Sample records for non-volcanic hydrothermal activity

  1. Catastrophic volcanic collapse: relation to hydrothermal processes.

    PubMed

    López, D L; Williams, S N

    1993-06-18

    Catastrophic volcanic collapse, without precursory magmatic activity, is characteristic of many volcanic disasters. The extent and locations of hydrothermal discharges at Nevado del Ruiz volcano, Colombia, suggest that at many volcanoes collapse may result from the interactions between hydrothermal fluids and the volcanic edifice. Rock dissolution and hydrothermal mineral alteration, combined with physical triggers such as earth-quakes, can produce volcanic collapse. Hot spring water compositions, residence times, and flow paths through faults were used to model potential collapse at Ruiz. Caldera dimensions, deposits, and alteration mineral volumes are consistent with parameters observed at other volcanoes.

  2. Hydrothermal reservoir beneath Taal Volcano (Philippines): Implications to volcanic activity

    NASA Astrophysics Data System (ADS)

    Nagao, T.; Alanis, P. B.; Yamaya, Y.; Takeuchi, A.; Bornas, M. V.; Cordon, J. M.; Puertollano, J.; Clarito, C. J.; Hashimoto, T.; Mogi, T.; Sasai, Y.

    2012-12-01

    Taal Volcano is one of the most active volcanoes in the Philippines. The first recorded eruption was in 1573. Since then it has erupted 33 times resulting in thousands of casualties and large damages to property. In 1995, it was declared as one of the 15 Decade Volcanoes. Beginning in the early 1990s it has experienced several phases of abnormal activity, including seismic swarms, episodes of ground deformation, ground fissuring and hydrothermal activities, which continues up to the present. However, it has been noted that past historical eruptions of Taal Volcano may be divided into 2 distinct cycles, depending on the location of the eruption center, either at Main Crater or at the flanks. Between 1572-1645, eruptions occurred at the Main Crater, in 1707 to 1731, they occurred at the flanks. In 1749, eruptions moved back to the Main Crater until 1911. During the 1965 and until the end of the 1977 eruptions, eruptive activity once again shifted to the flanks. As part of the PHIVOLCS-JICA-SATREPS Project magnetotelluric and audio-magnetotelluric surveys were conducted on Volcano Island in March 2011 and March 2012. Two-dimensional (2-D) inversion and 3-D forward modeling reveals a prominent and large zone of relatively high resistivity between 1 to 4 kilometers beneath the volcano almost directly beneath the Main Crater, surrounded by zones of relatively low resistivity. This anomalous zone of high resistivity is hypothesized to be a large hydrothermal reservoir filled with volcanic fluids. The presence of this large hydrothermal reservoir could be related to past activities of Taal Volcano. In particular we believe that the catastrophic explosion described during the 1911 eruption was the result of the hydrothermal reservoir collapsing. During the cycle of Main Crater eruptions, this hydrothermal reservoir is depleted, while during a cycle of flank eruptions this reservoir is replenished with hydrothermal fluids.

  3. Volcanic and Hydrothermal Activity of the North Su Volcano: New Insights from Repeated Bathymetric Surveys and ROV Observations

    NASA Astrophysics Data System (ADS)

    Thal, J.; Bach, W.; Tivey, M.; Yoerger, D.

    2013-12-01

    Bathymetric data from cruises in 2002, 2006, and 2011 were combined and compared to determine the evolution of volcanic activity, seafloor structures, erosional features and to identify and document the distribution of hydrothermal vents on North Su volcano, SuSu Knolls, eastern Manus Basin (Papua New Guinea). Geologic mapping based on ROV observations from 2006 (WHOI Jason-2) and 2011 (MARUM Quest-4000) combined with repeated bathymetric surveys from 2002 and 2011 are used to identify morphologic features on the slopes of North Su and to track temporal changes. ROV MARUM Quest-4000 bathymetry was used to develop a 10 m grid of the top of North Su to precisely depict recent changes. In 2006, the south slope of North Su was steeply sloped and featured numerous white smoker vents discharging acid sulfate waters. These vents were covered by several tens of meters of sand- to gravel-sized volcanic material in 2011. The growth of this new cone changed the bathymetry of the south flank of North Su up to ~50 m and emplaced ~0.014 km3 of clastic volcanic material. This material is primarily comprised of fractured altered dacite and massive fresh dacite as well as crystals of opx, cpx, olivine and plagioclase. There is no evidence for pyroclastic fragmentation, so we hypothesize that the fragmentation is likely related to hydrothermal explosions. Hydrothermal activity varies over a short (~50 m) lateral distance from 'flashing' black smokers to acidic white smoker vents. Within 2 weeks of observation time in 2011, the white smoker vents varied markedly in activity suggesting a highly episodic hydrothermal system. Based on ROV video recordings, we identified steeply sloping (up to 30°) slopes exposing pillars and walls of hydrothermal cemented volcaniclastic material representing former fluid upflow zones. These features show that hydrothermal activity has increased slope stability as hydrothermal cementation has prevented slope collapse. Additionally, in some places

  4. Geologic field-trip guide to the volcanic and hydrothermal landscape of the Yellowstone Plateau

    USGS Publications Warehouse

    Morgan Morzel, Lisa Ann; Shanks, W. C. Pat; Lowenstern, Jacob B.; Farrell, Jamie M.; Robinson, Joel E.

    2017-11-20

    Yellowstone National Park, a nearly 9,000 km2 (~3,468 mi2) area, was preserved in 1872 as the world’s first national park for its unique, extraordinary, and magnificent natural features. Rimmed by a crescent of older mountainous terrain, Yellowstone National Park has at its core the Quaternary Yellowstone Plateau, an undulating landscape shaped by forces of late Cenozoic explosive and effusive volcanism, on-going tectonism, glaciation, and hydrothermal activity. The Yellowstone Caldera is the centerpiece of the Yellowstone Plateau. The Yellowstone Plateau lies at the most northeastern front of the 17-Ma Yellowstone hot spot track, one of the few places on Earth where time-transgressive processes on continental crust can be observed in the volcanic and tectonic (faulting and uplift) record at the rate and direction predicted by plate motion. Over six days, this field trip presents an intensive overview into volcanism, tectonism, and hydrothermal activity on the Yellowstone Plateau (fig. 1). Field stops are linked directly to conceptual models related to monitoring of the various volcanic, geochemical, hydrothermal, and tectonic aspects of the greater Yellowstone system. Recent interest in young and possible future volcanism at Yellowstone as well as new discoveries and synthesis of previous studies, (for example, tomographic, deformation, gas, aeromagnetic, bathymetric, and seismic surveys), provide a framework in which to discuss volcanic, hydrothermal, and seismic activity in this dynamic region.

  5. Exploring for Volcanic and Hydrothermal Activity Above Off-axis Melt Lenses near the East Pacific Rise

    NASA Astrophysics Data System (ADS)

    White, S. M.; Lee, A. J.; Rubin, K. H.

    2015-12-01

    Two Alvin dives (AL 4771 and 4774) transected the seafloor directly above the two largest Off-Axis Melt Lenses (O-AML) east of the East Pacific Rise (EPR) axis at 9 39'N and 9 54'N. In 2008, a 3D high-resolution seismic reflection survey (MGL-0812) discovered O-AMLs 3-7 km from the EPR at 2-3 km below the seafloor. Several other O-AML in the crust have been subsequently detected in several locations up to 20 km from the spreading axis at fast and intermediate spreading ridges; understanding their impacts is increasingly important. During the dives, no currently active hydrothermal venting or fresh lava was seen, suggesting that these features do not constantly power off-axis geological activity. However, the seafloor appears much younger at small volcanic seamounts in the 9 39'N than at the 9 54'N site. At 9 39'N, we used Alvin to explore the off-axis volcanic mound complex, reaching the summit of the three largest mounds. Although no evidence for on-going hydrothermal or volcanic activity was detected, the seafloor wore a thin sediment layer of ~10cm and thin Mn-coatings on 9 rock samples, suggesting volcanism more recently than would be expected based on the spreading-rate age of the crust. At 9 54'N, the Alvin trackline started south of a prominent abyssal hill, which has an unusual D-shape over 1 km wide in the center, crossed the abyssal hill, visited two local hummocks on top, and then attempted to find volcanic activity on the near slope of EPR axis by going as far west was possible during the dive. Heavy sediment everywhere on the abyssal hill, to the depth of push cores (~30 cm) and probably much deeper in many areas and 4 rock samples from the abyssal hill were quite weathered with little glass intact, suggest that this site is unaffected by the underlying O-AML. Upslope toward the EPR west of the abyssal hill, 4 rocks collected appear somewhat younger, and sediment became thinner. In addition, 3 CTD tow-yos over each O-AML found no evidence of active

  6. Exploring for Volcanic and Hydrothermal Activity Above Off-axis Melt Lenses near the East Pacific Rise

    NASA Astrophysics Data System (ADS)

    West, A. J.; Torres, M. A.; Nealson, K. H.

    2014-12-01

    Two Alvin dives (AL 4771 and 4774) transected the seafloor directly above the two largest Off-Axis Melt Lenses (O-AML) east of the East Pacific Rise (EPR) axis at 9 39'N and 9 54'N. In 2008, a 3D high-resolution seismic reflection survey (MGL-0812) discovered O-AMLs 3-7 km from the EPR at 2-3 km below the seafloor. Several other O-AML in the crust have been subsequently detected in several locations up to 20 km from the spreading axis at fast and intermediate spreading ridges; understanding their impacts is increasingly important. During the dives, no currently active hydrothermal venting or fresh lava was seen, suggesting that these features do not constantly power off-axis geological activity. However, the seafloor appears much younger at small volcanic seamounts in the 9 39'N than at the 9 54'N site. At 9 39'N, we used Alvin to explore the off-axis volcanic mound complex, reaching the summit of the three largest mounds. Although no evidence for on-going hydrothermal or volcanic activity was detected, the seafloor wore a thin sediment layer of ~10cm and thin Mn-coatings on 9 rock samples, suggesting volcanism more recently than would be expected based on the spreading-rate age of the crust. At 9 54'N, the Alvin trackline started south of a prominent abyssal hill, which has an unusual D-shape over 1 km wide in the center, crossed the abyssal hill, visited two local hummocks on top, and then attempted to find volcanic activity on the near slope of EPR axis by going as far west was possible during the dive. Heavy sediment everywhere on the abyssal hill, to the depth of push cores (~30 cm) and probably much deeper in many areas and 4 rock samples from the abyssal hill were quite weathered with little glass intact, suggest that this site is unaffected by the underlying O-AML. Upslope toward the EPR west of the abyssal hill, 4 rocks collected appear somewhat younger, and sediment became thinner. In addition, 3 CTD tow-yos over each O-AML found no evidence of active

  7. A multidisciplinary approach to quantify the permeability of the Whakaari/White Island volcanic hydrothermal system (Taupo Volcanic Zone, New Zealand)

    NASA Astrophysics Data System (ADS)

    Heap, Michael J.; Kennedy, Ben M.; Farquharson, Jamie I.; Ashworth, James; Mayer, Klaus; Letham-Brake, Mark; Reuschlé, Thierry; Gilg, H. Albert; Scheu, Bettina; Lavallée, Yan; Siratovich, Paul; Cole, Jim; Jolly, Arthur D.; Baud, Patrick; Dingwell, Donald B.

    2017-02-01

    Our multidisciplinary study aims to better understand the permeability of active volcanic hydrothermal systems, a vital prerequisite for modelling and understanding their behaviour and evolution. Whakaari/White Island volcano (an active stratovolcano at the north-eastern end of the Taupo Volcanic Zone of New Zealand) hosts a highly reactive hydrothermal system and represents an ideal natural laboratory to undertake such a study. We first gained an appreciation of the different lithologies at Whakaari and (where possible) their lateral and vertical extent through reconnaissance by land, sea, and air. The main crater, filled with tephra deposits, is shielded by a volcanic amphitheatre comprising interbedded lavas, lava breccias, and tuffs. We deployed field techniques to measure the permeability and density/porosity of (1) > 100 hand-sized sample blocks and (2) layered unlithified deposits in eight purpose-dug trenches. Our field measurements were then groundtruthed using traditional laboratory techniques on almost 150 samples. Our measurements highlight that the porosity of the materials at Whakaari varies from ∼ 0.01 to ∼ 0.7 and permeability varies by eight orders of magnitude (from ∼ 10-19 to ∼ 10-11 m2). The wide range in physical and hydraulic properties is the result of the numerous lithologies and their varied microstructures and alteration intensities, as exposed by a combination of macroscopic and microscopic (scanning electron microscopy) observations, quantitative mineralogical studies (X-ray powder diffraction), and mercury porosimetry. An understanding of the spatial distribution of lithology and alteration style/intensity is therefore important to decipher fluid flow within the Whakaari volcanic hydrothermal system. We align our field observations and porosity/permeability measurements to construct a schematic cross section of Whakaari that highlights the salient findings of our study. Taken together, the alteration typical of a volcanic

  8. Mars Volcanic Cone with Hydrothermal Deposits

    NASA Image and Video Library

    2010-10-31

    This false color image from NASA Mars Reconnaissance Orbiter indicates that the volcanic cone in the Nili Patera caldera on Mars has hydrothermal mineral deposits on the southern flanks and nearby terrains.

  9. Learning about hydrothermal volcanic activity by modeling induced geophysical changes

    NASA Astrophysics Data System (ADS)

    Currenti, Gilda M.; Napoli, Rosalba

    2017-05-01

    Motivated by ongoing efforts to understand the nature and the energy potential of geothermal resources, we devise a coupled numerical model (hydrological, thermal, mechanical), which may help in the characterization and monitoring of hydrothermal systems through computational experiments. Hydrothermal areas in volcanic regions arise from a unique combination of geological and hydrological features which regulate the movement of fluids in the vicinity of magmatic sources capable of generating large quantities of steam and hot water. Numerical simulations help in understanding and characterizing rock-fluid interaction processes and the geophysical observations associated with them. Our aim is the quantification of the response of different geophysical observables (i.e. deformation, gravity and magnetic field) to hydrothermal activity on the basis of a sound geological framework (e.g. distribution and pathways of the flows, the presence of fractured zones, caprock). A detailed comprehension and quantification of the evolution and dynamics of the geothermal systems and the definition of their internal state through a geophysical modeling approach are essential to identify the key parameters for which the geothermal system may fulfill the requirements to be exploited as a source of energy. For the sake of illustration only, the numerical computations are focused on a conceptual model of the hydrothermal system of Vulcano Island by simulating a generic 1-year unrest and estimating different geophysical changes. We solved (i) the mass and energy balance equations of flow in porous media for temperature, pressure and density changes, (ii) the elastostatic equation for the deformation field and (iii) the Poisson’s equations for gravity and magnetic potential fields. Under the model assumptions, a generic unrest of 1-year engenders on the ground surface low amplitude changes in the investigated geophysical observables, that are, however, above the accuracies of the modern

  10. Hydrothermal activity at slow-spreading ridges: variability and importance of magmatic controls

    NASA Astrophysics Data System (ADS)

    Escartin, Javier

    2016-04-01

    Hydrothermal activity along mid-ocean ridge axes is ubiquitous, associated with mass, chemical, and heat exchanges between the deep lithosphere and the overlying envelopes, and sustaining chemiosynthetic ecosystems at the seafloor. Compared with hydrothermal fields at fast-spreading ridges, those at slow spreading ones show a large variability as their location and nature is controlled or influenced by several parameters that are inter-related: a) tectonic setting, ranging from 'volcanic systems' (along the rift valley floor, volcanic ridges, seamounts), to 'tectonic' ones (rift-bounding faults, oceanic detachment faults); b) the nature of the host rock, owing to compositional heterogeneity of slow-spreading lithosphere (basalt, gabbro, peridotite); c) the type of heat source (magmatic bodies at depth, hot lithosphere, serpentinization reactions); d) and the associated temperature of outflow fluids (high- vs.- low temperature venting and their relative proportion). A systematic review of the distribution and characteristics of hydrothermal fields along the slow-spreading Mid-Atlantic Ridge suggests that long-lived hydrothermal activity is concentrated either at oceanic detachment faults, or along volcanic segments with evidence of robust magma supply to the axis. A detailed study of the magmatically robust Lucky Strike segment suggests that all present and past hydrothermal activity is found at the center of the segment. The association of these fields to central volcanos, and the absence of indicators of hydrothermal activity along the remaining of the ridge segment, suggests that long-lived hydrothermal activity in these volcanic systems is maintained by the enhanced melt supply and the associated magma chamber(s) required to build these volcanic edifices. In this setting, hydrothermal outflow zones at the seafloor are systematically controlled by faults, indicating that hydrothermal fluids in the shallow crust exploit permeable fault zones to circulate. While

  11. Hydrothermal monitoring in a quiescent volcanic arc: Cascade Range, northwestern United States

    USGS Publications Warehouse

    Ingebritsen, S.E.; Randolph-Flagg, N. G.; Gelwick, K.D.; Lundstrom, E.A.; Crankshaw, I.M.; Murveit, A.M.; Schmidt, M.E.; Bergfeld, D.; Spicer, K.R.; Tucker, D.S.; Mariner, R.H.; Evans, William C.

    2014-01-01

    Ongoing (1996–present) volcanic unrest near South Sister, Oregon, is accompanied by a striking set of hydrothermal anomalies, including elevated temperatures, elevated major ion concentrations, and 3He/4He ratios as large as 8.6 RA in slightly thermal springs. These observations prompted the US Geological Survey to begin a systematic hydrothermal-monitoring effort encompassing 25 sites and 10 of the highest-risk volcanoes in the Cascade volcanic arc, from Mount Baker near the Canadian border to Lassen Peak in northern California. A concerted effort was made to develop hourly, multiyear records of temperature and/or hydrothermal solute flux, suitable for retrospective comparison with other continuous geophysical monitoring data. Targets included summit fumarole groups and springs/streams that show clear evidence of magmatic influence in the form of high 3He/4He ratios and/or anomalous fluxes of magmatic CO2 or heat. As of 2009–2012, summit fumarole temperatures in the Cascade Range were generally near or below the local pure water boiling point; the maximum observed superheat was 3 during periods of hourly record. Hydrothermal responses to these small seismic stimuli were generally undetectable or ambiguous. Evaluation of multiyear to multidecadal trends indicates that whereas the hydrothermal system at Mount St. Helens is still fast-evolving in response to the 1980–present eruptive cycle, there is no clear evidence of ongoing long-term trends in hydrothermal activity at other Cascade Range volcanoes that have been active or restless during the past century (Baker, South Sister, and Lassen). Experience gained during the Cascade Range hydrothermal-monitoring experiment informs ongoing efforts to capture entire unrest cycles at more active but generally less accessible volcanoes such as those in the Aleutian arc.

  12. Explosive Deep Sea Volcanism Produces Composite Volcanoes (Stratocones) with Predominantly Diffuse Flow Hydrothermal Ecosystems

    NASA Astrophysics Data System (ADS)

    Rubin, K. H.; Chadwick, W. C.; Embley, R. W.; Butterfield, D. A.

    2018-05-01

    Newly-discovered extensive explosive deep sea volcanism produces distinct stratovolcano structures and physical rock characteristics, and host primarily diffuse flow hydrothermal activity, unlike focused flow systems at effusive submarine volcanoes.

  13. Back-Projection Imaging of extended, diffuse seismic sources in volcanic and hydrothermal systems

    NASA Astrophysics Data System (ADS)

    Kelly, C. L.; Lawrence, J. F.; Beroza, G. C.

    2017-12-01

    Volcanic and hydrothermal systems exhibit a wide range of seismicity that is directly linked to fluid and volatile activity in the subsurface and that can be indicative of imminent hazardous activity. Seismograms recorded near volcanic and hydrothermal systems typically contain "noisy" records, but in fact, these complex signals are generated by many overlapping low-magnitude displacements and pressure changes at depth. Unfortunately, excluding times of high-magnitude eruptive activity that typically occur infrequently relative to the length of a system's entire eruption cycle, these signals often have very low signal-to-noise ratios and are difficult to identify and study using established seismic analysis techniques (i.e. phase-picking, template matching). Arrays of short-period and broadband seismic sensors are proven tools for monitoring short- and long-term changes in volcanic and hydrothermal systems. Time-reversal techniques (i.e. back-projection) that are improved by additional seismic observations have been successfully applied to locating volcano-seismic sources recorded by dense sensor arrays. We present results from a new computationally efficient back-projection method that allows us to image the evolution of extended, diffuse sources of volcanic and hydrothermal seismicity. We correlate short time-window seismograms from receiver-pairs to find coherent signals and propagate them back in time to potential source locations in a 3D subsurface model. The strength of coherent seismic signal associated with any potential source-receiver-receiver geometry is equal to the correlation of the short time-windows of seismic records at appropriate time lags as determined by the velocity structure and ray paths. We stack (sum) all short time-window correlations from all receiver-pairs to determine the cumulative coherence of signals at each potential source location. Through stacking, coherent signals from extended and/or repeating sources of short-period energy

  14. Active hydrothermal and non-active massive sulfide mound investigation using a new multiparameter chemical sensor

    NASA Astrophysics Data System (ADS)

    Han, C.; Wu, G.; Qin, H.; Wang, Z.

    2012-12-01

    Investigation of active hydrothermal mound as well as non-active massive sulfide mound are studied recently. However, there is still lack of in-situ detection method for the non-active massive sulfide mound. Even though Transient ElectroMagnetic (TEM) and Electric Self-potential (SP) methods are good, they both are labour, time and money cost work. We proposed a new multiparameter chemical sensor method to study the seafloor active hydrothermal mound as well as non-active massive sulfide mound. This sensor integrates Eh, S2- ions concentration and pH electrochemical electrodes together, and could found chemical change caused by the active hydrothermal vent, even weak chemical abnormalities by non-active massive sulfide hydrothermal mound which MARP and CTD sometimes cannot detect. In 2012, the 1st Leg of the Chinese 26th cruise, the multiparameter chemical sensor was carried out with the deepsea camera system over the Carlsberg Ridge in Indian Ocean by R/V DAYANGYIHAO. It was shown small Eh and S2- ions concentration abnormal around a site at Northwest Indian ridge. This site was also evidenced by the TV grab. In the 2nd Leg of the same cruise in June, this chemical sensor was carried out with TEM and SP survey system. The chemical abnormalities are matched very well with both TEM and SP survey results. The results show that the multiparameter chemical sensor method not only can detect active hydrothermal mound, but also can find the non-active massive sulfide hydrothermal mound.

  15. Hydrothermal Solute Flux from Ebeko Volcanic Center, Paramushir, Kuril Islands

    NASA Astrophysics Data System (ADS)

    Taran, Y.; Kalacheva, E.; Kotenko, T.; Chaplygin, I.

    2014-12-01

    Ebeko volcano on the northern part of Paramushir Island, Northern Kurils, is characterized by frequent phreatic eruptions, a strong low-temperature fumarolic activity at the summit and was the object of comprehensive volcanological and geochemical studies during the last half a century. The volcanic center is composed of several Pleistocene volcanic structures aadjacent to Ebeko and hosts a hydrothermal system with a high outflow rate of hot SO4-Cl acidic water (Upper Yurieva springs) with the current maximum temperature of ~85oC, pH 1.3 and TDS ~ 10 g/L. All discharging thermal waters are drained by the Yurieva River to the Sea of Okhotsk. The hot springs have been changing in time, generally decreasing their activity from near boiling in 1960s, with TDS ~ 20 g/L and the presence of a small steaming field at the upper part of the ~ 700 m long discharging area, to a much lower discharge rate of main vents, lower temperature and the absence of the steaming ground. The spring chemistry did not react to the Ebeko volcanic activity (14 strong phreato-magmatic events during the last 60 years).The total measured outputs of chloride and sulfur from the system last time (2006-2010) were estimated on average as 730 g/s and 980 g/s, respectively, which corresponds to the equivalent fluxes of 64 t/d of HCl and 169 t/d of SO2. These values are higher than the fumarolic volatile output from Ebeko. The estimated discharge rate of hot (85oC) water from the system with ~ 3500 ppm of chloride is about 0.3 m3/s which is much higher than the thermal water discharge from El Chichon or Copahue volcano-hydrothermal systems and among the highest hot water natural outputs ever measured for a volcano-hydrothermal system. We also report the chemical composition (major and ~ 60 trace elements including REE) of water from the main hot spring vents and the Yurieva river mouth.

  16. River solute fluxes reflecting active hydrothermal chemical weathering of the Yellowstone Plateau Volcanic Field, USA

    USGS Publications Warehouse

    Hurwitz, S.; Evans, William C.; Lowenstern, J. B.

    2010-01-01

    In the past few decades numerous studies have quantified the load of dissolved solids in large rivers to determine chemical weathering rates in orogenic belts and volcanic areas, mainly motivated by the notion that over timescales greater than ~100kyr, silicate hydrolysis may be the dominant sink for atmospheric CO2, thus creating a feedback between climate and weathering. Here, we report the results of a detailed study during water year 2007 (October 1, 2006 to September 30, 2007) in the major rivers of the Yellowstone Plateau Volcanic Field (YPVF) which hosts Earth's largest "restless" caldera and over 10,000 thermal features. The chemical compositions of rivers that drain thermal areas in the YPVF differ significantly from the compositions of rivers that drain non-thermal areas. There are large seasonal variations in river chemistry and solute flux, which increases with increasing water discharge. The river chemistry and discharge data collected periodically over an entire year allow us to constrain the annual solute fluxes and to distinguish between low-temperature weathering and hydrothermal flux components. The TDS flux from Yellowstone Caldera in water year 2007 was 93t/km2/year. Extensive magma degassing and hydrothermal interaction with rocks accounts for at least 82% of this TDS flux, 83% of the cation flux and 72% of the HCO3- flux. The low-temperature chemical weathering rate (17t/km2/year), calculated on the assumption that all the Cl- is of thermal origin, could include a component from low-temperature hydrolysis reactions induced by CO2 ascending from depth rather than by atmospheric CO2. Although this uncertainty remains, the calculated low-temperature weathering rate of the young rhyolitic rocks in the Yellowstone Caldera is comparable to the world average of large watersheds that drain also more soluble carbonates and evaporates but is slightly lower than calculated rates in other, less-silicic volcanic regions. Long-term average fluxes at

  17. Stable isotopes evidence of recycled subduction fluids in the hydrothermal/volcanic activity across Nicaragua and Costa Rica

    NASA Astrophysics Data System (ADS)

    Ramírez-Leiva, A.; Sánchez-Murillo, R.; Martínez-Cruz, M.; Calderón, H.; Esquivel-Hernández, G.; Delgado, V.; Birkel, C.; Gazel, E.; Alvarado, G. E.; Soulsby, C.

    2017-10-01

    The Central America volcanic front provides a unique opportunity to study hydrothermal inputs and their interaction and mixing with modern meteoric waters. The objectives of this study were to: a) characterize the isotopic composition (δ18O, δ2H, d-excess, and lc-excess) of hydrothermal/volcanic systems, b) analyze the influence of kinetic fractionation and meteoric water inputs in the isotopic composition of hydrothermal waters, and c) estimate the 'andesitic water' contribution (recycled subduction fluids) within the volcanic front of Nicaragua and Costa Rica. Hydrothermal evaporation lines are described as: δ2H = 4.7·δ18O - 13.0 (Costa Rica) and δ2H = 2.7·δ18O - 31.6 (Nicaragua). These regressions are significantly (p < 0.001) deviated from their respective meteoric water lines: δ2H = 7.6·δ18O + 7.4 (Costa Rica) and δ2H = 7.4·δ18O + 5.2 (Nicaragua). The greater rainfall inputs in Costa Rica with respect to Nicaragua, resulted in the attenuation of the evaporative effect as observed in the strong bimodal distribution of the hydrothermal waters, which can be divided in fluids: a) isotopically-close to meteoric conditions and b) isotopically-altered by the interaction with recycled subduction fluids and kinetic fractionation. The latter is clearly depicted in the significantly (p < 0.001) low d-excess and lc-excess median values between Costa Rica (+ 5.10‰, - 5.25‰) and Nicaragua (- 2.42‰, - 10.65‰), respectively. Poor correlations between δ18O/δ2H and the elevation gradient emphasize that the contribution of recycled subduction fluids and subsequent surface kinetic fractionation are the main drivers of the isotopic departure from the orographic distillation trend captured in the rainfall isoscapes. End-member mixing calculations resulted in a significant difference (p < 0.001) between the mean 'andesitic water' contribution to the hydrothermal systems of 15.3 ± 10.8 (%, ± 1σ) (Nicaragua) and 19.7 ± 10.3 (%, ± 1σ) (Costa Rica). The

  18. Investigating Volcanic-Hydrothermal Systems in Dominica, Lesser Antilles: Temporal Changes in the Chemical Composition of Hydrothermal Fluids for Volcanic Monitoring Using Geothermometers

    NASA Astrophysics Data System (ADS)

    Onyeali, M. M. C.; Joseph, E. P.; Frey, H. M.

    2017-12-01

    Dominica has an abundance of volcanic activity, with nine potentially active volcanoes, many of which have highly active volcanic-hydrothermal systems. The waters are predominantly acid-sulphate in character (SO4=100-4200 mg/L, pH≤4), and likely formed because of dilution of acidic gases in near surface oxygenated groundwater. The waters are of primarily meteoric origin, but are likely affected by evaporation effects at/near the surface, with δ18O ranging from -1.75 to 10.67‰, and δD from -6.1 to 14.5‰. With updated water chemistry and isotopic data from five hydrothermal areas (Boiling Lake, Valley of Desolation, Sulphur Springs, Wotten Waven, Cold Soufriere) for the period 2014 to 2017, we will re-evaluate the characteristics of these systems, which were last reported in 2011. We will present updated reservoir temperatures using a variety of geothermometers and provide insight into water-rock interactions taking place in the reservoirs. Recent changes in chemistry of the waters have indicated that while the origin of the hydrothermal systems are still dominantly meteoric (δ18O = -3 to 8‰ and δD = -5 to 18‰), surface evaporation effects and variable amounts of mixing with shallow ground waters play an important role. Fumaroles appear to reflect a deeper source contribution as compared to thermal waters with differences in acidity, temperature, TDS, δ18O, and δD observed. The general composition of the waters for most of the hydrothermal systems studied indicate no significant changes, with the exception of the Boiling Lake, which experienced a draining event in November 2016 which lasted for 6 weeks. Decreases in temperature, pH, Na, K, and Cl were seen post draining, while SO4 remained relatively low (66 ppm), but showed a small increase. The chemistry of the Boiling Lake appears to show significant changes in response to changes in the groundwater system. Changes in the groundwater system at the lake observed during the 2004/2005 draining, which

  19. 600 kyr of Hydrothermal Activity on the Cleft Segment of the Juan de Fuca Ridge

    NASA Astrophysics Data System (ADS)

    Middleton, J. L.; Mukhopadhyay, S.; Langmuir, C. H.; Costa, K.; McManus, J. F.; Katz, R. F.; Huybers, P. J.; Winckler, G.; Li, Y.

    2017-12-01

    Pressure fluctuations caused by glacially driven variations in sea level may modulate magmatic and hydrothermal output at submarine volcanic centers, with falling sea level driving increased volcanic activity. In turn, glacially paced changes in submarine volcanism could induce globally synchronous variations in the delivery of bioavailable iron and CO2 from mid-ocean ridges and thus provide solid-Earth feedbacks into the climate system. While evaluation of submarine volcanic output on orbital-timescales is technically challenging, near-ridge sediment cores hosting hydrothermal plume precipitates provide continuous, spatially integrated, and datable records to investigate the long-term behavior of hydrothermal systems. We will present new sedimentary records of hydrothermal variability spanning the past 600 kyr on the Cleft Segment of the Juan de Fuca Ridge in the Northeast Pacific. As an intermediate spreading-rate ridge, the Juan de Fuca Ridge is hypothesized to be particularly sensitive to sea level forcing at the Milankovitch frequencies of Pleistocene glacial cycles. Thus, the new records can be used to examine the connection between sea level and hydrothermal activity over multiple glacial cycles. Hydrothermal input is determined from iron and copper, with a titanium-based correction for lithogenic contributions. Sedimentary fluxes are then constrained using excess thorium-230 and extraterrestrial helium-3 as constant flux proxies. Preliminary results indicate 10-fold changes in hydrothermal iron and copper fluxes over the past 600 kyr and suggest a quasiperiodic variability in hydrothermal deposition on 100 to 120 kyr cycles. Comparison of the Juan de Fuca record with model predictions for an intermediate spreading ridge forced by Pleistocene glacial cycles finds frequent coincidence between predicted positive anomalies in magmatic output and observed peaks in hydrothermal deposition. This work encourages the continued exploration of the relationship between

  20. Hydrothermal activity lowers trophic diversity in Antarctic hydrothermal sediments

    NASA Astrophysics Data System (ADS)

    Bell, James B.; Reid, William D. K.; Pearce, David A.; Glover, Adrian G.; Sweeting, Christopher J.; Newton, Jason; Woulds, Clare

    2017-12-01

    Hydrothermal sediments are those in which hydrothermal fluid is discharged through sediments and are one of the least studied deep-sea ecosystems. We present a combination of microbial and biochemical data to assess trophodynamics between and within hydrothermal and background areas of the Bransfield Strait (1050-1647 m of depth). Microbial composition, biomass, and fatty acid signatures varied widely between and within hydrothermally active and background sites, providing evidence of diverse metabolic activity. Several species had different feeding strategies and trophic positions between hydrothermally active and inactive areas, and the stable isotope values of consumers were not consistent with feeding morphology. Niche area and the diversity of microbial fatty acids was lowest at the most hydrothermally active site, reflecting trends in species diversity. Faunal uptake of chemosynthetically produced organics was relatively limited but was detected at both hydrothermal and non-hydrothermal sites, potentially suggesting that hydrothermal activity can affect trophodynamics over a much wider area than previously thought.

  1. The North Tanganyika hydrothermal fields, East African Rift system: Their tectonic control and relationship to volcanism and rift segmentation

    NASA Astrophysics Data System (ADS)

    Coussement, C.; Gente, P.; Rolet, J.; Tiercelin, J.-J.; Wafula, M.; Buku, S.

    1994-10-01

    The two branches of the East African Rift system include numerous hydrothermal fields, which are closely related to the present fault motion and to volcanic and seismic activity. In this study structural data from Pemba and Cape Banza hydrothermal fields (western branch, North Tanganyika, Zaire) are discussed in terms of neotectonic phenomena. Different types of records, such as fieldwork (onshore and underwater) and LANDSAT and SPOT imagery, are used to explain structural controls on active and fossil hydrothermal systems and their significance. The Pemba site is located at the intersection of 000-020°-trending normal faults belonging to the Uvira Border Fault System and a 120-130°-trending transtensional fault zone and is an area of high seismicity, with events of relatively large magnitude ( Ms < 6.5). The Cape Banza site occurs at the northern end of the Ubawari Peninsula horst. It is bounded by two fault systems trending 015° and is characterized seismically by events of small magnitude ( Ms < 4). The hydrothermal area itself is tectonically controlled by structures striking 170-180° and 080°. The analysis of both hydrothermal areas demonstrates the rejuvenation of older Proterozoic structures during Recent rift faulting and the location of the hydrothermal activity at the junctions of submeridian and transverse faults. The fault motion is compatible with a regional direction of extension of 090-110°. The Cape Banza and Pemba hydrothermal fields may testify to magma chambers existing below the junctions of the faults. They appear to form at structural nodes and may represent a future volcanic province. Together with the four surface volcanic provinces existing along the western branch, they possibly indicate an incipient rift segmentation related to 'valley-valley' or 'transverse fault-valley' junctions, contrasting with the spacing of the volcanoes measured in the eastern branch. These spacings appear to express the different elastic thicknesses between

  2. Volcanism and hydrothermalism on a hotspot-influenced ridge: Comparing Reykjanes Peninsula and Reykjanes Ridge, Iceland

    NASA Astrophysics Data System (ADS)

    Pałgan, Dominik; Devey, Colin W.; Yeo, Isobel A.

    2017-12-01

    Current estimates indicate that the number of high-temperature vents (one of the primary pathways for the heat extraction from the Earth's mantle) - at least 1 per 100 km of axial length - scales with spreading rate and should scale with crustal thickness. But up to present, shallow ridge axes underlain by thick crust show anomalously low incidences of high-temperature activity. Here we compare the Reykjanes Ridge, an abnormally shallow ridge with thick crust and only one high-temperature vent known over 900 km axial length, to the adjacent subaerial Reykjanes Peninsula (RP), which is characterized by high-temperature geothermal sites confined to four volcanic systems transected by fissure swarms with young (Holocene) volcanic activity, multiple faults, cracks and fissures, and continuous seismic activity. New high-resolution bathymetry (gridded at 60 m) of the Reykjanes Ridge between 62°30‧N and 63°30‧N shows seven Axial Volcanic Ridges (AVR) that, based on their morphology, geometry and tectonic regime, are analogues for the volcanic systems and fissure swarms on land. We investigate in detail the volcano-tectonic features of all mapped AVRs and show that they do not fit with the previously suggested 4-stage evolution model for AVR construction. Instead, we suggest that AVR morphology reflects the robust or weak melt supply to the system and two (or more) eruption mechanisms may co-exist on one AVR (in contrast to 4-stage evolution model). Our interpretations indicate that, unlike on the Reykjanes Peninsula, faults on and around AVRs do not cluster in orientation domains but all are subparallel to the overall strike of AVRs (orthogonal to spreading direction). High abundance of seamounts shows that the region centered at 62°47‧N and 25°04‧W (between AVR-5 and -6) is volcanically robust while the highest fault density implies that AVR-1 and southern part of AVR-6 rather undergo period of melt starvation. Based on our observations and interpretations we

  3. The NOAA/PMEL Vents Program - 1983 to 2013: A History of Deep-Sea Volcanic and Hydrothermal Exploration and Research

    NASA Astrophysics Data System (ADS)

    Hammond, S. R.; Baker, E. T.; Embley, R. W.

    2015-12-01

    Inspiration for the Vents program arose from two serendipitous events: the discovery of seafloor spreading-center hydrothermal venting on the Galápagos Rift in 1977, and NOAA's deployment of the first US civilian research multibeam bathymetric sonar on the NOAA Ship Surveyor in 1979. Multibeam mapping in the NE Pacific revealed an unprecedented and revolutionary perspective of the Gorda and Juan de Fuca spreading centers, thus stimulating a successful exploration for volcanic and hydrothermal activity at numerous locations along both. After the 1986 discovery of the first "megaplume,", quickly recognized as the water column manifestation of a deep submarine volcanic eruption, the Vents program embarked on a multi-decadal effort to discover and understand local-, regional-, and, ultimately, global-scale physical, chemical, and biological ocean environmental impacts of submarine volcanism and hydrothermal venting. The Vents program made scores of scientific discoveries, many of which owed their success to the program's equally innovative and productive technological prowess. These discoveries were documented in hundreds of peer-reviewed papers by Vents researchers and their colleagues around the world. An emblematic success was the internationally recognized, first-ever detection, location, and study of an active deep volcanic eruption in 1993. To continue the Vents mission and further enhance its effectiveness in marine science and technology innovation, the program was reorganized in 2014 into two distinct, but closely linked, programs: Earth-Oceans Interactions and Acoustics. Both are currently engaged in expeditions and projects that maintain the Vents tradition of pioneering ocean exploration and research.

  4. The interplay of evolved seawater and magmatic-hydrothermal fluids in the 3.24 Ga panorama volcanic-hosted massive sulfide hydrothermal system, North Pilbara Craton, Western Australia

    USGS Publications Warehouse

    Drieberg, Susan L.; Hagemann, Steffen G.; Huston, David L.; Landis, Gary; Ryan, Chris G.; Van Achterbergh, Esmé; Vennemann, Torsten

    2013-01-01

    The ~3240 Ma Panorama volcanic-hosted massive sulfide (VHMS) district is unusual for its high degree of exposure and low degree of postdepositional modification. In addition to typical seafloor VHMS deposits, this district contains greisen- and vein-hosted Mo-Cu-Zn-Sn mineral occurrences that are contemporaneous with VHMS orebodies and are hosted by the Strelley granite complex, which also drove VHMS circulation. Hence the Panorama district is a natural laboratory to investigate the role of magmatic-hydrothermal fluids in VHMS hydrothermal systems. Regional and proximal high-temperature alteration zones in volcanic rocks underlying the VHMS deposits are dominated by chlorite-quartz ± albite assemblages, with lesser low-temperature sericite-quartz ± K-feldspar assemblages. These assemblages are typical of VHMS hydrothermal systems. In contrast, the alteration assemblages associated with granite-hosted greisens and veins include quartz-topaz-muscovite-fluorite and quartz-muscovite (sericite)-chlorite-ankerite. These vein systems generally do not extend into the overlying volcanic pile. Fluid inclusion and stable isotope studies suggest that the greisens were produced by high-temperature (~590°C), high-salinity (38–56 wt % NaCl equiv) fluids with high densities (>1.3 g/cm3) and high δ18O (9.3 ± 0.6‰). These fluids are compatible with the measured characteristics of magmatic fluids evolved from the Strelley granite complex. In contrast, fluids in the volcanic pile (including the VHMS ore-forming fluids) were of lower temperature (90°–270°C), lower salinity (5.0–11.2 wt % NaCl equiv), with lower densities (0.88–1.01 g/cm3) and lower δ18O (−0.8 ± 2.6‰). These fluids are compatible with evolved Paleoarchean seawater. Fluids that formed the quartz-chalcopyrite-sphalerite-cassiterite veins, which are present within the granite complex near the contact with the volcanic pile, were intermediate in temperature and isotopic composition between the greisen

  5. Hydrothermal nontronite formation at Eolo Seamount (Aeolian volcanic arc, Tyrrhenian Sea)

    USGS Publications Warehouse

    Dekov, V.M.; Kamenov, George D.; Stummeyer, Jens; Thiry, M.; Savelli, C.; Shanks, Wayne C.; Fortin, D.; Kuzmann, E.; Vertes, A.

    2007-01-01

    A sediment core containing a yellowish-green clay bed was recovered from an area of extensive hydrothermal deposition at the SE slope of the Eolo Seamount, Tyrrhenian Sea. The clay bed is composed of pure nontronite (described for the first time in the Tyrrhenian Sea), which appears to be the most aluminous nontronite ever found among the seafloor hydrothermal deposits. The high Al content suggests precipitation from Al-containing hydrothermal solutions. The REE distribution of the Eolo nontronite has a V-shape pattern. The heavy REE enrichment is in part due to their preferential partitioning in the nontronite structure. This enrichment was possibly further enhanced by the HREE preferential sorption on bacterial cell walls. The light REE enrichment is the result of scavenging uptake by one of the nontronite precursors, i.e., poorly-ordered Fe-oxyhydroxides, from the hydrothermal fluids. Oxygen isotopic composition of the nontronite yields a formation temperature of 30????C, consistent with a low-temperature hydrothermal origin. The relatively radiogenic Nd isotopic signature of the nontronite compared to the present-day Mediterranean seawater indicates that approximately half of Nd, and presumably the rest of the LREE, are derived from local volcanic sources. On the other hand, 87Sr/86Sr is dominated by present-day seawater Sr. Scanning electron microscopy investigation revealed that the nontronite is composed of aggregates of lepispheres and tube-like filaments, which are indicative of bacteria assisted precipitation. Bacteria inhabiting this hydrothermal site likely acted as reactive geochemical surfaces on which poorly-ordered hydrothermal Fe-oxyhydroxides and silica precipitated. Upon aging, the interactions of these primary hydrothermal precipitates coating bacterial filaments and cell walls likely led to the formation of nontronite. Finally, the well-balanced interlayer and layer charges of the crystal lattice of seafloor hydrothermal nontronite decrease its

  6. Radon surveys and monitoring at active volcanoes: an open window on deep hydrothermal systems and their dynamics

    NASA Astrophysics Data System (ADS)

    Cigolini, Corrado; Laiolo, Marco; Coppola, Diego

    2017-04-01

    The behavior of fluids in hydrothermal systems is critical in volcano monitoring and geothermal prospecting. Analyzing the time series of radon emissions on active volcanoes is strategic for detecting and interpreting precursory signals of changes in volcanic activity, eventually leading to eruptions. Radon is a radioactive gas generated from the decay of U bearing rocks, soils and magmas. Although radon has been regarded as a potential precursor of earthquakes, radon anomalies appear to be better suited to forecast volcanic eruptions since we know where paroxysms may occur and we can follow the evolution of volcanic activity. Radon mapping at active volcanoes is also a reliable tool to assess diffuse and concentrated degassing as well as efficiently detecting earthquake-volcano interactions. Systematic radon monitoring has been shown to be a key factor for evaluating the rise of volcanic and hydrothermal fluids. In fact, the decay properties of radon, the duration of radon anomalies together with sampling rates may be cross-checked with the chemistry of hydrothermal fluids (and their transport properties) to constrain fluids ascent rates and to infer the permeability and porosity of rocks in sectors surrounding the active conduits. We hereby further discuss the data of radon surveys and monitoring at Somma-Vesuvius, Stromboli and La Soufrière (Guadeloupe, Lesser Antilles). The integrated analysis of seismic and geochemical data, including radon emissions, may be successfully used in testing temperature distributions and variations of porosity and permeability in volcanic hydrothermal systems and can be used as a proxy to analyze geothermal reservoirs.

  7. Geochemical and Visual Indicators of Hydrothermal Fluid Flow through a Sediment-Hosted Volcanic Ridge in the Central Bransfield Basin (Antarctica)

    PubMed Central

    Aquilina, Alfred; Connelly, Douglas P.; Copley, Jon T.; Green, Darryl R. H.; Hawkes, Jeffrey A.; Hepburn, Laura E.; Huvenne, Veerle A. I.; Marsh, Leigh; Mills, Rachel A.; Tyler, Paul A.

    2013-01-01

    In the austral summer of 2011 we undertook an investigation of three volcanic highs in the Central Bransfield Basin, Antarctica, in search of hydrothermal activity and associated fauna to assess changes since previous surveys and to evaluate the extent of hydrothermalism in this basin. At Hook Ridge, a submarine volcanic edifice at the eastern end of the basin, anomalies in water column redox potential (Eh) were detected close to the seafloor, unaccompanied by temperature or turbidity anomalies, indicating low-temperature hydrothermal discharge. Seepage was manifested as shimmering water emanating from the sediment and from mineralised structures on the seafloor; recognisable vent endemic fauna were not observed. Pore fluids extracted from Hook Ridge sediment were depleted in chloride, sulfate and magnesium by up to 8% relative to seawater, enriched in lithium, boron and calcium, and had a distinct strontium isotope composition (87Sr/86Sr  = 0.708776 at core base) compared with modern seawater (87Sr/86Sr ≈0.70918), indicating advection of hydrothermal fluid through sediment at this site. Biogeochemical zonation of redox active species implies significant moderation of the hydrothermal fluid with in situ diagenetic processes. At Middle Sister, the central ridge of the Three Sisters complex located about 100 km southwest of Hook Ridge, small water column Eh anomalies were detected but visual observations of the seafloor and pore fluid profiles provided no evidence of active hydrothermal circulation. At The Axe, located about 50 km southwest of Three Sisters, no water column anomalies in Eh, temperature or turbidity were detected. These observations demonstrate that the temperature anomalies observed in previous surveys are episodic features, and suggest that hydrothermal circulation in the Bransfield Strait is ephemeral in nature and therefore may not support vent biota. PMID:23359806

  8. Volcanic Centers in the East Africa Rift: Volcanic Processes with Seismic Stresses to Identify Potential Hydrothermal Vents

    NASA Astrophysics Data System (ADS)

    Patlan, E.; Wamalwa, A. M.; Kaip, G.; Velasco, A. A.

    2015-12-01

    The Geothermal Development Company (GDC) in Kenya actively seeks to produce geothermal energy, which lies within the East African Rift System (EARS). The EARS, an active continental rift zone, appears to be a developing tectonic plate boundary and thus, has a number of active as well as dormant volcanoes throughout its extent. These volcanic centers can be used as potential sources for geothermal energy. The University of Texas at El Paso (UTEP) and the GDC deployed seismic sensors to monitor several volcanic centers: Menengai, Silali, and Paka, and Korosi. We identify microseismic, local events, and tilt like events using automatic detection algorithms and manual review to identify potential local earthquakes within our seismic network. We then perform the double-difference location method of local magnitude less than two to image the boundary of the magma chamber and the conduit feeding the volcanoes. In the process of locating local seismicity, we also identify long-period, explosion, and tremor signals that we interpret as magma passing through conduits of the magma chamber and/or fluid being transported as a function of magma movement or hydrothermal activity. We used waveform inversion and S-wave shear wave splitting to approximate the orientation of the local stresses from the vent or fissure-like conduit of the volcano. The microseismic events and long period events will help us interpret the activity of the volcanoes. Our goal is to investigate basement structures beneath the volcanoes and identify the extent of magmatic modifications of the crust. Overall, these seismic techniques will help us understand magma movement and volcanic processes in the region.

  9. Diffuse emissions of Volatile Organic Compounds (VOCs) from soil in volcanic and hydrothermal systems: evidences for the influence of microbial activity on the carbon budget

    NASA Astrophysics Data System (ADS)

    Venturi, Stefania; Tassi, Franco; Fazi, Stefano; Vaselli, Orlando; Crognale, Simona; Rossetti, Simona; Cabassi, Jacopo; Capecchiacci, Francesco

    2017-04-01

    Soils in volcanic and hydrothermal areas are affected by anomalously high concentrations of gases released from the deep reservoirs, which consists of both inorganic (mainly CO2 and H2S) and organic (volatile organic compounds; VOCs) species. VOCs in volcanic and hydrothermal fluids are mainly composed of saturated and unsaturated hydrocarbons (alkanes, aromatics, alkenes, and cyclics), with variable concentrations of O- and S-bearing compounds and halocarbons, depending on the physicochemical conditions at depth. VOCs in interstitial soil gases and fumarolic emissions from four volcanic and hydrothermal systems in the Mediterranean area (Solfatara Crater, Poggio dell'Olivo and Cava dei Selci, in Italy, and Nisyros Island, in Greece) evidenced clear compositional differences, suggesting that their behavior is strongly affected by secondary processes occurring at shallow depths and likely controlled by microbial activity. Long-chain saturated hydrocarbons were significantly depleted in interstitial soil gases with respect to those from fumarolic discharges, whereas enrichments in O-bearing compounds (e.g. aldehydes, ketones), DMSO2 and cyclics were commonly observed. Benzene was recalcitrant to degradation processes, whereas methylated aromatics were relatively instable. The chemical and isotopic (δ13C in CO2 and CH4) composition of soil gases collected along vertical profiles down to 50 cm depth at both Solfatara Crater and Poggio dell'Olivo (Italy) showed evidences of relevant oxidation processes in the soil, confirming that microbial activity likely plays a major role in modifying the composition of deep-derived VOCs. Despite their harsh conditions, being typically characterized by high temperatures, low pH, and high toxic gases and metal contents, the variety of habitats characterizing volcanic and hydrothermal environments offers ideal biomes to extremophilic microbes, whose metabolic activity can consume and/or produce VOCs. In the Solfatara Crater, microbial

  10. Oxygen isotope evidence for hydrothermal alteration within a Quaternary stratovolcano, Lassen Volcanic National Park, California

    NASA Astrophysics Data System (ADS)

    Rose, Timothy P.; Criss, Robert E.; Mughannam, Andrew J.; Clynne, Michael A.

    1994-11-01

    Brokeoff volcano, a Quaternary stratocone located in the Lassen volcanic center in northern California, has been deeply eroded, exposing a 10-sq km meteoric hydrothermal alteration zone at the core of the volcano. Portions of the former volcanic edifice are sufficiently well preserved that an unusual opportunity exists wherein the alteration pattern can be correlated with the position of the volcanic cone. The delta(O-18) analyses of more than 100 whole rock samples, consisting primarily of andesitic lavas, vary from +9.8 to +0.6 per mil. The highest delta(O-18) values occur in bleached, solfatarically altered rocks that have interacted with low-pH, fumarolic hot springs associated with the present-day hydrothermal system. Low delta(O-18) values are found in propylitically altered rocks that underwent isotopic exchange with meteoric hydrothermal fluids at elevated temperatures, mostly during the stratovolcanic stage (650-400 ka) of the hydrothermal system, but probably continuing today at depth. Electron microprobe analyses of secondary layer silicate minerals in strongly propylitized samples (delta(O-18) is less than +5.0) revealed the presence of discrete chlorite, suggesting that temperatures up to 200 to 250 C were attained in the shallow levels of the system. Two zones of pervasive meteoric hydrothermal alteration, defined by concentric O-18 contours that are probably interconnected at depth, are located within the original topographic edifice of the volcano. The most intensely altered rocks within these equant zones of alteration define NNW trends that coincide with stream valleys and with regional structural patterns. A comparison of the characteristics of the O-18-depleted zone at Brokeoff with those of more deeply eroded volcanic centers, such as the Comstock Lode mining district (Criss and Champion, 1991), permits the construction of composite O-18 cross sections through a hypothetical intact stratovolcano. At both Brokeoff and Comstock, hydrothermal

  11. Investigating Crustal Scale Fault Systems Controlling Volcanic and Hydrothermal Fluid Processes in the South-Central Andes, First Results from a Magnetotelluric Survey

    NASA Astrophysics Data System (ADS)

    Pearce, R.; Mitchell, T. M.; Moorkamp, M.; Araya, J.; Cembrano, J. M.; Yanez, G. A.; Hammond, J. O. S.

    2017-12-01

    At convergent plate boundaries, volcanic orogeny is largely controlled by major thrust fault systems that act as magmatic and hydrothermal fluid conduits through the crust. In the south-central Andes, the volcanically and seismically active Tinguiririca and Planchon-Peteroa volcanoes are considered to be tectonically related to the major El Fierro thrust fault system. These large scale reverse faults are characterized by 500 - 1000m wide hydrothermally altered fault cores, which possess a distinct conductive signature relative to surrounding lithology. In order to establish the subsurface architecture of these fault systems, such conductivity contrasts can be detected using the magnetotelluric method. In this study, LEMI fluxgate-magnetometer long-period and Metronix broadband MT data were collected at 21 sites in a 40km2 survey grid that surrounds this fault system and associated volcanic complexes. Multi-remote referencing techniques is used together with robust processing to obtain reliable impedance estimates between 100 Hz and 1,000s. Our preliminary inversion results provide evidence of structures within the 10 - 20 km depth range that are attributed to this fault system. Further inversions will be conducted to determine the approximate depth extent of these features, and ultimately provide constraints for future geophysical studies aimed to deduce the role of these faults in volcanic orogeny and hydrothermal fluid migration processes in this region of the Andes.

  12. Vein networks in hydrothermal systems provide constraints for the monitoring of active volcanoes.

    PubMed

    Cucci, Luigi; Di Luccio, Francesca; Esposito, Alessandra; Ventura, Guido

    2017-03-10

    Vein networks affect the hydrothermal systems of many volcanoes, and variations in their arrangement may precede hydrothermal and volcanic eruptions. However, the long-term evolution of vein networks is often unknown because data are lacking. We analyze two gypsum-filled vein networks affecting the hydrothermal field of the active Lipari volcanic Island (Italy) to reconstruct the dynamics of the hydrothermal processes. The older network (E1) consists of sub-vertical, N-S striking veins; the younger network (E2) consists of veins without a preferred strike and dip. E2 veins have larger aperture/length, fracture density, dilatancy, and finite extension than E1. The fluid overpressure of E2 is larger than that of E1 veins, whereas the hydraulic conductance is lower. The larger number of fracture intersections in E2 slows down the fluid movement, and favors fluid interference effects and pressurization. Depths of the E1 and E2 hydrothermal sources are 0.8 km and 4.6 km, respectively. The decrease in the fluid flux, depth of the hydrothermal source, and the pressurization increase in E2 are likely associated to a magma reservoir. The decrease of fluid discharge in hydrothermal fields may reflect pressurization at depth potentially preceding hydrothermal explosions. This has significant implications for the long-term monitoring strategy of volcanoes.

  13. Extensive hydrothermal activity in the NE Lau basin revealed by ROV dives

    NASA Astrophysics Data System (ADS)

    Embley, R. W.; Resing, J. A.; Tebo, B.; Baker, E. T.; Butterfield, D. A.; Chadwick, B.; Davis, R.; de Ronde, C. E. J.; Lilley, M. D.; Lupton, J. E.; Merle, S. G.; Rubin, K. H.; Shank, T. M.; Walker, S. L.; Arculus, R. J.; Bobbitt, A. M.; Buck, N. J.; Caratori Tontini, F.; Crowhurst, P. V.; Mitchell, E.; Olson, E. J.; Ratmeyer, V.; Richards, S.; Roe, K. K.; Kenner-Chavis, P.; Martinez-Lyons, A.; Sheehan, C.; Brian, R.

    2014-12-01

    Dives with the QUEST 4000 ROV (Remotely Operated Vehicle) in September 2012 discovered nine hydrothermal sites in the arc and rear-arc region of the NE Lau Basin in 1150 m to 2630 m depth. These sites, originally detected by water column and seafloor surveys conducted in 2008-2011, include: (1) a paired sulfur-rich/black smoker field on the summit of a tectonically deformed magmatic arc volcano (Niua), (2) fracture-controlled black smoker venting on several small en echelon seamounts (north Matas) that lie between the magmatic arc and the backarc spreading center and (3) a magmatic degassing site on the summit of a dacite cone within a large (~12 km diameter) caldera volcano (Niuatahi). Dives at West Mata Seamount, which was undergoing strombolian volcanic activity and effusive rift-zone eruptions from 2008 to 2010, revealed a dormant volcanic phase in September 2012, with continued low-temperature diffuse venting. The high-temperature venting is likely driven by magmatic heat indicative of underlying partial melt zones and/or melt pockets distributed through the region. The occurrence of the youngest known boninite eruptions on the Mata volcanoes is consistent with subduction fluid flux melting extending into the rear-arc zone. Extension related to the transition from subduction to strike-slip motion of the northern Tonga Arc over the active Subduction-Transform Edge Propagator (STEP) fault probably contributes to the enhanced volcanism/hydrothermal activity in the NE Lau Basin. Chemosynthetic ecosystems at these sites range from mostly motile, lower diversity ecosystems at the eruptive/magmatically-degassing sites to higher diversity ecosystems with less mobile faunal components at the black-smoker systems. The wide range of fluid chemistry, water depth and geologic settings of the hydrothermal systems in this area provides an intriguing template to study the interaction of hydrothermal fluid chemistry, chemosynthetic habitats and their geologic underpinning

  14. Hyperactive hydrothermal activity in the NE Lau basin revealed by ROV dives

    NASA Astrophysics Data System (ADS)

    Embley, R. W.; Resing, J. A.; Tebo, B.; Baker, E. T.; Butterfield, D. A.; Chadwick, B.; Davis, R.; de Ronde, C. E.; Lilley, M. D.; Lupton, J. E.; Merle, S. G.; Rubin, K. H.; Shank, T. M.; Walker, S. L.; Arculus, R. J.; Bobbitt, A. M.; Buck, N.; Caratori Tontini, F.; Crowhurst, P. V.; Mitchell, E.; Olson, E. J.; Ratmeyer, V.; Richards, S.; Roe, K. K.; Keener, P.; Martinez Lyons, A.; Sheehan, C.; Brian, R.

    2013-12-01

    Dives with the QUEST 4000 ROV (Remotely Operated Vehicle) in September 2012 discovered nine hydrothermal sites in the arc and rear-arc region of the NE Lau Basin in 1150 m to 2630 m depth. These sites, originally detected by water column and seafloor surveys conducted in 2008-2011, include: (1) a paired sulfur-rich/black smoker field on the summit of a tectonically deformed magmatic arc volcano (Niua), (2) fracture-controlled black smoker venting on several small en echelon seamounts (north Matas) that lie between the magmatic arc and the backarc spreading center and (3) a magmatic degassing site on the summit of a dacite cone within a large (~12 km diameter) caldera volcano (Niuatahi). Dives at West Mata Seamount, which was undergoing strombolian volcanic activity and effusive rift-zone eruptions from 2008 to 2010, revealed a dormant volcanic phase in September 2012, with continued low-temperature diffuse venting. The high-temperature venting is likely driven by magmatic heat indicative of underlying partial melt zones and/or melt pockets distributed through the region. The occurrence of the youngest known boninite eruptions on the Mata volcanoes is consistent with subduction fluid flux melting extending into the rear-arc zone. Extension related to the transition from subduction to strike-slip motion of the northern Tonga Arc over the active Subduction-Transform Edge Propagator (STEP) fault probably contributes to the enhanced volcanism/hydrothermal activity in the NE Lau Basin. Chemosynthetic ecosystems at these sites range from mostly motile, lower diversity ecosystems at the eruptive/magmatically-degassing sites to higher diversity ecosystems with less mobile faunal components at the black-smoker systems. The wide range of fluid chemistry, water depth and geologic settings of the hydrothermal systems in this area provides an intriguing template to study the interaction of hydrothermal fluid chemistry, chemosynthetic habitats and their geologic underpinning

  15. Monitoring diffuse volcanic degassing during volcanic unrests: the case of Campi Flegrei (Italy).

    PubMed

    Cardellini, C; Chiodini, G; Frondini, F; Avino, R; Bagnato, E; Caliro, S; Lelli, M; Rosiello, A

    2017-07-28

    In volcanoes with active hydrothermal systems, diffuse CO 2 degassing may constitute the primary mode of volcanic degassing. The monitoring of CO 2 emissions can provide important clues in understanding the evolution of volcanic activity especially at calderas where the interpretation of unrest signals is often complex. Here, we report eighteen years of CO 2 fluxes from the soil at Solfatara of Pozzuoli, located in the restless Campi Flegrei caldera. The entire dataset, one of the largest of diffuse CO 2 degassing ever produced, is made available for the scientific community. We show that, from 2003 to 2016, the area releasing deep-sourced CO 2 tripled its extent. This expansion was accompanied by an increase of the background CO 2 flux, over most of the surveyed area (1.4 km 2 ), with increased contributions from non-biogenic source. Concurrently, the amount of diffusively released CO 2 increased up to values typical of persistently degassing active volcanoes (up to 3000 t d -1 ). These variations are consistent with the increase in the flux of magmatic fluids injected into the hydrothermal system, which cause pressure increase and, in turn, condensation within the vapor plume feeding the Solfatara emission.

  16. The Role of Siliceous Hydrothermal Breccias in the Genesis of Volcanic Massive Sulphide Deposits - Ancient and Recent Systems

    NASA Astrophysics Data System (ADS)

    Costa, I. A.; Barriga, F. J.; Fouquet, Y.

    2014-12-01

    Siliceous hydrothermal breccias were sampled in two Mid-Atlantic Ridge active sites: Lucky Strike and Menez Gwen. These hydrothermal fields are located in the border of the Azorean plateau, southwest of the Azores islands where the alteration processes affecting basaltic rocks are prominent (Costa et al., 2003). The hydrothermal breccias are genetically related with the circulation of low temperature hydrothermal fluids in diffuse vents. The groundmass of these breccias precipitates from the fluid and consolidates the clastic fragments mostly composed of basalt. The main sources are the surrounding volcanic hills. Breccias are found near hydrothermal vents and may play an important role in the protection of subseafloor hydrothermal deposits forming an impermeable cap due to the high content in siliceous material. The amorphous silica tends to precipitate when the fluid is conductively cooled as proposed by Fouquet et al. (1998) after Fournier (1983). The process evolves gradually from an initial stage where we have just the fragments and circulating seawater. The ascending hydrothermal fluid mixes with seawater, which favours the precipitation of the sulphide components. Sealing of the initially loose fragments begins, the temperature rises below this crust, and the processes of mixing fluid circulation and conductive cooling are simultaneous. At this stage the fluid becomes oversaturated with respect to amorphous silica. This form of silica can precipitate in the open spaces of the porous sulphides and seal the system. Normally this can happen at low temperatures. At this stage the hydrothermal breccia is formed creating a progressively less permeable, eventually impermeable cap rock at the surface. Once the fluid is trapped under this impermeable layer, conductive cooling is enhanced and mixing with seawater is restricted, making the precipitation of amorphous silica more efficient. Since the first discovery and description of recent mineralized submarine

  17. Hydrothermal alteration in oceanic ridge volcanics: A detailed study at the Galapagos Fossil Hydrothermal Field

    USGS Publications Warehouse

    Ridley, W.I.; Perfit, M.R.; Josnasson, I.R.; Smith, M.F.

    1994-01-01

    The Galapagos Fossil Hydrothermal Field is composed of altered oceanic crust and extinct hydrothermal vents within the eastern Galapagos Rift between 85??49???W and 85??55???W. The discharge zone of the hydrothermal system is revealed along scarps, thus providing an opportunity to examine the uppermost mineralized, and highly altered interior parts of the crust. Altered rocks collected in situ by the submersible ALVIN show complex concentric alteration zones. Microsamples of individual zones have been analysed for major/minor, trace elements, and strontium isotopes in order to describe the complex compositional details of the hydrothermal alteration. Interlayered chlorite-smectite and chlorite with disequilibrium compositions dominate the secondary mineralogy as replacement phases of primary glass and acicular pyroxene. Phenocrysts and matrix grains of plagioclase are unaffected during alteration. Using a modification of the Gresens' equation we demonstrate that the trivalent rare earth elements (REEs) are relatively immobile, and calculate degrees of enrichment and depletion in other elements. Strontium isotopic ratios increase as Sr concentrations decrease from least-altered cores to most-altered rims and cross-cutting veins in individual samples, and can be modeled by open system behaviour under low fluid-rock ratio (< 10) conditions following a period of lower-temperature weathering of volcanics within the rift zone. The complex patterns of element enrichment and depletion and strontium isotope variations indicate mixing between pristine seawater and ascending hot fluids to produce a compositional spectrum of fluids. The precipitation of base-metal sulfides beneath the seafloor is probably a result of fluid mixing and cooling. If, as suggested here, the discharge zone alteration occurred under relatively low fluid-rock ratios, then this shallow region must play an important role in determining the exit composition of vent fluids in marine hydrothermal systems

  18. Phreatic activity and hydrothermal alteration in the Valley of Desolation, Dominica, Lesser Antilles

    NASA Astrophysics Data System (ADS)

    Mayer, Klaus; Scheu, Bettina; Yilmaz, Tim I.; Montanaro, Cristian; Albert Gilg, H.; Rott, Stefanie; Joseph, Erouscilla P.; Dingwell, Donald B.

    2017-12-01

    Phreatic eruptions are possibly the most dramatic surface expressions of hydrothermal activity, and they remain poorly understood. The near absence of precursory signals makes phreatic eruptions unpredictable with respect to both time and magnitude. The Valley of Desolation (VoD), Dominica, located close to the Boiling Lake, the second largest high-temperature volcanic crater lake in the world, hosts vigorous hydrothermal activity with hot springs, mud pools, fumaroles, and steaming ground. A phreatic or phreatomagmatic eruption from this site is considered to be the most likely scenario for future volcanic activity on Dominica. Yet there is little information regarding the trigger mechanisms and eruption processes of explosive events at this active hydrothermal center, and only a very small number of studies have investigated hydrothermal activity in the VoD. We therefore conducted two field campaigns in the VoD to map hydrothermal activity and its surficial phenomena. We also investigated alteration processes and their effects on degassing and phreatic eruption processes. We collected in situ petrophysical properties of clay-rich unconsolidated samples, and together with consolidated rock samples, we investigated the range of supergene and hydrothermal alteration in the laboratory. In addition, we performed rapid decompression experiments on unconsolidated soil samples. Our results show that alteration leads to an increasing abundance of clay minerals and a decrease in both strength and permeability of the rocks. In the immediate vicinity of degassing acid-sulfate fluids, advanced argillic alteration yields a mineral zoning which is influenced by meteoric water. The water-saturated basal zone is dominated by kaolinite run 0whereas alunite formation is favored at and above the groundwater table where atmospheric oxidation of H2S to H2SO4 occurs (e.g., steam-heated alteration). Alteration effects may in turn inhibit degassing at the surface, increasing the

  19. Hydrothermal Venting at Hinepuia Submarine Volcano, Kermadec Arc: Understanding Magmatic-Hydrothermal Fluid Chemistry

    NASA Astrophysics Data System (ADS)

    Stucker, Valerie K.; Walker, Sharon L.; de Ronde, Cornel E. J.; Caratori Tontini, Fabio; Tsuchida, Shinji

    2017-10-01

    The Hinepuia volcanic center is made up of two distinct edifices aligned northwest to southeast, with an active cone complex in the SE. Hinepuia is one of several active volcanoes in the northern segment of the Kermadec arc. Regional magnetic data show no evidence for large-scale hydrothermal alteration at Hinepuia, yet plume data confirm present-day hydrothermal discharge, suggesting that the hydrothermal system may be too young to have altered the host rocks with respect to measurable changes in magnetic signal. Gravity data are consistent with crustal thinning and shallow mantle under the volcanic center. Following the discovery of hydrothermal plumes over Hinepuia, the submersible Shinkai 6500 was used to explore the SE cone and sample hydrothermal fluids. The chemistry of hydrothermal fluids from submarine arc and backarc volcanoes is typically dominated by water-rock interactions and/or magmatic degassing. Chemical analyses of vent fluids show that Hinepuia does not quite fit either traditional model. Moreover, the Hinepuia samples fall between those typically ascribed to both end-member fluid types when plotted on a K-Mg-SO4 ternary diagram. Due to evidence of strong degassing, abundant native sulfur deposition, and H2S presence, the vent sampled at Hinepuia is ultimately classified as a magmatic-hydrothermal system with a water-rock influence. This vent is releasing water vapor and magmatic volatiles with a notable lack of salinity due to subcritical boiling and phase separation. Magmatic-hydrothermal fluid chemistry appears to be controlled by a combination of gas flux, phase separation processes, and volcano evolution and/or distance from the magma source.

  20. Gravimetric control of active volcanic processes

    NASA Astrophysics Data System (ADS)

    Saltogianni, Vasso; Stiros, Stathis

    2017-04-01

    Volcanic activity includes phases of magma chamber inflation and deflation, produced by movement of magma and/or hydrothermal processes. Such effects usually leave their imprint as deformation of the ground surfaces which can be recorded by GNSS and other methods, on one hand, and on the other hand they can be modeled as elastic deformation processes, with deformation produced by volcanic masses of finite dimensions such as spheres, ellipsoids and parallelograms. Such volumes are modeled on the basis of inversion (non-linear, numerical solution) of systems of equations relating the unknown dimensions and location of magma sources with observations, currently mostly GNSS and INSAR data. Inversion techniques depend on the misfit between model predictions and observations, but because systems of equations are highly non-linear, and because adopted models for the geometry of magma sources is simple, non-unique solutions can be derived, constrained by local extrema. Assessment of derived magma models can be provided by independent observations and models, such as micro-seismicity distribution and changes in geophysical parameters. In the simplest case magmatic intrusions can be modeled as spheres with diameters of at least a few tens of meters at a depth of a few kilometers; hence they are expected to have a gravimetric signature in permanent recording stations on the ground surface, while larger intrusions may also have an imprint in sensors in orbit around the earth or along precisely defined air paths. Identification of such gravimetric signals and separation of the "true" signal from the measurement and ambient noise requires fine forward modeling of the wider areas based on realistic simulation of the ambient gravimetric field, and then modeling of its possible distortion because of magmatic anomalies. Such results are useful to remove ambiguities in inverse modeling of ground deformation, and also to detect magmatic anomalies offshore.

  1. Hydrothermal Petroleum in Active Continental Rift: Lake Chapala, Western Mexico, Initial Results.

    NASA Astrophysics Data System (ADS)

    Zarate-del Valle, P. F.; Simoneit, B. R.; Ramirez-Sanchez, H. U.

    2003-12-01

    Lake Chapala in western Mexico is located partially in the Citala Rift, which belongs to the well-known neotectonic Jalisco continental triple junction. The region is characterized by active volcanism (Ceboruco, Volcan de Fuego), tectonic (1995 earthquake, M=8, 40-50 mm to SW) and hydrothermal (San Juan Cosala & Villa Corona spas and La Calera sinter deposit) activities. Hydrothermal petroleum has been described in active continental rift (East African Rift) and marine spreading zones (Guaymas Basin, Gulf of California). In 1868 the Mexican local press reported that manifestations of bitumen were appearing in front of the Columba Cap on the mid south shore of Lake Chapala. This bitumen is linked to the lake bottom and when the water level decreases sufficiently it is possible to access these tar bodies as islands. Because of these manifestations the Mexican oil company (PEMEX) drilled an exploration well (2,348m) at Tizapan El Alto without success. Hydrothermal activity is evident in the tar island zone as three in-shore thermal springs (26.8 m depth, 48.5° C, pH 7.8 and oriented N-S). The preliminary analyses by GC-MS of the tar from these islands indicate hydrothermal petroleum derived from lake sedimentary organic matter, generated at low temperatures (150° -200° C). The tars contain no n-alkanes, no PAH or other aromatics, but a major UCM of branched and cyclic hydrocarbons and mature biomarkers derived from lacustrine biota. The biomarkers consist of mainly 17α (H),21β (H)-hopanes ranging from C27 to C34 (no C28), gammacerane, tricyclic terpanes (C20-C26), carotane and its cracking products, and drimanes (C14-C16). The biomarker composition indicates an organic matter source from bacteria and algae, typical of lacustrine ecosystems. 14C dating of samples from two tar islands yielded ages exceeding 40 kyrs, i.e., old carbon from hydrothermal/tectonic remobilization of bitumen from deeper horizons to the surface. The occurrence of hydrothermal petroleum in

  2. Igneous activity and related ore deposits in the western and southern Tushar Mountains, Marysvale volcanic field, west-central Utah

    USGS Publications Warehouse

    Steven, Thomas A.

    1984-01-01

    PART A: Igneous activity in the Marysvale volcanic field of western Utah can be separated into many episodes of extrusion, intrusion, and hydrothermal activity. The rocks of the western Tushar Mountains, near the western part of the volcanic field, include intermediate-composition, calc-alkalic volcanic rocks erupted from scattered volcanoes in Oligocene through earliest Miocene time and related monzonitic intrusions emplaced 24-23 m.y. ago. Beginning 22-21 m.y. ago and extending through much of the later Cenozoic, a bimodal basalt-rhyolite assemblage was erupted widely throughout the volcanic field. Only volcanic and intrusive rocks belonging to the rhyolitic end member of this bimodal assemblage are present in the western Tushar Mountains; most of these rocks either fill the Mount Belknap caldera (19 m.y. old) or are part of the rhyolite of Gillies Hill (9---8 m.y. old). Episodic hydrothermal activity altered and mineralized rocks at many places in the western Tushar Mountains during Miocene time. The earliest activity took place in and adjacent to monzonitic calcalkalic intrusions emplaced in the vicinity of Indian Creek and Cork Ridge. These rocks were widely propylitized, and gold-bearing quartz-pyrite-carbonate veins formed in local fractures. Hydrothermal activity associated with the Mount Belknap caldera mobilized and redeposited uranium contained in the caldera-fill rocks and formed primary concentrations of lithophile elements (including molybdenum and uranium) in the vicinity of intrusive bodies. Hydrothermal activity associated with the rhyolite of Gillies Hill altered and mineralized rocks at several places along the fault zone that marks the western margin of the Tushar Mountains; the zoned alunite and gold deposits at Sheep Rock, the gold deposit at the Sunday Mine, and an alunite deposit near Indian Creek were thus produced. Resetting of isotopic ages suggests that another center of hydrothermally altered rocks associated with a buried pluton about

  3. Heat flow evidence for hydrothermal circulation in the volcanic basement of subducting plates

    NASA Astrophysics Data System (ADS)

    Harris, R. N.; Spinelli, G. A.; Fisher, A. T.

    2017-12-01

    We summarize and interpret evidence for hydrothermal circulation in subducting oceanic basement from the Nankai, Costa Rica, south central Chile, Haida Gwaii, and Cascadia margins and explore the influence of hydrothermal circulation on plate boundary temperatures in these settings. Heat flow evidence for hydrothermal circulation in the volcanic basement of incoming plates includes: (a) values that are well below conductive (lithospheric) predictions due to advective heat loss, and (b) variability about conductive predictions that cannot be explained by variations in seafloor relief or thermal conductivity. We construct thermal models of these systems that include an aquifer in the upper oceanic crust that enhances heat transport via a high Nusselt number proxy for hydrothermal circulation. At the subduction zones examined, patterns of seafloor heat flow are not well fit by purely conductive simulations, and are better explained by simulations that include the influence of hydrothermal circulation. This result is consistent with the young basement ages (8-35 Ma) of the incoming igneous crust at these sites as well as results from global heat flow analyses showing a significant conductive heat flow deficit for crustal ages less than 65 Ma. Hydrothermal circulation within subducting oceanic basement can have a profound influence on temperatures close to the plate boundary and, in general, leads to plate boundary temperatures that are cooler than those where fluid flow does not occur. The magnitude of cooling depends on the permeability structure of the incoming plate and the evolution of permeability with depth and time. Resolving complex relationships between subduction processes, the permeability structure in the ocean crust, and the dynamics of hydrothermal circulation remains an interdisciplinary frontier.

  4. Hydrothermal alteration of felsic volcanic rocks at the Helen Siderite Deposit, Wawa, Ontario

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Morton, R.L.; Nebel, M.L.

    1984-09-01

    Felsic lavas and pyroclastic rocks, underlying the Archean Helen iron-formation, have been variably altered by hydrothermal solutions which, when discharged onto the sea floor, formed the Helen siderite deposit. Within the footwall volcanic sequence five chemically and mineralogically distinct alteration types have been defined: least altered, sericite, chlorite chloritoid, and ankerite. Based on mineralogy and chemistry of the altered rocks and on the geometry of the alteration zones, an alteration model is proposed.

  5. Structural features related to the volcanic gases in Southern Okinawa Trough

    NASA Astrophysics Data System (ADS)

    Wang, H. F.; Hsu, S. K.; Tsia, C. H.; Chen, S. C.; Wu, M. F.

    2016-12-01

    The Okinawa Trough is a rifted back-arc basin, heavily sedimented and formed in an intracontinental rift zone behind the Ryukyu trench-arc system. The Southern Okinawa Trough (SOT) east of Taiwan is the place where post-collisional extension happened. The collision moved southwestward and the Ryukyu trench-arc extension westward, Arc volcanism is dominant in the Northern Ryukyu volcanic arc and back-arc volcanism in the Southern Okinawa Trough. Marine geophysical data including side-scan sonar (SSS), sub-bottom profiler (SBP) and echo sounder system (EK60) data are used in this study. Active fluid activities out of seafloor are obvious from various images observed on these data, such as gas plumes. These hydrothermal vents have been located at a water depth of 1400 m. Our preliminary results show that gas seepage structures appear in the location where is a week zone, such as a normal fault in the slope. The hydrothermal activity within the Okinawa Trough is associated with volcanism located in rift zones in the Southern Okinawa Trough. However, the origin of the submarine hydrothermal fluids within the Okinawa Trough is diverse with contributions from volcanic, sedimentary and magmatic sources, needed further investigations.

  6. The geochemistry of fluids from an active shallow submarine hydrothermal system: Milos island, Hellenic Volcanic Arc

    NASA Astrophysics Data System (ADS)

    Valsami-Jones, E.; Baltatzis, E.; Bailey, E. H.; Boyce, A. J.; Alexander, J. L.; Magganas, A.; Anderson, L.; Waldron, S.; Ragnarsdottir, K. V.

    2005-10-01

    Geothermal activity in the Aegean island of Milos (Greece), associated with island-arc volcanism, is abundant both on-and off-shore. Hydrothermal fluids venting from several sites, mainly shallow submarine (up to 10 m), but also just above seawater level in one locality, were sampled over four summer field seasons. Some of the discharging fluids are associated with the formation of hydrothermal edifices. Overall, the main characteristics of the hydrothermal fluids are low pH and variable chlorinity. The lowest recorded pH was 1.7, and chlorinity ranged from 0.1 to 2.5 times that of seawater. The highest fluid temperatures recorded on site were 115 °C. Two main types of fluids were identified: low-chlorinity fluids containing low concentrations of alkalis (potassium, lithium, sodium) and calcium, and high concentrations of silica and sulphate; and high-chlorinity fluids containing high concentrations of alkalis and calcium, and lower concentrations of silica and sulphate. The type locality of the high-chlorinity fluids is shallow submarine in Palaeochori, near the east end of the south coast of the island, whereas the type locality of the low-chlorinity fluids is a cave to the west of Palaeochori. The two fluid types are therefore often referred to as "submarine" and "cave" fluids respectively. Both fluid types had low magnesium and high metal concentrations but were otherwise consistently different from each other. The low-chlorinity fluids had the highest cobalt, nickel, aluminium, iron and chromium (up to 1.6 μM, 3.6 μM, 1586 μM, 936 μM and 3.0 μM, respectively) and the high-chlorinity fluids had the highest zinc, cadmium, manganese and lead (up to 4.1 μM, 1.0 μM, 230 μM and 32 μM, respectively). Geochemical modelling suggests that metals in the former are likely to have been transported as sulphate species or free ions and in the latter as chloride species or free ions. Isotopic values for both water types range between δD -12 to 33‰ and δ 18O 1

  7. The role of magmas in the formation of hydrothermal ore deposits

    USGS Publications Warehouse

    Hedenquist, Jeffrey W.; Lowenstern, Jacob B.

    1994-01-01

    Magmatic fluids, both vapour and hypersaline liquid, are a primary source of many components in hydrothermal ore deposits formed in volcanic arcs. These components, including metals and their ligands, become concentrated in magmas in various ways from various sources, including subducted oceanic crust. Leaching of rocks also contributes components to the hydrothermal fluid—a process enhanced where acid magmatic vapours are absorbed by deeply circulating meteoric waters. Advances in understanding the hydrothermal systems that formed these ore deposits have come from the study of their active equivalents, represented at the surface by hot springs and volcanic fumaroles.

  8. Stable isotope geochemistry of fumaroles: an insight into volcanic surveillance

    NASA Astrophysics Data System (ADS)

    Panichi, C.; La Ruffa, G.

    2001-12-01

    In active volcanic environments magmatic water may accumulate in the volcanic-hosted geothermal systems, or, more rarely may reach the surface along deep fractures inside the volcano crater. Knowledge of magmatic contribution to emerging fluids in volcanic active areas is critical to understanding the chemical evolution of the magma, the conditions in which it exists in the crust, and the mechanisms by which it erupts in the crust. The source of volatiles (especially water) is also of interest when eruptions are driven by the expansion of hydrothermal fluids against atmospheric pressure, without the involvement of fresh magma ('hydrothermal' or 'phreatomagmatic' eruptions). In both cases the occurrence of volcanic and/or phreatic activities is likely to be preceded by substantial isotopic and chemical changes in the crater fumarolic systems. H and O isotopic composition of condensed water from crater fumaroles appear to be able to give strong evidence for the existence of magmatic waters in the high-temperature manifestations of the volcanic systems. Isotopic data and specific hydrological models from seven different volcanic systems (Galeras Volcano, Colombia, Kilauea Volcano, Hawaii, Kudryvy Volcano, Kuril volcanic arc, Mt St Helens, USA; Guagua Pichincha, Ecuador; Vulcano island, Italy; the Aegean Volcanic Arc, Greece) are discussed in order to highlight the possibility to use those isotopic parameters in the assessment of the environmental risks of an active volcanic area.

  9. Relation of compositions of deep fluids in geothermal activity of Pleistocene-Holocene volcanic fields of Lesser Caucasus

    NASA Astrophysics Data System (ADS)

    Meliksetian, Khachatur; Lavrushin, Vassily; Shahinyan, Hrach; Aidarkozhina, Altin; Navasardyan, Gevorg; Ermakov, Alexander; Zakaryan, Shushan; Prasolov, Edward; Manucharyan, Davit; Gyulnazaryan, Shushan; Grigoryan, Edmond

    2017-04-01

    It is widely accepted, that geothermal activity in the conductive heat flow processes, such as volcanism and hydrothermal activity, is manifestation of the thermal mass transfer process in the Earth's crust, where geothermal and geochemical processes are closely connected. Therefore, geochemistry and isotope compositions of thermal mineral waters within and on periphery of volcanic clusters may represent key indicators for better understanding of geothermal activity in geodynamically active zones. Geochemical features of heat and mass transport in hydrothermal systems related to active volcanic and fault systems in continental collision related orogenic elevated plateaus such as Anatolian-Armenian-Iranian highlands are still poorly understood. In this contribution we attempt to fill these gaps in our knowledge of relations of geochemical and geothermal processes in collision zones. We present new data on chemical compositions, trace element geochemistry of thermal waters of Lesser Caucasus, (Armenia) as well as isotope analysis of free gases such as {}3He/{}4He, {}40Ar/{}36Ar, δ{}13?(CO{}2), nitrogen δ{}15N(N{}2) and oxygen and hydrogen isotopes in water phases (δD, δ{}18O). To reveal some specific features of formation of fluid systems related to thermal activity in the areas of collision related active volcanism and active geodynamics a complex geochemical (SiO{}2, K-Na, Na-Li, Li-Mg) and isotope geothermometers (δ{}18O(CaCO{}3) - δ{}18O(H{}2O)) were applied. The distribution of δ{}13?(??{}2) values in free gases of mineral waters of Armenia demonstrates that gases related to Quaternary volcanic fields are characterized by relatively light δ{}13?(CO{}2) values close to mantle derived gases, while on periphery of volcanic systems relatively heavy values of δ{}13?(CO{}2) indicate strong influence of metamorphic and sedimentary derived carbon dioxide. Distribution of nitrogen isotopes δ{}15N(N{}2) demonstrate an inverse correlation with δ{}13?(CO{}2

  10. Hydrothermal and tectonic activity in northern Yellowstone Lake, Wyoming

    USGS Publications Warehouse

    Johnson, S.Y.; Stephenson, W.J.; Morgan, L.A.; Shanks, Wayne C.; Pierce, K.L.

    2003-01-01

    Yellowstone National Park is the site of one of the world's largest calderas. The abundance of geothermal and tectonic activity in and around the caldera, including historic uplift and subsidence, makes it necessary to understand active geologic processes and their associated hazards. To that end, we here use an extensive grid of high-resolution seismic reflection profiles (???450 km) to document hydrothermal and tectonic features and deposits in northern Yellowstone Lake. Sublacustrine geothermal features in northern Yellowstone Lake include two of the largest known hydrothermal explosion craters, Mary Bay and Elliott's. Mary Bay explosion breccia is distributed uniformly around the crater, whereas Elliott's crater breccia has an asymmetric distribution and forms a distinctive, ???2-km-long, hummocky lobe on the lake floor. Hydrothermal vents and low-relief domes are abundant on the lake floor; their greatest abundance is in and near explosion craters and along linear fissures. Domed areas on the lake floor that are relatively unbreached (by vents) are considered the most likely sites of future large hydrothermal explosions. Four submerged shoreline terraces along the margins of northern Yellowstone Lake add to the Holocene record or postglacial lake-level fluctuations attributed to "heavy breathing" of the Yellowstone magma reservoir and associated geothermal system. The Lake Hotel fault cuts through northwestern Yellowstone Lake and represents part of a 25-km-long distributed extensional deformation zone. Three postglacial ruptures indicate a slip rate of ???0.27 to 0.34 mm/yr. The largest (3.0 m slip) and most recent event occurred in the past ???2100 yr. Although high heat flow in the crust limits the rupture area of this fault zone, future earthquakes of magnitude ???5.3 to 6.5 are possible. Earthquakes and hydrothermal explosions have probably triggered landslides, common features around the lake margins. Few high-resolution seismic reflection surveys have

  11. Carbon dioxide diffuse emission and thermal energy release from hydrothermal systems at Copahue-Caviahue Volcanic Complex (Argentina)

    NASA Astrophysics Data System (ADS)

    Chiodini, Giovanni; Cardellini, Carlo; Lamberti, María Clara; Agusto, Mariano; Caselli, Alberto; Liccioli, Caterina; Tamburello, Giancarlo; Tassi, Franco; Vaselli, Orlando; Caliro, Stefano

    2015-10-01

    The north-western sector of Caviahue caldera (Argentina), close to the active volcanic system of Copahue, is characterized by the presence of several hydrothermal sites that host numerous fumarolic emissions, anomalous soil diffuse degassing of CO2 and hot soils. In March 2014, measurements of soil CO2 fluxes in 5 of these sites (namely, Las Máquinas, Las Maquinitas I, Las Maquinitas II, Anfiteatro, and Termas de Copahue) allowed an estimation that 165 t of deeply derived CO2 is daily released. The gas source is likely related to a relatively shallow geothermal reservoir containing a single vapor phase as also suggested by both the geochemical data from the 3 deep wells drilled in the 1980s and gas geoindicators applied to the fumarolic discharges. Gas equilibria within the H-C-O gas system indicate the presence of a large, probably unique, single phase vapor zone at 200-210 °C feeding the hydrothermal manifestations of Las Máquinas, Las Maquinitas I and II and Termas de Copahue. A natural thermal release of 107 MW was computed by using CO2 as a tracer of the original vapor phase. The magmatic signature of the incondensable fumarolic gases, the wide expanse of the hydrothermal areas and the remarkable high amount of gas and heat released by fluid expulsion seem to be compatible with an active magmatic intrusion beneath this portion of the Caviahue caldera.

  12. The hydrothermal system of the Domuyo volcanic complex (Argentina): A conceptual model based on new geochemical and isotopic evidences

    NASA Astrophysics Data System (ADS)

    Tassi, F.; Liccioli, C.; Agusto, M.; Chiodini, G.; Vaselli, O.; Calabrese, S.; Pecoraino, G.; Tempesti, L.; Caponi, C.; Fiebig, J.; Caliro, S.; Caselli, A.

    2016-12-01

    The Domuyo volcanic complex (Neuquén Province, Argentina) hosts one of the most promising geothermal systems of Patagonia, giving rise to thermal manifestations discharging hot and Cl--rich fluids. This study reports a complete geochemical dataset of gas and water samples collected in three years (2013, 2014 and 2015) from the main fluid discharges of this area. The chemical and isotopic composition (δD-H2O and δ18O-H2O) of waters indicates that rainwater and snow melting are the primary recharge of a hydrothermal reservoir located at relative shallow depth (400-600 m) possibly connected to a second deeper (2-3 km) reservoir. Reactive magmatic gases are completely scrubbed by the hydrothermal aquifer(s), whereas interaction of meteoric waters at the surface causes a significant air contamination and dilution of the fluid discharges located along the creeks at the foothill of the Cerro Domuyo edifice. Thermal discharges located at relatively high altitude ( 3150 m a.s.l.), namely Bramadora, are less affected by this process, as also shown by their relatively high R/Ra values (up to 6.91) pointing to the occurrence of an actively degassing magma batch located at an unknown depth. Gas and solute geothermometry suggests equilibrium temperatures up to 220-240 °C likely referred to the shallower hydrothermal reservoir. These results, confirming the promising indications of the preliminary surveys carried out in the 1980‧s, provide useful information for a reliable estimation of the geothermal potential of this extinct volcanic system, although a detailed geophysical measurements is required for the correct estimation of depth and dimensions of the fluid reservoir(s).

  13. Hydrothermal mineralization at seafloor spreading centers

    NASA Astrophysics Data System (ADS)

    Rona, Peter A.

    1984-01-01

    The recent recognition that metallic mineral deposits are concentrated by hydrothermal processes at seafloor spreading centers constitutes a scientific breakthrough that opens active sites at seafloor spreading centers as natural laboratories to investigate ore-forming processes of such economically useful deposits as massive sulfides in volcanogenic rocks on land, and that enhances the metallic mineral potential of oceanic crust covering two-thirds of the Earth both beneath ocean basins and exposed on land in ophiolite belts. This paper reviews our knowledge of processes of hydrothermal mineralization and the occurrence and distribution of hydrothermal mineral deposits at the global oceanic ridge-rift system. Sub-seafloor hydrothermal convection involving circulation of seawater through fractured rocks of oceanic crust driven by heat supplied by generation of new lithosphere is nearly ubiquitous at seafloor spreading centers. However, ore-forming hydrothermal systems are extremely localized where conditions of anomalously high thermal gradients and permeability increase hydrothermal activity from the ubiquitous low-intensity background level (⩽ 200°C) to high-intensity characterized by high temperatures ( > 200-c.400°C), and a rate and volume of flow sufficient to sustain chemical reactions that produce acid, reducing, metal-rich primary hydrothermal solutions. A series of mineral phases with sulfides and oxides as high- and low-temperature end members, respectively, are precipitated along the upwelling limb and in the discharge zone of single-phase systems as a function of increasing admixture of normal seawater. The occurrence of hydrothermal mineral deposits is considered in terms of spatial and temporal frames of reference. Spatial frames of reference comprise structural features along-axis (linear sections that are the loci of seafloor spreading alternating with transform faults) and perpendicular to axis (axial zone of volcanic extrusion and marginal

  14. Mainshock-Aftershocks Clustering Detection in Volcanic Regions

    NASA Astrophysics Data System (ADS)

    Garza Giron, R.; Brodsky, E. E.; Prejean, S. G.

    2017-12-01

    Crustal earthquakes tend to break their general Poissonean process behavior by gathering into two main kinds of seismic bursts: swarms and mainshock-aftershocks sequences. The former is commonly related to volcanic or geothermal processes whereas the latter is a characteristic feature of tectonically driven seismicity. We explore the mainshock-aftershock clustering behavior of different active volcanic regions in Japan and its comparison to non-volcanic regions. We find that aftershock production in volcanoes shows mainshock-aftershocks clustering similar to what is observed in non-volcanic areas. The ratio of volanic areas that cluster in mainshock-aftershocks sequences vs the areas that do not is comparable to the ratio of non-volcanic regions that show clustering vs the ones that do not. Furthermore, the level of production of aftershocks for most volcanic areas where clustering is present seems to be of the same order of magnitude, or slightly higher, as the median of the non-volcanic regions. An interesting example of highly aftershock-productive volcanoes emerges from the 2000 Miyakejima dike intrusion. A big seismic cluster started to build up rapidly in the south-west flank of Miyakejima to later propagate to the north-west towards the Kozushima and Niijima volcanoes. In Miyakejima the seismicity showed a swarm-like signature with a constant earthquake rate, whereas Kozushima and Niijima both had expressions of highly productive mainshock-aftershocks sequences. These findings are surprising given the alternative mechanisms available in volcanic systems for releasing deviatoric strain. We speculate that aftershock behavior might hold a relationship with the rheological properties of the rocks of each system and with the capacity of a system to accumulate or release the internal pressures caused by magmatic or hydrothermal systems.

  15. Drilling of Submarine Shallow-water Hydrothermal Systems in Volcanic Arcs of the Tyrrhenian Sea, Italy

    NASA Astrophysics Data System (ADS)

    Petersen, S.; Augustin, N.; de Benedetti, A.; Esposito, A.; Gaertner, A.; Gemmell, B.; Gibson, H.; He, G.; Huegler, M.; Kleeberg, R.; Kuever, J.; Kummer, N. A.; Lackschewitz, K.; Lappe, F.; Monecke, T.; Perrin, K.; Peters, M.; Sharpe, R.; Simpson, K.; Smith, D.; Wan, B.

    2007-12-01

    Seafloor hydrothermal systems related to volcanic arcs are known from several localities in the Tyrrhenian Sea in water depths ranging from 650 m (Palinuro Seamount) to less than 50 m (Panarea). At Palinuro Seamount 13 holes (<5m) were drilled using Rockdrill 1 of the British Geological Survey 1 into the heavily sediment-covered deposit recovering 11 m of semi-massive to massive sulfides. Maximum recovery within a single core was 4.8 m of massive sulfides/sulfates with abundant late native sulfur overprint. The deposit is open to all sides and to depth since all drill holes ended in mineralization. Metal enrichment at the top of the deposit is evident in some cores with polymetallic (Zn, Pb, Ag) sulfides overlying more massive and dense pyritic ore. The massive sulfide mineralization at Palinuro Seamount contains a number of unusual minerals, including enargite, tennantite, luzonite, and Ag-sulfosalts, that are not commonly encountered in mid-ocean ridge massive sulfides. In analogy to epithermal deposits forming on land, the occurrence of these minerals suggests a high sulfidation state of the hydrothermal fluids during deposition implying that the mineralizing fluids were acidic and oxidizing rather than near-neutral and reducing as those forming typical base metal rich massive sulfides along mid-ocean ridges. Oxidizing conditions during sulfide deposition can probably be related to the presence of magmatic volatiles in the mineralizing fluids that may be derived from a degassing magma chamber. Elevated temperatures within sediment cores and TV-grab stations (up to 60°C) indicate present day hydrothermal fluid flow. This is also indicated by the presence of small tube-worm bushes present on top the sediment. A number of drill holes were placed around the known phreatic gas-rich vents of Panarea and recovered intense clay-alteration in some holes as well as abundant massive anhydrite/gypsum with only trace sulfides along a structural depression suggesting the

  16. Gas geochemistry of the magmatic-hydrothermal fluid reservoir in the Copahue-Caviahue Volcanic Complex (Argentina)

    NASA Astrophysics Data System (ADS)

    Agusto, M.; Tassi, F.; Caselli, A. T.; Vaselli, O.; Rouwet, D.; Capaccioni, B.; Caliro, S.; Chiodini, G.; Darrah, T.

    2013-05-01

    Copahue volcano is part of the Caviahue-Copahue Volcanic Complex (CCVC), which is located in the southwestern sector of the Caviahue volcano-tectonic depression (Argentina-Chile). This depression is a pull-apart basin accommodating stresses between the southern Liquiñe-Ofqui strike slip and the northern Copahue-Antiñir compressive fault systems, in a back-arc setting with respect to the Southern Andean Volcanic Zone. In this study, we present chemical (inorganic and organic) and isotope compositions (δ13C-CO2, δ15N, 3He/4He, 40Ar/36Ar, δ13C-CH4, δD-CH4, and δD-H2O and δ18O-H2O) of fumaroles and bubbling gases of thermal springs located at the foot of Copahue volcano sampled in 2006, 2007 and 2012. Helium isotope ratios, the highest observed for a Southern American volcano (R/Ra up to 7.94), indicate a non-classic arc-like setting, but rather an extensional regime subdued to asthenospheric thinning. δ13C-CO2 values (from - 8.8‰ to - 6.8‰ vs. V-PDB), δ15N values (+ 5.3‰ to + 5.5‰ vs. Air) and CO2/3He ratios (from 1.4 to 8.8 × 109) suggest that the magmatic source is significantly affected by contamination of subducted sediments. Gases discharged from the northern sector of the CCVC show contribution of 3He-poor fluids likely permeating through local fault systems. Despite the clear mantle isotope signature in the CCVC gases, the acidic gas species have suffered scrubbing processes by a hydrothermal system mainly recharged by meteoric water. Gas geothermometry in the H2O-CO2-CH4-CO-H2 system suggests that CO and H2 re-equilibrate in a separated vapor phase at 200°-220 °C. On the contrary, rock-fluid interactions controlling CO2, CH4 production from Sabatier reaction and C3H8 dehydrogenation seem to occur within the hydrothermal reservoir at temperatures ranging from 250° to 300 °C. Fumarole gases sampled in 2006-2007 show relatively low N2/He and N2/Ar ratios and high R/Ra values with respect to those measured in 2012. Such compositional and

  17. Development of a mixed seawater-hydrothermal fluid geochemical signature during alteration of volcanic rocks in the Archean (∼2.7 Ga) Abitibi Greenstone Belt, Canada

    NASA Astrophysics Data System (ADS)

    Brengman, Latisha A.; Fedo, Christopher M.

    2018-04-01

    We investigated a group of silicified volcanic rocks from the ∼2.72 Ga Hunter Mine Group (HMG), Abitibi Greenstone Belt, Canada, in order to document progressive compositional change associated with alteration in a subaqueous caldera system. Rocks of the HMG divide into three groups based on mineralogy and texture for petrographic and geochemical analyses. Volcanic features (phenocrysts, pseudomorphs after primary glass shards, lapilli, volcanic clasts) are preserved in all groups, despite changing mineralogy from primarily quartz, feldspar, chlorite (Groups 1 and 2), to quartz, hematite and carbonate (Groups 2 and 3). Compositionally, Group 1 rocks resemble volcanic rocks in the region, while Group 2 and 3 rocks show a change in mineralogy to iron, silica, and carbonate minerals, which is associated with depletion of many major and trace elements associated with volcanic rocks (Al2O3, Na2O, K2O, Zr). In addition, rare earth elements display a clear progression from volcanic signatures in Group 1 (PrSN/YbSN = 1.7-2.96, EuSN/EuSN∗ = 0.84-1.72, Y/Ho = 25.20-27.41, LaSN/LaSN∗ = 0.97-1.29, and Zr/Hf = 38.38-42.09) to transitional mixed volcanic, hydrothermal, and seawater signatures in Group 2 (PrSN/YbSN 1.33-2.89, EuSN/EuSN∗ 1.33-2.5, Y/Ho = 23.94-30, LaSN/LaSN∗ 0.93-1.34, and Zr/Hf = 40-70), to mixed hydrothermal and seawater signatures in Group 3 (PrSN/YbSN 0.62-2.88, EuSN/EuSN∗ 1.30-7.15, LaSN/LaSN∗ 1.02-1.86, Y/Ho = 25.56-55, and Zr/Hf = 35-50). We interpret that silicification of volcanic rocks (Group 1) produced transitional altered volcanic rocks (Group 2), and siliceous and jaspilitic rocks (Group 3), based on preservation of delicate volcanic features. Building on this explanation, we interpret that major, trace- and rare-earth element mobility occurred during the process of silicification, during which siliceous and jaspilitic rocks (Group 3) acquired aspects of the rare-earth element geochemical signatures of marine chemical precipitates. We

  18. Stratigraphic development and hydrothermal activity in the central western Cascade Range, Oregon

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Cummings, M.L.; Bull, M.K.; Pollock, J.M.

    1990-11-10

    Two volcanic sequences bounded by erosional unconformities compose the stratigraphy of the North Santiam mining district, Western Cascade Range, Oregon. Diorite, grandodiorite, and leucocratic quartz porphyry dikes, stocks, and sills intrude the breccias, flows, and tuffs of a volcanic center in the older Sardine Formation. Tourmaline-bearing breccia pipes are associated with the porphyritic granodiorite intrusions. An erosional unconformity separates the Sardine Formation from the overlying Elk Lake formation. The alteration patterns in the two formations are consistent with the development of hydrothermal systems during the eruption of each formation. However, the development of the two hydrothermal systems is separated bymore » a period of erosion of the older volcanic pile. Early formation of mineralization that resembles porphyry copper deposits occurred within the Sardine Formation, and later, after eruption of the Elk Lake formation, epithermal veins and alteration developed along faults, fractures, and the margins of dikes in the Sardine Formation.« less

  19. Biogeochemistry of hydrothermally and adjacent non-altered soils

    USDA-ARS?s Scientific Manuscript database

    As a field/lab project, students in the Soil Biogeochemistry class of the University of Nevada, Reno described and characterized seven pedons, developed in hydrothermally and adjacent non-hydrothermally altered andesitic parent material near Reno, NV. Hydrothermally altered soils had considerably lo...

  20. A large hydrothermal reservoir beneath Taal Volcano (Philippines) revealed by magnetotelluric observations and its implications to the volcanic activity.

    PubMed

    Alanis, Paul K B; Yamaya, Yusuke; Takeuchi, Akihiro; Sasai, Yoichi; Okada, Yoshihiro; Nagao, Toshiyasu

    2013-01-01

    Taal Volcano is one of the most active volcanoes in the Philippines. The magnetotelluric 3D forward analyses indicate the existence of a large high resistivity anomaly (∼100 Ω·m) with a volume of at least 3 km×3 km×3 km, which is capped by a conductive layer (∼10 Ω·m), beneath the Main Crater. This high resistivity anomaly is hypothesized to be a large hydrothermal reservoir, consisting of the aggregate of interconnected cracks in rigid and dense host rocks, which are filled with hydrothermal fluids coming from a magma batch below the reservoir. The hydrothermal fluids are considered partly in gas phase and liquid phase. The presence of such a large hydrothermal reservoir and the stagnant magma below may have influences on the volcano's activity. Two possibilities are presented. First, the 30 January 1911 explosion event was a magmatic hydrothermal eruption rather than a base-surge associated with a phreato-magmatic eruption. Second, the earlier proposed four eruption series may be better interpreted by two cycles, each consisting of series of summit and flank eruptions.

  1. Meteorite organics in planetary environments: hydrothermal release, surface activity, and microbial utilization

    NASA Technical Reports Server (NTRS)

    Mautner, M. N.; Leonard, R. L.; Deamer, D. W.

    1995-01-01

    Up to 50% of the organics in the Murchison meteorite, possibly including some of the polymer, is released in high temperature and pressure aqueous environments, to 350 degrees C and 250 bar, that simulate submarine volcanic, hydrothermal or impact-induced conditions. Meteorite organics of prebiotic significance, such as nonanoic acid, glycine, and pyrene survive the hydrothermal conditions. The released material is surface active with surface pressures up to 19.8 x 10(-3) N m-1, and exhibits an extended surface tension isotherm which suggests a mixture of amphiphilic components. One component, nonanoic acid, is shown to form vesicles. The materials extracted under mild conditions, at 120 degrees C, are nutrients for the humic acid bacterium Pseudomonas maltophilia and efficient nutrients for the oligotroph Flavobacterium oryzihabitans, demonstrating the capability of microorganisms to metabolize extraterrestrial organics.

  2. An authoritative global database for active submarine hydrothermal vent fields

    NASA Astrophysics Data System (ADS)

    Beaulieu, Stace E.; Baker, Edward T.; German, Christopher R.; Maffei, Andrew

    2013-11-01

    The InterRidge Vents Database is available online as the authoritative reference for locations of active submarine hydrothermal vent fields. Here we describe the revision of the database to an open source content management system and conduct a meta-analysis of the global distribution of known active vent fields. The number of known active vent fields has almost doubled in the past decade (521 as of year 2009), with about half visually confirmed and others inferred active from physical and chemical clues. Although previously known mainly from mid-ocean ridges (MORs), active vent fields at MORs now comprise only half of the total known, with about a quarter each now known at volcanic arcs and back-arc spreading centers. Discoveries in arc and back-arc settings resulted in an increase in known vent fields within exclusive economic zones, consequently reducing the proportion known in high seas to one third. The increase in known vent fields reflects a number of factors, including increased national and commercial interests in seafloor hydrothermal deposits as mineral resources. The purpose of the database now extends beyond academic research and education and into marine policy and management, with at least 18% of known vent fields in areas granted or pending applications for mineral prospecting and 8% in marine protected areas.

  3. Fungal colonization of an Ordovician impact-induced hydrothermal system

    PubMed Central

    Ivarsson, Magnus; Broman, Curt; Sturkell, Erik; Ormö, Jens; Siljeström, Sandra; van Zuilen, Mark; Bengtson, Stefan

    2013-01-01

    Impacts are common geologic features on the terrestrial planets throughout the solar system, and on at least Earth and Mars impacts have induced hydrothermal convection. Impact-generated hydrothermal systems have been suggested to possess the same life supporting capability as hydrothermal systems associated with volcanic activity. However, evidence of fossil microbial colonization in impact-generated hydrothermal systems is scarce in the literature. Here we report of fossilized microorganisms in association with cavity-grown hydrothermal minerals from the 458 Ma Lockne impact structure, Sweden. Based on morphological characteristics the fossilized microorganisms are interpreted as fungi. We further infer the kerogenization of the microfossils, and thus the life span of the fungi, to be contemporaneous with the hydrothermal activity and migration of hydrocarbons in the system. Our results from the Lockne impact structure show that hydrothermal systems associated with impact structures can support colonization by microbial life. PMID:24336641

  4. Fungal colonization of an Ordovician impact-induced hydrothermal system

    NASA Astrophysics Data System (ADS)

    Ivarsson, Magnus; Broman, Curt; Sturkell, Erik; Ormö, Jens; Siljeström, Sandra; van Zuilen, Mark; Bengtson, Stefan

    2013-12-01

    Impacts are common geologic features on the terrestrial planets throughout the solar system, and on at least Earth and Mars impacts have induced hydrothermal convection. Impact-generated hydrothermal systems have been suggested to possess the same life supporting capability as hydrothermal systems associated with volcanic activity. However, evidence of fossil microbial colonization in impact-generated hydrothermal systems is scarce in the literature. Here we report of fossilized microorganisms in association with cavity-grown hydrothermal minerals from the 458 Ma Lockne impact structure, Sweden. Based on morphological characteristics the fossilized microorganisms are interpreted as fungi. We further infer the kerogenization of the microfossils, and thus the life span of the fungi, to be contemporaneous with the hydrothermal activity and migration of hydrocarbons in the system. Our results from the Lockne impact structure show that hydrothermal systems associated with impact structures can support colonization by microbial life.

  5. Fungal colonization of an Ordovician impact-induced hydrothermal system.

    PubMed

    Ivarsson, Magnus; Broman, Curt; Sturkell, Erik; Ormö, Jens; Siljeström, Sandra; van Zuilen, Mark; Bengtson, Stefan

    2013-12-16

    Impacts are common geologic features on the terrestrial planets throughout the solar system, and on at least Earth and Mars impacts have induced hydrothermal convection. Impact-generated hydrothermal systems have been suggested to possess the same life supporting capability as hydrothermal systems associated with volcanic activity. However, evidence of fossil microbial colonization in impact-generated hydrothermal systems is scarce in the literature. Here we report of fossilized microorganisms in association with cavity-grown hydrothermal minerals from the 458 Ma Lockne impact structure, Sweden. Based on morphological characteristics the fossilized microorganisms are interpreted as fungi. We further infer the kerogenization of the microfossils, and thus the life span of the fungi, to be contemporaneous with the hydrothermal activity and migration of hydrocarbons in the system. Our results from the Lockne impact structure show that hydrothermal systems associated with impact structures can support colonization by microbial life.

  6. A large hydrothermal reservoir beneath Taal Volcano (Philippines) revealed by magnetotelluric observations and its implications to the volcanic activity

    PubMed Central

    ALANIS, Paul K. B.; YAMAYA, Yusuke; TAKEUCHI, Akihiro; SASAI, Yoichi; OKADA, Yoshihiro; NAGAO, Toshiyasu

    2013-01-01

    Taal Volcano is one of the most active volcanoes in the Philippines. The magnetotelluric 3D forward analyses indicate the existence of a large high resistivity anomaly (∼100 Ω·m) with a volume of at least 3 km × 3 km × 3 km, which is capped by a conductive layer (∼10 Ω·m), beneath the Main Crater. This high resistivity anomaly is hypothesized to be a large hydrothermal reservoir, consisting of the aggregate of interconnected cracks in rigid and dense host rocks, which are filled with hydrothermal fluids coming from a magma batch below the reservoir. The hydrothermal fluids are considered partly in gas phase and liquid phase. The presence of such a large hydrothermal reservoir and the stagnant magma below may have influences on the volcano’s activity. Two possibilities are presented. First, the 30 January 1911 explosion event was a magmatic hydrothermal eruption rather than a base-surge associated with a phreato-magmatic eruption. Second, the earlier proposed four eruption series may be better interpreted by two cycles, each consisting of series of summit and flank eruptions. PMID:24126286

  7. Hydrothermal systems and volcano geochemistry

    USGS Publications Warehouse

    Fournier, R.O.

