a colder equatorial eastern-central Pacific during P2. Therefore, tropical Pacific climate differences between the two negative IPO phases are aftereffects of global warming. These aftereffects are supported by the results of coupled climate model experiments, with and without global warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140007330','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140007330"><span>Use of Machine Learning Techniques for Iidentification of Robust Teleconnections to East African Rainfall <span class="hlt">Variability</span> in <span class="hlt">Observations</span> and Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roberts, J. Brent; Robertson, Franklin R.; Funk, Chris</p> <p>2014-01-01</p> <p>Providing advance warning of East African rainfall variations is a particular focus of several groups including those participating in the Famine Early Warming Systems Network. Both seasonal and long-term model projections of climate <span class="hlt">variability</span> are being used to examine the societal impacts of hydrometeorological <span class="hlt">variability</span> on seasonal to interannual and longer time scales. The NASA / USAID SERVIR project, which leverages satellite and modeling-based resources for environmental decision making in developing nations, is focusing on the evaluation of both seasonal and climate model projections to develop downscaled scenarios for using in impact modeling. The utility of these projections is reliant on the ability of current models to capture the embedded relationships between East African rainfall and evolving forcing within the coupled ocean-atmosphere-land climate system. Previous studies have posited relationships between variations in El Niño, the Walker circulation, Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> (PDV), and anthropogenic forcing. This study applies machine learning methods (e.g. clustering, probabilistic graphical model, nonlinear PCA) to <span class="hlt">observational</span> datasets in an attempt to expose the importance of local and remote forcing mechanisms of East African rainfall <span class="hlt">variability</span>. The ability of the NASA Goddard Earth <span class="hlt">Observing</span> System (GEOS5) coupled model to capture the associated relationships will be evaluated using Coupled Model Intercomparison Project Phase 5 (CMIP5) simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70186672','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70186672"><span><span class="hlt">Observations</span> and 3D hydrodynamics-based modeling of <span class="hlt">decadal</span>-scale shoreline change along the Outer Banks, North Carolina</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Safak, Ilgar; List, Jeffrey; Warner, John C.; Kumar, Nirnimesh</p> <p>2017-01-01</p> <p>Long-term <span class="hlt">decadal</span>-scale shoreline change is an important parameter for quantifying the stability of coastal systems. The <span class="hlt">decadal</span>-scale coastal change is controlled by processes that occur on short time scales (such as storms) and long-term processes (such as prevailing waves). The ability to predict <span class="hlt">decadal</span>-scale shoreline change is not well established and the fundamental physical processes controlling this change are not well understood. Here we investigate the processes that create large-scale long-term shoreline change along the Outer Banks of North Carolina, an uninterrupted 60 km stretch of coastline, using both <span class="hlt">observations</span> and a numerical modeling approach. Shoreline positions for a 24-yr period were derived from aerial photographs of the Outer Banks. Analysis of the shoreline position data showed that, although <span class="hlt">variable</span>, the shoreline eroded an average of 1.5 m/yr throughout this period. The modeling approach uses a three-dimensional hydrodynamics-based numerical model coupled to a spectral wave model and simulates the full 24-yr time period on a spatial grid running on a short (second scale) time-step to compute the sediment transport patterns. The <span class="hlt">observations</span> and the model results show similar magnitudes (O(105 m3/yr)) and patterns of alongshore sediment fluxes. Both the <span class="hlt">observed</span> and the modeled alongshore sediment transport rates have more rapid changes at the north of our section due to continuously curving coastline, and possible effects of alongshore variations in shelf bathymetry. The southern section with a relatively uniform orientation, on the other hand, has less rapid transport rate changes. Alongshore gradients of the modeled sediment fluxes are translated into shoreline change rates that have agreement in some locations but vary in others. Differences between <span class="hlt">observations</span> and model results are potentially influenced by geologic framework processes not included in the model. Both the <span class="hlt">observations</span> and the model results show higher rates of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GMD....11..351P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GMD....11..351P"><span>Parametric <span class="hlt">decadal</span> climate forecast recalibration (DeFoReSt 1.0)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pasternack, Alexander; Bhend, Jonas; Liniger, Mark A.; Rust, Henning W.; Müller, Wolfgang A.; Ulbrich, Uwe</p> <p>2018-01-01</p> <p>Near-term climate predictions such as <span class="hlt">decadal</span> climate forecasts are increasingly being used to guide adaptation measures. For near-term probabilistic predictions to be useful, systematic errors of the forecasting systems have to be corrected. While methods for the calibration of probabilistic forecasts are readily available, these have to be adapted to the specifics of <span class="hlt">decadal</span> climate forecasts including the long time horizon of <span class="hlt">decadal</span> climate forecasts, lead-time-dependent systematic errors (drift) and the errors in the representation of long-term changes and <span class="hlt">variability</span>. These features are compounded by small ensemble sizes to describe forecast uncertainty and a relatively short period for which typically pairs of reforecasts and <span class="hlt">observations</span> are available to estimate calibration parameters. We introduce the <span class="hlt">Decadal</span> Climate Forecast Recalibration Strategy (DeFoReSt), a parametric approach to recalibrate <span class="hlt">decadal</span> ensemble forecasts that takes the above specifics into account. DeFoReSt optimizes forecast quality as measured by the continuous ranked probability score (CRPS). Using a toy model to generate synthetic forecast <span class="hlt">observation</span> pairs, we demonstrate the positive effect on forecast quality in situations with pronounced and limited predictability. Finally, we apply DeFoReSt to <span class="hlt">decadal</span> surface temperature forecasts from the MiKlip prototype system and find consistent, and sometimes considerable, improvements in forecast quality compared with a simple calibration of the lead-time-dependent systematic errors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AAN...529....1W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AAN...529....1W"><span><span class="hlt">Observing</span> campaign on 5 <span class="hlt">variables</span> in Cygnus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waagen, Elizabeth O.</p> <p>2015-10-01</p> <p>Dr. George Wallerstein (University of Washington) has requested AAVSO assistance in monitoring 5 <span class="hlt">variable</span> stars in Cygnus now through December 2015. He is working to complete the radial velocity curves for these stars, and needs optical light curves for correlation with the spectra he will be obtaining. Wallerstein writes: "I need to know the time of max or min so I can assign a phase to each spectrum. Most classical Cepheids are quite regular so once a time of max or min can be established I can derive the phase of each <span class="hlt">observation</span> even if my obs are several cycles away from the established max or min. MZ Cyg is a type II Cepheid and they are less regular than their type I cousins." SZ Cyg, X Cyg, VX Cyg, and TX Cyg are all classical Cepheids. V and visual <span class="hlt">observations</span> are requested. These are long-period Cepheids, so nightly <span class="hlt">observations</span> are sufficient. Finder charts with sequence may be created using the AAVSO <span class="hlt">Variable</span> Star Plotter (https://www.aavso.org/vsp). <span class="hlt">Observations</span> should be submitted to the AAVSO International Database. See full Alert Notice for more details.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1127130','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1127130"><span>Collaborative Research: Separating Forced and Unforced <span class="hlt">Decadal</span> Predictability in Models and <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tippett, Michael K.</p> <p>2014-04-09</p> <p>This report is a progress report of the accomplishments of the research grant “Collaborative Research: Separating Forced and Unforced <span class="hlt">Decadal</span> Predictability in Models and Observa- tions” during the period 1 May 2011- 31 August 2013. This project is a collaborative one between Columbia University and George Mason University. George Mason University will submit a final technical report at the conclusion of their no-cost extension. The purpose of the proposed research is to identify unforced predictable components on <span class="hlt">decadal</span> time scales, distinguish these components from forced predictable components, and to assess the reliability of model predictions of these components. Components ofmore » unforced <span class="hlt">decadal</span> predictability will be isolated by maximizing the Average Predictability Time (APT) in long, multimodel control runs from state-of-the-art climate models. Components with <span class="hlt">decadal</span> predictability have large APT, so maximizing APT ensures that components with <span class="hlt">decadal</span> predictability will be detected. Optimal fingerprinting techniques, as used in detection and attribution analysis, will be used to separate variations due to natural and anthropogenic forcing from those due to unforced <span class="hlt">decadal</span> predictability. This methodology will be applied to the <span class="hlt">decadal</span> hindcasts generated by the CMIP5 project to assess the reliability of model projections. The question of whether anthropogenic forcing changes <span class="hlt">decadal</span> predictability, or gives rise to new forms of <span class="hlt">decadal</span> predictability, also will be investigated.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4938Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4938Z"><span><span class="hlt">Decadal</span> predictions of Southern Ocean sea ice : testing different initialization methods with an Earth-system Model of Intermediate Complexity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zunz, Violette; Goosse, Hugues; Dubinkina, Svetlana</p> <p>2013-04-01</p> <p>The sea ice extent in the Southern Ocean has increased since 1979 but the causes of this expansion have not been firmly identified. In particular, the contribution of internal <span class="hlt">variability</span> and external forcing to this positive trend has not been fully established. In this region, the lack of <span class="hlt">observations</span> and the overestimation of internal <span class="hlt">variability</span> of the sea ice by contemporary General Circulation Models (GCMs) make it difficult to understand the behaviour of the sea ice. Nevertheless, if its evolution is governed by the internal <span class="hlt">variability</span> of the system and if this internal <span class="hlt">variability</span> is in some way predictable, a suitable initialization method should lead to simulations results that better fit the reality. Current GCMs <span class="hlt">decadal</span> predictions are generally initialized through a nudging towards some <span class="hlt">observed</span> fields. This relatively simple method does not seem to be appropriated to the initialization of sea ice in the Southern Ocean. The present study aims at identifying an initialization method that could improve the quality of the predictions of Southern Ocean sea ice at <span class="hlt">decadal</span> timescales. We use LOVECLIM, an Earth-system Model of Intermediate Complexity that allows us to perform, within a reasonable computational time, the large amount of simulations required to test systematically different initialization procedures. These involve three data assimilation methods: a nudging, a particle filter and an efficient particle filter. In a first step, simulations are performed in an idealized framework, i.e. data from a reference simulation of LOVECLIM are used instead of <span class="hlt">observations</span>, herein after called pseudo-<span class="hlt">observations</span>. In this configuration, the internal <span class="hlt">variability</span> of the model obviously agrees with the one of the pseudo-<span class="hlt">observations</span>. This allows us to get rid of the issues related to the overestimation of the internal <span class="hlt">variability</span> by models compared to the <span class="hlt">observed</span> one. This way, we can work out a suitable methodology to assess the efficiency of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.6423S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.6423S"><span>Two centuries of <span class="hlt">observed</span> atmospheric <span class="hlt">variability</span> and change over the North Sea region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stendel, Martin; van den Besselaar, Else; Hannachi, Abdel; Kent, Elizabeth; Lefebvre, Christiana; Rosenhagen, Gudrun; Schenk, Frederik; van der Schrier, Gerard; Woollings, Tim</p> <p>2016-04-01</p> <p>In the upcoming North Sea Region Climate Change Assessment (NOSCCA), we present a synthesis of current knowledge about past, present and possible future climate change in the North Sea region. A climate change assessment from published scientific work has been conducted as a kind of regional IPCC report, and a book has been produced that will be published by Springer in 2016. In the framework of the NOSCCA project, we examine past and present studies of <span class="hlt">variability</span> and changes in atmospheric <span class="hlt">variables</span> within the North Sea region over the instrumental period, roughly the past 200 years, based on <span class="hlt">observations</span> and reanalyses. The <span class="hlt">variables</span> addressed in this presentation are large-scale circulation, pressure and wind, surface air temperature, precipitation and radiative properties (clouds, solar radiation, and sunshine duration). While air temperature over land, not unexpectedly, has increased everywhere in the North Sea region, with strongest trends in spring and in the north of the region, a precipitation increase has been <span class="hlt">observed</span> in the north and a decrease in the south of the region. This pattern goes along with a north-eastward shift of storm tracks and is in agreement with climate model projections under enhanced greenhouse gas concentrations. For other <span class="hlt">variables</span>, it is not obvious which part of the <span class="hlt">observed</span> changes may be due to anthropogenic activities and which is internally forced. It remains also unclear to what extent atmospheric circulation over the North Sea region is influenced by distant factors, in particular Arctic sea-ice decline in recent <span class="hlt">decades</span>. There are indications of an increase in the number of deep cyclones (but not in the total number of cyclones), while storminess since the late 19th century shows no robust trends. The persistence of circulation types appears to have increased over the last century, and consequently, there is an indication for 'more extreme' extreme events. However, changes in extreme weather events are difficult to assess</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1280976','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1280976"><span>Initialized <span class="hlt">decadal</span> prediction for transition to positive phase of the Interdecadal Pacific Oscillation</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Meehl, Gerald A.; Hu, Aixue; Teng, Haiyan</p> <p></p> <p>The negative phase of the Interdecadal Pacific Oscillation (IPO), a dominant mode of multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of sea surface temperatures (SSTs) in the Pacific, contributed to the reduced rate of global surface temperature warming in the early 2000s. Here, a proposed mechanism for IPO multidecadal <span class="hlt">variability</span> indicates that the presence of <span class="hlt">decadal</span> timescale upper ocean heat content in the off-equatorial western tropical Pacific can provide conditions for an interannual El Nino/Southern Oscillation event to trigger a transition of tropical Pacific SSTs to the opposite IPO phase. Here we show that a <span class="hlt">decadal</span> prediction initialized in 2013 simulates predicted Nino3.4 SSTs thatmore » have qualitatively tracked the <span class="hlt">observations</span> through 2015. The year three to seven average prediction (2015-2019) from the 2013 initial state shows a transition to the positive phase of the IPO from the previous negative phase and a resumption of larger rates of global warming over the 2013-2022 period consistent with a positive IPO phase.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1280976-initialized-decadal-prediction-transition-positive-phase-interdecadal-pacific-oscillation','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1280976-initialized-decadal-prediction-transition-positive-phase-interdecadal-pacific-oscillation"><span>Initialized <span class="hlt">decadal</span> prediction for transition to positive phase of the Interdecadal Pacific Oscillation</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Meehl, Gerald A.; Hu, Aixue; Teng, Haiyan</p> <p>2016-06-02</p> <p>The negative phase of the Interdecadal Pacific Oscillation (IPO), a dominant mode of multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of sea surface temperatures (SSTs) in the Pacific, contributed to the reduced rate of global surface temperature warming in the early 2000s. Here, a proposed mechanism for IPO multidecadal <span class="hlt">variability</span> indicates that the presence of <span class="hlt">decadal</span> timescale upper ocean heat content in the off-equatorial western tropical Pacific can provide conditions for an interannual El Nino/Southern Oscillation event to trigger a transition of tropical Pacific SSTs to the opposite IPO phase. Here we show that a <span class="hlt">decadal</span> prediction initialized in 2013 simulates predicted Nino3.4 SSTs thatmore » have qualitatively tracked the <span class="hlt">observations</span> through 2015. The year three to seven average prediction (2015-2019) from the 2013 initial state shows a transition to the positive phase of the IPO from the previous negative phase and a resumption of larger rates of global warming over the 2013-2022 period consistent with a positive IPO phase.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H31F1268H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H31F1268H"><span>Water Cycle Missions for the Next <span class="hlt">Decade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houser, P. R.</p> <p>2013-12-01</p> <p>The global water cycle describes the circulation of water as a vital and dynamic substance in its liquid, solid, and vapor phases as it moves through the atmosphere, oceans and land. Life in its many forms exists because of water, and modern civilization depends on learning how to live within the constraints imposed by the availability of water. The scientific challenge posed by the need to <span class="hlt">observe</span> the global water cycle is to integrate in situ and space-borne <span class="hlt">observations</span> to quantify the key water-cycle state <span class="hlt">variables</span> and fluxes. The vision to address that challenge is a series of Earth <span class="hlt">observation</span> missions that will measure the states, stocks, flows, and residence times of water on regional to global scales followed by a series of coordinated missions that will address the processes, on a global scale, that underlie <span class="hlt">variability</span> and changes in water in all its three phases. The accompanying societal challenge is to foster the improved use of water data and information as a basis for enlightened management of water resources, to protect life and property from effects of extremes in the water cycle. A major change in thinking about water science that goes beyond its physics to include its role in ecosystems and society is also required. Better water-cycle <span class="hlt">observations</span>, especially on the continental and global scales, will be essential. Water-cycle predictions need to be readily available globally to reduce loss of life and property caused by water-related natural hazards. Building on the 2007 Earth Science <span class="hlt">Decadal</span> Survey, NASA's Plan for a Climate-Centric Architecture for Earth <span class="hlt">Observations</span> and Applications from Space , and the 2012 Chapman Conference on Remote Sensing of the Terrestrial Water Cycle, a workshop was held in April 2013 to gather wisdom and determine how to prepare for the next generation of water cycle missions in support of the second Earth Science <span class="hlt">Decadal</span> Survey. This talk will present the outcomes of the workshop including the intersection between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC41B1095S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC41B1095S"><span>An Investigation of the Hydroclimate <span class="hlt">Variability</span> of Eastern Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, K. A.; Semazzi, F. H. M.</p> <p>2015-12-01</p> <p>The flow of the Victoria Nile, and the productivity of the dams along it, is determined by the level of Lake Victoria, which is primarily dictated by the rainfall and temperature <span class="hlt">variability</span> over the Lake Victoria Basin. Notwithstanding the indisputable decline of water resources over the lake basin during the Long Rains of March - May, there is a strong indication based on IPCC climate projections that this trend, which has persisted for several <span class="hlt">decades</span>, will reverse in the next few <span class="hlt">decades</span>. This phenomenon has come to be known as the Eastern-Central African climate change paradox and could have profound implications on sustainable development for the next few <span class="hlt">decades</span> in Lake Victoria Basin. The purpose of this study is to investigate the climate <span class="hlt">variability</span> associated with the East African Climate Change Paradox for the recent <span class="hlt">decades</span>. This research analyzes <span class="hlt">observations</span> to understand the sources of <span class="hlt">variability</span> and potential physical mechanisms related to the decline in precipitation over Eastern Africa. We then investigate the hydrological factors involved in the decline of Lake Victoria levels in the context of the decline in rainfall. While East Africa has been experiencing persistent decline of the Long Rains for multiple <span class="hlt">decades</span>, this same decline is not seen in annual rainfall. The remaining seasons show an increase in rainfall which is compensating for the decline of the Long Rains. It is possible that the Long Rains season is shifting in such a way that the season starts earlier, in February, and ending sooner. The corresponding annual Lake Victoria levels modeled using <span class="hlt">observed</span> rainfall do not decline in the recent <span class="hlt">decades</span>, except when the Long Rains seasonal <span class="hlt">variability</span> is considered without <span class="hlt">variability</span> from other seasons. This shift could impact hydroelectric power planning on a monthly or seasonal time scale, and could potentially have a large impact on agriculture, since it would shift the growing season in the region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRC..119.1237Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRC..119.1237Z"><span><span class="hlt">Decadal</span> variations of Pacific North Equatorial Current bifurcation from multiple ocean products</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhai, Fangguo; Wang, Qingye; Wang, Fujun; Hu, Dunxin</p> <p>2014-02-01</p> <p>In this study, we examine the <span class="hlt">decadal</span> variations of the Pacific North Equatorial Current (NEC) bifurcation latitude (NBL) averaged over upper 100 m and underlying dynamics over the past six <span class="hlt">decades</span> using 11 ocean products, including seven kinds of ocean reanalyzes based on ocean data assimilation systems, two kinds of numerical simulations without assimilating <span class="hlt">observations</span> and two kinds of objective analyzes based on in situ <span class="hlt">observations</span> only. During the period of 1954-2007, the multiproduct mean of <span class="hlt">decadal</span> NBL anomalies shows maxima around 1965/1966, 1980/1981, 1995/1996, and 2003/2004, and minima around 1958, 1971/1972, 1986/1987, and 2000/2001, respectively. The NBL <span class="hlt">decadal</span> variations are related to the first Empirical Orthogonal Function mode of <span class="hlt">decadal</span> anomalies of sea surface height (SSH) in the northwestern tropical Pacific Ocean, which shows spatially coherent variation over the whole region and explains most of the total variance. Further regression and composite analyzes indicate that northerly/southerly NBL corresponds to negative/positive SSH anomalies and cyclonic/anticyclonic gyre anomalies in the northwestern tropical Pacific Ocean. These <span class="hlt">decadal</span> circulation variations and thus the <span class="hlt">decadal</span> NBL variations are governed mostly by the first two vertical modes and attribute the most to the first baroclinic mode. The NBL <span class="hlt">decadal</span> variation is highly positively correlated with the tropical Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> (TPDV) around the zero time lag. With a lead of about half the <span class="hlt">decadal</span> cycle the NBL displays closer but negative relationship to TPDV in four ocean products, possibly manifesting the dynamical role of the circulation in the northwestern tropical Pacific in the phase-shifting of TPDV.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50.1471K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50.1471K"><span>Model under-representation of <span class="hlt">decadal</span> Pacific trade wind trends and its link to tropical Atlantic bias</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kajtar, Jules B.; Santoso, Agus; McGregor, Shayne; England, Matthew H.; Baillie, Zak</p> <p>2018-02-01</p> <p>The strengthening of the Pacific trade winds in recent <span class="hlt">decades</span> has been unmatched in the <span class="hlt">observational</span> record stretching back to the early twentieth century. This wind strengthening has been connected with numerous climate-related phenomena, including accelerated sea-level rise in the western Pacific, alterations to Indo-Pacific ocean currents, increased ocean heat uptake, and a slow-down in the rate of global-mean surface warming. Here we show that models in the Coupled Model Intercomparison Project phase 5 underestimate the <span class="hlt">observed</span> range of <span class="hlt">decadal</span> trends in the Pacific trade winds, despite capturing the range in <span class="hlt">decadal</span> sea surface temperature (SST) <span class="hlt">variability</span>. Analysis of <span class="hlt">observational</span> data suggests that tropical Atlantic SST contributes considerably to the Pacific trade wind trends, whereas the Atlantic feedback in coupled models is muted. Atmosphere-only simulations forced by <span class="hlt">observed</span> SST are capable of recovering the time-variation and the magnitude of the trade wind trends. Hence, we explore whether it is the biases in the mean or in the anomalous SST patterns that are responsible for the under-representation in fully coupled models. Over interannual time-scales, we find that model biases in the patterns of Atlantic SST anomalies are the strongest source of error in the precipitation and atmospheric circulation response. In contrast, on <span class="hlt">decadal</span> time-scales, the magnitude of the model biases in Atlantic mean SST are directly linked with the trade wind <span class="hlt">variability</span> response.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AAS...22915803L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AAS...22915803L"><span>Caroline Furness and the Evolution of Visual <span class="hlt">Variable</span> Star <span class="hlt">Observing</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Larsen, Kristine</p> <p>2017-01-01</p> <p>An Introduction to the Study of <span class="hlt">Variable</span> Stars by Dr. Caroline Ellen Furness (1869-1936), Director of the Vassar College Observatory, was published in October 2015. Issued in honor of the fiftieth anniversary of the founding of Vassar College, the work was meant to fill a void in the literature, namely as both an introduction to the topic of <span class="hlt">variable</span> stars as well as a manual explaining how they should be <span class="hlt">observed</span> and the resulting data analyzed. It was judged to be one of the hundred best books written by an American woman in the last hundred years at the 1933 World’s Fair in Chicago. The book covers the relevant history of and background on types of <span class="hlt">variable</span> stars, star charts, catalogs, and the magnitude scale, then describes <span class="hlt">observing</span> techniques, including visual, photographic, and photoelectric photometry. The work finishes with a discussion of light curves and patterns of <span class="hlt">variability</span>, with a special emphasis on eclipsing binaries and long period <span class="hlt">variables</span>. Furness’s work is therefore a valuable snapshot of the state of astronomical knowledge, technology, and <span class="hlt">observing</span> techniques from a century ago. Furness’s book and its reception in the scientific community are analyzed, and parallels with (and departures from) the current advice given by the AAVSO to beginning <span class="hlt">variable</span> star <span class="hlt">observers</span> today are highlighted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27573049','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27573049"><span><span class="hlt">Decadal</span>-Scale Forecasting of Climate Drivers for Marine Applications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Salinger, J; Hobday, A J; Matear, R J; O'Kane, T J; Risbey, J S; Dunstan, P; Eveson, J P; Fulton, E A; Feng, M; Plagányi, É E; Poloczanska, E S; Marshall, A G; Thompson, P A</p> <p></p> <p>Climate influences marine ecosystems on a range of time scales, from weather-scale (days) through to climate-scale (hundreds of years). Understanding of interannual to <span class="hlt">decadal</span> climate <span class="hlt">variability</span> and impacts on marine industries has received less attention. Predictability up to 10 years ahead may come from large-scale climate modes in the ocean that can persist over these time scales. In Australia the key drivers of climate <span class="hlt">variability</span> affecting the marine environment are the Southern Annular Mode, the Indian Ocean Dipole, the El Niño/Southern Oscillation, and the Interdecadal Pacific Oscillation, each has phases that are associated with different ocean circulation patterns and regional environmental <span class="hlt">variables</span>. The roles of these drivers are illustrated with three case studies of extreme events-a marine heatwave in Western Australia, a coral bleaching of the Great Barrier Reef, and flooding in Queensland. Statistical and dynamical approaches are described to generate forecasts of climate drivers that can subsequently be translated to useful information for marine end users making decisions at these time scales. Considerable investment is still needed to support <span class="hlt">decadal</span> forecasting including improvement of ocean-atmosphere models, enhancement of <span class="hlt">observing</span> systems on all scales to support initiation of forecasting models, collection of important biological data, and integration of forecasts into decision support tools. Collaboration between forecast developers and marine resource sectors-fisheries, aquaculture, tourism, biodiversity management, infrastructure-is needed to support forecast-based tactical and strategic decisions that reduce environmental risk over annual to <span class="hlt">decadal</span> time scales. © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.B11G..04P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.B11G..04P"><span>Wetland inventory and <span class="hlt">variability</span> over the last two <span class="hlt">decades</span> at a global scale</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prigent, C.; Papa, F.; Aires, F.; Rossow, W. B.; Matthews, E.</p> <p>2011-12-01</p> <p>Remote sensing techniques employing visible, infrared, and microwave <span class="hlt">observations</span> offer varying success in estimating wetlands and inundation extent and in monitoring their natural and anthropogenic variations. Low spatial resolution (e.g., 30 km) limits detection to large wetlands but has the advantage of frequent coverage. High spatial resolution (e.g., 100 m), while providing more environmental information, suffers from poor temporal resolution, with <span class="hlt">observations</span> for just high/low water or warm/cold seasons. Most existing wetland data sets are limited to a few regions, for specific times in the year. The only global inventories of wetland dynamics over a long period of time is derived from a remote-sensing technique employing a suite of complementary satellite <span class="hlt">observations</span>: it uses passive microwave land-surface microwave emissivities, scatterometer responses, and visible and near infrared reflectances. Combining <span class="hlt">observations</span> from different instruments makes it possible to capitalize on their complementary strengths, and to extract maximum information about inundation characteristics. The technique is globally applicable without any tuning for particular environments. The satellite data are used to calculate monthly-mean inundated fractions of equal-area grid cells (0.25°x0.25° at the equator), taking into account the contribution of vegetation to the passive microwave signal (Prigent et al., 2001, 2007). Several adjustments to the initial technique have been applied to account for changes in satellite instruments (Papa et al., 2010). The resulting data set now covers 1993-2008 and has been carefully evaluated. We will present the inter-annual <span class="hlt">variability</span> of the water surface extents under different environments, and relate these variations to other hydrological <span class="hlt">variables</span> such as river height, precipitation, water runoff, or Grace data. Natural wetlands are the world's largest methane source and dominate the inter-annual <span class="hlt">variability</span> of atmospheric methane</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000112946','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000112946"><span><span class="hlt">Decadal</span> <span class="hlt">Variability</span> and Temperature Trends in the Middle Atmosphere From Historical Rocketsonde Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dunkerton, Timothy J.</p> <p>2000-01-01</p> <p><span class="hlt">Observational</span> studies were performed using historical rocketsonde data to investigate long-term temperature trends, solar-cycle variations, and interactions between tropical and extratropical latitudes in the middle atmosphere. Evidence from tropical, subtropical, and midlatitude North American rocketsonde stations indicated a consistent downward trend over 25 years, with a solar cycle component superposed. The trend is about -1.4 to -2.0 K per <span class="hlt">decade</span> and the amplitude of the <span class="hlt">decadal</span> oscillation is about 1.1 K. Prior to trend derivation it was necessary for us to correct temperatures for aerodynamic heating in the early years. The empirically derived correction profile agrees well with a theoretical profile of Krumins and Lyons. A study was also performed of the correlation between equatorial winds and north polar temperatures in winter, showing that the entire stratospheric wind profile near the equator -- including the quasi-biennial oscillation (QBO) and stratopause semiannual oscillation (SAO) -- is important to the extratropical flow, not merely the QBO component as previously thought. A strong correlation was discovered between winter polar temperatures and equatorial winds in the upper stratosphere during the preceding September, suggesting a role for the second cycle of the SAO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4103L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4103L"><span>A Possible Cause for Recent <span class="hlt">Decadal</span> Atlantic Meridional Overturning Circulation Decline</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Latif, Mojib; Park, Taewook; Park, Wonsun</p> <p>2017-04-01</p> <p>The Atlantic Meridional Overturning Circulation (AMOC) is a major oceanic current system with widespread climate impacts. AMOC influences have been discussed among others with regard to Atlantic hurricane activity, regional sea level <span class="hlt">variability</span>, and surface air temperature and precipitation changes on land areas adjacent to the North Atlantic Ocean. Most climate models project significant AMOC slowing during the 21st century, if atmospheric greenhouse gas concentrations continue to rise unabatedly. Recently, a marked <span class="hlt">decadal</span> decline in AMOC strength has been <span class="hlt">observed</span>, which was followed by strongly reduced oceanic poleward heat transport and record low sea surface temperature in parts of the North Atlantic. Here, we provide evidence from <span class="hlt">observations</span>, re-analyses and climate models that the AMOC decline was due to the combined action of the North Atlantic Oscillation and East Atlantic Pattern, the two leading modes of North Atlantic atmospheric surface pressure <span class="hlt">variability</span>, which prior to the decline both transitioned into their negative phases. This change in atmospheric circulation diminished oceanic heat loss over the Labrador Sea and forced ocean circulation changes lowering upper ocean salinity transport into that region. As a consequence, Labrador Sea deep convection weakened, which eventually slowed the AMOC. This study suggests a new mechanism for <span class="hlt">decadal</span> AMOC <span class="hlt">variability</span>, which is important to multiyear climate predictability and climate change detection in the North Atlantic sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSOD24B2461H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSOD24B2461H"><span>The Gulf of Mexico Coastal Ocean <span class="hlt">Observing</span> System: A <span class="hlt">Decade</span> of Data Aggregation and Services.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Howard, M.; Gayanilo, F.; Kobara, S.; Baum, S. K.; Currier, R. D.; Stoessel, M. M.</p> <p>2016-02-01</p> <p>The Gulf of Mexico Coastal Ocean <span class="hlt">Observing</span> System Regional Association (GCOOS-RA) celebrated its 10-year anniversary in 2015. GCOOS-RA is one of 11 RAs organized under the NOAA-led U.S. Integrated Ocean <span class="hlt">Observing</span> System (IOOS) Program Office to aggregate regional data and make these data publicly-available in preferred forms and formats via standards-based web services. Initial development of GCOOS focused on building elements of the IOOS Data Management and Communications Plan which is a framework for end-to-end interoperability. These elements included: data discovery, catalog, metadata, online-browse, data access and transport. Initial data types aggregated included near real-time physical oceanographic, marine meteorological and satellite data. Our focus in the middle of the past <span class="hlt">decade</span> was on the production of basic products such as maps of current oceanographic conditions and quasi-static datasets such as bathymetry and climatologies. In the latter part of the <span class="hlt">decade</span> we incorporated historical physical oceanographic datasets and historical coastal and offshore water quality data into our holdings and added our first biological dataset. We also developed web environments and products to support Citizen Scientists and stakeholder groups such as recreational boaters. Current efforts are directed towards applying data quality assurance (testing and flagging) to non-federal data, data archiving at national repositories, serving and visualizing numerical model output, providing data services for glider operators, and supporting marine biodiversity <span class="hlt">observing</span> networks. GCOOS Data Management works closely with the Gulf of Mexico Research Initiative Information and Data Cooperative and various groups involved with Gulf Restoration. GCOOS-RA has influenced attitudes and behaviors associated with good data stewardship and data management practices across the Gulf and will to continue to do so into the next <span class="hlt">decade</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ThApC.tmp..179L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ThApC.tmp..179L"><span>Inter-<span class="hlt">decadal</span> change in potential predictability of the East Asian summer monsoon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Jiao; Ding, Ruiqiang; Wu, Zhiwei; Zhong, Quanjia; Li, Baosheng; Li, Jianping</p> <p>2018-05-01</p> <p>The significant inter-<span class="hlt">decadal</span> change in potential predictability of the East Asian summer monsoon (EASM) has been investigated using the signal-to-noise ratio method. The relatively low potential predictability appears from the early 1950s through the late 1970s and during the early 2000s, whereas the potential predictability is relatively high from the early 1980s through the late 1990s. The inter-<span class="hlt">decadal</span> change in potential predictability of the EASM can be attributed mainly to variations in the external signal of the EASM. The latter is mostly caused by the El Niño-Southern Oscillation (ENSO) inter-<span class="hlt">decadal</span> <span class="hlt">variability</span>. As a major external signal of the EASM, the ENSO inter-<span class="hlt">decadal</span> <span class="hlt">variability</span> experiences phase transitions from negative to positive phases in the late 1970s, and to negative phases in the late 1990s. Additionally, ENSO is generally strong (weak) during a positive (negative) phase of the ENSO inter-<span class="hlt">decadal</span> <span class="hlt">variability</span>. The strong ENSO is expected to have a greater influence on the EASM, and vice versa. As a result, the potential predictability of the EASM tends to be high (low) during a positive (negative) phase of the ENSO inter-<span class="hlt">decadal</span> <span class="hlt">variability</span>. Furthermore, a suite of Pacific Pacemaker experiments suggests that the ENSO inter-<span class="hlt">decadal</span> <span class="hlt">variability</span> may be a key pacemaker of the inter-<span class="hlt">decadal</span> change in potential predictability of the EASM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026788','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026788"><span>Tree-ring based reconstructions of interannual to <span class="hlt">decadal</span> scale precipitation <span class="hlt">variability</span> for northeastern Utah since 1226 A.D.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gray, S.T.; Jackson, S.T.; Betancourt, J.L.</p> <p>2004-01-01</p> <p>Samples from 107 pin??on pines (Pinus edulis) at four sites were used to develop a proxy record of annual (June to June) precipitation spanning the 1226 to 2001 AD interval for the Uinta Basin Watershed of northeastern Utah. The reconstruction reveals significant precipitation <span class="hlt">variability</span> at interannual to <span class="hlt">decadal</span> scales. Single-year dry events before the instrumental period tended to be more severe than those after 1900. In general, <span class="hlt">decadal</span> scale dry events were longer and more severe prior to 1900. In particular, dry events in the late 13th, 16th, and 18th Centuries surpass the magnitude and duration of droughts seen in the Uinta Basin after 1900. The last four <span class="hlt">decades</span> of the 20th Century also represent one of the wettest periods in the reconstruction. The proxy record indicates that the instrumental record (approximately 1900 to the Present) underestimates the potential frequency and severity of severe, sustained droughts in this area, while over representing the prominence of wet episodes. In the longer record, the empirical probability of any <span class="hlt">decadal</span> scale drought exceeding the duration of the 1954 through 1964 drought is 94 percent, while the probability for any wet event exceeding the duration of the 1965 through 1999 wet spell is only 1 percent. Hence, estimates of future water availability in the Uinta Basin and forecasts for exports to the Colorado River, based on the 1961 to 1990 and 1971 to 2000 "normal" periods, may be overly optimistic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29760117','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29760117"><span>Inter-<span class="hlt">decadal</span> <span class="hlt">variability</span> of phytoplankton biomass along the coastal West Antarctic Peninsula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Hyewon; Ducklow, Hugh W; Abele, Doris; Ruiz Barlett, Eduardo M; Buma, Anita G J; Meredith, Michael P; Rozema, Patrick D; Schofield, Oscar M; Venables, Hugh J; Schloss, Irene R</p> <p>2018-06-28</p> <p>The West Antarctic Peninsula (WAP) is a climatically sensitive region where periods of strong warming have caused significant changes in the marine ecosystem and food-web processes. Tight coupling between phytoplankton and higher trophic levels implies that the coastal WAP is a bottom-up controlled system, where changes in phytoplankton dynamics may largely impact other food-web components. Here, we analysed the inter-<span class="hlt">decadal</span> time series of year-round chlorophyll- a (Chl) collected from three stations along the coastal WAP: Carlini Station at Potter Cove (PC) on King George Island, Palmer Station on Anvers Island and Rothera Station on Adelaide Island. There were trends towards increased phytoplankton biomass at Carlini Station (PC) and Palmer Station, while phytoplankton biomass declined significantly at Rothera Station over the studied period. The impacts of two relevant climate modes to the WAP, the El Niño-Southern Oscillation and the Southern Annular Mode, on winter and spring phytoplankton biomass appear to be different among the three sampling stations, suggesting an important role of local-scale forcing than large-scale forcing on phytoplankton dynamics at each station. The inter-annual <span class="hlt">variability</span> of seasonal bloom progression derived from considering all three stations together captured ecologically meaningful, seasonally co-occurring bloom patterns which were primarily constrained by water-column stability strength. Our findings highlight a coupled link between phytoplankton and physical and climate dynamics along the coastal WAP, which may improve our understanding of overall WAP food-web responses to climate change and <span class="hlt">variability</span>.This article is part of the theme issue 'The marine system of the West Antarctic Peninsula: status and strategy for progress in a region of rapid change'. © 2018 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000707','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000707"><span>A <span class="hlt">Decade</span> of Volcanic <span class="hlt">Observations</span> from Aura and the A-Train</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carn, Simon A.; Krotkov, Nickolay Anatoly; Yang, Kai; Krueger, Arlin J.; Hughes, Eric J.; Wang, Jun; Flower, Verity; Telling, Jennifer</p> <p>2014-01-01</p> <p>Aura <span class="hlt">observations</span> have made many seminal contributions to volcanology. Prior to the Aura launch, satellite <span class="hlt">observations</span> of volcanic degassing (e.g., from TOMS) were mostly restricted to large eruptions. However, the vast majority of volcanic gases are released during quiescent 'passive' degassing between eruptions. The improved sensitivity of Aura OMI permitted the first daily, space-borne measurements of passive volcanic SO2 degassing, providing improved constraints on the source locations and magnitude of global SO2 emissions for input to atmospheric chemistry and climate models. As a result of this unique sensitivity to volcanic activity, OMI data were also the first satellite SO2 measurements to be routinely used for volcano monitoring at several volcano observatories worldwide. Furthermore, the Aura OMI SO2 data also offer unprecedented sensitivity to volcanic clouds in the UTLS, elucidating the transport, fate and lifetime of volcanic SO2 and providing critical input to aviation hazard mitigation efforts. Another major advance has been the improved vertical resolution of volcanic clouds made possible by synergy between Aura and other A-Train instruments (e.g., AIRS, CALIPSO, CloudSat), advanced UV SO2 altitude retrievals, and inverse trajectory modeling of detailed SO2 cloud maps. This altitude information is crucial for climate models and aviation hazards. We will review some of the highlights of a <span class="hlt">decade</span> of Aura <span class="hlt">observations</span> of volcanic activity and look ahead to the future of volcanic <span class="hlt">observations</span> from space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS51A1975L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS51A1975L"><span>Tropical Atlantic Impacts on the <span class="hlt">Decadal</span> Climate <span class="hlt">Variability</span> of the Tropical Ocean and Atmosphere.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, X.; Xie, S. P.; Gille, S. T.; Yoo, C.</p> <p>2015-12-01</p> <p>Previous studies revealed atmospheric bridges between the tropical Pacific, Atlantic, and Indian Ocean. In particular, several recent works indicate that the Atlantic sea surface temperature (SST) may contribute to the climate <span class="hlt">variability</span> over the equatorial Pacific. Inspired by these studies, our work aims at investigating the impact of the tropical Atlantic on the entire tropical climate system, and uncovering the physical dynamics under these tropical teleconnections. We first performed a 'pacemaker' simulation by restoring the satellite era tropical Atlantic SST changes in a fully coupled model - the CESM1. Results reveal that the Atlantic warming heats the Indo-Western Pacific and cools the Eastern Pacific, enhances the Walker circulation and drives the subsurface Pacific to a La Niña mode, contributing to 60-70% of the above tropical changes in the past 30 years. The same pan-tropical teleconnections have been validated by the statistics of <span class="hlt">observations</span> and 106 CMIP5 control simulations. We then used a hierarchy of atmospheric and oceanic models with different complexities, to single out the roles of atmospheric dynamics, atmosphere-ocean fluxes, and oceanic dynamics in these teleconnections. With these simulations we established a two-step mechanism as shown in the schematic figure: 1) Atlantic warming generates an atmospheric deep convection and induces easterly wind anomalies over the Indo-Western Pacific in the form of Kelvin waves, and westerly wind anomalies over the eastern equatorial Pacific as Rossby waves, in line with Gill's solution. This circulation changes warms the Indo-Western Pacific and cools the Eastern Pacific with the wind-evaporation-SST effect, forming a temperature gradient over the Indo-Pacific basins. 2) The temperature gradient further generates a secondary atmospheric deep convection, which reinforces the easterly wind anomalies over the equatorial Pacific and enhances the Walker circulation, triggering the Pacific to a La Ni</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17731486','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17731486"><span>Galactic water vapor emission: further <span class="hlt">observations</span> of <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Knowles, S H; Mayer, C H; Sullivan, W T; Cheung, A C</p> <p>1969-10-10</p> <p>Recent <span class="hlt">observations</span> of the 1.35-centimeter line emission of water vapor from galactic sources show short-term <span class="hlt">variability</span> in the spectra of several sources. Two additional sources, Cygnus 1 and NGC 6334N, have been <span class="hlt">observed</span>, and the spectra of W49 and VY Canis Majoris were measured over a wider range of radial velocity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...94a2047R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...94a2047R"><span>Control of <span class="hlt">variable</span> speed <span class="hlt">variable</span> pitch wind turbine based on a disturbance <span class="hlt">observer</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, Haijun; Lei, Xin</p> <p>2017-11-01</p> <p>In this paper, a novel sliding mode controller based on disturbance <span class="hlt">observer</span> (DOB) to optimize the efficiency of <span class="hlt">variable</span> speed <span class="hlt">variable</span> pitch (VSVP) wind turbine is developed and analyzed. Due to the highly nonlinearity of the VSVP system, the model is linearly processed to obtain the state space model of the system. Then, a conventional sliding mode controller is designed and a DOB is added to estimate wind speed. The proposed control strategy can successfully deal with the random nature of wind speed, the nonlinearity of VSVP system, the uncertainty of parameters and external disturbance. Via adding the <span class="hlt">observer</span> to the sliding mode controller, it can greatly reduce the chattering produced by the sliding mode switching gain. The simulation results show that the proposed control system has the effectiveness and robustness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A51C0048Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A51C0048Z"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of the position and strength of the South Atlantic Convergence Zone and its relationship to precipitation <span class="hlt">variability</span> and extremes over Southeastern Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zilli, M. T.; Carvalho, L. V.; Lintner, B. R.</p> <p>2016-12-01</p> <p>The South Atlantic Convergence Zone (SACZ) is a diagonally oriented zone of low-level convergence, convective cloudiness, and rainfall originating over South America and extending to the southeast over the Atlantic Ocean. The objective of this study is to investigate the role of <span class="hlt">variability</span> in the position and strength of the SACZ in causing precipitation <span class="hlt">variability</span> and extremes over the southeastern Brazilian coast (SE). To that end, we perform Empirical Orthogonal Function (EOF) analysis of total summer (DJF) precipitation from 1979 to 2013, using the National Center for Environmental Prediction (NCEP) Climate Forecast System Reanalysis (CFSR), at 0.5° spatial resolution. The first mode (EOF-1) explains 22.7% of total variance and is characterized by a dipole-like structure, with opposite signs over central South America and over central South Atlantic along the northern margin of the SACZ. The time-coefficient or principal component of EOF-1 indicates a transition from a predominantly negative phase over 1999 to 2005 to a predominantly positive phase after 2006. The positive phase is associated with an increase in total precipitation over the continent and a reduction over the central South Atlantic, along the northern margin of the SACZ. These results provide evidence of the poleward shift of the SACZ and weakening of convergence along its northern margin over the past <span class="hlt">decade</span>, consistent with the <span class="hlt">observed</span> recent trends in extreme precipitation over SE. Compositing reanalysis fields with respect to the PC of EOF-1 suggests changes in moisture availability and circulation that could have affected precipitation regimes over SE. In particular, an increase in available precipitable water may have enhanced convective activity over the southern portion of SE Brazil, whereas the weakening of the northerly winds may be responsible for the weakening of convergence over the northern flank of the SACZ, inhibiting convection in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AAN...471....1W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AAN...471....1W"><span>Cataclysmic <span class="hlt">variables</span> to be monitored for HST <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waagen, Elizabeth O.</p> <p>2012-09-01</p> <p>Drs. Boris Gaensicke (Warwick University), Joseph Patterson (Columbia University, Center for Backyard Astrophysics), and Arne Henden (AAVSO), on behalf of a consortium of 16 astronomers, requested the help of AAVSO <span class="hlt">observers</span> in monitoring the ~40 cataclysmic <span class="hlt">variables</span> in support of Hubble Space Telescope <span class="hlt">observations</span> in the coming months. The HST COS (Cosmic Origins Spectrograph) will be carrying out far-ultraviolet spectroscopy of ~40 CVs sequentially, with the aim to measure the temperatures, atmospheric compositions, rotation rates, and eventually masses of their white dwarfs. The primary purpose of the monitoring is to know whether each target is in quiescence immediately prior to the <span class="hlt">observation</span> window; if it is in outburst it will be too bright for the HST instrumentation. Based on the information supplied by the AAVSO, the HST scheduling team will make the decision (usually) the evening before the scheduled <span class="hlt">observing</span> time as to whether to go forward with the HST <span class="hlt">observations</span>. For CCD <span class="hlt">observers</span>, simultaneous photometry [shortly before, during, and after the HST <span class="hlt">observations</span>] would be ideal. B filter would be best for a light curve, although for the magnitude estimates, V would be best. Finder charts may be created using the AAVSO <span class="hlt">Variable</span> Star Plotter (http://www.aavso.org/vsp). <span class="hlt">Observations</span> should be submitted to the AAVSO International Database. If the target is seen in outburst, please contact the AAVSO immediately and post a message to the <span class="hlt">Observations</span> and Campaigns & <span class="hlt">Observations</span> Reports forum (http://www.aavso.org/forum). This campaign will run the better part of a year or longer. See full Alert Notice for more details and list of objects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010100393','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010100393"><span><span class="hlt">Variability</span> of Antarctic Sea Ice 1979-1998</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Comiso, Josefino C.; Parkinson, Claire L.; Cavalieri, Donald J.; Gloersen, Per; Koblinsky, Chester J. (Technical Monitor)</p> <p>2001-01-01</p> <p>The principal characteristics of the <span class="hlt">variability</span> of Antarctic sea ice cover as previously described from satellite passive-microwave <span class="hlt">observations</span> are also evident in a systematically-calibrated and analyzed data set for 20.2 years (1979-1998). The total Antarctic sea ice extent (concentration > 15 %) increased by 13,440 +/- 4180 sq km/year (+1.18 +/- 0.37%/<span class="hlt">decade</span>). The area of sea ice within the extent boundary increased by 16,960 +/- 3,840 sq km/year (+1.96 +/- 0.44%/<span class="hlt">decade</span>). Regionally, the trends in extent are positive in the Weddell Sea (1.5 +/- 0.9%/<span class="hlt">decade</span>), Pacific Ocean (2.4 +/- 1.4%/<span class="hlt">decade</span>), and Ross (6.9 +/- 1.1 %/<span class="hlt">decade</span>) sectors, slightly negative in the Indian Ocean (-1.5 +/- 1.8%/<span class="hlt">decade</span>, and strongly negative in the Bellingshausen-Amundsen Seas sector (-9.5 +/- 1.5%/<span class="hlt">decade</span>). For the entire ice pack, small ice increases occur in all seasons with the largest increase during autumn. On a regional basis, the trends differ season to season. During summer and fall, the trends are positive or near zero in all sectors except the Bellingshausen-Amundsen Seas sector. During winter and spring, the trends are negative or near zero in all sectors except the Ross Sea, which has positive trends in all seasons. Components of interannual <span class="hlt">variability</span> with periods of about 3 to 5 years are regionally large, but tend to counterbalance each other in the total ice pack. The interannual <span class="hlt">variability</span> of the annual mean sea-ice extent is only 1.6% overall, compared to 5% to 9% in each of five regional sectors. Analysis of the relation between regional sea ice extents and spatially-averaged surface temperatures over the ice pack gives an overall sensitivity between winter ice cover and temperature of -0.7% change in sea ice extent per K. For summer, some regional ice extents vary positively with temperature and others negatively. The <span class="hlt">observed</span> increase in Antarctic sea ice cover is counter to the <span class="hlt">observed</span> decreases in the Arctic. It is also qualitatively consistent with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ESSD...10..919C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESSD...10..919C"><span>ReOBS: a new approach to synthesize long-term multi-<span class="hlt">variable</span> dataset and application to the SIRTA supersite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chiriaco, Marjolaine; Dupont, Jean-Charles; Bastin, Sophie; Badosa, Jordi; Lopez, Julio; Haeffelin, Martial; Chepfer, Helene; Guzman, Rodrigo</p> <p>2018-05-01</p> <p>A scientific approach is presented to aggregate and harmonize a set of 60 geophysical <span class="hlt">variables</span> at hourly timescale over a <span class="hlt">decade</span>, and to allow multiannual and multi-<span class="hlt">variable</span> studies combining atmospheric dynamics and thermodynamics, radiation, clouds and aerosols from ground-based <span class="hlt">observations</span>. Many datasets from ground-based <span class="hlt">observations</span> are currently in use worldwide. They are very valuable because they contain complete and precise information due to their spatio-temporal co-localization over more than a <span class="hlt">decade</span>. These datasets, in particular the synergy between different type of <span class="hlt">observations</span>, are under-used because of their complexity and diversity due to calibration, quality control, treatment, format, temporal averaging, metadata, etc. Two main results are presented in this article: (1) a set of methods available for the community to robustly and reliably process ground-based data at an hourly timescale over a <span class="hlt">decade</span> is described and (2) a single netCDF file is provided based on the SIRTA supersite <span class="hlt">observations</span>. This file contains approximately 60 geophysical <span class="hlt">variables</span> (atmospheric and in ground) hourly averaged over a <span class="hlt">decade</span> for the longest <span class="hlt">variables</span>. The netCDF file is available and easy to use for the community. In this article, <span class="hlt">observations</span> are <q>re-analyzed</q>. The prefix <q>re</q> refers to six main steps: calibration, quality control, treatment, hourly averaging, homogenization of the formats and associated metadata, as well as expertise on more than a <span class="hlt">decade</span> of <span class="hlt">observations</span>. In contrast, previous studies (i) took only some of these six steps into account for each <span class="hlt">variable</span>, (ii) did not aggregate all <span class="hlt">variables</span> together in a single file and (iii) did not offer an hourly resolution for about 60 <span class="hlt">variables</span> over a <span class="hlt">decade</span> (for the longest <span class="hlt">variables</span>). The approach described in this article can be applied to different supersites and to additional <span class="hlt">variables</span>. The main implication of this work is that complex atmospheric <span class="hlt">observations</span> are made readily available</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160013301&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160013301&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsea"><span>Assessment of Arctic and Antarctic Sea Ice Predictability in CMIP5 <span class="hlt">Decadal</span> Hindcasts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yang, Chao-Yuan; Liu, Jiping (Inventor); Hu, Yongyun; Horton, Radley M.; Chen, Liqi; Cheng, Xiao</p> <p>2016-01-01</p> <p>This paper examines the ability of coupled global climate models to predict <span class="hlt">decadal</span> <span class="hlt">variability</span> of Arctic and Antarctic sea ice. We analyze <span class="hlt">decadal</span> hindcasts/predictions of 11 Coupled Model Intercomparison Project Phase 5 (CMIP5) models. <span class="hlt">Decadal</span> hindcasts exhibit a large multimodel spread in the simulated sea ice extent, with some models deviating significantly from the <span class="hlt">observations</span> as the predicted ice extent quickly drifts away from the initial constraint. The anomaly correlation analysis between the <span class="hlt">decadal</span> hindcast and <span class="hlt">observed</span> sea ice suggests that in the Arctic, for most models, the areas showing significant predictive skill become broader associated with increasing lead times. This area expansion is largely because nearly all the models are capable of predicting the <span class="hlt">observed</span> decreasing Arctic sea ice cover. Sea ice extent in the North Pacific has better predictive skill than that in the North Atlantic (particularly at a lead time of 3-7 years), but there is a reemerging predictive skill in the North Atlantic at a lead time of 6-8 years. In contrast to the Arctic, Antarctic sea ice <span class="hlt">decadal</span> hindcasts do not show broad predictive skill at any timescales, and there is no obvious improvement linking the areal extent of significant predictive skill to lead time increase. This might be because nearly all the models predict a retreating Antarctic sea ice cover, opposite to the <span class="hlt">observations</span>. For the Arctic, the predictive skill of the multi-model ensemble mean outperforms most models and the persistence prediction at longer timescales, which is not the case for the Antarctic. Overall, for the Arctic, initialized <span class="hlt">decadal</span> hindcasts show improved predictive skill compared to uninitialized simulations, although this improvement is not present in the Antarctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010111482','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010111482"><span>Constraints on <span class="hlt">Variability</span> of Brightness and Surface Magnetism on Time Scales of <span class="hlt">Decades</span> to Centuries in the Sun and Sun-Like Stars: A Source of Potential Terrestrial Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Baliunas, Sallie L.; Sharber, James (Technical Monitor)</p> <p>2001-01-01</p> <p>These four points summarize our work to date. (1) Conciliation of solar and stellar photometric <span class="hlt">variability</span>. Previous research by us and colleagues suggested that the Sun might at present be showing unusually low photometric <span class="hlt">variability</span> compared to other sun-like stars. Those early results would question the suitability of the technique of using sun-like stars as proxies for solar irradiance change on time scales of <span class="hlt">decades</span> to centuries. However, our results indicate the contrary: the Sun's <span class="hlt">observed</span> short-term (seasonal) and longterm (year-to-year) brightness variations closely agree with <span class="hlt">observed</span> brightness variations in stars of similar mass and age. (2) We have demonstrated an inverse correlation between the global temperature of the terrestrial lower troposphere, inferred from the NASA Microwave Sounding Unit (MSU) radiometers, and the total area of the Sun covered by coronal holes from January 1979 to present (up to May 2000). <span class="hlt">Variable</span> fluxes of either solar charged particles or cosmic rays, or both, may influence the terrestrial tropospheric temperature. The geographical pattern of the correlation is consistent with our interpretation of an extra-terrestrial charged particle forcing. (3) Possible climate mechanism amplifying the impact of solar ultraviolet irradiance variations. The key points of our proposed climate hypersensitivity mechanism are: (a) The Sun is more <span class="hlt">variable</span> in the UV (ultraviolet) than in the visible. However, the increased UV irradiance is mainly absorbed in the lower stratosphere/upper troposphere rather than at the surface. (b) Absorption in the stratosphere raises the temperature moderately around the vicinity of the tropopause, and tends to stabilize the atmosphere against vertical convective/diffusive transport, thus decreasing the flux of heat and moisture carried upward from surface. (c) The decrease in the upward convection of heat and moisture tends to raise the surface temperature because a drier upper atmosphere becomes less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AuJAn..29...89H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AuJAn..29...89H"><span><span class="hlt">Observations</span> of red-giant <span class="hlt">variable</span> stars by Aboriginal Australians</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamacher, Duane W.</p> <p>2018-04-01</p> <p>Aboriginal Australians carefully <span class="hlt">observe</span> the properties and positions of stars, including both overt and subtle changes in their brightness, for subsistence and social application. These <span class="hlt">observations</span> are encoded in oral tradition. I examine two Aboriginal oral traditions from South Australia that describe the periodic changing brightness in three pulsating, red-giant <span class="hlt">variable</span> stars: Betelgeuse (Alpha Orionis), Aldebaran (Alpha Tauri), and Antares (Alpha Scorpii). The Australian Aboriginal accounts stand as the only known descriptions of pulsating <span class="hlt">variable</span> stars in any Indigenous oral tradition in the world. Researchers examining these oral traditions over the last century, including anthropologists and astronomers, missed the description of these stars as being <span class="hlt">variable</span> in nature as the ethnographic record contained several misidentifications of stars and celestial objects. Arguably, ethnographers working on Indigenous Knowledge Systems should have academic training in both the natural and social sciences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1244792-interannual-modulation-subtropical-atlantic-boreal-summer-dust-variability-enso','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1244792-interannual-modulation-subtropical-atlantic-boreal-summer-dust-variability-enso"><span>Interannual Modulation of Subtropical Atlantic Boreal Summer Dust <span class="hlt">Variability</span> by ENSO</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>DeFlorio, Mike; Goodwin, Ian D.; Cayan, Dan</p> <p>2016-01-01</p> <p>Dust <span class="hlt">variability</span> in the climate system has been studied for several <span class="hlt">decades</span>, yet there remains an incomplete understanding of the dynamical mechanisms controlling interannual and <span class="hlt">decadal</span> variations in dust transport. The sparseness of multi-year <span class="hlt">observational</span> datasets has limited our understanding of the relationship between climate variations and atmospheric dust. We use available <span class="hlt">observations</span> and a century-length fully coupled Community Earth System Model (CESM) simulation to show that the El Niño- Southern Oscillation (ENSO) exerts a control on North African dust transport during boreal summer. In CESM, this relationship is stronger over the dusty tropical North Atlantic than near Barbados, onemore » of the few sites having a multi-<span class="hlt">decadal</span> <span class="hlt">observed</span> record. During strong La Niña summers in CESM, a statistically significant increase in lower tropospheric easterly wind is associated with an increase in North African dust transport over the Atlantic. Barbados dust and Pacific SST <span class="hlt">variability</span> are only weakly correlated in both <span class="hlt">observations</span> and CESM, suggesting that other processes are controlling the crossbasin <span class="hlt">variability</span> of dust. We also use our CESM simulation to show that the relationship between downstream North African dust transport and ENSO fluctuates on multidecadal timescales and may be modulated by the North Atlantic Oscillation (NAO). Our findings indicate that existing <span class="hlt">observations</span> of dust over the tropical North Atlantic are not extensive enough to completely describe the <span class="hlt">variability</span> of dust and dust transport, and demonstrate the importance of global models to supplement and interpret <span class="hlt">observational</span> records.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy..tmp..379M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy..tmp..379M"><span>Statistical link between external climate forcings and modes of ocean <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malik, Abdul; Brönnimann, Stefan; Perona, Paolo</p> <p>2017-07-01</p> <p>In this study we investigate statistical link between external climate forcings and modes of ocean <span class="hlt">variability</span> on inter-annual (3-year) to centennial (100-year) timescales using de-trended semi-partial-cross-correlation analysis technique. To investigate this link we employ <span class="hlt">observations</span> (AD 1854-1999), climate proxies (AD 1600-1999), and coupled Atmosphere-Ocean-Chemistry Climate Model simulations with SOCOL-MPIOM (AD 1600-1999). We find robust statistical evidence that Atlantic multi-<span class="hlt">decadal</span> oscillation (AMO) has intrinsic positive correlation with solar activity in all datasets employed. The strength of the relationship between AMO and solar activity is modulated by volcanic eruptions and complex interaction among modes of ocean <span class="hlt">variability</span>. The <span class="hlt">observational</span> dataset reveals that El Niño southern oscillation (ENSO) has statistically significant negative intrinsic correlation with solar activity on <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> timescales (16-27-year) whereas there is no evidence of a link on a typical ENSO timescale (2-7-year). In the <span class="hlt">observational</span> dataset, the volcanic eruptions do not have a link with AMO on a typical AMO timescale (55-80-year) however the long-term datasets (proxies and SOCOL-MPIOM output) show that volcanic eruptions have intrinsic negative correlation with AMO on inter-annual to multi-<span class="hlt">decadal</span> timescales. The Pacific <span class="hlt">decadal</span> oscillation has no link with solar activity, however, it has positive intrinsic correlation with volcanic eruptions on multi-<span class="hlt">decadal</span> timescales (47-54-year) in reconstruction and <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> timescales (16-32-year) in climate model simulations. We also find evidence of a link between volcanic eruptions and ENSO, however, the sign of relationship is not consistent between <span class="hlt">observations</span>/proxies and climate model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913575P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913575P"><span>Calibration of <span class="hlt">decadal</span> ensemble predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pasternack, Alexander; Rust, Henning W.; Bhend, Jonas; Liniger, Mark; Grieger, Jens; Müller, Wolfgang; Ulbrich, Uwe</p> <p>2017-04-01</p> <p><span class="hlt">Decadal</span> climate predictions are of great socio-economic interest due to the corresponding planning horizons of several political and economic decisions. Due to uncertainties of weather and climate, forecasts (e.g. due to initial condition uncertainty), they are issued in a probabilistic way. One issue frequently <span class="hlt">observed</span> for probabilistic forecasts is that they tend to be not reliable, i.e. the forecasted probabilities are not consistent with the relative frequency of the associated <span class="hlt">observed</span> events. Thus, these kind of forecasts need to be re-calibrated. While re-calibration methods for seasonal time scales are available and frequently applied, these methods still have to be adapted for <span class="hlt">decadal</span> time scales and its characteristic problems like climate trend and lead time dependent bias. Regarding this, we propose a method to re-calibrate <span class="hlt">decadal</span> ensemble predictions that takes the above mentioned characteristics into account. Finally, this method will be applied and validated to <span class="hlt">decadal</span> forecasts from the MiKlip system (Germany's initiative for <span class="hlt">decadal</span> prediction).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H23N1077W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H23N1077W"><span>Quasi-<span class="hlt">decadal</span> Oscillation in the CMIP5 and CMIP3 Climate Model Simulations: California Case</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, J.; Yin, H.; Reyes, E.; Chung, F. I.</p> <p>2014-12-01</p> <p>The ongoing three drought years in California are reminding us of two other historical long drought periods: 1987-1992 and 1928-1934. This kind of interannual <span class="hlt">variability</span> is corresponding to the dominating 7-15 yr quasi-<span class="hlt">decadal</span> oscillation in precipitation and streamflow in California. When using global climate model projections to assess the climate change impact on water resources planning in California, it is natural to ask if global climate models are able to reproduce the <span class="hlt">observed</span> interannual <span class="hlt">variability</span> like 7-15 yr quasi-<span class="hlt">decadal</span> oscillation. Further spectral analysis to tree ring retrieved precipitation and historical precipitation record proves the existence of 7-15 yr quasi-<span class="hlt">decadal</span> oscillation in California. But while implementing spectral analysis to all the CMIP5 and CMIP3 global climate model historical simulations using wavelet analysis approach, it was found that only two models in CMIP3 , CGCM 2.3.2a of MRI and NCAP PCM1.0, and only two models in CMIP5, MIROC5 and CESM1-WACCM, have statistically significant 7-15 yr quasi-<span class="hlt">decadal</span> oscillations in California. More interesting, the existence of 7-15 yr quasi-<span class="hlt">decadal</span> oscillation in the global climate model simulation is also sensitive to initial conditions. 12-13 yr quasi-<span class="hlt">decadal</span> oscillation occurs in one ensemble run of CGCM 2.3.2a of MRI but does not exist in the other four ensemble runs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyd..560..461F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyd..560..461F"><span><span class="hlt">Decadal</span> changes of reference crop evapotranspiration attribution: Spatial and temporal <span class="hlt">variability</span> over China 1960-2011</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fan, Ze-Xin; Thomas, Axel</p> <p>2018-05-01</p> <p>Atmospheric evaporative demand can be used as a measure of the hydrological cycle and the global energy balance. Its long-term variation and the role of driving climatic factors have received increasingly attention in climate change studies. FAO-Penman-Monteith reference crop evapotranspiration rates were estimated for 644 meteorological stations over China for the period 1960-2011 to analyze spatial and temporal attribution <span class="hlt">variability</span>. Attribution of climatic <span class="hlt">variables</span> to reference crop evapotranspiration rates was not stable over the study period. While for all of China the contribution of sunshine duration remained relatively stable, the importance of relative humidity increased considerably during the last two <span class="hlt">decades</span>, particularly in winter. Spatially distributed attribution analysis shows that the position of the center of maximum contribution of sunshine duration has shifted from Southeast to Northeast China while in West China the contribution of wind speed has decreased dramatically. In contrast relative humidity has become an important factor in most parts of China. Changes in the Asian Monsoon circulation may be responsible for altered patterns of cloudiness and a general decrease of wind speeds over China. The continuously low importance of temperature confirms that global warming does not necessarily lead to rising atmospheric evaporative demand.