Sample records for frequency scaling dvfs

  1. Static and Dynamic Frequency Scaling on Multicore CPUs

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

    Bao, Wenlei; Hong, Changwan; Chunduri, Sudheer

    2016-12-28

    Dynamic voltage and frequency scaling (DVFS) adapts CPU power consumption by modifying a processor’s operating frequency (and the associated voltage). Typical approaches employing DVFS involve default strategies such as running at the lowest or the highest frequency, or observing the CPU’s runtime behavior and dynamically adapting the voltage/frequency configuration based on CPU usage. In this paper, we argue that many previous approaches suffer from inherent limitations, such as not account- ing for processor-specific impact of frequency changes on energy for different workload types. We first propose a lightweight runtime-based approach to automatically adapt the frequency based on the CPU workload,more » that is agnostic of the processor characteristics. We then show that further improvements can be achieved for affine kernels in the application, using a compile-time characterization instead of run-time monitoring to select the frequency and number of CPU cores to use. Our framework relies on a one-time energy characterization of CPU-specific DVFS profiles followed by a compile-time categorization of loop-based code segments in the application. These are combined to determine a priori of the frequency and the number of cores to use to execute the application so as to optimize energy or energy-delay product, outperforming runtime approach. Extensive evaluation on 60 benchmarks and five multi-core CPUs show that our approach systematically outperforms the powersave Linux governor, while improving overall performance.« less

  2. Energy Conservation Using Dynamic Voltage Frequency Scaling for Computational Cloud

    PubMed Central

    Florence, A. Paulin; Shanthi, V.; Simon, C. B. Sunil

    2016-01-01

    Cloud computing is a new technology which supports resource sharing on a “Pay as you go” basis around the world. It provides various services such as SaaS, IaaS, and PaaS. Computation is a part of IaaS and the entire computational requests are to be served efficiently with optimal power utilization in the cloud. Recently, various algorithms are developed to reduce power consumption and even Dynamic Voltage and Frequency Scaling (DVFS) scheme is also used in this perspective. In this paper we have devised methodology which analyzes the behavior of the given cloud request and identifies the associated type of algorithm. Once the type of algorithm is identified, using their asymptotic notations, its time complexity is calculated. Using best fit strategy the appropriate host is identified and the incoming job is allocated to the victimized host. Using the measured time complexity the required clock frequency of the host is measured. According to that CPU frequency is scaled up or down using DVFS scheme, enabling energy to be saved up to 55% of total Watts consumption. PMID:27239551

  3. Energy Conservation Using Dynamic Voltage Frequency Scaling for Computational Cloud.

    PubMed

    Florence, A Paulin; Shanthi, V; Simon, C B Sunil

    2016-01-01

    Cloud computing is a new technology which supports resource sharing on a "Pay as you go" basis around the world. It provides various services such as SaaS, IaaS, and PaaS. Computation is a part of IaaS and the entire computational requests are to be served efficiently with optimal power utilization in the cloud. Recently, various algorithms are developed to reduce power consumption and even Dynamic Voltage and Frequency Scaling (DVFS) scheme is also used in this perspective. In this paper we have devised methodology which analyzes the behavior of the given cloud request and identifies the associated type of algorithm. Once the type of algorithm is identified, using their asymptotic notations, its time complexity is calculated. Using best fit strategy the appropriate host is identified and the incoming job is allocated to the victimized host. Using the measured time complexity the required clock frequency of the host is measured. According to that CPU frequency is scaled up or down using DVFS scheme, enabling energy to be saved up to 55% of total Watts consumption.

  4. Dynamic Voltage Frequency Scaling Simulator for Real Workflows Energy-Aware Management in Green Cloud Computing

    PubMed Central

    Cotes-Ruiz, Iván Tomás; Prado, Rocío P.; García-Galán, Sebastián; Muñoz-Expósito, José Enrique; Ruiz-Reyes, Nicolás

    2017-01-01

    Nowadays, the growing computational capabilities of Cloud systems rely on the reduction of the consumed power of their data centers to make them sustainable and economically profitable. The efficient management of computing resources is at the heart of any energy-aware data center and of special relevance is the adaptation of its performance to workload. Intensive computing applications in diverse areas of science generate complex workload called workflows, whose successful management in terms of energy saving is still at its beginning. WorkflowSim is currently one of the most advanced simulators for research on workflows processing, offering advanced features such as task clustering and failure policies. In this work, an expected power-aware extension of WorkflowSim is presented. This new tool integrates a power model based on a computing-plus-communication design to allow the optimization of new management strategies in energy saving considering computing, reconfiguration and networks costs as well as quality of service, and it incorporates the preeminent strategy for on host energy saving: Dynamic Voltage Frequency Scaling (DVFS). The simulator is designed to be consistent in different real scenarios and to include a wide repertory of DVFS governors. Results showing the validity of the simulator in terms of resources utilization, frequency and voltage scaling, power, energy and time saving are presented. Also, results achieved by the intra-host DVFS strategy with different governors are compared to those of the data center using a recent and successful DVFS-based inter-host scheduling strategy as overlapped mechanism to the DVFS intra-host technique. PMID:28085932

  5. Dynamic Voltage Frequency Scaling Simulator for Real Workflows Energy-Aware Management in Green Cloud Computing.

    PubMed

    Cotes-Ruiz, Iván Tomás; Prado, Rocío P; García-Galán, Sebastián; Muñoz-Expósito, José Enrique; Ruiz-Reyes, Nicolás

    2017-01-01

    Nowadays, the growing computational capabilities of Cloud systems rely on the reduction of the consumed power of their data centers to make them sustainable and economically profitable. The efficient management of computing resources is at the heart of any energy-aware data center and of special relevance is the adaptation of its performance to workload. Intensive computing applications in diverse areas of science generate complex workload called workflows, whose successful management in terms of energy saving is still at its beginning. WorkflowSim is currently one of the most advanced simulators for research on workflows processing, offering advanced features such as task clustering and failure policies. In this work, an expected power-aware extension of WorkflowSim is presented. This new tool integrates a power model based on a computing-plus-communication design to allow the optimization of new management strategies in energy saving considering computing, reconfiguration and networks costs as well as quality of service, and it incorporates the preeminent strategy for on host energy saving: Dynamic Voltage Frequency Scaling (DVFS). The simulator is designed to be consistent in different real scenarios and to include a wide repertory of DVFS governors. Results showing the validity of the simulator in terms of resources utilization, frequency and voltage scaling, power, energy and time saving are presented. Also, results achieved by the intra-host DVFS strategy with different governors are compared to those of the data center using a recent and successful DVFS-based inter-host scheduling strategy as overlapped mechanism to the DVFS intra-host technique.

  6. Adaptive real-time methodology for optimizing energy-efficient computing

    DOEpatents

    Hsu, Chung-Hsing [Los Alamos, NM; Feng, Wu-Chun [Blacksburg, VA

    2011-06-28

    Dynamic voltage and frequency scaling (DVFS) is an effective way to reduce energy and power consumption in microprocessor units. Current implementations of DVFS suffer from inaccurate modeling of power requirements and usage, and from inaccurate characterization of the relationships between the applicable variables. A system and method is proposed that adjusts CPU frequency and voltage based on run-time calculations of the workload processing time, as well as a calculation of performance sensitivity with respect to CPU frequency. The system and method are processor independent, and can be applied to either an entire system as a unit, or individually to each process running on a system.

  7. Adaptive real-time methodology for optimizing energy-efficient computing

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

    Hsu, Chung-Hsing; Feng, Wu-Chun

    Dynamic voltage and frequency scaling (DVFS) is an effective way to reduce energy and power consumption in microprocessor units. Current implementations of DVFS suffer from inaccurate modeling of power requirements and usage, and from inaccurate characterization of the relationships between the applicable variables. A system and method is proposed that adjusts CPU frequency and voltage based on run-time calculations of the workload processing time, as well as a calculation of performance sensitivity with respect to CPU frequency. The system and method are processor independent, and can be applied to either an entire system as a unit, or individually to eachmore » process running on a system.« less

  8. The Assessment of Protective Behavioral Strategies: Comparing the Absolute Frequency and Contingent Frequency Response Scales

    PubMed Central

    Kite, Benjamin A.; Pearson, Matthew R.; Henson, James M.

    2016-01-01

    The purpose of the present studies was to examine the effects of response scale on the observed relationships between protective behavioral strategies (PBS) measures and alcohol-related outcomes. We reasoned that an ‘absolute frequency’ scale (stem: “how many times…”; response scale: 0 times to 11+ times) conflates the frequency of using PBS with the frequency of consuming alcohol; thus, we hypothesized that the use of an absolute frequency response scale would result in positive relationships between types of PBS and alcohol-related outcomes. Alternatively, a ‘contingent frequency’ scale (stem: “When drinking…how often…”; response scale: never to always) does not conflate frequency of alcohol use with use of PBS; therefore, we hypothesized that use of a contingent frequency scale would result in negative relationships between use of PBS and alcohol-related outcomes. Two published measures of PBS were used across studies: the Protective Behavioral Strategies Survey (PBSS) and the Strategy Questionnaire (SQ). Across three studies, we demonstrate that when measured using a contingent frequency response scale, PBS measures relate negatively to alcohol-related outcomes in a theoretically consistent manner; however, when PBS measures were measured on an absolute frequency response scale, they were non-significantly or positively related to alcohol-related outcomes. We discuss the implications of these findings for the assessment of PBS. PMID:23438243

  9. Scaling of Yb-Fiber Frequency Combs

    NASA Astrophysics Data System (ADS)

    Ruehl, Axel; Marcinkevicius, Andrius; Fermann, Martin E.; Hartl, Ingmar

    2010-06-01

    Immediately after their introduction in 1999, femtosecond laser frequency combs revolutionized the field of precision optical frequency metrology and are key elements in many experiments. Frequency combs based on femtosecond Er-fiber lasers based were demonstrated in 2005, allowing additionally rugged, compact set-ups and reliable unattended long-term operation. The introduction of Yb-fiber technology led to an dramatic improvement in fiber-comb performance in various aspects. Low-noise Yb-fiber femtosecond oscillators enabled a reduction of relative comb tooth linewidth to the sub-Hz level as well as scaling of the fundamental comb spacings up to 1 GHz. This is beneficial for any frequency-domain comb application due to the higher power per comb-mode. Many spectroscopic applications require, however, frequency combs way beyond the wavelength range accessible with broad band laser materials, so nonlinear conversion and hence higher peak intensity is required. We demonstrated power scaling of Yb-fiber frequency combs up to 80 W average power in a strictly linear chirped-pulse amplification schemes compatible with low-noise phase control. These high-power Yb-fiber-frequency combs facilitated not only the extension to the mid-IR spectral region. When coupled to a passive enhancement cavity, the average power can be further scaled to the kW-level opening new capabilities for XUV frequency combs via high-harmonic generation. All these advances of fiber-based frequency combs will trigger many novel applications both in fundamental and applied sciences. Schibli et al., Nature Photonics 2 355 (2008). Hartl et al., MF9 in Advanced Solid-State Photonics. 2009, Optical Society of America. Ruehl et al., AWC7 in Advanced Solid-State Photonics. 2010, Optical Society of America. Adler et al., Optics Letters 34 1330 (2009). Yost et al., Nature Physics 5 815 (2009).

  10. Automatic Energy Schemes for High Performance Applications

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

    Sundriyal, Vaibhav

    Although high-performance computing traditionally focuses on the efficient execution of large-scale applications, both energy and power have become critical concerns when approaching exascale. Drastic increases in the power consumption of supercomputers affect significantly their operating costs and failure rates. In modern microprocessor architectures, equipped with dynamic voltage and frequency scaling (DVFS) and CPU clock modulation (throttling), the power consumption may be controlled in software. Additionally, network interconnect, such as Infiniband, may be exploited to maximize energy savings while the application performance loss and frequency switching overheads must be carefully balanced. This work first studies two important collective communication operations, all-to-allmore » and allgather and proposes energy saving strategies on the per-call basis. Next, it targets point-to-point communications to group them into phases and apply frequency scaling to them to save energy by exploiting the architectural and communication stalls. Finally, it proposes an automatic runtime system which combines both collective and point-to-point communications into phases, and applies throttling to them apart from DVFS to maximize energy savings. The experimental results are presented for NAS parallel benchmark problems as well as for the realistic parallel electronic structure calculations performed by the widely used quantum chemistry package GAMESS. Close to the maximum energy savings were obtained with a substantially low performance loss on the given platform.« less

  11. Low frequency steady-state brain responses modulate large scale functional networks in a frequency-specific means.

    PubMed

    Wang, Yi-Feng; Long, Zhiliang; Cui, Qian; Liu, Feng; Jing, Xiu-Juan; Chen, Heng; Guo, Xiao-Nan; Yan, Jin H; Chen, Hua-Fu

    2016-01-01

    Neural oscillations are essential for brain functions. Research has suggested that the frequency of neural oscillations is lower for more integrative and remote communications. In this vein, some resting-state studies have suggested that large scale networks function in the very low frequency range (<1 Hz). However, it is difficult to determine the frequency characteristics of brain networks because both resting-state studies and conventional frequency tagging approaches cannot simultaneously capture multiple large scale networks in controllable cognitive activities. In this preliminary study, we aimed to examine whether large scale networks can be modulated by task-induced low frequency steady-state brain responses (lfSSBRs) in a frequency-specific pattern. In a revised attention network test, the lfSSBRs were evoked in the triple network system and sensory-motor system, indicating that large scale networks can be modulated in a frequency tagging way. Furthermore, the inter- and intranetwork synchronizations as well as coherence were increased at the fundamental frequency and the first harmonic rather than at other frequency bands, indicating a frequency-specific modulation of information communication. However, there was no difference among attention conditions, indicating that lfSSBRs modulate the general attention state much stronger than distinguishing attention conditions. This study provides insights into the advantage and mechanism of lfSSBRs. More importantly, it paves a new way to investigate frequency-specific large scale brain activities. © 2015 Wiley Periodicals, Inc.

  12. Chip-Scale Architectures for Precise Optical Frequency Synthesis

    NASA Astrophysics Data System (ADS)

    Yang, Jinghui

    Scientists and engineers have investigated various types of stable and accurate optical synthesizers, where mode-locked laser based optical frequency comb synthesizers have been widely investigated. These frequency combs bridge the frequencies from optical domain to microwave domain with orders of magnitude difference, providing a metrological tool for various platforms. The demand for highly robust, scalable, compact and cost-effective femtosecond-laser synthesizers, however, are of great importance for applications in air- or space-borne platforms, where low cost and rugged packaging are particularly required. This has been afforded in the past several years due to breakthroughs in chip-scale nanofabrication, bringing advances in optical frequency combs down to semiconductor chips. These platforms, with significantly enhanced light-matter interaction, provide a fertile sandbox for research rich in nonlinear dynamics, and offer a reliable route towards low-phase noise photonic oscillators, broadband optical frequency synthesizers, miniaturized optical clockwork, and coherent terabit communications. The dissertation explores various types of optical frequency comb synthesizers based on nonlinear microresonators. Firstly, the fundamental mechanism of mode-locking in a high-quality factor microresonator is examined, supported by ultrafast optical characterizations, analytical closed-form solutions and numerical modeling. In the evolution of these frequency microcombs, the key nonlinear dynamical effect governing the comb state coherence is rigorously analyzed. Secondly, a prototype of chip-scale optical frequency synthesizer is demonstrated, with the laser frequency comb stabilized down to instrument-limited 50-mHz RF frequency inaccuracies and 10-16 fractional frequency inaccuracies, near the fundamental limits. Thirdly, a globally stable Turing pattern is achieved and characterized in these nonlinear resonators with high-efficiency conversion, subsequently

  13. Application configuration selection for energy-efficient execution on multicore systems

    DOE PAGES

    Wang, Shinan; Luo, Bing; Shi, Weisong; ...