    2007-01-01

    The upward intrusion of magma from deeper to shallower levels beneath volcanoes obviously plays an important role in their surface deformation. This chapter will examine less obvious roles that hydrothermal processes might play in volcanic deformation. Emphasis will be placed on the effect that the transition from brittle to plastic behavior of rocks is likely to have on magma degassing and hydrothermal processes, and on the likely chemical variations in brine and gas compositions that occur as a result of movement of aqueous-rich fluids from plastic into brittle rock at different depths. To a great extent, the model of hydrothermal processes in sub-volcanic systems that is presented here is inferential, based in part on information obtained from deep drilling for geothermal resources, and in part on the study of ore deposits that are thought to have formed in volcanic and shallow plutonic environments.

  8. Searching for evidence of hydrothermal activity at Apollinaris Mons, Mars

    USGS Publications Warehouse

    El Maarry, M.R.; Dohm, J.M.; Marzo, G.A.; Fergason, R.; Goetz, W.; Heggy, E.; Pack, A.; Markiewicz, W.J.

    2012-01-01

    A multidisciplinary approach involving various remote sensing instruments is used to investigate Apollinaris Mons, a prominent volcano on Mars, as well as the surrounding plains for signs of prolonged hydrologic and volcanic, and possibly hydrothermal activity. The main findings include (1) evidence from laser altimetry indicating the large thickness (1.5-2. km at some locations) of the fan deposits draping the southern flank contrary to previous estimates, coupled with possible layering which point to a significant emplacement phase at Apollinaris Mons, (2) corroboration of Robinson et al. (Robinson, M.S., Mouginis-Mark, P.J., Zimbelman, J.R., Wu, S.S.C., Ablin, K.K., Howington-Kraus, A.E. [1993]. Icarus 104, 301-323) hypothesis regarding the formation of incised valleys on the western flanks by density current erosion which would indicate magma-water interaction or, alternatively, volatile-rich magmas early in the volcano's history, (3) mounds of diverse geometric shapes, many of which display summit depressions and occur among faults and fractures, possibly marking venting, (4) strong indicators on the flanks of the volcano for lahar events, and possibly, a caldera lake, (5) ubiquitous presence of impact craters displaying fluidized ejecta in both shield-forming (flank and caldera) materials and materials that surround the volcano that are indicative of water-rich target materials at the time of impact, (6) long-term complex association in time among shield-forming materials and Medusae Fossae Formation.The findings point to a site of extensive volcanic and hydrologic activity with possibly a period of magma-water interaction and hydrothermal activity. Finally, we propose that the mound structures around Apollinaris should be prime targets for further in situ exploration and search for possible exobiological signatures. ?? 2011 Elsevier Inc..

  9. Searching for evidence of hydrothermal activity at Apollinaris Mons, Mars

    USGS Publications Warehouse

    El Maarry, M. Ramy; Dohm, James M.; Marzo, Giuseppe A.; Fergason, Robin; Goetz, Walter; Heggy, Essam; Pack, Andreas; Markiewicz, Wojciech J.

    2012-01-01

    A multidisciplinary approach involving various remote sensing instruments is used to investigate Apollinaris Mons, a prominent volcano on Mars, as well as the surrounding plains for signs of prolonged hydrologic and volcanic, and possibly hydrothermal activity. The main findings include (1) evidence from laser altimetry indicating the large thickness (1.5–2 km at some locations) of the fan deposits draping the southern flank contrary to previous estimates, coupled with possible layering which point to a significant emplacement phase at Apollinaris Mons, (2) corroboration of Robinson et al. (Robinson, M.S., Mouginis-Mark, P.J., Zimbelman, J.R., Wu, S.S.C., Ablin, K.K., Howington-Kraus, A.E. [1993]. Icarus 104, 301–323) hypothesis regarding the formation of incised valleys on the western flanks by density current erosion which would indicate magma–water interaction or, alternatively, volatile-rich magmas early in the volcano’s history, (3) mounds of diverse geometric shapes, many of which display summit depressions and occur among faults and fractures, possibly marking venting, (4) strong indicators on the flanks of the volcano for lahar events, and possibly, a caldera lake, (5) ubiquitous presence of impact craters displaying fluidized ejecta in both shield-forming (flank and caldera) materials and materials that surround the volcano that are indicative of water-rich target materials at the time of impact, (6) long-term complex association in time among shield-forming materials and Medusae Fossae Formation. The findings point to a site of extensive volcanic and hydrologic activity with possibly a period of magma–water interaction and hydrothermal activity. Finally, we propose that the mound structures around Apollinaris should be prime targets for further in situ exploration and search for possible exobiological signatures.

  10. Towards understanding the puzzling lack of acid geothermal springs in Tibet (China): Insight from a comparison with Yellowstone (USA) and some active volcanic hydrothermal systems

    USGS Publications Warehouse

    Nordstrom, D. Kirk; Guo, Qinghai; McCleskey, R. Blaine

    2014-01-01

    Explanations for the lack of acid geothermal springs in Tibet are inferred from a comprehensive hydrochemical comparison of Tibetan geothermal waters with those discharged from Yellowstone (USA) and two active volcanic areas, Nevado del Ruiz (Colombia) and Miravalles (Costa Rica) where acid springs are widely distributed and diversified in terms of geochemical characteristic and origin. For the hydrothermal areas investigated in this study, there appears to be a relationship between the depths of magma chambers and the occurrence of acid, chloride-rich springs formed via direct magmatic fluid absorption. Nevado del Ruiz and Miravalles with magma at or very close to the surface (less than 1–2 km) exhibit very acidic waters containing HCl and H2SO4. In contrast, the Tibetan hydrothermal systems, represented by Yangbajain, usually have fairly deep-seated magma chambers so that the released acid fluids are much more likely to be fully neutralized during transport to the surface. The absence of steam-heated acid waters in Tibet, however, may be primarily due to the lack of a confining layer (like young impermeable lavas at Yellowstone) to separate geothermal steam from underlying neutral chloride waters and the possible scenario that the deep geothermal fluids below Tibet carry less H2S than those below Yellowstone.

  11. Towards understanding the puzzling lack of acid geothermal springs in Tibet (China): Insight from a comparison with Yellowstone (USA) and some active volcanic hydrothermal systems

    NASA Astrophysics Data System (ADS)

    Guo, Qinghai; Kirk Nordstrom, D.; Blaine McCleskey, R.

    2014-11-01

    Explanations for the lack of acid geothermal springs in Tibet are inferred from a comprehensive hydrochemical comparison of Tibetan geothermal waters with those discharged from Yellowstone (USA) and two active volcanic areas, Nevado del Ruiz (Colombia) and Miravalles (Costa Rica) where acid springs are widely distributed and diversified in terms of geochemical characteristic and origin. For the hydrothermal areas investigated in this study, there appears to be a relationship between the depths of magma chambers and the occurrence of acid, chloride-rich springs formed via direct magmatic fluid absorption. Nevado del Ruiz and Miravalles with magma at or very close to the surface (less than 1-2 km) exhibit very acidic waters containing HCl and H2SO4. In contrast, the Tibetan hydrothermal systems, represented by Yangbajain, usually have fairly deep-seated magma chambers so that the released acid fluids are much more likely to be fully neutralized during transport to the surface. The absence of steam-heated acid waters in Tibet, however, may be primarily due to the lack of a confining layer (like young impermeable lavas at Yellowstone) to separate geothermal steam from underlying neutral chloride waters and the possible scenario that the deep geothermal fluids below Tibet carry less H2S than those below Yellowstone.

  12. Hydrothermal uranium deposits containing molybdenum and fluorite in the Marysvale volcanic field, west-central Utah

    USGS Publications Warehouse

    Cunningham, C.G.; Rasmussen, J.D.; Steven, T.A.; Rye, R.O.; Rowley, P.D.; Romberger, S.B.; Selverstone, J.

    1998-01-01

    Uranium deposits containing molybdenum and fluorite occur in the Central Mining Area, near Marysvale, Utah, and formed in an epithermal vein system that is part of a volcanic/hypabyssal complex. They represent a known, but uncommon, type of deposit; relative to other commonly described volcanic-related uranium deposits, they are young, well-exposed and well-documented. Hydrothermal uranium-bearing quartz and fluorite veins are exposed over a 300 m vertical range in the mines. Molybdenum, as jordisite (amorphous MoS2, together with fluorite and pyrite, increase with depth, and uranium decreases with depth. The veins cut 23-Ma quartz monzonite, 20-Ma granite, and 19-Ma rhyolite ash-flow tuff. The veins formed at 19-18 Ma in a 1 km2 area, above a cupola of a composite, recurrent, magma chamber at least 24 ?? 5 km across that fed a sequence of 21- to 14-Ma hypabyssal granitic stocks, rhyolite lava flows, ash-flow tuffs, and volcanic domes. Formation of the Central Mining Area began when the intrusion of a rhyolite stock, and related molybdenite-bearing, uranium-rich, glassy rhyolite dikes, lifted the fractured roof above the stock. A breccia pipe formed and relieved magmatic pressures, and as blocks of the fractured roof began to settle back in place, flat-lying, concave-downward, 'pull-apart' fractures were formed. Uranium-bearing, quartz and fluorite veins were deposited by a shallow hydrothermal system in the disarticulated carapace. The veins, which filled open spaces along the high-angle fault zones and flat-lying fractures, were deposited within 115 m of the ground surface above the concealed rhyolite stock. Hydrothermal fluids with temperatures near 200??C, ??18OH2O ~ -1.5, ?? -1.5, ??DH2O ~ -130, log fO2 about -47 to -50, and pH about 6 to 7, permeated the fractured rocks; these fluids were rich in fluorine, molybdenum, potassium, and hydrogen sulfide, and contained uranium as fluoride complexes. The hydrothermal fluids reacted with the wallrock resulting in

  13. Hydrothermal processes above the Yellowstone magma chamber: Large hydrothermal systems and large hydrothermal explosions

    USGS Publications Warehouse

    Morgan, L.A.; Shanks, W.C. Pat; Pierce, K.L.

    2009-01-01

    Hydrothermal explosions are violent and dramatic events resulting in the rapid ejection of boiling water, steam, mud, and rock fragments from source craters that range from a few meters up to more than 2 km in diameter; associated breccia can be emplaced as much as 3 to 4 km from the largest craters. Hydrothermal explosions occur where shallow interconnected reservoirs of steam- and liquid-saturated fluids with temperatures at or near the boiling curve underlie thermal fields. Sudden reduction in confi ning pressure causes fluids to fl ash to steam, resulting in signifi cant expansion, rock fragmentation, and debris ejection. In Yellowstone, hydrothermal explosions are a potentially signifi cant hazard for visitors and facilities and can damage or even destroy thermal features. The breccia deposits and associated craters formed from hydrothermal explosions are mapped as mostly Holocene (the Mary Bay deposit is older) units throughout Yellowstone National Park (YNP) and are spatially related to within the 0.64-Ma Yellowstone caldera and along the active Norris-Mammoth tectonic corridor. In Yellowstone, at least 20 large (>100 m in diameter) hydrothermal explosion craters have been identifi ed; the scale of the individual associated events dwarfs similar features in geothermal areas elsewhere in the world. Large hydrothermal explosions in Yellowstone have occurred over the past 16 ka averaging ??1 every 700 yr; similar events are likely in the future. Our studies of large hydrothermal explosion events indicate: (1) none are directly associated with eruptive volcanic or shallow intrusive events; (2) several historical explosions have been triggered by seismic events; (3) lithic clasts and comingled matrix material that form hydrothermal explosion deposits are extensively altered, indicating that explosions occur in areas subjected to intense hydrothermal processes; (4) many lithic clasts contained in explosion breccia deposits preserve evidence of repeated fracturing

  14. Castro ring zone: a 4,500-km2 fossil hydrothermal system in the Challis volcanic field, central Idaho.

    USGS Publications Warehouse

    Criss, R.E.; Ekren, E.B.; Hardyman, R.F.

    1984-01-01

    The largest fossil hydrothermal system occupying a 4500 km2 area in central Idaho is revealed by delta 18O studies. The remains of this meteoric-hydrothermal system are preserved within a sharply bounded, 15 km wide, 70-km-diameter annulus of low delta 18O rock (+2.0 to -8.8per mille) termed the Castro ring zone. The zone is centred on a less depleted (+4.5) core zone consisting of granitic rocks of the Castro pluton. This 700-km2 Eocene subvolcanic batholith has intruded, domed, and hydrothermally metamorphosed a thick sequence of Challis Volcanics, the stratigraphically low rocks in the 2000-km2 Van Horn Peak and the 1000-km2 Thunder Mountain cauldron complexes being most strongly altered. Less extreme 18O depletions occur in the youngest major ash-flow sheets of these complexes, indicating a vertical 18O gradient. Water/rock ratios of geothermal systems are surprisingly insensitive to the circulation scale.-L.-di H.

  15. Evidence of a modern deep water magmatic hydrothermal system in the Canary Basin (eastern central Atlantic Ocean)

    NASA Astrophysics Data System (ADS)

    Medialdea, T.; Somoza, L.; González, F. J.; Vázquez, J. T.; de Ignacio, C.; Sumino, H.; Sánchez-Guillamón, O.; Orihashi, Y.; León, R.; Palomino, D.