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1112005M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1112005M"><span>Quantifying the role of ocean initial conditions in <span class="hlt">decadal</span> prediction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matei, D.; Pohlmann, H.; Müller, W.; Haak, H.; Jungclaus, J.; Marotzke, J.</p> <p>2009-04-01</p> <p>The forecast skill of <span class="hlt">decadal</span> climate predictions is investigated using two different initialization strategies. First we apply an assimilation of ocean synthesis data provided by the GECCO project (Köhl and Stammer 2008) as initial conditions for the coupled model ECHAM5/MPI-OM. The results show promising skill up to <span class="hlt">decadal</span> time scales particularly over the North Atlantic (see also Pohlmann et al. 2009). However, mismatches between the ocean climates of GECCO and the MPI-OM model may lead to inconsistencies in the representation of water masses. Therefore, we pursue an alternative approach to the representation of the <span class="hlt">observed</span> North Atlantic climate for the period 1948-2007. Using the same MPI-OM ocean model as in the coupled system, we perform an ensemble of four NCEP integrations. The ensemble mean temperature and salinity anomalies are then nudged into the coupled model, followed by hindcast/forecast experiments. The model gives dynamically consistent three-dimensional temperature and salinity fields, thereby avoiding the problems of model drift that were encountered when the assimilation experiment was only driven by reconstructed SSTs (Keenlyside et al. 2008, Pohlmann et al. 2009). Differences between the two assimilation approaches are discussed by comparing them with the <span class="hlt">observational</span> data in key regions and processes, such as North Atlantic and Tropical Pacific climate, MOC <span class="hlt">variability</span>, Subpolar Gyre <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PolSc..10..199T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PolSc..10..199T"><span>Relationship between the Arctic oscillation and surface air temperature in multi-<span class="hlt">decadal</span> time-scale</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, Hiroshi L.; Tamura, Mina</p> <p>2016-09-01</p> <p>In this study, a simple energy balance model (EBM) was integrated in time, considering a hypothetical long-term <span class="hlt">variability</span> in ice-albedo feedback mimicking the <span class="hlt">observed</span> multi-<span class="hlt">decadal</span> temperature <span class="hlt">variability</span>. A natural <span class="hlt">variability</span> was superimposed on a linear warming trend due to the increasing radiative forcing of CO2. The result demonstrates that the superposition of the natural <span class="hlt">variability</span> and the background linear trend can offset with each other to show the warming hiatus for some period. It is also stressed that the rapid warming during 1970-2000 can be explained by the superposition of the natural <span class="hlt">variability</span> and the background linear trend at least within the simple model. The key process of the fluctuating planetary albedo in multi-<span class="hlt">decadal</span> time scale is investigated using the JRA-55 reanalysis data. It is found that the planetary albedo increased for 1958-1970, decreased for 1970-2000, and increased for 2000-2012, as expected by the simple EBM experiments. The multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> in the planetary albedo is compared with the time series of the AO mode and Barents Sea mode of surface air temperature. It is shown that the recent AO negative pattern showing warm Arctic and cold mid-latitudes is in good agreement with planetary albedo change indicating negative anomaly in high latitudes and positive anomaly in mid-latitudes. Moreover, the Barents Sea mode with the warm Barents Sea and cold mid-latitudes shows long-term <span class="hlt">variability</span> similar to planetary albedo change. Although further studies are needed, the natural <span class="hlt">variabilities</span> of both the AO mode and Barents Sea mode indicate some possible link to the planetary albedo as suggested by the simple EBM to cause the warming hiatus in recent years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27651068','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27651068"><span><span class="hlt">Variability</span> in functional brain networks predicts expertise during action <span class="hlt">observation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Amoruso, Lucía; Ibáñez, Agustín; Fonseca, Bruno; Gadea, Sebastián; Sedeño, Lucas; Sigman, Mariano; García, Adolfo M; Fraiman, Ricardo; Fraiman, Daniel</p> <p>2017-02-01</p> <p><span class="hlt">Observing</span> an action performed by another individual activates, in the <span class="hlt">observer</span>, similar circuits as those involved in the actual execution of that action. This activation is modulated by prior experience; indeed, sustained training in a particular motor domain leads to structural and functional changes in critical brain areas. Here, we capitalized on a novel graph-theory approach to electroencephalographic data (Fraiman et al., 2016) to test whether <span class="hlt">variability</span> in functional brain networks implicated in Tango <span class="hlt">observation</span> can discriminate between groups differing in their level of expertise. We found that experts and beginners significantly differed in the functional organization of task-relevant networks. Specifically, networks in expert Tango dancers exhibited less <span class="hlt">variability</span> and a more robust functional architecture. Notably, these expertise-dependent effects were captured within networks derived from electrophysiological brain activity recorded in a very short time window (2s). In brief, <span class="hlt">variability</span> in the organization of task-related networks seems to be a highly sensitive indicator of long-lasting training effects. This finding opens new methodological and theoretical windows to explore the impact of domain-specific expertise on brain plasticity, while highlighting <span class="hlt">variability</span> as a fruitful measure in neuroimaging research. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS43C..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS43C..03S"><span>The impact of multi-<span class="hlt">decadal</span> sub-surface circulation changes on sea surface chlorophyll patterns in the tropical Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schollaert Uz, S.; Busalacchi, A. J.; Smith, T. M.; Evans, M. N.; Brown, C.; Hackert, E. C.; Wang, X.</p> <p>2016-12-01</p> <p>The tropical Pacific is a region of strong forcing where physical oceanography primarily controls biological <span class="hlt">variability</span> over the seasonal to interannual time scales <span class="hlt">observed</span> since dedicated ocean color satellite remote sensing began in 1997. To quantify how multi-<span class="hlt">decadal</span>, climate-scale changes impact marine biological dynamics, we used the correlation with sea-surface temperature and height to reconstruct a 50-year time series of surface chlorophyll concentrations. The reconstruction demonstrates greatest skill away from the coast and within 10o of the equator where chlorophyll variance is greatest and primarily associated with El Niño Southern Oscillation (ENSO) dynamics and secondarily associated with <span class="hlt">decadal</span> <span class="hlt">variability</span>. We <span class="hlt">observe</span> significant basin-wide differences between east and central Pacific events when the El Niño events are strong: chlorophyll increases with La Niña and decreases with El Niño, with larger declines east of 180o for remotely-forced east Pacific events and west of 180o for locally-forced central Pacific events. Chlorophyll variations also reflect the physical dynamics of Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> with small but significant differences between cool and warm eras: consistent with advection <span class="hlt">variability</span> west of 180o and likely driven by subsurface changes in the nutricline depth between 110-140oW. Comparisons with output from a fully-coupled biogeochemical model support the hypothesis that this anomalous region is controlled by lower frequency changes in subsurface circulation patterns that transport nutrients to the surface. Basin-wide chlorophyll distributions exhibiting spatial heterogeneity in response to multi-<span class="hlt">decadal</span> climate forcing imply similar long-term changes in phytoplankton productivity, with implications for the marine food web and the ocean's role as a carbon sink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26160379','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26160379"><span>GLOBAL WARMING. Recent hiatus caused by <span class="hlt">decadal</span> shift in Indo-Pacific heating.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nieves, Veronica; Willis, Josh K; Patzert, William C</p> <p>2015-07-31</p> <p>Recent modeling studies have proposed different scenarios to explain the slowdown in surface temperature warming in the most recent <span class="hlt">decade</span>. Some of these studies seem to support the idea of internal <span class="hlt">variability</span> and/or rearrangement of heat between the surface and the ocean interior. Others suggest that radiative forcing might also play a role. Our examination of <span class="hlt">observational</span> data over the past two <span class="hlt">decades</span> shows some significant differences when compared to model results from reanalyses and provides the most definitive explanation of how the heat was redistributed. We find that cooling in the top 100-meter layer of the Pacific Ocean was mainly compensated for by warming in the 100- to 300-meter layer of the Indian and Pacific Oceans in the past <span class="hlt">decade</span> since 2003. Copyright © 2015, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50..801V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50..801V"><span>Historical analysis of interannual rainfall <span class="hlt">variability</span> and trends in southeastern Brazil based on <span class="hlt">observational</span> and remotely sensed data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vásquez P., Isela L.; de Araujo, Lígia Maria Nascimento; Molion, Luiz Carlos Baldicero; de Araujo Abdalad, Mariana; Moreira, Daniel Medeiros; Sanchez, Arturo; Barbosa, Humberto Alves; Rotunno Filho, Otto Corrêa</p> <p>2018-02-01</p> <p>The Brazilian Southeast is considered a humid region. It is also prone to landslides and floods, a result of significant increases in rainfall during spring and summer caused by the South Atlantic Convergence Zone (SACZ). Recently, however, the region has faced a striking rainfall shortage, raising serious concerns regarding water availability. The present work endeavored to explain the meteorological drought that has led to hydrological imbalance and water scarcity in the region. Hodrick-Prescott smoothing and wavelet transform techniques were applied to long-term hydrologic and sea surface temperature (SST)—based climate indices monthly time series data in an attempt to detect cycles and trends that could help explain rainfall patterns and define a framework for improving the predictability of extreme events in the region. Historical <span class="hlt">observational</span> hydrologic datasets available include monthly precipitation amounts gauged since 1888 and 1940 and stream flow measured since the 1930s. The spatial representativeness of rain gauges was tested against gridded rainfall satellite estimates from 2000 to 2015. The analyses revealed <span class="hlt">variability</span> in four time scale domains—infra-annual, interannual, quasi-<span class="hlt">decadal</span> and inter-<span class="hlt">decadal</span> or multi-<span class="hlt">decadal</span>. The strongest oscillations periods revealed were: for precipitation—8 months, 2, 8 and 32 years; for Pacific SST in the Niño-3.4 region—6 months, 2, 8 and 35.6 years, for North Atlantic SST variability—6 months, 2, 8 and 32 years and for Pacific <span class="hlt">Decadal</span> Oscillation (PDO) index—6.19 months, 2.04, 8.35 and 27.31 years. Other periodicities less prominent but still statistically significant were also highlighted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050180360&hterms=gravity+earth&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dgravity%2Bearth','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050180360&hterms=gravity+earth&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dgravity%2Bearth"><span>Excitation of Earth Rotation Variations "<span class="hlt">Observed</span>" by Time-<span class="hlt">Variable</span> Gravity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chao, Ben F.; Cox, C. M.</p> <p>2005-01-01</p> <p>Time <span class="hlt">variable</span> gravity measurements have been made over the past two <span class="hlt">decades</span> using the space geodetic technique of satellite laser ranging, and more recently by the GRACE satellite mission with improved spatial resolutions. The degree-2 harmonic components of the time-<span class="hlt">variable</span> gravity contain important information about the Earth s length-of-day and polar motion excitation functions, in a way independent to the traditional "direct" Earth rotation measurements made by, for example, the very-long-baseline interferometry and GPS. In particular, the (degree=2, order= 1) components give the mass term of the polar motion excitation; the (2,O) component, under certain mass conservation conditions, gives the mass term of the length-of-day excitation. Combining these with yet another independent source of angular momentum estimation calculated from global geophysical fluid models (for example the atmospheric angular momentum, in both mass and motion terms), in principle can lead to new insights into the dynamics, particularly the role or the lack thereof of the cores, in the excitation processes of the Earth rotation variations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoJI.207..228W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoJI.207..228W"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> in core surface flows deduced from geomagnetic observatory monthly means</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Whaler, K. A.; Olsen, N.; Finlay, C. C.</p> <p>2016-10-01</p> <p>Monthly means of the magnetic field measurements at ground observatories are a key data source for studying temporal changes of the core magnetic field. However, when they are calculated in the usual way, contributions of external (magnetospheric and ionospheric) origin may remain, which make them less favourable for studying the field generated by dynamo action in the core. We remove external field predictions, including a new way of characterizing the magnetospheric ring current, from the data and then calculate revised monthly means using robust methods. The geomagnetic secular variation (SV) is calculated as the first annual differences of these monthly means, which also removes the static crustal field. SV time-series based on revised monthly means are much less scattered than those calculated from ordinary monthly means, and their variances and correlations between components are smaller. On the annual to <span class="hlt">decadal</span> timescale, the SV is generated primarily by advection in the fluid outer core. We demonstrate the utility of the revised monthly means by calculating models of the core surface advective flow between 1997 and 2013 directly from the SV data. One set of models assumes flow that is constant over three months; such models exhibit large and rapid temporal variations. For models of this type, less complex flows achieve the same fit to the SV derived from revised monthly means than those from ordinary monthly means. However, those obtained from ordinary monthly means are able to follow excursions in SV that are likely to be external field contamination rather than core signals. Having established that we can find models that fit the data adequately, we then assess how much temporal <span class="hlt">variability</span> is required. Previous studies have suggested that the flow is consistent with torsional oscillations (TO), solid body-like oscillations of fluid on concentric cylinders with axes aligned along the Earth's rotation axis. TO have been proposed to explain <span class="hlt">decadal</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AdAtS..35..495L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AdAtS..35..495L"><span>ENSO Frequency Asymmetry and the Pacific <span class="hlt">Decadal</span> Oscillation in <span class="hlt">Observations</span> and 19 CMIP5 Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, Renping; Zheng, Fei; Dong, Xiao</p> <p>2018-05-01</p> <p>Using <span class="hlt">observational</span> data and the pre-industrial simulations of 19 models from the Coupled Model Intercomparison Project Phase 5 (CMIP5), the El Niño (EN) and La Niña (LN) events in positive and negative Pacific <span class="hlt">Decadal</span> Oscillation (PDO) phases are examined. In the <span class="hlt">observational</span> data, with EN (LN) events the positive (negative) SST anomaly in the equatorial eastern Pacific is much stronger in positive (negative) PDO phases than in negative (positive) phases. Meanwhile, the models cannot reasonably reproduce this difference. Besides, the modulation of ENSO frequency asymmetry by the PDO is explored. Results show that, in the <span class="hlt">observational</span> data, EN is 300% more (58% less) frequent than LN in positive (negative) PDO phases, which is significant at the 99% confidence level using the Monte Carlo test. Most of the CMIP5 models exhibit results that are consistent with the <span class="hlt">observational</span> data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613459P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613459P"><span>Influence of synoptic weather patterns on solar irradiance <span class="hlt">variability</span> in Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parding, Kajsa; Hinkelman, Laura; Liepert, Beate; Ackerman, Thomas; Dagestad, Knut-Frode; Asle Olseth, Jan</p> <p>2014-05-01</p> <p>Solar radiation is important for many aspects of existence on Earth, including the biosphere, the hydrological cycle, and creatures living on the planet. Previous studies have reported <span class="hlt">decadal</span> trends in <span class="hlt">observational</span> records of surface shortwave (SW) irradiance around the world, too strong to be caused by varying solar output. These <span class="hlt">observed</span> <span class="hlt">decadal</span> trends have been dubbed "solar dimming and brightening" and are believed to be related to changes in atmospheric aerosols and cloud cover. Because the <span class="hlt">observed</span> solar <span class="hlt">variability</span> coincides with qualitative air pollution histories, the dimming and brightening have become almost synonymous with shortwave attenuation by anthropogenic aerosols. However, there are indications that atmospheric circulation patterns have influenced the dimming and brightening in some regions, e.g., Alaska and Scandinavia. In this work, we focus on the role of atmospheric circulation patterns in modifying shortwave irradiance. An examination of European SW irradiance data from the Global Energy Balance Archive (GEBA) shows that while there are periods of predominantly decreasing (~1970-1985) and increasing (~1985-2007) SW irradiance, the changes are not spatially uniform within Europe and in a majority of locations not statistically significant. To establish a connection between weather patterns and sunshine, regression models of SW irradiance are fitted using a daily classification of European weather called Grosswetterlagen (GWL). The GWL reconstructions of shortwave irradiance represent the part of the solar <span class="hlt">variability</span> that is related to large scale weather patterns, which should be effectively separated from the influence of varying anthropogenic aerosol emissions. The correlation (R) between <span class="hlt">observed</span> and reconstruced SW irradiance is between 0.31 and 0.75, depending on station and season, all statistically significant (p<0.05, estimated with a bootstrap test). In central and eastern parts of Europe, the <span class="hlt">observed</span> <span class="hlt">decadal</span> SW <span class="hlt">variability</span> is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JHyd..543..818X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JHyd..543..818X"><span>Landsat and GRACE <span class="hlt">observations</span> of arid wetland dynamics in a dryland river system under multi-<span class="hlt">decadal</span> hydroclimatic extremes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xie, Zunyi; Huete, Alfredo; Ma, Xuanlong; Restrepo-Coupe, Natalia; Devadas, Rakhesh; Clarke, Kenneth; Lewis, Megan</p> <p>2016-12-01</p> <p>Arid wetlands are important for biodiversity conservation, but sensitive and vulnerable to climate <span class="hlt">variability</span> and hydroclimatic events. Amplification of the water cycle, including the increasing frequency and severity of droughts and wet extremes, is expected to alter spatial and temporal hydrological patterns in arid wetlands globally, with potential threats to ecosystem services and their functioning. Despite these pressing challenges, the ecohydrological interactions and resilience of arid wetlands to highly <span class="hlt">variable</span> water regimes over long time periods remain largely unknown. Recent broad-scale drought and floods over Australia provide unique opportunities to improve our understanding of arid wetland ecosystem responses to hydroclimatic extremes. Here we analysed the ecohydrological dynamics of the Coongie Lakes arid wetland in central Australia, one of the world's largest Ramsar-designated wetlands, using more than two <span class="hlt">decades</span> (1988-2011) of vegetation and floodwater extent retrievals derived from Landsat satellite <span class="hlt">observations</span>. To explore the impacts of large-scale hydrological fluctuations on the arid wetland, we further coupled Landsat measurements with Total Water Storage Anomaly (TWSA) data obtained from the Gravity Recovery and Climate Experiment (GRACE) satellites. Pronounced seasonal and inter-annual <span class="hlt">variabilities</span> of flood and vegetation activities were <span class="hlt">observed</span> over the wetland, with variations in vegetation growth extent highly correlated with flood extent (r = 0.64, p < 0.05) that ranged from nearly zero to 3456 km2. We reported the hydrological dynamics and associated ecosystem responses to be largely driven by the two phases (El Niño and La Niña) of the El Nino-Southern Oscillation (ENSO) ocean-atmosphere system. Changes in flood and vegetation extent were better explained by GRACE-TWSA (r = 0.8, lag = 0 month) than rainfall (r = 0.34, lag = 3 months) over the water source area, demonstrating that TWS is a valuable hydrological indicator for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG51B..03R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG51B..03R"><span>Characterizing Transitions Between <span class="hlt">Decadal</span> States of the Tropical Pacific using State Space Reconstruction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ramesh, N.; Cane, M. A.</p> <p>2017-12-01</p> <p>The complex coupled ocean-atmosphere system of the Tropical Pacific generates <span class="hlt">variability</span> on timescales from intraseasonal to multidecadal. Pacific <span class="hlt">Decadal</span> <span class="hlt">Variability</span> (PDV) is among the key drivers of global climate, with effects on hydroclimate on several continents, marine ecosystems, and the rate of global mean surface temperature rise under anthropogenic greenhouse gas forcing. Predicting phase shifts in the PDV would therefore be highly useful. However, the small number of PDV phase shifts that have occurred in the <span class="hlt">observational</span> record pose a substantial challenge to developing an understanding of the mechanisms that underlie <span class="hlt">decadal</span> <span class="hlt">variability</span>. In this study, we use a 100,000-year unforced simulation from an intermediate-complexity model of the Tropical Pacific region that has been shown to produce PDV comparable to that in the real world. We apply the Simplex Projection method to the NINO3 index from this model to reconstruct a shadow manifold that preserves the topology of the true attractor of this system. We find that the high- and low-variance phases of PDV emerge as a pair of regimes in a 3-dimensional state space, and that the transitions between <span class="hlt">decadal</span> states lie in a highly predictable region of the attractor. We then use a random forest algorithm to develop a physical interpretation of the processes associated with these highly-predictable transitions. We find that transitions to low-variance states are most likely to occur approximately 2.5 years after an El Nino event, and that ocean-atmosphere <span class="hlt">variables</span> in the southeastern Tropical Pacific play a crucial role in driving these transitions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AJ....155...16C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AJ....155...16C"><span>Uncertain Classification of <span class="hlt">Variable</span> Stars: Handling <span class="hlt">Observational</span> GAPS and Noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Castro, Nicolás; Protopapas, Pavlos; Pichara, Karim</p> <p>2018-01-01</p> <p>Automatic classification methods applied to sky surveys have revolutionized the astronomical target selection process. Most surveys generate a vast amount of time series, or “lightcurves,” that represent the brightness <span class="hlt">variability</span> of stellar objects in time. Unfortunately, lightcurves’ <span class="hlt">observations</span> take several years to be completed, producing truncated time series that generally remain without the application of automatic classifiers until they are finished. This happens because state-of-the-art methods rely on a variety of statistical descriptors or features that present an increasing degree of dispersion when the number of <span class="hlt">observations</span> decreases, which reduces their precision. In this paper, we propose a novel method that increases the performance of automatic classifiers of <span class="hlt">variable</span> stars by incorporating the deviations that scarcity of <span class="hlt">observations</span> produces. Our method uses Gaussian process regression to form a probabilistic model of each lightcurve’s <span class="hlt">observations</span>. Then, based on this model, bootstrapped samples of the time series features are generated. Finally, a bagging approach is used to improve the overall performance of the classification. We perform tests on the MAssive Compact Halo Object (MACHO) and Optical Gravitational Lensing Experiment (OGLE) catalogs, results show that our method effectively classifies some <span class="hlt">variability</span> classes using a small fraction of the original <span class="hlt">observations</span>. For example, we found that RR Lyrae stars can be classified with ~80% accuracy just by <span class="hlt">observing</span> the first 5% of the whole lightcurves’ <span class="hlt">observations</span> in the MACHO and OGLE catalogs. We believe these results prove that, when studying lightcurves, it is important to consider the features’ error and how the measurement process impacts it.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.7181P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.7181P"><span>Mechanisms underlying recent <span class="hlt">decadal</span> changes in subpolar North Atlantic Ocean heat content</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Piecuch, Christopher G.; Ponte, Rui M.; Little, Christopher M.; Buckley, Martha W.; Fukumori, Ichiro</p> <p>2017-09-01</p> <p>The subpolar North Atlantic (SPNA) is subject to strong <span class="hlt">decadal</span> <span class="hlt">variability</span>, with implications for surface climate and its predictability. In 2004-2005, SPNA <span class="hlt">decadal</span> upper ocean and sea-surface temperature trends reversed from warming during 1994-2004 to cooling over 2005-2015. This recent <span class="hlt">decadal</span> trend reversal in SPNA ocean heat content (OHC) is studied using a physically consistent, <span class="hlt">observationally</span> constrained global ocean state estimate covering 1992-2015. The estimate's physical consistency facilitates quantitative causal attribution of ocean variations. Closed heat budget diagnostics reveal that the SPNA OHC trend reversal is the result of heat advection by midlatitude ocean circulation. Kinematic decompositions reveal that changes in the deep and intermediate vertical overturning circulation cannot account for the trend reversal, but rather ocean heat transports by horizontal gyre circulations render the primary contributions. The shift in horizontal gyre advection reflects anomalous circulation acting on the mean temperature gradients. Maximum covariance analysis (MCA) reveals strong covariation between the anomalous horizontal gyre circulation and variations in the local wind stress curl, suggestive of a Sverdrup response. Results have implications for <span class="hlt">decadal</span> predictability.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912345I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912345I"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> of drought conditions over the southern part of Europe based on Principal Oscillation Pattern Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ionita-Scholz, Monica; Tallaksen, Lena M.; Scholz, Patrick</p> <p>2017-04-01</p> <p>This study introduces a novel method of estimating the decay time, mean period and forcing statistics of drought conditions over large spatial domains, demonstrated here for southern part of Europe (10°E - 40°E, 35°N - 50°N). It uses a two-dimensional stochastically forced damped linear oscillator model with the model parameters estimated from a Principal Oscillation Pattern (POP) analysis and associated <span class="hlt">observed</span> power spectra. POP is a diagnostic technique that aims to derive the space-time characteristics of a data set objectively. This analysis is performed on an extended <span class="hlt">observational</span> time series of 114 years (1902 - 2015) of the Standardized Precipitation Evapotranspiration Index for an accumulation period of 12 months (SPEI12), based on the Climate Research Unit (CRU TS v. 3.24) data set. The POP analysis reveals four exceptionally stable modes of <span class="hlt">variability</span>, which together explain more than 62% of the total explained variance. The most stable POP mode, which explains 16.3% of the total explained variance, is characterized by a period of oscillation of 14 years and a decay time of 31 years. The real part of POP1 is characterized by a monopole-like structure with the highest loadings over Portugal, western part of Spain and Turkey. The second stable mode, which explains 15.9% of the total explained variance, is characterized by a period of oscillation of 20 years and a decay time of 26.4 years. The spatial structure of the real part of POP2 has a dipole-like structure with the highest positive loadings over France, southern Germany and Romania and negative loadings over southern part of Spain. The third POP mode, in terms of stability, explains 14.0% of the total variance and is characterized by a period of oscillation of 33 years and a decay time of 43.5 years. The real part of POP3 is characterized by negative loadings over the eastern part of Europe and positive loadings over Turkey. The fourth stable POP mode, explaining 15.5% of the total variance</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002iaf..confE.275B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002iaf..confE.275B"><span><span class="hlt">Observations</span> on Complexity and Costs for Over Three <span class="hlt">Decades</span> of Communications Satellites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bearden, David A.</p> <p>2002-01-01</p> <p>This paper takes an objective look at approximately thirty communications satellites built over three <span class="hlt">decades</span> using a complexity index as an economic model. The complexity index is derived from a number of technical parameters including dry mass, end-of-life- power, payload type, communication bands, spacecraft lifetime, and attitude control approach. Complexity is then plotted versus total satellite cost and development time (defined as contract start to first launch). A comparison of the relative cost and development time for various classes of communications satellites and conclusions regarding dependence on system complexity are presented. <span class="hlt">Observations</span> regarding inherent differences between commercially acquired systems and those procured by government organizations are also presented. A process is described where a new communications system in the formative stage may be compared against similarly "complex" missions of the recent past to balance risk within allotted time and funds. 1</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990064613&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990064613&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DParkinsons"><span><span class="hlt">Variability</span> of Arctic Sea Ice as Determined from Satellite <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.</p> <p>1999-01-01</p> <p>The compiled, quality-controlled satellite multichannel passive-microwave record of polar sea ice now spans over 18 years, from November 1978 through December 1996, and is revealing considerable information about the Arctic sea ice cover and its <span class="hlt">variability</span>. The information includes data on ice concentrations (percent areal coverages of ice), ice extents, ice melt, ice velocities, the seasonal cycle of the ice, the interannual <span class="hlt">variability</span> of the ice, the frequency of ice coverage, and the length of the sea ice season. The data reveal marked regional and interannual <span class="hlt">variabilities</span>, as well as some statistically significant trends. For the north polar ice cover as a whole, maximum ice extents varied over a range of 14,700,000 - 15,900,000 sq km, while individual regions experienced much greater percent variations, for instance, with the Greenland Sea having a range of 740,000 - 1,110,000 sq km in its yearly maximum ice coverage. In spite of the large variations from year to year and region to region, overall the Arctic ice extents showed a statistically significant, 2.80% / <span class="hlt">decade</span> negative trend over the 18.2-year period. Ice season lengths, which vary from only a few weeks near the ice margins to the full year in the large region of perennial ice coverage, also experienced interannual <span class="hlt">variability</span>, along with spatially coherent overall trends. Linear least squares trends show the sea ice season to have lengthened in much of the Bering Sea, Baffin Bay, the Davis Strait, and the Labrador Sea, but to have shortened over a much larger area, including the Sea of Okhotsk, the Greenland Sea, the Barents Sea, and the southeastern Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.G21B0799B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.G21B0799B"><span>A <span class="hlt">Decade</span> of Shear-Wave Splitting <span class="hlt">Observations</span> in Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bellesiles, A. K.; Christensen, D. H.; Abers, G. A.; Hansen, R. A.; Pavlis, G. L.; Song, X.</p> <p>2010-12-01</p> <p>Over the last <span class="hlt">decade</span> four PASSCAL experiments have been conducted in different regions of Alaska. ARCTIC, BEAAR and MOOS form a north-south transect across the state, from the Arctic Ocean to Price Williams Sound, while the STEEP experiment is currently deployed to the east of that line in the St Elias Mountains of Southeastern Alaska. Shear-wave splitting <span class="hlt">observations</span> from these networks in addition to several permanent stations of the Alaska Earthquake Information Center were determined in an attempt to understand mantle flow under Alaska in a variety of different geologic settings. Results show two dominant splitting patterns in Alaska, separated by the subducted Pacific Plate. North of the subducted Pacific Plate fast directions are parallel to the trench (along strike of the subducted Pacific Plate) indicating large scale mantle flow in the northeast-southwest direction with higher anisotropy (splitting times) within the mantle wedge. Within or below the Pacific Plate fast directions are normal to the trench in the direction of Pacific Plate convergence. In addition to these two prominent splitting patterns there are several regions that do not match either of these trends. These more complex regions which include the results from STEEP could be due to several factors including effects from the edge of the Pacific Plate. The increase of station coverage that Earthscope will bring to Alaska will aid in developing a more complete model for anisotropy and mantle flow in Alaska.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1211601','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1211601"><span>Amplitude <span class="hlt">Variability</span> in gamma Dor and delta Sct Stars <span class="hlt">Observed</span> by Kepler</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Guzik, Joyce Ann; Kosak, Mary Katherine; Bradley, Paul Andrew</p> <p>2015-08-17</p> <p>The NASA Kepler spacecraft data revealed a large number of new multimode nonradially pulsating gamma Dor and delta Sct <span class="hlt">variable</span> stars. The Kepler high-precision long time-series photometry makes it possible to study amplitude variations of the frequencies, and recent literature on amplitude and frequency variations in nonradially pulsating <span class="hlt">variables</span> is summarized. Several methods are applied to study amplitude <span class="hlt">variability</span> in about a dozen gamma Doradus or delta Scuti candidate <span class="hlt">variable</span> stars <span class="hlt">observed</span> for several quarters as part of the Kepler Guest <span class="hlt">Observer</span> program. The magnitude and timescale of the amplitude variations are discussed, along with the presence or absence ofmore » correlations between amplitude variations for different frequencies of a given star. Proposed causes of amplitude spectrum <span class="hlt">variability</span> that will require further investigation are also discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A21A..05O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A21A..05O"><span>Wind Stress <span class="hlt">Variability</span> <span class="hlt">Observed</span> Over Coastal Waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz-Suslow, D. G.; Haus, B. K.; Laxague, N.; Williams, N. J.; Graber, H. C.</p> <p>2016-02-01</p> <p>The wind stress on the ocean surface generates waves, drives currents, and enhances gas exchange; and a significant amount of work has been done to characterize the air-sea momentum flux in terms of bulk oceanographic and atmospheric parameters. However, the majority of this work to develop operational algorithms has been focused on the deep ocean and the suitability of these methods in the coastal regime has not been evaluated. The findings from a two-part field campaign will be presented which highlight the divergence of nearshore wind stress <span class="hlt">observations</span> from conventional, deep water results. The first set of data comes from a coastal region near a relatively small, natural tidal inlet. A high degree of spatial <span class="hlt">variability</span> was <span class="hlt">observed</span> in both the wind stress magnitude and direction, suggestive of coastal processes (e.g., depth-limited wave affects and horizontal current shear) modulating the momentum flux from the atmosphere to the ocean surface. These shallow-water processes are typically not accounted for in conventional parameterizations. Across the experimental domain and for a given wind speed, the stress magnitude was found to be nearly 2.5 times that predicted by conventional methods; also, a high propensity for stress steering off the mean azimuthal wind direction (up to ±70 degrees) was <span class="hlt">observed</span> and linked to horizontal current gradients produced by the tidal inlet. The preliminary findings from a second data set taken in the vicinity of the macrotidal Columbia River Mouth will also be presented. Compared to the first data set, a similar degree of <span class="hlt">variability</span> is <span class="hlt">observed</span> here, but the processes responsible for this are present at a much larger scale. Specifically, the Columbia River Mouth <span class="hlt">observations</span> were made in the presence of significant swell wave energy and during periods of very high estuarine discharge. The relative angle between the wind and swell direction is expected to be significant with regards to the <span class="hlt">observed</span> momentum flux. Also, these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP41D..08H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP41D..08H"><span>Tropical Pacific forcing on <span class="hlt">decadal</span>-to-centennial NAO-dominated precipitation <span class="hlt">variability</span> in northern Mediterranean over the past 6500 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, H. M.; Shen, C. C.; Michel, V.; Jiang, X.; Mii, H. S.; Wang, Y.; Valensi, P.</p> <p>2017-12-01</p> <p>We present a multi-annual-resolved absolute-dated stalagmite-inferred precipitation record, with age precision as good as ±2 years, from northern Italy, to reflect North Atlantic Oscillation (NAO) dynamics since 6.5 ka (thousand years ago, before 1950 C.E.). Our record features millennial precipitation fluctuations punctuated by several centennial-scale drought periods centered at 5.6, 6.2, 4.2, 3.0 and 2.3 ka. The phase relationship with previous NAO-sensitive records suggests a multi-millennial southward migration of the northern Westerlies and enhanced NAO <span class="hlt">variability</span> from the middle- to late-Holocene. We also found the multi-<span class="hlt">decadal</span> to centennial rainfall amount could dramatically vary within few <span class="hlt">decades</span>, possibly affecting ancient Mediterranean civilizations. Concurrence between northern Mediterranean precipitation and western tropical Pacific sea surface temperature records suggests the remote forcing on this NAO-dominated rainfall. We argue that the irregular NAO change nowadays could be related to high frequency of El Niño-Southern Oscillation events and might cause an inevitable abrupt hydroclimate change and irreparable impacts on the regional human society in the near future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4319Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4319Y"><span>Underestimated AMOC <span class="hlt">Variability</span> and Implications for AMV and Predictability in CMIP Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Xiaoqin; Zhang, Rong; Knutson, Thomas R.</p> <p>2018-05-01</p> <p>The Atlantic Meridional Overturning Circulation (AMOC) has profound impacts on various climate phenomena. Using both <span class="hlt">observations</span> and simulations from the Coupled Model Intercomparison Project Phase 3 and 5, here we show that most models underestimate the amplitude of low-frequency AMOC <span class="hlt">variability</span>. We further show that stronger low-frequency AMOC <span class="hlt">variability</span> leads to stronger linkages between the AMOC and key <span class="hlt">variables</span> associated with the Atlantic multidecadal <span class="hlt">variability</span> (AMV), and between the subpolar AMV signal and northern hemisphere surface air temperature. Low-frequency extratropical northern hemisphere surface air temperature <span class="hlt">variability</span> might increase with the amplitude of low-frequency AMOC <span class="hlt">variability</span>. Atlantic <span class="hlt">decadal</span> predictability is much higher in models with stronger low-frequency AMOC <span class="hlt">variability</span> and much lower in models with weaker or without AMOC <span class="hlt">variability</span>. Our results suggest that simulating realistic low-frequency AMOC <span class="hlt">variability</span> is very important, both for simulating realistic linkages between AMOC and AMV-related <span class="hlt">variables</span> and for achieving substantially higher Atlantic <span class="hlt">decadal</span> predictability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.7919Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.7919Z"><span>A <span class="hlt">decadal</span> tropical Pacific condition unfavorable to central Pacific El Niño</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhong, Wenxiu; Zheng, Xiao-Tong; Cai, Wenju</p> <p>2017-08-01</p> <p>The frequency of central Pacific (CP) El Niño events displays strong <span class="hlt">decadal</span> <span class="hlt">variability</span> but the associated dynamics are unclear. The Interdecadal Pacific Oscillation (IPO) and the tropical Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> (TPDV) are two dominant modes of tropical Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> that can interact with high-frequency activities. Using a 500 year control integration from the Geophysical Fluid Dynamics Laboratory Earth System Model, we find that the difference in mean state between the low-frequency and high-frequency CP El Niño periods is similar to the <span class="hlt">decadal</span> background condition concurrently contributed by a negative IPO and a positive TPDV. This <span class="hlt">decadal</span> state features strengthened trade winds west of the International Date Line and anomalous cool sea surface temperatures across the central tropical Pacific. As such, positive zonal advection feedback is difficult to be generated over the central to western tropical Pacific during the CP El Niño developing season, resulting in the low CP El Niño frequency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B53C0476C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B53C0476C"><span>Constraining land carbon cycle process understanding with <span class="hlt">observations</span> of atmospheric CO2 <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Collatz, G. J.; Kawa, S. R.; Liu, Y.; Zeng, F.; Ivanoff, A.</p> <p>2013-12-01</p> <p>We evaluate our understanding of the land biospheric carbon cycle by benchmarking a model and its variants to atmospheric CO2 <span class="hlt">observations</span> and to an atmospheric CO2 inversion. Though the seasonal cycle in CO2 <span class="hlt">observations</span> is well simulated by the model (RMSE/standard deviation of <span class="hlt">observations</span> <0.5 at most sites north of 15N and <1 for Southern Hemisphere sites) different model setups suggest that the CO2 seasonal cycle provides some constraint on gross photosynthesis, respiration, and fire fluxes revealed in the amplitude and phase at northern latitude sites. CarbonTracker inversions (CT) and model show similar phasing of the seasonal fluxes but agreement in the amplitude varies by region. We also evaluate interannual <span class="hlt">variability</span> (IAV) in the measured atmospheric CO2 which, in contrast to the seasonal cycle, is not well represented by the model. We estimate the contributions of biospheric and fire fluxes, and atmospheric transport <span class="hlt">variability</span> to explaining <span class="hlt">observed</span> <span class="hlt">variability</span> in measured CO2. Comparisons with CT show that modeled IAV has some correspondence to the inversion results >40N though fluxes match poorly at regional to continental scales. Regional and global fire emissions are strongly correlated with <span class="hlt">variability</span> <span class="hlt">observed</span> at northern flask sample sites and in the global atmospheric CO2 growth rate though in the latter case fire emissions anomalies are not large enough to account fully for the <span class="hlt">observed</span> <span class="hlt">variability</span>. We discuss remaining unexplained <span class="hlt">variability</span> in CO2 <span class="hlt">observations</span> in terms of the representation of fluxes by the model. This work also demonstrates the limitations of the current network of CO2 <span class="hlt">observations</span> and the potential of new denser surface measurements and space based column measurements for constraining carbon cycle processes in models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACP....1510385K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACP....1510385K"><span><span class="hlt">Variability</span> in Antarctic ozone loss in the last <span class="hlt">decade</span> (2004-2013): high-resolution simulations compared to Aura MLS <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuttippurath, J.; Godin-Beekmann, S.; Lefèvre, F.; Santee, M. L.; Froidevaux, L.; Hauchecorne, A.</p> <p>2015-09-01</p> <p>A detailed analysis of the polar ozone loss processes during 10 recent Antarctic winters is presented with high-resolution MIMOSA-CHIM (Modèle Isentrope du transport Méso-échelle de l'Ozone Stratosphérique par Advection avec CHIMie) model simulations and high-frequency polar vortex <span class="hlt">observations</span> from the Aura microwave limb sounder (MLS) instrument. The high-frequency measurements and simulations help to characterize the winters and assist the interpretation of interannual <span class="hlt">variability</span> better than either data or simulations alone. Our model results for the Antarctic winters of 2004-2013 show that chemical ozone loss starts in the edge region of the vortex at equivalent latitudes (EqLs) of 65-67° S in mid-June-July. The loss progresses with time at higher EqLs and intensifies during August-September over the range 400-600 K. The loss peaks in late September-early October, when all EqLs (65-83° S) show a similar loss and the maximum loss (> 2 ppmv - parts per million by volume) is found over a broad vertical range of 475-550 K. In the lower stratosphere, most winters show similar ozone loss and production rates. In general, at 500 K, the loss rates are about 2-3 ppbv sh-1 (parts per billion by volume per sunlit hour) in July and 4-5 ppbv sh-1 in August-mid-September, while they drop rapidly to 0 by mid-October. In the middle stratosphere, the loss rates are about 3-5 ppbv sh-1 in July-August and October at 675 K. On average, the MIMOSA-CHIM simulations show that the very cold winters of 2005 and 2006 exhibit a maximum loss of ~ 3.5 ppmv around 550 K or about 149-173 DU over 350-850 K, and the warmer winters of 2004, 2010, and 2012 show a loss of ~ 2.6 ppmv around 475-500 K or 131-154 DU over 350-850 K. The winters of 2007, 2008, and 2011 were moderately cold, and thus both ozone loss and peak loss altitudes are between these two ranges (3 ppmv around 500 K or 150 ± 10 DU). The modeled ozone loss values are in reasonably good agreement with those estimated from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011avsa.book.....W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011avsa.book.....W"><span>Advancing <span class="hlt">Variable</span> Star Astronomy: The Centennial History of the American Association of <span class="hlt">Variable</span> Star <span class="hlt">Observers</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, Thomas R.; Saladyga, Michael</p> <p>2011-05-01</p> <p>Preface; Part I. Pioneers in <span class="hlt">Variable</span> Star Astronomy Prior to 1909: 1. The emergence of <span class="hlt">variable</span> star astronomy - a need for <span class="hlt">observations</span>; 2. A need for <span class="hlt">observers</span>; Part II. The Founding of the AAVSO - The William Tyler Olcott Era: 3. The amateur's amateur; 4. Amateurs in the service of science; Part III. The Leon Campbell Era: 5. Leon Campbell to the rescue; 6. Formalizing relationships; 7. The Pickering Memorial Endowment; 8. Fading of the Old Guard; 9. Growing pains and distractions; Part IV. The Service Bureau - The Margaret Mayall Era: 10. Learning about independence; 11. Eviction from Harvard College Observatory; 12. Actions and reactions; 13. In search of a home; 14. Survival on Brattle Street; 15. AAVSO achievements; 16. Breathing room on Concord Avenue; Part V. Analysis and Science: The Janet Mattei Era: 17. The growth of a director; 18. Learning the ropes the hard way; 19. Managing with renewed confidence; 20. Expanding the scientific charter; Part VI. Accelerating <span class="hlt">Observational</span> Science - The Arne Henden Era: 21. Bridging the gap; 22. Accelerating the science - the Henden era begins; Epilogue; Appendices; Index.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ClDy...47.3593M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ClDy...47.3593M"><span><span class="hlt">Decadal</span> prediction of Sahel rainfall: where does the skill (or lack thereof) come from?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohino, Elsa; Keenlyside, Noel; Pohlmann, Holger</p> <p>2016-12-01</p> <p>Previous works suggest <span class="hlt">decadal</span> predictions of Sahel rainfall could be skillful. However, the sources of such skill are still under debate. In addition, previous results are based on short validation periods (i.e. less than 50 years). In this work we propose a framework based on multi-linear regression analysis to study the potential sources of skill for predicting Sahel trends several years ahead. We apply it to an extended <span class="hlt">decadal</span> hindcast performed with the MPI-ESM-LR model that span from 1901 to 2010 with 1 year sampling interval. Our results show that the skill mainly depends on how well we can predict the timing of the global warming (GW), the Atlantic multidecadal <span class="hlt">variability</span> (AMV) and, to a lesser extent, the inter-<span class="hlt">decadal</span> Pacific oscillation signals, and on how well the system simulates the associated SST and West African rainfall response patterns. In the case of the MPI-ESM-LR <span class="hlt">decadal</span> extended hindcast, the <span class="hlt">observed</span> timing is well reproduced only for the GW and AMV signals. However, only the West African rainfall response to the AMV is correctly reproduced. Thus, for most of the lead times the main source of skill in the <span class="hlt">decadal</span> hindcast of West African rainfall is from the AMV. The GW signal degrades skill because the response of West African rainfall to GW is incorrectly captured. Our results also suggest that initialized <span class="hlt">decadal</span> predictions of West African rainfall can be further improved by better simulating the response of global SST to GW and AMV. Furthermore, our approach may be applied to understand and attribute prediction skill for other <span class="hlt">variables</span> and regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGC43D1084F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGC43D1084F"><span>An Evaluation of CMIP5 Precipitation <span class="hlt">Variability</span> for China Relative to <span class="hlt">Observations</span> and CMIP3</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frauenfeld, O. W.; Chen, L.</p> <p>2013-12-01</p> <p>Precipitation represents an important link between the atmosphere, hydrosphere, and biosphere and is thus a key component of the climate system. As indicated by the Fourth Assessment Report (AR4) of the Intergovernmental Panel on Climate Change (IPCC), global surface air temperatures increased by 0.74°C during the 20th century, with further warming of 0.2°C/<span class="hlt">decade</span> projected by the 2030s. Projected changes in precipitation, however, are much more <span class="hlt">variable</span>, and exhibit more complex temporal and spatial patterns. This presentation focuses on precipitation <span class="hlt">variability</span> based on 20 general circulation models (GCMs) participating in the fifth coupled model intercomparison project (CMIP5). Specifically, we focus on China and provide a comprehensive evaluation of the CMIP5 models compared to historical 20th century precipitation <span class="hlt">variability</span> from two <span class="hlt">observational</span> precipitation products: the University of East Anglia's Climatic Research Unit (CRU) time series (TS) dataset version 3.10, and the Global Precipitation Climatology Centre (GPCC) version 6. We also reassess the performance of the third CMIP (CMIP3) to quantify potential improvements in CMIP5 over the previous generation of GCMs. Finally, we provide 21st century precipitation projections for China based on three representative concentration pathways (RCP): RCP 8.5, 4.5, and 2.6. These future precipitation projections are presented in light of the <span class="hlt">observed</span> 20th century biases in the models. We find that CMIP5 models are able to better reproduce the general spatial pattern of <span class="hlt">observed</span> 20th century precipitation than CMIP3. However, for China as a whole, the annual precipitation magnitude is overestimated in CMIP5, more so than in CMIP3. This smaller overestimation in CMIP3 was primarily driven by a large underestimation of summer precipitation. Spatially, overestimated precipitation magnitudes are evident for most regions of China, especially along the eastern margin of the Tibetan Plateau. Over southeastern China</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.2358L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.2358L"><span><span class="hlt">Decadal</span> changes in South Pacific sea surface temperatures and the relationship to the Pacific <span class="hlt">decadal</span> oscillation and upper ocean heat content</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Linsley, Braddock K.; Wu, Henry C.; Dassié, Emilie P.; Schrag, Daniel P.</p> <p>2015-04-01</p> <p><span class="hlt">Decadal</span> changes in Pacific sea surface temperatures (SSTs) and upper ocean heat content (OHC) remain poorly understood. We present an annual average composite coral Sr/Ca-derived SST time series extending back to 1791 from Fiji, Tonga, and Rarotonga (FTR) in the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) sensitive region of the southwest Pacific. <span class="hlt">Decadal</span> SST maxima between 1805 and 1830 Common Era (C.E.) indicate unexplained elevated SSTs near the end of the Little Ice Age. The mean period of <span class="hlt">decadal</span> SST <span class="hlt">variability</span> in this region has a period near 25 years. <span class="hlt">Decades</span> of warmer (cooler) FTR SST co-occur with PDO negative (positive) phases since at least ~1930 C.E. and positively correlate with South Pacific OHC (0-700 m). FTR SST is also inversely correlated with <span class="hlt">decadal</span> changes in equatorial Pacific SST as measured by coral Sr/Ca. Collectively, these results support the fluctuating trade wind-shallow meridional overturning cell mechanism for <span class="hlt">decadal</span> modulation of Pacific SSTs and OHC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1395319-decadal-climate-prediction-project-dcpp-contribution-cmip6','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1395319-decadal-climate-prediction-project-dcpp-contribution-cmip6"><span>The <span class="hlt">Decadal</span> Climate Prediction Project (DCPP) contribution to CMIP6</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Boer, George J.; Smith, Douglas M.; Cassou, Christophe; ...</p> <p>2016-01-01</p> <p>The <span class="hlt">Decadal</span> Climate Prediction Project (DCPP) is a coordinated multi-model investigation into <span class="hlt">decadal</span> climate prediction, predictability, and <span class="hlt">variability</span>. The DCPP makes use of past experience in simulating and predicting <span class="hlt">decadal</span> <span class="hlt">variability</span> and forced climate change gained from the fifth Coupled Model Intercomparison Project (CMIP5) and elsewhere. It builds on recent improvements in models, in the reanalysis of climate data, in methods of initialization and ensemble generation, and in data treatment and analysis to propose an extended comprehensive <span class="hlt">decadal</span> prediction investigation as a contribution to CMIP6 (Eyring et al., 2016) and to the WCRP Grand Challenge on Near Term Climate Predictionmore » (Kushnir et al., 2016). The DCPP consists of three components. Component A comprises the production and analysis of an extensive archive of retrospective forecasts to be used to assess and understand historical <span class="hlt">decadal</span> prediction skill, as a basis for improvements in all aspects of end-to-end <span class="hlt">decadal</span> prediction, and as a basis for forecasting on annual to <span class="hlt">decadal</span> timescales. Component B undertakes ongoing production, analysis and dissemination of experimental quasi-real-time multi-model forecasts as a basis for potential operational forecast production. Component C involves the organization and coordination of case studies of particular climate shifts and variations, both natural and naturally forced (e.g. the “hiatus”, volcanoes), including the study of the mechanisms that determine these behaviours. Furthermore, groups are invited to participate in as many or as few of the components of the DCPP, each of which are separately prioritized, as are of interest to them.The <span class="hlt">Decadal</span> Climate Prediction Project addresses a range of scientific issues involving the ability of the climate system to be predicted on annual to <span class="hlt">decadal</span> timescales, the skill that is currently and potentially available, the mechanisms involved in long timescale <span class="hlt">variability</span>, and the production</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..124...42S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..124...42S"><span><span class="hlt">Decadal</span> <span class="hlt">variability</span> in coastal phytoplankton community composition in a changing West Antarctic Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schofield, Oscar; Saba, Grace; Coleman, Kaycee; Carvalho, Filipa; Couto, Nicole; Ducklow, Hugh; Finkel, Zoe; Irwin, Andrew; Kahl, Alex; Miles, Travis; Montes-Hugo, Martin; Stammerjohn, Sharon; Waite, Nicole</p> <p>2017-06-01</p> <p>The coastal waters of the West Antarctic Peninsula (WAP) are associated with large phytoplankton blooms dominated by large (>20 μm) diatoms however, nanoplankton (<20 μm) are also an important component of the food web. The dominant nanoflagellates in the WAP are cryptomonad algae. Using a twenty-year time series collected by the Palmer Long Term Ecological Research program at the United States Palmer Research Station, we assessed long-term patterns and stability in the coastal phytoplankton communities in the WAP. There was significant interannual <span class="hlt">variability</span> in the integrated water column chlorophyll a (chl-a) concentrations, which varied by a factor of 5 over the 20-year time series. There has been a significant positive increase in the seasonally integrated concentration of chl-a over the time series. The dominant phytoplankton were diatoms, with cryptophytes the second most abundant. Mixed flagellates also constituted a significant fraction of the chl-a but showed less interannual <span class="hlt">variability</span> than diatoms and cryophytes. Peak phytoplankton biomass was <span class="hlt">observed</span> in summer months, when monthly averaged wind speed was lower than in the fall and autumn. Cryptophytes were most abundant during the summer months (December-January) after the seasonal retreat of sea ice. While diatoms were <span class="hlt">observed</span> over the full range of <span class="hlt">observed</span> salinities 32-34.5) as well as over the full range of in situ temperatures (-1.5 to 2.5 °C), the cryptophyte populations were <span class="hlt">observed</span> in locations with lower salinity 32.5-33.75) and colder water (-1 to 1 °C). Environmental factors that favored a shallower seasonal mixed layer resulted in larger diatom blooms compared to the other phytoplankton taxa. During summer with lower phytoplankton biomass, a larger proportion of the chlorophyll a was associated with cryptophytes. These results demonstrate that continued temperature changes along the West Antarctic Peninsula will result in changes in phytoplankton concentration and community</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS31C1736S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS31C1736S"><span><span class="hlt">Decadal</span> changes in the Canary Current Upwelling Ecosystem</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santos, A. M.; Luis, J. M.; Relvas-Almeida, P.</p> <p>2013-12-01</p> <p>The Canary Current Upwelling System (CCUS) covers the latitudinal range 12-43 degrees N and has some singularities in relation to the other three major Eastern Boundary Upwelling Systems (EBUS), namely a major interruption in the continuity of the system at the Strait of Gibraltar and it is the only one with a sardine species from a different genus (Sardina vs Sardinops). Long-term trends in ocean temperature and coastal upwelling were investigated using the AVHRR Pathfinder SST (sea surface temperature) Version 5.1 dataset, in situ SST from the International Comprehensive Ocean-Atmosphere Data Set (ICOADS), and upwelling indices from the Pacific Fisheries Environmental Laboratory (PFEL). The analysis is applied to the eastern boundary of the North Atlantic, from 10 to 45 degrees N extending until 30 degrees W, focusing mainly in the CCUS because the strong dynamic link between the atmosphere and the ocean makes upwelling regions highly sensitive to global change and ideal to monitor and investigate its effects. The detail in SST <span class="hlt">variability</span> results in a large extent from the fine analysis and the numerical processing carefully designed to avoid trend bias in the climatological studies. The obtained fields of SST trends show a generalized warming of the entire region. However, alternate patches of significantly different warming rates are <span class="hlt">observed</span>, ranging from large scale down to mesoscale. Known coastal upwelling features are seen to warm at a lower rate than corresponding offshore waters, pointing to an intensification of the upwelling in the last <span class="hlt">decades</span>. Wind data are used to attempt to explain the <span class="hlt">variability</span> of some upwelling structures. Our results evidence the main role that mesoscale processes play in the modulation of the spatial and temporal <span class="hlt">variability</span> of SST, namely at the <span class="hlt">decadal</span> scale. This result prevents any global conclusion about the intensification of the upwelling at the scale of the entire CCUS. The bulk of the sardine population is located</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT........19T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT........19T"><span>What controls the <span class="hlt">variability</span> of oxygen in the subpolar North Pacific?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takano, Yohei</p> <p></p> <p>Dissolved oxygen is a widely <span class="hlt">observed</span> chemical quantity in the oceans along with temperature and salinity. Changes in the dissolved oxygen have been <span class="hlt">observed</span> over the world oceans. <span class="hlt">Observed</span> oxygen in the Ocean Station Papa (OSP, 50°N, 145°W) in the Gulf of Alaska exhibits strong <span class="hlt">variability</span> over interannual and <span class="hlt">decadal</span> timescales, however, the mechanisms driving the <span class="hlt">observed</span> <span class="hlt">variability</span> are not yet fully understood. Furthermore, irregular sampling frequency and relatively short record length make it difficult to detect a low-frequency <span class="hlt">variability</span>. Motivated by these <span class="hlt">observations</span>, we investigate the mechanisms driving the low-frequency <span class="hlt">variability</span> of oxygen in the subpolar North Pacific. The specific purposes of this study are (1) to evaluate the robustness of the <span class="hlt">observed</span> low-frequency <span class="hlt">variability</span> of dissolved oxygen and (2) to determine the mechanisms driving the <span class="hlt">observed</span> <span class="hlt">variability</span> using statistical data analysis and numerical simulations. To evaluate the robustness of the low-frequency <span class="hlt">variability</span>, we conducted spectral analyses on the <span class="hlt">observed</span> oxygen at OSP. To address the irregular sampling frequency we randomly sub-sampled the raw data to form 500 ensemble members with a regular time interval, and then performed spectral analyses. The resulting power spectrum of oxygen exhibits a robust low-frequency <span class="hlt">variability</span> and a statistically significant spectral peak is identified at a timescale of 15--20 years. The wintertime oceanic barotropic streamfunction is significantly correlated with the <span class="hlt">observed</span> oxygen anomaly at OSP with a north-south dipole structure over the North Pacific. We hypothesize that the <span class="hlt">observed</span> low-frequency <span class="hlt">variability</span> is primarily driven by the <span class="hlt">variability</span> of large-scale ocean circulation in the North Pacific. To test this hypothesis, we simulate the three-dimensional distribution of oxygen anomaly between 1952 to 2001 using data-constrained circulation fields. The simulated oxygen anomaly shows an outstanding <span class="hlt">variability</span> in the Gulf of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.2931B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.2931B"><span>Changes in intense tropical cyclone activity for the western North Pacific during the last <span class="hlt">decades</span> derived from a regional climate model simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barcikowska, Monika; Feser, Frauke; Zhang, Wei; Mei, Wei</p> <p>2017-11-01</p> <p>An atmospheric regional climate model (CCLM) was employed to dynamically downscale atmospheric reanalyses (NCEP/NCAR 1, ERA 40) over the western North Pacific and South East Asia. This approach is used for the first time to reconstruct a tropical cyclone climatology, which extends beyond the satellite era and serves as an alternative data set for inhomogeneous <span class="hlt">observation</span>-derived records (Best Track Data sets). The simulated TC climatology skillfully reproduces <span class="hlt">observations</span> of the recent <span class="hlt">decades</span> (1978-2010), including spatial patterns, frequency, lifetime, trends, <span class="hlt">variability</span> on interannual and <span class="hlt">decadal</span> time scales and their association with the large-scale circulation patterns. These skills, facilitated here with the spectral nudging method, seem to be a prerequisite to understand the factors determining spatio-temporal <span class="hlt">variability</span> of TC activity over the western North Pacific. Long-term trends (1948-2011 and 1959-2001) in both simulations show a strong increase of intense tropical cyclone activity. This contrasts with pronounced multidecadal variations found in <span class="hlt">observations</span>. The discrepancy may partly originate from temporal inhomogeneities in atmospheric reanalyses and Best Track Data, which affect both the model-based and <span class="hlt">observational</span>-based trends. An adjustment, which removes the simulated upward trend, reduces the apparent discrepancy. Ultimately, our <span class="hlt">observational</span> and modeling analysis suggests an important contribution of multi-<span class="hlt">decadal</span> fluctuations in the TC activity during the last six <span class="hlt">decades</span>. Nevertheless, due to the uncertainties associated with the inconsistencies and quality changes of those data sets, we call for special caution when reconstructing long-term TC statistics either from atmospheric reanalyses or Best Track Data.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000358','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000358"><span>Highlights from a <span class="hlt">Decade</span> of OMI-TOMS Total Ozone <span class="hlt">Observations</span> on EOS Aura</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Haffner, David P.; Bhartia, Pawan K.; McPeters, Richard D.; Joiner, Joanna; Ziemke, Jerald R.; Vassilkov, Alexander; Labow, Gordon J.; Chiou, Er-Woon</p> <p>2014-01-01</p> <p>Total ozone measurements from OMI have been instrumental in meeting Aura science objectives. In the last <span class="hlt">decade</span>, OMI has extended the length of the TOMS total ozone record to over 35 years to monitor stratospheric ozone recovery. OMI-TOMS total ozone measurements have also been combined synergistically with measurements from other Aura instruments and MLS in particular, which provides vertically resolved information that complements the total O3 mapping capability of OMI. With this combined approach, the EOS Aura platform has produced more accurate and detailed measurements of tropospheric ozone. This has led in turn to greater understanding of the sources and transport of tropospheric ozone as well as its radiative forcing effect. The combined use of OMI and MLS data was also vital to the analysis of the severe Arctic ozone depletion event of 2011. The quality of OMI-TOMS total O3 data used in these studies is the result of several factors: a mature and well-validated algorithm, the striking stability of the OMI instrument, and OMI's hyperspectral capabilities used to derive cloud pressures. The latter has changed how we think about the effects of clouds on total ozone retrievals. We will discuss the evolution of the operational V8.5 algorithm and provide an overview and motivation for V9. After reviewing results and developments of the past <span class="hlt">decade</span>, we finally highlight how ozone <span class="hlt">observations</span> from EOS Aura are playing an important role in new ozone mapping missions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A24D..03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A24D..03W"><span>A <span class="hlt">Decade</span> of Global Lidar Cloud and Aerosol Profiling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winker, D. M.</p> <p>2016-12-01</p> <p>The CALIPSO satellite was developed as a collaboration between NASA and CNES with the objective of globally profiling aerosols and clouds for the first time. Launched in April 2006, CALIPSO has now flown for a <span class="hlt">decade</span> as part of the A-train satellite constellation, producing an unprecedented 3D <span class="hlt">observational</span> record and more than a thousand publications to date. Originally planned as a three-year mission, the unanticipated duration of the CALIPSO mission has allowed the characterization of seasonal and interannual <span class="hlt">variability</span> of aerosols and clouds. This presentation will discuss highlights among the scientific findings from CALIPSO, including contributions to our understanding of Earth's climate and climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51L..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51L..02D"><span>Role of the North Atlantic Ocean in Low Frequency Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Danabasoglu, G.; Yeager, S. G.; Kim, W. M.; Castruccio, F. S.</p> <p>2017-12-01</p> <p>The Atlantic Ocean is a unique basin with its extensive, North - South overturning circulation, referred to as the Atlantic meridional overturning circulation (AMOC). AMOC is thought to represent the dynamical memory of the climate system, playing an important role in <span class="hlt">decadal</span> and longer time scale climate <span class="hlt">variability</span> as well as prediction of the earth's future climate on these time scales via its large heat and salt transports. This oceanic memory is communicated to the atmosphere primarily through the influence of persistent sea surface temperature (SST) variations. Indeed, many modeling studies suggest that ocean circulation, i.e., AMOC, is largely responsible for the creation of coherent SST <span class="hlt">variability</span> in the North Atlantic, referred to as Atlantic Multidecadal <span class="hlt">Variability</span> (AMV). AMV has been linked to many (multi)<span class="hlt">decadal</span> climate variations in, e.g., Sahel and Brazilian rainfall, Atlantic hurricane activity, and Arctic sea-ice extent. In the absence of long, continuous <span class="hlt">observations</span>, much of the evidence for the ocean's role in (multi)<span class="hlt">decadal</span> <span class="hlt">variability</span> comes from model simulations. Although models tend to agree on the role of the North Atlantic Oscillation in creating the density anomalies that proceed the changes in ocean circulation, model fidelity in representing <span class="hlt">variability</span> characteristics, mechanisms, and air-sea interactions remains a serious concern. In particular, there is increasing evidence that models significantly underestimate low frequency <span class="hlt">variability</span> in the North Atlantic compared to available <span class="hlt">observations</span>. Such model deficiencies can amplify the relative influence of external or stochastic atmospheric forcing in generating (multi)<span class="hlt">decadal</span> <span class="hlt">variability</span>, i.e., AMV, at the expense of ocean dynamics. Here, a succinct overview of the current understanding of the (North) Atlantic Ocean's role on the regional and global climate, including some outstanding questions, will be presented. In addition, a few examples of the climate impacts of the AMV via</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC54C2279D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC54C2279D"><span>Can unforced radiative <span class="hlt">variability</span> explain the "hiatus"?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Donohoe, A.</p> <p>2016-02-01</p> <p>The paradox of the "hiatus" is characterized as a <span class="hlt">decade</span> long period over which global mean surface temperature remained relatively constant even though greenhouse forcing forcing is believed to have been positive and increasing. Explanations of the hiatus have focused on two primary lines of thought: 1. There was a net radiative imbalance at the top of atmosphere (TOA) but this energy input was stored in the ocean without increasing surface temperature or 2. There was no radiative imbalance at the TOA because the greenhouse forcing was offset by other climate forcings. Here, we explore a third hypothesis: that there was no TOA radiative imbalance over the <span class="hlt">decade</span> due to unforced, natural modes of radiative <span class="hlt">variability</span> that are unrelated to global mean temperature. Is it possible that the Earth could emit enough radiation to offset greenhouse forcing without increasing its temperature due to internal modes of climate <span class="hlt">variability</span>? Global mean TOA energy imbalance is estimated to be 0.65 W m-2 as determined from the long term change in ocean heat content - where the majority of the energy imbalance is stored. Therefore, in order to offset this TOA energy imbalance natural modes of radiative <span class="hlt">variability</span> with amplitudes of order 0.5 W m-2 at the <span class="hlt">decadal</span> timescale are required. We demonstrate that unforced coupled climate models have global mean radiative <span class="hlt">variability</span> of the required magnitude (2 standard deviations of 0.57 W m-2 in the inter-model mean) and that the vast majority (>90%) of this <span class="hlt">variability</span> is unrelated to surface temperature radiative feedbacks. However, much of this <span class="hlt">variability</span> is at shorter (monthly and annual) timescales and does not persist from year to year making the possibility of a <span class="hlt">decade</span> long natural interruption of the energy accumulation in the climate system unlikely due to natural radiative <span class="hlt">variability</span> alone given the magnitude of the greenhouse forcing on Earth. Comparison to <span class="hlt">observed</span> satellite data suggest the models capture the magnitude</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017xru..conf...36A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017xru..conf...36A"><span>Optical <span class="hlt">variability</span> properties of the largest AGN sample <span class="hlt">observed</span> with Kepler/K2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aranzana, E.; Koerding, E.; Uttley, P.; Scaringi, S.; Steven, B.