    2015-09-21

    Balanced performance and energy consumption are incorporated in the design of modern computer systems. Several runtime factors, such as concurrency levels, thread mapping strategies, and dynamic voltage and frequency scaling (DVFS) should be considered in order to achieve optimal energy efficiency fora workload. Selecting appropriate run-time factors, however, is one of the most challenging tasks because the run-time factors are architecture-specific and workload-specific. And while most existing works concentrate on either static analysis of the workload or run-time prediction results, we present a hybrid two-step method that utilizes concurrency levels and DVFS settings to achieve the energy efficiency configuration formore » a worldoad. The experimental results based on a Xeon E5620 server with NPB and PARSEC benchmark suites show that the model is able to predict the energy efficient configuration accurately. On average, an additional 10% EDP (Energy Delay Product) saving is obtained by using run-time DVFS for the entire system. An off-line optimal solution is used to compare with the proposed scheme. Finally, the experimental results show that the average extra EDP saved by the optimal solution is within 5% on selective parallel benchmarks.« less

  14. Time and frequency domain characteristics of detrending-operation-based scaling analysis: Exact DFA and DMA frequency responses

    NASA Astrophysics Data System (ADS)

    Kiyono, Ken; Tsujimoto, Yutaka

    2016-07-01

    We develop a general framework to study the time and frequency domain characteristics of detrending-operation-based scaling analysis methods, such as detrended fluctuation analysis (DFA) and detrending moving average (DMA) analysis. In this framework, using either the time or frequency domain approach, the frequency responses of detrending operations are calculated analytically. Although the frequency domain approach based on conventional linear analysis techniques is only applicable to linear detrending operations, the time domain approach presented here is applicable to both linear and nonlinear detrending operations. Furthermore, using the relationship between the time and frequency domain representations of the frequency responses, the frequency domain characteristics of nonlinear detrending operations can be obtained. Based on the calculated frequency responses, it is possible to establish a direct connection between the root-mean-square deviation of the detrending-operation-based scaling analysis and the power spectrum for linear stochastic processes. Here, by applying our methods to DFA and DMA, including higher-order cases, exact frequency responses are calculated. In addition, we analytically investigate the cutoff frequencies of DFA and DMA detrending operations and show that these frequencies are not optimally adjusted to coincide with the corresponding time scale.

  15. Time and frequency domain characteristics of detrending-operation-based scaling analysis: Exact DFA and DMA frequency responses.

    PubMed

    Kiyono, Ken; Tsujimoto, Yutaka

    2016-07-01

    We develop a general framework to study the time and frequency domain characteristics of detrending-operation-based scaling analysis methods, such as detrended fluctuation analysis (DFA) and detrending moving average (DMA) analysis. In this framework, using either the time or frequency domain approach, the frequency responses of detrending operations are calculated analytically. Although the frequency domain approach based on conventional linear analysis techniques is only applicable to linear detrending operations, the time domain approach presented here is applicable to both linear and nonlinear detrending operations. Furthermore, using the relationship between the time and frequency domain representations of the frequency responses, the frequency domain characteristics of nonlinear detrending operations can be obtained. Based on the calculated frequency responses, it is possible to establish a direct connection between the root-mean-square deviation of the detrending-operation-based scaling analysis and the power spectrum for linear stochastic processes. Here, by applying our methods to DFA and DMA, including higher-order cases, exact frequency responses are calculated. In addition, we analytically investigate the cutoff frequencies of DFA and DMA detrending operations and show that these frequencies are not optimally adjusted to coincide with the corresponding time scale.

  16. Selective visual scaling of time-scale processes facilitates broadband learning of isometric force frequency tracking.

    PubMed

    King, Adam C; Newell, Karl M

    2015-10-01

    The experiment investigated the effect of selectively augmenting faster time scales of visual feedback information on the learning and transfer of continuous isometric force tracking tasks to test the generality of the self-organization of 1/f properties of force output. Three experimental groups tracked an irregular target pattern either under a standard fixed gain condition or with selectively enhancement in the visual feedback display of intermediate (4-8 Hz) or high (8-12 Hz) frequency components of the force output. All groups reduced tracking error over practice, with the error lowest in the intermediate scaling condition followed by the high scaling and fixed gain conditions, respectively. Selective visual scaling induced persistent changes across the frequency spectrum, with the strongest effect in the intermediate scaling condition and positive transfer to novel feedback displays. The findings reveal an interdependence of the timescales in the learning and transfer of isometric force output frequency structures consistent with 1/f process models of the time scales of motor output variability.

  17. Achieving energy efficiency during collective communications

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

    Sundriyal, Vaibhav; Sosonkina, Masha; Zhang, Zhao

    2012-09-13

    Energy consumption has become a major design constraint in modern computing systems. With the advent of petaflops architectures, power-efficient software stacks have become imperative for scalability. Techniques such as dynamic voltage and frequency scaling (called DVFS) and CPU clock modulation (called throttling) are often used to reduce the power consumption of the compute nodes. To avoid significant performance losses, these techniques should be used judiciously during parallel application execution. For example, its communication phases may be good candidates to apply the DVFS and CPU throttling without incurring a considerable performance loss. They are often considered as indivisible operations although littlemore » attention is being devoted to the energy saving potential of their algorithmic steps. In this work, two important collective communication operations, all-to-all and allgather, are investigated as to their augmentation with energy saving strategies on the per-call basis. The experiments prove the viability of such a fine-grain approach. They also validate a theoretical power consumption estimate for multicore nodes proposed here. While keeping the performance loss low, the obtained energy savings were always significantly higher than those achieved when DVFS or throttling were switched on across the entire application run« less

  18. Large scale modulation of high frequency acoustic waves in periodic porous media.

    PubMed

    Boutin, Claude; Rallu, Antoine; Hans, Stephane

    2012-12-01

    This paper deals with the description of the modulation at large scale of high frequency acoustic waves in gas saturated periodic porous media. High frequencies mean local dynamics at the pore scale and therefore absence of scale separation in the usual sense of homogenization. However, although the pressure is spatially varying in the pores (according to periodic eigenmodes), the mode amplitude can present a large scale modulation, thereby introducing another type of scale separation to which the asymptotic multi-scale procedure applies. The approach is first presented on a periodic network of inter-connected Helmholtz resonators. The equations governing the modulations carried by periodic eigenmodes, at frequencies close to their eigenfrequency, are derived. The number of cells on which the carrying periodic mode is defined is therefore a parameter of the modeling. In a second part, the asymptotic approach is developed for periodic porous media saturated by a perfect gas. Using the "multicells" periodic condition, one obtains the family of equations governing the amplitude modulation at large scale of high frequency waves. The significant difference between modulations of simple and multiple mode are evidenced and discussed. The features of the modulation (anisotropy, width of frequency band) are also analyzed.

  19. Computational Thermochemistry: Scale Factor Databases and Scale Factors for Vibrational Frequencies Obtained from Electronic Model Chemistries.

    PubMed

    Alecu, I M; Zheng, Jingjing; Zhao, Yan; Truhlar, Donald G

    2010-09-14

    Optimized scale factors for calculating vibrational harmonic and fundamental frequencies and zero-point energies have been determined for 145 electronic model chemistries, including 119 based on approximate functionals depending on occupied orbitals, 19 based on single-level wave function theory, three based on the neglect-of-diatomic-differential-overlap, two based on doubly hybrid density functional theory, and two based on multicoefficient correlation methods. Forty of the scale factors are obtained from large databases, which are also used to derive two universal scale factor ratios that can be used to interconvert between scale factors optimized for various properties, enabling the derivation of three key scale factors at the effort of optimizing only one of them. A reduced scale factor optimization model is formulated in order to further reduce the cost of optimizing scale factors, and the reduced model is illustrated by using it to obtain 105 additional scale factors. Using root-mean-square errors from the values in the large databases, we find that scaling reduces errors in zero-point energies by a factor of 2.3 and errors in fundamental vibrational frequencies by a factor of 3.0, but it reduces errors in harmonic vibrational frequencies by only a factor of 1.3. It is shown that, upon scaling, the balanced multicoefficient correlation method based on coupled cluster theory with single and double excitations (BMC-CCSD) can lead to very accurate predictions of vibrational frequencies. With a polarized, minimally augmented basis set, the density functionals with zero-point energy scale factors closest to unity are MPWLYP1M (1.009), τHCTHhyb (0.989), BB95 (1.012), BLYP (1.013), BP86 (1.014), B3LYP (0.986), MPW3LYP (0.986), and VSXC (0.986).

  20. Frequencies and Flutter Speed Estimation for Damaged Aircraft Wing Using Scaled Equivalent Plate Analysis

    NASA Technical Reports Server (NTRS)

    Krishnamurthy, Thiagarajan

    2010-01-01

    Equivalent plate analysis is often used to replace the computationally expensive finite element analysis in initial design stages or in conceptual design of aircraft wing structures. The equivalent plate model can also be used to design a wind tunnel model to match the stiffness characteristics of the wing box of a full-scale aircraft wing model while satisfying strength-based requirements An equivalent plate analysis technique is presented to predict the static and dynamic response of an aircraft wing with or without damage. First, a geometric scale factor and a dynamic pressure scale factor are defined to relate the stiffness, load and deformation of the equivalent plate to the aircraft wing. A procedure using an optimization technique is presented to create scaled equivalent plate models from the full scale aircraft wing using geometric and dynamic pressure scale factors. The scaled models are constructed by matching the stiffness of the scaled equivalent plate with the scaled aircraft wing stiffness. It is demonstrated that the scaled equivalent plate model can be used to predict the deformation of the aircraft wing accurately. Once the full equivalent plate geometry is obtained, any other scaled equivalent plate geometry can be obtained using the geometric scale factor. Next, an average frequency scale factor is defined as the average ratio of the frequencies of the aircraft wing to the frequencies of the full-scaled equivalent plate. The average frequency scale factor combined with the geometric scale factor is used to predict the frequency response of the aircraft wing from the scaled equivalent plate analysis. A procedure is outlined to estimate the frequency response and the flutter speed of an aircraft wing from the equivalent plate analysis using the frequency scale factor and geometric scale factor. The equivalent plate analysis is demonstrated using an aircraft wing without damage and another with damage. Both of the problems show that the scaled

  1. Ultrafast dynamics and stabilization in chip-scale optical frequency combs (Conference Presentation)

    NASA Astrophysics Data System (ADS)

    Huang, Shu Wei

    2017-02-01

    Optical frequency comb technology has been the cornerstone for scientific breakthroughs such as precision frequency metrology, re-definition of time, extreme light-matter interaction, and attosecond sciences. Recently emerged Kerr-active microresonators are promising alternatives to the current benchmark femtosecond laser platform. These chip-scale frequency combs, or Kerr combs, are unique in their compact footprints and offer the potential for monolithic electronic and feedback integration, thereby expanding the already remarkable applications of optical frequency combs. In this talk, I will first report the generation and characterization of low-phase-noise Kerr frequency combs. Measurements of the Kerr comb ultrafast dynamics and phase noise will be presented and discussed. Then I will describe novel strategies to fully stabilize Kerr comb line frequencies towards chip-scale optical frequency synthesizers with a relative uncertainty better than 2.7×10-16. I will show that the unique generation physics of Kerr frequency comb can provide an intrinsic self-referenced access to the Kerr comb line frequencies. The strategy improves the optical frequency stability by more than two orders of magnitude, while preserving the Kerr comb's key advantage of low SWaP and potential for chip-scale electronic and photonic integration.

  2. Network-State Modulation of Power-Law Frequency-Scaling in Visual Cortical Neurons

    PubMed Central

    Béhuret, Sébastien; Baudot, Pierre; Yger, Pierre; Bal, Thierry; Destexhe, Alain; Frégnac, Yves

    2009-01-01

    Various types of neural-based signals, such as EEG, local field potentials and intracellular synaptic potentials, integrate multiple sources of activity distributed across large assemblies. They have in common a power-law frequency-scaling structure at high frequencies, but it is still unclear whether this scaling property is dominated by intrinsic neuronal properties or by network activity. The latter case is particularly interesting because if frequency-scaling reflects the network state it could be used to characterize the functional impact of the connectivity. In intracellularly recorded neurons of cat primary visual cortex in vivo, the power spectral density of Vm activity displays a power-law structure at high frequencies with a fractional scaling exponent. We show that this exponent is not constant, but depends on the visual statistics used to drive the network. To investigate the determinants of this frequency-scaling, we considered a generic recurrent model of cortex receiving a retinotopically organized external input. Similarly to the in vivo case, our in computo simulations show that the scaling exponent reflects the correlation level imposed in the input. This systematic dependence was also replicated at the single cell level, by controlling independently, in a parametric way, the strength and the temporal decay of the pairwise correlation between presynaptic inputs. This last model was implemented in vitro by imposing the correlation control in artificial presynaptic spike trains through dynamic-clamp techniques. These in vitro manipulations induced a modulation of the scaling exponent, similar to that observed in vivo and predicted in computo. We conclude that the frequency-scaling exponent of the Vm reflects stimulus-driven correlations in the cortical network activity. Therefore, we propose that the scaling exponent could be used to read-out the “effective” connectivity responsible for the dynamical signature of the population signals measured

  3. Network-state modulation of power-law frequency-scaling in visual cortical neurons.

    PubMed

    El Boustani, Sami; Marre, Olivier; Béhuret, Sébastien; Baudot, Pierre; Yger, Pierre; Bal, Thierry; Destexhe, Alain; Frégnac, Yves

    2009-09-01

    Various types of neural-based signals, such as EEG, local field potentials and intracellular synaptic potentials, integrate multiple sources of activity distributed across large assemblies. They have in common a power-law frequency-scaling structure at high frequencies, but it is still unclear whether this scaling property is dominated by intrinsic neuronal properties or by network activity. The latter case is particularly interesting because if frequency-scaling reflects the network state it could be used to characterize the functional impact of the connectivity. In intracellularly recorded neurons of cat primary visual cortex in vivo, the power spectral density of V(m) activity displays a power-law structure at high frequencies with a fractional scaling exponent. We show that this exponent is not constant, but depends on the visual statistics used to drive the network. To investigate the determinants of this frequency-scaling, we considered a generic recurrent model of cortex receiving a retinotopically organized external input. Similarly to the in vivo case, our in computo simulations show that the scaling exponent reflects the correlation level imposed in the input. This systematic dependence was also replicated at the single cell level, by controlling independently, in a parametric way, the strength and the temporal decay of the pairwise correlation between presynaptic inputs. This last model was implemented in vitro by imposing the correlation control in artificial presynaptic spike trains through dynamic-clamp techniques. These in vitro manipulations induced a modulation of the scaling exponent, similar to that observed in vivo and predicted in computo. We conclude that the frequency-scaling exponent of the V(m) reflects stimulus-driven correlations in the cortical network activity. Therefore, we propose that the scaling exponent could be used to read-out the "effective" connectivity responsible for the dynamical signature of the population signals measured

  4. Frequency-dependent scaling from mesoscale to macroscale in viscoelastic random composites

    PubMed Central

    Zhang, Jun

    2016-01-01

    This paper investigates the scaling from a statistical volume element (SVE; i.e. mesoscale level) to representative volume element (RVE; i.e. macroscale level) of spatially random linear viscoelastic materials, focusing on the quasi-static properties in the frequency domain. Requiring the material statistics to be spatially homogeneous and ergodic, the mesoscale bounds on the RVE response are developed from the Hill–Mandel homogenization condition adapted to viscoelastic materials. The bounds are obtained from two stochastic initial-boundary value problems set up, respectively, under uniform kinematic and traction boundary conditions. The frequency and scale dependencies of mesoscale bounds are obtained through computational mechanics for composites with planar random chessboard microstructures. In general, the frequency-dependent scaling to RVE can be described through a complex-valued scaling function, which generalizes the concept originally developed for linear elastic random composites. This scaling function is shown to apply for all different phase combinations on random chessboards and, essentially, is only a function of the microstructure and mesoscale. PMID:27274689

  5. Scaling laws and fluctuations in the statistics of word frequencies

    NASA Astrophysics Data System (ADS)

    Gerlach, Martin; Altmann, Eduardo G.