    2017-08-01

    New seismic profiles, bathymetric data, and sediment-rock sampling document for the first time the discovery of hydrothermal vent complexes and volcanic cones at 4800-5200 m depth related to recent volcanic and intrusive activity in an unexplored area of the Canary Basin (Eastern Atlantic Ocean, 500 km west of the Canary Islands). A complex of sill intrusions is imaged on seismic profiles showing saucer-shaped, parallel, or inclined geometries. Three main types of structures are related to these intrusions. Type I consists of cone-shaped depressions developed above inclined sills interpreted as hydrothermal vents. Type II is the most abundant and is represented by isolated or clustered hydrothermal domes bounded by faults rooted at the tips of saucer-shaped sills. Domes are interpreted as seabed expressions of reservoirs of CH4 and CO2-rich fluids formed by degassing and contact metamorphism of organic-rich sediments around sill intrusions. Type III are hydrothermal-volcanic complexes originated above stratified or branched inclined sills connected by a chimney to the seabed volcanic edifice. Parallel sills sourced from the magmatic chimney formed also domes surrounding the volcanic cones. Core and dredges revealed that these volcanoes, which must be among the deepest in the world, are constituted by OIB-type, basanites with an outer ring of blue-green hydrothermal Al-rich smectite muds. Magmatic activity is dated, based on lava samples, at 0.78 ± 0.05 and 1.61 ± 0.09 Ma (K/Ar methods) and on tephra layers within cores at 25-237 ky. The Subvent hydrothermal-volcanic complex constitutes the first modern system reported in deep water oceanic basins related to intraplate hotspot activity.Plain Language SummarySubmarine <span class="hlt">volcanism</span> and associated <span class="hlt">hydrothermal</span> systems are relevant processes for the evolution of the ocean basins, due their impact on the geochemistry of the oceans, their potential to form significant ore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4606B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4606B"><span>Asymmetrical <span class="hlt">hydrothermal</span> system below Merapi volcano imaged by geophysical data.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Byrdina, Svetlana; Friedel, Sven; Budi-Santoso, Agus; Suryanto, Wiwit; Suhari, Aldjarishy; Vandemeulebrouck, Jean; Rizal, Mohhamed H.; Grandis, Hendra</p> <p>2017-04-01</p> <p>, while the liquid water flows down to the base of the <span class="hlt">volcanic</span> dome. Our ERT results suggest the existence of a peripheral <span class="hlt">hydrothermal</span> system below the south and west flanks in agreement with previous electromagnetic studies. In contrast, no evidence of <span class="hlt">hydrothermal</span> system is found below the north flank, where the resistivity values are too high to be assigned to a <span class="hlt">hydrothermal</span> system, at least to the ERT investigation depth. A probable cause of this asymmetry could be a <span class="hlt">non</span>-axial location of the magmatic heat source. Such <span class="hlt">non</span>-axial location of the magmatic source relative to the edifice is suggested by the shift of the <span class="hlt">volcanic</span> <span class="hlt">activity</span> to the south as proposed in the geological model by Camus et al, (2000). In addition, the hypocenters of seismic events located by Budi-Santoso et al, (2013) seem to be distributed to the SW from the <span class="hlt">active</span> crater suggesting that the magma conduits and likely, the magmatic source, are shifted to the SW with respect to the actual crater.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160003149','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160003149"><span>Differentiating <span class="hlt">Hydrothermal</span>, Pedogenic, and Glacial Weathering in a Cold <span class="hlt">Volcanic</span> Mars-Analog Environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Scudder, N. A.; Horgan, B.; Havig, J.; Rutledge, A.; Rampe, E. B.; Hamilton, T.</p> <p>2016-01-01</p> <p>Although the current cold, dry environment of Mars extends back through much of its history, its earliest periods experienced significant water- related surface <span class="hlt">activity</span>. Both geomorphic features (e.g., paleolakes, deltas, and river valleys) and hydrous mineral detections (e.g., clays and salts) have historically been interpreted to imply a "warm and wet" early Mars climate. More recently, atmospheric modeling studies have struggled to produce early climate conditions with temperatures above 0degC, leading some studies to propose a "cold and icy" early Mars dominated by widespread glaciation with transient melting. However, the alteration mineralogy produced in subglacial environments is not well understood, so the extent to which cold climate glacial weathering can produce the diverse alteration mineralogy observed on Mars is unknown. This summer, we will be conducting a field campaign in a glacial weathering environment in the Cascade Range, OR in order to determine the types of minerals that these environments produce. However, we must first disentangle the effects of glacial weathering from other significant alteration processes. Here we attempt a first understanding of glacial weathering by differentiating rocks and sediments weathered by <span class="hlt">hydrothermal</span>, pedogenic, and glacial weathering processes in the Cascades <span class="hlt">volcanic</span> range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JVGR..189..257J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JVGR..189..257J"><span>Seismicity and fluid geochemistry at Lassen <span class="hlt">Volcanic</span> National Park, California: Evidence for two circulation cells in the <span class="hlt">hydrothermal</span> system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janik, Cathy J.; McLaren, Marcia K.</p> <p>2010-01-01</p> <p>Seismic analysis and geochemical interpretations provide evidence that two separate <span class="hlt">hydrothermal</span> cells circulate within the greater Lassen <span class="hlt">hydrothermal</span> system. One cell originates south to SW of Lassen Peak and within the Brokeoff Volcano depression where it forms a reservoir of hot fluid (235-270 °C) that boils to feed steam to the high-temperature fumarolic areas, and has a plume of degassed reservoir liquid that flows southward to emerge at Growler and Morgan Hot Springs. The second cell originates SSE to SE of Lassen Peak and flows southeastward along inferred faults of the Walker Lane belt (WLB) where it forms a reservoir of hot fluid (220-240 °C) that boils beneath Devils Kitchen and Boiling Springs Lake, and has an outflow plume of degassed liquid that boils again beneath Terminal Geyser. Three distinct seismogenic zones (identified as the West, Middle, and East seismic clusters) occur at shallow depths (< 6 km) in Lassen <span class="hlt">Volcanic</span> National Park, SW to SSE of Lassen Peak and adjacent to areas of high-temperature (≤ 161 °C) fumarolic <span class="hlt">activity</span> (Sulphur Works, Pilot Pinnacle, Little Hot Springs Valley, and Bumpass Hell) and an area of cold, weak gas emissions (Cold Boiling Lake). The three zones are located within the inferred Rockland caldera in response to interactions between deeply circulating meteoric water and hot brittle rock that overlies residual magma associated with the Lassen <span class="hlt">Volcanic</span> Center. Earthquake focal mechanisms and stress inversions indicate primarily N-S oriented normal faulting and E-W extension, with some oblique faulting and right lateral shear in the East cluster. The different focal mechanisms as well as spatial and temporal earthquake patterns for the East cluster indicate a greater influence by regional tectonics and inferred faults within the WLB. A fourth, deeper (5-10 km) seismogenic zone (the Devils Kitchen seismic cluster) occurs SE of the East cluster and trends NNW from Sifford Mountain toward the Devils Kitchen thermal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1966T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1966T"><span><span class="hlt">Hydrothermal</span> <span class="hlt">activities</span> around Dragon Horn Area (49.7°E) on ultra-slow spreading Southwest Indian Ridge (SWIR)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tao, C.; Liang, J.; Zhang, H.; Li, H.; Egorov, I. V.; Liao, S.</p> <p>2016-12-01</p> <p>The Dragon Horn Area (49.7°E), is located at the west end of the EW trending Segment 28 of Southwest Indian Ridge between Indomed and Gallieni FZ. The segment is characterized by highly asymmetric topography. The northern flank is deeper and develops typical parallel linear fault escarpments. Meanwhile, the southern flank, where the Dragon Horn lies, is shallower and bears corrugations. The indicative corrugated surface which extends some 5×5 km was interpreted to be of Dragon Flag OCC origin (Zhao et al., 2013). Neo-<span class="hlt">volcanic</span> ridge extends along the middle of the rifted valley and is bounded by two <span class="hlt">non</span>-transform offsets to the east and west. Our investigations revealed 6 <span class="hlt">hydrothermal</span> fields/anomalies in this area, including 2 confirmed sulfide fields, 1 carbonate field, and 3 inferred <span class="hlt">hydrothermal</span> anomalies based on methane and turbidity data from 2016 AUV survey. Longqi-1(Dragon Flag) vent system lies to the northwest edge of Dragon Flag OCC. It is one of the largest <span class="hlt">hydrothermal</span> venting systems along Mid-Ocean Ridges, with maximum temperature at vent site DFF6 of 'M zone' up to 379.3 °C (Tao et al, 2016). Massive sulfides (49.73 °E, 37.78 °S) were sampled 10 km east to Longqi-1, representing independent <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> controlled by respective local structures. According to geological mapping and interpretation, both sulfide fields are located on the hanging wall of the Dragon Flag OCC detachment. Combined with the inferred <span class="hlt">hydrothermal</span> anomaly to the east of the massive sulfide site, we suppose that they are controlled by different fault phases during the detachment of oceanic core complex. Moreover, consolidated carbonate sediments were widely observed and sampled on the corrugated surface and its west side, they are proposed to be precipitated during the serpentinization of ultramafic rocks, representing low-temperature <span class="hlt">hydrothermal</span> process. These <span class="hlt">hydrothermal</span> <span class="hlt">activities</span>, distributed within 20km, may be controlled by the same Dragon Flag OCC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP21A1238W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP21A1238W"><span>Constraining Silicate Weathering Processes in an <span class="hlt">Active</span> <span class="hlt">Volcanic</span> Complex: Implications for the Long-term 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>Washington, K.; West, A. J.; Hartmann, J.; Amann, T.; Hosono, T.; Ide, K.</p> <p>2017-12-01</p> <p>While analyzing geochemical archives and carbon cycle modelling can further our understanding of the role of silicate weathering as a sink in the long-term carbon cycle, it is necessary to study modern weathering processes to inform these efforts. A recent compilation of data from rivers draining basaltic catchments estimates that rock weathering in <span class="hlt">active</span> <span class="hlt">volcanic</span> fields (AVFs) consumes atmospheric CO2 approximately three times faster than in inactive <span class="hlt">volcanic</span> fields (IVFs), suggesting that the eruption and subsequent weathering of large igneous provinces likely played a major role in the carbon cycle in the geologic past [1]. The study demonstrates a significant correlation between catchment mean annual temperature (MAT) and atmospheric CO2 consumption rate for IVFs. However CO2 consumption due to weathering of AVFs is not correlated with MAT as the relationship is complicated by variability in <span class="hlt">hydrothermal</span> fluxes, reactive surface area, and groundwater flow paths. To investigate the controls on weathering processes in AVFs, we present data for dissolved and solid weathering products from Mount Aso Caldera, Japan. Aso Caldera is an ideal site for studying the how the chemistry of rivers draining an AVF is impacted by high-temperature water/rock interactions, <span class="hlt">volcanic</span> ash weathering, and varied groundwater flow paths and residence times. Samples were collected over five field seasons from two rivers and their tributaries, cold groundwater springs, and thermal springs. These samples capture the region's temperature and precipitation seasonality. Solid samples of unaltered <span class="hlt">volcanic</span> rocks, <span class="hlt">hydrothermally</span>-altered materials, <span class="hlt">volcanic</span> ash, a soil profile, and suspended and bedload river sediments were also collected. The hydrochemistry of dissolved phases were analyzed at the University of Hamburg, while the mineralogy and geochemical compositions of solid phases were analyzed at the Natural History Museum of Los Angeles. This work will be discussed in the context of</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/2015EGUGA..1711982L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711982L"><span>Whakaari (White Island volcano, New Zealand): Magma-<span class="hlt">hydrothermal</span> laboratory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lavallee, Yan; Heap, Michael J.; Reuschle, Thierry; Mayer, Klaus; Scheu, Bettina; Gilg, H. Albert; Kennedy, Ben M.; Letham-Brake, Mark; Jolly, Arthur; Dingwell, Donald B.</p> <p>2015-04-01</p> <p>Whakaari, <span class="hlt">active</span> andesitic stratovolcano of the Taupo <span class="hlt">Volcanic</span> Zone (New Zealand), hosts an open, highly reactive <span class="hlt">hydrothermal</span> system in the amphitheatre of an earlier sector collapse. Its recent <span class="hlt">volcanic</span> <span class="hlt">activity</span> is primarily characterized by sequences of steam-driven (phreatic) and phreatomagmatic explosive eruptions, although a lava dome briefly extruded in 2012. The volcano provides a natural laboratory for the study of aggressive fluids on the permeability of the <span class="hlt">hydrothermal</span> system, on phreatomagmatic <span class="hlt">volcanism</span> as well as on the volcano edifice structural stability. Here, we present a holistic experimental dataset on the reservoir rocks properties (mineralogy, permeability, seismic velocity) and their response to changes in stress (strength, deformation mechanisms, fragmentation) and temperature (mineralogical breakdown). We show that the advance degree of alteration in the system, nearly replaced all the original rock-forming minerals. This alteration has produced generally weak rocks, which, when subjected to a differential stress, can undergo transition from a dilatant response (brittle) to a compactant response with a mere confining pressure of about 15-20 MPa (corresponding to depth of about 1 km). Thermal stressing experiments reveal that the alteration phases breakdown at 500 °C (alunite) and 700 °C (dehydrated alum and sulphur), generating much weakened skeletal rocks, deteriorated by a mass loss of 20 wt.%, resulting in an increase in porosity and permeability of about 15 vol.% and an order of magnitude, respectively. Novel thermal stressing tests at high-heating rates (<1000 K/min) suggest that the onset of this mineralogical debilitation is pushed to higher temperatures with heating rates, carrying implication for the stability of the reservoir rocks and explosions during magma movement at variable rates in the upper edifice. Rock strength imposes an important control on the stability of <span class="hlt">volcanic</span> edifices and of the <span class="hlt">hydrothermal</span> reservoir rocks</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030071123&hterms=life+Norway&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dlife%2BNorway','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030071123&hterms=life+Norway&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dlife%2BNorway"><span><span class="hlt">Hydrothermal</span> Origin for Carbonate Globules in Martian Meteorite ALH84001: A Terrestrial Analogue from Spitsbergen (Norway)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Treiman, Allan H.; Amundsen, Hans E. F.; Blake, David F.; Bunch, Ted</p> <p>2002-01-01</p> <p>Carbonate minerals in the ancient Martian meteorite ALH84001 are the only known solid phases that bear witness to the processing of volatile and biologically critical compounds (CO2, H2O) on early Mars. Similar carbonates have been found in xenoliths and their host basalts from Quaternary <span class="hlt">volcanic</span> centers in northern Spitsbergen (Norway). These carbonates were deposited by hot (i.e., <span class="hlt">hydrothermal</span>) waters associated with the <span class="hlt">volcanic</span> <span class="hlt">activity</span>. By analogy with the Spitsbergen carbonates, the ALH84001 carbonates were probably also deposited by hot water. <span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> was probably common and widespread on Early Mars, which featured abundant basaltic rocks, water as ice or liquid, and heat from volcanos and asteroid impacts. On Earth, descendants of the earliest life forms still prefer <span class="hlt">hydrothermal</span> environments, which are now shown to have been present on early Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011921','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011921"><span>East Pacific rise at 21°N: the <span class="hlt">volcanic</span>, tectonic, and <span class="hlt">hydrothermal</span> processes of the central axis</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ballard, Richard D.; Francheteau, Jean; Juteau, Tierre; Rangan, Claude; Normark, William</p> <p>1981-01-01</p> <p>Photographs obtained by the ANGUS survey system at 21°N reveal many similarities to the geological processes delineated at other spreading centers and in particular those observed in the Galapagos Rift at 86°W. The region of recent <span class="hlt">volcanism</span> is restricted to a narrow zone (Zone 1) approximately 1 km wide. This suggests that the width of the magma chamber feeding these flows is also narrow at the top. Variations in sediment cover are used to subdivide the flows within Zone 1 into three sheet-flow/pillow-flow pairs. The youngest pair appears to have erupted form a linear fissure 8 km long running parallel to the valley axis. This fissure is part of a larger en echelon pattern of eruptive fissures. <span class="hlt">Active</span> <span class="hlt">hydrothermal</span> vents associated with the youngest flows are situated directly above the apparent eruptive fissure. The high (350°C) temperature for some of the fluids exiting from the vents suggests a highly restricted circulation system involving, at times, little to no mixing with cold seawater. The lava terrain in the remainder of Zone 1 and bordering regions is characterized by extensive fracturing, further suggesting a narrow upper dimension to the magma chamber and also that subsurface <span class="hlt">hydrothermal</span> deposition of massive sulfides may lead to a reduction in the mixing processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70197144','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70197144"><span>East Pacific Rise at 21 °N: The <span class="hlt">volcanic</span>, tectonic, and <span class="hlt">hydrothermal</span> processes of the central axis</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ballard, Richard D.; Francheteau, Jean; Juteau, Tierre; Rangan, Claude; Normark, William R.</p> <p>1981-01-01</p> <p>Photographs obtained by the ANGUS survey system at 21°N reveal many similarities to the geological processes delineated at other spreading centers and in particular those observed in the Galapagos Rift at 86°W. The region of recent <span class="hlt">volcanism</span> is restricted to a narrow zone (Zone l) approximately l km wide. This suggests that the width of the magma chamber feeding these flows is also narrow at the top. Variations in sediment cover are used to subdivide the flows within Zone 1 into three sheet-flow/pillow-flow pairs. The youngest pair appears to have erupted form a linear fissure 8 km long running parallel to the valley axis. This fissure is part of a larger en echelon pattern of eruptive fissures. <span class="hlt">Active</span> <span class="hlt">hydrothermal</span> vents associated with the youngest flows are situated directly above the apparent eruptive fissure. The high (350°C) temperature for some of the fluids exiting from the vents suggests a highly restricted circulation system involving, at times, little to no mixing with cold seawater. The lava terrain in the remainder of Zone l and bordering regions is characterized by extensive fracturing, further suggesting a narrow upper dimension to the magma chamber and also that subsurface <span class="hlt">hydrothermal</span> deposition of massive sulfides may lead to a reduction in the mixing processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981E%26PSL..55....1B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981E%26PSL..55....1B"><span>East Pacific rise at 21°N: The <span class="hlt">volcanic</span>, tectonic, and <span class="hlt">hydrothermal</span> processes of the central axis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ballard, Robert D.; Francheteau, Jean; Juteau, Tierre; Rangan, Claude; Normark, William</p> <p>1981-09-01</p> <p>Photographs obtained by the ANGUS survey system at 21°N reveal many similarities to the geological processes delineated at other spreading centers and in particular those observed in the Galapagos Rift at 86°W. The region of recent <span class="hlt">volcanism</span> is restricted to a narrow zone (Zone 1) approximately 1 km wide. This suggests that the width of the magma chamber feeding these flows is also narrow at the top. Variations in sediment cover are used to subdivide the flows within Zone 1 into three sheet-flow/pillow-flow pairs. The youngest pair appears to have erupted form a linear fissure 8 km long running parallel to the valley axis. This fissure is part of a larger en echelon pattern of eruptive fissures. <span class="hlt">Active</span> <span class="hlt">hydrothermal</span> vents associated with the youngest flows are situated directly above the apparent eruptive fissure. The high (350°C) temperature for some of the fluids exiting from the vents suggests a highly restricted circulation system involving, at times, little to no mixing with cold seawater. The lava terrain in the remainder of Zone 1 and bordering regions is characterized by extensive fracturing, further suggesting a narrow upper dimension to the magma chamber and also that subsurface <span class="hlt">hydrothermal</span> deposition of massive sulfides may lead to a reduction in the mixing processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DSRI..116..127K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DSRI..116..127K"><span>Extensive <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> revealed by multi-tracer survey in the Wallis and Futuna region (SW Pacific)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konn, C.; Fourré, E.; Jean-Baptiste, P.; Donval, J. P.; Guyader, V.; Birot, D.; Alix, A. S.; Gaillot, A.; Perez, F.; Dapoigny, A.; Pelleter, E.; Resing, J. A.; Charlou, J. L.; Fouquet, Y.</p> <p>2016-10-01</p> <p>The study area is close to the Wallis and Futuna Islands in the French EEZ. It exists on the western boundary of the fastest tectonic area in the world at the junction of the Lau and North-Fiji basins. At this place, the unstable back-arc accommodates the plate motion in three ways: (i) the north Fiji transform fault, (ii) numerous unstable spreading ridges, and (iii) large areas of recent <span class="hlt">volcanic</span> <span class="hlt">activity</span>. This instability creates bountiful opportunity for <span class="hlt">hydrothermal</span> discharge to occur. Based on geochemical (CH4, TDM, 3He) and geophysical (nephelometry) tracer surveys: (1) no <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> could be found on the Futuna Spreading Centre (FSC) which sets the western limit of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>; (2) four distinct <span class="hlt">hydrothermal</span> <span class="hlt">active</span> areas were identified: Kulo Lasi Caldera, Amanaki Volcano, Fatu Kapa and Tasi Tulo areas; (3) extensive and diverse <span class="hlt">hydrothermal</span> manifestations were observed and especially a 2D distribution of the sources. At Kulo Lasi, our data and especially tracer ratios (CH4/3He 50×106 and CH4/TDM 4.5) reveal a transient CH4 input, with elevated levels of CH4 measured in 2010, that had vanished in 2011, most likely caused by an eruptive magmatic event. By contrast at Amanaki, vertical tracer profiles and tracer ratios point to typical seawater/basalt interactions. Fatu Kapa is characterised by a substantial spatial variability of the <span class="hlt">hydrothermal</span> water column anomalies, most likely due to widespread focused and diffuse <span class="hlt">hydrothermal</span> discharge in the area. In the Tasi Tulo zone, the <span class="hlt">hydrothermal</span> signal is characterised by a total lack of turbidity, although other tracer anomalies are in the same range as in nearby Fatu Kapa. The background data set revealed the presence of a Mn and 3He chronic plume due to the extensive and cumulative venting over the entire area. To that respect, we believe that the joined domain composed of our <span class="hlt">active</span> area and the nearby <span class="hlt">active</span> area discovered in the East by Lupton et al. (2012) highly contribute to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26925957','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26925957"><span>Seafloor doming driven by degassing processes unveils sprouting <span class="hlt">volcanism</span> in coastal areas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Passaro, Salvatore; Tamburrino, Stella; Vallefuoco, Mattia; Tassi, Franco; Vaselli, Orlando; Giannini, Luciano; Chiodini, Giovanni; Caliro, Stefano; Sacchi, Marco; Rizzo, Andrea Luca; Ventura, Guido</p> <p>2016-03-01</p> <p>We report evidences of <span class="hlt">active</span> seabed doming and gas discharge few kilometers offshore from the Naples harbor (Italy). Pockmarks, mounds, and craters characterize the seabed. These morphologies represent the top of shallow crustal structures including pagodas, faults and folds affecting the present-day seabed. They record upraise, pressurization, and release of He and CO2 from mantle melts and decarbonation reactions of crustal rocks. These gases are likely similar to those that feed the <span class="hlt">hydrothermal</span> systems of the Ischia, Campi Flegrei and Somma-Vesuvius <span class="hlt">active</span> volcanoes, suggesting the occurrence of a mantle source variously mixed to crustal fluids beneath the Gulf of Naples. The seafloor swelling and breaching by gas upraising and pressurization processes require overpressures in the order of 2-3 MPa. Seabed doming, faulting, and gas discharge are manifestations of <span class="hlt">non-volcanic</span> unrests potentially preluding submarine eruptions and/or <span class="hlt">hydrothermal</span> explosions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4772541','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4772541"><span>Seafloor doming driven by degassing processes unveils sprouting <span class="hlt">volcanism</span> in coastal areas</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Passaro, Salvatore; Tamburrino, Stella; Vallefuoco, Mattia; Tassi, Franco; Vaselli, Orlando; Giannini, Luciano; Chiodini, Giovanni; Caliro, Stefano; Sacchi, Marco; Rizzo, Andrea Luca; Ventura, Guido</p> <p>2016-01-01</p> <p>We report evidences of <span class="hlt">active</span> seabed doming and gas discharge few kilometers offshore from the Naples harbor (Italy). Pockmarks, mounds, and craters characterize the seabed. These morphologies represent the top of shallow crustal structures including pagodas, faults and folds affecting the present-day seabed. They record upraise, pressurization, and release of He and CO2 from mantle melts and decarbonation reactions of crustal rocks. These gases are likely similar to those that feed the <span class="hlt">hydrothermal</span> systems of the Ischia, Campi Flegrei and Somma-Vesuvius <span class="hlt">active</span> volcanoes, suggesting the occurrence of a mantle source variously mixed to crustal fluids beneath the Gulf of Naples. The seafloor swelling and breaching by gas upraising and pressurization processes require overpressures in the order of 2–3 MPa. Seabed doming, faulting, and gas discharge are manifestations of <span class="hlt">non-volcanic</span> unrests potentially preluding submarine eruptions and/or <span class="hlt">hydrothermal</span> explosions. PMID:26925957</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.T52C..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.T52C..02R"><span>Along-strike supply of <span class="hlt">volcanic</span> rifted margins: Implications for plume-influenced rifting and sudden along-strike transitions between <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> rifted margins</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ranero, C. R.; Phipps Morgan, J.</p> <p>2006-12-01</p> <p>The existence of sudden along-strike transitions between <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> rifted margins is an important constraint for conceptual models of rifting and continental breakup. We think there is a promising indirect approach to infer the maximum width of the region of upwelling that exists beneath a rifted margin during the transition from rifting to seafloor-spreading. We infer this width of ~30km from the minimum length of the ridge-offsets that mark the limits of the `region of influence' of on-ridge plumes on the axial relief, axial morphology, and crustal thickness along the ridge and at the terminations of fossil <span class="hlt">volcanic</span> rifted margins. We adopt Vogt's [1972] hypothesis for along-ridge asthenospheric flow in a narrow vertical slot beneath the axis of plume-influenced `macro-segments' and <span class="hlt">volcanic</span> rifted margins. We find that: (1) There is a threshold distance to the lateral offsets that bound plume-influenced macrosegments; all such `barrier offsets' are greater than ~30km, while smaller offsets do not appear to be a barrier to along-axis flow. This pattern is seen in the often abrupt transitions between <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> rifted margins; these transitions coincide with >30km ridge offsets that mark the boundary between the smooth seafloor morphology and thick crust of a plume- influenced <span class="hlt">volcanic</span> margin and a neighboring <span class="hlt">non-volcanic</span> margin, as recorded in 180Ma rifting of the early N. Atlantic, the 42Ma rifting of the Kerguelen-Broken Ridge, and the 66Ma Seychelles-Indian rifting in the Indian Ocean. (2) A similar pattern is seen in the often abrupt transitions between `normal' and plume-influenced mid- ocean ridge segments, which is discussed in a companion presentation by Phipps Morgan and Ranero (this meeting). (3) The coexistance of adjacent <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> rifted margin segments is readily explained in this conceptual framework. If the <span class="hlt">volcanic</span> margin macrosegment is plume-fed by hot asthenosphere along an axial ridge slot</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.G41A0703C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.G41A0703C"><span>Monitoring the Sumatra <span class="hlt">volcanic</span> arc with InSAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chaussard, E.; Hong, S.; Amelung, F.</p> <p>2009-12-01</p> <p>The Sumatra <span class="hlt">volcanic</span> arc is the result of the subduction of the Indo-Australian plate under the Sunda plate. The arc consists of 35 known <span class="hlt">volcanic</span> centers, subaerials on the west coast of the Sumatra and Andaman Islands and submarines between these islands. Six <span class="hlt">active</span> centers are known in the Sumatra <span class="hlt">volcanic</span> arc. Surface deformation in <span class="hlt">volcanic</span> areas usually indicates movement of magma or <span class="hlt">hydrothermal</span> fluids at depth. Here we present a satellite-based Interferometric synthetic aperture radar (InSAR) survey of the Sumatra <span class="hlt">volcanic</span> arc using ALOS data. Spanning the years 2007 to beginning of 2009, our survey reveals the background level of <span class="hlt">activity</span> of the 35 volcanoes. We processed data from 40 tracks (24 in descending orbit and 16 in ascending orbit) to cover the whole Sumatra arc. In the first results five of these six known <span class="hlt">active</span> centers show no sign of <span class="hlt">activity</span>: Dempo, Kaba, Marapi, Talang and Peuet. The remaining <span class="hlt">active</span> volcano, Mount Kerinci, has an ambiguous signal. We used pair-wise logic and InSAR time series of the available ALOS data to determine if the observed InSAR signal is caused by ground deformation or by atmospheric delays.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JVGR..304..324D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JVGR..304..324D"><span>A study of the <span class="hlt">hydrothermal</span> alteration in Paleoproterozoic <span class="hlt">volcanic</span> centers, São Félix do Xingu region, Amazonian Craton, Brazil, using short-wave infrared spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>da Cruz, Raquel Souza; Fernandes, Carlos Marcello Dias; Villas, Raimundo Netuno Nobre; Juliani, Caetano; Monteiro, Lena Virgínia Soares; de Almeida, Teodoro Isnard Ribeiro; Lagler, Bruno; de Carvalho Carneiro, Cleyton; Misas, Carlos Mario Echeverri</p> <p>2015-10-01</p> <p>Hypogene <span class="hlt">hydrothermal</span> minerals have been identified by short-wave infrared spectroscopy in <span class="hlt">hydrothermally</span> altered rocks from the Sobreiro and Santa Rosa formations, which belong to a Paleoproterozoic volcano-plutonic system in Amazonian craton. Three clay minerals are spectrally recognized: montmorillonite, kaolinite, and illite. The integration of these data with those available in the literature, including gold occurrences, suggests that those rocks are <span class="hlt">hydrothermal</span> products of both <span class="hlt">volcanic</span> thermal sources and later crustal intrusions, as evidenced by variable styles of propylitic, sericitic, potassic, and intermediate argillic alteration. The influence of meteoric fluids is emphasized. This low cost exploratory technique, which can be applied to hand samples, seems to be promising in the separation of <span class="hlt">hydrothermally</span> altered volcano-plutonic centers in regions submitted to severe weathering conditions, in addition to aid elaborating models for prospecting mineral deposits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70111059','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70111059"><span>Dynamics of the Yellowstone <span class="hlt">hydrothermal</span> system</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hurwitz, Shaul; Lowenstern, Jacob B.</p> <p>2014-01-01</p> <p>The Yellowstone Plateau <span class="hlt">Volcanic</span> Field is characterized by extensive seismicity, episodes of uplift and subsidence, and a <span class="hlt">hydrothermal</span> system that comprises more than 10,000 thermal features, including geysers, fumaroles, mud pots, thermal springs, and <span class="hlt">hydrothermal</span> explosion craters. The diverse chemical and isotopic compositions of waters and gases derive from mantle, crustal, and meteoric sources and extensive water-gas-rock interaction at variable pressures and temperatures. The thermal features are host to all domains of life that utilize diverse inorganic sources of energy for metabolism. The unique and exceptional features of the <span class="hlt">hydrothermal</span> system have attracted numerous researchers to Yellowstone beginning with the Washburn and Hayden expeditions in the 1870s. Since a seminal review published a quarter of a century ago, research in many fields has greatly advanced our understanding of the many coupled processes operating in and on the <span class="hlt">hydrothermal</span> system. Specific advances include more refined geophysical images of the magmatic system, better constraints on the time scale of magmatic processes, characterization of fluid sources and water-rock interactions, quantitative estimates of heat and magmatic volatile fluxes, discovering and quantifying the role of thermophile microorganisms in the geochemical cycle, defining the chronology of <span class="hlt">hydrothermal</span> explosions and their relation to glacial cycles, defining possible links between <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>, deformation, and seismicity; quantifying geyser dynamics; and the discovery of extensive <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in Yellowstone Lake. Discussion of these many advances forms the basis of this review.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015DSRI..106..167G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015DSRI..106..167G"><span>Differences in recovery between deep-sea <span class="hlt">hydrothermal</span> vent and vent-proximate communities after a <span class="hlt">volcanic</span> eruption</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gollner, Sabine; Govenar, Breea; Arbizu, Pedro Martinez; Mills, Susan; Le Bris, Nadine; Weinbauer, Markus; Shank, Timothy M.; Bright, Monika</p> <p>2015-12-01</p> <p>Deep-sea <span class="hlt">hydrothermal</span> vents and the surrounding basalt seafloor are subject to major natural disturbance events such as <span class="hlt">volcanic</span> eruptions. In the near future, anthropogenic disturbance in the form of deep-sea mining could also significantly affect the faunal communities of <span class="hlt">hydrothermal</span> vents. In this study, we monitor and compare the recovery of insular, highly productive vent communities and vent-proximate basalt communities following a <span class="hlt">volcanic</span> eruption that destroyed almost all existing communities at the East Pacific Rise, 9°50‧N in 2006. To study the recovery patterns of the benthic communities, we placed settlement substrates at vent sites and their proximate basalt areas and measured the prokaryotic abundance and compared the meio- and macrofaunal species richness and composition at one, two and four years after the eruption. In addition, we collected samples from the overlying water column with a pelagic pump, at one and two years after the <span class="hlt">volcanic</span> eruption, to determine the abundance of potential meiofauna colonisers. One year after eruption, mean meio- and macrofaunal abundances were not significantly different from pre-eruption values in vent habitats (meio: 8-1838 ind. 64 cm-2 in 2006; 3-6246 ind. 64 cm-2 in 2001/02; macro: 95-1600 ind. 64 cm-2 in 2006; 205-4577 ind. 64 cm-2 in 2001/02) and on <span class="hlt">non</span>-vent basalt habitats (meio: 10-1922 ind. 64 cm-2 in 2006; 8-328 ind. 64 cm-2 in 2003/04; macro: 14-3351 ind. 64 cm-2 in 2006; 2-63 ind. 64 cm-2 in 2003/04), but species recovery patterns differed between the two habitat types. In the vent habitat, the initial community recovery was relatively quick but incomplete four years after eruption, which may be due to the good dispersal capabilities of vent endemic macrofauna and vent endemic dirivultid copepods. At vents, 42% of the pre-eruption meio- and 39% of macrofaunal species had returned. In addition, some new species not evident prior to the eruption were found. At the tubeworm site Tica, a total of 26</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034028','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034028"><span>Seismicity and fluid geochemistry at Lassen <span class="hlt">Volcanic</span> National Park, California: Evidence for two circulation cells in the <span class="hlt">hydrothermal</span> system</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Janik, Cathy J.; McLaren, Marcia K.</p> <p>2010-01-01</p> <p>Seismic analysis and geochemical interpretations provide evidence that two separate <span class="hlt">hydrothermal</span> cells circulate within the greater Lassen <span class="hlt">hydrothermal</span> system. One cell originates south to SW of Lassen Peak and within the Brokeoff Volcano depression where it forms a reservoir of hot fluid (235–270°C) that boils to feed steam to the high-temperature fumarolic areas, and has a plume of degassed reservoir liquid that flows southward to emerge at Growler and Morgan Hot Springs. The second cell originates SSE to SE of Lassen Peak and flows southeastward along inferred faults of the Walker Lane belt (WLB) where it forms a reservoir of hot fluid (220–240°C) that boils beneath Devils Kitchen and Boiling Springs Lake, and has an outflow plume of degassed liquid that boils again beneath Terminal Geyser. Three distinct seismogenic zones (identified as the West, Middle, and East seismic clusters) occur at shallow depths (<6 km) in Lassen <span class="hlt">Volcanic</span> National Park, SW to SSE of Lassen Peak and adjacent to areas of high-temperature (≤161°C) fumarolic <span class="hlt">activity</span> (Sulphur Works, Pilot Pinnacle, Little Hot Springs Valley, and Bumpass Hell) and an area of cold, weak gas emissions (Cold Boiling Lake). The three zones are located within the inferred Rockland caldera in response to interactions between deeply circulating meteoric water and hot brittle rock that overlies residual magma associated with the Lassen <span class="hlt">Volcanic</span> Center. Earthquake focal mechanisms and stress inversions indicate primarily N–S oriented normal faulting and E–W extension, with some oblique faulting and right lateral shear in the East cluster. The different focal mechanisms as well as spatial and temporal earthquake patterns for the East cluster indicate a greater influence by regional tectonics and inferred faults within the WLB. A fourth, deeper (5–10 km) seismogenic zone (the Devils Kitchen seismic cluster) occurs SE of the East cluster and trends NNW from Sifford Mountain toward the Devils Kitchen</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..349..351T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..349..351T"><span>Relationship between <span class="hlt">volcanic</span> <span class="hlt">activity</span> and shallow <span class="hlt">hydrothermal</span> system at Meakandake volcano, Japan, inferred from geomagnetic and audio-frequency magnetotelluric measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takahashi, Kosuke; Takakura, Shinichi; Matsushima, Nobuo; Fujii, Ikuko</p> <p>2018-01-01</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> at Meakandake volcano, Japan, from 2004 to 2014 was investigated by using long-term geomagnetic field observations and audio-frequency magnetotelluric (AMT) surveys. The total intensity of the geomagnetic field has been measured around the summit crater Ponmachineshiri since 1992 by Kakioka Magnetic Observatory. We reanalyzed an 11-year dataset of the geomagnetic total intensity distribution and used it to estimate the thermomagnetic source models responsible for the surface geomagnetic changes during four time periods (2004-2006, 2006-2008, 2008-2009 and 2013-2014). The modeled sources suggest that the first two periods correspond to a cooling phase after a phreatic eruption in 1998, the third one to a heating phase associated with a phreatic eruption in 2008, and the last one to a heating phase accompanying minor internal <span class="hlt">activity</span> in 2013. All of the thermomagnetic sources were beneath a location on the south side of Ponmachineshiri crater. In addition, we conducted AMT surveys in 2013 and 2014 at Meakandake and constructed a two-dimensional model of the electrical resistivity structure across the volcano. Combined, the resistivity information and thermomagnetic models revealed that the demagnetization source associated with the 2008 eruptive <span class="hlt">activity</span>, causing a change in magnetic moment about 30 to 50 times greater than the other sources, was located about 1000 m beneath Ponmachineshiri crater, within or below a zone of high conductivity (a few ohm meters), whereas the other three sources were near each other and above this zone. We interpret the conductive zone as either a <span class="hlt">hydrothermal</span> reservoir or an impermeable clay-rich layer acting as a seal above the <span class="hlt">hydrothermal</span> reservoir. Along with other geophysical observations, our models suggest that the 2008 phreatic eruption was triggered by a rapid influx of heat into the <span class="hlt">hydrothermal</span> reservoir through fluid-rich fractures developed during recent seismic swarms. The <span class="hlt">hydrothermal</span> reservoir</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFMOS42E..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMOS42E..06G"><span><span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> Along the Central Indian Ridge: Ridges, Hotspots and Philately.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>German, C. R.; Connelly, D. P.; Evans, A. J.; Murton, B. J.; Curewitz, D.; Okino, K.; Statham, P. J.; Parson, L. M.</p> <p>2001-12-01</p> <p>The global mid-ocean ridge crest extends 50-60,000km and the majority remains unexplored for <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Even those areas which are reasonably familiar continue to spring surprises (e.g. the "Lost City" site found in late 2000). Within the confines of conceivable research budgets, therefore, choosing new areas for investigation and exploration demands an intelligent approach, beyond flicking through holiday brochures or identifying missing entries for the John Edmond Memorial Stamp Collection. With that caveat, the Southampton Oceanography Centre led a 10-week expedition to the Central Indian Ridge, earlier this year, based in and around Mauritius. During cruise CD127 (23 April-23 May) we conducted a systematic investigation of the ridge crest (seafloor and overlying water column) between 18 deg 16 min and 20 deg 49 min South. We chose this area to investigate the distribution of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> both close to, and away from, that section of the ridge crest which continues to reflect past influence of the migrating Rodrigues hot-spot. Our hypothesis was that the high incidence of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> we had located previously, near the Azores Triple Junction, may result from waning influence of the Azores Hot-Spot nearby and that similar effects might be found resulting from interaction of the CIR with the Rodrigues hot-spot. The primary scientific package we employed was the SOC's TOBI deep-tow sidescan vehicle, now up-graded with an extra Light Scattering Sensor string. In concert, this instrumentation allowed us to prospect for particle-laden <span class="hlt">hydrothermal</span> plumes in the water column overlying the ridge-crest, in real-time, whilst simultaneously acquiring high-resolution sidescan images of the underlying seafloor. Using this approach, particle-rich anomalies were observed at 5 locations along ca. 300km of surveyed ridge-crest, including 4 sites all within the extended (hot-spot influenced) segment 15, which stretches from 18 deg 45 to 20 deg 14</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.8487B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8487B"><span>Distribution, structure and temporal variability of <span class="hlt">hydrothermal</span> outflow at a slow-spreading <span class="hlt">hydrothermal</span> field from seafloor image mosaics.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barreyre, Thibaut; Escartin, Javier; Cannat, Mathilde; Garcia, Rafael; Science Party, Momar'08; Science Party, Bathyluck'09</p> <p>2010-05-01</p> <p>The Lucky Strike <span class="hlt">hydrothermal</span> site, located South of the Azores along the Mid-Atlantic Ridge, is one of the largest and best-known <span class="hlt">active</span> <span class="hlt">hydrothermal</span> fields along the ridge system. This site within the MoMAR area is also the target for the installation in 2010 of a pilot deep-sea observatory with direct telemetry to land, to be part of the European Seafloor Observatory Network (ESONET). The Lucky Strike <span class="hlt">hydrothermal</span> site has seen extensive high-resolution, near-bottom geophysical surveys in 1996 (Lustre'96), 2006 (Momareto06), 2008 (MOMAR08) and 2009 (Bathyluck09). Vertically acquired black-and-white electronic still camera images have been projected and georeferenced to obtain 3 image mosaics covering the zone of <span class="hlt">active</span> venting, extending ~ 700x800 m2, and with full image resolution (~10 mm pixels). These data allow us to study how <span class="hlt">hydrothermal</span> outflow is structured, including the relationships between the zones of <span class="hlt">active</span> high-temperature venting, areas of diffuse outflow, and the geological structure (nature of the substrate, faults and fissures, sediments, etc.). <span class="hlt">Hydrothermal</span> outflow is systematically associated with bacterial mats that are easily identified in the imagery, allowing us to study temporal variability at two different scales. Over the 13-year period we can potentially track changes in both the geometry and intensity of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> throughout the system; our preliminary study of the Eiffel Tower, White Castle and Mt Segur indicate that <span class="hlt">activity</span> has been sustained in recent times, with small changes in the detailed geometry of the diffuse outflow and its intensity. At longer times scales (hundreds to 1000 years?) imagery also shows evidence of areas of venting that are no longer <span class="hlt">active</span>, often associated with the <span class="hlt">active</span> structures. In combination with the high-resolution bathymetry, the imagery data thus allow us to characterize the shallow structure of <span class="hlt">hydrothermal</span> outflow at depth, the structural and <span class="hlt">volcanic</span> control, and ultimately</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..310L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..310L"><span>Chronic exposure to <span class="hlt">volcanic</span> air pollution and DNA damage in Furnas Volcano (São Miguel Island, Azores, Portugal) inhabitants</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Linhares, Diana; Garcia, Patricia; Silva, Catarina; Ferreira, Teresa; Barroso, Joana; Camarinho, Ricardo; Rodrigues, Armindo</p> <p>2015-04-01</p> <p>Many studies in <span class="hlt">volcanic</span> air pollution only have in consideration the acute toxic effects of gas or ash releases however the impact of chronic exposure to ground gas emissions in human health is yet poorly known. In the Azores archipelago (Portugal), São Miguel island has one of the most <span class="hlt">active</span> and dangerous volcanoes: Furnas Volcano. Highly <span class="hlt">active</span> fumarolic fields, hot springs and soil diffuse degassing phenomena are the main secondary <span class="hlt">volcanic</span> phenomena that can be seen at the volcano surroundings. One of the main gases released in these diffuse degassing areas is radon (222Rn), which decay results in solid particles that readily settle within the airways. These decay particles emit alpha radiation that is capable of causing severe DNA damage that cumulatively can eventually cause cancer. Previous studies have established that chronic exposure to chromosome-damaging agents can lead to the formation of nuclear anomalies, such as micronuclei that is used for monitoring DNA damage in human populations. The present study was designed to evaluate whether chronic exposure to <span class="hlt">volcanic</span> air pollution, associated to 222Rn, might result in DNA damage in human oral epithelial cells. A cross sectional study was performed in a study group of 142 individuals inhabiting an area where <span class="hlt">volcanic</span> <span class="hlt">activity</span> is marked by <span class="hlt">active</span> fumarolic fields and soil degassing (<span class="hlt">hydrothermal</span> area), and a reference group of 368 individuals inhabiting an area without these secondary manifestations of <span class="hlt">volcanism</span> (<span class="hlt">non-hydrothermal</span> area). For each individual, 1000 buccal epithelial cells were analyzed for the frequency of micronucleated cells (MNc) and the frequency of cells with other nuclear anomalies (ONA: pyknosis, karyolysis and karyorrhexis), by using the micronucleus assay. Information on lifestyle factors and an informed consent were obtained from each participant. Assessment of indoor radon was performed with the use of radon detectors. Data were analyzed with logistic regression models, adjusted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.V52A1037M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.V52A1037M"><span>The Online GVP/USGS Weekly <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Report: Providing Timely Information About Worldwide <span class="hlt">Volcanism</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mayberry, G. C.; Guffanti, M. C.; Luhr, J. F.; Venzke, E. A.; Wunderman, R. L.</p> <p>2001-12-01</p> <p>The awesome power and intricate inner workings of volcanoes have made them a popular subject with scientists and the general public alike. About 1500 known volcanoes have been <span class="hlt">active</span> on Earth during the Holocene, approximately 50 of which erupt per year. With so much <span class="hlt">activity</span> occurring around the world, often in remote locations, it can be difficult to find up-to-date information about current <span class="hlt">volcanism</span> from a reliable source. To satisfy the desire for timely volcano-related information the Smithsonian Institution and US Geological Survey combined their strengths to create the Weekly <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Report. The Smithsonian's Global <span class="hlt">Volcanism</span> Program (GVP) has developed a network of correspondents while reporting worldwide <span class="hlt">volcanism</span> for over 30 years in their monthly Bulletin of the Global <span class="hlt">Volcanism</span> Network. The US Geological Survey's Volcano Hazards Program studies and monitors volcanoes in the United States and responds (upon invitation) to selected <span class="hlt">volcanic</span> crises in other countries. The Weekly <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Report is one of the most popular sites on both organization's websites. The core of the Weekly <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Report is the brief summaries of current <span class="hlt">volcanic</span> <span class="hlt">activity</span> around the world. In addition to discussing various types of <span class="hlt">volcanism</span>, the summaries also describe precursory <span class="hlt">activity</span> (e.g. <span class="hlt">volcanic</span> seismicity, deformation, and gas emissions), secondary <span class="hlt">activity</span> (e.g. debris flows, mass wasting, and rockfalls), <span class="hlt">volcanic</span> ash hazards to aviation, and preventative measures. The summaries are supplemented by links to definitions of technical terms found in the USGS photoglossary of volcano terms, links to information sources, and background information about reported volcanoes. The site also includes maps that highlight the location of reported volcanoes, an archive of weekly reports sorted by volcano and date, and links to commonly used acronyms. Since the Weekly <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Report's inception in November 2000, <span class="hlt">activity</span> has been reported at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6579B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6579B"><span>Silicon isotopes fractionation in meteoric chemical weathering and <span class="hlt">hydrothermal</span> alteration systems of <span class="hlt">volcanic</span> rocks (Mayotte)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Basile-Doelsch, Isabelle; Puyraveau, Romain-Arnaud; Guihou, Abel; Haurine, Frederic; Deschamps, Pierre; rad, Setareh; Nehlig, Pierre</p> <p>2017-04-01</p> <p>Low temperature chemical weathering fractionates silicon (Si) isotopes while forming secondary silicates. The Si fractionation ranges of high temperature secondary phyllosilicates formed in <span class="hlt">hydrothermal</span> alteration environments have not been investigated to date. Several parameters, including temperature, reaction rates, pH, ionic concentrations in solution, precipitation/dissolution series or kinetic versus equilibrium regime are not the same in <span class="hlt">hydrothermal</span> alteration and surface weathering systems and may lead to different fractionation factors. In this work, we analyzed Si isotopes in these two types of alteration conditions in two profiles sampled on the <span class="hlt">volcanic</span> island of Mayotte. In both profiles, Si-bearing secondary mineral was kaolinite. Both profiles showed 30Si depletion as a function of the degree of alteration but each with a distinct pattern. In the meteoric weathering profile, from the bottom to the top, a gradual decrease of the δ30Si from parent rock (-0.29 ± 0.13 ‰) towards the most weathered product (-2.05 ± 0.13 ‰) was observed. In the <span class="hlt">hydrothermal</span> alteration profile, in which meteoric weathering was also superimposed at the top of the profile, an abrupt transition of the δ30Si was measured at the interface between parent-rock (-0.21 ± 0.11 ‰) and the altered products, with a minimum value of -3.06 ± 0.16 ‰˙ At the scale of Si-bearing secondary minerals, in the chemical weathering system, a Δ30Sikaol-parentrock of -1.9 ‰ was observed, in agreement with results in the literature. A low temperature kinetic fractionation 30ɛ of -2.29 ‰ was calculated using a simple steady state model. However, an unexpected Δ30Sikaol-parentrock of -2.85 ‰ was measured in the <span class="hlt">hydrothermal</span> alteration site, pointing to possible mechanisms linked to dissolution/precipitation series and/or to ionic composition of the solution as the main controlling factors of fractionation in <span class="hlt">hydrothermal</span> conditions. At the scale of the profiles, both δ30Si</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('http://adsabs.harvard.edu/abs/2018JVGR..352...38M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..352...38M"><span>Geochemical characterisation of Taal volcano-<span class="hlt">hydrothermal</span> system and temporal evolution during continued phases of unrest (1991-2017)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maussen, Katharine; Villacorte, Edgardo; Rebadulla, Ryan R.; Maximo, Raymond Patrick; Debaille, Vinciane; Bornas, Ma. Antonia; Bernard, Alain</p> <p>2018-02-01</p> <p>Taal volcano (Luzon Island, Philippines) has last erupted in 1977 but has known some periods of increased <span class="hlt">activity</span>, characterised by seismic swarms, ground deformation, increased carbon dioxide flux and in some cases temperature anomalies and the opening of fissures. We studied major, trace element and sulphur and strontium isotopic composition of Taal lake waters and hot springs over a period of 25 years to investigate the geochemical evolution of Taal volcano's <span class="hlt">hydrothermal</span> system and its response to <span class="hlt">volcanic</span> unrest. Long-term evolution of Main Crater Lake (MCL) composition shows a slow but consistent decrease of acidity, SO4, Mg, Fe and Al concentrations and a trend from light to heavy sulphate, consistent with a general decrease of <span class="hlt">volcanic</span> gases dissolving in the <span class="hlt">hydrothermal</span> system. Na, K and Cl concentrations remain constant indicating a <span class="hlt">non-volcanic</span> origin for these elements. Sulphate and strontium isotopic data suggest this neutral chloride-rich component represents input of geothermal water into Taal <span class="hlt">hydrothermal</span> system. A significant deviation from the long-term baseline can be seen in two samples from 1995. That year, pH dropped from 2.6 to 2.2, F, Si and Fe concentrations increased and Na, K and Cl concentrations decreased. Sulphate was depleted in 34S and temperature was 4 °C above baseline level at the time of sampling. We attribute these changes to the shallow intrusion of a degassing magma body during the unrest in 1991-1994. More recent unrest periods have not caused significant changes in the geochemistry of Taal <span class="hlt">hydrothermal</span> waters and are therefore unlikely to have been triggered by shallow magma intrusion. A more likely cause for these events is thus pressurisation of the <span class="hlt">hydrothermal</span> reservoir by increasing degassing from a stagnant magma reservoir. Our study indicates that new magmatic intrusions that might lead to the next eruption of Taal volcano are expected to change the geochemistry of MCL in the same way as in 1994-1995, with the most</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.3231N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3231N"><span>The structural architecture of the Los Humeros <span class="hlt">volcanic</span> complex and geothermal field, Trans-Mexican <span class="hlt">Volcanic</span> Belt, Central Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norini, Gianluca; Groppelli, Gianluca; Sulpizio, Roberto; Carrasco Núñez, Gerardo; Davila Harris, Pablo</p> <p>2014-05-01</p> <p>The development of geothermal energy in Mexico is a very important goal, given the presence of a large heat anomaly, associated with the Trans-Mexican <span class="hlt">Volcanic</span> Belt, the renewability of the resource and the low environmental impact. The Quaternary Los Humeros <span class="hlt">volcanic</span> complex is an important geothermal target, whose evolution involved at least two caldera events, that alternated with other explosive and effusive <span class="hlt">activity</span>. The first caldera forming event was the 460 ka eruption that produced the Xaltipan ignimbrite and formed a 15-20 km wide caldera. The second collapse event occurred 100 ka with the formation of the Zaragoza ignimbrite and a nested 8-10 km wide caldera. The whole volcano structure, the style of the collapses and the exact location of the calderas scarps and ring faults are still a matter of debate. The Los Humeros volcano hosts the productive Los Humeros Geothermal Field, with an installed capacity of 40 MW and additional 75 MW power plants under construction. Recent models of the geothermal reservoir predict the existence of at least two reservoirs in the geothermal system, separated by impermeable rock units. Hydraulic connectivity and <span class="hlt">hydrothermal</span> fluids circulation occurs through faults and fractures, allowing deep steam to ascend while condensate flows descend. As a consequence, the plans for the exploration and exploitation of the geothermal reservoir have been based on the identification of the main channels for the circulation of <span class="hlt">hydrothermal</span> fluids, constituted by faults, so that the full comprehension of the structural architecture of the caldera is crucial to improve the efficiency and minimize the costs of the geothermal field operation. In this study, we present an analysis of the Los Humeros <span class="hlt">volcanic</span> complex focused on the Quaternary tectonic and volcanotectonics features, like fault scarps and aligned/elongated monogenetic <span class="hlt">volcanic</span> centres. Morphostructural analysis and field mapping reveal the geometry, kinematics and dynamics of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/143826-redox-control-gas-compositions-philippine-volcanic-hydrothermal-systems','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/143826-redox-control-gas-compositions-philippine-volcanic-hydrothermal-systems"><span>Redox control of gas compositions in Philippine <span class="hlt">volcanic-hydrothermal</span> systems</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>Giggenbach, W.F.</p> <p>1993-10-01</p> <p>Gas samples from five <span class="hlt">volcanic-hydrothermal</span> systems in the Philippines were analyzed for CO{sub 2}, H{sub 2}S, NH{sub 3}, H{sub 2}, He, Ne, Ar, N{sub 2}, CH{sub 4} and CO. Even in systems with sulfate minerals as common components of alteration assemblages, indicating highly immature, oxidizing conditions at depth, the redox potential governing the concentrations of the reactive gases CO{sub 2}, H{sub 2}S, H{sub 2}, CH{sub 4} and CO approaches closely that expected for attainment of equilibrium with rock in more mature, reduced systems. The finding suggests that overall fluid compositions reflect more closely redox conditions established at the advancing frontmore » of interaction with primary rock rather than those of equilibrium with the set of secondary minerals left behind. With the exception of CO and NH{sub 3}, the close agreement in the compositions of gas samples, taken from pools and deep wells indicates that the secondary processes have only a slight effect on the vapors during their rise from drilled depths (1.8 km) to the surface and that samples from natural features may be taken to be representative of redox conditions at drilled depths.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12529639','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12529639"><span>Discovery of abundant <span class="hlt">hydrothermal</span> venting on the ultraslow-spreading Gakkel ridge in the Arctic Ocean.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Edmonds, H N; Michael, P J; Baker, E T; Connelly, D P; Snow, J E; Langmuir, C H; Dick, H J B; Mühe, R; German, C R; Graham, D W</p> <p>2003-01-16</p> <p>Submarine <span class="hlt">hydrothermal</span> venting along mid-ocean ridges is an important contributor to ridge thermal structure, and the global distribution of such vents has implications for heat and mass fluxes from the Earth's crust and mantle and for the biogeography of vent-endemic organisms. Previous studies have predicted that the incidence of <span class="hlt">hydrothermal</span> venting would be extremely low on ultraslow-spreading ridges (ridges with full spreading rates <2 cm x yr(-1)-which make up 25 per cent of the global ridge length), and that such vent systems would be hosted in ultramafic in addition to <span class="hlt">volcanic</span> rocks. Here we present evidence for <span class="hlt">active</span> <span class="hlt">hydrothermal</span> venting on the Gakkel ridge, which is the slowest spreading (0.6-1.3 cm x yr(-1)) and least explored mid-ocean ridge. On the basis of water column profiles of light scattering, temperature and manganese concentration along 1,100 km of the rift valley, we identify <span class="hlt">hydrothermal</span> plumes dispersing from at least nine to twelve discrete vent sites. Our discovery of such abundant venting, and its apparent localization near <span class="hlt">volcanic</span> centres, requires a reassessment of the geologic conditions that control <span class="hlt">hydrothermal</span> circulation on ultraslow-spreading ridges.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.4647M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.4647M"><span>Geochemical and thermodynamic specificity of <span class="hlt">volcanic</span>, <span class="hlt">hydrothermal</span> and soil aerosols</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mukhamadiyarova, Renata V.; Alekhin, Yury V.; Karpov, Gennady A.; Makarova, Marina A.</p> <p>2010-05-01</p> <p>On the basis of element composition analyses results (ICP-MS) of <span class="hlt">hydrothermal</span> and soil aerosols condensates, and also results of diagnostics of ultradisperse phases by means of power dispersive x-ray spectrometers features of phase and microelement composition of issue aerosols are discussed. Our researches of streams of polyelement issue from a soil cover and specificity of structure of <span class="hlt">volcanic</span> aerosols have led us to a conclusion that is geochemistry area practically is not developed in the relation of microelement migration in lithosphere - atmosphere. Nanoaerosol particles (0,001 - 1 microns) submit to laws of gas dynamics and in fluid streams are steady enough. Experimental researches of polyelement emission streams from soils and low-temperature microelements migration have allowed to detail the reasons of rather high values of the soil issue. Complexity of authentic definition of forms of carrying over, structure and dispersion of particles of the gas phase emitting from a soil cover, is substantially connected with absence of methodically well-founded receptions of selection of water condensates, free from aerosol components, and methods of their reliable division in a stationary stage of processes of issue and condensation. Reception of the information on factors of distribution of metals between pore solutions, true gas complexes and mineral phases of soils, an estimation of a role gas electrophoresis at transition to molecular cluster and to water colloid aerosols (0.1 microns and less) have allowed us to clear up estimations of streams of soil issue. The differentiation of a multicomponent gas phase in near surface conditions at powerful Tolbachinsky eruption (PTE) 1975 - 1976 to formation of many native metals - gold, silver, copper, lead, bismuth, tungsten, numerous intermetallic compounds. In eruption ashes of Kamchatka volcanoes - Karymsky, Bezymyanny, Kljuchevskoy and Shivelutch we found not only iron oxides but also numerous grains of native</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010LPICo1538.5257S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010LPICo1538.5257S"><span>Differential Bacterial Colonization of <span class="hlt">Volcanic</span> Minerals in Deep Thermal Basalts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, A. R.; Popa, R.; Fisk, M. R.; Nielsen, M.; Wheat, G.; Jannasch, H.; Fisher, A.; Sievert, S.</p> <p>2010-04-01</p> <p>There are reports of microbial weathering patterns in <span class="hlt">volcanic</span> glass and minerals of both terrestrial and Martian origin. <span class="hlt">Volcanic</span> minerals are colonized differentially in subsurface <span class="hlt">hydrothermal</span> environments by a variety of physiological types.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3741630','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3741630"><span>New insights into <span class="hlt">hydrothermal</span> vent processes in the unique shallow-submarine arc-volcano, Kolumbo (Santorini), Greece</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kilias, Stephanos P.; Nomikou, Paraskevi; Papanikolaou, Dimitrios; Polymenakou, Paraskevi N.; Godelitsas, Athanasios; Argyraki, Ariadne; Carey, Steven; Gamaletsos, Platon; Mertzimekis, Theo J.; Stathopoulou, Eleni; Goettlicher, Joerg; Steininger, Ralph; Betzelou, Konstantina; Livanos, Isidoros; Christakis, Christos; Bell, Katherine Croff; Scoullos, Michael</p> <p>2013-01-01</p> <p>We report on integrated geomorphological, mineralogical, geochemical and biological investigations of the <span class="hlt">hydrothermal</span> vent field located on the floor of the density-stratified acidic (pH ~ 5) crater of the Kolumbo shallow-submarine arc-volcano, near Santorini. Kolumbo features rare geodynamic setting at convergent boundaries, where arc-<span class="hlt">volcanism</span> and seafloor <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> are occurring in thinned continental crust. Special focus is given to unique enrichments of polymetallic spires in Sb and Tl (±Hg, As, Au, Ag, Zn) indicating a new hybrid seafloor analogue of epithermal-to-<span class="hlt">volcanic</span>-hosted-massive-sulphide deposits. Iron microbial-mat analyses reveal dominating ferrihydrite-type phases, and high-proportion of microbial sequences akin to "Nitrosopumilus maritimus", a mesophilic Thaumarchaeota strain capable of chemoautotrophic growth on <span class="hlt">hydrothermal</span> ammonia and CO2. Our findings highlight that acidic shallow-submarine <span class="hlt">hydrothermal</span> vents nourish marine ecosystems in which nitrifying Archaea are important and suggest ferrihydrite-type Fe3+-(hydrated)-oxyhydroxides in associated low-temperature iron mats are formed by anaerobic Fe2+-oxidation, dependent on microbially produced nitrate. PMID:23939372</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..346...28T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..346...28T"><span><span class="hlt">Hydrothermal</span> systems of the Karymsky <span class="hlt">Volcanic</span> Centre, Kamchatka: Geochemistry, time evolution and solute fluxes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taran, Yuri; Kalacheva, Elena; Inguaggiato, Salvatore; Cardellini, Carlo; Karpov, Gennady</p> <p>2017-10-01</p> <p>Karymsky <span class="hlt">Volcanic</span> Centre (KVC) at the middle of the frontal <span class="hlt">volcanic</span> chain of the Kamchatka arc consists of two joined calderas (Akademii Nauk and Karymsky volcano) and hosts two <span class="hlt">hydrothermal</span> systems: Akademii Nauk (AN) and Karymsky (K). The AN is a typical boiling system, with Na-Cl waters (TDS 1 g/l), low gas content (CO2-N2), with deep calculated temperatures of 200 °C. In contrast, springs of the K system have lower temperatures (up to 42 °C), strong gas bubbling, TDS 2.5 g/l, and are enriched in HCO3- and SO42 -, with Mg2 + as the main cation. There are two intriguing characteristics of the K field: (i) their CO2-rich gas (> 97 mol%) has the highest 3He/4He ratios ever measured for <span class="hlt">hydrothermal</span> systems in Kamchatka of 8 Ra (where Ra = 1.4 × 10- 6) and (ii) their thermal waters have an unusual cation composition (Mg > Na > Ca). After the 1996 sublimnic eruption within AN caldera, new hot springs appeared close to the eruption site. In this paper we synthesize all published and new geochemical data sets. The Karymsky Lake and post-1996 new thermal springs demonstrate exponential decreases in their main dissolved species, with a characteristic time of 5 to 8 years. The chemistry of AN and K springs did not change after the eruption. However, the concentration of chloride in the lake water approached 35 mg/l, compared with a background of 8-11 mg/l revealing a possible new source of hot water within the Karymsky Lake. All thermal fields of the KVC are drained by the Karymsky River with an outflow rate at the source of 2 m3/s (flowing out from Karymsky Lake) and at the exit from the Karymsky caldera of 4.5 m3/s. Using the measured solute fluxes at the source (AN springs) and at the exit (AN + K springs) the natural heat flux from the two systems can be estimated as 67 MW and 120 MW, respectively, and ≥ 20 t/d for the chloride output from both systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V51F0433Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V51F0433Y"><span>Impact of <span class="hlt">hydrothermal</span> alteration on time-dependent tunnel deformation in Neogene <span class="hlt">volcanic</span> rock sequence in Japan: Petrology, Geochemistry and Geophysical investigation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamazaki, S.; Okazaki, K.; Niwa, H.; Arai, T.; Murayama, H.; Kurahashi, T.; Ito, Y.</p> <p>2017-12-01</p> <p>Time-dependent tunnel deformation is one of remaining geological problems for mountain tunneling. As a case study of time-dependent tunnel deformation, we investigated petrographical, mineral and chemical compositions of boring core samples and seismic exploration along a tunnel that constructed into Neogene <span class="hlt">volcanic</span> rock sequence of andesite to dacite pyroclastic rocks and massive lavas with mafic enclaves. The tunnel has two zones of floor heaving that deformed time-dependently about 2 month after the tunnel excavation. The core samples around the deformed zones are characterized secondary mineral assemblages of smectite, cristobalite, tridymite, sulfides (pyrite and marcasite) and partially or completely reacted carbonates (calcite and siderite), which were formed by <span class="hlt">hydrothermal</span> alteration under neutral to acidic condition below about 100 °C. The core samples also showed localized deterioration, such as crack formation and expansion, which occurred from few days to months after the drilling. The deterioration could be explained as a result of the cyclic physical and chemical weathering process with the oxidation of sulfide minerals, dissolution of carbonate mineral cementation and volumetric expantion of smectite. This weathering process is considered as a key factor for time-dependent tunnel deformation in the <span class="hlt">hydrothermally</span> altered <span class="hlt">volcanic</span> rocks. The zones of time-dependent deformation along a tunnel route can be predicted by the variations of whole-rock chemical compositions such as Na, Ca, Sr, Ba and S.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S53B0690Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S53B0690Y"><span>Earthquake swarm in the <span class="hlt">non-volcanic</span> area north of Harrat Lunayyir, western Saudi Arabia: observations and imaging</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Youssof, M.; Mai, P. M.; Parisi, L.; Tang, Z.; Zahran, H. M.; El-Hadidy, S. Y.; Al-Raddadi, W.; Sami, M.; El-Hadidy, M. S. Y.</p> <p>2017-12-01</p> <p>We report on an unusual earthquake swarm in a <span class="hlt">non-volcanic</span> area of western Saudi Arabia. Since March 2017, hundreds of earthquakes were recorded, reaching magnitude Ml 3.7, which occurred within a very narrowly defined rock volume. The seismicity is shallow, mostly between 4 to 8 km depths, with some events reaching as deep as 16 km. One set of events aligns into a well-defined horizontal tube of 2 km height, 1 km width, and 4-5 km E-W extent. Other event clusters exist, but are less well-defined. The focal mechanism solutions of the largest earthquakes indicate normal faulting, which agree with the regional stress field. The earthquake swarm occurs 75 km NW of Harrat Lunayyir. However, the area of interest doesn't seem to be associated with the well-known <span class="hlt">volcanic</span> area of Harrat Lunayyir, which experienced a magmatic dike intrusion in 2009 with intense seismic <span class="hlt">activity</span> (including a surface rupturing Mw 5.7 earthquake). Furthermore, the study area is characterized by a complex shear system, which host gold mineralization. Therefore, the exact origin of the swarm sequence is enigmatic as it's the first of its kind in this region. By using continuous seismological data recorded by the Saudi Geological Survey (SGS) that operates three permanent seismic stations and a temporary network of 11 broadband sensors, we analyze the seismic patterns in space and time. For the verified detected events, we assemble the body wave arrival times that are inverted for the velocity structures along with events hypocenters to investigate possible causes of this swarm sequence, that is, whether the <span class="hlt">activity</span> is of tectonic- or <span class="hlt">hydro-thermal</span> origin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JVGR..296...40K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JVGR..296...40K"><span>Geochemistry and solute fluxes of volcano-<span class="hlt">hydrothermal</span> systems of Shiashkotan, Kuril Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kalacheva, Elena; Taran, Yuri; Kotenko, Tatiana</p> <p>2015-04-01</p> <p>Shiashkotan Island belongs to the Northern Kuril island arc and consists of two joined volcanoes, Sinarka and Kuntomintar, with about 18 km of distance between the summits. Both volcanoes are <span class="hlt">active</span>, with historic eruptions, and both emit fumarolic gases. Sinarka volcano is degassing through the extrusive dome with inaccessible strong and hot (> 400 °C) fumaroles. A large fumarolic field of the Kuntomintar volcano situated in a wide eroded caldera-like crater hosts many fumarolic vents with temperatures from boiling point to 480 °C. Both volcanoes are characterized by intense <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> discharging acid SO4-Cl waters, which are drained to the Sea of Okhotsk by streams. At least 4 groups of near-neutral Na-Mg-Ca-Cl-SO4 springs with temperatures in the range of 50-80 °C are located at the sea level, within tide zones and discharge slightly altered diluted seawater. <span class="hlt">Volcanic</span> gas of Kuntomintar as well as all types of <span class="hlt">hydrothermal</span> manifestations of both volcanoes were collected and analyzed for major and trace elements and water isotopes. <span class="hlt">Volcanic</span> gases are typical for arc volcanoes with 3He/4He corrected for air contamination up to 6.4 Ra (Ra = 1.4 × 10- 6, the air ratio) and δ13C (CO2) within - 10‰ to - 8 ‰ VPDB. Using a saturation indices approach it is shown that acid <span class="hlt">volcanic</span> waters are formed at a shallow level, whereas waters of the coastal springs are partially equilibrated with rocks at ~ 180 °C. Trace element distribution and concentrations and the total REE depend on the water type, acidity and Al + Fe concentration. The REE pattern for acidic waters is unusual but similar to that found in some acidic crater lake waters. The total <span class="hlt">hydrothermal</span> discharge of Cl and S from the island associated with <span class="hlt">volcanic</span> <span class="hlt">activity</span> is estimated at ca. 20 t/d and 40 t/d, respectively, based on the measurements of flow rates of the draining streams and their chemistry. The chemical erosion of the island by surface and thermal waters is estimated at 27 and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.V31B2142V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.V31B2142V"><span>Mercury and Iodine systematics of <span class="hlt">volcanic</span> arc fluids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Varekamp, J. C.; Kading, T.; Fehn, U.; Lu, Z.</p> <p>2008-12-01</p> <p>The mantle has low Mercury and Iodine concentrations, but these elements occur in <span class="hlt">volcanic</span> gases and <span class="hlt">hydrothermal</span> fluids at ppb (Hg) and ppm (Iodine) levels. Possibly, the Hg and Iodine concentrations in <span class="hlt">volcanic</span> fluids reflect subducted sediment sources in arc magmas. Iodine is a biophilic element, and I129/I values indicate that subducted sediment (especially organic matter) is an important Iodine source for arc magmas. It is uncertain if this is true for Hg as well, although in the surface environment Hg is commonly associated with organic matter. We present 60 new analyses of Hg and I in fluids from volcanoes in Central America, New Zealand, Japan, and the Cascades. A first assessment suggests that Iodine is released to some degree in the early stage of subduction in the forearc, whereas Hg may be released largely below the main <span class="hlt">volcanic</span> arc. Isotope and trace element signatures of <span class="hlt">volcanic</span> rocks of the investigated volcanoes show no simple correlation with Hg or Iodine abundances. The acid hot spring fluids of Copahue volcano (Argentina) carried ~ 200 ppt Hg in January 1999, ~80 ppt Hg in March 2008, and 90 ppt Hg in the crater lake in March 1997. The dissolved Hg fluxes from the Copahue <span class="hlt">hydrothermal</span> system are ~300 gr Hg/year in 1999 and ~130 gr Hg/year in 2008. The bulk <span class="hlt">hydrothermal</span> Hg flux (particle bound+dissolved) in 2008 was ~ 350 gr Hg/year. The potential Mercury evasion from these <span class="hlt">hydrothermal</span> spring fluids into the air has not yet been incorporated in these estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189737','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189737"><span>Kawah Ijen <span class="hlt">volcanic</span> <span class="hlt">activity</span>: A review</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Caudron, Corentin; Syahbana, Devy Kamil; Lecocq, Thomas; van Hinsberg, Vincent; McCausland, Wendy; Triantafyllou, Antoine; Camelbeeck, Thierry; Bernard, Alain; Surono,</p> <p>2015-01-01</p> <p>Kawah Ijen is a composite volcano located at the easternmost part of Java island in Indonesia and hosts the largest natural acidic lake in the world. We have gathered all available historical reports on Kawah Ijen’s <span class="hlt">activity</span> since 1770 with the purpose of reviewing the temporal evolution of its <span class="hlt">activity</span>. Most of these observations and studies have been conducted from a geochemical perspective and in punctuated scientific campaigns. Starting in 1991, the seismic <span class="hlt">activity</span> and a set of <span class="hlt">volcanic</span> lake parameters began to be weekly available. We present a database of those measurements that, combined with historical reports, allow us to review each eruption/unrest that occurred during the last two centuries. As of 2010, the <span class="hlt">volcanic</span> <span class="hlt">activity</span> is monitored by a new multi-disciplinary network, including digital seismic stations, and lake level and temperature measurements. This detailed monitoring provides an opportunity for better classifying seismic events and forecasting <span class="hlt">volcanic</span> unrest at Kawah Ijen, but only with the understanding of the characteristics of this <span class="hlt">volcanic</span> system gained from the historical review presented here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/8204','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/8204"><span>Field Trip Guide to Serpentinite, Silica-Carbonate Alteration, and Related <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> in the Clear Lake Region, California</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>Fraser Goff; George Guthrie</p> <p>1999-06-01</p> <p>This guide is designed to familiarize scientists with the geology, structure, alteration, and fluids typical of California serpentinites for purposes of carbon dioxide sequestration (Lackner et al., 1995). Goff et al. (1997) and Goff and Lackner (1998) describe the geology and geochemistry of some of the serpentinites from this area. Mechanisms of silica-carbonate alteration were outlined by Barnes et al. (1973). Donnelly-Nolan et al. (1993) most recently reviewed relations between regional <span class="hlt">hydrothermal</span> alteration and Quarternary <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Stanley et al. (1998) summarized geophysical characteristics of the region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JVGR..148..315T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JVGR..148..315T"><span>The <span class="hlt">hydrothermal-volcanic</span> system of Rincon de la Vieja volcano (Costa Rica): A combined (inorganic and organic) geochemical approach to understanding the origin of the fluid discharges and its possible application to <span class="hlt">volcanic</span> surveillance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tassi, F.; Vaselli, O.; Capaccioni, B.; Giolito, C.; Duarte, E.; Fernandez, E.; Minissale, A.; Magro, G.</p> <p>2005-12-01</p> <p>In the period 1998-2002 thermal spring discharges of Rincon de la Vieja volcano (NW Costa Rica) have been sampled and analyzed for major, trace and isotopic ( 18O/ 16O and D/H in waters and 3He/ 4He and 13C/ 12C in CO 2 in gases) composition. The boiling pools hosted inside the summit crater (<span class="hlt">Active</span> Crater) are characterized by high contents of magmatic-related compounds (SO 2, HCl and HF) that strongly affect the chemistry of the crater lake. These chemical features are not shown by the thermal discharges seeping out in the surrounding area of the volcano. Here, the shallow aquifer apparently masks any possible clues related to the magmatic system. This suggests that the fluid vents located inside the <span class="hlt">Active</span> Crater are likely to represent the most appropriate sampling sites for geochemical surveillance purposes, although the high gas discharge rate from the lake may occasionally prevent any fluid sampling. Alternatively, as already suggested by recent studies on the behavior of light hydrocarbons in different <span class="hlt">volcanic</span> environments, the compositional features of the organic gas fraction in the more accessible outer flank thermal discharges could usefully be utilized, at least, to assess the thermodynamic conditions of the <span class="hlt">volcanic-hydrothermal</span> system, since these compounds are affected by secondary processes only at limited extent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..344...65H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..344...65H"><span>Modelling ground deformation patterns associated with <span class="hlt">volcanic</span> processes at the Okataina <span class="hlt">Volcanic</span> Centre</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holden, L.; Cas, R.; Fournier, N.; Ailleres, L.</p> <p>2017-09-01</p> <p>The Okataina <span class="hlt">Volcanic</span> Centre (OVC) is one of two large <span class="hlt">active</span> rhyolite centres in the modern Taupo <span class="hlt">Volcanic</span> Zone (TVZ) in the North Island of New Zealand. It is located in a complex section of the Taupo rift, a tectonically <span class="hlt">active</span> section of the TVZ. The most recent <span class="hlt">volcanic</span> unrest at the OVC includes the 1315 CE Kaharoa and 1886 Tarawera eruptions. Current monitoring <span class="hlt">activity</span> at the OVC includes the use of continuous GPS receivers (cGPS), lake levelling and seismographs. The ground deformation patterns preceding <span class="hlt">volcanic</span> <span class="hlt">activity</span> the OVC are poorly constrained and restricted to predictions from basic modelling and comparison to other volcanoes worldwide. A better understanding of the deformation patterns preceding renewed <span class="hlt">volcanic</span> <span class="hlt">activity</span> is essential to determine if observed deformation is related to <span class="hlt">volcanic</span>, tectonic or <span class="hlt">hydrothermal</span> processes. Such an understanding also means that the ability of the present day cGPS network to detect these deformation patterns can also be assessed. The research presented here uses the finite element (FE) modelling technique to investigate ground deformation patterns associated with magma accumulation and diking processes at the OVC in greater detail. A number of FE models are produced and tested using Pylith software and incorporate characteristics of the 1315 CE Kaharoa and 1886 Tarawera eruptions, summarised from the existing body of research literature. The influence of a simple ring fault structure at the OVC on the modelled deformation is evaluated. The ability of the present-day continuous GPS (cGPS) GeoNet monitoring network to detect or observe the modelled deformation is also considered. The results show the modelled horizontal and vertical displacement fields have a number of key features, which include prominent lobe based regions extending northwest and southeast of the OVC. The results also show that the ring fault structure increases the magnitude of the displacements inside the caldera, in particular in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA218651','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA218651"><span>Fluid Flow and Sound Generation at <span class="hlt">Hydrothermal</span> Vent Fields</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1988-04-01</p> <p>Pacific Rise The first evidence of vent sound generation came from data collected near <span class="hlt">hydrothermal</span> vents at 21 N on the EPR where an array of ocean...associated with <span class="hlt">hydrothermal</span> centers, one at 21 N on the East Pacific Rise (EPR) (Reidesel et al., 1982) and one on the Juan de Fuca Ridge (Bibee and Jacobson... East Pacific Rise at 210 N : the <span class="hlt">volcanic</span>, tectonic and <span class="hlt">hydrothermal</span> processes at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..328...45M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..328...45M"><span>Gravity monitoring of Tatun <span class="hlt">Volcanic</span> Group <span class="hlt">activities</span> and inference for underground fluid circulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mouyen, Maxime; Chao, Benjamin Fong; Hwang, Cheinway; Hsieh, Wen-Chi</p> <p>2016-12-01</p> <p>The Tatun Volcano Group (TVG), located on the northern coast of Taiwan adjacent to the city of Taipei, experiences <span class="hlt">active</span> <span class="hlt">hydrothermalism</span> but has no historical record of <span class="hlt">volcanic</span> eruption. Yet recent studies suggest that TVG is dormant-<span class="hlt">active</span> rather than extinct. To monitor mass transfers and to gain further understanding of this <span class="hlt">volcanic</span> area, gravity variations have been recorded continuously since 2012 using a superconducting gravimeter, and once every few months since 2005 using absolute gravimeters. We analyze the continuous gravity time series and propose a model that best explains the gravity variations due to local groundwater redistribution. By correcting these variations, we identify gravity changes as large as 35 μGal that occurred concomitantly to fluid pressure-induced earthquakes and changes in the gas composition at Dayoukeng, one of TVG's fumaroles, over 2005-2007. We examine several fluid movements that can match the gravity observations, yet too few additional constraints exist to favor any of them. In particular, no significant ground displacements are observed when these gravity variations occurred. On the other hand, the model of gravity changes due to local groundwater redistribution can be routinely computed and removed from the ongoing time gravity measurements in order to quickly identify any unusual mass transfer occurring beneath TVG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912745M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912745M"><span>Gravity monitoring of Tatun <span class="hlt">Volcanic</span> Group <span class="hlt">activities</span> and inference for underground fluid circulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mouyen, Maxime; Chao, Benjamin; Hwang, Cheinway; Hsieh, Wen-Chi</p> <p>2017-04-01</p> <p>The Tatun Volcano Group (TVG), located on the northern coast of Taiwan adjacent to the city of Taipei, experiences <span class="hlt">active</span> <span class="hlt">hydrothermalism</span> but has no historical record of <span class="hlt">volcanic</span> eruption. Yet recent studies suggest that TVG is dormant-<span class="hlt">active</span> rather than extinct. To monitor mass transfers and to gain further understanding of this <span class="hlt">volcanic</span> area, gravity variations have been recorded continuously since 2012 using a superconducting gravimeter, and once every few months since 2005 using absolute gravimeters. We analyze the continuous gravity time series and propose a model that best explain the gravity variations due to local groundwater redistribution. By correcting these variations, we identify gravity changes as large as 35 µGal that occurred concomitantly to fluid pressure-induced earthquakes and changes in the gas composition at Dayoukeng, one of TVG's fumaroles, over 2005-2007. We examine several fluid movements that can match the gravity observations, yet too few additional constraints exist to favor any of them. In particular, no significant ground displacements are observed when these gravity variations occurred. On the other hand, the model of gravity changes due to local groundwater redistribution can be routinely computed and removed from the ongoing time gravity measurements in order to quickly identify any unusual mass transfer occurring beneath TVG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000GeCoA..64.1791C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000GeCoA..64.1791C"><span>PGE in fresh basalt, <span class="hlt">hydrothermal</span> alteration products, and <span class="hlt">volcanic</span> incrustations of Kilauea volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crocket, James H.</p> <p>2000-05-01</p> <p>The concentrations of Os, Ir, Pd, and Au in fresh unaltered Kilauean tholeiite were determined by radiochemical neutron <span class="hlt">activation</span> analysis. For a suite of 18 samples, averages were: Os = 0.38 ± 0.23, Ir = 0.38 ± 0.14, Pd = 2.40 ± 1.04, and Au = 1.78 ± 0.57 (in ppb with a 1σ SD). Correlations of these metals with Co, Cr, Cu, Ni, and MgO in fresh basalts, and petrographic observations, indicate that Os and Ir are carried mainly in chromite, much of which occurs as inclusions in olivine phenocrysts. Palladium correlations suggest its occurrence partly in olivine and partly in the matrix whereas Au seems to be predominantly a matrix constituent. Altered basalts were analyzed for Ir, Pd, and Au in a suite of 19 samples from five different locations. Minor changes only in either concentrations or element ratios were found for Ir and Pd when fresh and altered rock data were compared. However, Au was consistently enriched in altered relative to fresh rocks. These results imply that Pd and Ir, in contrast to Au, will likely retain their eruptive signatures upon burial in a subaerial eruptive setting. High-temperature sulfate-dominated condensates generate incrustations enriched in Ir, Os, Au, and Pd by approximately 50, 20, 10, and 3×, respectively, relative to fresh rocks. In contrast, low-temperature native sulfur deposits are the most depleted material found in the study with Ir, Pd, and Au lower by factors of 10, 4, and 5 compared with fresh rock averages. The strong enrichments of Os and Ir in the high-temperature suite are attributed mainly to enhanced volatility in highly oxygenated magmatic <span class="hlt">hydrothermal</span> fluids contaminated by meteoric water near the structural top of <span class="hlt">volcanic</span> conduits. The relatively smaller Pd enrichment, which is dependent on the chloride content of fluids, implies that PGE partitioning into <span class="hlt">volcanic</span> fume may fractionate these metals (e.g., Pd versus Ir) relative to host basalt in the eruptive process.</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('https://www.ncbi.nlm.nih.gov/pubmed/26213665','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26213665"><span>Laboratory simulations of acid-sulfate weathering under <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> conditions: Implications for early Mars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marcucci, Emma C; Hynek, Brian M</p> <p>2014-03-01</p> <p>We have completed laboratory experiments and thermochemical equilibrium models to investigate secondary mineral formation under conditions akin to <span class="hlt">volcanic</span>, <span class="hlt">hydrothermal</span> acid-sulfate weathering systems. Our research used the basaltic mineralogy at Cerro Negro Volcano, Nicaragua, characterized by plagioclase, pyroxene, olivine, and <span class="hlt">volcanic</span> glass. These individual minerals and whole-rock field samples were reacted in the laboratory with 1 molal sulfuric acid at varying temperatures (65, 150, and 200°C), fluid:rock weight ratios (1:1, 4:1, and 10:1), and durations (1-60 days). Thermochemical equilibrium models were developed using Geochemist's Workbench. To understand the reaction products and fluids, we employed scanning electron microscopy/energy dispersive spectroscopy, X-ray diffraction, and inductively coupled plasma-atomic emission spectroscopy. The results of our experiments and models yielded major alteration minerals that include anhydrite, natroalunite, minor iron oxide, and amorphous Al-Si gel. We found that variations in experimental parameters did not drastically change the suite of minerals produced; instead, abundance, size, and crystallographic shape changed. Our results also suggest that it is essential to separate phases formed during experiments from those formed during fluid evaporation to fully understand the reaction processes. Our laboratory reacted and model predicted products are consistent with the mineralogy observed at places on Mars. However, our results indicate that determination of the formation conditions requires microscopic imagery and regional context, as well as a thorough understanding of contributions from both experiment precipitation and fluid evaporation minerals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4508920','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4508920"><span>Laboratory simulations of acid-sulfate weathering under <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> conditions: Implications for early Mars</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Marcucci, Emma C; Hynek, Brian M</p> <p>2014-01-01</p> <p>We have completed laboratory experiments and thermochemical equilibrium models to investigate secondary mineral formation under conditions akin to <span class="hlt">volcanic</span>, <span class="hlt">hydrothermal</span> acid-sulfate weathering systems. Our research used the basaltic mineralogy at Cerro Negro Volcano, Nicaragua, characterized by plagioclase, pyroxene, olivine, and <span class="hlt">volcanic</span> glass. These individual minerals and whole-rock field samples were reacted in the laboratory with 1 molal sulfuric acid at varying temperatures (65, 150, and 200°C), fluid:rock weight ratios (1:1, 4:1, and 10:1), and durations (1–60 days). Thermochemical equilibrium models were developed using Geochemist's Workbench. To understand the reaction products and fluids, we employed scanning electron microscopy/energy dispersive spectroscopy, X-ray diffraction, and inductively coupled plasma-atomic emission spectroscopy. The results of our experiments and models yielded major alteration minerals that include anhydrite, natroalunite, minor iron oxide, and amorphous Al-Si gel. We found that variations in experimental parameters did not drastically change the suite of minerals produced; instead, abundance, size, and crystallographic shape changed. Our results also suggest that it is essential to separate phases formed during experiments from those formed during fluid evaporation to fully understand the reaction processes. Our laboratory reacted and model predicted products are consistent with the mineralogy observed at places on Mars. However, our results indicate that determination of the formation conditions requires microscopic imagery and regional context, as well as a thorough understanding of contributions from both experiment precipitation and fluid evaporation minerals. PMID:26213665</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRB..11212206C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRB..11212206C"><span>Thermal monitoring of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> by permanent infrared automatic stations: Results obtained at Solfatara di Pozzuoli, Campi Flegrei (Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chiodini, G.; Vilardo, G.; Augusti, V.; Granieri, D.; Caliro, S.; Minopoli, C.; Terranova, C.</p> <p>2007-12-01</p> <p>A permanent automatic infrared (IR) station was installed at Solfatara crater, the most <span class="hlt">active</span> zone of Campi Flegrei caldera. After a positive in situ calibration of the IR camera, we analyze 2175 thermal IR images of the same scene from 2004 to 2007. The scene includes a portion of the steam heated hot soils of Solfatara. The experiment was initiated to detect and quantify temperature changes of the shallow thermal structure of a quiescent volcano such as Solfatara over long periods. Ambient temperature is the main parameter affecting IR temperatures, while air humidity and rain control image quality. A geometric correction of the images was necessary to remove the effects of slow movement of the camera. After a suitable correction the images give a reliable and detailed picture of the temperature changes, over the period October 2004 to January 2007, which suggests that origin of the changes were linked to anthropogenic <span class="hlt">activity</span>, vegetation growth, and the increase of the flux of <span class="hlt">hydrothermal</span> fluids in the area of the hottest fumaroles. Two positive temperature anomalies were registered after the occurrence of two seismic swarms which affected the <span class="hlt">hydrothermal</span> system of Solfatara in October 2005 and October 2006. It is worth noting that these signs were detected in a system characterized by a low level of <span class="hlt">activity</span> with respect to systems affected by real <span class="hlt">volcanic</span> crisis where more spectacular results will be expected. Results of the experiment show that this kind of monitoring system can be a suitable tool for <span class="hlt">volcanic</span> surveillance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010DPS....42.3406E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010DPS....42.3406E"><span><span class="hlt">Active</span> and Recent <span class="hlt">Volcanism</span> and Hydrogeothermal <span class="hlt">Activity</span> on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edgett, Kenneth S.; Cantor, B. A.; Harrison, T. N.; Kennedy, M. R.; Lipkaman, L. J.; Malin, M. C.; Posiolova, L. V.; Shean, D. E.</p> <p>2010-10-01</p> <p>There are no <span class="hlt">active</span> volcanoes or geysers on Mars today, nor in the very recent past. Since 1997, we have sought evidence from targeted narrow angle camera images and daily, global wide angle images for <span class="hlt">active</span> or very recent (decades to < 10 Ma) <span class="hlt">volcanism</span> or hydrogeothermal events on Mars. Despite > 11 years of daily global imaging and coverage of > 60% of Mars at ≤ 6 m/pixel (with the remaining < 40% largely outside of <span class="hlt">volcanic</span> regions), we have found no such evidence, although one lava field in Aeolis (5°N, 220°W) stands out as possibly the site of the most recent <span class="hlt">volcanism</span>. Authors of impact crater size-frequency studies suggest some <span class="hlt">volcanic</span> landforms on Mars are as young as tens to hundreds of Ma. This interpreted youth has implications for understanding the internal geophysical state of Mars and has encouraged those seeking sources for trace gases (methane) in the atmosphere and those seeking "warm havens for life” (Jakosky 1996, New Scientist 150, 38-42). We targeted thousands of Mars Global Surveyor (MGS) MOC and Mars Reconnaissance Orbiter (MRO) CTX (and HiRISE) images to examine <span class="hlt">volcanic</span> regions; we also studied every MGS MOC and MRO MARCI wide angle image. For evidence of <span class="hlt">active</span> <span class="hlt">volcanism</span>, we sought eruption plumes, new vents, new tephra deposits, and new volcanogenic flows not observed in earlier images. For recent <span class="hlt">volcanism</span>, we sought volcanogenic flows with zero or few superposed impact craters and minimal regolith development or superposed eolian sediment. Targets included all <span class="hlt">volcanic</span> landforms identified in research papers as "recent” as well as areas speculated to have exhibited eruptive plumes. An independent search for endogenic heat sources, a key Mars Odyssey THEMIS objective, has also not produced a positive result (Christensen et al. 2005, P24A-01, Eos, Trans. Am. Geophys. Union 86/52).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7431H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7431H"><span>Diffuse CO_{2} degassing monitoring of the oceanic <span class="hlt">active</span> <span class="hlt">volcanic</span> island of El Hierro, Canary Islands, Spain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hernández, Pedro A.; Norrie, Janice; Withoos, Yannick; García-Merino, Marta; Melián, Gladys; Padrón, Eleazar; Barrancos, José; Padilla, Germán; Rodríguez, Fátima; Pérez, Nemesio M.</p> <p>2017-04-01</p> <p>Even during repose periods, volcanoes release large amounts of gases from both visible (fumaroles, solfataras, plumes) and <span class="hlt">non</span>-visible emanations (diffuse degassing). In the last 20 years, there has been considerable interest in the study of diffuse degassing as a powerful tool in volcano monitoring programs, particularly in those <span class="hlt">volcanic</span> areas where there are no visible <span class="hlt">volcanic-hydrothermal</span> gas emissions. Historically, soil gas and diffuse degassing surveys in <span class="hlt">volcanic</span> environments have focused mainly on CO2 because it is, after water vapor, the most abundant gas dissolved in magma. As CO2 travels upward by advective-diffusive transport mechanisms and manifests itself at the surface, changes in its flux pattern over time provide important information for monitoring <span class="hlt">volcanic</span> and seismic <span class="hlt">activity</span>. Since 1998, diffuse CO2 emission has been monitored at El Hierro Island, the smallest and south westernmost island of the Canarian archipelago with an area of 278 km2. As no visible emanations occur at the surface environment of El Hierro, diffuse degassing studies have become the most useful geochemical tool to monitor the <span class="hlt">volcanic</span> <span class="hlt">activity</span> in this <span class="hlt">volcanic</span> island. The island experienced a volcano-seismic unrest that began in July 2011, characterized by the location of a large number of relatively small earthquakes (M<2.5) beneath El Hierro at depths between 8 and 15 km. On October 12, 2011, a submarine eruption was confirmed during the afternoon of October 12, 2011 by visual observations off the coast of El Hierro, about 2 km south of the small village of La Restinga in the southernmost part of the island. During the pre-eruptive and eruptive periods, the time series of the diffuse CO2 emission released by the whole island experienced two significant increases. The first started almost 2 weeks before the onset of the submarine eruption, reflecting a clear geochemical anomaly in CO2 emission, most likely due to increasing release of deep seated magmatic gases to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912815C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912815C"><span>Monitoring diffuse <span class="hlt">volcanic</span> degassing during <span class="hlt">volcanic</span> unrests: the case of Campi Flegrei (Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cardellini, Carlo; Chiodini, Giovanni; Avino, Rosario; Bagnato, Emanuela; Caliro, Stefano; Frondini, Francesco; Lelli, Matteo; Rosiello, Angelo</p> <p>2017-04-01</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> at Solfatara of Pozzuoli (Campi Flegrei caldera, Italy) results on a large area of hot soils, diffuse CO2 degassing and numerous fumaroles, releasing at the surface large amounts of gasses and thermal energy. Solfatara is one of the first sites of the world where the techniques for measuring and interpreting soil CO2 diffuse degassing were developed during 1990's and, more recently, it has become a sort of natural laboratory for testing new types of measurements of the CO2 fluxes from <span class="hlt">hydrothermal</span> sites. The results of 30 diffuse CO2 flux surveys performed at Solfatara from 1998 to 2016 are presented and discussed. CO2 soil fluxes were measured over an area of about 1.2  1.2 km including the Solfatara crater and the <span class="hlt">hydrothermal</span> site of Pisciarelli using the accumulation chamber technique. Each survey consisted in a number of CO2 flux measurements varying from 372 to 583 resulting in a total of 13158 measurements. This data set is one of the largest dataset ever made in the world on a single degassing <span class="hlt">volcanic-hydrothermal</span> system. It is particularly relevant in the frame of volcanological sciences because it was acquired during a long period of unrest at Campi Flegrei caldera and because Solfatara release an amount of CO2 comparable to that released by medium-large <span class="hlt">volcanic</span> plumes. Statistical and geostatistical elaborations of CO2 flux data allowed to characterise the sources of soil diffuse degassing, to define the extent of the area interested by the release of <span class="hlt">hydrothermal</span> CO2 (Solfatara DDS) and to quantify the total amount of released CO2. During the last eighteen years relevant variations affected Solfatara degassing, and in particular the "background" CO2 emission , the extent of DDS and the total CO2 output, that may reflect variations in the subterraneous gas plume feeding the Solfatara and Pisciarelli emissions. In fact, the most relevant variations in Solfatara diffuse degassing well correlates with steam condensation and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021914','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021914"><span><span class="hlt">Active</span> <span class="hlt">Volcanism</span> on Io: Global Distribution and Variations in <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lopes-Gautier, R.; McEwen, A.S.; Smythe, W.B.; Geissler, P.E.; Kamp, L.; Davies, A.G.; Spencer, J.R.; Keszthelyi, L.; Carlson, R.; Leader, F.E.; Mehlman, R.; Soderblom, L.</p> <p>1999-01-01</p> <p>Io's <span class="hlt">volcanic</span> <span class="hlt">activity</span> has been monitored by instruments aboard the Galileo spacecraft since June 28, 1996. We present results from observations by the near-infrared mapping spectrometer (NIMS) for the first 10 orbits of Galileo, correlate them with results from the Solid State Imaging System (SSI) and from groundbased observations, and compare them to what was known about Io's <span class="hlt">volcanic</span> <span class="hlt">activity</span> from observations made during the two Voyager flybys in 1979. A total of 61 <span class="hlt">active</span> <span class="hlt">volcanic</span> centers have been identified from Voyager, groundbased, and Galileo observations. Of these, 41 are hot spots detected by NIMS and/or SSI. Another 25 locations were identified as possible <span class="hlt">active</span> <span class="hlt">volcanic</span> centers, mostly on the basis of observed surface changes. Hot spots are correlated with surface colors, particularly dark and red deposits, and generally anti-correlated with white, SO2-rich areas. Surface features corresponding to the hot spots, mostly calderas or flows, were identified from Galileo and Voyager images. Hot spot temperatures obtained from both NIMS and SSI are consistent with silicate <span class="hlt">volcanism</span>, which appears to be widespread on Io. Two types of hot spot <span class="hlt">activity</span> are present: persistent-type <span class="hlt">activity</span>, lasting from months to years, and sporadic events, which may represent either short-lived <span class="hlt">activity</span> or low-level <span class="hlt">activity</span> that occasionally flares up. Sporadic events are not often detected, but may make an important contribution to Io's heat flow and resurfacing. The distribution of <span class="hlt">active</span> <span class="hlt">volcanic</span> centers on the surface does not show any clear correlation with latitude, longitude, Voyager-derived global topography, or heat flow patterns predicted by the asthenosphere and deep mantle tidal dissipation models. However, persistent hot spots and <span class="hlt">active</span> plumes are concentrated toward lower latitudes, and this distribution favors the asthenosphere rather than the deep mantle tidal dissipation model. ?? 1999 Academic Press.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79...83M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79...83M"><span><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> and subsoil complexity: implication for degassing processes at Solfatara crater, Campi Flegrei caldera</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montanaro, Cristian; Mayer, Klaus; Isaia, Roberto; Gresse, Marceau; Scheu, Bettina; Yilmaz, Tim I.; Vandemeulebrouck, Jean; Ricci, Tullio; Dingwell, Donald B.</p> <p>2017-12-01</p> <p>The Solfatara area and its fumaroles are the main surface expression of the vigorous <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> within the <span class="hlt">active</span> Campi Flegrei caldera system. At depth, a range of <span class="hlt">volcanic</span> and structural processes dictate the actual state of the <span class="hlt">hydrothermal</span> system below the crater. The presence of a large variety of <span class="hlt">volcanic</span> products at shallow depth (including pyroclastic fallout ash beds, pyroclastic density current deposits, breccias, and lavas), and the existence of a maar-related fault system appears to exert major controls on the degassing and alteration behavior. Adding further to the complexity of this environment, variations in permeability and porosity, due to subsoil lithology and alteration effects, may further influence fluid flow towards the surface. Here, we report results from a field campaign conducted in July 2015 that was designed to characterize the in situ physical (temperature, humidity) and mechanical (permeability, strength, stiffness) properties of the Solfatara crater subsoil. The survey also included a mapping of the surficial <span class="hlt">hydrothermal</span> features and their distributions. Finally, laboratory measurements (porosity, granulometry) of selected samples were performed. Our results enable the discrimination of four main subsoils around the crater: (1) the Fangaia domain located in a topographic low in the southwestern sector, (2) the silica flat domain on the western altered side, (3) the new crust domain in the central area, and (4) the crusted hummocks domain that dominates the north, east, and south parts. These domains are surrounded by encrusted areas, reworked material, and vegetated soil. The distribution of these heterogeneous subsoils suggests that their formation is mostly related to (i) the presence of the Fangaia domain within the crater and (ii) a system of ring faults bordering it. The subsoils show an alternation between very high and very low permeabilities, a fact which seems to affect both the temperature distribution and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..357..399F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..357..399F"><span>The <span class="hlt">active</span> submarine NW termination of the South Aegean <span class="hlt">Active</span> <span class="hlt">Volcanic</span> Arc: The Submarine Pausanias <span class="hlt">Volcanic</span> Field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Foutrakis, Panagiotis M.; Anastasakis, George</p> <p>2018-05-01</p> <p>Methana peninsula shows the longest recorded <span class="hlt">volcanic</span> history at the western end of the South Aegean <span class="hlt">Active</span> <span class="hlt">Volcanic</span> Arc, including <span class="hlt">volcanic</span> products from the Upper Pliocene to recent times. The <span class="hlt">volcanic</span> rocks comprise widespread dacite domes and andesite lava flows from several small <span class="hlt">volcanic</span> centers and are only imprecisely dated. In this paper, the integrated analysis of swath bathymetry, side scan sonar data, and high resolution seismic reflection profiles correlated with core samples, has allowed detailed mapping, characterization and precise chronological identification of the Pausanias submarine <span class="hlt">volcanic</span> field <span class="hlt">activity</span> offshore northern Methana. Six <span class="hlt">volcanic</span> cones or domes are recognized, typically 1-3 km in diameter, some elongated NE-SW and some with a small central crater. On their flanks, the acoustically reflective <span class="hlt">volcanic</span> rocks pass laterally into incoherent transparent seismic facies interpreted as volcaniclastic deposits, possibly including hyaloclastites, that interfinger with the regional basin sediments. A sea-bottom hummocky field, is interpreted as <span class="hlt">volcanic</span> avalanche and appears to be the submarine continuation of the volcaniclastic apron of northern Methana peninsula. A robust chronostratigraphic framework has been established, based on the recognition of shoreline progradational units and their connection with Quaternary eustatic sea level cycles. Relative dating of the different phases of submarine <span class="hlt">volcanic</span> <span class="hlt">activity</span> during the Upper Quaternary has been achieved by correlating the imaged volcaniclastic flows, interlayered within the chronostratigraphically dated sediments. Dating by stratigraphic position, relative to 2D imaged eustatic sea level clinoform wedges appears to be more precise than radiometric methods on land. Three main submarine <span class="hlt">Volcanic</span> Events (VE) are recognized: VE3 at 450 ka, a less precisely dated interval at 200-130 ka (VE2), and VE1 at 14 ka. Based on chronostratigraphic constraints, subsidence rates of 0.16 (±0.008) m</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003TrGeo...6..181G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003TrGeo...6..181G"><span><span class="hlt">Hydrothermal</span> Processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>German, C. R.; von Damm, K. L.</p> <p>2003-12-01</p> <p> (after C. A. Stein and S. Stein, 1994). The first geochemical evidence for the existence of <span class="hlt">hydrothermal</span> vents on the ocean floor came in the mid-1960s when investigations in the Red Sea revealed deep basins filled with hot, salty water (40-60 °C) and underlain by thick layers of metal-rich sediment (Degens and Ross, 1969). Because the Red Sea represents a young, rifting, ocean basin it was speculated that the phenomena observed there might also prevail along other young MOR spreading centers. An analysis of core-top sediments from throughout the world's oceans ( Figure 2) revealed that such metalliferous sediments did, indeed, appear to be concentrated along the newly recognized global ridge crest (Boström et al., 1969). Another early indication of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> came from the detection of plumes of excess 3He in the Pacific Ocean Basin (Clarke et al., 1969) - notably the >2,000 km wide section in the South Pacific ( Lupton and Craig, 1981) - because 3He present in the deep ocean could only be sourced through some form of <span class="hlt">active</span> degassing of the Earth's interior, at the seafloor. (62K)Figure 2. Global map of the (Al+Fe+Mn):Al ratio for surficial marine sediments. Highest ratios mimic the trend of the global MOR axis (after Boström et al., 1969). One area where early heat-flow studies suggested <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> was likely to occur was along the Galapagos Spreading Center in the eastern equatorial Pacific Ocean (Anderson and Hobart, 1976). In 1977, scientists diving at this location found <span class="hlt">hydrothermal</span> fluids discharging chemically altered seawater from young <span class="hlt">volcanic</span> seafloor at elevated temperatures up to 17 °C ( Edmond et al., 1979). Two years later, the first high-temperature (380±30 °C) vent fluids were found at 21° N on the East Pacific Rise (EPR) (Spiess et al., 1980) - with fluid compositions remarkably close to those predicted from the lower-temperature Galapagos findings ( Edmond et al., 1979). Since that time, <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> has been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2007/5094/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2007/5094/"><span>Preliminary volcano-hazard assessment for the Tanaga <span class="hlt">volcanic</span> cluster, Tanaga Island, Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Coombs, Michelle L.; McGimsey, Robert G.; Browne, Brandon L.</p> <p>2007-01-01</p> <p>Summary of Volcano Hazards at Tanaga <span class="hlt">Volcanic</span> Cluster The Tanaga <span class="hlt">volcanic</span> cluster lies on the northwest part of Tanaga Island, about 100 kilometers west of Adak, Alaska, and 2,025 kilometers southwest of Anchorage, Alaska. The cluster consists of three volcanoes-from west to east, they are Sajaka, Tanaga, and Takawangha. All three volcanoes have erupted in the last 1,000 years, producing lava flows and tephra (ash) deposits. A much less frequent, but potentially more hazardous phenomenon, is <span class="hlt">volcanic</span> edifice collapse into the sea, which likely happens only on a timescale of every few thousands of years, at most. Parts of the <span class="hlt">volcanic</span> bedrock near Takawangha have been altered by <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and are prone to slope failure, but such events only present a local hazard. Given the <span class="hlt">volcanic</span> cluster's remote location, the primary hazard from the Tanaga volcanoes is airborne ash that could affect aircraft. In this report, we summarize the major <span class="hlt">volcanic</span> hazards associated with the Tanaga <span class="hlt">volcanic</span> cluster.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V43B2861B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V43B2861B"><span>Using <span class="hlt">Volcanic</span> Lightning Measurements to Discern Variations in Explosive <span class="hlt">Volcanic</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Behnke, S. A.; Thomas, R. J.; McNutt, S. R.; Edens, H. E.; Krehbiel, P. R.; Rison, W.</p> <p>2013-12-01</p> <p>VHF observations of <span class="hlt">volcanic</span> lightning have been made during the recent eruptions of Augustine Volcano (2006, Alaska, USA), Redoubt Volcano (2009, Alaska, USA), and Eyjafjallajökull (2010, Iceland). These show that electrical <span class="hlt">activity</span> occurs both on small scales at the vent of the volcano, concurrent with an eruptive event and on large scales throughout the eruption column during and subsequent to an eruptive event. The small-scale discharges at the vent of the volcano are often referred to as 'vent discharges' and are on the order of 10-100 meters in length and occur at rates on the order of 1000 per second. The high rate of vent discharges produces a distinct VHF signature that is sometimes referred to as 'continuous RF' radiation. VHF radiation from vent discharges has been observed at sensors placed as far as 100 km from the volcano. VHF and infrasound measurements have shown that vent discharges occur simultaneously with the onset of eruption, making their detection an unambiguous indicator of explosive <span class="hlt">volcanic</span> <span class="hlt">activity</span>. The fact that vent discharges are observed concurrent with explosive <span class="hlt">volcanic</span> <span class="hlt">activity</span> indicates that <span class="hlt">volcanic</span> ejecta are charged upon eruption. VHF observations have shown that the intensity of vent discharges varies between eruptive events, suggesting that fluctuations in eruptive processes affect the electrification processes giving rise to vent discharges. These fluctuations may be variations in eruptive vigor or variations in the type of eruption; however, the data obtained so far do not show a clear relationship between eruption parameters and the intensity or occurrence of vent discharges. Further study is needed to clarify the link between vent discharges and eruptive behavior, such as more detailed lightning observations concurrent with tephra measurements and other measures of eruptive strength. Observations of vent discharges, and <span class="hlt">volcanic</span> lightning observations in general, are a valuable tool for volcano monitoring, providing a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70160647','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70160647"><span><span class="hlt">Hydrothermal</span> response to a volcano-tectonic earthquake swarm, Lassen, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ingebritsen, Steven E.; Shelly, David R.; Hsieh, Paul A.; Clor, Laura; P.H. Seward,; Evans, William C.</p> <p>2015-01-01</p> <p>The increasing capability of seismic, geodetic, and <span class="hlt">hydrothermal</span> observation networks allows recognition of <span class="hlt">volcanic</span> unrest that could previously have gone undetected, creating an imperative to diagnose and interpret unrest episodes. A November 2014 earthquake swarm near Lassen <span class="hlt">Volcanic</span> National Park, California, which included the largest earthquake in the area in more than 60 years, was accompanied by a rarely observed outburst of <span class="hlt">hydrothermal</span> fluids. Although the earthquake swarm likely reflects upward migration of endogenous H2O-CO2 fluids in the source region, there is no evidence that such fluids emerged at the surface. Instead, shaking from the modest sized (moment magnitude 3.85) but proximal earthquake caused near-vent permeability increases that triggered increased outflow of <span class="hlt">hydrothermal</span> fluids already present and equilibrated in a local <span class="hlt">hydrothermal</span> aquifer. Long-term, multiparametric monitoring at Lassen and other well-instrumented volcanoes enhances interpretation of unrest and can provide a basis for detailed physical modeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V51F0436B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V51F0436B"><span>Fluid circulation and structural system of Cerritos Colorados geothermal field in La Primavera <span class="hlt">volcanic</span> caldera (Mexico) inferred from geophysical surveys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bolós, X.; Cifuentes-Nava, G.; Macias, J. L.; Sosa-Ceballos, G.; García-Tenorio, F.; Albor, M., III; Juarez, M.; Gamez, V.</p> <p>2017-12-01</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> in <span class="hlt">volcanic</span> calderas is the consequence of energy transfer between deep magmatic chambers and subsurface layers saturated in water. This <span class="hlt">hydrothermal</span> system is generated by convection of the groundwater supplied by meteoric water recharged and the ascent of hot <span class="hlt">volcanic</span> gasses exsolved from deep magma reservoirs. Calderas are heterogeneous geological structures that due to their formation and evolution produced a complex stratigraphy. All of these heterogeneities can be affected by deformation and also by the presence of fractures and faults which constitute the main pathways whereby <span class="hlt">hydrothermal</span> fluids can move easily through the surface as spring discharges and fumarolic <span class="hlt">activity</span>. Geophysical methods have been used in the last decades to investigate the relationship between structural geology and <span class="hlt">hydrothermal</span> systems in different <span class="hlt">volcanic</span> areas around the world. In this work, we have focused on the role of subsurface structures to understand and localize the pathways of fluids related to the <span class="hlt">hydrothermal</span> system of the Cerritos Colorados geothermal field. We focused in the central area of the caldera (P12 well and Cerritos Colorados graben), where <span class="hlt">active</span> <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> is evidenced by fumaroles, thermal anomalies, CO2 diffuse emission, and sulfur precipitation. We have applied a self-potential method (SP) that combined with temperature measurements that allowed to identify the main infiltration and ascending fluid zones in the area, and their specific surface temperature coinciding with fumarolic <span class="hlt">activity</span>. From this data we an applied Electrical Resistivity Tomography (ERT) survey in two selected places. One ERT profile (1.2 km in length) was located in the P12 well area. A 3D resistivity model used with the equatorial method was carried out on the Cerritos Colorados graben area. Combining the results of the SP, TºC, and ERT data with a detailed structural map we identified the main degassing zones (i.e. fumaroles) that correspond to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhDT.......165G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhDT.......165G"><span>Crustal deformation and <span class="hlt">volcanism</span> at <span class="hlt">active</span> plate boundaries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geirsson, Halldor</p> <p></p> <p>Most of Earth's volcanoes are located near <span class="hlt">active</span> tectonic plate boundaries, where the tectonic plates move relative to each other resulting in deformation. Likewise, subsurface magma movement and pressure changes in magmatic systems can cause measurable deformation of the Earth's surface. The study of the shape of Earth and therefore studies of surface deformation is called geodesy. Modern geodetic techniques allow precise measurements (˜1 mm accuracy) of deformation of tectonic and magmatic systems. Because of the spatial correlation between tectonic boundaries and <span class="hlt">volcanism</span>, the tectonic and <span class="hlt">volcanic</span> deformation signals can become intertwined. Thus it is often important to study both tectonic and <span class="hlt">volcanic</span> deformation processes simultaneously, when one is trying to study one of the systems individually. In this thesis, I present research on crustal deformation and magmatic processes at <span class="hlt">active</span> plate boundaries. The study areas cover divergent and transform plate boundaries in south Iceland and convergent and transform plate boundaries in Central America, specifically Nicaragua and El Salvador. The study is composed of four main chapters: two of the chapters focus on the magma plumbing system of Hekla volcano, Iceland and the plate boundary in south Iceland; one chapter focuses on shallow controls of explosive <span class="hlt">volcanism</span> at Telica volcano, Nicaragua; and the fourth chapter focuses on co- and post-seismic deformation from a Mw = 7.3 earthquake which occurred offshore El Salvador in 2012. Hekla volcano is located at the intersection of a transform zone and a rift zone in Iceland and thus is affected by a combination of shear and extensional strains, in addition to co-seismic and co-rifting deformation. The inter-eruptive deformation signal from Hekla is subtle, as observed by a decade (2000-2010) of GPS data in south Iceland. A simultaneous inversion of this data for parameters describing the geometry and source characteristics of the magma chamber at Hekla, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSM.V33A..04R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSM.V33A..04R"><span><span class="hlt">Volcanic</span> deformation in the Andes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riddick, S.; Fournier, T.; Pritchard, M.</p> <p>2009-05-01</p> <p>We present the results from an InSAR survey of <span class="hlt">volcanic</span> <span class="hlt">activity</span> in South America. We use data from the Japanese Space Agency's ALOS L-band radar satellite from 2006-2009. The L-band instrument provides better coherence in densely vegetated regions, compared to the shorter wave length C-band data. The survey reveals volcano related deformation in regions, north, central and southern, of the Andes <span class="hlt">volcanic</span> arc. Since observations are limited to the austral summer, comprehensive coverage of all volcanoes is not possible. Yet, our combined observations reveal <span class="hlt">volcanic/hydrothermal</span> deformation at Lonquimay, Llaima, Laguna del Maule, and Chaitén volcanoes, extend deformation measurements at Copahue, and illustrate temporal complexity to the previously described deformation at Cerro Hudson and Cordón Caulle. No precursory deformation is apparent before the large Chaitén eruption (VEI_5) of 2 May 2008, (at least before 16 April) suggesting rapid magma movement from depth at this long dormant volcano. Subsidence at Ticsani Volcano occurred coincident with an earthquake swarm in the same region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28383164','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28383164"><span>Ferrous iron- and ammonium-rich diffuse vents support habitat-specific communities in a shallow <span class="hlt">hydrothermal</span> field off the Basiluzzo Islet (Aeolian <span class="hlt">Volcanic</span> Archipelago).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bortoluzzi, G; Romeo, T; La Cono, V; La Spada, G; Smedile, F; Esposito, V; Sabatino, G; Di Bella, M; Canese, S; Scotti, G; Bo, M; Giuliano, L; Jones, D; Golyshin, P N; Yakimov, M M; Andaloro, F</p> <p>2017-09-01</p> <p>Ammonium- and Fe(II)-rich fluid flows, known from deep-sea <span class="hlt">hydrothermal</span> systems, have been extensively studied in the last decades and are considered as sites with high microbial diversity and <span class="hlt">activity</span>. Their shallow-submarine counterparts, despite their easier accessibility, have so far been under-investigated, and as a consequence, much less is known about microbial communities inhabiting these ecosystems. A field of shallow expulsion of <span class="hlt">hydrothermal</span> fluids has been discovered at depths of 170-400 meters off the base of the Basiluzzo Islet (Aeolian <span class="hlt">Volcanic</span> Archipelago, Southern Tyrrhenian Sea). This area consists predominantly of both <span class="hlt">actively</span> diffusing and inactive 1-3 meters-high structures in the form of vertical pinnacles, steeples and mounds covered by a thick orange to brown crust deposits hosting rich benthic fauna. Integrated morphological, mineralogical, and geochemical analyses revealed that, above all, these crusts are formed by ferrihydrite-type Fe 3+ oxyhydroxides. Two cruises in 2013 allowed us to monitor and sampled this novel ecosystem, certainly interesting in terms of shallow-water iron-rich site. The main objective of this work was to characterize the composition of extant communities of iron microbial mats in relation to the environmental setting and the observed patterns of macrofaunal colonization. We demonstrated that iron-rich deposits contain complex and stratified microbial communities with a high proportion of prokaryotes akin to ammonium- and iron-oxidizing chemoautotrophs, belonging to Thaumarchaeota, Nitrospira, and Zetaproteobacteria. Colonizers of iron-rich mounds, while composed of the common macrobenthic grazers, predators, filter-feeders, and tube-dwellers with no representatives of vent endemic fauna, differed from the surrounding populations. Thus, it is very likely that reduced electron donors (Fe 2+ and NH 4 + ) are important energy sources in supporting primary production in microbial mats, which form a habitat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29844515','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29844515"><span>Caldera unrest driven by CO2-induced drying of the deep <span class="hlt">hydrothermal</span> system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Moretti, R; Troise, C; Sarno, F; De Natale, G</p> <p>2018-05-29</p> <p>Interpreting <span class="hlt">volcanic</span> unrest is a highly challenging and <span class="hlt">non</span>-unique problem at calderas, since large <span class="hlt">hydrothermal</span> systems may either hide or amplify the dynamics of buried magma(s). Here we use the exceptional ground displacement and geochemical datasets from the <span class="hlt">actively</span> degassing Campi Flegrei caldera (Southern Italy) to show that ambiguities disappear when the thermal evolution of the deep <span class="hlt">hydrothermal</span> system is accurately tracked. By using temperatures from the CO 2 -CH 4 exchange of 13 C and thermodynamic analysis of gas ascending in the crust, we demonstrate that after the last 1982-84 crisis the deep <span class="hlt">hydrothermal</span> system evolved through supercritical conditions under the continuous isenthalpic inflow of hot CO 2 -rich gases released from the deep (~8 km) magma reservoir of regional size. This resulted in the drying of the base of the hot <span class="hlt">hydrothermal</span> system, no more buffered along the liquid-vapour equilibrium, and excludes any shallow arrival of new magma, whose abundant steam degassing due to decompression would have restored liquid-vapour equilibrium. The consequent CO 2 -infiltration and progressive heating of the surrounding deforming rock volume cause the build-up of pore pressure in aquifers, and generate the striking temporal symmetry that characterizes the ongoing uplift and the post-1984 subsidence, both originated by the same but reversed deformation mechanism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFMPP42C..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFMPP42C..06D"><span><span class="hlt">Hydrothermal</span> Links Between the Caribbean Plateau and OAE2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duncan, R. A.; Snow, L. J.</p> <p>2003-12-01</p> <p>A popular current model for the sporadic occurrence of ocean anoxic events (OAEs) in the Cretaceous ties <span class="hlt">hydrothermally</span>-induced changes in ocean chemistry (bio-limiting trace metals) during ocean plateau (LIP) <span class="hlt">volcanism</span> to increased surface productivity, followed by mid-to-deep water oxygen depletion and accumulation of organic-rich sediments. This proposed connection is far from accepted, and important unresolved aspects include the timing of events and yet-to-be-proved synchroneity of <span class="hlt">volcanism</span> and OAEs, the sensitivity of phytoplankton to bio-limiting (and toxic) trace metals, the difference in biotic responses at various OAEs, and the source of the <span class="hlt">hydrothermal</span> inputs (sea floor spreading centers or ocean plateaus). To test this hypothesis we have measured the distribution of major, minor and trace element abundances in five pelagic carbonate and black shale sequences that bracket the OAE2, defined by a prominent positive excursion in the global seawater d13C record. Sedimentary sections at Rock Creek Canyon (Pueblo, CO), ODP Site 1138 (Kerguelen Plateau), Bass River (NJ), Totuma well (Venezuela) and Baranca el Canyon (Mexico) were chosen to examine potential trace metal patterns and gradients around the proposed source of <span class="hlt">hydrothermal</span> inputs - the Caribbean Plateau, whose initial <span class="hlt">volcanic</span> <span class="hlt">activity</span> has been dated at 93-89 Ma. ICP-AES and ICP-MS elemental abundances from whole rock samples are normalized to Zr to remove the effect of terrestrial inputs. We find prominent trace metal "spikes" (up to 50 times background) for elements known to be concentrated in volatile degassing of magmas and in <span class="hlt">hydrothermal</span> plumes resulting from seawater-rock reactions. These anomalies begin at the onset and continue well into the d13C excusion at all five sites. Furthermore, the magnitude of the anomalies decreases with distance from the Caribbean region, and the pattern of elements shifts from a wide range of metals near-source to predominantly long residence time metals far</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988MarGR..10...91K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988MarGR..10...91K"><span>Geologic setting of the Snake Pit <span class="hlt">hydrothermal</span> site: An <span class="hlt">active</span> vent field on the Mid-Atlantic Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karson, Jeffrey A.; Brown, Jennifer R.</p> <p>1988-03-01</p> <p>The Snake Pit <span class="hlt">Hydrothermal</span> Site lies on the axis of the Mid-Atlantic Ridge at 23°22' N latitude, about 30 km south of the Kane Transform Intersection. <span class="hlt">Active</span> ‘black smoker’ vents and a surrounding field of <span class="hlt">hydrothermal</span> sediment occur at the crest of a laterally extensive neovolcanic ridge. It is one of the first <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vent fields to be found on a slow-spreading ridge axis and despite significant differences in its geologic setting from those of the East Pacific Rise, has many similarities to its fast-spreading counterparts. Although preliminary reports have documented many interesting aspects of these vents and their surroundings, new data collected from the manned submersible ALVIN and the deep-towed ANGUS camera system define the regional tectonic setting as well as the local geologic environment of this fascinating area. The Snake Pit vents are located on a local peak of a <span class="hlt">volcanic</span> constructional ridge at a depth of 3450 m, 700 800 m deeper than vents known from the East Pacific Rise, Galapagos, or Juan de Fuca spreading centers. The vent field is at least 600 m long and up to 200 m wide and is covered by a thick blanket of greenish to yellow-orange <span class="hlt">hydrothermal</span> sediment. Both <span class="hlt">active</span> and extinct vents are perched along the crests of steep-sided sulfide mounds that reach heights of over 40 m. High-temperature (350° C) fluids are vented from black smoker chimneys and low-temperature (226° C) fluids seep from sulphide domes and subordinate anhydrite constructions. Water temperatures, flow rates, fluid chemistries, and mineralization are strikingly similar to vents of faster spreading ridge crests; however, a somewhat distinct fauna inhabit the area.</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('http://adsabs.harvard.edu/abs/2016AGUFM.V23D3022J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V23D3022J"><span>Investigations of the geochemical controls on anomalous arsenic enrichment in the Santiago Peak <span class="hlt">Volcanics</span> of Southern California: implications for arsenic distribution in <span class="hlt">volcanic</span> arc systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnston, E. C.; Pollock, M.; Cathcart, E. M.; AlBashaireh, A.; O'shea, B. M.</p> <p>2016-12-01</p> <p>The Santiago Peak <span class="hlt">Volcanics</span> (SPV) of Southern CA and Northern Baja CA, Mexico are remnants of a Cretaceous subaerial <span class="hlt">volcanic</span> arc system that underwent greenschist facies metamorphism contemporaneous with <span class="hlt">volcanism</span>. Observed SPV exposed at the surface of Black Mountain Open Space Park (San Diego, CA) exhibit anomalous arsenic (As) enrichment (100 - 480,000 ppm) up to five orders of magnitude greater than average for igneous rocks (1.5 ppm). We hypothesize that these rocks underwent localized syn-<span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> alteration along a highly fractured zone that today trends between N10°W and N20°W, leading to anomalous As enrichment on the spatial scale of tens of meters. We suspect that such As has been further mobilized by modern water-rock interactions. Using standard geochemical techniques (e.g. XRD, XRF, EDX) and mass balance analyses, we aim to (1) summarize the extent of As enrichment in altered SPV, and (2) present an integrated view of the interactions between ancient <span class="hlt">hydrothermal</span> <span class="hlt">volcanic</span> arc processes, surficial weathering, and observed As anomalies. Alteration textures of samples range from partially altered phenocrysts (i.e. minimally altered) to massive <span class="hlt">hydrothermal</span> replacement, in which virtually all primary phases are altered to new <span class="hlt">hydrothermal</span> minerals such as epidote, Fe-rich chlorite, and sericite (i.e. highly altered). Highly altered rocks contain average As concentrations (mean = 37,680 +/- 15,396 ppm, n = 23) >10,000 times that of minimally altered SPV (mean = 26 +/- 6 ppm As, n = 19). In some rocks, As-rich iron oxide and gypsum containing up to 900 ppm As are present as surficial rinds, suggesting modern day remobilization of As from <span class="hlt">hydrothermal</span> host minerals, like arsenopyrite. These findings indicate that such As is highly soluble and, therefore, may be further mobilized by physical and chemical weathering. No other trace metals (e.g. Pb, Cu, Ag, Au) are consistently enriched above upper-crustal averages, and As does not always occur</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.P33A1917S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.P33A1917S"><span>Experimental constraints on <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> in Enceladus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sekine, Y.; Shibuya, T.; Suzuki, K.; Kuwatani, T.</p> <p>2012-12-01</p> <p>One of the most remarkable findings by the Cassini-Huygens mission is perhaps water-rich plumes erupting from the south-pole region of Enceladus [1]. Given such geological <span class="hlt">activity</span> and the detection of sodium salts in the plume, the interior of Enceladus is highly likely to contain an interior ocean interacting with the rock core [2]. A primary question regarding astrobiology and planetary science is whether Enceladus has (or had) <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> in the interior ocean. Because N2 might be formed by thermal dissociation of primordial NH3 [3], the presence of N2 in the plume may be a possible indicator for the presence of <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> in Enceladus. However, the Cassini UVIS revealed that the plumes do not contain large amounts of N2 [4]. Although these observations may not support the presence of <span class="hlt">hydrothermal</span> <span class="hlt">activities</span>, whether NH3 dissociation proceeds strongly depends on the kinetics of <span class="hlt">hydrothermal</span> reactions and interactions with the rock components, which remain largely unknown. Furthermore, the Cassini CDA recently showed that small amounts of SiO2 might have been included in the plume dusts [5]. Formation of amorphous SiO2 usually occurs when high-temperature and/or high-pH solution with high concentrations of dissolved SiO2 cools and/or is neutralized. Thus, the presence of SiO2 in the plume dusts may suggest the presence of a temperature and/or pH gradient in the ocean. However, no laboratory experiments have investigated what processes control pH and SiO2 concentrations in <span class="hlt">hydrothermal</span> fluids possibly existing in Enceladus. Here, we show the results of laboratory experiments simulating <span class="hlt">hydrothermal</span> systems on Enceladus. As the initial conditions, we used both aqueous solution of high concentrations (0.01-2%) of NH3 and NaHCO3 and powdered olivine as an analog for the rock components. Our experimental results show that formation of N2 from NH3 is kinetically and thermodynamically inhibited even under high temperature conditions (< 400</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5456S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5456S"><span>Aquifers as indicators of <span class="hlt">volcanic</span> unrest - models of hydrological responses to magmatic <span class="hlt">activity</span> and their geophysical signals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Strehlow, Karen; Gottsmann, Jo</p> <p>2014-05-01</p> <p>Aquifers respond to and modify the surface expressions of magmatic <span class="hlt">activity</span>, and they can also become agents of unrest themselves. Therefore, monitoring the hydrology can provide a valuable window into subsurface processes in <span class="hlt">volcanic</span> areas. Interpretations of unrest signals as groundwater responses to changes in the magmatic system can be found for many volcanoes. Changes in temperature and strain conditions, seismic excitation or the injection of magmatic fluids into <span class="hlt">hydrothermal</span> systems are just a few of the proposed processes induced by magmatic <span class="hlt">activity</span> that affect the local hydrology. Aquifer responses are described to include changes in water table levels, changes in temperature or composition of <span class="hlt">hydrothermal</span> waters and pore pressure-induced ground deformation. We can observe these effects at the surface via geophysical and geochemical signals. To fully to utilise these indicators as monitoring and forecasting tools, however, it is necessary to improve our still poor understanding of the ongoing mechanisms in the interactions of hydrological and magmatic systems. An extensive literature research provided an overview on reported effects, which we investigate in detail using numerical modelling. The hydrogeophysical study uses finite element analysis to quantitatively test proposed mechanisms of aquifer excitation and the resultant geophysical signals. We present a set of generic models for two typical <span class="hlt">volcanic</span> landforms - a stratovolcano and a caldera - that simulate the interaction between deeper magmatic systems with shallow-seated aquifers, focusing on strain and temperature effects. They predict pore pressure induced hydraulic head changes in the aquifer as well as changing groundwater temperatures and strain induced fluid migration. Volcano observatories can track these hydrological effects for example with potential field investigations or the monitoring of wells. The models allow us to explore the parameter space, contributing to a better understanding</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015145','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015145"><span>New evidence on the <span class="hlt">hydrothermal</span> system in Long Valley caldera, California, from wells, fluid sampling, electrical geophysics, and age determinations of hot-spring deposits</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sorey, M.L.; Suemnicht, G.A.; Sturchio, N.C.; Nordquist, G.A.