</p> <p>2017-10-01</p> <p>We present the first short time-scale ( hours to days) optical <span class="hlt">variability</span> study of a large sample of Active Galactic Nuclei (AGN) <span class="hlt">observed</span> with the Kepler/K2 mission. The sample contains 275 AGN <span class="hlt">observed</span> over four campaigns with ˜30-minute cadence selected from the Million Quasar Catalogue with R magnitude < 19. We performed time series analysis to determine their <span class="hlt">variability</span> properties by means of the power spectral densities (PSDs) and applied Monte Carlo techniques to find the best model parameters that fit the <span class="hlt">observed</span> power spectra. A power-law model is sufficient to describe all the PSDs of the AGN in our sample. The average power-law slope is 2.5±0.5, steeper than the PSDs <span class="hlt">observed</span> in X-rays, and the rest-frame amplitude <span class="hlt">variability</span> in the frequency range of 6×10^{-6}-10^{-4} Hz varies from 1-10 % with an average of 2.6 %. We explore correlations between the <span class="hlt">variability</span> amplitude and key parameters of the AGN, finding a significant correlation of rest-frame short-term <span class="hlt">variability</span> amplitude with redshift, but no such correlation with luminosity. We attribute these effects to the known 'bluer when brighter <span class="hlt">variability</span> of quasars combined with the fixed bandpass of Kepler. This study enables us to distinguish between Seyferts and Blazar and confirm AGN candidates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H43D1677D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H43D1677D"><span>Trend and <span class="hlt">variability</span> in western and central Africa streamflow, and major drivers of <span class="hlt">variability</span> between 1950 and 2005</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dieppois, B.; Sidibe, M.; Mahe, G. M.; Paturel, J. E.; Anifowose, B. A.; Lawler, D.; Amoussou, E.</p> <p>2017-12-01</p> <p>Unprecedented drought episodes that struck western and central Africa between the late 1960s and 1980s, triggered many studies investigating rainfall <span class="hlt">variability</span> and its impacts on water resources and food production systems. However, most studies were focused at the catchment scale. In this study, we aim at investigating the key large-scale controls determining and modulating climate-river flows relationships at the subcontinental scale between 1950 and 2005. Using the first complete monthly streamflow data set (1950-2005) over western and central Africa, streamflow trend and <span class="hlt">variability</span> are seasonally assessed at this subcontinental scale and compared to those <span class="hlt">observed</span> in other hydroclimatic <span class="hlt">variables</span> (precipitation, temperature and potential evapotranspiration). Long-term trends and <span class="hlt">variability</span> in streamflow are mainly consistent with trends in rainfall. In particular, the recent post-1990s partial recovery in Sahel rainfall could have, at least partially, positively impacted river flows (e.g. the Senegal and Niger rivers). However, these relationships may have been moderated by: i) changes in land use; and ii) contributions from groundwater resources. In addition, the time-evolution of river flows is shown to be primarily driven by very strong <span class="hlt">decadal</span> fluctuations, which can be interpreted as modulations in the baseflow, as determined using multi-temporal trend and continuous wavelet analysis. These <span class="hlt">decadal</span> fluctuations, which are also significantly detected in rainfall, are likely related to large-scale sea-surface temperature (SST) anomaly patterns (such as the tropical Atlantic SST <span class="hlt">variability</span>, the Atlantic Multidecadal Oscillation, the Interdecadal Pacific Oscillation and the Pacific <span class="hlt">Decadal</span> Oscillation), which are together modulating the West African monsoon. Furthermore, influences of the catchment properties (e.g. size, vegetation and land use cover, soil properties, direction of stream flow across climate zones) on these <span class="hlt">decadal</span> fluctuations in river</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70100468','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70100468"><span><span class="hlt">Decadal</span> surface water quality trends under <span class="hlt">variable</span> climate, land use, and hydrogeochemical setting in Iowa, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Green, Christopher T.; Bekins, Barbara A.; Kalkhoff, Stephen J.; Hirsch, Robert M.; Liao, Lixia; Barnes, Kimberlee K.</p> <p>2014-01-01</p> <p>Understanding how nitrogen fluxes respond to changes in agriculture and climate is important for improving water quality. In the midwestern United States, expansion of corn cropping for ethanol production led to increasing N application rates in the 2000s during a period of extreme <span class="hlt">variability</span> of annual precipitation. To examine the effects of these changes, surface water quality was analyzed in 10 major Iowa Rivers. Several <span class="hlt">decades</span> of concentration and flow data were analyzed with a statistical method that provides internally consistent estimates of the concentration history and reveals flow-normalized trends that are independent of year-to-year streamflow variations. Flow-normalized concentrations of nitrate+nitrite-N decreased from 2000 to 2012 in all basins. To evaluate effects of annual discharge and N loading on these trends, multiple conceptual models were developed and calibrated to flow-weighted annual concentrations. The recent declining concentration trends can be attributed to both very high and very low discharge in the 2000s and to the long (e.g., 8 year) subsurface residence times in some basins. Dilution of N and depletion of stored N occurs in years with high discharge. Reduced N transport and increased N storage occurs in low-discharge years. Central Iowa basins showed the greatest reduction in flow-normalized concentrations, likely because of smaller storage volumes and shorter residence times. Effects of land-use changes on the water quality of major Iowa Rivers may not be noticeable for years or <span class="hlt">decades</span> in peripheral basins of Iowa, and may be obscured in the central basins where extreme flows strongly affect annual concentration trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Obs...136..168O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Obs...136..168O"><span>Early-20th-century visual <span class="hlt">observations</span> of M13 <span class="hlt">variable</span> stars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osborn, W.; Barnard, E. E.</p> <p>2016-08-01</p> <p>In 1900 E. E. Barnard published 37 visual <span class="hlt">observations</span> of <span class="hlt">Variable</span> 2 (V2) in the globular clustter M13 made in 1899 and 1900. A review of Barnard's notebooks revealed he made many additional brightness estimates up to 1911, and he had also recorded the variations of V1 starting in 1904. These data provide the earliest-epoch light curves for these stars and thus are useful for studying their period changes. This paper presents Barnard's <span class="hlt">observations</span> of the M13 <span class="hlt">variables</span> along with their derived heliocentric Julian Dates and approximate V magnitudes. These include 231 unpublished <span class="hlt">observations</span> of V2 and 94 of V1. How these data will be of value for determing period changes by these stars is described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110013132','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110013132"><span>New Insights in Tropospheric Ozone and its <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Oman, Luke D.; Douglass, Anne R.; Ziemke, Jerry R.; Rodriquez, Jose M.</p> <p>2011-01-01</p> <p>We have produced time-slice simulations using the Goddard Earth <span class="hlt">Observing</span> System Version 5 (GEOS-5) coupled to a comprehensive stratospheric and tropospheric chemical mechanism. These simulations are forced with <span class="hlt">observed</span> sea surface temperatures over the past 25 years and use constant specified surface emissions, thereby providing a measure of the dynamically controlled ozone response. We examine the model performance in simulating tropospheric ozone and its <span class="hlt">variability</span>. Here we show targeted comparisons results from our simulations with a multi-<span class="hlt">decadal</span> tropical tropospheric column ozone dataset obtained from satellite <span class="hlt">observations</span> of total column ozone. We use SHADOZ ozonesondes to gain insight into the <span class="hlt">observed</span> vertical response and compare with the simulated vertical structure. This work includes but is not limited to ENSO related <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.1829K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.1829K"><span><span class="hlt">Variability</span> and evolution of the midlatitude stratospheric aerosol budget from 22 years of ground-based lidar and satellite <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khaykin, Sergey M.; Godin-Beekmann, Sophie; Keckhut, Philippe; Hauchecorne, Alain; Jumelet, Julien; Vernier, Jean-Paul; Bourassa, Adam; Degenstein, Doug A.; Rieger, Landon A.; Bingen, Christine; Vanhellemont, Filip; Robert, Charles; DeLand, Matthew; Bhartia, Pawan K.</p> <p>2017-02-01</p> <p>The article presents new high-quality continuous stratospheric aerosol <span class="hlt">observations</span> spanning 1994-2015 at the French Observatoire de Haute-Provence (OHP, 44° N, 6° E) obtained by two independent, regularly maintained lidar systems operating within the Network for Detection of Atmospheric Composition Change (NDACC). Lidar series are compared with global-coverage <span class="hlt">observations</span> by Stratospheric Aerosol and Gas Experiment (SAGE II), Global Ozone Monitoring by Occultation of Stars (GOMOS), Optical Spectrograph and InfraRed Imaging System (OSIRIS), Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP), and Ozone Mapping Profiling Suite (OMPS) satellite instruments, altogether covering the time span of OHP lidar measurements. Local OHP and zonal-mean satellite series of stratospheric aerosol optical depth are in excellent agreement, allowing for accurate characterization of stratospheric aerosol evolution and <span class="hlt">variability</span> at northern midlatitudes during the last 2 <span class="hlt">decades</span>. The combination of local and global <span class="hlt">observations</span> is used for a careful separation between volcanically perturbed and quiescent periods. While the volcanic signatures dominate the stratospheric aerosol record, the background aerosol abundance is found to be modulated remotely by the poleward transport of convectively cleansed air from the deep tropics and aerosol-laden air from the Asian monsoon region. The annual cycle of background aerosol at midlatitudes, featuring a minimum during late spring and a maximum during late summer, correlates with that of water vapor from the Aura Microwave Limb Sounder (MLS). <span class="hlt">Observations</span> covering two volcanically quiescent periods over the last 2 <span class="hlt">decades</span> provide an indication of a growth in the nonvolcanic component of stratospheric aerosol. A statistically significant factor of 2 increase in nonvolcanic aerosol since 1998, seasonally restricted to late summer and fall, is associated with the influence of the Asian monsoon and growing pollution therein.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E.551E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E.551E"><span><span class="hlt">Observations</span> of GAIA-identified Cataclysmic <span class="hlt">Variables</span> Using the TUBITAK National Observatory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esenoglu, Hasan H.; Kirbiyik, Halil; Kaynar, Suleyman; Okuyan, Oguzhan; Hamitoglu, Irek; Galeev, Almaz; Uluc, Kadir; Kocak, Murat; Kilic, Sila E.; Parmaksizoglu, Murat; Erece, Orhan; Ozisik, Tuncay; Gulsecen, Hulusi</p> <p>2016-07-01</p> <p>TUBITAK National Observatory supports the GAIA alerts with <span class="hlt">observations</span> using three telescopes (RTT150, T100, T60) at the site with a limited time quota. We have <span class="hlt">observed</span> 10 <span class="hlt">variable</span> stars among GAIA sources discovered in the years 2014-2016 that may be candidate Cataclysmic <span class="hlt">Variables</span> (CVs). Our TUG <span class="hlt">observations</span> at this stage involve photometry and spectroscopy to aid the identification of these sources. The first preliminary result of our <span class="hlt">observations</span> of Gaia14aat among them showed a dwarf nova outburst with an amplitude of 2.69 mag. We aim to construct a GAIA astrophysics group to study CVs along with supported studies using the SRG (Spectrum Roentgen Gamma astrophysical observatory) after the year of 2016. These <span class="hlt">observations</span> will basically involve spectroscopy, narrow-band CCD imaging and photometry using several filters to aid the identification of these sources. RTT150 <span class="hlt">observations</span> with very narrow filters (like H-alpha, SII, OIII with band width of range of 2 to 5 nm) will reveal whether shell around the SRG sources to aid identification novae among them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002PrOce..55..235W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002PrOce..55..235W"><span>Flatfish recruitment response to <span class="hlt">decadal</span> climatic <span class="hlt">variability</span> and ocean conditions in the eastern Bering Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilderbuer, T. K.; Hollowed, A. B.; Ingraham, W. J.; Spencer, P. D.; Conners, M. E.; Bond, N. A.; Walters, G. E.</p> <p>2002-10-01</p> <p>This paper provides a retrospective analysis of the relationship of physical oceanography and biology and recruitment of three Eastern Bering Sea flatfish stocks: flathead sole ( Hippoglossoides elassodon), northern rock sole ( Lepidopsetta polyxystra), and arrowtooth flounder ( Atheresthes stomias) for the period 1978-1996. Temporal trends in flatfish production in the Eastern Bering Sea are consistent with the hypothesis that <span class="hlt">decadal</span> scale climate <span class="hlt">variability</span> influences marine survival during the early life history period. Density-dependence (spawning stock size) is statistically significant in a Ricker model of flatfish recruitment, which includes environmental terms. Wind-driven advection of flatfish larvae to favorable nursery grounds was also found to coincide with years of above-average recruitment through the use of an ocean surface current simulation model (OSCURS). Ocean forcing of Bristol Bay surface waters during springtime was mostly shoreward (eastward) during the 1980s and seaward (westerly) during the 1990s, corresponding with periods of good and poor recruitment. Distance from shore and water depth at the endpoint of 90-day drift periods (estimated time of settlement) were also found to correspond with flatfish productivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860017433&hterms=Andromeda&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAndromeda','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860017433&hterms=Andromeda&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DAndromeda"><span>A <span class="hlt">decade</span> of SETI <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dixon, R. S.</p> <p>1986-01-01</p> <p>A full time dedicated search for extraterrestrial radio signals of intelligent origin has been in progress at the Ohio State University Radio Observatory since 1973. The radio telescope has a collecting area of 2200 square meters, which is equivalent to a circular dish 175 feet in diameter. The search concentrates on a 500 kHz bandwidth centered on the 1420 MHz hydrogen line, Doppler corrected to the galactic standard of rest. A large portion of the sky visible from Ohio was searched, with particulat emphasis on the galactic center region and the M31 Andromeda galaxy. The survey is largely computer automated, and all data reduction is done in real time. Two distinct populations of signals were detected. The first is a relatively small number of signals which persist for over a minute and which are clearly extraterrestrial in origin. The second is the large number of signals which persist less than 10 seconds whose locations are anticorrelated with the galactic plane but show clumps along the galactic axis. None of these signals were <span class="hlt">observed</span> to recur, despite repeated <span class="hlt">observations</span>. The cause of these signals were not determined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20787613-comment-all-quantum-observables-hidden-variable-model-must-commute-simultaneously','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20787613-comment-all-quantum-observables-hidden-variable-model-must-commute-simultaneously"><span>Comment on 'All quantum <span class="hlt">observables</span> in a hidden-<span class="hlt">variable</span> model must commute simultaneously'</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Nagata, Koji</p> <p></p> <p>Malley discussed [Phys. Rev. A 69, 022118 (2004)] that all quantum <span class="hlt">observables</span> in a hidden-<span class="hlt">variable</span> model for quantum events must commute simultaneously. In this comment, we discuss that Malley's theorem is indeed valid for the hidden-<span class="hlt">variable</span> theoretical assumptions, which were introduced by Kochen and Specker. However, we give an example that the local hidden-<span class="hlt">variable</span> (LHV) model for quantum events preserves noncommutativity of quantum <span class="hlt">observables</span>. It turns out that Malley's theorem is not related to the LHV model for quantum events, in general.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060037970&hterms=Mount+Rainier&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DMount%2BRainier','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060037970&hterms=Mount+Rainier&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DMount%2BRainier"><span>(abstract) Mount Rainier: New Remote Sensing <span class="hlt">Observations</span> of a <span class="hlt">Decade</span> Volcano</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Realmuto, V. J.; Zebker, H. A.; Frank, D.</p> <p>1994-01-01</p> <p>Mount Rainier was selected as a <span class="hlt">Decade</span> Volcano by the International Association of Volcanology and Chemistry of the Earth's Interior. The purpose of this selection is to focus scientific and public attention on Mount Rainier during the current <span class="hlt">decade</span>, the United Nations-designated International <span class="hlt">Decade</span> of Natural Hazard Reduction. The Mount Rainier science plan calls for remote sensing surveys to monitor the volcano. To date, we have conducted airborne surveys with visible and near-infrared, thermal infrared, and interferometric radar instruments. Our preliminary analysis of some night-time time-series thermal infrared survey data sets of the summit suggests that, aside from seasonal variations in snow cover, there have been no qualitative changes in the size or pattern of the summit hot spots. Day-time airborne surveys were done to record the current surface appearance of the volcano and map hydrothermal alteration in the summit region. An interferometric radar survey yielded a high-resolution digital elevation model (DEM) which serves as a base for the registration of the other remote sensing data sets. More importantly, the DEM documents the current topography of glaciers and valleys. Planned biannual radar survey of mount rainier will produce a data set from which seasonal changes in glacier and valley topography can be characterized. Such characterization is essential if we are to recognize geothermally induced changes in snow and ice cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19750044107&hterms=effect+global+warming&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Deffect%2Bglobal%2Bwarming','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19750044107&hterms=effect+global+warming&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Deffect%2Bglobal%2Bwarming"><span>Recent advances in satellite <span class="hlt">observations</span> of solar <span class="hlt">variability</span> and global atmospheric ozone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Heath, D. F.</p> <p>1974-01-01</p> <p>A description is given of the temporal behavior of the sun as an ultraviolet <span class="hlt">variable</span> star in relation to daily zonal means of atmospheric ozone from the total amount to that above the 10-mb and 4-mb pressure levels. A significant correlation has been <span class="hlt">observed</span> between enhancements in the ultraviolet solar irradiances and terrestrial passages of the solar magnetic field sector boundary structure. However, it has not yet been possible to separate solar from the dynamical effects on the <span class="hlt">variability</span> in the zonal means of ozone. Attention is given to global changes in ozone which have been derived from the satellite <span class="hlt">observations</span> in terms of season, solar <span class="hlt">variability</span>, and major stratospheric disturbances such as stratospheric warmings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033816','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033816"><span>An 1800-yr record of <span class="hlt">decadal</span>-scale hydroclimatic <span class="hlt">variability</span> in the upper Arkansas River basin from bristlecone pine</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Woodhouse, C.A.; Pederson, G.T.; Gray, S.T.</p> <p>2011-01-01</p> <p>Bristlecone pine trees are exceptionally long-lived, and with the incorporation of remnant material have been used to construct multi-millennial length ring-width chronologies. These chronologies can provide valuable information about past temperature and moisture <span class="hlt">variability</span>. In this study, we outline a method to build a moisture-sensitive bristlecone chronology and assess the robustness and consistency of this sensitivity over the past 1200. yr using new reconstructions of Arkansas River flow (AD 1275-2002 and 1577-2002) and the summer Palmer Drought Sensitivity Index. The chronology, a composite built from parts of three collections in the central Rocky Mountains, is a proxy for <span class="hlt">decadal</span>-scale moisture <span class="hlt">variability</span> for the past 18 centuries. Since the sample size is small in some portions of the time series, the chronology should be considered preliminary; the timing and duration of drought events are likely the most robust characteristics. This chronology suggests that the region experienced increased aridity during the medieval period, as did much of western North America, but that the timing and duration of drought episodes within this period were somewhat different from those in other western locations, such as the upper Colorado River basin. ?? 2010 University of Washington.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A31E0112Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A31E0112Y"><span><span class="hlt">Decadal</span> Variation's Offset of Global Warming in Recent Tropical Pacific Climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yeo, S. R.; Yeh, S. W.; Kim, K. Y.; Kim, W.</p> <p>2015-12-01</p> <p>Despite the increasing greenhouse gas concentration, there is no significant warming in the sea surface temperature (SST) over the tropical eastern Pacific since about 2000. This counterintuitive <span class="hlt">observation</span> has generated substantial interest in the role of low-frequency variation over the Pacific Ocean such as Pacific <span class="hlt">Decadal</span> Oscillation (PDO) or Interdecadal Pacific Oscillation (IPO). Therefore, it is necessary to appropriately separate low-frequency <span class="hlt">variability</span> and global warming from SST records. Here we present three primary modes of global SST as a secular warming trend, a low-frequency <span class="hlt">variability</span>, and a biennial oscillation through the use of novel statistical method. By analyzing temporal behavior of the three-mode, it is found that the opposite contributions of secular warming trend and cold phase of low-frequency <span class="hlt">variability</span> since 1999 account for the warming hiatus in the tropical eastern Pacific. This result implies that the low-frequency <span class="hlt">variability</span> modulates the manifestation of global warming signal in the tropical Pacific SST. Furthermore, if the low-frequency <span class="hlt">variability</span> turns to a positive phase, warming in the tropical eastern Pacific will be amplified and also strong El Niño events will occur more frequently in the near future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1513194K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1513194K"><span>What Causes the North Sea Level to Rise Faster over the Last <span class="hlt">Decade</span> ?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karpytchev, Mikhail; Letetrel, Camille</p> <p>2013-04-01</p> <p>We combined tide gauge records (PSMSL) and satellite altimetry data (TOPEX/POSEIDON-JASON 1-2) to reconstruct the mean level of the North Sea and the Norwegian Sea Shelf (NS-NSS) over 1950-2012. The reconstructed NS-NSS mean sea level fluctuations reveal a pronounced interannual <span class="hlt">variability</span> and a strong sea level acceleration since the mid-1990's. In order to understand the causes of this acceleration, the NS-NSS mean sea level was cross-correlated with the North Atlantic Oscillation and Arctic Oscillation indices. While the interannual <span class="hlt">variability</span> of the mean sea level correlates well with the NAO/AO indices, the <span class="hlt">observed</span> acceleration in the NS-NSS mean level is not linked linearly to the NAO/AO fluctuations. On the other hand, the Empirical Orthogonal Functions (EOF) analysis of steric sea level variations in the eastern North Atlantic gives a dominant EOF pattern (55% of variance explained) that varies on a <span class="hlt">decadal</span> scale very closely to the NS-NSS mean level flcutuations. Also, the amplification in the temporal amplitude of the dominant steric sea level EOF corresponds to the acceleration <span class="hlt">observed</span> in the NS-NSS mean sea level signal. This suggests that <span class="hlt">decadal</span> variations in the mean level of the North Sea - the Norwegian Sea Shelf reflect changes in the Subpolar Front currents (Rossby, 1996).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APh....80....8G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APh....80....8G"><span>Optimal strategies for <span class="hlt">observation</span> of active galactic nuclei <span class="hlt">variability</span> with Imaging Atmospheric Cherenkov Telescopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giomi, Matteo; Gerard, Lucie; Maier, Gernot</p> <p>2016-07-01</p> <p><span class="hlt">Variable</span> emission is one of the defining characteristic of active galactic nuclei (AGN). While providing precious information on the nature and physics of the sources, <span class="hlt">variability</span> is often challenging to <span class="hlt">observe</span> with time- and field-of-view-limited astronomical observatories such as Imaging Atmospheric Cherenkov Telescopes (IACTs). In this work, we address two questions relevant for the <span class="hlt">observation</span> of sources characterized by AGN-like <span class="hlt">variability</span>: what is the most time-efficient way to detect such sources, and what is the <span class="hlt">observational</span> bias that can be introduced by the choice of the <span class="hlt">observing</span> strategy when conducting blind surveys of the sky. Different <span class="hlt">observing</span> strategies are evaluated using simulated light curves and realistic instrument response functions of the Cherenkov Telescope Array (CTA), a future gamma-ray observatory. We show that strategies that makes use of very small <span class="hlt">observing</span> windows, spread over large periods of time, allows for a faster detection of the source, and are less influenced by the <span class="hlt">variability</span> properties of the sources, as compared to strategies that concentrate the <span class="hlt">observing</span> time in a small number of large <span class="hlt">observing</span> windows. Although derived using CTA as an example, our conclusions are conceptually valid for any IACTs facility, and in general, to all observatories with small field of view and limited duty cycle.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003425','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003425"><span>West African Monsoon <span class="hlt">Decadal</span> <span class="hlt">Variability</span> and Surface-Related Forcings: Second West African Monsoon Modeling and Evaluation Project Experiment (WAMME II)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Xue, Yongkang; De Sales, Fernando; Lau, William K-M; Boone, Aaron; Kim, Kyu-Myong; Mechoso, Carlos R.; Wang, Guiling; Kucharski, Fred; Schiro, Kathleen; Hosaka, Masahiro; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170003425'); toggleEditAbsImage('author_20170003425_show'); toggleEditAbsImage('author_20170003425_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170003425_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170003425_hide"></p> <p>2016-01-01</p> <p>The second West African Monsoon Modeling and Evaluation Project Experiment (WAMME II) is designed to improve understanding of the possible roles and feedbacks of sea surface temperature (SST), land use land cover change (LULCC), and aerosols forcings in the Sahel climate system at seasonal to <span class="hlt">decadal</span> scales. The WAMME II strategy is to apply prescribed <span class="hlt">observationally</span> based anomaly forcing, i.e., idealized but realistic forcing, in simulations by climate models to test the relative impacts of such forcings in producingamplifying the Sahelian seasonal and <span class="hlt">decadal</span> climate <span class="hlt">variability</span>, including the great 20th century drought. This is the first multi-model experiment specifically designed to simultaneously evaluate relative contributions of multiple external forcings to the Sahel <span class="hlt">decadal</span> precipitation anomalies between the 1980s and the 1950s that is used to characterize the Sahel 1980s drought in this study. The WAMME II models have consistently demonstrated that SST is the major contributor to the 20th century Sahel drought. Under the influence of the maximum possible SST forcing, WAMME II model ensemble mean can produce up to 60 of the precipitation difference between the 1980s and the 1950s. The present paper also delineated the role of SSTs in triggering and maintaining the Sahel drought. The impact of SSTs in individual oceans is also examined and consensus and discrepancies are reported. Among the different ocean basins, the WAMME II models show the consensus that the Indian Ocean SST has the largest impact on the precipitation temporal evolution associated with the ITCZ movement before the WAM onset while the Pacific Ocean SST greatly contributes to the summer WAM drought. This paper also compares the SST effect with the LULCC effect. Results show that with prescribed land forcing the WAMME II model ensemble mean produces about 40 of the precipitation difference between the 1980s and the 1950s, which is less than the SST contribution but still of first order</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28288628','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28288628"><span>Assessing the reporting of categorised quantitative <span class="hlt">variables</span> in <span class="hlt">observational</span> epidemiological studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mabikwa, Onkabetse V; Greenwood, Darren C; Baxter, Paul D; Fleming, Sarah J</p> <p>2017-03-14</p> <p>One aspect to consider when reporting results of <span class="hlt">observational</span> studies in epidemiology is how quantitative risk factors are analysed. The STROBE (Strengthening the Reporting of <span class="hlt">Observational</span> Studies in Epidemiology) guidelines recommend that researchers describe how they handle quantitative <span class="hlt">variables</span> when analysing data. For categorised quantitative <span class="hlt">variables</span>, the authors are required to provide reasons and justifications informing their practice. We investigated and assessed the practices and reporting of categorised quantitative <span class="hlt">variables</span> in epidemiology. The assessment was based on five medical journals that publish epidemiological research. <span class="hlt">Observational</span> studies published between April and June 2015 and investigating the relationships between quantitative exposures (or risk factors) and the outcomes were considered for assessment. A standard form was used to collect the data, and the reporting patterns amongst eligible studies were quantified and described. Out of 61 articles assessed for eligibility, 23 <span class="hlt">observational</span> studies were included in the assessment. Categorisation of quantitative exposures occurred in 61% of these studies and reasons informing the practice were rarely provided. Only one article explained the choice of categorisation in the analysis. Transformation of quantitative exposures into four or five groups was common and dominant amongst studies using equally spaced categories. Dichotomisation was not popular; the practice featured in one article. Overall, the majority (86%) of the studies preferred ordered or arbitrary group categories. Other criterions used to decide categorical boundaries were based on established guidelines such as consensus statements and WHO standards. Categorisation of continuous <span class="hlt">variables</span> remains a dominant practice in epidemiological studies. The reasons informing the practice of categorisation within published work are limited and remain unknown in most articles. The existing STROBE guidelines could provide stronger</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150023592','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150023592"><span>Spatial <span class="hlt">Variability</span> of Trace Gases During DISCOVER-AQ: Planning for Geostationary <span class="hlt">Observations</span> of Atmospheric Composition</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Follette-Cook, Melanie B.; Pickering, K.; Crawford, J.; Appel, W.; Diskin, G.; Fried, A.; Loughner, C.; Pfister, G.; Weinheimer, A.</p> <p>2015-01-01</p> <p>Results from an in-depth analysis of trace gas <span class="hlt">variability</span> in MD indicated that the <span class="hlt">variability</span> in this region was large enough to be <span class="hlt">observable</span> by a TEMPO-like instrument. The <span class="hlt">variability</span> <span class="hlt">observed</span> in MD is relatively similar to the other three campaigns with a few exceptions: CO <span class="hlt">variability</span> in CA was much higher than in the other regions; HCHO <span class="hlt">variability</span> in CA and CO was much lower; MD showed the lowest <span class="hlt">variability</span> in NO2All model simulations do a reasonable job simulating O3 <span class="hlt">variability</span>. For CO, the CACO simulations largely under over estimate the <span class="hlt">variability</span> in the <span class="hlt">observations</span>. The <span class="hlt">variability</span> in HCHO is underestimated for every campaign. NO2 <span class="hlt">variability</span> is slightly overestimated in MD, more so in CO. The TX simulation underestimates the <span class="hlt">variability</span> in each trace gas. This is most likely due to missing emissions sources (C. Loughner, manuscript in preparation).Future Work: Where reasonable, we will use these model outputs to further explore the resolvability from space of these key trace gases using analyses of tropospheric column amounts relative to satellite precision requirements, similar to Follette-Cook et al. (2015).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914238D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914238D"><span>Harmonising and semantically linking key <span class="hlt">variables</span> from in-situ <span class="hlt">observing</span> networks of an Integrated Atlantic Ocean <span class="hlt">Observing</span> System, AtlantOS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Darroch, Louise; Buck, Justin</p> <p>2017-04-01</p> <p>Atlantic Ocean <span class="hlt">observation</span> is currently undertaken through loosely-coordinated, in-situ <span class="hlt">observing</span> networks, satellite <span class="hlt">observations</span> and data management arrangements at regional, national and international scales. The EU Horizon 2020 AtlantOS project aims to deliver an advanced framework for the development of an Integrated Atlantic Ocean <span class="hlt">Observing</span> System that strengthens the Global Ocean <span class="hlt">Observing</span> System (GOOS) and contributes to the aims of the Galway Statement on Atlantic Ocean Cooperation. One goal is to ensure that data from different and diverse in-situ <span class="hlt">observing</span> networks are readily accessible and useable to a wider community, including the international ocean science community and other stakeholders in this field. To help achieve this goal, the British Oceanographic Data Centre (BODC) produced a parameter matrix to harmonise data exchange, data flow and data integration for the key <span class="hlt">variables</span> acquired by multiple in-situ AtlantOS <span class="hlt">observing</span> networks such as ARGO, Seafloor Mapping and OceanSITES. Our solution used semantic linking of controlled vocabularies and metadata for parameters that were "mappable" to existing EU and international standard vocabularies. An AtlantOS Essential <span class="hlt">Variables</span> list of terms (aggregated level) based on Global Climate <span class="hlt">Observing</span> System (GCOS) Essential Climate <span class="hlt">Variables</span> (ECV), GOOS Essential Ocean <span class="hlt">Variables</span> (EOV) and other key network <span class="hlt">variables</span> was defined and published on the Natural Environment Research Council (NERC) Vocabulary Server (version 2.0) as collection A05 (http://vocab.nerc.ac.uk/collection/A05/current/). This new vocabulary was semantically linked to standardised metadata for <span class="hlt">observed</span> properties and units that had been validated by the AtlantOS community: SeaDataNet parameters (P01), Climate and Forecast (CF) Standard Names (P07) and SeaDataNet units (P06). <span class="hlt">Observed</span> properties were mapped to biological entities from the internationally assured AphiaID from the WOrld Register of Marine Species (WoRMS), http</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160006656','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160006656"><span>Atmospheric CO2 <span class="hlt">Variability</span> <span class="hlt">Observed</span> From ASCENDS Flight Campaigns</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lin, Bing; Browell, Edward; Campbell, Joel; Choi, Yonghoon; Dobler, Jeremy; Fan, Tai-Fang; Harrison, F. Wallace; Kooi, Susan; Liu, Zhaoyan; Meadows, Byron; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160006656'); toggleEditAbsImage('author_20160006656_show'); toggleEditAbsImage('author_20160006656_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160006656_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160006656_hide"></p> <p>2015-01-01</p> <p>Significant atmospheric CO2 variations on various spatiotemporal scales were <span class="hlt">observed</span> during ASCENDS flight campaigns. For example, around 10-ppm CO2 changes were found within free troposphere in a region of about 200x300 sq km over Iowa during a summer 2014 flight. Even over extended forests, about 2-ppm CO2 column <span class="hlt">variability</span> was measured within about 500-km distance. For winter times, especially over snow covered ground, relatively less horizontal CO2 <span class="hlt">variability</span> was <span class="hlt">observed</span>, likely owing to minimal interactions between the atmosphere and land surface. Inter-annual variations of CO2 drawdown over cornfields in the Mid-West were found to be larger than 5 ppm due to slight differences in the corn growing phase and meteorological conditions even in the same time period of a year. Furthermore, considerable differences in atmospheric CO2 profiles were found during winter and summer campaigns. In the winter CO2 was found to decrease from about 400 ppm in the atmospheric boundary layer (ABL) to about 392 ppm above 10 km, while in the summer CO2 increased from 386 ppm in the ABL to about 396 ppm in free troposphere. These and other CO2 <span class="hlt">observations</span> are discussed in this presentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009CoAst.160....2L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009CoAst.160....2L"><span><span class="hlt">Observations</span> of candidate oscillating eclipsing binaries and two newly discovered pulsating <span class="hlt">variables</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liakos, A.; Niarchos, P.</p> <p>2009-03-01</p> <p>CCD <span class="hlt">observations</span> of 24 eclipsing binary systems with spectral types ranging between A0-F0, candidate for containing pulsating components, were obtained. Appropriate exposure times in one or more photometric filters were used so that short-periodic pulsations could be detected. Their light curves were analyzed using the Period04 software in order to search for pulsational behaviour. Two new <span class="hlt">variable</span> stars, namely GSC 2673-1583 and GSC 3641-0359, were discov- ered as by-product during the <span class="hlt">observations</span> of eclipsing <span class="hlt">variables</span>. The Fourier analysis of the <span class="hlt">observations</span> of each star, the dominant pulsation frequencies and the derived frequency spectra are also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900031734&hterms=Symbiotic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DSymbiotic','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900031734&hterms=Symbiotic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DSymbiotic"><span>Multifrequency <span class="hlt">observations</span> of symbiotic stars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kenyon, Scott J.</p> <p>1988-01-01</p> <p>The discovery of symbiotic stars is described, and the results of multifrequency <span class="hlt">observations</span> made during the past two <span class="hlt">decades</span> are presented. <span class="hlt">Observational</span> data identify symbiotic stars as long-period binary systems that can be divided into two basic physical classes: detached symbiotics containing a red giant (or a Mira <span class="hlt">variable</span>), and semidetached symbiotics containing a lobe-filling red giant and a solar-type main sequence star. Three components are typically <span class="hlt">observed</span>: (1) the cool giant component with an effective temperature of 2500-4000 K, which can be divided by the IR spectral classification into normal M giants (S-types) and heavily reddened Mira <span class="hlt">variables</span> (D-types); (2) the hot companion displaying a bright blue continuum at UV wavelengths, which is sometimes also an X-ray source; and (3) a gaseous nebula enveloping the binary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610430','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610430"><span>Enceladus Plume Structure and Time <span class="hlt">Variability</span>: Comparison of Cassini <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Perry, Mark E.; Hansen, Candice J.; Waite, J. Hunter; Porco, Carolyn C.; Spencer, John R.; Howett, Carly J. A.</p> <p>2017-01-01</p> <p>Abstract During three low-altitude (99, 66, 66 km) flybys through the Enceladus plume in 2010 and 2011, Cassini's ion neutral mass spectrometer (INMS) made its first high spatial resolution measurements of the plume's gas density and distribution, detecting in situ the individual gas jets within the broad plume. Since those flybys, more detailed Imaging Science Subsystem (ISS) imaging <span class="hlt">observations</span> of the plume's icy component have been reported, which constrain the locations and orientations of the numerous gas/grain jets. In the present study, we used these ISS imaging results, together with ultraviolet imaging spectrograph stellar and solar occultation measurements and modeling of the three-dimensional structure of the vapor cloud, to constrain the magnitudes, velocities, and time <span class="hlt">variability</span> of the plume gas sources from the INMS data. Our results confirm a mixture of both low and high Mach gas emission from Enceladus' surface tiger stripes, with gas accelerated as fast as Mach 10 before escaping the surface. The vapor source fluxes and jet intensities/densities vary dramatically and stochastically, up to a factor 10, both spatially along the tiger stripes and over time between flyby <span class="hlt">observations</span>. This complex spatial <span class="hlt">variability</span> and dynamics may result from time-<span class="hlt">variable</span> tidal stress fields interacting with subsurface fissure geometry and tortuosity beyond detectability, including changing gas pathways to the surface, and fluid flow and boiling in response evolving lithostatic stress conditions. The total plume gas source has 30% uncertainty depending on the contributions assumed for adiabatic and nonadiabatic gas expansion/acceleration to the high Mach emission. The overall vapor plume source rate exhibits stochastic time <span class="hlt">variability</span> up to a factor ∼5 between <span class="hlt">observations</span>, reflecting that found in the individual gas sources/jets. Key Words: Cassini at Saturn—Geysers—Enceladus—Gas dynamics—Icy satellites. Astrobiology 17, 926–940. PMID:28872900</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.3241R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.3241R"><span>Does mesoscale matters in <span class="hlt">decadal</span> changes <span class="hlt">observed</span> in the northern Canary upwelling system?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Relvas, P.; Luís, J.; Santos, A. M. P.</p> <p>2009-04-01</p> <p>The Western Iberia constitutes the northern limb of the Canary Current Upwelling System, one of the four Eastern Boundary Upwelling Systems of the world ocean. The strong dynamic link between the atmosphere and the ocean makes these systems highly sensitive to global change, ideal to monitor and investigate its effects. In order to investigate <span class="hlt">decadal</span> changes of the mesoscale patterns in the Northern Canary upwelling system (off Western Iberia), the field of the satellite-derived sea surface temperature (SST) trends was built at the pixel scale (4x4 km) for the period 1985-2007, based on the monthly mean data from the Advanced Very High Resolution Radiometer (AVHRR) on board NOAA series satellites, provided by the NASA Physical Oceanography Distributed Active Archive Center (PO.DAAC) at the Jet Propulsion Laboratory. The time series were limited to the nighttime passes to avoid the solar heating effect and a suite of procedures were followed to guarantee that the temperature trends were not biased towards the seasonally more abundant summer data, when the sky is considerably clear. A robust linear fit was applied to each individual pixel, crossing along the time the same pixel in all the processed monthly mean AVHRR SST images from 1985 until 2007. The field of the SST trends was created upon the slopes of the linear fits applied to each pixel. Monthly mean SST time series from the one degree enhanced International Comprehensive Ocean-Atmosphere Data Set (ICOADS) and from near-shore measurements collected on a daily basis by the Portuguese Meteorological Office (IM) are also used to compare the results and extend the analysis back until 1960. A generalized warming trend is detected in the coastal waters off Western Iberia during the last <span class="hlt">decades</span>, no matter which data set we analyse. However, significant spatial differences in the warming rates are <span class="hlt">observed</span> in the satellite-derived SST trends. Remarkably, off the southern part of the Western Iberia the known</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2335P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2335P"><span>An effective drift correction for dynamical downscaling of <span class="hlt">decadal</span> global climate predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paeth, Heiko; Li, Jingmin; Pollinger, Felix; Müller, Wolfgang A.; Pohlmann, Holger; Feldmann, Hendrik; Panitz, Hans-Jürgen</p> <p>2018-04-01</p> <p>Initialized <span class="hlt">decadal</span> climate predictions with coupled climate models are often marked by substantial climate drifts that emanate from a mismatch between the climatology of the coupled model system and the data set used for initialization. While such drifts may be easily removed from the prediction system when analyzing individual <span class="hlt">variables</span>, a major problem prevails for multivariate issues and, especially, when the output of the global prediction system shall be used for dynamical downscaling. In this study, we present a statistical approach to remove climate drifts in a multivariate context and demonstrate the effect of this drift correction on regional climate model simulations over the Euro-Atlantic sector. The statistical approach is based on an empirical orthogonal function (EOF) analysis adapted to a very large data matrix. The climate drift emerges as a dramatic cooling trend in North Atlantic sea surface temperatures (SSTs) and is captured by the leading EOF of the multivariate output from the global prediction system, accounting for 7.7% of total <span class="hlt">variability</span>. The SST cooling pattern also imposes drifts in various atmospheric <span class="hlt">variables</span> and levels. The removal of the first EOF effectuates the drift correction while retaining other components of intra-annual, inter-annual and <span class="hlt">decadal</span> <span class="hlt">variability</span>. In the regional climate model, the multivariate drift correction of the input data removes the cooling trends in most western European land regions and systematically reduces the discrepancy between the output of the regional climate model and <span class="hlt">observational</span> data. In contrast, removing the drift only in the SST field from the global model has hardly any positive effect on the regional climate model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012SPIE.8524E..0TC','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012SPIE.8524E..0TC"><span>A <span class="hlt">decadal</span> <span class="hlt">observation</span> of vegetation dynamics using multi-resolution satellite images</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chiang, Yang-Sheng; Chen, Kun-Shan; Chu, Chang-Jen</p> <p>2012-10-01</p> <p>Vegetation cover not just affects the habitability of the earth, but also provides potential terrestrial mechanism for mitigation of greenhouse gases. This study aims at quantifying such green resources by incorporating multi-resolution satellite images from different platforms, including Formosat-2(RSI), SPOT(HRV/HRG), and Terra(MODIS), to investigate vegetation fractional cover (VFC) and its inter-/intra-annual variation in Taiwan. Given different sensor capabilities in terms of their spatial coverage and resolution, infusion of NDVIs at different scales was used to determine fraction of vegetation cover based on NDVI. Field campaign has been constantly conducted on a monthly basis for 6 years to calibrate the critical NDVI threshold for the presence of vegetation cover, with test sites covering IPCC-defined land cover types of Taiwan. Based on the proposed method, we analyzed spatio- temporal changes of VFC for the entire Taiwan Island. A bimodal sequence of VFC was <span class="hlt">observed</span> for intra-annual variation based on MODIS data, with level around 5% and two peaks in spring and autumn marking the principal dual-cropping agriculture pattern in southwestern Taiwan. Compared to anthropogenic-prone variation, the inter-annual VFC (Aug.-Oct.) derived from HRV/HRG/RSI reveals that the moderate variations (3%) and the oscillations were strongly linked with regional climate pattern and major disturbances resulting from extreme weather events. Two distinct cycles (2002-2005 and 2005-2009) were identified in the <span class="hlt">decadal</span> <span class="hlt">observations</span>, with VFC peaks at 87.60% and 88.12% in 2003 and 2006, respectively. This time-series mapping of VFC can be used to examine vegetation dynamics and its response associated with short-term and long-term anthropogenic/natural events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.4171G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.4171G"><span>Interannual and low-frequency <span class="hlt">variability</span> of Upper Indus Basin winter/spring precipitation in <span class="hlt">observations</span> and CMIP5 models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Greene, Arthur M.; Robertson, Andrew W.</p> <p>2017-12-01</p> <p>An assessment is made of the ability of general circulation models in the CMIP5 ensemble to reproduce <span class="hlt">observed</span> modes of low-frequency winter/spring precipitation <span class="hlt">variability</span> in the region of the Upper Indus basin (UIB) in south-central Asia. This season accounts for about two thirds of annual precipitation totals in the UIB and is characterized by "western disturbances" propagating along the eastward extension of the Mediterranean storm track. <span class="hlt">Observational</span> data are utilized for for spatiotemporal characterization of the precipitation seasonal cycle, to compute seasonalized spectra and finally, to examine teleconnections, in terms of large-scale patterns in sea-surface temperature (SST) and atmospheric circulation. Annual and lowpassed variations are found to be associated primarily with SST modes in the tropical and extratropical Pacific. A more obscure link to North Atlantic SST, possibly related to the North Atlantic Oscillation, is also noted. An ensemble of 31 CMIP5 models is then similarly assessed, using unforced preindustrial multi-century control runs. Of these models, eight are found to reproduce well the two leading modes of the <span class="hlt">observed</span> seasonal cycle. This model subset is then assessed in the spectral domain and with respect to teleconnection patterns, where a range of behaviors is noted. Two model families each account for three members of this subset. The degree of within-family similarity in behavior is shown to reflect underlying model differences. The results provide estimates of unforced regional hydroclimate <span class="hlt">variability</span> over the UIB on interannual and <span class="hlt">decadal</span> scales and the corresponding far-field influences, and are of potential relevance for the estimation of uncertainties in future water availability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920056261&hterms=worlds+oceans&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dworlds%2Boceans','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920056261&hterms=worlds+oceans&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dworlds%2Boceans"><span>Unforced <span class="hlt">decadal</span> fluctuations in a coupled model of the atmosphere and ocean mixed layer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barnett, T. P.; Del Genio, A. D.; Ruedy, R. A.</p> <p>1992-01-01</p> <p>Global average temperature in a 100-year control run of a model used for greenhouse gas response simulations showed low-frequency natural <span class="hlt">variability</span> comparable in magnitude to that <span class="hlt">observed</span> over the last 100 years. The model <span class="hlt">variability</span> was found to be barotropic in the atmosphere, and located in the tropical strip with largest values near the equator in the Pacific. The model variations were traced to complex, low-frequency interactions between the meridional sea surface temperature gradients in the eastern equatorial Pacific, clouds at both high and low levels, and features of the tropical atmospheric circulation. The variations in these and other model parameters appear to oscillate between two limiting climate states. The physical scenario accounting for the oscillations on <span class="hlt">decadal</span> time scales is almost certainly not found in the real world on shorter time scales due to limited resolution and the omission of key physics (e.g., equatorial ocean dynamics) in the model. The real message is that models with dynamical limitations can still produce significant long-term <span class="hlt">variability</span>. Only a thorough physical diagnosis of such simulations and comparisons with <span class="hlt">decadal</span>-length data sets will allow one to decide if faith in the model results is, or is not, warranted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1747960','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1747960"><span>Tobacco use in popular movies during the past <span class="hlt">decade</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mekemson, C; Glik, D; Titus, K; Myerson, A; Shaivitz, A; Ang, A; Mitchell, S</p> <p>2004-01-01</p> <p>Objective: The top 50 commercially successful films released per year from 1991 to 2000 were content coded to assess trends in tobacco use over time and attributes of films predictive of higher smoking rates. Design: This <span class="hlt">observational</span> study used media content analysis methods to generate data about tobacco use depictions in films studied (n = 497). Films are the basic unit of analysis. Once films were coded and preliminary analysis completed, outcome data were transformed to approximate multivariate normality before being analysed with general linear models and longitudinal mixed method regression methods. Main outcome measures: Tobacco use per minute of film was the main outcome measure used. Predictor <span class="hlt">variables</span> include attributes of films and actors. Tobacco use was defined as any cigarette, cigar, and chewing tobacco use as well as the display of smoke and cigarette paraphernalia such as ashtrays, brand names, or logos within frames of films reviewed. Results: Smoking rates in the top films fluctuated yearly over the <span class="hlt">decade</span> with an overall modest downward trend (p < 0.005), with the exception of R rated films where rates went up. Conclusions: The decrease in smoking rates found in films in the past <span class="hlt">decade</span> is modest given extensive efforts to educate the entertainment industry on this issue over the past <span class="hlt">decade</span>. Monitoring, education, advocacy, and policy change to bring tobacco depiction rates down further should continue. PMID:15564625</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15564625','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15564625"><span>Tobacco use in popular movies during the past <span class="hlt">decade</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mekemson, C; Glik, D; Titus, K; Myerson, A; Shaivitz, A; Ang, A; Mitchell, S</p> <p>2004-12-01</p> <p>The top 50 commercially successful films released per year from 1991 to 2000 were content coded to assess trends in tobacco use over time and attributes of films predictive of higher smoking rates. This <span class="hlt">observational</span> study used media content analysis methods to generate data about tobacco use depictions in films studied (n = 497). Films are the basic unit of analysis. Once films were coded and preliminary analysis completed, outcome data were transformed to approximate multivariate normality before being analysed with general linear models and longitudinal mixed method regression methods. Tobacco use per minute of film was the main outcome measure used. Predictor <span class="hlt">variables</span> include attributes of films and actors. Tobacco use was defined as any cigarette, cigar, and chewing tobacco use as well as the display of smoke and cigarette paraphernalia such as ashtrays, brand names, or logos within frames of films reviewed. Smoking rates in the top films fluctuated yearly over the <span class="hlt">decade</span> with an overall modest downward trend (p < 0.005), with the exception of R rated films where rates went up. The decrease in smoking rates found in films in the past <span class="hlt">decade</span> is modest given extensive efforts to educate the entertainment industry on this issue over the past <span class="hlt">decade</span>. Monitoring, education, advocacy, and policy change to bring tobacco depiction rates down further should continue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021246','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021246"><span><span class="hlt">Decadal</span> variations in the strength of ENSO teleconnections with precipitation in the western United States</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McCabe, G.J.; Dettinger, M.D.</p> <p>1999-01-01</p> <p>Changing patterns of correlations between the historical average June-November Southern Oscillation Index (SOI) and October-March precipitation totals for 84 climate divisions in the western US indicate a large amount of <span class="hlt">variability</span> in SOI/precipitation relations on <span class="hlt">decadal</span> time scales. Correlations of western US precipitation with SOI and other indices of tropical El Nino-Southern Oscillation (ENSO) processes were much weaker from 1920 to 1950 than during recent <span class="hlt">decades</span>. This <span class="hlt">variability</span> in teleconnections is associated with the character of tropical air-sea interactions as indexed by the number of out-of-phase SOI/tropical sea surface temperature (SST) episodes, and with <span class="hlt">decadal</span> <span class="hlt">variability</span> in the North Pacific Ocean as indexed by the Pacific <span class="hlt">Decadal</span> Oscillation (PDO). ENSO teleconnections with precipitation in the western US are strong when SOI and NINO3 are out-of-phase and PDO is negative. ENSO teleconnections are weak when SOI and NINO3 are weakly correlated and PDO is positive. <span class="hlt">Decadal</span> modes of tropical and North Pacific Ocean climate <span class="hlt">variability</span> are important indicators of periods when ENSO indices, like SOI, can be used as reliable predictors of winter precipitation in the US.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5135338','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5135338"><span>Reducing uncertainties in <span class="hlt">decadal</span> <span class="hlt">variability</span> of the global carbon budget with multiple datasets</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Li, Wei; Ciais, Philippe; Wang, Yilong; Peng, Shushi; Broquet, Grégoire; Ballantyne, Ashley P.; Canadell, Josep G.; Cooper, Leila; Friedlingstein, Pierre; Le Quéré, Corinne; Myneni, Ranga B.; Peters, Glen P.; Piao, Shilong; Pongratz, Julia</p> <p>2016-01-01</p> <p>Conventional calculations of the global carbon budget infer the land sink as a residual between emissions, atmospheric accumulation, and the ocean sink. Thus, the land sink accumulates the errors from the other flux terms and bears the largest uncertainty. Here, we present a Bayesian fusion approach that combines multiple <span class="hlt">observations</span> in different carbon reservoirs to optimize the land (B) and ocean (O) carbon sinks, land use change emissions (L), and indirectly fossil fuel emissions (F) from 1980 to 2014. Compared with the conventional approach, Bayesian optimization decreases the uncertainties in B by 41% and in O by 46%. The L uncertainty decreases by 47%, whereas F uncertainty is marginally improved through the knowledge of natural fluxes. Both ocean and net land uptake (B + L) rates have positive trends of 29 ± 8 and 37 ± 17 Tg C⋅y−2 since 1980, respectively. Our Bayesian fusion of multiple <span class="hlt">observations</span> reduces uncertainties, thereby allowing us to isolate important <span class="hlt">variability</span> in global carbon cycle processes. PMID:27799533</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43F1135C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43F1135C"><span>Large-Scale Atmospheric Teleconnection Patterns Associated with the Interannual <span class="hlt">Variability</span> of Heatwaves in East Asia and Its <span class="hlt">Decadal</span> Changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choi, N.; Lee, M. I.; Lim, Y. K.; Kim, K. M.</p> <p>2017-12-01</p> <p>Heatwave is an extreme hot weather event which accompanies fatal damage to human health. The heatwave has a strong relationship with the large-scale atmospheric teleconnection patterns. In this study, we examine the spatial pattern of heatwave in East Asia by using the EOF analysis and the relationship between heatwave frequency and large-scale atmospheric teleconnection patterns. We also separate the time scale of heatwave frequency as the time scale longer than a <span class="hlt">decade</span> and the interannual time scale. The long-term variation of heatwave frequency in East Asia shows a linkage with the sea surface temperature (SST) <span class="hlt">variability</span> over the North Atlantic with a <span class="hlt">decadal</span> time scale (a.k.a. the Atlantic Multidecadal Oscillation; AMO). On the other hands, the interannual variation of heatwave frequency is linked with the two dominant spatial patterns associated with the large-scale teleconnection patterns mimicking the Scandinavian teleconnection (SCAND-like) pattern and the circumglobal teleconnection (CGT-like) pattern, respectively. It is highlighted that the interannual variation of heatwave frequency in East Asia shows a remarkable change after mid-1990s. While the heatwave frequency was mainly associated with the CGT-like pattern before mid-1990s, the SCAND-like pattern becomes the most dominant one after mid-1990s, making the CGT-like pattern as the second. This study implies that the large-scale atmospheric teleconnection patterns play a key role in developing heatwave events in East Asia. This study further discusses possible mechanisms for the <span class="hlt">decadal</span> change in the linkage between heatwave frequency and the large-scale teleconnection patterns in East Asia such as early melting of snow cover and/or weakening of East Asian jet stream due to global warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JCli...11.2351M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JCli...11.2351M"><span><span class="hlt">Variability</span> of the Tropical Ocean Surface Temperatures at <span class="hlt">Decadal</span>-Multidecadal Timescales. Part I: The Atlantic Ocean.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mehta, Vikram M.</p> <p>1998-09-01</p> <p>Gridded time series from the Global Ocean Surface Temperature Atlas were analyzed with a variety of techniques to identify spatial structures and oscillation periods of the tropical Atlantic sea surface temperature (SST) variations at <span class="hlt">decadal</span> timescales, and to develop physical interpretations of statistical patterns of <span class="hlt">decadal</span> SST variations. Each time series was 110 yr (1882-1991) long. The tropical Atlantic SST variations were compared with <span class="hlt">decadal</span> variations in a 74-yr-long (1912-85) north Nordeste Brazil rainfall time series and a 106-yr-long (1886-1991) tropical Atlantic cyclone activity index time series. The tropical Atlantic SST variations were also compared with <span class="hlt">decadal</span> variations in the extratropical Atlantic SST.Multiyear to multidecadal variations in the cross-equatorial dipole pattern identified as a dominant empirical pattern of the tropical Atlantic SST variations in earlier and present studies are shown to be variations in the approximately north-south gradient of SST anomalies. It is also shown that there was no dynamical-thermodynamical, dipole mode of SST variations during the analysis period. There was a distinct <span class="hlt">decadal</span> timescale (12-13 yr) of SST variations in the tropical South Atlantic, whereas no distinct <span class="hlt">decadal</span> timescale was found in the tropical North Atlantic SST variations. Approximately 80% of the coherent <span class="hlt">decadal</span> variance in the cross-equatorial SST gradient was `explained' by coherent <span class="hlt">decadal</span> oscillations in the tropical South Atlantic SSTs. There were three, possibly physical, modes of <span class="hlt">decadal</span> variations in the tropical Atlantic SSTs during the analysis period. In the more energetic mode of the North Atlantic <span class="hlt">decadal</span> SST variations, anomalies traveled into the tropical North Atlantic from the extratropical North Atlantic along the eastern boundary of the basin. The anomalies strengthened and resided in the tropical North Atlantic for several years, then frequently traveled northward into the mid-high-latitude North Atlantic along</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27126518','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27126518"><span>Juvenile recruitment in loggerhead sea turtles linked to <span class="hlt">decadal</span> changes in ocean circulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ascani, François; Van Houtan, Kyle S; Di Lorenzo, Emanuele; Polovina, Jeffrey J; Jones, T Todd</p> <p>2016-11-01</p> <p>Given the threats of climate change, understanding the relationship of climate with long-term population dynamics is critical for wildlife conservation. Previous studies have linked <span class="hlt">decadal</span> climate oscillations to indices of juvenile recruitment in loggerhead sea turtles (Caretta caretta), but without a clear understanding of mechanisms. Here, we explore the underlying processes that may explain these relationships. Using the eddy-resolving Ocean General Circulation Model for the Earth Simulator, we generate hatch-year trajectories for loggerhead turtles emanating from Japan over six <span class="hlt">decades</span> (1950-2010). We find that the proximity of the high-velocity Kuroshio Current to the primary nesting areas in southern Japan is remarkably stable and that hatchling dispersal to oceanic habitats itself does not vary on <span class="hlt">decadal</span> timescales. However, we <span class="hlt">observe</span> a shift in latitudes of trajectories, consistent with the Pacific <span class="hlt">Decadal</span> Oscillation (PDO). In a negative PDO phase, the Kuroshio Extension Current (KEC) is strong and acts as a physical barrier to the northward transport of neonates. As a result, hatch-year trajectories remain mostly below 35°N in the warm, unproductive region south of the Transition Zone Chlorophyll Front (TZCF). During a positive PDO phase, however, the KEC weakens facilitating the neonates to swim north of the TZCF into cooler and more productive waters. As a result, annual cohorts from negative PDO years may face a lack of resources, whereas cohorts from positive PDO years may find sufficient resources during their pivotal first year. These model outputs indicate that the ocean circulation dynamics, combined with navigational swimming behavior, may be a key factor in the <span class="hlt">observed</span> <span class="hlt">decadal</span> <span class="hlt">variability</span> of sea turtle populations. © 2016 John Wiley & Sons Ltd.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26912856','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26912856"><span>A <span class="hlt">decade</span> of sea level rise slowed by climate-driven hydrology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Reager, J T; Gardner, A S; Famiglietti, J S; Wiese, D N; Eicker, A; Lo, M-H</p> <p>2016-02-12</p> <p>Climate-driven changes in land water storage and their contributions to sea level rise have been absent from Intergovernmental Panel on Climate Change sea level budgets owing to <span class="hlt">observational</span> challenges. Recent advances in satellite measurement of time-<span class="hlt">variable</span> gravity combined with reconciled global glacier loss estimates enable a disaggregation of continental land mass changes and a quantification of this term. We found that between 2002 and 2014, climate <span class="hlt">variability</span> resulted in an additional 3200 ± 900 gigatons of water being stored on land. This gain partially offset water losses from ice sheets, glaciers, and groundwater pumping, slowing the rate of sea level rise by 0.71 ± 0.20 millimeters per year. These findings highlight the importance of climate-driven changes in hydrology when assigning attribution to <span class="hlt">decadal</span> changes in sea level. Copyright © 2016, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010fym..confE..13K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010fym..confE..13K"><span>Monitoring <span class="hlt">variable</span> X-ray sources in nearby galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kong, A. K. H.</p> <p>2010-12-01</p> <p>In the last <span class="hlt">decade</span>, it has been possible to monitor <span class="hlt">variable</span> X-ray sources in nearby galaxies. In particular, since the launch of Chandra, M31 has been regularly <span class="hlt">observed</span>. It is perhaps the only nearby galaxy which is <span class="hlt">observed</span> by an X-ray telescope regularly throughout operation. With 10 years of <span class="hlt">observations</span>, the center of M31 has been <span class="hlt">observed</span> with Chandra for nearly 1 Msec and the X-ray skies of M31 consist of many transients and <span class="hlt">variables</span>. Furthermore, the X-ray Telescope of Swift has been monitoring several ultraluminous X-ray sources in nearby galaxies regularly. Not only can we detect long-term X-ray <span class="hlt">variability</span>, we can also find spectral variation as well as possible orbital period. In this talk, I will review some of the important Chandra and Swift monitoring <span class="hlt">observations</span> of nearby galaxies in the past 10 years. I will also present a "high-definition" movie of M31 and discuss the possibility of detecting luminous transients in M31 with MAXI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012cosp...39.1770S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012cosp...39.1770S"><span><span class="hlt">Variability</span> of trace gas concentrations over Asian region: satellite <span class="hlt">observations</span> vs model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sheel, Varun; Richter, Andreas; Srivastava, Shuchita; Lal, Shyam</p> <p>2012-07-01</p> <p>Nitrogen dioxide (NO_2) and Carbon Monoxide (CO) play a key role in the chemistry of the tropospheric ozone and are emitted mainly by anthropogenic processes. These emissions have been increasing over Asia over the past few years due to rapid economic growth and yet there are very few systematic ground based <span class="hlt">observations</span> of these species over this region. We have analysed ten years of data from space borne instruments: Global Ozone Monitoring Experiment (GOME), SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) and Measurements of Pollution in the Troposphere (MOPITT), which have been measuring the tropospheric abundance of these trace gases. We have examined trends over the period 1996-2008 in NO_2 and CO over a few Indian regions where high economic growth in the present <span class="hlt">decade</span> is likely to see increased emissions for these species. However, even the highest growth rate of these species seen in the present study, is less when compared with similar polluted regions of China, where a much more rapid increase has been <span class="hlt">observed</span>. In order to understand the trends and <span class="hlt">variability</span> in atmospheric trace gas concentrations, one must take into account changes in emissions and transport. Only by assessing the relevance of each of these factors will it be possible to predict future changes with reasonable confidence. To this effect we have used a global chemical transport model, MOZART, to simulate concentrations of NO_2 and CO using the POET (European) and REAS (Asian) emission inventories. These are compared with satellite measurements to study seasonal variations and the discrepancies are discussed. The combined uncertainties of the emission inventory and retrieval of the satellite data could be contributing factors to the discrepancies. It may be thus worthwhile to develop emission inventories for India at a higher resolution to include local level activity data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AAS...21642604T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AAS...21642604T"><span>The American Association of <span class="hlt">Variable</span> Star <span class="hlt">Observers</span>: Serving the Research Community in 2010 and Beyond</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Templeton, Matthew R.; Henden, A. A.; Davis, K.; Kinne, R.; Watson, C.; Saladyga, M.; Waagen, E.; Beck, S.; Menali, G.; Price, A.; Turner, R.</p> <p>2010-05-01</p> <p>The American Association of <span class="hlt">Variable</span> Star <span class="hlt">Observers</span> (AAVSO) holds the largest single online database of <span class="hlt">variable</span> star data in the world, collected from thousands of amateur and professional <span class="hlt">observers</span> during the past century. One of our core missions is to preserve and distribute these data to the research community in service to the science of <span class="hlt">variable</span> star astronomy. But as an organization, the AAVSO is much more than a data archive. Our services to the research community include: monitoring for and announcement of major astronomical events like novae and supernovae; organization and management of <span class="hlt">observing</span> campaigns; support for satellite and other TOO <span class="hlt">observing</span> programs by the professional community; creation of comparison star sequences and generation of charts for the <span class="hlt">observer</span> community; and <span class="hlt">observational</span> and other support for the amateur, professional, and educator communities in all things related to <span class="hlt">variable</span> stars. As we begin a new century of <span class="hlt">variable</span> star astronomy we invite you to take advantage of the services the AAVSO can provide, and to become a part of our organization yourselves. In this poster, we highlight some of the most important services the AAVSO can provide to the professional research community, as well as suggest ways in which your research may be enhanced with support from the AAVSO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EPSC....9...86F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EPSC....9...86F"><span>A <span class="hlt">Decade</span> of Cassini Radio Science <span class="hlt">Observations</span> of the Saturn System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>French, R.; Armstrong, J.; Flasar, M.; Iess, L.; Kliore, A.; Marouf, E.; McGhee, C.; Nagy, A.; Rappaport, N.; Schinder, P.; Tortora, P.; Anabtawi, A.; Asmar, S.; Barbinis, E.; Fleischmann, D.; Kahan, D.