    2014-11-01

    In this paper, we combine statistical analysis of written texts and simple stochastic models to explain the appearance of scaling laws in the statistics of word frequencies. The average vocabulary of an ensemble of fixed-length texts is known to scale sublinearly with the total number of words (Heaps’ law). Analyzing the fluctuations around this average in three large databases (Google-ngram, English Wikipedia, and a collection of scientific articles), we find that the standard deviation scales linearly with the average (Taylor's law), in contrast to the prediction of decaying fluctuations obtained using simple sampling arguments. We explain both scaling laws (Heaps’ and Taylor) by modeling the usage of words using a Poisson process with a fat-tailed distribution of word frequencies (Zipf's law) and topic-dependent frequencies of individual words (as in topic models). Considering topical variations lead to quenched averages, turn the vocabulary size a non-self-averaging quantity, and explain the empirical observations. For the numerous practical applications relying on estimations of vocabulary size, our results show that uncertainties remain large even for long texts. We show how to account for these uncertainties in measurements of lexical richness of texts with different lengths.

  6. Kinetic scale structure of low-frequency waves and fluctuations

    NASA Astrophysics Data System (ADS)

    Lopez Herrera, R. A.; Figueroa-Vinas, A.; Araneda, J. A.; Yoon, P. H.

    2017-12-01

    The dissipation of solar wind turbulence at kinetic scales is believed to be important for heating the corona and accelerating the wind. Linear Vlasov kinetic theory is a useful tool in identifying various wave modes, including kinetic Alfvén, fast magnetosonic/whistler, ion-acoustic (or kinetic slow mode), and their possible roles in the dissipation. However, kinetic mode structure near the vicinity of ion cyclotron modes is not clearly understood. The present poster aims to further elucidate the structure of these low-frequency waves by introducing discrete particle effects through hybrid simulations and Klimontovich formalism of spontaneous emission theory. The theory and simulation of spontaneously emitted low-frequency fluctuations are employed to identify and distinguish the detailed mode structures associated with ion Bernstein versus quasi modes. The spontaneous emission theory and simulation also confirm the findings of Vlasov theory in that the kinetic Alfvén wave can be defined over a wide range of frequencies, including the proton cyclotron frequency and its harmonics, especially for high beta plasmas. This implies that these low-frequency modes may play predominant roles even in the fully kinetic description of kinetic scale turbulence and dissipation despite the fact that cyclotron harmonic and Bernstein modes may also play important roles in wave-particle interactions.

  7. Kinetic Scale Structure of Low-frequency Waves and Fluctuations

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

    López, Rodrigo A.; Yoon, Peter H.; Viñas, Adolfo F.

    The dissipation of solar wind turbulence at kinetic scales is believed to be important for the heating of the corona and for accelerating the wind. The linear Vlasov kinetic theory is a useful tool for identifying various wave modes, including kinetic Alfvén, fast magnetosonic/whistler, and ion-acoustic (or kinetic slow), and their possible roles in the dissipation. However, the kinetic mode structure in the vicinity of ion-cyclotron modes is not clearly understood. The present paper aims to further elucidate the structure of these low-frequency waves by introducing discrete particle effects through hybrid simulations and Klimontovich formalism of spontaneous emission theory. Themore » theory and simulation of spontaneously emitted low-frequency fluctuations are employed to identify and distinguish the detailed mode structures associated with ion-Bernstein modes versus quasi-modes. The spontaneous emission theory and simulation also confirm the findings of the Vlasov theory in that the kinetic Alfvén waves can be defined over a wide range of frequencies, including the proton cyclotron frequency and its harmonics, especially for high-beta plasmas. This implies that these low-frequency modes may play predominant roles even in the fully kinetic description of kinetic scale turbulence and dissipation despite the fact that cyclotron harmonic and Bernstein modes may also play important roles in wave–particle interactions.« less

  8. Micro-scale piezoelectric vibration energy harvesting: From fixed-frequency to adaptable-frequency devices

    NASA Astrophysics Data System (ADS)

    Miller, Lindsay Margaret

    hundred milliwatts and are falling steadily as improvements are made, it is feasible to use energy harvesting to power WSNs. This research begins by presenting the results of a thorough survey of ambient vibrations in the machine room of a large campus building, which found that ambient vibrations are low frequency, low amplitude, time varying, and multi-frequency. The modeling and design of fixed-frequency micro scale energy harvesters are then presented. The model is able to take into account rotational inertia of the harvester's proof mass and it accepts arbitrary measured acceleration input, calculating the energy harvester's voltage as an output. The fabrication of the micro electromechanical system (MEMS) energy harvesters is discussed and results of the devices harvesting energy from ambient vibrations are presented. The harvesters had resonance frequencies ranging from 31 - 232 Hz, which was the lowest reported in literature for a MEMS device, and produced 24 pW/g2 - 10 nW/g2 of harvested power from ambient vibrations. A novel method for frequency modification of the released harvester devices using a dispenser printed mass is then presented, demonstrating a frequency shift of 20 Hz. Optimization of the MEMS energy harvester connected to a resistive load is then presented, finding that the harvested power output can be increased to several microwatts with the optimized design as long as the driving frequency matches the harvester's resonance frequency. A framework is then presented to allow a similar optimization to be conducted with the harvester connected to a synchronously switched pre-bias circuit. With the realization that the optimized energy harvester only produces usable amounts of power if the resonance frequency and driving frequency match, which is an unrealistic situation in the case of ambient vibrations which change over time and are not always known a priori, an adaptable-frequency energy harvester was designed. The adaptable-frequency

  9. Effect of Logarithmic and Linear Frequency Scales on Parametric Modelling of Tissue Dielectric Data.

    PubMed

    Salahuddin, Saqib; Porter, Emily; Meaney, Paul M; O'Halloran, Martin

    2017-02-01

    The dielectric properties of biological tissues have been studied widely over the past half-century. These properties are used in a vast array of applications, from determining the safety of wireless telecommunication devices to the design and optimisation of medical devices. The frequency-dependent dielectric properties are represented in closed-form parametric models, such as the Cole-Cole model, for use in numerical simulations which examine the interaction of electromagnetic (EM) fields with the human body. In general, the accuracy of EM simulations depends upon the accuracy of the tissue dielectric models. Typically, dielectric properties are measured using a linear frequency scale; however, use of the logarithmic scale has been suggested historically to be more biologically descriptive. Thus, the aim of this paper is to quantitatively compare the Cole-Cole fitting of broadband tissue dielectric measurements collected with both linear and logarithmic frequency scales. In this way, we can determine if appropriate choice of scale can minimise the fit error and thus reduce the overall error in simulations. Using a well-established fundamental statistical framework, the results of the fitting for both scales are quantified. It is found that commonly used performance metrics, such as the average fractional error, are unable to examine the effect of frequency scale on the fitting results due to the averaging effect that obscures large localised errors. This work demonstrates that the broadband fit for these tissues is quantitatively improved when the given data is measured with a logarithmic frequency scale rather than a linear scale, underscoring the importance of frequency scale selection in accurate wideband dielectric modelling of human tissues.

  10. Effect of Logarithmic and Linear Frequency Scales on Parametric Modelling of Tissue Dielectric Data

    PubMed Central

    Salahuddin, Saqib; Porter, Emily; Meaney, Paul M.; O’Halloran, Martin

    2016-01-01

    The dielectric properties of biological tissues have been studied widely over the past half-century. These properties are used in a vast array of applications, from determining the safety of wireless telecommunication devices to the design and optimisation of medical devices. The frequency-dependent dielectric properties are represented in closed-form parametric models, such as the Cole-Cole model, for use in numerical simulations which examine the interaction of electromagnetic (EM) fields with the human body. In general, the accuracy of EM simulations depends upon the accuracy of the tissue dielectric models. Typically, dielectric properties are measured using a linear frequency scale; however, use of the logarithmic scale has been suggested historically to be more biologically descriptive. Thus, the aim of this paper is to quantitatively compare the Cole-Cole fitting of broadband tissue dielectric measurements collected with both linear and logarithmic frequency scales. In this way, we can determine if appropriate choice of scale can minimise the fit error and thus reduce the overall error in simulations. Using a well-established fundamental statistical framework, the results of the fitting for both scales are quantified. It is found that commonly used performance metrics, such as the average fractional error, are unable to examine the effect of frequency scale on the fitting results due to the averaging effect that obscures large localised errors. This work demonstrates that the broadband fit for these tissues is quantitatively improved when the given data is measured with a logarithmic frequency scale rather than a linear scale, underscoring the importance of frequency scale selection in accurate wideband dielectric modelling of human tissues. PMID:28191324

  11. Acoustic Treatment Design Scaling Methods. Volume 2; Advanced Treatment Impedance Models for High Frequency Ranges

    NASA Technical Reports Server (NTRS)

    Kraft, R. E.; Yu, J.; Kwan, H. W.

    1999-01-01

    The primary purpose of this study is to develop improved models for the acoustic impedance of treatment panels at high frequencies, for application to subscale treatment designs. Effects that cause significant deviation of the impedance from simple geometric scaling are examined in detail, an improved high-frequency impedance model is developed, and the improved model is correlated with high-frequency impedance measurements. Only single-degree-of-freedom honeycomb sandwich resonator panels with either perforated sheet or "linear" wiremesh faceplates are considered. The objective is to understand those effects that cause the simple single-degree-of- freedom resonator panels to deviate at the higher-scaled frequency from the impedance that would be obtained at the corresponding full-scale frequency. This will allow the subscale panel to be designed to achieve a specified impedance spectrum over at least a limited range of frequencies. An advanced impedance prediction model has been developed that accounts for some of the known effects at high frequency that have previously been ignored as a small source of error for full-scale frequency ranges.

  12. Spanish adaptation of social withdrawal motivation and frequency scales.

    PubMed

    Indias García, Sílvia; De Paúl Ochotorena, Joaquín

    2016-11-01

    To adapt into Spanish three scales measuring frequency (SWFS) and motivation for social withdrawal (CSPS and SWMS) and to develop a scale capable of assessing the five motivations for social withdrawal. Participants were 1,112 Spanish adolescents, aged 12-17 years. The sample was randomly split into two groups in which exploratory and confirmatory (CFA) factor analyses were performed separately. A sample of adolescents in residential care (n = 128) was also used to perform discriminant validity analyses. SWFS was reduced to eight items that account for 40% of explained variance (PVE), and its reliability is high. SWMS worked adequately in the original version, according to CFA. Some items from the CSPS were removed from the final Spanish version. The newly developed scale (SWMS-5D) is composed of 20 items including five subscales: Peer Isolation, Unsociability, Shyness, Low Mood and Avoidance. Analyses reveal adequate convergent and discriminant validities. The resulting SWFS-8 and SWMS-5D could be considered useful instruments to assess frequency and motivation for social withdrawal in Spanish samples.

  13. Climate, orography and scale controls on flood frequency in Triveneto (Italy)

    NASA Astrophysics Data System (ADS)

    Persiano, Simone; Castellarin, Attilio; Salinas, Jose Luis; Domeneghetti, Alessio; Brath, Armando

    2016-05-01

    The growing concern about the possible effects of climate change on flood frequency regime is leading Authorities to review previously proposed reference procedures for design-flood estimation, such as national flood frequency models. Our study focuses on Triveneto, a broad geographical region in North-eastern Italy. A reference procedure for design flood estimation in Triveneto is available from the Italian NCR research project "VA.PI.", which considered Triveneto as a single homogeneous region and developed a regional model using annual maximum series (AMS) of peak discharges that were collected up to the 1980s by the former Italian Hydrometeorological Service. We consider a very detailed AMS database that we recently compiled for 76 catchments located in Triveneto. All 76 study catchments are characterized in terms of several geomorphologic and climatic descriptors. The objective of our study is threefold: (1) to inspect climatic and scale controls on flood frequency regime; (2) to verify the possible presence of changes in flood frequency regime by looking at changes in time of regional L-moments of annual maximum floods; (3) to develop an updated reference procedure for design flood estimation in Triveneto by using a focused-pooling approach (i.e. Region of Influence, RoI). Our study leads to the following conclusions: (1) climatic and scale controls on flood frequency regime in Triveneto are similar to the controls that were recently found in Europe; (2) a single year characterized by extreme floods can have a remarkable influence on regional flood frequency models and analyses for detecting possible changes in flood frequency regime; (3) no significant change was detected in the flood frequency regime, yet an update of the existing reference procedure for design flood estimation is highly recommended and we propose the RoI approach for properly representing climate and scale controls on flood frequency in Triveneto, which cannot be regarded as a single

  14. Subgrid-scale parameterization and low-frequency variability: a response theory approach

    NASA Astrophysics Data System (ADS)

    Demaeyer, Jonathan; Vannitsem, Stéphane

    2016-04-01

    Weather and climate models are limited in the possible range of resolved spatial and temporal scales. However, due to the huge space- and time-scale ranges involved in the Earth System dynamics, the effects of many sub-grid processes should be parameterized. These parameterizations have an impact on the forecasts or projections. It could also affect the low-frequency variability present in the system (such as the one associated to ENSO or NAO). An important question is therefore to know what is the impact of stochastic parameterizations on the Low-Frequency Variability generated by the system and its model representation. In this context, we consider a stochastic subgrid-scale parameterization based on the Ruelle's response theory and proposed in Wouters and Lucarini (2012). We test this approach in the context of a low-order coupled ocean-atmosphere model, detailed in Vannitsem et al. (2015), for which a part of the atmospheric modes is considered as unresolved. A natural separation of the phase-space into a slow invariant set and its fast complement allows for an analytical derivation of the different terms involved in the parameterization, namely the average, the fluctuation and the long memory terms. Its application to the low-order system reveals that a considerable correction of the low-frequency variability along the invariant subset can be obtained. This new approach of scale separation opens new avenues of subgrid-scale parameterizations in multiscale systems used for climate forecasts. References: Vannitsem S, Demaeyer J, De Cruz L, Ghil M. 2015. Low-frequency variability and heat transport in a low-order nonlinear coupled ocean-atmosphere model. Physica D: Nonlinear Phenomena 309: 71-85. Wouters J, Lucarini V. 2012. Disentangling multi-level systems: averaging, correlations and memory. Journal of Statistical Mechanics: Theory and Experiment 2012(03): P03 003.