</p> <p>1991-01-01</p> <p>Data collected since 1985 from test drilling, fluid sampling, and geologic and geophysical investigations provide a clearer definition of the <span class="hlt">hydrothermal</span> system in Long Valley caldera than was previously available. This information confirms the existence of high-temperature (> 200??C) reservoirs within the <span class="hlt">volcanic</span> fill in parts of the west moat. These reservoirs contain fluids which are chemically similar to thermal fluids encountered in the central and eastern parts of the caldera. The roots of the present-day <span class="hlt">hydrothermal</span> system (the source reservoir, principal zones of upflow, and the magmatic heat source) most likely occur within metamorphic basement rocks beneath the western part of the caldera. Geothermometer-temperature estimates for the source reservoir range from 214 to 248??C. Zones of upflow of hot water could exist beneath the plateau of moat rhyolite located west of the resurgent dome or beneath Mammoth Mountain. Lateral flow of thermal water away from such upflow zones through reservoirs in the Bishop Tuff and early rhyolite accounts for temperature reversals encountered in most existing wells. Dating of hot-spring deposits from <span class="hlt">active</span> and inactive thermal areas confirms previous interpretations of the evolution of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> that suggest two periods of extensive hot-spring discharge, one peaking about 300 ka and another extending from about 40 ka to the present. The onset of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> around 40 ka coincides with the initiation of rhyolitic <span class="hlt">volcanism</span> along the Mono-Inyo Craters <span class="hlt">volcanic</span> chain that extends beneath the caldera's west moat. ?? 1991.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79...27D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79...27D"><span>Contrasting origin of two clay-rich debris flows at Cayambe <span class="hlt">Volcanic</span> Complex, Ecuador</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Detienne, M.; Delmelle, P.; Guevara, A.; Samaniego, P.; Opfergelt, S.; Mothes, P. A.</p> <p>2017-04-01</p> <p>We investigate the sedimentological and mineralogical properties of a debris flow deposit west of Cayambe <span class="hlt">Volcanic</span> Complex, an ice-clad edifice in Ecuador. The deposit exhibits a matrix facies containing up to 16 wt% of clays. However, the stratigraphic relationship of the deposit with respect to the Canguahua Formation, a widespread indurated volcaniclastic material in the Ecuadorian inter-Andean Valley, and the deposit alteration mineralogy differ depending on location. Thus, two different deposits are identified. The Río Granobles debris flow deposit ( 1 km3) is characterised by the alteration mineral assemblage smectite + jarosite, and sulphur isotopic analyses point to a supergene <span class="hlt">hydrothermal</span> alteration environment. This deposit probably derives from a debris avalanche initiated before 14-21 ka by collapse of a <span class="hlt">hydrothermally</span> altered rock mass from the volcano summit. In contrast, the alteration mineralogy of the second debris flow deposit, which may itself comprise more than one unit, is dominated by halloysite + smectite and relates to a shallower and more recent (<13 ky) mass movement of high-altitude (>3200 m) <span class="hlt">volcanic</span> soils. Our study reinforces the significance of <span class="hlt">hydrothermal</span> alteration in weakening volcano flanks and in favouring rapid transformation of a <span class="hlt">volcanic</span> debris avalanche into a clay-rich debris flow. It also demonstrates that mineralogical analysis provides crucial information for resolving the origin of a debris flow deposit in <span class="hlt">volcanic</span> terrains. Finally, we posit that slope instability, promoted by ongoing subglacial <span class="hlt">hydrothermal</span> alteration, remains a significant hazard at Cayambe <span class="hlt">Volcanic</span> Complex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.137..480P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.137..480P"><span>Beyond the vent: New perspectives on <span class="hlt">hydrothermal</span> plumes and pelagic biology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phillips, Brennan T.</p> <p>2017-03-01</p> <p>Submarine <span class="hlt">hydrothermal</span> vent fields introduce buoyant plumes of chemically altered seawater to the deep-sea water column. Chemoautotrophic microbes exploit this energy source, facilitating seafloor-based primary production that evidence suggests may transfer to pelagic consumers. While most <span class="hlt">hydrothermal</span> plumes have relatively small volumes, there are recent examples of large-scale plume events associated with periods of eruptive <span class="hlt">activity</span>, which have had a pronounced effect on water-column biology. This correlation suggests that <span class="hlt">hydrothermal</span> plumes may have influenced basin-scale ocean chemistry during periods of increased submarine <span class="hlt">volcanism</span> during the Phanerozoic eon. This paper synthesizes a growing body of scientific evidence supporting the hypothesis that <span class="hlt">hydrothermal</span> plumes are the energetic basis of unique deep-sea pelagic food webs. While many important questions remain concerning the biology of <span class="hlt">hydrothermal</span> plumes, this discussion is not present in ongoing management efforts related to seafloor massive sulfide (SMS) mining. Increased research efforts, focused on high-resolution surveys of midwater biology relative to plume structures, are recommended to establish baseline conditions and monitor the impact of future mining-based disturbances to the pelagic biosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS22B..03G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS22B..03G"><span><span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> on the Mid-Cayman Rise: ROV Jason sampling and site characterization at the Von Damm and Piccard <span class="hlt">hydrothermal</span> fields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>German, C. R.</p> <p>2012-12-01</p> <p>In January 2012 our multi-national and multi-disciplinary team conducted a series of 10 ROV Jason dives to conduct first detailed and systematic sampling of the Mid Cayman Rise <span class="hlt">hydrothermal</span> systems at the Von Damm and Piccard <span class="hlt">hydrothermal</span> fields. At Von Damm, <span class="hlt">hydrothermal</span> venting is focused at and around a large conical structure that is approximately 120 m in diameter and rises at least 80m from the surrounding, largely sedimented seafloor. Clear fluids emitted from multiple sites around the flanks of the mound fall in the temperature range 110-130°C and fall on a common mixing line with hotter (>200°C) clear fluids emitted from an 8m tall spire at the summit which show clear evidence of ultramafic influence. Outcrop close to the vent-site is rare and the cone itself appear to consist of clay minerals derived from highly altered host rock. The dominant fauna at the summit of Von Damm are a new species of chemosynthetic shrimp but elsewhere the site also hosts two distinct species of chemosynthetic tube worm as well as at least one species of gastropod. The adjacent Piccard site, at ~5000m depth comprises 7 distinct sulfide mounds, 3 of which are currently <span class="hlt">active</span>: Beebe Vents, Beebe Woods and Beebe Sea. Beebe Vents consists of 5 vigorous black smoker chimneys with maximum temperatures in the range 400-403°C while at Beebe Woods a more highly colonized thicket of up to 8m tall chimneys includes predominantly beehive diffusers with rare black smokers emitting fluids up to 353°C. Beebe Sea a diffuse site emitting fluids at 38°C Tmax, is the largest of the currently <span class="hlt">active</span> mounds and immediately abuts a tall (8m) rift that strikes NE-SW bisecting the host Axial <span class="hlt">Volcanic</span> Ridge. The fauna at Piccard are less diverse than at Von Damm and, predominantly, comprise the same species of MCR shrimp, a distinct gastropod species and abundant anemones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70170212','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70170212"><span>The Chahnaly low sulfidation epithermal gold deposit, western Makran <span class="hlt">volcanic</span> arc, southeastern Iran</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sholeh, Ali; Rastad, Ebrahim; Huston, David L.; Gemmell, J. Bruce; Taylor, Ryan D.</p> <p>2016-01-01</p> <p>The Chahnaly Au deposit formed during the early stages of magmatism. LA-ICP-MS zircon U-Pb geochronology of host andesite and 40Ar/39Ar dating of two samples of gold-associated adularia show that the ore-stage adularia (19.83 ± 0.10 and 19.2 ± 0.5 Ma) is younger, by as much as 1.5 million years, than the <span class="hlt">volcanic</span> host rock (20.32 ± 0.4 Ma). Therefore, either <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> continued well after <span class="hlt">volcanism</span> or a second magmatic event rejuvenated <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. This second magmatic event may be related to eruption of porphyritic andesite at ~20.32 ± 0.40 Ma, which is within error of ~19.83 ± 0.10 Ma adularia. The new LA-ICP-MS zircon U-Pb host rock and vein adularia 40Ar/39Ar ages suggest that early Miocene magmatism and mineralization in the Bazman area is of a similar age to that of the Saindak porphyry and Tanjeel porphyry center of the giant Reko Diq deposit. This confirms the existence of early Miocene arc magmatism and mineralization along the Iranian part of the Makran <span class="hlt">volcanic</span> arc. Ore, alteration mineralogy, and alteration patterns indicate that the Chahnaly deposit is a typical low-sulfidation epithermal Au deposit, located in a poorly explored part of the Makran <span class="hlt">volcanic</span> arc in Iran.                   </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/pp729g/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/pp729g/"><span>The Quaternary and Pliocene Yellowstone Plateau <span class="hlt">volcanic</span> field of Wyoming, Idaho, and Montana</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Christiansen, Robert L.</p> <p>2001-01-01</p> <p>This region of Yellowstone National Park has been the <span class="hlt">active</span> focus of one of the Earth's largest magmatic systems for more than 2 million years. The resulting <span class="hlt">volcanism</span> has been characterized by the eruption of voluminous rhyolites and subordinate basalts but virtually no lavas of intermediate composition. The magmatic system at depth remains <span class="hlt">active</span> and drives the massive <span class="hlt">hydrothermal</span> circulation for which the park is widely known. Studies of the <span class="hlt">volcanic</span> field using geologic mapping and petrology have defined three major cycles of rhyolitic <span class="hlt">volcanism</span>, each climaxed by the eruption of a rhyolitic ash-flow sheet having a volume of hundreds of thousands of cubic kilometers. The field also has been analyzed in terms of its magmatic and tectonic evolution, including its regional relation to the Snake River plain and to basin-range tectonic extension.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V24A..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V24A..01S"><span>ORP and pH measurements to detect redox and acid-base anomalies from <span class="hlt">hydrothermal</span> <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santana-Casiano, J. M.; González-Dávila, M.; Fraile-Nuez, E.</p> <p>2017-12-01</p> <p>The Tagoro submarine volcano is located 1.8 km south of the Island of El Hierro at 350 m depth and rises up to 88 m below sea level. It was erupting melting material for five months, from October 2011 to March 2012, changing drastically the physical-chemical properties of the water column in the area. After this eruption, the system evolved to a <span class="hlt">hydrothermal</span> system. The character of both reduced and acid of the <span class="hlt">hydrothermal</span> emissions in the Tagoro submarine volcano allowed us to detect anomalies related with changes in the chemical potential and the proton concentration using ORP and pH sensors, respectively. Tow-yos using a CTD-rosette with these two sensors provided the locations of the emissions plotting δ(ORP)/δt and ΔpH versus the latitude or longitude. The ORP sensor responds very quickly to the presence of reduced chemicals in the water column. Changes in potential are proportional to the amount of reduced chemical species present in the water. The magnitude of these changes are examined by the time derivative of ORP, δ(ORP)/δt. To detect changes in the pH, the mean pH for each depth at a reference station in an area not affected by the vent emission is subtracted from each point measured near the <span class="hlt">volcanic</span> edifice, defining in this way ΔpH. Detailed surveys of the <span class="hlt">volcanic</span> edifice were carried out between 2014 and 2016 using several CTD-pH-ORP tow-yo studies, localizing the ORP and pH changes, which were used to obtain surface maps of anomalies. Moreover, meridional tow-yos were used to calculate the amount of <span class="hlt">volcanic</span> CO2 added to the water column. The inputs of CO2 along multiple sections combined with measurements of oceanic currents produced an estimated <span class="hlt">volcanic</span> CO2 flux = 6.0 105 ± 1.1 105 kg d-1 which increases the acidity above the volcano by 20%. Sites like the Tagoro submarine volcano, in its degasification stage, provide an excellent opportunity to study the carbonate system in a high CO2 world, the <span class="hlt">volcanic</span> contribution to the global</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V51C0362B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V51C0362B"><span>Insights on the Origin of Volatiles from the Geochemical Investigation of <span class="hlt">Hydrothermal</span> Gas Discharges from Dominica, Lesser Antilles.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buskop, J.; Joseph, E. P.; Inguaggiato, S.; Varekamp, J. C.; Ku, T.</p> <p>2017-12-01</p> <p>The major goals of volcano <span class="hlt">hydrothermal</span> monitoring are to obtain information on temperature, origin, and changes in chemical composition of <span class="hlt">volcanic</span> fluids. This data contributes to the baseline geochemical monitoring of <span class="hlt">volcanic</span> <span class="hlt">activity</span> and informs on potential <span class="hlt">volcanic</span> hazards to which the public may be exposed. The origins of <span class="hlt">hydrothermal</span> fluids are diverse and can be magmatic, crustal and atmospheric. Studies of isotopes, inert gases, and thermodynamic calculations help elucidate the origin in each case and determine provenance of volatiles and a re-evaluation of reservoir temperatures. Sulphur isotope ratio (δ34S) for H2S leached from rock is <0 ‰, of magmatic origin = 0‰ and of marine origin >0 ‰. Low δ15N (-7.3 ‰) is indicative of low sediment addition to source magmas, while high δ15N (+2.1 ‰) indicates greater sediment contribution in magma formation. Baseline monitoring of <span class="hlt">hydrothermal</span> gases of Dominica for the period 2000 - 2006 show compositions typical of those found in arc-type settings, with N2 excess and low amounts of He and Ar. The dry gas is dominated by CO2 (ranging from 492 to 993 mmol/mol), and has a <span class="hlt">hydrothermal</span> signature with hydrogen sulphide as the main sulphurous gas. Over the past decade, Dominica has experienced <span class="hlt">volcanic</span> and tectonic seismicity and a sudden draining episode at the Boiling Lake in November 2016. This study evaluates data obtained in 2017 on gas composition from five (5) <span class="hlt">hydrothermal</span> areas across the island (Valley of Desolation, Sulphur Spring, Watten Waven, Galion and Penville cold Soufriere) to determine temporal and spatial deviations from baseline geochemical conditions. This study also presents new data, obtained in 2017, on sulphur and nitrogen isotopes to evaluate contributions from various source components. Preliminary results show high CH4/CO2 ratios for gases from Sulphur Springs and Galion, indicative of a significant <span class="hlt">hydrothermal</span> contribution to these fluids. However, high helium isotope</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024492','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024492"><span>High-resolution aeromagnetic mapping of <span class="hlt">volcanic</span> terrain, Yellowstone National Park</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Finn, C.A.; Morgan, L.A.</p> <p>2002-01-01</p> <p>High-resolution aeromagnetic data acquired over Yellowstone National Park (YNP) show contrasting patterns reflecting differences in rock composition, types and degree of alteration, and crustal structures that mirror the variable geology of the Yellowstone Plateau. The older, Eocene, Absaroka <span class="hlt">Volcanic</span> Supergroup, a series of mostly altered, andesitic <span class="hlt">volcanic</span> and volcaniclastic rocks partially exposed in mountains on the eastern margin of YNP, produces high-amplitude, positive magnetic anomalies, strongly contrasting with the less magnetic, younger, latest Cenozoic, Yellowstone Plateau Group, primarily a series of fresh and variably altered rhyolitic rocks covering most of YNP. The Yellowstone caldera is the centerpiece of the Yellowstone Plateau; part of its boundary can be identified on the aeromagnetic map as a series of discontinuous, negative magnetic anomalies that reflect faults or zones along which extensive <span class="hlt">hydrothermal</span> alteration is localized. The large-volume rhyolitic ignimbrite deposits of the 0.63-Ma Lava Creek Tuff and the 2.1-Ma Huckleberry Ridge Tuff, which are prominent lithologies peripheral to the Yellowstone caldera, produce insignificant magnetic signatures. A zone of moderate amplitude positive anomalies coincides with the mapped extent of several post-caldera rhyolitic lavas. Linear magnetic anomalies reflect the rectilinear fault systems characteristic of resurgent domes in the center of the caldera. Peripheral to the caldera, the high-resolution aeromagnetic map clearly delineates flow unit boundaries of pre- and post-caldera basalt flows, which occur stratigraphically below the post-caldera rhyolitic lavas and are not exposed extensively at the surface. All of the hot spring and geyser basins, such as Norris, Upper and Lower Geyser Basins, West Thumb, and Gibbon, are associated with negative magnetic anomalies, reflecting <span class="hlt">hydrothermal</span> alteration that has destroyed the magnetic susceptibility of minerals in the <span class="hlt">volcanic</span> rocks. Within</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.V53D..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.V53D..05M"><span>Distribution of <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> at the Lau ISS: Possible Controlling Parameters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martinez, F.; Baker, E. T.; Resing, J. A.; Edwards, M. H.; Walker, S. L.; Buck, N.</p> <p>2008-12-01</p> <p> the above hypothesis. This may suggest that <span class="hlt">hydrothermal</span> fluids are efficiently channeled to the axis even if cooling off-axis crustal regions. Alternatively, at the back-arc VFR/ELSC subduction controls on magmatic productivity may play an important role in modifying the usual relationships observed at MORs among spreading rate, seismic low velocity zone width, faulting, sedimentation and <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. For example, the fast spreading ELSC is magmatically deficient for its spreading rate, forms a deep faulted axial floor and has no continuous axial magma lens seismic reflector. This may lead to a narrower LVZ at the ELSC relative to MORs spreading at the same rate. At the intermediate rate and arc- proximal VFR excess magmatic productivity and volatile-rich <span class="hlt">volcanics</span> form a peaked shallow axis, few flanking faults and a sediment drape of volcaniclastics from the ridge axis (and nearby arc volcanoes). These effects may act to suppress fault-related permeability on ridge flanks or may rapidly blanket ridge-flanking <span class="hlt">hydrothermal</span> systems. Some of these issues may be further clarified when planned seismic tomographic and moored hydrophone studies are carried out beginning next year at the ELSC/VFR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..356..331N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..356..331N"><span>Characterising <span class="hlt">hydrothermal</span> fluid pathways beneath Aluto volcano, Main Ethiopian Rift, using shear wave splitting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nowacki, Andy; Wilks, Matthew; Kendall, J.-Michael; Biggs, Juliet; Ayele, Atalay</p> <p>2018-05-01</p> <p>Geothermal resources are frequently associated with silicic calderas which show evidence of geologically-recent <span class="hlt">activity</span>. Hence development of geothermal sites requires both an understanding of the <span class="hlt">hydrothermal</span> system of these volcanoes, as well as the deeper magmatic processes which drive them. Here we use shear wave splitting to investigate the <span class="hlt">hydrothermal</span> system at the silicic peralkaline volcano Aluto in the Main Ethiopian Rift, which has experienced repeated uplift and subsidence since at least 2004. We make over 370 robust observations of splitting, showing that anisotropy is confined mainly to the top ∼3 km of the <span class="hlt">volcanic</span> edifice. We find up to 10% shear wave anisotropy (SWA) is present with a maximum centred at the geothermal reservoir. Fast shear wave orientations away from the reservoir align NNE-SSW, parallel to the present-day minimum compressive stress. Orientations on the edifice, however, are rotated NE-SW in a manner we predict from field observations of faults at the surface, providing fluid pressures are sufficient to hold two fracture sets open. These fracture sets may be due to the repeated deformation experienced at Aluto and initiated in caldera formation. We therefore attribute the observed anisotropy to aligned cracks held open by over-pressurised gas-rich fluids within and above the reservoir. This study demonstrates that shear wave splitting can be used to map the extent and style of fracturing in <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> systems. It also lends support to the hypothesis that deformation at Aluto arises from variations of fluid pressures in the <span class="hlt">hydrothermal</span> system. These constraints will be crucial for future characterisation of other <span class="hlt">volcanic</span> and geothermal systems, in rift systems and elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GeCoA.117..313L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeCoA.117..313L"><span>Multiple sources of selenium in ancient seafloor <span class="hlt">hydrothermal</span> systems: Compositional and Se, S, and Pb isotopic evidence from <span class="hlt">volcanic</span>-hosted and <span class="hlt">volcanic</span>-sediment-hosted massive sulfide deposits of the Finlayson Lake District, Yukon, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Layton-Matthews, Daniel; Leybourne, Matthew I.; Peter, Jan M.; Scott, Steven D.; Cousens, Brian; Eglington, Bruce M.</p> <p>2013-09-01</p> <p><span class="hlt">Volcanic</span>-hosted massive sulfide (VHMS) and <span class="hlt">volcanic</span>-sediment-hosted massive sulfide (VSHMS; i.e., hosted by both <span class="hlt">volcanic</span> and sedimentary rocks) deposits in the Finlayson Lake District, Yukon, Canada, provide a unique opportunity to study the influence of seafloor and sub-seafloor <span class="hlt">hydrothermal</span> processes on the formation of Se-poor (GP4F VHMS deposit; 7 ppm Se average), intermediate (Kudz Ze Kayah—KZK VHMS deposit; 200 ppm Se average), and Se-enriched (Wolverine VSHMS deposit; 1100 ppm Se average) mineralization. All three deposits are hosted by mid-Paleozoic (˜360-346 Ma) felsic <span class="hlt">volcanic</span> rocks, but only the Wolverine deposit has voluminous coeval carbonaceous argillites (black shales) in the host rock package. Here we report the first application of Se isotope analyses to ancient seafloor mineralization and use these data, in conjunction with Pb and S isotope analyses, to better understand the source(s) and depositional process(es) of Se within VHMS and VSHMS systems. The wide range of δ82Se (-10.2‰ to 1.3‰, relative to NIST 3149), δ34S (+2.0‰ to +12.8‰ CDT), and elevated Se contents (up to 5865 ppm) within the Wolverine deposit contrast with the narrower range of δ82Se (-3.8‰ to -0.5‰), δ34S (9.8‰ to 13.0‰), and lower Se contents (200 ppm average) of the KZK deposit. The Wolverine and KZK deposits have similar sulfide depositional histories (i.e., deposition at the seafloor, with concomitant zone refining). The Se in the KZK deposit is magmatic (leaching or degassing) in origin, whereas the Wolverine deposit requires an additional large isotopically negative Se source (i.e. ˜-15‰ δ82Se). The negative δ82Se values for the Wolverine deposit are at the extreme light end for measured terrestrial samples, and the lightest observed for hypogene sulfide minerals, but are within calculated equilibrium values of δ82Se relative to NIST 3149 (˜30‰ at 25 °C between SeO4 and Se2-). We propose that the most negative Se isotope values at the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5706G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5706G"><span>Transition from phreatic to phreatomagmatic explosive <span class="hlt">activity</span> of Zhupanovsky volcano (Kamchatka) in 2013-2016 due to <span class="hlt">volcanic</span> cone collapse</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gorbach, Natalia; Plechova, Anastasiya; Portnyagin, Maxim</p> <p>2017-04-01</p> <p>Zhupanovsky volcano, situated 70 km north from Petropavlovsk-Kamchatsky city, resumed its <span class="hlt">activity</span> in October 2013 [3]. In 2014 and in the first half of 2015, episodic explosions with ash plumes rising up to 6-8 km above sea level occurred on Priemish cone - one of four cones on the Zhupanovsky <span class="hlt">volcanic</span> edifice [1]. In July 2015 after a series of seismic and explosive events, the southern sector of the <span class="hlt">active</span> cone collapsed. The landslide and lahar deposits resulted from the collapse formed a large field on the volcano slopes [2]. In November 2015 and January-March 2016, a series of powerful explosions took place sending ash up to 8-10 km above sea level. No pure magmatic, effusive or extrusive, <span class="hlt">activity</span> has been observed on Zhupanovsky in 2013-2016. We have studied the composition, morphology and textural features of ash particles produced by the largest explosive events of Zhupanovsky in the period from October 2013 to March 2016. The main components of the ash were found to be <span class="hlt">hydrothermally</span> altered particles and lithics, likely originated by the defragmentation of rocks composing the <span class="hlt">volcanic</span> edifice. Juvenile glass fragments occur in very subordinate quantities. The maximum amount of glass particles (up to 7%) was found in the ash erupted in January-March 2016, after the cone collapse. We suggest that the phreatic to phreatomagmatic explosive <span class="hlt">activity</span> of Zhupanovsky volcano in 2013-2016 was initially caused by the intrusion of a new magma batch under the volcano. The intrusion and associated degassing of magma led to heating, overpressure and instability in the <span class="hlt">hydrothermal</span> system of the volcano, causing episodic, predominantly phreatic explosions. Decompression of the shallow magmatic and <span class="hlt">hydrothermal</span> system of the volcano due to the cone collapse in July 2015 facilitated a larger involvement of the magmatic component in the eruption and more powerful explosions. [1] Girina O.A. et al., 2016 Geophysical Research Abstracts Vol. 18, EGU2016-2101, doi: 10</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JVGR..288...76W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JVGR..288...76W"><span>Mechanical and physical properties of <span class="hlt">hydrothermally</span> altered rocks, Taupo <span class="hlt">Volcanic</span> Zone, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wyering, L. D.; Villeneuve, M. C.; Wallis, I. C.; Siratovich, P. A.; Kennedy, B. M.; Gravley, D. M.; Cant, J. L.</p> <p>2014-11-01</p> <p>Mechanical characterization of <span class="hlt">hydrothermally</span> altered rocks from geothermal reservoirs will lead to an improved understanding of rock mechanics in a geothermal environment. To characterize rock properties of the selected formations, we prepared samples from intact core for <span class="hlt">non</span>-destructive (porosity, density and ultrasonic wave velocities) and destructive laboratory testing (uniaxial compressive strength). We characterised the <span class="hlt">hydrothermal</span> alteration assemblage using optical mineralogy and existing petrography reports and showed that lithologies had a spread of secondary mineralisation that occurred across the smectite, argillic and propylitic alteration zones. The results from the three geothermal fields show a wide variety of physical rock properties. The testing results for the <span class="hlt">non</span>-destructive testing shows that samples that originated from the shallow and low temperature section of the geothermal field had higher porosity (15 - 56%), lower density (1222 - 2114 kg/m3) and slower ultrasonic waves (1925 - 3512 m/s (vp) and 818 - 1980 m/s (vs)), than the samples from a deeper and higher temperature section of the field (1.5 - 20%, 2072 - 2837 kg/m3, 2639 - 4593 m/s (vp) and 1476 - 2752 m/s (vs), respectively). The shallow lithologies had uniaxial compressive strengths of 2 - 75 MPa, and the deep lithologies had strengths of 16 - 211 MPa. Typically samples of the same lithologies that originate from multiple wells across a field have variable rock properties because of the different alteration zones from which each sample originates. However, in addition to the alteration zones, the primary rock properties and burial depth of the samples also have an impact on the physical and mechanical properties of the rock. Where this data spread exists, we have been able to derive trends for this specific dataset and subsequently have gained an improved understanding of how <span class="hlt">hydrothermal</span> alteration affects physical and mechanical properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015005','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015005"><span>A Sr-isotopic comparison between thermal waters, rocks, and <span class="hlt">hydrothermal</span> calcites, Long Valley caldera, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Goff, F.; Wollenberg, H.A.; Brookins, D.C.; Kistler, R.W.</p> <p>1991-01-01</p> <p>The 87Sr/86Sr values of thermal waters and <span class="hlt">hydrothermal</span> calcites of the Long Valley caldera geothermal system are more radiogenic than those of young intracaldera <span class="hlt">volcanic</span> rocks. Five thermal waters display 87Sr/86Sr of 0.7081-0.7078 but show systematically lighter values from west to east in the direction of lateral flow. We believe the decrease in ratio from west to east signifies increased interaction of deeply circulating thermal water with relatively fresh <span class="hlt">volcanic</span> rocks filling the caldera depression. All types of pre-, syn-, and post-caldera <span class="hlt">volcanic</span> rocks in the west and central caldera have (87Sr/86Sr)m between about 0.7060 and 0.7072 and values for Sierra Nevada granodiorites adjacent to the caldera are similar. Sierran pre-intrusive metavolcanic and metasedimentary rocks can have considerably higher Sr-isotope ratios (0.7061-0.7246 and 0.7090-0.7250, respectively). <span class="hlt">Hydrothermally</span> altered <span class="hlt">volcanic</span> rocks inside the caldera have (87Sr/86Sr)m slightly heavier than their fresh <span class="hlt">volcanic</span> equivalents and <span class="hlt">hydrothermal</span> calcites (0.7068-0.7105) occupy a midrange of values between the <span class="hlt">volcanic</span>/plutonic rocks and the Sierran metamorphic rocks. These data indicate that the Long Valley geothermal reservoir is first equilibrated in a basement complex that contains at least some metasedimentary rocks. Reequilibration of Sr-isotope ratios to lower values occurs in thermal waters as convecting geothermal fluids flow through the isotopically lighter <span class="hlt">volcanic</span> rocks of the caldera fill. ?? 1991.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFMOS11A0338B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMOS11A0338B"><span>The Third Dimension of an <span class="hlt">Active</span> Back-arc <span class="hlt">Hydrothermal</span> System: ODP Leg 193 at PACMANUS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Binns, R.; Barriga, F.; Miller, D.</p> <p>2001-12-01</p> <p>This first sub-seafloor examination of an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system hosted by felsic <span class="hlt">volcanics</span>, at a convergent margin, obtained drill core from a high-T "smoker" site (penetrated to sim200 mbsf) and a low-T site of diffuse venting (~400mbsf). We aimed to delineate the lateral and vertical variability in mineralisation and alteration patterns, so as to understand links between volcanological, structural and <span class="hlt">hydrothermal</span> phenomena and the sources of fluids, and to establish the nature and extent of microbial <span class="hlt">activity</span> within the system. Technological breakthroughs included deployment of a new hard-rock re-entry system, and direct comparison in a hardrock environment of structural images obtained by wireline methods and logging-while-drilling. The PACMANUS <span class="hlt">hydrothermal</span> site, at the 1700m-deep crest of a 500m-high layered sequence of dacitic lavas, is notable for baritic massive sulfide chimneys rich in Cu, Zn, Au and Ag. Below an extensive cap 5-40m thick of fresh dacite-rhyodacite, we found unexpectedly pervasive <span class="hlt">hydrothermal</span> alteration of vesicular and flow-banded precursors, accompanied by variably intense fracturing and anhydrite-pyrite veining. Within what appears one major <span class="hlt">hydrothermal</span> event affecting the entire drilled sequence, there is much overprinting and repetition of distinctly allochemical argillaceous (illite-chlorite), acid-sulfate (pyrophyllite-anhydrite) and siliceous assemblages. The alteration profiles include a transition from metastable cristobalite to quartz at depth, and are similar under low-T and high-T vent sites but are vertically condensed in a manner suggesting higher thermal gradients beneath the latter. The altered rocks are surprisingly porous (average 25%). Retention of intergranular pore spaces and open vesicles at depth implies elevated <span class="hlt">hydrothermal</span> pressures, whereas evidence from fluid inclusions and <span class="hlt">hydrothermal</span> brecciation denotes local or sporadic phase separation. A maximum measured temperature of 313 degC measured 8 days</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U43A..02F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U43A..02F"><span>Patterns of seismicity in a complex <span class="hlt">volcanic</span> crisis at Brava, Cabo Verde</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faria, B. V. E.; Day, S. J.</p> <p>2017-12-01</p> <p>Brava is the smallest inhabited island of the Cape Verde archipelago, with an area of 62.5 km2 and a population of 6000. Geologically recent <span class="hlt">volcanism</span> on Brava has produced lava (including carbonatite) flows, phonolite lava domes, pyroclastic density current deposits, and many phreatomagmatic craters in central Brava (where most of the population lives). Recent geological studies indicate that last eruptive period is about 1000 years old. Brava has experienced recurrent seismic swarms and felt earthquakes. The first permanent seismic station was installed in 1999, and a small network in 2011. From then until 2015 the seismic rate was near constant with sporadic peaks. Most seismic events were located offshore and associated with submarine volcanoes. However, the pattern of <span class="hlt">activity</span> has been very different since 25th September 2015, when a M4 earthquake occurred in the submarine slopes of Brava. Subsequently, the seismicity became very complex with frequent volcano-tectonic (VT) earthquake swarms beneath Brava itself, with a few offshore events in some months. In addition, long-period, hybrid and <span class="hlt">hydrothermal</span> events and likely very weak <span class="hlt">volcanic</span> tremor episodes have been recorded. These <span class="hlt">non</span>-VT events support the hypothesis that magma emplacement beneath Brava is at the origin of the abnormal seismic <span class="hlt">activity</span>. The VT swarms indicate deformation around the magma body and possible dike intrusions, and there are indications of perturbation of a shallow <span class="hlt">hydrothermal</span> system. The largest swarm occurred on the 1st and 2nd August 2016, with almost 1000 shallow events, including a M3.7 VT earthquake, medium-frequency events and weak <span class="hlt">volcanic</span> tremor. An alert for a possible eruption was issued and a village (about 300 people) was evacuated as a precaution. Distributions of the cumulative number of events with depth in the main swarms suggest that the hypocenters are becoming shallower with time. Thus a possible eruption in the near future cannot be ruled out.</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/2015HESS...19.3937H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015HESS...19.3937H"><span>Groundwater flow processes and mixing in <span class="hlt">active</span> <span class="hlt">volcanic</span> systems: the case of Guadalajara (Mexico)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hernández-Antonio, A.; Mahlknecht, J.; Tamez-Meléndez, C.; Ramos-Leal, J.; Ramírez-Orozco, A.; Parra, R.; Ornelas-Soto, N.; Eastoe, C. J.</p> <p>2015-09-01</p> <p> other <span class="hlt">active</span> <span class="hlt">volcanic</span> systems on Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030111067&hterms=discrimination&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Ddiscrimination','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030111067&hterms=discrimination&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Ddiscrimination"><span>Discrimination of Hydrovolcanic Tephras from <span class="hlt">Volcanic</span> and <span class="hlt">Non-Volcanic</span> Backgrounds in Hyperspectral Data of Pavant Butte and Tabernacle Hill, Utah: Relevance for Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Farrand, W. H.</p> <p>2003-01-01</p> <p>Water-magma, or ice-magma, interactions have long been theorized as an important process in the Martian geologic record [1-3]. The ability to unambiguously recognize tephra deposits and <span class="hlt">volcanic</span> edifices produced by H2O-magma interactions is important for understanding the geologic history of Mars and for understanding the genesis of the major components of the Martian surface layer. Recognizing <span class="hlt">volcanic</span> edifices produced by H2Omagma interactions on the basis of morphology alone is difficult.can be definitively identified as such. One means of providing supporting evidence for the identification of hydrovolcanic landforms and tephra deposits is through spectroscopy. Tephras produced by hydrovolcanic <span class="hlt">activity</span> range from fresh basaltic glass (sideromelane) to glasses that have been completely altered to palagonite. A study of the visible through short-wave infrared (Vis-IR) reflectance of tephras composing tuff rings and tuff cones showed that the different stages of this alteration sequence have recognizable reflectance signatures [6,7]. However, the ability to recognize these different types of tephras against <span class="hlt">volcanic</span> and nonvolcanic background materials has yet to be fully demonstrated. In this research, hyperspectral Vis-IR data over <span class="hlt">volcanic</span> and hydrovolcanic terrains in the Black Rock Desert of Utah were analyzed in order to determine the separability of the component materials from <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> backgrounds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..289H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..289H"><span>Regional Triggering of <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Following Large Magnitude Earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hill-Butler, Charley; Blackett, Matthew; Wright, Robert</p> <p>2015-04-01</p> <p>There are numerous reports of a spatial and temporal link between <span class="hlt">volcanic</span> <span class="hlt">activity</span> and high magnitude seismic events. In fact, since 1950, all large magnitude earthquakes have been followed by <span class="hlt">volcanic</span> eruptions in the following year - 1952 Kamchatka M9.2, 1960 Chile M9.5, 1964 Alaska M9.2, 2004 & 2005 Sumatra-Andaman M9.3 & M8.7 and 2011 Japan M9.0. While at a global scale, 56% of all large earthquakes (M≥8.0) in the 21st century were followed by increases in thermal <span class="hlt">activity</span>. The most significant change in <span class="hlt">volcanic</span> <span class="hlt">activity</span> occurred between December 2004 and April 2005 following the M9.1 December 2004 earthquake after which new eruptions were detected at 10 volcanoes and global <span class="hlt">volcanic</span> flux doubled over 52 days (Hill-Butler et al. 2014). The ability to determine a volcano's <span class="hlt">activity</span> or 'response', however, has resulted in a number of disparities with <50% of all volcanoes being monitored by ground-based instruments. The advent of satellite remote sensing for volcanology has, therefore, provided researchers with an opportunity to quantify the timing, magnitude and character of <span class="hlt">volcanic</span> events. Using data acquired from the MODVOLC algorithm, this research examines a globally comparable database of satellite-derived radiant flux alongside USGS NEIC data to identify changes in <span class="hlt">volcanic</span> <span class="hlt">activity</span> following an earthquake, February 2000 - December 2012. Using an estimate of background temperature obtained from the MODIS Land Surface Temperature (LST) product (Wright et al. 2014), thermal radiance was converted to radiant flux following the method of Kaufman et al. (1998). The resulting heat flux inventory was then compared to all seismic events (M≥6.0) within 1000 km of each volcano to evaluate if changes in <span class="hlt">volcanic</span> heat flux correlate with regional earthquakes. This presentation will first identify relationships at the temporal and spatial scale, more complex relationships obtained by machine learning algorithms will then be examined to establish favourable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMOS21A1474R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMOS21A1474R"><span>Seismological evidence for an along-axis <span class="hlt">hydrothermal</span> flow at the Lucky Strike <span class="hlt">hydrothermal</span> vents site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rai, A.; Wang, H.; Singh, S. C.; Crawford, W. C.; Escartin, J.; Cannat, M.</p> <p>2010-12-01</p> <p><span class="hlt">Hydrothermal</span> circulation at ocean spreading centres plays fundamental role in crustal accretion process, heat extraction from the earth and helps to maintain very rich ecosystem in deep Ocean. Recently, it has been suggested that <span class="hlt">hydrothermal</span> circulation is mainly along the ridge axis at fast spreading centres above along axis melt lens (AMC). Using a combination of micro-earthquake and seismic reflection data, we show that the <span class="hlt">hydrothermal</span> circulation at the Lucky Strike segment of slow spreading Mid-Atlantic Ridge is also along axis in a narrow (~1 km) zone above a wide (2-3 km) AMC. We find that the seismicity mainly lies above the seismically imaged 3 km wide 7 km long melt lens at 3.2 km depth. We observe a vertical plume of seismicity above a weak AMC reflection just north of the <span class="hlt">hydrothermal</span> vent fields that initiates just above the AMC and continues to the seafloor. This zone is collocated with <span class="hlt">active</span> rifting of the seafloor in the neo-<span class="hlt">volcanic</span> zone. Beneath the <span class="hlt">hydrothermal</span> vents sites, where a strong melt lens is imaged, the seismicity initiates at 500 m above the AMC and continues to the seafloor. Just south of the <span class="hlt">hydrothermal</span> field, where the AMC is widest and strongest, the seismicity band lies 500 m above the melt lens in a 800 m thick zone, which does not continue to the seafloor. The presence the weak melt lens reflection could be due to a cooled and crystallised AMC (mush) that permits the penetration of <span class="hlt">hydrothermal</span> fluids down to the top of the AMC indicated by seismicity plume and might be the in-flow zone for <span class="hlt">hydrothermal</span> circulation. The strong AMC reflection could be due to fresh supply of melt in the AMC (pure melt), which has pushed the cracking front 500 m above the AMC. Beneath the <span class="hlt">hydrothermal</span> fields, the strong AMC reflection and seismicity 500 above the AMC to the seafloor could represent cracking along the up-flow zone. The 800 m thick zone of seismicity above the pure melt zone could be the zone of <span class="hlt">hydrothermal</span> cracking zone. We do</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70137865','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70137865"><span>Major off-axis <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> on the northern Gorda Ridge</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rona, Peter A.; Denlinger, Roger P.; Fisk, M. R.; Howard, K. J.; Taghon, G. L.; Klitgord, Kim D.; McClain, James S.; McMurray, G. R.; Wiltshire, J. C.</p> <p>1990-01-01</p> <p>The first <span class="hlt">hydrothermal</span> field on the northern Gorda Ridge, the Sea Cliff <span class="hlt">hydrothermal</span> field, was discovered and geologic controls of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in the rift valley were investigated on a dive series using the DSV Sea Cliff. The Sea Cliff <span class="hlt">hydrothermal</span> field was discovered where predicted at the intersection of axis-oblique and axis-parallel faults at the south end of a linear ridge at mid-depth (2700 m) on the east wall. Preliminary mapping and sampling of the field reveal: a setting nested on nearly sediment-free fault blocks 300 m above the rift valley floor 2.6 km from the axis; a spectrum of venting types from seeps to black smokers; high conductive heat flow estimated to be equivalent to the convective flux of multiple black smokers through areas of the sea floor sealed by a caprock of elastic breccia primarily derived from basalt with siliceous cement and barite pore fillings; and a vent biota with Juan de Fuca Ridge affinites. These findings demonstrate the importance of off-axis <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and the role of the intersection of tectonic lineations in controlling <span class="hlt">hydrothermal</span> sites at sea-floor spreading centers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T33F..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T33F..02D"><span>Slab dehydration in Cascadia and its relationship to <span class="hlt">volcanism</span>, seismicity, and <span class="hlt">non-volcanic</span> tremor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delph, J. R.; Levander, A.; Niu, F.</p> <p>2017-12-01</p> <p>. Siletzia also contains most of the young arc volcanoes in the Cascades, indicating that water is retained in the slab to depths where it can feed arc <span class="hlt">volcanism</span>. Thus, the along strike variations in <span class="hlt">volcanic</span> <span class="hlt">activity</span> and seismic <span class="hlt">activity</span> in Cascadia appear to be related to variations in depth of dewatering of the downgoing oceanic lithosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030110811&hterms=geology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dgeology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030110811&hterms=geology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dgeology"><span>Gish Bar Patera, Io: Geology and <span class="hlt">Volcanic</span> <span class="hlt">Activity</span>, 1996-2001</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perry, Jason; Radebaugh, Jani; Lopes, Rosaly; McEwen, Alfred; Keszthelyi, Laszlo</p> <p>2003-01-01</p> <p>Since the two Voyagers passed by Jupiter in 1979, it has been known that <span class="hlt">volcanic</span> <span class="hlt">activity</span> is ubiquitous on the surface of Io. With over 400 <span class="hlt">volcanic</span> centers, Io is even more <span class="hlt">volcanically</span> <span class="hlt">active</span> than the earth with massive flood basalt-style eruptions and komatitite lavas a common occurrence. Additionally, some volcanoes appear to be giant lava lakes, with violent <span class="hlt">activity</span> churning the crust of the lake for periods of 20 years or more. Finally, sulfur is believed to play a large role in Io's <span class="hlt">volcanism</span>, be it as a primary lava or as a secondary product of large, high-temperature eruptions. By studying one volcano in particular, Gish Bar Patera, one can observe many of these characteristics in one <span class="hlt">volcanic</span> center.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V41D2843K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V41D2843K"><span>Explosive <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> at Extreme Depths: Evidence from the Charles Darwin <span class="hlt">Volcanic</span> Field, Cape Verdes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kwasnitschka, T.; Devey, C. W.; Hansteen, T. H.; Freundt, A.; Kutterolf, S.</p> <p>2013-12-01</p> <p><span class="hlt">Volcanic</span> eruptions on the deep sea floor have traditionally been assumed to be <span class="hlt">non</span>-explosive as the high-pressure environment should greatly inhibit steam-driven explosions. Nevertheless, occasional evidence both from (generally slow-) spreading axes and intraplate seamounts has hinted at explosive <span class="hlt">activity</span> at large water depths. Here we present evidence from a submarine field of <span class="hlt">volcanic</span> cones and pit craters called Charles Darwin <span class="hlt">Volcanic</span> Field located at about 3600 m depth on the lower southwestern slope of the Cape Verdean Island of Santo Antão. We examined two of these submarine <span class="hlt">volcanic</span> edifices (Tambor and Kolá), each featuring a pit crater of 1 km diameter, using photogrammetric reconstructions derived from ROV-based imaging followed by 3D quantification using a novel remote sensing workflow, aided by sampling. The measured and calculated parameters of physical volcanology derived from the 3D model allow us, for the first time, to make quantitative statements about <span class="hlt">volcanic</span> processes on the deep seafloor similar to those generated from land-based field observations. Tambor cone, which is 2500 m wide and 250 m high, consists of dense, probably monogenetic medium to coarse-grained volcaniclastic and pyroclastic rocks that are highly fragmented, probably as a result of thermal and viscous granulation upon contact with seawater during several consecutive cycles of <span class="hlt">activity</span>. Tangential joints in the outcrops indicate subsidence of the crater floor after primary emplacement. Kolá crater, which is 1000 m wide and 160 m deep, appears to have been excavated in the surrounding seafloor and shows stepwise sagging features interpreted as ring fractures on the inner flanks. Lithologically, it is made up of a complicated succession of highly fragmented deposits, including spheroidal juvenile lapilli, likely formed by spray granulation. It resembles a maar-type deposit found on land. The eruption apparently entrained blocks of MORB-type gabbroic country rocks with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025117','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025117"><span>Groundwater flow, heat transport, and water table position within <span class="hlt">volcanic</span> edifices: Implications for <span class="hlt">volcanic</span> processes in the Cascade Range</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hurwitz, S.; Kipp, K.L.; Ingebritsen, S.E.; Reid, M.E.</p> <p>2003-01-01</p> <p>The position of the water table within a <span class="hlt">volcanic</span> edifice has significant implications for volcano hazards, geothermal energy, and epithermal mineralization. We have modified the <span class="hlt">HYDROTHERM</span> numerical simulator to allow for a free-surface (water table) upper boundary condition and a wide range of recharge rates, heat input rates, and thermodynamic conditions representative of continental volcano-<span class="hlt">hydrothermal</span> systems. An extensive set of simulations was performed on a hypothetical stratovolcano system with unconfined groundwater flow. Simulation results suggest that the permeability structure of the <span class="hlt">volcanic</span> edifice and underlying material is the dominant control on water table elevation and the distribution of pressures, temperatures, and fluid phases at depth. When permeabilities are isotropic, water table elevation decreases with increasing heat flux and increases with increasing recharge, but when permeabilities are anisotropic, these effects can be much less pronounced. Several conditions facilitate the ascent of a <span class="hlt">hydrothermal</span> plume into a <span class="hlt">volcanic</span> edifice: a sufficient source of heat and magmatic volatiles at depth, strong buoyancy forces, and a relatively weak topography-driven flow system. Further, the plume must be connected to a deep heat source through a pathway with a time-averaged effective permeability ???1 ?? 10-16 m2, which may be maintained by frequent seismicity. Topography-driven flow may be retarded by low permeability in the edifice and/or the lack of precipitation recharge; in the latter case, the water table may be relatively deep. Simulation results were compared with observations from the Quaternary stratovolcanoes along the Cascade Range of the western United States to infer <span class="hlt">hydrothermal</span> processes within the edifices. Extensive ice caps on many Cascade Range stratovolcanoes may restrict recharge on the summits and uppermost flanks. Both the simulation results and limited observational data allow for the possibility that the water table</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JVGR..301..221N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JVGR..301..221N"><span>Structural analysis and thermal remote sensing of the Los Humeros <span class="hlt">Volcanic</span> Complex: Implications for volcano structure and geothermal exploration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norini, G.; Groppelli, G.; Sulpizio, R.; Carrasco-Núñez, G.; Dávila-Harris, P.; Pellicioli, C.; Zucca, F.; De Franco, R.</p> <p>2015-08-01</p> <p>The Los Humeros <span class="hlt">Volcanic</span> Complex (LHVC) is an important geothermal target in the Trans-Mexican <span class="hlt">Volcanic</span> Belt. Understanding the structure of the LHVC and its influence on the occurrence of thermal anomalies and <span class="hlt">hydrothermal</span> fluids is important to get insights into the interplay between the volcano-tectonic setting and the characteristics of the geothermal resources in the area. In this study, we present a structural analysis of the LHVC, focused on Quaternary tectonic and volcano-tectonic features, including the areal distribution of monogenetic <span class="hlt">volcanic</span> centers. Morphostructural analysis and structural field mapping revealed the geometry, kinematics and dynamics of the structural features in the study area. Also, thermal infrared remote sensing analysis has been applied to the LHVC for the first time, to map the main endogenous thermal anomalies. These data are integrated with newly proposed Unconformity Bounded Stratigraphic Units, to evaluate the implications for the structural behavior of the caldera complex and geothermal field. The LHVC is characterized by a multistage formation, with at least two major episodes of caldera collapse: Los Humeros Caldera (460 ka) and Los Potreros Caldera (100 ka). The study suggests that the geometry of the first collapse recalls a trap-door structure and impinges on a thick <span class="hlt">volcanic</span> succession (10.5-1.55 Ma), now hosting the geothermal reservoir. The main ring-faults of the two calderas are buried and sealed by the widespread post-calderas <span class="hlt">volcanic</span> products, and for this reason they probably do not have enough permeability to be the main conveyers of the <span class="hlt">hydrothermal</span> fluid circulation. An <span class="hlt">active</span>, previously unrecognized fault system of volcano-tectonic origin has been identified inside the Los Potreros Caldera. This fault system is the main geothermal target, probably originated by <span class="hlt">active</span> resurgence of the caldera floor. The <span class="hlt">active</span> fault system defines three distinct structural sectors in the caldera floor, where the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.473..122B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.473..122B"><span>Amazonian <span class="hlt">volcanism</span> inside Valles Marineris on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brož, Petr; Hauber, Ernst; Wray, James J.; Michael, Gregory</p> <p>2017-09-01</p> <p>The giant trough system of Valles Marineris is one of the most spectacular landforms on Mars, yet its origin is still unclear. Although often referred to as a rift, it also shows some characteristics that are indicative of collapse processes. For decades, one of the major open questions was whether <span class="hlt">volcanism</span> was <span class="hlt">active</span> inside the Valles Marineris. Here we present evidence for a <span class="hlt">volcanic</span> field on the floor of the deepest trough of Valles Marineris, Coprates Chasma. More than 130 individual edifices resemble scoria and tuff cones, and are associated with units that are interpreted as lava flows. Crater counts indicate that the <span class="hlt">volcanic</span> field was emplaced sometime between ∼0.4 Ga and ∼0.2 Ga. The spatial distribution of the cones displays a control by trough-parallel subsurface structures, suggesting magma ascent in feeder dikes along trough-bounding normal faults. Spectral data reveal an opaline-silica-rich unit associated with at least one of the cones, indicative of <span class="hlt">hydrothermal</span> processes. Our results point to magma-water interaction, an environment of astrobiological interest, perhaps associated with late-stage <span class="hlt">activity</span> in the evolution of Valles Marineris, and suggest that the floor of Coprates Chasma is promising target for the in situ exploration of Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41B1946S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41B1946S"><span>NOAA Deepwater Exploration of the Marianas 2016: <span class="hlt">Volcanic</span> arc and Backarc Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stern, R. J.; Brounce, M. N.; Chadwick, B.; Fryer, P. B.; Glickson, D.; Merle, S. G.</p> <p>2016-12-01</p> <p>Legs 1 and 3 of NOAA Okeanos Explorer EX1605 devoted a total of 17 ROV dives to exploring the Mariana magmatic arc and backarc basin (BAB). Dives were carried out on 11 submarine arc volcanoes, the submerged slopes of two <span class="hlt">volcanic</span> islands, and at 3 BAB sites along 1000 km of the Mariana arc system. Four of the studied arc volcanoes are extinct, three are dormant, and six are <span class="hlt">active</span>. All BAB dives were on the spreading ridge between 15-17°N, which is <span class="hlt">volcanically</span> <span class="hlt">active</span>. Geologic highpoints of these dives include: 1) discovery of an extinct <span class="hlt">hydrothermal</span> chimney ( 15m tall) in Fina Nagu A (Leg 1, Dive 7; L1D7); 2) observations of very fresh (<3 years old) BAB pillow basalts (L1D9); 3) discovery of a very <span class="hlt">active</span> BAB <span class="hlt">hydrothermal</span> field (T 340°C, <span class="hlt">active</span> chimneys up to 30m tall; L1D11); 4) examination of Esmeralda Bank crater floor (<span class="hlt">active</span> venting but too murky to find vents; L1D19); 5) discovery of <span class="hlt">hydrothermal</span> vents with vent fauna on Chamorro volcano (L3D7; T 30°C, <span class="hlt">active</span> chimneys 2m tall); and 6) examination of <span class="hlt">active</span> venting and S degassing at 500-350 m depth on Daikoku volcano (L3D9). Video clips of some of the most exciting discoveries and examinations will be presented. We plan to compare previous bathymetry over the <span class="hlt">active</span> volcanoes with what was collected during EX1605 to quantify how these edifices have changed since when these were previously mapped, over the past 13 years or less. These dives also provided visual evidence in support of the hypothesis that individual edifices of the Fina Nagu <span class="hlt">Volcanic</span> Complex increase in age from NE to SW, interpreted as due to the motion of <span class="hlt">actively</span>-extending lithosphere of the southern Mariana BAB to the SW over a relatively fixed source of arc magma above the subducting Pacific plate (Brounce et al. G3 2016). Continuous interaction between biologists and geologists on EX1605 allowed us to identify regions of high faunal density on hard substrates around some <span class="hlt">active</span> volcanoes, for example Esmeralda Bank, presumably</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030950','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030950"><span><span class="hlt">Non-volcanic</span> tremor driven by large transient shear stresses</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rubinstein, J.L.; Vidale, J.E.; Gomberg, J.; Bodin, P.; Creager, K.C.; Malone, S.D.</p> <p>2007-01-01</p> <p><span class="hlt">Non</span>-impulsive seismic radiation or 'tremor' has long been observed at volcanoes and more recently around subduction zones. Although the number of observations of <span class="hlt">non-volcanic</span> tremor is steadily increasing, the causative mechanism remains unclear. Some have attributed <span class="hlt">non-volcanic</span> tremor to the movement of fluids, while its coincidence with geodetically observed slow-slip events at regular intervals has led others to consider slip on the plate interface as its cause. Low-frequency earthquakes in Japan, which are believed to make up at least part of <span class="hlt">non-volcanic</span> tremor, have focal mechanisms and locations that are consistent with tremor being generated by shear slip on the subduction interface. In Cascadia, however, tremor locations appear to be more distributed in depth than in Japan, making them harder to reconcile with a plate interface shear-slip model. Here we identify bursts of tremor that radiated from the Cascadia subduction zone near Vancouver Island, Canada, during the strongest shaking from the moment magnitude Mw = 7.8, 2002 Denali, Alaska, earthquake. Tremor occurs when the Love wave displacements are to the southwest (the direction of plate convergence of the overriding plate), implying that the Love waves trigger the tremor. We show that these displacements correspond to shear stresses of approximately 40 kPa on the plate interface, which suggests that the effective stress on the plate interface is very low. These observations indicate that tremor and possibly slow slip can be instantaneously induced by shear stress increases on the subduction interface - effectively a frictional failure response to the driving stress. ??2007 Nature Publishing Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17671500','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17671500"><span><span class="hlt">Non-volcanic</span> tremor driven by large transient shear stresses.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rubinstein, Justin L; Vidale, John E; Gomberg, Joan; Bodin, Paul; Creager, Kenneth C; Malone, Stephen D</p> <p>2007-08-02</p> <p><span class="hlt">Non</span>-impulsive seismic radiation or 'tremor' has long been observed at volcanoes and more recently around subduction zones. Although the number of observations of <span class="hlt">non-volcanic</span> tremor is steadily increasing, the causative mechanism remains unclear. Some have attributed <span class="hlt">non-volcanic</span> tremor to the movement of fluids, while its coincidence with geodetically observed slow-slip events at regular intervals has led others to consider slip on the plate interface as its cause. Low-frequency earthquakes in Japan, which are believed to make up at least part of <span class="hlt">non-volcanic</span> tremor, have focal mechanisms and locations that are consistent with tremor being generated by shear slip on the subduction interface. In Cascadia, however, tremor locations appear to be more distributed in depth than in Japan, making them harder to reconcile with a plate interface shear-slip model. Here we identify bursts of tremor that radiated from the Cascadia subduction zone near Vancouver Island, Canada, during the strongest shaking from the moment magnitude M(w) = 7.8, 2002 Denali, Alaska, earthquake. Tremor occurs when the Love wave displacements are to the southwest (the direction of plate convergence of the overriding plate), implying that the Love waves trigger the tremor. We show that these displacements correspond to shear stresses of approximately 40 kPa on the plate interface, which suggests that the effective stress on the plate interface is very low. These observations indicate that tremor and possibly slow slip can be instantaneously induced by shear stress increases on the subduction interface-effectively a frictional failure response to the driving stress.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41B1947R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41B1947R"><span><span class="hlt">Hydrothermal</span> exploration of the Mariana Back Arc Basin: Chemical Characterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resing, J. A.; Chadwick, B.; Baker, E. T.; Butterfield, D. A.; Baumberger, T.; Buck, N. J.; Walker, S. L.; Merle, S. G.; Michael, S.</p> <p>2016-12-01</p> <p>In November and December 2015, we visited the Southern Mariana back-arc on R/V Falkor (cruise FK151121) to explore for <span class="hlt">hydrothermal</span> and <span class="hlt">volcanic</span> <span class="hlt">activity</span>. We conducted our study using the SENTRY AUV, a CTD rosette designed to do tows and vertical casts into the deep back-arc, and a trace metal CTD-package for the upper 1000m of the water column to examine transport form the nearby arc. We conducted 7 SENTRY dives, 12 tow-yos, 7 vertical casts, and 14 trace metal casts. We also mapped 24,050 km2 of the seafloor using the Falkor EM 302 multibeam. We discovered four new <span class="hlt">hydrothermal</span> vent sites, and at one of them we found that some of the venting was coming from recently erupted lava flows. That lava flow is the deepest contemporary eruption yet discovered (at 4100-4450 m), and the first to be documented on a slow-spreading ridge. In addition, we were able to map the previously known Alice Springs <span class="hlt">hydrothermal</span> site in unprecedented detail with AUV Sentry. The distribution of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> as well as chemistry of the plumes above them will be discussed. Plume chemistry data will include , Fe, Mn, CH4, H2, and 3He. The ship time for this project was provided by the Schmidt Ocean Institute with science funding provided by NOAA-Ocean Exploration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..346..104W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..346..104W"><span>Characterisation and origin of <span class="hlt">hydrothermal</span> waters at São Miguel (Azores) inferred by chemical and isotopic composition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woitischek, Julia; Dietzel, Martin; Inguaggiato, Claudio; Böttcher, Michael E.; Leis, Albrecht; Cruz, J. Virgílio; Gehre, Matthias</p> <p>2017-10-01</p> <p>This study focuses on the characterisation and origin of <span class="hlt">hydrothermal</span> waters discharging from three main <span class="hlt">active</span> volcanoes (Furnas, Fogo and Sete Cidades) at São Miguel, where 33 water with temperatures ranging between 13 and 97 °C, and 5 precipitate samples were collected. The developed conceptual model for this <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system reveals that all waters can be classified by Na-HCO3, Na-Cl and Na-SO4 types and are of meteoric origin. This is confirmed by the stable hydrogen and oxygen isotope data that are positioned close to the local meteoric water line (- 4.1‰ ≤ δ18OH2O ≤ 5.2‰; - 17.6‰ ≤ δDH2O ≤ 20.4‰), except for the Na-Cl type water at Ferraria (Sete Cidades area), which is characterized by admixing of seawater. The stable isotope composition of São Miguel <span class="hlt">hydrothermal</span> solutions (δ34SSO4 range from 21.3 to - 3.7; δ18OSO4 range between 0.5 and 10.5‰; δ13CTDIC = - 4.5 ± 3.2‰) indicate that waters are individually evolved by several processes: evaporation, uptake of volcanogenic sulphur and carbon dioxide, leaching of local <span class="hlt">volcanic</span> rocks (driven by high CO2 contents and/or elevated temperature), and biological <span class="hlt">activity</span>. Latter hydrochemical superimposition is displayed by stromatolitic structures in the precipitates at the given site. Dissolved REE data show similar pattern as local <span class="hlt">volcanic</span> rocks. In particular the distinct Eu anomaly hints to preferential leaching of locally occurring trachyte. The strongly acidic Na-SO4 waters sampled in boiling pools at Fogo and Furnas Lake indicate high leaching levels and LREE depletion versus HREE compared with the <span class="hlt">volcanic</span> local rock compositions. Depletion in LREE is most likely caused by its preferential removal compared to HREE by the co-precipitation with alunite.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1651691','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1651691"><span><span class="hlt">Volcanic</span> <span class="hlt">activity</span>: a review for health professionals.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Newhall, C G; Fruchter, J S</p> <p>1986-01-01</p> <p>Volcanoes erupt magma (molten rock containing variable amounts of solid crystals, dissolved volatiles, and gas bubbles) along with pulverized pre-existing rock (ripped from the walls of the vent and conduit). The resulting <span class="hlt">volcanic</span> rocks vary in their physical and chemical characteristics, e.g., degree of fragmentation, sizes and shapes of fragments, minerals present, ratio of crystals to glass, and major and trace elements composition. Variability in the properties of magma, and in the relative roles of magmatic volatiles and groundwater in driving an eruption, determine to a great extent the type of an eruption; variability in the type of an eruption in turn influences the physical characteristics and distribution of the eruption products. The principal <span class="hlt">volcanic</span> hazards are: ash and larger fragments that rain down from an explosion cloud (airfall tephra and ballistic fragments); flows of hot ash, blocks, and gases down the slopes of a volcano (pyroclastic flows); "mudflows" (debris flows); lava flows; and concentrations of <span class="hlt">volcanic</span> gases in topographic depressions. Progress in volcanology is bringing improved long- and short-range forecasts of <span class="hlt">volcanic</span> <span class="hlt">activity</span>, and thus more options for mitigation of hazards. Collaboration between health professionals and volcanologists helps to mitigate health hazards of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Images FIGURE 1 FIGURE 2 FIGURE 6a-6e FIGURE 6a-6e FIGURE 8 FIGURE 9 FIGURE 10 FIGURE 11 PMID:3946726</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037323','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037323"><span>Snowmelt hydrograph interpretation: Revealing watershed scale hydrologic characteristics of the Yellowstone <span class="hlt">volcanic</span> plateau</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Payton, Gardner W.; Susong, D.D.; Kip, Solomon D.; Heasler, H.</p> <p>2010-01-01</p> <p>Snowmelt hydrograph analysis and groundwater age dates of cool water springs on the Yellowstone <span class="hlt">volcanic</span> plateau provide evidence of high volumes of groundwater circulation in watersheds comprised of quaternary Yellowstone <span class="hlt">volcanics</span>. Ratios of maximum to minimum mean daily discharge and average recession indices are calculated for watersheds within and surrounding the Yellowstone <span class="hlt">volcanic</span> plateau. A model for snowmelt recession is used to separate groundwater discharge from overland runoff, and compare groundwater systems. Hydrograph signal interpretation is corroborated with chlorofluorocarbon (CFC) and tritium concentrations in cool water springs on the Yellowstone <span class="hlt">volcanic</span> plateau. Hydrograph parameters show a spatial pattern correlated with watershed geology. Watersheds comprised dominantly of quaternary Yellowstone <span class="hlt">volcanics</span> are characterized by slow streamflow recession, low maximum to minimum flow ratios. Cool springs sampled within the Park contain CFC's and tritium and have apparent CFC age dates that range from about 50 years to modern. Watersheds comprised of quaternary Yellowstone <span class="hlt">volcanics</span> have a large volume of <span class="hlt">active</span> groundwater circulation. A large, advecting groundwater field would be the dominant mechanism for mass and energy transport in the shallow crust of the Yellowstone <span class="hlt">volcanic</span> plateau, and thus control the Yellowstone <span class="hlt">hydrothermal</span> system. ?? 2009 Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BVol...75..729Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BVol...75..729Y"><span>A large <span class="hlt">hydrothermal</span> reservoir beneath Taal Volcano (Philippines) revealed by magnetotelluric resistivity survey: 2D resistivity modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamaya, Y.; Alanis, P. K. B.; Takeuchi, A.; Cordon, J. M.; Mogi, T.; Hashimoto, T.; Sasai, Y.; Nagao, T.</p> <p>2013-07-01</p> <p>Taal Volcano, located in the southwestern part of Luzon Island, Philippines, has frequently experienced catastrophic eruptions from both the Main Crater on Volcano Island and flank eruptions. These eruptions have been magmatic, phreatomagmatic, and <span class="hlt">hydrothermal</span>, with the latter implying the existence of a large-scale <span class="hlt">hydrothermal</span> system beneath the volcano. We conducted an electrical resistivity survey using the magnetotelluric method in order to identify the location and geometry of the <span class="hlt">hydrothermal</span> reservoir and sealing cap rock. Two-dimensional inversion using the observed data indicates four similar resistivity sections. The structure at shallow depths corresponds to <span class="hlt">volcanic</span> deposits and an aquifer. Below 1 km, the structure features a relatively resistive zone beneath the main crater surrounded by a conductive shell. We interpreted these to be a large <span class="hlt">hydrothermal</span> reservoir with an impermeable cap rock sealing it. Recent ground deformation detected by GPS measurements suggests that the <span class="hlt">hydrothermal</span> reservoir is <span class="hlt">active</span>. The interpreted cap rock thins just beneath the main crater and could easily be destroyed by an imbalance in the <span class="hlt">hydrothermal</span> system. We conclude that this <span class="hlt">hydrothermal</span> reservoir plays a significant role in driving catastrophic eruptions that begin with a <span class="hlt">hydrothermal</span> explosion at the main crater.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..353....1C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..353....1C"><span>Gas discharges from the Kueishantao <span class="hlt">hydrothermal</span> vents, offshore northeast Taiwan: Implications for drastic variations of magmatic/<span class="hlt">hydrothermal</span> <span class="hlt">activities</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Xue-Gang; Lyu, Shuang-Shuang; Zhang, Ping-Ping; Yu, Ming-Zhen; Chen, Chen-Tung Arthur; Chen, Yun-Jie; Li, Xiaohu; Jin, Aimin; Zhang, Hai-Yan; Duan, Wei; Ye, Ying</p> <p>2018-03-01</p> <p>The chemical compositions of gas discharges from the Kueishantao (KST) <span class="hlt">hydrothermal</span> field changed dramatically from 2000 to 2014. In this study, we established a gas mixing model for the KST gases. The N2, Ar, and CO2 contents were mixed from a magmatic endmember with CO2 of about 990 mmol/mol, a <span class="hlt">hydrothermal</span> and an atmospheric endmember enriched in N2 and Ar. More than 71% KST gas components were mantle-derived/magmatic. The calculated endmember N2/Ar ratio and Ar contents of the <span class="hlt">hydrothermal</span> endmember (percolated fluid) are about 140 and 5.28-5.52 mmol/mol, respectively. This relatively elevated N2/Ar ratio was probably caused by the thermogenic addition of N2. The log(CH4/CO2) values of the KST gas samples correlate well with the mixing temperature that estimated from the mixing ratio between the percolated fluid and the magmatic endmember. It is indicated that the KST CH4 and CO2 may have attained chemical equilibrium. The temporal variations of the KST gas compositions are determined by the mixing ratio, which is dependent on the magmatic <span class="hlt">activity</span> underneath the KST field. With the decreasing of magmatic <span class="hlt">activity</span> since 2005, the proportion of the <span class="hlt">hydrothermal</span> endmember increased, along with the increasing of N2, Ar, and CH4 contents. This study proposed an effective model to quantitatively assess the sources of gas components discharged from submarine <span class="hlt">hydrothermal</span> vents. In addition, it is suggested that the mixing between a magmatic and a <span class="hlt">hydrothermal</span> endmember may play an important role in the concentrations of CO2 and CH4 in <span class="hlt">hydrothermal</span> gas discharges.</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('http://adsabs.harvard.edu/abs/2018MinDe..53..417B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MinDe..53..417B"><span>Origin of native copper in the Paraná <span class="hlt">volcanic</span> province, Brazil, integrating Cu stable isotopes in a multi-analytical approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baggio, Sérgio Benjamin; Hartmann, Léo Afraneo; Lazarov, Marina; Massonne, Hans-Joachim; Opitz, Joachim; Theye, Thomas; Viefhaus, Tillmann</p> <p>2018-03-01</p> <p>Different hypotheses exist on the origin of native copper mineralization in the Paraná <span class="hlt">volcanic</span> province that invoke magmatic, late magmatic, or <span class="hlt">hydrothermal</span> events. The average copper content in the host basalts is 200 ppm. Native copper occurs as dendrites in cooling joints, fractures, and cavities within amygdaloidal crusts. Cuprite, tenorite, chrysocolla, malachite, and azurite occur in breccias at the top of the lava flows. Chemical analyses, X-ray diffraction, Raman spectrometry, electron microprobe analyses, LA-ICP-MS, and Cu isotope analyses were used to evaluate the origin of native copper in the <span class="hlt">volcanic</span> province. Copper contents in magnetite of the host basalt are close to 1 wt.%, whereas clinopyroxene contains up to 0.04 wt.% Cu. Cretaceous <span class="hlt">hydrothermal</span> alteration of magnetite and clinopyroxene released copper to generate <span class="hlt">hydrothermal</span> copper mineralization. The isotopic composition of the native copper in the Paraná <span class="hlt">volcanic</span> province varies from -0.9‰ in the southeastern portion (Rio Grande do Sul state) to 1.9‰ in the central portion (Paraná state) of the province. This study supports a <span class="hlt">hydrothermal</span> origin followed by supergene enrichment for native copper in the Paraná <span class="hlt">volcanic</span> province.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..596S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..596S"><span>Seismo-<span class="hlt">volcanic</span> monitoring at Furnas Volcano (Azores): radon (222Rn) concentration in groundwater</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Silva, Catarina; Virgílio Cruz, José; Ferreira, Teresa; Viveiros, Fátima; Freire, Pedro; Allard, Patrick</p> <p>2017-04-01</p> <p>The Azores archipelago, located in the middle of the North Atlantic Ocean, is composed of nine <span class="hlt">volcanic</span> islands that formed at the triple junction of the North American, Eurasian and African (Nubian) tectonic plates. These <span class="hlt">volcanic</span> islands were the sites of several eruptions and destructive earthquakes since human settlement in the 15th century. S. Miguel Island, the largest and most densely populated island of the Azores, hosts three <span class="hlt">active</span> strato-volcanoes with calderas. Furnas Volcano is one of these. Its eruptive <span class="hlt">activity</span> has been essentially explosive, involving magmas with trachytic (s.l.) composition. In the last 5000 years at least 10 explosive eruptions occurred inside the caldera of Furnas. The last one occurred in 1630 and was subplinian in character. Since then an intense <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> has persisted, involving four main fumarolic fields, thermal springs, CO2-rich springs, several soil diffuse degassing areas (CO2 and 222Rn), as well as occasional <span class="hlt">hydrothermal</span> explosions. In the past decade we have developed a radon survey of Furnas <span class="hlt">hydrothermal</span> manifestations. Here we report on the radon survey of twelve water springs, located inside the caldera, and representative of the different water types encountered at the volcano (orthothermal, thermal and CO2-rich springs). Bimonthly sampling and determination of radon <span class="hlt">activity</span> and water temperature was performed in the selected springs between years 2007 and 2011. At each sampling point two water samples were collected for radon dosing in laboratory with the RAD7 equipment. A decay correction was applied to each sample. The average radon <span class="hlt">activities</span> were found to vary between 1.15 Bq/L and 29.77 Bq/L, while water temperatures ranged between 16.5 °C and 76.2 °C. As a whole radon <span class="hlt">activities</span> inversely correlate with water temperature, with orthothermal springs showing higher radon <span class="hlt">activity</span> than thermal springs. Temporal variations in both parameters appear to be mainly determined by seasonal variations of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150020807','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150020807"><span>Astrobiology, Mars Exploration and Lassen <span class="hlt">Volcanic</span> National Park</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Des Marais, David J.</p> <p>2015-01-01</p> <p>The search for evidence of life beyond Earth illustrates how the charters of NASA and the National Park Service share common ground. The mission of NPS is to preserve unimpaired the natural and cultural resources of the National Park System for the enjoyment, education and inspiration of this and future generations. NASA's Astrobiology program seeks to understand the origins, evolution and distribution of life in the universe, and it abides by the principles of planetary stewardship, public outreach, and education. We cannot subject planetary exploration destinations to Earthly biological contamination both for ethical reasons and to preserve their scientific value for astrobiology. We respond to the public's interest in the mysteries of life and the cosmos by honoring their desire to participate in the process of discovery. We involve youth in order to motivate career choices in science and technology and to perpetuate space exploration. The search for evidence of past life on Mars illustrates how the missions of NASA and NPS can become synergistic. <span class="hlt">Volcanic</span> <span class="hlt">activity</span> occurs on all rocky planets in our Solar System and beyond, and it frequently interacts with water to create <span class="hlt">hydrothermal</span> systems. On Earth these systems are oases for microbial life. The Mars Exploration Rover Spirit has found evidence of extinct <span class="hlt">hydrothermal</span> system in Gusev crater, Mars. Lassen <span class="hlt">Volcanic</span> National Park provides a pristine laboratory for investigating how microorganisms can both thrive and leave evidence of their former presence in <span class="hlt">hydrothermal</span> systems. NASA scientists, NPS interpretation personnel and teachers can collaborate on field-oriented programs that enhance Mars mission planning, engage students and the public in science and technology, and emphasize the ethics of responsible exploration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016160','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016160"><span>Organic matter in <span class="hlt">hydrothermal</span> metal ores and <span class="hlt">hydrothermal</span> fluids</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Orem, W.H.; Spiker, E. C.; Kotra, R.K.</p> <p>1990-01-01</p> <p>Massive polymetallic sulfides are currently being deposited around <span class="hlt">active</span> submarine <span class="hlt">hydrothermal</span> vents associated with spreading centers. Chemoautolithotrophic bacteria are responsible for the high production of organic matter also associated with modern submarine <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Thus, there is a significant potential for organic matter/metal interactions in these systems. We have studied modern and ancient <span class="hlt">hydrothermal</span> metal ores and modern <span class="hlt">hydrothermal</span> fluids in order to establish the amounts and origin of the organic matter associated with the metal ores. Twenty-six samples from modern and ancient <span class="hlt">hydrothermal</span> systems were surveyed for their total organic C contents. Organic C values ranged from 0.01% to nearly 4.0% in these samples. Metal ores from modern and ancient sediment-covered <span class="hlt">hydrothermal</span> systems had higher organic C values than those from modern and ancient <span class="hlt">hydrothermal</span> systems lacking appreciable sedimentary cover. One massive pyrite sample from the Galapagos spreading center (3% organic C) had stable isotope values of -27.4% (??13C) and 2.1% (??15N), similar to those in benthic siphonophors from <span class="hlt">active</span> vents and distinct from seep sea sedimentary organic matter. This result coupled with other analyses (e.g. 13C NMR, pyrolysis/GC, SEM) of this and other samples suggests that much of the organic matter may originate from chemoautolithotrophic bacteria at the vents. However, the organic matter in <span class="hlt">hydrothermal</span> metal ores from sediment covered vents probably arises from complex sedimentary organic matter by <span class="hlt">hydrothermal</span> pyrolysis. The dissolved organic C concentrations of <span class="hlt">hydrothermal</span> fluids from one site (Juan de Fuca Ridge) were found to be the same as that of background seawater. This result may indicate that dissolved organic C is effectively scavenged from <span class="hlt">hydrothermal</span> fluids by biological <span class="hlt">activity</span> or by co-precipitation with metal ores. ?? 1990.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V24A..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V24A..06R"><span>Characterizing the dynamics of <span class="hlt">hydrothermal</span> systems with muon tomography: the case of La Soufrière de Guadeloupe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rosas-Carbajal, M.; Marteau, J.; Tramontini, M.; de Bremond d Ars, J.; Le Gonidec, Y.; Carlus, B.; Ianigro, J. C.; Deroussi, S.; Komorowski, J. C.; Gibert, D.</p> <p>2017-12-01</p> <p>Muon imaging has recently emerged as a powerful method to complement standard geophysical tools in the study of the Earth's subsurface. Muon measurements yield a radiography of the average density along the muon path, allowing to image large volumes of a geological body from a single observation point. Long-term measurements allow to infer density changes by tracking the associated variations in the muon flux. In the context of <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> systems, this approach helps to characterize zones of steam formation, condensation, water infiltration and storage. We present results of imaging the La Soufrière de Guadeloupe dome and shallow <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system with a network of muon telescopes viewing the dome from different positions around its base. First, we jointly invert the muon radiographies of the different telescopes with gravity data to obtain a three-dimensional density model of the lava dome. The model reveals an extended low density region where the <span class="hlt">hydrothermal</span> system is most <span class="hlt">active</span>. We then analyze the dynamics of the <span class="hlt">hydrothermal</span> system from long-term measurements (more than 2 years of almost <span class="hlt">non</span>-interrupted acquisition) with 5 simultaneous muon telescopes. We identify a periodicity of 1-2 months in the density increase/decrease in the most <span class="hlt">active</span> zones below fumaroles and acid boiling ponds. Our simultaneous-muon telescope strategy provides constraints on the three-dimensional location of the density changes and an improved quantification of the associated mass flux changes. We compare the temporal trends acquired by the different muon telescopes to time-series of rainfall on the summit recharge area as well as to ground temperature profiles in the vicinity of thermal anomalies and high-discharge summit fumaroles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918174J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918174J"><span>Sill induced <span class="hlt">hydrothermal</span> venting: A summary of our current understanding</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jerram, Dougal; Svenesn, Henrik; Planke, Sverre; Millett, John; Reynolds, Pete</p> <p>2017-04-01</p> <p><span class="hlt">Hydrothermal</span> vent structures which are predominantly related with the emplacement of large (>1000 km3) intrusions into the sub-<span class="hlt">volcanic</span> basins represent a specific style of piercement structure, where climate-forcing gases can be transferred into the atmosphere and hydrosphere. In this case, the types and volumes of gas produced by intrusions is heavily dependent on the host-rock sediment properties that they intrude through. The distribution of vent structures can be shown to be widespread in Large Igneous Provinces for example on both the Norwegian and the Greenland margins of the North Atlantic Igneous Province (NAIP). In this overview we assess the distribution, types and occurrence of <span class="hlt">hydrothermal</span> vent structures associated with LIPs. There is particular focus on those within the NAIP using mapped examples from offshore seismic data as well as outcrop analogues, highlighting the variability of these structures and their deposits. As the availability of 3D data from offshore and onshore increases, the full nature of the <span class="hlt">volcanic</span> stratigraphy from the subvolcanic intrusive complexes, through the main eruption cycles into the piercing vent structures, can be realised along the entirety of <span class="hlt">volcanic</span> rifted margins and LIPs. This will help greatly in our understanding of the evolving palaeo-environments, and climate contributions during the evolution of these short lived massive <span class="hlt">volcanic</span> events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20110016075&hterms=Thordarson&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThordarson','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20110016075&hterms=Thordarson&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DThordarson"><span>Integrating Multiple Space Ground Sensors to Track <span class="hlt">Volcanic</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chien, Steve; Davies, Ashley; Doubleday, Joshua; Tran, Daniel; Jones, Samuel; Kjartansson, Einar; Thorsteinsson, Hrobjartur; Vogfjord, Kristin; Guomundsson, Magnus; Thordarson, Thor; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20110016075'); toggleEditAbsImage('author_20110016075_show'); toggleEditAbsImage('author_20110016075_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20110016075_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20110016075_hide"></p> <p>2011-01-01</p> <p><span class="hlt">Volcanic</span> <span class="hlt">activity</span> can occur with little or no warning. Increasing numbers of space borne assets can enable coordinated measurements of <span class="hlt">volcanic</span> events to enhance both scientific study and hazard response. We describe the use of space and ground measurements to target further measurements as part of a worldwide volcano monitoring system. We utilize a number of alert systems including the MODVOLC, GOESVOLC, US Air Force Weather Advisory, and <span class="hlt">Volcanic</span> Ash Advisory Center (VAAC) alert systems. Additionally we use in-situ data from ground instrumentation at a number of <span class="hlt">volcanic</span> sites, including Iceland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5723M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5723M"><span>Tellurium in <span class="hlt">active</span> <span class="hlt">volcanic</span> environments: Preliminary results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milazzo, Silvia; Calabrese, Sergio; D'Alessandro, Walter; Brusca, Lorenzo; Bellomo, Sergio; Parello, Francesco</p> <p>2014-05-01</p> <p>Tellurium is a toxic metalloid and, according to the Goldschmidt classification, a chalcophile element. In the last years its commercial importance has considerably increased because of its wide use in solar cells, thermoelectric and electronic devices of the last generation. Despite such large use, scientific knowledge about volcanogenic tellurium is very poor. Few previous authors report result of tellurium concentrations in <span class="hlt">volcanic</span> plume, among with other trace metals. They recognize this element as volatile, concluding that <span class="hlt">volcanic</span> gases and sulfur deposits are usually enriched with tellurium. Here, we present some results on tellurium concentrations in <span class="hlt">volcanic</span> emissions (plume, fumaroles, ash leachates) and in environmental matrices (soils and plants) affected by <span class="hlt">volcanic</span> emissions and/or deposition. Samples were collected at Etna and Vulcano (Italy), Turrialba (Costa Rica), Miyakejima, Aso, Asama (Japan), Mutnovsky (Kamchatka) at the crater rims by using common filtration techniques for aerosols (polytetrafluoroethylene filters). Filters were both eluted with Millipore water and acid microwave digested, and analyzed by inductively coupled plasma mass spectrometry (ICP-MS). <span class="hlt">Volcanic</span> ashes emitted during explosive events on Etna and Copahue (Argentina) were analyzed for tellurium bulk composition and after leaching experiments to evaluate the soluble fraction of tellurium. Soils and leaves of vegetation were also sampled close to <span class="hlt">active</span> <span class="hlt">volcanic</span> vents (Etna, Vulcano, Nisyros, Nyiragongo, Turrialba, Gorely and Masaya) and investigated for tellurium contents. Preliminary results showed very high enrichments of tellurium in <span class="hlt">volcanic</span> emissions comparing with other volatile elements like mercury, arsenic, thallium and bismuth. This suggests a primary transport in the volatile phase, probably in gaseous form (as also suggested by recent studies) and/or as soluble salts (halides and/or sulfates) adsorbed on the surface of particulate particles and ashes. First</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033475','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033475"><span>Diffuse flow <span class="hlt">hydrothermal</span> manganese mineralization along the <span class="hlt">active</span> Mariana and southern Izu-Bonin arc system, western Pacific</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hein, J.R.; Schulz, M.S.; Dunham, R.E.; Stern, R.J.; Bloomer, S.H.</p> <p>2008-01-01</p> <p>Abundant ferromanganese oxides were collected along 1200 km of the <span class="hlt">active</span> Izu-Bonin-Mariana arc system. Chemical compositions and mineralogy show that samples were collected from two deposit types: Fe-Mn crusts of mixed hydrogenetic/<span class="hlt">hydrothermal</span> origin and <span class="hlt">hydrothermal</span> Mn oxide deposits; this paper addresses only the second type. Mn oxides cement volcaniclastic and biogenic sandstone and breccia layers (Mn sandstone) and form discrete dense stratabound layers along bedding planes and within beds (stratabound Mn). The Mn oxide was deposited within coarse-grained sediments from diffuse flow systems where precipitation occurred below the seafloor. Deposits were exposed at the seabed by faulting, mass wasting, and erosion. Scanning electron microscopy and microprobe analyses indicate the presence of both amorphous and crystalline 10 ?? and 7 ?? manganate minerals, the fundamental chemical difference being high water contents in the amorphous Mn oxides. Alternation of amorphous and crystalline laminae occurs in many samples, which likely resulted from initial rapid precipitation of amorphous Mn oxides from waxing pulses of <span class="hlt">hydrothermal</span> fluids followed by precipitation of slow forming crystallites during waning stages. The chemical composition is characteristic of a <span class="hlt">hydrothermal</span> origin including strong fractionation between Fe (mean 0.9 wt %) and Mn (mean 48 wt %) for the stratabound Mn, generally low trace metal contents, and very low rare earth element and platinum group element contents. However, Mo, Cd, Zn, Cu, Ni, and Co occur in high concentrations in some samples and may be good indicator elements for proximity to the heat source or to massive sulfide deposits. For the Mn sandstones, Fe (mean-8.4%) and Mn (12.4%) are not significantly fractionated because of high Fe contents in the volcaniclastic material. However, the proportion of <span class="hlt">hydrothermal</span> Fe (nondetrital Fe) to total Fe is remarkably constant (49-58%) for all the sample groups, regardless of the degree of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JGRB..113.8S14H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JGRB..113.8S14H"><span>Diffuse flow <span class="hlt">hydrothermal</span> manganese mineralization along the <span class="hlt">active</span> Mariana and southern Izu-Bonin arc system, western Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hein, James R.; Schulz, Marjorie S.; Dunham, Rachel E.; Stern, Robert J.; Bloomer, Sherman H.</p> <p>2008-08-01</p> <p>Abundant ferromanganese oxides were collected along 1200 km of the <span class="hlt">active</span> Izu-Bonin-Mariana arc system. Chemical compositions and mineralogy show that samples were collected from two deposit types: Fe-Mn crusts of mixed hydrogenetic/<span class="hlt">hydrothermal</span> origin and <span class="hlt">hydrothermal</span> Mn oxide deposits; this paper addresses only the second type. Mn oxides cement volcaniclastic and biogenic sandstone and breccia layers (Mn sandstone) and form discrete dense stratabound layers along bedding planes and within beds (stratabound Mn). The Mn oxide was deposited within coarse-grained sediments from diffuse flow systems where precipitation occurred below the seafloor. Deposits were exposed at the seabed by faulting, mass wasting, and erosion. Scanning electron microscopy and microprobe analyses indicate the presence of both amorphous and crystalline 10 Å and 7 Å manganate minerals, the fundamental chemical difference being high water contents in the amorphous Mn oxides. Alternation of amorphous and crystalline laminae occurs in many samples, which likely resulted from initial rapid precipitation of amorphous Mn oxides from waxing pulses of <span class="hlt">hydrothermal</span> fluids followed by precipitation of slow forming crystallites during waning stages. The chemical composition is characteristic of a <span class="hlt">hydrothermal</span> origin including strong fractionation between Fe (mean 0.9 wt %) and Mn (mean 48 wt %) for the stratabound Mn, generally low trace metal contents, and very low rare earth element and platinum group element contents. However, Mo, Cd, Zn, Cu, Ni, and Co occur in high concentrations in some samples and may be good indicator elements for proximity to the heat source or to massive sulfide deposits. For the Mn sandstones, Fe (mean 8.4%) and Mn (12.4%) are not significantly fractionated because of high Fe contents in the volcaniclastic material. However, the proportion of <span class="hlt">hydrothermal</span> Fe (nondetrital Fe) to total Fe is remarkably constant (49-58%) for all the sample groups, regardless of the degree of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatAs...1..841C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatAs...1..841C"><span>Powering prolonged <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> inside Enceladus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choblet, Gaël; Tobie, Gabriel; Sotin, Christophe; Běhounková, Marie; Čadek, Ondřej; Postberg, Frank; Souček, Ondřej</p> <p>2017-12-01</p> <p>Geophysical data from the Cassini spacecraft imply the presence of a global ocean underneath the ice shell of Enceladus1, only a few kilometres below the surface in the South Polar Terrain2-4. Chemical analyses indicate that the ocean is salty5 and is fed by ongoing <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>6-8. In order to explain these observations, an abnormally high heat power (>20 billion watts) is required, as well as a mechanism to focus endogenic <span class="hlt">activity</span> at the south pole9,10. Here, we show that more than 10 GW of heat can be generated by tidal friction inside the unconsolidated rocky core. Water transport in the tidally heated permeable core results in hot narrow upwellings with temperatures exceeding 363 K, characterized by powerful (1-5 GW) hotspots at the seafloor, particularly at the south pole. The release of heat in narrow regions favours intense interaction between water and rock, and the transport of <span class="hlt">hydrothermal</span> products from the core to the plume sources. We are thus able to explain the main global characteristics of Enceladus: global ocean, strong dissipation, reduced ice-shell thickness at the south pole and seafloor <span class="hlt">activity</span>. We predict that this endogenic <span class="hlt">activity</span> can be sustained for tens of millions to billions of years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V13C3144U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V13C3144U"><span>Dynamic of the <span class="hlt">volcanic</span> <span class="hlt">activity</span> of La Soufrière volcano (Guadeloupe, Lesser Antillles): Evidence for shallow fluid seismic sources</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ucciani, G.; Beauducel, F.; Bouin, M. P.; Nercessian, A.</p> <p>2015-12-01</p> <p>La Soufrière is one of the many hazardous volcanoes in the inner arc of Lesser Antilles. Located South of Basse-Terre island, it is the only <span class="hlt">active</span> volcano of the Guadeloupe archipelago. Since the last significant magmatic eruption in 1535 AD, the <span class="hlt">activity</span> has been exculsively phreatic. Since 1992 and the abrupt renewal of seismic and fumarollic <span class="hlt">activities</span>, the Guadeloupe Volcanological and Seismological Observatory (OVSG-IPGP) has recorded a progressive increasing of seismicity and degassing that led scientists and authorities to set the alert level ``Vigilance'' and hold it until today. According to the recent geophysical, geochemical and geological studies, the current <span class="hlt">volcanic</span> <span class="hlt">activity</span> of la Soufrière volcano seems to be exclusively associated to the <span class="hlt">hydrothermal</span> system, while the link with seismic <span class="hlt">activity</span> is still poorly studied. In this context of possible pre-eruptive unrest, we investigated the spatial and temporal variations of the seismicity recorded between 1981 and 2013. From a consistent seismological framework coupling spectral, statistical, signal processing, clustering, and inverse problems methods, we demonstrate that this seismicity is largely generated by shallow <span class="hlt">hydrothermal</span> fluid sources located in a complex plumbing system. Spatial variations of Vp/Vs ratio and B-value in seismogenic structures allow us to document three main seismic zones associated to : (1) migration of magmatic gas, (2) the storage and mixing of underground water and gas and (3) the shallow migration of <span class="hlt">hydrothermal</span> fluids in high fractured and heterogeneous system. Waveform analysis revealed a low number of significant families consistent with fracturing process, and the temporal evolution of multiplet <span class="hlt">activities</span> highlighted several variations associated with surface manifestations and brutal dynamic changes after major local tectonic earthquakes of Les Saintes (21 November 2004, Mw=6.3), its main aftershock (14 February 2005, Mw=5.7) and the last major earthquake of la</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4771442','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4771442"><span>3.5-Ga <span class="hlt">hydrothermal</span> fields and diamictites in the Barberton Greenstone Belt—Paleoarchean crust in cold environments</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>de Wit, Maarten J.; Furnes, Harald</p> <p>2016-01-01</p> <p>Estimates of ocean temperatures on Earth 3.5 billion years ago (Ga) range between 26° and 85°C. We present new data from 3.47- to 3.43-Ga <span class="hlt">volcanic</span> rocks and cherts in South Africa suggesting that these temperatures reflect mixing of hot <span class="hlt">hydrothermal</span> fluids with cold marine and terrestrial waters. We describe fossil <span class="hlt">hydrothermal</span> pipes that formed at ~200°C on the sea floor >2 km below sea level. This ocean floor was uplifted tectonically to sea level where a subaerial <span class="hlt">hydrothermal</span> system was <span class="hlt">active</span> at 30° to 270°C. We also describe shallow-water glacial diamictites and diagenetic sulfate mineral growth in abyssal muds. These new observations reveal that both <span class="hlt">hydrothermal</span> systems operated in relatively cold environments and that Earth’s surface temperatures in the early Archean were similar to those in more recent times. PMID:26933677</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T13B2708W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T13B2708W"><span>Time-dependent changes in magmatic and <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> at the Costa Rica Rift recorded by variations in oceanic crustal structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, D. J.; Peirce, C.; Hobbs, R. W.; Gregory, E. P. M.; Zhang, L.</p> <p>2016-12-01</p> <p>Geophysical studies of crustal structure at a diverse range of ridges have provided evidence that the balance between spreading rate and magma supply determines whether spreading predominantly occurs by magmatic accretion of new oceanic crust or through tectonic stretching of the whole lithosphere. Asymmetric spreading, patterns of on- and off-axis <span class="hlt">volcanism</span>, the evolution of oceanic core complexes and the distribution of <span class="hlt">hydrothermal</span> systems all indicate that the process of spreading is not constant over geologically short timescales. The structure of the resulting crust reflects this complexity in origin. Studies along flow-lines across ridges spreading at intermediate rates suggest variations in topographic style and crustal structure have periodically occurred, controlled by the interplay between magmatic accretion and tectonic stretching, and coupled to the degree of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Seismic reflection images and tomographic models derived from wide-angle seismic data have enabled a detailed examination of the oceanic crust that formed at the fast-to-intermediate-spreading (36 mm yr-1) Costa Rica Rift over the last 6 Ma, to look for any temporal variation in basement topography, upper crust (layer 2) P-wave velocity/density structure and crustal thickness. Coincident marine gravity and magnetic data not only allow us to test the validity of the final velocity-density model but also review variability in half-spreading rate, respectively. Collectively our analyses allow us to investigate the timescale and cyclicity of crustal structure variations and, having determined the spreading rate over time, consider how this may reflect changes in magma supply and/or <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> at the Costa Rica Rift, using borehole 504B as the ground-truth. This research is part of a major, interdisciplinary NERC-funded collaboration entitled: Oceanographic and Seismic Characterisation of heat dissipation and alteration by <span class="hlt">hydrothermal</span> fluids at an Axial Ridge (OSCAR).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1999/0448/pdf/1997SummaryofEventsAVO.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1999/0448/pdf/1997SummaryofEventsAVO.pdf"><span>1997 <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Alaska and Kamchatka: summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Wallace, Kristi L.</p> <p>1999-01-01</p> <p>The Alaska Volcano Observatory (AVO) monitors over 40 historically <span class="hlt">active</span> volcanoes along the Aleutian Arc. Twenty are seismically monitored and for the rest, the AVO monitoring program relies mainly on pilot reports, observations of local residents and ship crews, and daily analysis of satellite images. In 1997, AVO responded to eruptive <span class="hlt">activity</span> or suspect <span class="hlt">volcanic</span> <span class="hlt">activity</span> at 11 <span class="hlt">volcanic</span> centers: Wrangell, Sanford, Shrub mud volcano, Iliamna, the Katmai group (Martin, Mageik, Snowy, and Kukak volcanoes), Chiginagak, Pavlof, Shishaldin, Okmok, Cleveland, and Amukta. Of these, AVO has real-time, continuously recording seismic networks at Iliamna, the Katmai group, and Pavlof. The phrase “suspect <span class="hlt">volcanic</span> activity” (SVA), used to characterize several responses, is an eruption report or report of unusual <span class="hlt">activity</span> that is subsequently determined to be normal or enhanced fumarolic <span class="hlt">activity</span>, weather-related phenomena, or a <span class="hlt">non-volcanic</span> event. In addition to responding to eruptive <span class="hlt">activity</span> at Alaska volcanoes, AVO also disseminated information for the Kamchatkan <span class="hlt">Volcanic</span> Eruption Response Team (KVERT) about the 1997 <span class="hlt">activity</span> of 5 Russian volcanoes--Sheveluch, Klyuchevskoy, Bezymianny, Karymsky, and Alaid (SVA). This report summarizes <span class="hlt">volcanic</span> <span class="hlt">activity</span> and SVA in Alaska during 1997 and the AVO response, as well as information on the reported <span class="hlt">activity</span> at the Russian volcanoes. Only those reports or inquiries that resulted in a “significant” investment of staff time and energy (here defined as several hours or more for reaction, tracking, and follow-up) are included. AVO typically receives dozens of reports throughout the year of steaming, unusual cloud sightings, or eruption rumors. Most of these are resolved quickly and are not tabulated here as part of the 1997 response record.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150006657&hterms=hydrothermal+plumes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dhydrothermal%2Bplumes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150006657&hterms=hydrothermal+plumes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dhydrothermal%2Bplumes"><span>Enceladus: Starting <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Matson, D. L.; Castillo-Rogez, J. C.; Johnson, T. V.; Lunine, J. I.; Davies, A. G.</p> <p>2011-01-01</p> <p>We describe a process for starting the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in Enceladus' South Polar Region. The process takes advantage of fissures that reach the water table, about 1 kilometer below the surface. Filling these fissures with fresh ocean water initiates a flow of water up from an ocean that can be self-sustaining. In this hypothesis the heat to sustain the thermal anomalies and the plumes comes from a slightly warm ocean at depth. The heat is brought to the surface by water that circulates up, through the crust and then returns to the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMNH13B1929M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMNH13B1929M"><span>California's Vulnerability to <span class="hlt">Volcanic</span> Hazards: What's at Risk?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mangan, M.; Wood, N. J.; Dinitz, L.</p> <p>2015-12-01</p> <p>California is a leader in comprehensive planning for devastating earthquakes, landslides, floods, and tsunamis. Far less attention, however, has focused on the potentially devastating impact of <span class="hlt">volcanic</span> eruptions, despite the fact that they occur in the State about as frequently as the largest earthquakes on the San Andreas Fault Zone. At least 10 eruptions have occurred in the past 1,000 years—most recently in northern California (Lassen Peak 1914 to 1917)—and future <span class="hlt">volcanic</span> eruptions are inevitable. The likelihood of renewed <span class="hlt">volcanism</span> in California is about one in a few hundred to one in a few thousand annually. Eight young volcanoes, ranked as Moderate to Very High Threat [1] are dispersed throughout the State. Partially molten rock (magma) resides beneath at least seven of these—Medicine Lake Volcano, Mount Shasta, Lassen <span class="hlt">Volcanic</span> Center, Clear Lake <span class="hlt">Volcanic</span> Field, Long Valley <span class="hlt">Volcanic</span> Region, Coso <span class="hlt">Volcanic</span> Field, and Salton Buttes— causing earthquakes, toxic gas emissions, <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>, and (or) ground deformation. Understanding the hazards and identifying what is at risk are the first steps in building community resilience to <span class="hlt">volcanic</span> disasters. This study, prepared in collaboration with the State of California Governor's Office of Emergency Management and the California Geological Survey, provides a broad perspective on the State's exposure to volcano hazards by integrating mapped volcano hazard zones with geospatial data on at-risk populations, infrastructure, and resources. The study reveals that ~ 16 million acres fall within California's volcano hazard zones, along with ~ 190 thousand permanent and 22 million transitory populations. Additionally, far-field disruption to key water delivery systems, agriculture, utilities, and air traffic is likely. Further site- and sector-specific analyses will lead to improved hazard mitigation efforts and more effective disaster response and recovery. [1] "<span class="hlt">Volcanic</span> Threat and Monitoring Capabilities</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V43A2847A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V43A2847A"><span>Field occurrence and lithology of Archean <span class="hlt">hydrothermal</span> systems in the 3.2Ga Dixon Island Formation, Western Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aihara, Y.; Kiyokawa, S.; Ito, T.; Ikehara, M.; Yamaguchi, K. E.; Horie, K.; Sakamoto, R.; Miki, T.</p> <p>2013-12-01</p> <p> Si and K and depleted in Mg, occurred earlier than the formation of black chert veins and probably during sedimentation of the overlying Black Chert member. Petrographycally, tourmaline in Type1 veins formed by <span class="hlt">hydrothermal</span> processes and can be used to infer physicochemical conditions of the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Fragmentation of black chert and <span class="hlt">volcanic</span> rocks within Type 2 veins was probably due to high pressure caused by <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70046832','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70046832"><span>Learning to recognize <span class="hlt">volcanic</span> <span class="hlt">non</span>-eruptions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Poland, Michael P.</p> <p>2010-01-01</p> <p>An important goal of volcanology is to answer the questions of when, where, and how a volcano will erupt—in other words, eruption prediction. Generally, eruption predictions are based on insights from monitoring data combined with the history of the volcano. An outstanding example is the A.D. 1980–1986 lava dome growth at Mount St. Helens, Washington (United States). Recognition of a consistent pattern of precursors revealed by geophysical, geological, and geochemical monitoring enabled successful predictions of more than 12 dome-building episodes (Swanson et al., 1983). At <span class="hlt">volcanic</span> systems that are more complex or poorly understood, probabilistic forecasts can be useful (e.g., Newhall and Hoblitt, 2002; Marzocchi and Woo, 2009). In such cases, the probabilities of different types of <span class="hlt">volcanic</span> events are quantified, using historical accounts and geological studies of a volcano's past <span class="hlt">activity</span>, supplemented by information from similar volcanoes elsewhere, combined with contemporary monitoring information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V23A0469S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V23A0469S"><span>Assessing <span class="hlt">volcanic</span> hazard at the most populated caldera in the world: Campi Flegrei, Southern Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Somma, R.; de Natale, G.; Troise, C.; Kilburn, C.; Moretti, R.</p> <p>2017-12-01</p> <p>Naples and its hinterland in Southern Italy are one of the most urbanized areas in the world under threat from <span class="hlt">volcanic</span> <span class="hlt">activity</span>. The region lies within range of three <span class="hlt">active</span> <span class="hlt">volcanic</span> centers: Vesuvius, Campi Flegrei, and Ischia. The Campi Flegrei caldera, in particular, has been in unrest for six decades. The unrest followed four centuries of quiescence and has heightened concern about an increased potential for eruption. Innovative geochemical and geophysical analysis, combined with scientific drilling, are being used to investigate Campi Flegrei. Results highlight key directions for better understanding the mechanisms of caldera formation and the respective roles of magma intrusion and <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in determining the volcano's behavior. They also provide a framework for evaluating and mitigating the risk from this caldera and other large ones worldwide.</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/2013AGUFMGP13A1133C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGP13A1133C"><span>High-resolution AUV-based near bottom magnetic surveys at Palinuro <span class="hlt">volcanic</span> complex (Southern Tyrrhenian Sea)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cocchi, L.; Plunkett, S.; Augustin, N.; Petersen, S.</p> <p>2013-12-01</p> <p>In this paper we present the preliminary results of new near bottom magnetic datasets collected during the recent POS442 cruise using the autonomous underwater vehicle (AUV) Abyss. The Southern Tyrrhenian basin is characterized by deep seafloor interspersed with huge <span class="hlt">volcanic</span> seamounts (e.g Vavilov and Marsili and those associated to the Aeolian <span class="hlt">volcanic</span> arc), which were formed during eastward roll back of the Apennine subduction system. These submarine edifices often are affected by significant <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and associated mineral deposits such as those observed at Marsili, Palinuro and Panarea. The western part of the Palinuro <span class="hlt">volcanic</span> complex is characterized by a half rim of a caldera-like structure and hosts <span class="hlt">hydrothermal</span> barite-pyrite deposits. Until recently, the full extent of the <span class="hlt">hydrothermal</span> system remained poorly defined, as exploration has been limited to a few specific sites. In November 2012, a set of high resolution near seafloor geophysical surveys were carried out using GEOMAR's AUV Abyss to attempt to better define the <span class="hlt">hydrothermal</span> mineralization at Palinuro. Five AUV dives were performed, mapping a total area of 3.7 km2 over the western part of Palinuro. Geomar's Abyss AUV (a Remus6000 class vehicle) was equipped with an Applied Physics Systems flux gate magnetometer, writing to a stand alone data logger, powered by the AUV's main batteries. The 5 dives were performed within the same area but with different primary geophysical sensors (multibeam, sidescan sonar, subbottom profiler), survey altitudes above seafloor (100m, 40m) and line spacing (150m, 100m, 20m). Magnetic data was collect on all five dives. At the beginning of each dive, the AUV performed a set of calibration manoeuvres, involving a 360 degree heading variation, a set of three upwards/downwards pitches, and three port and starboard yaws. This magnetic data reveals the magnetization features of the seafloor in unprecedented detail, highlighting a complex pattern mostly due to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1411673E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1411673E"><span>High resolution imaging of the Methana <span class="hlt">volcanic</span> complex, Greece, with magnetotelluric and aeromagnetic data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Efstathiou, A.; Tzanis, A.; Chailas, S.; Lagios, E.; Stamatakis, M.</p> <p>2012-04-01</p> <p>The Methana calc-alkaline <span class="hlt">volcanic</span> complex is located off the NE coast of Argolis Peninsula (Peloponnesus, Greece) at the NW terminus of the Hellenic <span class="hlt">Volcanic</span> Arc (HVA). It consists of approximately 32 domes, with the most recent eruptive episodes dated to 258 BCE and 1700 CE. Herein, we report the results an attempt to investigate the volcano's interior with joint interpretation of Magnetotelluric and Aeromagnetic data. The aeromagnetic data was inverted with the UBC-GIF 3D magnetic inversion suite, constrained by several in-situ susceptibility measurements. At depths to 2 km, the inversion resolves individual intrusions corresponding to known phases of <span class="hlt">volcanic</span> <span class="hlt">activity</span> (domes), with susceptibilities >0.1. At depths greater than 4.5 km, a more weakly magnetized domain is detected (~0.025); its ceiling is well resolved; its floor cannot be placed with certainty but extends to at least 7 km. The depths are comparable to those of magma chambers. Based on the palaeomagnetic analysis of nearby <span class="hlt">volcanic</span> rocks, it may be safely suggested that its temperature should not be higher than 550-600°C, but also not considerably lower. It may comprise a magma chamber, inasmuch as it compares well with the temperatures and locations of known magma chambers along the HVA. Finally, there's exists evidence of the location of the vents through which the extrusive <span class="hlt">activity</span> has taken place. A Magnetotelluric survey comprising 14 stations was conducted IN 1992, as part of a geothermal project. Herein, this data is reevaluated with modern analysis methods and re-interpreted with 2D inversion. The results indicate the presence of conductors at depths of 1500-2500 m beneath the centre of the Peninsula, extensive horizontal conductors at, or just below sea level and conductive protrusions above sea level. The joint interpretation of the susceptibility and geoelectric images is based on the premise that they both are generated by <span class="hlt">hydrothermal</span> circulation which depresses resistivity and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020773','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020773"><span><span class="hlt">Active</span> <span class="hlt">Volcanism</span> on Io as Seen by Galileo SSI</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McEwen, A.S.; Keszthelyi, L.; Geissler, P.; Simonelli, D.P.; Carr, M.H.; Johnson, T.V.; Klaasen, K.P.; Breneman, H.H.; Jones, T.J.; Kaufman, J.M.; Magee, K.P.; Senske, D.A.; Belton, M.J.S.; Schubert, G.</p> <p>1998-01-01</p> <p><span class="hlt">Active</span> <span class="hlt">volcanism</span> on Io has been monitored during the nominal Galileo satellite tour from mid 1996 through late 1997. The Solid State Imaging (SSI) experiment was able to observe many manifestations of this <span class="hlt">active</span> <span class="hlt">volcanism</span>, including (1) changes in the color and albedo of the surface, (2) <span class="hlt">active</span> airborne plumes, and (3) glowing vents seen in eclipse. About 30 large-scale (tens of kilometers) surface changes are obvious from comparison of the SSI images to those acquired by Voyager in 1979. These include new pyroclastic deposits of several colors, bright and dark flows, and caldera-floor materials. There have also been significant surface changes on Io during the Galileo mission itself, such as a new 400-km-diameter dark pyroclastic deposit around Pillan Patera. While these surface changes are impressive, the number of large-scale changes observed in the four months between the Voyager 1 and Voyager 2 flybys in 1979 suggested that over 17 years the cumulative changes would have been much more impressive. There are two reasons why this was not actually the case. First, it appears that the most widespread plume deposits are ephemeral and seem to disappear within a few years. Second, it appears that a large fraction of the <span class="hlt">volcanic</span> <span class="hlt">activity</span> is confined to repeated resurfacing of dark calderas and flow fields that cover only a few percent of Io's surface. The plume monitoring has revealed 10 <span class="hlt">active</span> plumes, comparable to the 9 plumes observed by Voyager. One of these plumes was visible only in the first orbit and three became <span class="hlt">active</span> in the later orbits. Only the Prometheus plume has been consistently <span class="hlt">active</span> and easy to detect. Observations of the Pele plume have been particularly intriguing since it was detected only once by SSI, despite repeated attempts, but has been detected several times by the Hubble Space Telescope at 255 nm. Pele's plume is much taller (460 km) than during Voyager 1 (300 km) and much fainter at visible wavelengths. Prometheus-type plumes (50</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998Icar..135..181M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998Icar..135..181M"><span><span class="hlt">Active</span> <span class="hlt">Volcanism</span> on Io as Seen by Galileo SSI</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McEwen, Alfred S.; Keszthelyi, Laszlo; Geissler, Paul; Simonelli, Damon P.; Carr, Michael H.; Johnson, Torrence V.; Klaasen, Kenneth P.; Breneman, H. Herbert; Jones, Todd J.; Kaufman, James M.; Magee, Kari P.; Senske, David A.; Belton, Michael J. S.; Schubert, Gerald</p> <p>1998-09-01</p> <p><span class="hlt">Active</span> <span class="hlt">volcanism</span> on Io has been monitored during the nominal Galileo satellite tour from mid 1996 through late 1997. The Solid State Imaging (SSI) experiment was able to observe many manifestations of this <span class="hlt">active</span> <span class="hlt">volcanism</span>, including (1) changes in the color and albedo of the surface, (2) <span class="hlt">active</span> airborne plumes, and (3) glowing vents seen in eclipse. About 30 large-scale (tens of kilometers) surface changes are obvious from comparison of the SSI images to those acquired by Voyager in 1979. These include new pyroclastic deposits of several colors, bright and dark flows, and caldera-floor materials. There have also been significant surface changes on Io during the Galileo mission itself, such as a new 400-km-diameter dark pyroclastic deposit around Pillan Patera. While these surface changes are impressive, the number of large-scale changes observed in the four months between the Voyager 1 and Voyager 2 flybys in 1979 suggested that over 17 years the cumulative changes would have been much more impressive. There are two reasons why this was not actually the case. First, it appears that the most widespread plume deposits are ephemeral and seem to disappear within a few years. Second, it appears that a large fraction of the <span class="hlt">volcanic</span> <span class="hlt">activity</span> is confined to repeated resurfacing of dark calderas and flow fields that cover only a few percent of Io's surface. The plume monitoring has revealed 10 <span class="hlt">active</span> plumes, comparable to the 9 plumes observed by Voyager. One of these plumes was visible only in the first orbit and three became <span class="hlt">active</span> in the later orbits. Only the Prometheus plume has been consistently <span class="hlt">active</span> and easy to detect. Observations of the Pele plume have been particularly intriguing since it was detected only once by SSI, despite repeated attempts, but has been detected several times by the Hubble Space Telescope at 255 nm. Pele's plume is much taller (460 km) than during Voyager 1 (300 km) and much fainter at visible wavelengths. Prometheus-type plumes (50</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..354..102N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..354..102N"><span>Furthering the investigation of eruption styles through quantitative shape analyses of <span class="hlt">volcanic</span> ash particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nurfiani, D.; Bouvet de Maisonneuve, C.</p> <p>2018-04-01</p> <p><span class="hlt">Volcanic</span> ash morphology has been quantitatively investigated for various aims such as studying the settling velocity of ash for modelling purposes and understanding the fragmentation processes at the origin of explosive eruptions. In an attempt to investigate the usefulness of ash morphometry for monitoring purposes, we analyzed the shape of <span class="hlt">volcanic</span> ash particles through a combination of (1) traditional shape descriptors such as solidity, convexity, axial ratio and form factor and (2) fractal analysis using the Euclidean Distance transform (EDT) method. We compare ash samples from the <span class="hlt">hydrothermal</span> eruptions of Iwodake (Japan) in 2013, Tangkuban Perahu (Indonesia) in 2013 and Marapi (Sumatra, Indonesia) in 2015, the dome explosions of Merapi (Java, Indonesia) in 2013, the Vulcanian eruptions of Merapi in 2010 and Tavurvur (Rabaul, Papaua New Guinea) in 2014, and the Plinian eruption of Kelud (Indonesia) in 2014. Particle size and shape measurements were acquired from a Particle Size Analyzer with a microscope camera attached to the instrument. Clear differences between dense/blocky particles from <span class="hlt">hydrothermal</span> or dome explosions and vesicular particles produced by the fragmentation of gas-bearing molten magma are well highlighted by conventional shape descriptors and the fractal method. In addition, subtle differences between dense/blocky particles produced by <span class="hlt">hydrothermal</span> explosions, dome explosions, or quench granulation during phreatomagmatic eruptions can be evidenced with the fractal method. The combination of shape descriptors and fractal analysis is therefore potentially able to distinguish between juvenile and <span class="hlt">non</span>-juvenile magma, which is of importance for eruption monitoring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018616','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018616"><span><span class="hlt">Hydrothermal</span> mineralization along submarine rift zones, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hein, J.R.; Gibbs, A.E.; Clague, D.A.; Torresan, M.</p> <p>1996-01-01</p> <p>Describes mineralization of midplate submarine rift zones and <span class="hlt">hydrothermal</span> manganese oxide mineralization of midplate <span class="hlt">volcanic</span> edifices. <span class="hlt">Hydrothermal</span> Mn oxides were recovered from submarine extensions of two Hawaiian rift zones, along Haleakala and Puna Ridges. These Mn oxides form two types of deposits, metallic stratiform layers in volcaniclastic rocks and cement for clastic rocks; both deposit types are composed of todorokite and birnessite. Unlike most other <span class="hlt">hydrothermal</span> Mn oxide deposits, those from Hawaiian rift zones are enriched in the trace metals Zn, Co, Ba, Mo, Sr, V, and especially Ni. Metals are derived from three sources: mafic and ultramafic rocks leached by circulating <span class="hlt">hydrothermal</span> fluids, clastic material (in Mn-cemented sandstone), and seawater that mixed with the <span class="hlt">hydrothermal</span> fluids. Precipitation of Mn oxide below the seafloor is indicated by its occurrence as cement, growth textures that show mineralizing fluids were introduced from below, and pervasive replacement of original matrix of clastic rocks.<span class="hlt">Hydrothermal</span> Mn oxides were recovered from submarine extensions of two Hawaiian rift zones, along Haleakala and Puna Ridges. These Mn oxides form two types of deposits, metallic stratiform layers in volcaniclastic rocks and cement for clastic rocks. Both deposit types are composed of todorokite and birnessite. This article describes in detail the specific characteristics of these Mn oxides.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T23F..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T23F..06D"><span>Amagmatic Accretionary Segments, Ultraslow Spreading and <span class="hlt">Non-Volcanic</span> Rifted Margins (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dick, H. J.; Snow, J. E.</p> <p>2009-12-01</p> <p>The evolution of <span class="hlt">non-volcanic</span> rifted margins is key to understanding continental breakup and the early evolution of some of the world’s most productive hydrocarbon basins. However, the early stages of such rifting are constrained by limited observations on ancient heavily sedimented margins such as Newfoundland and Iberia. Ultraslow spreading ridges, however, provide a modern analogue for early continental rifting. Ultraslow spreading ridges (<20 mm/yr) comprise ~30% of the global ridge system (e.g. Gakkel, Southwest Indian, Terceira, and Knipovitch Ridges). They have unique tectonics with widely spaced <span class="hlt">volcanic</span> segments and amagmatic accretionary ridge segments. The <span class="hlt">volcanic</span> segments, though far from hot spots, include some of the largest axial volcanoes on the global ridge system, and have, unusual magma chemistry, often showing local isotopic and incompatible element enrichment unrelated to mantle hot spots. The transition from slow to ultraslow tectonics and spreading is not uniquely defined by spreading rate, and may also be moderated by magma supply and mantle temperature. Amagmatic accretionary segments are the 4th class of plate boundary structure, and, we believe, the defining tectonic feature of early continental breakup. They form at effective spreading rates <12 mm/yr, assume any orientation to spreading, and replace transform faults and magmatic segments. At amagmatic segments the earth splits apart with the mantle emplaced directly to the seafloor, and great slabs of peridotite are uplifted to form the rift mountains. A thick conductive lid suppresses mantle melting, and magmatic segments form only at widely spaced intervals, with only scattered <span class="hlt">volcanics</span> in between. Amagmatic segments link with the magmatic segments forming curvilinear plate boundaries, rather than the step-like morphology found at faster spreading ridges. These are all key features of <span class="hlt">non-volcanic</span> rifted margins; explaining, for example, the presence of mantle peridotites emplaced</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BVol...80...31D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BVol...80...31D"><span>Changes in heat released by <span class="hlt">hydrothermal</span> circulation monitored during an eruptive cycle at Mt. Etna (Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Diliberto, I. S.; Gagliano Candela, E.; Morici, S.; Pecoraino, G.; Bellomo, S.; Bitetto, M.; Longo, M.</p> <p>2018-04-01</p> <p>The shallow vertical temperature profile has been measured in the proximity of an eruptive fissure far about 4 km north-northeast from Mt. Etna central craters. The monitoring site was a steam-heated soil lying between a group of flank fractures on the upper northeast flank of Mt. Etna (Italy), i.e., on the northeast rift. We chose this area because it was close to an eruptive fissure, that opened in 2002 and extended from about 2500 to about 1500 m a.s.l., with our aim being to determine a connection between this fracture system and the ongoing <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Heat flux anomalies from the ground from September 2009 to September 2012 were evaluated. Changes in the <span class="hlt">hydrothermal</span> release—which can be related to variations in <span class="hlt">volcanic</span> activity—are discussed and compared to the published geophysical data. The heat flux ranges varied during the pre-eruptive (from about 7 to 38 W × m-2), syn-eruptive (from about 3 to 49 W × m-2), and post-eruptive phases, with the heat released being lowest at the latter phase (from about 1 to 20 W × m-2). Moreover, the heat flux time variation was strongly correlated with the eruption rate from the new southeast crater between January 2011 and April 2012. The migration of magma through <span class="hlt">active</span> conduits acts as a changing heating source for steam-heated soils located above the <span class="hlt">active</span> fractures. Our findings suggest that tracking the heat flux above <span class="hlt">active</span> fractures constitutes a useful investigation field for low-cost thermal monitoring of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Time variations in their emissions could highlight the relationship between a <span class="hlt">hydrothermal</span> circuit and the local network of fractures, possibly indicating variation in the structural weakness of a <span class="hlt">volcanic</span> edifice. Continuous monitoring of heat flux, combined with a realistic model, would contribute to multidisciplinary investigations aimed at evaluating changes in volcano dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT........46S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT........46S"><span>Intraplate <span class="hlt">volcanism</span> of the Western Pacific: New insights from geological and geophysical observations in the Pigafetta Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stadler, Timothy J.</p> <p></p> <p>Understanding intraplate <span class="hlt">volcanism</span> is a key to deciphering the Earth's magmatic history. One of the largest intraplate <span class="hlt">volcanic</span> events occurred during the mid Cretaceous, roughly 75 to 125 Ma in the western Pacific. To investigate the origin and effects of this <span class="hlt">volcanism</span> on various Earth systems, we present the first comprehensive study of <span class="hlt">volcanism</span> in the Pigafetta Basin using seismic surveys, magnetic and gravity modeling, and Ocean Drilling Program drill core and well log data from Site 801. Our results show that intraplate <span class="hlt">volcanism</span> in the Pigafetta Basin coincides with the rest of the western Pacific, supporting the plumelets scenario for the origin of intraplate <span class="hlt">volcanism</span> during the mid Cretaceous <span class="hlt">volcanic</span> event. We also discover that the late stage <span class="hlt">volcanism</span> does not overprint the original ocean crust in the Pigafetta Basin, and hence, marine magnetic anomalies recorded in the Jurassic basement are preserved. Also, the formerly identified Rough Smooth Boundary (RSB) is indistinguishable from any other rough-smooth topographic boundaries throughout the survey area suggesting that the RSB is unlikely to be a Cretaceous sill-Jurassic basement boundary. Lastly, the apparent ages and spatial distribution of <span class="hlt">volcanic</span> features suggests a dynamic history of <span class="hlt">hydrothermal</span> circulation in the Pigafetta Basin, indicating that <span class="hlt">hydrothermal</span> circulation was ongoing well past 100 Ma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GGG....16.3015S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GGG....16.3015S"><span>Intraplate <span class="hlt">volcanism</span> of the western Pacific: New insights from geological and geophysical observations in the Pigafetta Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stadler, Timothy J.; Tominaga, Masako</p> <p>2015-09-01</p> <p>Understanding intraplate <span class="hlt">volcanism</span> is a key to deciphering the Earth's magmatic history. One of the largest intraplate <span class="hlt">volcanic</span> events occurred during the mid-Cretaceous, roughly 75-125 Ma in the western Pacific. To investigate the origin of this <span class="hlt">volcanism</span> we present the first comprehensive study of <span class="hlt">volcanism</span> in the Pigafetta Basin using seismic surveys, magnetic and gravity modeling, and Ocean Drilling Program (ODP) drill core and well log data from Site 801. Our results show that intraplate <span class="hlt">volcanism</span> in the Pigafetta Basin coincides with the rest of the western Pacific seamount provinces, supporting the previously suggested plumelets scenario for the origin of intraplate <span class="hlt">volcanism</span> during the mid-Cretaceous <span class="hlt">volcanic</span> events. Our magnetic modeling suggests that the late-stage <span class="hlt">volcanism</span> does not overprint the remanant magnetization acquired by the Jurassic ocean crust in the Pigafetta Basin, and hence, marine magnetic anomalies recorded in the Jurassic basement are preserved. Also, the formerly identified Rough-Smooth Boundary (RSB) is indistinguishable from any other rough-smooth topographic boundaries throughout the survey area suggesting that the RSB is unlikely to be a Cretaceous sill-Jurassic basement boundary. Lastly, the apparent ages and spatial distribution of <span class="hlt">volcanic</span> features suggests a dynamic history of <span class="hlt">hydrothermal</span> circulation in the Pigafetta Basin, indicating that <span class="hlt">hydrothermal</span> circulation was ongoing well past 100 Ma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780006564&hterms=Nogal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DNogal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780006564&hterms=Nogal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DNogal"><span>LANDSAT detection of <span class="hlt">hydrothermal</span> alteration in the Nogal Canyon Cauldron, New Mexico</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vincent, R. K.; Rouse, G.</p> <p>1977-01-01</p> <p>In 1974 a circular-shaped iron oxide anomaly was observed in an image of a LANDSAT frame centered near Truth or Consequences, New Mexico. Field examination of the anomaly has shown that it coincides with a zone of <span class="hlt">hydrothermal</span> alteration on the northern edge of the Nogal Canyon Cauldron. The altered area contains clay minerals ranging in colors from white to vivid red, the latter presumably resulting from hematite staining. In situ gas measurements showed no evidence of <span class="hlt">active</span> hydrogen sulfide seepage. Preliminary geochemical analyses of grab samples have detected no significant amounts of mineralization. Whereas this area does not at present appear to be economically important, it provides an example of how LANDSAT can be utilized in reconnaissance mapping for cauldrons, calderas, and other <span class="hlt">volcanic</span> features which display <span class="hlt">hydrothermal</span> alteration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021743','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021743"><span>A geochemical reconnaissance of the Alid <span class="hlt">volcanic</span> center and geothermal system, Danakil depression, Eritrea</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lowenstern, J. B.; Janik, C.J.; Fournier, R.O.; Tesfai, T.; Duffield, W.A.; Clynne, M.A.; Smith, James G.; Woldegiorgis, L.; Weldemariam, K.; Kahsai, G.</p> <p>1999-01-01</p> <p>Geological and geochemical studies indicate that a high-temperature geothermal system underlies the Alid <span class="hlt">volcanic</span> center in the northern Danakil depression of Eritrea. Alid is a very late-Pleistocene structural dome formed by shallow intrusion of rhyolitic magma, some of which vented as lavas and pyroclastic flows. Fumaroles and boiling pools distributed widely over an area of ~10 km2 on the northern half of Alid suggest that an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system underlies much of that part of the mountain. Geothermometers indicate that the fumarolic gases are derived from a geothermal system with temperatures >225??C. The isotopic composition of condensed fumarolic steam is consistent with these temperatures and implies that the source water is derived primarily from either lowland meteoric waters or fossil Red Sea water, or both. Some gases vented from the system (CO2, H2S and He) are largely magmatic in origin. Permeability beneath the <span class="hlt">volcanic</span> center may be high, given the amount of intrusion-related deformation and the <span class="hlt">active</span> normal faulting within the Danakil depression.Geological and geochemical studies indicate that a high-temperature geothermal system underlies the Alid <span class="hlt">volcanic</span> center in the northern Danakil depression of Eritrea. Alid is a very late-Pleistocene structural dome formed by shallow intrusion of rhyolitic magma, some of which vented as lavas and pyroclastic flows. Fumaroles and boiling pools distributed widely over an area of approx. 10 km2 on the northern half of Alid suggest that an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system underlies much of that part of the mountain. Geothermometers indicate that the fumarolic gases are derived from a geothermal system with temperatures >225??C. The isotopic composition of condensed fumarolic steam is consistent with these temperatures and implies that the source water is derived primarily from either lowland meteoric waters or fossil Red Sea water, or both. Some gases vented from the system (CO2, H2S and He) are largely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910675D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910675D"><span>Multiteide Project: Multiparametric characterization of the <span class="hlt">activity</span> of Teide-Pico Viejo <span class="hlt">volcanic</span> system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Domínguez Cerdeña, Itahiza; Villasante-Marcos, Victor; Meletlidis, Stavros; Sainz-Maza, Sergio; Abella, Rafael; Torres, Pedro A.; Sánchez, Nieves; Luengo-Oroz, Natividad; José Blanco, María; García-Cañada, Laura; Pereda de Pablo, Jorge; Lamolda, Héctor; Moure, David; Del Fresno, Carmen; Finizola, Anthony; Felepto, Alicia</p> <p>2017-04-01</p> <p> addition, they will allow identifying the response of all the analyzed parameters to specific events that are traditionally studied with a single technique, such as short episodes of tremor (sporadically registered in Teide-Pico Viejo surroundings) or changes in <span class="hlt">activity</span> of the <span class="hlt">hydrothermal</span> system of the <span class="hlt">volcanic</span> complex. We present here the first multiparametric results obtained from the project, including locations with the seismic array, CO2 and temperature maps of Teide fumaroles zones and magnetometric measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29769655','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29769655"><span>Influences of Sedimentary Environments and <span class="hlt">Volcanic</span> Sources on Diagenetic Alteration of <span class="hlt">Volcanic</span> Tuffs in South China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gong, Nina; Hong, Hanlie; Huff, Warren D; Fang, Qian; Bae, Christopher J; Wang, Chaowen; Yin, Ke; Chen, Shuling</p> <p>2018-05-16</p> <p>Permian-Triassic (P-Tr) altered <span class="hlt">volcanic</span> ashes (tuffs) are widely distributed within the P-Tr boundary successions in South China. <span class="hlt">Volcanic</span> altered ashes from terrestrial section-Chahe (CH) and marine section-Shangsi (SS) are selected to further understand the influence of sedimentary environments and <span class="hlt">volcanic</span> sources on diagenetic alterarion on <span class="hlt">volcanic</span> tuffs. The zircon 206 Pb/ 238 U ages of the corresponding beds between two sections are almost synchronous. Sedimentary environment of the altered tuffs was characterized by a low pH and did not experience a <span class="hlt">hydrothermal</span> process. The dominant clay minerals of all the tuff beds are illite-smectite (I-S) minerals, with minor chlorite and kaolinite. I-S minerals of CH (R3) are more ordered than SS (R1), suggesting that CH also shows a higher diagenetic grade and more intensive chemical weathering. Besides, the nature of the <span class="hlt">volcanism</span> of the tuff beds studied is derived from different magma sources. The clay mineral compositions of tuffs have little relation with the types of source <span class="hlt">volcanism</span> and the depositional environments. Instead, the degree of the mixed-layer clay minerals and the REE distribution are mainly dependent upon the sedimentary environments. Thus, the mixed-layer clay minerals ratio and their geochemical index can be used as the paleoenvironmental indicator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014380','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014380"><span>Mineralization, alteration, and <span class="hlt">hydrothermal</span> metamorphism of the ophiolite-hosted Turner-Albright sulfide deposit, southwestern Oregon</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zierenberg, R.A.; Shanks, Wayne C.; Seyfried, W.E.; Koski, R.A.; Strickler, M.D.