</p> <p>2014-04-01</p> <p>The Cassini Radio Science Subsystem (RSS) on board the Cassini spacecraft has returned a wealth ofinformation about the Saturn system during its first <span class="hlt">decade</span> of <span class="hlt">observations</span>. The instrumentation is quite versatile, operating in up to three wavelengths simultaneously (S, X, and Ka bands), and tied to a very stable frequency standard either on board or uplinked to the spacecraft from a maser-controlled transmitter as part of the Deep Space Network. Over the course of the mission so far, dozens of occultations by Saturn's rings have been <span class="hlt">observed</span>, revealing the detailed structure and scattering properties of the rings at sub-km resolution. A companion set of atmospheric occultations by Saturn and Titan have provided detailed vertical profiles of the temperature of the neutral atmosphere and the electron density of the ionosphere, spanning a range of latitudes and a significant fraction of a Saturn season. Operatin in a bistatic mode, the RSS instrument has transmitted signals to the surface of Titan at the specular point such that the reflected signal is received on the earth, revealing the dielectric properties of Titan's surface. Finally, exquisitely accurate measurements of the gravitationally induced Dopper shift of the RSS transmitted signal have provided measurements of the gravitations fields and probes of the internal structure of several of Saturn's major satellites, most notably indicating the presence of sub-surface oceans on both Titan and Enceladus. During the upcoming three-year finale of the Cassini mission, highlights of the remaining RSS science objectives include high- SNR measurements of the rings at their most favorable geometry of the entire Cassini orbital tour, and a set of close orbital fly-bys of Saturn itself, enabling the determination of the planet's gravitational field to an accuracy comparable to that expected for the Juno mission to Jupiter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010NatGe...3..688O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010NatGe...3..688O"><span>External forcing as a metronome for Atlantic multidecadal <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Otterå, Odd Helge; Bentsen, Mats; Drange, Helge; Suo, Lingling</p> <p>2010-10-01</p> <p>Instrumental records, proxy data and climate modelling show that multidecadal <span class="hlt">variability</span> is a dominant feature of North Atlantic sea-surface temperature variations, with potential impacts on regional climate. To understand the <span class="hlt">observed</span> <span class="hlt">variability</span> and to gauge any potential for climate predictions it is essential to identify the physical mechanisms that lead to this <span class="hlt">variability</span>, and to explore the spatial and temporal characteristics of multidecadal <span class="hlt">variability</span> modes. Here we use a coupled ocean-atmosphere general circulation model to show that the phasing of the multidecadal fluctuations in the North Atlantic during the past 600 years is, to a large degree, governed by changes in the external solar and volcanic forcings. We find that volcanoes play a particularly important part in the phasing of the multidecadal <span class="hlt">variability</span> through their direct influence on tropical sea-surface temperatures, on the leading mode of northern-hemisphere atmosphere circulation and on the Atlantic thermohaline circulation. We suggest that the implications of our findings for <span class="hlt">decadal</span> climate prediction are twofold: because volcanic eruptions cannot be predicted a <span class="hlt">decade</span> in advance, longer-term climate predictability may prove challenging, whereas the systematic post-eruption changes in ocean and atmosphere may hold promise for shorter-term climate prediction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...842...78V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...842...78V"><span>The Viewing Geometry of Brown Dwarfs Influences Their <span class="hlt">Observed</span> Colors and <span class="hlt">Variability</span> Amplitudes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vos, Johanna M.; Allers, Katelyn N.; Biller, Beth A.</p> <p>2017-06-01</p> <p>In this paper we study the full sample of known Spitzer [3.6 μm] and J-band <span class="hlt">variable</span> brown dwarfs. We calculate the rotational velocities, v\\sin I, of 16 <span class="hlt">variable</span> brown dwarfs using archival Keck NIRSPEC data and compute the inclination angles of 19 <span class="hlt">variable</span> brown dwarfs. The results obtained show that all objects in the sample with mid-IR <span class="hlt">variability</span> detections are inclined at an angle > 20^\\circ , while all objects in the sample displaying J-band <span class="hlt">variability</span> have an inclination angle > 35^\\circ . J-band <span class="hlt">variability</span> appears to be more affected by inclination than Spitzer [3.6 μm] <span class="hlt">variability</span>, and is strongly attenuated at lower inclinations. Since J-band <span class="hlt">observations</span> probe deeper into the atmosphere than mid-IR <span class="hlt">observations</span>, this effect may be due to the increased atmospheric path length of J-band flux at lower inclinations. We find a statistically significant correlation between the color anomaly and inclination of our sample, where field objects viewed equator-on appear redder than objects viewed at lower inclinations. Considering the full sample of known <span class="hlt">variable</span> L, T, and Y spectral type objects in the literature, we find that the <span class="hlt">variability</span> properties of the two bands display notably different trends that are due to both intrinsic differences between bands and the sensitivity of ground-based versus space-based searches. However, in both bands we find that <span class="hlt">variability</span> amplitude may reach a maximum at ˜7-9 hr periods. Finally, we find a strong correlation between color anomaly and <span class="hlt">variability</span> amplitude for both the J-band and mid-IR <span class="hlt">variability</span> detections, where redder objects display higher <span class="hlt">variability</span> amplitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810032372&hterms=MOOS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DMOOS','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810032372&hterms=MOOS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DMOOS"><span><span class="hlt">Observations</span> from earth orbit and <span class="hlt">variability</span> of the polar aurora on Jupiter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Clarke, J. T.; Moos, H. W.; Atreya, S. K.; Lane, A. L.</p> <p>1980-01-01</p> <p>Spatially resolved spectra of Jupiter taken with the International Ultraviolet Explorer satellite show enhanced emissions from the polar regions at H L-alpha (1216 A) and in the Lyman and Werner bands of H2 (1175-1650 A). Two types of <span class="hlt">variability</span> in emission brightness have been <span class="hlt">observed</span> in these aurorae: an increase in the <span class="hlt">observed</span> emission as the auroral oval rotates with Jupiter's magnetic pole to face toward the earth and a general variation in brightness of more than an order of magnitude under nearly identical <span class="hlt">observing</span> conditions. In addition, the spectral character of these aurorae (determined by the ratio of H L-alpha to H2 brightnesses) appears <span class="hlt">variable</span>, indicating that the depth of penetration of the auroral particles is not constant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22660998-bayesian-techniques-comparing-time-dependent-grmhd-simulations-variable-event-horizon-telescope-observations','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22660998-bayesian-techniques-comparing-time-dependent-grmhd-simulations-variable-event-horizon-telescope-observations"><span>BAYESIAN TECHNIQUES FOR COMPARING TIME-DEPENDENT GRMHD SIMULATIONS TO <span class="hlt">VARIABLE</span> EVENT HORIZON TELESCOPE <span class="hlt">OBSERVATIONS</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kim, Junhan; Marrone, Daniel P.; Chan, Chi-Kwan</p> <p>2016-12-01</p> <p>The Event Horizon Telescope (EHT) is a millimeter-wavelength, very-long-baseline interferometry (VLBI) experiment that is capable of <span class="hlt">observing</span> black holes with horizon-scale resolution. Early <span class="hlt">observations</span> have revealed <span class="hlt">variable</span> horizon-scale emission in the Galactic Center black hole, Sagittarius A* (Sgr A*). Comparing such <span class="hlt">observations</span> to time-dependent general relativistic magnetohydrodynamic (GRMHD) simulations requires statistical tools that explicitly consider the <span class="hlt">variability</span> in both the data and the models. We develop here a Bayesian method to compare time-resolved simulation images to <span class="hlt">variable</span> VLBI data, in order to infer model parameters and perform model comparisons. We use mock EHT data based on GRMHD simulations to explore themore » robustness of this Bayesian method and contrast it to approaches that do not consider the effects of <span class="hlt">variability</span>. We find that time-independent models lead to offset values of the inferred parameters with artificially reduced uncertainties. Moreover, neglecting the <span class="hlt">variability</span> in the data and the models often leads to erroneous model selections. We finally apply our method to the early EHT data on Sgr A*.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ApJ...832..156K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ApJ...832..156K"><span>Bayesian Techniques for Comparing Time-dependent GRMHD Simulations to <span class="hlt">Variable</span> Event Horizon Telescope <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Junhan; Marrone, Daniel P.; Chan, Chi-Kwan; Medeiros, Lia; Özel, Feryal; Psaltis, Dimitrios</p> <p>2016-12-01</p> <p>The Event Horizon Telescope (EHT) is a millimeter-wavelength, very-long-baseline interferometry (VLBI) experiment that is capable of <span class="hlt">observing</span> black holes with horizon-scale resolution. Early <span class="hlt">observations</span> have revealed <span class="hlt">variable</span> horizon-scale emission in the Galactic Center black hole, Sagittarius A* (Sgr A*). Comparing such <span class="hlt">observations</span> to time-dependent general relativistic magnetohydrodynamic (GRMHD) simulations requires statistical tools that explicitly consider the <span class="hlt">variability</span> in both the data and the models. We develop here a Bayesian method to compare time-resolved simulation images to <span class="hlt">variable</span> VLBI data, in order to infer model parameters and perform model comparisons. We use mock EHT data based on GRMHD simulations to explore the robustness of this Bayesian method and contrast it to approaches that do not consider the effects of <span class="hlt">variability</span>. We find that time-independent models lead to offset values of the inferred parameters with artificially reduced uncertainties. Moreover, neglecting the <span class="hlt">variability</span> in the data and the models often leads to erroneous model selections. We finally apply our method to the early EHT data on Sgr A*.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8302S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8302S"><span>Trend and <span class="hlt">variability</span> in western and central Africa streamflow, and their relation to climate <span class="hlt">variability</span> between 1950 and 2010</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sidibe, Moussa; Dieppois, Bastien; Mahé, Gil; Paturel, Jean-Emmanuel; Rouché, Nathalie; Amoussou, Ernest; Anifowose, Babatunde; Lawler, Damian</p> <p>2017-04-01</p> <p>Unprecedented drought episodes that struck western and central Africa between the late 1960s and 1980s. This triggered many studies investigating rainfall <span class="hlt">variability</span> and its impacts on food production systems. However, most studies were focused at the catchment scale. In this study, we examine how rainfall <span class="hlt">variability</span> has impacted on river flow at the subcontinental scale between 1950 and 2010, as well as the key large-scale controls on this relationship. For the first time, we establish a complete, gap-filled, monthly streamflow data set, which extends from 1950 to 2010, over the western and central African region. To achieve this, we used linear regression modelling across and between 600 flow gauging stations (see initial database information at http://www.hydrosciences.fr/sierem/index_en.htm). Streamflow trend and <span class="hlt">variability</span> are then seasonally assessed at this subcontinental scale and compared to those <span class="hlt">observed</span> in three different rainfall data sets (i.e. CRU TS3.24, GPCC V7, IRD-HSM). Long-term trends and <span class="hlt">variability</span> in streamflow are mainly consistent with trends in rainfall. However, these relationships may have been moderated by: i) changes in land use; and ii) contributions from groundwater resources. In particular, we note that the recent post 1990s partial recovery in Sahel rainfall could have, at least partially, positively impacted river flows (e.g. the Senegal and Niger rivers). Using multi-temporal trend and continuous wavelet analysis, the time-evolution of western and central African river flows are analysed, and are all characterized by very strong <span class="hlt">decadal</span> fluctuations, which can be interpreted as modulations in the baseflow. These <span class="hlt">decadal</span> fluctuations, which are also significantly detected in rainfall, are likely related to large-scale sea-surface temperature (SST) anomaly patterns, such as the tropical Atlantic SST <span class="hlt">variability</span>, the Atlantic Multidecadal Oscillation, the Interdecadal Pacific Oscillation and/or the Pacific <span class="hlt">Decadal</span> Oscillation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23113610T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23113610T"><span>Two-<span class="hlt">Decade</span> Monitoring of MWC349 in Optical and Radio: New Results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomashow, Eydon; Jorgenson, Regina A.; Strelnitski, Vladimir; Walker, Gary; Maria Mitchell Observatory (MMO) Research Experiences for Undergraduate (REU) Interns, 2017</p> <p>2018-01-01</p> <p>Maria Mitchell Observatory (MMO) has completed the two-<span class="hlt">decade</span> long monitoring of MWC 349 in the optical and radio domains. This poster presentation will be primarily devoted to the new results obtained by optical photometry with broad and narrow band filters and <span class="hlt">observations</span> of the <span class="hlt">variability</span> in the masing H30 radio line during the <span class="hlt">observational</span> season of 2017. The H30 emission arises in the circumstellar disk of the MWC 349A component of the visual double star (with 2.4 arcsec separation between the A and B components). <span class="hlt">Variable</span> optical emission is also believed to be due to star A. By combining our optical <span class="hlt">observations</span> with earlier MMO <span class="hlt">observations</span>, we not only confirmed the previously known quasi-period of ~230 days, but confirmed a second period of ~700 days. One of the most interesting results of radio monitoring is the long-term <span class="hlt">variability</span> of the systemic radial velocity of star A, as determined through averaging the radial velocities of the two masing peaks arising in the circumstellar disk. This may be the first case where a possible hidden close companion of a star (a lower mass star or a massive protoplanet) is detected by monitoring the radial velocity of the star via the spectral line radiation from its disk. E.T. completed this project as a 2017 MMO NSF REU intern and would like to thank the other interns for their help in conducting the optical <span class="hlt">observations</span>. This project was supported in part by the NSF REU grant AST-1358980 and by the Nantucket Maria Mitchell Association.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4851402M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4851402M"><span>Recent <span class="hlt">Variability</span> <span class="hlt">Observations</span> of Solar System Giant Planets: Fresh Context for Understanding Exoplanet and Brown Dwarf Weather</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marley, Mark S.; Kepler Giant Planet Variability Team, Spitzer Ice Giant Variability Team</p> <p>2016-10-01</p> <p>Over the past several years a number of of high cadence photometric <span class="hlt">observations</span> of solar system giant planets have been acquired by various platforms. Such <span class="hlt">observations</span> are of interest as they provide points of comparison to the already expansive set of brown dwarf <span class="hlt">variability</span> <span class="hlt">observations</span> and the small, but growing, set of exoplanet <span class="hlt">variability</span> <span class="hlt">observations</span>. By measuring how rapidly the integrated light from solar system giant planets can evolve, <span class="hlt">variability</span> <span class="hlt">observations</span> of substellar objects that are unlikely to ever be resolved can be placed in a fuller context. Examples of brown dwarf <span class="hlt">variability</span> <span class="hlt">observations</span> include extensive work from the ground (e.g., Radigan et al. 2014), Spitzer (e.g., Metchev et al. 2015), Kepler (Gizis et al. 2015), and HST (Yang et al. 2015). <span class="hlt">Variability</span> has been measured on the planetary mass companion to the brown dwarf 2MASS 1207b (Zhou et al. 2016) and further searches are planned in thermal emission for the known directly imaged planets with ground based telescopes (Apai et al. 2016) and in reflected light with future space based telescopes. Recent solar system <span class="hlt">variability</span> <span class="hlt">observations</span> include Kepler monitoring of Neptune (Simon et al. 2016) and Uranus, Spitzer <span class="hlt">observations</span> of Neptune (Stauffer et al. 2016), and Cassini <span class="hlt">observations</span> of Jupiter (West et al. in prep). The Cassini <span class="hlt">observations</span> are of particular interest as they measured the <span class="hlt">variability</span> of Jupiter at a phase angle of ˜60○, comparable to the viewing geometry expected for space based direct imaging of cool extrasolar Jupiters in reflected light. These solar system analog <span class="hlt">observations</span> capture many of the characteristics seen in brown dwarf <span class="hlt">variability</span>, including large amplitudes and rapid light curve evolution on timescales as short as a few rotation periods. Simon et al. (2016) attribute such variations at Neptune to a combination of large scale, stable cloud structures along with smaller, more rapidly varying, cloud patches. The <span class="hlt">observed</span> brown dwarf and exoplanet</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160012390','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160012390"><span>Recent <span class="hlt">Variability</span> <span class="hlt">Observations</span> of Solar System Giant Planets: Fresh Context for Understanding Exoplanet and Brown Dwarf Weather</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Marley, Mark Scott</p> <p>2016-01-01</p> <p>Over the past several years a number of high cadence photometric <span class="hlt">observations</span> of solar system giant planets have been acquired by various platforms. Such <span class="hlt">observations</span> are of interest as they provide points of comparison to the already expansive set of brown dwarf <span class="hlt">variability</span> <span class="hlt">observations</span> and the small, but growing, set of exoplanet <span class="hlt">variability</span> <span class="hlt">observations</span>. By measuring how rapidly the integrated light from solar system giant planets can evolve, <span class="hlt">variability</span> <span class="hlt">observations</span> of substellar objects that are unlikely to ever be resolved can be placed in a fuller context. Examples of brown dwarf <span class="hlt">variability</span> <span class="hlt">observations</span> include extensive work from the ground (e.g., Radigen et al. 2014), Spitzer (e.g., Metchev et al. 2015), Kepler (Gizis et al. 2015), and HST (Yang et al. 2015).<span class="hlt">Variability</span> has been measured on the planetary mass companion to the brown dwarf 2MASS 1207b (Zhou et al. 2016) and further searches are planned in thermal emission for the known directly imaged planets with ground based telescopes (Apai et al. 2016) and in reflected light with future space based telescopes. Recent solar system <span class="hlt">variability</span> <span class="hlt">observations</span> include Kepler monitoring of Neptune (Simon et al. 2016) and Uranus, Spitzer <span class="hlt">observations</span> of Neptune (Stauffer et al. 2016), and Cassini <span class="hlt">observations</span> of Jupiter (West et al. in prep). The Cassini <span class="hlt">observations</span> are of particular interest as they measured the <span class="hlt">variability</span> of Jupiter at a phase angle of approximately 60 deg, comparable to the viewing geometry expected for space based direct imaging of cool extrasolar Jupiters in reflected light. These solar system analog <span class="hlt">observations</span> capture many of the characteristics seen in brown dwarf <span class="hlt">variability</span>, including large amplitudes and rapid light curve evolution on timescales as short as a few rotation periods. Simon et al. (2016) attribute such variations at Neptune to a combination of large scale, stable cloud structures along with smaller, more rapidly varying, cloud patches. The <span class="hlt">observed</span> brown dwarf and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.7753D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.7753D"><span>Sub-Seasonal <span class="hlt">Variability</span> of Tropical Rainfall <span class="hlt">Observed</span> by TRMM and Ground-based Polarimetric Radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dolan, Brenda; Rutledge, Steven; Lang, Timothy; Cifelli, Robert; Nesbitt, Stephen</p> <p>2010-05-01</p> <p>Studies of tropical precipitation characteristics from the TRMM-LBA and NAME field campaigns using ground-based polarimetric S-band data have revealed significant differences in microphysical processes occurring in the various meteorological regimes sampled in those projects. In TRMM-LMA (January-February 1999 in Brazil; a TRMM ground validation experiment), <span class="hlt">variability</span> is driven by prevailing low-level winds. During periods of low-level easterlies, deeper and more intense convection is <span class="hlt">observed</span>, while during periods of low-level westerlies, weaker convection embedded in widespread stratiform precipitation is common. In the NAME region (North American Monsoon Experiment, summer 2004 along the west coast of Mexico), strong terrain <span class="hlt">variability</span> drives differences in precipitation, with larger drops and larger ice mass aloft associated with convection occurring over the coastal plain compared to convection over the higher terrain of the Sierra Madre Occidental, or adjacent coastal waters. Comparisons with the TRMM precipitation radar (PR) indicate that such sub-seasonal <span class="hlt">variability</span> in these two regions are not well characterized by the TRMM PR reflectivity and rainfall statistics. TRMM PR reflectivity profiles in the LBA region are somewhat lower than S-Pol values, particularly in the more intense easterly regime convection. In NAME, mean reflectivities are even more divergent, with TRMM profiles below those of S-Pol. In both regions, the TRMM PR does not capture rain rates above 80 mm hr-1 despite much higher rain rates estimated from the S-Pol polarimetric data, and rain rates are generally lower for a given reflectivity from TRMM PR compared to S-Pol. These differences between TRMM PR and S-Pol may arise from the inability of Z-R relationships to capture the full <span class="hlt">variability</span> of microphysical conditions or may highlight problems with TRMM retrievals over land. In addition to the TRMM-LBA and NAME regions, analysis of sub-seasonal precipitation <span class="hlt">variability</span> and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20640691-all-quantum-observables-hidden-variable-model-must-commute-simultaneously','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20640691-all-quantum-observables-hidden-variable-model-must-commute-simultaneously"><span>All quantum <span class="hlt">observables</span> in a hidden-<span class="hlt">variable</span> model must commute simultaneously</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Malley, James D.</p> <p></p> <p>Under a standard set of assumptions for a hidden-<span class="hlt">variable</span> model for quantum events we show that all <span class="hlt">observables</span> must commute simultaneously. This seems to be an ultimate statement about the inapplicability of the usual hidden-<span class="hlt">variable</span> model for quantum events. And, despite Bell's complaint that a key condition of von Neumann's was quite unrealistic, we show that these conditions, under which von Neumann produced the first no-go proof, are entirely equivalent to those introduced by Bell and Kochen and Specker. As these conditions are also equivalent to those under which the Bell-Clauster-Horne inequalities are derived, we see that the experimental violationsmore » of the inequalities demonstrate only that quantum <span class="hlt">observables</span> do not commute.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GPC...112...33C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GPC...112...33C"><span>Inter-<span class="hlt">decadal</span> modulation of ENSO teleconnections to the Indian Ocean in a coupled model: Special emphasis on decay phase of El Niño</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chowdary, J. S.; Parekh, Anant; Gnanaseelan, C.; Sreenivas, P.</p> <p>2014-01-01</p> <p>Inter-<span class="hlt">decadal</span> modulation of El Niño-Southern Oscillation (ENSO) teleconnections to tropical Indian Ocean (TIO) is investigated in the coupled general circulation model Climate Forecast System (CFS) using a hundred year integration. The model is able to capture the periodicity of El Niño <span class="hlt">variability</span>, which is similar to that of the <span class="hlt">observations</span>. The maximum TIO/north Indian Ocean (NIO) SST warming (during spring following the decay phase of El Niño) associated with El Niño is well captured by the model. Detailed analysis reveals that the surface heat flux variations mainly contribute to the El Niño forced TIO SST variations both in <span class="hlt">observations</span> and model. However, spring warming is nearly stationary throughout the model integration period, indicating poor inter-<span class="hlt">decadal</span> El Niño teleconnections. The <span class="hlt">observations</span> on the other hand displayed maximum SST warming with strong seasonality from epoch to epoch. The model El Niño decay delayed by more than two seasons, results in persistent TIO/NIO SST warming through the following December unlike in the <span class="hlt">observations</span>. The ocean wave adjustments and persistent westerly wind anomalies over the equatorial Pacific are responsible for late decay of El Niño in the model. Consistent late decay of El Niño, throughout the model integration period (low variance), is mainly responsible for the poor inter-<span class="hlt">decadal</span> ENSO teleconnections to TIO/NIO. This study deciphers that the model needs to produce El Niño decay phase <span class="hlt">variability</span> correctly to obtain <span class="hlt">decadal</span>-modulations in ENSO teleconnection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31C0924M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31C0924M"><span>Temporal <span class="hlt">variability</span> of the Antarctic Ice sheet <span class="hlt">observed</span> from space-based geodesy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Memin, A.; King, M. A.; Boy, J. P.; Remy, F.</p> <p>2017-12-01</p> <p>Quantifying the Antarctic Ice Sheet (AIS) mass balance still remains challenging as several processes compete to differing degrees at the basin scale with regional variations, leading to multiple mass redistribution patterns. For instance, analysis of linear trends in surface-height variations from 1992-2003 and 2002-2006 shows that the AIS is subject to decimetric scale <span class="hlt">variability</span> over periods of a few years. Every year, snowfalls in Antarctica represent the equivalent of 6 mm of the mean sea level. Therefore, any fluctuation in precipitation can lead to changes in sea level. Besides, over the last <span class="hlt">decade</span>, several major glaciers have been thinning at an accelerating rate. Understanding the processes that interact on the ice sheet is therefore important to precisely determine the response of the ice sheet to a rapid changing climate and estimate its contribution to sea level changes. We estimate seasonal and interannual changes of the AIS between January 2003 and October 2010 and to the end of 2016 from a combined analysis of surface-elevation and surface-mass changes derived from Envisat data and GRACE solutions, and from GRACE solutions only, respectively. While we obtain a good correlation for the interannual signal between the two techniques, important differences (in amplitude, phase, and spatial pattern) are obtained for the seasonal signal. We investigate these discrepancies by comparing the crustal motion <span class="hlt">observed</span> by GPS and those predicted using monthly surface mass balance derived from the regional atmospheric climate model RACMO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSA32A..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSA32A..02S"><span>Longitudinal Ionospheric <span class="hlt">Variability</span> <span class="hlt">Observed</span> by LITES on the ISS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stephan, A. W.; Finn, S. C.; Cook, T.; Geddes, G.; Chakrabarti, S.; Budzien, S. A.</p> <p>2017-12-01</p> <p>The Limb-Imaging Ionospheric and Thermospheric Extreme-Ultraviolet Spectrograph (LITES) is an imaging spectrograph designed to measure altitude profiles (150-350 km) of extreme- and far-ultraviolet airglow emissions that originate from photochemical processes in the ionosphere and thermosphere. During the daytime, LITES <span class="hlt">observes</span> the bright O+ 83.4 nm emission from which the ionospheric profile can be inferred. At night, recombination emissions at 91.1 and 135.6 nm provide a direct measure of the electron content along the line of sight. LITES was launched and installed on the International Space Station (ISS) in late February 2017 where it has been operating along with the highly complementary GPS Radio Occultation and Ultraviolet Photometry - Colocated (GROUP-C) experiment. We will present some of the first <span class="hlt">observations</span> from LITES in April 2017 that show longitudinal patterns in ionospheric density and the daily <span class="hlt">variability</span> in those patterns. LITES vertical imaging from a vantage point near 410 km enables a particularly unique perspective on the altitude of the ionospheric peak density at night that can complement and inform other ground- and space-based measurements, and track the longitude-altitude <span class="hlt">variability</span> that is reflective of changes in equatorial electrodynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EOSTr..95..196L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EOSTr..95..196L"><span>Tropical Pacific <span class="hlt">Observing</span> for the Next <span class="hlt">Decade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Legler, David M.; Hill, Katherine</p> <p>2014-06-01</p> <p>More than 60 scientists and program officials from 13 countries met at the Scripps Institution of Oceanography for the Tropical Pacific <span class="hlt">Observing</span> System (TPOS) 2020 Workshop. The workshop, although motivated in part by the dramatic decline of NOAA's Tropical Atmosphere Ocean (TAO) buoy reporting from mid-2012 to early 2014 (see http://www.bloomberg.com/news/2014-03-07/aging-el-nino-buoys-getting-fixed-as-weather-forecasts-at-risk.html), evaluated the needs for tropical Pacific <span class="hlt">observing</span> and initiated efforts to develop a more resilient and integrative <span class="hlt">observing</span> system for the future.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014DSRII.103..264A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014DSRII.103..264A"><span>Understanding interannual, <span class="hlt">decadal</span> level <span class="hlt">variability</span> in paralytic shellfish poisoning toxicity in the Gulf of Maine: The HAB Index</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anderson, Donald M.; Couture, Darcie A.; Kleindinst, Judith L.; Keafer, Bruce A.; McGillicuddy, Dennis J., Jr.; Martin, Jennifer L.; Richlen, Mindy L.; Hickey, J. Michael; Solow, Andrew R.</p> <p>2014-05-01</p> <p>A major goal in harmful algal bloom (HAB) research has been to identify mechanisms underlying interannual <span class="hlt">variability</span> in bloom magnitude and impact. Here the focus is on <span class="hlt">variability</span> in Alexandrium fundyense blooms and paralytic shellfish poisoning (PSP) toxicity in Maine, USA, over 34 years (1978-2011). The Maine coastline was divided into two regions - eastern and western Maine, and within those two regions, three measures of PSP toxicity (the percent of stations showing detectable toxicity over the year, the cumulative amount of toxicity per station measured in all shellfish (mussel) samples during that year, and the duration of measurable toxicity) were examined for each year in the time series. These metrics were combined into a simple HAB Index that provides a single measure of annual toxin severity across each region. The three toxin metrics, as well as the HAB Index that integrates them, reveal significant <span class="hlt">variability</span> in overall toxicity between individual years as well as long-term, <span class="hlt">decadal</span> patterns or regimes. Based on different conceptual models of the system, we considered three trend formulations to characterize the long-term patterns in the Index - a three-phase (mean-shift) model, a linear two-phase model, and a pulse-decline model. The first represents a “regime shift” or multiple equilibria formulation as might occur with alternating periods of sustained high and low cyst abundance or favorable and unfavorable growth conditions, the second depicts a scenario of more gradual transitions in cyst abundance or growth conditions of vegetative cells, and the third characterizes a ”sawtooth” pattern in which upward shifts in toxicity are associated with major cyst recruitment events, followed by a gradual but continuous decline until the next pulse. The fitted models were compared using both residual sum of squares and Akaike's Information Criterion. There were some differences between model fits, but none consistently gave a better fit than the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4058790','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4058790"><span>Understanding interannual, <span class="hlt">decadal</span> level <span class="hlt">variability</span> in paralytic shellfish poisoning toxicity in the Gulf of Maine: the HAB Index</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Anderson, Donald M.; Couture, Darcie A.; Kleindinst, Judith L.; Keafer, Bruce A.; McGillicuddy, Dennis J.; Martin, Jennifer L.; Richlen, Mindy L.; Hickey, J. Michael; Solow, Andrew R.</p> <p>2013-01-01</p> <p>A major goal in harmful algal bloom (HAB) research has been to identify mechanisms underlying interannual <span class="hlt">variability</span> in bloom magnitude and impact. Here the focus is on <span class="hlt">variability</span> in Alexandrium fundyense blooms and paralytic shellfish poisoning (PSP) toxicity in Maine, USA, over 34 years (1978 – 2011). The Maine coastline was divided into two regions -eastern and western Maine, and within those two regions, three measures of PSP toxicity (the percent of stations showing detectable toxicity over the year, the cumulative amount of toxicity per station measured in all shellfish (mussel) samples during that year, and the duration of measurable toxicity) were examined for each year in the time series. These metrics were combined into a simple HAB Index that provides a single measure of annual toxin severity across each region. The three toxin metrics, as well as the HAB Index that integrates them, reveal significant <span class="hlt">variability</span> in overall toxicity between individual years as well as long-term, <span class="hlt">decadal</span> patterns or regimes. Based on different conceptual models of the system, we considered three trend formulations to characterize the long-term patterns in the Index – a three-phase (mean-shift) model, a linear two-phase model, and a pulse-decline model. The first represents a “regime shift” or multiple equilibria formulation as might occur with alternating periods of sustained high and low cyst abundance or favorable and unfavorable growth conditions, the second depicts a scenario of more gradual transitions in cyst abundance or growth conditions of vegetative cells, and the third characterizes a ”sawtooth” pattern in which upward shifts in toxicity are associated with major cyst recruitment events, followed by a gradual but continuous decline until the next pulse. The fitted models were compared using both residual sum of squares and Akaike's Information Criterion. There were some differences between model fits, but none consistently gave a better fit than</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016RvGeo..54....5B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016RvGeo..54....5B"><span><span class="hlt">Observations</span>, inferences, and mechanisms of the Atlantic Meridional Overturning Circulation: A review</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buckley, Martha W.; Marshall, John</p> <p>2016-03-01</p> <p>This is a review about the Atlantic Meridional Overturning Circulation (AMOC), its mean structure, temporal <span class="hlt">variability</span>, controlling mechanisms, and role in the coupled climate system. The AMOC plays a central role in climate through its heat and freshwater transports. Northward ocean heat transport achieved by the AMOC is responsible for the relative warmth of the Northern Hemisphere compared to the Southern Hemisphere and is thought to play a role in setting the mean position of the Intertropical Convergence Zone north of the equator. The AMOC is a key means by which heat anomalies are sequestered into the ocean's interior and thus modulates the trajectory of climate change. Fluctuations in the AMOC have been linked to low-frequency <span class="hlt">variability</span> of Atlantic sea surface temperatures with a host of implications for climate <span class="hlt">variability</span> over surrounding landmasses. On intra-annual timescales, <span class="hlt">variability</span> in AMOC is large and primarily reflects the response to local wind forcing; meridional coherence of anomalies is limited to that of the wind field. On interannual to <span class="hlt">decadal</span> timescales, AMOC changes are primarily geostrophic and related to buoyancy anomalies on the western boundary. A pacemaker region for <span class="hlt">decadal</span> AMOC changes is located in a western "transition zone" along the boundary between the subtropical and subpolar gyres. <span class="hlt">Decadal</span> AMOC anomalies are communicated meridionally from this region. AMOC <span class="hlt">observations</span>, as well as the expanded ocean <span class="hlt">observational</span> network provided by the Argo array and satellite altimetry, are inspiring efforts to develop <span class="hlt">decadal</span> predictability systems using coupled atmosphere-ocean models initialized by ocean data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013019','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013019"><span>North Pacific <span class="hlt">Decadal</span> <span class="hlt">Variability</span> in the GEOS-5 Atmosphere-Ocean Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Achuthavarier, Deepthi; Schubert, Siegfried D.; Vikhliaev, Yury V.</p> <p>2013-01-01</p> <p>This study examines the mechanisms of the Pacific <span class="hlt">decadal</span> oscillation (PDO) in the GEOS-5 general circulation model. The model simulates a realistic PDO pattern that is resolved as the first empirical orthogonal function (EOF) of winter sea surface temperature (SST). The simulated PDO is primarily forced by Aleutian low through Ekman transport and surface fluxes, and shows a red spectrum without any preferred periodicity. This differs from the <span class="hlt">observations</span>, which indicate a greater role of El Nino-Southern Oscillation (ENSO) forcing, and likely reflects the too short time scale of the simulated ENSO. The geostrophic transport in response to the Aleutian low is limited to the Kuroshio-Oyashio Extension, and is unlikely the main controlling factor in this model, although it reinforces the Ekman-induced SST anomalies. The delay between the Aleutian low and the PDO is relatively short (1 year) suggesting that the fast Ekman response (rather than Rossby wave propagation) sets the SST pattern immediately following an Aleutian low fluctuation. The atmospheric feedback (response to the SST) is only about 25 of the forcing and never evolves into an Aleutian low completely, instead projecting onto the North Pacific Oscillation (NPO), a meridional dipole in sea level pressure (SLP). The lack of preferred periodicity and weak atmospheric response bothindicate a coupled oscillation is an unlikely mechanism for the PDO in this model. In agreement with recent studies, the NPO is correlated with the North Pacific Gyre Oscillation (NPGO), which is another leading EOF of the North Pacific SST. A possible connection between the PDO and the NPGO is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998ClDy...14..117M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998ClDy...14..117M"><span><span class="hlt">Decadal</span> time scale <span class="hlt">variability</span> recorded in the Quelccaya summit ice core δ18O isotopic ratio series and its relation with the sea surface temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mélice, J. L.; Roucou, P.</p> <p></p> <p> Quelccaya summit with its tropical North Atlantic isotopic signature. It is also suggested from this described stability of the <span class="hlt">decadal</span> time scale <span class="hlt">variability</span> <span class="hlt">observed</span> in the Quelccaya isotopic series, that the <span class="hlt">decadal</span> time scale GSST <span class="hlt">variability</span> was also stable during the last five centuries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19255371','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19255371"><span><span class="hlt">Variability</span> of attention processes in ADHD: <span class="hlt">observations</span> from the classroom.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rapport, Mark D; Kofler, Michael J; Alderson, R Matt; Timko, Thomas M; Dupaul, George J</p> <p>2009-05-01</p> <p>Classroom- and laboratory-based efforts to study the attentional problems of children with ADHD are incongruent in elucidating attentional deficits; however, none have explored within- or between-minute <span class="hlt">variability</span> in the classroom attentional processing in children with ADHD. High and low attention groups of ADHD children defined via cluster analysis, and 36 typically developing children, were <span class="hlt">observed</span> while completing academic assignments in their general education classrooms. All children oscillated between attentive and inattentive states; however, children in both ADHD groups switched states more frequently and remained attentive for shorter durations relative to typically developing children. Overall differences in attention and optimal ability to maintain attention among the groups are consistent with laboratory studies of increased ADHD-related interindividual and intergroup <span class="hlt">variability</span> but inconsistent with laboratory results of increased intra-individual <span class="hlt">variability</span> and attention decrements over time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110023540','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110023540"><span>Interannual to <span class="hlt">Decadal</span> <span class="hlt">Variability</span> of Atlantic Water in the Nordic and Adjacent Seas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carton, James A.; Chepurin, Gennady A.; Reagan, James; Haekkinen, Sirpa</p> <p>2011-01-01</p> <p>Warm salty Atlantic Water is the main source water for the Arctic Ocean and thus plays an important role in the mass and heat budget of the Arctic. This study explores interannual to <span class="hlt">decadal</span> <span class="hlt">variability</span> of Atlantic Water properties in the Nordic Seas area where Atlantic Water enters the Arctic, based on a reexamination of the historical hydrographic record for the years 1950-2009, obtained by combining multiple data sets. The analysis shows a succession of four multi-year warm events where temperature anomalies at 100m depth exceed 0.4oC, and three cold events. Three of the four warm events lasted 3-4 years, while the fourth began in 1999 and persists at least through 2009. This most recent warm event is anomalous in other ways as well, being the strongest, having the broadest geographic extent, being surface-intensified, and occurring under exceptional meteorological conditions. Three of the four warm events were accompanied by elevated salinities consistent with enhanced ocean transport into the Nordic Seas, with the exception of the event spanning July 1989-July 1993. Of the three cold events, two lasted for four years, while the third lasted for nearly 14 years. Two of the three cold events are associated with reduced salinities, but the cold event of the 1960s had elevated salinities. The relationship of these events to meteorological conditions is examined. The results show that local surface heat flux variations act in some cases to reinforce the anomalies, but are too weak to be the sole cause.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=335747','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=335747"><span>Dynamic Evaluation of Two <span class="hlt">Decades</span> of CMAQ Simulations ...</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>This presentation focuses on the dynamic evaluation of the CMAQ model over the continental United States using multi-<span class="hlt">decadal</span> simulations for the period from 1990 to 2010 to examine how well the changes in <span class="hlt">observed</span> ozone air quality induced by variations in meteorology and/or emissions are simulated by the model. We applied spectral decomposition of the ozone time-series using the KZ filter to assess the variations in the strengths of synoptic (weather-induced variations) and baseline (long-term variation) forcings, embedded in the simulated and <span class="hlt">observed</span> concentrations. The results reveal that CMAQ captured the year-to-year <span class="hlt">variability</span> (more so in the later years than the earlier years) and the synoptic forcing in accordance with what the <span class="hlt">observations</span> are showing. The National Exposure Research Laboratory (NERL) Computational Exposure Division (CED) develops and evaluates data, decision-support tools, and models to be applied to media-specific or receptor-specific problem areas. CED uses modeling-based approaches to characterize exposures, evaluate fate and transport, and support environmental diagnostics/forensics with input from multiple data sources. It also develops media- and receptor-specific models, process models, and decision support tools for use both within and outside of EPA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC13B0633G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC13B0633G"><span>Water Stress on U.S. Power Production at <span class="hlt">Decadal</span> Time Horizons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ganguli, P.; Kumar, D.; Yun, J.; Short, G.; Klausner, J.; Ganguly, A. R.</p> <p>2014-12-01</p> <p>Thermoelectric power production at risk, owing to current and projected water scarcity and rising stream temperatures, is assessed for the continental United States (US) at <span class="hlt">decadal</span> scales. Regional water scarcity is driven by climate <span class="hlt">variability</span> and change, as well as by multi-sector water demand. While a planning horizon of zero to about thirty years is occasionally prescribed by stakeholders, the challenges to risk assessment at these scales include the difficulty in delineating <span class="hlt">decadal</span> climate trends from intrinsic natural or multiple model <span class="hlt">variability</span>. Current generation global climate or earth system models are not credible at the spatial resolutions of power plants, especially for surface water quantity and stream temperatures, which further exacerbates the assessment challenge. Population changes, which are anyway difficult to project, cannot serve as adequate proxies for changes in the water demand across sectors. The hypothesis that robust assessments of power production at risks are possible, despite the uncertainties, has been examined as a proof of concept. An approach is presented for delineating water scarcity and temperature from climate models, <span class="hlt">observations</span> and population storylines, as well as for assessing power production at risk by examining geospatial correlations of power plant locations within regions where the usable water supply for energy production happens to be scarcer and warmer. Acknowledgment: Funding provided by US DOE's ARPA-E through Award DE-AR0000374.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110015263','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110015263"><span>Sea Surface Salinity <span class="hlt">Variability</span> from Simulations and <span class="hlt">Observations</span>: Preparing for Aquarius</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jacob, S. Daniel; LeVine, David M.</p> <p>2010-01-01</p> <p>Oceanic fresh water transport has been shown to play an important role in the global hydrological cycle. Sea surface salinity (SSS) is representative of the surface fresh water fluxes and the upcoming Aquarius mission scheduled to be launched in December 2010 will provide excellent spatial and temporal SSS coverage to better estimate the net exchange. In most ocean general circulation models, SSS is relaxed to climatology to prevent model drift. While SST remains a well <span class="hlt">observed</span> <span class="hlt">variable</span>, relaxing to SST reduces the range of SSS <span class="hlt">variability</span> in the simulations (Fig.1). The main objective of the present study is to simulate surface tracers using a primitive equation ocean model for multiple forcing data sets to identify and establish a baseline SSS <span class="hlt">variability</span>. The simulated <span class="hlt">variability</span> scales are compared to those from near-surface argo salinity measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://elibrary.unm.edu/sora/JFO/v053n02/p0159-p0167.pdf','USGSPUBS'); return false;" href="http://elibrary.unm.edu/sora/JFO/v053n02/p0159-p0167.pdf"><span><span class="hlt">Observer</span> <span class="hlt">variability</span> in estimating numbers: An experiment</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Erwin, R.M.</p> <p>1982-01-01</p> <p>Census estimates of bird populations provide an essential framework for a host of research and management questions. However, with some exceptions, the reliability of numerical estimates and the factors influencing them have received insufficient attention. Independent of the problems associated with habitat type, weather conditions, cryptic coloration, ete., estimates may vary widely due only to intrinsic differences in <span class="hlt">observers</span>? abilities to estimate numbers. Lessons learned in the field of perceptual psychology may be usefully applied to 'real world' problems in field ornithology. Based largely on dot discrimination tests in the laboratory, it was found that numerical abundance, density of objects, spatial configuration, color, background, and other <span class="hlt">variables</span> influence individual accuracy in estimating numbers. The primary purpose of the present experiment was to assess the effects of <span class="hlt">observer</span>, prior experience, and numerical range on accuracy in estimating numbers of waterfowl from black-and-white photographs. By using photographs of animals rather than black dots, I felt the results could be applied more meaningfully to field situations. Further, reinforcement was provided throughout some experiments to examine the influence of training on accuracy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020080613','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020080613"><span>Subtropical Gyre <span class="hlt">Variability</span> <span class="hlt">Observed</span> by Ocean Color Satellites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McClain, Charles R.; Signorini, Sergio R.; Christian, James R.</p> <p>2002-01-01</p> <p>The subtropical gyres of the world are extensive, coherent regions that occupy about 40% of the surface of the earth. Once thought to be homogeneous and static habitats, there is increasing evidence that mid-latitude gyres exhibit substantial physical and biological <span class="hlt">variability</span> on a variety of time scales. While biological productivity within these oligotrophic regions may be relatively small, their immense size makes their total contribution significant. Global distributions of dynamic height derived from satellite altimeter data, and chlorophyll concentration derived from satellite ocean color data, show that the dynamic center of the gyres, the region of maximum dynamic height where the thermocline is deepest, does not coincide with the region of minimum chlorophyll concentration. The physical and biological processes by which this distribution of ocean properties is maintained, and the spatial and temporal scales of <span class="hlt">variability</span> associated with these processes, are analyzed using global surface chlorophyll-a concentrations, sea surface height, sea surface temperature and surface winds from operational satellite and meteorological sources, and hydrographic data from climatologies and individual surveys. Seasonal and interannual <span class="hlt">variability</span> in the areal extent of the subtropical gyres are examined using 8 months (November 1996 - June 1997) of OCTS and nearly 5 years (September 1997 - June 02) of SeaWiFS ocean color data and are interpreted in the context of climate <span class="hlt">variability</span> and measured changes in other ocean properties (i.e., wind forcing, surface currents, Ekman pumping, and vertical mixing). The North Pacific and North Atlantic gyres are <span class="hlt">observed</span> to be shrinking over this period, while the South Pacific, South Atlantic, and South Indian Ocean gyres appear to be expanding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C42A..06H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C42A..06H"><span>Effects of ice shelf basal melt <span class="hlt">variability</span> on evolution of Thwaites Glacier</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoffman, M. J.; Fyke, J. G.; Price, S. F.; Asay-Davis, X.; Perego, M.</p> <p>2017-12-01</p> <p>Theory, modeling, and <span class="hlt">observations</span> indicate that marine ice sheets on a retrograde bed, including Thwaites Glacier, Antarctica, are only conditionally stable. Previous modeling studies have shown that rapid, unstable retreat can occur when steady ice-shelf basal melting causes the grounding line to retreat past restraining bedrock bumps. Here we explore the initiation and evolution of unstable retreat of Thwaites Glacier when the ice-shelf basal melt forcing includes temporal <span class="hlt">variability</span> mimicking realistic climate <span class="hlt">variability</span>. We use the three-dimensional, higher-order Model for Prediction Across Scales-Land Ice (MPASLI) model forced with an ice shelf basal melt parameterization derived from previous coupled ice sheet/ocean simulations. We add sinusoidal temporal <span class="hlt">variability</span> to the melt parameterization that represents shoaling and deepening of Circumpolar Deep Water. We perform an ensemble of 250 year duration simulations with different values for the amplitude, period, and phase of the <span class="hlt">variability</span>. Preliminary results suggest that, overall, <span class="hlt">variability</span> leads to slower grounding line retreat and less mass loss than steady simulations. Short period (2 yr) <span class="hlt">variability</span> leads to similar results as steady forcing, whereas <span class="hlt">decadal</span> <span class="hlt">variability</span> can result in up to one-third less mass loss. Differences in phase lead to a large range in mass loss/grounding line retreat, but it is always less than the steady forcing. The timing of ungrounding from each restraining bedrock bump, which is strongly affected by the melt <span class="hlt">variability</span>, is the rate limiting factor, and <span class="hlt">variability</span>-driven delays in ungrounding at each bump accumulate. Grounding line retreat in the regions between bedrock bumps is relatively unaffected by ice shelf melt <span class="hlt">variability</span>. While the results are sensitive to the form of the melt parameterization and its <span class="hlt">variability</span>, we conclude that <span class="hlt">decadal</span> period ice shelf melt <span class="hlt">variability</span> could potentially delay marine ice sheet instability by up to many <span class="hlt">decades</span>. However</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031802','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031802"><span>High nutrient pulses, tidal mixing and biological response in a small California estuary: <span class="hlt">Variability</span> in nutrient concentrations from <span class="hlt">decadal</span> to hourly time scales</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Caffrey, J.M.; Chapin, T.P.; Jannasch, H.W.; Haskins, J.C.</p> <p>2007-01-01</p> <p>Elkhorn Slough is a small estuary in Central California, where nutrient inputs are dominated by runoff from agricultural row crops, a golf course, and residential development. We examined the <span class="hlt">variability</span> in nutrient concentrations from <span class="hlt">decadal</span> to hourly time scales in Elkhorn Slough to compare forcing by physical and biological factors. Hourly data were collected using in situ nitrate analyzers and water quality data sondes, and two <span class="hlt">decades</span> of monthly monitoring data were analyzed. Nutrient concentrations increased from the mid 1970s to 1990s as pastures and woodlands were converted to row crops and population increased in the watershed. Climatic <span class="hlt">variability</span> was also a significant factor controlling interannual nutrient <span class="hlt">variability</span>, with higher nutrient concentrations during wet than drought years. Elkhorn Slough has a Mediterranean climate with dry and rainy seasons. Dissolved inorganic nitrogen (DIN) concentrations were relatively low (10-70 ??mol L-1) during the dry season and high (20-160 ??mol L-1) during the rainy season. Dissolved inorganic phosphorus (DIP) concentrations showed the inverse pattern, with higher concentrations during the dry season. Pulsed runoff events were a consistent feature controlling nitrate concentrations during the rainy season. Peak nitrate concentrations lagged runoff events by 1 to 6 days. Tidal exchange with Monterey Bay was also an important process controlling nutrient concentrations, particularly near the mouth of the Slough. Biological processes had the greatest effect on nitrate concentrations during the dry season and were less important during the rainy season. While primary production was enhanced by nutrient pulses, chlorophyll a concentrations were not. We believe that the generally weak biological response compared to the strong physical forcing in Elkhorn Slough occurred because the short residence time and tidal mixing rapidly diluted nutrient pulses. ?? 2006 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060012295','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060012295"><span>A Model Assessment of Satellite <span class="hlt">Observed</span> Trends in Polar Sea Ice Extents</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vinnikov, Konstantin Y.; Cavalieri, Donald J.; Parkinson, Claire L.</p> <p>2005-01-01</p> <p>For more than three <span class="hlt">decades</span> now, satellite passive microwave <span class="hlt">observations</span> have been used to monitor polar sea ice. Here we utilize sea ice extent trends determined from primarily satellite data for both the Northern and Southern Hemispheres for the period 1972(73)-2004 and compare them with results from simulations by eleven climate models. In the Northern Hemisphere, <span class="hlt">observations</span> show a statistically significant decrease of sea ice extent and an acceleration of sea ice retreat during the past three <span class="hlt">decades</span>. However, from the modeled natural <span class="hlt">variability</span> of sea ice extents in control simulations, we conclude that the acceleration is not statistically significant and should not be extrapolated into the future. <span class="hlt">Observations</span> and model simulations show that the time scale of climate <span class="hlt">variability</span> in sea ice extent in the Southern Hemisphere is much larger than in the Northern Hemisphere and that the Southern Hemisphere sea ice extent trends are not statistically significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.212.1218C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.212.1218C"><span><span class="hlt">Decadal</span> variation in Earth's oblateness (J2) from satellite laser ranging data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheng, Minkang; Ries, John C.</p> <p>2018-02-01</p> <p>For four <span class="hlt">decades</span>, satellite laser ranging has recorded the global nature of the long-wavelength hydrological mass redistribution within the Earth system, which results in significant variations in the Earth's dynamical oblateness, characterized by the second degree zonal geopotential spherical harmonic J2 (or C20). Analysis of the J2 time-series has shown a significant variation related to the strong El Niño-Southern Oscillation events with periods of 2-6 yr. In particular, the variation related to the powerful 2015-2016 El Niño that peaked during 2015 November-December was one of the strongest on record, comparable with the 1982-1983 and 1997-1998 events. In this study, we investigate further the hydrological mass transfer between atmosphere-ocean-land and their signature in the <span class="hlt">decadal</span> variations of J2 with timescales of ˜10 yr. We found that the ˜6.4-yr variations can be accounted for by the atmosphere and ocean mass variations based on the improved Atmosphere-Ocean De-aliasing data, and the <span class="hlt">observed</span> <span class="hlt">decadal</span> variation in J2 correlates well with the <span class="hlt">decadal</span> tropical <span class="hlt">variability</span> characterized by the 5-yr running mean of the El Niño-Southern Oscillation Index, although existing physical models, especially the land water storage, are limited for the purpose of further studies of the excitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19087944','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19087944"><span><span class="hlt">Decadal</span> climate prediction (project GCEP).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Haines, Keith; Hermanson, Leon; Liu, Chunlei; Putt, Debbie; Sutton, Rowan; Iwi, Alan; Smith, Doug</p> <p>2009-03-13</p> <p><span class="hlt">Decadal</span> prediction uses climate models forced by changing greenhouse gases, as in the International Panel for Climate Change, but unlike longer range predictions they also require initialization with <span class="hlt">observations</span> of the current climate. In particular, the upper-ocean heat content and circulation have a critical influence. <span class="hlt">Decadal</span> prediction is still in its infancy and there is an urgent need to understand the important processes that determine predictability on these timescales. We have taken the first Hadley Centre <span class="hlt">Decadal</span> Prediction System (DePreSys) and implemented it on several NERC institute compute clusters in order to study a wider range of initial condition impacts on <span class="hlt">decadal</span> forecasting, eventually including the state of the land and cryosphere. The eScience methods are used to manage submission and output from the many ensemble model runs required to assess predictive skill. Early results suggest initial condition skill may extend for several years, even over land areas, but this depends sensitively on the definition used to measure skill, and alternatives are presented. The Grid for Coupled Ensemble Prediction (GCEP) system will allow the UK academic community to contribute to international experiments being planned to explore <span class="hlt">decadal</span> climate predictability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OEJV..187....4B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OEJV..187....4B"><span>The <span class="hlt">variables</span> V477 Peg and MW Com <span class="hlt">observation</span> results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bahý, V.; Gajtanska, M.; Hanisko, P.; Krišták, L.</p> <p>2018-04-01</p> <p>The paper deals with our results of the photometric <span class="hlt">observations</span> of two <span class="hlt">variable</span> stars and with basic interprettions of our results. We have <span class="hlt">observed</span> the V477 Pegassi and MW Comae systems. We have obtained their light curves in the integral light and in the B, V, R and I filters. The color indices have been computed and there have been realized the models of the both systems by the usage of the BM3 software. These models are presented in our study too.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160001394','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160001394"><span>The Seyfert 2 Galaxy NGC 2110: Hard X-Ray Emission <span class="hlt">Observed</span> by NuStar and <span class="hlt">Variability</span> of the Iron K-Alpha Line</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Marinucci, A.; Matt, G.; Bianchi, S.; Lu, T. N.; Arevalo, P.; Balokovic, M.; Ballantyne, D.; Bauer, F. E.; Boggs, S. E.; Stern, D.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160001394'); toggleEditAbsImage('author_20160001394_show'); toggleEditAbsImage('author_20160001394_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160001394_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160001394_hide"></p> <p>2014-01-01</p> <p>We present NuSTAR <span class="hlt">observations</span> of the bright Seyfert 2 galaxy NGC 2110 obtained in 2012, when the source was at the highest flux level ever <span class="hlt">observed</span>, and in 2013, when the source was at a more typical flux level. We include archival <span class="hlt">observations</span> from other X-ray satellites, namely XMM-Newton, Suzaku, BeppoSAX, Chandra and Swift. Simultaneous NuSTAR and Swift broad band spectra (in the 3-80 keV range) indicate a cutoff energy E(sub c) greater than 210 keV, with no detectable contribution from Compton reflection. NGC 2110 is one of the very few sources where no evidence for distant Compton thick scattering is found and, by using temporal information collected over more than a <span class="hlt">decade</span>, we investigate variations of the iron K(alpha) line on time scales of years. The Fe K alpha line is likely the sum of two components: one constant (originating from distant Compton-thick material) and the other one <span class="hlt">variable</span> and linearly correlated with the source flux (possibly arising from Compton-thin material much closer to the black hole).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24078353','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24078353"><span>Influence and predictive capacity of climate anomalies on daily to <span class="hlt">decadal</span> extremes in canopy photosynthesis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Desai, Ankur R</p> <p>2014-02-01</p> <p>Significant advances have been made over the past <span class="hlt">decades</span> in capabilities to simulate diurnal and seasonal variation of leaf-level and canopy-scale photosynthesis in temperate and boreal forests. However, long-term prediction of future forest productivity in a changing climate may be more dependent on how climate and biological anomalies influence extremes in interannual to <span class="hlt">decadal</span> <span class="hlt">variability</span> of canopy ecosystem carbon exchanges. These exchanges can differ markedly from leaf level responses, especially owing to the prevalence of long lags in nutrient and water cycling. Until recently, multiple long-term (10+ year) high temporal frequency (daily) <span class="hlt">observations</span> of canopy exchange were not available to reliably assess this claim. An analysis of one of the longest running North American eddy covariance flux towers reveals that single climate <span class="hlt">variables</span> do not adequately explain carbon exchange anomalies beyond the seasonal timescale. Daily to weekly lagged anomalies of photosynthesis positively autocorrelate with daily photosynthesis. This effect suggests a negative feedback in photosynthetic response to climate extremes, such as anomalies in evapotranspiration and maximum temperature. Moisture stress in the prior season did inhibit photosynthesis, but mechanisms are difficult to assess. A complex interplay of integrated and lagged productivity and moisture-limiting factors indicate a critical role of seasonal thresholds that limit growing season length and peak productivity. These results lead toward a new conceptual framework for improving earth system models with long-term flux tower <span class="hlt">observations</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.3363D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.3363D"><span>Mechanisms of long-term mean sea level <span class="hlt">variability</span> in the North Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dangendorf, Sönke; Calafat, Francisco; Øie Nilsen, Jan Even; Richter, Kristin; Jensen, Jürgen</p> <p>2015-04-01</p> <p>We examine mean sea level (MSL) variations in the North Sea on timescales ranging from months to <span class="hlt">decades</span> under the consideration of different forcing factors since the late 19th century. We use multiple linear regression models, which are validated for the second half of the 20th century against the output of a state-of-the-art tide+surge model (HAMSOM), to determine the barotropic response of the ocean to fluctuations in atmospheric forcing. We demonstrate that local atmospheric forcing mainly triggers MSL <span class="hlt">variability</span> on timescales up to a few years, with the inverted barometric effect dominating the <span class="hlt">variability</span> along the UK and Norwegian coastlines and wind (piling up the water along the coast) controlling the MSL <span class="hlt">variability</span> in the south from Belgium up to Denmark. However, in addition to the large inter-annual sea level <span class="hlt">variability</span> there is also a considerable fraction of <span class="hlt">decadal</span> scale <span class="hlt">variability</span>. We show that on <span class="hlt">decadal</span> timescales MSL <span class="hlt">variability</span> in the North Sea mainly reflects steric changes, which are mostly remotely forced. A spatial correlation analysis of altimetry <span class="hlt">observations</span> and baroclinic ocean model outputs suggests evidence for a coherent signal extending from the Norwegian shelf down to the Canary Islands. This supports the theory of longshore wind forcing along the eastern boundary of the North Atlantic causing coastally trapped waves to propagate along the continental slope. With a combination of oceanographic and meteorological measurements we demonstrate that ~80% of the <span class="hlt">decadal</span> sea level <span class="hlt">variability</span> in the North Sea can be explained as response of the ocean to longshore wind forcing, including boundary wave propagation in the Northeast Atlantic. These findings have important implications for (i) detecting significant accelerations in North Sea MSL, (ii) the conceptual set up of regional ocean models in terms of resolution and boundary conditions, and (iii) the development of adequate and realistic regional climate change projections.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26444265','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26444265"><span>Trends in upper gastrointestinal diagnosis over four <span class="hlt">decades</span> in Lusaka, Zambia: a retrospective analysis of endoscopic findings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kayamba, Violet; Sinkala, Edford; Mwanamakondo, Stayner; Soko, Rose; Kawimbe, Boniface; Amadi, Beatrice; Zulu, Isaac; Nzaisenga, Jean-Baptiste; Banda, Themba; Mumbwe, Chipasha; Phiri, Evans; Munkonge, Philip; Kelly, Paul</p> <p>2015-10-06</p> <p>There a shortage of robust information about profiles of gastrointestinal disease in sub-Saharan Africa. The endoscopy unit of the University Teaching Hospital in Lusaka has been running without interruption since 1977 and this 38-year record is largely intact. We report an analysis of endoscopic findings over this period. Written endoscopy records from 29th September 1977 to 16th December 2014 were recovered, computerised, coded by two experienced endoscopists and analysed. Temporal trends were analysed using tables, graphs, and unconditional logistic regression, with age, sex of patient, <span class="hlt">decade</span>, and endoscopist as independent <span class="hlt">variables</span> to adjust for inter-<span class="hlt">observer</span> variation. Sixteen thousand nine hundred fifty-three records were identified and analysed. Diagnosis of gastric ulcer rose by 22 %, and that of duodenal ulcer fell by 14 % per <span class="hlt">decade</span>. Endoscopically diagnosed oesophageal cancer increased by 32 % per <span class="hlt">decade</span>, but gastric cancer rose only in patients under 60 years of age (21 % per <span class="hlt">decade</span>). Oesophageal varices were the commonest finding in patients presenting with haematemesis, increasing by 14 % per <span class="hlt">decade</span> in that patient group. Two HIV-related diagnoses, oesophageal candidiasis and Kaposi's sarcoma, rose from almost zero to very high levels in the 1990s but fell substantially after 2005 when anti-retroviral therapy became widely available. This useful dataset suggests that there are important trends in some endoscopic findings over four <span class="hlt">decades</span>. These trends are not explained by inter-<span class="hlt">observer</span> variation. Reasons for the divergent trends in incidence of peptic ulceration and apparent trends in diagnosis of upper gastrointestinal cancers merit further exploration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012CliPD...8.5455K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012CliPD...8.5455K"><span>On the origin of multi-<span class="hlt">decadal</span> to centennial Greenland temperature anomalies over the past 800 yr</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kobashi, T.; Shindell, D. T.; Kodera, K.; Box, J. E.; Nakaegawa, T.; Kawamura, K.</p> <p>2012-11-01</p> <p>The surface temperature of the Greenland ice sheet is among the most important climate <span class="hlt">variables</span> for assessing how climate change may impact human societies associated with accelerating sea level rise. However, the causes of multi-<span class="hlt">decadal</span>-to-centennial temperature changes in Greenland are not well understood, largely owing to short <span class="hlt">observational</span> records. To examine the causes of the Greenland temperature <span class="hlt">variability</span>, we calculated the Greenland temperature anomalies (GTA(G-NH)) over the past 800 yr by subtracting the standardised NH temperature from the standardised Greenland temperature. It decomposes the Greenland temperature variation into background climate (NH); Polar amplification; and Regional <span class="hlt">variability</span> (GTA(G-NH)). The Central Greenland polar amplification factor as expressed by the variance ratio = Greenland/NH is 2.6 over the past 161 yr, and 3.3-4.2 over the past 800 yr. The GTA explains 31-35% of the variation of Greenland temperature in the multi-<span class="hlt">decadal</span>-to-centennial time scale over the past 800 yr. Another orthogonal component of the Greenland and NH temperatures, GTP(G+NH) (Greenland temperature plus = standardized Greenland temperature + standardized NH temperature) exhibited the multi-<span class="hlt">decadal</span> variations that were likely induced by large volcanic eruptions, increasing greenhouse gasses, and internal variation of climate. We found that the GTA(G-NH) has been influenced by solar-induced changes in atmospheric circulation patterns such as those produced by North Atlantic Oscillation/Arctic Oscillation (NAO/AO). Climate modelling indicates that the anomaly is also likely linked to solar-paced changes in the Atlantic meridional overturning circulation (AMOC) and to associated changes in northward oceanic heat transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060036747&hterms=Mahoney&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D50%26Ntt%3DMahoney','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060036747&hterms=Mahoney&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D50%26Ntt%3DMahoney"><span>Gamma-Ray Spectra & <span class="hlt">Variability</span> of Cygnus X-1 <span class="hlt">Observed</span> by BATSE</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ling, J. C.; Wheaton, A.; Wallyn, P.; Mahoney, W. A.; Paciesas, W. W.; Harmon, B. A.; Fishman, G. J.; Zhang, S. N.; Hua, X. M.</p> <p>1996-01-01</p> <p>We present new BATSE Earth occultation <span class="hlt">observations</span> of the 25 keV-1.8 MeV spectrum and <span class="hlt">variability</span> of Cygnus X-1 made between August 1993 and May 1994. We <span class="hlt">observed</span> that the normal soft gamma-ray spectrum (gamma2) of Cygnus X-1 has two components: a Comptonized part seen below 30keV, and a high-energy tail in the 0.3-2 MeV range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140007379','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140007379"><span>Co-variation of Temperature and Precipitation in CMIP5 Models and Satellite <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, Chunlei; Allan, Richard P.; Huffman, George J.</p> <p>2013-01-01</p> <p>Current <span class="hlt">variability</span> of precipitation (P) and its response to surface temperature (T) are analysed using coupled (CMIP5) and atmosphere-only (AMIP5) climate model simulations and compared with <span class="hlt">observational</span> estimates.There is striking agreement between Global Precipitation Climatology Project (GPCP) <span class="hlt">observed</span> and AMIP5)simulated P anomalies over land both globally and in the tropics suggesting that prescribed sea surface temperature and realistic radiative forcings are sufficient for simulating the interannual <span class="hlt">variability</span> in continental P. Differences between the <span class="hlt">observed</span> and simulated P <span class="hlt">variability</span> over the ocean, originate primarily from the wet tropical regions, in particular the western Pacific, but are reduced slightly after 1995. All datasets show positive responses of P to T globally of around 2 % K for simulations and 3-4 % K in GPCP <span class="hlt">observations</span> but model responses over the tropical oceans are around 3 times smaller than GPCP over the period 1988-2005. The <span class="hlt">observed</span> anticorrelation between land and ocean P, linked with El Nio Southern Oscillation, is captured by the simulations. All data sets over the tropical ocean show a tendency for wet regions to become wetter and dry regions drier with warming. Over the wet region (greater than or equal to 75 precipitation percentile), the precipitation response is 13-15%K for GPCP and 5%K for models while trends in P are 2.4% <span class="hlt">decade</span> for GPCP, 0.6% <span class="hlt">decade</span> for CMIP5 and 0.9<span class="hlt">decade</span> for AMIP5 suggesting that models are underestimating the precipitation responses or a deficiency exists in the satellite datasets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037567','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037567"><span>Analysis of the Arctic system for freshwater cycle intensification: <span class="hlt">Observations</span> and expectations</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rawlins, M.A.; Steele, M.; Holland, M.M.; Adam, J.C.; Cherry, J.E.; Francis, J.A.; Groisman, P.Y.; Hinzman, L.D.; Huntington, T.G.; Kane, D.L.; Kimball, J.S.; Kwok, R.; Lammers, R.B.; Lee, C.M.; Lettenmaier, D.P.; McDonald, K.C.; Podest, E.; Pundsack, J.W.; Rudels, B.; Serreze, Mark C.; Shiklomanov, A.; Skagseth, O.; Troy, T.J.; Vorosmarty, C.J.; Wensnahan, M.; Wood, E.F.; Woodgate, R.; Yang, D.; Zhang, K.; Zhang, T.