  15. Combining agreement and frequency rating scales to optimize psychometrics in measuring behavioral health functioning.

    PubMed

    Marfeo, Elizabeth E; Ni, Pengsheng; Chan, Leighton; Rasch, Elizabeth K; Jette, Alan M

    2014-07-01

    The goal of this article was to investigate optimal functioning of using frequency vs. agreement rating scales in two subdomains of the newly developed Work Disability Functional Assessment Battery: the Mood & Emotions and Behavioral Control scales. A psychometric study comparing rating scale performance embedded in a cross-sectional survey used for developing a new instrument to measure behavioral health functioning among adults applying for disability benefits in the United States was performed. Within the sample of 1,017 respondents, the range of response category endorsement was similar for both frequency and agreement item types for both scales. There were fewer missing values in the frequency items than the agreement items. Both frequency and agreement items showed acceptable reliability. The frequency items demonstrated optimal effectiveness around the mean ± 1-2 standard deviation score range; the agreement items performed better at the extreme score ranges. Findings suggest an optimal response format requires a mix of both agreement-based and frequency-based items. Frequency items perform better in the normal range of responses, capturing specific behaviors, reactions, or situations that may elicit a specific response. Agreement items do better for those whose scores are more extreme and capture subjective content related to general attitudes, behaviors, or feelings of work-related behavioral health functioning. Copyright © 2014 Elsevier Inc. All rights reserved.

  16. Exploiting variability for energy optimization of parallel programs

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

    Lavrijsen, Wim; Iancu, Costin; de Jong, Wibe

    2016-04-18

    Here in this paper we present optimizations that use DVFS mechanisms to reduce the total energy usage in scientific applications. Our main insight is that noise is intrinsic to large scale parallel executions and it appears whenever shared resources are contended. The presence of noise allows us to identify and manipulate any program regions amenable to DVFS. When compared to previous energy optimizations that make per core decisions using predictions of the running time, our scheme uses a qualitative approach to recognize the signature of executions amenable to DVFS. By recognizing the "shape of variability" we can optimize codes withmore » highly dynamic behavior, which pose challenges to all existing DVFS techniques. We validate our approach using offline and online analyses for one-sided and two-sided communication paradigms. We have applied our methods to NWChem, and we show best case improvements in energy use of 12% at no loss in performance when using online optimizations running on 720 Haswell cores with one-sided communication. With NWChem on MPI two-sided and offline analysis, capturing the initialization, we find energy savings of up to 20%, with less than 1% performance cost.« less

  17. Large-scale derived flood frequency analysis based on continuous simulation

    NASA Astrophysics Data System (ADS)

    Dung Nguyen, Viet; Hundecha, Yeshewatesfa; Guse, Björn; Vorogushyn, Sergiy; Merz, Bruno

    2016-04-01

    There is an increasing need for spatially consistent flood risk assessments at the regional scale (several 100.000 km2), in particular in the insurance industry and for national risk reduction strategies. However, most large-scale flood risk assessments are composed of smaller-scale assessments and show spatial inconsistencies. To overcome this deficit, a large-scale flood model composed of a weather generator and catchments models was developed reflecting the spatially inherent heterogeneity. The weather generator is a multisite and multivariate stochastic model capable of generating synthetic meteorological fields (precipitation, temperature, etc.) at daily resolution for the regional scale. These fields respect the observed autocorrelation, spatial correlation and co-variance between the variables. They are used as input into catchment models. A long-term simulation of this combined system enables to derive very long discharge series at many catchment locations serving as a basic for spatially consistent flood risk estimates at the regional scale. This combined model was set up and validated for major river catchments in Germany. The weather generator was trained by 53-year observation data at 528 stations covering not only the complete Germany but also parts of France, Switzerland, Czech Republic and Australia with the aggregated spatial scale of 443,931 km2. 10.000 years of daily meteorological fields for the study area were generated. Likewise, rainfall-runoff simulations with SWIM were performed for the entire Elbe, Rhine, Weser, Donau and Ems catchments. The validation results illustrate a good performance of the combined system, as the simulated flood magnitudes and frequencies agree well with the observed flood data. Based on continuous simulation this model chain is then used to estimate flood quantiles for the whole Germany including upstream headwater catchments in neighbouring countries. This continuous large scale approach overcomes the several

  18. Industrial-scale radio frequency treatments for insect control in lentils

    USDA-ARS?s Scientific Manuscript database

    Radio frequency (RF) treatments are considered to be a potential postharvest technology for disinfesting legumes of internal seed pests such as the cowpea weevil. After treatment protocols are shown to control postharvest insects without significant quality degradation, it is important to scale-up l...

  19. Large-scale frequency- and time-domain quantum entanglement over the optical frequency comb (Conference Presentation)

    NASA Astrophysics Data System (ADS)

    Pfister, Olivier

    2017-05-01

    When it comes to practical quantum computing, the two main challenges are circumventing decoherence (devastating quantum errors due to interactions with the environmental bath) and achieving scalability (as many qubits as needed for a real-life, game-changing computation). We show that using, in lieu of qubits, the "qumodes" represented by the resonant fields of the quantum optical frequency comb of an optical parametric oscillator allows one to create bona fide, large scale quantum computing processors, pre-entangled in a cluster state. We detail our recent demonstration of 60-qumode entanglement (out of an estimated 3000) and present an extension to combining this frequency-tagged with time-tagged entanglement, in order to generate an arbitrarily large, universal quantum computing processor.

  20. Multi-Frequency Signal Detection Based on Frequency Exchange and Re-Scaling Stochastic Resonance and Its Application to Weak Fault Diagnosis.

    PubMed

    Liu, Jinjun; Leng, Yonggang; Lai, Zhihui; Fan, Shengbo

    2018-04-25

    Mechanical fault diagnosis usually requires not only identification of the fault characteristic frequency, but also detection of its second and/or higher harmonics. However, it is difficult to detect a multi-frequency fault signal through the existing Stochastic Resonance (SR) methods, because the characteristic frequency of the fault signal as well as its second and higher harmonics frequencies tend to be large parameters. To solve the problem, this paper proposes a multi-frequency signal detection method based on Frequency Exchange and Re-scaling Stochastic Resonance (FERSR). In the method, frequency exchange is implemented using filtering technique and Single SideBand (SSB) modulation. This new method can overcome the limitation of "sampling ratio" which is the ratio of the sampling frequency to the frequency of target signal. It also ensures that the multi-frequency target signals can be processed to meet the small-parameter conditions. Simulation results demonstrate that the method shows good performance for detecting a multi-frequency signal with low sampling ratio. Two practical cases are employed to further validate the effectiveness and applicability of this method.

  1. Multi-Frequency Signal Detection Based on Frequency Exchange and Re-Scaling Stochastic Resonance and Its Application to Weak Fault Diagnosis

    PubMed Central

    Leng, Yonggang; Fan, Shengbo

    2018-01-01

    Mechanical fault diagnosis usually requires not only identification of the fault characteristic frequency, but also detection of its second and/or higher harmonics. However, it is difficult to detect a multi-frequency fault signal through the existing Stochastic Resonance (SR) methods, because the characteristic frequency of the fault signal as well as its second and higher harmonics frequencies tend to be large parameters. To solve the problem, this paper proposes a multi-frequency signal detection method based on Frequency Exchange and Re-scaling Stochastic Resonance (FERSR). In the method, frequency exchange is implemented using filtering technique and Single SideBand (SSB) modulation. This new method can overcome the limitation of "sampling ratio" which is the ratio of the sampling frequency to the frequency of target signal. It also ensures that the multi-frequency target signals can be processed to meet the small-parameter conditions. Simulation results demonstrate that the method shows good performance for detecting a multi-frequency signal with low sampling ratio. Two practical cases are employed to further validate the effectiveness and applicability of this method. PMID:29693577

  2. Insights in Low Frequency Earthquake Source Processes from Observations of Their Size-Duration Scaling

    NASA Astrophysics Data System (ADS)

    Farge, G.; Shapiro, N.; Frank, W.; Mercury, N.; Vilotte, J. P.

    2017-12-01

    Low frequency earthquakes (LFE) are detected in association with volcanic and tectonic tremor signals as impulsive, repeated, low frequency (1-5 Hz) events originating from localized sources. While the mechanism causing this depletion of the high frequency content of their signal is still unknown, this feature may indicate that the source processes at the origin of LFE are different from those for regular earthquakes. Tectonic LFE are often associated with slip instabilities in the brittle-ductile transition zones of active faults and volcanic LFE with fluid transport in magmatic and hydrothermal systems. Key constraints on the LFE-generating physical mechanisms can be obtained by establishing scaling laws between their sizes and durations. We apply a simple spectral analysis method to the S-waveforms of each LFE to retrieve its seismic moment and corner frequency. The former characterizes the earthquake's size while the latter is inversely proportional to its duration. First, we analyze a selection of tectonic LFE from the Mexican "Sweet Spot" (Guerrero, Mexico). We find characteristic values of M ˜ 1013 N.m (Mw ˜ 2.6) and fc ˜ 2 Hz. The moment-corner frequency distribution compared to values reported in previous studies in tectonic contexts is consistent with the scaling law suggested by Bostock et al. (2015): fc ˜ M-1/10 . We then apply the same source- parameters determination method to deep volcanic LFE detected in the Klyuchevskoy volcanic group in Kamtchatka, Russia. While the seismic moments for these earthquakes are slightly smaller, they still approximately follow the fc ˜ M-1/10 scaling. This size-duration scaling observed for LFE is very different from the one established for regular earthquakes (fc ˜ M-1/3) and from the scaling more recently suggested by Ide et al. (2007) for the broad class of "slow earthquakes". The scaling observed for LFE suggests that they are generated by sources of nearly constant size with strongly varying intensities

  3. Scaling behavior of EEG amplitude and frequency time series across sleep stages

    NASA Astrophysics Data System (ADS)

    Kantelhardt, Jan W.; Tismer, Sebastian; Gans, Fabian; Schumann, Aicko Y.; Penzel, Thomas

    2015-10-01

    We study short-term and long-term persistence properties (related with auto-correlations) of amplitudes and frequencies of EEG oscillations in 176 healthy subjects and 40 patients during nocturnal sleep. The amplitudes show scaling from 2 to 500 seconds (depending on the considered band) with large fluctuation exponents during (nocturnal) wakefulness (0.73-0.83) and small ones during deep sleep (0.50-0.69). Light sleep is similar to deep sleep, while REM sleep (0.64-0.76) is closer to wakefulness except for the EEG γ band. Some of the frequency time series also show long-term scaling, depending on the selected bands and stages. Only minor deviations are seen for patients with depression, anxiety, or Parkinson's disease.

  4. Cross-sectional fluctuation scaling in the high-frequency illiquidity of Chinese stocks

    NASA Astrophysics Data System (ADS)

    Cai, Qing; Gao, Xing-Lu; Zhou, Wei-Xing; Stanley, H. Eugene

    2018-03-01

    Taylor's law of temporal and ensemble fluctuation scaling has been ubiquitously observed in diverse complex systems including financial markets. Stock illiquidity is an important nonadditive financial quantity, which is found to comply with Taylor's temporal fluctuation scaling law. In this paper, we perform the cross-sectional analysis of the 1 min high-frequency illiquidity time series of Chinese stocks and unveil the presence of Taylor's law of ensemble fluctuation scaling. The estimated daily Taylor scaling exponent fluctuates around 1.442. We find that Taylor's scaling exponents of stock illiquidity do not relate to the ensemble mean and ensemble variety of returns. Our analysis uncovers a new scaling law of financial markets and might stimulate further investigations for a better understanding of financial markets' dynamics.

  5. Comparison of manual scaled and predicted foE and foF1 critical frequencies. Technical report

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

    Gamache, R.R.; Kersey, W.T.

    1990-07-01

    The CCIR and Titheridge foE critical frequency prediction routines were tested by comparison with 1875 manually scaled values. The foF1 critical frequency prediction routine of Millman et al was tested by comparison with 1005 manually scaled values. Plots and statistics of the comparisons are presented and discussed. From the results recommendations are made to help improve autoscaling.

  6. Detecting damage in full-scale honeycomb sandwich composite curved fuselage panels through frequency response

    NASA Astrophysics Data System (ADS)

    Leone, Frank A., Jr.; Ozevin, Didem; Mosinyi, Bao; Bakuckas, John G., Jr.; Awerbuch, Jonathan; Lau, Alan; Tan, Tein-Min

    2008-03-01

    Preliminary tests were conducted using frequency response (FR) characteristics to determine damage initiation and growth in a honeycomb sandwich graphite/epoxy curved panel. This investigation was part of a more general study investigating the damage tolerance characteristics of several such panels subjected to quasi-static internal pressurization combined with hoop and axial loading. The panels were tested at the Full-Scale Aircraft Structural Test Evaluation and Research (FASTER) facility located at the Federal Aviation Administration William J. Hughes Technical Center in Atlantic City, NJ. The overall program objective was to investigate the damage tolerance characteristics of full-scale composite curved aircraft fuselage panels and the evolution of damage under quasi-static loading up to failure. This paper focuses on one aspect of this comprehensive investigation: the effect of state-of-damage on the characteristics of the frequency response of the subject material. The results presented herein show that recording the frequency response could be used for real-time monitoring of damage growth and in determining damage severity in full-scale composites fuselage aircraft structures.

  7. Software and Critical Technology Protection Against Side-Channel Analysis Through Dynamic Hardware Obfuscation

    DTIC Science & Technology

    2011-03-01

    resampling a second time . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82 70 Plot of RSA bitgroup exponentiation with DAILMOM after a...14 DVFS Dynamic Voltage and Frequency Switching . . . . . . . . . . . . . . . . . . . 14 MDPL Masked Dual-Rail...algorithms to prevent whole-sale discovery of PINs and other simple methods to prevent employee tampering [5]. In time , cryptographic systems have

  8. Chip Scale Atomic Resonator Frequency Stabilization System With Ultra-Low Power Consumption for Optoelectronic Oscillators.

    PubMed

    Zhao, Jianye; Zhang, Yaolin; Lu, Haoyuan; Hou, Dong; Zhang, Shuangyou; Wang, Zhong

    2016-07-01

    We present a long-term chip scale stabilization scheme for optoelectronic oscillators (OEOs) based on a rubidium coherent population trapping (CPT) atomic resonator. By locking a single mode of an OEO to the (85)Rb 3.035-GHz CPT resonance utilizing an improved phase-locked loop (PLL) with a PID regulator, we achieved a chip scale frequency stabilization system for the OEO. The fractional frequency stability of the stabilized OEO by overlapping Allan deviation reaches 6.2 ×10(-11) (1 s) and  ∼ 1.45 ×10 (-11) (1000 s). This scheme avoids a decrease in the extra phase noise performance induced by the electronic connection between the OEO and the microwave reference in common injection locking schemes. The total physical package of the stabilization system is [Formula: see text] and the total power consumption is 400 mW, which provides a chip scale and portable frequency stabilization approach with ultra-low power consumption for OEOs.