</p> <p>1988-01-01</p> <p>The Turner-Albright sulfide deposit, part of the Josephine ophiolite, formed on and below the seafloor during Late Jurassic <span class="hlt">volcanism</span> at a back arc spreading center. Ore fluids were probably localized by faults which were <span class="hlt">active</span> on the seafloor at the time of sulfide deposition. The uppermost massive sulfide formed on the seafloor at <span class="hlt">hydrothermal</span> vents. The bulk of the sulfide mineralization formed below the seafloor within olivine basalt hyaloclastite erupted near the time of mineralization. Infiltration of <span class="hlt">hydrothermal</span> fluid into the hyaloclastite altered the rock. The fluid responsible for the <span class="hlt">hydrothermal</span> alteration was evolved seawater with low pH and Mg and high Fe. The average value of sulfide and the difference between sulfide and contemporaneous seawater sulfate values are similar to ophiolite-hosted sulfide deposits in Cyprus. Mudstone and clinopyroxene basalt above the sulfide horizons were not altered by the ore-transporting <span class="hlt">hydrothermal</span> fluid, but these rocks were <span class="hlt">hydrothermally</span> metamorphosed by altered seawater heated by deep circulation into hot oceanic crust. This subseafloor metamorphism produced a mineral assemblage typical of prehnite-pumpellyite facies metamorphism. Exchange with altered seawater increased the whole-rock ??18O of the basalts to values of 9.4-11.2%. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFMOS43A0986W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFMOS43A0986W"><span><span class="hlt">Volcanic</span> Structure of the Gakkel Ridge at 85°E</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willis, C.; Humphris, S.; Soule, S. A.; Reves-Sohn, R.; Shank, T.; Singh, H.</p> <p>2007-12-01</p> <p>We present an initial volcanologic interpretation of a magmatically-robust segment of the ultra-slow spreading (3- 7 mm/yr) Gakkel Ridge at 85°E in the eastern Arctic Basin based on surveys conducted during the July 2007 Arctic GAkkel Vents Expedition (AGAVE). A previous expedition (2001 AMORE) and seismic stations in the area found evidence for <span class="hlt">active</span> <span class="hlt">hydrothermal</span> circulation and seismicity that suggested <span class="hlt">volcanic</span> <span class="hlt">activity</span> may be ongoing at 85°E. We examine multi-beam bathymetric data, digital imagery, and rock and sediment samples in order to determine the nature of <span class="hlt">volcanic</span> accretion that is occurring in this environment including the distribution of flow types and their relationship to features of the axial valley. Raw multi-beam bathymetric data was logged by the Kongsberg EM 120 1°x1° multi-beam echo sounder aboard the icbreaker IB Oden. Digital imagery was recorded on five video and still cameras mounted on the CAMPER fiber-optic wireline vehicle, which was towed 1-3m above the seafloor. Digital imagery was recorded on thirteen CAMPER drift-dives over interesting bathymetry including: a <span class="hlt">volcanic</span> ridge in the axial valley named Duque's Hill, and Oden and Loke volcanoes that are part of the newly discovered Asgard <span class="hlt">volcanic</span> chain. Talus, lava flows, and volcaniclastics were sampled with the clamshell grabber and slurp suction sampler on CAMPER. A variety of lava morphologies are identified in the imagery including large basalt pillows with buds and other surface ornamentation, lava tubes, lobates, sheet flows, and a thick cover of volcaniclastic sediment over extensive areas suggestive of explosive <span class="hlt">volcanic</span> <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JSAES..80..559A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JSAES..80..559A"><span>Emplacement dynamics and <span class="hlt">hydrothermal</span> alteration of the Atengo ignimbrite, southern Sierra Madre Occidental, northwestern Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Agarwal, Amar; Alva-Valdivia, L. M.; Rivas-Sánchez, M. L.; Herrero-Bervera, E.; Urrutia-Fucugauchi, J.; Espejel-García, V.</p> <p>2017-12-01</p> <p>The Sierra Madre Occidental is a thick continental arc related to the subduction of the Farallon plate beneath North America resulting in a very intense and widespread Cretaceous to Cenozoic magmatic and tectonic <span class="hlt">activity</span>. The 28 My old Atengo ignimbrite outcrops in the southern Sierra Madre Occidental, northwestern Mexico. From 12 sites that belong to various pyroclastic and lava flows emplaced during two pulses in the Oligocene (ca. 32-28 Ma) and Early Miocene (ca. 24-20 Ma), 97 rock specimens were drilled. The mineralogical and rock magnetic properties of the Atengo ignimbrite are compared with the surrounding <span class="hlt">volcanic</span> rocks to identify the eruption mechanism, and with the El Castillo Ignimbrite, Veracruz, Mexico, to understand the depositional conditions. The comparisons reveal that the Atengo ignimbrite erupted from a single source, but less violently than the El Castillo ignimbrite, and cooled rapidly, inhibiting the formation of subhedral grains. The source of the Atengo Ignimbrite was a Plinian-type eruption, and the characteristic mineralogical and textural properties of each flow are related to different stages of the Plinian-type eruption. Further more, <span class="hlt">hydrothermal</span> fluids were <span class="hlt">active</span> during the last stages of <span class="hlt">volcanism</span>, and caused moderate to intense alteration, especially in the ignimbrites, where high permeability aided the movement of <span class="hlt">hydrothermal</span> fluids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79...21S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79...21S"><span><span class="hlt">Volcanic</span> gas composition changes during the gradual decrease of the gigantic degassing <span class="hlt">activity</span> of Miyakejima volcano, Japan, 2000-2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shinohara, Hiroshi; Geshi, Nobuo; Matsushima, Nobuo; Saito, Genji; Kazahaya, Ryunosuke</p> <p>2017-02-01</p> <p>The composition of <span class="hlt">volcanic</span> gases discharged from Miyakejima volcano has been monitored during the intensive degassing <span class="hlt">activity</span> that began after the eruption in 2000. During the 15 years from 2000 to 2015, Miyakejima volcano discharged 25.5 Mt of SO2, which required degassing of 3 km3 of basaltic magma. The SO2 emission rate peaked at 50 kt/day at the end of 2000 and quickly decreased to 5 kt/day by 2003. During the early degassing period, the <span class="hlt">volcanic</span> gas composition was constant with the CO2/SO2 = 0.8 (mol ratio), H2O/SO2 = 35, HCl/SO2 = 0.08, and SO2/H2S = 15. The SO2 emission rate decreased gradually to 0.5 kt/day by 2012, and the gas composition also changed gradually to CO2/SO2 = 1.5, H2O/SO2 = 150, HCl/SO2 = 0.15, and SO2/H2S = 6. The compositional changes are not likely caused by changes in degassing pressure or volatile heterogeneity of a magma chamber but are likely attributed to an increase of <span class="hlt">hydrothermal</span> scrubbing caused by large decrease of the <span class="hlt">volcanic</span> gas emission rate, suggesting a supply of gases with constant composition during the 15 years. The intensive degassing was modeled based on degassing of a convecting magma conduit. The gradual SO2 emission rate that decrease without changes in <span class="hlt">volcanic</span> gas composition is attributed to a reduction of diameter of the convecting magma conduit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.V14B..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.V14B..04C"><span>Unusual <span class="hlt">Volcanic</span> Tremor Observations in Fogo Island, Cape Verde</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Custodio, S. I.; Heleno, S. I.</p> <p>2004-12-01</p> <p><span class="hlt">Volcanic</span> tremor is a ground motion characterized by well-defined frequencies, and has traditionally been explained by the movement of fluids, namely magma, in conduits or cracks (Chouet, 1996). Thus tremor has the potential to reveal key aspects of <span class="hlt">volcanic</span> structure and dynamics. Two types of previously unreported seismic signals have been observed in Fogo volcano: a) tide-modulated seismic noise and <span class="hlt">volcanic</span> tremor, and b) high-frequency low-attenuation harmonic tremor. Amplitude modulation of seismic noise can be detected by simple eye-inspection of raw data in some stations of the VIGIL Network, Fogo Volcano. A more detailed analysis shows that certain frequency bands which we interpret as <span class="hlt">volcanic</span> tremor, mainly in the range 2.0-3.0Hz, are preferentially modulated. The main frequency of modulation is 1.93 c.p.d., which corresponds to M2, the semi-diurnal lunar harmonic. Air pressure and temperature, which are continuously monitored in Fogo Island, have been analyzed and cannot explain the observed periodicity. Thus we conclude that seismic noise and tremor amplitudes are controlled by tides (Custodio et al., 2003). A relation between the tidal modulation and <span class="hlt">hydrothermal</span> systems <span class="hlt">activity</span> is suspected and under investigation. High-frequency (HF) tremor (5-20 Hz) has been recorded simultaneously in several stations in Fogo Island and even in different islands of the Cape Verde archipelago (up to distances of 120 km). In <span class="hlt">volcanic</span> environments high-frequency motions are normally recorded in a small area close to the source, due to the strong attenuation of seismic waves. <span class="hlt">Non-volcanic</span> origins for HF tremor were examined: cultural noise, whale vocalizations, ship noise, electronic/processing artifacts and path and/or site effects were all considered and dismissed. Emergent arrivals and strong site effects render source location a difficult task, but the analysis of wave polarizations and amplitude distributions seems to point to an offshore source. Two alternative</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V11A2491I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V11A2491I"><span>Evolution of Morphology and Crystallinity of Silica Minerals Under <span class="hlt">Hydrothermal</span> Conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Isobe, H.</p> <p>2011-12-01</p> <p>Silica minerals are quite common mineral species in surface environment of the terrestrial planets. They are good indicator of terrestrial processes including <span class="hlt">hydrothermal</span> alteration, diagenesis and soil formation. <span class="hlt">Hydrothermal</span> quartz, metastable low temperature cristobalite and amorphous silica show characteristic morphology and crystallinity depending on their formation processes and kinetics under wide range of temperature, pressure, acidity and thermal history. In this study, silica minerals produced by acidic <span class="hlt">hydrothermal</span> alteration related to <span class="hlt">volcanic</span> <span class="hlt">activities</span> and <span class="hlt">hydrothermal</span> crystallization experiments from diatom sediment are examined with crystallographic analysis and morphologic observations. Low temperature form of cistobalite is a metastable phase and a common alteration product occured in highly acidic <span class="hlt">hydrothermal</span> environment around fumaroles in geothermal / <span class="hlt">volcanic</span> areas. XRD analysis revealed that the alteration degree of whole rock is represented by abundance of cristobalite. Detailed powder XRD analysis show that the primary diffraction peak of cristobalite composed with two or three phases with different d-spacing and FWHM by peak profile fitting analysis. Shorter d-spacing and narrower FWHM cristobalite crystallize from precursor materials with less-crystallized, longer d-spacing and wider FWHM cristobalite. Textures of <span class="hlt">hydrothermal</span> cristobalite in altered rock shows remnant of porphylitic texture of the host rock, pyroxene-amphibole andesite. Diatom has amorphous silica shell and makes diatomite sediment. Diatomite found in less diagenetic Quarternary formation keeps amorphous silica diatom shells. <span class="hlt">Hydrothermal</span> alteration experiments of amorphous silica diatomite sediment are carried out from 300 °C to 550 °C. Mineral composition of run products shows crystallization of cristobalite and quartz progress depending on temperature and run durations. Initial crystallization product, cristobalite grains occur as characteristic lepispheres 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_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/2012AGUFMOS42A..07Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS42A..07Z"><span>Shallow water submarine <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> - A case study in the assessment of ocean acidification and fertilization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, J.; Yoshida, K.; Hagiwara, T.; Nagao, K.; Kusakabe, M.; Wang, B.; Chen, C. A.</p> <p>2012-12-01</p> <p>Most natural Shallow Water submarine <span class="hlt">Hydrothermal</span> <span class="hlt">activates</span> (SWH) along coastlines are related to <span class="hlt">hydrothermal</span> eruptions involving heating of groundwater with the <span class="hlt">volcanic</span> gas. These SWHs supply nutrients such as phosphorus and micro nutrients like iron to the euphotic zone, contributing to the overall natural fertility and primary productivity of coastal waters. However, SWHs also have a negative effect, dispersing toxic materials such as mercury and arsenic, and affecting the acidification of the surrounding waters. In this study, we evaluate the impact of "iron supply" and "ocean acidification" on the primary production in a coastal marine environment, at a SWH area discovered off Gueshandao Island, northeast Taiwan. In the past three years, expeditions were conducted and observations made around this SWH site. Divers, small boats and a research vessel (R/V OR1, Ocean University National Taiwan) were used to survey successively larger areas around the site. Some of the results obtained are as follows. <span class="hlt">Hydrothermal</span> vents are located in a hilly terrain rich with hot spring water with gas erupting intermittently. There are two types of vents, roughly divided by color, yellow hot spring water with higher temperature >110 degC ejected from sulfur chimneys of various sizes, and colorless water with lower temperature ~80 degC ejected directly from the crevices of the andesitic bedrock. Natural sulfur solidifying in the mouth of a small chimney was captured by a video camera, and explosions were also observed at intervals of a few minutes. Sediment, sand and particles of sulfur were deposited on the sides to a radius of about 50 m condensing around the chimney. The bottom type changes from sand/particles to outcrop/rock away from the vents. Moreover, gas samples were collected from the vents; the ratios of gas concentrations (N2/Ar) and isotopic composition of noble gas (3He/4He) suggest that these <span class="hlt">volcanic</span> gases are mantle-derived. <span class="hlt">Hydrothermal</span> fluid with high p</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S41B2729G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S41B2729G"><span>Ambient Noise Surface Wave Tomography of the <span class="hlt">volcanic</span> systems of eastern Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Green, R. G.; Priestley, K. F.; White, R. S.</p> <p>2015-12-01</p> <p>The Vatnajökull region of central-east Iceland lies above the head of the Iceland mantle plume where the crust is thickest due to enhanced melt supply. As a result the region contains a high density of <span class="hlt">volcanic</span> rift systems, with six large subglacial central volcanoes. Due to the ice cover, the geological structure of the area and the location of past eruptions are poorly known. Imaging of the crustal velocity heterogeneities beneath the ice sheet aims to reveal much in terms of the structure of these <span class="hlt">volcanic</span> plumbing systems. Mapping of significant velocity changes through time may also be indicative of movement of melt around the central volcanoes; one of which (Bárðarbunga) experienced a major rifting event in August 2014 (Sigmundsson et al. Nature 2015, Green et al. Nature Geosci. 2015). We present results from tomographic imaging of the <span class="hlt">volcanic</span> systems in the region, using continuous data from a local broadband seismic network in central-east Iceland which provides excellent ray path coverage of the <span class="hlt">volcanic</span> systems. This is supplemented by data from the HOTSPOT and ICEMELT experiments and the permanent monitoring stations of the Icelandic Meteorological Office. We process the continuous data following Benson et al. 2007 and automatic frequency-time analysis (FTAN) routines are used to extract more than 9000 dispersion measurements. We then generate Rayleigh wave group velocity maps which we present here. We find low velocity regions beneath the Vatnajökull icecap which are bounded by the surface expression of the <span class="hlt">volcanic</span> rift systems. The lower velocities also extend north-west to the <span class="hlt">volcanic</span> system under the Hofsjökull ice cap, and northwards towards Askja and the <span class="hlt">volcanic</span> systems of the northern <span class="hlt">volcanic</span> zone. We also produce locations and focal mechanisms of earthquakes caused by magmatic and <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> to correlate structure with the <span class="hlt">activity</span> of the <span class="hlt">volcanic</span> systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930049255&hterms=low+emissivity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dlow%2Bemissivity','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930049255&hterms=low+emissivity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dlow%2Bemissivity"><span>Recent <span class="hlt">volcanic</span> <span class="hlt">activity</span> on Venus - Evidence from radiothermal emissivity measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robinson, Cordula A.; Wood, John A.</p> <p>1993-01-01</p> <p>Radiothermal emissivity measurements are analyzed in order to study large <span class="hlt">volcanic</span> constructs on Venus and to correlate details of the reflectivity/emissivity patterns with geological landforms and stratigraphy visible in corresponding SAR images. There appears to be a correlation between locations on Venus where high emissivity at high altitudes and low emissivity at low altitudes are observed. These phenomena are attributed here to relatively recent <span class="hlt">volcanic</span> <span class="hlt">activity</span>: the former to summit eruptions that have not had time to weather to the low-emissivity state, the latter to continuing emission of <span class="hlt">volcanic</span> gases from neighboring small plains volcanoes. The pattern of reflectivity and emissivity on Maat Mons is examined in the light of these findings. It is concluded that Maat Mons has undergone the most recent episode of <span class="hlt">volcanic</span> <span class="hlt">activity</span> of all the volcanoes studied here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeCoA.215..247A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeCoA.215..247A"><span>The radiogenic and stable Sr isotope geochemistry of basalt weathering in Iceland: Role of <span class="hlt">hydrothermal</span> calcite and implications for long-term climate regulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andrews, M. Grace; Jacobson, Andrew D.</p> <p>2017-10-01</p> <p>Several studies have examined the geochemistry of Icelandic rivers to quantify the relationship between basalt weathering and long-term climate regulation. Recent research has suggested that the chemical weathering of <span class="hlt">hydrothermal</span> and metamorphic calcite contributes significant quantities of HCO3- to the Icelandic riverine flux (Jacobson et al., 2015). Because the HCO3- derives from <span class="hlt">volcanic</span> CO2 that was sequestered in mineral form prior to atmospheric injection, the strength of the basalt weathering feedback occurring in Iceland may be lower than previously realized. To test these hypotheses, we analyzed the radiogenic and stable Sr isotope composition (87Sr/86Sr and δ88/86Sr) of the same suite of water, rock, and mineral samples as examined in Jacobson et al. (2015), and we developed a simple model of the long-term C cycle that considers the transformation of <span class="hlt">volcanic</span> CO2 to HCO3- during subsurface silicate weathering, which is a precursor to <span class="hlt">hydrothermal</span> calcite formation. Interpretations based on 87Sr/86Sr and Ca/Sr ratios suggest that conservative, three-component mixing between basalt, calcite, and atmospheric deposition adequately explains river geochemistry. On average, the δ88/86Sr values of glacial and <span class="hlt">non</span>-glacial rivers (0.414‰ and 0.388‰, respectively) are generally higher than those for basalt (0.276‰); however, calcite δ88/86Sr values (0.347‰) are also higher than those for basalt and span the range of riverine values. Thus, riverine δ88/86Sr values are also consistent three-component mixing between basalt, calcite, and atmospheric deposition. Isotopic fractionation is not required to explain riverine trends. Finally, model equations for the long-term C cycle demonstrate that subsurface silicate weathering reduces the magnitude of the <span class="hlt">volcanic</span> CO2 degassing flux, which in turn causes the atmosphere to stabilize at lower pCO2 values compared to the case where no subsurface silicate weathering occurs. However, the proportion of the net</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP52B..08M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP52B..08M"><span>Topographic stress and catastrophic collapse of <span class="hlt">volcanic</span> islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moon, S.; Perron, J. T.; Martel, S. J.</p> <p>2017-12-01</p> <p>Flank collapse of <span class="hlt">volcanic</span> islands can devastate coastal environments and potentially induce tsunamis. Previous studies have suggested that factors such as <span class="hlt">volcanic</span> eruption events, gravitational spreading, the reduction of material strength due to <span class="hlt">hydrothermal</span> alteration, steep coastal cliffs, or sea level change may contribute to slope instability and induce catastrophic collapse of <span class="hlt">volcanic</span> flanks. In this study, we examine the potential influence of three-dimensional topographic stress perturbations on flank collapses of <span class="hlt">volcanic</span> islands. Using a three-dimensional boundary element model, we calculate subsurface stress fields for the Canary and Hawaiian islands to compare the effects of stratovolcano and shield volcano shapes on topographic stresses. Our model accounts for gravitational stresses from the actual shapes of <span class="hlt">volcanic</span> islands, ambient stress in the underlying plate, and the influence of pore water pressure. We quantify the potential for slope failure of <span class="hlt">volcanic</span> flanks using a combined model of three-dimensional topographic stress and slope stability. The results of our analysis show that subsurface stress fields vary substantially depending on the shapes of volcanoes, and can influence the size and spatial distribution of flank failures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995JVGR...66..149F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995JVGR...66..149F"><span><span class="hlt">Volcanic</span> ash in ancient Maya ceramics of the limestone lowlands: implications for prehistoric <span class="hlt">volcanic</span> <span class="hlt">activity</span> in the Guatemala highlands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ford, Anabel; Rose, William I.</p> <p>1995-07-01</p> <p>In the spirit of collaborative research, Glicken and Ford embarked on the problem of identifying the source of <span class="hlt">volcanic</span> ash used as temper in prehistoric Maya ceramics. Verification of the presence of glass shards and associated <span class="hlt">volcanic</span> mineralogy in thin sections of Maya ceramics was straightforward and pointed to the Guatemala Highland <span class="hlt">volcanic</span> chain. Considering seasonal wind rose patterns, target volcanoes include those from the area west of and including Guatemala City. Joint field research conducted in 1983 by Glicken and Ford in the limestone lowlands of Belize and neighboring Guatemala, 300 km north of the <span class="hlt">volcanic</span> zone and 150 km from the nearest identified ash deposits, was unsuccessful in discovering local <span class="hlt">volcanic</span> ash deposits. The abundance of the ash in common Maya ceramic vessels coupled with the difficulties of long-distance procurement without draft animals lead Glicken to suggest that ashfall into the lowlands would most parsimoniously explain prehistoric procurement; it literally dropped into their hands. A major archaeological problem with this explanation is that the use of <span class="hlt">volcanic</span> ash occurring over several centuries of the Late Classic Period (ca. 600-900 AD). To accept the ashfall hypothesis for ancient Maya <span class="hlt">volcanic</span> ash procurement, one would have to demonstrate a long span of consistent <span class="hlt">volcanic</span> <span class="hlt">activity</span> in the Guatemala Highlands for the last half of the first millennium AD. Should this be documented through careful petrographic, microprobe and tephrachronological studies, a number of related archaeological phenomena would be explained. In addition, the proposed model of <span class="hlt">volcanic</span> <span class="hlt">activity</span> has implications for understanding <span class="hlt">volcanism</span> and potential <span class="hlt">volcanic</span> hazards in Central America over a significantly longer time span than the historic period. These avenues are explored and a call for further collaborative research of this interdisciplinary problem is extended in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V23E0514Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V23E0514Y"><span><span class="hlt">Volcanic</span> Gases and Hot Spring Water to Evaluate the <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> of the Mt. Baekdusan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yun, S. H.; Lee, S.; Chang, C.</p> <p>2017-12-01</p> <p>This study performed the analysis on the <span class="hlt">volcanic</span> gases and hot spring waters from the Julong hot spring at Mt. Baekdu, also known as Changbaishan on the North Korea(DPRK)-China border, during the period from July 2015 to August 2016. Also, we confirmed the errors that HCO3- concentrations of hot spring waters in the previous study (Lee et al. 2014) and tried to improve the problem. Dissolved CO2 in hot spring waters was analyzed using gas chromatograph in Lee et al.(2014). Improving this, from 2015, we used TOC-IC to analysis dissolved CO2. Also, we analyzed the Na2CO3 standard solutions of different concentrations using GC, and confirmed the correlation between the analytical concentrations and the real concentrations. However, because the analytical results of the Julong hot spring water were in discord with the estimated values based on this correlation, we can't estimate the HCO3-concentrations of 2014 samples. During the period of study, CO2/CH4 ratios in <span class="hlt">volcanic</span> gases are gradually decreased, and this can be interpreted in two different ways. The first interpretation is that the conditions inside the <span class="hlt">volcanic</span> edifice are changing into more reduction condition, and carbon in <span class="hlt">volcanic</span> gases become more favorable to distribute into CH4 or CO than CO2. The second interpretation is that the interaction between <span class="hlt">volcanic</span> gases and water becomes greater than past, and the concentrations of CO2which have much higher solubility in water decreased, relatively. In general, the effect of scrubbing of <span class="hlt">volcanic</span> gas is strengthened during the quiet periods of <span class="hlt">volcanic</span> <span class="hlt">activity</span> rather than <span class="hlt">active</span> periods. Meanwhile, the analysis of hot spring waters was done on the anion of acidic gases species, the major cations, and some trace elements (As, Cd, Re).This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMIPA 2015-3060.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890011975','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890011975"><span>Catastrophic <span class="hlt">volcanism</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lipman, Peter W.</p> <p>1988-01-01</p> <p>Since primitive times, catastrophes due to <span class="hlt">volcanic</span> <span class="hlt">activity</span> have been vivid in the mind of man, who knew that his <span class="hlt">activities</span> in many parts of the world were threatened by lava flows, mudflows, and ash falls. Within the present century, increasingly complex interactions between <span class="hlt">volcanism</span> and the environment, on scales not previously experienced historically, have been detected or suspected from geologic observations. These include enormous hot pyroclastic flows associated with collapse at source calderas and fed by eruption columns that reached the stratosphere, relations between huge flood basalt eruptions at hotspots and the rifting of continents, devastating laterally-directed <span class="hlt">volcanic</span> blasts and pyroclastic surges, great <span class="hlt">volcanic</span>-generated tsunamis, climate modification from <span class="hlt">volcanic</span> release of ash and sulfur aerosols into the upper atmosphere, modification of ocean circulation by <span class="hlt">volcanic</span> constructs and attendent climatic implications, global pulsations in intensity of <span class="hlt">volcanic</span> <span class="hlt">activity</span>, and perhaps triggering of some intense terrestrial <span class="hlt">volcanism</span> by planetary impacts. Complex feedback between <span class="hlt">volcanic</span> <span class="hlt">activity</span> and additional seemingly unrelated terrestrial processes likely remains unrecognized. Only recently has it become possible to begin to evaluate the degree to which such large-scale <span class="hlt">volcanic</span> processes may have been important in triggering or modulating the tempo of faunal extinctions and other evolutionary events. In this overview, such processes are examined from the viewpoint of a field volcanologist, rather than as a previous participant in controversies concerning the interrelations between extinctions, impacts, and <span class="hlt">volcanism</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.P43C2022V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.P43C2022V"><span>Modeling Seasonal Thermal Radiance Cycles for Change Detection at <span class="hlt">Volcanic</span> / Geothermal Areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vaughan, R.; Beuttel, B. S.</p> <p>2013-12-01</p> <p>Remote sensing observations of thermal features associated with (and often preceding) <span class="hlt">volcanic</span> <span class="hlt">activity</span> have been used for decades to detect and monitor <span class="hlt">volcanism</span>. However, anomalous thermal precursors to <span class="hlt">volcanic</span> eruptions are usually only recognized retrospectively. One of the reasons for this is that precursor thermal <span class="hlt">activity</span> is often too subtle in magnitude (spatially, temporally, or in absolute temperature) to be unambiguously detected in time to issue warnings or forecasts. Part of the reason for this is the trade-off between high spatial and high temporal resolution associated with satellite imaging systems. Thus, the goal of this work has been to develop some techniques for using high-temporal-resolution, coarse-spatial-resolution imagery to try to detect subtle thermal anomalies. To identify anomalies, background thermal <span class="hlt">activity</span> must first be characterized. Every <span class="hlt">active</span>, or potentially <span class="hlt">active</span>, volcano has a unique thermal history that provides information about normal background thermal <span class="hlt">activity</span> due to seasonal or diurnal variations. Understanding these normal variations allows recognition of anomalous <span class="hlt">activity</span> that may be due to <span class="hlt">volcanic</span> / <span class="hlt">hydrothermal</span> processes - ultimately with a lead time that may be sufficient to issue eruption warnings or forecasts. Archived MODIS data, acquired ~daily from 2000 to 2012, were used to investigate seasonal thermal cycles at three <span class="hlt">volcanic</span> areas with different types of thermal features: Mount St. Helens, which had a dacite dome-building eruption from 2004-2008; Mount Ruapehu, which has a 500-m diameter <span class="hlt">active</span> summit crater lake; and Yellowstone, which is a large <span class="hlt">active</span> geothermal system that has hundreds of hot springs and fumarole fields spread out over a very large area. The focus has been on using MODIS 1-km sensor radiance data in the MIR and TIR wavelength regions that are sensitive to thermal emission from features that range in temperature from hundreds of °C, down to tens of °C (below the boiling temperature</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V11G..07F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V11G..07F"><span>The bulk isotopic composition of hydrocarbons in subaerial <span class="hlt">volcanic-hydrothermal</span> emissions from different tectonic settings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fiebig, J.; Tassi, F.; Vaselli, O.; Viveiros, M. F.; Silva, C.; Lopez, T. M.; D'Alessandro, W.; Stefansson, A.</p> <p>2015-12-01</p> <p>Assuming that methane and its higher chain homologues derive from a common source, carbon isotope patterns have been applied as a criterion to identify occurrences of abiogenic hydrocarbons. Based on these, it has been postulated that abiogenic hydrocarbon production occurs within several (ultra)mafic environments. More evolved <span class="hlt">volcanic-hydrothermal</span> systems may also provide all the prerequisites necessary for abiogenic hydrocarbon production, such as availability of inorganic CO2, hydrogen and heat. We have investigated the chemical and isotopic composition of n-alkanes contained within subaerial <span class="hlt">hydrothermal</span> discharges emitted from a range of hot spot, subduction and rift-related volcanoes to determine the origin of hydrocarbons in these systems. Amongst these are Nisyros (Greece), Vesuvio, Campi Flegrei, Ischia, Pantelleria and Vulcano (all Italy), Mt. Mageik and Trident (USA), Copahue (Argentina), Teide (Spain), Furnas and Fogo (Portugal). The carbon isotopic composition of methane emitted from these sites varies from -65 to -8‰ , whereas δ13C of ethane and propane exhibit a much narrower variation from -17‰ to -31‰. Methane that occurs most enriched in 13C is also characterized by relatively positive δD values ranging up to -80‰. Carbon isotope reversals between methane and ethane are only observed for locations exhibiting δ13C-CH4 values > -20‰, such as Teide, Pantelleria, Trident and Furnas. At Furnas, δ13C-CH4 varies by 50‰ within a relatively short distance of <50m between two vents, whereas δ13C-C2H6 varies by less than 2‰ only. For some of the investigated locations apparent carbon isotopic temperatures between methane and CO2 are in agreement with those derived from gas concentration geothermometers. At these locations methane, however seems to be in disequilibrium with ethane and propane. These findings imply that methane on the one hand and the C2+ hydrocarbons on the other hand often might derive from distinct sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025896','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025896"><span>Geology of the Ivanhoe Hg-Au district, northern Nevada: Influence of Miocene <span class="hlt">volcanism</span>, lakes, and <span class="hlt">active</span> faulting on epithermal mineralization</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wallace, A.R.</p> <p>2003-01-01</p> <p>The mercury-gold deposits of the Ivanhoe mining district in northern Nevada formed when middle Miocene rhyolitic <span class="hlt">volcanism</span> and high-angle faulting disrupted a shallow lacustrine environment. Sinter and replacement mercury deposits formed at and near the paleosurface, and disseminated gold deposits and high-grade gold-silver veins formed beneath the hot spring deposits. The lacustrine environment provided abundant meteoric water; the rhyolites heated the water; and the faults, flow units, and lakebeds provided fluid pathways for the <span class="hlt">hydrothermal</span> fluids. A shallow lake began to develop in the Ivanhoe area about 16.5 Ma. The lake progressively expanded and covered the entire area with fine-grained lacustrine sediments. Lacustrine sedimentation continued to at least 14.4 Ma, and periodic fluctuations in the size and extent of the lake may have been responses to both climate and nearby <span class="hlt">volcanism</span>. The eruption of rhyolite and andesite flows and domes periodically disrupted the lacustrine environment and produced interfingered flows and lake sediments. The major pulse of rhyolitic <span class="hlt">volcanism</span> took place between 15.16 ± 0.05 and 14.92 ± 0.05 Ma. High-angle faulting began in the basement about 15.2 Ma, penetrated to and disrupted the paleosurface after 15.10 ± 0.06 Ma, and largely ceased by 14.92 ± 0.05 Ma. Ground motion related to both faulting and <span class="hlt">volcanism</span> created debris flows and soft-sediment deformation in the lakebeds. Mercury-gold mineralization was coeval with rhyolite <span class="hlt">volcanism</span> and high-angle faulting, and it took place about 15.2 to 14.9 Ma. At and near the paleosurface, <span class="hlt">hydrothermal</span> fluids migrated through tuffaceous sediments above relatively impermeable <span class="hlt">volcanic</span> and Paleozoic units, creating chalcedonic, cinnabar-bearing replacement bodies and sinters. Disseminated gold was deposited in sedimentary and <span class="hlt">volcanic</span> rocks beneath the mercury deposits, although the hydrologic path between the two ore types is unclear. Higher-grade gold-silver deposits formed in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028809','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028809"><span>Sensor web enables rapid response to <span class="hlt">volcanic</span> <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Davies, Ashley G.; Chien, Steve; Wright, Robert; Miklius, Asta; Kyle, Philip R.; Welsh, Matt; Johnson, Jeffrey B.; Tran, Daniel; Schaffer, Steven R.; Sherwood, Robert</p> <p>2006-01-01</p> <p>Rapid response to the onset of <span class="hlt">volcanic</span> <span class="hlt">activity</span> allows for the early assessment of hazard and risk [Tilling, 1989]. Data from remote volcanoes and volcanoes in countries with poor communication infrastructure can only be obtained via remote sensing [Harris et al., 2000]. By linking notifications of <span class="hlt">activity</span> from ground-based and spacebased systems, these volcanoes can be monitored when they erupt.Over the last 18 months, NASA's Jet Propulsion Laboratory (JPL) has implemented a Volcano Sensor Web (VSW) in which data from ground-based and space-based sensors that detect current <span class="hlt">volcanic</span> <span class="hlt">activity</span> are used to automatically trigger the NASA Earth Observing 1 (EO-1) spacecraft to make highspatial-resolution observations of these volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.9436I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.9436I"><span>The Geothermal Systems along the Watukosek fault system (East Java, Indonesia):The Arjuno-Welirang <span class="hlt">Volcanic</span> Complex and the Lusi Mud-Eruption</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inguaggiato, Salvatore; Mazzini, Adriano; Vita, Fabio; Sciarra, Alessandra</p> <p>2016-04-01</p> <p>The Java Island is characterized by an intense <span class="hlt">volcanic</span> <span class="hlt">activity</span> with more then 100 <span class="hlt">active</span> volcanoes. Moreover, this island is also known by the presence of many mud volcanoes and <span class="hlt">hydrothermal</span> springs. In particular, in the 2006 several sudden hot mud eruptions, with fluids around 100° C, occurred in the NE side of the island resulting in a prominent eruption named Lusi (contraction of Lumpur Sidoarjo) located along the major Watukosek strike-slip fault zone. The Watukosek fault system, strikes from the Arjuno-Welirang <span class="hlt">volcanic</span> complex, intersects Lusi and extends towards the NE of the Java island. Conversely of the normal mud eruptions (cold fluids emitted in a short time period of few days), the Lusi eruption was characterized by a persistent effusive hot fluids emissions for a long-time period of, so far, nearly a decade. Moreover, the isotopic composition of emitted gases like Helium showed a clear magmatic origin. For this reasons we decided to investigate the near Arjuno-Welirang complex located on the same strike-slip fault. Arjuno-Welirang is a twin strato-volcano system located in the East of Java along the Watukosek fault, at about 25 km SW respect to the Lusi volcano system. It features two main peaks: Arjuno (3339 masl) and Welirang (3156 masl). The last recorded eruptive <span class="hlt">activity</span> took place in August 1950 from the flanks of Kawah Plupuh and in October 1950 from the NW part of the Gunung Welirang. This strato-volcano is characterized by a S-rich area, with high T-vent fumarole at least up to 220° C (and likely higher), located mainly in the Welirang crater. In addition, several hot springs vent from the flanks of the volcano, indicate the presence of a large <span class="hlt">hydrothermal</span> system. During July 2015, in the framework of the Lusi Lab project (ERC grant n° 308126), we carried out a geochemical field campaign on the Arjuno-Welirang volcano <span class="hlt">hydrothermal</span> system area, sampling water and dissolved gases from the thermal and cold springs located on the flanks of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70042390','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70042390"><span>Rapid response of a hydrologic system to <span class="hlt">volcanic</span> <span class="hlt">activity</span>: Masaya volcano, Nicaragua</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pearson, S.C.P.; Connor, C.B.; Sanford, W.E.</p> <p>2008-01-01</p> <p>Hydrologic systems change in response to <span class="hlt">volcanic</span> <span class="hlt">activity</span>, and in turn may be sensitive indicators of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Here we investigate the coupled nature of magmatic and hydrologic systems using continuous multichannel time series of soil temperature collected on the flanks of Masaya volcano, Nicaragua, one of the most <span class="hlt">active</span> volcanoes in Central America. The soil temperatures were measured in a low-temperature fumarole field located 3.5 km down the flanks of the volcano. Analysis of these time series reveals that they respond extremely rapidly, on a time scale of minutes, to changes in <span class="hlt">volcanic</span> <span class="hlt">activity</span> also manifested at the summit vent. These rapid temperature changes are caused by increased flow of water vapor through flank fumaroles during <span class="hlt">volcanism</span>. The soil temperature response, ~5 °C, is repetitive and complex, with as many as 13 pulses during a single <span class="hlt">volcanic</span> episode. Analysis of the frequency spectrum of these temperature time series shows that these anomalies are characterized by broad frequency content during <span class="hlt">volcanic</span> <span class="hlt">activity</span>. They are thus easily distinguished from seasonal trends, diurnal variations, or individual rainfall events, which triggered rapid transient increases in temperature during 5% of events. We suggest that the mechanism responsible for the distinctive temperature signals is rapid change in pore pressure in response to magmatism, a response that can be enhanced by meteoric water infiltration. Monitoring of distal fumaroles can therefore provide insight into coupled <span class="hlt">volcanic</span>-hydrologic-meteorologic systems, and has potential as an inexpensive monitoring tool.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918866N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918866N"><span>Period and amplitude of <span class="hlt">non-volcanic</span> tremors and repeaters: a dimensional analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nielsen, Stefan</p> <p>2017-04-01</p> <p>Since its relatively recent discovery, the origin of <span class="hlt">non-volcanic</span> tremor has been source of great curiosity and debate. Two main interpretations have been proposed, one based on fluid migration, the other relating to slow slip events on a plate boundary (the latter hypothesis has recently gained considerable ground). Here I define the conditions of slip of one or more small asperities embedded within a larger creeping fault patch. The radiation-damping equation coupled with rate-and-state friction evolution equations results in a system of ordinary differential equations. For a finite size asperity, the system equates to a peculiar <span class="hlt">non</span>-linear damped oscillator, converging to a limit cycle. Dimensional analysis shows that period and amplitude of the oscillations depend on dimensional parameter combinations formed from a limited set of parameters: asperity dimension Γ, rate and state friction parameters (a, b, L), shear stiffness of the medium G, mass density ρ, background creep rate ˙V and normal stress σ. Under realistic parameter ranges, the asperity may show (1) tremor-like short period oscillations, accelerating to radiate sufficient energy to be barely detectable and a periodicity of the order of one to ten Hertz, as observed for <span class="hlt">non-volcanic</span> tremor <span class="hlt">activity</span> at the base of large inter-plate faults; (2) isolated stick-slip events with intervals in the order of days to months, as observed in repeater events of modest magnitude within creeping fault sections.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ysc..conf....5V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ysc..conf....5V"><span>Modern <span class="hlt">volcanic</span> <span class="hlt">activity</span> on the Moon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vidmachenko, A. P.</p> <p>2018-05-01</p> <p><span class="hlt">Volcanic</span> <span class="hlt">activity</span> on the Moon began when its surface cooled, and the nucleus and mantle were clearly separated inside. Fragments of <span class="hlt">volcanic</span> eruptions were discovered in the lunar soil, which was delivered to the Earth by "Apollo" spacecrafts. As shown by the analysis of some lunar meteorites, the first eruptions occurred 4.35 billion years ago. This is evidenced by the unique composition of the oxygen atoms for the Moon and on the radiocarbon analysis data. Well-visible on its surface, the dark "seas", which emerged shortly after the formation of the Moon, when the lowlands and large old craters were filled by liquid basaltic magma, rich in iron. The lunar "seas" are mostly on the visible side of the Moon, and cover almost a third of it; on the reverse side-the seas occupy less than 2%. Smooth surfaces of the seas mean that the lunar lava was very liquid. Therefore, at low gravity, it easily spread over a large area, almost without creating large cone-shaped peaks, but forming many small cone <span class="hlt">volcanic</span> systems with an age of 3-4 billion years ago. On the images of the visible side of the Moon obtained with the help of the LRO, evidence is provided that <span class="hlt">volcanic</span> eruptions on its surface were possible even a few million years ago.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V31F..02F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V31F..02F"><span>Identifying Water on Mt. Baker and Mt. St. Helens, WA with Geophysics: Implications for <span class="hlt">Volcanic</span> Landslide Hazards</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finn, C.; Bedrosian, P.; Wisniewski, M.; Deszcz-Pan, M.</p> <p>2015-12-01</p> <p>Groundwater position, abundance, and flow rates within a volcano affect the transmission of fluid pressure, transport of mass and heat and formation of mechanically weak <span class="hlt">hydrothermal</span> alteration influencing the stability of volcanoes. In addition, eruptions can shatter <span class="hlt">volcanic</span> rocks, weakening the edifice. Helicopter magnetic and electromagnetic (HEM) data collected over Mt. Baker and Mt. St. Helens volcanoes reveal the distribution of water, shattered <span class="hlt">volcanic</span> rocks and <span class="hlt">hydrothermal</span> alteration essential to evaluating <span class="hlt">volcanic</span> landslide hazards. These data, combined with geological mapping and rock property measurements, indicate the presence of localized <100 m thick zones of water-saturated <span class="hlt">hydrothermally</span> altered rock beneath Sherman Crater and the Dorr Fumarole Fields at Mt. Baker. Nuclear magnetic resonance data indicate that the <span class="hlt">hydrothermal</span> clays contain ~50% bound water with no evidence for free water ponded beneath the ice. The HEM data suggest water-saturated fresh <span class="hlt">volcanic</span> rocks from the surface to the detection limit (~100 m) over the entire summit of Mt. Baker (below the ice). A 50-100 m thick high resistivity layer (>1500 ohm-m) corresponding to domes, debris avalanche, <span class="hlt">volcanic</span> rocks and glaciers mantles the crater at Mt. St. Helens. Shallow low resistivity layers corresponding to fresh, cold water and hot brines are observed below the high resistivity surface in EM data. Shallow ground water mainly concentrates in shattered dome material in the crater of Mt. St. Helens. Aeromagnetic data indicate the location of basalts sandwiched between debris avalanche deposits and shattered dome material. The combination of the EM and magnetic data help map the location of the shattered dome material that is considered to be the failure surface for the 1980 debris avalanche. The EM data image the regional groundwater table near the base of the volcano. The geophysical identification of groundwater and weak layers constrain landslide hazards assessments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7525J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7525J"><span>A seismic network to investigate the sedimentary hosted <span class="hlt">hydrothermal</span> Lusi system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Javad Fallahi, Mohammad; Mazzini, Adriano; Lupi, Matteo; Obermann, Anne; Karyono, Karyono</p> <p>2016-04-01</p> <p>The 29th of May 2006 marked the beginning of the sedimentary hosted <span class="hlt">hydrothermal</span> Lusi system. During the last 10 years we witnessed numerous alterations of the Lusi system behavior that coincide with the frequent seismic and <span class="hlt">volcanic</span> <span class="hlt">activity</span> occurring in the region. In order to monitor the effect that the seismicity and the <span class="hlt">activity</span> of the <span class="hlt">volcanic</span> arc have on Lusi, we deployed a ad hoc seismic network. This temporary network consist of 10 broadband and 21 short period stations and is currently operating around the Arjuno-Welirang <span class="hlt">volcanic</span> complex, along the Watukosek fault system and around Lusi, in the East Java basin since January 2015. We exploit this dataset to investigate surface wave and shear wave velocity structure of the upper-crust beneath the Arjuno-Welirang-Lusi complex in the framework of the Lusi Lab project (ERC grant n° 308126). Rayleigh and Love waves travelling between each station-pair are extracted by cross-correlating long time series of ambient noise data recorded at the stations. Group and phase velocity dispersion curves are obtained by time-frequency analysis of cross-correlation functions, and are tomographically inverted to provide 2D velocity maps corresponding to different sampling depths. 3D shear wave velocity structure is then acquired by inverting the group velocity maps.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMNH13C..08A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMNH13C..08A"><span>Towards Developing Systematics for Using Periodic Studies of the <span class="hlt">Hydrothermal</span> Manifestations as Effective Tool for Monitoring Largely 'inaccessible' Volcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alam, M.</p> <p>2010-12-01</p> <p>The San José and Tupungatito volcanoes, located near Santiago (Chile), are the potential hazards, given their geological and historical record of explosive eruptions with pyroclastic flows, most recently in 1960 and 1987 respectively (Global <span class="hlt">Volcanism</span> Program, Smithsonian Institution). What aggravates the potential risk of these very high (>5290m elevation) snow- and ice-covered volcanoes is their location at the source of relatively narrow mountain drainage systems that feed into the Maipo River, flowing through the southern outskirts of Santiago. Sector-collapse and debris-flow, as a result of volcano-ice/snow interaction, can form lahars causing immense destruction to the life and property in the Maipo Valley (Cajón del Maipo). These lahars can cause submergence and burial of vast downstream areas under several meters thick sediment, as in the case of 1980 eruption of Mount St. Helens, USA. In the event of a major eruption, Santiago city will be at peril, with all the drinking water supply installations either destroyed or contaminated to the extent of being abandoned. Besides, ash and tephra will halt the air traffic in the region, particularly in Santiago-Mendoza sector between Chile and Argentina. In a proposed research project (for which funding is awaited from CONICYT, Chile under its Initiation into Research Funding Competition), <span class="hlt">hydrothermal</span> systems associated with the aforementioned volcanoes will be periodically studied to monitor these volcanoes, in order to develop a Systematics for using the peripheral <span class="hlt">hydrothermal</span> manifestations, together with nearby surface water bodies, as means for monitoring the <span class="hlt">activities</span> of the volcano(es). Basic premise of this proposal is to use the relationship between <span class="hlt">volcanic</span> and <span class="hlt">hydrothermal</span> <span class="hlt">activities</span>. Although this association has been observed at many <span class="hlt">volcanic</span> centers, no attempt has been made to use this relation effectively as a tool for monitoring the volcanoes. Before an eruption or even with increased</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V43B2881J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V43B2881J"><span>A Proposed Community Network For Monitoring <span class="hlt">Volcanic</span> Emissions In Saint Lucia, Lesser Antilles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Joseph, E. P.; Beckles, D. M.; Robertson, R. E.; Latchman, J. L.; Edwards, S.</p> <p>2013-12-01</p> <p>Systematic geochemical monitoring of <span class="hlt">volcanic</span> systems in the English-speaking islands of the Lesser Antilles was initiated by the UWI Seismic Research Centre (SRC) in 2000, as part of its <span class="hlt">volcanic</span> surveillance programme for the English-speaking islands of the Lesser Antilles. This programme provided the first time-series observations used for the purpose of volcano monitoring in Dominica and Saint Lucia, permitted the characterization of the geothermal fluids associated with them, and established baseline studies for understanding of the <span class="hlt">hydrothermal</span> systems during periods of quiescence (Joseph et al., 2011; Joseph et al., 2013). As part of efforts to improve and expand the capacity of SRC to provide <span class="hlt">volcanic</span> surveillance through its geothermal monitoring programme, it is necessary to develop economically sustainable options for the monitoring of <span class="hlt">volcanic</span> emissions/pollutants. Towards this effort we intend to work in collaboration with local authorities in Saint Lucia, to develop a monitoring network for quantifying the background exposure levels of ambient concentrations of <span class="hlt">volcanic</span> pollutants, SO2 in air and As in waters (as health significant marker elements in the geothermal emissions) that would serve as a model for the emissions monitoring network for other <span class="hlt">volcanic</span> islands. This programme would facilitate the building of local capacity and training to monitor the hazardous exposure, through the application and transfer of a regionally available low-cost and low-technology SO2 measurement/detection system in Saint Lucia. Existing monitoring technologies to inform evidence based health practices are too costly for small island Caribbean states, and no government policies or health services measures currently exist to address/mitigate these influences. Gases, aerosols and toxic elements from eruptive and <span class="hlt">non</span>-eruptive <span class="hlt">volcanic</span> <span class="hlt">activity</span> are known to adversely affect human health and the environment (Baxter, 2000; Zhang et al., 2008). Investigations into the</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/2015AGUFM.V23A3085W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V23A3085W"><span>Frequency Based <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Detection through 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>Worden, A. K.; Dehn, J.; Webley, P. W.</p> <p>2015-12-01</p> <p>Satellite remote sensing has proved to offer a useful and relatively inexpensive method for monitoring large areas where field work is logistically unrealistic, and potentially dangerous. Current sensors are able to detect the majority of explosive <span class="hlt">volcanic</span> <span class="hlt">activity</span>; those that tend to effect and represent larger scale changes in the <span class="hlt">volcanic</span> systems, eventually relating to ash producing periods of extended eruptive <span class="hlt">activity</span>, and effusive <span class="hlt">activity</span>. As new spaceborne sensors are developed, the ability to detect <span class="hlt">activity</span> improves so that a system to gauge the frequency of <span class="hlt">volcanic</span> <span class="hlt">activity</span> can be used as a useful monitoring tool. Four volcanoes were chosen for development and testing of a method to monitor explosive <span class="hlt">activity</span>: Stromboli (Italy); Shishaldin and Cleveland (Alaska, USA); and Karymsky (Kamchatka, Russia). Each volcano studied had similar but unique signatures of pre-cursory and eruptive <span class="hlt">activity</span>. This study has shown that this monitoring tool could be applied to a wide range of volcanoes and still produce useful and robust data. Our method deals specifically with the detection of small scale explosive <span class="hlt">activity</span>. The method described here could be useful in an operational setting, especially at remote volcanoes that have the potential to impact populations, infrastructure, and the aviation community. A number of important factors will affect the validity of application of this method. They are: (1) the availability of a continuous and continually populated dataset; (2) appropriate and reasonable sensor resolutions; (3) a recorded history of the volcano's previous <span class="hlt">activity</span>; and, if available, (4) some ground-based monitoring system. We aim to develop the method further to be able to capture and evaluate the frequency of other <span class="hlt">volcanic</span> processes such as lava flows, phreatomagmatic eruptions and dome growth and collapse. The work shown here has served to illustrate the capability of this method and monitoring tool for use at remote, un-instrumented volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JVGR..286..233C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JVGR..286..233C"><span><span class="hlt">Volcanic</span> ash leachate compositions and assessment of health and agricultural hazards from 2012 <span class="hlt">hydrothermal</span> eruptions, Tongariro, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cronin, S. J.; Stewart, C.; Zernack, A. V.; Brenna, M.; Procter, J. N.; Pardo, N.; Christenson, B.; Wilson, T.; Stewart, R. B.; Irwin, M.</p> <p>2014-10-01</p> <p>After almost 80 years of quiescence, the upper Te Maari vent on Mt. Tongariro erupted suddenly at 2352 h (NZ time) on 6 August 2012. The short-lived <span class="hlt">hydrothermal</span> eruption distributed a fine ash of minor volume (~ 5 × 105 m3) over 200 km from source. The threat of further eruptions prompted an investigation of the possible health and agricultural impacts of any future eruptions from this volcano, particularly since the most recent large-scale ash falls in New Zealand in 1995-1996 had generated significant agricultural problems, including livestock deaths. Deposited ash was sampled between 5 and 200 km from the volcano as soon as possible after the eruption. Two sub-lobes of ash were identified from different vent areas and displayed subtly different leaching properties. The first was an initial small lobe directed NNE, likely formed from drifting low-level clouds associated with the initial lateral explosive blast and surges. The main fall lobe, directed eastward, was sourced from a short-lived vertical plume that rose up to c. 8 km. Ash from the initial fall lobe had higher concentrations of F and Al, in single-step leaches as well as in the totals of three, sequential extractions. Further, the initial lobe showed a higher proportion of soluble F and Al extracted in the first leach, compared to totals. A linear relationship between concentrations of Al and F in single leaches from the 6 August eruption was highly significant (Pearson correlation coefficient r = 0.987 for 1:20 leaching ratios and r = 0.971 for 1:100), suggesting the presence of soluble alumino-fluoride complexes (AlFx+ 3 - x). An even more significant 1:1 ratio is displayed for the largest concentration leached ions of Ca and SO4, which correspond to the presence of crystalline gypsum throughout the newly excavated <span class="hlt">hydrothermal</span> system. Although no fresh magma was erupted in this event, a shallow intrusion prior to the <span class="hlt">hydrothermal</span> explosion apparently provided significant contents of <span class="hlt">volcanic</span> gas</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..319...12M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..319...12M"><span>Internal structure and <span class="hlt">volcanic</span> hazard potential of Mt Tongariro, New Zealand, from 3D gravity and magnetic models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Craig A.; Williams-Jones, Glyn</p> <p>2016-06-01</p> <p>A new 3D geophysical model of the Mt Tongariro <span class="hlt">Volcanic</span> Massif (TgVM), New Zealand, provides a high resolution view of the volcano's internal structure and <span class="hlt">hydrothermal</span> system, from which we derive implications for <span class="hlt">volcanic</span> hazards. Geologically constrained 3D inversions of potential field data provides a greater level of insight into the <span class="hlt">volcanic</span> structure than is possible from unconstrained models. A complex region of gravity highs and lows (± 6 mGal) is set within a broader, 20 mGal gravity low. A magnetic high (1300 nT) is associated with Mt Ngauruhoe, while a substantial, thick, demagnetised area occurs to the north, coincident with a gravity low and interpreted as representing the <span class="hlt">hydrothermal</span> system. The <span class="hlt">hydrothermal</span> system is constrained to the west by major faults, interpreted as an impermeable barrier to fluid migration and extends to basement depth. These faults are considered low probability areas for future eruption sites, as there is little to indicate they have acted as magmatic pathways. Where the <span class="hlt">hydrothermal</span> system coincides with steep topographic slopes, an increased likelihood of landslides is present and the newly delineated <span class="hlt">hydrothermal</span> system maps the area most likely to have phreatic eruptions. Such eruptions, while small on a global scale, are important hazards at the TgVM as it is a popular hiking area with hundreds of visitors per day in close proximity to eruption sites. The model shows that the volume of <span class="hlt">volcanic</span> material erupted over the lifespan of the TgVM is five to six times greater than previous estimates, suggesting a higher rate of magma supply, in line with global rates of andesite production. We suggest that our model of physical property distribution can be used to provide constraints for other models of dynamic geophysical processes occurring at the TgVM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS51E..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS51E..02C"><span>Near-Seafloor Magnetic Exploration of Submarine <span class="hlt">Hydrothermal</span> Systems in the Kermadec Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caratori Tontini, F.; de Ronde, C. E. J.; Tivey, M.; Kinsey, J. C.</p> <p>2014-12-01</p> <p>Magnetic data can provide important information about <span class="hlt">hydrothermal</span> systems because <span class="hlt">hydrothermal</span> alteration can drastically reduce the magnetization of the host <span class="hlt">volcanic</span> rocks. Near-seafloor data (≤70 m altitude) are required to map <span class="hlt">hydrothermal</span> systems in detail; Autonomous Underwater Vehicles (AUVs) are the ideal platform to provide this level of resolution. Here, we show the results of high-resolution magnetic surveys by the ABE and Sentry AUVs for selected submarine volcanoes of the Kermadec arc. 3-D magnetization models derived from the inversion of magnetic data, when combined with high resolution seafloor bathymetry derived from multibeam surveys, provide important constraints on the subseafloor geometry of <span class="hlt">hydrothermal</span> upflow zones and the structural control on the development of seafloor <span class="hlt">hydrothermal</span> vent sites as well as being a tool for the discovery of previously unknown <span class="hlt">hydrothermal</span> sites. Significant differences exist between the magnetic expressions of <span class="hlt">hydrothermal</span> sites at caldera volcanoes ("donut" pattern) and cones ("Swiss cheese" pattern), respectively. Subseafloor 3-D magnetization models also highlight structural differences between focused and diffuse vent sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..324..156L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..324..156L"><span>Evidence of recent deep magmatic <span class="hlt">activity</span> at Cerro Bravo-Cerro Machín <span class="hlt">volcanic</span> complex, central Colombia. Implications for future <span class="hlt">volcanic</span> <span class="hlt">activity</span> at Nevado del Ruiz, Cerro Machín and other volcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Londono, John Makario</p> <p>2016-09-01</p> <p>In the last nine years (2007-2015), the Cerro Bravo-Cerro Machín <span class="hlt">volcanic</span> complex (CBCMVC), located in central Colombia, has experienced many changes in <span class="hlt">volcanic</span> <span class="hlt">activity</span>. In particular at Nevado del Ruiz volcano (NRV), Cerro Machin volcano (CMV) and Cerro Bravo (CBV) volcano. The recent <span class="hlt">activity</span> of NRV, as well as increasing seismic <span class="hlt">activity</span> at other <span class="hlt">volcanic</span> centers of the CBCMVC, were preceded by notable changes in various geophysical and geochemical parameters, that suggests renewed magmatic <span class="hlt">activity</span> is occurring at the <span class="hlt">volcanic</span> complex. The onset of this <span class="hlt">activity</span> started with seismicity located west of the <span class="hlt">volcanic</span> complex, followed by seismicity at CBV and CMV. Later in 2010, strong seismicity was observed at NRV, with two small eruptions in 2012. After that, seismicity has been observed intermittently at other <span class="hlt">volcanic</span> centers such as Santa Isabel, Cerro España, Paramillo de Santa Rosa, Quindío and Tolima volcanoes, which persists until today. Local deformation was observed from 2007 at NRV, followed by possible regional deformation at various <span class="hlt">volcanic</span> centers between 2011 and 2013. In 2008, an increase in CO2 and Radon in soil was observed at CBV, followed by a change in helium isotopes at CMV between 2009 and 2011. Moreover, SO2 showed an increase from 2010 at NRV, with values remaining high until the present. These observations suggest that renewed magmatic <span class="hlt">activity</span> is currently occurring at CBCMVC. NRV shows changes in its <span class="hlt">activity</span> that may be related to this new magmatic <span class="hlt">activity</span>. NRV is currently exhibiting the most <span class="hlt">activity</span> of any volcano in the CBCMVC, which may be due to it being the only open <span class="hlt">volcanic</span> system at this time. This suggests that over the coming years, there is a high probability of new unrest or an increase in <span class="hlt">volcanic</span> <span class="hlt">activity</span> of other volcanoes of the CBCMVC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.479..120C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.479..120C"><span><span class="hlt">Hydrothermal</span> deposition on the Juan de Fuca Ridge over multiple glacial-interglacial cycles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Costa, Kassandra M.; McManus, Jerry F.; Middleton, Jennifer L.; Langmuir, Charles H.; Huybers, Peter J.; Winckler, Gisela; Mukhopadhyay, Sujoy</p> <p>2017-12-01</p> <p><span class="hlt">Hydrothermal</span> systems play an important role in modern marine chemistry, but little is known about how they may have varied on 100,000 year timescales. Here we present high-resolution records of <span class="hlt">non</span>-lithogenic metal fluxes within sediment cores covering the last 500,000 years of <span class="hlt">hydrothermal</span> deposition on the flanks of the Juan de Fuca Ridge. Six adjacent, gridded cores were analyzed by x-ray fluorescence for Fe, Mn, and Cu concentrations, corrected for lithogenic inputs with Ti, and normalized to excess initial 230Th to generate <span class="hlt">non</span>-lithogenic metal flux records that provide the longest orbitally resolved reconstructions of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> currently available. Fe fluxes vary with global sea level over the last two glacial cycles, suggesting higher <span class="hlt">hydrothermal</span> deposition during interglacial periods. The observed negative relationship between Fe and Mn indicates variable sediment redox conditions and diagenetic remobilization of sedimentary Mn over time. Thus, Mn fluxes may not be a reliable indicator for <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in the Juan de Fuca Ridge sediment cores. Cu fluxes show substantial high-frequency variability that may be linked to changes in vent temperature related to increased magmatic production during glacial periods. Deglacial <span class="hlt">hydrothermal</span> peaks on the Juan de Fuca Ridge are consistent with previously published records from the Mid-Atlantic Ridge and the East Pacific Rise. Moreover, on the Juan de Fuca Ridge, the deglacial peaks in <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> are followed by relatively high <span class="hlt">hydrothermal</span> fluxes throughout the ensuing interglacial periods relative to the previous glacial period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMIN23A1493J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMIN23A1493J"><span>Classifying <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Using an Empirical Decision Making Algorithm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Junek, W. N.; Jones, W. L.; Woods, M. T.</p> <p>2012-12-01</p> <p>Detection and classification of developing <span class="hlt">volcanic</span> <span class="hlt">activity</span> is vital to eruption forecasting. Timely information regarding an impending eruption would aid civil authorities in determining the proper response to a developing crisis. In this presentation, <span class="hlt">volcanic</span> <span class="hlt">activity</span> is characterized using an event tree classifier and a suite of empirical statistical models derived through logistic regression. Forecasts are reported in terms of the United States Geological Survey (USGS) volcano alert level system. The algorithm employs multidisciplinary data (e.g., seismic, GPS, InSAR) acquired by various volcano monitoring systems and source modeling information to forecast the likelihood that an eruption, with a <span class="hlt">volcanic</span> explosivity index (VEI) > 1, will occur within a quantitatively constrained area. Logistic models are constructed from a sparse and geographically diverse dataset assembled from a collection of historic <span class="hlt">volcanic</span> unrest episodes. Bootstrapping techniques are applied to the training data to allow for the estimation of robust logistic model coefficients. Cross validation produced a series of receiver operating characteristic (ROC) curves with areas ranging between 0.78-0.81, which indicates the algorithm has good predictive capabilities. The ROC curves also allowed for the determination of a false positive rate and optimum detection for each stage of the algorithm. Forecasts for historic <span class="hlt">volcanic</span> unrest episodes in North America and Iceland were computed and are consistent with the actual outcome of the events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SGeo...36..683Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SGeo...36..683Q"><span>Crustal Structure of the Tengchong Intra-plate <span class="hlt">Volcanic</span> Area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qian, Rongyi; Tong, Vincent C. H.</p> <p>2015-09-01</p> <p>We here provide an overview of our current understanding of the crustal structure of Tengchong in southwest China, a key intra-plate <span class="hlt">volcanic</span> area along the Himalayan geothermal belt. Given that there is hitherto a lack of information about the near-surface structure of intra-plate <span class="hlt">volcanic</span> areas, we present the first seismic reflection and velocity constraints on the shallow crust between intra-plate volcanoes. Our near-surface seismic images reveal the existence of dome-shaped seismic reflectors (DSRs) in the shallow crust between intra-plate <span class="hlt">volcanic</span> clusters in Tengchong. The two DSRs are both ~2 km wide, and the shallowest parts of the DSRs are found at the depth of 200-300 m. The velocity model shows that the shallow low-velocity layer (<4 km/s) is anomalously thick (~1 km) in the region where the DSRs are observed. The presence of DSRs indicates significant levels of intra-plate magmatism beneath the along-axis gap separating two volcano clusters. Along-axis gaps between volcano clusters are therefore not necessarily an indicator of lower levels of magmatism. The seismic images obtained in this technically challenging area for controlled-source seismology allow us to conclude that shallow crustal structures are crucial for understanding the along-axis variations of magmatism and <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> in intra-plate <span class="hlt">volcanic</span> areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CoMP..173...40K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CoMP..173...40K"><span>Constraints on the source of Cu in a submarine magmatic-<span class="hlt">hydrothermal</span> system, Brothers volcano, Kermadec island arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keith, Manuel; Haase, Karsten M.; Klemd, Reiner; Smith, Daniel J.; Schwarz-Schampera, Ulrich; Bach, Wolfgang</p> <p>2018-05-01</p> <p>Most magmatic-<span class="hlt">hydrothermal</span> Cu deposits are genetically linked to arc magmas. However, most continental or oceanic arc magmas are barren, and hence new methods have to be developed to distinguish between barren and mineralised arc systems. Source composition, melting conditions, the timing of S saturation and an initial chalcophile element-enrichment represent important parameters that control the potential of a subduction setting to host an economically valuable deposit. Brothers volcano in the Kermadec island arc is one of the best-studied examples of arc-related submarine magmatic-<span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. This study, for the first time, compares the chemical and mineralogical composition of the Brothers seafloor massive sulphides and the associated dacitic to rhyolitic lavas that host the <span class="hlt">hydrothermal</span> system. Incompatible trace element ratios, such as La/Sm and Ce/Pb, indicate that the basaltic melts from L'Esperance volcano may represent a parental analogue to the more evolved Brothers lavas. Copper-rich magmatic sulphides (Cu > 2 wt%) identified in fresh <span class="hlt">volcanic</span> glass and phenocryst phases, such as clinopyroxene, plagioclase and Fe-Ti oxide suggest that the surrounding lavas that host the Brothers <span class="hlt">hydrothermal</span> system represent a potential Cu source for the sulphide ores at the seafloor. Thermodynamic calculations reveal that the Brothers melts reached volatile saturation during their evolution. Melt inclusion data and the occurrence of sulphides along vesicle margins indicate that an exsolving volatile phase extracted Cu from the silicate melt and probably contributed it to the overlying <span class="hlt">hydrothermal</span> system. Hence, the formation of the Cu-rich seafloor massive sulphides (up to 35.6 wt%) is probably due to the contribution of Cu from a bimodal source including wall rock leaching and magmatic degassing, in a mineralisation style that is hybrid between Cyprus-type <span class="hlt">volcanic</span>-hosted massive sulphide and subaerial epithermal-porphyry deposits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43B2883S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43B2883S"><span>Modeling <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> on Enceladus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stamper, T., Jr.; Farough, A.</p> <p>2017-12-01</p> <p>Cassini's mass spectrometer data and gravitational field measurements imply water-rock interactions around the porous core of Enceladus. Using such data we characterize global heat and fluid transport properties of the core and model the ongoing <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> on Enceladus. We assume that within the global ocean beneath the surface ice, seawater percolates downward into the core where it is heated and rises to the oceanfloor where it emanates in the form of diffuse discharge. We utilize the data from Hsu et al., [2015] with models of diffuse flow in seafloor <span class="hlt">hydrothermal</span> systems by Lowell et al., [2015] to characterize the global heat transport properties of the Enceladus's core. Based on direct observations the gravitational acceleration (g) is calculated 0.123 m s-2. We assume fluid's density (ρ) is 10­3 kg m-3 and the specific heat of the fluid (cf) is 4000 Jkg-1 °C-1. From these values effective thermal diffusivity (a*) is calculated as 10­-6 m2 s-1. We also assume the coefficient of thermal expansion of fluid (αf) and the kinematic viscosity of fluid (ν) to be 10-4 °C-1 and 10­-6 m2 s-1 respectively. The estimated Rayleigh number (Ra) ranges between 0.11-2468.0, for core porosity (φ) of 5-15%, permeability (k) between 10-12-10-8 m2 and temperature between 90-200 °C and the depth of fluid circulation of 100 m. High values of Rayleigh number, cause vigorous convection within the core of Enceladus. Numerical modeling of reactive transport in multicomponent, multiphase systems is required to obtain a full understanding of the characteristics and evolution of the <span class="hlt">hydrothermal</span> system on Enceladus, but simple scaling laws can provide insight into the physics of water-rock interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1337250-global-volcanic-aerosol-properties-derived-from-emissions-using-cesm1-waccm-volcanic-aerosols-derived-from-emissions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1337250-global-volcanic-aerosol-properties-derived-from-emissions-using-cesm1-waccm-volcanic-aerosols-derived-from-emissions"><span>Global <span class="hlt">volcanic</span> aerosol properties derived from emissions, 1990-2014, using CESM1(WACCM): <span class="hlt">VOLCANIC</span> AEROSOLS DERIVED FROM EMISSIONS</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>Mills, Michael J.; Schmidt, Anja; Easter, Richard</p> <p></p> <p>Accurate representation of global stratospheric aerosol properties from <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> sulfur emissions is key to understanding the cooling effects and ozone-loss enhancements of recent <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Attribution of climate and ozone variability to <span class="hlt">volcanic</span> <span class="hlt">activity</span> is of particular interest in relation to the post-2000 slowing in the apparent rate of global average temperature increases, and variable recovery of the Antarctic ozone hole. We have developed a climatology of global aerosol properties from 1990 to 2014 calculated based on <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> emissions of sulfur sources. We have complied a database of <span class="hlt">volcanic</span> SO2 emissions and plume altitudes for eruptionsmore » between 1990 and 2014, and a new prognostic capability for simulating stratospheric sulfate aerosols in version 5 of the Whole Atmosphere Community Climate Model, a component of the Community Earth System Model. Our climatology shows remarkable agreement with ground-based lidar observations of stratospheric aerosol optical depth (SAOD), and with in situ measurements of aerosol surface area density (SAD). These properties are key parameters in calculating the radiative and chemical effects of stratospheric aerosols. Our SAOD climatology represents a significant improvement over satellite-based analyses, which ignore aerosol extinction below 15 km, a region that can contain the vast majority of stratospheric aerosol extinction at mid- and high-latitudes. Our SAD climatology significantly improves on that provided for the Chemistry-Climate Model Initiative, which misses 60% of the SAD measured in situ. Our climatology of aerosol properties is publicly available on the Earth System Grid.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26438396','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26438396"><span>Increased thyroid cancer incidence in a basaltic <span class="hlt">volcanic</span> area is associated with <span class="hlt">non</span>-anthropogenic pollution and biocontamination.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Malandrino, Pasqualino; Russo, Marco; Ronchi, Anna; Minoia, Claudio; Cataldo, Daniela; Regalbuto, Concetto; Giordano, Carla; Attard, Marco; Squatrito, Sebastiano; Trimarchi, Francesco; Vigneri, Riccardo</p> <p>2016-08-01</p> <p>The increased thyroid cancer incidence in <span class="hlt">volcanic</span> areas suggests an environmental effect of <span class="hlt">volcanic</span>-originated carcinogens. To address this problem, we evaluated environmental pollution and biocontamination in a <span class="hlt">volcanic</span> area of Sicily with increased thyroid cancer incidence. Thyroid cancer epidemiology was obtained from the Sicilian Regional Registry for Thyroid Cancer. Twenty-seven trace elements were measured by quadrupole mass spectrometry in the drinking water and lichens (to characterize environmental pollution) and in the urine of residents (to identify biocontamination) in the Mt. Etna <span class="hlt">volcanic</span> area and in adjacent control areas. Thyroid cancer incidence was 18.5 and 9.6/10(5) inhabitants in the <span class="hlt">volcanic</span> and the control areas, respectively. The increase was exclusively due to the papillary histotype. Compared with control areas, in the <span class="hlt">volcanic</span> area many trace elements were increased in both drinking water and lichens, indicating both water and atmospheric pollution. Differences were greater for water. Additionally, in the urine of the residents of the <span class="hlt">volcanic</span> area, the average levels of many trace elements were significantly increased, with values higher two-fold or more than in residents of the control area: cadmium (×2.1), mercury (×2.6), manganese (×3.0), palladium (×9.0), thallium (×2.0), uranium (×2.0), vanadium (×8.0), and tungsten (×2.4). Urine concentrations were significantly correlated with values in water but not in lichens. Our findings reveal a complex <span class="hlt">non</span>-anthropogenic biocontamination with many trace elements in residents of an <span class="hlt">active</span> <span class="hlt">volcanic</span> area where thyroid cancer incidence is increased. The possible carcinogenic effect of these chemicals on the thyroid and other tissues cannot be excluded and should be investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28682665','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28682665"><span>Can Life Begin on Enceladus? A Perspective from <span class="hlt">Hydrothermal</span> Chemistry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Deamer, David; Damer, Bruce</p> <p>2017-09-01</p> <p>Enceladus is a target of future missions designed to search for existing life or its precursors. Recent flybys of Enceladus by the Cassini probe have confirmed the existence of a long-lived global ocean laced with organic compounds and biologically available nitrogen. This immediately suggests the possibility that life could have begun and may still exist on Enceladus. Here we will compare the properties of two proposed sites for the origin of life on Earth-<span class="hlt">hydrothermal</span> vents on the ocean floor and <span class="hlt">hydrothermal</span> <span class="hlt">volcanic</span> fields at the surface-and ask whether similar conditions could have fostered the origin of life on Enceladus. The answer depends on which of the two sites would be more conducive for the chemical evolution leading to life's origin. A <span class="hlt">hydrothermal</span> vent origin would allow life to begin in the Enceladus ocean, but if the origin of life requires freshwater <span class="hlt">hydrothermal</span> pools undergoing wet-dry cycles, the Enceladus ocean could be habitable but lifeless. These arguments also apply directly to Europa and indirectly to early Mars. Key Words: Enceladus-<span class="hlt">Hydrothermal</span> vents-<span class="hlt">Hydrothermal</span> fields-Origin of life. Astrobiology 17, 834-839.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610390','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610390"><span>Can Life Begin on Enceladus? A Perspective from <span class="hlt">Hydrothermal</span> Chemistry</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Damer, Bruce</p> <p>2017-01-01</p> <p>Abstract Enceladus is a target of future missions designed to search for existing life or its precursors. Recent flybys of Enceladus by the Cassini probe have confirmed the existence of a long-lived global ocean laced with organic compounds and biologically available nitrogen. This immediately suggests the possibility that life could have begun and may still exist on Enceladus. Here we will compare the properties of two proposed sites for the origin of life on Earth—<span class="hlt">hydrothermal</span> vents on the ocean floor and <span class="hlt">hydrothermal</span> <span class="hlt">volcanic</span> fields at the surface—and ask whether similar conditions could have fostered the origin of life on Enceladus. The answer depends on which of the two sites would be more conducive for the chemical evolution leading to life's origin. A <span class="hlt">hydrothermal</span> vent origin would allow life to begin in the Enceladus ocean, but if the origin of life requires freshwater <span class="hlt">hydrothermal</span> pools undergoing wet-dry cycles, the Enceladus ocean could be habitable but lifeless. These arguments also apply directly to Europa and indirectly to early Mars. Key Words: Enceladus—<span class="hlt">Hydrothermal</span> vents—<span class="hlt">Hydrothermal</span> fields—Origin of life. Astrobiology 17, 834–839. PMID:28682665</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816744P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816744P"><span>Diffuse H_{2} emission: a useful geochemical tool to monitor the <span class="hlt">volcanic</span> <span class="hlt">activity</span> at El Hierro volcano system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pérez, Nemesio M.; Melián, Gladys; González-Santana, Judit; Barrancos, José; Padilla, Germán; Rodríguez, Fátima; Padrón, Eleazar; Hernández, Pedro A.</p> <p>2016-04-01</p> <p>The occurrence of interfering processes affecting reactive gases as CO2 during its ascent from magmatic bodies or <span class="hlt">hydrothermal</span> systems toward the surface environment hinders the interpretation of their enrichments in the soil atmosphere and fluxes for volcano monitoring purposes (Marini and Gambardella, 2005). These processes include gas scrubbing by ground-waters and interaction with rocks, decarbonatation processes, biogenic production, etc. Within the rest of the soil gases, particularly interest has been addressed to light and highly mobile gases. They offer important advantages for the detection of vertical permeability structures, because their interaction with the surrounding rocks or fluids during the ascent toward the surface is minimum. H2 is one of the most abundant trace species in volcano-<span class="hlt">hydrothermal</span> systems and is a key participant in many redox reactions occurring in the <span class="hlt">hydrothermal</span> reservoir gas (Giggenbach, 1987). Although H2 can be produced in soils by N2-fixing and fertilizing bacteria, soils are considered nowadays as sinks of molecular hydrogen (Smith-Downey et al., 2006). Because of its chemical and physical characteristics, H2 generated within the crust moves rapidly and escapes to the atmosphere. These characteristics make H2 one of the best geochemical indicators of magmatic and geothermal <span class="hlt">activity</span> at depth. El Hierro is the youngest and the SW-most of the Canary Islands and the scenario of the last <span class="hlt">volcanic</span> eruption of the archipelago, a submarine eruption that took place 2 km off the southern coast of the island from October 2011 to March 2012. Since at El Hierro Island there are not any surface geothermal manifestations (fumaroles, etc), we have focused our studies on soil degassing surveys. Here we show the results of soil H2 emission surveys that have been carried out regularly since mid-2012. Soil gas samples were collected in ˜600 sites selected based on their accessibility and geological criteria. Soil gases were sampled at ˜40</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1412541R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1412541R"><span>Future <span class="hlt">volcanic</span> lake research: revealing secrets from poorly studied lakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rouwet, D.; Tassi, F.; Mora-Amador, R. A.</p> <p>2012-04-01</p> <p><span class="hlt">Volcanic</span> lake research boosted after the 1986 Lake Nyos lethal gas burst, a limnic rather than <span class="hlt">volcanic</span> event. This led to the formation of the IAVCEI-Commission on <span class="hlt">Volcanic</span> Lakes, which grew out into a multi-disciplinary scientific community since the 1990's. At Lake Nyos, a degassing pipe is functional since 2001, and two additional pipes were added in 2011, aimed to prevent further limnic eruption events. There are between 150 and 200 <span class="hlt">volcanic</span> lakes on Earth. Some acidic crater lakes topping <span class="hlt">active</span> magmatic-<span class="hlt">hydrothermal</span> systems are monitored continuously or discontinuously. Such detailed studies have shown their usefulness in <span class="hlt">volcanic</span> surveillance (e.g. Ruapehu, Yugama-Kusatsu-Shiran, Poás). Others are "Nyos-type" lakes, with possible gas accumulation in bottom waters and thus potentially hazardous. "Nyos-type" lakes tend to remain stably stratified in tropical and sub-tropical climates (meromictic), leading to long-term gas build-up and thus higher potential risk. In temperate climates, such lakes tend to turn over in winter (monomictic), and thus liberating its gas charge yearly. We line out research strategies for the different types of lakes. We believe a complementary, multi-disciplinary approach (geochemistry, geophysics, limnology, biology, statistics, etc.) will lead to new insights and ideas, which can be the base for future following-up and monitoring. After 25 years of pioneering studies on rather few lakes, the scientific community should be challenged to study the many poorly studied <span class="hlt">volcanic</span> lakes, in order to better constrain the related hazard, based on probabilistic approaches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25881434','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25881434"><span>[Micro-area characteristics of laminated chert in the <span class="hlt">volcanic</span> rocks of Xionger Group of Ruyang area and its geological significances].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Luo, An; Li, Hong-zhong; Zhao, Ming-zhen; Yang, Zhi-jun; Liang, Jin; He, Jun-guo</p> <p>2014-12-01</p> <p> sedimentation contributed to the bands (or lamellars) with minerals of much smaller grain size, which therefore resulted in diversities from the other bands (or lamellars). According to this, the repeated bands (or lamellars) denoted the <span class="hlt">volcanic</span> <span class="hlt">activities</span> were cyclic during the formation of the chert. What's more, the carbonate vein came from the precipitation of subsequent <span class="hlt">hydrothermal</span> fluids in the fracture of the chert, which contributed to the changes (e. g. rising in crystallinity degree of silica and formation of micro-structure of new silicate) near the interface between chert and the carbonate vein. Although there were many impurity minerals with complex genesis, the relatively lower content of silica in the chert of Xionger Group was due to the <span class="hlt">volcanic</span> mineral mainly. Since there were impurity minerals of <span class="hlt">volcanic</span> genesis in relatively large amount, the content of silica in the chert of Xionger Group was hence relatively low. In this study, the Raman analysis was witnessed to be an effective way in the researches on the chert, and could open out the type of mineral, micro-structure and degrees of crystallinity (or order). These characteristics were well kept in the micro-area, and played significant roles to reflect and understand the formation mechanism and subsequent evolution of the chert.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V13A2587C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V13A2587C"><span>A new comprehensive database of global <span class="hlt">volcanic</span> gas analyses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clor, L. E.; Fischer, T. P.; Lehnert, K. A.; McCormick, B.; Hauri, E. H.</p> <p>2013-12-01</p> <p><span class="hlt">Volcanic</span> volatiles are the driving force behind eruptions, powerful indicators of magma provenance, present localized hazards, and have implications for climate. Studies of <span class="hlt">volcanic</span> emissions are necessary for understanding volatile cycling from the mantle to the atmosphere. Gas compositions vary with <span class="hlt">volcanic</span> <span class="hlt">activity</span>, making it important to track their chemical variability over time. As studies become increasingly interdisciplinary, it is critical to have a mechanism to integrate decades of gas studies across disciplines. Despite the value of this research to a variety of fields, there is currently no integrated network to house all <span class="hlt">volcanic</span> and <span class="hlt">hydrothermal</span> gas data, making spatial, temporal, and interdisciplinary comparison studies time-consuming. To remedy this, we are working to establish a comprehensive database of <span class="hlt">volcanic</span> gas emissions and compositions worldwide, as part of the Deep Carbon Observatory's DECADE (Deep Carbon Degassing) initiative. <span class="hlt">Volcanic</span> gas data have been divided into two broad categories: 1) chemical analyses from samples collected directly at the <span class="hlt">volcanic</span> source, and 2) measurements of gas concentrations and fluxes, such as remotely by mini-DOAS or satellite, or in-plume such as by multiGAS. The gas flux database effort is realized by the Global <span class="hlt">Volcanism</span> Program of the Smithsonian Institution (abstract by Brendan McCormick, this meeting). The direct-sampling data is the subject of this presentation. Data from direct techniques include samples of gases collected at the <span class="hlt">volcanic</span> source from fumaroles and springs, tephras analyzed for gas contents, filter pack samples of gases collected in a plume, and any other data types that involve collection of a sample. Data are incorporated into the existing framework of the Petrological Database, PetDB. Association with PetDB is advantageous as it will allow <span class="hlt">volcanic</span> gas data to be linked to chemical data from lava or tephra samples, forming more complete ties between the eruptive products and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26279090','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26279090"><span>Magma injection beneath the urban area of Naples: a new mechanism for the 2012-2013 <span class="hlt">volcanic</span> unrest at Campi Flegrei caldera.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>D'Auria, Luca; Pepe, Susi; Castaldo, Raffaele; Giudicepietro, Flora; Macedonio, Giovanni; Ricciolino, Patrizia; Tizzani, Pietro; Casu, Francesco; Lanari, Riccardo; Manzo, Mariarosaria; Martini, Marcello; Sansosti, Eugenio; Zinno, Ivana</p> <p>2015-08-17</p> <p>We found the first evidence, in the last 30 years, of a renewed magmatic <span class="hlt">activity</span> at Campi Flegrei caldera from January 2012 to June 2013. The ground deformation, observed through satellite interferometry and GPS measurements, have been interpreted as the effect of the intrusion at shallow depth (3090 ± 138 m) of 0.0042 ± 0.0002 km(3) of magma within a sill. This interrupts about 28 years of dominant <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and occurs in the context of an unrest phase which began in 2005 and within a more general ground uplift that goes on since 1950. This discovery has implications on the evaluation of the <span class="hlt">volcanic</span> risk and in the <span class="hlt">volcanic</span> surveillance of this densely populated area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..122...41J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..122...41J"><span>Geochemistry of <span class="hlt">hydrothermal</span> vent fluids and its implications for subsurface processes at the <span class="hlt">active</span> Longqi <span class="hlt">hydrothermal</span> field, Southwest Indian Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ji, Fuwu; Zhou, Huaiyang; Yang, Qunhui; Gao, Hang; Wang, Hu; Lilley, Marvin D.</p> <p>2017-04-01</p> <p>The Longqi <span class="hlt">hydrothermal</span> field at 49.6°E on the Southwest Indian Ridge was the first <span class="hlt">active</span> <span class="hlt">hydrothermal</span> field found at a bare-rock ultra-slow spreading mid-ocean ridge. Here we report the chemistry of the <span class="hlt">hydrothermal</span> fluids, for the first time, that were collected from the S zone and the M zone of the Longqi field by gas-tight isobaric samplers by the HOV "Jiaolong" diving cruise in January 2015. According to H2, CH4 and other chemical data of the vent fluid, we suggest that the basement rock at the Longqi field is dominantly mafic. This is consistent with the observation that the host rock of the <span class="hlt">active</span> Longqi <span class="hlt">Hydrothermal</span> field is dominated by extensively distributed basaltic rock. It was very interesting to detect simultaneously discharging brine and vapor caused by phase separation at vents DFF6, DFF20, and DFF5 respectively, in a distance of about 400 m. Based on the end-member fluid chemistry and distance between the vents, we propose that there is a single fluid source at the Longqi field. The fluid branches while rising to the seafloor, and two of the branches reach S zone and M zone and phase separate at similar conditions of about 28-30.2 MPa and 400.6-408.3 °C before they discharge from the vents. The end-member fluid compositions of these vents are comparable with or within the range of variation of known global seafloor <span class="hlt">hydrothermal</span> fluid chemical data from fast, intermediate and slow spreading ridges, which confirms that the spreading rate is not the key factor that directly controls <span class="hlt">hydrothermal</span> fluid chemistry. The composition of basement rock, water-rock interaction and phase separation are the major factors that control the composition of the vent fluids in the Longqi field.</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://adsabs.harvard.edu/abs/2018IJEaS.tmp....6J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IJEaS.tmp....6J"><span>Mixed biogenic and <span class="hlt">hydrothermal</span> quartz in Permian lacustrine shale of Santanghu Basin, NW China: implications for penecontemporaneous transformation of silica minerals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiao, Xin; Liu, Yiqun; Yang, Wan; Zhou, Dingwu; Wang, Shuangshuang; Jin, Mengqi; Sun, Bin; Fan, Tingting</p> <p>2018-01-01</p> <p>The cycling of various isomorphs of authigenic silica minerals is a complex and long-term process. A special type of composite quartz (Qc) grains in tuffaceous shale of Permian Lucaogou Formation in the sediment-starved <span class="hlt">volcanically</span> and <span class="hlt">hydrothermally</span> <span class="hlt">active</span> intracontinental lacustrine Santanghu rift basin (NW China) is studied in detail to demonstrate such processes. Samples from one well in the central basin were subject to petrographic, elemental chemical, and fluid inclusion analyses. About 200 Qc-bearing laminae are 0.1-2 mm and mainly 1 mm thick and intercalated within tuffaceous shale laminae. The Qc grains occur as framework grains and are dispersed in igneous feldspar-dominated matrix, suggesting episodic accumulation. The Qc grains are bedding-parallel, uniform in size (100 s µm), elongate, and radial in crystal pattern, suggesting a biogenic origin. Qc grains are composed of a core of anhedral microcrystalline quartz and an outer part of subhedral mega-quartz grains, whose edges are composed of small euhedral quartz crystals, indicating multiple episodic processes of recrystallization and overgrowth. Abundance of Al and Ti in quartz crystals and estimated temperature from fluid inclusions in Qc grains indicate that processes are related to <span class="hlt">hydrothermal</span> fluids. Finally, the Qc grains are interpreted as original silica precipitation in microorganism (algae?) cysts, which were reworked by bottom currents and altered by <span class="hlt">hydrothermal</span> fluids to recrystalize and overgrow during penecontemporaneous shallow burial. It is postulated that episodic <span class="hlt">volcanic</span> and <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> had changed lake water chemistry, temperature, and nutrient supply, resulting in variations in microorganic productivities and silica cycling. The transformation of authigenic silica from amorphous to well crystallized had occurred in a short time span during shallow burial.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoOD..56..169F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoOD..56..169F"><span>Mineral types of <span class="hlt">hydrothermal</span> alteration zones in the Dukat ore field and their relationships to leucogranite and epithermal gold-silver ore, northeastern Russia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Filimonova, L. G.; Trubkin, N. V.; Chugaev, A. V.</p> <p>2014-05-01</p> <p>The paper considers the localization of potassic and propylitic <span class="hlt">hydrothermal</span> alteration zones in the domal <span class="hlt">volcanic</span>-plutonic structure controlling the position of the Dukat ore field with the eponymous unique epithermal Au-Ag deposit. Comprehensive mineralogical and geochemical data on rocks and minerals in <span class="hlt">hydrothermal</span> alteration zones and associated intrusions have shown that quartz-jarosite-sericite, quartz-pyrite-sericite, and quartz-adularia-chlorite alterations were formed with the participation of fluid flows related to a fingerlike projection of a high-K leucogranite porphyry intrusion with large phenocrysts. These <span class="hlt">hydrothermal</span> alterations developed in the rifted graben under conditions of divergent plate boundaries, whereas quartz-clinozoisite-calcite, epidote-chlorite, and garnet-calcite-chlorite alterations were linked to K-Na leucogranite intrusive bodies and developed under conditions of convergent plate boundaries reactivated as a result of formation of the marginal Okhotsk-Chukotka <span class="hlt">volcanic</span> belt. Phase separation and coagulation of specific portions of ascending fluids resulted in the formation and stabilization of small-sized particles of native silver and other ore components, which enabled involvement in flows of secondary geothermal solutions and ore-forming fluids. The Sr, Nd, and Pb isotopic compositions of rocks and minerals from the <span class="hlt">hydrothermal</span> alteration zones, associated intrusions, and economic orebodies at the Dukat deposit indicate that their components have been derived from the juvenile continental crust, which was altered in pre-Cretaceous periods of endogenic <span class="hlt">activity</span>. The components of gangue minerals of potassic and propylitic hydrothertmal alterations and associated intrusions have been taken from deep sources differing in 87Sr/86Sr and 143Nd/144Nd at similar U/Pb and Th/Pb ratios. Chalcophile lead in products of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and melanocratic inclusions in leucogranite has been taken from regions with elevated U/Pb and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999LPI....30.1887B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999LPI....30.1887B"><span><span class="hlt">Hydrothermal</span> Alteration Products as Key to Formation of Duricrust and Rock Coatings on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bishop, J. L.</p> <p>1999-03-01</p> <p>A model is presented for the formation of duricrust and rock coatings on Mars. <span class="hlt">Hydrothermal</span> alteration of <span class="hlt">volcanic</span> tephra may produce a corrosive agent that attacks rock surfaces and binds dust particles to form duricrust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..320...75D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..320...75D"><span>Paleoproterozoic <span class="hlt">volcanic</span> centers of the São Félix do Xingu region, Amazonian craton, Brazil: <span class="hlt">Hydrothermal</span> alteration and metallogenetic potential</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>da Cruz, Raquel Souza; Fernandes, Carlos Marcello Dias; Villas, Raimundo Netuno Nobre; Juliani, Caetano; Monteiro, Lena Virgínia Soares; Lagler, Bruno; Misas, Carlos Mario Echeverri</p> <p>2016-06-01</p> <p>Geological, petrographic, scanning electron microscopy, and X-ray diffraction studies revealed <span class="hlt">hydrothermalized</span> lithotypes evidenced by overprinted zones of potassic, propylitic, sericitic, and intermediate argillic alterations types, with pervasive and fracture-controlled styles, in Paleoproterozoic volcano-plutonic units of the São Félix do Xingu region, Amazonian craton, northern Brazil. The Sobreiro Formation presents propylitic (epidote + chlorite + carbonate + clinozoisite + sericite + quartz ± albite ± hematite ± pyrite), sericitic (sericite + quartz + carbonate), and potassic (potassic feldspar + hematite) alterations. The prehnite-pumpellyite pair that is common in geothermal fields also occurs in this unit. The Santa Rosa Formation shows mainly potassic (biotite + microcline ± magnetite), sericitic (sericite + quartz + carbonate ± chlorite ± gold), and intermediate argillic (montmorillonite + kaolinite/halloysite + illite) alterations. These findings strongly suggest the involvement of magma-sourced and meteoric fluids and draw attention to the metallogenetic potential of these <span class="hlt">volcanic</span> units for Paleoproterozoic epithermal and rare and base metal porphyry-type mineralizations, similar to those already identified in other portions of the Amazonian craton.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060036492&hterms=right+Mexican&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dright%2BMexican','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060036492&hterms=right+Mexican&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dright%2BMexican"><span><span class="hlt">Volcanic</span> Hazards Survey in the Trans Mexican <span class="hlt">Volcanic</span> Belt</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abrams, Michael; Siebe, Claus; Macias, Jose Luis</p> <p>1996-01-01</p> <p>We have assembled a digital mosaic of 11 Landsat Thematic images to serve as a mapping base for reconnaissance <span class="hlt">activities</span> within the Trans Mexican <span class="hlt">Volcanic</span> Belt. This will aid us in interpretation and in the evaluation of potential <span class="hlt">activity</span> of all the <span class="hlt">volcanic</span> centers there. One result is a <span class="hlt">volcanic</span> hazards map of the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5079M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5079M"><span><span class="hlt">Volcanic</span> hazard management in dispersed <span class="hlt">volcanism</span> areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marrero, Jose Manuel; Garcia, Alicia; Ortiz, Ramon</p> <p>2014-05-01</p> <p>Traditional <span class="hlt">volcanic</span> hazard methodologies were developed mainly to deal with the big stratovolcanoes. In such type of volcanoes, the hazard map is an important tool for decision-makers not only during a <span class="hlt">volcanic</span> crisis but also for territorial planning. According to the past and recent eruptions of a volcano, all possible <span class="hlt">volcanic</span> hazards are modelled and included in the hazard map. Combining the hazard map with the Event Tree the impact area can be zoned and defining the likely eruptive scenarios that will be used during a real <span class="hlt">volcanic</span> crisis. But in areas of disperse <span class="hlt">volcanism</span> is very complex to apply the same <span class="hlt">volcanic</span> hazard methodologies. The event tree do not take into account unknown vents, because the spatial concepts included in it are only related with the distance reached by <span class="hlt">volcanic</span> hazards. The <span class="hlt">volcanic</span> hazard simulation is also difficult because the vent scatter modifies the results. The <span class="hlt">volcanic</span> susceptibility try to solve this problem, calculating the most likely areas to have an eruption, but the differences between low and large values obtained are often very small. In these conditions the traditional hazard map effectiveness could be questioned, making necessary a change in the concept of hazard map. Instead to delimit the potential impact areas, the hazard map should show the expected behaviour of the <span class="hlt">volcanic</span> <span class="hlt">activity</span> and how the differences in the landscape and internal geo-structures could condition such behaviour. This approach has been carried out in La Palma (Canary Islands), combining the concept of long-term hazard map with the short-term <span class="hlt">volcanic</span> scenario to show the expected <span class="hlt">volcanic</span> <span class="hlt">activity</span> behaviour. The objective is the decision-makers understand how a <span class="hlt">volcanic</span> crisis could be and what kind of mitigation measurement and strategy could be used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29403480','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29403480"><span><span class="hlt">Volcanic</span> Ash <span class="hlt">Activates</span> the NLRP3 Inflammasome in Murine and Human Macrophages.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Damby, David E; Horwell, Claire J; Baxter, Peter J; Kueppers, Ulrich; Schnurr, Max; Dingwell, Donald B; Duewell, Peter</p> <p>2017-01-01</p> <p><span class="hlt">Volcanic</span> ash is a heterogeneous mineral dust that is typically composed of a mixture of amorphous (glass) and crystalline (mineral) fragments. It commonly contains an abundance of the crystalline silica (SiO 2 ) polymorph cristobalite. Inhalation of crystalline silica can induce inflammation by stimulating the NLRP3 inflammasome, a cytosolic receptor complex that plays a critical role in driving inflammatory immune responses. Ingested material results in the assembly of NLRP3, ASC, and caspase-1 with subsequent secretion of the interleukin-1 family cytokine IL-1β. Previous toxicology work suggests that cristobalite-bearing <span class="hlt">volcanic</span> ash is minimally reactive, calling into question the reactivity of <span class="hlt">volcanically</span> derived crystalline silica, in general. In this study, we target the NLRP3 inflammasome as a crystalline silica responsive element to clarify <span class="hlt">volcanic</span> cristobalite reactivity. We expose immortalized bone marrow-derived macrophages of genetically engineered mice and primary human peripheral blood mononuclear cells (PBMCs) to ash from the Soufrière Hills volcano as well as representative, pure-phase samples of its primary componentry (<span class="hlt">volcanic</span> glass, feldspar, cristobalite) and measure NLRP3 inflammasome <span class="hlt">activation</span>. We demonstrate that respirable Soufrière Hills <span class="hlt">volcanic</span> ash induces the <span class="hlt">activation</span> of caspase-1 with subsequent release of mature IL-1β in a NLRP3 inflammasome-dependent manner. Macrophages deficient in NLRP3 inflammasome components are incapable of secreting IL-1β in response to <span class="hlt">volcanic</span> ash ingestion. Cellular uptake induces lysosomal destabilization involving cysteine proteases. Furthermore, the response involves <span class="hlt">activation</span> of mitochondrial stress pathways leading to the generation of reactive oxygen species. Considering ash componentry, cristobalite is the most reactive pure-phase with other components inducing only low-level IL-1β secretion. Inflammasome <span class="hlt">activation</span> mediated by inhaled ash and its potential relevance in chronic pulmonary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70195128','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70195128"><span><span class="hlt">Volcanic</span> ash <span class="hlt">activates</span> the NLRP3 inflammasome in murine and human macrophages</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Damby, David; Horwell, Claire J.; Baxter, Peter J.; Kueppers, Ulrich; Schnurr, Max; Dingwell, Donald B.; Duewell, Peter</p> <p>2018-01-01</p> <p><span class="hlt">Volcanic</span> ash is a heterogeneous mineral dust that is typically composed of a mixture of amorphous (glass) and crystalline (mineral) fragments. It commonly contains an abundance of the crystalline silica (SiO2) polymorph cristobalite. Inhalation of crystalline silica can induce inflammation by stimulating the NLRP3 inflammasome, a cytosolic receptor complex that plays a critical role in driving inflammatory immune responses. Ingested material results in the assembly of NLRP3, ASC, and caspase-1 with subsequent secretion of the interleukin-1 family cytokine IL-1β. Previous toxicology work suggests that cristobalite-bearing <span class="hlt">volcanic</span> ash is minimally reactive, calling into question the reactivity of <span class="hlt">volcanically</span> derived crystalline silica, in general. In this study, we target the NLRP3 inflammasome as a crystalline silica responsive element to clarify <span class="hlt">volcanic</span> cristobalite reactivity. We expose immortalized bone marrow-derived macrophages of genetically engineered mice and primary human peripheral blood mononuclear cells (PBMCs) to ash from the Soufrière Hills volcano as well as representative, pure-phase samples of its primary componentry (<span class="hlt">volcanic</span> glass, feldspar, cristobalite) and measure NLRP3 inflammasome <span class="hlt">activation</span>. We demonstrate that respirable Soufrière Hills <span class="hlt">volcanic</span> ash induces the <span class="hlt">activation</span> of caspase-1 with subsequent release of mature IL-1β in a NLRP3 inflammasome-dependent manner. Macrophages deficient in NLRP3 inflammasome components are incapable of secreting IL-1β in response to <span class="hlt">volcanic</span> ash ingestion. Cellular uptake induces lysosomal destabilization involving cysteine proteases. Furthermore, the response involves <span class="hlt">activation</span> of mitochondrial stress pathways leading to the generation of reactive oxygen species. Considering ash componentry, cristobalite is the most reactive pure-phase with other components inducing only low-level IL-1β secretion. Inflammasome <span class="hlt">activation</span> mediated by inhaled ash and its potential relevance in chronic pulmonary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5786523','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5786523"><span><span class="hlt">Volcanic</span> Ash <span class="hlt">Activates</span> the NLRP3 Inflammasome in Murine and Human Macrophages</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Damby, David E.; Horwell, Claire J.; Baxter, Peter J.; Kueppers, Ulrich; Schnurr, Max; Dingwell, Donald B.; Duewell, Peter</p> <p>2018-01-01</p> <p><span class="hlt">Volcanic</span> ash is a heterogeneous mineral dust that is typically composed of a mixture of amorphous (glass) and crystalline (mineral) fragments. It commonly contains an abundance of the crystalline silica (SiO2) polymorph cristobalite. Inhalation of crystalline silica can induce inflammation by stimulating the NLRP3 inflammasome, a cytosolic receptor complex that plays a critical role in driving inflammatory immune responses. Ingested material results in the assembly of NLRP3, ASC, and caspase-1 with subsequent secretion of the interleukin-1 family cytokine IL-1β. Previous toxicology work suggests that cristobalite-bearing <span class="hlt">volcanic</span> ash is minimally reactive, calling into question the reactivity of <span class="hlt">volcanically</span> derived crystalline silica, in general. In this study, we target the NLRP3 inflammasome as a crystalline silica responsive element to clarify <span class="hlt">volcanic</span> cristobalite reactivity. We expose immortalized bone marrow-derived macrophages of genetically engineered mice and primary human peripheral blood mononuclear cells (PBMCs) to ash from the Soufrière Hills volcano as well as representative, pure-phase samples of its primary componentry (<span class="hlt">volcanic</span> glass, feldspar, cristobalite) and measure NLRP3 inflammasome <span class="hlt">activation</span>. We demonstrate that respirable Soufrière Hills <span class="hlt">volcanic</span> ash induces the <span class="hlt">activation</span> of caspase-1 with subsequent release of mature IL-1β in a NLRP3 inflammasome-dependent manner. Macrophages deficient in NLRP3 inflammasome components are incapable of secreting IL-1β in response to <span class="hlt">volcanic</span> ash ingestion. Cellular uptake induces lysosomal destabilization involving cysteine proteases. Furthermore, the response involves <span class="hlt">activation</span> of mitochondrial stress pathways leading to the generation of reactive oxygen species. Considering ash componentry, cristobalite is the most reactive pure-phase with other components inducing only low-level IL-1β secretion. Inflammasome <span class="hlt">activation</span> mediated by inhaled ash and its potential relevance in chronic pulmonary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNS21C..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNS21C..08F"><span>Identifying Alteration and Water on MT. Baker, WA with Geophysics: Implications for <span class="hlt">Volcanic</span> Landslide Hazards</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finn, C.; Deszcz-Pan, M.; Bedrosian, P.; Minsley, B. J.</p> <p>2016-12-01</p> <p>Helicopter magnetic and electromagnetic (HEM) data, along with rock property measurements, local ground-based gravity, time domain electromagnetic (TEM) and nuclear magnetic resonance (NMR) data help identify alteration and water-saturated zones on Mount Baker, Washington. <span class="hlt">Hydrothermally</span> altered rocks, particularly if water-saturated, can weaken <span class="hlt">volcanic</span> edifices, increasing the potential for catastrophic sector collapses that can lead to far traveled and destructive debris flows. At Mount Baker volcano, collapses of <span class="hlt">hydrothermally</span> altered rocks from the edifice have generated numerous debris flows that constitute their greatest <span class="hlt">volcanic</span> hazards. Critical to quantifying this hazard is knowledge of the three-dimensional distribution of pervasively altered rock, shallow groundwater and ice that plays an important role in transforming debris avalanches to far traveled lahars. The helicopter geophysical data, combined with geological mapping and rock property measurements, indicate the presence of localized zones of less than 100 m thickness of water-saturated <span class="hlt">hydrothermally</span> altered rock beneath Sherman Crater and the Dorr Fumarole Fields at Mt. Baker. New stochastic inversions of the HEM data indicate variations in resistivity in inferred perched aquifers—distinguishing between fresh and saline waters, possibly indicating the influence of nearby alteration and/or <span class="hlt">hydrothermal</span> systems on water quality. The new stochastic results better resolve ice thickness than previous inversions, and also provide important estimates of uncertainty on ice thickness and other parameters. New gravity data will help constrain the thickness of the ice and alteration. Nuclear magnetic resonance data indicate that the <span class="hlt">hydrothermal</span> clays contain 50% water with no evidence for water beneath the ice. The HEM data identify water-saturated fresh <span class="hlt">volcanic</span> rocks from the surface to the detection limit ( 100 m) over the entire summit of Mt. Baker. Localized time domain EM soundings indicate that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V53A1743F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V53A1743F"><span>Stratigraphy, <span class="hlt">Hydrothermal</span> Alteration and Evolution of the Mangakino Geothermal System, Taupo <span class="hlt">Volcanic</span> Zone, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fagan, C. J.; Wilson, C. J.; Spinks, K. D.; Browne, P. R.; Simmons, S. F.</p> <p>2006-12-01</p> <p>A major part of the ca. 1.6 Myr history of the Taupo <span class="hlt">Volcanic</span> Zone (TVZ) is represented by buried and <span class="hlt">hydrothermally</span> altered rocks penetrated by geothermal exploration wells. The geothermal field at Mangakino is sited in the oldest TVZ caldera on the western edge of the TVZ. Four exploration wells into the field reveal a thick sequence of flat-lying ignimbrites. Basement Mesozoic greywacke metasediments were not reached by the deepest well, MA2 (3192 m), implying the presence of a thick caldera infill. Ignimbrites exposed at the surface nearby have distinct mineralogies and crystal contents, which enable correlation with down-hole lithologies. Five ignimbrites are identified in the wells: the 0.32 Ma Whakamaru, 0.93 Ma Marshall, 1.0 Ma Rocky Hill, 1.18 Ma Ahuroa and 1.25 Ma Ongatiti ignimbrites, two of which are >800m thick. The Whakamaru and Marshall units are separated by a thick sequence of lacustrine and volcaniclastic deposits related to infilling of the Mangakino caldera. The ignimbrite sequence is continuous between all wells, with no fault offset, and only well MA3 intersects two rhyolite intrusions at 1190 m and 1850 m that are thought to be feeder dikes to post-0.32 Ma rhyolite domes to the east of Mangakino. Alteration assemblages include epidote and wairakite in MA2 below 2200 m. Adularia occurs in MA2 and MA3 where it replaces, wholly or in part, primary andesine. Adularia is also locally replaced by illite, indicating a shift in <span class="hlt">hydrothermal</span> conditions. Other minerals present are chlorite, quartz, calcite, titanite and pyrite. Secondary quartz and calcite veins are seen in thin section, with a first appearance in the lacustrine sediments at 550 m in both MA2 and MA3. Fluid inclusions in secondary calcite show high temperatures (300 and 315 °C) while inclusions in primary quartz show ca. 165 °C (the current temperature at the sampled depth), recording current conditions. The modern maximum temperature is 250 °C at 3000 m in MA2. Evidence for two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021065','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021065"><span>The deep structure of a sea-floor <span class="hlt">hydrothermal</span> deposit</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zierenberg, R.A.; Fouquet, Y.; Miller, D.J.; Bahr, J.M.; Baker, P.A.; Bjerkgard, T.; Brunner, C.A.; Duckworth, R.C.; Gable, R.; Gieskes, J.; Goodfellow, W.D.; Groschel-Becker, H. M.; Guerin, G.; Ishibashi, J.; Iturrino, G.; James, R.H.; Lackschewitz, K.S.; Marquez, L.L.; Nehlig, P.; Peter, J.M.; Rigsby, C.A.; Schultheiss, P.; Shanks, Wayne C.; Simoneit, B.R.T.; Summit, M.; Teagle, D.A.H.; Urbat, M.; Zuffa, G.G.</p> <p>1998-01-01</p> <p><span class="hlt">Hydrothermal</span> circulation at the crests of mid-ocean ridges plays an important role in transferring heat from the interior of the Earth. A consequence of this <span class="hlt">hydrothermal</span> circulation is the formation of metallic ore bodies known as <span class="hlt">volcanic</span>-associated massive sulphide deposits. Such deposits, preserved on land, were important sources of copper for ancient civilizations and continue to provide a significant source of base metals (for example, copper and zinc). Here we present results from Ocean Drilling Program Leg 169, which drilled through a massive sulphide deposit on the northern Juan de Fuca spreading centre and penetrated the <span class="hlt">hydrothermal</span> feeder zone through which the metal-rich fluids reached the sea floor. We found that the style of feeder-zone mineralization changes with depth in response to changes in the pore pressure of the <span class="hlt">hydrothermal</span> fluids and discovered a stratified zone of high-grade copper-rich replacement mineralization below the massive sulphide deposit. This copper-rich zone represents a type of mineralization not previously observed below sea-floor deposits, and may provide new targets for land-based mineral exploration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70187322','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70187322"><span>The <span class="hlt">volcanic</span>, sedimentologic, and paleolimnologic history of the Crater Lake caldera floor, Oregon:Evidence for small caldera evolution</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nelson, C. Hans; Bacon, Charles R.; Robinson, Stephen W.; Adam, David P.; Bradbury, J. Platt; Barber, John H.; Schwartz, Deborah; Vagenas, Ginger</p> <p>1994-01-01</p> <p>Apparent phreatic explosion craters, caldera-floor <span class="hlt">volcanic</span> cones, and geothermal features outline a ring fracture zone along which Mount Mazama collapsed to form the Crater Lake caldera during its climactic eruption about 6,850 yr B.P. Within a few years, subaerial deposits infilled the phreatic craters and then formed a thick wedge (10-20 m) of mass flow deposits shed from caldera walls. Intense <span class="hlt">volcanic</span> <span class="hlt">activity</span> (phreatic explosions, subaerial flows, and <span class="hlt">hydrothermal</span> venting) occurred during this early postcaldera stage, and a central platform of subaerial andesite flows and scoria formed on the caldera floor.Radiocarbon ages suggest that deposition of Iacustrine hemipelagic sediment began on the central platform about 150 yr after the caldera collapse. This is the minimum time to fill the lake halfway with water and cover the platform assuming present hydrologic conditions of precipitation and evaporation but with negligible leakage of lake water. Wizard Island formed during the final part of the 300-yr lake-filling period as shown by its (1) upper subaerial lava flows from 0 to -70 m below present water level and lower subaqueous lava flows from -70 to -500 m and by (2) lacustrine turbidite sand derived from Wizard Island that was deposited on the central platform about 350 yr after the caldera collapse. Pollen stratigraphy indicates that the warm and dry climate of middle Holocene time correlates with the early lake deposits. Diatom stratigraphy also suggests a more thermally stratified and phosphate-rich environment associated respectively with this climate and greater <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> during the early lake history.Apparent coarse-grained and thick-bedded turbidites of the early lake beds were deposited throughout northwest, southwest, and eastern basins during the time that <span class="hlt">volcanic</span> and seismic <span class="hlt">activity</span> formed the subaqueous Wizard Island, Merriam Cone, and rhyodacite dome. The last known postcaldera <span class="hlt">volcanic</span> <span class="hlt">activity</span> produced a subaqueous rhyodacite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAfES.129..623R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAfES.129..623R"><span>Geothermal <span class="hlt">activity</span> and <span class="hlt">hydrothermal</span> mineral deposits at southern Lake Bogoria, Kenya Rift Valley: Impact of lake level changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Renaut, Robin W.; Owen, R. Bernhart; Ego, John K.</p> <p>2017-05-01</p> <p>Lake Bogoria, a saline alkaline closed-lake in a drainage basin of Neogene <span class="hlt">volcanic</span> rocks in the central Kenya Rift, is fed partly by ∼200 hot alkaline springs located in three groups along its margins. Hot springs along the midwest shoreline (Loburu, Chemurkeu) and their travertine deposits have been studied, but little is known about the geothermal <span class="hlt">activity</span> at southern Lake Bogoria. Observations, field measurements and analyses (geochemical and mineralogical) of the spring waters and deposits, spanning three decades, show that the southern spring waters are more saline, the <span class="hlt">hydrothermal</span> alteration there is more intense, and that most hot spring deposits are siliceous. Geothermal <span class="hlt">activity</span> at southern Lake Bogoria (Ng'wasis, Koibobei, Losaramat) includes littoral boiling springs and geysers, with fumaroles at slightly higher elevations. Modern spring deposits are ephemeral sodium carbonates, opal-A crusts and silica gels. Local fossil spring deposits include diatomaceous silica-cemented conglomerates that formed subaqueously when the lake was then dilute and higher than today, and outlying calcite tufa deposits. In contrast, mineral deposits around neighbouring fumarole vents and sites of <span class="hlt">hydrothermal</span> alteration include clays (kaolinite), sulfate minerals (jarosite, alunite), and Fe-oxyhydroxides linked to rising acidic fluids. When lake level falls, the zone of acidity moves downwards and may overprint older alkaline spring deposits. In contrast, rising lake level leads to lake water dilution and vents in the lower parts of the acidic zone may become dilute alkaline springs. The new evidence at Lake Bogoria shows the potential for using the mineralogy of geothermal sediments to indicate former changes in lake level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1973Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1973Y"><span>Drilling constraints on bimodal <span class="hlt">volcanism</span> and subsequent formation of contrasted uppermost crustal compositions at the middle Okinawa Trough</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamasaki, T.; Takaya, Y.; Mukae, N.; Nagase, T.; Tindell, T.; Totsuka, S.; Uno, Y.; Yonezu, K.; Nozaki, T.; Ishibashi, J. I.; Kumagai, H.; Maeda, L.; Shipboard Scientist, C.</p> <p>2016-12-01</p> <p>The Okinawa Trough (OT) is a young and <span class="hlt">actively</span> spreading back-arc basin, extending behind the Ryukyu arc-trench system in the southeastern margin of the East China Sea. The OT is believed to be in an initial rifting stage (starting from 6-9 Ma), prior to the normal/stable seafloor spreading which constitutes the main stage of back-arc basin formation. Two drilling cruises ‒ the IODP Exp. 331 and SIP CK14-04 D/V Chikyu Cruise (Exp. 907) in 2010 and 2014 ‒ were conducted at the Iheya North Knoll, middle OT. The Iheya North Knoll is a domal <span class="hlt">volcanic</span> complex consisting of small <span class="hlt">volcanic</span> bodies. On these cruises, pumiceous gravel and altered rhyolitic rocks, as well as hemi-pelagic sediments, <span class="hlt">hydrothermal</span> clay and Kuroko-type ores, were recovered from the upper 200 m of the crust. From Feb. 11, 2016 to Mar. 17, 2016, the SIP CK16-01 (Exp. 908) D/V Chikyu cruise was conducted at Iheya North Knoll and the sediment-covered rifting center of the Iheya-Minor Ridge area, middle OT. The Iheya-Minor ridge area is also an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> field, located 25 km southeast of the Iheya North Knoll. In this area, basaltic rocks are widely distributed, and drilling has confirmed that the basaltic materials continue to 120 m below the seafloor. From an igneous petrological point of view, the <span class="hlt">volcanic</span> rocks in the Okinawa Trough are characterized by bimodal basaltic and rhyolitic compositions, with a compositional gap between SiO2 = 56-66 wt%. The origin of the rhyolitic rock has been interpreted as magmatic differentiation of basaltic magma. However, the existence of an <span class="hlt">active</span> basalt-hosted <span class="hlt">hydrothermal</span> field in the Iheya-Minor ridge area suggests the presence of hot basaltic rocks at a shallow position in the crust, and reaching recharged seawater at this depth. Furthermore, the composition of felsic rocks just after the compositional gap (SiO2 = 67 wt%) is very similar to that of the minimum melt of a granitic system, and experimental partial melt of hydrous basalt. Therefore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V21A4722T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V21A4722T"><span>Geochemical Evidence for Recent <span class="hlt">Hydrothermal</span> Alteration of Marine Sediments in Mid-Okinawa Trough, Southwest Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, A.; Abe, G.; Yamaguchi, K. E.</p> <p>2014-12-01</p> <p>Recent studies have shown that submarine <span class="hlt">hydrothermal</span> system supports diverse microbial life. Bio-essential metals supporting such microbial communities were released from basalts by high-temperature water-rock interaction in deeper part of the oceanic crust and carried by submarine fluid flow. Its total quantity in global <span class="hlt">hydrothermal</span> settings has been estimated to be on the order of ~1019 g/yr, which is surprisingly on the same order of the total river flows (Urabe et al., 2011). Therefore, it is important to explore how submarine river system works, i.e., to understand mechanism and extent of elemental transport, which should lead to understanding of the roles of <span class="hlt">hydrothermal</span> circulation in oceanic crust in controlling elemental budget in the global ocean and geochemical conditions to support deep hot biosphere.  We performed REE analysis of marine sediments influenced by submarine <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in Mid-Okinawa Trough. The sediment samples used in this study are from IODP site at Iheya North region and JADE site at Izena region. The samples show alternation between <span class="hlt">volcanic</span> and clastic sediments. <span class="hlt">Hydrothermal</span> fluids of this area contain elevated concentrations of volatile components such as H2, CO2, CH4, NH4+, and H2S, supporting diverse chemoautotrophic microbial community (Nakagawa et al., 2005). The purpose of this study is to examine the effect of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> on the REE signature of the sediments. Chondrite-normalized REE patterns of the samples show relative enrichment of light over heavy REEs, weak positive Ce anomalies, and variable degrees of negative Eu anomalies. The REE patterns suggest the sediments source was mainly basalt, suggesting insignificant input of continental materials. Negative Eu anomalies found in the IODP site become more pronounced with increasing depth, suggesting progressive increase of <span class="hlt">hydrothermal</span> alteration where Eu was reductively dissolved into fluids by decomposition of feldspars. Contrary, at the JADE site</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5867533','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5867533"><span>A <span class="hlt">Hydrothermal</span>-Sedimentary Context for the Origin of Life</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hickman-Lewis, K.; Hinman, N.; Gautret, P.; Campbell, K.A.; Bréhéret, J.G.; Foucher, F.; Hubert, A.; Sorieul, S.; Dass, A.V.; Kee, T.P.; Georgelin, T.; Brack, A.</p> <p>2018-01-01</p> <p>Abstract Critical to the origin of life are the ingredients of life, of course, but also the physical and chemical conditions in which prebiotic chemical reactions can take place. These factors place constraints on the types of Hadean environment in which life could have emerged. Many locations, ranging from <span class="hlt">hydrothermal</span> vents and pumice rafts, through <span class="hlt">volcanic</span>-hosted splash pools to continental springs and rivers, have been proposed for the emergence of life on Earth, each with respective advantages and certain disadvantages. However, there is another, hitherto unrecognized environment that, on the Hadean Earth (4.5–4.0 Ga), would have been more important than any other in terms of spatial and temporal scale: the sedimentary layer between oceanic crust and seawater. Using as an example sediments from the 3.5–3.33 Ga Barberton Greenstone Belt, South Africa, analogous at least on a local scale to those of the Hadean eon, we document constant permeation of the porous, carbonaceous, and reactive sedimentary layer by <span class="hlt">hydrothermal</span> fluids emanating from the crust. This partially UV-protected, subaqueous sedimentary environment, characterized by physical and chemical gradients, represented a widespread system of miniature chemical reactors in which the production and complexification of prebiotic molecules could have led to the origin of life. Key Words: Origin of life—Hadean environment—Mineral surface reactions—<span class="hlt">Hydrothermal</span> fluids—Archean <span class="hlt">volcanic</span> sediments. Astrobiology 18, 259–293. PMID:29489386</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2006/3139/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2006/3139/"><span>U.S. Geological Survey's Alert Notification System for <span class="hlt">Volcanic</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gardner, Cynthia A.; Guffanti, Marianne C.</p> <p>2006-01-01</p> <p>The United States and its territories have about 170 volcanoes that have been <span class="hlt">active</span> during the past 10,000 years, and most could erupt again in the future. In the past 500 years, 80 U.S. volcanoes have erupted one or more times. About 50 of these recently <span class="hlt">active</span> volcanoes are monitored, although not all to the same degree. Through its five volcano observatories, the U.S. Geological Survey (USGS) issues information and warnings to the public about <span class="hlt">volcanic</span> <span class="hlt">activity</span>. For clarity of warnings during <span class="hlt">volcanic</span> crises, the USGS has now standardized the alert-notification system used at its observatories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S33D2461J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S33D2461J"><span>Micro-seismic earthquakes characteristics at natural and exploited <span class="hlt">hydrothermal</span> systems in West Java, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jousset, P. G.; Jaya, M. S.; Sule, R.; Diningrat, W.; Gassner, A.; Akbar, F.; Ryannugroho, R.; Hendryana, A.; Kusnadi, Y.; Syahbana, D.; Nugraha, A. D.; Umar, M.; Indrinanto, Y.; Erbas, K.</p> <p>2013-12-01</p> <p>The assessment of geothermal resources requires the understanding of the structure and the dynamics of geothermal reservoirs. We deployed a multidisciplinary geophysical network around geothermal areas in the south of Bandung, West Java, Indonesia. The first deployment included a network of 30 broadband and 4 short-period seismic stations with Güralp and Trillium sensors (0.008 - 100 Hz) since October 2012. In a second step, we extended the network in June 2013 with 16 short-period (1 Hz) seismometers. We describe the set-up of the seismic networks and discuss first observations and results. The co-existence of a large variety of intense surface manifestations like geysers, hot-steaming grounds, hot water pools, and <span class="hlt">active</span> volcanoes suggest an intimate coupling between <span class="hlt">volcanic</span>, tectonic and <span class="hlt">hydrothermal</span> processes in this area. Preliminary location of earthquakes is performed using a <span class="hlt">non</span>-linear algorithm, which allows us to define at least 3 seismic clusters. We discuss this seismic pattern within the geothermal fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GGG....13.9006L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GGG....13.9006L"><span>Tectonic and magmatic controls on <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in the Woodlark Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Laurila, T. E.; Petersen, S.; Devey, C. W.; Baker, E. T.; Augustin, N.; Hannington, M. D.</p> <p>2012-09-01</p> <p>The Woodlark Basin is one of the rare places on earth where the transition from continental breakup to seafloor spreading can be observed. The potential juxtaposition of continental rocks, a large magmatic heat source, crustal-scale faulting, and <span class="hlt">hydrothermal</span> circulation has made the Woodlark Basin a prime target for seafloor mineral exploration. However, over the past 20 years, only two locations of <span class="hlt">active</span> <span class="hlt">hydrothermalism</span> had been found. In 2009 we surveyed 435 km of the spreading axis for the presence of <span class="hlt">hydrothermal</span> plumes. Only one additional plume was found, bringing the total number of plumes known over 520 km of ridge axis to only 3, much less than at ridges with similar spreading rates globally. Particularly the western half of the basin (280 km of axis) is apparently devoid of high temperature plumes despite having thick crust and a presumably high magmatic budget. This paucity of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> may be related to the peculiar tectonic setting at Woodlark, where repeated ridge jumps and a re-location of the rotation pole both lead to axial magmatism being more widely distributed than at many other, more mature and stable mid-ocean ridges. These factors could inhibit the development of both a stable magmatic heat source and the deeply penetrating faults needed to create long-lived <span class="hlt">hydrothermal</span> systems. We conclude that large seafloor massive sulfide deposits, potential targets for seafloor mineral exploration, will probably not be present along the spreading axis of the Woodlark Basin, especially in its younger, western portion.</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://adsabs.harvard.edu/abs/2017AGUFM.V11A0339F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V11A0339F"><span>An Overview of Thermal Measurements (IR) at the Summit of Piton de la Fournaise <span class="hlt">Active</span> Volcano and Inferences on the Structure and Dynamics of its <span class="hlt">Hydrothermal</span> System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fontaine, F.; Peltier, A.; Kowalski, P.; Di Muro, A.; Villeneuve, N.; Ferrazzini, V.; Staudacher, T.</p> <p>2017-12-01</p> <p>Piton de la Fournaise, located on La Réunion Island in the South East Indian Ocean, is one of the most <span class="hlt">active</span> basaltic volcanoes (hotspot) of the world with a mean eruption frequency <6 months over the last 20 years. The central dome of the shield is thought to host an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system evidenced by self-potential techniques early in the 90's and mining heat from a magmatic source located about 2-2.5 km below the summit. Surface manifestations of this <span class="hlt">activity</span> such as fumeroles or hot grounds have however never been observed before 2007 when deep magma withdrawal from the magmatic horizon during the "eruption of the century" (>100×106 m3) on the island, led to the formation of a 400-m-deep, 1000-m-large, funnel-shaped summit caldera. Since then, the floor and inner flanks of this summit depression hosting hot grounds and <span class="hlt">active</span> fumaroles, are monitored using an infra-red camera device permanently installed on the caldera rim.This thermal dataset constitutes the first opportunity to understand the structure and dynamics of the <span class="hlt">hydrothermal</span> system and its ability to relay deep-seated heat and mass perturbations. We present in this communication an overview of this thermal datasets focusing on ground/fumaroles temperature evolution during <span class="hlt">volcanic</span> crisis and rest periods and analyzing correlations with the other permanently acquired data such as the temporal evolution of gas geochemistry (CO2, SO2, H2S), ground deformation and micro-seismic <span class="hlt">activity</span>. We finally propose a conceptual model of fluid flow architecture within the edifice which paves the way for future quantitative models of <span class="hlt">hydrothermal</span> heat and mass transfers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMOS21A1485H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMOS21A1485H"><span>Discovery Of An Extensive <span class="hlt">Hydrothermal</span> Sulfide/Sulfate Mounds Field In East Diamante Caldera, Mariana <span class="hlt">Volcanic</span> Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hein, J. R.; de Ronde, C. E.; Ditchburn, R.; Leybourne, M. I.; Tamura, Y.; Stern, R. J.; Conrad, T. A.; Nichols, A. R.; Shukuno, H.; Embley, R. W.; Bloomer, S. H.; Ishizuka, O.; Hirahara, Y.; Senda, R.; Nunokawa, A.; Jordan, E.; Wada, I.</p> <p>2010-12-01</p> <p>An elongate field of <span class="hlt">hydrothermal</span> mounds was discovered along the NE flank of a cluster of resurgent dacite domes in East Diamante Caldera using the ROV Hyper-Dolphin aboard the R.V. Natsushima in June 2009 and July 2010. East Diamante seamount lies about 80 km north of Saipan and is the northernmost volcano of the Southern Seamount Province of the Mariana magmatic arc. East Diamante is an irregular caldera about 10 km x 4 km that is breached on the north and south sides. The caldera floor has a maximum water depth of about 700 m. After caldera collapse, dacitic domes intruded into the center of the caldera providing the heat source for production and circulation of <span class="hlt">hydrothermal</span> fluids that generated the large mounds field and two nearby chimney fields, one <span class="hlt">active</span> and one inactive, found in 2004 during a NOAA Ring-of-Fire cruise. The mounds field is more than 100 m long and about 25-30 m wide and occurs along a NE-SW rift valley at water depths of about 365-400 m b.s.l. Individual <span class="hlt">hydrothermal</span> mounds and ridges along this trend vary in size and the bases of the mounds are buried beneath <span class="hlt">hydrothermal</span> sediment so that only minimum dimensions can be determined. Mounds are typically 1-3 m tall and 0.5-2 m wide, with lengths of about 3 to more than 5 m. The sulfide/sulfate mounds are layered and an iron- and manganese-oxide subsidiary mound venting low-temperature fluids caps some of them. Some mounds also support inactive sulfide/sulfate chimneys and spires; chimneys rarely occur as independent structures within the mounds field. The mounds are composed primarily of barite layers and sphalerite (high cadmium, low iron) plus galena layers with up to 470 ppm silver and 3 ppm gold. The subsidiary mounds are composed of 7A manganate and goethite that occur around a delicate network of 2-10 mm diameter anastomosing channels. Similar oxides cover the seabed throughout the mounds field and precipitated from diffuse fluid flow throughout the region, but formed by both diffuse</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA00703.