</p> <p>2010-01-01</p> <p>Hydrologic cycle intensification is an expected manifestation of a warming climate. Although positive trends in several global average quantities have been reported, no previous studies have documented broad intensification across elements of the Arctic freshwater cycle (FWC). In this study, the authors examine the character and quantitative significance of changes in annual precipitation, evapotranspiration, and river discharge across the terrestrial pan-Arctic over the past several <span class="hlt">decades</span> from <span class="hlt">observations</span> and a suite of coupled general circulation models (GCMs). Trends in freshwater flux and storage derived from <span class="hlt">observations</span> across the Arctic Ocean and surrounding seas are also described. With few exceptions, precipitation, evapotranspiration, and river discharge fluxes from <span class="hlt">observations</span> and the GCMs exhibit positive trends. Significant positive trends above the 90% confidence level, however, are not present for all of the <span class="hlt">observations</span>. Greater confidence in the GCM trends arises through lower interannual <span class="hlt">variability</span> relative to trend magnitude. Put another way, intrinsic <span class="hlt">variability</span> in the <span class="hlt">observations</span> tends to limit confidence in trend robustness. Ocean fluxes are less certain, primarily because of the lack of long-term <span class="hlt">observations</span>. Where available, salinity and volume flux data suggest some decrease in saltwater inflow to the Barents Sea (i.e., a decrease in freshwater outflow) in recent <span class="hlt">decades</span>. A decline in freshwater storage across the central Arctic Ocean and suggestions that large-scale circulation plays a dominant role in freshwater trends raise questions as to whether Arctic Ocean freshwater flows are intensifying. Although oceanic fluxes of freshwater are highly <span class="hlt">variable</span> and consistent trends are difficult to verify, the other components of the Arctic FWC do show consistent positive trends over recent <span class="hlt">decades</span>. The broad-scale increases provide evidence that the Arctic FWC is experiencing intensification. Efforts that aim to develop an adequate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ESASP.739E..91S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ESASP.739E..91S"><span>Forest Dragon-3: <span class="hlt">Decadal</span> Trends of Northeastern Forests in China from Earth <span class="hlt">Observation</span> Synergy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmullius, C.; Balling, J.; Schratz, P.; Thiel, C.; Santoro, M.; Wegmuller, U.; Li, Z.; Yong, P.</p> <p>2016-08-01</p> <p>In Forest DRAGON 3, synergy of Earth <span class="hlt">Observation</span> products to derive information of <span class="hlt">decadal</span> trends of forest in northeast China was investigated. Following up the results of Forest-DRAGON 1 and 2, Growing Stock Volume (GSV) products from different years were investigated to derive information on vegetational in north- east China. The BIOMASAR maps of 2005 and 2010, produced within the previous DRAGON projects, set the base for all analyses. We took a closer look at scale problems regarding GSV derivation, which are introduced by differing landcover within one pixel, to investigate differences throughout pixel classes with varying landcover class percentages. We developed an approach to select pixels containing forest only with the aim of undertaking a detailed analysis on retrieved GSV values for such pixels for the years 2005 and 2010. Using existing land cover products at different scales, the plausibility of changes in the BIOMASAR maps were checked.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ThApC.120..673X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ThApC.120..673X"><span>Whether the <span class="hlt">decadal</span> shift of South Asia High intensity around the late 1970s exists or not</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, Xu; Chen, Wen; Nath, Debashis; Zhou, Dingwen</p> <p>2015-05-01</p> <p>This study compares the <span class="hlt">decadal</span> means of the seasonal (June-July-August (JJA)) mean geopotential heights available from the NCEP1 and ERA-40 reanalysis data in the Northern Hemisphere. The interdecadal changes in the South Asia High (SAH) intensity derived from the reanalysis data are also compared with ground-based radiosonde <span class="hlt">observations</span> and atmospheric model outputs. The JJA mean geopotential heights in the 1980s are distinctly larger than the 1970s in NCEP1 over most of the regions in the Northern Hemisphere, while no obvious difference is <span class="hlt">observed</span> in ERA-40. The interannual variation of the SAH strength is very close in the two reanalysis data, so that it is appropriate to utilize the reanalysis data to study the interannual variation of SAH strength after removing the interdecadal trend. However, the discrepancy in SAH intensity between NCEP1 and ERA-40 mainly exists on the interdecadal time scale. The SAH intensity in the NCEP1 was close to that in the ERA-40 before the late 1970s but became remarkably stronger after the late 1970s, leading to a much larger <span class="hlt">decadal</span> strengthening during the period 1970-1990. Based on the six radiosonde <span class="hlt">observation</span> stations in the area of the SAH, the results indicate that the <span class="hlt">decadal</span> reinforcing in the SAH strength occurs around the mid-1980s. Thus, NCEP1 may overestimate the <span class="hlt">decadal</span> shift in the SAH intensity around the late 1970s, while ERA-40 may underestimate it. Much attention needs to be paid when we use the reanalysis data to study the <span class="hlt">decadal</span> <span class="hlt">variability</span> of the SAH intensity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004ClDy...22..701B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ClDy...22..701B"><span>Simulated <span class="hlt">variability</span> of the Atlantic meridional overturning circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bentsen, M.; Drange, H.; Furevik, T.; Zhou, T.</p> <p></p> <p>To examine the multi-annual to <span class="hlt">decadal</span> scale <span class="hlt">variability</span> of the Atlantic Meridional Overturning Circulation (AMOC) we conducted a four-member ensemble with a daily reanalysis forced, medium-resolution global version of the isopycnic coordinate ocean model MICOM, and a 300-years integration with the fully coupled Bergen Climate Model (BCM). The simulations of the AMOC with both model systems yield a long-term mean value of 18 Sv and <span class="hlt">decadal</span> <span class="hlt">variability</span> with an amplitude of 1-3 Sv. The power spectrum of the inter-annual to <span class="hlt">decadal</span> scale <span class="hlt">variability</span> of the AMOC in BCM generally follows the theoretical red noise spectrum, with indications of increased power near the 20-years period. Comparison with <span class="hlt">observational</span> proxy indices for the AMOC, e.g. the thickness of the Labrador Sea Water, the strength of the baroclinic gyre circulation in the North Atlantic Ocean, and the surface temperature anomalies along the mean path of the Gulf Stream, shows similar trends and phasing of the <span class="hlt">variability</span>, indicating that the simulated AMOC <span class="hlt">variability</span> is robust and real. Mixing indices have been constructed for the Labrador, the Irminger and the Greenland-Iceland-Norwegian (GIN) seas. While convective mixing in the Labrador and the GIN seas are in opposite phase, and linked to the NAO as <span class="hlt">observations</span> suggest, the convective mixing in the Irminger Sea is in phase with or leads the Labrador Sea. Newly formed deep water is seen as a slow, anomalous cold and fresh, plume flowing southward along the western continental slope of the Atlantic Ocean, with a return flow of warm and saline water on the surface. In addition, fast-travelling topographically trapped waves propagate southward along the continental slope towards equator, where they go east and continue along the eastern rim of the Atlantic. For both types of experiments, the Northern Hemisphere sea level pressure and 2 m temperature anomaly patterns computed based on the difference between climate states with strong and weak AMOC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003A%26A...406..629M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003A%26A...406..629M"><span>X-ray <span class="hlt">variability</span> of Pleiades late-type stars as <span class="hlt">observed</span> with the ROSAT-PSPC</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marino, A.; Micela, G.; Peres, G.; Sciortino, S.</p> <p>2003-08-01</p> <p>We present a comprehensive analysis of X-ray <span class="hlt">variability</span> of the late-type (dF7-dM) Pleiades stars, detected in all ROSAT-PSPC <span class="hlt">observations</span>; X-ray variations on short (hours) and medium (months) time scales have been explored. We have grouped the stars in two samples: 89 <span class="hlt">observations</span> of 42 distinct dF7-dK2 stars and 108 <span class="hlt">observations</span> of 61 dK3-dM stars. The Kolmogorov-Smirnov test applied on all X-ray photon time series show that the percentage of cases of significant <span class="hlt">variability</span> is quite similar on both samples, suggesting that the presence of <span class="hlt">variability</span> does not depend on mass for the time scales and mass range explored. The comparison between the Time X-ray Amplitude Distribution functions (XAD) of the set of dF7-dK2 and of the dK3-dM show that, on short time scales, dK3-dM stars show larger variations than dF7-dK2. A subsample of eleven dF7-dK2 and eleven dK3-dM Pleiades stars allows the study of <span class="hlt">variability</span> on longer time scales: we found that <span class="hlt">variability</span> on medium - long time scales is relatively more common among dF7-dK2 stars than among dK3-dM ones. For both dF7-dK2 Pleiades stars and dF7-dK2 field stars, the <span class="hlt">variability</span> on short time scales depends on Lx while this dependence has not been <span class="hlt">observed</span> among dK3-dM stars. It may be that the <span class="hlt">variability</span> among dK3-dM stars is dominated by flares that have a similar luminosity distribution for stars of different Lx, while flaring distribution in dF7-dK2 stars may depend on X-ray luminosity. The lowest mass stars show significant rapid <span class="hlt">variability</span> (flares?) and no evidence of rotation modulation or cycles. On the contrary, dF7-dK2 Pleiades stars show both rapid <span class="hlt">variability</span> and variations on longer time scales, likely associated with rotational modulation or cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999GeoRL..26.1337O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999GeoRL..26.1337O"><span>Salinity signature of the Pacific <span class="hlt">Decadal</span> Oscillation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Overland, James E.; Salo, Sigrid; Adams, Jennifer Miletta</p> <p></p> <p>Three sites in the North Pacific have temperature and salinity <span class="hlt">observations</span> in most months for several years before and after 1977. The Gulf of Alaska station (57°N, 148°W) showed a 2°C warming and a 0.6 freshening in salinity at 10 m depth in the 1980s compared to the 1970s. OWS PAPA (50°N, 145°W) and PAPA line station 7 (49.1°N, 132.4°W) show warming of 0.6°C and 0.9°C, with no major salinity change. The decrease in density and increase in stratification in the Gulf of Alaska after 1977 corresponds primarily to a decrease in salinity in the upper 150 m. We propose that while the Pacific <span class="hlt">Decadal</span> Oscillation has an east/west character in temperature, the salinity signature will have a NNW/SSE character, similar to the pattern of interannual <span class="hlt">variability</span> in precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CNSNS..59..165P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CNSNS..59..165P"><span>About the relationships among <span class="hlt">variables</span> <span class="hlt">observed</span> in the real world</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petkov, Boyan H.</p> <p>2018-06-01</p> <p>Since a stationary chaotic system is determined by nonlinear equations connecting its components, the appurtenance of two <span class="hlt">variables</span> to such a system has been considered a sign of nontrivial relationships between them including also other quantities. These relationships could remain hidden for the approach usually employed in the research analyses, which is based on the extent of the correlation that characterises the dependence of one <span class="hlt">variable</span> on the other. The appurtenance to the same system can be hypothesized if the topological features of the attractors reconstructed from two time series representing the evolution of the corresponding <span class="hlt">variables</span> are close to each other. However, the possibility that both attractors represent different systems with similar behaviour cannot be excluded. For that reason, an approach allowing the reconstruction of the attractor by using jointly two time series was proposed and the conclusion about the common origin of the <span class="hlt">variables</span> under study can be made if this attractor is topologically similar to those built separately from the two time series. In the present study, the features of the attractors were presented by the correlation dimension and the largest Lyapunov exponent and the proposed algorithm has been tested on numerically generated sequences obtained from various maps. It is believed that this approach could be used to reveal connections among the <span class="hlt">variables</span> <span class="hlt">observed</span> in experiments or field measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30..595C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30..595C"><span>When can ocean acidification impacts be detected from <span class="hlt">decadal</span> alkalinity measurements?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carter, B. R.; Frölicher, T. L.; Dunne, J. P.; Rodgers, K. B.; Slater, R. D.; Sarmiento, J. L.</p> <p>2016-04-01</p> <p>We use a large initial condition suite of simulations (30 runs) with an Earth system model to assess the detectability of biogeochemical impacts of ocean acidification (OA) on the marine alkalinity distribution from <span class="hlt">decadally</span> repeated hydrographic measurements such as those produced by the Global Ship-Based Hydrographic Investigations Program (GO-SHIP). Detection of these impacts is complicated by alkalinity changes from <span class="hlt">variability</span> and long-term trends in freshwater and organic matter cycling and ocean circulation. In our ensemble simulation, <span class="hlt">variability</span> in freshwater cycling generates large changes in alkalinity that obscure the changes of interest and prevent the attribution of <span class="hlt">observed</span> alkalinity redistribution to OA. These complications from freshwater cycling can be mostly avoided through salinity normalization of alkalinity. With the salinity-normalized alkalinity, modeled OA impacts are broadly detectable in the surface of the subtropical gyres by 2030. Discrepancies between this finding and the finding of an earlier analysis suggest that these estimates are strongly sensitive to the patterns of calcium carbonate export simulated by the model. OA impacts are detectable later in the subpolar and equatorial regions due to slower responses of alkalinity to OA in these regions and greater seasonal equatorial alkalinity <span class="hlt">variability</span>. OA impacts are detectable later at depth despite lower <span class="hlt">variability</span> due to smaller rates of change and consistent measurement uncertainty.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930072109&hterms=koji&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dkoji','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930072109&hterms=koji&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dkoji"><span>Extreme Ultraviolet Explorer <span class="hlt">observations</span> of the magnetic cataclysmic <span class="hlt">variable</span> RE 1938-461</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Warren, John K.; Vallerga, John V.; Mauche, Christopher W.; Mukai, Koji; Siegmund, Oswald H. W.</p> <p>1993-01-01</p> <p>The magnetic cataclysmic <span class="hlt">variable</span> RE 1938-461 was <span class="hlt">observed</span> by the Extreme Ultraviolet Explorer (EUVE) Deep Survey instrument on 1992 July 8-9 during in-orbit calibration. It was detected in the Lexan/ boron (65-190 A) band, with a quiescent count rate of 0.0062 +/- 0.0017/s, and was not detected in the aluminum/carbon (160-360 A) band. The Lexan/boron count rate is lower than the corresponding ROSAT wide-field camera Lexan/boron count rate. This is consistent with the fact that the source was in a low state during an optical <span class="hlt">observation</span> performed just after the EUVE <span class="hlt">observation</span>, whereas it was in an optical high state during the ROSAT <span class="hlt">observation</span>. The quiescent count rates are consistent with a virtual cessation of accretion. Two transient events lasting about 1 hr occurred during the Lexan/boron pointing, the second at a count rate of 0.050 +/- 0.006/s. This appears to be the first detection of an EUV transient during the low state of a magnetic cataclysmic <span class="hlt">variable</span>. We propose two possible explanations for the transient events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29703895','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29703895"><span>Limits on determining the skill of North Atlantic Ocean <span class="hlt">decadal</span> predictions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Menary, Matthew B; Hermanson, Leon</p> <p>2018-04-27</p> <p>The northern North Atlantic is important globally both through its impact on the Atlantic Meridional Overturning Circulation (AMOC) and through widespread atmospheric teleconnections. The region has been shown to be potentially predictable a <span class="hlt">decade</span> ahead with the skill of <span class="hlt">decadal</span> predictions assessed against reanalyses of the ocean state. Here, we show that the prediction skill in this region is strongly dependent on the choice of reanalysis used for validation, and describe the causes. Multiannual skill in key metrics such as Labrador Sea density and the AMOC depends on more than simply the choice of the prediction model. Instead, this skill is related to the similarity between the nature of interannual density <span class="hlt">variability</span> in the underlying climate model and the chosen reanalysis. The climate models used in these <span class="hlt">decadal</span> predictions are also used in climate projections, which raises questions about the sensitivity of these projections to the models' innate North Atlantic density <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPA11D..08W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPA11D..08W"><span>Economic Value of Narrowing the Uncertainty in Climate Sensitivity: <span class="hlt">Decadal</span> Change in Shortwave Cloud Radiative Forcing and Low Cloud Feedback</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wielicki, B. A.; Cooke, R. M.; Golub, A. A.; Mlynczak, M. G.; Young, D. F.; Baize, R. R.</p> <p>2016-12-01</p> <p>Several previous studies have been published on the economic value of narrowing the uncertainty in climate sensitivity (Cooke et al. 2015, Cooke et al. 2016, Hope, 2015). All three of these studies estimated roughly 10 Trillion U.S. dollars for the Net Present Value and Real Option Value at a discount rate of 3%. This discount rate is the nominal discount rate used in the U.S. Social Cost of Carbon Memo (2010). The Cooke et al studies approached this problem by examining advances in accuracy of global temperature measurements, while the Hope 2015 study did not address the type of <span class="hlt">observations</span> required. While temperature change is related to climate sensitivity, large uncertainties of a factor of 3 in current anthropogenic radiative forcing (IPCC, 2013) would need to be solved for advanced <span class="hlt">decadal</span> temperature change <span class="hlt">observations</span> to assist the challenge of narrowing climate sensitivity. The present study takes a new approach by extending the Cooke et al. 2015,2016 papers to replace <span class="hlt">observations</span> of temperature change to <span class="hlt">observations</span> of <span class="hlt">decadal</span> change in the effects of changing clouds on the Earths radiative energy balance, a measurement known as Cloud Radiative Forcing, or Cloud Radiative Effect. <span class="hlt">Decadal</span> change in this <span class="hlt">observation</span> is direclty related to the largest uncertainty in climate sensitivity which is cloud feedback from changing amount of low clouds, primarily low clouds over the world's oceans. As a result, <span class="hlt">decadal</span> changes in shortwave cloud radiative forcing are more directly related to cloud feedback uncertainty which is the dominant uncertainty in climate sensitivity. This paper will show results for the new approach, and allow an examination of the sensitivity of economic value results to different <span class="hlt">observations</span> used as a constraint on uncertainty in climate sensitivity. The analysis suggests roughly a doubling of economic value to 20 Trillion Net Present Value or Real Option Value at 3% discount rate. The higher economic value results from two changes: a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018yCatp004013601O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018yCatp004013601O"><span>VizieR Online Data Catalog: Early <span class="hlt">observations</span> of M13 <span class="hlt">variables</span> (Osborn,+, 2016)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osborn, W.; Barnard, E. E.</p> <p>2018-05-01</p> <p>In 1900 E.E. Barnard published 37 visual <span class="hlt">observations</span> of <span class="hlt">Variable</span> 2 (V2) in the globular cluster M13 made in 1899 and 1900. A review of Barnard's notebooks revealed he made many additional brightness estimates up to 1911, and he had also recorded the variations of V1 starting in 1904. These data provide the earliest-epoch light curves for these stars and thus are useful for studying their period changes. This paper presents Barnard's <span class="hlt">observations</span> of the M13 <span class="hlt">variables</span> along with their derived heliocentric Julian dates and approximate V magnitudes. These include 231 unpublished <span class="hlt">observations</span> of V2 and 94 of V1. How these data will be of value for determining period changes by these stars is described. (5 data files).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830052666&hterms=iav&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Diav','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830052666&hterms=iav&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Diav"><span>Interannual <span class="hlt">variability</span> and climatic noise in satellite-<span class="hlt">observed</span> outgoing longwave radiation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Short, D. A.; Cahalan, R. F.</p> <p>1983-01-01</p> <p>Upwelling-IR <span class="hlt">observations</span> of the North Pacific by polar orbiters NOAA 3, 4, 5, and 6 and TIROS-N from 1974 to 1981 are analyzed statistically in terms of interannual <span class="hlt">variability</span> (IAV) in monthly averages and climatic noise due to short-term weather fluctuations. It is found that although the daily variance in the <span class="hlt">observations</span> is the same in summer and winter months, and although IAV in winter is smaller than that in summer, the climatic noise in winter is so much smaller that a greater fraction of winter anomalies are statistically significant. The smaller winter climatic noise level is shown to be due to shorter autocorrelation times. It is demonstrated that increasing averaging area does not reduce the climatic noise level, suggesting that continuing collection of high-resolution satellite IR data on a global basis is necessary if better models of short-term <span class="hlt">variability</span> are to be constructed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P51E..04A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P51E..04A"><span>The LUVOIR <span class="hlt">Decadal</span> Mission Concept</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arney, G. N.; Crooke, J.; Domagal-Goldman, S. D.; Fischer, D.; Peterson, B.; Schmidt, B. E.; Stdt, T. L. T.</p> <p>2017-12-01</p> <p>The Large UV-Optical-Infrared (LUVOIR) Surveyor is one of four mission concepts being studied by NASA in preparation for the 2020 Astrophysics <span class="hlt">Decadal</span> Survey. LUVOIR is a general-purpose space-based observatory with a large aperture in the 8-16 m range and a total bandpass spanning from the far-UV to the near-infrared. This observatory will enable revolutionary new studies in many areas of astronomy, including planetary science within and beyond our Solar System. Because LUVOIR is being considered for the next <span class="hlt">decadal</span> survey, it must be capable of advancing our understanding of astronomical targets, including exoplanets, far beyond what will be achieved by the next two <span class="hlt">decades</span> of <span class="hlt">observations</span> from other space- or ground-based facilities. This means that the mission must move past planet detection, which is happening now with Kepler and ground-based measurements and will continue with TESS (Transiting Exoplanet Survey Satellite) and WFIRST (Wide Field Infrared Survey Telescope). It must also move beyond the chemical characterization of gas giants, which has begun with <span class="hlt">observations</span> from Spitzer, Hubble, and ground-based telescopes and will greatly advances with the upcoming JWST (James Webb Space Telescope) and WFIRST coronagraph. Therefore, one of LUVOIR's main science objectives will be to directly image rocky Earth-sized planets in the habitable zones of other stars, measure their spectra, analyze the chemistry of their atmospheres, and obtain information about their surfaces. Such <span class="hlt">observations</span> will allow us to evaluate these worlds' habitability and potential for life. We will review the specific <span class="hlt">observational</span> strategies needed for astrobiological assessments of exoplanetary environments, including the wavelength range and spectral resolution required for these habitability analyses and biosignature searches. Further, we will discuss how the <span class="hlt">observational</span> requirements to make measurements of "Earthlike" worlds will allow high-quality <span class="hlt">observations</span> of a wide</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1393980-statistical-characteristics-cloud-variability-part-retrieved-cloud-liquid-water-path-three-arm-sites-observed-cloud-variability-arm-sites','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1393980-statistical-characteristics-cloud-variability-part-retrieved-cloud-liquid-water-path-three-arm-sites-observed-cloud-variability-arm-sites"><span>Statistical characteristics of cloud <span class="hlt">variability</span>. Part 1: Retrieved cloud liquid water path at three ARM sites: <span class="hlt">Observed</span> cloud <span class="hlt">variability</span> at ARM sites</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Huang, Dong; Campos, Edwin; Liu, Yangang</p> <p>2014-09-17</p> <p>Statistical characteristics of cloud <span class="hlt">variability</span> are examined for their dependence on averaging scales and best representation of probability density function with the <span class="hlt">decade</span>-long retrieval products of cloud liquid water path (LWP) from the tropical western Pacific (TWP), Southern Great Plains (SGP), and North Slope of Alaska (NSA) sites of the Department of Energy’s Atmospheric Radiation Measurement Program. The statistical moments of LWP show some seasonal variation at the SGP and NSA sites but not much at the TWP site. It is found that the standard deviation, relative dispersion (the ratio of the standard deviation to the mean), and skewness allmore » quickly increase with the averaging window size when the window size is small and become more or less flat when the window size exceeds 12 h. On average, the cloud LWP at the TWP site has the largest values of standard deviation, relative dispersion, and skewness, whereas the NSA site exhibits the least. Correlation analysis shows that there is a positive correlation between the mean LWP and the standard deviation. The skewness is found to be closely related to the relative dispersion with a correlation coefficient of 0.6. The comparison further shows that the log normal, Weibull, and gamma distributions reasonably explain the <span class="hlt">observed</span> relationship between skewness and relative dispersion over a wide range of scales.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012689','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012689"><span>Quantitative Comparison of the <span class="hlt">Variability</span> in <span class="hlt">Observed</span> and Simulated Shortwave Reflectance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roberts, Yolanda, L.; Pilewskie, P.; Kindel, B. C.; Feldman, D. R.; Collins, W. D.</p> <p>2013-01-01</p> <p>The Climate Absolute Radiance and Refractivity Observatory (CLARREO) is a climate <span class="hlt">observation</span> system that has been designed to monitor the Earth's climate with unprecedented absolute radiometric accuracy and SI traceability. Climate <span class="hlt">Observation</span> System Simulation Experiments (OSSEs) have been generated to simulate CLARREO hyperspectral shortwave imager measurements to help define the measurement characteristics needed for CLARREO to achieve its objectives. To evaluate how well the OSSE-simulated reflectance spectra reproduce the Earth s climate <span class="hlt">variability</span> at the beginning of the 21st century, we compared the <span class="hlt">variability</span> of the OSSE reflectance spectra to that of the reflectance spectra measured by the Scanning Imaging Absorption Spectrometer for Atmospheric Cartography (SCIAMACHY). Principal component analysis (PCA) is a multivariate decomposition technique used to represent and study the <span class="hlt">variability</span> of hyperspectral radiation measurements. Using PCA, between 99.7%and 99.9%of the total variance the OSSE and SCIAMACHY data sets can be explained by subspaces defined by six principal components (PCs). To quantify how much information is shared between the simulated and <span class="hlt">observed</span> data sets, we spectrally decomposed the intersection of the two data set subspaces. The results from four cases in 2004 showed that the two data sets share eight (January and October) and seven (April and July) dimensions, which correspond to about 99.9% of the total SCIAMACHY variance for each month. The spectral nature of these shared spaces, understood by examining the transformed eigenvectors calculated from the subspace intersections, exhibit similar physical characteristics to the original PCs calculated from each data set, such as water vapor absorption, vegetation reflectance, and cloud reflectance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994ClDy....9..303T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994ClDy....9..303T"><span><span class="hlt">Decadal</span> atmosphere-ocean variations in the Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trenberth, Kevin E.; Hurrell, James W.</p> <p>1994-03-01</p> <p>Considerable evidence has emerged of a substantial <span class="hlt">decade</span>-long change in the north Pacific atmosphere and ocean lasting from about 1976 to 1988. <span class="hlt">Observed</span> significant changes in the atmospheric circulation throughout the troposphere revealed a deeper and eastward shifted Aleutian low pressure system in the winter half year which advected warmer and moister air along the west coast of North America and into Alaska and colder air over the north Pacific. Consequently, there were increases in temperatures and sea surface temperatures (SSTs) along the west coast of North America and Alaska but decreases in SSTs over the central north Pacific, as well as changes in coastal rainfall and streamflow, and decreases in sea ice in the Bering Sea. Associated changes occurred in the surface wind stress, and, by inference, in the Sverdrup transport in the north Pacific Ocean. Changes in the monthly mean flow were accompanied by a southward shift in the storm tracks and associated synoptic eddy activity and in the surface ocean sensible and latent heat fluxes. In addition to the changes in the physical environment, the deeper Aleutian low increased the nutrient supply as seen through increases in total chlorophyll in the water column, phytoplankton and zooplankton. These changes, along with the altered ocean currents and temperatures, changed the migration patterns and increased the stock of many fish species. A north Pacific (NP) index is defined to measure the <span class="hlt">decadal</span> variations, and the temporal <span class="hlt">variability</span> of the index is explored on daily, annual, interannual and <span class="hlt">decadal</span> time scales. The dominant atmosphere-ocean relation in the north Pacific is one where atmospheric changes lead SSTs by one to two months. However, strong ties are revealed with events in the tropical Pacific, with changes in tropical Pacific SSTs leading SSTs in the north Pacific by three months. Changes in the storm tracks in the north Pacific help to reinforce and maintain the anomalous circulation in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JMS...161...26C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JMS...161...26C"><span>Developing priority <span class="hlt">variables</span> ("ecosystem Essential Ocean <span class="hlt">Variables</span>" - eEOVs) for <span class="hlt">observing</span> dynamics and change in Southern Ocean ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Constable, Andrew J.; Costa, Daniel P.; Schofield, Oscar; Newman, Louise; Urban, Edward R.; Fulton, Elizabeth A.; Melbourne-Thomas, Jessica; Ballerini, Tosca; Boyd, Philip W.; Brandt, Angelika; de la Mare, Willaim K.; Edwards, Martin; Eléaume, Marc; Emmerson, Louise; Fennel, Katja; Fielding, Sophie; Griffiths, Huw; Gutt, Julian; Hindell, Mark A.; Hofmann, Eileen E.; Jennings, Simon; La, Hyoung Sul; McCurdy, Andrea; Mitchell, B. Greg; Moltmann, Tim; Muelbert, Monica; Murphy, Eugene; Press, Anthony J.; Raymond, Ben; Reid, Keith; Reiss, Christian; Rice, Jake; Salter, Ian; Smith, David C.; Song, Sun; Southwell, Colin; Swadling, Kerrie M.; Van de Putte, Anton; Willis, Zdenka</p> <p>2016-09-01</p> <p>Reliable statements about <span class="hlt">variability</span> and change in marine ecosystems and their underlying causes are needed to report on their status and to guide management. Here we use the Framework on Ocean <span class="hlt">Observing</span> (FOO) to begin developing ecosystem Essential Ocean <span class="hlt">Variables</span> (eEOVs) for the Southern Ocean <span class="hlt">Observing</span> System (SOOS). An eEOV is a defined biological or ecological quantity, which is derived from field <span class="hlt">observations</span>, and which contributes significantly to assessments of Southern Ocean ecosystems. Here, assessments are concerned with estimating status and trends in ecosystem properties, attribution of trends to causes, and predicting future trajectories. eEOVs should be feasible to collect at appropriate spatial and temporal scales and are useful to the extent that they contribute to direct estimation of trends and/or attribution, and/or development of ecological (statistical or simulation) models to support assessments. In this paper we outline the rationale, including establishing a set of criteria, for selecting eEOVs for the SOOS and develop a list of candidate eEOVs for further evaluation. Other than habitat <span class="hlt">variables</span>, nine types of eEOVs for Southern Ocean taxa are identified within three classes: state (magnitude, genetic/species, size spectrum), predator-prey (diet, foraging range), and autecology (phenology, reproductive rate, individual growth rate, detritus). Most candidates for the suite of Southern Ocean taxa relate to state or diet. Candidate autecological eEOVs have not been developed other than for marine mammals and birds. We consider some of the spatial and temporal issues that will influence the adoption and use of eEOVs in an <span class="hlt">observing</span> system in the Southern Ocean, noting that existing operations and platforms potentially provide coverage of the four main sectors of the region - the East and West Pacific, Atlantic and Indian. Lastly, we discuss the importance of simulation modelling in helping with the design of the <span class="hlt">observing</span> system in the long</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003802','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003802"><span>Hinode: A <span class="hlt">Decade</span> of Success in Capturing Solar Activity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Savage, S.; Elrod, S.; Deluca, E.; Doschek, G.; Tarbell, T.</p> <p>2017-01-01</p> <p>As the present solar cycle passes into its minimum phase, the Hinode mission marks its tenth year of investigating solar activity. Hinode's <span class="hlt">decade</span> of successful <span class="hlt">observations</span> have provided us with immeasurable insight into the solar processes that invoke space weather and thereby affect the interplanetary environment in which we reside. The mission's complementary suite of instruments allows us to probe transient, high energy events alongside long-term, cycle-dependent phenomena from magnetic fields at the Sun's surface out to highly thermalized coronal plasma enveloping active regions (ARs). These rich data sets have already changed the face of solar physics and will continue to provoke exciting research as new <span class="hlt">observational</span> paradigms are pursued. Hinode was launched as part of the Science Mission Directorate's (SMD) Solar Terrestrial Probes Program in 2006. It is a sophisticated spacecraft equipped with a Solar Optical Telescope (SOT), an Extreme-ultraviolet Imaging Spectrometer (EIS), and an X-Ray Telescope (XRT) (see x 4). With high resolution and sensitivity, Hinode serves as a microscope for the Sun, providing us with unique capabilities for <span class="hlt">observing</span> magnetic fields near the smallest scales achievable, while also rendering full-Sun coronal context in the highest thermal regimes. The 2014 NASA SMD strategic goals objective to "Understand the Sun and its interactions with the Earth and the solar system, including space weather" forms the basis of three underlying Heliophysics Science Goals. While Hinode relates to all three, the observatory primarily addresses: Explore the physical processes in the space environment from the Sun to the Earth and through the solar system. Within the NASA National Research Council (NRC) <span class="hlt">Decadal</span> Survey Priorities, Hinode targets: (a) Determine the origins of the Sun's activity and predict the variations of the space environment and (d) Discover and characterize fundamental processes that occur both within the heliosphere and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511114S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511114S"><span>Evaluation of <span class="hlt">decadal</span> hindcasts using satellite simulators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spangehl, Thomas; Mazurkiewicz, Alex; Schröder, Marc</p> <p>2013-04-01</p> <p>The evaluation of dynamical ensemble forecast systems requires a solid validation of basic processes such as the global atmospheric water and energy cycle. The value of any validation approach strongly depends on the quality of the <span class="hlt">observational</span> data records used. Current approaches utilize in situ measurements, remote sensing data and reanalyses. Related data records are subject to a number of uncertainties and limitations such as representativeness, spatial and temporal resolution and homogeneity. However, recently several climate data records with known and sufficient quality became available. In particular, the satellite data records offer the opportunity to obtain reference information on global scales including the oceans. Here we consider the simulation of satellite radiances from the climate model output enabling an evaluation in the instrument's parameter space to avoid uncertainties stemming from the application of retrieval schemes in order to minimise uncertainties on the reference side. Utilizing the CFMIP <span class="hlt">Observation</span> Simulator Package (COSP) we develop satellite simulators for the Tropical Rainfall Measuring Mission precipitation radar (TRMM PR) and the Infrared Atmospheric Sounding Interferometer (IASI). The simulators are applied within the MiKlip project funded by BMBF (German Federal Ministry of Education and Research) to evaluate <span class="hlt">decadal</span> climate predictions performed with the MPI-ESM developed at the Max Planck Institute for Meteorology. While TRMM PR enables the evaluation of the vertical structure of precipitation over tropical and sub-tropical areas, IASI is used to support the global evaluation of clouds and radiation. In a first step the reliability of the developed simulators needs to be explored. The simulation of radiances in the instrument space requires the generation of sub-grid scale <span class="hlt">variability</span> from the climate model output. Furthermore, assumptions are made to simulate radiances such as, for example, the distribution of different</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080015493','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080015493"><span>SABER <span class="hlt">Observations</span> of the OH Meinel Airglow <span class="hlt">Variability</span> Near the Mesopause</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Marsh, Daniel R.; Smith, Anne K.; Mlynczak, Martin G.</p> <p>2005-01-01</p> <p>The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument, one of four on board the TIMED satellite, <span class="hlt">observes</span> the OH Meinel emission at 2.0 m that peaks near the mesopause. The emission results from reactions between members of the oxygen and hydrogen chemical families that can be significantly affected by mesopause dynamics. In this study we compare SABER measurements of OH Meinel emission rates and temperatures with predictions from a 3-dimensional chemical dynamical model. In general, the model is capable of reproducing both the <span class="hlt">observed</span> diurnal and seasonal OH Meinel emission <span class="hlt">variability</span>. The results indicate that the diurnal tide has a large effect on the overall magnitude and temporal variation of the emission in low latitudes. This tidal <span class="hlt">variability</span> is so dominant that the seasonal cycle in the nighttime emission depends very strongly on the local time of the analysis. At higher latitudes, the emission has an annual cycle that is due mainly to transport of oxygen by the seasonally reversing mean circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/8057','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/8057"><span>Interannual/<span class="hlt">decadal</span> <span class="hlt">variability</span> in MJO activity as diagnosed in the 40-year NCEP/NCAR reanalysis and simulated in an ensemble of GISST integrations</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Slingo, J. M.; Rowell, D. P.; Sperber, K. R.</p> <p>1999-04-21</p> <p>The Madden-Julian Oscillation (MJO) is the dominant mode of tropical <span class="hlt">variability</span> at intraseasonal timescales. It displays substantial interannual <span class="hlt">variability</span> in intensity which may have important implications for the predictability of the coupled system. The reasons for this interannual <span class="hlt">variability</span> are not understood. The interannual behaviour of the MJO has been diagnosed initially in the 40-year NCEP/NCAR Reanalysis by calculating the variance of the 20-100 day filtered zonal mean zonal wind (10 o N-10 o S averaged) in a 100- day moving window. The results suggest that prior to the mid-1970s the activity of the MJO was consistently lower than duringmore » the latter part of the record. This may be related to either inadequacies in the data coverage, particularly over the tropical Indian Ocean prior to the introduction of satellite <span class="hlt">observations</span>, or to the real effects of a <span class="hlt">decadal</span> timescale warming in the tropical SSTs. This interdecadal trend is captured by the dominant EOF (explaining 28% of the variance) of the monthly mean SSTs (after removal of the mean seasonal cycle), as used in the NCEP/NCAR Reanalysis for the region of the tropics where the MJO is convectively active (i.e., 60 o E-180 o E, 20 o S-20 o N). During the latter part of 1970s there was an abrupt change from a predominantly negative PC1 (i.e. colder Indian Ocean) to a positive PC1 (i.e. warmer Indian Ocean), indicative of a general warming of the tropical Indian Ocean by at least 0.5 o K over the last 40 years. However, on interannual timescales, the teleconnection patterns between MJO activity and SST show only a weak, barely significant, influence of El Niño in which the MJO is more active during the cold phase. As well as the NCEP/NCAR Reanalysis, a 4-member ensemble of 45 year integrations with the Hadley Centre climate model (HADAM2a), forced by <span class="hlt">observed</span> SSTs for 1949-93, has been used to investigate the relationship between MJO activity and SST. HADAM2a is known to give a reasonable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5384G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5384G"><span>North Atlantic sea-level <span class="hlt">variability</span> during the last millennium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gehrels, Roland; Long, Antony; Saher, Margot; Barlow, Natasha; Blaauw, Maarten; Haigh, Ivan; Woodworth, Philip</p> <p>2014-05-01</p> <p>Climate modelling studies have demonstrated that spatial and temporal sea-level <span class="hlt">variability</span> <span class="hlt">observed</span> in North Atlantic tide-gauge records is controlled by a complex array of processes, including ice-ocean mass exchange, freshwater forcing, steric changes, changes in wind fields, and variations in the speed of the Gulf Stream. Longer records of sea-level change, also covering the pre-industrial period, are important as a 'natural' and long-term baseline against which to test model performance and to place recent and future sea-level changes and ice-sheet change into a long-term context. Such records can only be reliably and continuously reconstructed from proxy methods. Salt marshes are capable of recording decimetre-scale sea-level variations with high precision and accuracy. In this paper we present four new high-resolution proxy records of (sub-) <span class="hlt">decadal</span> sea-level <span class="hlt">variability</span> reconstructed from salt-marsh sediments in Iceland, Nova Scotia, Maine and Connecticut that span the past 400 to 900 years. Our records, based on more than 100 new radiocarbon analyses, Pb-210 and Cs-137 measurements as well as other biological and geochemical age markers, together with hundreds of new microfossil <span class="hlt">observations</span> from contemporary and fossil salt marshes, capture not only the rapid 20th century sea-level rise, but also small-scale (decimetre, multi-<span class="hlt">decadal</span>) sea-level fluctuations during preceding centuries. We show that in Iceland three periods of rapid sea-level rise are synchronous with the three largest positive shifts of the reconstructed North Atlantic Oscillation (NAO) index. Along the North American east coast we compare our data with salt-marsh records from New Jersey, North Carolina and Florida and <span class="hlt">observe</span> a trend of increased pre-industrial sea-level <span class="hlt">variability</span> from south to north (Florida to Nova Scotia). Mass changes and freshwater forcing cannot explain this pattern. Based on comparisons with instrumental sea-level data and modelling studies we hypothesise that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=302477','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=302477"><span>Intra- to Multi-<span class="hlt">Decadal</span> Temperature <span class="hlt">Variability</span> over the Continental United States: 1896-2012</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>The Optimal Ranking Regime (ORR) method was used to identify intra- to multi-<span class="hlt">decadal</span> (IMD) time windows containing significant ranking sequences in U.S. climate division temperature data. The simplicity of the ORR procedure’s output – a time series’ most significant non-overlapping periods of high o...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2342S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2342S"><span>Contrasting spatial structures of Atlantic Multidecadal Oscillation between <span class="hlt">observations</span> and slab ocean model simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Cheng; Li, Jianping; Kucharski, Fred; Xue, Jiaqing; Li, Xiang</p> <p>2018-04-01</p> <p>The spatial structure of Atlantic multidecadal oscillation (AMO) is analyzed and compared between the <span class="hlt">observations</span> and simulations from slab ocean models (SOMs) and fully coupled models. The <span class="hlt">observed</span> sea surface temperature (SST) pattern of AMO is characterized by a basin-wide monopole structure, and there is a significantly high degree of spatial coherence of <span class="hlt">decadal</span> SST variations across the entire North Atlantic basin. The <span class="hlt">observed</span> SST anomalies share a common <span class="hlt">decadal</span>-scale signal, corresponding to the basin-wide average (i. e., the AMO). In contrast, the simulated AMO in SOMs (AMOs) exhibits a tripole-like structure, with the mid-latitude North Atlantic SST showing an inverse relationship with other parts of the basin, and the SOMs fail to reproduce the <span class="hlt">observed</span> strong spatial coherence of <span class="hlt">decadal</span> SST variations associated with the AMO. The <span class="hlt">observed</span> spatial coherence of AMO SST anomalies is identified as a key feature that can be used to distinguish the AMO mechanism. The tripole-like SST pattern of AMOs in SOMs can be largely explained by the atmosphere-forced thermodynamics mechanism due to the surface heat flux changes associated with the North Atlantic Oscillation (NAO). The thermodynamic forcing of AMOs by the NAO gives rise to a simultaneous inverse NAO-AMOs relationship at both interannual and <span class="hlt">decadal</span> timescales and a seasonal phase locking of the AMOs <span class="hlt">variability</span> to the cold season. However, the NAO-forced thermodynamics mechanism cannot explain the <span class="hlt">observed</span> NAO-AMO relationship and the seasonal phase locking of <span class="hlt">observed</span> AMO <span class="hlt">variability</span> to the warm season. At <span class="hlt">decadal</span> timescales, a strong lagged relationship between NAO and AMO is <span class="hlt">observed</span>, with the NAO leading by up to two <span class="hlt">decades</span>, while the simultaneous correlation of NAO with AMO is weak. This lagged relationship and the spatial coherence of AMO can be well understood from the view point of ocean dynamics. A time-integrated NAO index, which reflects the variations in Atlantic meridional overturning</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GSL.....5....3F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GSL.....5....3F"><span>The Indonesian throughflow, its <span class="hlt">variability</span> and centennial change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feng, Ming; Zhang, Ningning; Liu, Qinyan; Wijffels, Susan</p> <p>2018-12-01</p> <p>The Indonesian Throughflow (ITF) is an important component of the upper cell of the global overturning circulation that provides a low-latitude pathway for warm, fresh waters from the Pacific to enter the Indian Ocean. <span class="hlt">Variability</span> and changes of the ITF have significant impacts on Indo-Pacific oceanography and global climate. In this paper, the <span class="hlt">observed</span> features of the ITF and its interannual to <span class="hlt">decadal</span> <span class="hlt">variability</span> are reviewed, and processes that influence the centennial change of the ITF under the influence of the global warming are discussed. The ITF flows across a region that comprises the intersection of two ocean waveguides—those of the equatorial Pacific and equatorial Indian Ocean. The ITF geostrophic transport is stronger during La Niñas and weaker during El Niños due to the influences through the Pacific waveguide. The Indian Ocean wind <span class="hlt">variability</span> associated with the Indian Ocean Dipole (IOD) in many years offsets the Pacific ENSO influences on the ITF geostrophic transport during the developing and mature phases of El Niño and La Niña through the Indian Ocean waveguide, due to the co-varying IOD <span class="hlt">variability</span> with ENSO. <span class="hlt">Decadal</span> and multi-<span class="hlt">decadal</span> changes of the geostrophic ITF transport have been revealed: there was a weakening change from the mid-1970s climate regime shift followed by a strengthening trend of about 1Sv every 10 year during 1984-2013. These <span class="hlt">decadal</span> changes are mostly due to the ITF responses to <span class="hlt">decadal</span> variations of the trade winds in the Pacific. Thus, Godfrey's Island Rule, as well as other ITF proxies, appears to be able to quantify <span class="hlt">decadal</span> variations of the ITF. Climate models project a weakening trend of the ITF under the global warming. Both climate models and downscaled ocean model show that this ITF weakening is not directly associated with the changes of the trade winds in the Pacific into the future, and the reduction of deep upwelling in the Pacific basin is mainly responsible for the ITF weakening. There is a need to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29458900','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29458900"><span>Inter-<span class="hlt">observer</span> <span class="hlt">variability</span> in fetal biometric measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kilani, Rami; Aleyadeh, Wesam; Atieleh, Luay Abu; Al Suleimat, Abdul Mane; Khadra, Maysa; Hawamdeh, Hassan M</p> <p>2018-02-01</p> <p>To evaluate inter-<span class="hlt">observer</span> <span class="hlt">variability</span> and reproducibility of ultrasound measurements for fetal biometric parameters. A prospective cohort study was implemented in two tertiary care hospitals in Amman, Jordan; Prince Hamza Hospital and Albashir Hospital. 192 women with a singleton pregnancy at a gestational age of 18-36 weeks were the participants in the study. Transabdominal scans for fetal biometric parameter measurement were performed on study participants from the period of November 2014 to March 2015. Women who agreed to participate in the study were administered two ultrasound scans for head circumference, abdominal circumference and femur length. The correlation coefficient was calculated. Bland-Altman plots were used to analyze the degree of measurement agreement between <span class="hlt">observers</span>. Limits of agreement ± 2 SD for the differences in fetal biometry measurements in proportions of the mean of the measurements were derived. Main outcome measures examine the reproducibility of fetal biometric measurements by different <span class="hlt">observers</span>. High inter-<span class="hlt">observer</span> inter-class correlation coefficient (ICC) was found for femur length (0.990) and abdominal circumference (0.996) where Bland-Altman plots showed high degrees of agreement. The highest degrees of agreement were noted in the measurement of abdominal circumference followed by head circumference. The lowest degree of agreement was found for femur length measurement. We used a paired-sample t-test and found that the mean difference between duplicate measurements was not significant (P > 0.05). Biometric fetal parameter measurements may be reproducible by different operators in the clinical setting with similar results. Fetal head circumference, abdominal circumference and femur length were highly reproducible. Large organized studies are needed to ensure accurate fetal measurements due to the important clinical implications of inaccurate measurements. Copyright © 2018. Published by Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.2035M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.2035M"><span>Predicting <span class="hlt">decadal</span> trends in cloud droplet number concentration using reanalysis and satellite data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McCoy, Daniel T.; Bender, Frida A.-M.; Grosvenor, Daniel P.; Mohrmann, Johannes K.; Hartmann, Dennis L.; Wood, Robert; Field, Paul R.</p> <p>2018-02-01</p> <p>Cloud droplet number concentration (CDNC) is the key state <span class="hlt">variable</span> that moderates the relationship between aerosol and the radiative forcing arising from aerosol-cloud interactions. Uncertainty related to the effect of anthropogenic aerosol on cloud properties represents the largest uncertainty in total anthropogenic radiative forcing. Here we show that regionally averaged time series of the Moderate-Resolution Imaging Spectroradiometer (MODIS) <span class="hlt">observed</span> CDNC of low, liquid-topped clouds is well predicted by the MERRA2 reanalysis near-surface sulfate mass concentration over <span class="hlt">decadal</span> timescales. A multiple linear regression between MERRA2 reanalyses masses of sulfate (SO4), black carbon (BC), organic carbon (OC), sea salt (SS), and dust (DU) shows that CDNC across many different regimes can be reproduced by a simple power-law fit to near-surface SO4, with smaller contributions from BC, OC, SS, and DU. This confirms previous work using a less sophisticated retrieval of CDNC on monthly timescales. The analysis is supported by an examination of remotely sensed sulfur dioxide (SO2) over maritime volcanoes and the east coasts of North America and Asia, revealing that maritime CDNC responds to changes in SO2 as <span class="hlt">observed</span> by the ozone monitoring instrument (OMI). This investigation of aerosol reanalysis and top-down remote-sensing <span class="hlt">observations</span> reveals that emission controls in Asia and North America have decreased CDNC in their maritime outflow on a <span class="hlt">decadal</span> timescale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=hormone&pg=3&id=EJ929082','ERIC'); return false;" href="https://eric.ed.gov/?q=hormone&pg=3&id=EJ929082"><span>Puberty and Its Measurement: A <span class="hlt">Decade</span> in Review</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Dorn, Lorah D.; Biro, Frank M.</p> <p>2011-01-01</p> <p>Since the early 1980s, the focus on the importance of puberty to adolescent development has continued with <span class="hlt">variability</span> in the methodology selected to measure puberty. To capture the relevant and important issues regarding the measurement of puberty in the last <span class="hlt">decade</span>, this paper will address (1) the neuroendocrine aspects of puberty and its…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020039168','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020039168"><span><span class="hlt">Variability</span> and Predictability of Land-Atmosphere Interactions: <span class="hlt">Observational</span> and Modeling Studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roads, John; Oglesby, Robert; Marshall, Susan; Robertson, Franklin R.</p> <p>2002-01-01</p> <p>The overall goal of this project is to increase our understanding of seasonal to interannual <span class="hlt">variability</span> and predictability of atmosphere-land interactions. The project objectives are to: 1. Document the low frequency <span class="hlt">variability</span> in land surface features and associated water and energy cycles from general circulation models (GCMs), <span class="hlt">observations</span> and reanalysis products. 2. Determine what relatively wet and dry years have in common on a region-by-region basis and then examine the physical mechanisms that may account for a significant portion of the <span class="hlt">variability</span>. 3. Develop GCM experiments to examine the hypothesis that better knowledge of the land surface enhances long range predictability. This investigation is aimed at evaluating and predicting seasonal to interannual <span class="hlt">variability</span> for selected regions emphasizing the role of land-atmosphere interactions. Of particular interest are the relationships between large, regional and local scales and how they interact to account for seasonal and interannual <span class="hlt">variability</span>, including extreme events such as droughts and floods. North and South America, including the Global Energy and Water Cycle Experiment Continental International Project (GEWEX GCIP), MacKenzie, and LBA basins, are currently being emphasized. We plan to ultimately generalize and synthesize to other land regions across the globe, especially those pertinent to other GEWEX projects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22281878','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22281878"><span>Critical discussion of evaluation parameters for inter-<span class="hlt">observer</span> <span class="hlt">variability</span> in target definition for radiation therapy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fotina, I; Lütgendorf-Caucig, C; Stock, M; Pötter, R; Georg, D</p> <p>2012-02-01</p> <p>Inter-<span class="hlt">observer</span> studies represent a valid method for the evaluation of target definition uncertainties and contouring guidelines. However, data from the literature do not yet give clear guidelines for reporting contouring <span class="hlt">variability</span>. Thus, the purpose of this work was to compare and discuss various methods to determine <span class="hlt">variability</span> on the basis of clinical cases and a literature review. In this study, 7 prostate and 8 lung cases were contoured on CT images by 8 experienced <span class="hlt">observers</span>. Analysis of <span class="hlt">variability</span> included descriptive statistics, calculation of overlap measures, and statistical measures of agreement. Cross tables with ratios and correlations were established for overlap parameters. It was shown that the minimal set of parameters to be reported should include at least one of three volume overlap measures (i.e., generalized conformity index, Jaccard coefficient, or conformation number). High correlation between these parameters and scatter of the results was <span class="hlt">observed</span>. A combination of descriptive statistics, overlap measure, and statistical measure of agreement or reliability analysis is required to fully report the interrater <span class="hlt">variability</span> in delineation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC31H1204F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC31H1204F"><span>Comprehensive Evaluation of 1850-2100 Active Layer Thickness and Thawing Index <span class="hlt">Variability</span> across the Northern Hemisphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frauenfeld, O. W.; Peng, X.; Zhang, T.</p> <p>2016-12-01</p> <p>Both the thawing index (TI) and active layer thickness (ALT) can be useful indicators of climate change in cold regions and have important implications for various surface-atmosphere interactions. Here, we analyze the spatial and temporal <span class="hlt">variability</span> of the Northern Hemisphere TI and ALT under historical and projected climate change. We combine gridded and station-based <span class="hlt">observations</span> to assess the multi-model ensemble mean of 16 of the Coupled Model Intercomparison Project phase 5 (CMIP5) models over 1850-2005. The TI and ALT are assessed based on 1901-2014 Climatic Research Unit (CRU) data, and <span class="hlt">observational</span> ALT from 348 station locations across the Northern Hemisphere. We then employ three representative concentration pathways (RCP 2.6, 4.5, and 8.5) from the same CMIP5 multi-model ensemble means to evaluate changes for 2006-2100. Over the historical period, the TI varies from 0-11,000°C-days in the Northern Hemisphere, and we find good agreement between CMIP5 models and CRU data; however, the models generally underestimate <span class="hlt">observed</span> TI and its long-term trends. Over the 2006-2100 period, the multi-model ensemble averaged TI increases significantly for all three RCPs, ranging from 1.5°C-days/yr for RCP 2.6, to 14°C-days/yr for RCP 8.5. The spatial variations in ALT from <span class="hlt">observing</span> stations exhibit significant <span class="hlt">variability</span> and generally range from 80-320 cm across the Northern Hemisphere, with some extreme values of 900 cm in the European Alps. Calculating <span class="hlt">observational</span> ALT for 1971-2000 from CRU, we find lower values (30-650 cm). The CMIP5 climatology agrees well with the CRU estimates. ALT trends over the <span class="hlt">observational</span> period are generally less than 1.5 cm/<span class="hlt">decade</span>, but as high as 3 cm/<span class="hlt">decade</span> in some isolated regions. While this general trend magnitude agrees with that from CMIP5, the multi-model ensemble underestimates trends and exhibits much less spatial <span class="hlt">variability</span>. Projected trends range from 0.77 cm/<span class="hlt">decade</span> in RCP 2.6, to 6.5 cm/<span class="hlt">decade</span> in RCP 8.5 in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120016294','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120016294"><span>Multi-<span class="hlt">Decadal</span> Change of Atmospheric Aerosols and Their Effect on Surface Radiation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chin, Mian; Diehl, Thomas; Tan, Qian; Wild, Martin; Qian, Yun; Yu, Hongbin; Bian, Huisheng; Wang, Weiguo</p> <p>2012-01-01</p> <p>We present an investigation on multi-<span class="hlt">decadal</span> changes of atmospheric aerosols and their effects on surface radiation using a global chemistry transport model along with the near-term to long-term data records. We focus on a 28-year time period of satellite era from 1980 to 2007, during which a suite of aerosol data from satellite <span class="hlt">observations</span> and ground-based remote sensing and in-situ measurements have become available. We analyze the long-term global and regional aerosol optical depth and concentration trends and their relationship to the changes of emissions" and assess the role aerosols play in the multi-<span class="hlt">decadal</span> change of solar radiation reaching the surface (known as "dimming" or "brightening") at different regions of the world, including the major anthropogenic source regions (North America, Europe, Asia) that have been experiencing considerable changes of emissions, dust and biomass burning regions that have large interannual <span class="hlt">variabilities</span>, downwind regions that are directly affected by the changes in the source area, and remote regions that are considered to representing "background" conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020068102&hterms=Ph&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DPh','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020068102&hterms=Ph&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DPh"><span>Understanding the Long-Term Spectral <span class="hlt">Variability</span> of Cygnus X-1 from BATSE and ASM <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zdziarski, Andrzej A.; Poutanen, Juri; Paciesas, William S.; Wen, Linqing; Six, N. Frank (Technical Monitor)</p> <p>2002-01-01</p> <p>We present a spectral analysis of <span class="hlt">observations</span> of Cygnus X-1 by the RXTE/ASM (1.5-12 keV) and CGRO/BATSE (20-300 keV), including about 1200 days of simultaneous data. We find a number of correlations between intensities and hardnesses in different energy bands from 1.5 keV to 300 keV. In the hard (low) spectral state, there is a negative correlation between the ASM 1.5-12 keV flux and the hardness at any energy. In the soft (high) spectral state, the ASM flux is positively correlated with the ASM hardness (as previously reported) but uncorrelated with the BATSE hardness. In both spectral states, the BATSE hardness correlates with the flux above 100 keV, while it shows no correlation with the flux in the 20-100 keV range. At the same time, there is clear correlation between the BATSE fluxes below and above 100 keV. In the hard state, most of the <span class="hlt">variability</span> can be explained by softening the overall spectrum with a pivot at approximately 50 keV. The <span class="hlt">observations</span> show that there has to be another, independent <span class="hlt">variability</span> pattern of lower amplitude where the spectral shape does not change when the luminosity changes. In the soft state, the <span class="hlt">variability</span> is mostly caused by a <span class="hlt">variable</span> hard (Comptonized) spectral component of a constant shape superimposed on a constant soft blackbody component. These <span class="hlt">variability</span> patterns are in agreement with the dependence of the rms <span class="hlt">variability</span> on the photon energy in the two states. We interpret the <span class="hlt">observed</span> correlations in terms of theoretical Comptonization models. In the hard state, the <span class="hlt">variability</span> appears to be driven mostly by changing flux in seed photons Comptonized in a hot thermal plasma cloud with an approximately constant power supply. In the soft state, the <span class="hlt">variability</span> is consistent with flares of hybrid, thermal/nonthermal, plasma with <span class="hlt">variable</span> power above a stable cold disk. Also, based on broadband pointed <span class="hlt">observations</span> simultaneous with those of the ASM and BATSE, we find the intrinsic bolometric luminosity increases by a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1165903-variable-hard-ray-emission-ngc-observed-nustar','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1165903-variable-hard-ray-emission-ngc-observed-nustar"><span>The <span class="hlt">Variable</span> Hard X-Ray Emission of NGC 4945 as <span class="hlt">Observed</span> by NUSTAR</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Puccetti, Simonetta; Comastri, Andrea; Fiore, Fabrizio; ...</p> <p>2014-09-02</p> <p>Here, we present a broadband (~0.5-79 keV) spectral and temporal analysis of multiple NuSTAR <span class="hlt">observations</span> combined with archival Suzaku and Chandra data of NGC 4945, the brightest extragalactic source at 100 keV. We <span class="hlt">observe</span> hard X-ray (>10 keV) flux and spectral <span class="hlt">variability</span>, with flux variations of a factor of two on timescales of 20 ks. A <span class="hlt">variable</span> primary continuum dominates the high-energy spectrum (>10 keV) in all states, while the reflected/scattered flux that dominates at E <10 keV stays approximately constant. From modeling the complex reflection/transmission spectrum, we derive a Compton depth along the line of sight of τThomson ~more » 2.9, and a global covering factor for the circumnuclear gas of ~0.15. This agrees with the constraints derived from the high-energy <span class="hlt">variability</span>, which implies that most of the high-energy flux is transmitted rather than Compton-scattered. This demonstrates the effectiveness of spectral analysis at constraining the geometric properties of the circumnuclear gas, and validates similar methods used for analyzing the spectra of other bright, Compton-thick active galactic nuclei (AGNs). The lower limits on the e-folding energy are between 200 and 300 keV, consistent with previous BeppoSAX, Suzaku, and Swift Burst Alert Telescope <span class="hlt">observations</span>. The accretion rate, estimated from the X-ray luminosity and assuming a bolometric correction typical of type 2 AGN, is in the range ~0.1-0.3 λEdd depending on the flux state. As a result, the substantial <span class="hlt">observed</span> X-ray luminosity <span class="hlt">variability</span> of NGC 4945 implies that large errors can arise from using single-epoch X-ray data to derive L/L Edd values for obscured AGNs.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913474C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913474C"><span>A <span class="hlt">decade</span> of infrared versus visible AOD analysis within the dust belt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Capelle, Virginie; Chédin, Alain; Pondrom, Marc; Crevoisier, Cyril; Armante, Raymond; Crépeau, Laurent; Scott, Noëlle</p> <p>2017-04-01</p> <p>Aerosols represent one of the dominant uncertainties in radiative forcing, partly because of their very high spatiotemporal <span class="hlt">variability</span>, a still insufficient knowledge of their microphysical and optical properties, or of their vertical distribution. A better understanding and forecasting of their impact on climate therefore requires precise <span class="hlt">observations</span> of dust emission and transport. <span class="hlt">Observations</span> from space offer a good opportunity to follow, day by day and at high spatial resolution, dust evolution at global scale and over long time series. In this context, infrared <span class="hlt">observations</span>, by allowing retrieving simultaneously dust optical depth (AOD) as well as the mean dust layer altitude, daytime and nighttime, over oceans and over continents, in particular over desert, appears highly complementary to <span class="hlt">observations</span> in the visible. In this study, a <span class="hlt">decade</span> of infrared <span class="hlt">observations</span> (Metop-A/IASI and AIRS/AQUA) has been processed pixel by pixel, using a "Look-Up-Table" (LUT) physical approach. The retrieved infrared 10µm coarse-mode AOD is compared with the Spectral Deconvolution Algorithm (SDA) 500nm coarse mode AOD <span class="hlt">observed</span> at 50 ground-based Aerosol RObotic NETwork (AERONET) sites located within the dust belt. Analyzing their brings into evidence an important geographical <span class="hlt">variability</span>. Lowest values are found close to dust sources ( 0.45 for the Sahel or Arabian Peninsula, 0.6-0.7 for the Northern part of Africa or India), whereas the ratio increases for transported dust with values of 0.9-1 for the Caribbean and for the Mediterranean basin. This <span class="hlt">variability</span> is interpreted as a marker of clays abundance, and might be linked to the dust particle illite to kaolinite ratio, a recognized tracer of dust sources and transport. More generally, it suggests that the difference between the radiative impact of dust aerosols in the visible and in the infrared depends on the type of particles <span class="hlt">observed</span>. This highlights the importance of taking into account the specificity of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7429S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7429S"><span>Interannual <span class="hlt">variability</span> (1979-2013) of the North-Western Mediterranean deep water mass formation: past <span class="hlt">observation</span> reanalysis and coupled ocean-atmosphere high-resolution modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Somot, Samuel; Houpert, Loic; Sevault, Florence; Testor, Pierre; Bosse, Anthony; Durrieu de Madron, Xavier; Dubois, Clotilde; Herrmann, Marine; Waldman, Robin; Bouin, Marie-Noëlle; Cassou, Christophe</p> <p>2015-04-01</p> <p>The North-Western Mediterranean Sea is known as one of the only place in the world where open-sea deep convection occurs (often up to more than 2000m) with the formation of the Western Mediterranean Deep Water (WMDW). This phenomena is mostly driven by local preconditioning of the water column and strong buoyancy losses during Winter. At the event scale, the WMDW formation is characterized by different phases (preconditioning, strong mixing, restratification and spreading), intense air-sea interaction and strong meso-scale activity but, on a longer time scale, it also shows a large interannual <span class="hlt">variability</span> and may be strongly affected by climate change with impact on the regional biogeochemistry. Therefore <span class="hlt">observing</span>, simulating and understanding the long-term temporal <span class="hlt">variability</span> of the North-Western Mediterranean deep water formation is still today a very challenging task. We try here to tackle those issues thanks to (1) a thorough reanalysis of past in-situ <span class="hlt">observations</span> (CTD, Argo, surface and deep moorings, gliders) and (2) an ERA-Interim driven simulation using a recently-developed fully coupled Regional Climate System Model (CNRM-RCSM4, Sevault et al. 2014). The multi-<span class="hlt">decadal</span> simulation (1979-2013) is designed to be temporally and spatially homogeneous with a realistic chronology, a high resolution representation of both the regional ocean and atmosphere, specific initial conditions, a long-term spin-up and a full ocean-atmosphere coupling without constraint at the air-sea interface. The <span class="hlt">observation</span> reanalysis allows to reconstruct interannual time series of deep water formation indicators (ocean surface <span class="hlt">variables</span>, mixed layer depth, surface of the convective area, dense water volumes and characteristics of the deep water). Using the <span class="hlt">observation</span>-based indicators and the model outputs, the 34 Winters of the period 1979-2013 are analysed in terms of weather regimes, related Winter air-sea fluxes, ocean preconditioning, mixed layer depth, surface of the convective</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PrOce.152...15T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PrOce.152...15T"><span>Managing living marine resources in a dynamic environment: The role of seasonal to <span class="hlt">decadal</span> climate forecasts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tommasi, Desiree; Stock, Charles A.; Hobday, Alistair J.; Methot, Rick; Kaplan, Isaac C.; Eveson, J. Paige; Holsman, Kirstin; Miller, Timothy J.; Gaichas, Sarah; Gehlen, Marion; Pershing, Andrew; Vecchi, Gabriel A.; Msadek, Rym; Delworth, Tom; Eakin, C. Mark; Haltuch, Melissa A.; Séférian, Roland; Spillman, Claire M.; Hartog, Jason R.; Siedlecki, Samantha; Samhouri, Jameal F.; Muhling, Barbara; Asch, Rebecca G.; Pinsky, Malin L.; Saba, Vincent S.; Kapnick, Sarah B.; Gaitan, Carlos F.; Rykaczewski, Ryan R.; Alexander, Michael A.; Xue, Yan; Pegion, Kathleen V.; Lynch, Patrick; Payne, Mark R.; Kristiansen, Trond; Lehodey, Patrick; Werner, Francisco E.</p> <p>2017-03-01</p> <p>Recent developments in global dynamical climate prediction systems have allowed for skillful predictions of climate <span class="hlt">variables</span> relevant to living marine resources (LMRs) at a scale useful to understanding and managing LMRs. Such predictions present opportunities for improved LMR management and industry operations, as well as new research avenues in fisheries science. LMRs respond to climate <span class="hlt">variability</span> via changes in physiology and behavior. For species and systems where climate-fisheries links are well established, forecasted LMR responses can lead to anticipatory and more effective decisions, benefitting both managers and stakeholders. Here, we provide an overview of climate prediction systems and advances in seasonal to <span class="hlt">decadal</span> prediction of marine-resource relevant environmental <span class="hlt">variables</span>. We then describe a range of climate-sensitive LMR decisions that can be taken at lead-times of months to <span class="hlt">decades</span>, before highlighting a range of pioneering case studies using climate predictions to inform LMR decisions. The success of these case studies suggests that many additional applications are possible. Progress, however, is limited by <span class="hlt">observational</span> and modeling challenges. Priority developments include strengthening of the mechanistic linkages between climate and marine resource responses, development of LMR models able to explicitly represent such responses, integration of climate driven LMR dynamics in the multi-driver context within which marine resources exist, and improved prediction of ecosystem-relevant <span class="hlt">variables</span> at the fine regional scales at which most marine resource decisions are made. While there are fundamental limits to predictability, continued advances in these areas have considerable potential to make LMR managers and industry decision more resilient to climate <span class="hlt">variability</span> and help sustain valuable resources. Concerted dialog between scientists, LMR managers and industry is essential to realizing this potential.