  9. A broadband chip-scale optical frequency synthesizer at 2.7 × 10−16 relative uncertainty

    PubMed Central

    Huang, Shu-Wei; Yang, Jinghui; Yu, Mingbin; McGuyer, Bart H.; Kwong, Dim-Lee; Zelevinsky, Tanya; Wong, Chee Wei

    2016-01-01

    Optical frequency combs—coherent light sources that connect optical frequencies with microwave oscillations—have become the enabling tool for precision spectroscopy, optical clockwork, and attosecond physics over the past decades. Current benchmark systems are self-referenced femtosecond mode-locked lasers, but Kerr nonlinear dynamics in high-Q solid-state microresonators has recently demonstrated promising features as alternative platforms. The advance not only fosters studies of chip-scale frequency metrology but also extends the realm of optical frequency combs. We report the full stabilization of chip-scale optical frequency combs. The microcomb’s two degrees of freedom, one of the comb lines and the native 18-GHz comb spacing, are simultaneously phase-locked to known optical and microwave references. Active comb spacing stabilization improves long-term stability by six orders of magnitude, reaching a record instrument-limited residual instability of 3.6mHz/τ. Comparing 46 nitride frequency comb lines with a fiber laser frequency comb, we demonstrate the unprecedented microcomb tooth-to-tooth relative frequency uncertainty down to 50 mHz and 2.7 × 10−16, heralding novel solid-state applications in precision spectroscopy, coherent communications, and astronomical spectrography. PMID:27152341

  10. Correcting Spatial Variance of RCM for GEO SAR Imaging Based on Time-Frequency Scaling.

    PubMed

    Yu, Ze; Lin, Peng; Xiao, Peng; Kang, Lihong; Li, Chunsheng

    2016-07-14

    Compared with low-Earth orbit synthetic aperture radar (SAR), a geosynchronous (GEO) SAR can have a shorter revisit period and vaster coverage. However, relative motion between this SAR and targets is more complicated, which makes range cell migration (RCM) spatially variant along both range and azimuth. As a result, efficient and precise imaging becomes difficult. This paper analyzes and models spatial variance for GEO SAR in the time and frequency domains. A novel algorithm for GEO SAR imaging with a resolution of 2 m in both the ground cross-range and range directions is proposed, which is composed of five steps. The first is to eliminate linear azimuth variance through the first azimuth time scaling. The second is to achieve RCM correction and range compression. The third is to correct residual azimuth variance by the second azimuth time-frequency scaling. The fourth and final steps are to accomplish azimuth focusing and correct geometric distortion. The most important innovation of this algorithm is implementation of the time-frequency scaling to correct high-order azimuth variance. As demonstrated by simulation results, this algorithm can accomplish GEO SAR imaging with good and uniform imaging quality over the entire swath.

  11. Correcting Spatial Variance of RCM for GEO SAR Imaging Based on Time-Frequency Scaling

    PubMed Central

    Yu, Ze; Lin, Peng; Xiao, Peng; Kang, Lihong; Li, Chunsheng

    2016-01-01

    Compared with low-Earth orbit synthetic aperture radar (SAR), a geosynchronous (GEO) SAR can have a shorter revisit period and vaster coverage. However, relative motion between this SAR and targets is more complicated, which makes range cell migration (RCM) spatially variant along both range and azimuth. As a result, efficient and precise imaging becomes difficult. This paper analyzes and models spatial variance for GEO SAR in the time and frequency domains. A novel algorithm for GEO SAR imaging with a resolution of 2 m in both the ground cross-range and range directions is proposed, which is composed of five steps. The first is to eliminate linear azimuth variance through the first azimuth time scaling. The second is to achieve RCM correction and range compression. The third is to correct residual azimuth variance by the second azimuth time-frequency scaling. The fourth and final steps are to accomplish azimuth focusing and correct geometric distortion. The most important innovation of this algorithm is implementation of the time-frequency scaling to correct high-order azimuth variance. As demonstrated by simulation results, this algorithm can accomplish GEO SAR imaging with good and uniform imaging quality over the entire swath. PMID:27428974

  12. Computational thermochemistry: Automated generation of scale factors for vibrational frequencies calculated by electronic structure model chemistries

    NASA Astrophysics Data System (ADS)

    Yu, Haoyu S.; Fiedler, Lucas J.; Alecu, I. M.; Truhlar, Donald G.

    2017-01-01

    We present a Python program, FREQ, for calculating the optimal scale factors for calculating harmonic vibrational frequencies, fundamental vibrational frequencies, and zero-point vibrational energies from electronic structure calculations. The program utilizes a previously published scale factor optimization model (Alecu et al., 2010) to efficiently obtain all three scale factors from a set of computed vibrational harmonic frequencies. In order to obtain the three scale factors, the user only needs to provide zero-point energies of 15 or 6 selected molecules. If the user has access to the Gaussian 09 or Gaussian 03 program, we provide the option for the user to run the program by entering the keywords for a certain method and basis set in the Gaussian 09 or Gaussian 03 program. Four other Python programs, input.py, input6, pbs.py, and pbs6.py, are also provided for generating Gaussian 09 or Gaussian 03 input and PBS files. The program can also be used with data from any other electronic structure package. A manual of how to use this program is included in the code package.

  13. Dependence of exponents on text length versus finite-size scaling for word-frequency distributions

    NASA Astrophysics Data System (ADS)

    Corral, Álvaro; Font-Clos, Francesc

    2017-08-01

    Some authors have recently argued that a finite-size scaling law for the text-length dependence of word-frequency distributions cannot be conceptually valid. Here we give solid quantitative evidence for the validity of this scaling law, using both careful statistical tests and analytical arguments based on the generalized central-limit theorem applied to the moments of the distribution (and obtaining a novel derivation of Heaps' law as a by-product). We also find that the picture of word-frequency distributions with power-law exponents that decrease with text length [X. Yan and P. Minnhagen, Physica A 444, 828 (2016), 10.1016/j.physa.2015.10.082] does not stand with rigorous statistical analysis. Instead, we show that the distributions are perfectly described by power-law tails with stable exponents, whose values are close to 2, in agreement with the classical Zipf's law. Some misconceptions about scaling are also clarified.

  14. Statistical Analysis of Instantaneous Frequency Scaling Factor as Derived from Optical Disdrometer Measurements at VW Bands

    NASA Technical Reports Server (NTRS)

    Zemba, Michael; Nessel, James; Tarasenko, Nicholas; Lane, Steven

    2017-01-01

    Since October 2015, NASA Glenn Research Center (GRC) and the Air Force Research Laboratory (AFRL) have collaboratively operated an RF terrestrial link in Albuquerque, New Mexico to characterize atmospheric propagation phenomena at 72 and 84 GHz. The WV-band Terrestrial Link Experiment (WTLE) consists of coherent transmitters at each frequency on the crest of the Sandia Mountains and a corresponding pair of receivers in south Albuquerque. The beacon receivers provide a direct measurement of the link attenuation, while concurrent weather instrumentation provides a measurement of the atmospheric conditions.Among the available weather instruments is an optical disdrometer which yields an optical measurement of rain rate, as well as droplet size and velocity distributions (DSD, DVD). In particular, the DSD can be used to derive an instantaneous scaling factor (ISF) by which the measured data at one frequency can be scaled to another for example, scaling the 72 GHz to an expected 84 GHz timeseries. Given the availability of both the DSD prediction and the directly observed 84 GHz attenuation, WTLE is thus uniquely able assess DSD-derived instantaneous frequency scaling at the VW-bands. Previous work along these lines has investigated the DSD-derived ISF at Ka and Q-band (20 GHz to 40 GHz) using a satellite beacon receiver experiment in Milan, Italy [1-3]. This work will expand the investigation to terrestrial links in the VW-bands, where the frequency scaling factor is lower and where the link is also much more sensitive to attenuation by rain, clouds, and other atmospheric effects.

  15. Disturbance Frequency Determines Morphology and Community Development in Multi-Species Biofilm at the Landscape Scale

    PubMed Central

    Milferstedt, Kim; Santa-Catalina, Gaëlle; Godon, Jean-Jacques; Escudié, Renaud; Bernet, Nicolas

    2013-01-01

    Many natural and engineered biofilm systems periodically face disturbances. Here we present how the recovery time of a biofilm between disturbances (expressed as disturbance frequency) shapes the development of morphology and community structure in a multi-species biofilm at the landscape scale. It was hypothesized that a high disturbance frequency favors the development of a stable adapted biofilm system while a low disturbance frequency promotes a dynamic biofilm response. Biofilms were grown in laboratory-scale reactors over a period of 55-70 days and exposed to the biocide monochloramine at two frequencies: daily or weekly pulse injections. One untreated reactor served as control. Biofilm morphology and community structure were followed on comparably large biofilm areas at the landscape scale using automated image analysis (spatial gray level dependence matrices) and community fingerprinting (single-strand conformation polymorphisms). We demonstrated that a weekly disturbed biofilm developed a resilient morphology and community structure. Immediately after the disturbance, the biofilm simplified but recovered its initial complex morphology and community structure between two biocide pulses. In the daily treated reactor, one organism largely dominated a morphologically simple and stable biofilm. Disturbances primarily affected the abundance distribution of already present bacterial taxa but did not promote growth of previously undetected organisms. Our work indicates that disturbances can be used as lever to engineer biofilms by maintaining a biofilm between two developmental states. PMID:24303024

  16. Direction of information flow in large-scale resting-state networks is frequency-dependent.

    PubMed

    Hillebrand, Arjan; Tewarie, Prejaas; van Dellen, Edwin; Yu, Meichen; Carbo, Ellen W S; Douw, Linda; Gouw, Alida A; van Straaten, Elisabeth C W; Stam, Cornelis J

    2016-04-05

    Normal brain function requires interactions between spatially separated, and functionally specialized, macroscopic regions, yet the directionality of these interactions in large-scale functional networks is unknown. Magnetoencephalography was used to determine the directionality of these interactions, where directionality was inferred from time series of beamformer-reconstructed estimates of neuronal activation, using a recently proposed measure of phase transfer entropy. We observed well-organized posterior-to-anterior patterns of information flow in the higher-frequency bands (alpha1, alpha2, and beta band), dominated by regions in the visual cortex and posterior default mode network. Opposite patterns of anterior-to-posterior flow were found in the theta band, involving mainly regions in the frontal lobe that were sending information to a more distributed network. Many strong information senders in the theta band were also frequent receivers in the alpha2 band, and vice versa. Our results provide evidence that large-scale resting-state patterns of information flow in the human brain form frequency-dependent reentry loops that are dominated by flow from parieto-occipital cortex to integrative frontal areas in the higher-frequency bands, which is mirrored by a theta band anterior-to-posterior flow.

  17. A holistic approach for large-scale derived flood frequency analysis

    NASA Astrophysics Data System (ADS)

    Dung Nguyen, Viet; Apel, Heiko; Hundecha, Yeshewatesfa; Guse, Björn; Sergiy, Vorogushyn; Merz, Bruno

    2017-04-01

    Spatial consistency, which has been usually disregarded because of the reported methodological difficulties, is increasingly demanded in regional flood hazard (and risk) assessments. This study aims at developing a holistic approach for deriving flood frequency at large scale consistently. A large scale two-component model has been established for simulating very long-term multisite synthetic meteorological fields and flood flow at many gauged and ungauged locations hence reflecting the spatially inherent heterogeneity. The model has been applied for the region of nearly a half million km2 including Germany and parts of nearby countries. The model performance has been multi-objectively examined with a focus on extreme. By this continuous simulation approach, flood quantiles for the studied region have been derived successfully and provide useful input for a comprehensive flood risk study.

  18. Statistical Analysis of Instantaneous Frequency Scaling Factor as Derived from Optical Disdrometer Measurements at V/W Bands

    NASA Technical Reports Server (NTRS)

    Zemba, Michael; Nessel, James; Tarasenko, Nicholas; Lane, Steven

    2017-01-01

    Since October 2015, NASA Glenn Research Center (GRC) and the Air Force Research Laboratory (AFRL) have collaboratively operated an RF terrestrial link in Albuquerque, New Mexico to characterize atmospheric propagation phenomena at 72 and 84 GHz. The W/V-band Terrestrial Link Experiment (WTLE) consists of coherent transmitters at each frequency on the crest of the Sandia Mountains and a corresponding pair of receivers in south Albuquerque. The beacon receivers provide a direct measurement of the link attenuation, while concurrent weather instrumentation provides a measurement of the atmospheric conditions. Among the available weather instruments is an optical disdrometer which yields an optical measurement of rain rate, as well as droplet size and velocity distributions (DSD, DVD). In particular, the DSD can be used to derive an instantaneous scaling factor (ISF) by which the measured data at one frequency can be scaled to another - for example, scaling the 72 GHz to an expected 84 GHz timeseries. Given the availability of both the DSD prediction and the directly observed 84 GHz attenuation, WTLE is thus uniquely able assess DSD-derived instantaneous frequency scaling at the V/W-bands. Previous work along these lines has investigated the DSD-derived ISF at Ka and Q-band (20 GHz to 40 GHz) using a satellite beacon receiver experiment in Milan, Italy. This work will expand the investigation to terrestrial links in the V/W-bands, where the frequency scaling factor is lower and where the link is also much more sensitive to attenuation by rain, clouds, and other atmospheric effects.

  19. Compensatory mechanisms of balance to the scaling of arm-swing frequency.

    PubMed

    Ko, Ji Hyun; Wang, Zheng; Challis, John H; Newell, Karl M

    2015-11-05

    The present study investigated the contribution of the Hof (2007) mechanism 1 (M1-moving the center of pressure (COP) with respect to the vertical projection of the center of mass (COMTotal)); and mechanism 2 (M2-rotating the trunk and upper limbs around the COMTotal) to postural control and the stability of COP-COMTotal cophase as a function of lateral arm-swing frequency. Young adults were instructed to stand still on a force platform while alternating their arm swinging from above the head to the side of their thigh to create perturbations to postural control. Scaling the frequency of arm-swing (random step changes of 0.2 Hz within a bandwidth of 0.2 to 1.6 Hz) increased the SD of COP but decreased the SD of COMTotal. Increments in arm-swing frequency induced a progressive increase in M1 and decrease in M2 in terms of their relative contribution to postural stability. The cophase between COP and COMTotal became more tightly in-phase over increments of arm-swing frequency. These findings show an adaptive compensatory role of M1 and M2 within the stability of COP-COMTotal coupling in the regulation of human balance control. Copyright © 2015 Elsevier Ltd. All rights reserved.

  20. Large-scale transmission-type multifunctional anisotropic coding metasurfaces in millimeter-wave frequencies

    NASA Astrophysics Data System (ADS)

    Cui, Tie Jun; Wu, Rui Yuan; Wu, Wei; Shi, Chuan Bo; Li, Yun Bo

    2017-10-01

    We propose fast and accurate designs to large-scale and low-profile transmission-type anisotropic coding metasurfaces with multiple functions in the millimeter-wave frequencies based on the antenna-array method. The numerical simulation of an anisotropic coding metasurface with the size of 30λ × 30λ by the proposed method takes only 20 min, which however cannot be realized by commercial software due to huge memory usage in personal computers. To inspect the performance of coding metasurfaces in the millimeter-wave band, the working frequency is chosen as 60 GHz. Based on the convolution operations and holographic theory, the proposed multifunctional anisotropic coding metasurface exhibits different effects excited by y-polarized and x-polarized incidences. This study extends the frequency range of coding metasurfaces, filling the gap between microwave and terahertz bands, and implying promising applications in millimeter-wave communication and imaging.