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA00703.html"><span><span class="hlt">Active</span> <span class="hlt">Volcanic</span> Plumes on Io</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1998-03-26</p> <p>This color image, acquired during NASA Galileo ninth orbit around Jupiter, shows two <span class="hlt">volcanic</span> plumes on Io. One plume was captured on the bright limb or edge of the moon, erupting over a caldera <span class="hlt">volcanic</span> depression named Pillan Patera.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5627351-hydrothermal-activity-lau-back-arc-basin-sulfides-water-chemistry','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5627351-hydrothermal-activity-lau-back-arc-basin-sulfides-water-chemistry"><span><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> in the Lau back-arc basin: Sulfides and water chemistry</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>Fouquet, Y.; Charlou, J.L.; Donval, J.P.</p> <p>1991-04-01</p> <p>The submersible Nautile completed 22 dives during the Nautilau cruise (R/V Nadir, April 17-May 10, 1989) for a detailed investigation of the southern Lau basin near Tonga. The objective of the scientific team from France, Germany, and Tonga was to understand the process of sea-floor ore formation associated with <span class="hlt">hydrothermal</span> circulation along the Valu Fa back-arc ridge behind the Tonga-Kermadec trench. The four diving areas, between lat21{degree}25'S and 22{degree}40'S in water{approximately}2000 m deep, were selected on the basis of results from cruises of the R/V Jean Charcot and R/V Sonne. The Nadir cruise provided proof of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>-in all formore » areas, over more than 100 km-as indicated by the widespread occurence of <span class="hlt">hydrothermal</span> deposits and by heat flow, conductivity, and temperature measurements near the sea bottom. The most spectacular findings were high-temperature white and black smokers and associated fauna and ore deposits. <span class="hlt">Hydrothermal</span> water chemistry and sulfide composition data presented here indicate that this <span class="hlt">hydrothermal</span> field is very different from the <span class="hlt">hydrothermal</span> fields in oceanic ridges. This difference is seen in water chemistry of the <span class="hlt">hydrothermal</span> fluid (pH=2 and high metal content) and the chemical composition of sulfides (enrichment in Ba, As, and Pb).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS13A1707T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS13A1707T"><span>ESR dating of submarine <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> using barite in sulfide deposition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toyoda, S.; Fujiwara, T.; Ishibashi, J.; Isono, Y.; Uchida, A.; Takamasa, A.; Nakai, S.</p> <p>2012-12-01</p> <p>The temporal change of submarine <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> has been an important issue in the aspect of the evolution of <span class="hlt">hydrothermal</span> systems which is related with ore formation (Urabe, 1995) and biological systems sustained by the chemical species arising from <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> (Macdonald et al., 1980). Determining the ages of the <span class="hlt">hydrothermal</span> deposit will provide essential information on such studies. Dating methods using disequilibrium between radioisotopes such as U-Th method (e.g. You and Bickle, 1998), 226}Ra-{210Pb and 228}Ra-{228Th method (e.g. Noguchi et al., 2011) have been applied to date submarine <span class="hlt">hydrothermal</span> deposits. ESR (electron spin resonance) dating method is commonly applied to fossil teeth, shells, and quartz of Quaternay period where the natural accumulated dose is obtained from the intensities of the ESR signals which are created by natural radiation. The natural dose is divided by the dose rate to the mineral/sample to deduce the age. Okumura et al., (2010) made the first practical application of ESR (electron spin resonance) dating technique to a sample of submarine <span class="hlt">hydrothermal</span> barite (BaSO4) to obtain preliminary ages, where Kasuya et al. (1991) first pointed out that barite can be used for ESR dating. Knowing that ESR dating of barite is promising, in this paper, we will present how we have investigated each factor that contributes ESR dating of barite in submarine <span class="hlt">hydrothermal</span> sulfide deposition. (1) The best ESR condition for measuring the SO3- signal in barite is with the microwave power of 1mW and modulation amplitude of 0.1mT. (2) As results of heating experiments, the signal was found to be stable for the dating age range of several thousands. (3) 226Ra replacing Ba in barite is the source of the radiation. The amount of radioactive elements in sulfide mineral surrounding barite is negligible. (4) The external radiation from the sea water is negligible even in the submarine <span class="hlt">hydrothermal</span> area where the radiation level is much</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5904459','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5904459"><span>Metaproteogenomic Profiling of Microbial Communities Colonizing <span class="hlt">Actively</span> Venting <span class="hlt">Hydrothermal</span> Chimneys</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Pjevac, Petra; Meier, Dimitri V.; Markert, Stephanie; Hentschker, Christian; Schweder, Thomas; Becher, Dörte; Gruber-Vodicka, Harald R.; Richter, Michael; Bach, Wolfgang; Amann, Rudolf; Meyerdierks, Anke</p> <p>2018-01-01</p> <p>At <span class="hlt">hydrothermal</span> vent sites, chimneys consisting of sulfides, sulfates, and oxides are formed upon contact of reduced <span class="hlt">hydrothermal</span> fluids with oxygenated seawater. The walls and surfaces of these chimneys are an important habitat for vent-associated microorganisms. We used community proteogenomics to investigate and compare the composition, metabolic potential and relative in situ protein abundance of microbial communities colonizing two <span class="hlt">actively</span> venting <span class="hlt">hydrothermal</span> chimneys from the Manus Basin back-arc spreading center (Papua New Guinea). We identified overlaps in the in situ functional profiles of both chimneys, despite differences in microbial community composition and venting regime. Carbon fixation on both chimneys seems to have been primarily mediated through the reverse tricarboxylic acid cycle and fueled by sulfur-oxidation, while the abundant metabolic potential for hydrogen oxidation and carbon fixation via the Calvin–Benson–Bassham cycle was hardly utilized. Notably, the highly diverse microbial community colonizing the analyzed black smoker chimney had a highly redundant metabolic potential. In contrast, the considerably less diverse community colonizing the diffusely venting chimney displayed a higher metabolic versatility. An increased diversity on the phylogenetic level is thus not directly linked to an increased metabolic diversity in microbial communities that colonize <span class="hlt">hydrothermal</span> chimneys. PMID:29696004</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Natur.519..207H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Natur.519..207H"><span>Ongoing <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> within Enceladus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hsu, Hsiang-Wen; Postberg, Frank; Sekine, Yasuhito; Shibuya, Takazo; Kempf, Sascha; Horányi, Mihály; Juhász, Antal; Altobelli, Nicolas; Suzuki, Katsuhiko; Masaki, Yuka; Kuwatani, Tatsu; Tachibana, Shogo; Sirono, Sin-Iti; Moragas-Klostermeyer, Georg; Srama, Ralf</p> <p>2015-03-01</p> <p>Detection of sodium-salt-rich ice grains emitted from the plume of the Saturnian moon Enceladus suggests that the grains formed as frozen droplets from a liquid water reservoir that is, or has been, in contact with rock. Gravitational field measurements suggest a regional south polar subsurface ocean of about 10 kilometres thickness located beneath an ice crust 30 to 40 kilometres thick. These findings imply rock-water interactions in regions surrounding the core of Enceladus. The resulting chemical `footprints' are expected to be preserved in the liquid and subsequently transported upwards to the near-surface plume sources, where they eventually would be ejected and could be measured by a spacecraft. Here we report an analysis of silicon-rich, nanometre-sized dust particles (so-called stream particles) that stand out from the water-ice-dominated objects characteristic of Saturn. We interpret these grains as nanometre-sized SiO2 (silica) particles, initially embedded in icy grains emitted from Enceladus' subsurface waters and released by sputter erosion in Saturn's E ring. The composition and the limited size range (2 to 8 nanometres in radius) of stream particles indicate ongoing high-temperature (>90 °C) <span class="hlt">hydrothermal</span> reactions associated with global-scale geothermal <span class="hlt">activity</span> that quickly transports <span class="hlt">hydrothermal</span> products from the ocean floor at a depth of at least 40 kilometres up to the plume of Enceladus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.U33C..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.U33C..05S"><span>Hazards in <span class="hlt">volcanic</span> arcs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sparks, S. R.</p> <p>2008-12-01</p> <p><span class="hlt">Volcanic</span> eruptions in arcs are complex natural phenomena, involving the movement of magma to the Earth's surface and interactions with the surrounding crust during ascent and with the surface environment during eruption, resulting in secondary hazards. Magma changes its properties profoundly during ascent and eruption and many of the underlying processes of heat and mass transfer and physical property changes that govern <span class="hlt">volcanic</span> flows and magmatic interactions with the environment are highly <span class="hlt">non</span>-linear. Major direct hazards include tephra fall, pyroclastic flows from explosions and dome collapse, <span class="hlt">volcanic</span> blasts, lahars, debris avalanches and tsunamis. There are also health hazards related to emissions of gases and very fine <span class="hlt">volcanic</span> ash. These hazards and progress in their assessment are illustrated mainly from the ongoing eruption of the Soufriere Hills volcano. Montserrat. There are both epistemic and aleatory uncertainties in the assessment of <span class="hlt">volcanic</span> hazards, which can be large, making precise prediction a formidable objective. Indeed in certain respects <span class="hlt">volcanic</span> systems and hazardous phenomena may be intrinsically unpredictable. As with other natural phenomena, predictions and hazards inevitably have to be expressed in probabilistic terms that take account of these uncertainties. Despite these limitations significant progress is being made in the ability to anticipate <span class="hlt">volcanic</span> <span class="hlt">activity</span> in <span class="hlt">volcanic</span> arcs and, in favourable circumstances, make robust hazards assessments and predictions. Improvements in monitoring ground deformation, gas emissions and seismicity are being combined with more advanced models of <span class="hlt">volcanic</span> flows and their interactions with the environment. In addition more structured and systematic methods for assessing hazards and risk are emerging that allow impartial advice to be given to authorities during <span class="hlt">volcanic</span> crises. There remain significant issues of how scientific advice and associated uncertainties are communicated to provide effective</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.2255F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.2255F"><span>Multidimensional analysis and probabilistic model of <span class="hlt">volcanic</span> and seismic <span class="hlt">activities</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fedorov, V.</p> <p>2009-04-01</p> <p>A search for space and time regularities in <span class="hlt">volcanic</span> and seismic events for the purpose of forecast method development seems to be of current concern, both scientifically and practically. The seismic and <span class="hlt">volcanic</span> processes take place in the Earth's field of gravity which in turn is closely related to gravitational fields of the Moon, the Sun, and the planets of the Solar System. It is mostly gravity and tidal forces that exercise control over the Earth's configuration and relief. Dynamic gravitational interaction between the Earth and other celestial bodies makes itself evident in tidal phenomena and other effects in the geospheres (including the Earth's crust). Dynamics of the tidal and attractive forces is responsible for periodical changes in gravity force, both in value and direction [Darwin, 1965], in the rate of rotation and orbital speed; that implies related changes in the endogenic <span class="hlt">activity</span> of the Earth. The Earth's rotation in the alternating gravitational field accounts to a considerable extent for regular pattern of crustal deformations and dislocations; it is among principal factors that control the Earth's form and structure, distribution of oceans and continents and, probably, continental drift [Peive, 1969; Khain, 1973; Kosygin, 1983]. The energy of gravitational interaction is transmitted through the tidal energy to planetary spheres and feeds various processes there, including <span class="hlt">volcanic</span> and seismic ones. To determine degree, character and special features of tidal force contribution to the <span class="hlt">volcanic</span> and seismic processes is of primary importance for understanding of genetic and dynamic aspects of <span class="hlt">volcanism</span> and seismicity. Both <span class="hlt">volcanic</span> and seismic processes are involved in evolution of celestial bodies; they are operative on the planets of the Earth group and many satellites [Essays…, 1981; Lukashov, 1996]. From this standpoint, studies of those processes are essential with a view to development of scenarios of the Earth's evolution as a celestial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1410054A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1410054A"><span>The Lanzarote Geodynamic Laboratory: new capabilities for monitoring of <span class="hlt">volcanic</span> <span class="hlt">activity</span> at Canary Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arnoso, J.; Vélez, E. J.; Soler, V.; Montesinos, F. G.; Benavent, M.</p> <p>2012-04-01</p> <p>The <span class="hlt">volcanic</span> island of Lanzarote is located at the northeastern end of the Canary Islands. Together with Fuerteventura Island, Lanzarote constitutes the emergent part of the East Canary Ridge, which presents a NNE-SSW <span class="hlt">volcanic</span> alignment. Last eruptive events took place in 1824 and during the period 1730-1736, which is the largest to occur in the archipelago and throw out about 1.3 km3 of <span class="hlt">volcanic</span> materials. The Lanzarote Geodynamic Laboratory (LGL) was created in 1986 with the idea of making Lanzarote as a natural laboratory to carry out studies in order to acquire more knowledge about its origin, present status and evolution (Vieira et al., 1991; 2006). The LGL has a multidisciplinary scientific purpose and, among others, various objectives are devoted to investigate mass distribution in the Earth system and surface displacements associated to <span class="hlt">volcanic</span> and/or seismic <span class="hlt">activity</span> in the island. The influence of LGL is extended throughout the whole geographical area of Lanzarote, including small islands located at the north. The laboratory has 3 observing modules distributed along the island according to its infrastructure and scientific objectives, where more than 70 sensors are recording continuously gravity variations, ground deformations, sea level, seismic <span class="hlt">activity</span>, meteorological parameters, etc. All these observations are supplemented by periodic measurement of geodetic and geophysical networks that allow us to make studies at local, insular and regional scales. The application of geodetic and geophysical techniques to identify geodynamic signals related to <span class="hlt">volcanic</span> processes is then a permanent research <span class="hlt">activity</span> of the laboratory. Nowadays, this fact becomes more interesting due to the ongoing <span class="hlt">volcanic</span> eruption that is taking place in other island of the Canary Archipelago, El Hierro, since past July 2011. That is, the multidisciplinary research carry on up to now at the LGL allow us to apply multiparameter observations of different kinds of <span class="hlt">volcanic</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoJI.205..562B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoJI.205..562B"><span>3-D linear inversion of gravity data: method and application to Basse-Terre <span class="hlt">volcanic</span> island, Guadeloupe, Lesser Antilles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barnoud, Anne; Coutant, Olivier; Bouligand, Claire; Gunawan, Hendra; Deroussi, Sébastien</p> <p>2016-04-01</p> <p>We use a Bayesian formalism combined with a grid node discretization for the linear inversion of gravimetric data in terms of 3-D density distribution. The forward modelling and the inversion method are derived from seismological inversion techniques in order to facilitate joint inversion or interpretation of density and seismic velocity models. The Bayesian formulation introduces covariance matrices on model parameters to regularize the ill-posed problem and reduce the <span class="hlt">non</span>-uniqueness of the solution. This formalism favours smooth solutions and allows us to specify a spatial correlation length and to perform inversions at multiple scales. We also extract resolution parameters from the resolution matrix to discuss how well our density models are resolved. This method is applied to the inversion of data from the <span class="hlt">volcanic</span> island of Basse-Terre in Guadeloupe, Lesser Antilles. A series of synthetic tests are performed to investigate advantages and limitations of the methodology in this context. This study results in the first 3-D density models of the island of Basse-Terre for which we identify: (i) a southward decrease of densities parallel to the migration of <span class="hlt">volcanic</span> <span class="hlt">activity</span> within the island, (ii) three dense anomalies beneath Petite Plaine Valley, Beaugendre Valley and the Grande-Découverte-Carmichaël-Soufrière Complex that may reflect the trace of former major <span class="hlt">volcanic</span> feeding systems, (iii) shallow low-density anomalies in the southern part of Basse-Terre, especially around La Soufrière <span class="hlt">active</span> volcano, Piton de Bouillante edifice and along the western coast, reflecting the presence of <span class="hlt">hydrothermal</span> systems and fractured and altered rocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFMNS34A..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFMNS34A..05F"><span>Airborne Magnetic and Electromagnetic Data map Rock Alteration and Water Content at Mount Adams, Mount Baker and Mount Rainier, Washington: Implications for Lahar Hazards and <span class="hlt">Hydrothermal</span> Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finn, C. A.; Deszcz-Pan, M.; Horton, R.; Breit, G.; John, D.</p> <p>2007-12-01</p> <p>High resolution helicopter-borne magnetic and electromagnetic (EM) data flown over the rugged, ice-covered, highly magnetic and mostly resistive volcanoes of Mount Rainier, Mount Adams and Mount Baker, along with rock property measurements, reveal the distribution of alteration, water and <span class="hlt">hydrothermal</span> fluids that are essential to evaluating <span class="hlt">volcanic</span> landslide hazards and understanding <span class="hlt">hydrothermal</span> systems. <span class="hlt">Hydrothermally</span> altered rocks, particularly if water saturated, can weaken stratovolcanoes, thereby increasing the potential for catastrophic sector collapses that can lead to far-traveled, destructive debris flows. Intense <span class="hlt">hydrothermal</span> alteration significantly reduces the magnetization and resistivity of <span class="hlt">volcanic</span> rock resulting in clear recognition of altered rock by helicopter magnetic and EM measurements. Magnetic and EM data, combined with geological mapping and rock property measurements, indicate the presence of appreciable thicknesses of <span class="hlt">hydrothermally</span> altered rock west of the modern summit of Mount Rainier in the Sunset Amphitheater region, in the central core of Mount Adams north of the summit, and in much of the central cone of Mount Baker. We identify the Sunset Amphitheater region and steep cliffs at the western edge of the central altered zone at Mount Adams as likely sources for future debris flows. In addition, the EM data identified water-saturated rocks in the upper 100-200 m of the three volcanoes. The water-saturated zone could extend deeper, but is beyond the detection limits of the EM data. Water in <span class="hlt">hydrothermal</span> fluids reacts with the <span class="hlt">volcanic</span> rock to produce clay minerals. The formation of clay minerals and presence of free water reduces the effective stress, thereby increasing the potential for slope failure, and acts, with entrained melting ice, as a lubricant to transform debris avalanches into lahars. Therefore, knowing the distribution of water is also important for hazard assessments. Finally, modeling requires extremely low</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS41B..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS41B..02C"><span>Seismic Reflection Imaging of the Heat Source of an Ultramafic-Hosted <span class="hlt">Hydrothermal</span> System (Rainbow, Mid-Atlantic Ridge 36° 10-17'N)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Canales, J. P.; Dunn, R. A.; Sohn, R. A.; Horning, G.; Arai, R.; Paulatto, M.</p> <p>2015-12-01</p> <p>Most of our understanding of <span class="hlt">hydrothermal</span> systems and the nature of their heat sources comes from models and observations at fast and intermediate spreading ridges. In these settings, <span class="hlt">hydrothermal</span> systems are mainly located within the axial zone of a spreading segment, hosted in basaltic rock, and primarily driven by heat extracted from crystallization of crustal melt sills. In contrast, <span class="hlt">hydrothermal</span> systems at slow-spreading ridges like the Mid-Atlantic Ridge (MAR) show a great variety of venting styles and host-rock lithology, and are located in diverse tectonic settings like axial <span class="hlt">volcanic</span> ridges, <span class="hlt">non</span>-transform discontinuities (NTDs), the foot of ridge valley walls, and off-axis inside corner highs. Among MAR systems, the Rainbow <span class="hlt">hydrothermal</span> field (RHF) stands out as an end-member of this diversity: an ultramafic-hosted system emitting H2 and CH4-rich fluids at high temperatures and high flow rates, which suggests a magmatic heat source despite the lack of evidence for recent <span class="hlt">volcanism</span> and its location within an NTD with presumably low magma budget. We present 2D multichannel seismic reflection images across the Rainbow massif from the NSF-funded MARINER multidisciplinary geophysical study that reveal, for the first time, the magmatic system driving <span class="hlt">hydrothermal</span> circulation in an ultramafic setting. Data were acquired in 2013 onboard the RV M. Langseth with an 8-km-long hydrophone streamer. The images have been obtained from pre-stack depth migrations using a regional 3D P-wave velocity model from a coincident controlled-source seismic tomography experiment using ocean bottom seismometers. Our images show a complex magmatic system centered beneath the RHF occupying an areal extent of ~3.7x6 km2, with partially molten sills ranging in depth between ~3.4 km and ~6.9 km below the seafloor. Our data also image high-amplitude dipping reflections within the massif coincident with strong lateral velocity gradients that may arise from detachment fault planes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025918','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025918"><span>The Tuscarora Au-Ag district: Eocene <span class="hlt">volcanic</span>-hosted epithermal deposits in the Carlin gold region, Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Castor, S.B.; Boden, D.R.; Henry, C.D.; Cline, J.S.; Hofstra, A.H.; McIntosh, W.C.; Tosdal, R.M.; Wooden, J.P.</p> <p>2003-01-01</p> <p>The Tuscarora mining district contains the oldest and the only productive Eocene epithermal deposits in Nevada. The district is a particularly clear example of association of low-sulfidation deposits with igneous <span class="hlt">activity</span> and structure, and it is unusual in that it consists of two adjoining but physically and chemically distinct types of low-sulfidation deposits. Moreover, Tuscarora deposits are of interest because they formed contemporaneously with nearby, giant Carlin-type gold deposits. The Tuscarora deposits formed within the 39.9 to 39.3 Ma Tuscarora <span class="hlt">volcanic</span> field, along and just outside the southeastern margin of the caldera-like Mount Blitzen <span class="hlt">volcanic</span> center. Both deposit types formed at 39.3 Ma, contemporaneous with the only major intrusive <span class="hlt">activity</span> in the <span class="hlt">volcanic</span> field. No deposits are known to have formed during any of the intense <span class="hlt">volcanic</span> phases of the field. Intrusions were the apparent heat source, and structures related to the Mount Blitzen center were conduits for <span class="hlt">hydrothermal</span> circulation. The ore-forming fluids interacted dominantly with Eocene igneous rocks. The two deposit types occur in a northern silver-rich zone that is characterized by relatively high Ag/Au ratios (110-150), narrow alteration zones, and quartz and carbonate veins developed mostly in intrusive dacite, and in a southern gold-rich zone that is typified by relatively low Ag/Au ratios (4-14), more widespread alteration, and quartz-fissure and stockwork veins commonly developed in tuffaceous sedimentary rocks. The deposit types have similar fluid inclusion and Pb and S isotope characteristics but different geochemical signatures. Quartz veins from both zones have similar thermal and paragenetic histories and contain fluid inclusions that indicate that fluids cooled from between 260?? and 230??C to less than 200??C. Fluid boiling may have contributed to precious-metal deposition. Veins in both zones have relatively high As and Sb and low Bi, Te, and W. The silver zone has high Ca</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29035519','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29035519"><span><span class="hlt">Hydrothermally</span> <span class="hlt">Activated</span> Graphene Fiber Fabrics for Textile Electrodes of Supercapacitors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Zheng; Huang, Tieqi; Gao, Weiwei; Xu, Zhen; Chang, Dan; Zhang, Chunxiao; Gao, Chao</p> <p>2017-11-28</p> <p>Carbon textiles are promising electrode materials for wearable energy storage devices owing to their conductive, flexible, and lightweight features. However, there still lacks a perfect choice for high-performance carbon textile electrodes with sufficient electrochemical <span class="hlt">activity</span>. Graphene fiber fabrics (GFFs) are newly discovered carbon textiles, exhibiting various attractive properties, especially a large variability on the microstructure. Here we report the fabrication of hierarchical GFFs with significantly enlarged specific surface area using a <span class="hlt">hydrothermal</span> <span class="hlt">activation</span> strategy. By carefully optimize the <span class="hlt">activation</span> process, the <span class="hlt">hydrothermally</span> <span class="hlt">activated</span> graphene fiber fabrics (HAGFFs) could achieve an areal capacitance of 1060 mF cm -2 in a very thin thickness (150 μm) and the capacitance is easily magnified by overlaying several layers of HAGFFs, even up to a record value of 7398 mF cm -2 . Meanwhile, a good rate capability and a long cycle life are also attained. As compared with other carbon textiles, including the commercial carbon fiber cloths, our HAGFFs present much better capacitive performance. Therefore, the mechanically stable, flexible, conductive, and highly <span class="hlt">active</span> HAGFFs have provided an option for high-performance textile electrodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.B12A..08O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.B12A..08O"><span>Alteration of submarine <span class="hlt">volcanic</span> rocks in oxygenated Archean oceans</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohmoto, H.; Bevacqua, D.; Watanabe, Y.</p> <p>2009-12-01</p> <p>Most submarine <span class="hlt">volcanic</span> rocks, including basalts in diverging plate boundaries and andesites/dacites in converging plate boundaries, have been altered by low-temperature seawater and/or <span class="hlt">hydrothermal</span> fluids (up to ~400°C) under deep oceans; the <span class="hlt">hydrothermal</span> fluids evolved from shallow/deep circulations of seawater through the underlying hot igneous rocks. Volcanogenic massive sulfide deposits (VMSDs) and banded iron formations (BIFs) were formed by mixing of submarine <span class="hlt">hydrothermal</span> fluids with local seawater. Therefore, the behaviors of various elements, especially of redox-sensitive elements, in altered submarine <span class="hlt">volcanic</span> rocks, VMSDs and BIFs can be used to decipher the chemical evolution of the oceans and atmosphere. We have investigated the mineralogy and geochemistry of >500 samples of basalts from a 260m-long drill core section of Hole #1 of the Archean Biosphere Drilling Project (ABDP #1) in the Pilbara Craton, Western Australia. The core section is comprised of ~160 m thick Marble Bar Chert/Jasper Unit (3.46 Ga) and underlying, inter-bedded, and overlying submarine basalts. Losses/gains of 65 elements were quantitatively evaluated on the basis of their concentration ratios against the least mobile elements (Ti, Zr and Nb). We have recognized that mineralogical and geochemical characteristics of many of these samples are essentially the same as those of <span class="hlt">hydrothermally</span>-altered modern submarine basalts and also those of altered <span class="hlt">volcanic</span> rocks that underlie Phanerozoic VMSDs. The similarities include, but are not restricted to: (1) the alteration mineralogy (chlorite ± sericite ± pyrophyllite ± carbonates ± hematite ± pyrite ± rutile); (2) the characteristics of whole-rock δ18O and δ34S values; (3) the ranges of depletion and enrichment of Si, Al, Mg, Ca, K, Na, Fe, Mn, and P; (4) the enrichment of Ba (as sulfate); (5) the increases in Fe3+/Fe2+ ratios; (6) the enrichment of U; (7) the depletion of Cr; and (8) the negative Ce anomalies. Literature data</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4538569','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4538569"><span>Magma injection beneath the urban area of Naples: a new mechanism for the 2012–2013 <span class="hlt">volcanic</span> unrest at Campi Flegrei caldera</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>D’Auria, Luca; Pepe, Susi; Castaldo, Raffaele; Giudicepietro, Flora; Macedonio, Giovanni; Ricciolino, Patrizia; Tizzani, Pietro; Casu, Francesco; Lanari, Riccardo; Manzo, Mariarosaria; Martini, Marcello; Sansosti, Eugenio; Zinno, Ivana</p> <p>2015-01-01</p> <p>We found the first evidence, in the last 30 years, of a renewed magmatic <span class="hlt">activity</span> at Campi Flegrei caldera from January 2012 to June 2013. The ground deformation, observed through satellite interferometry and GPS measurements, have been interpreted as the effect of the intrusion at shallow depth (3090 ± 138 m) of 0.0042 ± 0.0002 km3 of magma within a sill. This interrupts about 28 years of dominant <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and occurs in the context of an unrest phase which began in 2005 and within a more general ground uplift that goes on since 1950. This discovery has implications on the evaluation of the <span class="hlt">volcanic</span> risk and in the <span class="hlt">volcanic</span> surveillance of this densely populated area. PMID:26279090</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS11B1488T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS11B1488T"><span>First <span class="hlt">hydrothermal</span> <span class="hlt">active</span> vent discovered on the Galapagos Microplate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tao, C.; Li, H.; Wu, G.; Su, X.; Zhang, G.; Chinese DY115-21 Leg 3 Scientific Party</p> <p>2011-12-01</p> <p>The Galapagos Microplate (GM) lies on the western Gaplapagos Spreading Center (GSC), representing one of the classic Ridge-Ridge-Ridge (R-R-R) plate boundaries of the Nazca, Cocos, and Pacific plates. The presence of the 'black smoke' and <span class="hlt">hydrothermal</span> vent community were firstly confirmed on the GSC. Lots of <span class="hlt">hydrothermal</span> fields were discovered on the center and eastern GSC, while the western GSC has not been well investigated. During 17th Oct. to 9th Nov. 2009, the 3rd leg of Chinese DY115-21 cruise with R/V Dayangyihao has been launched along 2°N-5°S near equatorial East Pacific Rise (EPR). Two new <span class="hlt">hydrothermal</span> fields were confirmed. One is named 'Precious Stone Mountain', which is the first <span class="hlt">hydrothermal</span> field on the GM. The other is found at 101.47°W, 0.84°S EPR. The 'Precious Stone Mountain' <span class="hlt">hydrothermal</span> field (at 101.49°W, 1.22°N) is located at an off-axial seamount on the southern GM boundary, with a depth from 1,450 to 1,700m. <span class="hlt">Hydrothermal</span> fluids emitting from the fissures and <span class="hlt">hydrothermal</span> fauna were captured by deep-tow video. Few mineral clasts of pyrite and chalcopyrite were separated from one sediment sample, but no sulfide chimney was found yet. <span class="hlt">Hydrothermal</span> fauna such as alive mussels, crabs, shrimps, tubeworms, giant clams, as well as rock samples were collected by TV-Grab. The study of the seafloor classification with Simrad EM120 multi-beam echosounder has been conducted on the 'Precious Stone Mountain' <span class="hlt">hydrothermal</span> field. The result indicates that seafloor materials around the <span class="hlt">hydrothermal</span> field can be characterized into three types, such as the fresh lava, <span class="hlt">hydrothermal</span> sediment, and altered rock.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS52A..05B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS52A..05B"><span>Event Detection for <span class="hlt">Hydrothermal</span> Plumes: A case study at Grotto Vent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bemis, K. G.; Ozer, S.; Xu, G.; Rona, P. A.; Silver, D.</p> <p>2012-12-01</p> <p>Evidence is mounting that geologic events such as <span class="hlt">volcanic</span> eruptions (and intrusions) and earthquakes (near and far) influence the flow rates and temperatures of <span class="hlt">hydrothermal</span> systems. Connecting such suppositions to observations of <span class="hlt">hydrothermal</span> output is challenging, but new ongoing time series have the potential to capture such events. This study explores using <span class="hlt">activity</span> detection, a technique modified from computer vision, to identify pre-defined events within an extended time series recorded by COVIS (Cabled Observatory Vent Imaging Sonar) and applies it to a time series, with gaps, from Sept 2010 to the present; available measurements include plume orientation, plume rise rate, and diffuse flow area at the NEPTUNE Canada Observatory at Grotto Vent, Main Endeavour Field, Juan de Fuca Ridge. <span class="hlt">Activity</span> detection is the process of finding a pattern (<span class="hlt">activity</span>) in a data set containing many different types of patterns. Among many approaches proposed to model and detect <span class="hlt">activities</span>, we have chosen a graph-based technique, Petri Nets, as they do not require training data to model the <span class="hlt">activity</span>. They use the domain expert's knowledge to build the <span class="hlt">activity</span> as a combination of feature states and their transitions (actions). Starting from a conceptual model of how <span class="hlt">hydrothermal</span> plumes respond to daily tides, we have developed a Petri Net based detection algorithm that identifies deviations from the specified response. Initially we assumed that the orientation of the plume would change smoothly and symmetrically in a consistent daily pattern. However, results indicate that the rate of directional changes varies. The present Petri Net detects unusually large and rapid changes in direction or amount of bending; however inspection of Figure 1 suggests that many of the events detected may be artifacts resulting from gaps in the data or from the large temporal spacing. Still, considerable complexity overlies the "normal" tidal response pattern (the data has a dominant frequency of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..231a2089X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..231a2089X"><span>Experimental study on the effect of calcination on the <span class="hlt">volcanic</span> ash <span class="hlt">activity</span> of diatomite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, Liguang; Pang, Bo</p> <p>2017-09-01</p> <p>The <span class="hlt">volcanic</span> ash <span class="hlt">activity</span> of diatomite was studied under the conditions of aerobic calcination and vacuum calcination by the combined water rate method, it was characterized by XRD, BET and SEM. The results showed that the <span class="hlt">volcanic</span> ash <span class="hlt">activity</span> of diatomite under vacuum conditions was higher than that of aerobic calcination, 600°C vacuum calcination 2h, the combined water rate of diatomite-Ca(OH)2-H2O system was increased from 6.24% to 71.43%, the <span class="hlt">volcanic</span> ash <span class="hlt">activity</span> reached the maximum value, the specific surface</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('http://adsabs.harvard.edu/abs/2009DSRII..56.1632L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DSRII..56.1632L"><span>Macrobenthos community structure and trophic relationships within <span class="hlt">active</span> and inactive Pacific <span class="hlt">hydrothermal</span> sediments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Levin, Lisa A.; Mendoza, Guillermo F.; Konotchick, Talina; Lee, Raymond</p> <p>2009-09-01</p> <p><span class="hlt">Hydrothermal</span> fluids passing through sediments create a habitat hypothesized to influence the community structure of infaunal macrobenthos. Here we characterize the density, biomass, species composition, diversity, distributions, lifestyle, and nutritional sources of macroinfauna in <span class="hlt">hydrothermal</span> sediments in NE and SW Pacific settings, and draw comparisons in search of faunal attributes characteristic of this habitat. There is increasing likelihood that seafloor massive sulfide deposits, associated with <span class="hlt">active</span> and inactive <span class="hlt">hydrothermal</span> venting, will be mined commercially. This creates a growing imperative for a more thorough understanding of the structure, dynamics, and resilience of the associated sediment faunas, and has stimulated the research presented here. Macrobenthic assemblages were studied at Manus Basin (1430-1634 m, Papua New Guinea [PNG]) as a function of location (South Su vs. Solwara 1), and <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> (<span class="hlt">active</span> vs. inactive), and at Middle Valley (2406-2411 m, near Juan de Fuca Ridge) as a function of habitat (<span class="hlt">active</span> clam bed, microbial mat, hot mud, inactive background sediment). The studies conducted in PNG formed part of the environmental impact assessment work for the Solwara 1 Project of Nautilus Minerals Niugini Limited. We hypothesized that <span class="hlt">hydrothermally</span> <span class="hlt">active</span> sites should support (a) higher densities and biomass, (b) greater dominance and lower diversity, (c) a higher fraction of deposit feeders, and (d) greater isotopic evidence for chemosynthetic food sources than inactive sites. Manus Basin macrofauna generally had low density (<1000 ind. m -2) and low biomass (0.1-1.07 g m -2), except for the South Su <span class="hlt">active</span> site, which had higher density (3494 ind. m -2) and biomass (11.94 g m -2), greater dominance (R1D=76%), lower diversity and more spatial (between-core) homogeneity than the Solwara 1 and South Su inactive sites. Dominant taxa at Manus Basin were Spionidae ( Prionospio sp.) in <span class="hlt">active</span> sediments, and tanaids and deposit</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040058023&hterms=bleeding&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dbleeding','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040058023&hterms=bleeding&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dbleeding"><span><span class="hlt">Volcanic</span> <span class="hlt">Activity</span> at Tvashtar Catena, Io</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Milazzo, M. P.; Keszthelyi, L. P.; Radebaugh, J.; Davies, A. G.; McEwen, A. S.</p> <p>2004-01-01</p> <p>Tvashtar Catena (63 N, 120 W) is one of the most interesting features on Io. This chain of large paterae (caldera-like depressions) has exhibited highly variable <span class="hlt">volcanic</span> <span class="hlt">activity</span> in a series of observations. Tvashtar is the type example of a style of <span class="hlt">volcanism</span> seen only at high latitudes, with short-lived Pele-type plumes and short-lived by intense thermal events. Evidence for a hot spot at Tvashtar was first detected in an eclipse observation in April 1997 (orbit G7) by the Solid State Imager (SSI) on the Galileo Spacecraft. Tvashtar was originally targeted for observation at higher resolution in the close flyby in November 1999 (I25) because of its interesting large-scale topography. There are relatively few but generally larger paterae at high latitudes on Io. I25 images revealed a 25 km long, 1-2 km high lava curtain via a pattern of saturation and bleeding in the CCD image, which requires very high temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5270560','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5270560"><span>Defining boundaries for the distribution of microbial communities beneath the sediment-buried, <span class="hlt">hydrothermally</span> <span class="hlt">active</span> seafloor</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yanagawa, Katsunori; Ijiri, Akira; Breuker, Anja; Sakai, Sanae; Miyoshi, Youko; Kawagucci, Shinsuke; Noguchi, Takuroh; Hirai, Miho; Schippers, Axel; Ishibashi, Jun-ichiro; Takaki, Yoshihiro; Sunamura, Michinari; Urabe, Tetsuro; Nunoura, Takuro; Takai, Ken</p> <p>2017-01-01</p> <p>Subseafloor microbes beneath <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vents are thought to live near the upper temperature limit for life on Earth. We drilled and cored the Iheya North <span class="hlt">hydrothermal</span> field in the Mid-Okinawa Trough, and examined the phylogenetic compositions and the products of metabolic functions of sub-vent microbial communities. We detected microbial cells, metabolic <span class="hlt">activities</span> and molecular signatures only in the shallow sediments down to 15.8 m below the seafloor at a moderately distant drilling site from the <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vents (450 m). At the drilling site, the profiles of methane and sulfate concentrations and the δ13C and δD isotopic compositions of methane suggested the laterally flowing <span class="hlt">hydrothermal</span> fluids and the in situ microbial anaerobic methane oxidation. In situ measurements during the drilling constrain the current bottom temperature of the microbially habitable zone to ~45 °C. However, in the past, higher temperatures of 106–198 °C were possible at the depth, as estimated from geochemical thermometry on <span class="hlt">hydrothermally</span> altered clay minerals. The 16S rRNA gene phylotypes found in the deepest habitable zone are related to those of thermophiles, although sequences typical of known hyperthermophilic microbes were absent from the entire core. Overall our results shed new light on the distribution and composition of the boundary microbial community close to the high-temperature limit for habitability in the subseafloor environment of a <span class="hlt">hydrothermal</span> field. PMID:27754478</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27754478','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27754478"><span>Defining boundaries for the distribution of microbial communities beneath the sediment-buried, <span class="hlt">hydrothermally</span> <span class="hlt">active</span> seafloor.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yanagawa, Katsunori; Ijiri, Akira; Breuker, Anja; Sakai, Sanae; Miyoshi, Youko; Kawagucci, Shinsuke; Noguchi, Takuroh; Hirai, Miho; Schippers, Axel; Ishibashi, Jun-Ichiro; Takaki, Yoshihiro; Sunamura, Michinari; Urabe, Tetsuro; Nunoura, Takuro; Takai, Ken</p> <p>2017-02-01</p> <p>Subseafloor microbes beneath <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vents are thought to live near the upper temperature limit for life on Earth. We drilled and cored the Iheya North <span class="hlt">hydrothermal</span> field in the Mid-Okinawa Trough, and examined the phylogenetic compositions and the products of metabolic functions of sub-vent microbial communities. We detected microbial cells, metabolic <span class="hlt">activities</span> and molecular signatures only in the shallow sediments down to 15.8 m below the seafloor at a moderately distant drilling site from the <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vents (450 m). At the drilling site, the profiles of methane and sulfate concentrations and the δ 13 C and δD isotopic compositions of methane suggested the laterally flowing <span class="hlt">hydrothermal</span> fluids and the in situ microbial anaerobic methane oxidation. In situ measurements during the drilling constrain the current bottom temperature of the microbially habitable zone to ~45 °C. However, in the past, higher temperatures of 106-198 °C were possible at the depth, as estimated from geochemical thermometry on <span class="hlt">hydrothermally</span> altered clay minerals. The 16S rRNA gene phylotypes found in the deepest habitable zone are related to those of thermophiles, although sequences typical of known hyperthermophilic microbes were absent from the entire core. Overall our results shed new light on the distribution and composition of the boundary microbial community close to the high-temperature limit for habitability in the subseafloor environment of a <span class="hlt">hydrothermal</span> field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900033508&hterms=Volcanic+eruptions&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DVolcanic%2Beruptions','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900033508&hterms=Volcanic+eruptions&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DVolcanic%2Beruptions"><span><span class="hlt">Volcanic</span> eruptions and solar <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stothers, Richard B.</p> <p>1989-01-01</p> <p>The historical record of large <span class="hlt">volcanic</span> eruptions from 1500 to 1980 is subjected to detailed time series analysis. In two weak but probably statistically significant periodicities of about 11 and 80 yr, the frequency of <span class="hlt">volcanic</span> eruptions increases (decreases) slightly around the times of solar minimum (maximum). Time series analysis of the volcanogenic acidities in a deep ice core from Greenland reveals several very long periods ranging from about 80 to about 350 yr which are similar to the very slow solar cycles previously detected in auroral and C-14 records. Solar flares may cause changes in atmospheric circulation patterns that abruptly alter the earth's spin. The resulting jolt probably triggers small earthquakes which affect <span class="hlt">volcanism</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70010976','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70010976"><span>Mapping of <span class="hlt">hydrothermally</span> altered rocks using airborne multispectral scanner data, Marysvale, Utah, mining district</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Podwysocki, M.H.; Segal, D.B.; Jones, O.D.</p> <p>1983-01-01</p> <p>Multispectral data covering an area near Marysvale, Utah, collected with the airborne National Aeronautics and Space Administration (NASA) 24-channel Bendix multispectral scanner, were analyzed to detect areas of <span class="hlt">hydrothermally</span> altered, potentially mineralized rocks. Spectral bands were selected for analysis that approximate those of the Landsat 4 Thematic Mapper and which are diagnostic of the presence of <span class="hlt">hydrothermally</span> derived products. <span class="hlt">Hydrothermally</span> altered rocks, particularly <span class="hlt">volcanic</span> rocks affected by solutions rich in sulfuric acid, are commonly characterized by concentrations of argillic minerals such as alunite and kaolinite. These minerals are important for identifying <span class="hlt">hydrothermally</span> altered rocks in multispectral images because they have intense absorption bands centered near a wavelength of 2.2 ??m. Unaltered <span class="hlt">volcanic</span> rocks commonly do not contain these minerals and hence do not have the absorption bands. A color-composite image was constructed using the following spectral band ratios: 1.6??m/2.2??m, 1.6??m/0.48??m, and 0.67??m/1.0??m. The particular bands were chosen to emphasize the spectral contrasts that exist for argillic versus <span class="hlt">non</span>-argillic rocks, limonitic versus nonlimonitic rocks, and rocks versus vegetation, respectively. The color-ratio composite successfully distinguished most types of altered rocks from unaltered rocks. Some previously unrecognized areas of <span class="hlt">hydrothermal</span> alteration were mapped. The altered rocks included those having high alunite and/or kaolinite content, siliceous rocks containing some kaolinite, and ash-fall tuffs containing zeolitic minerals. The color-ratio-composite image allowed further division of these rocks into limonitic and nonlimonitic phases. The image did not allow separation of highly siliceous or hematitically altered rocks containing no clays or alunite from unaltered rocks. A color-coded density slice image of the 1.6??m/2.2??m band ratio allowed further discrimination among the altered units. Areas</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH33A0242D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH33A0242D"><span>Characterizing <span class="hlt">volcanic</span> <span class="hlt">activity</span>: Application of freely-available webcams</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dehn, J.; Harrild, M.; Webley, P. W.</p> <p>2017-12-01</p> <p>In recent years, freely-available web-based cameras, or webcams, have become more readily available allowing an increased level of monitoring at <span class="hlt">active</span> volcanoes across the globe. While these cameras have been extensively used as qualitative tools, they provide a unique dataset to perform quantitative analyzes of the changing behavior of the particular volcano within the cameras field of view. We focus on the multitude of these freely-available webcams and present a new algorithm to detect changes in <span class="hlt">volcanic</span> <span class="hlt">activity</span> using nighttime webcam data. Our approach uses a quick, efficient, and fully automated algorithm to identify changes in webcam data in near real-time, including techniques such as edge detection, Gaussian mixture models, and temporal/spatial statistical tests, which are applied to each target image. Often the image metadata (exposure, gain settings, aperture, focal length, etc.) are unknown, meaning we developed our algorithm to identify the quantity of <span class="hlt">volcanically</span> incandescent pixels as well as the number of specific algorithm tests needed to detect thermal <span class="hlt">activity</span>, instead of directly correlating brightness in the webcam to eruption temperatures. We compared our algorithm results to a manual analysis of webcam data for several volcanoes and determined a false detection rate of less than 3% for the automated approach. In our presentation, we describe the different tests integrated into our algorithm, lessons learned, and how we applied our method to several volcanoes across the North Pacific during its development and implementation. We will finish with a discussion on the global applicability of our approach and how to build a 24/7, 365 day a year tool that can be used as an additional data source for real-time analysis of <span class="hlt">volcanic</span> <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.V12D1009Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.V12D1009Z"><span>Decline of a <span class="hlt">Hydrothermal</span> Vent Field - Escanaba Trough 12 Years Later</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zierenberg, R. A.; Clague, D. A.; Davis, A. S.; Lilley, M. D.; McClain, J. S.; Olson, E. S.; Ross, S. L.; Von Damm, K. L.</p> <p>2001-12-01</p> <p><span class="hlt">Hydrothermal</span> venting was discovered in Escanaba Trough, the southern sediment-covered portion of the Gorda Ridge, in 1988. Large pyrrhotite-rich massive sulfide mounds are abundant at each of the <span class="hlt">volcanic</span>/intrusive centers that have been investigated in Escanaba Trough, but the only area of known <span class="hlt">hydrothermal</span> venting is the NESCA site along the ridge axis at 41\\deg N. <span class="hlt">Hydrothermal</span> fluids venting at 217\\deg C and 108\\deg C were sampled in 1988 on two sulfide mounds separated by about 275 m. The end-member fluid compositions were indistinguishable within analytical errors. Several sulfide mounds were observed in 1988 which had diffusely venting low temperature (< 20\\deg C) fluids that supported extensive vent communities dominated by fields of Ridgia. Nine holes were drilled in the NESCA area in 1996 on ODP Leg 169, including Hole 1036I that penetrated to basaltic basement at 405 m below sea floor (mbsf). Surveys of the area using the drill string camera located only one area of <span class="hlt">active</span> venting at the same mound where 217\\deg C vent fluids were sampled from two <span class="hlt">active</span> vents in 1988. Drill hole 1036A was spudded between the two <span class="hlt">active</span> vents on this sulfide mound (approximately 4 and 8 m away) and penetrated to 115 mbsf. The NESCA site was revisited in 2000 using MBARI's R/V Western Flyer and ROV Tiburon. The <span class="hlt">hydrothermal</span> vents appeared essentially identical to observations made from the drill string camera in 1996 despite the presence of a drill hole within meters of the two vents. The maximum vent temperature measured in 2000 was 212\\deg C. Fluid samples have major element and isotopic compositions very similar to those collected in 1988. The vent fluids have higher methane ( ~19 mmol/kg) than those from the geologically similar Middle Valley vent field, but lower values than those at Guaymas Basin. Drill hole 1036A was weakly venting, but the diffuse <span class="hlt">hydrothermal</span> fluids could not be sampled with the equipment available. The walls of the drill hole were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12110886','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12110886"><span>A satellite geodetic survey of large-scale deformation of <span class="hlt">volcanic</span> centres in the central Andes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, Matthew E; Simons, Mark</p> <p>2002-07-11</p> <p>Surface deformation in <span class="hlt">volcanic</span> areas usually indicates movement of magma or <span class="hlt">hydrothermal</span> fluids at depth. Stratovolcanoes tend to exhibit a complex relationship between deformation and eruptive behaviour. The characteristically long time spans between such eruptions requires a long time series of observations to determine whether deformation without an eruption is common at a given edifice. Such studies, however, are logistically difficult to carry out in most <span class="hlt">volcanic</span> arcs, as these tend to be remote regions with large numbers of volcanoes (hundreds to even thousands). Here we present a satellite-based interferometric synthetic aperture radar (InSAR) survey of the remote central Andes <span class="hlt">volcanic</span> arc, a region formed by subduction of the Nazca oceanic plate beneath continental South America. Spanning the years 1992 to 2000, our survey reveals the background level of <span class="hlt">activity</span> of about 900 volcanoes, 50 of which have been classified as potentially <span class="hlt">active</span>. We find four centres of broad (tens of kilometres wide), roughly axisymmetric surface deformation. None of these centres are at volcanoes currently classified as potentially <span class="hlt">active</span>, although two lie within about 10 km of volcanoes with known <span class="hlt">activity</span>. Source depths inferred from the patterns of deformation lie between 5 and 17 km. In contrast to the four new sources found, we do not observe any deformation associated with recent eruptions of Lascar, Chile.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028556','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028556"><span>Multiple edifice-collapse events in the Eastern Mexican <span class="hlt">Volcanic</span> Belt: The role of sloping substrate and implications for hazard assessment</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Carrasco-Nunez, Gerardo; Diaz-Castellon, Rodolfo; Siebert, L.; Hubbard, B.; Sheridan, M.F.; Rodriguez, Sergio R.</p> <p>2006-01-01</p> <p>The Citlalte??petl-Cofre de Perote <span class="hlt">volcanic</span> chain forms an important physiographic barrier that separates the Central Altiplano (2500??masl) from the Gulf Coastal Plain (GCP) (1300??masl). The abrupt eastward drop in relief between these provinces gives rise to unstable conditions and consequent gravitational collapse of large <span class="hlt">volcanic</span> edifices built at the edge of the Altiplano. Eastward sloping substrate, caused by the irregular configuration of the basement rocks, is the dominant factor that controls the direction of collapsing sectors in all major volcanoes in the region to be preferentially towards the GCP. These collapses produced voluminous debris avalanches and lahars that inundated the well-developed drainages and clastic aprons that characterize the Coastal Plain. Large catastrophic collapses from Citlalte??petl, Las Cumbres, and Cofre de Perote volcanoes are well documented in the geologic record. Some of the avalanches and transformed flows have exceptionally long runouts and reach the Gulf of Mexico traveling more than 120??km from their source. So far, no direct evidence has been found for magmatic <span class="hlt">activity</span> associated with the initiation of these catastrophic flank-collapses. Apparently, instability of the <span class="hlt">volcanic</span> edifices has been strongly favored by very intense <span class="hlt">hydrothermal</span> alteration, abrupt topographic change, and intense fracturing. In addition to the eastward slope of the substrate, the reactivation of pre-<span class="hlt">volcanic</span> basement structures during the Late Tertiary, and the E-W to ENE-SSW oriented regional stress regimes may have played an important role in the preferential movement direction of the avalanches and flows. In addition to magmatic-<span class="hlt">hydrothermal</span> processes, high amounts of rainfall in the area is another factor that enhances alteration and eventually weakens the rocks. It is very likely that seismic <span class="hlt">activity</span> may be the principal triggering mechanism that caused the flank collapse of large <span class="hlt">volcanic</span> edifices in the Eastern Mexican <span class="hlt">Volcanic</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914748H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914748H"><span><span class="hlt">Volcanic</span> rock properties control sector collapse events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Amy; Kendrick, Jackie; Lavallée, Yan; Hornby, Adrian; Di Toro, Giulio</p> <p>2017-04-01</p> <p>Volcanoes constructed by superimposed layers of varying <span class="hlt">volcanic</span> materials are inherently unstable structures. The heterogeneity of weak and strong layers consisting of ash, tephra and lavas, each with varying coherencies, porosities, crystallinities, glass content and ultimately, strength, can promote <span class="hlt">volcanic</span> flank and sector collapses. These volcanoes often exist in areas with complex regional tectonics adding to instability caused by heterogeneity, flank overburden, magma movement and emplacement in addition to <span class="hlt">hydrothermal</span> alteration and anomalous geothermal gradients. Recent studies conducted on the faulting properties of <span class="hlt">volcanic</span> rocks at variable slip rates show the rate-weakening dependence of the friction coefficients (up to 90% reduction)[1], caused by a wide range of factors such as the generation of gouge and frictional melt lubrication [2]. Experimental data from experiments conducted on <span class="hlt">volcanic</span> products suggests that frictional melt occurs at slip rates similar to those of plug flow in <span class="hlt">volcanic</span> conduits [1] and the bases of mass material movements such as debris avalanches from <span class="hlt">volcanic</span> flanks [3]. In <span class="hlt">volcanic</span> rock, the generation of frictional heat may prompt the remobilisation of interstitial glass below melting temperatures due to passing of the glass transition temperature at ˜650-750 ˚C [4]. In addition, the crushing of pores in high porosity samples can lead to increased comminution and strain localisation along slip surfaces. Here we present the results of friction tests on both high density, glass rich samples from Santaguito (Guatemala) and synthetic glass samples with varying porosities (0-25%) to better understand frictional properties underlying <span class="hlt">volcanic</span> collapse events. 1. Kendrick, J.E., et al., Extreme frictional processes in the <span class="hlt">volcanic</span> conduit of Mount St. Helens (USA) during the 2004-2008 eruption. J. Structural Geology, 2012. 2. Di Toro, G., et al., Fault lubrication during earthquakes. Nature, 2011. 471(7339): p. 494-498. 3</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860013624','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860013624"><span>Barberton greenstone belt <span class="hlt">volcanism</span>: Succession, style and petrogenesis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Byerly, G. R.; Lowe, D. R.</p> <p>1986-01-01</p> <p>The Barberton Mountain Land is an early Archean greenstone belt along the eastern margin of the Kaapvaal Craton of southern Africa. Detailed mapping in the southern portion of the belt leads to the conclusion that a substantial thickness is due to original deposition of <span class="hlt">volcanics</span> and sediments. In the area mapped, a minimum thickness of 12km of predominantly mafic and ultramafic <span class="hlt">volcanics</span> comprise the Komati, Hooggenoeg, and Kromberg Formations of the Onverwacht Group, and at least one km of predominantly pyroclastic and epiclastic sediments derived from dacitic <span class="hlt">volcanics</span> comprise the Fig Tree Group. The Barberton greenstone belt formed primarily by ultramafic to mafic <span class="hlt">volcanism</span> on a shallow marine platform which underwent little or no concurrent extension. Vents for this igneous <span class="hlt">activity</span> were probably of the <span class="hlt">non</span>-constructional fissure type. Dacitic <span class="hlt">volcanism</span> occurred throughout the sequence in minor amounts. Large, constructional vent complexes were formed, and explosive eruptions widely dispersed pyroclastic debris. Only in the final stages of evolution of the belt did significant thrust-faulting occur, generally after, though perhaps overlapping with, the final stage of dacitic igneous <span class="hlt">activity</span>. A discussion follows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1110353F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1110353F"><span>The main factors controlling petrophysical alteration in <span class="hlt">hydrothermal</span> systems of the Kuril-Kamchatka island arch</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frolova, J.; Ladygin, V.; Rychagov, S.; Shanina, V.; Blyumkina, M.</p> <p>2009-04-01</p> <p>This report is based on the results of petrophysical studies obtained on a number of <span class="hlt">hydrothermal</span> systems in the Kuril-Kamchatka island arc (Pauzhetsky, Mutnovsky, Koshelevsky, Essovsky, a volcano of Ebeko, Oceansky). Mineral composition and pore-space structure of primary rocks change intensively during <span class="hlt">hydrothermal</span> process, results in alteration of petrophysical properties - porosity, density, permeability, hygroscopy, sonic velocity, elastic modulus, mechanical properties, thermal and magnetic characteristics. Petrophysical alterations gradually lead to the change of the structure of <span class="hlt">hydrothermal</span> system, and its hydrodynamic and temperature regime. The tendency of petrophysical alteration can be different. In some cases rocks "improvement" is observed i.e. consolidation, hardening, decrease of porosity and permeability, removal of hygroscopy. In other cases rocks "deterioration" occurs, i.e. formation of secondary porosity and permeability, a decrease of density, strength, and elastic modulus, and occurrence of hygroscopic moisture. The classical example of cardinal petrophysical alteration is the transformation of hard basalts to plastic clays. The opposite example is the transformation of only slightly consolidates porous tuffs to hard and dense secondary quartzite. The character of petrophysical alteration depends on a number of factors including peculiarities of primary rocks, temperature, pressure and composition of thermal fluids, duration of fluid-rock interaction, and condition of fluid (steam, water, boiling water). The contribution of each factor to change of <span class="hlt">volcanic</span> rocks properties is considered and analyzed in details. In particular, primary rocks controls speed, intensity and character of petrophysical alterations. Factors favorable for alteration are high porosity and permeability, micro crakes, weak cementation, glassy structure, basaltic composition. Kuril-Kamchatka region represents the <span class="hlt">volcanic</span> island arch so host rocks in <span class="hlt">hydrothermal</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Litho.302..359D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Litho.302..359D"><span>A model for Nb-Zr-REE-Ga enrichment in Lopingian altered alkaline <span class="hlt">volcanic</span> ashes: Key evidence of H-O isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dai, Shifeng; Nechaev, Victor P.; Chekryzhov, Igor Yu.; Zhao, Lixin; Vysotskiy, Sergei V.; Graham, Ian; Ward, Colin R.; Ignatiev, Alexander V.; Velivetskaya, Tatyana A.; Zhao, Lei; French, David; Hower, James C.</p> <p>2018-03-01</p> <p>Clay-altered <span class="hlt">volcanic</span> ash with highly-elevated concentrations of Nb(Ta), Zr(Hf), rare earth elements (REE), and Ga, is a new type of critical metal deposit with high commercial prospects that has been discovered in Yunnan Province, southwest China. Previous studies showed that the <span class="hlt">volcanic</span> ashes had been subjected to <span class="hlt">hydrothermal</span> fluids, the nature of which, however, is not clear. Here we show that the <span class="hlt">volcanic</span> ashes were originated from alkaline magmatism, followed by a continuous <span class="hlt">hydrothermal</span>-weathering process. Heated meteoric waters, which were sourced from acidic rains and mixed with CO2 from degassing of the Emeishan plume, have caused partial, but widespread, acidic leaching of Nb, Ta, Zr, Hf, REE, and Ga into ground water and residual enrichment of these elements, along with Al and Ti, in the deeply altered rocks. Subsequent alteration occurring under cooler, neutral or alkaline conditions, caused by water-rock interaction, resulted in precipitation of the leached critical metals in the deposit. Polymetallic mineralization of similar origin may be found in other continental regions subjected to explosive alkaline <span class="hlt">volcanism</span> associated with deep weathering in humid conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5701667','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5701667"><span>Episodes of fluvial and <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Mangala Valles, Mars</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Keske, Amber L.; Hamilton, Christopher W.; McEwen, Alfred S.; Daubar, Ingrid J.</p> <p>2017-01-01</p> <p>A new mapping-based study of the 900-km-long Mangala Valles outflow system was motivated by the availability of new high-resolution images and continued debates about the roles of water and lava in outflow channels on Mars. This study uses photogeologic analysis, geomorphic surface mapping, cratering statistics, and relative stratigraphy. Results show that Mangala Valles underwent at least two episodes of fluvial <span class="hlt">activity</span> and at least three episodes of <span class="hlt">volcanic</span> <span class="hlt">activity</span> during the Late Amazonian. The occurrence of scoured bedrock at the base of the mapped stratigraphy, in addition to evidence provided by crater retention ages, suggests that fluvial <span class="hlt">activity</span> preceded the deposition of two of the <span class="hlt">volcanic</span> units. Crater counts performed at 30 locations throughout the area have allowed us to construct the following timeline: (1) formation of Noachian Highlands and possible initial flooding event(s) before ~1 Ga, (2) emplacement of Tharsis lava flows in the valley from ~700 to 1000 Ma, (3) a megaflooding event at ~700–800 Ma sourced from Mangala Fossa, (4) valley fill by a sequence of lava flows sourced from Mangala Fossa ~400–500 Ma, (5) another megaflooding event from ~400 Ma, (6) a final phase of <span class="hlt">volcanism</span> sourced from Mangala Fossa ~300–350 Ma, and (7) emplacement of eolian sedimentary deposits in the northern portion of the valley ~300 Ma. These results are consistent with alternating episodes of aqueous flooding and <span class="hlt">volcanism</span> in the valles. This pattern of geologic <span class="hlt">activity</span> is similar to that of other outflow systems, such as Kasei Valles, suggesting that there is a recurring, and perhaps coupled, nature of these processes on Mars. PMID:29176911</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29176911','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29176911"><span>Episodes of fluvial and <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Mangala Valles, Mars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Keske, Amber L; Hamilton, Christopher W; McEwen, Alfred S; Daubar, Ingrid J</p> <p>2015-01-01</p> <p>A new mapping-based study of the 900-km-long Mangala Valles outflow system was motivated by the availability of new high-resolution images and continued debates about the roles of water and lava in outflow channels on Mars. This study uses photogeologic analysis, geomorphic surface mapping, cratering statistics, and relative stratigraphy. Results show that Mangala Valles underwent at least two episodes of fluvial <span class="hlt">activity</span> and at least three episodes of <span class="hlt">volcanic</span> <span class="hlt">activity</span> during the Late Amazonian. The occurrence of scoured bedrock at the base of the mapped stratigraphy, in addition to evidence provided by crater retention ages, suggests that fluvial <span class="hlt">activity</span> preceded the deposition of two of the <span class="hlt">volcanic</span> units. Crater counts performed at 30 locations throughout the area have allowed us to construct the following timeline: (1) formation of Noachian Highlands and possible initial flooding event(s) before ~1 Ga, (2) emplacement of Tharsis lava flows in the valley from ~700 to 1000 Ma, (3) a megaflooding event at ~700-800 Ma sourced from Mangala Fossa, (4) valley fill by a sequence of lava flows sourced from Mangala Fossa ~400-500 Ma, (5) another megaflooding event from ~400 Ma, (6) a final phase of <span class="hlt">volcanism</span> sourced from Mangala Fossa ~300-350 Ma, and (7) emplacement of eolian sedimentary deposits in the northern portion of the valley ~300 Ma. These results are consistent with alternating episodes of aqueous flooding and <span class="hlt">volcanism</span> in the valles. This pattern of geologic <span class="hlt">activity</span> is similar to that of other outflow systems, such as Kasei Valles, suggesting that there is a recurring, and perhaps coupled, nature of these processes on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T31C0640Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T31C0640Z"><span>Axial crustal structure of the Costa Rica Rift: Implications for along-axis <span class="hlt">hydrothermal</span> circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, L.; Tong, V.; Hobbs, R. W.; Peirce, C.; Lowell, R. P.; Haughton, G.; Murton, B. J.; Morales Maqueda, M. A.; Harris, R. N.; Robinson, A. H.</p> <p>2017-12-01</p> <p>In 2015, a multidisciplinary geophysical cruise surveyed the Costa Rica Rift (CRR) in the Panama Basin of the equatorial East Pacific, acquiring a grid of multichannel seismic and wide-angle profiles to determine the mode of oceanic crustal accretion at intermediate-spreading ridges, and how the crustal structure may be influenced by <span class="hlt">hydrothermal</span> fluid flow. Analysis of 69,000 P-wave first arrivals recorded by 25 ocean-bottom seismographs deployed over a 20 × 20 km area that straddles the ridge axis, reveals a 3D velocity-depth model of upper crustal structure. In particular, the model shows a low velocity anomaly that extends to 2 km below seabed centred on a small-offset <span class="hlt">non</span>-transform discontinuity (NTD), and a pattern of increasing velocity with distance off-axis that may reflect changes in porosity and permeability in layer 2 of the crust. Assuming the upper crustal velocity anomalies are linked with porosity and hence represent the ability of fluid to flow, comparison of the tomographic model with the <span class="hlt">volcanic</span> seabed morphology suggests that the broad low velocity zone beneath the NTD may be a region of extensive fracturing. Hence, we infer that this region may provide a primary pathway for the recharge of seawater into the crust. Further west along the axis, beneath the bathymetric dome, which is the shallowest portion along the axis, the low-velocity anomaly is less pronounced, suggesting that fractures are less open and that fluid-rock interaction has encouraged mineral precipitation and alteration, as a result of a longer established <span class="hlt">hydrothermal</span> fluid flow driven by the axial magma lens observed beneath it. This interpretation is supported by the presence of a plume from an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vent system. Hence, we infer that the variable velocity structure of the upper crust of the CRR is a proxy that reflects the primary porosity, faulting and fracturing related to phases of magma-driven accretion and/or ridge geometry re-adjustment, and that there is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27079264','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27079264"><span>Soil radon measurements as a potential tracer of tectonic and <span class="hlt">volcanic</span> <span class="hlt">activity</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Neri, Marco; Ferrera, Elisabetta; Giammanco, Salvatore; Currenti, Gilda; Cirrincione, Rosolino; Patanè, Giuseppe; Zanon, Vittorio</p> <p>2016-04-15</p> <p>In Earth Sciences there is a growing interest in studies concerning soil-radon <span class="hlt">activity</span>, due to its potential as a tracer of numerous natural phenomena. Our work marks an advance in the comprehension of the interplay between tectonic <span class="hlt">activity</span>, <span class="hlt">volcanic</span> eruptions and gas release through faults. Soil-radon measurements, acquired on Mt. Etna volcano in 2009-2011, were analyzed. Our radon probe is sensitive to changes in both <span class="hlt">volcanic</span> and seismic <span class="hlt">activity</span>. Radon data were reviewed in light of the meteorological parameters. Soil samples were analyzed to characterize their uranium content. All data have been summarized in a physical model which identifies the radon sources, highlights the mechanism of radon transport and envisages how such a mechanism may change as a consequence of seismicity and <span class="hlt">volcanic</span> events. In the NE of Etna, radon is released mainly from a depth of <1400 m, with an ascent speed of >50 m/day. Three periods of anomalous gas release were found (February 2010, January and February 2011). The trigger of the first anomaly was tectonic, while the second and third had a <span class="hlt">volcanic</span> origin. These results mark a significant step towards a better understanding of the endogenous mechanisms that cause changes in soil-radon emission at <span class="hlt">active</span> volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...624581N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...624581N"><span>Soil radon measurements as a potential tracer of tectonic and <span class="hlt">volcanic</span> <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neri, Marco; Ferrera, Elisabetta; Giammanco, Salvatore; Currenti, Gilda; Cirrincione, Rosolino; Patanè, Giuseppe; Zanon, Vittorio</p> <p>2016-04-01</p> <p>In Earth Sciences there is a growing interest in studies concerning soil-radon <span class="hlt">activity</span>, due to its potential as a tracer of numerous natural phenomena. Our work marks an advance in the comprehension of the interplay between tectonic <span class="hlt">activity</span>, <span class="hlt">volcanic</span> eruptions and gas release through faults. Soil-radon measurements, acquired on Mt. Etna volcano in 2009-2011, were analyzed. Our radon probe is sensitive to changes in both <span class="hlt">volcanic</span> and seismic <span class="hlt">activity</span>. Radon data were reviewed in light of the meteorological parameters. Soil samples were analyzed to characterize their uranium content. All data have been summarized in a physical model which identifies the radon sources, highlights the mechanism of radon transport and envisages how such a mechanism may change as a consequence of seismicity and <span class="hlt">volcanic</span> events. In the NE of Etna, radon is released mainly from a depth of <1400 m, with an ascent speed of >50 m/day. Three periods of anomalous gas release were found (February 2010, January and February 2011). The trigger of the first anomaly was tectonic, while the second and third had a <span class="hlt">volcanic</span> origin. These results mark a significant step towards a better understanding of the endogenous mechanisms that cause changes in soil-radon emission at <span class="hlt">active</span> volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4832328','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4832328"><span>Soil radon measurements as a potential tracer of tectonic and <span class="hlt">volcanic</span> <span class="hlt">activity</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>Neri, Marco; Ferrera, Elisabetta; Giammanco, Salvatore; Currenti, Gilda; Cirrincione, Rosolino; Patanè, Giuseppe; Zanon, Vittorio</p> <p>2016-01-01</p> <p>In Earth Sciences there is a growing interest in studies concerning soil-radon <span class="hlt">activity</span>, due to its potential as a tracer of numerous natural phenomena. Our work marks an advance in the comprehension of the interplay between tectonic <span class="hlt">activity</span>, <span class="hlt">volcanic</span> eruptions and gas release through faults. Soil-radon measurements, acquired on Mt. Etna volcano in 2009–2011, were analyzed. Our radon probe is sensitive to changes in both <span class="hlt">volcanic</span> and seismic <span class="hlt">activity</span>. Radon data were reviewed in light of the meteorological parameters. Soil samples were analyzed to characterize their uranium content. All data have been summarized in a physical model which identifies the radon sources, highlights the mechanism of radon transport and envisages how such a mechanism may change as a consequence of seismicity and <span class="hlt">volcanic</span> events. In the NE of Etna, radon is released mainly from a depth of <1400 m, with an ascent speed of >50 m/day. Three periods of anomalous gas release were found (February 2010, January and February 2011). The trigger of the first anomaly was tectonic, while the second and third had a <span class="hlt">volcanic</span> origin. These results mark a significant step towards a better understanding of the endogenous mechanisms that cause changes in soil-radon emission at <span class="hlt">active</span> volcanoes. PMID:27079264</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/2018EP%26S...70...61A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EP%26S...70...61A"><span>Seismic evidence for arc segmentation, <span class="hlt">active</span> magmatic intrusions and syn-rift fault system in the northern Ryukyu <span class="hlt">volcanic</span> arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arai, Ryuta; Kodaira, Shuichi; Takahashi, Tsutomu; Miura, Seiichi; Kaneda, Yoshiyuki</p> <p>2018-04-01</p> <p>Tectonic and <span class="hlt">volcanic</span> structures of the northern Ryukyu arc are investigated on the basis of multichannel seismic (MCS) reflection data. The study area forms an <span class="hlt">active</span> <span class="hlt">volcanic</span> front in parallel to the <span class="hlt">non-volcanic</span> island chain in the eastern margin of the Eurasian plate and has been undergoing regional extension on its back-arc side. We carried out a MCS reflection experiment along two across-arc lines, and one of the profiles was laid out across the Tokara Channel, a linear bathymetric depression which demarcates the northern and central Ryukyu arcs. The reflection image reveals that beneath this topographic valley there exists a 3-km-deep sedimentary basin atop the arc crust, suggesting that the arc segment boundary was formed by rapid and focused subsidence of the arc crust driven by the arc-parallel extension. Around the <span class="hlt">volcanic</span> front, magmatic conduits represented by tubular transparent bodies in the reflection images are well developed within the shallow sediments and some of them are accompanied by small fragments of dipping seismic reflectors indicating intruded sills at their bottoms. The spatial distribution of the conduits may suggest that the arc <span class="hlt">volcanism</span> has multiple <span class="hlt">active</span> outlets on the seafloor which bifurcate at crustal depths and/or that the location of the <span class="hlt">volcanic</span> front has been migrating trenchward over time. Further distant from the <span class="hlt">volcanic</span> front toward the back-arc (> 30 km away), these <span class="hlt">volcanic</span> features vanish, and alternatively wide rift basins become predominant where rapid transitions from normal-fault-dominant regions to strike-slip-fault-dominant regions occur. This spatial variation in faulting patterns indicates complex stress regimes associated with arc/back-arc rifting in the northern Okinawa Trough.[Figure not available: see fulltext.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..671O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..671O"><span>Late Cenozoic Samtskhe-Javakheti <span class="hlt">Volcanic</span> Highland, Georgia:The Result of Mantle Plumes <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Okrostsvaridze, Avtandil</p> <p>2017-04-01</p> <p>Late Cenozoic Samtskhe-Javakheti continental <span class="hlt">volcanic</span> highland (1500-2500 m a.s.l) is located in the SW part of the Lesser Caucasus. In Georgia the highland occupies more than 4500 km2, however its large part spreads towards the South over the territories of Turkey and Armenia. One can point out three stages of magmatic <span class="hlt">activity</span> in this <span class="hlt">volcanic</span> highland: 1. Early Pliocene <span class="hlt">activity</span> (5.2-2.8 Ma; zircons U-Pb age) - when a large part of the highland was built up. It is formed from <span class="hlt">volcanic</span> lava-breccias of andesite-dacitic composition, pyroclastic rocks and andesite-basalt lava flow. The evidences of this structure are: a large volume of <span class="hlt">volcanic</span> material (>1500 km3); big thickness (700-1100 m in average), large-scale of lava flows (length 35 km, width 2.5-3.5 km, thickness 30-80 m), big thickness of <span class="hlt">volcanic</span> ash horizons (300 cm at some places) and big size of <span class="hlt">volcanic</span> breccias (diameter >1 m). Based on this data we assume that a source of this structure was a supervolcano (Okrostsvaridze et al., 2016); 2. Early Pleistocene <span class="hlt">activity</span> (2.4 -1.6 Ma; zircons U-Pb age) - when continental flood basalts of 100-300 m thickness were formed. The flow is fully crystalline, coarse-grained, which mainly consist of olivine and basic labradorite. There 143Nd/144Nd parameter varies in the range of +0.41703 - +0.52304, and 87Sr/88Sr - from 0.7034 to 0.7039; 3. Late Pleistocene <span class="hlt">activity</span> (0.35-0.021 Ma; zircons U-Pb age) - when intraplate Abul-Samsari linear <span class="hlt">volcanic</span> ridge of andesite composition was formed stretching to the S-N direction for 40 km with the 8-12 km width and contains more than 20 <span class="hlt">volcanic</span> edifices. To the South of the Abul-Samsari ridge the oldest (0.35-0.30 Ma; zircons U-Pb age) volcano Didi Abuli (3305 m a.s.l.) is located. To the North ages of volcano edifices gradually increase. Farther North the youngest volcano Tavkvetili (0.021-0. 030 Ma) is located (2583 m a.s.l.). One can see from this description that the Abul-Samsari ridge has all signs characterizing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1414398V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1414398V"><span>Evidence of <span class="hlt">non</span>-extensivity and complexity in the seismicity observed during 2011-2012 at the Santorini <span class="hlt">volcanic</span> complex, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vallianatos, F.; Tzanis, A.; Michas, G.; Papadakis, G.</p> <p>2012-04-01</p> <p>Since the middle of summer 2011, an increase in the seismicity rates of the <span class="hlt">volcanic</span> complex system of Santorini Island, Greece, was observed. In the present work, the temporal distribution of seismicity, as well as the magnitude distribution of earthquakes, have been studied using the concept of <span class="hlt">Non</span>-Extensive Statistical Physics (NESP; Tsallis, 2009) along with the evolution of Shanon entropy H (also called information entropy). The analysis is based on the earthquake catalogue of the Geodynamic Institute of the National Observatory of Athens for the period July 2011-January 2012 (http://www.gein.noa.gr/). <span class="hlt">Non</span>-Extensive Statistical Physics, which is a generalization of Boltzmann-Gibbs statistical physics, seems a suitable framework for studying complex systems. The observed distributions of seismicity rates at Santorini can be described (fitted) with NESP models to exceptionally well. This implies the inherent complexity of the Santorini <span class="hlt">volcanic</span> seismicity, the applicability of NESP concepts to <span class="hlt">volcanic</span> earthquake <span class="hlt">activity</span> and the usefulness of NESP in investigating phenomena exhibiting multifractality and long-range coupling effects. Acknowledgments. This work was supported in part by the THALES Program of the Ministry of Education of Greece and the European Union in the framework of the project entitled "Integrated understanding of Seismicity, using innovative Methodologies of Fracture mechanics along with Earthquake and <span class="hlt">non</span> extensive statistical physics - Application to the geodynamic system of the Hellenic Arc. SEISMO FEAR HELLARC". GM and GP wish to acknowledge the partial support of the Greek State Scholarships Foundation (ΙΚΥ).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70013650','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70013650"><span>Oxygen isotope evidence for submarine <span class="hlt">hydrothermal</span> alteration of the Del Puerto ophiolite, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Schiffman, P.; Williams, A.E.; Evarts, R.C.</p> <p>1984-01-01</p> <p>The oxygen isotope compositions and metamorphic mineral assemblages of <span class="hlt">hydrothermally</span> altered rocks from the Del Puerto ophiolite and overlying volcaniclastic sedimentary rocks at the base of the Great Valley sequence indicate that their alteration occurred in a submarine <span class="hlt">hydrothermal</span> system. Whole rock ??18O compositions decrease progressively down section (with increasing metamorphic grade): +22.4??? (SMOW) to +13.8 for zeolite-bearing volcaniclastic sedimentary rocks overlying the ophiolite; +19.6 to +11.6 for pumpellyite-bearing metavolcanic rocks in the upper part of the ophiolite's <span class="hlt">volcanic</span> member; +12.3 to +8.1 for epidote-bearing metavolcanic rocks in the lower part of the <span class="hlt">volcanic</span> member; +8.5 to +5.7 for greenschist facies rocks from the ophiolite's plutonic member; +7.6 to +5.8 for amphibolite facies or unmetamorphosed rocks from the plutonic member. Modelling of fluid-rock interaction in the Del Puerto ophiolite indicates that the observed pattern of upward enrichment in whole rock ??18O can be best explained by isotopic exchange with discharging 18O-shifted seawater at fluid/rock mass ratios near 2 and temperatures below 500??C. 18O-depleted plutonic rocks necessarily produced during <span class="hlt">hydrothermal</span> circulation were later removed as a result of tectonism. Submarine weathering and later burial metamorphism at the base of the Great Valley sequence cannot by itself have produced the zonation of <span class="hlt">hydrothermal</span> minerals and the corresponding variations in oxygen isotope compositions. The pervasive zeolite and prehnite-pumpellyite facies mineral assemblages found in the Del Puerto ophiolite may reflect its origin near an island arc rather than deep ocean spreading center. ?? 1984.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20480029','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20480029"><span>Origin and distribution of thiophenes and furans in gas discharges from <span class="hlt">active</span> volcanoes and geothermal systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tassi, Franco; Montegrossi, Giordano; Capecchiacci, Francesco; Vaselli, Orlando</p> <p>2010-03-31</p> <p>The composition of <span class="hlt">non</span>-methane organic volatile compounds (VOCs) determined in 139 thermal gas discharges from 18 different geothermal and <span class="hlt">volcanic</span> systems in Italy and Latin America, consists of C(2)-C(20) species pertaining to the alkanes, alkenes, aromatics and O-, S- and N-bearing classes of compounds. Thiophenes and mono-aromatics, especially the methylated species, are strongly enriched in fluids emissions related to <span class="hlt">hydrothermal</span> systems. Addition of hydrogen sulphide to dienes and electrophilic methylation involving halogenated radicals may be invoked for the formation of these species. On the contrary, the formation of furans, with the only exception of C(4)H(8)O, seems to be favoured at oxidizing conditions and relatively high temperatures, although mechanisms similar to those hypothesized for the production of thiophenes can be suggested. Such thermodynamic features are typical of fluid reservoirs feeding high-temperature thermal discharges of volcanoes characterised by strong degassing <span class="hlt">activity</span>, which are likely affected by conspicuous contribution from a magmatic source. The composition of heteroaromatics in fluids naturally discharged from <span class="hlt">active</span> volcanoes and geothermal areas can then be considered largely dependent on the interplay between <span class="hlt">hydrothermal</span> vs. magmatic contributions. This implies that they can be used as useful geochemical tools to be successfully applied in both <span class="hlt">volcanic</span> monitoring and geothermal prospection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2871125','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2871125"><span>Origin and Distribution of Thiophenes and Furans in Gas Discharges from <span class="hlt">Active</span> Volcanoes and Geothermal Systems</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tassi, Franco; Montegrossi, Giordano; Capecchiacci, Francesco; Vaselli, Orlando</p> <p>2010-01-01</p> <p>The composition of <span class="hlt">non</span>-methane organic volatile compounds (VOCs) determined in 139 thermal gas discharges from 18 different geothermal and <span class="hlt">volcanic</span> systems in Italy and Latin America, consists of C2–C20 species pertaining to the alkanes, alkenes, aromatics and O-, S- and N-bearing classes of compounds. Thiophenes and mono-aromatics, especially the methylated species, are strongly enriched in fluids emissions related to <span class="hlt">hydrothermal</span> systems. Addition of hydrogen sulphide to dienes and electrophilic methylation involving halogenated radicals may be invoked for the formation of these species. On the contrary, the formation of furans, with the only exception of C4H8O, seems to be favoured at oxidizing conditions and relatively high temperatures, although mechanisms similar to those hypothesized for the production of thiophenes can be suggested. Such thermodynamic features are typical of fluid reservoirs feeding high-temperature thermal discharges of volcanoes characterised by strong degassing <span class="hlt">activity</span>, which are likely affected by conspicuous contribution from a magmatic source. The composition of heteroaromatics in fluids naturally discharged from <span class="hlt">active</span> volcanoes and geothermal areas can then be considered largely dependent on the interplay between <span class="hlt">hydrothermal</span> vs. magmatic contributions. This implies that they can be used as useful geochemical tools to be successfully applied in both <span class="hlt">volcanic</span> monitoring and geothermal prospection. PMID:20480029</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1985R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1985R"><span>Signs of Recent <span class="hlt">Volcanism</span> and <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> Along the Eastern Segment of the Galapagos Spreading Center</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raineault, N.; Smart, C.; Mayer, L. A.; Ballard, R. D.; Fisher, C. R.; Marsh, L.; Shank, T. M.</p> <p>2016-12-01</p> <p>Since the initial discovery of the Galápagos Spreading Center (GSC) vents in 1977, large-scale disturbances resulting from eruptive and tectonic <span class="hlt">activity</span> have both destroyed and created vent habitats along the GSC. In 2015, the E/V Nautilus returned to the GSC with remotely operated vehicles (ROVs) to explore 17 kilometers of the rift valley from the Rosebud site in the west, to a previously unexplored temperature anomaly east of the Tempus Fugit vent site. In the years to over a decade since scientists last visited the Rosebud, Rose Garden, and Tempus Fugit sites, there were many changes. Most notably, the Rosebud site, where scientists found a nascent vent community and left site markers in 2002, was apparently covered with glassy basaltic sheet flows. In addition to visual exploration, oceanographic sensor measurements and direct sampling, we used the ROV Hercules imaging suite, comprised of stereo cameras and a structured light laser sensor to map an area of diffuse flow in the Tempus Fugit field (100 m x 150 m). The centimeter-level photographic and bathymetric maps created with this system, along with ROV HD video, samples, and environmental sensors, documented <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and changes in biological community structure (e.g., Riftia tubeworms observed in nascent stages of community development in 2011 were now, in 2015, in greater abundance (with tubes almost 4 m in length). The detection of <span class="hlt">active</span> venting and associated faunal assemblages will provide insight into the temporal and spatial variability of venting <span class="hlt">activity</span> at the Tempus Fugit site. On a visual survey of the Rift east of the Tempus Fugit site, extinct sulfide chimney structures were discovered and sampled. There were several chimneys and sulfide deposits in a span of over 8 km that ranged in height from over a half meter to 1.5 m tall. Diffuse flow hosting white and blue bacterial mats was observed near the chimneys complexes. The base of a large chimney structure, venting white fluids</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P11D..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P11D..03P"><span>Refractory Organic Compounds in Enceladus' Ice Grains and <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Postberg, F.; Khawaja, N.; Hsu, H. W.; Sekine, Y.; Shibuya, T.</p> <p>2015-12-01</p> <p>Cassini's Cosmic Dust Analyzer (CDA) generates time-of-flight mass spectra of individual grains impinging on the instruments target-plate. Following the analysis of salt rich ice grains emitted by Enceladus that indicated a salt-water ocean in contact with the moon's rocky core [1,2] a recent CDA analysis of nano-phase silica particles pointed at <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> at the moon's rock/water interface [3]. The results imply temperatures above 80 - 90°C and alkaline pH values around 10 reminiscent of alkaline <span class="hlt">hydrothermal</span> vents on Earth like the Lost City <span class="hlt">Hydrothermal</span> Field. In this context the compositional analysis of organic components in CDA mass spectra of the ejected ice grains is of particular relevance. A multitude of volatile organic species has already been identified in the gas component of the plume [4]. As expected, we find more complex organic molecules in ice grains than in the gas indicating aromatic species, amines, and carbonyl group species. The composition of organic-bearing ice grains displays a great diversity indicating a variety of different organic species in varying concentrations. Recent spatially resolved CDA in situ measurements inside Enceladus' plume indicate that these organic compounds are especially frequent in 'young' ice grains that have just been ejected by high velocity jets. We investigate the implications of our findings with respect to ice grain formation at the water surface and inside the icy vents. We constrain the generation of organic compounds at the rock/water interface in the light of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and the potential for the formation of life precursor molecules in Enceladus' ocean. Ref:[1] Postberg et al., Nature 459, 1098-1101 (2009). [2] Postberg et al., Nature 474, 620-622 (2011). [3]. Hsu, Postberg, Sekine et al., Nature, 519, 207-210 (2015). [4] Waite et al., Nature 460, 487-490 (2009).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JGRB..107.2130B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JGRB..107.2130B"><span><span class="hlt">Hydrothermal</span> venting along Earth's fastest spreading center: East Pacific Rise, 27.5°-32.3°</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baker, E. T.; Hey, R. N.; Lupton, J. E.; Resing, J. A.; Feely, R. A.; Gharib, J. J.; Massoth, G. J.; Sansone, F. J.; Kleinrock, M.; Martinez, F.; Naar, D. F.; Rodrigo, C.; Bohnenstiehl, D.; Pardee, D.</p> <p>2002-07-01</p> <p>During March/April 1998 we conducted detailed mapping and sampling of <span class="hlt">hydrothermal</span> plumes along six segments of Earth's fasting spreading mid-ocean ridge, 27.5°-32.3°S on the East Pacific Rise. We compared the distribution and chemistry of <span class="hlt">hydrothermal</span> plumes to geological indicators of long-term (spreading rate) and moderate-term (ridge inflation) variations in magmatic budget. In this large-offset, propagating rift setting, these geological indices span virtually the entire range found along fast spreading ridges worldwide. <span class="hlt">Hydrothermal</span> plumes overlaid ~60% of the length of superfast (>130 km/Myr) spreading axis surveyed and defined at least 14 separate vent fields. We observed no plumes over the slower spreading propagating segments. Finer-scale variations in the magmatic budget also correlated with <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>, as the location of the five most intense plumes corresponded to subsegment peaks in ridge inflation. Along the entire ridge crest, the more inflated a ridge location the more likely it was to be overlain by a <span class="hlt">hydrothermal</span> plume. Plume chemistry mostly reflected discharge from mature vent fields apparently unperturbed by magmatic <span class="hlt">activity</span> within the last few years. Plume samples with high volatile/metal ratios, generally indicating recent seafloor <span class="hlt">volcanism</span>, were scarce. Along-axis trends in both volatile (3He; CH4; ΔpH, a proxy for CO2; and particulate S) and nonvolatile (Fe, Mn) species showed a first-order agreement with the trend of ridge inflation. Nevertheless, a broad correspondence between the concentration of volatile species in plumes and geological proxies of magma supply identifies a pervasive magmatic imprint on this superfast spreading group of ridge segments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016158','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016158"><span>Epithermal gold-siver deposits in the western United States: time-space products of evolving plutonic, <span class="hlt">volcanic</span> and tectonic environments</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Berger, Byron R.; Bonham, Harold F.</p> <p>1990-01-01</p> <p>The western United States has been the locus of considerable subaerial <span class="hlt">volcanic</span> and plutonic igneous <span class="hlt">activity</span> since the mid-Mesozoic. After the destruction of the Jurassic-Cretaceous magmatic arc-trench system, subduction was re-established in the Late Mesozoic with low-angle underthrusting of the oceanic plate beneath western North America. This resulted in crustal shortening during the Late Cretaceous to Early Tertiary and removal of the mantle lithosphere west of the Rocky Mountains. Commencing in the Eocene, flat subduction ceased, the <span class="hlt">volcanic</span> arc began to re-establish itself along the continental margin, and the hingeline along the steepening subducting plate migrated from east to west. The crust east of the migrating hingeline was exposed to hot asthenosphere, and widespread tectonics and <span class="hlt">volcanic</span> <span class="hlt">activity</span> resulted. <span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> accompanied the <span class="hlt">volcanism</span> resulting in numerous epithermal gold-silver deposits. The temporal and spatial distributions of epithermal deposits in the region are therefore systematic and can be subdivided into discrete time intervals which are related to widespread changes in magmatic <span class="hlt">activity</span>. Time intervals selected for discussion are Pre-Cenozoic, 66-55 Ma, 54-43 Ma, 42-34 Ma, 33-24 Ma, 23-17 Ma, and <17 Ma. Many of these intervals contain both sedimentary-rock and two varieties of <span class="hlt">volcanic</span>-rock hosted deposits (adularia-sericite and alunite-kaolinite ± pyrophyllite). Continental rifting is important to the formation of deposits, and, within any given region, it is at the initiation of deep rifting that alunite-kaolinite ± pyrophyllite type epithermal deposits are formed. Adularia-sericite type deposits are most common, being related to all compositions and styles of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Therefore, the volcano-tectonic context of the western United States provides a unified framework in which to understand and explore for epithermal type deposits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014NHESS..14..485F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NHESS..14..485F"><span>Investigating <span class="hlt">volcanic</span> hazard in Cape Verde Islands through geophysical monitoring: network description and first results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faria, B.; Fonseca, J. F. B. D.</p> <p>2014-02-01</p> <p>We describe a new geophysical network deployed in the Cape Verde Archipelago for the assessment and monitoring of <span class="hlt">volcanic</span> hazards as well as the first results from the network. Across the archipelago, the ages of <span class="hlt">volcanic</span> <span class="hlt">activity</span> range from ca. 20 Ma to present. In general, older islands are in the east and younger ones are in the west, but there is no clear age progression of eruptive <span class="hlt">activity</span> as widely separated islands have erupted contemporaneously on geological timescales. The overall magmatic rate is low, and there are indications that eruptive <span class="hlt">activity</span> is episodic, with intervals between episodes of intense <span class="hlt">activity</span> ranging from 1 to 4 Ma. Although only Fogo Island has experienced eruptions (mainly effusive) in the historic period (last 550 yr), Brava and Santo Antão have experienced numerous geologically recent eruptions, including violent explosive eruptions, and show felt seismic <span class="hlt">activity</span> and geothermal <span class="hlt">activity</span>. Evidence for recent <span class="hlt">volcanism</span> in the other islands is more limited and the emphasis has therefore been on monitoring of the three critical islands of Fogo, Brava and Santo Antão, where <span class="hlt">volcanic</span> hazard levels are highest. Geophysical monitoring of all three islands is now in operation. The first results show that on Fogo, the seismic <span class="hlt">activity</span> is dominated by <span class="hlt">hydrothermal</span> events and volcano-tectonic events that may be related to settling of the edifice after the 1995 eruption; in Brava by volcano-tectonic events (mostly offshore), and in Santo Antão by volcano-tectonic events, medium-frequency events and harmonic tremor. Both in Brava and in Santo Antão, the recorded seismicity indicates that relatively shallow magmatic systems are present and causing deformation of the edifices that may include episodes of dike intrusion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000080790&hterms=Hydrology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DHydrology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000080790&hterms=Hydrology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DHydrology"><span>Hydrology in the Durius Valles Region: Evaluation of Possible Correlation with <span class="hlt">Volcanism</span> and Magnetic Anomalies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cabrol, Natalie A.; Marinangeli, Lucia; Grin, Edmond A.</p> <p>2000-01-01</p> <p>We envision the contribution of subglacial flows, <span class="hlt">hydrothermalism</span> and sapping in the Durius Valles system and the consequences in term of climate on Mars in recent geological times. We evaluate the possible correlation of the hydrology with <span class="hlt">volcanism</span> and magnetic anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JVGR..178..184V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JVGR..178..184V"><span>The <span class="hlt">volcanic</span> acidification of glacial Lake Caviahue, Province of Neuquen, Argentina</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Varekamp, Johan C.</p> <p>2008-12-01</p> <p>Lake Caviahue (northern Patagonia, Argentina) is a large glacial lake acidified by <span class="hlt">volcanic</span> fluids from Copahue volcano. The lake and the feeding rivers were sampled annually from 1997 till early 2006, including the eruptive period of 2000. Lake Caviahue waters evolved over time, with the most concentrated waters in 2000 during the eruptive period, followed by gradual dilution that was interrupted by renewed acidification in 2003-2004. Inversion of the lake water data and application of a dynamic <span class="hlt">non</span>-steady state model for the lake provides our best quantitative estimates for the variation in element fluxes over the 9-year period. The model flux results agree well with most of the measured fluxes. The Copahue <span class="hlt">hydrothermal</span> system had gently declining element fluxes between 1997 and mid-1999, although the lake was still becoming more concentrated. About 2-3 months before the 2000 eruption, element fluxes increased strongly, but the <span class="hlt">hydrothermal</span> fluxes almost shutoff directly after the main eruptive events. The fluxes of several elements recovered post-2001, with an increase in element fluxes in 2003-2004; the lake became more dilute between 2004 and 2006. The intrusion of new magma into the <span class="hlt">hydrothermal</span> system just prior to the 2000 eruption led to enhanced water rock interaction, with higher concentrations of the rock forming elements in the fluids, and the hot spring flow rate increased as a result of the higher pressure in the reservoir. The fluids became saturated in alunite and jarosite, and they were already saturated with anhydrite. Precipitation of these minerals possibly led to a decreased permeability of the <span class="hlt">hydrothermal</span> reservoir, leading to the strongly reduced element fluxes just after the eruption. In addition, K, Al and S were retained in the newly precipitated minerals as well, further diminishing their export. The acidification in 2003-2004 may have resulted from a new small intrusion of magma or resulted from seismic <span class="hlt">activity</span> that created new</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MarGR..38...71Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MarGR..38...71Y"><span>230Th/238U dating of <span class="hlt">hydrothermal</span> sulfides from Duanqiao <span class="hlt">hydrothermal</span> field, Southwest Indian Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Weifang; Tao, Chunhui; Li, Huaiming; Liang, Jin; Liao, Shili; Long, Jiangping; Ma, Zhibang; Wang, Lisheng</p> <p>2017-06-01</p> <p>Duanqiao <span class="hlt">hydrothermal</span> field is located between the Indomed and Gallieni fracture zones at the central volcano, at 50°28'E in the ultraslow-spreading Southwest Indian Ridge (SWIR). Twenty-eight subsamples from a relict chimney and massive sulfides were dated using the 230Th/238U method. Four main episodes of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> were determined according to the restricted results: 68.9-84.3, 43.9-48.4, 25.3-34.8, and 0.7-17.3 kyrs. <span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> of Duanqiao probably started about 84.3 (±0.5) kyrs ago and ceased about 0.737 (±0.023) kyrs ago. The periodic character of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> may be related to the heat source provided by the interaction of local magmatism and tectonism. The estimated mean growth rate of the sulfide chimney is <0.02 mm/yr. This study is the first to estimate the growth rate of chimneys in the SWIR. The maximum age of the relict chimney in Duanqiao <span class="hlt">hydrothermal</span> filed is close to that of the chimneys from Mt. Jourdanne (70 kyrs). The <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in Dragon Flag field is much more recent than that of Duanqiao or Mt. Jourdanne fields. The massive sulfides are younger than the sulfides from other <span class="hlt">hydrothermal</span> fields such as Rainbow, Sonne and Ashadze-2. The preliminarily estimated reserves of sulfide ores of Duanqiao are approximately 0.5-2.9 million tons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..341..104R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..341..104R"><span>Structural controls on fluid circulation at the Caviahue-Copahue <span class="hlt">Volcanic</span> Complex (CCVC) geothermal area (Chile-Argentina), revealed by soil CO2 and temperature, self-potential, and helium isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roulleau, Emilie; Bravo, Francisco; Pinti, Daniele L.; Barde-Cabusson, Stéphanie; Pizarro, Marcela; Tardani, Daniele; Muñoz, Carlos; Sanchez, Juan; Sano, Yuji; Takahata, Naoto; de la Cal, Federico; Esteban, Carlos; Morata, Diego</p> <p>2017-07-01</p> <p>Natural geothermal systems are limited areas characterized by anomalously high heat flow caused by recent tectonic or magmatic <span class="hlt">activity</span>. The heat source at depth is the result of the emplacement of magma bodies, controlled by the regional volcano-tectonic setting. In contrast, at a local scale a well-developed fault-fracture network favors the development of <span class="hlt">hydrothermal</span> cells, and promotes the vertical advection of fluids and heat. The Southern <span class="hlt">Volcanic</span> Zone (SVZ), straddling Chile and Argentina, has an important, yet unexplored and undeveloped geothermal potential. Studies on the lithological and tectonic controls of the <span class="hlt">hydrothermal</span> circulation are therefore important for a correct assessment of the geothermal potential of the region. Here, new and dense self-potential (SP), soil CO2 and temperature (T) measurements, and helium isotope data measured in fumaroles and thermal springs from the geothermal area located in the north-eastern flank of the Copahue <span class="hlt">volcanic</span> edifice, within the Caviahue Caldera (the Caviahue-Copahue <span class="hlt">Volcanic</span> Complex - CCVC) are presented. Our results allowed to the constraint of the structural origin of the <span class="hlt">active</span> thermal areas and the understanding of the evolution of the geothermal system. NE-striking faults in the area, characterized by a combination of SP, CO2, and T maxima and high 3He/4He ratios (up to 8.16 ± 0.21Ra, whereas atmospheric Ra is 1.382 × 10- 6), promote the formation of vertical permeability preferential pathways for fluid circulation. WNW-striking faults represent low-permeability pathways for <span class="hlt">hydrothermal</span> fluid ascent, but promote infiltration of meteoric water at shallow depths, which dilute the <span class="hlt">hydrothermal</span> input. The region is scattered with SP, CO2, and T minima, representing self-sealed zones characterized by impermeable altered rocks at depth, which create local barriers for fluid ascent. The NE-striking faults seem to be associated with the upflowing zones of the geothermal system, where the boiling process</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.6053N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.6053N"><span>Submarine <span class="hlt">Volcanic</span> Morphology of Santorini Caldera, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nomikou, P.; Croff Bell, K.; Carey, S.; Bejelou, K.; Parks, M.; Antoniou, V.</p> <p>2012-04-01</p> <p>Santorini <span class="hlt">volcanic</span> group form the central part of the modern Aegean <span class="hlt">volcanic</span> arc, developed within the Hellenic arc and trench system, because of the ongoing subduction of the African plate beneath the European margin throughout Cenozoic. It comprises three distinct <span class="hlt">volcanic</span> structures occurring along a NE-SW direction: Christianna form the southwestern part of the group, Santorini occupies the middle part and Koloumbo <span class="hlt">volcanic</span> rift zone extends towards the northeastern part. The geology of the Santorini volcano has been described by a large number of researchers with petrological as well as geochronological data. The offshore area of the Santorini <span class="hlt">volcanic</span> field has only recently been investigated with emphasis mainly inside the Santorini caldera and the submarine volcano of Kolumbo. In September 2011, cruise NA-014 on the E/V Nautilus carried out new surveys on the submarine <span class="hlt">volcanism</span> of the study area, investigating the seafloor morphology with high-definition video imaging. Submarine <span class="hlt">hydrothermal</span> vents were found on the seafloor of the northern basin of the Santorini caldera with no evidence of high temperature fluid discharges or massive sulphide formations, but only low temperature seeps characterized by meter-high mounds of bacteria-rich sediment. This vent field is located in line with the normal fault system of the Kolumbo rift, and also near the margin of a shallow intrusion that occurs within the sediments of the North Basin. Push cores have been collected and they will provide insights for their geochemical characteristics and their relationship to the <span class="hlt">active</span> vents of the Kolumbo underwater volcano. Similar vent mounds occur in the South Basin, at shallow depths around the islets of Nea and Palaia Kameni. ROV exploration at the northern slopes of Nea Kameni revealed a fascinating underwater landscape of lava flows, lava spines and fractured lava blocks that have been formed as a result of 1707-1711 and 1925-1928 AD eruptions. A hummocky topography at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V51A3035S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V51A3035S"><span>Magnesium isotopic behavior during the formation of chlorite-rich <span class="hlt">hydrothermal</span> sediment in the middle Okinawa Trough</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shao, H.; Yang, S.; Teng, F. Z.; Cai, D.; Humphris, S. E.</p> <p>2016-12-01</p> <p>Chlorite is a common alteration product during water-rock reactions in seafloor <span class="hlt">hydrothermal</span> systems. This chlorite is commonly characterized by high concentrations of magnesium. However, the source of the Mg and its behavior during <span class="hlt">hydrothermal</span> alteration have yet to be clarified. Mg isotopes have been used in recent years to investigate a variety of geological processes, including low temperature weathering and metamorphism processes, and Mg cycling in sediments. In this study, we investigate the source of Mg and its behavior in chlorite-rich sediments collected during IODP Expedition 331 from the <span class="hlt">active</span> <span class="hlt">hydrothermal</span> Iheya North Knoll field in the middle Okinawa Trough — an intra-continental rift in continental crust. This area is characterized by hemipelagic muds with interbedded thick layers of felsic pumiceous <span class="hlt">volcanic</span> material. Based on mineralogical, geochemical, and isotopic data, we have previously suggested that the chlorite-rich sediments resulted from <span class="hlt">hydrothermal</span> alteration of the pumiceous layers at temperatures of 220-300°C. Prior to Mg isotope analysis, all selected samples were pretreated with 1N HCl in order to remove carbonates and other unstable minerals, and measurements were made on both the residues (mainly chlorite) and leachates, as well as on bulk samples. The residues are expected to show higher δ26Mg than the leachates reflecting the Mg isotopic signature of the pumiceous material precursor and provide insight into the behavior of Mg isotopes during the high-temperature <span class="hlt">hydrothermal</span> processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V41A..08D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V41A..08D"><span>Fluid and Melt Inclusions as a tool to understand two high risk <span class="hlt">volcanic</span> systems: Vesuvius and Campi Flegrei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Vivo, B.</p> <p>2017-12-01</p> <p>In the Campania region (Southern Italy) major <span class="hlt">active</span> <span class="hlt">volcanic</span> systems occur in the greater metropolitan area of Naples: Mt. Somma-Vesuvius (SV) and the Campi Flegrei (CF). These <span class="hlt">volcanic</span> systems have been studied for centuries, yet significant differences of opinions exist about their origins and behaviors. Here, I present some alternative views on issues based on more than 25 years of research, focusing the attention on role played by fluids and magmas based on fluid inclusions (FI) and melt inclusions (MI). In particular, FI and MI data from the Neapolitan volcanoes provide valuable information on the nature of fluid and melt phases trapped during the late evolutionary stages of the alkaline magmatic rocks; such data from past eruptions might be applied to predict the imminence of <span class="hlt">volcanic</span> eruptions and help protect the population from such hazards. In my and my collaborator studies, FI and MI data have been also used to address the problem of bradyseism in the CF. Using FI and MI, to explain the bradyseism phenomena at CF, my collaborators and I described a new model that involves only <span class="hlt">hydrothermal</span> fluids of magmatic or meteoric/marine origin with no direct involvement of the magma, other than as a heat source to explain the ground deformation. My collaborators and I explain the bradyseism as a purely <span class="hlt">hydrothermal</span> model, using processes in porphyry systems as an analogue to those of the CF. SV <span class="hlt">activity</span> is characterized by cyclic events, and in terms of <span class="hlt">volcanic</span> risk assessment, a crucial aspect to understand is when a potential next explosive eruption might occur. Evaluating <span class="hlt">volcanic</span> hazards requires knowledge of the processes that trigger eruptions and the nature and timing of geophysical/geochemical signals related to these processes. One approach to addressing this need is to link observable signals to pre-eruptive magmatic events deduced from studies of erupted magmas. I believe that a way to work in this direction is to determine the residence time, through</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..356...24C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..356...24C"><span>Multi-year high-frequency <span class="hlt">hydrothermal</span> monitoring of selected high-threat Cascade Range volcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crankshaw, I. M.; Archfield, S. A.; Newman, A. C.; Bergfeld, D.; Clor, L. E.; Spicer, K. R.; Kelly, P. J.; Evans, W. C.; Ingebritsen, S. E.</p> <p>2018-05-01</p> <p>From 2009 to 2015 the U.S. Geological Survey (USGS) systematically monitored <span class="hlt">hydrothermal</span> behavior at selected Cascade Range volcanoes in order to define baseline <span class="hlt">hydrothermal</span> and geochemical conditions. Gas and water data were collected regularly at 25 sites on 10 of the highest-risk volcanoes in the Cascade Range. These sites include near-summit fumarole groups and springs/streams that show clear evidence of magmatic influence (high 3He/4He ratios and/or large fluxes of magmatic CO2 or heat). Site records consist mainly of hourly temperature and <span class="hlt">hydrothermal</span>-flux data. Having established baseline conditions during a multiyear quiescent period, the USGS reduced monitoring frequency from 2015 to present. The archived monitoring data are housed at (doi:10.5066/F72N5088). These data (1) are suitable for retrospective comparison with other continuous geophysical monitoring data and (2) will provide context during future episodes of <span class="hlt">volcanic</span> unrest, such that unrest-related variations at these thoroughly characterized sites will be more clearly recognizable. Relatively high-frequency year-round data are essential to achieve these objectives, because many of the time series reveal significant diurnal, seasonal, and inter-annual variability that would tend to mask unrest signals in the absence of baseline data. Here we characterize normal variability for each site, suggest strategies to detect future <span class="hlt">volcanic</span> unrest, and explore deviations from background associated with recent unrest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NHESD...1.4997F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NHESD...1.4997F"><span>Investigating <span class="hlt">volcanic</span> hazard in Cape Verde Islands through geophysical monitoring: network description and first results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faria, B.; Fonseca, J. F. B. D.</p> <p>2013-09-01</p> <p>We describe a new geophysical network deployed in the Cape Verde archipelago for the assessment and monitoring of <span class="hlt">volcanic</span> hazards, and the first results from the network. Across the archipelago, the ages of <span class="hlt">volcanic</span> <span class="hlt">activity</span> range from ca. 20 Ma to present. In general, older islands are in the east and younger ones are in the west, but there is no clear age progression and widely-separated islands have erupted contemporaneously on geological time scales. The overall magmatic rate is low, and there are indications that eruptive <span class="hlt">activity</span> is episodic, with intervals between episodes of intense <span class="hlt">activity</span> ranging from 1 to 4 Ma. Although only Fogo island has experienced eruptions (mainly effusive) in the historic period (last 550 yr), Brava and Santo Antão have experienced numerous geologically recent eruptions including violent explosive eruptions, and show felt seismic <span class="hlt">activity</span> and geothermal <span class="hlt">activity</span>. Evidence for recent <span class="hlt">volcanism</span> in the other islands is more limited and the emphasis has therefore been on monitoring of the three critical islands of Fogo, Brava and Santo Antão, where <span class="hlt">volcanic</span> hazard levels are highest. Geophysical monitoring of all three islands is now in operation. The first results show that in Fogo the seismic <span class="hlt">activity</span> is dominated by <span class="hlt">hydrothermal</span> events and volcano-tectonic events that may be related to settling of the edifice after the 1995 eruption; in Brava by volcano-tectonic events (mostly offshore), and in Santo Antão by volcano-tectonic events, medium frequency events and harmonic tremor. Both in Brava and in Santo Antão, the recorded seismicity indicates that relatively shallow magmatic systems are present and causing deformation of the edifices that may include episodes of dike intrusion.</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/2017JAfES.134..299E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAfES.134..299E"><span><span class="hlt">Hydrothermal</span> barite mineralization at Chenarvardeh deposit, Markazi Province, Iran: Evidences from REE geochemistry and fluid inclusions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ehya, Farhad; Mazraei, Shaghayegh Moalaye</p> <p>2017-10-01</p> <p>Barite mineralization occurs at Chenarvardeh deposit as layers and lenses in Upper Eocene <span class="hlt">volcanic</span> and pyroclastic rocks. The host rocks are intensely saussuritized in most places. Barite is accompanied by calcite, Mn-oxides, galena and malachite as subordinate minerals. The amount of Sr in barites is low and varies between 0.11 and 0.30 wt%. The concentration of Rb, Zr, Y, Ta and Hf is also low (<5 ppm) in barite samples. The amount of total REEs (∑REE) is low in barites, ranging from 7.51 to 30.50 ppm. Chondrite-normalized REE patterns reveal LREE enrichment with respect to HREE, and positive Ce anomalies. Fluid inclusions are common in barite samples, being dominantly from liquid-rich two phase (L + V) type. Salinity values in fluid inclusions range from 9.41 to 18.69 wt% NaCl equivalent with most frequent salinities falling in the range of 10-15 wt% NaCl equivalent. Homogenization temperatures (Th) range between 160 and 220 °C, being the 180-200 °C range as the most common Th interval. A combination of factors, including geologic setting, host rock, mineral assemblages, REE geochemistry and fluid inclusion data are consistent with a submarine <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> model for barite formation at the Chenarvardeh deposit. Mineral-forming fluids originated from solutions related to submarine <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> deposited barite on seafloor as they encountered sulfate-bearing seawater.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050175907','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050175907"><span>An Approach to In-Situ Observations of <span class="hlt">Volcanic</span> Plumes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smythe, W. D.; Lopes, M. C.; Pieri, D. C.; Hall, J. L.</p> <p>2005-01-01</p> <p>Volcanoes have long been recognized as playing a dominant role in the birth, and possibly the death, of biological populations. They are possible sources of primordial gases, provide conditions sufficient for creating amino acids, strongly affect the heat balance in the atmosphere, and have been shown to sustain life (in oceanic vents.) Eruptions can have profound effects on local flora and fauna, and for very large eruptions, may alter global weather patterns and cause entire species to fail. Measurements of particulates, gases, and dynamics within a <span class="hlt">volcanic</span> plume are critical to understanding both how volcanoes work and how plumes affect populations, environment, and aviation. <span class="hlt">Volcanic</span> plumes and associated eruption columns are a miasma of toxic gases, corrosive condensates, and abrasive particulates that makes them hazardous to nearby populations and poses a significant risk to all forms of aviation. Plumes also provide a mechanism for sampling the <span class="hlt">volcanic</span> interior, which, for <span class="hlt">hydrothermal</span> environments, may host unique biological populations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..357..186C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..357..186C"><span>Volcano-<span class="hlt">hydrothermal</span> system and <span class="hlt">activity</span> of Sirung volcano (Pantar Island, Indonesia)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caudron, Corentin; Bernard, Alain; Murphy, Sam; Inguaggiato, Salvatore; Gunawan, Hendra</p> <p>2018-05-01</p> <p>Sirung is a frequently <span class="hlt">active</span> volcano located in the remote parts of Western Timor (Indonesia). Sirung has a crater with several <span class="hlt">hydrothermal</span> features including a crater lake. We present a timeseries of satellite images of the lake and chemical and isotope data from the hyperacid <span class="hlt">hydrothermal</span> system. The fluids sampled in the crater present the typical features of hyperacidic systems with high TDS, low pH and δ34SHSO4-δ34SS0 among the highest for such lakes. The cations concentrations are predominantly controlled by the precipitation of alunite, jarosite, silica phases, native sulfur and pyrite which dominate the shallow portions of the <span class="hlt">hydrothermal</span> system. These minerals may control shallow sealing processes thought to trigger phreatic eruptions elsewhere. Sparse Mg/Cl and SO4/Cl ratios and lake parameters derived from satellite images suggest gradual increase in heat and gas flux, most likely SO2-rich, prior to the 2012 phreatic eruption. An acidic river was sampled 8 km far from the crater and is genetically linked with the fluids rising toward the <span class="hlt">active</span> crater. This river would therefore be a relevant target for future remote monitoring purposes. Finally, several wells and springs largely exceeded the World Health Organization toxicity limits in total arsenic and fluoride.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014761','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014761"><span><span class="hlt">Volcanism</span> and massive sulfide formation at a sedimented spreading center, Escanaba Trough, Gorda Ridge, northeast Pacific.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Morton, J.L.; Holmes, M.L.; Koski, R.A.</p> <p>1987-01-01</p> <p>Seismic-reflection profiles over the sediment-filled Escanaba Trough at the southern Gorda Ridge reveal a series of <span class="hlt">volcanic</span> centers that pierce the sediment. The <span class="hlt">volcanic</span> edifices are 3 to 6 km in diameter and are spaced at 15 to 20 km intervals along the axis of the trough. Composition and form of sulfide samples obtained from the bank suggest significant interaction between <span class="hlt">hydrothermal</span> fluids and sediment at depth, and deposition of sulfide within the sediment pile.-from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17755532','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17755532"><span>The effect of magmatic <span class="hlt">activity</span> on <span class="hlt">hydrothermal</span> venting along the superfast-spreading East pacific rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Urabe, T; Baker, E T; Ishibashi, J; Feely, R A; Marumo, K; Massoth, G J; Maruyama, A; Shitashima, K; Okamura, K; Lupton, J E; Sonoda, A; Yamazaki, T; Aoki, M; Gendron, J; Greene, R; Kaiho, Y; Kisimoto, K; Lebon, G; Matsumoto, T; Nakamura, K; Nishizawa, A; Okano, O; Paradis, G; Roe, K; Shibata, T; Tennant, D; Vance, T; Walker, S L; Yabuki, T; Ytow, N</p> <p>1995-08-25</p> <p>A survey of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> along the superfast-spreading (approximately 150 millimeters per year) East Pacific Rise shows that <span class="hlt">hydrothermal</span> plumes overlay approximately 60 percent of the ridge crest between 13 degrees 50' and 18 degrees 40'S, a plume abundance nearly twice that known from any other rige portion of comparable length. Plumes were most abundant where the axial cross section is inflated and an axial magma chamber is present. Plumes with high ratios of volatile ((3)He, CH(4), and H(2)S) to nonvolatile (Mn and Fe) species marked where <span class="hlt">hydrothermal</span> circulation has been perturbed by recent magmatic <span class="hlt">activity</span>. The high proportion of volatile-rich plumes observed implies that such episodes are more frequent here than on slower spreading ridges.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4595843','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4595843"><span><span class="hlt">Volcanic</span> passive margins: another way to break up continents</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Geoffroy, L.; Burov, E. B.; Werner, P.</p> <p>2015-01-01</p> <p>Two major types of passive margins are recognized, i.e. <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span>, without proposing distinctive mechanisms for their formation. <span class="hlt">Volcanic</span> passive margins are associated with the extrusion and intrusion of large volumes of magma, predominantly mafic, and represent distinctive features of Larges Igneous Provinces, in which regional fissural <span class="hlt">volcanism</span> predates localized syn-magmatic break-up of the lithosphere. In contrast with <span class="hlt">non-volcanic</span> margins, continentward-dipping detachment faults accommodate crustal necking at both conjugate <span class="hlt">volcanic</span> margins. These faults root on a two-layer deformed ductile crust that appears to be partly of igneous nature. This lower crust is exhumed up to the bottom of the syn-extension extrusives at the outer parts of the margin. Our numerical modelling suggests that strengthening of deep continental crust during early magmatic stages provokes a divergent flow of the ductile lithosphere away from a central continental block, which becomes thinner with time due to the flow-induced mechanical erosion acting at its base. Crustal-scale faults dipping continentward are rooted over this flowing material, thus isolating micro-continents within the future oceanic domain. Pure-shear type deformation affects the bulk lithosphere at VPMs until continental breakup, and the geometry of the margin is closely related to the dynamics of an <span class="hlt">active</span> and melting mantle. PMID:26442807</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26442807','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26442807"><span><span class="hlt">Volcanic</span> passive margins: another way to break up continents.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Geoffroy, L; Burov, E B; Werner, P</p> <p>2015-10-07</p> <p>Two major types of passive margins are recognized, i.e. <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span>, without proposing distinctive mechanisms for their formation. <span class="hlt">Volcanic</span> passive margins are associated with the extrusion and intrusion of large volumes of magma, predominantly mafic, and represent distinctive features of Larges Igneous Provinces, in which regional fissural <span class="hlt">volcanism</span> predates localized syn-magmatic break-up of the lithosphere. In contrast with <span class="hlt">non-volcanic</span> margins, continentward-dipping detachment faults accommodate crustal necking at both conjugate <span class="hlt">volcanic</span> margins. These faults root on a two-layer deformed ductile crust that appears to be partly of igneous nature. This lower crust is exhumed up to the bottom of the syn-extension extrusives at the outer parts of the margin. Our numerical modelling suggests that strengthening of deep continental crust during early magmatic stages provokes a divergent flow of the ductile lithosphere away from a central continental block, which becomes thinner with time due to the flow-induced mechanical erosion acting at its base. Crustal-scale faults dipping continentward are rooted over this flowing material, thus isolating micro-continents within the future oceanic domain. Pure-shear type deformation affects the bulk lithosphere at VPMs until continental breakup, and the geometry of the margin is closely related to the dynamics of an <span class="hlt">active</span> and melting mantle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940016164&hterms=1043&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D%2526%25231043','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940016164&hterms=1043&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D%2526%25231043"><span>SO2 on Venus: IUE, HST and ground-based measurements, and the <span class="hlt">active</span> <span class="hlt">volcanism</span> connection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Na, C. Y.; Barker, E. S.; Stern, S. A.; Esposito, L. W.</p> <p>1993-01-01</p> <p>Magellan images have shown that the <span class="hlt">volcanic</span> features are widespread over the surface of Venus. The question of whether there is <span class="hlt">active</span> <span class="hlt">volcanism</span> is important for understanding both the atmospheric and the geological processes on Venus. The thick cloud cover of Venus precludes any direct observation of <span class="hlt">active</span> volcanoes even if they exist. The only means of monitoring the <span class="hlt">active</span> <span class="hlt">volcanism</span> on Venus at present seems to be remote sensing from Earth. Continuous monitoring of SO2 is important to establish the long term trend of SO2 abundance and to understand the physical mechanism responsible for the change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA602884','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA602884"><span>Impact of <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> on AMC Channel Operations</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-06-13</p> <p><span class="hlt">active</span> <span class="hlt">volcanic</span> settings in the world. The location and behavior of volcanoes are a direct result of tectonic plate boundaries and the dynamic nature...Figure 2: Ash Detected Outside Iceland within 40°–70°N and 40°W–30°E (Scientific Reports, 2014) The potential for tectonic plate movement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.V11B1937B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.V11B1937B"><span>Gravitational Failures of Lava Domes at Intersections With Tectonic Faults: Examples from Tatun <span class="hlt">Volcanic</span> Group, Northern Taiwan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belousova, M.; Belousov, A.; Chen, C.</p> <p>2009-12-01</p> <p> disintegration: material of the collapse is represented by big boulders with few fine grained matrix. Collapses of Cigu and Dajianhou volcanoes had the smallest volumes, ~ 0.01 km3, and their character is transitional to large rockfalls. The studied collapses occurred after the volcanoes had stopped erupting, and thus were not triggered by <span class="hlt">volcanic</span> <span class="hlt">activity</span>. <span class="hlt">Hydrothermally</span> altered rocks do not compose significant parts of the studied debris avalanches, although <span class="hlt">hydrothermal</span> fields are common in the scars of the collapses. Probably weakening of mechanical properties of the <span class="hlt">volcanic</span> edifices due to <span class="hlt">hydrothermal</span> alteration did not play a key role in the studied collapses, but elevated fluid pressure and <span class="hlt">hydrothermal</span> alteration in the foundations of the volcanoes might have had some role. Scars of the collapses are located on intersections of the edifices with <span class="hlt">active</span> tectonic faults of NNE-SSW and/or W-E strike, which are expressed in relief and clearly visible on space images. Thus, the collapsed parts of the <span class="hlt">volcanic</span> edifices were detached by tectonic motions, and the collapses were possibly triggered by seismic <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1983/0068/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1983/0068/report.pdf"><span>Eruptive history of the Dieng Mountains region, central Java, and potential hazards from future eruptions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Miller, C. Dan; Sushyar, R.; ,; Hamidi, S.</p> <p>1983-01-01</p> <p>The Dieng Mountains region consists of a complex of late Quaternary to recent <span class="hlt">volcanic</span> stratocones, parasitic vents, and explosion craters. Six age groups of <span class="hlt">volcanic</span> centers, eruptive products, and explosion craters are recognized in the region based on their morphology, degree of dissection, stratigraphic relationships, and degree of weathering. These features range in age from tens of thousands of years to events that have occurred this century. No magmatic eruptions have occurred in the Dieng Mountains region for at least several thousand years; <span class="hlt">volcanic</span> <span class="hlt">activity</span> during this time interval has consisted of phreatic eruptions and <span class="hlt">non</span>-explosive <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. If future <span class="hlt">volcanic</span> events are similar to those of the last few thousand years, they will consist of phreatic eruptions, associated small hot mudflows, emission of suffocating gases, and <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Future phreatic eruptions may follow, or accompany, periods of increased earthquake <span class="hlt">activity</span>; the epicenters for the seismicity may suggest where eruptive <span class="hlt">activity</span> will occur. Under such circumstances, the populace within several kilometers of a potential eruption site should be warned of a possible eruption, given instructions about what to do in the event of an eruption, or temporarily evacuated to a safer location.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992Tectp.206..245B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992Tectp.206..245B"><span>Morphostructural study and type of <span class="hlt">volcanism</span> of submarine volcanoes over the Pitcairn hot spot in the South Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Binard, Nicolas; Hékinian, Roger; Stoffers, Peter</p> <p>1992-06-01</p> <p>Undersea volcanoes found at about 80 km southeast of the island of Pitcairn, are believed to be the manifestation of a hot-spot <span class="hlt">activity</span> located near 129°30'W 25°10'S, along the strike of the Mururoa-Gambier-Pitcairn <span class="hlt">volcanic</span> alignment. <span class="hlt">Hydrothermal</span> <span class="hlt">activities</span> and recent <span class="hlt">volcanic</span> flows were observed on the two largest (20 km in basal diameter) and shallowest (60 m and 450 m depth) volcanoes. More than twenty other smaller <span class="hlt">volcanic</span> edifices ( < 500 m in height) were mapped during a Seabeam survey covering an area of about 8000 km 2. The edifices from the Pitcairn region are conical with a low degree of flatness (summit/basal diameters ratio <0.25), and consist of fresh alkali-enriched lava flows. The other truncated edifices with a high degree of flatness ( > 0.25) made up of ancient MORB-type tholeiitic rocks are inferred to be inherited from the EPR axial regions. The shallow <span class="hlt">volcanic</span> <span class="hlt">activity</span> which occurred on the two largest edifices are classified as: (1) reactive eruptions, with hydromagmatic <span class="hlt">activities</span>, giving rise to <span class="hlt">volcanic</span> ejecta, bombs, xenoliths, and ash, and (2) quiet eruptions which formed pillows and/or lobated lavas, and large massive flows. Intrusives (dyke and sill) were observed, cutting through the <span class="hlt">volcanic</span> ejecta near the summit ( < 500 m depth) of the seamounts. The general structural orientations of the rift zones recognized from the bathymetry of individual volcanoes (N160°-180°, N80°, N30° and N120°) are comparable to those observed in the Society and Austral hot-spot regions. These orientations were inferred as corresponding to the structural discontinuities of the ancient oceanic crust, and to the regional stress field of the Pacific plate. Rock samples from the Pitcairn region consist of alkali-basalts, basanites, trachyandesites, and trachytes which are closer in chemical composition to some of the <span class="hlt">volcanics</span> from the Society rather than to those from the Austral hot-spot regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMS...181....1L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMS...181....1L"><span>Tectonic environments and local geologic controls of potential <span class="hlt">hydrothermal</span> fields along the Southern Mid-Atlantic Ridge (12-14°S)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Bing; Shi, Xuefa; Wang, Jixin; Yan, Quanshu; Liu, Chenguang; DY125-21 (Leg 3) Science Party; DY125-22 (Legs 2-5) Science Party; DY125-26 (Leg 3) Science Party</p> <p>2018-05-01</p> <p>Systematic <span class="hlt">hydrothermal</span> exploration and multi-beam bathymetry mapping have been conducted along a 220-km-long section of the Southern Mid-Atlantic Ridge (SMAR) from 12°S (Bode Verde Fracture Zone) to 14°S (Cardno Fracture Zone), and previously reported deposits (Tao et al., 2011) are now being thoroughly investigated. Here, we present the characterization of three possible <span class="hlt">hydrothermal</span> fields, a complete bathymetry data set of the ridge segment, gravity data, and the petrologic characteristics of collected rock samples. The magmatism characteristics, evolution of the ridge segment, and the local geological controls of the possible <span class="hlt">hydrothermal</span> fields are then discussed. The studied segment can be divided into two segments by a <span class="hlt">Non</span>-Transform Discontinuity (NTD). Our morphotectonic analysis shows significant along-axis heterogeneity in the surveyed segments: three distinctive cross-axis grabens were identified in the northern segment, and two were identified in the southern segment. Moreover, based on the gravity data (a relatively low spherical Bouguer anomaly) and petrologic data (low Mg# values and relatively low FeO and relatively high Al2O3 and CaO contents compared to nearby seafloor samples), a <span class="hlt">volcanic</span> feature, the ZouYu seamount, on this segment is considered to be associated with strong magmatic <span class="hlt">activity</span>, and the magmatic <span class="hlt">activity</span> of the inside corner at the southern end of the segment has increased and decreased. The three possible <span class="hlt">hydrothermal</span> fields occur in different local geological settings: a shallow magmatic seamount (ZouYu), an NTD (TaiJi), and an inside-corner high (CaiFan). These potential <span class="hlt">hydrothermal</span> fields are significantly different from other fields in similar tectonic settings in terms of local geologic controls and products. The ZouYu field is primarily related to a newly formed cone, resulting in the production of sulfides, and differs from other fields on shallow magmatic seamounts. The TaiJi field is largely controlled by the tectonic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014366','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014366"><span>Mineral and whole-rock compositions of seawater-dominated <span class="hlt">hydrothermal</span> alteration at the Arctic volcanogenic massive sulfide prospect, Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Schmidt, J.M.</p> <p>1988-01-01</p> <p>The Arctic volcanogenic massive sulfide prospect, located in the Ambler mineral district of northwestern Alaska, includes three types of <span class="hlt">hydrothermally</span> altered rocks overlying, underlying, and interlayered with semimassive sulfide mineralization. <span class="hlt">Hydrothermal</span> alteration of wall rocks and deposition of sulfide and gangue minerals were contemporaneous with Late Devonian of Early Mississippian basalt-rhyolite <span class="hlt">volcanism</span>. Alteration developed asymmetrically around a linear fissure, suggesting fracture control of ore fluids rather than a point source. Microprobe analyses of phyllosilicates from the Arctic area indicate two discrete mineral populations. These differences in mineral chemistry are the result of differences in protolith composition caused by <span class="hlt">hydrothermal</span> alteration-metasomatism. -from Author</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS22A..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS22A..07S"><span>Discovery of Nascent Vents and Recent Colonization Associated with(Re)<span class="hlt">activated</span> <span class="hlt">Hydrothermal</span> Vent Fields by the GALREX 2011 Expedition on the Galápagos Rift</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shank, T. M.; Holden, J. F.; Herrera, S.; Munro, C.; Muric, T.; Lin, J.; Stuart, L.