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C11C..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C11C..05F"><span>A <span class="hlt">Decade</span> of Arctic Sea Ice Thickness Change from Airborne and Satellite Altimetry (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farrell, S. L.; Richter-Menge, J.; Kurtz, N. T.; McAdoo, D. C.; Newman, T.; Zwally, H.; Ruth, J.</p> <p>2013-12-01</p> <p>Altimeters on both airborne and satellite platforms provide direct measurements of sea ice freeboard from which sea ice thickness may be calculated. Satellite altimetry <span class="hlt">observations</span> of Arctic sea ice from ICESat and CryoSat-2 indicate a significant decline in ice thickness, and volume, over the last <span class="hlt">decade</span>. During this time the ice pack has experienced a rapid change in its composition, transitioning from predominantly thick, multi-year ice to thinner, increasingly seasonal ice. We will discuss the regional trends in ice thickness derived from ICESat and IceBridge altimetry between 2003 and 2013, contrasting <span class="hlt">observations</span> of the multi-year ice pack with seasonal ice zones. ICESat ceased operation in 2009, and the final, reprocessed data set became available recently. We extend our analysis to April 2013 using data from the IceBridge airborne mission, which commenced operations in 2009. We describe our current efforts to more accurately convert from freeboard to ice thickness, with a modified methodology that corrects for range errors, instrument biases, and includes an enhanced treatment of snow depth, with respect to ice type. With the planned launch by NASA of ICESat-2 in 2016 we can expect continuity of the sea ice thickness time series through the end of this <span class="hlt">decade</span>. Data from the ICESat-2 mission, together with ongoing <span class="hlt">observations</span> from CryoSat-2, will allow us to understand both the <span class="hlt">decadal</span> trends and inter-annual <span class="hlt">variability</span> in the Arctic sea ice thickness record. We briefly present the status of planned ICESat-2 sea ice data products, and demonstrate the utility of micro-pulse, photon-counting laser altimetry over sea ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC41A0995R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC41A0995R"><span>Impact of natural <span class="hlt">variability</span> on the perception of climate change for the upcoming <span class="hlt">decades</span>: Analysis of the CanESM2-LE and CESM-LE large ensembles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rondeau-Genesse, G.; Braun, M.; Chaumont, D.</p> <p>2017-12-01</p> <p>The pace of climate change can have a direct impact on the efforts required to adapt. However, for relatively short time scales, this pace can be masked by natural <span class="hlt">variability</span> (NV). In some cases, this <span class="hlt">variability</span> might cause, for a few <span class="hlt">decades</span>, climate change to exceed what would be expected from the greenhouse gas (GHG) emissions alone or, to the contrary, it might cause slowdowns or even hiatuses. This phenomenon is difficult to explore using ensembles such as CMIP5, which are composed of multiple climatological models and thus combine both NV and inter-model differences. This study analyses CanESM2-LE and CESM-LE, two state-of-the-art large ensembles (LE) comprised of multiple realizations from a single climatological model and a single GHG emission scenario. We explore the relationship between NV and climate change over the next few <span class="hlt">decades</span> in Canada and the United States. Temperature indices, namely the mean annual temperature and the 3-day maximum and minimum temperatures are assessed. Results indicate that under the RCP8.5, temperatures within most of the individual large ensemble members will increase in a roughly linear manner between 2021 and 2060. Nevertheless, in some regions such as parts of Canada and Alaska, there is a 20 to 35% probability that the temperature increase will slow down between 2021 and 2040. Such a slowdown in warming temperatures would provide some leeway for adaptation projects, but this phenomenon is caused by NV alone and, as such, is only temporary. Indeed, members of the large ensembles where a slowdown of warming is found during the 2021-2040 period are two to five times more likely to experience a period of very fast warming in the following <span class="hlt">decades</span>. The opposite scenario, where the changes expected by 2050 would occur early because of NV, remains fairly uncommon for the mean annual temperature. For the extreme temperature indices however, this early warming still occurs in 5 to 20% of the large ensemble members. As such</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711910C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711910C"><span><span class="hlt">Observations</span> of changes in the dissolved CO2 system in the North Sea, in four summers of the 2001-2011 <span class="hlt">decade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clargo, Nicola; Salt, Lesley; Thomas, Helmuth; de Baar, Hein</p> <p>2015-04-01</p> <p>Since the industrial revolution, atmospheric concentrations of carbon dioxide (CO2) have risen dramatically, largely due to the combustion of fossil fuels, changes in land-use patterns and the production of cement. The oceans have absorbed a large amount of this CO2, with resulting impacts on ocean chemistry. Coastal seas play a significant role in the mitigation of anthropogenic atmospheric CO2 as they contribute approximately 10-30% of global primary productivity despite accounting for only 7% of the surface area. The North Sea is a perfect natural laboratory in which to study the CO2 system as it consists of two biogeochemically distinct regions displaying both oceanic and relatively coastal behaviour. It has also been identified as a continental shelf pump with respect to CO2, transporting it to the deeper waters of the North Atlantic. Large scale forcing has been shown to have a significant impact on the CO2 system over varying time scales, often masking the effects of anthropogenic influence. Here, we present data from the North Sea spanning the 2001-2011 <span class="hlt">decade</span>. In order to investigate the dynamics of the dissolved CO2 system in this region in the face of climate change, four basin-wide cruises were conducted during the summers of 2001, 2005, 2008 and 2011. The acquired Dissolved Inorganic Carbon (DIC) and alkalinity data were then used to fully resolve the carbon system in order to assess trends over the 2001-2011 <span class="hlt">decade</span>. We find significant interannual <span class="hlt">variability</span>, but with a consistent, notable trend in decreasing pH. We found that surface alkalinity remained relatively constant over the <span class="hlt">decade</span>, whereas DIC increased, indicating that the pH decline is DIC-driven. We also found that the partial pressure of CO2 (pCO2) increased faster than concurrent atmospheric CO2 concentrations, and that the CO2 buffering capacity of the North Sea decreased over the <span class="hlt">decade</span>, with implications for future CO2 uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P54C..05K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P54C..05K"><span>Correlating Solar Wind Modulation with Ionospheric <span class="hlt">Variability</span> at Mars from MEX and MAVEN <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kopf, A. J.; Morgan, D. D.; Halekas, J. S.; Ruhunusiri, S.; Gurnett, D. A.; Connerney, J. E. P.</p> <p>2017-12-01</p> <p>The synthesis of <span class="hlt">observations</span> by the Mars Express and Mars Atmosphere and Volatiles Evolution (MAVEN) spacecraft allows for a unique opportunity to study <span class="hlt">variability</span> in the Martian ionosphere from multiple perspectives. One major source for this <span class="hlt">variability</span> is the solar wind. Due to its elliptical orbit which precesses over time, MAVEN periodically spends part of its orbit outside the Martian bow shock, allowing for direct measurements of the solar wind impacting the Martian plasma environment. When the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument aboard Mars Express is simultaneously sounding the ionosphere, the influence from changes in the solar wind can be <span class="hlt">observed</span>. Previous studies have suggested a positive correlation, connecting ionospheric density to the solar wind proton flux, but depended on Earth-based measurements for solar wind conditions. More recently, research has indicated that <span class="hlt">observations</span> of ionospheric <span class="hlt">variability</span> from these two spacecraft can be connected in special cases, such as shock wave impacts or specific solar wind magnetic field orientations. Here we extend this to more general solar wind conditions and examine how changes in the solar wind properties measured by MAVEN instruments correlate with ionospheric structure and dynamics <span class="hlt">observed</span> simultaneously in MARSIS remote and local measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2688L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2688L"><span>Untangling the causes a <span class="hlt">decadal</span>-scale drought: a case study in southeast Australia.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, Sophie; Gallant, Ailie</p> <p>2017-04-01</p> <p>Prolonged droughts on the order of multiple years to a <span class="hlt">decade</span> have recently afflicted many parts of highly populated regions around the globe, for example, the southwest United States and southeast Australia. However, the causes of these droughts remain unclear. A significant contribution from natural <span class="hlt">decadal</span>-scale climate <span class="hlt">variability</span> is likely, but there is also conflicting evidence of any contribution from anthropogenic climate change. This work aims to untangle the causes of a 13-year drought in southeast Australia spanning 1997-2009. A suite of historical and control simulations from fully coupled GCMs contained in the CMIP5 archive are employed, and the potential contributions of random climate <span class="hlt">variability</span>, SST forcing and anthropogenic forcing to the drought are examined. It is likely that random, <span class="hlt">decadal</span>-scale <span class="hlt">variability</span> played a significant role in producing the prolonged rainfall deficits across southeast Australia. These were reinforced by several years with El Niño-like conditions, which commonly induce drought in the region, and a lack of La Niña conditions, which are more likely to bring rain. Evidence of contribution of anthropogenic forcing to the drought is limited</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2721A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2721A"><span><span class="hlt">Decadal</span> variations in atmospheric water vapor time series estimated using GNSS, ERA-Interim, and synoptic data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alshawaf, Fadwa; Dick, Galina; Heise, Stefan; Balidakis, Kyriakos; Schmidt, Torsten; Wickert, Jens</p> <p>2017-04-01</p> <p>Ground-based GNSS (Global Navigation Satellite Systems) have efficiently been used since the 1990s as a meteorological <span class="hlt">observing</span> system. Recently scientists used GNSS time series of precipitable water vapor (PWV) for climate research although they may not be sufficiently long. In this work, we compare the trend estimated from GNSS time series with that estimated from European Center for Medium-RangeWeather Forecasts Reanalysis (ERA-Interim) data and meteorological measurements.We aim at evaluating climate evolution in Central Europe by monitoring different atmospheric <span class="hlt">variables</span> such as temperature and PWV. PWV time series were obtained by three methods: 1) estimated from ground-based GNSS <span class="hlt">observations</span> using the method of precise point positioning, 2) inferred from ERA-Interim data, and 3) determined based on daily surface measurements of temperature and relative humidity. The other <span class="hlt">variables</span> are available from surface meteorological stations or received from ERA-Interim. The PWV trend component estimated from GNSS data strongly correlates (>70%) with that estimated from the other data sets. The linear trend is estimated by straight line fitting over 30 years of seasonally-adjusted PWV time series obtained using the meteorological measurements. The results show a positive trend in the PWV time series with an increase of 0.2-0.7 mm/<span class="hlt">decade</span> with a mean standard deviations of 0.016 mm/<span class="hlt">decade</span>. In this paper, we present the results at three GNSS stations. The temporal increment of the PWV correlates with the temporal increase in the temperature levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9695L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9695L"><span>Evaluation of Oceanic Surface <span class="hlt">Observation</span> for Reproducing the Upper Ocean Structure in ECHAM5/MPI-OM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Hao; Zheng, Fei; Zhu, Jiang</p> <p>2017-12-01</p> <p>Better constraints of initial conditions from data assimilation are necessary for climate simulations and predictions, and they are particularly important for the ocean due to its long climate memory; as such, ocean data assimilation (ODA) is regarded as an effective tool for seasonal to <span class="hlt">decadal</span> predictions. In this work, an ODA system is established for a coupled climate model (ECHAM5/MPI-OM), which can assimilate all available oceanic <span class="hlt">observations</span> using an ensemble optimal interpolation approach. To validate and isolate the performance of different surface <span class="hlt">observations</span> in reproducing air-sea climate variations in the model, a set of <span class="hlt">observing</span> system simulation experiments (OSSEs) was performed over 150 model years. Generally, assimilating sea surface temperature, sea surface salinity, and sea surface height (SSH) can reasonably reproduce the climate <span class="hlt">variability</span> and vertical structure of the upper ocean, and assimilating SSH achieves the best results compared to the true states. For the El Niño-Southern Oscillation (ENSO), assimilating different surface <span class="hlt">observations</span> captures true aspects of ENSO well, but assimilating SSH can further enhance the accuracy of ENSO-related feedback processes in the coupled model, leading to a more reasonable ENSO evolution and air-sea interaction over the tropical Pacific. For ocean heat content, there are still limitations in reproducing the long time-scale <span class="hlt">variability</span> in the North Atlantic, even if SSH has been taken into consideration. These results demonstrate the effectiveness of assimilating surface <span class="hlt">observations</span> in capturing the interannual signal and, to some extent, the <span class="hlt">decadal</span> signal but still highlight the necessity of assimilating profile data to reproduce specific <span class="hlt">decadal</span> <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5987L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5987L"><span>A <span class="hlt">Decadal</span>-scale Air-sea Interaction Theory for North Atlantic Multidecadal <span class="hlt">Variability</span>: the NAT-NAO-AMOC-AMO Coupled Mode and Its Remote Influences</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Jianping; Sun, Cheng; Jin, Fei-Fei</p> <p>2017-04-01</p> <p>ABSTRACT North Atlantic region shows prominent multidecadal <span class="hlt">variability</span>. <span class="hlt">Observational</span> analysis shows that the North Atlantic Oscillation (NAO) leads the oceanic Atlantic Multidecadal Oscillation (AMO) by 15-20 years and the latter also leads the former by around 15 years. The mechanisms are investigated using simulations from a fully coupled model, and a NATNAO-AMOC-AMO Coupled Mode is proposed to explain the multidecadal <span class="hlt">variability</span> in North Atlantic region. The NAT-NAO-AMO-AMOC coupled mode has important remote influences on regional climates. <span class="hlt">Observational</span> analysis identifies a significant in-phase relationship between the AMV and Siberian warm season (May to October) precipitation. The physical mechanism for this relationship is investigated using both <span class="hlt">observations</span> and numerical simulations. North Atlantic sea surface temperature (SST) warming associated with the positive AMV phase can excite an eastward propagating wave train response across the entire Eurasian continent, which includes an east-west dipole structure over Siberia. The dipole then leads to anomalous southerly winds bringing moisture northward to Siberia; the precipitation increases correspondingly. Furthermore, a prominent teleconnection pattern of multidecadal <span class="hlt">variability</span> of cold season (November to April) upper-level atmospheric circulation over North Africa and Eurasia (NA-EA) is revealed by empirical orthogonal function analysis of the Twentieth Century Reanalysis data, and this teleconnection pattern is referred to as the Africa-Asia multidecadal teleconnection pattern (AAMT). A strong inphase relationship is <span class="hlt">observed</span> between the AAMT and Atlantic multidecadal <span class="hlt">variability</span> (AMV) and this connection is mainly due to Rossby wave dynamics. The AAMT acts as an atmospheric bridge conveying the influence of AMV onto the downstream multidecadal climate <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.H54D..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.H54D..03F"><span>Assimilating a <span class="hlt">decade</span> of hydrometeorological ship measurements across the North American Great Lakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fries, K. J.; Kerkez, B.</p> <p>2015-12-01</p> <p>We use a <span class="hlt">decade</span> of measurements made by the Volunteer <span class="hlt">Observing</span> Ships (VOS) program on the North American Great Lakes to derive spatial estimates of over-lake air temperature, sea surface temperature, dewpoint, and wind speed. This Lagrangian data set, which annually comprises over 200,000 point <span class="hlt">observations</span> from over 80,000 ship reports across a 244,000 square kilometer study area, is assimilated using a Gaussian Process machine learning algorithm. This algorithm classifies a model for each hydrometeorological <span class="hlt">variable</span> using a combination of latitudes, longitudes, seasons of the year, as well as predictions made by the National Digital Forecast Database (NDFD) and Great Lakes Coastal Forecasting System (GLCFS) operational models. We show that our data-driven method significantly improves the spatial and temporal estimation of overlake hydrometeorological <span class="hlt">variables</span>, while simultaneously providing uncertainty estimates that can be used to improve historical and future predictions on dense spatial and temporal scales. This method stands to improve the prediction of water levels on the Great Lakes, which comprise over 90% of America's surface fresh water, and impact the lives of millions of people living in the basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29623683','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29623683"><span>Essential ocean <span class="hlt">variables</span> for global sustained <span class="hlt">observations</span> of biodiversity and ecosystem changes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Miloslavich, Patricia; Bax, Nicholas J; Simmons, Samantha E; Klein, Eduardo; Appeltans, Ward; Aburto-Oropeza, Octavio; Andersen Garcia, Melissa; Batten, Sonia D; Benedetti-Cecchi, Lisandro; Checkley, David M; Chiba, Sanae; Duffy, J Emmett; Dunn, Daniel C; Fischer, Albert; Gunn, John; Kudela, Raphael; Marsac, Francis; Muller-Karger, Frank E; Obura, David; Shin, Yunne-Jai</p> <p>2018-04-05</p> <p>Sustained <span class="hlt">observations</span> of marine biodiversity and ecosystems focused on specific conservation and management problems are needed around the world to effectively mitigate or manage changes resulting from anthropogenic pressures. These <span class="hlt">observations</span>, while complex and expensive, are required by the international scientific, governance and policy communities to provide baselines against which the effects of human pressures and climate change may be measured and reported, and resources allocated to implement solutions. To identify biological and ecological essential ocean <span class="hlt">variables</span> (EOVs) for implementation within a global ocean <span class="hlt">observing</span> system that is relevant for science, informs society, and technologically feasible, we used a driver-pressure-state-impact-response (DPSIR) model. We (1) examined relevant international agreements to identify societal drivers and pressures on marine resources and ecosystems, (2) evaluated the temporal and spatial scales of <span class="hlt">variables</span> measured by 100+ <span class="hlt">observing</span> programs, and (3) analysed the impact and scalability of these <span class="hlt">variables</span> and how they contribute to address societal and scientific issues. EOVs were related to the status of ecosystem components (phytoplankton and zooplankton biomass and diversity, and abundance and distribution of fish, marine turtles, birds and mammals), and to the extent and health of ecosystems (cover and composition of hard coral, seagrass, mangrove and macroalgal canopy). Benthic invertebrate abundance and distribution and microbe diversity and biomass were identified as emerging EOVs to be developed based on emerging requirements and new technologies. The temporal scale at which any shifts in biological systems will be detected will vary across the EOVs, the properties being monitored and the length of the existing time-series. Global implementation to deliver useful products will require collaboration of the scientific and policy sectors and a significant commitment to improve human and infrastructure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ThApC.tmp....4F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ThApC.tmp....4F"><span><span class="hlt">Observed</span> soil temperature trends associated with climate change in the Tibetan Plateau, 1960-2014</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fang, Xuewei; Luo, Siqiong; Lyu, Shihua</p> <p>2018-01-01</p> <p>Soil temperature, an important indicator of climate change, has rarely explored due to scarce <span class="hlt">observations</span>, especially in the Tibetan Plateau (TP) area. In this study, changes <span class="hlt">observed</span> in five meteorological <span class="hlt">variables</span> obtained from the TP between 1960 and 2014 were investigated using two non-parametric methods, the modified Mann-Kendall test and Sen's slope estimator method. Analysis of annual series from 1960 to 2014 has shown that surface (0 cm), shallow (5-20 cm), deep (40-320 cm) soil temperatures (ST), mean air temperature (AT), and precipitation (P) increased with rates of 0.47 °C/<span class="hlt">decade</span>, 0.36 °C/<span class="hlt">decade</span>, 0.36 °C/<span class="hlt">decade</span>, 0.35 °C/<span class="hlt">decade</span>, and 7.36 mm/<span class="hlt">decade</span>, respectively, while maximum frozen soil depth (MFD) as well as snow cover depth (MSD) decreased with rates of 5.58 and 0.07 cm/<span class="hlt">decade</span>. Trends were significant at 99 or 95% confidence level for the <span class="hlt">variables</span>, with the exception of P and MSD. More impressive rate of the ST at each level than the AT indicates the clear response of soil to climate warming on a regional scale. Monthly changes <span class="hlt">observed</span> in surface ST in the past <span class="hlt">decades</span> were consistent with those of AT, indicating a central place of AT in the soil warming. In addition, with the exception of MFD, regional scale increasing trend of P as well as the decreasing MSD also shed light on the mechanisms driving soil trends. Significant negative-dominated correlation coefficients (α = 0.05) between ST and MSD indicate the decreasing MSD trends in TP were attributable to increasing ST, especially in surface layer. Owing to the frozen ground, the relationship between ST and P is complicated in the area. Higher P also induced higher ST, while the inhibition of freeze and thaw process on the ST in summer. With the increasing AT, P accompanied with the decreasing MFD, MSD should be the major factors induced the conspicuous soil warming of the TP in the past <span class="hlt">decades</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JHyd..479...75J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JHyd..479...75J"><span>How well do the GCMs/RCMs capture the multi-scale temporal <span class="hlt">variability</span> of precipitation in the Southwestern United States?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Peng; Gautam, Mahesh R.; Zhu, Jianting; Yu, Zhongbo</p> <p>2013-02-01</p> <p>SummaryMulti-scale temporal <span class="hlt">variability</span> of precipitation has an established relationship with floods and droughts. In this paper, we present the diagnostics on the ability of 16 General Circulation Models (GCMs) from Bias Corrected and Downscaled (BCSD) World Climate Research Program's (WCRP's) Coupled Model Inter-comparison Project Phase 3 (CMIP3) projections and 10 Regional Climate Models (RCMs) that participated in the North American Regional Climate Change Assessment Program (NARCCAP) to represent multi-scale temporal <span class="hlt">variability</span> determined from the <span class="hlt">observed</span> station data. Four regions (Los Angeles, Las Vegas, Tucson, and Cimarron) in the Southwest United States are selected as they represent four different precipitation regions classified by clustering method. We investigate how storm properties and seasonal, inter-annual, and <span class="hlt">decadal</span> precipitation <span class="hlt">variabilities</span> differed between GCMs/RCMs and <span class="hlt">observed</span> records in these regions. We find that current GCMs/RCMs tend to simulate longer storm duration and lower storm intensity compared to those from <span class="hlt">observed</span> records. Most GCMs/RCMs fail to produce the high-intensity summer storms caused by local convective heat transport associated with the summer monsoon. Both inter-annual and <span class="hlt">decadal</span> bands are present in the GCM/RCM-simulated precipitation time series; however, these do not line up to the patterns of large-scale ocean oscillations such as El Nino/La Nina Southern Oscillation (ENSO) and Pacific <span class="hlt">Decadal</span> Oscillation (PDO). Our results show that the studied GCMs/RCMs can capture long-term monthly mean as the examined data is bias-corrected and downscaled, but fail to simulate the multi-scale precipitation <span class="hlt">variability</span> including flood generating extreme events, which suggests their inadequacy for studies on floods and droughts that are strongly associated with multi-scale temporal precipitation <span class="hlt">variability</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AAN...543....1W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AAN...543....1W"><span>20 Cataclysmic <span class="hlt">variables</span> to be <span class="hlt">observed</span> by William Herschel Telescope</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waagen, Elizabeth O.</p> <p>2016-05-01</p> <p>Roque Ruiz-Carmona (Ph.D. candidate, Institute of Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen, The Netherlands) has requested AAVSO assistance with his campaign to <span class="hlt">observe</span> a set of 20 cataclysmic <span class="hlt">variables</span> (CVs) with the William Herschel Telescope (WHT) at La Palma TONIGHT. This campaign is identical in format to the ones successfully carried out by the AAVSO on his behalf in 2015 (AAVSO Alert Notices 524 and 527). The full details of and instructions for this campaign are included here although the first of the two nights for which data are requested has passed. In order for WHT to <span class="hlt">observe</span> each of the targets safely and to maximize the science value of the <span class="hlt">observations</span> obtained, it is essential to know whether they are in outburst or quiescence. To this end, the PI has requested our <span class="hlt">observers</span> to obtain one image of each target on each of TWO separate nights so he may analyze them to determine the final <span class="hlt">observing</span> list for WHT. The images must be taken and posted within a certain window. Links to finder charts as well as reporting instructions and other information may be found in the full Alert Notice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22498628','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22498628"><span>Aerosols implicated as a prime driver of twentieth-century North Atlantic climate <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Booth, Ben B B; Dunstone, Nick J; Halloran, Paul R; Andrews, Timothy; Bellouin, Nicolas</p> <p>2012-04-04</p> <p>Systematic climate shifts have been linked to multidecadal <span class="hlt">variability</span> in <span class="hlt">observed</span> sea surface temperatures in the North Atlantic Ocean. These links are extensive, influencing a range of climate processes such as hurricane activity and African Sahel and Amazonian droughts. The <span class="hlt">variability</span> is distinct from historical global-mean temperature changes and is commonly attributed to natural ocean oscillations. A number of studies have provided evidence that aerosols can influence long-term changes in sea surface temperatures, but climate models have so far failed to reproduce these interactions and the role of aerosols in <span class="hlt">decadal</span> <span class="hlt">variability</span> remains unclear. Here we use a state-of-the-art Earth system climate model to show that aerosol emissions and periods of volcanic activity explain 76 per cent of the simulated multidecadal variance in detrended 1860-2005 North Atlantic sea surface temperatures. After 1950, simulated <span class="hlt">variability</span> is within <span class="hlt">observational</span> estimates; our estimates for 1910-1940 capture twice the warming of previous generation models but do not explain the entire <span class="hlt">observed</span> trend. Other processes, such as ocean circulation, may also have contributed to <span class="hlt">variability</span> in the early twentieth century. Mechanistically, we find that inclusion of aerosol-cloud microphysical effects, which were included in few previous multimodel ensembles, dominates the magnitude (80 per cent) and the spatial pattern of the total surface aerosol forcing in the North Atlantic. Our findings suggest that anthropogenic aerosol emissions influenced a range of societally important historical climate events such as peaks in hurricane activity and Sahel drought. <span class="hlt">Decadal</span>-scale model predictions of regional Atlantic climate will probably be improved by incorporating aerosol-cloud microphysical interactions and estimates of future concentrations of aerosols, emissions of which are directly addressable by policy actions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814041S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814041S"><span>Potential impacts of a future Grand Solar Minimum on <span class="hlt">decadal</span> regional climate change and interannual hemispherical climate <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spiegl, Tobias; Langematz, Ulrike</p> <p>2016-04-01</p> <p>The political, technical and socio-economic developments of the next <span class="hlt">decades</span> will determine the magnitude of 21st century climate change, since they are inextricably linked to future anthropogenic greenhouse gas emissions. To assess the range of uncertainty that is related to these developments, it is common to assume different emission scenarios for 21st climate projections. While the uncertainties associated with the anthropogenic greenhouse gas forcing have been studied intensely, the contribution of natural climate drivers (particularly solar <span class="hlt">variability</span>) to recent and future climate change are subject of intense debate. The past 1,000 years featured at least 5 excursions (lasting 60-100 years) of exceptionally low solar activity, induced by a weak magnetic field of the Sun, so called Grand Solar Minima. While the global temperature response to such a decrease in solar activity is assumed to be rather small, nonlinear mechanisms in the climate system might amplify the regional temperature signal. This hypothesis is supported by the last Grand Solar Minimum (the Maunder Minimum, 1645-1715) which coincides with the Little Ice Age, an epoch which is characterized by severe cold and hardship over Europe, North America and Asia. The long-lasting minimum of Solar Cycle 23 as well as the overall weak maximum of Cycle 24 reveal the possibility for a return to Grand Solar Minimum conditions within the next <span class="hlt">decades</span>. The quantification of the implications of such a projected decrease in solar forcing is of ultimate importance, given the on-going public discussion of the role of carbon dioxide emissions for global warming, and the possible role a cooling due to decreasing solar activity could be ascribed to. Since there is still no clear consensus about the actual strength of the Maunder Minimum, we used 3 acknowledged solar reconstruction datasets that show significant differences in both, total solar irradiance (TSI) and spectral irradiance (SSI) to simulate a future</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29455118','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29455118"><span>Multivariate dynamic Tobit models with lagged <span class="hlt">observed</span> dependent <span class="hlt">variables</span>: An effectiveness analysis of highway safety laws.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dong, Chunjiao; Xie, Kun; Zeng, Jin; Li, Xia</p> <p>2018-04-01</p> <p>Highway safety laws aim to influence driver behaviors so as to reduce the frequency and severity of crashes, and their outcomes. For one specific highway safety law, it would have different effects on the crashes across severities. Understanding such effects can help policy makers upgrade current laws and hence improve traffic safety. To investigate the effects of highway safety laws on crashes across severities, multivariate models are needed to account for the interdependency issues in crash counts across severities. Based on the characteristics of the dependent <span class="hlt">variables</span>, multivariate dynamic Tobit (MVDT) models are proposed to analyze crash counts that are aggregated at the state level. Lagged <span class="hlt">observed</span> dependent <span class="hlt">variables</span> are incorporated into the MVDT models to account for potential temporal correlation issues in crash data. The state highway safety law related factors are used as the explanatory <span class="hlt">variables</span> and socio-demographic and traffic factors are used as the control <span class="hlt">variables</span>. Three models, a MVDT model with lagged <span class="hlt">observed</span> dependent <span class="hlt">variables</span>, a MVDT model with unobserved random <span class="hlt">variables</span>, and a multivariate static Tobit (MVST) model are developed and compared. The results show that among the investigated models, the MVDT models with lagged <span class="hlt">observed</span> dependent <span class="hlt">variables</span> have the best goodness-of-fit. The findings indicate that, compared to the MVST, the MVDT models have better explanatory power and prediction accuracy. The MVDT model with lagged <span class="hlt">observed</span> <span class="hlt">variables</span> can better handle the stochasticity and dependency in the temporal evolution of the crash counts and the estimated values from the model are closer to the <span class="hlt">observed</span> values. The results show that more lives could be saved if law enforcement agencies can make a sustained effort to educate the public about the importance of motorcyclists wearing helmets. Motor vehicle crash-related deaths, injuries, and property damages could be reduced if states enact laws for stricter text messaging rules, higher</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AIPC.1553...69M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AIPC.1553...69M"><span>Towards identification of relevant <span class="hlt">variables</span> in the <span class="hlt">observed</span> aerosol optical depth bias between MODIS and AERONET <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malakar, N. K.; Lary, D. J.; Gencaga, D.; Albayrak, A.; Wei, J.</p> <p>2013-08-01</p> <p>Measurements made by satellite remote sensing, Moderate Resolution Imaging Spectroradiometer (MODIS), and globally distributed Aerosol Robotic Network (AERONET) are compared. Comparison of the two datasets measurements for aerosol optical depth values show that there are biases between the two data products. In this paper, we present a general framework towards identifying relevant set of <span class="hlt">variables</span> responsible for the <span class="hlt">observed</span> bias. We present a general framework to identify the possible factors influencing the bias, which might be associated with the measurement conditions such as the solar and sensor zenith angles, the solar and sensor azimuth, scattering angles, and surface reflectivity at the various measured wavelengths, etc. Specifically, we performed analysis for remote sensing Aqua-Land data set, and used machine learning technique, neural network in this case, to perform multivariate regression between the ground-truth and the training data sets. Finally, we used mutual information between the <span class="hlt">observed</span> and the predicted values as the measure of similarity to identify the most relevant set of <span class="hlt">variables</span>. The search is brute force method as we have to consider all possible combinations. The computations involves a huge number crunching exercise, and we implemented it by writing a job-parallel program.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.475.1190Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.475.1190Y"><span>A <span class="hlt">decades</span>-long fast-rise-exponential-decay flare in low-luminosity AGN NGC 7213</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Zhen; Xie, Fu-Guo</p> <p>2018-03-01</p> <p>We analysed the four-<span class="hlt">decades</span>-long X-ray light curve of the low-luminosity active galactic nucleus (LLAGN) NGC 7213 and discovered a fast-rise-exponential-decay (FRED) pattern, i.e. the X-ray luminosity increased by a factor of ≈4 within 200 d, and then decreased exponentially with an e-folding time ≈8116 d (≈22.2 yr). For the theoretical understanding of the <span class="hlt">observations</span>, we examined three <span class="hlt">variability</span> models proposed in the literature: the thermal-viscous disc instability model, the radiation pressure instability model, and the TDE model. We find that a delayed tidal disruption of a main-sequence star is most favourable; either the thermal-viscous disc instability model or radiation pressure instability model fails to explain some key properties <span class="hlt">observed</span>, thus we argue them unlikely.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1414S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1414S"><span>The Baltic Sea natural long-term <span class="hlt">variability</span> of salinity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schimanke, Semjon; Markus Meier, H. E.</p> <p>2015-04-01</p> <p>The Baltic Sea is one of the largest brackish sea areas of the world. The sensitive state of the Baltic Sea is sustained by a fresh-water surplus by river discharge and precipitation on one hand as well as inflows of highly saline and oxygen-rich water masses from the North Sea on the other. Major inflows which are crucial for the renewal of the deep water occur very intermittent with a mean frequency of approximately one per year. Stagnation periods (periods without major inflows) lead for instance to a reduction of oxygen concentration in the deep Baltic Sea spreading hypoxic conditions. Depending on the amount of salt water inflow and fresh-water supply the deep water salinity of the Baltic Sea varies between 11 to 14 PSU on the <span class="hlt">decadal</span> scale. The goal of this study is to understand the contribution of different driving factors for the <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> <span class="hlt">variability</span> of salinity in the Baltic Sea. Continuous measurement series of salinity exist from the 1950 but are not sufficiently long for the investigation of long-term fluctuations. Therefore, a climate simulation of more than 800 years has been carried out with the Rossby Center Ocean model (RCO). RCO is a biogeochemical regional climate model which covers the entire Baltic Sea. It is driven with atmospheric data dynamical downscaled from a GCM mimicking natural climate <span class="hlt">variability</span>. The analysis focus on the role of variations in river discharge and precipitation, changes in wind speed and direction, fluctuations in temperature and shifts in large scale pressure patterns (e.g. NAO). Hereby, the length of the simulation will allow to identify mechanisms working on <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> time scales. Moreover, it will be discussed how likely long stagnation periods are under natural climate <span class="hlt">variability</span> and if the <span class="hlt">observed</span> exceptional long stagnation period between 1983-1993 might be related to beginning climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120000700&hterms=ammonia&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dammonia','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120000700&hterms=ammonia&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dammonia"><span>Quantifying Spatial and Seasonal <span class="hlt">Variability</span> in Atmospheric Ammonia with In Situ and Space-Based <span class="hlt">Observations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pinder, Robert W.; Walker, John T.; Bash, Jesse O.; Cady-Pereira, Karen E.; Henze, Daven K.; Luo, Mingzhao; Osterman, Gregory B.; Shepard, Mark W.</p> <p>2011-01-01</p> <p>Ammonia plays an important role in many biogeochemical processes, yet atmospheric mixing ratios are not well known. Recently, methods have been developed for retrieving NH3 from space-based <span class="hlt">observations</span>, but they have not been compared to in situ measurements. We have conducted a field campaign combining co-located surface measurements and satellite special <span class="hlt">observations</span> from the Tropospheric Emission Spectrometer (TES). Our study includes 25 surface monitoring sites spanning 350 km across eastern North Carolina, a region with large seasonal and spatial <span class="hlt">variability</span> in NH3. From the TES spectra, we retrieve a NH3 representative volume mixing ratio (RVMR), and we restrict our analysis to times when the region of the atmosphere <span class="hlt">observed</span> by TES is representative of the surface measurement. We find that the TES NH3 RVMR qualitatively captures the seasonal and spatial <span class="hlt">variability</span> found in eastern North Carolina. Both surface measurements and TES NH3 show a strong correspondence with the number of livestock facilities within 10 km of the <span class="hlt">observation</span>. Furthermore, we find that TES H3 RVMR captures the month-to-month <span class="hlt">variability</span> present in the surface <span class="hlt">observations</span>. The high correspondence with in situ measurements and vast spatial coverage make TES NH3 RVMR a valuable tool for understanding regional and global NH3 fluxes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010SPIE.7622E..0AD','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010SPIE.7622E..0AD"><span>A stepwedge-based method for measuring breast density: <span class="hlt">observer</span> <span class="hlt">variability</span> and comparison with human reading</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Diffey, Jenny; Berks, Michael; Hufton, Alan; Chung, Camilla; Verow, Rosanne; Morrison, Joanna; Wilson, Mary; Boggis, Caroline; Morris, Julie; Maxwell, Anthony; Astley, Susan</p> <p>2010-04-01</p> <p>Breast density is positively linked to the risk of developing breast cancer. We have developed a semi-automated, stepwedge-based method that has been applied to the mammograms of 1,289 women in the UK breast screening programme to measure breast density by volume and area. 116 images were analysed by three independent operators to assess inter-<span class="hlt">observer</span> <span class="hlt">variability</span>; 24 of these were analysed on 10 separate occasions by the same operator to determine intra-<span class="hlt">observer</span> <span class="hlt">variability</span>. 168 separate images were analysed using the stepwedge method and by two radiologists who independently estimated percentage breast density by area. There was little intra-<span class="hlt">observer</span> <span class="hlt">variability</span> in the stepwedge method (average coefficients of variation 3.49% - 5.73%). There were significant differences in the volumes of glandular tissue obtained by the three operators. This was attributed to variations in the operators' definition of the breast edge. For fatty and dense breasts, there was good correlation between breast density assessed by the stepwedge method and the radiologists. This was also <span class="hlt">observed</span> between radiologists, despite significant inter-<span class="hlt">observer</span> variation. Based on analysis of thresholds used in the stepwedge method, radiologists' definition of a dense pixel is one in which the percentage of glandular tissue is between 10 and 20% of the total thickness of tissue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150023316&hterms=bats&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbats','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150023316&hterms=bats&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbats"><span>The <span class="hlt">Variable</span> Hard X-Ray Emission of NGC4945 as <span class="hlt">Observed</span> by NuSTAR</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Puccetti, Simonetta; Comastri, Andrea; Fiore, Fabrizio; Arevalo, Patricia; Risaliti, Guido; Bauer, Franz E.; Brandt, William N.; Stern, Daniel; Harrison, Fiona A.; Alexander, David M.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150023316'); toggleEditAbsImage('author_20150023316_show'); toggleEditAbsImage('author_20150023316_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150023316_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150023316_hide"></p> <p>2014-01-01</p> <p>We present a broadband (approx. 0.5 - 79 keV) spectral and temporal analysis of multiple NuSTAR <span class="hlt">observations</span> combined with archival Suzaku and Chandra data of NGC4945, the brightest extragalactic source at 100 keV. We <span class="hlt">observe</span> hard X-ray (> 10 keV) flux and spectral <span class="hlt">variability</span>, with flux variations of a factor 2 on timescales of 20 ksec. A <span class="hlt">variable</span> primary continuum dominates the high energy spectrum (> 10 keV) in all the states, while the reflected/scattered flux which dominates at E< 10 keV stays approximately constant. From modelling the complex reflection/transmission spectrum we derive a Compton depth along the line of sight of Thomson approx.2.9, and a global covering factor for the circumnuclear gas of approx. 0.15. This agrees with the constraints derived from the high energy <span class="hlt">variability</span>, which implies that most of the high energy flux is transmitted, rather that Compton-scattered. This demonstrates the effectiveness of spectral analysis in constraining the geometric properties of the circumnuclear gas, and validates similar methods used for analyzing the spectra of other bright, Compton-thick AGN. The lower limits on the e-folding energy are between 200 - 300 keV, consistent with previous BeppoSAX, Suzaku and Swift BAT <span class="hlt">observations</span>. The accretion rate, estimated from the X-ray luminosity and assuming a bolometric correction typical of type 2 AGN, is in the range approx. 0.1 - 0.3 lambda(sub Edd) depending on the flux state. The substantial <span class="hlt">observed</span> X-ray luminosity <span class="hlt">variability</span> of NGC4945 implies that large errors can arise from using single-epoch X-ray data to derive L/L(sub Edd) values for obscured AGNs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120013713','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120013713"><span>Comparative Analysis of Upper Ocean Heat Content <span class="hlt">Variability</span> from Ensemble Operational Ocean Analyses</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Xue, Yan; Balmaseda, Magdalena A.; Boyer, Tim; Ferry, Nicolas; Good, Simon; Ishikawa, Ichiro; Rienecker, Michele; Rosati, Tony; Yin, Yonghong; Kumar, Arun</p> <p>2012-01-01</p> <p>Upper ocean heat content (HC) is one of the key indicators of climate <span class="hlt">variability</span> on many time-scales extending from seasonal to interannual to long-term climate trends. For example, HC in the tropical Pacific provides information on thermocline anomalies that is critical for the longlead forecast skill of ENSO. Since HC <span class="hlt">variability</span> is also associated with SST <span class="hlt">variability</span>, a better understanding and monitoring of HC <span class="hlt">variability</span> can help us understand and forecast SST <span class="hlt">variability</span> associated with ENSO and other modes such as Indian Ocean Dipole (IOD), Pacific <span class="hlt">Decadal</span> Oscillation (PDO), Tropical Atlantic <span class="hlt">Variability</span> (TAV) and Atlantic Multidecadal Oscillation (AMO). An accurate ocean initialization of HC anomalies in coupled climate models could also contribute to skill in <span class="hlt">decadal</span> climate prediction. Errors, and/or uncertainties, in the estimation of HC <span class="hlt">variability</span> can be affected by many factors including uncertainties in surface forcings, ocean model biases, and deficiencies in data assimilation schemes. Changes in <span class="hlt">observing</span> systems can also leave an imprint on the estimated <span class="hlt">variability</span>. The availability of multiple operational ocean analyses (ORA) that are routinely produced by operational and research centers around the world provides an opportunity to assess uncertainties in HC analyses, to help identify gaps in <span class="hlt">observing</span> systems as they impact the quality of ORAs and therefore climate model forecasts. A comparison of ORAs also gives an opportunity to identify deficiencies in data assimilation schemes, and can be used as a basis for development of real-time multi-model ensemble HC monitoring products. The OceanObs09 Conference called for an intercomparison of ORAs and use of ORAs for global ocean monitoring. As a follow up, we intercompared HC variations from ten ORAs -- two objective analyses based on in-situ data only and eight model analyses based on ocean data assimilation systems. The mean, annual cycle, interannual <span class="hlt">variability</span> and longterm trend of HC have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5548710','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5548710"><span>Time series analysis of patients seeking orthodontic treatment at Seoul National University Dental Hospital over the past <span class="hlt">decade</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lim, Hyun-Woo; Park, Ji-Hoon; Park, Hyun-Hee</p> <p>2017-01-01</p> <p>Objective This paper describes changes in the characteristics of patients seeking orthodontic treatment over the past <span class="hlt">decade</span> and the treatment they received, to identify any seasonal variations or trends. Methods This single-center retrospective cohort study included all patients who presented to Seoul National University Dental Hospital for orthodontic diagnosis and treatment between January 1, 2005 and December 31, 2015. The study analyzed a set of heterogeneous <span class="hlt">variables</span> grouped into the following categories: demographic (age, gender, and address), clinical (Angle Classification, anomaly, mode of orthodontic treatment, removable appliances for Phase 1 treatment, fixed appliances for Phase 2 treatment, orthognathic surgery, extraction, mini-plate, mini-implant, and patient transfer) and time-related <span class="hlt">variables</span> (date of first visit and orthodontic treatment time). Time series analysis was applied to each <span class="hlt">variable</span>. Results The sample included 14,510 patients with a median age of 19.5 years. The number of patients and their ages demonstrated a clear seasonal variation, which peaked in the summer and winter. Increasing trends were <span class="hlt">observed</span> for the proportion of male patients, use of non-extraction treatment modality, use of ceramic brackets, patients from provinces outside the Seoul region at large, patients transferred from private practitioners, and patients who underwent orthognathic surgery performed by university surgeons. Decreasing trends included the use of metal brackets and orthodontic treatment time. Conclusions Time series analysis revealed a seasonal variation in some characteristics, and several <span class="hlt">variables</span> showed changing trends over the past <span class="hlt">decade</span>. PMID:28861391</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080044879&hterms=Elsevier&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DElsevier','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080044879&hterms=Elsevier&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DElsevier"><span>Contrasts Between Precipitation over Mediterranean Sea and Adjacent Continental Areas Based on <span class="hlt">Decadal</span> Scale Satellite Estimates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, Eric A.</p> <p>2007-01-01</p> <p>Most knowledge concerning the last century's climatology and climate dynamics of precipitation over the Mediterranean Sea basin is based on <span class="hlt">observations</span> taken from rain gauges surrounding the sea itself. In turn, most of the <span class="hlt">observations</span> come from Southern Europe, with many fewer measurements taken from widely scattered sites situated over North Africa, the Middle East, and the Balkans. This aspect of research on the Mediterranean Sea basin is apparent in a recent compilation of studies presented in book form concerning climate <span class="hlt">variability</span> of the Mediterranean region [Lionello, P., P. Malanotte-Rizzoli, and R. Boscolo (eds.), 2006: Mediterranean Climate <span class="hlt">Variability</span>. Elsevier, Amsterdam, 9 chapters.] In light of this missing link to over-water <span class="hlt">observations</span>, this study (in conjunction with four companion studies by Z. Haddad, A. Mugnai, T. Nakazawa, and G. Stephens) will contrast the nature of precipitation <span class="hlt">variability</span> directly over the Mediterranean Sea to precipitation <span class="hlt">variability</span> over the surrounding land areas based on three <span class="hlt">decades</span> of satellite-based precipitation estimates which have stood up well to validation scrutiny. The satellite <span class="hlt">observations</span> are drawn from the Global Precipitation Climatology Project (GPCP) dataset extending back to 1979 and the TRMM Merged Algorithm 3b42 dataset extending back to 1998. Both datasets are mostly produced from microwave measurements, excepting the period from 1979 to mid-1987 when only infrared satellite measurements were available for the GPCP estimates. The purpose of this study is to emphasize how the salient properties of precipitation <span class="hlt">variability</span> over land and sea across a hierarchy of space and time scales, and the salient differences in these properties, might be used in guiding short-term climate models to better predictions of future climate states under different regional temperature-change scenarios.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017isms.confETA07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017isms.confETA07L"><span>Potential Line Structure <span class="hlt">Variability</span> in DIB Features <span class="hlt">Observed</span> in Pathfinder tres Survey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Law, Charles; Milisavljevic, Dan; Crabtree, Kyle N.; Johansen, Sommer Lynn</p> <p>2017-06-01</p> <p>The Diffuse Interstellar Bands (DIBs) are hundreds of spectral lines <span class="hlt">observed</span> in sightlines towards many stars in the optical and near-infrared. Although most of these transitions remain unassigned, four of them have recently been assigned to C_{60}^{+} and C_{70}^{+}. In earlier <span class="hlt">observations</span> of the visible spectrum of the extragalactic supernova SN 2012ap, we <span class="hlt">observed</span> changes in the equivalent widths of DIBs on the timescale of its light curve, which indicated that some DIB carriers might exist closer to massive stars then previously believed. Motivated by these findings, we undertook a pathfinder survey of 17 massive stars with the Tillinghast Reflector Echelle Spectrograph at Fred L. Whipple Observatory in search of temporal <span class="hlt">variability</span> in DIBs. In 3 of the 17 stars, we found possible evidence for variation in line substructure of DIBs λ5797 and λ6614. In this talk, we will discuss our efforts to model λ5797 toward MT-59 using contour simulations based on previously published spectral models from higher resolution <span class="hlt">observations</span>. Although the SNR of this spectrum was only 5-15, our preliminary results suggest that the variations in molecular spectra over time might arise from changes in carrier temperature. These early results demonstrate the need for higher SNR spectra taken at multiple epochs to further explore potential temporal <span class="hlt">variability</span>. If successful, time-variation could provide additional evidence to assist in identifying DIB carriers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1406716-recent-changes-county-level-corn-yield-variability-united-states-from-observations-crop-models','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1406716-recent-changes-county-level-corn-yield-variability-united-states-from-observations-crop-models"><span>Recent changes in county-level corn yield <span class="hlt">variability</span> in the United States from <span class="hlt">observations</span> and crop models</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Leng, Guoyong</p> <p></p> <p>The United States is responsible for 35% and 60% of global corn supply and exports. Enhanced supply stability through a reduction in the year-to-year <span class="hlt">variability</span> of US corn yield would greatly benefit global food security. Important in this regard is to understand how corn yield <span class="hlt">variability</span> has evolved geographically in the history and how it relates to climatic and non-climatic factors. Results showed that year-to-year variation of US corn yield has decreased significantly during 1980-2010, mainly in Midwest Corn Belt, Nebraska and western arid regions. Despite the country-scale decreasing <span class="hlt">variability</span>, corn yield <span class="hlt">variability</span> exhibited an increasing trend in South Dakota,more » Texas and Southeast growing regions, indicating the importance of considering spatial scales in estimating yield <span class="hlt">variability</span>. The <span class="hlt">observed</span> pattern is partly reproduced by process-based crop models, simulating larger areas experiencing increasing <span class="hlt">variability</span> and underestimating the magnitude of decreasing <span class="hlt">variability</span>. And 3 out of 11 models even produced a differing sign of change from <span class="hlt">observations</span>. Hence, statistical model which produces closer agreement with <span class="hlt">observations</span> is used to explore the contribution of climatic and non-climatic factors to the changes in yield <span class="hlt">variability</span>. It is found that climate <span class="hlt">variability</span> dominate the change trends of corn yield <span class="hlt">variability</span> in the Midwest Corn Belt, while the ability of climate <span class="hlt">variability</span> in controlling yield <span class="hlt">variability</span> is low in southeastern and western arid regions. Irrigation has largely reduced the corn yield <span class="hlt">variability</span> in regions (e.g. Nebraska) where separate estimates of irrigated and rain-fed corn yield exist, demonstrating the importance of non-climatic factors in governing the changes in corn yield <span class="hlt">variability</span>. The results highlight the distinct spatial patterns of corn yield <span class="hlt">variability</span> change as well as its influencing factors at the county scale. I also caution the use of process-based crop models, which have substantially</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED320969.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED320969.pdf"><span>The Elusive <span class="hlt">Decade</span> of Hispanics.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Cuban American National Council, Inc.</p> <p></p> <p>The 1980s were dubbed "The <span class="hlt">Decade</span> of Hispanics" by the news media, who realized that the rapid growth of the Hispanic American population could be used by them to demand equitable political empowerment and full participation in American social, economic, and educational life. But Hispanics did not move as rapidly as <span class="hlt">observers</span> had predicted because…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C11B..03G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C11B..03G"><span><span class="hlt">Observed</span> Differences between North American Snow Extent and Snow Depth <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ge, Y.; Gong, G.</p> <p>2006-12-01</p> <p>Snow extent and snow depth are two related characteristics of a snowpack, but they need not be mutually consistent. Differences between these two <span class="hlt">variables</span> at local scales are readily apparent. However at larger scales which interact with atmospheric circulation and climate, snow extent is typically the <span class="hlt">variable</span> used, while snow depth is often assumed to be minor and/or mutually consistent compared to snow extent, though this is rarely verified. In this study, a new regional/continental-scale gridded dataset derived from field <span class="hlt">observations</span> is utilized to quantitatively evaluate the relationship between snow extent and snow depth over North America. Various statistical methods are applied to assess the mutual consistency of monthly snow depth vs. snow extent, including correlations, composites and principal components. Results indicate that snow depth variations are significant in their own rights, and that depth and extent anomalies are largely unrelated, especially over broad high latitude regions north of the snowline. In the vicinity of the snowline, where precipitation and ablation can affect both snow extent and snow depth, the two <span class="hlt">variables</span> vary concurrently, especially in autumn and spring. It is also found that deeper winter snow translates into larger snow-covered area in the subsequent spring/summer season, which suggests a possible influence of winter snow depth on summer climate. The <span class="hlt">observed</span> lack of mutual consistency at continental/regional scales suggests that snowpack depth variations may be of sufficiently large magnitude, spatial scope and temporal duration to influence regional-hemispheric climate, in a manner unrelated to the more extensively studied snow extent variations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25752943','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25752943"><span>An atmospheric origin of the multi-<span class="hlt">decadal</span> bipolar seesaw.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Zhaomin; Zhang, Xiangdong; Guan, Zhaoyong; Sun, Bo; Yang, Xin; Liu, Chengyan</p> <p>2015-03-10</p> <p>A prominent feature of recent climatic change is the strong Arctic surface warming that is contemporaneous with broad cooling over much of Antarctica and the Southern Ocean. Longer global surface temperature <span class="hlt">observations</span> suggest that this contrasting pole-to-pole change could be a manifestation of a multi-<span class="hlt">decadal</span> interhemispheric or bipolar seesaw pattern, which is well correlated with the North Atlantic sea surface temperature <span class="hlt">variability</span>, and thus generally hypothesized to originate from Atlantic meridional overturning circulation oscillations. Here, we show that there is an atmospheric origin for this seesaw pattern. The results indicate that the Southern Ocean surface cooling (warming) associated with the seesaw pattern is attributable to the strengthening (weakening) of the Southern Hemisphere westerlies, which can be traced to Northern Hemisphere and tropical tropospheric warming (cooling). Antarctic ozone depletion has been suggested to be an important driving force behind the recently <span class="hlt">observed</span> increase in the Southern Hemisphere's summer westerly winds; our results imply that Northern Hemisphere and tropical warming may have played a triggering role at an stage earlier than the first detectable Antarctic ozone depletion, and enhanced Antarctic ozone depletion through decreasing the lower stratospheric temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G31C0931W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G31C0931W"><span>Temporal and spatial <span class="hlt">variabilities</span> of Antarctic ice mass changes inferred by GRACE in a Bayesian framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, L.; Davis, J. L.; Tamisiea, M. E.</p> <p>2017-12-01</p> <p>The Antarctic ice sheet (AIS) holds about 60% of all fresh water on the Earth, an amount equivalent to about 58 m of sea-level rise. <span class="hlt">Observation</span> of AIS mass change is thus essential in determining and predicting its contribution to sea level. While the ice mass loss estimates for West Antarctica (WA) and the Antarctic Peninsula (AP) are in good agreement, what the mass balance over East Antarctica (EA) is, and whether or not it compensates for the mass loss is under debate. Besides the different error sources and sensitivities of different measurement types, complex spatial and temporal <span class="hlt">variabilities</span> would be another factor complicating the accurate estimation of the AIS mass balance. Therefore, a model that allows for <span class="hlt">variabilities</span> in both melting rate and seasonal signals would seem appropriate in the estimation of present-day AIS melting. We present a stochastic filter technique, which enables the Bayesian separation of the systematic stripe noise and mass signal in <span class="hlt">decade</span>-length GRACE monthly gravity series, and allows the estimation of time-<span class="hlt">variable</span> seasonal and inter-annual components in the signals. One of the primary advantages of this Bayesian method is that it yields statistically rigorous uncertainty estimates reflecting the inherent spatial resolution of the data. By applying the stochastic filter to the <span class="hlt">decade</span>-long GRACE <span class="hlt">observations</span>, we present the temporal <span class="hlt">variabilities</span> of the AIS mass balance at basin scale, particularly over East Antarctica, and decipher the EA mass variations in the past <span class="hlt">decade</span>, and their role in affecting overall AIS mass balance and sea level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028074','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028074"><span>Multidecadal climate <span class="hlt">variability</span> of global lands and oceans</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McCabe, G.J.; Palecki, M.A.</p> <p>2006-01-01</p> <p>Principal components analysis (PCA) and singular value decomposition (SVD) are used to identify the primary modes of <span class="hlt">decadal</span> and multidecadal <span class="hlt">variability</span> in annual global Palmer Drought Severity Index (PDSI) values and sea-surface temperature (SSTs). The PDSI and SST data for 1925-2003 were detrended and smoothed (with a 10-year moving average) to isolate the <span class="hlt">decadal</span> and multidecadal <span class="hlt">variability</span>. The first two principal components (PCs) of the PDSI PCA explained almost 38% of the <span class="hlt">decadal</span> and multidecadal variance in the detrended and smoothed global annual PDSI data. The first two PCs of detrended and smoothed global annual SSTs explained nearly 56% of the <span class="hlt">decadal</span> <span class="hlt">variability</span> in global SSTs. The PDSI PCs and the SST PCs are directly correlated in a pairwise fashion. The first PDSI and SST PCs reflect <span class="hlt">variability</span> of the detrended and smoothed annual Pacific <span class="hlt">Decadal</span> Oscillation (PDO), as well as detrended and smoothed annual Indian Ocean SSTs. The second set of PCs is strongly associated with the Atlantic Multidecadal Oscillation (AMO). The SVD analysis of the cross-covariance of the PDSI and SST data confirmed the close link between the PDSI and SST modes of <span class="hlt">decadal</span> and multidecadal variation and provided a verification of the PCA results. These findings indicate that the major modes of multidecadal variations in SSTs and land-surface climate conditions are highly interrelated through a small number of spatially complex but slowly varying teleconnections. Therefore, these relations may be adaptable to providing improved baseline conditions for seasonal climate forecasting. Published in 2006 by John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870001020','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870001020"><span><span class="hlt">Observations</span> and a model of gravity-wave <span class="hlt">variability</span> in the middle atmosphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fritts, D. C.; Vincent, R. A.</p> <p>1986-01-01</p> <p>A major goal was to determine what portion of the gravity-wave frequency spectrum accounted for the majority of the momentum flux and divergence, as this has important implications for the middle atmosphere response. It was found that approx. 70% of the total flux and divergence was due to wave motions with <span class="hlt">observed</span> periods less than 1 hour, consistent with expectations based on the shape of the <span class="hlt">observed</span> gravity-wave spectrum (FrItts, 1984). This dominance of the momentum flux and divergence by high-frequency motions implies a potential for the modulation of those quantities by large-amplitude motions at lower frequencies. A second, striking aspect of the velocity and momentum flux data is its dramatic diurnal <span class="hlt">variability</span>, particularly at certain levels. This <span class="hlt">variability</span> is illustrated with the momentum flux, computed in 8-hr blocks. The dominant contributions here are due to waves with periods less than 1 hr. The <span class="hlt">variability</span> with height and size of the mean square velocity in the west beam and the momentum flux, energed over the 3-day period. A detailed analysis of the various tidal motions present during this data interval was performed, and it was determined that variations in the zontal wind profile imposed by the diurnal tidal motion are probably responsible for the modulation of the gravity-wave amplitudes and momentum fluxes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhDT........14A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhDT........14A"><span>An <span class="hlt">Observational</span> Study of Cataclysmic <span class="hlt">Variable</span> Evolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Araujo-Betancor, Sofia</p> <p>2004-03-01</p> <p>In this thesis I present an <span class="hlt">observational</span> study of the evolution of Cataclysmic <span class="hlt">Variables</span> (CVs). Disrupted magnetic braking has been the standard paradigm of CV evolution for the past twenty years. Unfortunately, some of its predictions are in strong disagreement with the <span class="hlt">observations</span>. In recent years, a number of additions/alternatives to the standard model have been proposed. Yet, none have been able to explain all of the features <span class="hlt">observed</span> in the currently known CV population. The work presented in this thesis is based mainly on a large-scale search for CVs. The primary aim of this project is to resolve the disagreement between theory and <span class="hlt">observations</span> by eliminating the <span class="hlt">observational</span> biases of the present CV sample. Here, I use two complementary approaches to search for CVs: (1) from the spectroscopic appearance in the Hamburg Quasar Survey (HQS), and (2) by using a combination of ROSAT and 2MASS archival data. So far, we have discovered 52 new CVs in the HQS and 11 new CVs (the majority of them magnetic) and 1 pre-CV in the ROSAT/2MASS. Follow-up <span class="hlt">observations</span> of two newly discovered HQS CVs, 1RXS J062518.2+733433 and HS 2331+3905, resulted in the classification of the first as an Intermediate Polar, with P_orb = 283.0 min and P_spin = 19.8 min, and the second as a short orbital period system, P_orb = 81.0 min, harbouring a white dwarf pulsator. In addition, we found that the dominant ~3.5 h radial velocity variation of HS 2331+3905 does not correspond to the orbital period of the system, contrary to all other CVs. Despite its novel selection criterion, the HQS does not provide many short-period CVs -- even though tests with the known CVs included in the survey have shown that it is very sensitive to those objects. The biggest surprise in the new HQS sample is the discovery of many new SW Sex stars. The clustering of SW Sex stars in the 3-4 h period range is probably an important feature in the evolution of CVs that we currently do not understand at all. To</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020108','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020108"><span>North-South precipitation patterns in western North America on interannual-to-<span class="hlt">decadal</span> timescales</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dettinger, M.D.; Cayan, D.R.; Diaz, Henry F.; Meko, D.M.</p> <p>1998-01-01</p> <p>The overall amount of precipitation deposited along the West Coast and western cordillera of North America from 25??to 55??N varies from year to year, and superimposed on this domain-average <span class="hlt">variability</span> are varying north-south contrasts on timescales from at least interannual to interdecadal. In order to better understand the north-south precipitation contrasts, their interannual and <span class="hlt">decadal</span> variations are studied in terms of how much they affect overall precipitation amounts and how they are related to large-scale climatic patterns. Spatial empirical orthogonal functions (EOFs) and spatial moments (domain average, central latitude, and latitudinal spread) of zonally averaged precipitation anomalies along the westernmost parts of North America are analyzed, and each is correlated with global sea level pressure (SLP) and sea surface temperature series, on interannual (defined here as 3-7 yr) and <span class="hlt">decadal</span> (>7 yr) timescales. The interannual band considered here corresponds to timescales that are particularly strong in tropical climate variations and thus is expected to contain much precipitation <span class="hlt">variability</span> that is related to El Nino-Southern Oscillation; the <span class="hlt">decadal</span> scale is defined so as to capture the whole range of long-term climatic variations affecting western North America. Zonal EOFs of the interannual and <span class="hlt">decadal</span> filtered versions of the zonal-precipitation series are remarkably similar. At both timescales, two leading EOFs describe 1) a north-south seesaw of precipitation pivoting near 40??N and 2) variations in precipitation near 40??N, respectively. The amount of overall precipitation <span class="hlt">variability</span> is only about 10% of the mean and is largely determined by precipitation variations around 40??-45??N and most consistently influenced by nearby circulation patterns; in this sense, domain-average precipitation is closely related to the second EOF. The central latitude and latitudinal spread of precipitation distributions are strongly influenced by precipitation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950053165&hterms=centennials&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcentennials','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950053165&hterms=centennials&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcentennials"><span><span class="hlt">Decadal</span>-to-centennial-scale climate <span class="hlt">variability</span>: Insights into the rise and fall of the Great Salt Lake</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mann, Michael E.; Lall, Upmanu; Saltzman, Barry</p> <p>1995-01-01</p> <p>We demonstrate connections between <span class="hlt">decadal</span> and secular global climatic variations, and historical variations in the volume of the Great Salt Lake. The <span class="hlt">decadal</span> variations correspond to a low-frequency shifting of storm tracks which influence winter precipitation and explain nearly 18% of the interannual and longer-term variance in the record of monthly volume change. The secular trend accounts for a more modest approximately 1.5% of the variance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19970024562&hterms=1047&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231047','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19970024562&hterms=1047&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231047"><span>X-ray and optical <span class="hlt">observations</span> of 2 new cataclysmic <span class="hlt">variables</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Singh, K. P.; Szkody, P.; Barrett, P.; Schlegel, E.; White, N. E.; Silber, A.; Fierce, E.; Hoard, D.; Hakala, P. J.; Piirola, V.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_19970024562'); toggleEditAbsImage('author_19970024562_show'); toggleEditAbsImage('author_19970024562_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_19970024562_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_19970024562_hide"></p> <p>1996-01-01</p> <p>The light curves and spectra of two ultra soft X-ray sources are presented. The sources, WGAJ 1047.1+6335 and WGAJ 1802.1+1804 were discovered during a search using the Rosat position sensitive proportional counter (PSPC). The X-ray spectra of both objects show an unusually strong black body component with respect to the harder bremsstrahlung component. Based on the optical <span class="hlt">observations</span> and on the analysis of the X-ray data, the two objects are identified with new AM Her type cataclysmic <span class="hlt">variables</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4682045','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4682045"><span>Atlantic multi-<span class="hlt">decadal</span> oscillation covaries with Agulhas leakage</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Biastoch, Arne; Durgadoo, Jonathan V.; Morrison, Adele K.; van Sebille, Erik; Weijer, Wilbert; Griffies, Stephen M.