  1. A chip-scale, telecommunications-band frequency conversion interface for quantum emitters.

    PubMed

    Agha, Imad; Ates, Serkan; Davanço, Marcelo; Srinivasan, Kartik

    2013-09-09

    We describe a chip-scale, telecommunications-band frequency conversion interface designed for low-noise operation at wavelengths desirable for common single photon emitters. Four-wave-mixing Bragg scattering in silicon nitride waveguides is used to demonstrate frequency upconversion and downconversion between the 980 nm and 1550 nm wavelength regions, with signal-to-background levels > 10 and conversion efficiency of ≈ -60 dB at low continuous wave input pump powers (< 50 mW). Finite element simulations and the split-step Fourier method indicate that increased input powers of ≈ 10 W (produced by amplified nanosecond pulses, for example) will result in a conversion efficiency > 25 % in existing geometries. Finally, we present waveguide designs that can be used to connect shorter wavelength (637 nm to 852 nm) quantum emitters with 1550 nm.

  2. High-resolution time-frequency representation of EEG data using multi-scale wavelets

    NASA Astrophysics Data System (ADS)

    Li, Yang; Cui, Wei-Gang; Luo, Mei-Lin; Li, Ke; Wang, Lina

    2017-09-01

    An efficient time-varying autoregressive (TVAR) modelling scheme that expands the time-varying parameters onto the multi-scale wavelet basis functions is presented for modelling nonstationary signals and with applications to time-frequency analysis (TFA) of electroencephalogram (EEG) signals. In the new parametric modelling framework, the time-dependent parameters of the TVAR model are locally represented by using a novel multi-scale wavelet decomposition scheme, which can allow the capability to capture the smooth trends as well as track the abrupt changes of time-varying parameters simultaneously. A forward orthogonal least square (FOLS) algorithm aided by mutual information criteria are then applied for sparse model term selection and parameter estimation. Two simulation examples illustrate that the performance of the proposed multi-scale wavelet basis functions outperforms the only single-scale wavelet basis functions or Kalman filter algorithm for many nonstationary processes. Furthermore, an application of the proposed method to a real EEG signal demonstrates the new approach can provide highly time-dependent spectral resolution capability.

  3. Evidence for a scale-limited low-frequency earthquake source process

    NASA Astrophysics Data System (ADS)

    Chestler, S. R.; Creager, K. C.

    2017-04-01

    We calculate the seismic moments for 34,264 low-frequency earthquakes (LFEs) beneath the Olympic Peninsula, Washington. LFE moments range from 1.4 × 1010 to 1.9 × 1012 N m (Mw = 0.7-2.1). While regular earthquakes follow a power law moment-frequency distribution with a b value near 1 (the number of events increases by a factor of 10 for each unit increase in Mw), we find that while for large LFEs the b value is 6, for small LFEs it is <1. The magnitude-frequency distribution for all LFEs is best fit by an exponential distribution with a mean seismic moment (characteristic moment) of 2.0 × 1011 N m. The moment-frequency distributions for each of the 43 LFE families, or spots on the plate interface where LFEs repeat, can also be fit by exponential distributions. An exponential moment-frequency distribution implies a scale-limited source process. We consider two end-member models where LFE moment is limited by (1) the amount of slip or (2) slip area. We favor the area-limited model. Based on the observed exponential distribution of LFE moment and geodetically observed total slip, we estimate that the total area that slips within an LFE family has a diameter of 300 m. Assuming an area-limited model, we estimate the slips, subpatch diameters, stress drops, and slip rates for LFEs during episodic tremor and slip events. We allow for LFEs to rupture smaller subpatches within the LFE family patch. Models with 1-10 subpatches produce slips of 0.1-1 mm, subpatch diameters of 80-275 m, and stress drops of 30-1000 kPa. While one subpatch is often assumed, we believe 3-10 subpatches are more likely.

  4. Beyond Word Frequency: Bursts, Lulls, and Scaling in the Temporal Distributions of Words

    PubMed Central

    Altmann, Eduardo G.; Pierrehumbert, Janet B.; Motter, Adilson E.

    2009-01-01

    Background Zipf's discovery that word frequency distributions obey a power law established parallels between biological and physical processes, and language, laying the groundwork for a complex systems perspective on human communication. More recent research has also identified scaling regularities in the dynamics underlying the successive occurrences of events, suggesting the possibility of similar findings for language as well. Methodology/Principal Findings By considering frequent words in USENET discussion groups and in disparate databases where the language has different levels of formality, here we show that the distributions of distances between successive occurrences of the same word display bursty deviations from a Poisson process and are well characterized by a stretched exponential (Weibull) scaling. The extent of this deviation depends strongly on semantic type – a measure of the logicality of each word – and less strongly on frequency. We develop a generative model of this behavior that fully determines the dynamics of word usage. Conclusions/Significance Recurrence patterns of words are well described by a stretched exponential distribution of recurrence times, an empirical scaling that cannot be anticipated from Zipf's law. Because the use of words provides a uniquely precise and powerful lens on human thought and activity, our findings also have implications for other overt manifestations of collective human dynamics. PMID:19907645

  5. SU-E-J-257: A PCA Model to Predict Adaptive Changes for Head&neck Patients Based On Extraction of Geometric Features From Daily CBCT Datasets

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

    Chetvertkov, M; Henry Ford Health System, Detroit, MI; Siddiqui, F

    2015-06-15

    Purpose: Using daily cone beam CTs (CBCTs) to develop principal component analysis (PCA) models of anatomical changes in head and neck (H&N) patients and to assess the possibility of using these prospectively in adaptive radiation therapy (ART). Methods: Planning CT (pCT) images of 4 H&N patients were deformed to model several different systematic changes in patient anatomy during the course of the radiation therapy (RT). A Pinnacle plugin was used to linearly interpolate the systematic change in patient for the 35 fraction RT course and to generate a set of 35 synthetic CBCTs. Each synthetic CBCT represents the systematic changemore » in patient anatomy for each fraction. Deformation vector fields (DVFs) were acquired between the pCT and synthetic CBCTs with random fraction-to-fraction changes were superimposed on the DVFs. A patient-specific PCA model was built using these DVFs containing systematic plus random changes. It was hypothesized that resulting eigenDVFs (EDVFs) with largest eigenvalues represent the major anatomical deformations during the course of treatment. Results: For all 4 patients, the PCA model provided different results depending on the type and size of systematic change in patient’s body. PCA was more successful in capturing the systematic changes early in the treatment course when these were of a larger scale with respect to the random fraction-to-fraction changes in patient’s anatomy. For smaller scale systematic changes, random changes in patient could completely “hide” the systematic change. Conclusion: The leading EDVF from the patientspecific PCA models could tentatively be identified as a major systematic change during treatment if the systematic change is large enough with respect to random fraction-to-fraction changes. Otherwise, leading EDVF could not represent systematic changes reliably. This work is expected to facilitate development of population-based PCA models that can be used to prospectively identify significant

  6. A high-frequency sonar for profiling small-scale subaqueous bedforms

    USGS Publications Warehouse

    Dingler, J.R.; Boylls, J.C.; Lowe, R.L.

    1977-01-01

    A high-resolution ultrasonic profiler has been developed which permits both laboratory and field studies of small-scale subaqueous bedforms. The device uses a 2.5-cm diameter piezoelectric ceramic crystal pulsed at a frequency of 4.5 MHz to obtain vertical accuracy and resolution of at least 1 mm. Compared to other small-scale profiling methods, this ultrasonic technique profiles the bottom more accurately and more rapidly without disturbing the bedforms. These characteristics are vital in wave-dominated nearshore zones where oscillatory flow and low visibility for the most part have stymied detailed bedform studies. In the laboratory the transducer is mounted directly to an instrument carriage. For field work the transducer housing is mounted in a 2 m long aluminum frame which is situated and operated by scuba divers. Observations using the device include ripple geometry and migration, the suspension height of sand during sheet flow, and long-term erosion/deposition at a point. ?? 1977.

  7. Internal Fluid Dynamics and Frequency Scaling of Sweeping Jet Fluidic Oscillators

    NASA Astrophysics Data System (ADS)

    Seo, Jung Hee; Salazar, Erik; Mittal, Rajat

    2017-11-01

    Sweeping jet fluidic oscillators (SJFOs) are devices that produce a spatially oscillating jet solely based on intrinsic flow instability mechanisms without any moving parts. Recently, SJFOs have emerged as effective actuators for flow control, but the internal fluid dynamics of the device that drives the oscillatory flow mechanism is not yet fully understood. In the current study, the internal fluid dynamics of the fluidic oscillator with feedback channels has been investigated by employing incompressible flow simulations. The study is focused on the oscillation mechanisms and scaling laws that underpin the jet oscillation. Based on the simulation results, simple phenomenological models that connect the jet deflection to the feedback flow are developed. Several geometric modifications are considered in order to explore the characteristic length scales and phase relationships associated with the jet oscillation and to assess the proposed phenomenological model. A scaling law for the jet oscillation frequency is proposed based on the detailed analysis. This research is supported by AFOSR Grant FA9550-14-1-0289 monitored by Dr. Douglas Smith.

  8. Multi-Objective Approach for Energy-Aware Workflow Scheduling in Cloud Computing Environments

    PubMed Central

    Kadima, Hubert; Granado, Bertrand

    2013-01-01

    We address the problem of scheduling workflow applications on heterogeneous computing systems like cloud computing infrastructures. In general, the cloud workflow scheduling is a complex optimization problem which requires considering different criteria so as to meet a large number of QoS (Quality of Service) requirements. Traditional research in workflow scheduling mainly focuses on the optimization constrained by time or cost without paying attention to energy consumption. The main contribution of this study is to propose a new approach for multi-objective workflow scheduling in clouds, and present the hybrid PSO algorithm to optimize the scheduling performance. Our method is based on the Dynamic Voltage and Frequency Scaling (DVFS) technique to minimize energy consumption. This technique allows processors to operate in different voltage supply levels by sacrificing clock frequencies. This multiple voltage involves a compromise between the quality of schedules and energy. Simulation results on synthetic and real-world scientific applications highlight the robust performance of the proposed approach. PMID:24319361

  9. Multi-objective approach for energy-aware workflow scheduling in cloud computing environments.

    PubMed

    Yassa, Sonia; Chelouah, Rachid; Kadima, Hubert; Granado, Bertrand

    2013-01-01

    We address the problem of scheduling workflow applications on heterogeneous computing systems like cloud computing infrastructures. In general, the cloud workflow scheduling is a complex optimization problem which requires considering different criteria so as to meet a large number of QoS (Quality of Service) requirements. Traditional research in workflow scheduling mainly focuses on the optimization constrained by time or cost without paying attention to energy consumption. The main contribution of this study is to propose a new approach for multi-objective workflow scheduling in clouds, and present the hybrid PSO algorithm to optimize the scheduling performance. Our method is based on the Dynamic Voltage and Frequency Scaling (DVFS) technique to minimize energy consumption. This technique allows processors to operate in different voltage supply levels by sacrificing clock frequencies. This multiple voltage involves a compromise between the quality of schedules and energy. Simulation results on synthetic and real-world scientific applications highlight the robust performance of the proposed approach.

  10. Statistical Analysis of Instantaneous Frequency Scaling Factor as Derived From Optical Disdrometer Measurements At KQ Bands

    NASA Technical Reports Server (NTRS)

    Zemba, Michael; Nessel, James; Houts, Jacquelynne; Luini, Lorenzo; Riva, Carlo

    2016-01-01

    The rain rate data and statistics of a location are often used in conjunction with models to predict rain attenuation. However, the true attenuation is a function not only of rain rate, but also of the drop size distribution (DSD). Generally, models utilize an average drop size distribution (Laws and Parsons or Marshall and Palmer. However, individual rain events may deviate from these models significantly if their DSD is not well approximated by the average. Therefore, characterizing the relationship between the DSD and attenuation is valuable in improving modeled predictions of rain attenuation statistics. The DSD may also be used to derive the instantaneous frequency scaling factor and thus validate frequency scaling models. Since June of 2014, NASA Glenn Research Center (GRC) and the Politecnico di Milano (POLIMI) have jointly conducted a propagation study in Milan, Italy utilizing the 20 and 40 GHz beacon signals of the Alphasat TDP#5 Aldo Paraboni payload. The Ka- and Q-band beacon receivers provide a direct measurement of the signal attenuation while concurrent weather instrumentation provides measurements of the atmospheric conditions at the receiver. Among these instruments is a Thies Clima Laser Precipitation Monitor (optical disdrometer) which yields droplet size distributions (DSD); this DSD information can be used to derive a scaling factor that scales the measured 20 GHz data to expected 40 GHz attenuation. Given the capability to both predict and directly observe 40 GHz attenuation, this site is uniquely situated to assess and characterize such predictions. Previous work using this data has examined the relationship between the measured drop-size distribution and the measured attenuation of the link]. The focus of this paper now turns to a deeper analysis of the scaling factor, including the prediction error as a function of attenuation level, correlation between the scaling factor and the rain rate, and the temporal variability of the drop size

  11. Statistical Analysis of Instantaneous Frequency Scaling Factor as Derived From Optical Disdrometer Measurements At KQ Bands

    NASA Technical Reports Server (NTRS)

    Zemba, Michael; Nessel, James; Houts, Jacquelynne; Luini, Lorenzo; Riva, Carlo

    2016-01-01

    The rain rate data and statistics of a location are often used in conjunction with models to predict rain attenuation. However, the true attenuation is a function not only of rain rate, but also of the drop size distribution (DSD). Generally, models utilize an average drop size distribution (Laws and Parsons or Marshall and Palmer [1]). However, individual rain events may deviate from these models significantly if their DSD is not well approximated by the average. Therefore, characterizing the relationship between the DSD and attenuation is valuable in improving modeled predictions of rain attenuation statistics. The DSD may also be used to derive the instantaneous frequency scaling factor and thus validate frequency scaling models. Since June of 2014, NASA Glenn Research Center (GRC) and the Politecnico di Milano (POLIMI) have jointly conducted a propagation study in Milan, Italy utilizing the 20 and 40 GHz beacon signals of the Alphasat TDP#5 Aldo Paraboni payload. The Ka- and Q-band beacon receivers provide a direct measurement of the signal attenuation while concurrent weather instrumentation provides measurements of the atmospheric conditions at the receiver. Among these instruments is a Thies Clima Laser Precipitation Monitor (optical disdrometer) which yields droplet size distributions (DSD); this DSD information can be used to derive a scaling factor that scales the measured 20 GHz data to expected 40 GHz attenuation. Given the capability to both predict and directly observe 40 GHz attenuation, this site is uniquely situated to assess and characterize such predictions. Previous work using this data has examined the relationship between the measured drop-size distribution and the measured attenuation of the link [2]. The focus of this paper now turns to a deeper analysis of the scaling factor, including the prediction error as a function of attenuation level, correlation between the scaling factor and the rain rate, and the temporal variability of the drop

  12. A two-scale model of radio-frequency electrosurgical tissue ablation

    NASA Astrophysics Data System (ADS)

    Karaki, Wafaa; Rahul; Lopez, Carlos A.; Borca-Tasciuc, Diana-Andra; De, Suvranu

    2017-12-01

    Radio-frequency electrosurgical procedures are widely used to simultaneously dissect and coagulate tissue. Experiments suggest that evaporation of cellular and intra-cellular water plays a significant role in the evolution of the temperature field at the tissue level, which is not adequately captured in a single scale energy balance equation. Here, we propose a two-scale model to study the effects of microscale phase change and heat dissipation in response to radiofrequency heating on the tissue level in electrosurgical ablation procedures. At the microscale, the conservation of mass along with thermodynamic and mechanical equilibrium is applied to obtain an equation-of-state relating vapor mass fraction to temperature and pressure. The evaporation losses are incorporated in the macro-level energy conservation and results are validated with mean experimental temperature distributions measured from electrosurgical ablation testing on ex vivo porcine liver at different power settings of the electrosurgical instrument. Model prediction of water loss and its effect on the temperature along with the effect of the mechanical properties on results are evaluated and discussed.