</p> <p>2011-12-01</p> <p>GALREX 2011 was a NOAA OER telepresence cruise that explored the diverse habitats and geologic settings of the deep Galápagos region. The expedition made12 Little Hercules ROV dives in July 2011.Abundant corals and a strong depth zonation of species (including deepwater coral communities) were found near 500 m depth on Paramount Seamount, likely influenced by past low sea level states, wave-cut terrace processes, and the historical presence of shallow reef structures. At fresh lava flows with associated (flocculent) <span class="hlt">hydrothermal</span> venting near 88° W, now known as Uka Pacha and Pegasus Vent Fields, rocks were coated with white microbial mat and lacked sessile fauna, with few mobile fauna (e.g., bythograeid crabs, alvinocarid shrimp, polynoid worms, zoarcid fish, and dirivultid copepods). This suggests a recent creation of <span class="hlt">hydrothermal</span> habitats through <span class="hlt">volcanic</span> eruptions and/or diking events, which may have taken place over a 15 km span separating the two vent fields. The Rosebud vent field at 86°W was not observed and may have been covered with lava since last visited in 2005. A <span class="hlt">hydrothermal</span> vent field near 86°W was discovered that is one of the largest vent fields known on the Rift (120m by 40m). Low-temperature vent habitats were colonized by low numbers of tubeworms including Riftia, Oasisia, and a potential Tevnia species (the latter not previously observed on the Galapagos Rift). Patches of tubeworms were observed with individuals less than 2cm in length, and the relatively few large Riftia had tube lengths near 70cm long. Large numbers of small (< 3cm long) bathymodiolin mussels lined cracks and crevices throughout the <span class="hlt">active</span> part of the field. Live clams, at least four species of gastropod limpets, three species of polynoid polychaetes, juvenile and adult alvinocarid shrimp, actinostolid anemones, and white microbial communities were observed on the underside and vertical surfaces of basalt rock surfaces. There were at least 13 species of vent-endemic fauna</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140002345','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140002345"><span>Multi-Source Autonomous Response for Targeting and Monitoring of <span class="hlt">Volcanic</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davies, Ashley G.; Doubleday, Joshua R.; Tran, Daniel Q.</p> <p>2014-01-01</p> <p>The study of volcanoes is important for both purely scientific and human survival reasons. From a scientific standpoint, <span class="hlt">volcanic</span> gas and ash emissions contribute significantly to the terrestrial atmosphere. Ash depositions and lava flows can also greatly affect local environments. From a human survival standpoint, many people live within the reach of <span class="hlt">active</span> volcanoes, and therefore can be endangered by both atmospheric (ash, debris) toxicity and lava flow. There are many potential information sources that can be used to determine how to best monitor <span class="hlt">volcanic</span> <span class="hlt">activity</span> worldwide. These are of varying temporal frequency, spatial regard, method of access, and reliability. The problem is how to incorporate all of these inputs in a general framework to assign/task/reconfigure assets to monitor events in a timely fashion. In situ sensing can provide a valuable range of complementary information such as seismographic, discharge, acoustic, and other data. However, many volcanoes are not instrumented with in situ sensors, and those that have sensor networks are restricted to a relatively small numbers of point sensors. Consequently, ideal <span class="hlt">volcanic</span> study synergistically combines space and in situ measurements. This work demonstrates an effort to integrate spaceborne sensing from MODIS (Terra and Aqua), ALI (EO-1), Worldview-2, and in situ sensing in an automated scheme to improve global volcano monitoring. Specifically, it is a "sensor web" concept in which a number of volcano monitoring systems are linked together to monitor <span class="hlt">volcanic</span> <span class="hlt">activity</span> more accurately, and this <span class="hlt">activity</span> measurement automatically tasks space assets to acquire further satellite imagery of ongoing <span class="hlt">volcanic</span> <span class="hlt">activity</span>. A general framework was developed for evidence combination that accounts for multiple information sources in a scientist-directed fashion to weigh inputs and allocate observations based on the confidence of an events occurrence, rarity of the event at that location, and other scientists</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2017/5077/sir20175077.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2017/5077/sir20175077.pdf"><span>2014 <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Alaska: Summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cameron, Cheryl E.; Dixon, James P.; Neal, Christina A.; Waythomas, Christopher F.; Schaefer, Janet R.; McGimsey, Robert G.</p> <p>2017-09-07</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptions, possible eruptions, <span class="hlt">volcanic</span> unrest or suspected unrest, and seismic events at 18 <span class="hlt">volcanic</span> centers in Alaska during 2014. The most notable <span class="hlt">volcanic</span> <span class="hlt">activity</span> consisted of intermittent ash eruptions from long-<span class="hlt">active</span> Cleveland and Shishaldin Volcanoes in the Aleutian Islands, and two eruptive episodes at Pavlof Volcano on the Alaska Peninsula. Semisopochnoi and Akutan volcanoes had seismic swarms, both likely the result of magmatic intrusion. The AVO also installed seismometers and infrasound instruments at Mount Cleveland during 2014.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000080681&hterms=interesting+pdf&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dinteresting%2Bpdf','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000080681&hterms=interesting+pdf&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dinteresting%2Bpdf"><span>Identification of Crystalline Minerals in <span class="hlt">Volcanic</span> Alteration Products and Applications to the Surface of Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bishop, J. L.; Madsen, M. B.; Murad, E.; Wagner, P. A.</p> <p>2000-01-01</p> <p>Visible, infrared and Mossbauer spectra have been measured for fine-grained alteration products of <span class="hlt">volcanic</span> tephra and ash. Comparison of the spectral and chemical properties for different size separates and related samples provides information about the crystalline materials in these samples and how they may have formed. <span class="hlt">Hydrothermal</span> processes can increase the alteration rates of the primary minerals and glass and provide S, Fe and/or water for formation of sulfates and hydrated minerals. Identification of crystalline alteration minerals on Mars may indicate <span class="hlt">hydrothermal</span> alteration and sites of interesting geologic processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4109938','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4109938"><span>Geosphere-Biosphere Interactions in Bio-<span class="hlt">Activity</span> <span class="hlt">Volcanic</span> Lakes: Evidences from Hule and Rìo Cuarto (Costa Rica)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cabassi, Jacopo; Tassi, Franco; Mapelli, Francesca; Borin, Sara; Calabrese, Sergio; Rouwet, Dmitri; Chiodini, Giovanni; Marasco, Ramona; Chouaia, Bessem; Avino, Rosario; Vaselli, Orlando; Pecoraino, Giovannella; Capecchiacci, Francesco; Bicocchi, Gabriele; Caliro, Stefano; Ramirez, Carlos; Mora-Amador, Raul</p> <p>2014-01-01</p> <p>Hule and Río Cuarto are maar lakes located 11 and 18 km N of Poás volcano along a 27 km long fracture zone, in the Central <span class="hlt">Volcanic</span> Range of Costa Rica. Both lakes are characterized by a stable thermic and chemical stratification and recently they were affected by fish killing events likely related to the uprising of deep anoxic waters to the surface caused by rollover phenomena. The vertical profiles of temperature, pH, redox potential, chemical and isotopic compositions of water and dissolved gases, as well as prokaryotic diversity estimated by DNA fingerprinting and massive 16S rRNA pyrosequencing along the water column of the two lakes, have highlighted that different bio-geochemical processes occur in these meromictic lakes. Although the two lakes host different bacterial and archaeal phylogenetic groups, water and gas chemistry in both lakes is controlled by the same prokaryotic functions, especially regarding the CO2-CH4 cycle. Addition of <span class="hlt">hydrothermal</span> CO2 through the bottom of the lakes plays a fundamental priming role in developing a stable water stratification and fuelling anoxic bacterial and archaeal populations. Methanogens and methane oxidizers as well as autotrophic and heterotrophic aerobic bacteria responsible of organic carbon recycling resulted to be stratified with depth and strictly related to the chemical-physical conditions and availability of free oxygen, affecting both the CO2 and CH4 chemical concentrations and their isotopic compositions along the water column. Hule and Río Cuarto lakes were demonstrated to contain a CO2 (CH4, N2)-rich gas reservoir mainly controlled by the interactions occurring between geosphere and biosphere. Thus, we introduced the term of bio-<span class="hlt">activity</span> <span class="hlt">volcanic</span> lakes to distinguish these lakes, which have analogues worldwide (e.g. Kivu: D.R.C.-Rwanda; Albano, Monticchio and Averno: Italy; Pavin: France) from <span class="hlt">volcanic</span> lakes only characterized by geogenic CO2 reservoir such as Nyos and Monoun (Cameroon). PMID</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25058537','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25058537"><span>Geosphere-biosphere interactions in bio-<span class="hlt">activity</span> <span class="hlt">volcanic</span> lakes: evidences from Hule and Rìo Cuarto (Costa Rica).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cabassi, Jacopo; Tassi, Franco; Mapelli, Francesca; Borin, Sara; Calabrese, Sergio; Rouwet, Dmitri; Chiodini, Giovanni; Marasco, Ramona; Chouaia, Bessem; Avino, Rosario; Vaselli, Orlando; Pecoraino, Giovannella; Capecchiacci, Francesco; Bicocchi, Gabriele; Caliro, Stefano; Ramirez, Carlos; Mora-Amador, Raul</p> <p>2014-01-01</p> <p>Hule and Río Cuarto are maar lakes located 11 and 18 km N of Poás volcano along a 27 km long fracture zone, in the Central <span class="hlt">Volcanic</span> Range of Costa Rica. Both lakes are characterized by a stable thermic and chemical stratification and recently they were affected by fish killing events likely related to the uprising of deep anoxic waters to the surface caused by rollover phenomena. The vertical profiles of temperature, pH, redox potential, chemical and isotopic compositions of water and dissolved gases, as well as prokaryotic diversity estimated by DNA fingerprinting and massive 16S rRNA pyrosequencing along the water column of the two lakes, have highlighted that different bio-geochemical processes occur in these meromictic lakes. Although the two lakes host different bacterial and archaeal phylogenetic groups, water and gas chemistry in both lakes is controlled by the same prokaryotic functions, especially regarding the CO2-CH4 cycle. Addition of <span class="hlt">hydrothermal</span> CO2 through the bottom of the lakes plays a fundamental priming role in developing a stable water stratification and fuelling anoxic bacterial and archaeal populations. Methanogens and methane oxidizers as well as autotrophic and heterotrophic aerobic bacteria responsible of organic carbon recycling resulted to be stratified with depth and strictly related to the chemical-physical conditions and availability of free oxygen, affecting both the CO2 and CH4 chemical concentrations and their isotopic compositions along the water column. Hule and Río Cuarto lakes were demonstrated to contain a CO2 (CH4, N2)-rich gas reservoir mainly controlled by the interactions occurring between geosphere and biosphere. Thus, we introduced the term of bio-<span class="hlt">activity</span> <span class="hlt">volcanic</span> lakes to distinguish these lakes, which have analogues worldwide (e.g. Kivu: D.R.C.-Rwanda; Albano, Monticchio and Averno: Italy; Pavin: France) from <span class="hlt">volcanic</span> lakes only characterized by geogenic CO2 reservoir such as Nyos and Monoun (Cameroon).</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://adsabs.harvard.edu/abs/2014AGUFMOS51E..05Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS51E..05Z"><span>Characteristics of <span class="hlt">Hydrothermal</span> Mineralization in Ultraslow Spreading Ridges</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, H.; Yang, Q.; Ji, F.; Dick, H. J.</p> <p>2014-12-01</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> is a major component of the processes that shape the composition and structure of the ocean crust, providing a major pathway for the exchange of heat and elements between the Earth's crust and oceans, and a locus for intense biological <span class="hlt">activity</span> on the seafloor and underlying crust. In other hand, the structure and composition of <span class="hlt">hydrothermal</span> systems are the result of complex interactions between heat sources, fluids, wall rocks, tectonic controls and even biological processes. Ultraslow spreading ridges, including the Southwest Indian Ridge, the Gakkel Ridge, are most remarkable end member in plate-boundary structures (Dick et al., 2003), featured with extensive tectonic amagmatic spreading and frequent exposure of peridotite and gabbro. With intensive surveys in last decades, it is suggested that ultraslow ridges are several times more effective than faster-spreading ridges in sustaining <span class="hlt">hydrothermal</span> <span class="hlt">activities</span>. This increased efficiency could attributed to deep mining of heat and even exothermic serpentinisation (Baker et al., 2004). Distinct from in faster spreading ridges, one characteristics of <span class="hlt">hydrothermal</span> mineralization on seafloor in ultraslow spreading ridges, including the <span class="hlt">active</span> Dragon Flag <span class="hlt">hydrothermal</span> field at 49.6 degree of the Southwest Indian Ridge, is abundant and pervasive distribution of lower temperature precipitated minerals ( such as Fe-silica or silica, Mn (Fe) oxides, sepiolite, pyrite, marcasite etc. ) in <span class="hlt">hydrothermal</span> fields. Structures formed by lower temperature <span class="hlt">activities</span> in <span class="hlt">active</span> and dead <span class="hlt">hydrothermal</span> fields are also obviously. High temperature precipitated minerals such as chalcopyrite etc. are rare or very limited in <span class="hlt">hydrothermal</span> chimneys. Distribution of diverse low temperature <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> is consistence with the deep heating mechanisms and <span class="hlt">hydrothermal</span> circulations in the complex background of ultraslow spreading tectonics. Meanwhile, deeper and larger mineralization at certain locations along the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210488S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210488S"><span>Characteristics of <span class="hlt">hydrothermal</span> alteration mineralogy and geochemistry of igneous rocks from the epithermal Co-O mine and district, Eastern Mindanao (Philippines)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sonntag, Iris; Hagemann, Steffen</p> <p>2010-05-01</p> <p>Detailed petrographic as well as hyperspectral analyses using PIMA (Portable Infrared Mineral Analyser) and geochemical (major, trace and rare earth elements) studies were conducted on samples of the epithermal, low sulfidation Co-O mine (47,869 ounces gold produced in 2009 with an average grade of 13.3 g/t gold) and district in Eastern Mindanao (Philippines). The aims of the study were to unravel the petrogenetic origin of the various <span class="hlt">volcanic</span> (host rocks) and intrusive rocks (potential fluid driver) as well as their relationship and influence on the <span class="hlt">hydrothermal</span> alteration zoning and fluid chemistry. The auriferous veins at the Co-O mine were formed during two <span class="hlt">hydrothermal</span> stages associated with the district wide D1 and D2 deformation events. Gold in stage 1 quartz veins is in equilibrium with galena and sphalerite, whereas in stage 2 it is associated with pyrite. Auriferous quartz veins of stage 1 reflect temperatures below 250° C or strong variations in pH and fO2 at higher temperatures, due to potential involvement of acidic gas or meteoric water. Cathodoluminescense studies revealed strong zonation of quartz associated with Au, presumably related to changes in the Al content, which is influenced by the pH. Plumose textures indicate times of rapid deposition, whereas saccharoidal quartz grains are related to potential calcite replacement. The geology of the Co-O mine and district is dominated by Miocene <span class="hlt">volcanic</span> rocks (basic to intermediate flows and pyroclastics units), which are partly covered by Pliocene <span class="hlt">volcanic</span> rocks and late Oligocene to Miocene limestones. The Miocene units are intruded by diorite (presumably Miocene in age). The epithermal mineralization event may be related to diorite intrusions. The geochemistry of all igneous rocks in the district is defined by a sub-alkaline affinity and is low to medium K in composition. Most units are related to a Miocene subduction zone with westward subduction, whereas the younger Pliocene rocks are related to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P33B2870E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P33B2870E"><span>Poás volcano in Costa Rica as a <span class="hlt">hydrothermal</span> analog for Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Elmaarry, M. R.; Hynek, B. M.</p> <p>2017-12-01</p> <p>Mars has experienced intensive <span class="hlt">volcanic</span> and impact <span class="hlt">activity</span> early in its history, coinciding with a similarly extensive hydrologic <span class="hlt">activity</span> on a global scale. These <span class="hlt">activities</span> constitute the main ingredients of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Data acquired from the study of Martian meteorites, remote sensing spectral observations, and robotic rovers has shown the surface of Mars to be mineralogically diverse including mineral assemblages that resemble those of analogous <span class="hlt">hydrothermal</span> systems on Earth. In particular, evidence for extensive acid-sulfate weathering has been observed by the MERs at Gusev and Meridiani, as well as by MSL at Gale crater. Furthermore, there is growing evidence for silicic <span class="hlt">volcanism</span> on Mars as indicated by the detection of silica-rich mudstone at Gale containing tridymite and cristobalite coupled with spectral observations indicative of felsic rocks in geographically disparate locations on Mars. For that, the Poás volcano in Costa Rica offers a geologic setting that can be analogous to similar environments on Mars. The Poás volcano is a basaltic andesite stratovolcano in central Costa Rica. Its caldera houses a highly acidic lake inside the caldera 130 m below the crater rim. The volcano has been <span class="hlt">active</span> in recent historical times, and is currently displaying intensive <span class="hlt">activity</span> since Apr 2017. Unaltered andesitic basalts collected from the 1953-1955 magmatic <span class="hlt">activity</span> are mainly composed of plagioclase and minor amounts of orthopyroxene and olivine. We collected samples during our fieldwork in March 2017 (few weeks before its eruption) from fumaroles inside the caldera. The fumaroles were emitting gases at 92°C, and the acidic lake < 20 m away had a pH of 1.5. XRD analysis of samples taken from 4 different fumaroles shows high concentrations of elemental sulfur, gypsum, alunite, and cristobalite along with minor abundances of hematite, anatase, and amorphous silica. Most of these minerals have been observed on Mars under potentially similar</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.U33A..08K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.U33A..08K"><span>Impact-generated <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span> at the Chicxulub Crater</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kring, D. A.; Zurcher, L.; Abramov, O.</p> <p>2007-05-01</p> <p>Borehole samples recovered from PEMEX exploration boreholes and an ICDP scientific borehole indicate the Chicxulub impact event generated <span class="hlt">hydrothermal</span> alteration throughout a large volume of the Maya Block beneath the crater floor and extending across the bulk of the ~180 km diameter crater. The first indications of <span class="hlt">hydrothermal</span> alteration were observed in the crater discovery samples from the Yucatan-6 borehole and manifest itself in the form of anhydrite and quartz veins. Continuous core from the Yaxcopoil-1 borehole reveal a more complex and temporally extensive alteration sequence: following a brief period at high temperatures, impact- melt-bearing polymict breccias and a thin, underlying unit of impact melt were subjected to metasomatism, producing alkali feldspar, sphene, apatite, and magnetite. As the system continued to cool, smectite-series phyllosilicates appeared. A saline solution was involved. Stable isotopes suggest the fluid was dominated by a basinal brine created mostly from existing groundwater of the Yucatan Peninsula, although contributions from down-welling water also occurred in some parts of the system. Numerical modeling of the <span class="hlt">hydrothermal</span> system suggests circulation occurred for 1.5 to 2.3 Myr, depending on the permeability of the system. Our understanding of the <span class="hlt">hydrothermal</span> system, however, is still crude. Additional core recovery projects, particularly into the central melt sheet, are needed to better evaluate the extent and duration of <span class="hlt">hydrothermal</span> alteration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..322..241B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..322..241B"><span>Structure and evolution of an <span class="hlt">active</span> resurgent dome evidenced by geophysical investigations: The Yenkahe dome-Yasur volcano system (Siwi caldera, Vanuatu)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brothelande, E.; Lénat, J.-F.; Chaput, M.; Gailler, L.; Finizola, A.; Dumont, S.; Peltier, A.; Bachèlery, P.; Barde-Cabusson, S.; Byrdina, S.; Menny, P.; Colonge, J.; Douillet, G. A.; Letort, J.; Letourneur, L.; Merle, O.; Di Gangi, F.; Nakedau, D.; Garaebiti, E.</p> <p>2016-08-01</p> <p>In this contribution, we focus on one of the most <span class="hlt">active</span> resurgences on Earth, that of the Yenkahe dome in the Siwi caldera (Tanna Island, Vanuatu), which is associated with the persistently <span class="hlt">active</span> Yasur volcano. Gravity and magnetic surveys have been carried out over the past few years in the area, as well as electrical methods including electrical resistivity tomography (ERT), time domain electro-magnetics (TDEM) and self-potential (SP). These investigations were completed by thermometry, CO2 soil gas measurements, field observations and sampling. This multi-method approach allows geological structures within the caldera to be identified, as well as associated <span class="hlt">hydrothermal</span> features. The global structure of the caldera is deduced from gravity data, which shows the caldera rim as a high density structure. Large lava fields, emplaced before and after the onset of resurgence, are evidenced by combined gravity, magnetic and resistivity signals. In the middle of the caldera, the Yenkahe dome apparently results from a combination of <span class="hlt">volcanic</span> and tectonic events, showing that lava extrusion and resurgence have been operating simultaneously or alternately during the Siwi caldera post-collapse history. There is a clear distinction between the western and eastern parts of the dome. The western part is older and records the growth of an initial <span class="hlt">volcanic</span> cone and the formation of a small caldera. This small caldera (paleo-Yasur caldera), partially filled with lava flows, is the present-day focus of <span class="hlt">volcanic</span> <span class="hlt">activity</span> and associated fluid circulation and alteration. The eastern part of the dome is presumably younger, and is characterized by intense, extensive <span class="hlt">hydrothermal</span> alteration and <span class="hlt">activity</span>. Its northern part is covered by lava flow piles and exhibits a shallow <span class="hlt">hydrothermal</span> zone in ERT. The southern part has <span class="hlt">hydrothermal</span> alteration and <span class="hlt">activity</span> extending at least down to the base of the resurgent dome. This part of the dome is built up of low cohesion rock and is thus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023078','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023078"><span><span class="hlt">Hydrothermal</span> element fluxes from Copahue, Argentina: A "beehive" volcano in turmoil</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Varekamp, J.C.; Ouimette, A.P.; Herman, S.W.; Bermudez, A.; Delpino, D.</p> <p>2001-01-01</p> <p>Copahue volcano erupted altered rock debris, siliceous dust, pyroclastic sulfur, and rare juvenile fragments between 1992 and 1995, and magmatic eruptions occurred in July-October 2000. Prior to 2000, the Copahue crater lake, acid hot springs, and rivers carried acid brines with compositions that reflected close to congruent rock dissolution. The ratio between rock-forming elements and chloride in the central zone of the volcano-<span class="hlt">hydrothermal</span> system has diminished over the past few years, reflecting increased water/rock ratios as a result of progressive rock dissolution. Magmatic <span class="hlt">activity</span> in 2000 provided fresh rocks for the acid fluids, resulting in higher ratios between rock-forming elements and chloride in the fluids and enhanced Mg fluxes. The higher Mg fluxes started several weeks prior to the eruption. Model data on the crater lake and river element flux determinations indicate that Copahue volcano was hollowed out at a rate of about 20 000-25 000 m3/yr, but that void space was filled with about equal amounts of silica and liquid elemental sulfur. The extensive rock dissolution has weakened the internal <span class="hlt">volcanic</span> structure, making flank collapse a <span class="hlt">volcanic</span> hazard at Copahue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.9061M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.9061M"><span>Global <span class="hlt">volcanic</span> aerosol properties derived from emissions, 1990-2015, using CESM1(WACCM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mills, Michael; Schmidt, Anja; Easter, Richard; Solomon, Susan; Kinnison, Douglas; Ghan, Steven; Neely, Ryan; Marsh, Daniel; Conley, Andrew; Bardeen, Charles; Gettelman, Andrew</p> <p>2016-04-01</p> <p>Accurate representation of global stratospheric aerosols from <span class="hlt">volcanic</span> and <span class="hlt">non-volcanic</span> sulfur emissions is key to understanding the cooling effects and ozone-losses that may be linked to <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Attribution of climate variability to <span class="hlt">volcanic</span> <span class="hlt">activity</span> is of particular interest in relation to the post-2000 slowing in the rate of global average temperature increases. We have compiled a database of <span class="hlt">volcanic</span> SO2 emissions and plume altitudes for eruptions from 1990 to 2015, and developed a new prognostic capability for simulating stratospheric sulfate aerosols in the Community Earth System Model (CESM). We combined these with other <span class="hlt">non-volcanic</span> emissions of sulfur sources to reconstruct global aerosol properties from 1990 to 2015. Our calculations show remarkable agreement with ground-based lidar observations of stratospheric aerosol optical depth (SAOD), and with in situ measurements of stratospheric aerosol surface area density (SAD). These properties are key parameters in calculating the radiative and chemical effects of stratospheric aerosols. Our SAOD calculations represent a clear improvement over available satellite-based analyses, which generally ignore aerosol extinction below 15 km, a region that can contain the vast majority of stratospheric aerosol extinction at mid- and high-latitudes. Our SAD calculations greatly improve on that provided for the Chemistry-Climate Model Initiative, which misses about 60% of the SAD measured in situ on average during both <span class="hlt">volcanically</span> <span class="hlt">active</span> and <span class="hlt">volcanically</span> quiescent periods. The stark differences in SAOD and SAD compared to other data sets will have significant effects on calculations of the radiative forcing of climate and global stratospheric chemistry over the period 2005-2015. In light of these results, the impact of <span class="hlt">volcanic</span> aerosols in reducing the rate of global average temperature increases since the year 2000 should be revisited. We have made our calculated aerosol properties from January 1990 to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035662','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035662"><span><span class="hlt">Volcanic</span> hazards to airports</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Guffanti, M.; Mayberry, G.C.; Casadevall, T.J.; Wunderman, R.</p> <p>2009-01-01</p> <p><span class="hlt">Volcanic</span> <span class="hlt">activity</span> has caused significant hazards to numerous airports worldwide, with local to far-ranging effects on travelers and commerce. Analysis of a new compilation of incidents of airports impacted by <span class="hlt">volcanic</span> <span class="hlt">activity</span> from 1944 through 2006 reveals that, at a minimum, 101 airports in 28 countries were affected on 171 occasions by eruptions at 46 volcanoes. Since 1980, five airports per year on average have been affected by <span class="hlt">volcanic</span> <span class="hlt">activity</span>, which indicates that <span class="hlt">volcanic</span> hazards to airports are not rare on a worldwide basis. The main hazard to airports is ashfall, with accumulations of only a few millimeters sufficient to force temporary closures of some airports. A substantial portion of incidents has been caused by ash in airspace in the vicinity of airports, without accumulation of ash on the ground. On a few occasions, airports have been impacted by hazards other than ash (pyroclastic flow, lava flow, gas emission, and phreatic explosion). Several airports have been affected repeatedly by <span class="hlt">volcanic</span> hazards. Four airports have been affected the most often and likely will continue to be among the most vulnerable owing to continued nearby <span class="hlt">volcanic</span> <span class="hlt">activity</span>: Fontanarossa International Airport in Catania, Italy; Ted Stevens Anchorage International Airport in Alaska, USA; Mariscal Sucre International Airport in Quito, Ecuador; and Tokua Airport in Kokopo, Papua New Guinea. The USA has the most airports affected by <span class="hlt">volcanic</span> <span class="hlt">activity</span> (17) on the most occasions (33) and hosts the second highest number of volcanoes that have caused the disruptions (5, after Indonesia with 7). One-fifth of the affected airports are within 30 km of the source volcanoes, approximately half are located within 150 km of the source volcanoes, and about three-quarters are within 300 km; nearly one-fifth are located more than 500 km away from the source volcanoes. The volcanoes that have caused the most impacts are Soufriere Hills on the island of Montserrat in the British West Indies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS43A2033H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS43A2033H"><span>Iron-Oxidizing Bacteria Found at Slow-Spreading Ridge: a Case Study of Capelinhos <span class="hlt">Hydrothermal</span> Vent (Lucky Strike, MAR 37°N)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Henri, P. A.; Rommevaux, C.; Lesongeur, F.; Emerson, D.; Leleu, T.; Chavagnac, V.</p> <p>2015-12-01</p> <p>Iron-oxidizing bacteria becomes increasingly described in different geological settings from <span class="hlt">volcanically</span> <span class="hlt">active</span> seamounts, coastal waters, to diffuse <span class="hlt">hydrothermal</span> vents near seafloor spreading centers [Emerson et al., 2010]. They have been mostly identified and described in Pacific Ocean, and have been only recently found in <span class="hlt">hydrothermal</span> systems associated to slow spreading center of the Mid-Atlantic Ridge (MAR) [Scott et al., 2015]. During the MoMARSAT'13 cruise at Lucky Strike <span class="hlt">hydrothermal</span> field (MAR), a new <span class="hlt">hydrothermal</span> site was discovered at about 1.5 km eastward from the lava lake and from the main <span class="hlt">hydrothermal</span> vents. This <span class="hlt">active</span> venting site, named Capelinhos, is therefore the most distant from the volcano, features many chimneys, both focused and diffuses. The <span class="hlt">hydrothermal</span> end-member fluids from Capelinhos are different from those of the other sites of Lucky Strike, showing the highest content of iron (Fe/Mn≈3.96) and the lowest chlorinity (270 mmol/l) [Leleu et al., 2015]. Most of the chimneys exhibit rust-color surfaces and bacterial mats near diffuse flows. During the MoMARSAT'15 cruise, an <span class="hlt">active</span> chimney, a small inactive one, and rust-color bacterial mat near diffuse flow were sampled at Capelinhos. Observations by SEM of the <span class="hlt">hydrothermal</span> samples revealed the presence of iron oxides in an assemblage of tubular "sheaths", assembled "stalks", helical "stalks" and amorphous aggregates. These features are similar to those described from the Loihi iron-mats deposits and argue for the occurrence of iron-oxidizing bacteria. Cultures under micro-aerobic and neutral pH conditions allowed us to isolate strains from the small inactive chimney. Pyrosequencing of the 16S rRNA gene of the isolates and environmental samples will soon be performed, which should confirm the presence of iron-oxidizing bacteria and reveal the organization of bacterial communities in this original and newly discovered <span class="hlt">hydrothermal</span> site of the slow spreading Mid-Atlantic Ridge. Emerson</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024075','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024075"><span>Geochemistry of fluid phases and sediments: Relevance to <span class="hlt">hydrothermal</span> circulation in Middle Valley, ODP Legs 139 and 169</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gieskes, J.M.; Simoneit, B.R.T.; Shanks, Wayne C.; Goodfellow, W.D.; James, R.H.; Baker, P.A.; Ishibashi, J.-I.</p> <p>2002-01-01</p> <p>Geochemical and isotopic studies of pore fluids and solid phases recovered from the Dead Dog and Bent Hill <span class="hlt">hydrothermal</span> sites in Middle Valley (Ocean Drilling Program Leg 169) have been compared with similar data obtained previously from these sites during Ocean Drilling Program Leg 139. Although generally the <span class="hlt">hydrothermal</span> systems reflect <span class="hlt">non</span>-steady state conditions, the data allow an assessment of the history of the <span class="hlt">hydrothermal</span> processes. Sediment K/A1 ratios as well as the distribution of anhydrite in the sediments suggest that the Dead Dog <span class="hlt">hydrothermal</span> field has been, and still is, <span class="hlt">active</span>. In contrast, similar data in the Bent Hill <span class="hlt">hydrothermal</span> field indicate a waning of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Pore fluid and <span class="hlt">hydrothermal</span> vent data in the Dead Dog <span class="hlt">hydrothermal</span> field are similar in nature to the data collected during ODP Leg 139. In the area of the Bent Hill sulfide deposit, however, the pore water data indicate that recent wholesale flushing of the sediment column with relatively unaltered seawater has obliterated a previous record of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in the pore fluids. Data from the deepest part of Hole 1035A in the Bent Hill locality show the presence of <span class="hlt">hydrothermal</span> fluids at greater depths in this area. This suggests the origin of the <span class="hlt">hydrothermal</span> fluids found to be emanating from Hole 1035F, which constitutes one of the first man made <span class="hlt">hydrothermal</span> vents in the Middle Valley <span class="hlt">hydrothermal</span> system. Similarly, CORKed Hole 858G, because of seal failures, has acted as a <span class="hlt">hydrothermal</span> vent, with sulfide deposits forming inside the CORK. ?? 2002 Elsevier Science Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GeCoA.101..191S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeCoA.101..191S"><span>Halocarbons and other trace heteroatomic organic compounds in <span class="hlt">volcanic</span> gases from Vulcano (Aeolian Islands, Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schwandner, Florian M.; Seward, Terry M.; Giże, Andrew P.; Hall, Keith; Dietrich, Volker J.</p> <p>2013-01-01</p> <p>Adsorbent-trapped <span class="hlt">volcanic</span> gases, sublimates and condensates from <span class="hlt">active</span> vents of the La Fossa crater on the island of Vulcano (Aeolian Islands, Italy) as well as ambient and industrial air were quantitatively analyzed by Short-Path Thermal Desorption-Solid Phase Microextraction-Cryotrapping-Gas Chromatography/Mass Spectrometry (SPTD-SPME-CF-GC-MS). Among the over 200 detected and quantified compounds are alkanes, alkenes, arenes, phenols, aldehydes, carboxylic acids, esters, ketones, nitriles, PAHs and their halogenated, methylated and sulfonated derivatives, as well as various heterocyclic compounds including thiophenes and furans. Most compounds are found at concentrations well above laboratory, ambient air, adsorbent and field blank levels. For some analytes (e.g., CFC-11, CH2Cl2, CH3Br), concentrations are up to several orders of magnitude greater than even mid-latitudinal industrial urban air maxima. Air or laboratory contamination is negligible or absent on the basis of noble gas measurements and their isotopic ratios. The organic compounds are interpreted as the product of abiogenic gas-phase radical reactions. On the basis of isomer abundances, n-alkane distributions and substitution patterns the compounds are thought to have formed by high-temperature (e.g., 900 °C) alkyl free radical reactions and halide electrophilic substitution on arenes, alkanes and alkenes. The apparent abiogenic organic chemistry of <span class="hlt">volcanic</span> gases may give insights into metal transport processes during the formation and alteration of <span class="hlt">hydrothermal</span> ore deposits, into the natural <span class="hlt">volcanic</span> source strength of ozone-depleting atmospheric trace gases (i.e., halocarbons), into possibly sensitive trace gas redox pairs as potential early indicators of subsurface changes on volcanoes in the state of imminent unrest, and into the possible <span class="hlt">hydrothermal</span> origin of early life on Earth, as indicated by the presence of simple amino acids, nitriles, and alkanoic acids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70177135','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70177135"><span>Monitoring the <span class="hlt">hydrothermal</span> system in Long Valley caldera, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Farrar, C.D.; Sorey, M.L.</p> <p>1985-01-01</p> <p>An ongoing program to monitor the <span class="hlt">hydrothermal</span> system in Long Valley for changes caused by <span class="hlt">volcanic</span> or tectonic processes has produced considerable data on the water chemistry and discharge of springs and fluid temperatures and pressures in wells. Chemical and isotopic data collected under this program have greatly expanded the knowledge of chemical variability both in space and time. Although no chemical or isotopic changes in hot spring waters can be attributed directly to <span class="hlt">volcanic</span> or tectonic processes, changes in hot spring chemistry that have been recorded probably relate to interactions between and variations in the quantity of liquid and gas discharged. Stable carbon isotope data are consistent with a carbon source either perform the mantle or from metamorphosed carbonate rocks. Continuous and periodic measurements of hot spring discharge at several sites show significant co seismic and a seismic changes since 1980.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011348','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011348"><span>Submarine <span class="hlt">hydrothermal</span> metamorphism of the Del Puerto ophiolite, California.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Evarts, R.C.; Schiffman, P.</p> <p>1983-01-01</p> <p>Metamorphic zonation overprinted on the <span class="hlt">volcanic</span> member and overlying volcanogenic sediments of the ophiolite complex increases downward in grade and is characterized by the sequential appearance with depth of zeolites, ferric pumpellyite and pistacitic epidote. Metamorphic assemblages of the plutonic member of the complex are characterized by the presence of calcic amphibole. The overprinting represents the effects of <span class="hlt">hydrothermal</span> metamorphism resulting from the massive interaction between hot igneous rocks and convecting sea-water in a submarine environment. A thermal gradient of 100oC/km is postulated to account for the zonal recrystallization effects in the <span class="hlt">volcanic</span> member. The diversity and sporadic distribution of mineral assemblages in the amphibole zone are considered due to the limited availability of H2O in the deeper part of the complex. Details of the zonation and representative microprobe analyses are tabulated.-M.S.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.3591O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3591O"><span><span class="hlt">Volcanic</span> Alert System (VAS) developed during the (2011-2013) El Hierro (Canary Islands) <span class="hlt">volcanic</span> process</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz, Ramon; Berrocoso, Manuel; Marrero, Jose Manuel; Fernandez-Ros, Alberto; Prates, Gonçalo; De la Cruz-Reyna, Servando; Garcia, Alicia</p> <p>2014-05-01</p> <p>In <span class="hlt">volcanic</span> areas with long repose periods (as El Hierro), recently installed monitoring networks offer no instrumental record of past eruptions nor experience in handling a <span class="hlt">volcanic</span> crisis. Both conditions, uncertainty and inexperience, contribute to make the communication of hazard more difficult. In fact, in the initial phases of the unrest at El Hierro, the perception of <span class="hlt">volcanic</span> risk was somewhat distorted, as even relatively low <span class="hlt">volcanic</span> hazards caused a high political impact. The need of a <span class="hlt">Volcanic</span> Alert System became then evident. In general, the <span class="hlt">Volcanic</span> Alert System is comprised of the monitoring network, the software tools for the analysis of the observables, the management of the <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Level, and the assessment of the threat. The <span class="hlt">Volcanic</span> Alert System presented here places special emphasis on phenomena associated to moderate eruptions, as well as on volcano-tectonic earthquakes and landslides, which in some cases, as in El Hierro, may be more destructive than an eruption itself. As part of the <span class="hlt">Volcanic</span> Alert System, we introduce here the <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Level which continuously applies a routine analysis of monitoring data (particularly seismic and deformation data) to detect data trend changes or monitoring network failures. The data trend changes are quantified according to the Failure Forecast Method (FFM). When data changes and/or malfunctions are detected, by an automated watchdog, warnings are automatically issued to the Monitoring Scientific Team. Changes in the data patterns are then translated by the Monitoring Scientific Team into a simple <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Level, that is easy to use and understand by the scientists and technicians in charge for the technical management of the unrest. The main feature of the <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> Level is its objectivity, as it does not depend on expert opinions, which are left to the Scientific Committee, and its capabilities for early detection of precursors. As a consequence of the El Hierro</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008cosp...37.2444P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008cosp...37.2444P"><span>Synthesis of hydrogen cyanide under simulated <span class="hlt">hydrothermal</span> conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pinedo-González, Paulina</p> <p></p> <p>Nitrogen is a fundamental element for life, where is present in structural (e.g., proteins), catalytic (e.g., enzymes and ribozymes), energy transfer (e.g., ATP) and information storage (RNA and DNA) biomolecules. Atmospheric and planetary models suggest that nitrogen was abundant in the early atmospheres of Earth as dinitrogen (N2 ), an inert gas under normal atmospheric conditions. To be available for prebiotic synthesis it must be converted into hydrogen cyanide (HCN), ammonia (NH3 ) and/or nitric oxide (NO), in a process referred to as nitrogen fixation. Due to the strength of the triple bond in N2 , nitrogen fixation, while thermodynamically favored is kinetically restricted. In a reducing atmosphere dominated by CH4 -N2 , thunderstorm lightning efficiently produces HCN and NH3 (Stribling and Miller, 1987). Nevertheless, photochemical and geochemical constraints strongly suggest that the early atmosphere was weakly reducing, dominated by CO2 and N2 with traces of CH4 , CO, and H2 (Kasting, 1993). Under these conditions, HCN is no longer synthesized in the lightning channel and instead NO is formed (Navarro-Gonźlez, et al., 2001). In <span class="hlt">volcanic</span> plumes, where magmatic gases a were more reducing than in the atmosphere, NO can also be formed by the lava heat (Mather et al., 2004) or <span class="hlt">volcanic</span> lightning (Navarro-Gonźlez et al., 1998). Surprisingly, dinitrogen can be a reduced to NH3 in <span class="hlt">hydrothermal</span> systems (Brandes et al., 1998), but the formation of HCN and its derivates were not investigated. The present work explores the possibility of the formation of HCN as well as other nitrile derivatives catalyzed by mineral surfaces in <span class="hlt">hydrothermal</span> vents. To simulate a <span class="hlt">hydrothermal</span> atmosphere, the experiments were carried out in a stainless steel Parr R minireactor with a 0.1 M NH4 HCO3 solution (200 ml) with or without a mineral surface exposed at 1 bar at temperatures ranging from 100 to 375° C. Different mineral matrices are been investigated. Our preliminary results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V14B..02T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V14B..02T"><span><span class="hlt">Volcanic</span> gas impacts on vegetation at Turrialba Volcano, Costa Rica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teasdale, R.; Jenkins, M.; Pushnik, J.; Houpis, J. L.; Brown, D. L.</p> <p>2010-12-01</p> <p>Turrialba volcano is an <span class="hlt">active</span> composite stratovolcano that is located approximately 40 km east of San Jose, Costa Rica. Seismic <span class="hlt">activity</span> and degassing have increased since 2005, and gas compositions reflect further increased <span class="hlt">activity</span> since 2007 peaking in January 2010 with a phreatic eruption. Gas fumes dispersed by trade winds toward the west, northwest, and southwest flanks of Turrialba volcano have caused significant vegetation kill zones, in areas important to local agriculture, including dairy pastures and potato fields, wildlife and human populations. In addition to extensive vegetative degradation is the potential for soil and water contamination and soil erosion. Summit fumarole temperatures have been measured over 200 degrees C and gas emissions are dominated by SO2; gas and vapor plumes reach up to 2 km (fumaroles and gases are measured regularly by OVSICORI-UNA). A recent network of passive air sampling, monitoring of water temperatures of <span class="hlt">hydrothermal</span> systems, and soil pH measurements coupled with measurement of the physiological status of surrounding plants using gas exchange and fluorescence measurements to: (1) identify physiological correlations between leaf-level gas exchange and chlorophyll fluorescence measurements of plants under long term stress induced by the <span class="hlt">volcanic</span> gas emissions, and (2) use measurements in tandem with remotely sensed reflectance-derived fluorescence ratio indices to track natural photo inhibition caused by <span class="hlt">volcanic</span> gas emissions, for use in monitoring plant stress and photosynthetic function. Results may prove helpful in developing potential land management strategies to maintain the biological health of the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024978','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024978"><span>Jovian dust streams: A monitor of Io's <span class="hlt">volcanic</span> plume <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kruger, H.; Geissler, P.; Horanyi, M.; Graps, A.L.; Kempf, S.; Srama, R.; Moragas-Klostermeyer, G.; Moissl, R.; Johnson, T.V.; Grun, E.</p> <p>2003-01-01</p> <p>Streams of high speed dust particles originate from Jupiter's moon Io. After release from Io, the particles collect electric charges in the Io plasma torus, gain energy from the co-rotating electric field of Jupiter's magnetosphere, and leave the Jovian system into interplanetary space with escape speeds over 200 km s-1. The Galileo spacecraft has continuously monitored the dust streams during 34 revolutions about Jupiter between 1996 and 2002. The observed dust fluxes exhibit large orbit-to-orbit variability due to systematic and stochastic changes. After removal of the systematic variations, the total dust emission rate of Io has been calculated. It varies between 10-3 and 10 kg s-1, and is typically in the range of 0.1 to 1 kg s-1. We compare the dust emission rate with other markers of <span class="hlt">volcanic</span> <span class="hlt">activity</span> on Io like large-area surface changes caused by <span class="hlt">volcanic</span> deposits and sightings of <span class="hlt">volcanic</span> plumes. Copyright 2003 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1044h/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1044h/report.pdf"><span>Reconnaissance of the <span class="hlt">hydrothermal</span> resources of Utah</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rush, F. Eugene</p> <p>1983-01-01</p> <p>Geologic factors in the Basin and Range province in Utah are more favorable for the occurrence of geothermal resources than in other areas on the Colorado Plateaus or in the Middle Rocky Mountains. These geologic factors are principally crustal extension and crustal thinning during the last 17 million years. Basalts as young as 10,000 years have been mapped in the area. High-silica <span class="hlt">volcanic</span> and intru­sive rocks of Quaternary age can be used to locate <span class="hlt">hydrothermal</span> convection systems. Drilling for hot, high-silica, buried rock bodies is most promising in the areas of recent <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Southwestern Utah has more geothermal potential than other parts of the Basin and Range province in Utah. The Roosevelt Hot Springs area, the Cove Fort-Sulphurdale area, and the area to the north as far as 60 kilome­ters from them probably have the best potential for geothermal devel­opment for generation of electricity. Other areas with estimated res­ervoir temperatures greater than 150°C are Thermo, Monroe, Red Hill (in the Monroe-Joseph Known Geothermal Resource Area), Joseph Hot Springs, and the Newcastle area. The rates of heat and water discharge are high at Crater, Meadow, and Hatton Hot Springs, but estimated reservoir temperatures there are less than 150°C. Ad­ditional exploration is needed to define the potential in three ad­ditional areas in the Escalante Desert.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70073840','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70073840"><span>Trace metal-rich Quaternary <span class="hlt">hydrothermal</span> manganese oxide and barite deposit, Milos Island, Greece</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hein, J.R.; Stamatakis, G.; Dowling, J.S.</p> <p>2000-01-01</p> <p>The Cape Vani Mn oxide and barite deposit on Milos Island offers an excellent opportunity to study the three-dimensional characteristics of a shallow-water <span class="hlt">hydrothermal</span> system. Milos Island is part of the <span class="hlt">active</span> Aegean <span class="hlt">volcanic</span> arc. A 1 km long basin located between two dacitic domes in northwest Milos is filled with a 35-50 m thick section of Quaternary volcaniclastic and pyroclastic rocks capped by reef limestone that were <span class="hlt">hydrothermally</span> mineralized by Mn oxides and barite. Manganese occurs as thin layers, as cement of sandstone and as metasomatic replacement of the limestone, including abundant fossil shells. Manganese minerals include chiefly δ-MnO2, pyrolusite and ramsdellite. The MnO contents for single beds range up to 60%. The Mn oxide deposits are rich in Pb (to 3.4%), BaO (to 3.1%), Zn (to 0.8%), As (to 0.3%), Sb (to 0.2%) and Ag (to 10 ppm). Strontium isotopic compositions of the Mn oxide deposits and sulphur isotopic compositions of the associated barite show that the mineralizing fluids were predominantly sea water. The Mn oxide deposit formed in close geographical proximity to sulphide-sulphate-Au-Ag deposits and the two deposit types probably formed from the same <span class="hlt">hydrothermal</span> system. Precipitation of Mn oxide took place at shallow burial depths and was promoted by the mixing of modified sea water (<span class="hlt">hydrothermal</span> fluid) from which the sulphides precipitated at depth and sea water that penetrated along faults and fractures in the Cape Vani volcaniclastic and tuff deposits. The <span class="hlt">hydrothermal</span> fluid was formed from predominantly sea water that was enriched in metals leached from the basement and overlying volcanogenic rocks. The <span class="hlt">hydrothermal</span> fluids were driven by convection sustained by heat from cooling magma chambers. Barite was deposited throughout the time of Mn oxide mineralization, which occurred in at least two episodes. Manganese mineralization occurred by both focused and diffuse flow, the fluids mineralizing the beds of greatest porosity and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980016866','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980016866"><span>Planetary <span class="hlt">Volcanism</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Antonenko, I.; Head, J. W.; Pieters, C. W.</p> <p>1998-01-01</p> <p>The final report consists of 10 journal articles concerning Planetary <span class="hlt">Volcanism</span>. The articles discuss the following topics: (1) lunar stratigraphy; (2) cryptomare thickness measurements; (3) spherical harmonic spectra; (4) late stage <span class="hlt">activity</span> of volcanoes on Venus; (5) stresses and calderas on Mars; (6) magma reservoir failure; (7) lunar mare basalt <span class="hlt">volcanism</span>; (8) impact and <span class="hlt">volcanic</span> glasses in the 79001/2 Core; (9) geology of the lunar regional dark mantle deposits; and (10) factors controlling the depths and sizes of magma reservoirs in Martian volcanoes.</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('https://www.osti.gov/servlets/purl/1379265','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1379265"><span>Metagenomic investigation of the geologically unique Hellenic <span class="hlt">Volcanic</span> Arc reveals a distinctive ecosystem with unexpected physiology: Metagenomic investigation of the Hellenic <span class="hlt">Volcanic</span> Arc</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>Oulas, Anastasis; Polymenakou, Paraskevi N.; Seshadri, Rekha</p> <p></p> <p><span class="hlt">Hydrothermal</span> vents represent a deep, hot, aphotic biosphere where chemosynthetic primary producers, fuelled by chemicals from Earth's subsurface, form the basis of life. In this study, we examined microbial mats from two distinct <span class="hlt">volcanic</span> sites within the Hellenic <span class="hlt">Volcanic</span> Arc (HVA). The HVA is geologically and ecologically unique, with reported emissions of CO 2-saturated fluids at temperatures up to 220°C and a notable absence of macrofauna. Metagenomic data reveals highly complex prokaryotic communities composed of chemolithoautotrophs, some methanotrophs, and to our surprise, heterotrophs capable of anaerobic degradation of aromatic hydrocarbons. Our data suggest that aromatic hydrocarbons may indeed be amore » significant source of carbon in these sites, and instigate additional research into the nature and origin of these compounds in the HVA. Novel physiology was assigned to several uncultured prokaryotic lineages; most notably, a SAR406 representative is attributed with a role in anaerobic hydrocarbon degradation. This dataset, the largest to date from submarine <span class="hlt">volcanic</span> ecosystems, constitutes a significant resource of novel genes and pathways with potential biotechnological applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1379265-metagenomic-investigation-geologically-unique-hellenic-volcanic-arc-reveals-distinctive-ecosystem-unexpected-physiology-metagenomic-investigation-hellenic-volcanic-arc','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1379265-metagenomic-investigation-geologically-unique-hellenic-volcanic-arc-reveals-distinctive-ecosystem-unexpected-physiology-metagenomic-investigation-hellenic-volcanic-arc"><span>Metagenomic investigation of the geologically unique Hellenic <span class="hlt">Volcanic</span> Arc reveals a distinctive ecosystem with unexpected physiology: Metagenomic investigation of the Hellenic <span class="hlt">Volcanic</span> Arc</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Oulas, Anastasis; Polymenakou, Paraskevi N.; Seshadri, Rekha; ...</p> <p>2015-12-21</p> <p><span class="hlt">Hydrothermal</span> vents represent a deep, hot, aphotic biosphere where chemosynthetic primary producers, fuelled by chemicals from Earth's subsurface, form the basis of life. In this study, we examined microbial mats from two distinct <span class="hlt">volcanic</span> sites within the Hellenic <span class="hlt">Volcanic</span> Arc (HVA). The HVA is geologically and ecologically unique, with reported emissions of CO 2-saturated fluids at temperatures up to 220°C and a notable absence of macrofauna. Metagenomic data reveals highly complex prokaryotic communities composed of chemolithoautotrophs, some methanotrophs, and to our surprise, heterotrophs capable of anaerobic degradation of aromatic hydrocarbons. Our data suggest that aromatic hydrocarbons may indeed be amore » significant source of carbon in these sites, and instigate additional research into the nature and origin of these compounds in the HVA. Novel physiology was assigned to several uncultured prokaryotic lineages; most notably, a SAR406 representative is attributed with a role in anaerobic hydrocarbon degradation. This dataset, the largest to date from submarine <span class="hlt">volcanic</span> ecosystems, constitutes a significant resource of novel genes and pathways with potential biotechnological applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.V24A..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.V24A..02G"><span>What governs the enrichment of Pb in the continental crust? An answer from the Mexican <span class="hlt">Volcanic</span> Belt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldstein, S. L.; Lagatta, A.; Langmuir, C. H.; Straub, S. M.; Martin-Del-Pozzo, A.</p> <p>2009-12-01</p> <p>One of Al Hofmann’s many important contributions to our understanding of geochemical cycling in the Earth is the observation that Pb behaves like the light rare earth elements Ce and Nd during melting to form oceanic basalts, but is enriched in the continental crust compared to the LREE by nearly an order of magnitude (Hofmann et al. 1986). This is unusual behavior, and has been called one of the Pb paradoxes, since in most cases, the ratios of elements are effectively the same in the continental crust and oceanic basalts if they show similar mantle melting behavior. One of several mechanisms suggested to mediate this special enrichment is <span class="hlt">hydrothermal</span> circulation at ocean ridges, which preferentially transports Pb compared to the REE from the interior of the ocean crust to the surface. We confirm the importance of <span class="hlt">hydrothermal</span> processes at the East Pacific to mediate Pb enrichment at the Trans-Mexican <span class="hlt">Volcanic</span> Belt (TMVB, through comparison of Pb isotope and Ce/Pb ratios of TMVB lavas with sediments from DSDP Site 487 near the Middle America trench. The lavas of the Trans-Mexican <span class="hlt">Volcanic</span> Belt include “high Nb” alkali basalts (HNAB), whose trace element patterns lack subduction signatures. The HNAB basalts and <span class="hlt">hydrothermally</span> affected sediments from DSDP 487, form end-members that bound calcalkaline lavas from volcanoes Colima, Toluca, Popocatépetl, and Malinche in Ce/Pb versus Pb isotope space. The HNAB represent the high Ce/Pb and high Pb-isotope end-member. The <span class="hlt">hydrothermal</span> sediments have Pb isotopes like Pacific MORB but Ce/Pb ratios typical of the arcs and the continental crust, and an order of magnitude lower than MORB. No analyzed calcalkaline lavas are have compositions outside of the bounds formed by the HNAB and the <span class="hlt">hydrothermal</span> sediments. The Ce/Pb and Pb isotope ratios show that the calcalkaline lava compositions are inconsistent with contributions from HNAB and EPR MORB, rather the contributions are from HNAB upper mantle and subducted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16943836','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16943836"><span>Discovery of a magma chamber and faults beneath a Mid-Atlantic Ridge <span class="hlt">hydrothermal</span> field.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Singh, Satish C; Crawford, Wayne C; Carton, Hélène; Seher, Tim; Combier, Violaine; Cannat, Mathilde; Pablo Canales, Juan; Düsünür, Doga; Escartin, Javier; Miranda, J Miguel</p> <p>2006-08-31</p> <p>Crust at slow-spreading ridges is formed by a combination of magmatic and tectonic processes, with magmatic accretion possibly involving short-lived crustal magma chambers. The reflections of seismic waves from crustal magma chambers have been observed beneath intermediate and fast-spreading centres, but it has been difficult to image such magma chambers beneath slow-spreading centres, owing to rough seafloor topography and associated seafloor scattering. In the absence of any images of magma chambers or of subsurface near-axis faults, it has been difficult to characterize the interplay of magmatic and tectonic processes in crustal accretion and <span class="hlt">hydrothermal</span> circulation at slow-spreading ridges. Here we report the presence of a crustal magma chamber beneath the slow-spreading Lucky Strike segment of the Mid-Atlantic Ridge. The reflection from the top of the magma chamber, centred beneath the Lucky Strike volcano and <span class="hlt">hydrothermal</span> field, is approximately 3 km beneath the sea floor, 3-4 km wide and extends up to 7 km along-axis. We suggest that this magma chamber provides the heat for the <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vent field above it. We also observe axial valley bounding faults that seem to penetrate down to the magma chamber depth as well as a set of inward-dipping faults cutting through the <span class="hlt">volcanic</span> edifice, suggesting continuous interactions between tectonic and magmatic processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1861c0033B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1861c0033B"><span><span class="hlt">Hydrothermal</span> system of the Papandayan Volcano from temperature, self-potential (SP) and geochemical measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Byrdina, Svetlana; Revil, André; Gunawan, Hendra; Saing, Ugan B.; Grandis, Hendra</p> <p>2017-07-01</p> <p>Papandayan volcano in West Java, Indonesia, is characterized by intense <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> manifested by numerous fumaroles at three craters or kawah, i.e. Mas, Manuk and Baru. The latter was created after November 2002 phreatic eruption. Since 2011, numerous volcano-tectonic B events are encountered and the volcano was set on alert status on several occasions. The purpose of the present study is to delineate the structure of the summital <span class="hlt">hydrothermal</span> system from Self-Potential (SP), soil temperature and gas concentrations in the soil (CO2, SO2 and H2S) data. This combination of geophysical and geochemical methods allows identification of the weak permeable zones serving as preferential pathways for <span class="hlt">hydrothermal</span> circulation and potential candidates to future landslides or flank collapses. This study is an on-going collaborative research project and we plan to conduct electrical resistivity tomography (ERT) and also Induced-Polarization (IP) surveys. Additional data would allow the 3D imaging of the studied area. The IP parameters will be used to characterise and to quantify the degree of alteration of the <span class="hlt">volcanic</span> rocks as has been shown very recently in the laboratory studies. There are also rocks and soil samples that will undergo laboratory analyses at ISTerre for IP and complex resistivity parameters at the sample scale that will help to interpret the survey results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28931949','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28931949"><span><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span>, functional diversity and chemoautotrophy are major drivers of seafloor carbon cycling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bell, James B; Woulds, Clare; Oevelen, Dick van</p> <p>2017-09-20</p> <p><span class="hlt">Hydrothermal</span> vents are highly dynamic ecosystems and are unusually energy rich in the deep-sea. In situ <span class="hlt">hydrothermal</span>-based productivity combined with sinking photosynthetic organic matter in a soft-sediment setting creates geochemically diverse environments, which remain poorly studied. Here, we use comprehensive set of new and existing field observations to develop a quantitative ecosystem model of a deep-sea chemosynthetic ecosystem from the most southerly <span class="hlt">hydrothermal</span> vent system known. We find evidence of chemosynthetic production supplementing the metazoan food web both at vent sites and elsewhere in the Bransfield Strait. Endosymbiont-bearing fauna were very important in supporting the transfer of chemosynthetic carbon into the food web, particularly to higher trophic levels. Chemosynthetic production occurred at all sites to varying degrees but was generally only a small component of the total organic matter inputs to the food web, even in the most <span class="hlt">hydrothermally</span> <span class="hlt">active</span> areas, owing in part to a low and patchy density of vent-endemic fauna. Differences between relative abundance of faunal functional groups, resulting from environmental variability, were clear drivers of differences in biogeochemical cycling and resulted in substantially different carbon processing patterns between habitats.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V13C2626D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V13C2626D"><span>Reconstructing Magmatic-<span class="hlt">Hydrothermal</span> Systems via Geologic Mapping of the Tilted, Cross-sectional Exposures of the Yerington District, Nevada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dilles, J. H.; Proffett, J. M.</p> <p>2011-12-01</p> <p>The Jurassic Yerington batholith was cut by Miocene to recent normal faults and tilted ~90° west (Proffett, 1977). Exposures range from the <span class="hlt">volcanic</span> environment to ~6 km depth in the batholith. Magmatic-<span class="hlt">hydrothermal</span> fluids derived from the Luhr Hill granite and associated porphyry dikes produced characteristic porphyry copper mineralization and rock alteration (K-silicate, sericitic, and advanced argillic) in near-vertical columnar zones above cupolas on the deep granite. In addition, saline brines derived from the early Mesozoic <span class="hlt">volcanic</span> and sedimentary section intruded by the batholith were heated and circulated through the batholith producing voluminous sodic-calcic and propylitic alteration. The magnetite-copper ore body at Pumpkin Hollow is hosted in early Mesozoic sedimentary rocks in the contact aureole of the batholith, and appears to be an IOCG type deposit produced where the sedimentary brines exited the batholith. Although many advances in understanding of Yerington have been made by lab-based geochronology and geochemistry studies, the first order igneous and <span class="hlt">hydrothermal</span> features were recognized first in the 1960s and 1970s and are best documented by geological mapping at a variety of scales ranging from 1:500 to 1:24,000. The Anaconda technique of mapping mine benches, trenches, and drill cores was perfected here (Einaudi, 1997), and other techniques were used for surface exposures. The geologic and <span class="hlt">hydrothermal</span> alteration maps establish that <span class="hlt">hydrothermal</span> alteration accompanied each of several porphyry dike intrusions, and affected more than 100 km3 of rock. Both zonation in alteration mineralogy and vein orientations allow reconstruction of source areas and >5 km-long flow-paths of <span class="hlt">hydrothermal</span> fluids through the batholith and contact aureole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001Geo....29.1059V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001Geo....29.1059V"><span><span class="hlt">Hydrothermal</span> element fluxes from Copahue, Argentina: A “beehive” volcano in turmoil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Varekamp, Johan C.; Ouimette, Andrew P.; Herman, Scott W.; Bermúdez, Adriana; Delpino, Daniel</p> <p>2001-11-01</p> <p>Copahue volcano erupted altered rock debris, siliceous dust, pyroclastic sulfur, and rare juvenile fragments between 1992 and 1995, and magmatic eruptions occurred in July October 2000. Prior to 2000, the Copahue crater lake, acid hot springs, and rivers carried acid brines with compositions that reflected close to congruent rock dissolution. The ratio between rock-forming elements and chloride in the central zone of the volcano-<span class="hlt">hydrothermal</span> system has diminished over the past few years, reflecting increased water/rock ratios as a result of progressive rock dissolution. Magmatic <span class="hlt">activity</span> in 2000 provided fresh rocks for the acid fluids, resulting in higher ratios between rock-forming elements and chloride in the fluids and enhanced Mg fluxes. The higher Mg fluxes started several weeks prior to the eruption. Model data on the crater lake and river element flux determinations indicate that Copahue volcano was hollowed out at a rate of about 20000 25000 m3/yr, but that void space was filled with about equal amounts of silica and liquid elemental sulfur. The extensive rock dissolution has weakened the internal <span class="hlt">volcanic</span> structure, making flank collapse a <span class="hlt">volcanic</span> hazard at Copahue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25311770','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25311770"><span>Characterization of the Etna <span class="hlt">volcanic</span> emissions through an <span class="hlt">active</span> biomonitoring technique (moss-bags): part 2--morphological and mineralogical features.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Calabrese, S; D'Alessandro, W</p> <p>2015-01-01</p> <p><span class="hlt">Volcanic</span> emissions were studied at Mount Etna (Italy) by using moss-bags technique. Mosses were exposed around the volcano at different distances from the <span class="hlt">active</span> vents to evaluate the impact of <span class="hlt">volcanic</span> emissions in the atmosphere. Morphology and mineralogy of <span class="hlt">volcanic</span> particulate intercepted by mosses were investigated using scanning electron microscopy (SEM) equipped with energy dispersive spectrometer (EDS). Particles emitted during passive degassing <span class="hlt">activity</span> from the two <span class="hlt">active</span> vents, Bocca Nuova and North East Crater (BNC and NEC), were identified as silicates, sulfates and halide compounds. In addition to <span class="hlt">volcanic</span> particles, we found evidences also of geogenic, anthropogenic and marine spray input. The study has shown the robustness of this <span class="hlt">active</span> biomonitoring technique to collect particles, very useful in <span class="hlt">active</span> <span class="hlt">volcanic</span> areas characterized by continuous degassing and often not easily accessible to apply conventional sampling techniques. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2007/5269/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2007/5269/"><span>2005 <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> in Alaska, Kamchatka, and the Kurile Islands: Summary of Events and Response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, R.G.; Neal, C.A.; Dixon, J.P.; Ushakov, Sergey</p> <p>2008-01-01</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptive <span class="hlt">activity</span> or suspected <span class="hlt">volcanic</span> <span class="hlt">activity</span> at or near 16 volcanoes in Alaska during 2005, including the high profile precursory <span class="hlt">activity</span> associated with the 2005?06 eruption of Augustine Volcano. AVO continues to participate in distributing information about eruptive <span class="hlt">activity</span> on the Kamchatka Peninsula, Russia, and in the Kurile Islands of the Russian Far East, in conjunction with the Kamchatkan <span class="hlt">Volcanic</span> Eruption Response Team (KVERT) and the Sakhalin <span class="hlt">Volcanic</span> Eruption Response Team (SVERT), respectively. In 2005, AVO helped broadcast alerts about <span class="hlt">activity</span> at 8 Russian volcanoes. The most serious hazard posed from <span class="hlt">volcanic</span> eruptions in Alaska, Kamchatka, or the Kurile Islands is the placement of ash into the atmosphere at altitudes traversed by jet aircraft along the North Pacific and Russian Trans East air routes. AVO, KVERT, and SVERT work collaboratively with the National Weather Service, Federal Aviation Administration, and the <span class="hlt">Volcanic</span> Ash Advisory Centers to provide timely warnings of <span class="hlt">volcanic</span> eruptions and the production and movement of ash clouds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1456/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1456/"><span>The Geology and Remarkable Thermal <span class="hlt">Activity</span> of Norris Geyser Basin, Yellowstone National Park, Wyoming</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>White, Donald Edward; Hutchinson, Roderick A.; Keith, Terry E.C.</p> <p>1988-01-01</p> <p>Norris Geyser Basin, normally shortened to Norris Basin, is adjacent to the north rim of the Yellowstone caldera at the common intersection of the caldera rim and the Norris-Mammoth Corridor, a zone of faults, <span class="hlt">volcanic</span> vents, and thermal <span class="hlt">activity</span> that strikes north from the caldera rim to Mammoth Hot Springs. An east-west fault zone terminates the Gallatin Range at its southern end and extends from Hebgen Lake, west of the park, to Norris Basin. No local evidence exists at the surface in Norris Basin for the two oldest Yellowstone <span class="hlt">volcanic</span> caldera cycles (~2.0 and 1.3 m.y.B.P.). The third and youngest cycle formed the Yellowstone caldera, which erupted the 600,000-year-old Lava Creek Tuff. No evidence is preserved of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> near Norris Basin during the first 300,000.years after the caldera collapse. Glaciation probably removed most of the early evidence, but erratics of hot-spring sinter that had been converted diagenetically to extremely hard, resistant chalcedonic sinter are present as cobbles in and on some moraines and till from the last two glacial stages, here correlated with the early and late stages of the Pinedale glaciation <150,000 years B.P.). Indirect evidence for the oldest <span class="hlt">hydrothermal</span> system at Norris Basin indicates an age probably older than both stages of Pinedale glaciation. Stream deposits consisting mainly of rounded quartz phenocrysts of the Lava Creek Tuff were subaerial, perhaps in part windblown and redeposited by streams. A few small rounded pebbles are interpreted as chalcedonic sinter of a still older cycle. None of these are precisely dated but are unlikely to be more than 150,000 to 200,000 years old. ...Most studies of <span class="hlt">active</span> <span class="hlt">hydrothermal</span> areas have noted chemical differences in fluids and alteration products but have given little attention to differences and models to explain evolution in types. This report, in contrast, emphasizes the kinds of changes in vents and their changing chemical types of waters and then</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNS43C1929Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNS43C1929Z"><span>Geothermic analysis of high temperature <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> area in Western plateau of Sichuan province, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, J.</p> <p>2016-12-01</p> <p>There is a high temperature <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> area in the western plateau of Sichuan. More than 200 hot springs points have been found in the region, including 11 hot spring water temperature above local boiling point. Most of these distribute along Jinshajjiang fracture, Dege-Xiangcheng fracture, Ganzi-Litang fracture as well as Xianshuihe fracture, and form three high-temperature <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> strips in the NW-SE direction. Using gravity, magnetic, seismic and helium isotope data, this paper analyzed the crust-mantle heat flow structure, crustal heat source distribution and water heating system. The results show that the geothermal <span class="hlt">activity</span> mainly controlled by the "hot" crust. The ratio of crustal heat flow and surface heat flow is higher than 60%. In the high temperature <span class="hlt">hydrothermal</span> <span class="hlt">activities</span> area, there is lower S wave velocity zone with Vs<3.2 km/s in 15 30 km depth in middle and lower crust. Basing on the S wave velocity inversion temperature of crust-mantle, it has been found that there is a high temperature layer with 850 1000 ° in 20 40 km depth. It is the main heat source of high temperature <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> area of western Sichuan. Our argument is that atmospheric precipitation, surface water infiltrated along the fault fracture into the crustal deep, heating by crustal hot source, and circulation to surface become high temperature hot water. Geothermal water mainly reserve in the Triassic strata of the containing water good carbonate rocks, and in the intrusive granite which is along the fault zone. The thermal energy of Surface heat thermal <span class="hlt">activities</span> mainly comes from the high-temperature hot source which is located in the middle and lower crust. Being in the deep crustal fracture, the groundwater infiltrated to the deep crust and absorbed heat, then, quickly got back to the surface and formed high hot springs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060036527&hterms=right+Mexican&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dright%2BMexican','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060036527&hterms=right+Mexican&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dright%2BMexican"><span>(abstract) Survey of <span class="hlt">Volcanic</span> Hazards in the Trans Mexican <span class="hlt">Volcanic</span> Belt</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abrams, M.; Siebe, C.; Macias, J.</p> <p>1997-01-01</p> <p>A substantial percentage of the world's population lives in areas vulnerable to the negative effects of future <span class="hlt">volcanic</span> <span class="hlt">activity</span>. This is especially true in Mexico, where within the Trans Mexican <span class="hlt">Volcanic</span> Belt (TMVB) one half of the country's 90 million inhabitants live. The TMVB is a 1 000 by 200 km area, dotted with hundreds of volcanoes and <span class="hlt">volcanic</span> centers. Most of the area has been poorly studied, and the <span class="hlt">volcanic</span> history is largely unknown. Our approach is to combine interpretations of satellite images, field work and mapping, laboratory analysis, and age dating to elucidate the <span class="hlt">volcanic</span> history and evaluate the potential eruptive hazards. Hazards evaluations are done in the form of risk maps.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26892716','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26892716"><span>Monitoring eruption <span class="hlt">activity</span> using temporal stress changes at Mount Ontake volcano.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Terakawa, Toshiko; Kato, Aitaro; Yamanaka, Yoshiko; Maeda, Yuta; Horikawa, Shinichiro; Matsuhiro, Kenjiro; Okuda, Takashi</p> <p>2016-02-19</p> <p><span class="hlt">Volcanic</span> <span class="hlt">activity</span> is often accompanied by many small earthquakes. Earthquake focal mechanisms represent the fault orientation and slip direction, which are influenced by the stress field. Focal mechanisms of volcano-tectonic earthquakes provide information on the state of volcanoes via stresses. Here we demonstrate that quantitative evaluation of temporal stress changes beneath Mt. Ontake, Japan, using the misfit angles of focal mechanism solutions to the regional stress field, is effective for eruption monitoring. The moving average of misfit angles indicates that during the precursory period the local stress field beneath Mt. Ontake was deviated from the regional stress field, presumably by stress perturbations caused by the inflation of magmatic/<span class="hlt">hydrothermal</span> fluids, which was removed immediately after the expulsion of <span class="hlt">volcanic</span> ejecta. The deviation of the local stress field can be an indicator of increases in <span class="hlt">volcanic</span> <span class="hlt">activity</span>. The proposed method may contribute to the mitigation of <span class="hlt">volcanic</span> hazards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4762890','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4762890"><span>Monitoring eruption <span class="hlt">activity</span> using temporal stress changes at Mount Ontake volcano</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Terakawa, Toshiko; Kato, Aitaro; Yamanaka, Yoshiko; Maeda, Yuta; Horikawa, Shinichiro; Matsuhiro, Kenjiro; Okuda, Takashi</p> <p>2016-01-01</p> <p><span class="hlt">Volcanic</span> <span class="hlt">activity</span> is often accompanied by many small earthquakes. Earthquake focal mechanisms represent the fault orientation and slip direction, which are influenced by the stress field. Focal mechanisms of volcano-tectonic earthquakes provide information on the state of volcanoes via stresses. Here we demonstrate that quantitative evaluation of temporal stress changes beneath Mt. Ontake, Japan, using the misfit angles of focal mechanism solutions to the regional stress field, is effective for eruption monitoring. The moving average of misfit angles indicates that during the precursory period the local stress field beneath Mt. Ontake was deviated from the regional stress field, presumably by stress perturbations caused by the inflation of magmatic/<span class="hlt">hydrothermal</span> fluids, which was removed immediately after the expulsion of <span class="hlt">volcanic</span> ejecta. The deviation of the local stress field can be an indicator of increases in <span class="hlt">volcanic</span> <span class="hlt">activity</span>. The proposed method may contribute to the mitigation of <span class="hlt">volcanic</span> hazards. PMID:26892716</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V21E2364S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V21E2364S"><span>Phreatic and <span class="hlt">Hydrothermal</span> Explosions: A Laboratory Approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scheu, B.; Dingwell, D. B.</p> <p>2010-12-01</p> <p>Phreatic eruptions are amongst the most common eruption types on earth. They might be precursory to another type of <span class="hlt">volcanic</span> eruption but often they stand on their one. Despite being the most common eruption type, they also are one of the most diverse eruptions, in appearance as well as on eruption mechanism. Yet steam is the common fuel behind all phreatic eruptions. The steam-driven explosions occur when water beneath the ground or on the surface is heated by magma, lava, hot rocks, or fresh <span class="hlt">volcanic</span> deposits (such as ignimbrites, tephra and pyroclastic-flow deposits) and result in crater, tuff rings and debris avalanches. The intense heat of such material may cause water to boil and flash to steam, thereby generating an explosion of steam, water, ash, blocks, and bombs. Another wide and important field affected by phreatic explosions are <span class="hlt">hydrothermal</span> areas; here phreatic explosions occur every few months creating explosion craters and resemble a significant hazard to <span class="hlt">hydrothermal</span> power plants. Despite of their hazard potential, phreatic explosions have so far been overlooked by the field of experimental volcanology. A part of their hazard potential in owned by the fact that phreatic explosions are hardly predictable in occurrence time and size as they have manifold triggers (variances in groundwater and heat systems, earthquakes, material fatigue, water level, etc..) A new set of experiments has been designed to focus on this phreatic type of steam explosion, whereas classical phreatomagmatic experiments use molten fuel-coolant interaction (e.g., Zimanowski, et al., 1991). The violent transition of the superheated water to vapour adds another degree of explosivity to the dry magmatic fragmentation, driven mostly by vesicle bursting due to internal gas overpressure. At low water fractions the fragmentation is strongly enforced by the mixture of these two effects and a large fraction of fine pyroclasts are produced, whereas at high water fraction in the sample the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51K..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51K..04C"><span>The response of tropical cyclone <span class="hlt">activity</span> to tropospheric aerosols, greenhouse gases and <span class="hlt">volcanic</span> eruptions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Camargo, S. J.; Sobel, A. H.; Polvani, L. M.; Emanuel, K.; Previdi, M. J.</p> <p>2017-12-01</p> <p>Previous work has shown that aerosol cooling reduces tropical cyclone (TC) potential intensity (PI) more strongly than greenhouse gas warming increases it. This has the consequence that PI shows only small increases in simulations of the historical period despite considerable global warming over that period. We use CMIP5 models, as well as offline radiative kernels, to better understand this result. The outsize effect of aerosol forcing is a consequence of the fact that tropospheric aerosols act in the shortwave while greenhouse gases act in the longwave. Shortwave forcing has a greater impact on PI than does longwave, because of the differences in the response of the surface energy budget to the direct, temperature-independent component of the forcing. Shortwave forcing mainly drives the climate system in the surface, while greenhouse gases do so at the top of the atmosphere, so that net longwave flux associated with a temperature change can be small, especially at high temperature. Our kernel results also indicate that the temperature-dependent longwave feedback component is also greater by approximately a factor of two for the shortwave than the longwave forcing. Recent papers using observations and proxy reconstructions suggested a reduction of frequency, duration and intensity of Atlantic TCs in the years following <span class="hlt">volcanic</span> eruptions. Observations show no significant reduction of TC <span class="hlt">activity</span> in the first season after three large <span class="hlt">volcanic</span> eruptions in the 20th Century, with the exception of the North Atlantic. The response to these <span class="hlt">volcanic</span> eruptions cannot be separated from the coinciding El Niño events either in observations or in reanalysis. Both the NCAR Large Ensemble and CMIP5 models show a strong reduction in the PI following large <span class="hlt">volcanic</span> eruptions. But, given that the models response to <span class="hlt">volcanic</span> aerosols is known to be too strong, when a bias correction is considered, the PI signal after the <span class="hlt">volcanic</span> eruptions becomes much smaller. Furthermore, there</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JPhCS.333a2016V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JPhCS.333a2016V"><span>Search for possible relationship between <span class="hlt">volcanic</span> ash particles and thunderstorm lightning <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Várai, A.; Vincze, M.; Lichtenberger, J.; Jánosi, I. M.</p> <p>2011-12-01</p> <p>Explosive <span class="hlt">volcanic</span> eruptions that eject columns of ash from the crater often generate lightning discharges strong enough to be remotely located by very low frequency radio waves. A fraction of <span class="hlt">volcanic</span> ash particles can stay and disperse long enough to have an effect on weather phenomena days later such as thunderstorms and lightnings. In this work we report on lightning <span class="hlt">activity</span> analysis over Europe following two recent series of <span class="hlt">volcanic</span> eruptions in order to identify possible correlations between ash release and subsequent thunderstorm flash frequency. Our attempts gave negative results which can be related to the fact that we have limited information on local atmospheric variables of high enough resolution, however lightning frequency is apparently determined by very local circumstances.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29035265','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29035265"><span><span class="hlt">Hydrothermal</span> impacts on trace element and isotope ocean biogeochemistry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>German, C R; Casciotti, K A; Dutay, J-C; Heimbürger, L E; Jenkins, W J; Measures, C I; Mills, R A; Obata, H; Schlitzer, R; Tagliabue, A; Turner, D R; Whitby, H</p> <p>2016-11-28</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> occurs in all ocean basins, releasing high concentrations of key trace elements and isotopes (TEIs) into the oceans. Importantly, the calculated rate of entrainment of the entire ocean volume through turbulently mixing buoyant <span class="hlt">hydrothermal</span> plumes is so vigorous as to be comparable to that of deep-ocean thermohaline circulation. Consequently, biogeochemical processes <span class="hlt">active</span> within deep-ocean <span class="hlt">hydrothermal</span> plumes have long been known to have the potential to impact global-scale biogeochemical cycles. More recently, new results from GEOTRACES have revealed that plumes rich in dissolved Fe, an important micronutrient that is limiting to productivity in some areas, are widespread above mid-ocean ridges and extend out into the deep-ocean interior. While Fe is only one element among the full suite of TEIs of interest to GEOTRACES, these preliminary results are important because they illustrate how inputs from seafloor venting might impact the global biogeochemical budgets of many other TEIs. To determine the global impact of seafloor venting, however, requires two key questions to be addressed: (i) What processes are <span class="hlt">active</span> close to vent sites that regulate the initial high-temperature <span class="hlt">hydrothermal</span> fluxes for the full suite of TEIs that are dispersed through <span class="hlt">non</span>-buoyant <span class="hlt">hydrothermal</span> plumes? (ii) How do those processes vary, globally, in response to changing geologic settings at the seafloor and/or the geochemistry of the overlying ocean water? In this paper, we review key findings from recent work in this realm, highlight a series of key hypotheses arising from that research and propose a series of new GEOTRACES modelling, section and process studies that could be implemented, nationally and internationally, to address these issues.This article is part of the themed issue 'Biological and climatic impacts of ocean trace element chemistry'. © 2015 The Authors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5069535','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5069535"><span><span class="hlt">Hydrothermal</span> impacts on trace element and isotope ocean biogeochemistry</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Dutay, J.-C.; Heimbürger, L. E.; Jenkins, W. J.; Measures, C. I.; Mills, R. A.; Obata, H.; Turner, D. R.; Whitby, H.</p> <p>2016-01-01</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activity</span> occurs in all ocean basins, releasing high concentrations of key trace elements and isotopes (TEIs) into the oceans. Importantly, the calculated rate of entrainment of the entire ocean volume through turbulently mixing buoyant <span class="hlt">hydrothermal</span> plumes is so vigorous as to be comparable to that of deep-ocean thermohaline circulation. Consequently, biogeochemical processes <span class="hlt">active</span> within deep-ocean <span class="hlt">hydrothermal</span> plumes have long been known to have the potential to impact global-scale biogeochemical cycles. More recently, new results from GEOTRACES have revealed that plumes rich in dissolved Fe, an important micronutrient that is limiting to productivity in some areas, are widespread above mid-ocean ridges and extend out into the deep-ocean interior. While Fe is only one element among the full suite of TEIs of interest to GEOTRACES, these preliminary results are important because they illustrate how inputs from seafloor venting might impact the global biogeochemical budgets of many other TEIs. To determine the global impact of seafloor venting, however, requires two key questions to be addressed: (i) What processes are <span class="hlt">active</span> close to vent sites that regulate the initial high-temperature <span class="hlt">hydrothermal</span> fluxes for the full suite of TEIs that are dispersed through <span class="hlt">non</span>-buoyant <span class="hlt">hydrothermal</span> plumes? (ii) How do those processes vary, globally, in response to changing geologic settings at the seafloor and/or the geochemistry of the overlying ocean water? In this paper, we review key findings from recent work in this realm, highlight a series of key hypotheses arising from that research and propose a series of new GEOTRACES modelling, section and process studies that could be implemented, nationally and internationally, to address these issues. This article is part of the themed issue ‘Biological and climatic impacts of ocean trace element chemistry’. PMID:29035265</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/2017JGRB..12210241M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..12210241M"><span>Seismic Signatures of <span class="hlt">Hydrothermal</span> Pathways Along the East Pacific Rise Between 9°16' and 9°56'N</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marjanović, Milena; Fuji, Nobuaki; Singh, Satish C.; Belahi, Thomas; Escartín, Javier</p> <p>2017-12-01</p> <p>We apply wave equation-based techniques to 2-D seismic data to characterize the nature of zero-age upper crust at the East Pacific Rise from 9°16' to 9°56'N. The final velocity model reveals a number of low-velocity anomalies, complex in shape, extending down to 1 km below the seafloor. We attribute them to the presence of <span class="hlt">hydrothermal</span> flow. Depending on their spatial correlation with the previously identified tectonic discontinuities in bathymetry and presence of venting, we classify them as downgoing and upgoing pathways, respectively. This distinction is not always clear; within the third-order discontinuities at 9°20' and 9°37'N, both pathways may be present. The region north of 9°44'N, known for its magmatic robustness and <span class="hlt">volcanic</span> <span class="hlt">activity</span>, is represented by five low-velocity perturbations. Three of these anomalies are spatially correlated with the fourth-order discontinuities and attributed to the presence of the on-axis recharge zones. The remaining two anomalies underlie two vent clusters, marked as <span class="hlt">hydrothermally</span> <span class="hlt">active</span> sites after the last documented eruption event. These velocity anomalies can be thus identified as the up-flow pathways or at least their remnants. By comparing our results to the available interdisciplinary data sets, we show that the interaction between the tectono-magmatic and <span class="hlt">hydrothermal</span> processes is not straightforward due to different timescales at which they operate. However, for developing, maintaining, and driving vigorous, high-temperature <span class="hlt">hydrothermal</span> flow, the high crustal permeability and high thermal regime must coexist in time and space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1044a/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1044a/report.pdf"><span>The <span class="hlt">hydrothermal</span> system of Long Valley Caldera, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sorey, M.L.; Lewis, Robert Edward; Olmsted, F.H.</p> <p>1978-01-01</p> <p>Long Valley caldera, an elliptical depression covering 450 km 2 on the eastern front of the Sierra Nevada in east-central California, contains a hot-water convection system with numerous hot springs and measured and estimated aquifer temperatures at depths of 180?C to 280?C. In this study we have synthesized the results of previous geologic, geophysical, geochemical, and hydrologic investigations of the Long Valley area to develop a generalized conceptual and mathematical model which describes the gross features of heat and fluid flow in the <span class="hlt">hydrothermal</span> system. Cenozoic <span class="hlt">volcanism</span> in the Long Valley region began about 3.2 m.y. (million years) ago and has continued intermittently until the present time. The major event that resulted in the formation of the Long Valley caldera took place about 0.7 m.y. ago with the eruption of 600 km 3 or more of Bishop Tuff of Pleistocene age, a rhyolitic ash flow, and subsequent collapse of the roof of the magma chamber along one or more steeply inclined ring fractures. Subsequent intracaldera <span class="hlt">volcanism</span> and uplift of the west-central part of the caldera floor formed a subcircular resurgent dome about 10 km in diameter surrounded by a moat containing rhyolitic, rhyodacitic, and basaltic rocks ranging in age from 0.5 to 0.05 m.y. On the basis of gravity and seismic studies, we estimate an aver- age thickness of fill of 2.4 km above the precaldera granitic and metamorphic basement rocks. A continuous layer of densely welded Bishop Tuff overlies the basement rocks, with an average thickness of 1.4 km; the fill above the welded Bishop Tuff consists of intercalated <span class="hlt">volcanic</span> flows and tuffs and fluvial and lacustrine deposits. Assuming the average grain density of the fill is between 2.45 and 2.65 g/cm 3 , we calculate the average bulk porosity of the total fill as from 0.11 to 0.21. Comparison of published values of porosity of the welded Bishop Tuff exposed southeast of the caldera with calculated values indicates average bulk porosity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EP%26S...70...72T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EP%26S...70...72T"><span>Contention between supply of <span class="hlt">hydrothermal</span> fluid and conduit obstruction: inferences from numerical simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, Ryo; Hashimoto, Takeshi; Matsushima, Nobuo; Ishido, Tsuneo</p> <p>2018-05-01</p> <p>We investigate a <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> system using numerical simulations, focusing on change in crater temperature. Both increases and decreases in crater temperature have been observed before phreatic eruptions. We follow the system's response for up to a decade after <span class="hlt">hydrothermal</span> fluid flux from the deep part of the system is increased and permeability is reduced at a certain depth in a conduit. Our numerical simulations demonstrate that: (1) changes in crater temperature are controlled by the magnitude of the increase in <span class="hlt">hydrothermal</span> fluid flux and the degree of permeability reduction; (2) significant increases in <span class="hlt">hydrothermal</span> flux with decreases in permeability induce substantial pressure changes in shallow depths in the edifice and decreases in crater temperature; (3) the location of maximum pressure change differs between the mechanisms. The results of this study imply that it is difficult to predict eruptions by crater temperature change alone. One should be as wary of large eruptions when crater temperature decreases as when crater temperature increases. It is possible to clarify the implications of changes in crater temperature with simultaneous observation of ground deformation.[Figure not available: see fulltext.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997E%26PSL.153..239F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997E%26PSL.153..239F"><span>Tide-related variability of TAG <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> observed by deep-sea monitoring system and OBSH</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fujioka, Kantaro; Kobayashi, Kazuo; Kato, Kazuhiro; Aoki, Misumi; Mitsuzawa, Kyohiko; Kinoshita, Masataka; Nishizawa, Azusa</p> <p>1997-12-01</p> <p><span class="hlt">Hydrothermal</span> <span class="hlt">activities</span> were monitored by an ocean bottom seismometer with hydrophone (OBSH) and a composite measuring system (Manatee) including CTD, current meter, transmission meter and cameras at a small depression on the TAG <span class="hlt">hydrothermal</span> mound in the Mid-Atlantic Ridge. Low-frequency pressure pulses detected by the hydrophone with semi-diurnal periodicity seem to correspond to cycles of <span class="hlt">hydrothermal</span> upflow from a small and short-lived smoker vent close to the observing site. The peaks of pressure pulses are synchronous with the maximum gradient of areal strain decrease due to tidal load release. Microearthquakes with very near epicenters occur sporadically and do not appear to be directly correlatable to <span class="hlt">hydrothermal</span> venting. Temporal variations in bottom water temperature also have semi-diurnal periodicity but are more complicated than the pressure events. Temperatures may be affected both by upwelling of hot water and by lateral flow of the bottom current changing its directions with ocean tide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26PSL.442..218D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.442..218D"><span>Short-period <span class="hlt">volcanic</span> gas precursors to phreatic eruptions: Insights from Poás Volcano, Costa Rica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Moor, J. M.; Aiuppa, A.; Pacheco, J.; Avard, G.; Kern, C.; Liuzzo, M.; Martínez, M.; Giudice, G.; Fischer, T. P.</p> <p>2016-05-01</p> <p><span class="hlt">Volcanic</span> eruptions involving interaction with water are amongst the most violent and unpredictable geologic phenomena on Earth. Phreatic eruptions are exceptionally difficult to forecast by traditional geophysical techniques. Here we report on short-term precursory variations in gas emissions related to phreatic blasts at Poás volcano, Costa Rica, as measured with an in situ multiple gas analyzer that was deployed at the edge of the erupting lake. Gas emitted from this hyper-acid crater lake approaches magmatic values of SO2/CO2 1-6 days prior to eruption. The SO2 flux derived from magmatic degassing through the lake is measureable by differential optical absorption spectrometry (sporadic campaign measurements), which allows us to constrain lake gas output and input for the major gas species during eruptive and <span class="hlt">non</span>-eruptive periods. We can further calculate power supply to the <span class="hlt">hydrothermal</span> system using volatile mass balance and thermodynamics, which indicates that the magmatic heat flux into the shallow <span class="hlt">hydrothermal</span> system increases from ∼27 MW during quiescence to ∼59 MW during periods of phreatic events. These transient pulses of gas and heat from the deeper magmatic system generate both phreatic eruptions and the observed short-term changes in gas composition, because at high gas flux scrubbing of sulfur by the <span class="hlt">hydrothermal</span> system is both kinetically and thermodynamically inhibited whereas CO2 gas is always essentially inert in hyperacid conditions. Thus, the SO2/CO2 of lake emissions approaches magmatic values as gas and power supply to the sub-limnic <span class="hlt">hydrothermal</span> system increase, vaporizing fluids and priming the <span class="hlt">hydrothermal</span> system for eruption. Our results suggest that high-frequency real-time gas monitoring could provide useful short-term eruptive precursors at volcanoes prone to phreatic explosions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175484','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175484"><span>Short-period <span class="hlt">volcanic</span> gas precursors to phreatic eruptions: Insights from Poás Volcano, Costa Rica</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>de Moor, Maarten; Aiuppa, Alessandro; Pacheco, Javier; Avard, Geoffroy; Kern, Christoph; Liuzzo, Marco; Martinez, Maria; Giudice, Gaetano; Fischer, Tobias P.</p> <p>2016-01-01</p> <p><span class="hlt">Volcanic</span> eruptions involving interaction with water are amongst the most violent and unpredictable geologic phenomena on Earth. Phreatic eruptions are exceptionally difficult to forecast by traditional geophysical techniques. Here we report on short-term precursory variations in gas emissions related to phreatic blasts at Poás volcano, Costa Rica, as measured with an in situ multiple gas analyzer that was deployed at the edge of the erupting lake. Gas emitted from this hyper-acid crater lake approaches magmatic values of SO2/CO2 1–6 days prior to eruption. The SO2 flux derived from magmatic degassing through the lake is measureable by differential optical absorption spectrometry (sporadic campaign measurements), which allows us to constrain lake gas output and input for the major gas species during eruptive and <span class="hlt">non</span>-eruptive periods. We can further calculate power supply to the <span class="hlt">hydrothermal</span> system using volatile mass balance and thermodynamics, which indicates that the magmatic heat flux into the shallow <span class="hlt">hydrothermal</span> system increases from ∼27 MW during quiescence to ∼59 MW during periods of phreatic events. These transient pulses of gas and heat from the deeper magmatic system generate both phreatic eruptions and the observed short-term changes in gas composition, because at high gas flux scrubbing of sulfur by the <span class="hlt">hydrothermal</span> system is both kinetically and thermodynamically inhibited whereas CO2gas is always essentially inert in hyperacid conditions. Thus, the SO2/CO2 of lake emissions approaches magmatic values as gas and power supply to the sub-limnic <span class="hlt">hydrothermal</span> system increase, vaporizing fluids and priming the <span class="hlt">hydrothermal</span> system for eruption. Our results suggest that high-frequency real-time gas monitoring could provide useful short-term eruptive precursors at volcanoes prone to phreatic explosions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...629899R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...629899R"><span>Volcano electrical tomography unveils edifice collapse hazard linked to <span class="hlt">hydrothermal</span> system structure and dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rosas-Carbajal, Marina; Komorowski, Jean-Christophe; Nicollin, Florence; Gibert, Dominique</p> <p>2016-07-01</p> <p>Catastrophic collapses of the flanks of stratovolcanoes constitute a major hazard threatening numerous lives in many countries. Although many such collapses occurred following the ascent of magma to the surface, many are not associated with magmatic reawakening but are triggered by a combination of forcing agents such as pore-fluid pressurization and/or mechanical weakening of the <span class="hlt">volcanic</span> edifice often located above a low-strength detachment plane. The volume of altered rock available for collapse, the dynamics of the <span class="hlt">hydrothermal</span> fluid reservoir and the geometry of incipient collapse failure planes are key parameters for edifice stability analysis and modelling that remain essentially hidden to current volcano monitoring techniques. Here we derive a high-resolution, three-dimensional electrical conductivity model of the La Soufrière de Guadeloupe volcano from extensive electrical tomography data. We identify several highly conductive regions in the lava dome that are associated to fluid saturated host-rock and preferential flow of highly acid hot fluids within the dome. We interpret this model together with the existing wealth of geological and geochemical data on the volcano to demonstrate the influence of the <span class="hlt">hydrothermal</span> system dynamics on the hazards associated to collapse-prone altered <span class="hlt">volcanic</span> edifices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27457494','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27457494"><span>Volcano electrical tomography unveils edifice collapse hazard linked to <span class="hlt">hydrothermal</span> system structure and dynamics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rosas-Carbajal, Marina; Komorowski, Jean-Christophe; Nicollin, Florence; Gibert, Dominique</p> <p>2016-07-26</p> <p>Catastrophic collapses of the flanks of stratovolcanoes constitute a major hazard threatening numerous lives in many countries. Although many such collapses occurred following the ascent of magma to the surface, many are not associated with magmatic reawakening but are triggered by a combination of forcing agents such as pore-fluid pressurization and/or mechanical weakening of the <span class="hlt">volcanic</span> edifice often located above a low-strength detachment plane. The volume of altered rock available for collapse, the dynamics of the <span class="hlt">hydrothermal</span> fluid reservoir and the geometry of incipient collapse failure planes are key parameters for edifice stability analysis and modelling that remain essentially hidden to current volcano monitoring techniques. Here we derive a high-resolution, three-dimensional electrical conductivity model of the La Soufrière de Guadeloupe volcano from extensive electrical tomography data. We identify several highly conductive regions in the lava dome that are associated to fluid saturated host-rock and preferential flow of highly acid hot fluids within the dome. We interpret this model together with the existing wealth of geological and geochemical data on the volcano to demonstrate the influence of the <span class="hlt">hydrothermal</span> system dynamics on the hazards associated to collapse-prone altered <span class="hlt">volcanic</span> edifices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3111178','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3111178"><span>The Biological Deep Sea <span class="hlt">Hydrothermal</span> Vent as a Model to Study Carbon Dioxide Capturing Enzymes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Minic, Zoran; Thongbam, Premila D.</p> <p>2011-01-01</p> <p>Deep sea <span class="hlt">hydrothermal</span> vents are located along the mid-ocean ridge system, near <span class="hlt">volcanically</span> <span class="hlt">active</span> areas, where tectonic plates are moving away from each other. Sea water penetrates the fissures of the <span class="hlt">volcanic</span> bed and is heated by magma. This heated sea water rises to the surface dissolving large amounts of minerals which provide a source of energy and nutrients to chemoautotrophic organisms. Although this environment is characterized by extreme conditions (high temperature, high pressure, chemical toxicity, acidic pH and absence of photosynthesis) a diversity of microorganisms and many animal species are specially adapted to this hostile environment. These organisms have developed a very efficient metabolism for the assimilation of inorganic CO2 from the external environment. In order to develop technology for the capture of carbon dioxide to reduce greenhouse gases in the atmosphere, enzymes involved in CO2 fixation and assimilation might be very useful. This review describes some current research concerning CO2 fixation and assimilation in the deep sea environment and possible biotechnological application of enzymes for carbon dioxide capture. PMID:21673885</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21673885','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21673885"><span>The biological deep sea <span class="hlt">hydrothermal</span> vent as a model to study carbon dioxide capturing enzymes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Minic, Zoran; Thongbam, Premila D</p> <p>2011-01-01</p> <p>Deep sea <span class="hlt">hydrothermal</span> vents are located along the mid-ocean ridge system, near <span class="hlt">volcanically</span> <span class="hlt">active</span> areas, where tectonic plates are moving away from each other. Sea water penetrates the fissures of the <span class="hlt">volcanic</span> bed and is heated by magma. This heated sea water rises to the surface dissolving large amounts of minerals which provide a source of energy and nutrients to chemoautotrophic organisms. Although this environment is characterized by extreme conditions (high temperature, high pressure, chemical toxicity, acidic pH and absence of photosynthesis) a diversity of microorganisms and many animal species are specially adapted to this hostile environment. These organisms have developed a very efficient metabolism for the assimilation of inorganic CO₂ from the external environment. In order to develop technology for the capture of carbon dioxide to reduce greenhouse gases in the atmosphere, enzymes involved in CO₂ fixation and assimilation might be very useful. This review describes some current research concerning CO₂ fixation and assimilation in the deep sea environment and possible biotechnological application of enzymes for carbon dioxide capture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7203Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7203Z"><span>Geophysical characterization of an <span class="hlt">active</span> <span class="hlt">hydrothermal</span> shear zone in granitic rocks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zahner, Tobias; Baron, Ludovic; Holliger, Klaus; Egli, Daniel</p> <p>2016-04-01</p> <p><span class="hlt">Hydrothermally</span> <span class="hlt">active</span> faults and shear zones in the crystalline massifs of the central Alps are currently of particular interest because of their potential similarities and analogies with planned deep petrothermal reservoirs in the Alpine foreland. In order to better understand such <span class="hlt">hydrothermal</span> systems, a near-vertical, <span class="hlt">hydrothermally</span> <span class="hlt">active</span> shear zone embedded in low-permeability granitic rocks has been drilled. This borehole is located on the Grimsel Pass in the central Swiss Alps, has an inclination of 24 degrees with regard to the vertical, and crosses the targeted shear zone between about 82 and 86 meters depth. The borehole has been fully cored and a comprehensive suite of geophysical logging data has been acquired. The latter comprises multi-frequency sonic, ground-penetrating radar, resistivity, self-potential, gamma-gamma, neutron-neutron, optical televiewer, and caliper log data. In addition to this, we have also performed a surface-to-borehole vertical seismic profiling experiment. The televiewer data and the retrieved core samples show a marked increase of the fracture density in the target region, which also finds its expression in rather pronounced and distinct signatures in all other log data. Preliminary results point towards a close correspondence between the ground-penetrating radar and the neutron-neutron log data, which opens the perspective of constraining the effective fracture porosity at vastly differing scales. There is also remarkably good agreement between the sonic log and the vertical seismic profiling data, which may allow for assessing the permeability of the probed fracture network by interpreting these data in a poroelastic context.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1996/0738/tableofcontents.html','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1996/0738/tableofcontents.html"><span>1995 <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Alaska and Kamchatka: summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Neal, Christina A.</p> <p>1996-01-01</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptive <span class="hlt">activity</span> or suspected <span class="hlt">volcanic</span> <span class="hlt">activity</span> (SVA) at 6 <span class="hlt">volcanic</span> centers in 1995: Mount Martin (Katmai Group), Mount Veniaminof, Shishaldin, Makushin, Kliuchef/Korovin, and Kanaga. In addition to responding to eruptive <span class="hlt">activity</span> at Alaska volcanoes, AVO also disseminated information for the Kamchatkan <span class="hlt">Volcanic</span> Eruption Response Team (KVERT) on the 1995 eruptions of 2 Russian volcanoes: Bezymianny and Karymsky. This report summarizes <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Alaska during 1995 and the AVO response, as well as information on the 2 Kamchatkan eruptions. Only those reports or inquiries that resulted in a "significant" investment of staff time and energy (here defined as several hours or more for reaction, tracking, and follow-up) are included. AVO typically receives dozens of phone calls throughout the year reporting steaming, unusual cloud sightings, or eruption rumors. Most of these are resolved quickly and are not tabulated here as part of the 1995 response record.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.V52G..08B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.V52G..08B"><span>Large Volume 18O-depleted Rhyolitic <span class="hlt">Volcanism</span>: the Bruneau-Jarbidge <span class="hlt">Volcanic</span> Field, Idaho</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boroughs, S.; Wolff, J.; Bonnichsen, B.; Godchaux, M. M.; Larson, P. B.</p> <p>2003-12-01</p> <p>The Bruneau-Jarbidge (BJ) <span class="hlt">volcanic</span> field is located in southern Idaho at the intersection of the western and eastern arms of the Snake River Plain. The BJ region is an oval structural basin of about 6000 km2, and is likely a system of nested caldera and collapse structures similar to, though larger than, the Yellowstone <span class="hlt">Volcanic</span> Plateau. BJ rocks are high-temperature rhyolite tuffs, high-temperature rhyolite lavas, and volumetrically minor basalts. Exposed volumes of individual rhyolite units range up to greater than 500 km3. We have analyzed feldspar and, where present, quartz from 30 rhyolite units emplaced throughout the history of the BJ center. All, including the Cougar Point Tuff, are 18O depleted (δ 18OFSP = -1.3 to 3.7‰ ), while petrographically, temporally, and chemically similar lavas erupted along the nearby Owyhee Front have "normal" rhyolite magmatic δ 18O values of 7 - 9‰ . There is no evidence for significant modification of δ 18O values by post-eruptive alteration. No correlation exists between δ 18O and age, magmatic temperature, major element composition or trace element abundances among depleted BJ rhyolites. The BJ and WSRP rhyolites possess the geochemical characteristics (depressed Al, Ca, Eu, and Sr contents, high Ga/Al and K/Na) expected of liquids derived from shallow melting of calc-alkaline granitoids with residual plagioclase and orthopyroxene (Patino-Douce, Geology v.25 p.743-746, 1997). The classic Yellowstone low δ 18O rhyolites are post-caldera collapse lavas, but at BJ, both lavas and caldera-forming ignimbrites are strongly 18O-depleted. The total volume of low δ 18O rhyolite may be as high as 10,000 km3, requiring massive involvement of meteoric-<span class="hlt">hydrothermally</span> altered crust in rhyolite petrogenesis. Regional <span class="hlt">hydrothermal</span> modification of the crust under the thermal influence of the Yellowstone hotspot apparently preceded voluminous rhyolite generation at Bruneau-Jarbidge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JSAES..37..191G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JSAES..37..191G"><span>Geochronology of the late Pliocene to recent <span class="hlt">volcanic</span> <span class="hlt">activity</span> in the Payenia back-arc <span class="hlt">volcanic</span> province, Mendoza Argentina</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gudnason, Jónas; Holm, Paul Martin; Søager, Nina; Llambías, Eduardo J.</p> <p>2012-08-01</p> <p>Eighteen samples originating from monogenetic cones and larger complexes in the back-arc Payenia <span class="hlt">volcanic</span> province, in Mendoza Argentina, have been dated by the 40Ar/39Ar method. Groundmass and plagioclase separates give plateau ages, ranging from 20.7 ± 0.5 to 0.06 ± 0.02 Ma. Payenia has been divided into six subfields based on the new and literature radiometric ages: Payún Matrú, Río Colorado, Llancanelo, and Nevado <span class="hlt">volcanic</span> fields, the Northern segment and the Andes retro-arc group. Fifteen samples are younger than 2.83 Ma and show correlation between geographic position and age. Eruption centres younger than 0.5 Ma are concentrated to the west of 69° W with few exceptions among new and literature data. This westward shift of <span class="hlt">activity</span> supports the rollback theory for the subducting Nazca plate since the late Pliocene. Furthermore, a northward progression of <span class="hlt">volcanism</span> on the San Rafael block from 2.8 Ma to around 0.5 Ma is recognized. We conclude that rollback was initiated in the southern part of Payenia in the early Pliocene and progressed >200 km northwards during the Pliocene-Pleistocene period creating conditions for hydrous magma generation beneath the eastern part of Payenia. The long lived <span class="hlt">activity</span> of the Payún Matrú complex is ascribed to the presence of a thermal anomaly in the underlying asthenosphere which could be plume-like.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2015/5110/sir20155110.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2015/5110/sir20155110.pdf"><span>2013 <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Alaska: summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dixon, James P.; Cameron, Cheryl; McGimsey, Robert G.; Neal, Christina A.; Waythomas, Chris</p> <p>2015-08-14</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptions, <span class="hlt">volcanic</span> unrest or suspected unrest, and seismic events at 18 <span class="hlt">volcanic</span> centers in Alaska during 2013. Beginning with the 2013 AVO Summary of Events, the annual description of the AVO seismograph network and <span class="hlt">activity</span>, once a stand-alone publication, is now part of this report. Because of this change, the annual summary now contains an expanded description of seismic <span class="hlt">activity</span> at Alaskan volcanoes. Eruptions occurred at three <span class="hlt">volcanic</span> centers in 2013: Pavlof Volcano in May and June, Mount Veniaminof Volcano in June through December, and Cleveland Volcano throughout the year. None of these three eruptive events resulted in 24-hour staffing at AVO facilities in Anchorage or Fairbanks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JVGR..178...32K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JVGR..178...32K"><span>A preparation zone for <span class="hlt">volcanic</span> explosions beneath Naka-dake crater, Aso volcano, as inferred from magnetotelluric surveys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kanda, Wataru; Tanaka, Yoshikazu; Utsugi, Mitsuru; Takakura, Shinichi; Hashimoto, Takeshi; Inoue, Hiroyuki</p> <p>2008-11-01</p> <p> conductor identified beneath the 1st crater is mainly composed of <span class="hlt">hydrothermally</span> altered zone that acts both as a cap to upwelling fluids supplied from deep-level magma and as a floor to infiltrating fluid from the crater lake. The relatively resistive body found beneath the 4th crater represents consolidated magma. These results suggest that the shallow conductor beneath the <span class="hlt">active</span> crater is closely related to a component of the mechanism that controls <span class="hlt">volcanic</span> <span class="hlt">activity</span> within Naka-dake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.2446B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.2446B"><span>Contrasted <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> along the South-East Indian Ridge (130°E-140°E): From crustal to ultramafic circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boulart, Cédric; Briais, Anne; Chavagnac, Valérie; Révillon, Sidonie; Ceuleneer, Georges; Donval, Jean-Pierre; Guyader, Vivien; Barrere, Fabienne; Ferreira, Nicolas; Hanan, Barry; Hémond, Christophe; Macleod, Sarah; Maia, Marcia; Maillard, Agnès.; Merkuryev, Sergey; Park, Sung-Hyun; Ruellan, Etienne; Schohn, Alexandre; Watson, Sally; Yang, Yun-Seok</p> <p>2017-07-01</p> <p>Using a combined approach of seafloor mapping, MAPR and CTD survey, we report evidence for <span class="hlt">active</span> <span class="hlt">hydrothermal</span> venting along the 130°-140°E section of the poorly-known South-East Indian Ridge (SEIR) from the Australia-Antarctic Discordance (AAD) to the George V Fracture Zone (FZ). Along the latter, we report Eh and CH4 anomalies in the water column above a serpentinite massif, which unambiguously testify for ultramafic-related fluid flow. This is the first time that such circulation is observed on an intermediate-spreading ridge. The ridge axis itself is characterized by numerous off-axis volcanoes, suggesting a high magma supply. The water column survey indicates the presence of at least ten distinct <span class="hlt">hydrothermal</span> plumes along the axis. The CH4:Mn ratios of the plumes vary from 0.37 to 0.65 denoting different underlying processes, from typical basalt-hosted to ultramafic-hosted high-temperature <span class="hlt">hydrothermal</span> circulation. Our data suggest that the change of mantle temperature along the SEIR not only regulates the magma supply, but also the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. The distribution of <span class="hlt">hydrothermal</span> plumes from a ridge segment to another implies secondary controls such as the presence of fractures and faults along the axis or in the axial discontinuities. We conclude from these results that <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> along the SEIR is controlled by magmatic processes at the regional scale and by the tectonics at the segment scale, which influences the type of <span class="hlt">hydrothermal</span> circulation and leads to various chemical compositions. Such variety may impact global biogeochemical cycles, especially in the Southern Ocean where <span class="hlt">hydrothermal</span> venting might be the only source of nutrients.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V43D0564B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V43D0564B"><span>Evidence for intense <span class="hlt">hydrothermal</span> alteration associated with flood basalt <span class="hlt">volcanism</span> during the birth of the Azores Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bach, W.; Busch, A.; Genske, F. S.; Beier, C.; Krumm, S.</p> <p>2017-12-01</p> <p> initial stages of flood basalt <span class="hlt">activity</span>. The extreme <span class="hlt">hydrothermal</span> alteration may hence be directly linked to the prolonged magmatic period during which excess melting produced a 13-km thick igneous crust. Our results indicate that marine plateau-forming events may cause transient highs in <span class="hlt">hydrothermal</span> flux rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992Tectp.214..277D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992Tectp.214..277D"><span>The Middle to Late Devonian Eden-Comerong-Yalwal <span class="hlt">Volcanic</span> Zone of Southeastern Australia: An ancient analogue of the Yellowstone-Snake River Plain region of the USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dadd, K. A.</p> <p>1992-11-01</p> <p>The Middle to Late Devonian Yalwal <span class="hlt">Volcanics</span>, Comerong <span class="hlt">Volcanics</span>, Boyd <span class="hlt">Volcanic</span> Complex and associated gabbroic and A-type granitic plutons form part of a continental volcano-tectonic belt, the Eden-Comerong-Yalwal <span class="hlt">Volcanic</span> Zone (EVZ), located parallel to the coast of southeastern Australia. The EVZ is characterised by an elongate outcrop pattern, bimodal basalt-rhyolite <span class="hlt">volcanism</span>, and a paucity of sedimentary rocks. <span class="hlt">Volcanic</span> centres were located along the length of the <span class="hlt">volcanic</span> zone at positions indicated by subvolcanic plutons, dykes, rhyolite lavas and other proximal vent indicators including surge bedforms in tuff rings, and <span class="hlt">hydrothermal</span> alteration. Previous interpretations that suggested the <span class="hlt">volcanic</span> zone was a fault bounded rift are rejected in favour of a volcano-tectonic belt. The Yellowstone-Snake River Plain region (Y-SRP) in the USA is an appropriate analogue. Both regions have basalt lavas which range in composition from olivine tholeiite to ferrobasalt, alkalic rhyolitic rocks enriched in Y, Zr and Th, large rhyolite lava flows, plains-type basalt lava flows, and a paucity of sedimentary rocks. The Y-SRP is inferred to have developed by migration of the American plate over a fixed hot spot leading to a northeast temporal progression of the focus of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Application of a similar hot spot model to the EVZ (using a length of 300 km and a time range for <span class="hlt">volcanic</span> <span class="hlt">activity</span> of 5-10 Ma), suggests that during the Middle to Late Devonian the Australian plate was moving at a rate of between 3 and 6 cm/yr relative to the hot spot and that the northern extent of the <span class="hlt">volcanic</span> zone at any time was a topographically high region with rhyolitic <span class="hlt">activity</span>, similar to present day Yellowstone. As the focus of <span class="hlt">activity</span> moved northward, the high region subsided and the depression was flooded by basalt. The EVZ was much wider (up to 70 km) and much longer than the belt defined by present-day outcrop and was of comparable scale to the Y-SRP. The main difference</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813503R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813503R"><span>Sensitivity to <span class="hlt">volcanic</span> field boundary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Runge, Melody; Bebbington, Mark; Cronin, Shane; Lindsay, Jan; Rashad Moufti, Mohammed</p> <p>2016-04-01</p> <p><span class="hlt">Volcanic</span> hazard analyses are desirable where there is potential for future <span class="hlt">volcanic</span> <span class="hlt">activity</span> to affect a proximal population. This is frequently the case for <span class="hlt">volcanic</span> fields (regions of distributed <span class="hlt">volcanism</span>) where low eruption rates, fertile soil, and attractive landscapes draw populations to live close by. Forecasting future <span class="hlt">activity</span> in <span class="hlt">volcanic</span> fields almost invariably uses spatial or spatio-temporal point processes with model selection and development based on exploratory analyses of previous eruption data. For identifiability reasons, spatio-temporal processes, and practically also spatial processes, the definition of a spatial region is required to which <span class="hlt">volcanism</span> is confined. However, due to the complex and predominantly unknown sub-surface processes driving <span class="hlt">volcanic</span> eruptions, definition of a region based solely on geological information is currently impossible. Thus, the current approach is to fit a shape to the known previous eruption sites. The class of boundary shape is an unavoidable subjective decision taken by the forecaster that is often overlooked during subsequent analysis of results. This study shows the substantial effect that this choice may have on even the simplest exploratory methods for hazard forecasting, illustrated using four commonly used exploratory statistical methods and two very different regions: the Auckland <span class="hlt">Volcanic</span> Field, New Zealand, and Harrat Rahat, Kingdom of Saudi Arabia. For Harrat Rahat, sensitivity of results to boundary definition is substantial. For the Auckland <span class="hlt">Volcanic</span> Field, the range of options resulted in similar shapes, nevertheless, some of the statistical tests still showed substantial variation in results. This work highlights the fact that when carrying out any hazard analysis on <span class="hlt">volcanic</span> fields, it is vital to specify how the <span class="hlt">volcanic</span> field boundary has been defined, assess the sensitivity of boundary choice, and to carry these assumptions and related uncertainties through to estimates of future <span class="hlt">activity</span> 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_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('http://adsabs.harvard.edu/abs/2006JAG....58..265Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JAG....58..265Z"><span>State of the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> of Soufrière of Guadeloupe volcano inferred by VLF surveys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zlotnicki, J.; Vargemezis, G.; Mille, A.; Bruère, F.; Hammouya, G.</p> <p>2006-04-01</p> <p>La Soufrière (1467 m) is the <span class="hlt">active</span> island arc volcano of Guadeloupe Island in the Lesser Antilles arc. Its historical eruptions are more or less violent phreatic outbursts the last of which, in 1976-1977, led to the evacuation of nearly 70 000 persons. The subsurface structure of the volcano consists of calderas, craters, and avalanche amphitheatres nested within the composite pile of eruptive products. Since the last magmatic eruption, dated ca. 1440 AD, the four phreatic eruptions have developed radial fractures on Soufrière dome favouring the development of a huge <span class="hlt">active</span> <span class="hlt">hydrothermal</span> system emphasized by a tropical environment. After the eruptions, the thermal state and the stable ground water flow are completely disorganised during several years during which the slow mineralization of rocks is becoming again preponderant. Sealing of fractures and decay of rocks permeability act as a cap for upward thermal transfers. Therefore Soufrière dome operates as a valve, resealing the <span class="hlt">hydrothermal</span> system underlying the volcano thus providing over pressurization that could lead to the next phreatic eruption. In 1992 new small seismic swarms have appeared. Several of them are recorded every year while the emission of acid gas slowly increases. In order to recognise the superficial electrical resistive and conductive zones (less than 100 m depth) as well as the cavities on Soufrière volcano, we have made Very Low Frequency (VLF) surveys in 2000. Electrical conductive zones are clearly associated with major radial faults starting from the summit in which the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> takes place. In the continuation of these <span class="hlt">active</span> <span class="hlt">hydrothermal</span> fractures hot springs are located down slope. Conversely some of the resistive zones are associated with inactive clayed and sealed or opened faults. The distribution of the conductive zones allows detailing the state of the superficial part of the <span class="hlt">hydrothermal</span> system of La Soufrière. The distribution of vertical clayed zones</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511102V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511102V"><span>Water and gas geochemistry of the Calatrava <span class="hlt">Volcanic</span> Province (CVP) <span class="hlt">hydrothermal</span> system (Ciudad Real, central Spain)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vaselli, Orlando; Nisi, Barbara; Tassi, Franco; Giannini, Luciano; Grandia, Fidel; Darrah, Tom; Capecchiacci, Francesco; del Villar, Pèrez</p> <p>2013-04-01</p> <p>An extensive geochemical and isotopic investigation was carried out in the water and gas discharges of the Late Miocene-Quaternary Calatrava <span class="hlt">Volcanic</span> Province (CVP) (Ciudad Real, Spain) with the aim reconstruct the fluid circulation in the area. CVP consists of a series of scattered (monogenetic) vents from where alkaline lava flows and pyroclastic deposits formed in two different periods. The first stage (8.7-6.4 Ma) mainly included ultra-potassic mafic extrusives, whilst the second stage (4.7-1.75 Ma) prevalently originated alkaline and ultra-alkaline <span class="hlt">volcanics</span>. Both stages were followed by a <span class="hlt">volcanic</span> <span class="hlt">activity</span> that extended up to 1.3 and 0.7 Ma, respectively. This area can likely be regarded as one of the most important emitting zones of CO2 in the whole Peninsular Spain along with that of Selva-Emporda in northeastern Spain (Cataluña) and it can be assumed as one of the best examples of natural analogues of CO2 leakages in Spain. This latter aspect is further evidenced by the relatively common water-gas blast events that characterize the CCVF. In the last few years the presence of a CO2-pressurized reservoir at a relatively shallow level as indeed caused several small-sized explosion particularly during the drilling of domestic wells. The fluid discharging sites are apparently aligned along well-defined directions: NW-SE and NNW-SSE and subordinately, ENE-WSW, indicating a clear relationship between the thermal discharges and the <span class="hlt">volcanic</span> centers that also distribute along these lineaments. The CVP waters are mostly hypothermal (up to 33 °C) and are generally Mg(Ca)-HCO3 in composition and occasionally show relatively high concentrations of Fe and Mn, with pH and electrical conductivity down to 5.5 and up to 6.5 mS/cm, respectively. The oxygen and hydrogen isotopes suggest a meteoric origin for these waters. The mantle source of these <span class="hlt">volcanic</span> products is apparently preserved in the many CO2-rich (up to 990,000 mmol/mol) gas discharges that characterize CVP</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2014/5034/pdf/sir2014-5034.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2014/5034/pdf/sir2014-5034.pdf"><span>2010 <span class="hlt">Volcanic</span> <span class="hlt">activity</span> in Alaska, Kamchatka, and the Kurile Islands: summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Neal, Christina A.; Herrick, Julie; Girina, O.A.; Chibisova, Marina; Rybin, Alexander; McGimsey, Robert G.; Dixon, Jim</p> <p>2014-01-01</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptions, possible eruptions, <span class="hlt">volcanic</span> unrest or suspected unrest at 12 <span class="hlt">volcanic</span> centers in Alaska during 2010. The most notable <span class="hlt">volcanic</span> <span class="hlt">activity</span> consisted of intermittent ash emissions from long-<span class="hlt">active</span> Cleveland volcano in the Aleutian Islands. AVO staff also participated in hazard communication regarding eruptions or unrest at seven volcanoes in Russia as part of an ongoing collaborative role in the Kamchatka and Sakhalin <span class="hlt">Volcanic</span> Eruption Response Teams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860040904&hterms=Eocene&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DEocene','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860040904&hterms=Eocene&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DEocene"><span>Seafloor <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and spreading rates - The Eocene carbon dioxide greenhouse revisited</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kasting, J. F.; Richardson, S. M.</p> <p>1985-01-01</p> <p>A suggestion has been made that enhanced rates of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> during the Eocene could have caused a global warming by adding calcium to the ocean and pumping CO2 into the atmosphere (Owen and Rea, 1984). This phenomenon was purported to be consistent with the predictions of the CO2 geochemical cycle model of Berner, Lasaga and Garrels (1983) (henceforth BLAG). In fact, however, the BLAG model predicts only a weak connection between <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and atmospheric CO2 levels. By contrast, it predicts a strong correlation between seafloor spreading rates and pCO2, since the release rate of CO2 from carbonate metamorphism is assumed to be proportional to the mean spreading rate. The Eocene warming can be conveniently explained if the BLAG model is extended by assuming that the rate of carbonate metamorphism is also proportional to the total length of the midocean ridges from which the spreading originates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089655&hterms=Eocene&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DEocene','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089655&hterms=Eocene&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DEocene"><span>Seafloor <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and spreading rates: the Eocene carbon dioxide greenhouse revisted</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kasting, J. F.; Richardson, S. M.</p> <p>1985-01-01</p> <p>A suggestion has been made that enhanced rates of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> during the Eocene could have caused a global warming by adding calcium to the ocean and pumping CO2 into the atmosphere (Owen and Rea, 1984). This phenomenon was purported to be consistent with the predictions of the CO2 geochemical cycle model of Berner, Lasaga and Garrels (1983) (henceforth BLAG). In fact, however, the BLAG model predicts only a weak connection between <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and atmospheric CO2 levels. By contrast, it predicts a strong correlation between seafloor spreading rates and pCO2, since the release rate of CO2 from carbonate metamorphism is assumed to be proportional to the mean spreading rate. The Ecocene warming can be conveniently explained if the BLAG model is extended by assuming that the rate of carbonate metamorphism is also proportional to the total length of the midocean ridges from which the spreading originates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5187427','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5187427"><span>Magmas near the critical degassing pressure drive <span class="hlt">volcanic</span> unrest towards a critical state</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chiodini, Giovanni; Paonita, Antonio; Aiuppa, Alessandro; Costa, Antonio; Caliro, Stefano; De Martino, Prospero; Acocella, Valerio; Vandemeulebrouck, Jean</p> <p>2016-01-01</p> <p>During the reawaking of a volcano, magmas migrating through the shallow crust have to pass through <span class="hlt">hydrothermal</span> fluids and rocks. The resulting magma–<span class="hlt">hydrothermal</span> interactions are still poorly understood, which impairs the ability to interpret volcano monitoring signals and perform hazard assessments. Here we use the results of physical and volatile saturation models to demonstrate that magmatic volatiles released by decompressing magmas at a critical degassing pressure (CDP) can drive <span class="hlt">volcanic</span> unrest towards a critical state. We show that, at the CDP, the abrupt and voluminous release of H2O-rich magmatic gases can heat <span class="hlt">hydrothermal</span> fluids and rocks, triggering an accelerating deformation that can ultimately culminate in rock failure and eruption. We propose that magma could be approaching the CDP at Campi Flegrei, a volcano in the metropolitan area of Naples, one of the most densely inhabited areas in the world, and where accelerating deformation and heating are currently being observed. PMID:27996976</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27996976','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27996976"><span>Magmas near the critical degassing pressure drive <span class="hlt">volcanic</span> unrest towards a critical state.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chiodini, Giovanni; Paonita, Antonio; Aiuppa, Alessandro; Costa, Antonio; Caliro, Stefano; De Martino, Prospero; Acocella, Valerio; Vandemeulebrouck, Jean</p> <p>2016-12-20</p> <p>During the reawaking of a volcano, magmas migrating through the shallow crust have to pass through <span class="hlt">hydrothermal</span> fluids and rocks. The resulting magma-<span class="hlt">hydrothermal</span> interactions are still poorly understood, which impairs the ability to interpret volcano monitoring signals and perform hazard assessments. Here we use the results of physical and volatile saturation models to demonstrate that magmatic volatiles released by decompressing magmas at a critical degassing pressure (CDP) can drive <span class="hlt">volcanic</span> unrest towards a critical state. We show that, at the CDP, the abrupt and voluminous release of H 2 O-rich magmatic gases can heat <span class="hlt">hydrothermal</span> fluids and rocks, triggering an accelerating deformation that can ultimately culminate in rock failure and eruption. We propose that magma could be approaching the CDP at Campi Flegrei, a volcano in the metropolitan area of Naples, one of the most densely inhabited areas in the world, and where accelerating deformation and heating are currently being observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5967V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5967V"><span>Implications of new stratigraphic data on <span class="hlt">volcanic</span> hazard assessment for Nisyros volcano, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volentik, A.; Vanderkluysen, L.; Principe, C.; Hernandez, J.; Hunziker, J. C.</p> <p>2003-04-01</p> <p>The <span class="hlt">active</span> quaternary Nisyros volcano, at the eastern end of the Aegean <span class="hlt">volcanic</span> arc, is composed of a succession of lava flows, tephra layers and interbedded epiclastic deposits. The volcano is topped by a recent caldera, on average 4 km in diameter and 200 m in depth. A detailed geological map including 35 stratigraphic units (lava flows, tephra layers and epiclastic deposits) has been recently completed at the 1:10'000 scale, based on new stratigraphical data. Based on the identification of new plinian sequences (Lakki and Melisseri pyroclastic series) in the lowermost section of the reconstructed stratigraphical succession, on the re-interpretation of previously described deposits and on the discovery of eruptive facies, we construct a set of hazard maps for <span class="hlt">volcanic</span> events at Nisyros. Sequences of sub-marine lavas to subaerial epiclastites combined with the occurrence of a marine terrace deposit in the north-western sector of the island highlight the potential for rapid vertical movements, in particular in the area of Mandraki. A period of intense off-centred strombolian to phreatomagmatic <span class="hlt">activity</span> occurred in quite recent times on Nisyros along the major tectonic trends (N^o030, No070, N^o120 and N^o340), building up several scoria cones and tuff cones all around the island. A number of these tectonic trends are still <span class="hlt">active</span>, as demonstrated by faults cutting through recent deposits (including the youngest deposits of the <span class="hlt">hydrothermal</span> eruptions, inside the present caldera of Nisyros). This implies that not only intra-caldera phreatic eruptions, but also potential magmatic eruption may occur along the island’s major zones of weakness, with increased hazards where magma/water interaction may take place. Finally a newly recognized debris avalanche deposit (the so-called Vunàri debris avalanche), affecting a wide sector in the northern part of the island, unveils a new type of <span class="hlt">volcanic</span> hazard on Nisyros, related to flank collapse and destruction of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GGG....17.4438C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GGG....17.4438C"><span>Application of the probabilistic model BET_UNREST during a <span class="hlt">volcanic</span> unrest simulation exercise in Dominica, Lesser Antilles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Constantinescu, Robert; Robertson, Richard; Lindsay, Jan M.; Tonini, Roberto; Sandri, Laura; Rouwet, Dmitri; Smith, Patrick; Stewart, Roderick</p> <p>2016-11-01</p> <p>We report on the first "real-time" application of the BET_UNREST (Bayesian Event Tree for <span class="hlt">Volcanic</span> Unrest) probabilistic model, during a VUELCO Simulation Exercise carried out on the island of Dominica, Lesser Antilles, in May 2015. Dominica has a concentration of nine potentially <span class="hlt">active</span> <span class="hlt">volcanic</span> centers and frequent <span class="hlt">volcanic</span> earthquake swarms at shallow depths, intense geothermal <span class="hlt">activity</span>, and recent phreatic explosions (1997) indicate the region is still <span class="hlt">active</span>. The exercise scenario was developed in secret by a team of scientists from The University of the West Indies (Trinidad and Tobago) and University of Auckland (New Zealand). The simulated unrest <span class="hlt">activity</span> was provided to the exercise's Scientific Team in three "phases" through exercise injects comprising processed monitoring data. We applied the newly created BET_UNREST model through its software implementation PyBetUnrest, to estimate the probabilities of having (i) unrest of (ii) magmatic, <span class="hlt">hydrothermal</span> or tectonic origin, which may or may not lead to (iii) an eruption. The probabilities obtained for each simulated phase raised controversy and intense deliberations among the members of the Scientific Team. The results were often considered to be "too high" and were not included in any of the reports presented to ODM (Office for Disaster Management) revealing interesting crisis communication challenges. We concluded that the PyBetUnrest application itself was successful and brought the tool one step closer to a full implementation. However, as with any newly proposed method, it needs more testing, and in order to be able to use it in the future, we make a series of recommendations for future applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...624128M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...624128M"><span><span class="hlt">Hydrothermal</span> synthesis of NiWO4 crystals for high performance <span class="hlt">non</span>-enzymatic glucose biosensors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mani, Sivakumar; Vediyappan, Veeramani; Chen, Shen-Ming; Madhu, Rajesh; Pitchaimani, Veerakumar; Chang, Jia-Yaw; Liu, Shang-Bin</p> <p>2016-04-01</p> <p>A facile <span class="hlt">hydrothermal</span> route for the synthesis of ordered NiWO4 nanocrystals, which show promising applications as high performance <span class="hlt">non</span>-enzymatic glucose sensor is reported. The NiWO4-modified electrodes showed excellent sensitivity (269.6 μA mM-1 cm-2) and low detection limit (0.18 μM) for detection of glucose with desirable selectivity, stability, and tolerance to interference, rendering their prospective applications as cost-effective, enzyme-free glucose sensors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27087561','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27087561"><span><span class="hlt">Hydrothermal</span> synthesis of NiWO4 crystals for high performance <span class="hlt">non</span>-enzymatic glucose biosensors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mani, Sivakumar; Vediyappan, Veeramani; Chen, Shen-Ming; Madhu, Rajesh; Pitchaimani, Veerakumar; Chang, Jia-Yaw; Liu, Shang-Bin</p> <p>2016-04-18</p> <p>A facile <span class="hlt">hydrothermal</span> route for the synthesis of ordered NiWO4 nanocrystals, which show promising applications as high performance <span class="hlt">non</span>-enzymatic glucose sensor is reported. The NiWO4-modified electrodes showed excellent sensitivity (269.6 μA mM(-1 )cm(-2)) and low detection limit (0.18 μM) for detection of glucose with desirable selectivity, stability, and tolerance to interference, rendering their prospective applications as cost-effective, enzyme-free glucose sensors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023395','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023395"><span>Stable isotopes in seafloor <span class="hlt">hydrothermal</span> systems: Vent fluids, <span class="hlt">hydrothermal</span> deposits, <span class="hlt">hydrothermal</span> alteration, and microbial processes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shanks, Wayne C.