</p> <p>2015-01-01</p> <p>The interoceanic transfer of seawater between the Indian Ocean and the Atlantic, ‘Agulhas leakage', forms a choke point for the overturning circulation in the global ocean. Here, by combining output from a series of high-resolution ocean and climate models with in situ and satellite <span class="hlt">observations</span>, we construct a time series of Agulhas leakage for the period 1870–2014. The time series demonstrates the impact of Southern Hemisphere westerlies on <span class="hlt">decadal</span> timescales. Agulhas leakage shows a correlation with the Atlantic Multi-<span class="hlt">decadal</span> Oscillation on multi-<span class="hlt">decadal</span> timescales; the former leading by 15 years. This is relevant for climate in the North Atlantic. PMID:26656850</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1259279-atlantic-multi-decadal-oscillation-covaries-agulhas-leakage','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1259279-atlantic-multi-decadal-oscillation-covaries-agulhas-leakage"><span>Atlantic multi-<span class="hlt">decadal</span> oscillation covaries with Agulhas leakage</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Biastoch, Arne; Durgadoo, Jonathan V.; Morrison, Adele K.; ...</p> <p>2015-12-10</p> <p>The interoceanic transfer of seawater between the Indian Ocean and the Atlantic, ‘Agulhas leakage’, forms a choke point for the overturning circulation in the global ocean. Here, by combining output from a series of high-resolution ocean and climate models with in situ and satellite <span class="hlt">observations</span>, we construct a time series of Agulhas leakage for the period 1870–2014. The time series demonstrates the impact of Southern Hemisphere westerlies on <span class="hlt">decadal</span> timescales. Agulhas leakage shows a correlation with the Atlantic Multi-<span class="hlt">decadal</span> Oscillation on multi-<span class="hlt">decadal</span> timescales; the former leading by 15 years. Lastly, this is relevant for climate in the North Atlantic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy..tmp..892C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy..tmp..892C"><span>Mechanisms of interannual- to <span class="hlt">decadal</span>-scale winter Labrador Sea ice <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Close, S.; Herbaut, C.; Houssais, M.-N.; Blaizot, A.-C.</p> <p>2017-12-01</p> <p>The <span class="hlt">variability</span> of the winter sea ice cover of the Labrador Sea region and its links to atmospheric and oceanic forcing are investigated using <span class="hlt">observational</span> data, a coupled ocean-sea ice model and a fully-coupled model simulation drawn from the CMIP5 archive. A consistent series of mechanisms associated with high sea ice cover are found amongst the various data sets. The highest values of sea ice area occur when the northern Labrador Sea is ice covered. This region is found to be primarily thermodynamically forced, contrasting with the dominance of mechanical forcing along the eastern coast of Baffin Island and Labrador, and the growth of sea ice is associated with anomalously fresh local ocean surface conditions. Positive fresh water anomalies are found to propagate to the region from a source area off the southeast Greenland coast with a 1 month transit time. These anomalies are associated with sea ice melt, driven by the enhanced offshore transport of sea ice in the source region, and its subsequent westward transport in the Irminger Current system. By combining sea ice transport through the Denmark Strait in the preceding autumn with the Greenland Blocking Index and the Atlantic Multidecadal Oscillation Index, strong correlation with the Labrador Sea ice area of the following winter is obtained. This relationship represents a dependence on the availability of sea ice to be melted in the source region, the necessary atmospheric forcing to transport this offshore, and a further multidecadal-scale link with the large-scale sea surface temperature conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008MNRAS.385.1471P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008MNRAS.385.1471P"><span>An Hα-selected sample of cataclysmic <span class="hlt">variables</span> - I. <span class="hlt">Observations</span> of newly discovered systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pretorius, Magaretha L.; Knigge, Christian</p> <p>2008-04-01</p> <p>Strong selection effects are present in <span class="hlt">observational</span> samples of cataclysmic <span class="hlt">variables</span> (CVs), complicating comparisons to theoretical predictions. The selection criteria used to define most CV samples discriminate heavily against the discovery of short-period, intrinsically faint systems. The situation can be improved by selecting CVs for the presence of emission lines. For this reason, we have constructed a homogeneous sample of CVs selected on the basis of Hα emission. We present discovery <span class="hlt">observations</span> of the 14 CVs and two additional CV candidates found in this search. The orbital periods of 11 of the new CVs were measured; all are above 3 h. There are two eclipsing systems in the sample, and one in which we <span class="hlt">observed</span> a quasi-periodic modulation on a ~1000s time-scale. We also detect the secondary star in the spectrum of one system, and measure its spectral type. Several of the new CVs have the spectroscopic appearance of nova-like <span class="hlt">variables</span>, and a few display what may be SW Sex star behaviour. In a companion paper, we discuss the implications of this new sample for CV evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4438Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4438Y"><span><span class="hlt">Observations</span> of Local Positive Low Cloud Feedback Patterns and Their Role in Internal <span class="hlt">Variability</span> and Climate Sensitivity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yuan, Tianle; Oreopoulos, Lazaros; Platnick, Steven E.; Meyer, Kerry</p> <p>2018-05-01</p> <p>Modeling studies have shown that cloud feedbacks are sensitive to the spatial pattern of sea surface temperature (SST) anomalies, while cloud feedbacks themselves strongly influence the magnitude of SST anomalies. <span class="hlt">Observational</span> counterparts to such patterned interactions are still needed. Here we show that distinct large-scale patterns of SST and low-cloud cover (LCC) emerge naturally from objective analyses of <span class="hlt">observations</span> and demonstrate their close coupling in a positive local SST-LCC feedback loop that may be important for both internal <span class="hlt">variability</span> and climate change. The two patterns that explain the maximum amount of covariance between SST and LCC correspond to the Interdecadal Pacific Oscillation and the Atlantic Multidecadal Oscillation, leading modes of multidecadal internal <span class="hlt">variability</span>. Spatial patterns and time series of SST and LCC anomalies associated with both modes point to a strong positive local SST-LCC feedback. In many current climate models, our analyses suggest that SST-LCC feedback strength is too weak compared to <span class="hlt">observations</span>. Modeled local SST-LCC feedback strength affects simulated internal <span class="hlt">variability</span> so that stronger feedback produces more intense and more realistic patterns of internal <span class="hlt">variability</span>. To the extent that the physics of the local positive SST-LCC feedback inferred from <span class="hlt">observed</span> climate <span class="hlt">variability</span> applies to future greenhouse warming, we anticipate significant amount of delayed warming because of SST-LCC feedback when anthropogenic SST warming eventually overwhelm the effects of internal <span class="hlt">variability</span> that may mute anthropogenic warming over parts of the ocean. We postulate that many climate models may be underestimating both future warming and the magnitude of modeled internal <span class="hlt">variability</span> because of their weak SST-LCC feedback.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AtmRe.182..200J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AtmRe.182..200J"><span>Analysis of trends and dominant periodicities in drought <span class="hlt">variables</span> in India: A wavelet transform based approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Joshi, Nitin; Gupta, Divya; Suryavanshi, Shakti; Adamowski, Jan; Madramootoo, Chandra A.</p> <p>2016-12-01</p> <p>In this study, seasonal trends as well as dominant and significant periods of <span class="hlt">variability</span> of drought <span class="hlt">variables</span> were analyzed for 30 rainfall subdivisions in India over 141 years (1871-2012). Standardized precipitation index (SPI) was used as a meteorological drought indicator, and various drought <span class="hlt">variables</span> (monsoon SPI, non-monsoon SPI, yearly SPI, annual drought duration, annual drought severity and annual drought peak) were analyzed. Discrete wavelet transform was used in conjunction with the Mann-Kendall test to analyze trends and dominant periodicities associated with the drought <span class="hlt">variables</span>. Furthermore, continuous wavelet transform (CWT) based global wavelet spectrum was used to analyze significant periods of <span class="hlt">variability</span> associated with the drought <span class="hlt">variables</span>. From the trend analysis, we <span class="hlt">observed</span> that over the second half of the 20th century, drought occurrences increased significantly in subdivisions of Northeast and Central India. In both short-term (2-8 years) and <span class="hlt">decadal</span> (16-32 years) periodicities, the drought <span class="hlt">variables</span> were found to influence the trend. However, CWT analysis indicated that the dominant periodic components were not significant for most of the geographical subdivisions. Although inter-annual and inter-<span class="hlt">decadal</span> periodic components play an important role, they may not completely explain the <span class="hlt">variability</span> associated with the drought <span class="hlt">variables</span> across the country.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22660924-spitzer-observations-long-term-infrared-variability-among-young-stellar-objects-chamaeleon','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22660924-spitzer-observations-long-term-infrared-variability-among-young-stellar-objects-chamaeleon"><span>SPITZER <span class="hlt">OBSERVATIONS</span> OF LONG-TERM INFRARED <span class="hlt">VARIABILITY</span> AMONG YOUNG STELLAR OBJECTS IN CHAMAELEON I</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Flaherty, Kevin M.; Herbst, William; DeMarchi, Lindsay</p> <p></p> <p>Infrared <span class="hlt">variability</span> is common among young stellar objects, with surveys finding daily to weekly fluctuations of a few tenths of a magnitude. Space-based <span class="hlt">observations</span> can produce highly sampled infrared light curves, but are often limited to total baselines of about 1 month due to the orientation of the spacecraft. Here we present <span class="hlt">observations</span> of the Chameleon I cluster, whose low declination makes it <span class="hlt">observable</span> by the Spitzer Space Telescope over a 200-day period. We <span class="hlt">observe</span> 30 young stellar objects with a daily cadence to better sample <span class="hlt">variability</span> on timescales of months. We find that such <span class="hlt">variability</span> is common, occurring inmore » ∼80% of the detected cluster members. The change in [3.6]–[4.5] color over 200 days for many of the sources falls between that expected for extinction and fluctuations in disk emission. With our high cadence and long baseline we can derive power spectral density curves covering two orders of magnitude in frequency and find significant power at low frequencies, up to the boundaries of our 200-day survey. Such long timescales are difficult to explain with variations driven by the interaction between the disk and stellar magnetic field, which has a dynamical timescale of days to weeks. The most likely explanation is either structural or temperature fluctuations spread throughout the inner ∼0.5 au of the disk, suggesting that the intrinsic dust structure is highly dynamic.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030025661&hterms=prospect&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dprospect','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030025661&hterms=prospect&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dprospect"><span>Time-<span class="hlt">Variable</span> Gravity from Space: Quarter Century of <span class="hlt">Observations</span>, Mysteries, and Prospects</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chao, Benjamin F.</p> <p>2003-01-01</p> <p>Any large mass transport in the Earth system produces changes in the gravity field. Via the space geodetic technique of satellite-laser ranging in the last quarter century, the Earth's dynamic oblateness J2 (the lowest-degree harmonic component of the gravity field) has been <span class="hlt">observed</span> to undergo a slight decrease -- until around 1998, when it switched quite suddenly to an increase trend which has continued to date. The secular decrease in J2 has long been attributed primarily to the post-glacial rebound in the mantle; the present increase signifies an even larger change in global mass distribution whose J2 effect overshadows that of the post-glacial rebound, at least over interannual timescales. Intriguing evidences have been found in the ocean water distribution, especially in the extratropical Pacific basins, that may be responsible for this J2 change. New techniques based on satellite-to-satellite tracking will yield greatly improved <span class="hlt">observations</span> for time-<span class="hlt">variable</span> gravity, with much higher precision and spatial resolution (i.e., much higher harmonic degrees). The most important example is the GRACE mission launched in March 2002, following the success of the CHAMP mission. In addition, although less precise than GRACE, the GPS/Meteorology constellation mission COSMIC, with 6 mini-satellites to be launched in late 2005, is expected to provide continued and complementary time-<span class="hlt">variable</span> gravity <span class="hlt">observations</span>. Such <span class="hlt">observations</span> are becoming a new and powerful tool for remote sensing of geophysical fluid processes that involve larger-scale mass transports.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A21B0029T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A21B0029T"><span>Ocean carbon and heat <span class="hlt">variability</span> in an Earth System Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomas, J. L.; Waugh, D.; Gnanadesikan, A.</p> <p>2016-12-01</p> <p>Ocean carbon and heat content are very important for regulating global climate. Furthermore, due to lack of <span class="hlt">observations</span> and dependence on parameterizations, there has been little consensus in the modeling community on the magnitude of realistic ocean carbon and heat content <span class="hlt">variability</span>, particularly in the Southern Ocean. We assess the differences between global oceanic heat and carbon content <span class="hlt">variability</span> in GFDL ESM2Mc using a 500-year, pre-industrial control simulation. The global carbon and heat content are directly out of phase with each other; however, in the Southern Ocean the heat and carbon content are in phase. The global heat mutli-<span class="hlt">decadal</span> <span class="hlt">variability</span> is primarily explained by <span class="hlt">variability</span> in the tropics and mid-latitudes, while the <span class="hlt">variability</span> in global carbon content is primarily explained by Southern Ocean <span class="hlt">variability</span>. In order to test the robustness of this relationship, we use three additional pre-industrial control simulations using different mesoscale mixing parameterizations. Three pre-industrial control simulations are conducted with the along-isopycnal diffusion coefficient (Aredi) set to constant values of 400, 800 (control) and 2400 m2 s-1. These values for Aredi are within the range of parameter settings commonly used in modeling groups. Finally, one pre-industrial control simulation is conducted where the minimum in the Gent-McWilliams parameterization closure scheme (AGM) increased to 600 m2 s-1. We find that the different simulations have very different multi-<span class="hlt">decadal</span> <span class="hlt">variability</span>, especially in the Weddell Sea where the characteristics of deep convection are drastically changed. While the temporal frequency and amplitude global heat and carbon content changes significantly, the overall spatial pattern of <span class="hlt">variability</span> remains unchanged between the simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2362Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2362Y"><span>A First Look at <span class="hlt">Decadal</span> Hydrological Predictability by Land Surface Ensemble Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yuan, Xing; Zhu, Enda</p> <p>2018-03-01</p> <p>The prediction of terrestrial hydrology at the <span class="hlt">decadal</span> scale is critical for managing water resources in the face of climate change. Here we conducted an assessment by global land model simulations following the design of the fifth Coupled Model Intercomparison Project (CMIP5) <span class="hlt">decadal</span> hindcast experiments, specifically testing for the sensitivity to perfect initial or boundary conditions. The memory for terrestrial water storage (TWS) is longer than 6 years over 11% of global land areas where the deep soil moisture and aquifer water have a long memory and a nonnegligible <span class="hlt">variability</span>. Ensemble <span class="hlt">decadal</span> predictions based on realistic initial conditions are skillful over 31%, 43%, and 59% of global land areas for TWS, deep soil moisture, and aquifer water, respectively. The fraction of skillful predictions for TWS increases by 10%-16% when conditioned on Pacific <span class="hlt">Decadal</span> Oscillation and Atlantic Multidecadal Oscillation indices. This study provides a first look at <span class="hlt">decadal</span> hydrological predictability, with an improved skill when incorporating low-frequency climate information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=307068','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=307068"><span>Trends and <span class="hlt">variability</span> of daily temperature extremes during 1960-2012 in the Yangtze River Basin, China</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>The <span class="hlt">variability</span> of temperature extremes has been the focus of attention during the past few <span class="hlt">decades</span>, and may exert a great influence on the global hydrologic cycle and energy balance through thermal forcing. Based on daily minimum and maximum temperature <span class="hlt">observed</span> by the China Meteorological Administ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10567E..2QP','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10567E..2QP"><span><span class="hlt">Variable</span> optical filters for earth-<span class="hlt">observation</span> imaging minispectrometers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Piegari, A.; Bulir, J.; Krasilnikova, A.; Dami, M.; Harnisch, B.</p> <p>2017-11-01</p> <p>Small-dimension, low-mass spectrometers are useful for both Earth <span class="hlt">observation</span> and planetary missions. A very compact multi-spectral mini-spectrometer that contains no moving parts, can be constructed combining a graded-thickness filter, having a spatially <span class="hlt">variable</span> narrow-band transmission, to a CCD array detector. The peak wavelength of the transmission filter is moving along one direction of the filter surface, such that each line of a two-dimensional array detector, equipped with this filter, will detect radiation in a different pass band. The spectrum of interest for image spectrometry of the Earth surface is very wide, 400-1000nm. This requirement along with the need of a very small dimension, makes this filter very difficult to manufacture. Preliminary results on metal-dielectric wedge filters, with a gradient of the transmission peak wavelength equal to 60nm/mm, are reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGC43C1067M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGC43C1067M"><span>Extension of the SIM Hydrometeorological Reanalysis Over the Entire 20th Century by Combination of <span class="hlt">Observations</span> and Statistical Downscaling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Minvielle, M.; Céron, J.; Page, C.</p> <p>2013-12-01</p> <p>The SAFRAN-ISBA-MODCOU (SIM) system is a combination of three different components: an atmospheric analysis system (SAFRAN) providing the atmospheric forcing for a land surface model (ISBA) that computes surface water and energy budgets and a hydrological model (MODCOU) that provides river flows and level of several aquifers. The <span class="hlt">variables</span> generated by the SIM chain constitute the SIM reanalysis and the current version only covers the 1958-2012 period. However, long climate datasets are required for evaluation and verification of climate hindcasts/forecasts and to isolate the contribution of natural <span class="hlt">decadal</span> <span class="hlt">variability</span> from that of anthropogenic forcing to climate variations. The aim of this work is to extend of the fine-mesh SIM reanalysis to the entire 20th century, especially focusing on temperature and rainfall over France, but also soil wetness and river flows. This extension will first allow a detailed investigation of the influence of <span class="hlt">decadal</span> <span class="hlt">variability</span> on France at very fine spatial scales and will provide crucial information for climate model evaluation. Before 1958, the density of available <span class="hlt">observations</span> from Météo-France necessary to force SAFRAN (rainfall, snow, wind, temperature, humidity, cloudiness) is much lower than today, and not sufficient to produce a correct SIM reanalysis. That's why is has been decided to use the available atmospheric <span class="hlt">observations</span> over the past <span class="hlt">decades</span> combined to a statistical downscaling algorithm to overcome the lack of <span class="hlt">observations</span>. The DSCLIM software package implemented by the CERFACS and using a weather typing based statistical methodology will be used as statistical downscaling method to reconstruct the atmospheric <span class="hlt">variables</span> necessary to force the ISBA-MODCOU hydrological component. The first stage of this work was to estimate and compare the bias and strengths of the two approaches in their ability to reconstruct the past <span class="hlt">decades</span>. In this sense, SIM hydro-meteorological experiments were performed for some recent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSAH21A..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSAH21A..07S"><span>Using present day <span class="hlt">observations</span> to detect when ocean acidification exceeds natural <span class="hlt">variability</span> of surface seawater Ωaragonite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sutton, A.; Sabine, C. L.; Feely, R. A.</p> <p>2016-02-01</p> <p>One of the major challenges to assessing the impact of ocean acidification on marine life is the need to better understand the magnitude of long-term change in the context of natural <span class="hlt">variability</span>. High-frequency moored <span class="hlt">observations</span> can be highly effective in defining interannual, seasonal, and subseasonal <span class="hlt">variability</span> at key locations. Here we present monthly aragonite saturation state (Ωaragonite) climatology for 15 open ocean, coastal, and coral reef locations using 3-hourly moored <span class="hlt">observations</span> of surface seawater pCO2 and pH collected together since as early as 2009. We then use these present day surface mooring <span class="hlt">observations</span> to estimate pre-industrial <span class="hlt">variability</span> at each location and compare these results to previous modeling studies addressing global-scale <span class="hlt">variability</span> and change. Our <span class="hlt">observations</span> suggest that open oceans sites, especially in the subtropics, are experiencing Ωaragonite values throughout much of the year which are outside the range of pre-industrial values. In coastal and coral reef ecosystems, which have higher natural <span class="hlt">variability</span>, seasonal patterns where present day Ωaragonite values exceeding pre-industrial bounds are emerging with some sites exhibiting subseasonal conditions approaching Ωaragonite = 1. Linking these seasonal patterns in carbonate chemistry to biological processes in these regions is critical to identify when and where marine life may encounter Ωaragonite values outside the conditions to which they have adapted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4088266','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4088266"><span>All varieties of encoding <span class="hlt">variability</span> are not created equal: Separating <span class="hlt">variable</span> processing from <span class="hlt">variable</span> tasks</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huff, Mark J.; Bodner, Glen E.</p> <p>2014-01-01</p> <p>Whether encoding <span class="hlt">variability</span> facilitates memory is shown to depend on whether item-specific and relational processing are both performed across study blocks, and whether study items are weakly versus strongly related. <span class="hlt">Variable</span>-processing groups studied a word list once using an item-specific task and once using a relational task. <span class="hlt">Variable</span>-task groups’ two different study tasks recruited the same type of processing each block. Repeated-task groups performed the same study task each block. Recall and recognition were greatest in the <span class="hlt">variable</span>-processing group, but only with weakly related lists. A <span class="hlt">variable</span>-processing benefit was also found when task-based processing and list-type processing were complementary (e.g., item-specific processing of a related list) rather than redundant (e.g., relational processing of a related list). That performing both item-specific and relational processing across trials, or within a trial, yields encoding-<span class="hlt">variability</span> benefits may help reconcile <span class="hlt">decades</span> of contradictory findings in this area. PMID:25018583</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26324900','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26324900"><span>Slowing down of North Pacific climate <span class="hlt">variability</span> and its implications for abrupt ecosystem change.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boulton, Chris A; Lenton, Timothy M</p> <p>2015-09-15</p> <p>Marine ecosystems are sensitive to stochastic environmental <span class="hlt">variability</span>, with higher-amplitude, lower-frequency--i.e., "redder"--<span class="hlt">variability</span> posing a greater threat of triggering large ecosystem changes. Here we show that fluctuations in the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) index have slowed down markedly over the <span class="hlt">observational</span> record (1900-present), as indicated by a robust increase in autocorrelation. This "reddening" of the spectrum of climate <span class="hlt">variability</span> is also found in regionally averaged North Pacific sea surface temperatures (SSTs), and can be at least partly explained by <span class="hlt">observed</span> deepening of the ocean mixed layer. The progressive reddening of North Pacific climate <span class="hlt">variability</span> has important implications for marine ecosystems. Ecosystem <span class="hlt">variables</span> that respond linearly to climate forcing will have become prone to much larger variations over the <span class="hlt">observational</span> record, whereas ecosystem <span class="hlt">variables</span> that respond nonlinearly to climate forcing will have become prone to more frequent "regime shifts." Thus, slowing down of North Pacific climate <span class="hlt">variability</span> can help explain the large magnitude and potentially the quick succession of well-known abrupt changes in North Pacific ecosystems in 1977 and 1989. When looking ahead, despite model limitations in simulating mixed layer depth (MLD) in the North Pacific, global warming is robustly expected to decrease MLD. This could potentially reverse the <span class="hlt">observed</span> trend of slowing down of North Pacific climate <span class="hlt">variability</span> and its effects on marine ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AtmRe.122...16B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AtmRe.122...16B"><span>Changes in temperature and precipitation extremes <span class="hlt">observed</span> in Modena, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boccolari, M.; Malmusi, S.</p> <p>2013-03-01</p> <p>Climate changes has become one of the most analysed subjects from researchers community, mainly because of the numerous extreme events that hit the globe. To have a better view of climate changes and trends, long <span class="hlt">observations</span> time series are needed. During last <span class="hlt">decade</span> a lot of Italian time series, concerning several surface meteorological <span class="hlt">variables</span>, have been analysed and published. No one of them includes one of the longest record in Italy, the time series of the Geophysical Observatory of the University of Modena and Reggio Emilia. Measurements, collected since early 19th century, always in the same position, except for some months during the second world war, embrace daily temperature, precipitation amount, relative humidity, pressure, cloudiness and other <span class="hlt">variables</span>. In this work we concentrated on the analysis of yearly and seasonal trends and climate extremes of temperature, both minimum and maximum, and precipitation time series, for the periods 1861-2010 and 1831-2010 respectively, in which continuous measurements are available. In general, our results confirm quite well those reported by IPCC and in many other studies over Mediterranean area. In particular, we found that minimum temperature has a non significant positive trend of + 0.1 °C per <span class="hlt">decade</span> considering all the period, the value increases to 0.9 °C per <span class="hlt">decade</span> for 1981-2010. For maximum temperature we <span class="hlt">observed</span> a non significant + 0.1 °C trend for all the period, while + 0.8 °C for the last thirty years. On the other hand precipitation is decreasing, -6.3 mm per <span class="hlt">decade</span>, considering all the analysed period, while the last thirty years are characterised by a great increment of 74.8 mm per <span class="hlt">decade</span>. For both <span class="hlt">variables</span> several climate indices have been analysed and they confirm what has been found for minimum and maximum temperatures and precipitation. In particular, during last 30 years frost days and ice days are decreasing, whereas summer days are increasing. During the last 30-year tropical nights</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/877008-variability-radiosonde-observed-precipitable-water-baltic-region','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/877008-variability-radiosonde-observed-precipitable-water-baltic-region"><span><span class="hlt">Variability</span> of Radiosonde-<span class="hlt">Observed</span> Precipitable Water in the Baltic Region</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Jakobson, Erko; Ohvril, H.; Okulov, O.</p> <p></p> <p>The total mass of columnar water vapor (precipitable water, W) is an important parameter of atmospheric thermodynamic and radiative models. In this work radiosonde <span class="hlt">observations</span> from 17 aerological stations in the Baltic region during 14 years, 1989?2002, were used to examine the <span class="hlt">variability</span> of precipitable water. A table of monthly and annual means of W for the stations is given. Seasonal and annual means of W are expressed as linear functions of geographical latitude. Linear formulas are also derived for parameterization of precipitable water as function of surface water vapor pressure at each station.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A21E0116R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A21E0116R"><span><span class="hlt">Observing</span> <span class="hlt">Decadal</span> Trends in Atmospheric Feedbacks and Climate Change with Zeus and CLARREO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Revercomb, H. E.; Best, F. A.; Knuteson, R. O.; Tobin, D. C.; Taylor, J. K.; Gero, P.; Adler, D. P.; Pettersen, C.; Mulligan, M.; Tobin, D. C.</p> <p>2012-12-01</p> <p>New technologies for <span class="hlt">observing</span> <span class="hlt">decadal</span> trends in atmospheric feedbacks and climate change from space have been recently demonstrated via a NASA Instrument Incubator Program (IIP) project of our group and the Anderson Group of Harvard University. Using these new technologies, a mission named Zeus has been proposed to the first NASA Earth Venture Instruments opportunity (EVI-1). Zeus would provide a low cost mechanism to initiate a new era in high spectral resolution IR climate Benchmark and Intercalibration <span class="hlt">observations</span>, the basis for which has been established by definition of the CLARREO mission in the 2007 NRC "<span class="hlt">Decadal</span> Survey" and by the Science Definition Team established by NASA LaRC to further the full blown CLARREO mission. Zeus EVI is a low-cost, low-risk, and high-value EVI mission that will deploy an Absolute Radiance Interferometer (ARI) instrument to measure absolute spectrally resolved infrared radiance over much of the Earth-emitted spectrum with ultra-high accuracy (<0.1 K 3-sigma brightness temperature). Zeus makes use of broad spectral coverage (3.7-50 microns) and high spectral resolution (<1 cm-1) to provide benchmark products for climate trending with much higher information content than traditional spectrally-integrated measurements. While ARI requirements for accuracy and spectral properties are demanding, the overall instrument is relatively simple and low-cost because of the limited requirements on spatial sampling (25-100 km nadir-only footprints spaced at < 250 km) and on noise performance (climate products are created by combining many samples). The orbit chosen for Zeus must provide coverage immune to time-of-day sampling errors. Because of its relatively high rate of precession, an attractive baseline option for Zeus EVI is the 51.6 degrees inclination orbit of the International Space Station (ISS). For Zeus deployment on the ISS, higher latitude climate benchmark information will be obtained from operational sounders intercalibrated by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OcSci..14..417S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OcSci..14..417S"><span>Transport <span class="hlt">variability</span> of the Brazil Current from <span class="hlt">observations</span> and a data assimilation model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmid, Claudia; Majumder, Sudip</p> <p>2018-06-01</p> <p>The Brazil Current transports from <span class="hlt">observations</span> and the Hybrid Coordinate Model (HYCOM) model are analyzed to improve our understanding of the current's structure and <span class="hlt">variability</span>. A time series of the <span class="hlt">observed</span> transport is derived from a three-dimensional field of the velocity in the South Atlantic covering the years 1993 to 2015 (hereinafter called Argo & SSH). The mean transports of the Brazil Current increases from 3.8 ± 2.2 Sv (1 Sv is 106 m3 s-1) at 25° S to 13.9 ± 2.6 Sv at 32° S, which corresponds to a mean slope of 1.4 ± 0.4 Sv per degree. Transport estimates derived from HYCOM fields are somewhat higher (5.2 ± 2.7 and 18.7 ± 7.1 Sv at 25 and 32° S, respectively) than those from Argo & SSH, but these differences are small when compared with the standard deviations. Overall, the <span class="hlt">observed</span> latitude dependence of the transport of the Brazil Current is in agreement with the wind-driven circulation in the super gyre of the subtropical South Atlantic. A mean annual cycle with highest (lowest) transports in austral summer (winter) is found to exist at selected latitudes (24, 35, and 38° S). The significance of this signal shrinks with increasing latitude (both in Argo & SSH and HYCOM), mainly due to mesoscale and interannual <span class="hlt">variability</span>. Both Argo & SSH, as well as HYCOM, reveal interannual <span class="hlt">variability</span> at 24 and 35° S that results in relatively large power at periods of 2 years or more in wavelet spectra. It is found that the interannual <span class="hlt">variability</span> at 24° S is correlated with the South Atlantic Subtropical Dipole Mode (SASD), the Southern Annular Mode (SAM), and the Niño 3.4 index. Similarly, correlations between SAM and the Brazil Current transport are also found at 35° S. Further investigation of the <span class="hlt">variability</span> reveals that the first and second mode of a coupled empirical orthogonal function of the meridional transport and the sea level pressure explain 36 and 15 % of the covariance, respectively. Overall, the results indicate that</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22127076-observations-thermal-flare-plasma-euv-variability-experiment','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22127076-observations-thermal-flare-plasma-euv-variability-experiment"><span><span class="hlt">OBSERVATIONS</span> OF THERMAL FLARE PLASMA WITH THE EUV <span class="hlt">VARIABILITY</span> EXPERIMENT</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Warren, Harry P.; Doschek, George A.; Mariska, John T.</p> <p>2013-06-20</p> <p>One of the defining characteristics of a solar flare is the impulsive formation of very high temperature plasma. The properties of the thermal emission are not well understood, however, and the analysis of solar flare <span class="hlt">observations</span> is often predicated on the assumption that the flare plasma is isothermal. The EUV <span class="hlt">Variability</span> Experiment (EVE) on the Solar Dynamics Observatory provides spectrally resolved <span class="hlt">observations</span> of emission lines that span a wide range of temperatures (e.g., Fe XV-Fe XXIV) and allow for thermal flare plasma to be studied in detail. In this paper we describe a method for computing the differential emission measuremore » distribution in a flare using EVE <span class="hlt">observations</span> and apply it to several representative events. We find that in all phases of the flare the differential emission measure distribution is broad. Comparisons of EVE spectra with calculations based on parameters derived from the Geostationary Operational Environmental Satellites soft X-ray fluxes indicate that the isothermal approximation is generally a poor representation of the thermal structure of a flare.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.476.2501A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.476.2501A"><span>Short time-scale optical <span class="hlt">variability</span> properties of the largest AGN sample <span class="hlt">observed</span> with Kepler/K2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aranzana, E.; Körding, E.; Uttley, P.; Scaringi, S.; Bloemen, S.</p> <p>2018-05-01</p> <p>We present the first short time-scale (˜hours to days) optical <span class="hlt">variability</span> study of a large sample of active galactic nuclei (AGNs) <span class="hlt">observed</span> with the Kepler/K2 mission. The sample contains 252 AGN <span class="hlt">observed</span> over four campaigns with ˜30 min cadence selected from the Million Quasar Catalogue with R magnitude <19. We performed time series analysis to determine their <span class="hlt">variability</span> properties by means of the power spectral densities (PSDs) and applied Monte Carlo techniques to find the best model parameters that fit the <span class="hlt">observed</span> power spectra. A power-law model is sufficient to describe all the PSDs of our sample. A variety of power-law slopes were found indicating that there is not a universal slope for all AGNs. We find that the rest-frame amplitude <span class="hlt">variability</span> in the frequency range of 6 × 10-6-10-4 Hz varies from 1to10 per cent with an average of 1.7 per cent. We explore correlations between the <span class="hlt">variability</span> amplitude and key parameters of the AGN, finding a significant correlation of rest-frame short-term <span class="hlt">variability</span> amplitude with redshift. We attribute this effect to the known `bluer when brighter' <span class="hlt">variability</span> of quasars combined with the fixed bandpass of Kepler data. This study also enables us to distinguish between Seyferts and blazars and confirm AGN candidates. For our study, we have compared results obtained from light curves extracted using different aperture sizes and with and without detrending. We find that limited detrending of the optimal photometric precision light curve is the best approach, although some systematic effects still remain present.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22663838-variable-stars-observed-galactic-disk-ast3-from-dome-antarctica','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22663838-variable-stars-observed-galactic-disk-ast3-from-dome-antarctica"><span><span class="hlt">Variable</span> Stars <span class="hlt">Observed</span> in the Galactic Disk by AST3-1 from Dome A, Antarctica</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Wang, Lingzhi; Ma, Bin; Hu, Yi</p> <p></p> <p>AST3-1 is the second-generation wide-field optical photometric telescope dedicated to time-domain astronomy at Dome A, Antarctica. Here, we present the results of an i -band images survey from AST3-1 toward one Galactic disk field. Based on time-series photometry of 92,583 stars, 560 <span class="hlt">variable</span> stars were detected with i magnitude ≤16.5 mag during eight days of <span class="hlt">observations</span>; 339 of these are previously unknown <span class="hlt">variables</span>. We tentatively classify the 560 <span class="hlt">variables</span> as 285 eclipsing binaries (EW, EB, and EA), 27 pulsating <span class="hlt">variable</span> stars ( δ Scuti, γ Doradus, δ Cephei <span class="hlt">variable</span>, and RR Lyrae stars), and 248 other types of <span class="hlt">variables</span> (unclassifiedmore » periodic, multiperiodic, and aperiodic <span class="hlt">variable</span> stars). Of the eclipsing binaries, 34 show O’Connell effects. One of the aperiodic <span class="hlt">variables</span> shows a plateau light curve and another <span class="hlt">variable</span> shows a secondary maximum after peak brightness. We also detected a complex binary system with an RS CVn-like light-curve morphology; this object is being followed-up spectroscopically using the Gemini South telescope.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/20472','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/20472"><span>Environmental <span class="hlt">variability</span> and indicators: a few <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>William F. Laudenslayer</p> <p>1991-01-01</p> <p>Abstract The environment of the earth is exceedingly complex and <span class="hlt">variable</span>. Indicator species are used to reduce thaf complexity and <span class="hlt">variability</span> to a level that can be more emily understood. In recent years, use of indicators has increased dramatically. For the Forest Service, as an example, regulations that interpret the National Forest Management Act require the use...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160012763','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160012763"><span>Contribution of Phenological and Physiological Variations on Northern Vegetation Productivity Changes over Last Three <span class="hlt">Decades</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ganguly, Sangram</p> <p>2015-01-01</p> <p>Plant phenology and maximum photosynthetic state determine spatiotemporal <span class="hlt">variability</span> of gross primary productivity (GPP) of vegetation. Recent warming induced impacts accelerate shifts of phenology and physiological status over Northern vegetated land. Thus, understanding and quantifying these changes are very important. Here, we investigate 1) how vegetation phenology and physiological status (maximum photosynthesis) are evolved over last three <span class="hlt">decades</span> and 2) how such components (phenology and physiological status) contribute on inter-annual variation of the GPP during the last three <span class="hlt">decades</span>. We utilized both long-term remotely sensed (GIMMS (Global Inventory Modeling and Mapping Studies), NDVI3g (Normalized Difference Vegetation Index 3rd generation) and MODIS (Moderate Resolution Imaging Spectroradiometer)) to extract larger scale phenology metrics (growing season start, end and duration); and productivity (i.e., growing season integrated vegetation index, GSIVI) to answer these questions. For evaluation purpose, we also introduced field-measured phenology and productivity datasets (e.g., FLUXNET) and possible remotely-sensed and modeled metrics at continental and regional scales. From this investigation, we found that onset of the growing season has advanced by 1.61 days per <span class="hlt">decade</span> and the growing season end has delayed by 0.67 days per <span class="hlt">decade</span> over the circumpolar region. This asymmetric extension of growing season results in a longer growing-season trend (2.96 days per <span class="hlt">decade</span>) and widespread increasing vegetation-productivity trend (2.96 GSIVI per <span class="hlt">decade</span>) over Northern land. However, the regionally-diverged phenology shift and maximum photosynthetic state contribute differently characterized productivity, inter-annual <span class="hlt">variability</span> and trend. We quantified that about 50 percent, 13 percent and 6.5 percent of Northern land's inter-annual <span class="hlt">variability</span> are dominantly controlled by the onset of the growing season, the end of the growing season and the maximum</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070038262&hterms=passive+transport&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dpassive%2Btransport','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070038262&hterms=passive+transport&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dpassive%2Btransport"><span>Interannual and <span class="hlt">Decadal</span> <span class="hlt">Variability</span> of Ocean Surface Latent Heat Flux as Seen from Passive Microwave Satellite Algorithms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robertson, Franklin R.; Jackson, Darren L.; Wick, Gary A.; Roberts, Brent; Miller, Tim L.</p> <p>2007-01-01</p> <p>Ocean surface turbulent fluxes are critical links in the climate system since they mediate energy exchange between the two fluid systems (ocean and atmosphere) whose combined heat transport determines the basic character of Earth's climate. Deriving physically-based latent and sensible heat fluxes from satellite is dependent on inferences of near surface moisture and temperature from coarser layer retrievals or satellite radiances. Uncertainties in these "retrievals" propagate through bulk aerodynamic algorithms, interacting as well with error properties of surface wind speed, also provided by satellite. By systematically evaluating an array of passive microwave satellite algorithms, the SEAFLUX project is providing improved understanding of these errors and finding pathways for reducing or eliminating them. In this study we focus on evaluating the interannual <span class="hlt">variability</span> of several passive microwave-based estimates of latent heat flux starting from monthly mean gridded data. The algorithms considered range from those based essentially on SSM/I (e.g. HOAPS) to newer approaches that consider additional moisture information from SSM/T-2 or AMSU-B and lower tropospheric temperature data from AMSU-A. On interannual scales, <span class="hlt">variability</span> arising from ENSO events and time-lagged responses of ocean turbulent and radiative fluxes in other ocean basins (as well as the extratropical Pacific) is widely recognized, but still not well quantified. Locally, these flux anomalies are of order 10-20 W/sq m and present a relevant "target" with which to verify algorithm performance in a climate context. On <span class="hlt">decadal</span> time scales there is some evidence from reanalyses and remotely-sensed fluxes alike that tropical ocean-averaged latent heat fluxes have increased 5-10 W/sq m since the early 1990s. However, significant uncertainty surrounds this estimate. Our work addresses the origin of these uncertainties and provides statistics on time series of tropical ocean averages, regional space</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915271B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915271B"><span>Where is PM gone? Trends and <span class="hlt">variability</span> of atmospheric PM10, PM2.5 and PM10-2.5 in the Po valley over the last <span class="hlt">decade</span> (and more).</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bigi, Alessandro; Ghermandi, Grazia</p> <p>2017-04-01</p> <p>The Po Valley is one of the largest European regions with a remarkably high concentration level of atmospheric pollutants, both for particulate and gaseous compounds. In the last <span class="hlt">decade</span> stringent regulations on air quality standards and on anthropogenic emissions have been set by the European Commission, leading to an overall improvement in air quality across Europe. In order to assess the <span class="hlt">decadal</span> pattern and <span class="hlt">variability</span> in PM across the Po valley we thoroughly investigated the time series of PM10, PM2.5 and PM10-2.5 from 41, 44 and 15 sites respectively (Bigi & Ghermandi 2014, 2016). PM2.5 and PM10-2.5 (PM10) series with a 7 (10) year or longer record have been analysed for long term trend in deseasonalized monthly means, annual quantiles and in monthly frequency distribution by robust statistical methods. A widespread and significant decreasing trend was <span class="hlt">observed</span> at several sites for all size fractions, with the drop, up to a few percent per year, occurring mainly in winter for PM2.5 and throughout the year for PM10. All series were tested for a significant weekly periodicity (a proxy to estimate the impact of primary anthropogenic emissions) by 3 different statistical methods, yielding positive results for summer PM2.5 and PM10, and for both summer and winter PM10-2.5. Hierarchical cluster analysis showed larger <span class="hlt">variability</span> for PM10 than for PM2.5. The former was split in five clusters: two encompassing the metropolitan areas of Turin and Milan and their respective nearby sites and the other three clusters gathering northeast, northwest and central Po Valley sites respectively. PM2.5 clusters divide the valley in western, eastern and southern/Apennines foothill sectors. The trend in atmospheric concentration was compared with the time series of local primary and precursor emissions, vehicular fleet details and fuel sales. A significant basin-wide drop in emissions occurred for gaseous pollutants, contrarily to primary emissions of PM10 and PM2.5, whose drop was</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PIAHS.364..526L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PIAHS.364..526L"><span>Reservoirs performances under climate <span class="hlt">variability</span>: a case study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Longobardi, A.; Mautone, M.; de Luca, C.</p> <p>2014-09-01</p> <p>A case study, the Piano della Rocca dam (southern Italy) is discussed here in order to quantify the system performances under climate <span class="hlt">variability</span> conditions. Different climate scenarios have been stochastically generated according to the tendencies in precipitation and air temperature <span class="hlt">observed</span> during recent <span class="hlt">decades</span> for the studied area. Climate <span class="hlt">variables</span> have then been filtered through an ARMA model to generate, at the monthly scale, time series of reservoir inflow volumes. Controlled release has been computed considering the reservoir is operated following the standard linear operating policy (SLOP) and reservoir performances have been assessed through the calculation of reliability, resilience and vulnerability indices (Hashimoto et al. 1982), comparing current and future scenarios of climate <span class="hlt">variability</span>. The proposed approach can be suggested as a valuable tool to mitigate the effects of moderate to severe and persistent droughts periods, through the allocation of new water resources or the planning of appropriate operational rules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9787E..1CD','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9787E..1CD"><span>Inter-<span class="hlt">observer</span> <span class="hlt">variability</span> within BI-RADS and RANZCR mammographic density assessment schemes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Damases, Christine N.; Mello-Thoms, Claudia; McEntee, Mark F.</p> <p>2016-03-01</p> <p>This study compares <span class="hlt">variability</span> associated with two visual mammographic density (MD) assessment methods using two separate samples of radiologists. The image test-set comprised of images obtained from 20 women (age 42-89 years). The images were assessed for their MD by twenty American Board of Radiology (ABR) examiners and twenty-six radiologists registered with the Royal Australian and New Zealand College of Radiologists (RANZCR). Images were assessed using the same technology and conditions, however the ABR radiologists used the BI-RADS and the RANZCR radiologists used the RANZCR breast density synoptic. Both scales use a 4-point assessment. The images were then grouped as low- and high-density; low including BIRADS 1 and 2 or RANZCR 1 and 2 and high including BI-RADS 3 and 4 or RANZCR 3 and 4. Four-point BI-RADS and RANZCR showed no or negligible correlation (ρ=-0.029 p<0.859). The average inter-<span class="hlt">observer</span> agreement on the BI-RADS scale had a Kappa of 0.565; [95% CI = 0.519 - 0.610], and ranged between 0.328-0.669 while the inter-<span class="hlt">observer</span> agreement using the RANZCR scale had a Kappa of 0.360; [95% CI = 0.308 - 0.412] and a range of 0.078-0.499. Our findings show a wider range of inter-<span class="hlt">observer</span> <span class="hlt">variability</span> among RANZCR registered radiologists than the ABR examiners.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001JGR...10631693T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001JGR...10631693T"><span><span class="hlt">Decadal</span> power in land air temperatures: Is it statistically significant?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thejll, Peter A.</p> <p>2001-12-01</p> <p>The geographical distribution and properties of the well-known 10-11 year signal in terrestrial temperature records is investigated. By analyzing the Global Historical Climate Network data for surface air temperatures we verify that the signal is strongest in North America and is similar in nature to that reported earlier by R. G. Currie. The <span class="hlt">decadal</span> signal is statistically significant for individual stations, but it is not possible to show that the signal is statistically significant globally, using strict tests. In North America, during the twentieth century, the <span class="hlt">decadal</span> <span class="hlt">variability</span> in the solar activity cycle is associated with the <span class="hlt">decadal</span> part of the North Atlantic Oscillation index series in such a way that both of these signals correspond to the same spatial pattern of cooling and warming. A method for testing statistical results with Monte Carlo trials on data fields with specified temporal structure and specific spatial correlation retained is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC13A1188R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC13A1188R"><span>Establishing a Real-Money Prediction Market for Climate on <span class="hlt">Decadal</span> Horizons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roulston, M. S.; Hand, D. J.; Harding, D. W.</p> <p>2016-12-01</p> <p>A plan to establish a not-for-profit prediction market that will allow participants to bet on the value of selected climate <span class="hlt">variables</span> <span class="hlt">decades</span> into the future will be presented. It is hoped that this market will provide an objective measure of the consensus view on climate change, including information concerning the uncertainty of climate projections. The proposed design of the market and the definition of the climate <span class="hlt">variables</span> underlying the contracts will be discussed, as well as relevant regulatory and legal issues.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040085502','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040085502"><span>Interannual <span class="hlt">Variability</span> of Snow and Ice and Impact on the Carbon Cycle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yung, Yuk L.</p> <p>2004-01-01</p> <p>The goal of this research is to assess the impact of the interannual <span class="hlt">variability</span> in snow/ice using global satellite data sets acquired in the last two <span class="hlt">decades</span>. This <span class="hlt">variability</span> will be used as input to simulate the CO2 interannual <span class="hlt">variability</span> at high latitudes using a biospheric model. The progress in the past few years is summarized as follows: 1) Albedo decrease related to spring snow retreat; 2) <span class="hlt">Observed</span> effects of interannual summertime sea ice variations on the polar reflectance; 3) The Northern Annular Mode response to Arctic sea ice loss and the sensitivity of troposphere-stratosphere interaction; 4) The effect of Arctic warming and sea ice loss on the growing season in northern terrestrial ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=carnegie&id=EJ1113154','ERIC'); return false;" href="https://eric.ed.gov/?q=carnegie&id=EJ1113154"><span>Investigating MBA Degrees Earned by Women: A <span class="hlt">Decade</span> of Change</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>McConnell, Cheryl; Rush, Douglas; Gartland, Myles</p> <p>2016-01-01</p> <p>The authors examined master of business administration (MBA) degrees earned by women at U.S. higher education institutions at three specific years spanning a <span class="hlt">decade</span>: 2003, 2008, and 2013 to determine whether there was a significant difference in the percentage of MBA degrees earned by women based on the independent <span class="hlt">variables</span> of institutional type,…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1212960M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1212960M"><span>Initializing <span class="hlt">decadal</span> climate predictions over the North Atlantic region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matei, Daniela Mihaela; Pohlmann, Holger; Jungclaus, Johann; Müller, Wolfgang; Haak, Helmuth; Marotzke, Jochem</p> <p>2010-05-01</p> <p><span class="hlt">Decadal</span> climate prediction aims to predict the internally-generated <span class="hlt">decadal</span> climate <span class="hlt">variability</span> in addition to externally-forced climate change signal. In order to achieve this it is necessary to start the predictions from the current climate state. In this study we investigate the forecast skill of the North Atlantic <span class="hlt">decadal</span> climate predictions using two different ocean initialization strategies. First we apply an assimilation of ocean synthesis data provided by the GECCO project (Köhl and Stammer, 2008) as initial conditions for the coupled model ECHAM5/MPI-OM. Hindcast experiments are then performed over the period 1952-2001. An alternative approach is one in which the subsurface ocean temperature and salinity are diagnosed from an ensemble of ocean model runs forced by the NCEP-NCAR atmospheric reanalyzes for the period 1948-2007, then nudge into the coupled model to produce initial conditions for the hindcast experiments. An anomaly coupling scheme is used in both approaches to avoid the hindcast drift and the associated initial shock. Differences between the two assimilation approaches are discussed by comparing them with the <span class="hlt">observational</span> data in key regions and processes. We asses the skill of the initialized <span class="hlt">decadal</span> hindcast experiments against the prediction skill of the non-initialized hindcasts simulation. We obtain an overview of the regions with the highest predictability from the regional distribution of the anomaly correlation coefficients and RMSE for the SAT. For the first year the hindcast skill is increased over almost all ocean regions in the NCEP-forced approach. This increase in the hindcast skill for the 1 year lead time is somewhat reduced in the GECCO approach. At lead time 5yr and 10yr, the skill enhancement is still found over the North Atlantic and North Pacific regions. We also consider the potential predictability of the Atlantic Meridional Overturning Circulation (AMOC) and Nordic Seas Overflow by comparing the predicted values to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoRL..41.3307S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoRL..41.3307S"><span>North American west coast summer low cloudiness: Broadscale <span class="hlt">variability</span> associated with sea surface temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schwartz, Rachel E.; Gershunov, Alexander; Iacobellis, Sam F.; Cayan, Daniel R.</p> <p>2014-05-01</p> <p>Six <span class="hlt">decades</span> of <span class="hlt">observations</span> at 20 coastal airports, from Alaska to southern California, reveal coherent interannual to interdecadal variation of coastal low cloudiness (CLC) from summer to summer over this broad region. The leading mode of CLC <span class="hlt">variability</span> represents coherent variation, accounting for nearly 40% of the total CLC variance spanning 1950-2012. This leading mode and the majority of individual airports exhibit decreased low cloudiness from the earlier to the later part of the record. Exploring climatic controls on CLC, we identify North Pacific Sea Surface Temperature anomalies, largely in the form of the Pacific <span class="hlt">Decadal</span> Oscillation (PDO) as well correlated with, and evidently helping to organize, the coherent patterns of summer coastal cloud <span class="hlt">variability</span>. Links from the PDO to summer CLC appear a few months in advance of the summer. These associations hold up consistently in interannual and interdecadal frequencies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4028693','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4028693"><span><span class="hlt">Decadal</span> Cycles in the Human Cardiovascular System</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Halberg, Franz; Cornelissen, Germaine; Sothern, Robert B.; Hillman, Dewayne; Watanabe, Yoshihiko; Haus, Erhard; Schwartzkopff, Othild; Best, William R.</p> <p>2013-01-01</p> <p>Seven of the eight authors of this report each performed physiologic self-surveillance, some around the clock for <span class="hlt">decades</span>. We here document the presence of long cycles (<span class="hlt">decadals</span>, including circaundecennians) in the time structure of systolic (S) and diastolic (D) blood pressure (BP) and heart rate (HR). Because of the non-stationary nature in time and space of these and other physiologic and environmental periodic components that, like the wind, can appear and disappear in a given or other geographic location at one or another time, they have been called “Aeolian”. The nonlinear estimation of the uncertainties of the periods (τs) of two or more <span class="hlt">variables</span> being compared has been used to determine whether these components are congruent or not, depending on whether their CIs (95% confidence intervals) overlap or not. Among others, congruence has been found for components with τs clustering around 10 years in us and around us. There is a selective assortment among individuals, <span class="hlt">variables</span> and cycle characteristics (mean and circadian amplitude and acrophase). Apart from basic interest, like other nonphotic solar signatures such as transyears with periods slightly longer than one year or about 33-year Brückner-Egeson-Lockyer (BEL) cycles, about 10-year and longer cycles present in 7 of 7 self-monitoring individuals are of interest in the diagnosis of Vascular <span class="hlt">Variability</span> Anomalies (VVAs), including MESOR-hypertension, and others. Some of the other VVAs, such as a circadian overswing, i.e., CHAT (Circadian Hyper-Aplitude-Tension), or an excessive pulse pressure, based on repeated 7-day around-the-clock records, can represent a risk of severe cardiovascular events, greater than that of a high BP. The differential diagnosis of physiologic cycles, infradians (components with a τ longer than 28 hours) as well as circadians awaits the collection of reference values for the infradian parameters of the cycles described herein. Just as in stroke-prone spontaneously</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.1857K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.1857K"><span>A data-model synthesis to explain <span class="hlt">variability</span> in calcification <span class="hlt">observed</span> during a CO2 perturbation mesocosm experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krishna, Shubham; Schartau, Markus</p> <p>2017-04-01</p> <p>The effect of ocean acidification on growth and calcification of the marine algae Emiliania huxleyi was investigated in a series of mesocosm experiments where enclosed water volumes that comprised a natural plankton community were exposed to different carbon dioxide (CO2) concentrations. Calcification rates <span class="hlt">observed</span> during those experiments were found to be highly <span class="hlt">variable</span>, even among replicate mesocosms that were subject to similar CO2 perturbations. Here, data from an ocean acidification mesocosm experiment are reanalysed with an optimality-based dynamical plankton model. According to our model approach, cellular calcite formation is sensitive to variations in CO2 at the organism level. We investigate the temporal changes and <span class="hlt">variability</span> in <span class="hlt">observations</span>, with a focus on resolving <span class="hlt">observed</span> differences in total alkalinity and particulate inorganic carbon (PIC). We explore how much of the <span class="hlt">variability</span> in the data can be explained by variations of the initial conditions and by the level of CO2 perturbation. Nine mesocosms of one experiment were sorted into three groups of high, medium, and low calcification rates and analysed separately. The spread of the three optimised ensemble model solutions captures most of the <span class="hlt">observed</span> <span class="hlt">variability</span>. Our results show that small variations in initial abundance of coccolithophores and the prevailing physiological acclimation states generate differences in calcification that are larger than those induced by ocean acidification. Accordingly, large deviations between optimal mass flux estimates of carbon and of nitrogen are identified even between mesocosms that were subject to similar ocean acidification conditions. With our model-based data analysis we document how an ocean acidification response signal in calcification can be disentangled from the <span class="hlt">observed</span> <span class="hlt">variability</span> in PIC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4196K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4196K"><span>The Angola Current and its seasonal <span class="hlt">variability</span> as <span class="hlt">observed</span> at 11°S</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kopte, Robert; Brandt, Peter; Dengler, Marcus; Claus, Martin; Greatbatch, Richard J.</p> <p>2016-04-01</p> <p>The eastern boundary circulation off the coast of Angola has been described only sparsely to date. The region off Angola, which connects the equatorial Atlantic and the Angola-Benguela upwelling regime, is of particular interest to understand the relative importance of transient equatorial versus local forcing of the <span class="hlt">observed</span> <span class="hlt">variability</span> in the coastal upwelling region. For the first time multi-year velocity <span class="hlt">observations</span> of the Angola Current at 11°S are available. From July 2013 to November 2015 a bottom shield equipped with an ADCP had been deployed at 500m water depth, accompanied by a mooring sitting on the 1200m-isobath with an ADCP being installed at 500m depth. Both upward-looking instruments measured the current speed up to about 50m below the sea surface. During the deployment period the Angola Current was characterized by a weak southward mean flow of 5-8 cm/s at 50m depth (slightly stronger at the in-shore mooring position), with the southward current penetrating down to about 200m depth. The alongshore velocity component reveals a pronounced seasonal <span class="hlt">variability</span>. It is dominated by 120-day, semi-annual, and annual oscillations with distinct baroclinic structures. Here we apply a reduced gravity model of the tropical Atlantic for the first five baroclinic modes forced with interannually varying wind stress to investigate the seasonal <span class="hlt">variability</span> along the equatorial and coastal waveguides. In the equatorial Atlantic the 120-day, semi-annual, and annual oscillations are associated with resonant basin modes of the 1st, 2nd, and 4th baroclinic mode, respectively. These basin modes are composed of equatorial Kelvin and Rossby waves as well as coastally trapped waves. The reduced gravity model is further used to study the respective role of the remote equatorial forcing, more specifically the influence of equatorial basin modes via coastally trapped waves, and the local forcing for the <span class="hlt">observed</span> seasonal <span class="hlt">variability</span> and associated baroclinic structure of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1339441','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1339441"><span>Water Stress on U.S. Power Production at <span class="hlt">Decadal</span> Time Horizons</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Ganguly, Auroop R.; Ganguli, Poulomi; Kumar, Devashish</p> <p>2014-09-01</p> <p>Thermoelectric power production at risk, owing to current and projected water scarcity and rising stream temperatures, is assessed for the contiguous United States at <span class="hlt">decadal</span> scales. Regional water scarcity is driven by climate <span class="hlt">variability</span> and change, as well as by multi-sector water demand. While a planning horizon of zero to about thirty years is occasionally prescribed by stakeholders, the challenges to risk assessment at these scales include the difficulty in delineating <span class="hlt">decadal</span> climate trends from intrinsic natural or multiple model <span class="hlt">variability</span>. Current generation global climate or earth system models are not credible at the spatial resolutions of power plants, especiallymore » for surface water quantity and stream temperatures, which further exacerbates the assessment challenge. Population changes, which are difficult to project, cannot serve as adequate proxies for changes in the water demand across sectors. The hypothesis that robust assessments of power production at risk are possible, despite the uncertainties, has been examined as a proof of concept. An approach is presented for delineating water scarcity and temperature from climate models, <span class="hlt">observations</span> and population storylines, as well as for assessing power production at risk by examining geospatial correlations of power plant locations within regions where the usable water supply for energy production happens to be scarcer and warmer. Our analyses showed that in the near term, more than 200 counties are likely to be exposed to water scarcity in the next three <span class="hlt">decades</span>. Further, we noticed that stream gauges in more than five counties in the 2030s and ten counties in the 2040s showed a significant increase in water temperature, which exceeded the power plant effluent temperature threshold set by the EPA. Power plants in South Carolina, Louisiana, and Texas are likely to be vulnerable owing to climate driven water stresses. In all, our analysis suggests that under various combinations of plausible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1806g0003H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1806g0003H"><span><span class="hlt">Variable</span> input <span class="hlt">observer</span> for structural health monitoring of high-rate systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hong, Jonathan; Laflamme, Simon; Cao, Liang; Dodson, Jacob</p> <p>2017-02-01</p> <p>The development of high-rate structural health monitoring methods is intended to provide damage detection on timescales of 10 µs -10ms where speed of detection is critical to maintain structural integrity. Here, a novel <span class="hlt">Variable</span> Input <span class="hlt">Observer</span> (VIO) coupled with an adaptive <span class="hlt">observer</span> is proposed as a potential solution for complex high-rate problems. The VIO is designed to adapt its input space based on real-time identification of the system's essential dynamics. By selecting appropriate time-delayed coordinates defined by both a time delay and an embedding dimension, the proper input space is chosen which allows more accurate estimations of the current state and a reduction of the convergence rate. The optimal time-delay is estimated based on mutual information, and the embedding dimension is based on false nearest neighbors. A simulation of the VIO is conducted on a two degree-of-freedom system with simulated damage. Results are compared with an adaptive Luenberger <span class="hlt">observer</span>, a fixed time-delay <span class="hlt">observer</span>, and a Kalman Filter. Under its preliminary design, the VIO converges significantly faster than the Luenberger and fixed <span class="hlt">observer</span>. It performed similarly to the Kalman Filter in terms of convergence, but with greater accuracy.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23G0304D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23G0304D"><span><span class="hlt">Decadal</span> climate simulations using the Climate Forecast System (CFS) coupled to the SSiB2 land surface model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Sales, F.; Xue, Y.; Marx, L.; Ek, M. B.</p> <p>2016-12-01</p> <p>The Simplified Simple Biophysical version 2 (SSiB2) model was implemented in the NCEP Climate Forecast System (CFS) for two 30-yr simulations. One simulation was initialized from CFS reanalysis data (EXP1), and the other from a 10-yr spin-up run (EXP2), in which the ocean model was allowed to run freely while the atmosphere and land surface were maintained constant to adjust inconsistencies in the initial conditions. EXP2 also includes an update in the SSiB2's average soil water potential calculation. The material presented highlights the model's performance in predicting spatial and temporal <span class="hlt">variability</span> of monthly precipitation and surface temperature and aims at determining the optimum configuration for longer simulations. In general, the model is able to reproduce the main features of large-scale precipitation, with spatial correlation (scorr) and RMSE of 0.8 and 1.4 mm day-1, respectively. A split ITCZ pattern is <span class="hlt">observed</span> in the Pacific and Indian oceans, which results in dry biases along the equator and wet-bias bands to its north and south. Positive biases are also <span class="hlt">observed</span> in the Atlantic ITCZ. The model generates consistent surface temperature climatology (scorr > 0.9, RMSE= 2.3°C). Warm biases are <span class="hlt">observed</span> especially over southern Asia during summer. Both experiments produce similar precipitation climatology patterns with similar biases. EXP2, however, improves the temperature simulation by reducing the global bias by 48% and 26% during boreal winter and summer, respectively; and improves the temperature <span class="hlt">decadal</span> <span class="hlt">variability</span> for many areas. Moreover, EXP2 generates a better continental surface air warming trend. In the attempt to improve the precipitation <span class="hlt">decadal</span> <span class="hlt">variability</span> in the simulations, remotely-sensed LAI and vegetation cover fraction have been implemented in the CFS/SSiB2 to substitute the look-up table originally used in EXP1 and 2. The satellite vegetation data has been processed into global monthly maps which are continuous updated throughout</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ERL.....7b4019D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ERL.....7b4019D"><span>A century of hydrological <span class="hlt">variability</span> and trends in the Fraser River Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Déry, Stephen J.; Hernández-Henríquez, Marco A.; Owens, Philip N.; Parkes, Margot W.; Petticrew, Ellen L.</p> <p>2012-06-01</p> <p>This study examines the 1911-2010 <span class="hlt">variability</span> and trends in annual streamflow at 139 sites across the Fraser River Basin (FRB) of British Columbia (BC), Canada. The Fraser River is the largest Canadian waterway flowing to the Pacific Ocean and is one of the world’s greatest salmon rivers. Our analyses reveal high runoff rates and low interannual <span class="hlt">variability</span> in alpine and coastal rivers, and low runoff rates and high interannual <span class="hlt">variability</span> in most streams in BC’s interior. The interannual <span class="hlt">variability</span> in streamflow is also low in rivers such as the Adams, Chilko, Quesnel and Stuart where the principal salmon runs of the Fraser River occur. A trend analysis shows a spatially coherent signal with increasing interannual <span class="hlt">variability</span> in streamflow across the FRB in recent <span class="hlt">decades</span>, most notably in spring and summer. The upward trend in the coefficient of variation in annual runoff coincides with a period of near-normal annual runoff for the Fraser River at Hope. The interannual <span class="hlt">variability</span> in streamflow is greater in regulated rather than natural systems; however, it is unclear whether it is predominantly flow regulation that leads to these <span class="hlt">observed</span> differences. Environmental changes such as rising air temperatures, more frequent polarity changes in large-scale climate teleconnections such as El Niño-Southern Oscillation and Pacific <span class="hlt">Decadal</span> Oscillation, and retreating glaciers may be contributing to the greater range in annual runoff fluctuations across the FRB. This has implications for ecological processes throughout the basin, for example affecting migrating and spawning salmon, a keystone species vital to First Nations communities as well as to commercial and recreational fisheries. To exemplify this linkage between <span class="hlt">variable</span> flows and biological responses, the unusual FRB runoff anomalies <span class="hlt">observed</span> in 2010 are discussed in the context of that year’s sockeye salmon run. As the climate continues to warm, greater <span class="hlt">variability</span> in annual streamflow, and hence in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22663416-understanding-solar-cycle-variability','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22663416-understanding-solar-cycle-variability"><span>Understanding Solar Cycle <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Cameron, R. H.; Schüssler, M., E-mail: cameron@mps.mpg.de</p> <p></p> <p>The level of solar magnetic activity, as exemplified by the number of sunspots and by energetic events in the corona, varies on a wide range of timescales. Most prominent is the 11-year solar cycle, which is significantly modulated on longer timescales. Drawing from dynamo theory, together with the empirical results of past solar activity and similar phenomena for solar-like stars, we show that the <span class="hlt">variability</span> of the solar cycle can be essentially understood in terms of a weakly nonlinear limit cycle affected by random noise. In contrast to ad hoc “toy models” for the solar cycle, this leads to amore » generic normal-form model, whose parameters are all constrained by <span class="hlt">observations</span>. The model reproduces the characteristics of the <span class="hlt">variable</span> solar activity on timescales between <span class="hlt">decades</span> and millennia, including the occurrence and statistics of extended periods of very low activity (grand minima). Comparison with results obtained with a Babcock–Leighton-type dynamo model confirm the validity of the normal-mode approach.