  13. An adjustable multi-scale single beam acoustic tweezers based on ultrahigh frequency ultrasonic transducer.

    PubMed

    Chen, Xiaoyang; Lam, Kwok Ho; Chen, Ruimin; Chen, Zeyu; Yu, Ping; Chen, Zhongping; Shung, K Kirk; Zhou, Qifa

    2017-11-01

    This paper reports the fabrication, characterization, and microparticle manipulation capability of an adjustable multi-scale single beam acoustic tweezers (SBAT) that is capable of flexibly changing the size of "tweezers" like ordinary metal tweezers with a single-element ultrahigh frequency (UHF) ultrasonic transducer. The measured resonant frequency of the developed transducer at 526 MHz is the highest frequency of piezoelectric single crystal based ultrasonic transducers ever reported. This focused UHF ultrasonic transducer exhibits a wide bandwidth (95.5% at -10 dB) due to high attenuation of high-frequency ultrasound wave, which allows the SBAT effectively excite with a wide range of excitation frequency from 150 to 400 MHz by using the "piezoelectric actuator" model. Through controlling the excitation frequency, the wavelength of ultrasound emitted from the SBAT can be changed to selectively manipulate a single microparticle of different sizes (3-100 μm) by using only one transducer. This concept of flexibly changing "tweezers" size is firstly introduced into the study of SBAT. At the same time, it was found that this incident ultrasound wavelength play an important role in lateral trapping and manipulation for microparticle of different sizes. Biotechnol. Bioeng. 2017;114: 2637-2647. © 2017 Wiley Periodicals, Inc. © 2017 Wiley Periodicals, Inc.

  14. Real-Time and Meter-Scale Absolute Distance Measurement by Frequency-Comb-Referenced Multi-Wavelength Interferometry.

    PubMed

    Wang, Guochao; Tan, Lilong; Yan, Shuhua

    2018-02-07

    We report on a frequency-comb-referenced absolute interferometer which instantly measures long distance by integrating multi-wavelength interferometry with direct synthetic wavelength interferometry. The reported interferometer utilizes four different wavelengths, simultaneously calibrated to the frequency comb of a femtosecond laser, to implement subwavelength distance measurement, while direct synthetic wavelength interferometry is elaborately introduced by launching a fifth wavelength to extend a non-ambiguous range for meter-scale measurement. A linearity test performed comparatively with a He-Ne laser interferometer shows a residual error of less than 70.8 nm in peak-to-valley over a 3 m distance, and a 10 h distance comparison is demonstrated to gain fractional deviations of ~3 × 10 -8 versus 3 m distance. Test results reveal that the presented absolute interferometer enables precise, stable, and long-term distance measurements and facilitates absolute positioning applications such as large-scale manufacturing and space missions.

  15. The Influence of Various Vibration Frequency on Barium Sulfate Scale Formation Of Vibrated Piping System In The Presence Citric Acid

    NASA Astrophysics Data System (ADS)

    Karaman, N.; Mangestiyono, W.; Muryanto, S.; Jamari, J.; Bayuseno, A. P.

    2018-01-01

    In this paper, the influence of vibrated piping system for BaSO4 scale formation was investigated. The vibration frequency and presence of citric acid were independent variables determining the kinetics, mass deposit and polymorph of the crystals. Correspondingly, induction time and mass of scale were obtained during the experiments. The crystalline scale was observed by scanning electron microscopy (SEM) and X-Ray Diffraction (XRD) to investigate the morphology and the phase mineral deposits, respectively. This effect indicated that the increase in vibration frequency promoted the increased deposition rate, while the pure barite with a plate-like morphology was produced in the experiments.

  16. Study on ion energy distribution in low-frequency oscillation time scale of Hall thrusters

    NASA Astrophysics Data System (ADS)

    Wei, Liqiu; Li, Wenbo; Ding, Yongjie; Han, Liang; Yu, Daren; Cao, Yong

    2017-11-01

    This paper reports on the dynamic characteristics of the distribution of ion energy during Hall thruster discharge in the low-frequency oscillation time scale through experimental studies, and a statistical analysis of the time-varying peak and width of ion energy and the ratio of high-energy ions during the low-frequency oscillation. The results show that the ion energy distribution exhibits a periodic change during the low-frequency oscillation. Moreover, the variation in the ion energy peak is opposite to that of the discharge current, and the variations in width of the ion energy distribution and the ratio of high-energy ions are consistent with that of the discharge current. The variation characteristics of the ion density and discharge potential were simulated by one-dimensional hybrid-direct kinetic simulations; the simulation results and analysis indicate that the periodic change in the distribution of ion energy during the low-frequency oscillation depends on the relationship between the ionization source term and discharge potential distribution during ionization in the discharge channel.

  17. Non-contact multi-frequency magnetic induction spectroscopy system for industrial-scale bio-impedance measurement

    NASA Astrophysics Data System (ADS)

    O'Toole, M. D.; Marsh, L. A.; Davidson, J. L.; Tan, Y. M.; Armitage, D. W.; Peyton, A. J.

    2015-03-01

    Biological tissues have a complex impedance, or bio-impedance, profile which changes with respect to frequency. This is caused by dispersion mechanisms which govern how the electromagnetic field interacts with the tissue at the cellular and molecular level. Measuring the bio-impedance spectra of a biological sample can potentially provide insight into the sample’s properties and its cellular structure. This has obvious applications in the medical, pharmaceutical and food-based industrial domains. However, measuring the bio-impedance spectra non-destructively and in a way which is practical at an industrial scale presents substantial challenges. The low conductivity of the sample requires a highly sensitive instrument, while the demands of industrial-scale operation require a fast high-throughput sensor of rugged design. In this paper, we describe a multi-frequency magnetic induction spectroscopy (MIS) system suitable for industrial-scale, non-contact, spectroscopic bio-impedance measurement over a bandwidth of 156 kHz-2.5 MHz. The system sensitivity and performance are investigated using calibration and known reference samples. It is shown to yield rapid and consistently sensitive results with good long-term stability. The system is then used to obtain conductivity spectra of a number of biological test samples, including yeast suspensions of varying concentration and a range of agricultural produce, such as apples, pears, nectarines, kiwis, potatoes, oranges and tomatoes.

  18. Symptom Frequency Characteristics of the Hamilton Depression Rating Scale of Major Depressive Disorder in Epilepsy.

    PubMed

    Wiglusz, Mariusz S; Landowski, Jerzy; Michalak, Lidia; Cubała, Wiesław J

    2015-09-01

    Depressive disorders are common among patients with epilepsy (PWE). The aim of this study was to explore symptom frequencies of 17-item Hamilton Depression Rating Scale (HDRS-17) and recognize the clinical characteristics of Major Depressive Disorder in PWE. A sample of 40 adults outpatients with epilepsy and depression was diagnosed using SCID-I for DSM-IV-TR and HDRS-17. The total HDRS-17 score was analysed followed by the exploratory analysis based on the hierarchical model. The frequencies of HDRS-17 items varied widely in this study. Insomnia related items and general somatic symptoms items as well as insomnia and somatic factors exhibited constant and higher frequency. Feeling guilty, suicide, psychomotor retardation and depressed mood showed relatively lower frequencies. Other symptoms had variable frequencies across the study population. Depressive disorders are common among PWE. In the study group insomnia and somatic symptoms displayed highest values which could represent atypical clinical features of mood disorders in PWE. There is a need for more studies with a use of standardized approach to the problem.

  19. Real-Time and Meter-Scale Absolute Distance Measurement by Frequency-Comb-Referenced Multi-Wavelength Interferometry

    PubMed Central

    Tan, Lilong; Yan, Shuhua

    2018-01-01

    We report on a frequency-comb-referenced absolute interferometer which instantly measures long distance by integrating multi-wavelength interferometry with direct synthetic wavelength interferometry. The reported interferometer utilizes four different wavelengths, simultaneously calibrated to the frequency comb of a femtosecond laser, to implement subwavelength distance measurement, while direct synthetic wavelength interferometry is elaborately introduced by launching a fifth wavelength to extend a non-ambiguous range for meter-scale measurement. A linearity test performed comparatively with a He–Ne laser interferometer shows a residual error of less than 70.8 nm in peak-to-valley over a 3 m distance, and a 10 h distance comparison is demonstrated to gain fractional deviations of ~3 × 10−8 versus 3 m distance. Test results reveal that the presented absolute interferometer enables precise, stable, and long-term distance measurements and facilitates absolute positioning applications such as large-scale manufacturing and space missions. PMID:29414897

  20. Comparison of Instantaneous Frequency Scaling from Rain Attenuation and Optical Disdrometer Measurements at K/Q bands

    NASA Technical Reports Server (NTRS)

    Nessel, James; Zemba, Michael; Luini, Lorenzo; Riva, Carlo

    2015-01-01

    Rain attenuation is strongly dependent on the rain rate, but also on the rain drop size distribution (DSD). Typically, models utilize an average drop size distribution, such as those developed by Laws and Parsons, or Marshall and Palmer. However, individual rain events may possess drop size distributions which could be significantly different from the average and will impact, for example, fade mitigation techniques which utilize channel performance estimates from a signal at a different frequency. Therefore, a good understanding of the characteristics and variability of the raindrop size distribution is extremely important in predicting rain attenuation and instantaneous frequency scaling parameters on an event-toevent basis. Since June 2014, NASA Glenn Research Center (GRC) and the Politecnico di Milano (POLIMI) have measured the attenuation due to rain in Milan, Italy, on the 20/40 GHz beacon signal broadcast from the Alphasat TDP#5 Aldo Paraboni Q/V-band Payload. Concomitant with these measurements are the measurements of drop size distribution and rain rate utilizing a Thies Clima laser precipitation monitor (disdrometer). In this paper, we discuss the comparison of the predicted rain attenuation at 20 and 40 GHz derived from the drop size distribution data with the measured rain attenuation. The results are compared on statistical and real-time bases. We will investigate the performance of the rain attenuation model, instantaneous frequency scaling, and the distribution of the scaling factor. Further, seasonal rain characteristics will be analysed.

  1. Neural-scaled entropy predicts the effects of nonlinear frequency compression on speech perception

    PubMed Central

    Rallapalli, Varsha H.; Alexander, Joshua M.

    2015-01-01

    The Neural-Scaled Entropy (NSE) model quantifies information in the speech signal that has been altered beyond simple gain adjustments by sensorineural hearing loss (SNHL) and various signal processing. An extension of Cochlear-Scaled Entropy (CSE) [Stilp, Kiefte, Alexander, and Kluender (2010). J. Acoust. Soc. Am. 128(4), 2112–2126], NSE quantifies information as the change in 1-ms neural firing patterns across frequency. To evaluate the model, data from a study that examined nonlinear frequency compression (NFC) in listeners with SNHL were used because NFC can recode the same input information in multiple ways in the output, resulting in different outcomes for different speech classes. Overall, predictions were more accurate for NSE than CSE. The NSE model accurately described the observed degradation in recognition, and lack thereof, for consonants in a vowel-consonant-vowel context that had been processed in different ways by NFC. While NSE accurately predicted recognition of vowel stimuli processed with NFC, it underestimated them relative to a low-pass control condition without NFC. In addition, without modifications, it could not predict the observed improvement in recognition for word final /s/ and /z/. Findings suggest that model modifications that include information from slower modulations might improve predictions across a wider variety of conditions. PMID:26627780

  2. A method to map errors in the deformable registration of 4DCT images1

    PubMed Central

    Vaman, Constantin; Staub, David; Williamson, Jeffrey; Murphy, Martin J.

    2010-01-01

    Purpose: To present a new approach to the problem of estimating errors in deformable image registration (DIR) applied to sequential phases of a 4DCT data set. Methods: A set of displacement vector fields (DVFs) are made by registering a sequence of 4DCT phases. The DVFs are assumed to display anatomical movement, with the addition of errors due to the imaging and registration processes. The positions of physical landmarks in each CT phase are measured as ground truth for the physical movement in the DVF. Principal component analysis of the DVFs and the landmarks is used to identify and separate the eigenmodes of physical movement from the error eigenmodes. By subtracting the physical modes from the principal components of the DVFs, the registration errors are exposed and reconstructed as DIR error maps. The method is demonstrated via a simple numerical model of 4DCT DVFs that combines breathing movement with simulated maps of spatially correlated DIR errors. Results: The principal components of the simulated DVFs were observed to share the basic properties of principal components for actual 4DCT data. The simulated error maps were accurately recovered by the estimation method. Conclusions: Deformable image registration errors can have complex spatial distributions. Consequently, point-by-point landmark validation can give unrepresentative results that do not accurately reflect the registration uncertainties away from the landmarks. The authors are developing a method for mapping the complete spatial distribution of DIR errors using only a small number of ground truth validation landmarks. PMID:21158288

  3. Assessment of multi-frequency electromagnetic induction for determining soil moisture patterns at the hillslope scale

    NASA Astrophysics Data System (ADS)

    Tromp-van Meerveld, H. J.; McDonnell, J. J.

    2009-04-01

    SummaryHillslopes are fundamental landscape units, yet represent a difficult scale for measurements as they are well-beyond our traditional point-scale techniques. Here we present an assessment of electromagnetic induction (EM) as a potential rapid and non-invasive method to map soil moisture patterns at the hillslope scale. We test the new multi-frequency GEM-300 for spatially distributed soil moisture measurements at the well-instrumented Panola hillslope. EM-based apparent conductivity measurements were linearly related to soil moisture measured with the Aqua-pro capacitance sensor below a threshold conductivity and represented the temporal patterns in soil moisture well. During spring rainfall events that wetted only the surface soil layers the apparent conductivity measurements explained the soil moisture dynamics at depth better than the surface soil moisture dynamics. All four EM frequencies (7.290, 9.090, 11.250, and 14.010 kHz) were highly correlated and linearly related to each other and could be used to predict soil moisture. This limited our ability to use the four different EM frequencies to obtain a soil moisture profile with depth. The apparent conductivity patterns represented the observed spatial soil moisture patterns well when the individually fitted relationships between measured soil moisture and apparent conductivity were used for each measurement point. However, when the same (master) relationship was used for all measurement locations, the soil moisture patterns were smoothed and did not resemble the observed soil moisture patterns very well. In addition the range in calculated soil moisture values was reduced compared to observed soil moisture. Part of the smoothing was likely due to the much larger measurement area of the GEM-300 compared to the soil moisture measurements.