</p> <p>2001-01-01</p> <p>The recognition of abundant and widespread <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and associated unique life-forms on the ocean floor is one of the great scientific discoveries of the latter half of the twentieth century. Studies of seafloor <span class="hlt">hydrothermal</span> processes have led to revolutions in understanding fluid convection and the cooling of the ocean crust, the chemical and isotopic mass balance of the oceans, the origin of stratiform and statabound massive-sulfide ore-deposits, the origin of greenstones and serpentinites, and the potential importance of the subseafloor biosphere. Stable isotope geochemistry has been a critical and definitive tool from the very beginning of the modern era of seafloor exploration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23760570','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23760570"><span><span class="hlt">Volcanic</span> mercury in Pinus canariensis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rodríguez Martín, José Antonio; Nanos, Nikos; Miranda, José Carlos; Carbonell, Gregoria; Gil, Luis</p> <p>2013-08-01</p> <p>Mercury (Hg) is a toxic element that is emitted to the atmosphere by both human <span class="hlt">activities</span> and natural processes. <span class="hlt">Volcanic</span> emissions are considered a natural source of mercury in the environment. In some cases, tree ring records taken close to volcanoes and their relation to <span class="hlt">volcanic</span> <span class="hlt">activity</span> over time are contradictory. In 1949, the Hoyo Negro volcano (La Palma-Canary Islands) produced significant pyroclastic flows that damaged the nearby stand of Pinus canariensis. Recently, 60 years after the eruption, we assessed mercury concentrations in the stem of a pine which survived volcano formation, located at a distance of 50 m from the crater. We show that Hg content in a wound caused by pyroclastic impacts (22.3 μg kg(-1)) is an order of magnitude higher than the Hg concentrations measured in the xylem before and after the eruption (2.3 μg kg(-1)). Thus, mercury emissions originating from the eruption remained only as a mark-in pyroclastic wounds-and can be considered a sporadic and very high mercury input that did not affect the overall Hg input in the xylem. In addition, mercury contents recorded in the phloem (9.5 μg kg(-1)) and bark (6.0 μg kg(-1)) suggest that mercury shifts towards <span class="hlt">non</span>-living tissues of the pine, an aspect that can be related to detoxification in <span class="hlt">volcanism</span>-adapted species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NW....100..739R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NW....100..739R"><span><span class="hlt">Volcanic</span> mercury in Pinus canariensis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rodríguez Martín, José Antonio; Nanos, Nikos; Miranda, José Carlos; Carbonell, Gregoria; Gil, Luis</p> <p>2013-08-01</p> <p>Mercury (Hg) is a toxic element that is emitted to the atmosphere by both human <span class="hlt">activities</span> and natural processes. <span class="hlt">Volcanic</span> emissions are considered a natural source of mercury in the environment. In some cases, tree ring records taken close to volcanoes and their relation to <span class="hlt">volcanic</span> <span class="hlt">activity</span> over time are contradictory. In 1949, the Hoyo Negro volcano (La Palma-Canary Islands) produced significant pyroclastic flows that damaged the nearby stand of Pinus canariensis. Recently, 60 years after the eruption, we assessed mercury concentrations in the stem of a pine which survived volcano formation, located at a distance of 50 m from the crater. We show that Hg content in a wound caused by pyroclastic impacts (22.3 μg kg-1) is an order of magnitude higher than the Hg concentrations measured in the xylem before and after the eruption (2.3 μg kg-1). Thus, mercury emissions originating from the eruption remained only as a mark—in pyroclastic wounds—and can be considered a sporadic and very high mercury input that did not affect the overall Hg input in the xylem. In addition, mercury contents recorded in the phloem (9.5 μg kg-1) and bark (6.0 μg kg-1) suggest that mercury shifts towards <span class="hlt">non</span>-living tissues of the pine, an aspect that can be related to detoxification in <span class="hlt">volcanism</span>-adapted species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960050123','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960050123"><span><span class="hlt">Volcanism</span> in Eastern Africa</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cauthen, Clay; Coombs, Cassandra R.</p> <p>1996-01-01</p> <p>In 1891, the Virunga Mountains of Eastern Zaire were first acknowledged as volcanoes, and since then, the Virunga Mountain chain has demonstrated its potentially violent <span class="hlt">volcanic</span> nature. The Virunga Mountains lie across the Eastern African Rift in an E-W direction located north of Lake Kivu. Mt. Nyamuragira and Mt. Nyiragongo present the most hazard of the eight mountains making up Virunga <span class="hlt">volcanic</span> field, with the most recent <span class="hlt">activity</span> during the 1970-90's. In 1977, after almost eighty years of moderate <span class="hlt">activity</span> and periods of quiescence, Mt. Nyamuragira became highly <span class="hlt">active</span> with lava flows that extruded from fissures on flanks circumscribing the volcano. The flows destroyed vast areas of vegetation and Zairian National Park areas, but no casualties were reported. Mt. Nyiragongo exhibited the same type <span class="hlt">volcanic</span> <span class="hlt">activity</span>, in association with regional tectonics that effected Mt. Nyamuragira, with variations of lava lake levels, lava fountains, and lava flows that resided in Lake Kivu. Mt. Nyiragongo, recently named a Decade volcano, presents both a direct and an indirect hazard to the inhabitants and properties located near the volcano. The Virunga volcanoes pose four major threats: <span class="hlt">volcanic</span> eruptions, lava flows, toxic gas emission (CH4 and CO2), and earthquakes. Thus, the volcanoes of the Eastern African <span class="hlt">volcanic</span> field emanate harm to the surrounding area by the forecast of <span class="hlt">volcanic</span> eruptions. During the JSC Summer Fellowship program, we will acquire and collate remote sensing, photographic (Space Shuttle images), topographic and field data. In addition, maps of the extent and morphology(ies) of the features will be constructed using digital image information. The database generated will serve to create a Geographic Information System for easy access of information of the Eastem African <span class="hlt">volcanic</span> field. The analysis of <span class="hlt">volcanism</span> in Eastern Africa will permit a comparison for those areas from which we have field data. Results from this summer's work will permit</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.860a2005K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.860a2005K"><span>Elemental characterization of Mt. Sinabung <span class="hlt">volcanic</span> ash, Indonesia by Neutron <span class="hlt">Activation</span> Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kusmartini, I.; Syahfitri, W. Y. N.; Kurniawati, S.; Lestiani, D. D.; Santoso, M.</p> <p>2017-06-01</p> <p>Mount Sinabung is a volcano located in North Sumatera, Indonesia which has been recorded not erupted since 1600. However in 2013 it has been erupted and cause of black thick smog, rain sand and <span class="hlt">volcanic</span> ash. <span class="hlt">Volcanic</span> ash containing trace elements material that can be utilized in various applications but still has potential danger of heavy metals. In order to obtain an elemental composition data of <span class="hlt">volcanic</span> ash, the characterization of <span class="hlt">volcanic</span> ash were carried out using Neutron <span class="hlt">Activation</span> Analysis. The <span class="hlt">volcanic</span> ash was taken from Mt. Sinabung eruption. Samples were irradiated at the rabbit system in the reactor G.A Siwabessy facilities with neutron flux ˜ 1013 n.cm-2.s-1 and then counted using HPGe detector. Method validation was carried out by SRM NIST Coal Fly Ash 1633b and NIST 2711a Montana II Soil with recovery values were in the range of 96-108% and 95-106% respectively. The results showed that major elements; Al, Na, Ca and Fe, concentrations were 8.7, 1.05, 2.98 and 7.44 %, respectively, minor elements K, Mg, Mn, Ti, V and Zn were 0.87%, 0.78%, 0.18%, 0.62%, 197.13 ppm and 109.35 ppm, respectively, heavy metals; As, Cr, Co and Sb, contents were 4.48, 11.75, 17.13 and 0.35 ppm, respectively while rare earth elements such as Ce, Eu, La, Nd, Sm, Yb were 45.33, 1.22, 19.63, 20.34, 3.86, and 2.57 ppm respectively. The results of the elemental contents of <span class="hlt">volcanic</span> ash that has been obtained can be used as the scientific based data for <span class="hlt">volcanic</span> material utilization by considering the economic potential of elements contained and also the danger of the heavy metals content.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JSSCh.186..247C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JSSCh.186..247C"><span>Microwave-assisted <span class="hlt">hydrothermal</span> synthesis of marigold-like ZnIn2S4 microspheres and their visible light photocatalytic <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Zhixin; Li, Danzhen; Xiao, Guangcan; He, Yunhui; Xu, Yi-Jun</p> <p>2012-02-01</p> <p>Marigold-like ZnIn2S4 microspheres were synthesized by a microwave-assisted <span class="hlt">hydrothermal</span> method with the temperature ranging from 80 to 195 °C. X-ray diffraction, X-ray photoelectron spectroscopy, nitrogen sorption analysis, UV-visible spectroscopy, scanning electron microscopy and transmission electron microscopy were used to characterize the products. It was found that the crystallographic structure and optical property of the products synthesized at different temperatures were almost the same. The degradation of methyl orange (MO) under the visible light irradiation has been used as a probe reaction to investigate the photocatalytic <span class="hlt">activity</span> of as-prepared ZnIn2S4, which shows that the ZnIn2S4 sample synthesized at 195 °C shows the best photocatalytic <span class="hlt">activity</span> for MO degradation. In addition, the photocatalytic <span class="hlt">activities</span> of all the samples prepared by the microwave-assisted <span class="hlt">hydrothermal</span> method are better than those prepared by a normal <span class="hlt">hydrothermal</span> method, which could be attributed to the formation of more defect sites during the microwave-assisted <span class="hlt">hydrothermal</span> treatment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014074','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014074"><span>EVALUATION OF LOW-SUN ILLUMINATED LANDSAT-4 THEMATIC MAPPER DATA FOR MAPPING <span class="hlt">HYDROTHERMALLY</span> ALTERED ROCKS IN SOUTHERN NEVADA.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Podwysocki, Melvin H.; Power, Marty S.; Salisbury, Jack; Jones, O.D.</p> <p>1984-01-01</p> <p>Landsat-4 Thematic Mapper (TM) data of southern Nevada collected under conditions of low-angle solar illumination were digitally processed to identify hydroxyl-bearing minerals commonly associated with <span class="hlt">hydrothermal</span> alteration in <span class="hlt">volcanic</span> terrains. Digital masking procedures were used to exclude shadow areas and vegetation and thus to produce a CRC image suitable for testing the new TM bands as a means to map <span class="hlt">hydrothermally</span> altered rocks. Field examination of a masked CRC image revealed that several different types of altered rocks displayed hues associated with spectral characteristics common to hydroxyl-bearing minerals. Several types of unaltered rocks also displayed similar hues.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993JVGR...56..319T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993JVGR...56..319T"><span>Eruption mechanism as inferred from geomagnetic changes with special attention to the 1989 1990 <span class="hlt">activity</span> of Aso volcano</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, Yoshikazu</p> <p>1993-06-01</p> <p>Geomagnetic changes associated with the <span class="hlt">volcanic</span> <span class="hlt">activity</span> of Aso volcano were detected with a dense network of continuously recording proton-precession magnetometers during the period from June 1989 to June 1990. Magnetic date clearly indicate that changes in the magnetization within the volcano are most probably caused by temperature changes. This <span class="hlt">activity</span> can be divided into five stages, which are characterized by magnetization and demagnetization of the volcano. These magnetic changes with durations of a few months are definitely correlated with some typical <span class="hlt">volcanic</span> events at the crater as well as the <span class="hlt">volcanic</span> tremor <span class="hlt">activity</span>. The demagnetization stage appears when the vent is covered by a water pool or the <span class="hlt">volcanic</span> <span class="hlt">activity</span> is enhanced. The magnetization stage follows the opening of a vent and several large explosions which make the vent permeable. The source of magnetic changes lies at a depth of about 200 m below the crater rim in the southwestern part of the <span class="hlt">active</span> crater. Magnetic moments responsible for observed magnetic changes at stages 1, 2 and 4 are 3.4, -5.2 and -2.2 Wbm, respectively. The corresponding source volume is estimated as a single sphere of radius 40-50 m or a spherical shell of 100 m or so. An effective mechanism of rapid heating/cooling exists, which is ascribed to the interaction of groundwater and superheated vapor, i.e., a shallow <span class="hlt">hydrothermal</span> system. This <span class="hlt">hydrothermal</span> system driven by the surface cap of the vent, controls every feature of the eruptions at the final outlet of Aso volcano.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1985EOSTr..66..153G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1985EOSTr..66..153G"><span>Dinasour extinction and <span class="hlt">volcanic</span> <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gledhill, J. A.</p> <p></p> <p>There is at present some controversy about the reason for the mass extinction of dinosaurs and other forms of life at the end of the Cretaceous. A suggestion by Alvarez et al. [1980] that this was due to the collision of the earth with a meteorite 10 km or so in diameter has excited considerable interest [Silver and Schultz, 1982] and also some criticism [Stanley, 1984]. A recent publication [Wood, 1984] describing the catastrophic effects of a relatively minor lava flow in Iceland suggests that intense <span class="hlt">volcanic</span> <span class="hlt">activity</span> could have played a large part in the extinctions. In this letter it is pointed out that the Deccan lava flows in India took place in the appropriate time and may well have been of sufficient magnitude to be a major factor in the Cretaceous-Tertiary (C-T) boundary catastrophe.</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://pubs.usgs.gov/of/1983/0788/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1983/0788/report.pdf"><span>Cenozoic <span class="hlt">volcanic</span> rocks of Saudi Arabia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Coleman, R.G.; Gregory, R.T.; Brown, G.F.</p> <p>2016-01-01</p> <p>The historical record of <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Saudi Arabia suggests that <span class="hlt">volcanism</span> is dormant. The harrats should be evaluated for their potential as <span class="hlt">volcanic</span> hazards and as sources of geothermal energy. The <span class="hlt">volcanic</span> rocks are natural traps for groundwater; thus water resources for agriculture may be significant and should be investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1215739H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1215739H"><span>Spain as an emergency air traffic hub during <span class="hlt">volcanic</span> air fall events? Evidence of past <span class="hlt">volcanic</span> ash air fall over Europe during the late Pleistocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hardiman, Mark; Lane, Christine; Blockley, Simon P. E.; Moreno, Ana; Valero-Garcés, Blas; Ortiz, José E.; Torres, Trino; Lowe, John J.; Menzies, Martin A.</p> <p>2010-05-01</p> <p>Past <span class="hlt">volcanic</span> eruptions often leave visible ash layers in the geological record, for example in marine or lake sedimentary sequences. Recent developments, however, have shown that <span class="hlt">non</span>-visible <span class="hlt">volcanic</span> ash layers are also commonly preserved in sedimentary deposits. These augment the record of past <span class="hlt">volcanic</span> events by demonstrating that past ash dispersals have been more numerous and widely disseminated in Europe than previously appreciated. The dispersal ‘footprints' of some large late Pleistocene European eruptions are examined here in the light of the recent Eyjafjallajökull eruption. For example, the Vedde Ash which was erupted from Iceland around 12 thousand years ago, delivered distal (and <span class="hlt">non</span>-visible) glass deposits as far south as Switzerland and as far east as the Ural Mountains in Russia, with an overall European distribution remarkably similar to the dominant tracks of the recent Eyjafjallajökull plumes. The Eyjafjallajökull eruption has demonstrated that relatively small amounts of distal <span class="hlt">volcanic</span> ash in the atmosphere can seriously disrupt aviation <span class="hlt">activity</span>, with attendant economic and other consequences. It has raised fundamental questions about the likelihood of larger or more prolonged <span class="hlt">volcanic</span> <span class="hlt">activity</span> in the near future, and the possibility of even more serious consequences than those experienced recently. Given that there are several other <span class="hlt">volcanic</span> centres that could cause such disruption in Europe (e.g. Campania and other <span class="hlt">volcanic</span> centres in Italy; Aegean volcanoes), a key question is whether there are parts of Europe less prone to ash plumes and which could therefore operate as emergency air traffic hubs during times of ash dispersal. Although not generated to answer this question, the recent geological record might provide a basis for seeking the answer. For example, four palaeo-records covering the time frame of 8 - 40 Ka BP that are geographically distributed across Spain have been examined for <span class="hlt">non</span>-visible distal ash content. All four have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800044072&hterms=Israel+humanity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DIsrael%2Bhumanity','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800044072&hterms=Israel+humanity&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DIsrael%2Bhumanity"><span>Time analysis of <span class="hlt">volcanic</span> <span class="hlt">activity</span> on Io by means of plasma observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mekler, Y.; Eviatar, A.</p> <p>1980-01-01</p> <p>A model of Io <span class="hlt">volcanism</span> in which the probability of <span class="hlt">activity</span> obeys a binomial distribution is presented. Observed values of the electron density obtained over a 3-year period by ground-based spectroscopy are fitted to such a distribution. The best fit is found for a total number of 15 volcanoes with a probability of individual <span class="hlt">activity</span> at any time of 0.143. The Pioneer 10 ultraviolet observations are reinterpreted as emissions of sulfur and oxygen ions and are found to be consistent with a plasma much less dense than that observed by the Voyager spacecraft. Late 1978 and the first half of 1979 are shown to be periods of anomalous <span class="hlt">volcanicity</span>. Rapid variations in electron density are related to enhanced radial diffusion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2014/5159/pdf/sir2014-5159.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2014/5159/pdf/sir2014-5159.pdf"><span>2011 <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Alaska: summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Maharrey, J. Zebulon; Neal, Christina A.</p> <p>2014-01-01</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptions, possible eruptions, and <span class="hlt">volcanic</span> unrest at or near three separate <span class="hlt">volcanic</span> centers in Alaska during 2011. The year was highlighted by the unrest and eruption of Cleveland Volcano in the central Aleutian Islands. AVO annual summaries no longer report on <span class="hlt">activity</span> at Russian volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V33F0568M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V33F0568M"><span>Using Spectroscopy to Infer the Eruption Style and Volatile History of <span class="hlt">Volcanic</span> Tephras</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McBride, M. J.; Horgan, B. H. N.; Rowe, M. C.; Wall, K. T.; Oxley, B. M.</p> <p>2017-12-01</p> <p>The interaction between volatiles and magma strongly influences <span class="hlt">volcanic</span> eruption styles, and results in an increase in the glass component of <span class="hlt">volcanic</span> tephra. On Earth, both phreatomagmatic and magmatic explosive eruptions create glassy tephras. Phreatomagmatic eruptions form abundant glass by quickly quenching lava through interaction with meteoric water while magmatic eruptions create less glass through slower cooling within larger pyroclasts or eruption columns. Wall et al. (2014) used X-ray diffraction (XRD) of diverse tephra samples to show that glass content correlates with eruption style, as magmatic samples contain less glass than phreatomagmatic samples. While use of XRD is limited to Earth and the Curiosity rover on Mars, orbital spectroscopy is much a more common technique in the exploration of terrestrial bodies. In this study, we evaluate whether or not spectroscopy can be used to infer eruption style and thus volatile history. Visible/near-infrared (VNIR) and thermal-infrared (TIR) spectra were collected of the Wall et al. (2014) tephra samples, and were analyzed for trends related to glass content and thus eruption style. VNIR spectra can detect glass at high abundances as well as <span class="hlt">hydrothermal</span> alteration minerals produced during interactions with meteoric water. Using TIR, glass abundances can be derived by deconvolving the spectra with a standard spectral library; however, due to the <span class="hlt">non</span>-unique spectral shape of glass, intermediate to high glass abundances in tephras are difficult to differentiate using TIR alone. Synthetic mixtures of glass and crystalline minerals verify these results. Therefore, the most effective method for determining glass abundance and thus eruption style from <span class="hlt">volcanic</span> deposits is a combination of VNIR and TIR spectral analysis. Using standard planetary remote sensing instrumentation to infer eruption styles will provide a new window into the <span class="hlt">volcanic</span> and volatile histories of terrestrial bodies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027150','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027150"><span>Tracing the history of submarine <span class="hlt">hydrothermal</span> inputs and the significance of <span class="hlt">hydrothermal</span> hafnium for the seawater budget - A combined Pb-Hf-Nd isotope approach</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>van de Flierdt, T.; Frank, M.; Halliday, A.N.; Hein, J.R.; Hattendorf, B.; Gunther, D.; Kubik, P.W.</p> <p>2004-01-01</p> <p>Secular variations in the Pb isotopic composition of a mixed hydrogenous-<span class="hlt">hydrothermal</span> ferromanganese crust from the Bauer Basin in the eastern Equatorial Pacific provide clear evidence for changes in <span class="hlt">hydrothermal</span> contributions during the past 7 Myr. The nearby Galapagos Rise spreading center provided a strong <span class="hlt">hydrothermal</span> flux prior to 6.5 Ma. After 6.5 Ma, the Pb became stepwise more radiogenic and more similar to Equatorial Pacific seawater, reflecting the westward shift of spreading to the presently <span class="hlt">active</span> East Pacific Rise (EPR). A second, previously unrecognized enhanced <span class="hlt">hydrothermal</span> period occurred between 4.4 and 2.9 Ma, which reflects either off-axis <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> in the Bauer Basin or a late-stage pulse of <span class="hlt">hydrothermal</span> Pb from the then <span class="hlt">active</span>, but waning Galapagos Rise spreading center. Hafnium isotope time-series of the same mixed hydrogenous-<span class="hlt">hydrothermal</span> crust show invariant values over the past 7 Myr. Hafnium isotope ratios, as well as Nd isotope ratios obtained for this crust, are identical to that of hydrogenous Equatorial Pacific deep water crusts and clearly indicate that <span class="hlt">hydrothermal</span> Hf, similar to Nd, does not travel far from submarine vents. Therefore, we suggest that <span class="hlt">hydrothermal</span> Hf fluxes do not contribute significantly to the global marine Hf budget. ?? 2004 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V53A1731O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V53A1731O"><span><span class="hlt">Volcanic</span> emissions from soils at the base of La Fossa volcano, Vulcano island, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Obenholzner, J. H.; Parks, J. L.</p> <p>2006-12-01</p> <p>A top-sealed plastic tube with a diameter of ca. 15 cm had been buried vertically at the base of La Fossa volcano, Volcano island, Italy, next to the front of the obsidian flow. The tube had been filled with quartz wool to condense vapors emanating from the soil. At ca. 75 cm below the surface the sample had been exposed to vapors from Sept. 2005 to April 2006. The leached sample had not been in touch with the ground. Another glass wool cushion (ca. 3 cm thick) had been underneath to minimize capillary effects. Leaching of the quartz wool and ICP-MS analysis documented positive values for: Mg, Al, Si, P, K, Ca, Cr, Mn, Ni, Cu, Zn, Cd, Sn, Pb. Leaching with nitric acid documented also V and Fe. Acid leaching produced higher values for all elements, except K and Sn, than leaching with deionized water. Negative values had been obtained for As, Se, Mo. Influence from soil breathing can be excluded as the <span class="hlt">active</span> fumaroles contain As and Se. This experiment documents for the first time an unknown element transport by vapors/gases through a <span class="hlt">volcanic</span> edifice interacting with <span class="hlt">hydrothermal</span> and magmatic gases. It remains unknown if elements detected are entering the atmosphere or are getting adsorbed onto the <span class="hlt">volcanic</span> ash soil particles derived from reworked surge beds. This question is very important as soils might be an unknown filter medium to filter <span class="hlt">volcanically</span> polluted air in case of major <span class="hlt">volcanic</span> crises. Data can be obtained from the authors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V43A3134L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V43A3134L"><span>Statistical Analysis of Time-Series from Monitoring of <span class="hlt">Active</span> <span class="hlt">Volcanic</span> Vents</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lachowycz, S.; Cosma, I.; Pyle, D. M.; Mather, T. A.; Rodgers, M.; Varley, N. R.</p> <p>2016-12-01</p> <p>Despite recent advances in the collection and analysis of time-series from volcano monitoring, and the resulting insights into <span class="hlt">volcanic</span> processes, challenges remain in forecasting and interpreting <span class="hlt">activity</span> from near real-time analysis of monitoring data. Statistical methods have potential to characterise the underlying structure and facilitate intercomparison of these time-series, and so inform interpretation of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. We explore the utility of multiple statistical techniques that could be widely applicable to monitoring data, including Shannon entropy and detrended fluctuation analysis, by their application to various data streams from <span class="hlt">volcanic</span> vents during periods of temporally variable <span class="hlt">activity</span>. Each technique reveals changes through time in the structure of some of the data that were not apparent from conventional analysis. For example, we calculate the Shannon entropy (a measure of the randomness of a signal) of time-series from the recent dome-forming eruptions of Volcán de Colima (Mexico) and Soufrière Hills (Montserrat). The entropy of real-time seismic measurements and the count rate of certain volcano-seismic event types from both volcanoes is found to be temporally variable, with these data generally having higher entropy during periods of lava effusion and/or larger explosions. In some instances, the entropy shifts prior to or coincident with changes in seismic or eruptive <span class="hlt">activity</span>, some of which were not clearly recognised by real-time monitoring. Comparison with other statistics demonstrates the sensitivity of the entropy to the data distribution, but that it is distinct from conventional statistical measures such as coefficient of variation. We conclude that each analysis technique examined could provide valuable insights for interpretation of diverse monitoring time-series.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.G11A1177F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.G11A1177F"><span>Application of ASAR-ENVISAT Data for Monitoring Andean <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> : Results From Lastarria-Azufre <span class="hlt">Volcanic</span> Complex (Chile-Argentina)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Froger, J.; Remy, D.; Bonvalot, S.; Franco Guerra, M.</p> <p>2005-12-01</p> <p>Since the pioneer study on Mount Etna by Massonnet et al., in 1995, several works have illustrated the promising potentiality of Synthetic Aperture Radar Interferometry (INSAR) for the monitoring of volcanoes. In the case of wide, remote or hazardous <span class="hlt">volcanic</span> areas, in particular, INSAR represents a safer and more economic way to acquire measurements than from ground based geodetic networks. Here we present the preliminary results of an interferometric survey made with ASAR-ENVISAT data on a selection of South American volcanoes where deformation signals had been previously evidenced or are expected. An interesting result is the detection of a present-day <span class="hlt">active</span> ground deformation on the Azufre-Lastarria area (Chile-Argentina) indicating that process, identified during 1998-2000 by Pritchard and Simmons (2004) from ERS data, is still <span class="hlt">active</span>. The phase signal visible on ASAR interferograms (03/2003-06/2005) is roughly elliptical with a 45 km NNE-SSW major axis. Its amplitude increases as a function of time and is compatible with ground uplift in the line of sight of the satellite. The ASAR time series (up to 840 days, 7 ASAR images) indicates variable deformation rate that might confirm the hypothesis of a <span class="hlt">non</span> uniform deformation process. We investigated the origin and the significance of the deformation using various source modelling strategies (analytical and numerical). The observed deformation can be explained by the infilling of an elliptical magmatic reservoir lying between 7 and 10 km depth. The deformation could represent the first stage of a new caldera forming as it is correlated with a large, although subtle, topographic depression surrounded by a crown of monogenetic centers. A short wavelength inflation has also been detected on Lastaria volcano. It could result from the on-going infilling of a small subsurface magmatic reservoir, eventually supplied by the deeper one. All these observations point out the need of a closer monitoring of this area in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2017/5104/sir20175104.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2017/5104/sir20175104.pdf"><span>2015 <span class="hlt">Volcanic</span> <span class="hlt">activity</span> in Alaska—Summary of events and response of the Alaska Volcano Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dixon, James P.; Cameron, Cheryl E.; Iezzi, Alexandra M.; Wallace, Kristi</p> <p>2017-09-28</p> <p>The Alaska Volcano Observatory (AVO) responded to eruptions, <span class="hlt">volcanic</span> unrest or suspected unrest, and seismic events at 14 <span class="hlt">volcanic</span> centers in Alaska during 2015. The most notable <span class="hlt">volcanic</span> <span class="hlt">activity</span> consisted of continuing intermittent ash eruptions from Cleveland and Shishaldin volcanoes in the Aleutian Islands. Two eruptive episodes, at Veniaminof and Pavlof, on the Alaska Peninsula ended in 2015. During 2015, AVO re-established the seismograph network at Aniakchak, installed six new broadband seismometers throughout the Aleutian Islands, and added a Multiple component Gas Analyzer System (MultiGAS) station on Augustine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028818','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028818"><span>Distribution of recent <span class="hlt">volcanism</span> and the morphology of seamounts and ridges in the GLIMPSE study area: Implications for the lithospheric cracking hypothesis for the origin of intraplate, <span class="hlt">non</span>-hot spot <span class="hlt">volcanic</span> chains</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Forsyth, D.W.; Harmon, N.; Scheirer, D.S.; Duncan, R.A.</p> <p>2006-01-01</p> <p>Lithospheric cracking by remotely applied stresses or thermoelastic stresses has been suggested to be the mechanism responsible for the formation of intraplate <span class="hlt">volcanic</span> ridges in the Pacific that clearly do not form above fixed hot spots. As part of the Gravity Lineations Intraplate Melting Petrology and Seismic Expedition (GLIMPSE) project designed to investigate the origin of these features, we have mapped two <span class="hlt">volcanic</span> chains that are <span class="hlt">actively</span> forming to the west of the East Pacific Rise using multibeam echo sounding and side-scan sonar. Side-scan sonar reveals the distribution of rough seafloor corresponding to recent, unsedimented lava flows. In the Hotu Matua <span class="hlt">volcanic</span> complex, recent flows and <span class="hlt">volcanic</span> edifices are distributed over a region 450 km long and up to 65 km wide, with an apparent, irregular age progression from older flows in the west to younger in the east. The 550-km-long Southern Cross Seamount/Sojourn Ridge/Brown Ridge chain appears to have been recently <span class="hlt">active</span> only at its eastern end near the East Pacific Rise. A third region of recent flows is found 120 km north of Southern Cross Seamount in seafloor approximately 9 Myr old. No indication of lithospheric extension in the form of faulting or graben formation paralleling the trend of the <span class="hlt">volcanic</span> chains is found in the vicinity of recent flows or anywhere else in the study area. Thermoelastic cracking could be a factor in the formation of a few small, very narrow <span class="hlt">volcanic</span> ridges, but most of the <span class="hlt">volcanic</span> <span class="hlt">activity</span> is broadly distributed in wide swaths with no indication of formation along narrow cracks. The Sojourn and Brown chains appear to begin as distributed zones of small seamounts that later develop into segmented ridges, perhaps under the influence of membrane stresses from self-loading. We suggest that the linear <span class="hlt">volcanic</span> chains are created by moving melting anomalies in the asthenosphere and that lithospheric cracking plays at most a secondary role. Copyright 2006 by the American</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V23E0512P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V23E0512P"><span>Observed anomalous changes on diffuse CO2 emission at the summit crater of Teide volcano (Tenerife, Canary Islands, Spain): a geochemical evidence of <span class="hlt">volcanic</span> unrest?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perez, N. M.; Melián, G.; Asensio-Ramos, M.; Padrón, E.; Alonso Cótchico, M.; Hernández, P. A.; Rodríguez, F.; D'Auria, L.; García-Merino, M.; Padilla, G. D.; Burns, F.; Amonte, C.; García, E.; García-Hernández, R.; Barrancos, J.; Morales-Ocaña, C.; Calvo, D.; Vela, V.; Pérez, A.</p> <p>2017-12-01</p> <p>Tenerife (2034 km2) is the largest of the Canary Islands and hosts a central <span class="hlt">volcanic</span> complex, Las Cañadas, which is characterized by the eruption of differentiated magmas. Laying inside Las Cañadas a twin stratovolcanoes system Pico Viejo and Teide, has been developed. Although Teide volcano shows weak fumarolic system, <span class="hlt">volcanic</span> gas emissions observed in the summit area are mainly controlled by high rates of diffuse CO2 degassing. Soil CO2 efflux surveys have been performed at the summit crater of Teide volcano since 1999 according to the accumulation chamber method to monitor changes of <span class="hlt">volcanic</span> <span class="hlt">activity</span>. Soil CO2 efflux and soil temperature have been measured in sites homogeneously distributed within an area of about 6,972 m2 inside the summit crater. Historical seismic <span class="hlt">activity</span> in Tenerife has been mainly characterized by low- to moderate-magnitude events (M <2.5), and most of epicenters clustered in an offshore area SE of Tenerife. Very few earthquakes have occurred in other areas, including Teide volcano. Since November 2016 more than 100 small magnitude earthquakes, with typical features of the microseismicity of <span class="hlt">hydrothermal</span> systems, at depths usually ranging between 5 and 15 km located beneath Teide volcano have been recorded. On January 6th 2017 a M=2.5 earthquake was recorded in the area, being one of the strongest events recorded since 2004. Between October 11 and December 13, 2016, a continuous increase on the diffuse CO2 emission was registered preceding the occurrence of the 2.5 seismic event, from 21.3±2.0 to 101.7±20.7 t d-1. In Febraury 2017, the diffuse CO2 emission rate showed a maximum value (176±35 t/d) and has remained at relatively high values in the range 67-176 t/d. The observed increase on the diffuse CO2 emission, likely due to the increase of fluid pressure in the <span class="hlt">hydrothermal</span>-magmatic system of Tenerife, might be a geochemical evidence of a future <span class="hlt">volcanic</span> unrest at Tenerife Island.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1812544B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1812544B"><span>Resistivity structure of the Furnas <span class="hlt">hydrothermal</span> system (Azores archipelago, Portugal) from AMT and ERT imaging.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Byrdina, Svetlana; Vandemeulebrouck, Jean; Rath, Volker; Silva, Catarina; Hogg, Colin; Kiyan, Duygu; Viveiros, Fatima; Eleuterio, Joana; Gresse, Marceau</p> <p>2016-04-01</p> <p>The Furnas <span class="hlt">volcanic</span> complex is located in the eastern part of the São Miguel Island and comprises a 5 km × 8 km summit depression filled by two nested calderas with several craters and a lake. Present-day <span class="hlt">volcanic</span> <span class="hlt">activity</span> of Furnas volcano is mostly located in the northern part of the caldera, within the Furnas village and north to Furnas Lake, where <span class="hlt">hydrothermal</span> manifestations are mainly fumarolic fields, steam vents, thermal springs, and intense soil diffuse degassing. Considering the Furnas volcano as a whole, the total integrated CO2 efflux is extremely high, with a total amount of CO2 close to 1000 ton per day (Viveiros et al., 2009). We present the first results of an electrical resistivity tomography (ERT), combined with audio-magneto-telluric (AMT) measurements aligned along two profiles inside the caldera. The purpose of this survey is to delimit the extent, the geometry, and the depth of the <span class="hlt">hydrothermal</span> system and to correlate the deep resistivity structure with high resolution cartography of diffuse CO2 flux (Viveiros et al, 2015). The ERT and AMT methods are complementary in terms of resolution and penetration depth: ERT can image the structural details of shallow <span class="hlt">hydrothermal</span> system (down to 100 m in our study) while AMT can image at lower resolution deeper structures at the roots of a volcano (down to 4 km in our study). Our first independent 2D inversions of the ERT-AMT data show a good agreement between the surficial and deeper features. Below the main fumarole area we observe a low resistivity body (less than 1 Ohmm) which corresponds well to the high CO2 flux at the surface and is associated with an extended conductive body at larger depth. These results strongly suggest the presence of <span class="hlt">hydrothermal</span> waters at depth or/and the presence of altered clay-rich material. On a larger scale however, the geometry of the conducting zones differs slightly from what was expected from earlier surface studies, and may not be directly related to fault zones</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.V41A0977D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.V41A0977D"><span>Observing <span class="hlt">Active</span> <span class="hlt">Volcanism</span> on Earth and Beyond With an Autonomous Science Investigation Capability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davies, A. G.; Mjolsness, E. D.; Fink, W.; Castano, R.; Park, H. G.; Zak, M.; Burl, M. C.</p> <p>2001-12-01</p> <p>Operational constraints imposed by restricted downlink and long communication delays make autonomous systems a necessity for exploring dynamic processes in the Solar System and beyond. Our objective is to develop an onboard, modular, automated science analysis tool that will autonomously detect unexpected events, identify rare events at predicted sites, quantify the processes under study, and prioritize the science data and analyses as they are collected. A primary target for this capability is terrestrial <span class="hlt">active</span> <span class="hlt">volcanism</span>. Our integrated, science-driven command and control package represents the next stage of the automatic monitoring of <span class="hlt">volcanic</span> <span class="hlt">activity</span> pioneered by GOES. The resulting system will maximize science return from day-to-day instrument use and provide immediate reaction to capture the fullest information from infrequent events. For example, a sensor suite consisting of a Galileo-like multi-filter visible wavelength camera and an infrared spectrometer, can acquire high-spatial resolution data of eruptions of lava and <span class="hlt">volcanic</span> plumes and identify large concentrations of <span class="hlt">volcanic</span> SO2. After image/spectrum formation, software is applied to the data which is capable of change detection (in the visible and infrared), feature identification (both in imagery and spectra), and novelty detection. In this particular case, the latter module detects change in the parameter space of an advanced multi-component black-body <span class="hlt">volcanic</span> thermal emission model by means of a novel technique called the "Grey-Box" method which analyzes time series data through a combination of deterministic and stochastic models. This approach can be demonstrated using data obtained by the Galileo spacecraft of ionian <span class="hlt">volcanism</span>. The system autonomously identifies the most scientifically important targets and prioritizes data and analyses for return. All of these techniques have been successfully demonstrated in laboratory experiments, and are ready to be tested in an operational environment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033796','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033796"><span>Evidence of <span class="hlt">volcanic</span> and glacial <span class="hlt">activity</span> in Chryse and Acidalia Planitiae, Mars</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Martinez-Alonso, Sara; Mellon, Michael T.; Banks, Maria E.; Keszthelyi, Laszlo P.; McEwen, Alfred S.</p> <p>2011-01-01</p> <p>Chryse and Acidalia Planitiae show numerous examples of enigmatic landforms previously interpreted to have been influenced by a water/ice-rich geologic history. These landforms include giant polygons bounded by kilometer-scale arcuate troughs, bright pitted mounds, and mesa-like features. To investigate the significance of the last we have analyzed in detail the region between 60°N, 290°E and 10°N, 360°E utilizing HiRISE (High Resolution Imaging Science Experiment) images as well as regional-scale data for context. The mesas may be analogous to terrestrial tuyas (emergent sub-ice volcanoes), although definitive proof has not been identified. We also report on a blocky unit and associated landforms (drumlins, eskers, inverted valleys, kettle holes) consistent with ice-emplaced <span class="hlt">volcanic</span> or volcano-sedimentary flows. The spatial association between tuya-like mesas, ice-emplaced flows, and further possible evidence of <span class="hlt">volcanism</span> (deflated flow fronts, <span class="hlt">volcanic</span> vents, columnar jointing, rootless cones), and an extensive fluid-rich substratum (giant polygons, bright mounds, rampart craters), allows for the possibility of glaciovolcanic <span class="hlt">activity</span> in the region.Landforms indicative of glacial <span class="hlt">activity</span> on Chryse/Acidalia suggest a paleoclimatic environment remarkably different from today's. Climate changes on Mars (driven by orbital/obliquity changes) or giant outflow channel <span class="hlt">activity</span> could have resulted in ice-sheet-related landforms far from the current polar caps.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGP11A..07F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGP11A..07F"><span>Absolute Magnetization Distribution on Back-arc Spreading Axis Hosting <span class="hlt">Hydrothermal</span> Vents; Insight from Shinkai 6500 Magnetic Survey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fujii, M.; Okino, K.; Honsho, C.; Mochizuki, N.; Szitkar, F.; Dyment, J.</p> <p>2013-12-01</p> <p>Near-bottom magnetic profiling using submersible, deep-tow, Remotely Operated Vehicle (ROV) and Autonomous Underwater Vehicle (AUV) make possible to conduct high-resolution surveys and depict detailed magnetic features reflecting, for instance, the presence of fresh lavas or <span class="hlt">hydrothermal</span> alteration, or geomagnetic paleo-intensity variations. We conducted near-bottom three component magnetic measurements onboard submersible Shinkai 6500 in the Southern Mariana Trough, where five <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vent fields (Snail, Yamanaka, Archean, Pica, and Urashima sites) have been found in both on- and off-axis areas of the <span class="hlt">active</span> back-arc spreading center, to detect signals from <span class="hlt">hydrothermally</span> altered rock and to distinguish old and new submarine lava flows. Fourteen dives were carried out at an altitude of 1-40 m during the R/V Yokosuka YK10-10 and YK10-11 cruises in 2010. We carefully corrected the effect of the induced and permanent magnetizations of the submersible by applying the correction method for the shipboard three-component magnetometer measurement modified for deep-sea measurement, and subtracted the IGRF values from the corrected data to obtain geomagnetic vector anomalies along the dive tracks. We then calculated the synthetic magnetic vector field produced by seafloor, assumed to be uniformly magnetized, using three dimensional forward modeling. Finally, values of the absolute magnetizations were estimated by using a linear transfer function in the Fourier domain from the observed and synthetic magnetic anomalies. The distribution of estimated absolute magnetization generally shows low values around the five <span class="hlt">hydrothermal</span> vent sites. This result is consistent with the equivalent magnetization distribution obtained from previous AUV survey data. The areas of low magnetization are also consistent with <span class="hlt">hydrothermal</span> deposits identified in video records. These results suggest that low magnetic signals are due to <span class="hlt">hydrothermal</span> alteration zones where host rocks are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..309...96B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..309...96B"><span>Geology of the Mid-Miocene Rooster Comb Caldera and Lake Owyhee <span class="hlt">Volcanic</span> Field, eastern Oregon: Silicic <span class="hlt">volcanism</span> associated with Grande Ronde flood basalt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benson, Thomas R.; Mahood, Gail A.</p> <p>2016-01-01</p> <p>The Lake Owyhee <span class="hlt">Volcanic</span> Field (LOVF) of eastern Oregon consists of rhyolitic caldera centers and lava fields contemporaneous with and spatially related to Mid-Miocene Columbia River flood basalt <span class="hlt">volcanism</span>. Previous studies delineated two calderas in the southeastern part of LOVF near Owyhee Reservoir, the result of eruptions of two ignimbrites, the Tuff of Leslie Gulch and the Tuff of Spring Creek. Our new interpretation is that these two map units are differentially altered parts of a single ignimbrite produced in a major phreatomagmatic eruption at 15.8 Ma. Areas previously mapped as Tuff of Spring Creek are locations where the ignimbrite contains abundant clinoptilolite ± mordenite, which made it susceptible to erosion. The resistant intracaldera Tuff of Leslie Gulch has an alteration assemblage of albite ± quartz, indicative of low-temperature <span class="hlt">hydrothermal</span> alteration. Our new mapping of caldera lake sediments and pre- and post-caldera rhyolitic lavas and intrusions that are chemically similar to intracaldera Tuff of Leslie Gulch point to a single 20 × 25 km caldera, which we name the Rooster Comb Caldera. Erosion of the resurgently uplifted southern half of the caldera created dramatic exposures of intracaldera Tuff of Leslie Gulch cut by post-caldera rhyolite dikes and intrusions that are the deeper-level equivalents of lava domes and flows that erupted into the caldera lake preserved in exposures to the northeast. The Rooster Comb Caldera has features in common with more southerly Mid-Miocene calderas of the McDermitt <span class="hlt">Volcanic</span> Field and High Rock Caldera Complex, including formation in a basinal setting shortly after flood basalt eruptions ceased in the region, and forming on eruption of peralkaline ignimbrite. The <span class="hlt">volcanism</span> at Rooster Comb Caldera postdates the main <span class="hlt">activity</span> at McDermitt and High Rock, but, like it, begins 300 ky after flood basalt <span class="hlt">volcanism</span> begins in the area, and while flood basalts don't erupt through the silicic focus, are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70178381','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70178381"><span>Geologic history of Martian regolith breccia Northwest Africa 7034: Evidence for <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and lithologic diversity in the Martian crust</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McCubbin, Francis M.; Boyce, Jeremy W.; Novak-Szabo, Timea; Santos, Alison; Tartese, Romain; Muttik, Nele; Domokos, Gabor; Vazquez, Jorge A.; Keller, Lindsay P.; Moser, Desmond E.; Jerolmack, Douglas J.; Shearer, Charles K.; Steele, Andrew; Elardo, Stephen M.; Rahman, Zia; Anand, Mahesh; Delhaye, Thomas; Agee, Carl B.</p> <p>2016-01-01</p> <p>The timing and mode of deposition for Martian regolith breccia Northwest Africa (NWA) 7034 were determined by combining petrography, shape analysis, and thermochronology. NWA 7034 is composed of igneous, impact, and brecciated clasts within a thermally annealed submicron matrix of pulverized crustal rocks and devitrified impact/<span class="hlt">volcanic</span> glass. The brecciated clasts are likely lithified portions of Martian regolith with some evidence of past <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Represented lithologies are primarily ancient crustal materials with crystallization ages as old as 4.4 Ga. One ancient zircon was hosted by an alkali-rich basalt clast, confirming that alkalic <span class="hlt">volcanism</span> occurred on Mars very early. NWA 7034 is composed of fragmented particles that do not exhibit evidence of having undergone bed load transport by wind or water. The clast size distribution is similar to terrestrial pyroclastic deposits. We infer that the clasts were deposited by atmospheric rainout subsequent to a pyroclastic eruption(s) and/or impact event(s), although the ancient ages of igneous components favor mobilization by impact(s). Despite ancient components, the breccia has undergone a single pervasive thermal event at 500–800°C, evident by groundmass texture and concordance of ~1.5 Ga dates for bulk rock K-Ar, U-Pb in apatite, and U-Pb in metamict zircons. The 1.5 Ga age is likely a thermal event that coincides with rainout/breccia lithification. We infer that the episodic process of regolith lithification dominated sedimentary processes during the Amazonian Epoch. The absence of pre-Amazonian high-temperature metamorphic events recorded in ancient zircons indicates source domains of static southern highland crust punctuated by episodic impact modification.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JVGR..121..271C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JVGR..121..271C"><span>Environmental hazards of fluoride in <span class="hlt">volcanic</span> ash: a case study from Ruapehu volcano, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cronin, Shane J.; Neall, V. E.; Lecointre, J. A.; Hedley, M. J.; Loganathan, P.</p> <p>2003-03-01</p> <p>The vent-hosted <span class="hlt">hydrothermal</span> system of Ruapehu volcano is normally covered by a c. 10 million m 3 acidic crater lake where <span class="hlt">volcanic</span> gases accumulate. Through analysis of eruption observations, granulometry, mineralogy and chemistry of <span class="hlt">volcanic</span> ash from the 1995-1996 Ruapehu eruptions we report on the varying influences on environmental hazards associated with the deposits. All measured parameters are more dependent on the eruptive style than on distance from the vent. Early phreatic and phreatomagmatic eruption phases from crater lakes similar to that on Ruapehu are likely to contain the greatest concentrations of environmentally significant elements, especially sulphur and fluoride. These elements are contained within altered xenolithic material extracted from the <span class="hlt">hydrothermal</span> system by steam explosions, as well as in residue <span class="hlt">hydrothermal</span> fluids adsorbed on to particle surfaces. In particular, total F in the ash may be enriched by a factor of 6 relative to original magmatic contents, although immediately soluble F does not show such dramatic increases. Highly soluble NaF and CaSiF 6 phases, demonstrated to be the carriers of 'available' F in purely magmatic eruptive systems, are probably not dominant in the products of phreatomagmatic eruptions through <span class="hlt">hydrothermal</span> systems. Instead, slowly soluble compounds such as CaF 2, AlF 3 and Ca 5(PO 4) 3F dominate. Fluoride in these phases is released over longer periods, where only one third is leached in a single 24-h water extraction. This implies that estimation of soluble F in such ashes based on a single leach leads to underestimation of the F impact, especially of a potential longer-term environmental hazard. In addition, a large proportion of the total F in the ash is apparently soluble in the digestive system of grazing animals. In the Ruapehu case this led to several thousand sheep deaths from fluorosis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B21A0329W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B21A0329W"><span><span class="hlt">Volcanic</span> Eruptions of the EPR and Ridge Axis Segmentation: An Interdisciplinary View</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>White, S.; Soule, S. A.; Tolstoy, M.; Waldhauser, F.; Rubin, K.</p> <p>2008-12-01</p> <p>The eruption of the EPR in 2005-06 provides an ideal window into the relationship between fine-scale segmentation of the ridge axis and individual eruptive episodes. Lava flow mapping of the eruption by visual and acoustic images, precise dates on multiple eruptive units, stress information from seismicity, long-term records of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>, and well known segment boundaries illustrate the relationships between eruptions and segmentation of mid-ocean ridges. Lava flows emerged from several sections of the axial summit trough (AST) during the eruption, presumably from en echelon fissures between 9 45'N and 9 57'N. Each en echelon fissure is a 4th order segment, and the overall area matches the 3rd Order segment between ~9 45'N and ~9 58'N. Within the eruption, the primary eruptive fissure jumped east by 600 m at 9 53'N, and ran along an inward facing fault scarp, although limited lava effusion also extended northward along the axial fissure. A zone of high seismicity connects the normal fault bounding the eastern fissure eruption with the main locus of eruption on the ridge axis to the south, suggesting that the offset eruption may have occurred in response to stress buildup on this fault. Radiometric ages indicate that the entire along-axis extent of the eruptive fissures <span class="hlt">activated</span> initially, but that <span class="hlt">volcanic</span> <span class="hlt">activity</span> focused to a single fourth-order segment within 1-3 months. Previously indentified breaks in the AST and its overall outline were largely unchanged by the eruption. These observations support the hypothesis that fourth-order segments are offsets controlled by the mechanics of dike emplacement, whereas third-order segments represent discrete <span class="hlt">volcanic</span> systems. Dike segmentation may be controlled by variations in underlying ridge structure or the magma reservoir. <span class="hlt">Hydrothermal</span> systems disrupted as far south as 9 37'N may be responding to cracking due to stress interaction or share a common deeper magmatic source. Comparisons between the 1991 EPR</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/2007AGUFM.V51F..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V51F..02S"><span>Seismic and GPS constraints on the dynamics and kinematics of the Yellowstone <span class="hlt">volcanic</span> field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, R. B.; Farrell, J.; Jordan, M.; Puskas, C.; Waite, G. P.</p> <p>2007-12-01</p> <p>The seismically and <span class="hlt">volcanically</span> Yellowstone hotspot resulted from interaction of a mantle plume with the overriding North America plate. This feature and related processes have modified continental lithosphere producing the Yellowstone-Snake River Plain-Newberry silicic <span class="hlt">volcanic</span> field (YSRPN) system, with its NE <span class="hlt">volcanically</span> <span class="hlt">active</span> Yellowstone <span class="hlt">volcanic</span> field. The size and accessibility of the Yellowstone area has allowed a range of geophysical experiments including earthquake monitoring and seismic and GPS imaging of this system. Seismicity is dominated by small-magnitude normal- to oblique-slip faulting earthquake swarms with shallow focal depths, maximum of ~5 km, restricted by high temperatures and a weak elastic layer. There is developing evidence of <span class="hlt">non</span>-double couple events. Outside the caldera, earthquakes are deeper, ~20 km, and capable of M 7+ earthquakes. We integrate the results from a multi-institution experiment that recorded data from 110 seismic stations and 180 GPS stations for 1999-2004. The tomographic images confirm the existence of a low Vp-body beneath the Yellowstone caldera at depths greater than 8 km, possibly representing hot, crystallizing magma. A key result of our study is a volume of anomalously low Vp and Vp/Vs in the northwestern part of the <span class="hlt">volcanic</span> field at shallow depths of <2.0 km. Theoretical calculations of changes in P- to S-wave velocity ratios indicate that these anomalies can be interpreted as porous, gas-filled rock. GPS-measured episodes of caldera kinematics reveals uplift and subsidence of the caldera at decadal scales with average rates of ~20 mm/yr but much higher short-term rates of up to 70 mm/yr of accelerated uplift, 2004-2007. The stress field inverted from seismic and GPS data is dominated by regional SW extension with superimposed volumetric expansion and uplift from local <span class="hlt">volcanic</span> sources. Mantle tomography derived from integrated inversion of teleseismic and local earthquake data constrained by geoid, crustal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70000042','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70000042"><span>Hawaiian oral tradition describes 400 years of <span class="hlt">volcanic</span> <span class="hlt">activity</span> at Kīlauea</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Swanson, Donald A.</p> <p>2008-01-01</p> <p>Culturally significant oral tradition involving Pele, the Hawaiian volcano deity, and her youngest sister Hi'iaka may involve the two largest <span class="hlt">volcanic</span> events to have taken place in Hawai'i since human settlement: the roughly 60-year-long ‘Ailā’au eruption during the 15th century and the following development of Kīlauea's caldera. In 1823, Rev. William Ellis and three others became the first Europeans to visit Kīlauea's summit and were told stories about Kīlauea's <span class="hlt">activity</span> that are consistent with the Pele–Hi'iaka account and extend the oral tradition through the 18th century. Recent geologic studies confirm the essence of the oral traditions and illustrate the potential value of examining other Hawaiian chants and stories for more information about past <span class="hlt">volcanic</span> <span class="hlt">activity</span> in Hawai‘i.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T13B2718A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T13B2718A"><span>Imaging <span class="hlt">hydrothermal</span> roots along the Endeavour segment of the Juan de Fuca ridge using elastic full waveform inversion.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arnulf, A. F.; Harding, A. J.; Kent, G. M.</p> <p>2016-12-01</p> <p>The Endeavour segment is a 90 km-long, medium-spreading-rate, oceanic spreading center located on the northern Juan de Fuca ridge (JDFR). The central part of this segment forms a 25-km-long <span class="hlt">volcanic</span> high that hosts five of the most <span class="hlt">hydrothermally</span> <span class="hlt">active</span> vent fields on the MOR system, namely (from north to south): Sasquatch, Salty Dawg, High Rise, Main Endeavour and Mothra. Mass, heat and chemical fluxes associated to vigorous <span class="hlt">hydrothermal</span> venting are large, however the geometry of the fluid circulation system through the oceanic crust remains almost completely undefined. To produce high-resolution velocity/reflectivity structures along the axis of the Endeavour segment, here, we combined a synthetic ocean bottom experiment (SOBE), 2-D traveltime tomography, 2D elastic full waveform and reverse time migration (RTM). We present velocity and reflectivity sections along Endeavour segment at unprecedented spatial resolutions. We clearly image a set of independent, geometrically complex, elongated low-velocity regions linking the top of the magma chamber at depth to the <span class="hlt">hydrothermal</span> vent fields on the seafloor. We interpret these narrow pipe-like units as focused regions of <span class="hlt">hydrothermal</span> fluid up-flow, where acidic and corrosive fluids form pipe-like alteration zones as previously observed in Cyprus ophiolites. Furthermore, the amplitude of these low-velocity channels is shown to be highly variable, with the strongest velocity drops observed at Main Endeavour, Mothra and Salty Dawg <span class="hlt">hydrothermal</span> vent fields, possibly suggesting more mature <span class="hlt">hydrothermal</span> cells. Interestingly, the near-seafloor structure beneath those three sites is very similar and highlights a sharp lateral transition in velocity (north to south). On the other hand, the High-Rise <span class="hlt">hydrothermal</span> vent field is characterized by several lower amplitudes up-flow zones and relatively slow near-surface velocities. Last, Sasquatch vent field is located in an area of high near-surface velocities and is not</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4960541','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4960541"><span>Volcano electrical tomography unveils edifice collapse hazard linked to <span class="hlt">hydrothermal</span> system structure and dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rosas-Carbajal, Marina; Komorowski, Jean-Christophe; Nicollin, Florence; Gibert, Dominique</p> <p>2016-01-01</p> <p>Catastrophic collapses of the flanks of stratovolcanoes constitute a major hazard threatening numerous lives in many countries. Although many such collapses occurred following the ascent of magma to the surface, many are not associated with magmatic reawakening but are triggered by a combination of forcing agents such as pore-fluid pressurization and/or mechanical weakening of the <span class="hlt">volcanic</span> edifice often located above a low-strength detachment plane. The volume of altered rock available for collapse, the dynamics of the <span class="hlt">hydrothermal</span> fluid reservoir and the geometry of incipient collapse failure planes are key parameters for edifice stability analysis and modelling that remain essentially hidden to current volcano monitoring techniques. Here we derive a high-resolution, three-dimensional electrical conductivity model of the La Soufrière de Guadeloupe volcano from extensive electrical tomography data. We identify several highly conductive regions in the lava dome that are associated to fluid saturated host-rock and preferential flow of highly acid hot fluids within the dome. We interpret this model together with the existing wealth of geological and geochemical data on the volcano to demonstrate the influence of the <span class="hlt">hydrothermal</span> system dynamics on the hazards associated to collapse-prone altered <span class="hlt">volcanic</span> edifices. PMID:27457494</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..341...70B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..341...70B"><span>Satellite observations of fumarole <span class="hlt">activity</span> at Aluto volcano, Ethiopia: Implications for geothermal monitoring and <span class="hlt">volcanic</span> hazard</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Braddock, Mathilde; Biggs, Juliet; Watson, Iain M.; Hutchison, William; Pyle, David M.; Mather, Tamsin A.</p> <p>2017-07-01</p> <p>Fumaroles are the surface manifestation of <span class="hlt">hydrothermal</span> circulation and can be influenced by magmatic, <span class="hlt">hydrothermal</span>, hydrological and tectonic processes. This study investigates the temporal changes in fumarole temperatures and spatial extent on Aluto, a restless volcano in the Main Ethiopian Rift (MER), in order to better understand the controls on fluid circulation and the interaction between the magmatic and <span class="hlt">hydrothermal</span> systems. Thermal infrared (TIR) satellite images, acquired by the Advanced Spaceborne Thermal Emission and Reflection radiometer (ASTER) over the period of 2004 to 2016, are used to generate time series of the fumarole temperatures and areas. The thermal anomalies identified in the ASTER images coincide with known fumaroles with temperatures > 80 °C and are located on or close to fault structures, which provide a pathway for the rising fluids. Most of the fumaroles, including those along the major zone of <span class="hlt">hydrothermal</span> upwelling, the Artu Jawe Fault Zone, have pixel-integrated temperature variations of only 2 ± 1.5 °C. The exception are the Bobesa fumaroles located on a hypothesised caldera ring fault which show pixel-integrated temperature changes of up to 9 °C consistent with a delayed response of the <span class="hlt">hydrothermal</span> system to precipitation. We conclude that fumaroles along major faults are strongly coupled to the magmatic-<span class="hlt">hydrothermal</span> system and are relatively stable with time, whereas those along shallower structures close to the rift flank are more strongly influenced by seasonal variations in groundwater flow. The use of remote sensing data to monitor the thermal <span class="hlt">activity</span> of Aluto provides an important contribution towards understanding the behaviour of this <span class="hlt">actively</span> deforming volcano. This method could be used at other volcanoes around the world for monitoring and geothermal exploration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..340...52W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..340...52W"><span>Seismicity associated with magmatism, faulting and <span class="hlt">hydrothermal</span> circulation at Aluto Volcano, Main Ethiopian Rift</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilks, Matthew; Kendall, J.-Michael; Nowacki, Andy; Biggs, Juliet; Wookey, James; Birhanu, Yelebe; Ayele, Atalay; Bedada, Tulu</p> <p>2017-06-01</p> <p>The silicic <span class="hlt">volcanic</span> centres of the Main Ethiopian Rift (MER) play a central role in facilitating continental rifting. Many of these volcanoes host geothermal resources and are located in heavily populated regions. InSAR studies have shown several are deforming, but regional seismic networks have detected little seismicity. A local network of 12 seismometers was deployed at Aluto Volcano from 2012 to 2014, and detected 2142 earthquakes within a 24-month period. We locate the events using a 1D velocity model that exploits a regional model and information from geothermal boreholes and calculate local magnitudes, b-values and focal mechanisms. Event depths generally range from the near surface to 15 km with most of the seismicity clustering in the upper 2 km. A significant amount of seismicity follows the Artu Jawa Fault Zone, which trends in alignment with the Wonji Fault Belt, NNE-SSW and is consistent with previous studies of strain localisation in the MER. Focal mechanisms are mostly normal in style, with the mean T-axes congruent to the orientation of extension in the rift at this latitude. Some show relatively small left-lateral strike-slip components and are likely associated with the reactivation of NE-ENE structures at the southern tip of the Aluto-Gedemsa segment. Events range from - 0.40 to 2.98 in magnitude and we calculate an overall b-value of 1.40 ± 0.14. This relatively elevated value suggests fluid-induced seismicity that is particularly evident in the shallow <span class="hlt">hydrothermal</span> reservoir and above it. Subdividing our observations according to depth identifies distinct regions beneath the <span class="hlt">volcanic</span> edifice: a shallow zone (- 2-0 km) of high seismicity and high b-values that corresponds to the <span class="hlt">hydrothermal</span> system and is influenced by a high fluid saturation and circulation; a relatively aseismic zone (0-2 km) with low b-values that is impermeable to ascending volatiles; a region of increased fluid-induced seismicity (2-9 km) that is driven by magmatic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V21A4730T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V21A4730T"><span>Study of <span class="hlt">hydrothermal</span> channels based on near-bottom magnetic prospecting: Application to Longqi <span class="hlt">hydrothermal</span> area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tao, W.; Tao, C.; Li, H.; Zhaocai, W.; Jinhui, Z.; Qinzhu, C.; Shili, L.</p> <p>2014-12-01</p> <p>Mid-ocean ridges, largely present far from the continental plates, are characterized by complex geological structures and numerous <span class="hlt">hydrothermal</span> systems with complex controlling factors. Exploring seafloor sulfide resources for industrial and scientific applications is a challenge. With the advent of geophysical surveys for seabed investigation, near-bottom magnetic prospecting, which yields shallow geological structure, is an efficient method for investigating <span class="hlt">active</span> and inactive <span class="hlt">hydrothermal</span> fields and for researching the structure of <span class="hlt">hydrothermal</span> systems (Tivey et al., 1993, 1996;German et al., 2008). We collected near-bottom magnetic data in the Longqi <span class="hlt">hydrothermal</span> area, located in the southwest Indian ridge (49.6° E; Zhu et al., 2010; Tao et al., 2014), using the autonomous benthic explorer, an autonomous underwater vehicle, during the second leg of the Chinese cruise DY115-19 on board R/V DaYangYiHao. Based on the results of the intensity of the spatial differential vector method (Seaman et al., 1993), we outline the <span class="hlt">hydrothermal</span> alternation zone. By building models, we subsequently infer a fault along the discovered <span class="hlt">hydrothermal</span> vents; this fault line may be connected to a detachment fault (Zhao et al., 2013). In addition, we discuss the channels of the <span class="hlt">hydrothermal</span> circulation system (Figure 1), and presume that heat was conducted to the sea subsurface by the detachment fault; the aqueous fluid that infiltrated the fault is heated and conveyed to the seafloor, promoting the circulation of the <span class="hlt">hydrothermal</span> system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS22B..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS22B..01B"><span>On the global distribution of <span class="hlt">hydrothermal</span> vent fields: One decade later</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beaulieu, S. E.; Baker, E. T.; German, C. R.</p> <p>2012-12-01</p> <p>Since the last global compilation one decade ago, the known number of <span class="hlt">active</span> submarine <span class="hlt">hydrothermal</span> vent fields has almost doubled. At the end of 2009, a total of 518 <span class="hlt">active</span> vent fields was catalogued, with about half (245) visually confirmed and others (273) inferred <span class="hlt">active</span> at the seafloor. About half (52%) of these vent fields are at mid-ocean ridges (MORs), 25% at <span class="hlt">volcanic</span> arcs, 21% at back-arc spreading centers (BASCs), and 2% at intra-plate volcanoes and other settings. One third are in high seas, and the nations with the most known <span class="hlt">active</span> vent fields within EEZs are Tonga, USA, Japan, and New Zealand. The increase in known vent fields reflects a number of factors, including increased national and commercial interests in seafloor <span class="hlt">hydrothermal</span> deposits as mineral resources. Here, we have comprehensively documented the percentage of strike length at MORs and BASCs that has been systematically explored for <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. As of the end of 2009, almost 30% of the ~60,000 km of MORs had been surveyed at least with spaced vertical profiles to detect <span class="hlt">hydrothermal</span> plumes. A majority of the vents discovered at MORs in the past decade occurred at segments with < 60 mm/yr full spreading rate. Discoveries at ultra-slow MORs in the past decade included the deepest known vent (Beebe at Mid-Cayman Rise) and high-temperature black smoker vents (e.g., Dragon at SWIR and Loki's Castle at Mohns Ridge), and the highest temperature vent was measured at the slow-spreading S MAR (Turtle Pits). Using a previously published equation for the linear relationship between the number of <span class="hlt">active</span> vent fields per 100 km strike length (F_s) vs. weighted-average full spreading rate (u_s), we predicted 676 vent fields remaining to be discovered at MORs. Even accounting for the lower F_s at slower spreading rates, almost half of the vents that are predicted remaining to be discovered at MORs are at ultra-slow to slow spreading rates (< 40 mm/yr) and about 1/3 at intermediate rates (40-80 mm</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA21442.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA21442.html"><span>Enceladus <span class="hlt">Hydrothermal</span> <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-04-13</p> <p>This graphic illustrates how scientists on NASA's Cassini mission think water interacts with rock at the bottom of the ocean of Saturn's icy moon Enceladus, producing hydrogen gas (H2). The Cassini spacecraft detected the hydrogen in the plume of gas and icy material spraying from Enceladus during its deepest and last dive through the plume on Oct. 28, 2015. Cassini also sampled the plume's composition during previous flybys, earlier in the mission. From these observations scientists have determined that nearly 98 percent of the gas in the plume is water vapor, about 1 percent is hydrogen, and the rest is a mixture of other molecules including carbon dioxide, methane and ammonia. The graphic shows water from the ocean circulating through the seafloor, where it is heated and interacts chemically with the rock. This warm water, laden with minerals and dissolved gases (including hydrogen and possibly methane) then pours into the ocean creating chimney-like vents. The hydrogen measurements were made using Cassini's Ion and Neutral Mass Spectrometer, or INMS, instrument, which sniffs gases to determine their composition. The finding is an independent line of evidence that <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> is taking place in the Enceladus ocean. Previous results from Cassini's Cosmic Dust Analyzer instrument, published in March 2015, suggested hot water is interacting with rock beneath the ocean; the new findings support that conclusion and indicate that the rock is reduced in its geochemistry. With the discovery of hydrogen gas, scientists can now conclude that there is a source of chemical free energy in Enceladus' ocean. https://photojournal.jpl.nasa.gov/catalog/PIA21442</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JVGR..276..132G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JVGR..276..132G"><span>Asymmetrical structure, <span class="hlt">hydrothermal</span> system and edifice stability: The case of Ubinas volcano, Peru, revealed by geophysical surveys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gonzales, Katherine; Finizola, Anthony; Lénat, Jean-François; Macedo, Orlando; Ramos, Domingo; Thouret, Jean-Claude; Fournier, Nicolas; Cruz, Vicentina; Pistre, Karine</p> <p>2014-04-01</p> <p>Ubinas volcano, the historically most <span class="hlt">active</span> volcano in Peru straddles a low-relief high plateau and the flank of a steep valley. A multidisciplinary geophysical study has been performed to investigate the internal structure and the fluids flow within the edifice. We conducted 10 self-potential (SP) radial (from summit to base) profiles, 15 audio magnetotelluric (AMT) soundings on the west flank and a detailed survey of SP and soil temperature measurements on the summit caldera floor. The typical “V” shape of the SP radial profiles has been interpreted as the result of a <span class="hlt">hydrothermal</span> zone superimposed on a hydrogeological zone in the upper parts of the edifice, and depicts a sub-circular SP positive anomaly, about 6 km in diameter. The latter is centred on the summit, and is characterised by a larger extension on the western flank located on the low-relief high plateau. The AMT resistivity model shows the presence of a conductive body beneath the summit at a depth comparable to that of the bottom of the inner south crater in the present-day caldera, where intense <span class="hlt">hydrothermal</span> manifestations occur. The lack of SP and temperature anomalies on the present caldera floor suggests a self-sealed <span class="hlt">hydrothermal</span> system, where the inner south crater acts as a pressure release valve. Although no resistivity data exists on the eastern flank, we presume, based on the asymmetry of the basement topography, and the amplitude of SP anomalies on the east flank, which are approximately five fold that on the west flank, that gravitational flow of <span class="hlt">hydrothermal</span> fluids may occur towards the deep valley of Ubinas. This hypothesis, supported by the presence of hot springs and faults on the eastern foot of the edifice, reinforces the idea that a large part of the southeast flank of the Ubinas volcano may be altered by <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and will tend to be less stable. One of the major findings that stems from this study is that the slope of the basement on which a volcano has grown</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P31B2058M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P31B2058M"><span>Connecting Io's <span class="hlt">volcanic</span> <span class="hlt">activity</span> to the Io plasma torus: comparison of Galileo/NIMS <span class="hlt">volcanic</span> and ground-based torus observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Magalhaes, F. P.; Lopes, R. M. C.; Rathbun, J. A.; Gonzalez, W. D.; Morgenthaler, J. P.; Echer, E.; Echer, M. P. D. S.</p> <p>2015-12-01</p> <p>Io, the innermost of the Jupiter's four Galilean moons, is a remarkable object in the Solar System, due to its intense and energetic <span class="hlt">volcanic</span> <span class="hlt">activity</span>. The <span class="hlt">volcanic</span> sulfur and oxygen in Io's tenuous atmosphere escapes forming an extended neutral cloud around Io and Jupiter. Subsequently, by ionization and pickup ions, a ring of charged particles encircling Jupiter is created, forming the Io plasma torus. Considering this scenario, it is reasonable to expect that the Io plasma torus should be affected by changes in Io's <span class="hlt">volcanism</span>. Interactions between Io and the Jovian environment is unique and yet not very well understood. Here we present two sets of observations. One from the Galileo Near-Infrared Imaging Spectrograph (NIMS) instrument, which obtained spectral image cubes between 0.7 and 5.2 microns. The other dataset is from ground-based observations of the [SII] 6731 Å emission lines from the Io plasma torus, obtained at McMath-Pierce Solar Telescope, at Kitt Peak. Our dataset from the [SII] 6731 Å emission lines cover more years than the one from the NIMS data. The years presented in this work for a comparative study are from 1998 through 2001. Using the NIMS instrument we were able to identify which volcanoes were <span class="hlt">active</span> and measure their level of <span class="hlt">activity</span>. From the [SII] 6731 Å emission lines we were able to trace the densest part of the torus and also the brightness of both ansa. By comparing the results from the Galileo instrument and the ground-based observations, we are exploring how the Io plasma torus responds to large eruptions from Io. We aim with this study to help improve our understanding of this complex coupled system, Jupiter-Io.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001535.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001535.html"><span><span class="hlt">Volcanic</span> <span class="hlt">Activity</span> at Shiveluch and Plosky Tolbachik</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>On March 7, 2013 the Terra satellite passed over eastern Russia, allowing the Moderate Resolution Imaging Spectroradiometer (MODIS) flying aboard to capture <span class="hlt">volcanic</span> <span class="hlt">activity</span> at Shiveluch and Plosky Tolbachik, on the Kamchatka Peninsula, in eastern Russia. This image was captured at 0050 UTC. Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1256/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1256/"><span>Compilation of Disruptions to Airports by <span class="hlt">Volcanic</span> <span class="hlt">Activity</span> (Version 1.0, 1944-2006)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Guffanti, Marianne; Mayberry, Gari C.; Casadevall, Thomas J.; Wunderman, Richard</p> <p>2008-01-01</p> <p><span class="hlt">Volcanic</span> <span class="hlt">activity</span> has caused significant hazards to numerous airports worldwide, with local to far-ranging effects on travelers and commerce. To more fully characterize the nature and scope of <span class="hlt">volcanic</span> hazards to airports, we collected data on incidents of airports throughout the world that have been affected by <span class="hlt">volcanic</span> <span class="hlt">activity</span>, beginning in 1944 with the first documented instance of damage to modern aircraft and facilities in Naples, Italy, and extending through 2006. Information was gleaned from various sources, including news outlets, volcanological reports (particularly the Smithsonian Institution's Bulletin of the Global <span class="hlt">Volcanism</span> Network), and previous publications on the topic. This report presents the full compilation of the data collected. For each incident, information about the affected airport and the <span class="hlt">volcanic</span> source has been compiled as a record in a Microsoft Access database. The database is incomplete in so far as incidents may not have not been reported or documented, but it does present a good sample from diverse parts of the world. Not included are en-route diversions to avoid airborne ash clouds at cruise altitudes. The database has been converted to a Microsoft Excel spreadsheet. To make the PDF version of table 1 in this open-file report resemble the spreadsheet, order the PDF pages as 12, 17, 22; 13, 18, 23; 14, 19, 24; 15, 20, 25; and 16, 21, 26. Analysis of the database reveals that, at a minimum, 101 airports in 28 countries were impacted on 171 occasions from 1944 through 2006 by eruptions at 46 volcanoes. The number of affected airports (101) probably is better constrained than the number of incidents (171) because recurring disruptions at a given airport may have been lumped together or not reported by news agencies, whereas the initial disruption likely is noticed and reported and thus the airport correctly counted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810971L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810971L"><span>Integrating science and education during an international, multi-parametric investigation of <span class="hlt">volcanic</span> <span class="hlt">activity</span> at Santiaguito volcano, Guatemala</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lavallée, Yan; Johnson, Jeffrey; Andrews, Benjamin; Wolf, Rudiger; Rose, William; Chigna, Gustavo; Pineda, Armand</p> <p>2016-04-01</p> <p>In January 2016, we held the first scientific/educational Workshops on Volcanoes (WoV). The workshop took place at Santiaguito volcano - the most <span class="hlt">active</span> volcano in Guatemala. 69 international scientists of all ages participated in this intensive, multi-parametric investigation of the <span class="hlt">volcanic</span> <span class="hlt">activity</span>, which included the deployment of seismometers, tiltmeters, infrasound microphones and mini-DOAS as well as optical, thermographic, UV and FTIR cameras around the <span class="hlt">active</span> vent. These instruments recorded <span class="hlt">volcanic</span> <span class="hlt">activity</span> in concert over a period of 3 to 9 days. Here we review the research <span class="hlt">activities</span> and present some of the spectacular observations made through this interdisciplinary efforts. Observations range from high-resolution drone and IR footage of explosions, monitoring of rock falls and quantification of the erupted mass of different gases and ash, as well as morphological changes in the dome caused by recurring explosions (amongst many other <span class="hlt">volcanic</span> processes). We will discuss the success of such integrative ventures in furthering science frontiers and developing the next generation of geoscientists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4989K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4989K"><span><span class="hlt">Volcanic</span> sulfur dioxide index and <span class="hlt">volcanic</span> explosivity index inferred from eruptive volume of volcanoes in Jeju Island, Korea: application to <span class="hlt">volcanic</span> hazard mitigation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ko, Bokyun; Yun, Sung-Hyo</p> <p>2016-04-01</p> <p>Jeju Island located in the southwestern part of Korea Peninsula is a <span class="hlt">volcanic</span> island composed of lavaflows, pyroclasts, and around 450 monogenetic volcanoes. The <span class="hlt">volcanic</span> <span class="hlt">activity</span> of the island commenced with phreatomagmatic eruptions under subaqueous condition ca. 1.8-2.0 Ma and lasted until ca. 1,000 year BP. For evaluating <span class="hlt">volcanic</span> <span class="hlt">activity</span> of the most recently erupted volcanoes with reported age, <span class="hlt">volcanic</span> explosivity index (VEI) and <span class="hlt">volcanic</span> sulfur dioxide index (VSI) of three volcanoes (Ilchulbong tuff cone, Songaksan tuff ring, and Biyangdo scoria cone) are inferred from their eruptive volumes. The quantity of eruptive materials such as tuff, lavaflow, scoria, and so on, is calculated using a model developed in Auckland <span class="hlt">Volcanic</span> Field which has similar <span class="hlt">volcanic</span> setting to the island. The eruptive volumes of them are 11,911,534 m3, 24,987,557 m3, and 9,652,025 m3, which correspond to VEI of 3, 3, and 2, respectively. According to the correlation between VEI and VSI, the average quantity of SO2 emission during an eruption with VEI of 3 is 2-8 × 103 kiloton considering that the island was formed under intraplate tectonic setting. Jeju Island was regarded as an extinct volcano, however, several studies have recently reported some <span class="hlt">volcanic</span> eruption ages within 10,000 year BP owing to the development in age dating technique. Thus, the island is a dormant volcano potentially implying high probability to erupt again in the future. The volcanoes might have explosive eruptions (vulcanian to plinian) with the possibility that SO2 emitted by the eruption reaches stratosphere causing climate change due to backscattering incoming solar radiation, increase in cloud reflectivity, etc. Consequently, recommencement of <span class="hlt">volcanic</span> eruption in the island is able to result in serious <span class="hlt">volcanic</span> hazard and this study provides fundamental and important data for <span class="hlt">volcanic</span> hazard mitigation of East Asia as well as the island. ACKNOWLEDGMENTS: This research was supported by a grant [MPSS</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175410','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175410"><span>Three-dimensional electrical resistivity model of the <span class="hlt">hydrothermal</span> system in Long Valley Caldera, California, from magnetotellurics</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Peacock, Jared R.; Mangan, Margaret T.; McPhee, Darcy K.; Wannamaker, Phil E.</p> <p>2016-01-01</p> <p>Though shallow flow of <span class="hlt">hydrothermal</span> fluids in Long Valley Caldera, California, has been well studied, neither the <span class="hlt">hydrothermal</span> source reservoir nor heat source has been well characterized. Here a grid of magnetotelluric data were collected around the Long Valley <span class="hlt">volcanic</span> system and modeled in 3-D. The preferred electrical resistivity model suggests that the source reservoir is a narrow east-west elongated body 4 km below the west moat. The heat source could be a zone of 2–5% partial melt 8 km below Deer Mountain. Additionally, a collection of hypersaline fluids, not connected to the shallow <span class="hlt">hydrothermal</span> system, is found 3 km below the medial graben, which could originate from a zone of 5–10% partial melt 8 km below the south moat. Below Mammoth Mountain is a 3 km thick isolated body containing fluids and gases originating from an 8 km deep zone of 5–10% basaltic partial melt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.B13A0172B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.B13A0172B"><span><span class="hlt">Hydrothermal</span> Mineral Deposits From a Young (0.1Ma) Abyssal Hill on the Flank of the Fast-Spreading East Pacific Rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benjamin, S. B.; Haymon, R. M.</p> <p>2004-12-01</p> <p>It has been estimated from heat flow measurements that at least 40% of the total <span class="hlt">hydrothermal</span> heat lost from oceanic lithosphere is removed from 0.1-5 Ma abyssal hill terrain on mid-ocean ridge flanks. Despite the large magnitude of estimated <span class="hlt">hydrothermal</span> heat loss from young abyssal hills, little is known about characteristics of <span class="hlt">hydrothermal</span> vents and mineral deposits in this setting. This study describes the first abyssal hill <span class="hlt">hydrothermal</span> samples to be collected on the flank of a fast-spreading ridge. The mineral deposits were discovered at "Tevnia Site" on the axis-facing fault scarp of an abyssal hill, located on ˜0.1 Ma lithosphere ˜5 km east of the East Pacific Rise (EPR) axis at 10\\deg 20'N. Observations of Galatheid crabs, "dandelion" siphonophores, and colonies of dead, yet still intact, Tevnia worm tubes at this site during Alvin dives in 1994 suggests relatively recent <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. The deposits are friable <span class="hlt">hydrothermal</span> precipitates incorporating <span class="hlt">volcanic</span> clasts brecciated at both the micro and macro scales. The petrographic sequence of brecciation, alteration, and cementation exhibited by the samples suggests that they formed from many pulses of <span class="hlt">hydrothermal</span> venting interspersed with, and perhaps triggered by, repeated tectonic events as the abyssal hill was uplifted and moved off-axis (see also Haymon et al., this session). Observed minerals include x-ray amorphous opaline silica and Fe-oxide phases, crystalline Mn-oxides (birnessite and todorokite), an irregularly stratified mixed layer nontronite-celadonite, and residual calcite in sediment-derived microfossils incorporated into the breccia matrix. This mineral assemblage suggests that the deposits precipitated from moderately low-temperature (<140\\deg C) fluids, enriched in K, Fe, Si, and Mn, with a near-neutral pH. The presence of tubeworm casings at the site is evidence that the <span class="hlt">hydrothermal</span> fluids carried H2S, however no metal sulfide phases were identified in the samples. Although</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27794445','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27794445"><span>Heavy metals in the <span class="hlt">volcanic</span> environment and thyroid cancer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vigneri, R; Malandrino, P; Gianì, F; Russo, M; Vigneri, P</p> <p>2017-12-05</p> <p>In the last two decades thyroid cancer incidence has increased worldwide more than any other cancer. Overdiagnosis of subclinical microcarcinomas has certainly contributed to this increase but many evidences indicate that a true increase, possibly due to environmental factors, has also occurred. Thyroid cancer incidence is markedly increased in <span class="hlt">volcanic</span> areas. Thus, the <span class="hlt">volcanic</span> environment is a good model to investigate the possible factors favoring thyroid cancer. In the <span class="hlt">volcanic</span> area of Mt. Etna in Sicily, as well as in other <span class="hlt">volcanic</span> areas, a <span class="hlt">non</span>-anthropogenic pollution with heavy metals has been documented, a consequence of gas, ash and lava emission. Soil, water and atmosphere contamination, via the food chain, biocontaminate the residents as documented by high levels in the urines and the scalp hair compared to individuals living in adjacent <span class="hlt">non-volcanic</span> areas. Trace amounts of metals are essential nutrients but, at higher concentrations, can be toxic for living cells. Metals can behave both as endocrine disruptors, perturbing the hormonal system, and as carcinogens, promoting malignant transformation. Similarly to other carcinogens, the transforming effect of heavy metals is higher in developing organisms as the fetus (contaminated via the mother) and individuals in early childhood. In the last decades environment metal pollution has greatly increased in industrialized countries. Although still within the "normal" limits for each single metal the hormesis effect (heavy metal <span class="hlt">activity</span> at very low concentration because of biphasic, <span class="hlt">non</span> linear cell response) and the possible potentiation effect resulting from the mixture of different metals acting synergistically can explain cell damage at very low concentrations. The effect of metals on the human thyroid is poorly studied: for some heavy metals no data are available. The scarce studies that have been performed mainly focus on metal effect as thyroid endocrine disruptors. The metal concentration in tissues has</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016742','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016742"><span>Geology and geochemistry of Summitville, Colorado: an epithermal acid sulfate deposit in a <span class="hlt">volcanic</span> dome</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, J.E.; Coolbaugh, M.F.</p> <p>1994-01-01</p> <p>Geologic studies during recent open-pit mining at Summitville, Colorado, have provided new information on an epithermal acid sulfate Au-Ag-Cu deposit formed in a <span class="hlt">volcanic</span> dome. Geologic mapping, geochemical studies of whole-rock samples from blast holes, and geologic and geochemical traverse studies refine the details of the evolution of the Summitville deposit. Six distinct events followed emplacement of the quartz latite <span class="hlt">volcanic</span> dome and define the development of the Summitville deposit: 1) an early stage of acid sulfate alteration, 2) subsequent Cu sulfide and gold mineralization, 3) widespread <span class="hlt">hydrothermal</span> brecciation, 4) volumetrically minor, base metal sulfide-bearing barite veining, 5) volumetrically minor, kaolinite matrix brecciation, and finally, 6) supergene oxidation. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V34A..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V34A..04C"><span>A seismological perspective of the shallow magma and <span class="hlt">hydrothermal</span> systems under Kilauea Caldera</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chouet, B. A.; Dawson, P. B.</p> <p>2011-12-01</p> <p>The past 20 years have seen great strides in our understanding of Kilauea Volcano, in large part due to technological developments and improvements in seismological instrumentation, which now allow the surface effects of subterranean <span class="hlt">volcanic</span> processes to be imaged in unprecedented detail. High-resolution tomography provided an image of 3D velocity anomalies down to a scale of a few hundred meters, providing indirect evidence for the presence of reservoirs under the summit region of Kilauea. A sharper image of a shallow <span class="hlt">hydrothermal</span> reservoir under Kilauea Caldera was obtained from frequency-slowness analyses of long-period (LP) seismicity recorded on three small-aperture seismic antennas deployed in the summit caldera. Located within the top 500 m below the caldera floor and extending ~0.6 km and ~1 km in the east-west and north-south directions, this <span class="hlt">hydrothermal</span> reservoir broadly overlaps the east wall of the Halemaumau pit crater. Further evidence of <span class="hlt">hydrothermal</span> processes within this zone was obtained from a study of a well-recorded LP event, indicating a source mechanism consistent with the resonance of a horizontal steam-filled crack at a depth of ~150 m near the eastern rim of Halemaumau. Recurring very-long-period (VLP) signals originating in the repeated <span class="hlt">activation</span> of a compact source region near sea level immediately beneath this <span class="hlt">hydrothermal</span> reservoir have allowed a gradually emerging view of the shallowest segment of the magma transport pathway under the caldera. Further elaboration of our image of the magma pathway structure, made possible through detailed modeling of VLP signals accompanying degassing <span class="hlt">activity</span> at a new vent formed in Halemaumau in March 2008, points to a dominant dike segment in the form of a nearly vertical east-trending dike. The inferred dike features a ~20° clockwise rotation in strike under the east edge of Halemaumau, where it intersects a sub-vertical north-striking dike. The triple junction made by the intersection of the</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://www.osti.gov/sciencecinema/biblio/1025989','SCIGOVIMAGE-SCICINEMA'); return false;" href="http://www.osti.gov/sciencecinema/biblio/1025989"><span>Modeling <span class="hlt">volcanic</span> ash dispersal</span></a></p> <p><a target="_blank" href="http://www.osti.gov/sciencecinema/">ScienceCinema</a></p> <p>Macedonio, Giovanni</p> <p>2018-05-22</p> <p>Explosive <span class="hlt">volcanic</span> eruptions inject into the atmosphere large amounts of <span class="hlt">volcanic</span> material (ash, blocks and lapilli). Blocks and larger lapilli follow ballistic and <span class="hlt">non</span>-ballistic trajectories and fall rapidly close to the volcano. In contrast, very fine ashes can remain entrapped in the atmosphere for months to years, and may affect the global climate in the case of large eruptions. Particles having sizes between these two end-members remain airborne from hours to days and can cover wide areas downwind. Such <span class="hlt">volcanic</span> fallout entails a serious threat to aircraft safety and can create many undesirable effects to the communities located around the volcano. The assessment of <span class="hlt">volcanic</span> fallout hazard is an important scientific, economic, and political issue, especially in densely populated areas. From a scientific point of view, considerable progress has been made during the last two decades through the use of increasingly powerful computational models and capabilities. Nowadays, models are used to quantify hazard scenarios and/or to give short-term forecasts during emergency situations. This talk will be focused on the main aspects related to modeling <span class="hlt">volcanic</span> ash dispersal and fallout with application to the well known problem created by the Eyjafjöll volcano in Iceland. Moreover, a short description of the main <span class="hlt">volcanic</span> monitoring techniques is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025839','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025839"><span>Exploration and discovery in Yellowstone Lake: Results from high-resolution sonar imaging, seismic reflection profiling, and submersible studies</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Morgan, L.A.; Shanks, Wayne C.; Lovalvo, D.A.; Johnson, S.Y.; Stephenson, W.J.; Pierce, K.L.; Harlan, S.S.; Finn, C.A.; Lee, G.; Webring, M.; Schulze, B.; Duhn, J.; Sweeney, R.; Balistrieri, L.</p> <p>2003-01-01</p> <p>Discoveries from multi-beam sonar mapping and seismic reflection surveys of the northern, central, and West Thumb basins of Yellowstone Lake provide new insight into the extent of post-collapse <span class="hlt">volcanism</span> and <span class="hlt">active</span> <span class="hlt">hydrothermal</span> processes occurring in a large lake environment above a large magma chamber. Yellowstone Lake has an irregular bottom covered with dozens of features directly related to <span class="hlt">hydrothermal</span>, tectonic, <span class="hlt">volcanic</span>, and sedimentary processes. Detailed bathymetric, seismic reflection, and magnetic evidence reveals that rhyolitic lava flows underlie much of Yellowstone Lake and exert fundamental control on lake bathymetry and localization of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Many previously unknown features have been identified and include over 250 <span class="hlt">hydrothermal</span> vents, several very large (>500 m diameter) <span class="hlt">hydrothermal</span> explosion craters, many small <span class="hlt">hydrothermal</span> vent craters (???1-200 m diameter), domed lacustrine sediments related to <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>, elongate fissures cutting post-glacial sediments, siliceous <span class="hlt">hydrothermal</span> spire structures, sublacustrine landslide deposits, submerged former shorelines, and a recently <span class="hlt">active</span> graben. Sampling and observations with a submersible remotely operated vehicle confirm and extend our understanding of the identified features. Faults, fissures, <span class="hlt">hydrothermally</span> inflated domal structures, <span class="hlt">hydrothermal</span> explosion craters, and sublacustrine landslides constitute potentially significant geologic hazards. Toxic elements derived from <span class="hlt">hydrothermal</span> processes also may significantly affect the Yellowstone ecosystem. Published by Elsevier Science B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4757712','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4757712"><span>The Guaymas Basin Hiking Guide to <span class="hlt">Hydrothermal</span> Mounds, Chimneys, and Microbial Mats: Complex Seafloor Expressions of Subsurface <span class="hlt">Hydrothermal</span> Circulation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Teske, Andreas; de Beer, Dirk; McKay, Luke J.; Tivey, Margaret K.; Biddle, Jennifer F.; Hoer, Daniel; Lloyd, Karen G.; Lever, Mark A.; Røy, Hans; Albert, Daniel B.; Mendlovitz, Howard P.; MacGregor, Barbara J.</p> <p>2016-01-01</p> <p>The <span class="hlt">hydrothermal</span> mats, mounds, and chimneys of the southern Guaymas Basin are the surface expression of complex subsurface <span class="hlt">hydrothermal</span> circulation patterns. In this overview, we document the most frequently visited features of this <span class="hlt">hydrothermal</span> area with photographs, temperature measurements, and selected geochemical data; many of these distinct habitats await characterization of their microbial communities and <span class="hlt">activities</span>. Microprofiler deployments on microbial mats and <span class="hlt">hydrothermal</span> sediments show their steep geochemical and thermal gradients at millimeter-scale vertical resolution. Mapping these <span class="hlt">hydrothermal</span> features and sampling locations within the southern Guaymas Basin suggest linkages to underlying shallow sills and heat flow gradients. Recognizing the inherent spatial limitations of much current Guaymas Basin sampling calls for comprehensive surveys of the wider spreading region. PMID:26925032</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29067531','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29067531"><span>Microbial community differentiation between <span class="hlt">active</span> and inactive sulfide chimneys of the Kolumbo submarine volcano, Hellenic <span class="hlt">Volcanic</span> Arc.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Christakis, Christos A; Polymenakou, Paraskevi N; Mandalakis, Manolis; Nomikou, Paraskevi; Kristoffersen, Jon Bent; Lampridou, Danai; Kotoulas, Georgios; Magoulas, Antonios</p> <p>2018-01-01</p> <p>Over the last decades, there has been growing interest about the ecological role of <span class="hlt">hydrothermal</span> sulfide chimneys, their microbial diversity and associated biotechnological potential. Here, we performed dual-index Illumina sequencing of bacterial and archaeal communities on <span class="hlt">active</span> and inactive sulfide chimneys collected from the Kolumbo <span class="hlt">hydrothermal</span> field, situated on a geodynamic convergent setting. A total of 15,701 OTUs (operational taxonomic units) were assigned to 56 bacterial and 3 archaeal phyla, 133 bacterial and 16 archaeal classes. <span class="hlt">Active</span> chimney communities were dominated by OTUs related to thermophilic members of Epsilonproteobacteria, Aquificae and Deltaproteobacteria. Inactive chimney communities were dominated by an OTU closely related to the archaeon Nitrosopumilus sp., and by members of Gammaproteobacteria, Deltaproteobacteria, Planctomycetes and Bacteroidetes. These lineages are closely related to phylotypes typically involved in iron, sulfur, nitrogen, hydrogen and methane cycling. Overall, the inactive sulfide chimneys presented highly diverse and uniform microbial communities, in contrast to the <span class="hlt">active</span> chimney communities, which were dominated by chemolithoautotrophic and thermophilic lineages. This study represents one of the most comprehensive investigations of microbial diversity in submarine chimneys and elucidates how the dissipation of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> affects the structure of microbial consortia in these extreme ecological niches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189999','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189999"><span>Oxygen and U-Th isotopes and the timescales of <span class="hlt">hydrothermal</span> exchange and melting in granitoid wall rocks at Mount Mazama, Crater Lake, Oregon</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ankney, Meagan E.; Bacon, Charles R.; Valley, John W.; Beard, Brian L.; Johnson, Clark M.</p> <p>2017-01-01</p> <p>We report new whole rock U-Th and in-situ oxygen isotope compositions for partially melted (0–50 vol% melt), low-δ18O Pleistocene granitoid blocks ejected during the ∼7.7 ka caldera-forming eruption of Mt. Mazama (Crater Lake, Oregon). The blocks are interpreted to represent wall rocks of the climactic magma chamber that, prior to eruption, experienced variable amounts of exchange with meteoric <span class="hlt">hydrothermal</span> fluids and subsequent partial melting. U-Th and oxygen isotope results allow us to examine the timescales of <span class="hlt">hydrothermal</span> circulation and partial melting, and provide an “outside in” perspective on the buildup to the climactic eruption of Mt. Mazama. Oxygen isotope compositions measured in the cores and rims of individual quartz (n = 126) and plagioclase (n = 91) crystals, and for transects across ten quartz crystals, document zonation in quartz (Δ18OCore-Rim ≤ 0.1–5.5‰), but show homogeneity in plagioclase (Δ18OCore-Rim ≤ ±0.8‰). We propose that oxygen isotope zonation in quartz records <span class="hlt">hydrothermal</span> exchange followed by high-temperature exchange in response to partial melting caused by injection of basaltic to andesitic recharge magma into the deeper portions of the chamber. Results of modeling of oxygen diffusion in quartz indicates that <span class="hlt">hydrothermal</span> exchange in quartz occurred over a period of ∼1000–63,000 years. Models also suggest that the onset of melting of the granitoids occurred a minimum of ∼10–200 years prior to the Mazama climactic eruption, an inference which is broadly consistent with results for magnetite homogenization and for Zr diffusion in melt previously reported by others.Uranium-thorium isotope compositions of most granitoid blocks are in 238U excess, and are in agreement with a 238U enriched array previously measured for <span class="hlt">volcanic</span> rocks at Mt. Mazama. Uranium excess in the granitoids is likely due to enrichment via <span class="hlt">hydrothermal</span> circulation, given their low δ18O values. The sample with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T21F..05H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T21F..05H"><span>Discovery of <span class="hlt">hydrothermally</span> <span class="hlt">active</span> and extinct talc mounds on the Mid-Cayman Rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodgkinson, M.; Murton, B. J.; Roberts, S.</p> <p>2013-12-01</p> <p>Since 1977, <span class="hlt">hydrothermal</span> vents have been the subject of intense scientific interest due to their role in cooling the oceanic crust and global geochemical cycles. Until now, two types of <span class="hlt">hydrothermal</span> system have been identified: one, driven by magmatic heat extruding ';black smoker' fluids; and another, involving serpentinisation of ultramafic rocks and the precipitation of carbonate/brucite chimneys. Here, we present details of a new, off-axis type of <span class="hlt">hydrothermal</span> system consisting of mounds of predominately botryoidal talc (a magnesium-silicate) with accessory silica and copper sulphides, and chimneys exhaling fluids of moderate temperature and pH. Discovered on the Mid-Cayman Rise (MCR) in 2010, the Von Damm Vent Field (VDVF) features a NNW-ESE-trending line of four overlapping cones, the largest of which is 75 m high by 150 m in diameter. The VDVF is hosted in the gabbroic footwall of the Mount Dent Oceanic Core Complex (MDOCC), which includes serpentinised peridotite at depth. The largest cone vents clear fluids from two main orifices at its summit, with primary temperatures of 215°C. Elsewhere, both focussed and diffuse flow areas emit fluids with temperatures of up to 150°C. The surrounding ~1 m thick pelagic sediment contains abundant pockmarks that emit methane-rich fluids at temperatures of less than 10°C. During the return to the MCR in early 2013, several other talc mounds were discovered within a kilometre of the <span class="hlt">active</span> VDVF. These inactive mounds also comprise an assemblage of botryoidal talc, silica, disseminated sulphides (including chalcopyrite) and sulphates. One of these mounds (Mystic Mount) is double the volume of the <span class="hlt">active</span> VDVF. The unique dominance of talc as the major mineral forming the <span class="hlt">hydrothermal</span> structures indicates unusual vent fluid compositions that are able to carry both copper (at high-temperatures) and precipitate magnesium silicate. Thermodynamic modelling indicates that talc precipitates on mixing a moderately acidic, silica</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BVol...77...53D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BVol...77...53D"><span>Xenopumice erupted on 15 October 2011 offshore of El Hierro (Canary Islands): a subvolcanic snapshot of magmatic, <span class="hlt">hydrothermal</span> and pyrometamorphic processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Del Moro, S.; Di Roberto, A.; Meletlidis, S.; Pompilio, M.; Bertagnini, A.; Agostini, S.; Ridolfi, F.; Renzulli, A.</p> <p>2015-06-01</p> <p>On 15 October 2011, a submarine eruption offshore of El Hierro Island gave rise to floating <span class="hlt">volcanic</span> products, known as xenopumices, i.e., pumiceous xenoliths partly mingled and coated with the juvenile basanitic magma. Over the last few years, no consensus in the scientific community in explaining the origin of these products has been reached. In order to better understand the formation of xenopumice, we present a textural, mineralogical, and geochemical study of the possible magmatic, <span class="hlt">hydrothermal</span>, and pyrometamorphic processes, which usually operate in the plumbing systems of <span class="hlt">active</span> volcanoes. We carried out a comprehensive SEM investigation and Sr-Nd-Pb isotope analyses on some samples representative of three different xenopumice facies. All the data were compared with previous studies, new data for El Hierro extrusives and a literature dataset of Canary Islands igneous and sedimentary rocks. In the investigated xenopumices, we emphasize the presence of restitic magmatic phases as well as crystallization of minerals (mainly olivine + pyroxene + magnetite aggregates) as pseudomorphs after pre-existing mafic phenocrysts, providing evidence of pyrometamorphism induced by the high-T juvenile basanitic magma. In addition, we identify veins consisting of zircon + REE-oxides + mullite associated with Si-rich glass and <span class="hlt">hydrothermal</span> quartz, which indicate the fundamental role played by <span class="hlt">hydrothermal</span> fluid circulation in the xenopumice protolith. The petrological data agree with a pre-syneruptive formation of the xenopumice, when El Hierro basanite magma intruded <span class="hlt">hydrothermally</span> altered trachyandesite to trachyte rocks and triggered local partial melting. Therefore, the El Hierro xenopumice represents a snapshot of the transient processes at the magma-wall rock interface, which normally occurs in the feeding system of <span class="hlt">active</span> volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoRL..39.4304I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoRL..39.4304I"><span>Monitoring <span class="hlt">volcanic</span> <span class="hlt">activity</span> using correlation patterns between infrasound and ground motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ichihara, M.; Takeo, M.; Yokoo, A.; Oikawa, J.; Ohminato, T.</p> <p>2012-02-01</p> <p>This paper presents a simple method to distinguish infrasonic signals from wind noise using a cross-correlation function of signals from a microphone and a collocated seismometer. The method makes use of a particular feature of the cross-correlation function of vertical ground motion generated by infrasound, and the infrasound itself. Contribution of wind noise to the correlation function is effectively suppressed by separating the microphone and the seismometer by several meters because the correlation length of wind noise is much shorter than wavelengths of infrasound. The method is applied to data from two recent eruptions of Asama and Shinmoe-dake volcanoes, Japan, and demonstrates that the method effectively detects not only the main eruptions, but also minor <span class="hlt">activity</span> generating weak infrasound hardly visible in the wave traces. In addition, the correlation function gives more information about <span class="hlt">volcanic</span> <span class="hlt">activity</span> than infrasound alone, because it reflects both features of incident infrasonic and seismic waves. Therefore, a graphical presentation of temporal variation in the cross-correlation function enables one to see qualitative changes of eruptive <span class="hlt">activity</span> at a glance. This method is particularly useful when available sensors are limited, and will extend the utility of a single microphone and seismometer in monitoring <span class="hlt">volcanic</span> <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS31C1418K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS31C1418K"><span>Water column imaging on <span class="hlt">hydrothermal</span> vent in Central Indian Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koh, J.; Park, Y.</p> <p>2017-12-01</p> <p>Water column imaging with Multibeam echosounder systems (MBES) is recently becoming of increasing interest for oceanographic studies. Especially gas bubbles and hot water exposed from <span class="hlt">hydrothermal</span> vents make acoustic impedance anomalies in cold seawater, water column imaging is very useful for the researchers who want to detect some kinds of <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. We conducted a <span class="hlt">hydrothermal</span> exploration program, called "INVENT17", using the MBES system, KONGBERG EM122 (12kHz, 1°×1°), mounted on R/V ISABU and we deployed other equipments including video guided hydraulic grab, tow-yo CTD and general CTD with MAPR (Miniature Autonomous Plume Recorder) in 2017. First, to evaluate its capabilities of detection of <span class="hlt">hydrothermal</span> vent, the surveys using the MBES were conducted at the Solitaire Field, previously identified <span class="hlt">hydrothermal</span> area of the Central Indian Ridge. The bathymetric data obtained from MBES provided information about detailed morphology of seafloor, but we were not able to achieve the information from the water column imaging data. But the clue of existence of <span class="hlt">active</span> <span class="hlt">hydrothermal</span> vent was detected through the values of ΔNTU, dEh/dt, and OPR gained from MAPR, the data means that the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> affects 100m from the seafloor. It could be the reason that we can't find the <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> because the range resolution of water column imaging is pretty rough so that the size of 100m-scaled <span class="hlt">activity</span> has low possibility to distinguish from seafloor. The other reason is there are no sufficient objects to cause strong scattering like as CO2 bubbles or droplets unlike in the mid-Okinawa Trough. And this suggests that can be a important standard to identify properties of <span class="hlt">hydrothermal</span> vent sites depending on the presence of scattering objects in water mass. To justify this, we should perform more chemical analysis of hot water emanating from <span class="hlt">hydrothermal</span> vent and collected several bottles of water sample to do that.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1212333M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1212333M"><span>First Evidence of Epithermal Gold Occurrences in the SE Afar Rift, Republic of Djibouti</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moussa, Nima; Fouquet, Yves; Caminiti, Antoine Marie; Le Gall, Bernard; Rolet, Joel; Bohn, Marcel; Etoubleau, Joel; Delacourt, Christophe; Jalludin, Mohamed</p> <p>2010-05-01</p> <p>The Republic of Djibouti, located at the SE part of the Afar <span class="hlt">volcanic</span> Triangle, is characterized by intense tectonic and bimodal <span class="hlt">volcanic</span> <span class="hlt">activity</span>, and is emplaced over an earlier magmatic rift system, as old as 25-30 Ma. Each magmatic event is accompanied by <span class="hlt">hydrothermal</span> <span class="hlt">activity</span>. Few works have been so far published on <span class="hlt">hydrothermal</span> mineralization in the Afar area. Mineralization generally occur as veins and are mainly associated with acidic <span class="hlt">volcanic</span> intrusions along the fractures at the edges of grabens established during the last 4 Ma. Eighty samples from <span class="hlt">hydrothermal</span> quartz ± carbonate veins and breccias were studied on 9 different sites representative of 4 main <span class="hlt">volcanic</span> events ranging in age from early Miocene up to Present. Gold was found in excess of 200 ppb in 30% of the samples. Mineralogical analyses based on optical reflected light microscopy, X-Ray diffractometry, X-Ray fluorescence, inductively coupled plasma mass spectroscopy and electron microprobe, led us to identify two types of gold mineralization (i) native gold, electrum, hessite and sulfides (chalcopyrite, pyrite, bornite, ± sphalerite, and galena) in massive quartz breccias and banded chalcedony, (ii) gold, electrum, hematite, magnetite, trace minerals (argentite) and adularia in banded chalcedony. Another group without gold is characterized by quartz, pyrite ± goethite. Secondary minerals are characterized by goethite, native silver and native copper. Arsenic is enriched in pyrite in samples with a high gold content. The bimodal <span class="hlt">volcanism</span>, the occurrence of adularia, the native gold and electrum in banded silica veins, are classically observed in neutral epithermal systems. The discovery of this type of mineralization in a recent-<span class="hlt">active</span> continental rift system supplies new insights about <span class="hlt">hydrothermal</span> processes associated with <span class="hlt">volcanic</span> <span class="hlt">activity</span> in a spreading context. Keywords: Republic of Djibouti, Afar Triangle, <span class="hlt">Hydrothermal</span>, Epithermal system, Gold</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023052','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023052"><span>Time-variation of <span class="hlt">hydrothermal</span> discharge at selected sites in the Western United States: Implications for monitoring</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ingebritsen, S.E.; Galloway, D.L.; Colvard, E.M.; Sorey, M.L.; Mariner, R.H.</p> <p>2001-01-01</p> <p>We compiled time series of <span class="hlt">hydrothermal</span> discharge consisting of 3593 chloride- or heat-flux measurements from 24 sites in the Yellowstone region, the northern Oregon Cascades, Lassen <span class="hlt">Volcanic</span> National Park and vicinity, and Long Valley, California. At all of these sites the <span class="hlt">hydrothermal</span> phenomena are believed to be as yet unaffected by human <span class="hlt">activity</span>, though much of the data collection was driven by mandates to collect environmental-baseline data in acticipation of geothermal development. The time series average 19 years in length and some of the Yellowstone sites have been monitored intermittently for over 30 years. Many sites show strong seasonality but few show clear long-term trends, and at most sites statistically significant decadal-scale trends are absent. Thus, the data provide robust estimates of advective heat flow ranging from ~130 MW in the north-central Oregon Cascades to ~6100 MW in the Yellowstone region, and also document Yellowstone <span class="hlt">hydrothermal</span> chloride and arsenic fluxes of 1740 and 15-20 g/s, respectively. The discharge time series show little sensitivity to regional tectonic events such as earthquakes or inflation/deflation cycles. Most long-term monitoring to date has focused on high-chloride springs and low-temperature fumaroles. The relative stability of these features suggests that discharge measurements done as part of volcano-monitoring programs should focus instead on high-temperature fumaroles, which may be more immediately linked to the magmatic heat source. ?? 2001 Elsevier Science B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003GGG.....4.1089K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003GGG.....4.1089K"><span>Short-lived and discontinuous intraplate <span class="hlt">volcanism</span> in the South Pacific: Hot spots or extensional <span class="hlt">volcanism</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koppers, Anthony A. P.; Staudigel, Hubert; Pringle, Malcolm S.; Wijbrans, Jan R.</p> <p>2003-10-01</p> <p>South Pacific intraplate volcanoes have been <span class="hlt">active</span> since the Early Cretaceous. Their HIMU-EMI-EMII mantle sources can be traced back into the West Pacific Seamount Province (WPSP) using plate tectonic reconstructions, implying that these distinctive components are enduring features within the Earth's mantle for, at least, the last 120 Myr. These correlations are eminent on the scale of the WPSP and the South Pacific Thermal and Isotopic Anomaly (SOPITA), but the evolution of single hot spots emerges notably more complicated. Hot spots in the WPSP and SOPITA mantle regions typically display intermittent <span class="hlt">volcanic</span> <span class="hlt">activity</span>, longevities shorter than 40 Myr, superposition of hot spot <span class="hlt">volcanism</span>, and motion relative to other hot spots. In this review, we use 40Ar/39Ar seamount ages and Sr-Nd-Pb isotopic signatures to map out Cretaceous <span class="hlt">volcanism</span> in the WPSP and to characterize its evolution with respect to the currently <span class="hlt">active</span> hot spots in the SOPITA region. Our plate tectonic reconstructions indicate cessation of <span class="hlt">volcanism</span> during the Cretaceous for the Typhoon and Japanese hot spots; whereas the currently <span class="hlt">active</span> Samoan, Society, Pitcairn and Marquesas hot spots lack long-lived counterparts in the WPSP. These hot spots may have become <span class="hlt">active</span> during the last 20 Myr only. The other WPSP seamount trails can be only "indirectly" reconciled with hot spots in the SOPITA region. Complex age distributions in the Magellan, Anewetak, Ralik and Ratak seamount trails would necessitate the superposition of multiple <span class="hlt">volcanic</span> trails generated by the Macdonald, Rurutu and Rarotonga hot spots during the Cretaceous; whereas HIMU-type seamounts in the Southern Wake seamount trail would require 350-500 km of hot spot motion over the last 100 Myr following its origination along the Mangaia-Rurutu "hotline" in the Cook-Austral Islands. These observations, however, violate all assumptions of the classical Wilson-Morgan hot spot hypothesis, indicating that long-lived, deep and fixed mantle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Litho.284..276M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Litho.284..276M"><span>Siderite deposits in northern Italy: Early Permian to Early Triassic <span class="hlt">hydrothermalism</span> in the Southern Alps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, Silvana; Toffolo, Luca; Moroni, Marilena; Montorfano, Carlo; Secco, Luciano; Agnini, Claudia; Nimis, Paolo; Tumiati, Simone</p> <p>2017-07-01</p> <p>We present a minero-petrographic, geochemical and geochronological study of siderite orebodies from different localities of the Southern Alps (northern Italy). Siderite occurs as veins cutting the Variscan basement and the overlying Lower Permian volcano-sedimentary cover (Collio Fm.), and as both veins and conformable stratabound orebodies in the Upper Permian (Verrucano Lombardo and Bellerophon Fms.) and Lower Triassic (Servino and Werfen Fms.) sedimentary sequences of the Lombardian and the Venetian Alps. All types of deposits show similar major- and rare-earth (REE)-element patterns, suggesting a common iron-mineralizing event. The compositions of coexisting siderite, Fe-rich dolomite and calcite suggest formation from <span class="hlt">hydrothermal</span> fluids at relatively high temperature conditions (≥ 250 °C). Geochemical modelling, supported by REE analyses and by literature and new δ13C and δ18O isotopic data, suggests that fluids responsible for the formation of siderite in the Variscan basement and in the overlying Lower Permian cover were derived from dominant fresh water, which leached Fe and C from <span class="hlt">volcanic</span> rocks (mainly rhyolites/rhyodacites) and organic carbon-bearing continental sediments. On the basis of U-Th-Pb microchemical dating of uraninite associated with siderite in the Val Vedello and Novazza deposits (Lombardian Alps), the onset of <span class="hlt">hydrothermalism</span> is constrained to 275 ± 13 Ma (Early-Mid Permian), i.e., it was virtually contemporaneous to the plutonism and the <span class="hlt">volcanic</span>-sedimentary cycle reported in the same area (Orobic Basin). The youngest iron-mineralizing event is represented by siderite veins and conformable orebodies hosted in Lower Triassic shallow-marine carbonatic successions. In this case, the siderite-forming fluids contained a seawater component, interacted with the underlying Permian successions and eventually replaced the marine carbonates at temperatures of ≥ 250 °C. The absence of siderite in younger rocks suggests an Early Triassic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EP%26S...70...68M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EP%26S...70...68M"><span>Chronology of the 2015 eruption of Hakone volcano, Japan: geological background, mechanism of <span class="hlt">volcanic</span> unrest and disaster mitigation measures during the crisis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mannen, Kazutaka; Yukutake, Yohei; Kikugawa, George; Harada, Masatake; Itadera, Kazuhiro; Takenaka, Jun</p> <p>2018-04-01</p> <p>The 2015 eruption of Hakone volcano was a very small phreatic eruption, with total erupted ash estimated to be in the order of only 102 m3 and ballistic blocks reaching less than 30 m from the vent. Precursors, however, had been recognized at least 2 months before the eruption and mitigation measures were taken by the local governments well in advance. In this paper, the course of precursors, the eruption and the post-eruptive <span class="hlt">volcanic</span> <span class="hlt">activity</span> are reviewed, and a preliminary model for the magma-<span class="hlt">hydrothermal</span> process that caused the unrest and eruption is proposed. Also, mitigation measures taken during the unrest and eruption are summarized and discussed. The first precursors observed were an inflation of the deep source and deep low-frequency earthquakes in early April 2015; an earthquake swarm then started in late April. On May 3, steam wells in Owakudani, the largest fumarolic area on the volcano, started to blowout. Seismicity reached its maximum in mid-May and gradually decreased; however, at 7:32 local time on June 29, a shallow open crack was formed just beneath Owakudani as inferred from sudden tilt change and InSAR analysis. The same day mud flows and/or debris flows likely started before 11:00 and ash emission began at about 12:30. The <span class="hlt">volcanic</span> unrest and the eruption of 2015 can be interpreted as a pressure increase in the <span class="hlt">hydrothermal</span> system, which was triggered by magma replenishment to a deep magma chamber. Such a pressure increase was also inferred from the 2001 unrest and other minor unrests of Hakone volcano during the twenty-first century. In fact, monitoring of repeated periods of unrest enabled alerting prior to the 2015 eruption. However, since open crack formation seems to occur haphazardly, eruption prediction remains impossible and evacuation in the early phase of <span class="hlt">volcanic</span> unrest is the only way to mitigate <span class="hlt">volcanic</span> hazard.[Figure not available: see fulltext.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190451','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190451"><span>Miocene magmatism in the Bodie Hills <span class="hlt">volcanic</span> field, California and Nevada: A long-lived eruptive center in the southern segment of the ancestral Cascades arc</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>John, David A.; du Bray, Edward A.; Blakely, Richard J.; Fleck, Robert J.; Vikre, Peter; Box, Stephen E.; Moring, Barry C.</p> <p>2012-01-01</p> <p>The Middle to Late Miocene Bodie Hills <span class="hlt">volcanic</span> field is a >700 km2, long-lived (∼9 Ma) but episodic eruptive center in the southern segment of the ancestral Cascades arc north of Mono Lake (California, U.S.). It consists of ∼20 major eruptive units, including 4 trachyandesite stratovolcanoes emplaced along the margins of the field, and numerous, more centrally located silicic trachyandesite to rhyolite flow dome complexes. Bodie Hills <span class="hlt">volcanism</span> was episodic with two peak periods of eruptive <span class="hlt">activity</span>: an early period ca. 14.7–12.9 Ma that mostly formed trachyandesite stratovolcanoes and a later period between ca. 9.2 and 8.0 Ma dominated by large trachyandesite-dacite dome fields. A final period of small silicic dome emplacement occurred ca. 6 Ma. Aeromagnetic and gravity data suggest that many of the Miocene volcanoes have shallow plutonic roots that extend to depths ≥1–2 km below the surface, and much of the Bodie Hills may be underlain by low-density plutons presumably related to Miocene <span class="hlt">volcanism</span>.Compositions of Bodie Hills <span class="hlt">volcanic</span> rocks vary from ∼50 to 78 wt% SiO2, although rocks with <55 wt% SiO2 are rare. They form a high-K calc-alkaline series with pronounced negative Ti-P-Nb-Ta anomalies and high Ba/Nb, Ba/Ta, and La/Nb typical of subduction-related continental margin arcs. Most Bodie Hills rocks are porphyritic, commonly containing 15–35 vol% phenocrysts of plagioclase, pyroxene, and hornblende ± biotite. The oldest eruptive units have the most mafic compositions, but <span class="hlt">volcanic</span> rocks oscillated between mafic and intermediate to felsic compositions through time. Following a 2 Ma hiatus in <span class="hlt">volcanism</span>, postsubduction rocks of the ca. 3.6–0.1 Ma, bimodal, high-K Aurora <span class="hlt">volcanic</span> field erupted unconformably onto rocks of the Miocene Bodie Hills <span class="hlt">volcanic</span> field.At the latitude of the Bodie Hills, subduction of the Farallon plate is inferred to have ended ca. 10 Ma, evolving to a transform plate margin. However, <span class="hlt">volcanism</span> in the region continued</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.T21A0443E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.T21A0443E"><span>Borehole Array Observations of <span class="hlt">Non-Volcanic</span> Tremor at SAFOD</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ellsworth, W. L.; Luetgert, J. H.; Oppenheimer, D. H.</p> <p>2005-12-01</p> <p>We report on the observation of <span class="hlt">non-volcanic</span> tremor made in the San Andreas Fault Observatory at Depth in May, 2005 during the deployment of a multi-level borehole seismic array in the SAFOD main hole. The seismic array consisted of 80 levels of hydraulically-clamped 3-component, 15 Hz omni-directional geophones spaced 15.24 m apart along a 1200 m section of the inclined borehole between 1538 and 2363 m below the ground surface. The array was provided by Paulsson Geophysical Services, Inc. (P/GSI), and recorded at a sample rate of 4000 sps on 24-bit Geode digital recorders provided by Geometrics, Inc. More than 2 TB of continuous data were recorded during the 2-week deployment. Selected local earthquakes and explosions recorded by the array are available at the Northern California Earthquake Data Center, and the entire unedited data set is available as assembled data at the IRIS Data Management Center. Both data sets are currently in the industry standard SEG2 format. Episodes of <span class="hlt">non-volcanic</span> tremor are common along this reach of the San Andreas Fault according to Nadeau and Dolenc [2004, DOI: 10.1126/science.1107142], with many originating about 30 km southeast of SAFOD beneath the southern end of the Parkfield segment and northern end of the Simmler segment of the fault. We identified tremor episodes using spectrograms routinely produced by the Northern California Seismic Network (http://quake.usgs.gov/cgi-bin/sgrampark.pl) on which they appear as periods of elevated noise relative to the background. A particularly strong tremor episode occurred on May 10, 2005 between 19:39 and 20:00 UTC. In SAFOD, tremor spectral levels exceed the instrumental noise floor to at least 40 Hz. The spatially unaliased recording of the tremor wavefield on the P/GSI array reveal individual phases that can be tracked continuously across the array. The wavefield is composed of both up- and down-going shear waves that form quasi-stationary interference patterns in which areas of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.9193S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.9193S"><span>ASI-<span class="hlt">Volcanic</span> Risk System (SRV): a pilot project to develop EO data processing modules and products for <span class="hlt">volcanic</span> <span class="hlt">activity</span> monitoring, first results.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Silvestri, M.; Musacchio, M.; Buongiorno, M. F.; Dini, L.</p> <p>2009-04-01</p> <p>The Project called Sistema Rischio Vulcanico (SRV) is funded by the Italian Space Agency (ASI) in the frame of the National Space Plan 2003-2005 under the Earth Observations section for natural risks management. The SRV Project is coordinated by the Istituto Nazionale di Geofisica e Vulcanologia (INGV) which is responsible at national level for the <span class="hlt">volcanic</span> monitoring. The project philosophy is to implement, by incremental versions, specific modules which allow to process, store and visualize through Web GIS tools geophysical parameters suitable for <span class="hlt">volcanic</span> risk management. The ASI-SRV is devoted to the development of an integrated system based on Earth Observation (EO) data to respond to specific needs of the Italian Civil Protection Department (DPC) and improve the monitoring of Italian <span class="hlt">active</span> volcanoes during all the risk phases (Pre Crisis, Crisis and Post Crisis). The ASI-SRV system provides support to risk managers during the different <span class="hlt">volcanic</span> <span class="hlt">activity</span> phases and its results are addressed to the Italian Civil Protection Department (DPC). SRV provides the capability to manage the import many different EO data into the system, it maintains a repository where the acquired data have to be stored and generates selected <span class="hlt">volcanic</span> products. The processing modules for EO Optical sensors data are based on procedures jointly developed by INGV and University of Modena. This procedures allow to estimate a number of parameters such as: surface thermal proprieties, gas, aerosol and ash emissions and to characterize the <span class="hlt">volcanic</span> products in terms of composition and geometry. For the analysis of the surface thermal characteristics, the available algorithms allow to extract information during the prevention phase and during the Warning and Crisis phase. In the prevention phase the thermal analysis is directed to the identification of temperature variation on <span class="hlt">volcanic</span> structure which may indicate a change in the <span class="hlt">volcanic</span> <span class="hlt">activity</span> state. At the moment the only sensor that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B11I0562B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B11I0562B"><span>Marine Subsurface Microbial Communities Across a <span class="hlt">Hydrothermal</span> Gradient in Okinawa Trough Sediments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brandt, L. D.; Hser Wah Saw, J.; Ettema, T.; House, C. H.</p> <p>2015-12-01</p> <p>IODP Expedition 331 to the Okinawa backarc basin provided an opportunity to study the microbial stratigraphy within the sediments surrounding a <span class="hlt">hydrothermal</span> vent. The Okinawa backarc basin is a sedimented region of the seafloor located on a continental margin, and also hosts a <span class="hlt">hydrothermal</span> network within the subsurface. Site C0014 within the Iheya North <span class="hlt">hydrothermal</span> field is located 450 m east of the <span class="hlt">active</span> vent and has a surface temperature of 5°C with no evidence of <span class="hlt">hydrothermal</span> alteration within the top 10 meters below sea floor (mbsf). Temperature increases with depth at an estimated rate of 3°C/m and transitions from <span class="hlt">non-hydrothermal</span> margin sediments to a <span class="hlt">hydrothermally</span> altered regime below 10 mbsf. In this study, we utilized deep 16S rRNA sequencing of DNA from IODP Expedition 331 Site C0014 sediment horizons in order to assess diversity throughout the sediment column as well as determine the potential limits of the biosphere. Analysis of the amplicon data shows a shift over 15 mbsf from a heterogeneous community of cosmopolitan marine subsurface taxa toward an archaeal-dominated community in the deepest horizons of the predicted biosphere. Notably, the phylum Chloroflexi represents a substantial taxon through most horizons, where it appears to be replaced below 10 mbsf by punctuations of thermophilic and methanotrophic Archaea and Miscellaneous Crenarchaeotic Group abundances. DNA from the aforementioned transition horizons was further analyzed using metagenomic sequencing. Preliminary taxonomic analysis of the metagenomic data agrees well with amplicon data in capturing the shift in relative abundance of Archaea increasing with depth. Additionally, reverse gyrase, a gene found exclusively in hyperthermophilic microorganisms, was recovered only in the metagenome of the deepest horizon. A BLAST search of this protein sequence against the GenBank <span class="hlt">non</span>-redudnant protein database produced top hits with reverse gyrase from Thermococcus and Pyrococcus, which are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ApSS..259..698X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ApSS..259..698X"><span>Preparation high photocatalytic <span class="hlt">activity</span> of CdS/halloysite nanotubes (HNTs) nanocomposites with <span class="hlt">hydrothermal</span> method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xing, Weinan; Ni, Liang; Huo, Pengwei; Lu, Ziyang; Liu, Xinlin; Luo, Yingying; Yan, Yongsheng</p> <p>2012-10-01</p> <p>A novel nanocatalyst CdS/halloysite nanotubes (HNTs) was synthesized by <span class="hlt">hydrothermal</span> method with direct growth of CdS nanoparticles on the surface of HNTs. The as-prepared photocatalysts had been characterized by scanning electron microscopy (SEM), transmission electron microscopy (TEM), X-ray energy dispersive spectroscopy (EDS), X-ray diffraction (XRD), UV-vis diffuse reflectance spectra (UV-vis DRS), Fourier transform infrared (FT-IR) and the thermo gravimetric analysis (TGA). The photocatalytic <span class="hlt">activity</span> of the sample was evaluated by the degradation of tetracycline (TC) under visible light irradiation. Benefit from the excellent properties of CdS and HNTs, the photocatalyst exhibited good photocatalytic <span class="hlt">activity</span> and stability. In order to find out the optimum synthesis condition to obtain the best photocatalytic <span class="hlt">activity</span>, a series of experiments were performed with different CdS loading capacity, different sources of sulfide and different <span class="hlt">hydrothermal</span> temperatures, etc. The best photodegradation rate could reach 93% in 60 min under visible light irradiation. Therefore, the combination of CdS nanoparticles with HNTs endowed this material with a potential use in environmental treatments in industries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V51D2715B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V51D2715B"><span>New structural, hydrogeological and <span class="hlt">hydrothermal</span> insights on Cumbre Vieja (La Palma, Canary Islands, Spain)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barde-Cabusson, S.; Finizola, A.; Torres, P.; Víctor Villasante-Marcos, V.; Abella, R.; Aragó, S.; Berthod, C.; Ibarra, P.; Geyer Traver, A.</p> <p>2013-12-01</p> <p>Determining the link between shallow structure and <span class="hlt">volcanism</span> is a topic of interest in Volcanology. We carried out a geophysical study devoted to the characterization of the major structural limits influencing <span class="hlt">volcanic</span> <span class="hlt">hydrothermal</span> <span class="hlt">activity</span> and underground meteoric circulations in La Palma (Canary Islands). Since 1 Ma <span class="hlt">volcanic</span> <span class="hlt">activity</span> concentrates at the southern half of the island, on the Cumbre Vieja <span class="hlt">volcanic</span> rift-zone. During the 1949 eruption a N-S fault system, facing west, developed in the summit area of Cumbre Vieja. This was interpreted as the surface expression of an incipient deformation zone on the western flank. The distribution of the recent <span class="hlt">activity</span> and faulting indicate that a discontinuity may be present beneath the western flank of Cumbre Vieja, along which a future collapse may occur. Our study, which combines the application of self-potential and soil temperature measurements, provides new information to characterize and locate the limits guiding upward or downward fluid circulation and possibly associated to future failures and potential landslides on the Cumbre Vieja rift-zone. We found a clear asymmetry of the self-potential signal between the eastern and the western flanks of Cumbre Vieja. Strong infiltration of meteoric water seems to affect most of the summit axis while we observe poor variation in the self-potential values on the western flank. This could be explained by a constant thickness of the vadose zone on this flank, i.e., the presence of an impermeable layer at constant depth. This layer could correspond to the landslide interface associated to the previous Cumbre Nueva edifice destruction, on which Cumbre Vieja is currently growing. This constant self-potential pattern is interrupted by at least one other main infiltration zone, near Tajuya volcano, at 1200 m a.s.l. on the western flank, where field observation allowed identifying a small horst-graben system. However it is not clear if this fault system results from local</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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