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC41B1095W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC41B1095W"><span>Advancing a Model-Validated Statistical Method for Decomposing the Key Oceanic Drivers of <span class="hlt">Observed</span> Regional Climate <span class="hlt">Variability</span> and Evaluating Model Performance: Focus on North African Rainfall in CESM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, F.; Notaro, M.; Yu, Y.; Mao, J.; Shi, X.; Wei, Y.</p> <p>2016-12-01</p> <p>North (N.) African rainfall is characterized by dramatic interannual to <span class="hlt">decadal</span> <span class="hlt">variability</span> with serious socio-economic ramifications. The Sahel and West African Monsoon (WAM) region experienced a dramatic shift to persistent drought by the late 1960s, while the Horn of Africa (HOA) underwent drying since the 1990s. Large disagreementregarding the dominant oceanic drivers of N. African hydrologic <span class="hlt">variability</span> exists among modeling studies, leading to notable spread in Sahel summer rainfall projections for this century among Coupled Model Intercomparison Project models. In order to gain a deeper understanding of the oceanic drivers of N. African rainfall and establish a benchmark for model evaluation, a statistical method, the multivariate Generalized Equilibrium Feedback Assessment, is validated and applied to <span class="hlt">observations</span> and a control run from the Community Earth System Model (CESM). This study represents the first time that the dominant oceanic drivers of N. African rainfall were evaluated and systematically compared between <span class="hlt">observations</span> and model simulations. CESM and the <span class="hlt">observations</span> consistently agree that tropical oceanic modes are the dominant controls of N. African rainfall. During the monsoon season, CESM and <span class="hlt">observations</span> agree that an anomalously warm eastern tropical Pacific shifts the Walker Circulation eastward, with its descending branch supporting Sahel drying. CESM and the <span class="hlt">observations</span> concur that a warmer tropical eastern Atlantic favors a southward-shifted Intertropical Convergence Zone, which intensifies WAM monsoonal rainfall. An <span class="hlt">observed</span> reduction in Sahel rainfall accompanies this enhanced WAM rainfall, yet is confined to the Atlantic in CESM. During the short rains, both <span class="hlt">observations</span> and CESM indicate that a positive phase of tropical Indian Ocean dipole (IOD) mode [anomalously warm (cold) in western (eastern) Indian] enhances HOA rainfall. The <span class="hlt">observed</span> IOD impacts are limited to the short rains, while the simulated impacts are year-round.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009DPS....41.1632T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DPS....41.1632T"><span>Rings Research in the Next <span class="hlt">Decade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tiscareno, Matthew S.; Albers, N.; Brahic, A.; Brooks, S. M.; Burns, J. A.; Chavez, C.; Colwell, J. E.; Cuzzi, J. N.; de Pater, I.; Dones, L.; Durisen, R. H.; Filacchione, G.; Giuliatti Winter, S. M.; Gordon, M. K.; Graps, A.; Hamilton, D. P.; Hedman, M. M.; Horanyi, M.; Kempf, S.; Krueger, H.; Lewis, M. C.; Lissauer, J. J.; Murray, C. D.; Nicholson, P. D.; Olkin, C. B.; Pappalardo, R. T.; Salo, H.; Schmidt, J.; Showalter, M. R.; Spahn, F.; Spilker, L. J.; Srama, R.; Sremcevic, M.; Stewart, G. R.; Yanamandra-Fisher, P.</p> <p>2009-12-01</p> <p>The study of planetary ring systems is a key component of planetary science for several reasons: 1) The evolution and current states of planets and their satellites are affected in many ways by rings, while 2) conversely, properties of planets and moons and other solar system populations are revealed by their effects on rings; 3) highly structured and apparently delicate ring systems may be bellwethers, constraining various theories of the origin and evolution of their entire planetary system; and finally, 4) planetary rings provide an easily <span class="hlt">observable</span> analogue to other astrophysical disk systems, enabling real "ground truth” results applicable to disks much more remote in space and/or time, including proto-planetary disks, circum-stellar disks, and even galaxies. Significant advances have been made in rings science in the past <span class="hlt">decade</span>. The highest-priority rings research recommendations of the last Planetary Science <span class="hlt">Decadal</span> Survey were to operate and extend the Cassini orbiter mission at Saturn; this has been done with tremendous success, accounting for much of the progress made on key science questions, as we will describe. Important progress in understanding the rings of Saturn and other planets has also come from Earth-based <span class="hlt">observational</span> and theoretical work, again as prioritized by the last <span class="hlt">Decadal</span> Survey. However, much important work remains to be done. At Saturn, the Cassini Solstice Mission must be brought to a successful completion. Priority should also be placed on sending spacecraft to Neptune and/or Uranus, now unvisited for more than 20 years. At Jupiter and Pluto, opportunities afforded by visiting spacecraft capable of studying rings should be exploited. On Earth, the need for continued research and analysis remains strong, including in-depth analysis of rings data already obtained, numerical and theoretical modeling work, laboratory analysis of materials and processes analogous to those found in the outer solar system, and continued Earth</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..4311295S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..4311295S"><span>Greenland Ice Sheet flow response to runoff <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stevens, Laura A.; Behn, Mark D.; Das, Sarah B.; Joughin, Ian; Noël, Brice P. Y.; Broeke, Michiel R.; Herring, Thomas</p> <p>2016-11-01</p> <p>We use <span class="hlt">observations</span> of ice sheet surface motion from a Global Positioning System network operating from 2006 to 2014 around North Lake in west Greenland to investigate the dynamical response of the Greenland Ice Sheet's ablation area to interannual <span class="hlt">variability</span> in surface melting. We find no statistically significant relationship between runoff season characteristics and ice flow velocities within a given year or season. Over the 7 year time series, annual velocities at North Lake decrease at an average rate of -0.9 ± 1.1 m yr-2, consistent with the negative trend in annual velocities <span class="hlt">observed</span> in neighboring regions over recent <span class="hlt">decades</span>. We find that net runoff integrated over several preceding years has a negative correlation with annual velocities, similar to findings from the two other available <span class="hlt">decadal</span> records of ice velocity in western Greenland. However, we argue that this correlation is not necessarily evidence for a direct hydrologic mechanism acting on the timescale of multiple years but could be a statistical construct. Finally, we stress that neither the <span class="hlt">decadal</span> slowdown trend nor the negative correlation between velocity and integrated runoff is predicted by current ice-sheet models, underscoring that these models do not yet capture all the relevant feedbacks between runoff and ice dynamics needed to predict long-term trends in ice sheet flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARG40005C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARG40005C"><span>Causes and implications of the growing divergence between climate model simulations and <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Curry, Judith</p> <p>2014-03-01</p> <p>For the past 15+ years, there has been no increase in global average surface temperature, which has been referred to as a 'hiatus' in global warming. By contrast, estimates of expected warming in the first several <span class="hlt">decades</span> of 21st century made by the IPCC AR4 were 0.2C/<span class="hlt">decade</span>. This talk summarizes the recent CMIP5 climate model simulation results and comparisons with <span class="hlt">observational</span> data. The most recent climate model simulations used in the AR5 indicate that the warming stagnation since 1998 is no longer consistent with model projections even at the 2% confidence level. Potential causes for the model-<span class="hlt">observation</span> discrepancies are discussed. A particular focus of the talk is the role of multi-<span class="hlt">decadal</span> natural internal <span class="hlt">variability</span> on the climate <span class="hlt">variability</span> of the 20th and early 21st centuries. The ``stadium wave'' climate signal is described, which propagates across the Northern Hemisphere through a network of ocean, ice, and atmospheric circulation regimes that self-organize into a collective tempo. The stadium wave hypothesis provides a plausible explanation for the hiatus in warming and helps explain why climate models did not predict this hiatus. Further, the new hypothesis suggests how long the hiatus might last. Implications of the hiatus are discussed in context of climate model sensitivity to CO2 forcing and attribution of the warming that was <span class="hlt">observed</span> in the last quarter of the 20th century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.1824C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.1824C"><span><span class="hlt">Decadal</span> reanalysis of biogeochemical indicators and fluxes in the North West European shelf-sea ecosystem</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ciavatta, S.; Kay, S.; Saux-Picart, S.; Butenschön, M.; Allen, J. I.</p> <p>2016-03-01</p> <p>This paper presents the first <span class="hlt">decadal</span> reanalysis simulation of the biogeochemistry of the North West European shelf, along with a full evaluation of its skill, confidence, and value. An error-characterized satellite product for chlorophyll was assimilated into a physical-biogeochemical model of the North East Atlantic, applying a localized Ensemble Kalman filter. The results showed that the reanalysis improved the model simulation of assimilated chlorophyll in 60% of the study region. Model validation metrics showed that the reanalysis had skill in matching a large data set of in situ <span class="hlt">observations</span> for 10 ecosystem <span class="hlt">variables</span>. Spearman rank correlations were significant and higher than 0.7 for physical-chemical <span class="hlt">variables</span> (temperature, salinity, and oxygen), ˜0.6 for chlorophyll and nutrients (phosphate, nitrate, and silicate), and significant, though lower in value, for partial pressure of dissolved carbon dioxide (˜0.4). The reanalysis captured the magnitude of pH and ammonia <span class="hlt">observations</span>, but not their <span class="hlt">variability</span>. The value of the reanalysis for assessing environmental status and <span class="hlt">variability</span> has been exemplified in two case studies. The first shows that between 325,000 and 365,000 km2 of shelf bottom waters were vulnerable to oxygen deficiency potentially threatening bottom fishes and benthos. The second application confirmed that the shelf is a net sink of atmospheric carbon dioxide, but the total amount of uptake varies between 36 and 46 Tg C yr-1 at a 90% confidence level. These results indicate that the reanalysis output data set can inform the management of the North West European shelf ecosystem, in relation to eutrophication, fishery, and <span class="hlt">variability</span> of the carbon cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005GeoJI.160..721M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005GeoJI.160..721M"><span>Electromagnetic torques in the core and resonant excitation of <span class="hlt">decadal</span> polar motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mound, Jon E.</p> <p>2005-02-01</p> <p>Motion of the rotation axis of the Earth contains <span class="hlt">decadal</span> variations with amplitudes on the order of 10 mas. The origin of these <span class="hlt">decadal</span> polar motions is unknown. A class of rotational normal modes of the core-mantle system termed torsional oscillations are known to affect the length of day (LOD) at <span class="hlt">decadal</span> periods and have also been suggested as a possible excitation source for the <span class="hlt">observed</span> <span class="hlt">decadal</span> polar motion. Torsional oscillations involve relative motion between the outer core and the surrounding solid bodies, producing electromagnetic torques at the inner-core boundary (ICB) and core-mantle boundary (CMB). It has been proposed that the ICB torque can explain the excitation of the approximately 30-yr-period polar motion termed the Markowitz wobble. This paper uses the results of a torsional oscillation model to calculate the torques generated at Markowitz and other <span class="hlt">decadal</span> periods and finds, in contrast to previous results, that electromagnetic torques at the ICB can not explain the <span class="hlt">observed</span> polar motion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180003016','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180003016"><span>ACE Objectives, Current Status and the 2017 <span class="hlt">Decadal</span> Survey</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Da Silva, Arlindo</p> <p>2018-01-01</p> <p>In this talk we present an overview of the Aerosol-Cloud-Ecosystems (ACE) preformulation studies, a tier-2 satellite mission recommended by the 2007 <span class="hlt">Decadal</span> Survey. We discuss the current status of ACE measurement concepts and associated retrieval algorithms. We conclude with a brief discussion of the recommendations by the 2017 <span class="hlt">Decadal</span> Survey and how ACE accomplishments can inform the future Aerosol and Cloud, Convection & Precipitation Designated <span class="hlt">Observables</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JASTP..71..644S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JASTP..71..644S"><span>Seasonal and diurnal <span class="hlt">variability</span> of the meteor flux at high latitudes <span class="hlt">observed</span> using PFISR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sparks, J. J.; Janches, D.; Nicolls, M. J.; Heinselman, C. J.</p> <p>2009-05-01</p> <p>We report in this and a companion paper [Fentzke, J.T., Janches, D., Sparks, J.J., 2008. Latitudinal and seasonal <span class="hlt">variability</span> of the micrometeor input function: A study using model predictions and <span class="hlt">observations</span> from Arecibo and PFISR. Journal of Atmospheric and Solar-Terrestrial Physics, this issue, doi:10.1016/j.jastp.2008.07.015] a complete seasonal study of the micrometeor input function (MIF) at high latitudes using meteor head-echo radar <span class="hlt">observations</span> performed with the Poker Flat Incoherent Scatter Radar (PFISR). This flux is responsible for a number of atmospheric phenomena; for example, it could be the source of meteoric smoke that is thought to act as condensation nuclei in the formation of ice particles in the polar mesosphere. The <span class="hlt">observations</span> presented here were performed for full 24-h periods near the summer and winter solstices and spring and autumn equinoxes, times at which the seasonal <span class="hlt">variability</span> of the MIF is predicted to be large at high latitudes [Janches, D., Heinselman, C.J., Chau, J.L., Chandran, A., Woodman, R., 2006. Modeling of the micrometeor input function in the upper atmosphere <span class="hlt">observed</span> by High Power and Large Aperture Radars, JGR, 11, A07317, doi:10.1029/2006JA011628]. Precise altitude and radar instantaneous line-of-sight (radial) Doppler velocity information are obtained for each of the hundreds of events detected every day. We show that meteor rates, altitude, and radial velocity distributions have a large seasonal dependence. This seasonal <span class="hlt">variability</span> can be explained by a change in the relative location of the meteoroid sources with respect to the <span class="hlt">observer</span>. Our results show that the meteor flux into the upper atmosphere is strongly anisotropic and its characteristics must be accounted for when including this flux into models attempting to explain related aeronomical phenomena. In addition, the measured acceleration and received signal strength distribution do not seem to depend on season; which may suggest that these <span class="hlt">observed</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Geomo.281....1P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Geomo.281....1P"><span><span class="hlt">Decadal</span> changes in North Atlantic atmospheric circulation patterns recorded by sand spits since 1800 CE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poirier, Clément; Tessier, Bernadette; Chaumillon, Éric; Bertin, Xavier; Fruergaard, Mikkel; Mouazé, Dominique; Noël, Suzanne; Weill, Pierre; Wöppelmann, Guy</p> <p>2017-03-01</p> <p>Present-day coastal barriers represent around 15% of the world's oceanic shorelines, and play an important role as early warning indicators of environmental change. Among them, wave-dominated barriers are dynamic landforms that tend to migrate landward in response to storms and sea-level change. High rates of sediment supply can locally offset the global retrogradation trend, providing valuable records of past environmental change occurring on transgressive coasts. However, geochronological control limits the temporal resolution of such records to millennial or centennial timescales, and the <span class="hlt">decadal</span> or even faster response of wave-built barriers to historical climate changes is therefore poorly understood. In this study, we show that shoreline dynamics of sand spits reconstructed from old cartographic documents has been synchronous on both margins of the North Atlantic Ocean since about 1800 CE. Spit growth accelerated drastically during three periods lasting about 15 years, characterised by positive North Atlantic Oscillation (NAO) and negative East Atlantic-West Russia (EA-WR) atmospheric circulation patterns. These changes are in phase with periods of increased volcanic activity. We use a high-resolution wave hindcast (1948-2014 CE) in a reference area to confirm the association between NAO and EA-WR as a proxy for offshore and nearshore wave height and for associated longshore sediment transport (LST) involved in spit growth. A 24-month lagged correlation between sediment transport and volcanic aerosol optical thickness (concentration of ashes in the atmosphere) is <span class="hlt">observed</span>, suggesting that spit shoreline dynamics at the <span class="hlt">decadal</span> timescale is partially forced by external climate drivers via cascading effects on atmospheric circulation patterns and wave climate. Our results imply that NAO <span class="hlt">variability</span> alone is not sufficient to understand the evolution of wave-built coastal environments. The associated sediment record can be used to reconstruct multi-<span class="hlt">decadal</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005QJRMS.131.2665C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005QJRMS.131.2665C"><span>Water-vapour <span class="hlt">variability</span> within a convective boundary-layer assessed by large-eddy simulations and IHOP_2002 <span class="hlt">observations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couvreux, F.; Guichard, F.; Redelsperger, J. L.; Kiemle, C.; Masson, V.; Lafore, J. P.; Flamant, C.</p> <p>2005-10-01</p> <p>This study presents a comprehensive analysis of the <span class="hlt">variability</span> of water vapour in a growing convective boundary-layer (CBL) over land, highlighting the complex links between advection, convective activity and moisture heterogeneity in the boundary layer. A Large-eddy Simulation (LES) is designed, based on <span class="hlt">observations</span>, and validated, using an independent data-set collected during the International H2O Project (IHOP 2002) fieldexperiment. Ample information about the moisture distribution in space and time, as well as other important CBL parameters are acquired by mesonet stations, balloon soundings, instruments on-board two aircraft and the DLR airborne water-vapour differential-absorption lidar. Because it can deliver two-dimensional cross-sections at high spatial resolution (140 m horizontal, 200 m vertical), the airborne lidar offers valuable insights of small-scale moisture-<span class="hlt">variability</span> throughout the CBL. The LES is able to reproduce the development of the CBL in the morning and early afternoon, as assessed by comparisons of simulated mean profiles of key meteorological <span class="hlt">variables</span> with sounding data. Simulated profiles of the variance of water-vapour mixing-ratio were found to be in good agreement with the lidar-derived counterparts. Finally, probability-density functions of potential temperature, vertical velocity and water-vapour mixing-ratio calculated from the LES show great consistency with those derived from aircraft in situ measurements in the middle of the CBL. Downdraughts entrained from above the CBL are governing the scale of moisture <span class="hlt">variability</span>. Characteristic length-scales are found to be larger for water-vapour mixing-ratio than for temperature.The <span class="hlt">observed</span> water-vapour <span class="hlt">variability</span> exhibits contributions from different scales. The influence of the mesoscale (larger than LES domain size, i.e. 10 km) on the smaller-scale <span class="hlt">variability</span> is assessed using LES and <span class="hlt">observations</span>. The small-scale <span class="hlt">variability</span> of water vapour is found to be important and to be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996IJCli..16..861H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996IJCli..16..861H"><span>Interannual Rainfall <span class="hlt">Variability</span> in North-East Brazil: <span class="hlt">Observation</span> and Model Simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harzallah, A.; Rocha de Aragão, J. O.; Sadourny, R.</p> <p>1996-08-01</p> <p>The relationship between interannual <span class="hlt">variability</span> of rainfall in north-east Brazil and tropical sea-surface temperature is studied using <span class="hlt">observations</span> and model simulations. The simulated precipitation is the average of seven independent realizations performed using the Laboratoire de Météorologie Dynamique atmospheric general model forced by the 1970-1988 <span class="hlt">observed</span> sea-surface temperature. The model reproduces very well the rainfall anomalies (correlation of 091 between <span class="hlt">observed</span> and modelled anomalies). The study confirms that precipitation in north-east Brazil is highly correlated to the sea-surface temperature in the tropical Atlantic and Pacific oceans. Using the singular value decomposition method, we find that Nordeste rainfall is modulated by two independent oscillations, both governed by the Atlantic dipole, but one involving only the Pacific, the other one having a period of about 10 years. Correlations between precipitation in north-east Brazil during February-May and the sea-surface temperature 6 months earlier indicate that both modes are essential to estimate the quality of the rainy season.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012RvGeo..50.2005W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012RvGeo..50.2005W"><span>A review of global terrestrial evapotranspiration: <span class="hlt">Observation</span>, modeling, climatology, and climatic <span class="hlt">variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Kaicun; Dickinson, Robert E.</p> <p>2012-06-01</p> <p>This review surveys the basic theories, <span class="hlt">observational</span> methods, satellite algorithms, and land surface models for terrestrial evapotranspiration, E (or λE, i.e., latent heat flux), including a long-term <span class="hlt">variability</span> and trends perspective. The basic theories used to estimate E are the Monin-Obukhov similarity theory (MOST), the Bowen ratio method, and the Penman-Monteith equation. The latter two theoretical expressions combine MOST with surface energy balance. Estimates of E can differ substantially between these three approaches because of their use of different input data. Surface and satellite-based measurement systems can provide accurate estimates of diurnal, daily, and annual <span class="hlt">variability</span> of E. But their estimation of longer time <span class="hlt">variability</span> is largely not established. A reasonable estimate of E as a global mean can be obtained from a surface water budget method, but its regional distribution is still rather uncertain. Current land surface models provide widely different ratios of the transpiration by vegetation to total E. This source of uncertainty therefore limits the capability of models to provide the sensitivities of E to precipitation deficits and land cover change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ACP....16..195B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ACP....16..195B"><span>Can we explain the <span class="hlt">observed</span> methane <span class="hlt">variability</span> after the Mount Pinatubo eruption?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bândă, N.; Krol, M.; van Weele, M.; van Noije, T.; Le Sager, P.; Röckmann, T.</p> <p>2016-01-01</p> <p>The CH4 growth rate in the atmosphere showed large variations after the Pinatubo eruption in June 1991. A decrease of more than 10 ppb yr-1 in the growth rate over the course of 1992 was reported, and a partial recovery in the following year. Although several reasons have been proposed to explain the evolution of CH4 after the eruption, their contributions to the <span class="hlt">observed</span> variations are not yet resolved. CH4 is removed from the atmosphere by the reaction with tropospheric OH, which in turn is produced by O3 photolysis under UV radiation. The CH4 removal after the Pinatubo eruption might have been affected by changes in tropospheric UV levels due to the presence of stratospheric SO2 and sulfate aerosols, and due to enhanced ozone depletion on Pinatubo aerosols. The perturbed climate after the eruption also altered both sources and sinks of atmospheric CH4. Furthermore, CH4 concentrations were influenced by other factors of natural <span class="hlt">variability</span> in that period, such as El Niño-Southern Oscillation (ENSO) and biomass burning events. Emissions of CO, NOX and non-methane volatile organic compounds (NMVOCs) also affected CH4 concentrations indirectly by influencing tropospheric OH levels.<p class="p">Potential drivers of CH4 <span class="hlt">variability</span> are investigated using the TM5 global chemistry model. The contribution that each driver had to the global CH4 <span class="hlt">variability</span> during the period 1990 to 1995 is quantified. We find that a decrease of 8-10 ppb yr-1 CH4 is explained by a combination of the above processes. However, the timing of the minimum growth rate is found 6&nash;9 months later than <span class="hlt">observed</span>. The long-term decrease in CH4 growth rate over the period 1990 to 1995 is well captured and can be attributed to an increase in OH concentrations over this time period. Potential uncertainties in our modelled CH4 growth rate include emissions of CH4 from wetlands, biomass burning emissions of CH4 and other compounds, biogenic NMVOC and the sensitivity of OH to NMVOC emission changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACPD...1519111B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACPD...1519111B"><span>Can we explain the <span class="hlt">observed</span> methane <span class="hlt">variability</span> after the Mount Pinatubo eruption?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bândă, N.; Krol, M.; van Weele, M.; van Noije, T.; Le Sager, P.; Röckmann, T.</p> <p>2015-07-01</p> <p>The CH4 growth rate in the atmosphere showed large variations after the Pinatubo eruption in June 1991. A decrease of more than 10 ppb yr-1 in the growth rate over the course of 1992 was reported and a partial recovery in the following year. Although several reasons have been proposed to explain the evolution of CH4 after the eruption, their contributions to the <span class="hlt">observed</span> variations are not yet resolved. CH4 is removed from the atmosphere by the reaction with tropospheric OH, which in turn is produced by O3 photolysis under UV radiation. The CH4 removal after the Pinatubo eruption might have been affected by changes in tropospheric UV levels due to the presence of stratospheric SO2 and sulfate aerosols, and due to enhanced ozone depletion on Pinatubo aerosols. The perturbed climate after the eruption also altered both sources and sinks of atmospheric CH4. Furthermore, CH4 concentrations were influenced by other factors of natural <span class="hlt">variability</span> in that period, such as ENSO and biomass burning events. Emissions of CO, NOX and NMVOCs also affected CH4 concentrations indirectly by influencing tropospheric OH levels. Potential drivers of CH4 <span class="hlt">variability</span> are investigated using the TM5 global chemistry model. The contribution that each driver had to the global CH4 <span class="hlt">variability</span> during the period 1990 to 1995 is quantified. We find that a decrease of 8-10 ppb yr-1 CH4 is explained by a combination of the above processes. However, the timing of the minimum growth rate is found 6-9 months later than <span class="hlt">observed</span>. The long-term decrease in CH4 growth rate over the period 1990 to 1995 is well captured and can be attributed to an increase in OH concentrations over this time period. Potential uncertainties in our modelled CH4 growth rate include emissions of CH4 from wetlands, biomass burning emissions of CH4 and other compounds, biogenic NMVOC and the sensitivity of OH to NMVOC emission changes. Two inventories are used for CH4 emissions from wetlands, ORCHIDEE and LPJ, to investigate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED040096.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED040096.pdf"><span>Tradition and Change in the Social Studies: Some <span class="hlt">Observations</span> on a <span class="hlt">Decade</span> of Reform.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Lunstrum, John P.</p> <p></p> <p>Trends in social studies education in the 1960's which appeared significant and which may well affect the developments of the next <span class="hlt">decade</span> include: (1) curriculum evangelism--the zealous, uncritical pursuit of fashionable educational ideas--and the institutionalization of innovative changes, (2) restraints on intellectual freedom by the radical…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ApPhL.109i3101M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ApPhL.109i3101M"><span>Sub-60 mV/<span class="hlt">decade</span> switching in 2D negative capacitance field-effect transistors with integrated ferroelectric polymer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McGuire, Felicia A.; Cheng, Zhihui; Price, Katherine; Franklin, Aaron D.</p> <p>2016-08-01</p> <p>There is a rising interest in employing the negative capacitance (NC) effect to achieve sub-60 mV/<span class="hlt">decade</span> (below the thermal limit) switching in field-effect transistors (FETs). The NC effect, which is an effectual amplification of the applied gate potential, is realized by incorporating a ferroelectric material in series with a dielectric in the gate stack of a FET. One of the leading challenges to such NC-FETs is the <span class="hlt">variable</span> substrate capacitance exhibited in 3D semiconductor channels (bulk, Fin, or nanowire) that minimizes the extent of sub-60 mV/<span class="hlt">decade</span> switching. In this work, we demonstrate 2D NC-FETs that combine the NC effect with 2D MoS2 channels to extend the steep switching behavior. Using the ferroelectric polymer, poly(vinylidene difluoride-trifluoroethylene) (P(VDF-TrFE)), these 2D NC-FETs are fabricated by modification of top-gated 2D FETs through the integrated addition of P(VDF-TrFE) into the gate stack. The impact of including an interfacial metal between the ferroelectric and dielectric is studied and shown to be critical. These 2D NC-FETs exhibit a decrease in subthreshold swing from 113 mV/<span class="hlt">decade</span> down to 11.7 mV/<span class="hlt">decade</span> at room temperature with sub-60 mV/<span class="hlt">decade</span> switching occurring over more than 4 <span class="hlt">decades</span> of current. The P(VDF-TrFE) proves to be an unstable option for a device technology, yet the superb switching behavior <span class="hlt">observed</span> herein opens the way for further exploration of nanomaterials for extremely low-voltage NC-FETs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915061R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915061R"><span>Analysis of the regional MiKlip <span class="hlt">decadal</span> prediction system over Europe: skill, added value of regionalization, and ensemble size dependeny</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reyers, Mark; Moemken, Julia; Pinto, Joaquim; Feldmann, Hendrik; Kottmeier, Christoph; MiKlip Module-C Team</p> <p>2017-04-01</p> <p><span class="hlt">Decadal</span> climate predictions can provide a useful basis for decision making support systems for the public and private sectors. Several generations of <span class="hlt">decadal</span> hindcasts and predictions have been generated throughout the German research program MiKlip. Together with the global climate predictions computed with MPI-ESM, the regional climate model (RCM) COSMO-CLM is used for regional downscaling by MiKlip Module-C. The RCMs provide climate information on spatial and temporal scales closer to the needs of potential users. In this study, two downscaled hindcast generations are analysed (named b0 and b1). The respective global generations are both initialized by nudging them towards different reanalysis anomaly fields. An ensemble of five starting years (1961, 1971, 1981, 1991, and 2001), each comprising ten ensemble members, is used for both generations in order to quantify the regional <span class="hlt">decadal</span> prediction skill for precipitation and near-surface temperature and wind speed over Europe. All datasets (including hindcasts, <span class="hlt">observations</span>, reanalysis, and historical MPI-ESM runs) are pre-processed in an analogue manner by (i) removing the long-term trend and (ii) re-gridding to a common grid. Our analysis shows that there is potential for skillful <span class="hlt">decadal</span> predictions over Europe in the regional MiKlip ensemble, but the skill is not systematic and depends on the PRUDENCE region and the <span class="hlt">variable</span>. Further, the differences between the two hindcast generations are mostly small. As we used detrended time series, the predictive skill found in our study can probably attributed to reasonable predictions of anomalies which are associated with the natural climate <span class="hlt">variability</span>. In a sensitivity study, it is shown that the results may strongly change when the long-term trend is kept in the datasets, as here the skill of predicting the long-term trend (e.g. for temperature) also plays a major role. The regionalization of the global ensemble provides an added value for <span class="hlt">decadal</span> predictions for</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915977C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915977C"><span>Multi-<span class="hlt">decadal</span> frontal change rates of tidewater glaciers in the Canadian Arctic Archipelago</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cook, Alison; Copland, Luke; Stokes, Chris; Bentley, Mike</p> <p>2017-04-01</p> <p>Recent studies of post-2000 <span class="hlt">observational</span> data have shown <span class="hlt">variability</span> in the dynamic ice discharge of tidewater glaciers throughout the Canadian Arctic Archipelago (CAA). Expanding this to all tidewater glaciers in the region on a <span class="hlt">decadal</span> time scale using earlier records can help identify when glacier retreat began, and determine longer-term temporal trends in mass balance. Our study shows that over 94% of 300 tidewater glaciers in the CAA (from southern Baffin Island to Ellesmere Island, excluding those on the northern coast) have retreated since the earliest <span class="hlt">observational</span> records (aerial photographs acquired in 1958-1960). Mean overall length change rate of the 211 glaciers in the Queen Elizabeth Islands (QEI) is -9.3 ma-1 (± 1.38 SE), and of the 89 glaciers on Baffin and Bylot Islands (BBI) is -7.1 ma-1 (± 0.72 SE). Mean frontal widths of tidewater glaciers in the QEI are greater than those on islands to the south, resulting in greater mean area loss from this region. Each glacier has 6 frontal positions digitised from a range of image sources at approximately <span class="hlt">decadal</span> intervals. Length change rates have been calculated across each time interval for each glacier, based on area changes divided by glacier frontal width. Results indicate a similar temporal pattern throughout the region, whereby glaciers show minimal change in early years with retreat rates slowly increasing, followed by acceleration in retreat rates since the late 1990s. Mean change rates in the QEI and BBI in the 1960s were -6.92 ma-1 and -0.51 ma-1 respectively, increasing to -28.96 ma-1 and -24.84 ma-1 since 2010. The same trend (at differing magnitudes) has been <span class="hlt">observed</span> within each latitudinal degree band, and for glaciers of differing frontal widths. Further <span class="hlt">observations</span> of glacier changes and links to climate change are revealed on the poster.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170002646','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170002646"><span>Regionalizing Africa: Patterns of Precipitation <span class="hlt">Variability</span> in <span class="hlt">Observations</span> and Global Climate Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Badr, Hamada S.; Dezfuli, Amin K.; Zaitchik, Benjamin F.; Peters-Lidard, Christa D.</p> <p>2016-01-01</p> <p>Many studies have documented dramatic climatic and environmental changes that have affected Africa over different time scales. These studies often raise questions regarding the spatial extent and regional connectivity of changes inferred from <span class="hlt">observations</span> and proxies and/or derived from climate models. Objective regionalization offers a tool for addressing these questions. To demonstrate this potential, applications of hierarchical climate regionalizations of Africa using <span class="hlt">observations</span> and GCM historical simulations and future projections are presented. First, Africa is regionalized based on interannual precipitation <span class="hlt">variability</span> using Climate Hazards Group Infrared Precipitation with Stations (CHIRPS) data for the period 19812014. A number of data processing techniques and clustering algorithms are tested to ensure a robust definition of climate regions. These regionalization results highlight the seasonal and even month-to-month specificity of regional climate associations across the continent, emphasizing the need to consider time of year as well as research question when defining a coherent region for climate analysis. CHIRPS regions are then compared to those of five GCMs for the historic period, with a focus on boreal summer. Results show that some GCMs capture the climatic coherence of the Sahel and associated teleconnections in a manner that is similar to <span class="hlt">observations</span>, while other models break the Sahel into uncorrelated subregions or produce a Sahel-like region of <span class="hlt">variability</span> that is spatially displaced from <span class="hlt">observations</span>. Finally, shifts in climate regions under projected twenty-first-century climate change for different GCMs and emissions pathways are examined. A projected change is found in the coherence of the Sahel, in which the western and eastern Sahel become distinct regions with different teleconnections. This pattern is most pronounced in high-emissions scenarios.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IJSS...48.3419L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IJSS...48.3419L"><span><span class="hlt">Observer</span> synthesis for a class of Takagi-Sugeno descriptor system with unmeasurable premise <span class="hlt">variable</span>. Application to fault diagnosis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>López-Estrada, F. R.; Astorga-Zaragoza, C. M.; Theilliol, D.; Ponsart, J. C.; Valencia-Palomo, G.; Torres, L.</p> <p>2017-12-01</p> <p>This paper proposes a methodology to design a Takagi-Sugeno (TS) descriptor <span class="hlt">observer</span> for a class of TS descriptor systems. Unlike the popular approach that considers measurable premise <span class="hlt">variables</span>, this paper considers the premise <span class="hlt">variables</span> depending on unmeasurable vectors, e.g. the system states. This consideration covers a large class of nonlinear systems and represents a real challenge for the <span class="hlt">observer</span> synthesis. Sufficient conditions to guarantee robustness against the unmeasurable premise <span class="hlt">variables</span> and asymptotic convergence of the TS descriptor <span class="hlt">observer</span> are obtained based on the H∞ approach together with the Lyapunov method. As a result, the designing conditions are given in terms of linear matrix inequalities (LMIs). In addition, sensor fault detection and isolation are performed by means of a generalised <span class="hlt">observer</span> bank. Two numerical experiments, an electrical circuit and a rolling disc system, are presented in order to illustrate the effectiveness of the proposed method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017WRR....53.2591L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017WRR....53.2591L"><span><span class="hlt">Observational</span> breakthroughs lead the way to improved hydrological predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lettenmaier, Dennis P.</p> <p>2017-04-01</p> <p>New data sources are revolutionizing the hydrological sciences. The capabilities of hydrological models have advanced greatly over the last several <span class="hlt">decades</span>, but until recently model capabilities have outstripped the spatial resolution and accuracy of model forcings (atmospheric <span class="hlt">variables</span> at the land surface) and the hydrologic state <span class="hlt">variables</span> (e.g., soil moisture; snow water equivalent) that the models predict. This has begun to change, as shown in two examples here: soil moisture and drought evolution over Africa as predicted by a hydrology model forced with satellite-derived precipitation, and <span class="hlt">observations</span> of snow water equivalent at very high resolution over a river basin in California's Sierra Nevada.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4673017','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4673017"><span>TraitEnactments as Density Distributions: The Role of Actors, Situations, and <span class="hlt">Observers</span> in Explaining Stability and <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Fleeson, William; Law, Mary Kate</p> <p>2015-01-01</p> <p>The purposes of this paper were to determine (i)whether the high consistency of individual differences in average aggregated behavior is due to actors’ personalities or to consistency in the situations those actors encounter; and(ii)whether the surprisingly high within-person <span class="hlt">variability</span> in trait enactment is a real phenomenon corroborated by <span class="hlt">observers</span>, or merely in individuals’ heads. Although traits are supposed to describe what individuals are like in everyday life, little evidence exists about the enactment of trait content in everyday life. Past experience-sampling studies have found both highly <span class="hlt">variable</span> and highly consistent trait enactment, but were restricted to self-report data and to naturally occurring situations. The current study used experience-sampling in controlled lab environments with 97 targets and 183 <span class="hlt">observers</span> to address these shortcomings. Targets attended hour-long lab sessions 20x each and <span class="hlt">observers</span> rated targets’ behavior. Parameters of distributions were highly consistent (r’s ~ .80), revealing that actors were responsible for consistency, not situations. Nonetheless, <span class="hlt">observer</span> ratings revealed that most <span class="hlt">variability</span> in trait enactment was within-person, confirming that even when people put it on the line in ways that affect others, they still varied rapidly in the traits they enacted. In the face of two historically vexing objections to traits, this paper supports the density distributions model of traits and argues that trait conceptualizations must accommodate large within-person <span class="hlt">variability</span>. PMID:26348598</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4850205F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4850205F"><span>Quantifying Precipitation <span class="hlt">Variability</span> on Titan Using a GCM and Implications for <span class="hlt">Observed</span> Geomorphology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faulk, Sean P.; Mitchell, Jonathan L.; Moon, Seulgi; Lora, Juan Manuel</p> <p>2016-10-01</p> <p>Titan's zonal-mean precipitation behavior has been widely investigated using general circulation models (GCMs), but the spatial and temporal <span class="hlt">variability</span> of rainfall in Titan's active hydrologic cycle is less well understood. We conduct statistical analyses of rainfall, diagnosed from GCM simulations of Titan's atmosphere, to determine storm intensity and frequency. Intense storms of methane have been proposed to be critical for enabling mechanical erosion of Titan's surface, as indicated by <span class="hlt">observations</span> of dendritic valley networks. Using precipitation outputs from the Titan Atmospheric Model (TAM), a GCM shown to realistically simulate many features of Titan's atmosphere, we quantify the precipitation <span class="hlt">variability</span> within eight separate latitude bins for a variety of initial surface liquid distributions. We find that while the overall wettest regions are indeed the poles, the most intense rainfall generally occurs in the high mid-latitudes, between 45-67.5 degrees, consistent with recent geomorphological <span class="hlt">observations</span> of alluvial fans concentrated at those latitudes. We also find that precipitation rates necessary for surface erosion, as estimated by Perron et al. (2006) J. Geophys. Res. 111, E11001, frequently occur at all latitudes, with recurrence intervals of less than one Titan year. Such analysis is crucial towards understanding the complex interaction between Titan's atmosphere and surface and defining the influence of precipitation on <span class="hlt">observed</span> geomorphology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSEC44B1251U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSEC44B1251U"><span>High Frequency Radar <span class="hlt">Observations</span> of Tidal Current <span class="hlt">Variability</span> in the Lower Chesapeake Bay</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Updyke, T. G.; Dusek, G.; Atkinson, L. P.</p> <p>2016-02-01</p> <p>Analysis of eight years of high frequency radar surface current <span class="hlt">observations</span> in the lower Chesapeake Bay is presented with a focus on the <span class="hlt">variability</span> of the tidal component of the surface circulation which accounts for a majority of the variance of the surface flow (typically 70-80% for the middle of the radar footprint). Variations in amplitude and phase of the major tidal constituents are examined in the context of water level, wind and river discharge data. Comparisons are made with harmonic analysis results from long-term records of current data measured by three current profilers operated by NOAA as part of the Chesapeake Bay Physical Oceanographic Real-Time System (PORTS). Preliminary results indicate that there is significant spatial <span class="hlt">variability</span> in the M2 amplitude over the HF radar grid as well as temporal <span class="hlt">variability</span> when harmonic analysis is performed using bi-monthly time segments over the course of the record.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040171555&hterms=systematic+reviews&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsystematic%2Breviews','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040171555&hterms=systematic+reviews&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsystematic%2Breviews"><span>Assimilation of Stratospheric Meteorological and Constituent <span class="hlt">Observations</span>: A Review</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rood, Richard B.; Pawson, Steven</p> <p>2004-01-01</p> <p>This talk reviews the assimilation of meteorological and constituent <span class="hlt">observations</span> of the stratosphere. The first efforts to assimilate <span class="hlt">observations</span> into stratospheric models were during the early 1980s, and a number of research studies followed during the next <span class="hlt">decade</span>. Since the launch of the Upper Atmospheric Research Satellite (UARS) in 1991, model-assimilated data sets of the stratospheric meteorological state have been routinely available. These assimilated data sets were critical in bringing together <span class="hlt">observations</span> from the different instruments on UARS as well as linking UARS <span class="hlt">observations</span> to measurements from other platforms. Using trajectory-mapping techniques, meteorological assimilation analyses are, now, widely used in the analysis of constituent <span class="hlt">observations</span> and have increased the level of quantitative study of stratospheric chemistry and transport. During the 1990s the use of winds and temperatures from assimilated data sets became standard for offline chemistry and transport modeling. <span class="hlt">variability</span> in middle latitudes. The transport experiments, however, reveal a set of shortcomings that become obvious as systematic errors are integrated over time. Generally, the tropics are not well represented, mixing between the tropics and middle latitudes is overestimated, and the residual circulation is not accurate. These shortcomings reveal underlying fundamental challenges related to bias and noise. Current studies using model simulation and data assimilation in controlled experimentation are highlighting the issues that must be addressed if assimilated data sets are to be convincingly used to study interannual <span class="hlt">variability</span> and <span class="hlt">decadal</span> change. <span class="hlt">observations</span>. The primary focus has been on stratospheric ozone, but there are efforts that investigate a suite of reactive chemical constituents. Recent progress in ozone assimilation shows the potential of assimilation to contribute to the validation of ozone <span class="hlt">observations</span> and, ultimately, the retrieval of ozone profiles from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016A%26A...593A.106R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016A%26A...593A.106R"><span>Short-term <span class="hlt">variability</span> and mass loss in Be stars. II. Physical taxonomy of photometric <span class="hlt">variability</span> <span class="hlt">observed</span> by the Kepler spacecraft</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rivinius, Th.; Baade, D.; Carciofi, A. C.</p> <p>2016-09-01</p> <p>Context. Classical Be stars have been established as pulsating stars. Space-based photometric monitoring missions contributed significantly to that result. However, whether Be stars are just rapidly rotating SPB or β Cep stars, or whether they have to be understood differently, remains debated in the view of their highly complex power spectra. Aims: Kepler data of three known Be stars are re-visited to establish their pulsational nature and assess the properties of additional, non-pulsational variations. The three program stars turned out to be one inactive Be star, one active, continuously outbursting Be star, and one Be star transiting from a non-outbursting into an outbursting phase, thus forming an excellent sample to distill properties of Be stars in the various phases of their life-cycle. Methods: The Kepler data was first cleaned from any long-term <span class="hlt">variability</span> with Lomb-Scargle based pre-whitening. Then a Lomb-Scargle analysis of the remaining short-term variations was compared to a wavelet analysis of the cleaned data. This offers a new view on the <span class="hlt">variability</span>, as it enables us to see the temporal evolution of the <span class="hlt">variability</span> and phase relations between supposed beating phenomena, which are typically not visualized in a Lomb-Scargle analysis. Results: The short-term photometric <span class="hlt">variability</span> of Be stars must be disentangled into a stellar and a circumstellar part. The stellar part is on the whole not different from what is seen in non-Be stars. However, some of the <span class="hlt">observed</span> phenomena might be to be due to resonant mode coupling, a mechanism not typically considered for B-type stars. Short-term circumstellar <span class="hlt">variability</span> comes in the form of either a group of relatively well-defined, short-lived frequencies during outbursts, which are called Štefl frequencies, and broad bumps in the power spectra, indicating aperiodic <span class="hlt">variability</span> on a time scale similar to typical low-order g-mode pulsation frequencies, rather than true periodicity. Conclusions: From a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS43C..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS43C..05M"><span>Complexity of Tropical Pacific Ecosystem and Biogeochemistry: Diurnal to <span class="hlt">Decadal</span>, Plankters to Penguins</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murtugudde, R. G.; Wang, X.; Valsala, V.; Karnauskas, K. B.</p> <p>2016-12-01</p> <p>Tropical Pacific spans nearly 50% of the global tropics allowing to have its own mind in terms of climate <span class="hlt">variability</span> and physical-biogeochemical interactions. While the El Niño-Southern Oscillation (ENSO) and its flavors get much attention, it is fairly clear by now that any further improvements in ENSO prediction skills and reliability of global warming projections must begin to <span class="hlt">observe</span> and represent bio-physical interactions in the climate and Earth System models. Coupled climate <span class="hlt">variability</span> over the tropical Pacific has a global reach with its diurnal to <span class="hlt">decadal</span> timescales being manifest in ecosystem and biogechemistry. Zonal and meridional contrasts in biogeochemistry across the tropical Pacific is closely related to seasonal <span class="hlt">variability</span>, ENSO diversity and the PDO. Apparent dominance of ocean dynamic controls on biogeochemistry belies the potential biogeochemical feedbacks on ocean dynamics which may well explain some of the chronic biases in the state-of-the-art climate models. The east Pacific cold-tongue is the most productive open ocean region in the world and home to a unique physical-biogeochmical laboratory, viz., the Galapagos. The Galapagos islands not only control the coupled climate <span class="hlt">variability</span> via their ability to terminate the equatorial undercurrent but also offer a clear example of a biological loophole in terms of their impact on local upwelling and an expanding penguin habitat in the face of global warming. The complex bio-physical interactions in the cold-tongue and their influence on climate predictions and projections require a holisti thinking on future <span class="hlt">observing</span> systems. Tropical Pacific offers a natural laboratory for designing a robust and sustained physical-biogeochemical <span class="hlt">observation</span> system that can effectively bridge climate predictions and projections into a unified framework for subseasonal to multidecadal timescales. Such a system will be a foundation for establishing similar systems over the rest of the World ocean to seemlessly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..813A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..813A"><span>Regional influence of <span class="hlt">decadal</span> to multidecadal Atlantic Oscillations during the last two millennia in Morocco, inferred from two high resolution δ18O speleothem records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ait Brahim, Yassine; Sifeddine, Abdelfettah; Khodri, Myriam; Bouchaou, Lhoussaine; Cruz, Francisco W.; Pérez-Zanón, Núria; Wassenburg, Jasper A.; Cheng, Hai</p> <p>2017-04-01</p> <p>Climate projections predict substantial increase of extreme heats and drought occurrences during the coming <span class="hlt">decades</span> in Morocco. It is however not clear what can be attributed to natural climate <span class="hlt">variability</span> and to anthropogenic forcing, as hydroclimate variations <span class="hlt">observed</span> in areas such as Morocco are highly influenced by the Atlantic climate modes. Since <span class="hlt">observational</span> data sets are too short to resolve properly natural modes of <span class="hlt">variability</span> acting on <span class="hlt">decadal</span> to multidecadal timescales, high resolution paleoclimate reconstructions are the only alternative to reconstruct climate <span class="hlt">variability</span> in the remote past. Herein, we present two high resolution and well dated speleothems oxygen isotope (δ18O) records sampled from Chaara and Ifoulki caves (located in Northeastern and Southwestern Morocco respectively) to investigate hydroclimate variations during the last 2000 years. Our results are supported by a monitoring network of δ18O in precipitation from 17 stations in Morocco. The new paleoclimate records are discussed in the light of existing continental and marine paleoclimate proxies in Morocco to identify significant correlations at various lead times with the main reconstructed oceanic and atmospheric <span class="hlt">variability</span> modes and possible climate teleconnections that have potentially influenced the climate during the last two millennia in Morocco. The results reveal substantial <span class="hlt">decadal</span> to multidecadal swings between dry and humid periods, consistent with regional paleorecords. Evidence of dry conditions exist during the Medieval Climate Anomaly (MCA) period and the Climate Warm Period (CWP) and humid conditions during the Little Ice Age (LIA) period. Statistical analyses suggest that the climate of southwestern Morocco remained under the combined influence of both the Atlantic Multidecadal Oscillation (AMO) and the North Atlantic Oscillation (NAO) over the last two millennia. Interestingly, the generally warmer MCA and colder LIA at longer multidecadal timescales probably</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150008964','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150008964"><span>Connecting Satellite <span class="hlt">Observations</span> with Water Cycle <span class="hlt">Variables</span> Through Land Data Assimilation: Examples Using the NASA GEOS-5 LDAS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reichle, Rolf H.; De Lannoy, Gabrielle J. M.; Forman, Barton A.; Draper, Clara S.; Liu, Qing</p> <p>2013-01-01</p> <p>A land data assimilation system (LDAS) can merge satellite <span class="hlt">observations</span> (or retrievals) of land surface hydrological conditions, including soil moisture, snow, and terrestrial water storage (TWS), into a numerical model of land surface processes. In theory, the output from such a system is superior to estimates based on the <span class="hlt">observations</span> or the model alone, thereby enhancing our ability to understand, monitor, and predict key elements of the terrestrial water cycle. In practice, however, satellite <span class="hlt">observations</span> do not correspond directly to the water cycle <span class="hlt">variables</span> of interest. The present paper addresses various aspects of this seeming mismatch using examples drawn from recent research with the ensemble-based NASA GEOS-5 LDAS. These aspects include (1) the assimilation of coarse-scale <span class="hlt">observations</span> into higher-resolution land surface models, (2) the partitioning of satellite <span class="hlt">observations</span> (such as TWS retrievals) into their constituent water cycle components, (3) the forward modeling of microwave brightness temperatures over land for radiance-based soil moisture and snow assimilation, and (4) the selection of the most relevant types of <span class="hlt">observations</span> for the analysis of a specific water cycle <span class="hlt">variable</span> that is not <span class="hlt">observed</span> (such as root zone soil moisture). The solution to these challenges involves the careful construction of an <span class="hlt">observation</span> operator that maps from the land surface model <span class="hlt">variables</span> of interest to the space of the assimilated <span class="hlt">observations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3924476','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3924476"><span>The Socioeconomic Determinants of Health: Economic Growth and Health in the OECD Countries during the Last Three <span class="hlt">Decades</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>López-Casasnovas, Guillem; Soley-Bori, Marina</p> <p>2014-01-01</p> <p>In times of economic crisis, most countries face the dual challenge of fighting unemployment while restraining social expenditures and closing budget deficits. The spending cuts and lack of employment affect a large number of decisions that have a direct or indirect impact on health. This impact is likely to be unevenly distributed among different groups within the population, and therefore not only health levels may be at risk, but also their distribution. The main purpose of this paper is to explore links between unemployment, economic growth, inequality, and health. We regress a measure of health, the Health Human Development Index (HHDI), against a set of explanatory <span class="hlt">variables</span> accounting for the countries’ economic performance (GDP growth, unemployment, and income inequality), and some institutional factors related to welfare spending and the nature of the health systems for the past three <span class="hlt">decades</span>. In addition, we explore the causes for different results obtained using an inequality-adjusted HHDI, vs. the unadjusted HHDI. We describe a panel data model, estimated by random effects, for 32 countries from 1980–2010, in five-year intervals. Our conclusion is that the high economic growth <span class="hlt">observed</span> in the last <span class="hlt">decades</span>, together with an increase in the levels of income inequality and/or poverty, explain the <span class="hlt">observed</span> changes of our index, particularly when this indicator is weighted by health inequality. The remaining institutional <span class="hlt">variables</span> (the share of social spending, health care expenditure, and the type of health systems) show the expected sign but are not statistically significant. A comment on the methodological pitfalls of the approach completes the analysis. PMID:24406664</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24406664','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24406664"><span>The socioeconomic determinants of health: economic growth and health in the OECD countries during the last three <span class="hlt">decades</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>López-Casasnovas, Guillem; Soley-Bori, Marina</p> <p>2014-01-08</p> <p>In times of economic crisis, most countries face the dual challenge of fighting unemployment while restraining social expenditures and closing budget deficits. The spending cuts and lack of employment affect a large number of decisions that have a direct or indirect impact on health. This impact is likely to be unevenly distributed among different groups within the population, and therefore not only health levels may be at risk, but also their distribution. The main purpose of this paper is to explore links between unemployment, economic growth, inequality, and health. We regress a measure of health, the Health Human Development Index (HHDI), against a set of explanatory <span class="hlt">variables</span> accounting for the countries' economic performance (GDP growth, unemployment, and income inequality), and some institutional factors related to welfare spending and the nature of the health systems for the past three <span class="hlt">decades</span>. In addition, we explore the causes for different results obtained using an inequality-adjusted HHDI, vs. the unadjusted HHDI. We describe a panel data model, estimated by random effects, for 32 countries from 1980-2010, in five-year intervals. Our conclusion is that the high economic growth <span class="hlt">observed</span> in the last <span class="hlt">decades</span>, together with an increase in the levels of income inequality and/or poverty, explain the <span class="hlt">observed</span> changes of our index, particularly when this indicator is weighted by health inequality. The remaining institutional <span class="hlt">variables</span> (the share of social spending, health care expenditure, and the type of health systems) show the expected sign but are not statistically significant. A comment on the methodological pitfalls of the approach completes the analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME24E0754M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME24E0754M"><span><span class="hlt">Decadal</span> to centennial oscillations in the upper and lower boundaries of the San Diego, California margin Oxygen Minimum Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Myhre, S. E.; Hill, T. M.; Frieder, C.; Grupe, B.</p> <p>2016-02-01</p> <p>Here we present two new marine sediment archives from the continental margin of San Diego, California, USA, which record <span class="hlt">decadal</span> to centennial oscillations in the hydrographic structure of the Eastern Pacific Oxygen Minimum Zone (OMZ). The two cores, located at 528 and 1,180 m water depth, record oceanographic history across overlapping timescales. Biotic communities, including Foraminifera, Echinodermata, Brachiopoda, Mollusca and Ostrocoda, were examined in subsurface (>10 cm sediment core depth) samples. Chronologies for both cores were developed with reservoir-corrected 14C dates of mixed planktonic Foraminifera and linearly interpolated sedimentation rates. Sediment ages for the cores range from 400-1,800 years before present. Indices of foraminiferal community density, diversity and evenness are applied as biotic proxies to track the intensification of the continental margin OMZ. Biotic communities at the shallower site reveal multi-<span class="hlt">decadal</span> to centennial timescales of OMZ intensification, whereas the deeper site exhibits <span class="hlt">decadal</span> to multi-<span class="hlt">decadal</span> scales of hydrographic <span class="hlt">variability</span>. Hypoxia-associated foraminiferal genera Uvigerina and Bolivina were compositionally dominant during intervals of peak foraminiferal density. Invertebrate assemblages often co-occurred across taxa groups, and thereby provide a broad trophic context for interpreting changes in the margin seafloor. <span class="hlt">Variability</span> in the advection of Pacific Equatorial Water may mechanistically contribute to this described hydrographic <span class="hlt">variability</span>. This investigation reconstructs historical timescales of OMZ intensification, seafloor ecological <span class="hlt">variability</span>, and synchrony between open-ocean processes and regional climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC24A2125U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC24A2125U"><span>Determining the Effect of the Lunar Nodal Cycle on Tidal Mixing and North Pacific Climate <span class="hlt">Variability</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ullman, D. J.; Schmittner, A.; Danabasoglu, G.; Norton, N. J.; Müller, M.</p> <p>2016-02-01</p> <p>Oscillations in the moon's orbit around the earth modulate regional tidal dissipation with a periodicity of 18.6 years. In regions where the diurnal tidal constituents dominate diapycnal mixing, this Lunar Nodal Cycle (LNC) may be significant enough to influence ocean circulation, sea surface temperature, and climate <span class="hlt">variability</span>. Such periodicity in the LNC as an external forcing may provide a mechanistic source for Pacific <span class="hlt">decadal</span> <span class="hlt">variability</span> (i.e. Pacific <span class="hlt">Decadal</span> Oscillation, PDO) where diurnal tidal constituents are strong. We have introduced three enhancements to the latest version of the Community Earth System Model (CESM) to better simulate tidal-forced mixing. First, we have produced a sub-grid scale bathymetry scheme that better resolves the vertical distribution of the barotropic energy flux in regions where the native CESM grid does not resolve high spatial-scale bathymetric features. Second, we test a number of alternative barotropic tidal constituent energy flux fields that are derived from various satellite altimeter <span class="hlt">observations</span> and tidal models. Third, we introduce modulations of the individual diurnal and semi-diurnal tidal constituents, ranging from monthly to <span class="hlt">decadal</span> periods, as derived from the full lunisolar tidal potential. Using both ocean-only and fully-coupled configurations, we test the influence of these enhancements, particularly the LNC modulations, on ocean mixing and bidecadal climate <span class="hlt">variability</span> in CESM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C53B1033S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C53B1033S"><span>Spatio-temporal <span class="hlt">Variability</span> of Stratified Snowpack Cold Content <span class="hlt">Observed</span> in the Rocky Mountains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, J. S.; Sexstone, G. A.; Serreze, M. C.</p> <p>2017-12-01</p> <p>Snowpack cold content (CCsnow) is the energy required to bring a snowpack to an isothermal temperature of 0.0°C. The spatio-temporal <span class="hlt">variability</span> of CCsnow is complex as it is a measure that integrates the response of a snowpack to each component of the snow-cover energy balance. Snow and ice at high elevation is climate sensitive water storage for the Western U.S. Therefore, an improved understanding of the spatio-temporal <span class="hlt">variability</span> of CCsnow may provide insight into snowpack dynamics and sensitivity to climate change. In this study, stratified snowpit <span class="hlt">observations</span> of snow water equivalent (SWE) and snow temperature (Tsnow) from the USGS Rocky Mountain Snowpack network (USGS RMS) were used to evaluate vertical CCsnow profiles over a 16-year period in Montana, Idaho, Wyoming, Colorado and New Mexico. Since 1993, USGS RMS has collected snow chemistry, snow temperature, and SWE data throughout the Rocky Mountain region, making it well positioned for Anthropocene cryosphere benchmarking and climate change interpretation. Spatial grouping of locations based on similar CCsnow characteristics was evaluated and trend analyses were performed. Additionally, we evaluated the regional relation of CCsnow to snowmelt timing. CCsnow was more precisely calculated and more representative using vertically stratified field <span class="hlt">observed</span> values than bulk values, which highlights the utility of the snowpack dataset presented here. Location specific annual and 16 year mean stratified snowpit profiles of SWE, Tsnow, and CCsnow well represent the physical geography and past weather patterns acting on the snowpack. <span class="hlt">Observed</span> trends and spatial <span class="hlt">variability</span> of CCsnow profiles explored by this study provides an improved understanding of changing snowpack behavior in the western U.S., and will be useful for assessing the regional sensitivity of snowpacks to future climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC51E1230W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC51E1230W"><span>Climate <span class="hlt">Variability</span> and Wildfires: Insights from Global Earth System Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ward, D. S.; Shevliakova, E.; Malyshev, S.; Lamarque, J. F.; Wittenberg, A. T.</p> <p>2016-12-01</p> <p>Better understanding of the relationship between <span class="hlt">variability</span> in global climate and emissions from wildfires is needed for predictions of fire activity on interannual to multi-<span class="hlt">decadal</span> timescales. Here we investigate this relationship using the long, preindustrial control simulations and historical ensembles of two Earth System models; CESM1 and the NOAA/GFDL ESM2Mb. There is smaller interannual <span class="hlt">variability</span> of global fires in both models than in present day inventories, especially in boreal regions where <span class="hlt">observed</span> fires vary substantially from year to year. Patterns of fire response to climate oscillation indices, including the El Niño / Southern Oscillation (ENSO), Pacific <span class="hlt">Decadal</span> Oscillation (PDO) and Atlantic Meridional Oscillation (AMO) are explored with the model results and compared to the response derived from satellite measurements and proxy <span class="hlt">observations</span>. Increases in fire emissions in southeast Asia and boreal North America are associated with positive ENSO and PDO, while United States fires and Sahel fires decrease for the same climate conditions. Boreal fire emissions decrease in CESM1 for the warm phase of the AMO, while ESM2Mb did not produce a reliable AMO. CESM1 produces a weak negative trend in global fire emissions for the period 1920 to 2005, while ESM2Mb produces a positive trend over the same period. Both trends are statistically significant at a confidence level of 95% or greater given the <span class="hlt">variability</span> derived from the respective preindustrial controls. In addition to climate <span class="hlt">variability</span> impacts on fires, we also explore the impacts of fire emissions on climate <span class="hlt">variability</span> and atmospheric chemistry. We analyze three long, free-evolving ESM2Mb simulations; one without fire emissions, one with constant year-over-year fire emissions based on a present day inventory, and one with interannually varying fire emissions coupled between the terrestrial and atmospheric components of the model, to gain a better understanding of the role of fire emissions in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4466746','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4466746"><span>Classification images reveal decision <span class="hlt">variables</span> and strategies in forced choice tasks</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Pritchett, Lisa M.; Murray, Richard F.</p> <p>2015-01-01</p> <p>Despite <span class="hlt">decades</span> of research, there is still uncertainty about how people make simple decisions about perceptual stimuli. Most theories assume that perceptual decisions are based on decision <span class="hlt">variables</span>, which are internal <span class="hlt">variables</span> that encode task-relevant information. However, decision <span class="hlt">variables</span> are usually considered to be theoretical constructs that cannot be measured directly, and this often makes it difficult to test theories of perceptual decision making. Here we show how to measure decision <span class="hlt">variables</span> on individual trials, and we use these measurements to test theories of perceptual decision making more directly than has previously been possible. We measure classification images, which are estimates of templates that <span class="hlt">observers</span> use to extract information from stimuli. We then calculate the dot product of these classification images with the stimuli to estimate <span class="hlt">observers</span>' decision <span class="hlt">variables</span>. Finally, we reconstruct each <span class="hlt">observer</span>'s “decision space,” a map that shows the probability of the observer’s responses for all values of the decision <span class="hlt">variables</span>. We use this method to examine decision strategies in two-alternative forced choice (2AFC) tasks, for which there are several competing models. In one experiment, the resulting decision spaces support the difference model, a classic theory of 2AFC decisions. In a second experiment, we find unexpected decision spaces that are not predicted by standard models of 2AFC decisions, and that suggest intrinsic uncertainty or soft thresholding. These experiments give new evidence regarding observers’ strategies in 2AFC tasks, and they show how measuring decision <span class="hlt">variables</span> can answer long-standing questions about perceptual decision making. PMID:26015584</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24816936','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24816936"><span>Cardiac valve calcifications on low-dose unenhanced ungated chest computed tomography: inter-<span class="hlt">observer</span> and inter-examination reliability, agreement and <span class="hlt">variability</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>van Hamersvelt, Robbert W; Willemink, Martin J; Takx, Richard A P; Eikendal, Anouk L M; Budde, Ricardo P J; Leiner, Tim; Mol, Christian P; Isgum, Ivana; de Jong, Pim A</p> <p>2014-07-01</p> <p>To determine inter-<span class="hlt">observer</span> and inter-examination <span class="hlt">variability</span> for aortic valve calcification (AVC) and mitral valve and annulus calcification (MC) in low-dose unenhanced ungated lung cancer screening chest computed tomography (CT). We included 578 lung cancer screening trial participants who were examined by CT twice within 3 months to follow indeterminate pulmonary nodules. On these CTs, AVC and MC were measured in cubic millimetres. One hundred CTs were examined by five <span class="hlt">observers</span> to determine the inter-<span class="hlt">observer</span> <span class="hlt">variability</span>. Reliability was assessed by kappa statistics (κ) and intra-class correlation coefficients (ICCs). <span class="hlt">Variability</span> was expressed as the mean difference ± standard deviation (SD). Inter-examination reliability was excellent for AVC (κ = 0.94, ICC = 0.96) and MC (κ = 0.95, ICC = 0.90). Inter-examination <span class="hlt">variability</span> was 12.7 ± 118.2 mm(3) for AVC and 31.5 ± 219.2 mm(3) for MC. Inter-<span class="hlt">observer</span> reliability ranged from κ = 0.68 to κ = 0.92 for AVC and from κ = 0.20 to κ = 0.66 for MC. Inter-<span class="hlt">observer</span> ICC was 0.94 for AVC and ranged from 0.56 to 0.97 for MC. Inter-<span class="hlt">observer</span> <span class="hlt">variability</span> ranged from -30.5 ± 252.0 mm(3) to 84.0 ± 240.5 mm(3) for AVC and from -95.2 ± 210.0 mm(3) to 303.7 ± 501.6 mm(3) for MC. AVC can be quantified with excellent reliability on ungated unenhanced low-dose chest CT, but manual detection of MC can be subject to substantial inter-<span class="hlt">observer</span> <span class="hlt">variability</span>. Lung cancer screening CT may be used for detection and quantification of cardiac valve calcifications. • Low-dose unenhanced ungated chest computed tomography can detect cardiac valve calcifications. • However, calcified cardiac valves are not reported by most radiologists. • Inter-<span class="hlt">observer</span> and inter-examination <span class="hlt">variability</span> of aortic valve calcifications is sufficient for longitudinal studies. • Volumetric measurement <span class="hlt">variability</span> of mitral valve and annulus calcifications is substantial.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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