  4. Analysis of Frequency of Use of Different Scar Assessment Scales Based on the Scar Condition and Treatment Method

    PubMed Central

    Bae, Seong Hwan

    2014-01-01

    Analysis of scars in various conditions is essential, but no consensus had been reached on the scar assessment scale to select for a given condition. We reviewed papers to determine the scar assessment scale selected depending on the scar condition and treatment method. We searched PubMed for articles published since 2000 with the contents of the scar evaluation using a scar assessment scale with a Journal Citation Report impact factor >0.5. Among them, 96 articles that conducted a scar evaluation using a scar assessment scale were reviewed and analyzed. The scar assessment scales were identified and organized by various criteria. Among the types of scar assessment scales, the Patient and Observer Scar Assessment Scale (POSAS) was found to be the most frequently used scale. As for the assessment of newly developed operative scars, the POSAS was most used. Meanwhile, for categories depending on the treatment methods for preexisting scars, the Vancouver Scar Scale (VSS) was used in 6 studies following a laser treatment, the POSAS was used in 7 studies following surgical treatment, and the POSAS was used in 7 studies following a conservative treatment. Within the 12 categories of scar status, the VSS showed the highest frequency in 6 categories and the POSAS showed the highest frequency in the other 6 categories. According to our reviews, the POSAS and VSS are the most frequently used scar assessment scales. In the future, an optimal, universal scar scoring system is needed in order to better evaluate and treat pathologic scarring. PMID:24665417

  5. Investigating the Small-Scale Spatial Variabilty of Precipitable Water Vapor by Adding Single-Frequency Receivers into an Existing Dual-Frequency Receiver Network

    NASA Astrophysics Data System (ADS)

    Krietemeyer, Andreas; ten Veldhuis, Marie-claire; van de Giesen, Nick

    2017-04-01

    Exploiting GNSS signal delays is one possibility to obtain Precipitable Water Vapor (PWV) estimates in the atmosphere. The technique is well known since the early 1990s and by now an established method in the meteorological community. The data is crucial for weather forecasting and its assimilation into numerical weather forecasting models is a topic of ongoing research. However, the spatial resolution of ground based GNSS receivers is usually low, in the order of tens of kilometres. Since severe weather events such as convective storms can be concentrated in spatial extent, existing GNSS networks are often not sufficient to retrieve small scale PWV fluctuations and need to be densified. For economic reasons, the use of low-cost single-frequency receivers is a promising solution. In this study, we will deploy a network of single-frequency receivers to densify an existing dual-frequency network in order to investigate the spatial and temporal PWV variations. We demonstrate a test network consisting of four single-frequency receivers in the Rotterdam area (Netherlands). In order to eliminate the delay caused by the ionosphere, the Satellite-specific Epoch-differenced Ionospheric Delay model (SEID) is applied, using a surrounding dual-frequency network distributed over a radius of approximately 25 km. With the synthesized L2 frequency, the tropospheric delays are estimated using the Precise Point Positioning (PPP) strategy and International GNSS Service (IGS) final orbits. The PWV time series are validated by a comparison of a collocated single-frequency and a dual-frequency receiver. The time series themselves form the basis for potential further studies like data assimilation into numerical weather models and GNSS tomography to study the impact of the increased spatial resolution on local heavy rain forecast.

  6. Process Inference from High Frequency Temporal Variations in Dissolved Organic Carbon (DOC) Dynamics Across Nested Spatial Scales

    NASA Astrophysics Data System (ADS)

    Tunaley, C.; Tetzlaff, D.; Lessels, J. S.; Soulsby, C.

    2014-12-01

    In order to understand aquatic ecosystem functioning it is critical to understand the processes that control the spatial and temporal variations in DOC. DOC concentrations are highly dynamic, however, our understanding at short, high frequency timescales is still limited. Optical sensors which act as a proxy for DOC provide the opportunity to investigate near-continuous DOC variations in order to understand the hydrological and biogeochemical processes that control concentrations at short temporal scales. Here we present inferred 15 minute stream water DOC data for a 12 month period at three nested scales (1km2, 3km2 and 31km2) for the Bruntland Burn, a headwater catchment in NE Scotland. High frequency data were measured using FDOM and CDOM probes which work by measuring the fluorescent component and coloured component, respectively, of DOC when exposed to ultraviolet light. Both FDOM and CDOM were strongly correlated (r2 >0.8) with DOC allowing high frequency estimations. Results show the close coupling of DOC with discharge throughout the sampling period at all three spatial scales. However, analysis at the event scale highlights anticlockwise hysteresis relationships between DOC and discharge due to the delay in DOC being flushed from the increasingly large areas of peaty soils as saturation zones expand and increase hydrological connectivity. Lag times vary between events dependent on antecedent conditions. During a 10 year drought period in late summer 2013 it was apparent that very small changes in discharge on a 15 minute timescale result in high increases in DOC. This suggests transport limitation during this period where DOC builds up in the soil and is not flushed regularly, therefore any subsequent increase in discharge results in large DOC peaks. The high frequency sensors also reveal diurnal variability during summer months related to the photo-oxidation, evaporative and biological influences of DOC during the day. This relationship is less

  7. Scaling of swim speed and stroke frequency in geometrically similar penguins: they swim optimally to minimize cost of transport

    PubMed Central

    Sato, Katsufumi; Shiomi, Kozue; Watanabe, Yuuki; Watanuki, Yutaka; Takahashi, Akinori; Ponganis, Paul J.

    2010-01-01

    It has been predicted that geometrically similar animals would swim at the same speed with stroke frequency scaling with mass−1/3. In the present study, morphological and behavioural data obtained from free-ranging penguins (seven species) were compared. Morphological measurements support the geometrical similarity. However, cruising speeds of 1.8–2.3 m s−1 were significantly related to mass0.08 and stroke frequencies were proportional to mass−0.29. These scaling relationships do not agree with the previous predictions for geometrically similar animals. We propose a theoretical model, considering metabolic cost, work against mechanical forces (drag and buoyancy), pitch angle and dive depth. This new model predicts that: (i) the optimal swim speed, which minimizes the energy cost of transport, is proportional to (basal metabolic rate/drag)1/3 independent of buoyancy, pitch angle and dive depth; (ii) the optimal speed is related to mass0.05; and (iii) stroke frequency is proportional to mass−0.28. The observed scaling relationships of penguins support these predictions, which suggest that breath-hold divers swam optimally to minimize the cost of transport, including mechanical and metabolic energy during dive. PMID:19906666

  8. High spectral purity Kerr frequency comb radio frequency photonic oscillator

    PubMed Central

    Liang, W.; Eliyahu, D.; Ilchenko, V. S.; Savchenkov, A. A.; Matsko, A. B.; Seidel, D.; Maleki, L.

    2015-01-01

    Femtosecond laser-based generation of radio frequency signals has produced astonishing improvements in achievable spectral purity, one of the basic features characterizing the performance of an radio frequency oscillator. Kerr frequency combs hold promise for transforming these lab-scale oscillators to chip-scale level. In this work we demonstrate a miniature 10 GHz radio frequency photonic oscillator characterized with phase noise better than −60 dBc Hz−1 at 10 Hz, −90 dBc Hz−1 at 100 Hz and −170 dBc Hz−1 at 10 MHz. The frequency stability of this device, as represented by Allan deviation measurements, is at the level of 10−10 at 1–100 s integration time—orders of magnitude better than existing radio frequency photonic devices of similar size, weight and power consumption. PMID:26260955

  9. Feedforward and feedback frequency-dependent interactions in a large-scale laminar network of the primate cortex.

    PubMed

    Mejias, Jorge F; Murray, John D; Kennedy, Henry; Wang, Xiao-Jing

    2016-11-01

    Interactions between top-down and bottom-up processes in the cerebral cortex hold the key to understanding attentional processes, predictive coding, executive control, and a gamut of other brain functions. However, the underlying circuit mechanism remains poorly understood and represents a major challenge in neuroscience. We approached this problem using a large-scale computational model of the primate cortex constrained by new directed and weighted connectivity data. In our model, the interplay between feedforward and feedback signaling depends on the cortical laminar structure and involves complex dynamics across multiple (intralaminar, interlaminar, interareal, and whole cortex) scales. The model was tested by reproducing, as well as providing insights into, a wide range of neurophysiological findings about frequency-dependent interactions between visual cortical areas, including the observation that feedforward pathways are associated with enhanced gamma (30 to 70 Hz) oscillations, whereas feedback projections selectively modulate alpha/low-beta (8 to 15 Hz) oscillations. Furthermore, the model reproduces a functional hierarchy based on frequency-dependent Granger causality analysis of interareal signaling, as reported in recent monkey and human experiments, and suggests a mechanism for the observed context-dependent hierarchy dynamics. Together, this work highlights the necessity of multiscale approaches and provides a modeling platform for studies of large-scale brain circuit dynamics and functions.

  10. Feedforward and feedback frequency-dependent interactions in a large-scale laminar network of the primate cortex

    PubMed Central

    Mejias, Jorge F.; Murray, John D.; Kennedy, Henry; Wang, Xiao-Jing

    2016-01-01

    Interactions between top-down and bottom-up processes in the cerebral cortex hold the key to understanding attentional processes, predictive coding, executive control, and a gamut of other brain functions. However, the underlying circuit mechanism remains poorly understood and represents a major challenge in neuroscience. We approached this problem using a large-scale computational model of the primate cortex constrained by new directed and weighted connectivity data. In our model, the interplay between feedforward and feedback signaling depends on the cortical laminar structure and involves complex dynamics across multiple (intralaminar, interlaminar, interareal, and whole cortex) scales. The model was tested by reproducing, as well as providing insights into, a wide range of neurophysiological findings about frequency-dependent interactions between visual cortical areas, including the observation that feedforward pathways are associated with enhanced gamma (30 to 70 Hz) oscillations, whereas feedback projections selectively modulate alpha/low-beta (8 to 15 Hz) oscillations. Furthermore, the model reproduces a functional hierarchy based on frequency-dependent Granger causality analysis of interareal signaling, as reported in recent monkey and human experiments, and suggests a mechanism for the observed context-dependent hierarchy dynamics. Together, this work highlights the necessity of multiscale approaches and provides a modeling platform for studies of large-scale brain circuit dynamics and functions. PMID:28138530

  11. Effect of slip-area scaling on the earthquake frequency-magnitude relationship

    NASA Astrophysics Data System (ADS)

    Senatorski, Piotr

    2017-06-01

    The earthquake frequency-magnitude relationship is considered in the maximum entropy principle (MEP) perspective. The MEP suggests sampling with constraints as a simple stochastic model of seismicity. The model is based on the von Neumann's acceptance-rejection method, with b-value as the parameter that breaks symmetry between small and large earthquakes. The Gutenberg-Richter law's b-value forms a link between earthquake statistics and physics. Dependence between b-value and the rupture area vs. slip scaling exponent is derived. The relationship enables us to explain observed ranges of b-values for different types of earthquakes. Specifically, different b-value ranges for tectonic and induced, hydraulic fracturing seismicity is explained in terms of their different triggering mechanisms: by the applied stress increase and fault strength reduction, respectively.

  12. Power Supply for Variable Frequency Induction Heating Using MERS Soft-Switching High Frequency Inverter

    NASA Astrophysics Data System (ADS)

    Isobe, Takanori; Kitahara, Tadayuki; Fukutani, Kazuhiko; Shimada, Ryuichi

    Variable frequency induction heating has great potential for industrial heating applications due to the possibility of achieving heating distribution control; however, large-scale induction heating with variable frequency has not yet been introduced for practical use. This paper proposes a high frequency soft-switching inverter for induction heating that can achieve variable frequency operation. One challenge of variable frequency induction heating is increasing power electronics ratings. This paper indicates that its current source type dc-link configuration and soft-switching characteristics can make it possible to build a large-scale system with variable frequency capability. A 90-kVA 150-1000Hz variable frequency experimental power supply for steel strip induction heating was developed. Experiments confirmed the feasibility of variable frequency induction heating with proposed converter and the advantages of variable frequency operation.

  13. The Interaction of Radio-Frequency Fields With Dielectric Materials at Macroscopic to Mesoscopic Scales

    PubMed Central

    Baker-Jarvis, James; Kim, Sung

    2012-01-01

    The goal of this paper is to overview radio-frequency (RF) electromagnetic interactions with solid and liquid materials from the macroscale to the nanoscale. The overview is geared toward the general researcher. Because this area of research is vast, this paper concentrates on currently active research areas in the megahertz (MHz) through gigahertz (GHz) frequencies, and concentrates on dielectric response. The paper studies interaction mechanisms both from phenomenological and fundamental viewpoints. Relaxation, resonance, interface phenomena, plasmons, the concepts of permittivity and permeability, and relaxation times are summarized. Topics of current research interest, such as negative-index behavior, noise, plasmonic behavior, RF heating, nanoscale materials, wave cloaking, polaritonic surface waves, biomaterials, and other topics are overviewed. Relaxation, resonance, and related relaxation times are overviewed. The wavelength and material length scales required to define permittivity in materials is discussed. PMID:26900513

  14. Regional flood frequency analysis in Triveneto (Italy): climate and scale controls

    NASA Astrophysics Data System (ADS)

    Persiano, Simone; Castellarin, Attilio; Domeneghetti, Alessio; Brath, Armando

    2016-04-01

    The growing concern about the possible effects of climate change on flood frequency regime is leading Authorities to review previously proposed procedures for design-flood estimation, such as national regionalization approaches. Our study focuses on the Triveneto region, a broad geographical area in North-eastern Italy consisting of the administrative regions of Trentino-Alto Adige, Veneto and Friuli-Venezia Giulia. A reference procedure for design flood estimation in Triveneto is available from the Italian NCR research project "VA.PI.", which developed a regional model using annual maximum series (AMS) of peak discharges that were collected up to the 80s by the former Italian Hydrometeorological Service. We consider a very detailed AMS database that we recently compiled for ~80 catchments located in Triveneto. Our dataset includes the historical data mentioned above, together with more recent data obtained from Regional Services and annual maximum peak streamflows extracted from inflow series to artificial reservoirs and provided by dam managers. All ~80 study catchments are characterized in terms of several geomorphologic and climatic descriptors. The main objectives of our study are: (1) to check whether climatic and scale controls on flood frequency regime in Triveneto are similar to the controls that were recently found in Europe; (2) to verify the possible presence of trends as well as abrupt changes in the intensity and frequency of flood extremes by looking at changes in time of regional L-moments of annual maximum floods; (3) to assess the reliability and representativeness of the reference procedure for design flood estimation relative to flood data that were not included in the VA.PI. dataset (i.e. more recent data collected after the 80s and historical data provided by dam managers); (4) to develop an updated reference procedure for design flood estimation in Triveneto by using a focused-pooling approach (i.e. Region of Influence, RoI).

  15. A search for long-time-scale, low-frequency radio transients

    NASA Astrophysics Data System (ADS)

    Murphy, Tara; Kaplan, David L.; Croft, Steve; Lynch, Christene; Callingham, J. R.; Bannister, Keith; Bell, Martin E.; Hurley-Walker, Natasha; Hancock, Paul; Line, Jack; Rowlinson, Antonia; Lenc, Emil; Intema, H. T.; Jagannathan, P.; Ekers, Ronald D.; Tingay, Steven; Yuan, Fang; Wolf, Christian; Onken, Christopher A.; Dwarakanath, K. S.; For, B.-Q.; Gaensler, B. M.; Hindson, L.; Johnston-Hollitt, M.; Kapińska, A. D.; McKinley, B.; Morgan, J.; Offringa, A. R.; Procopio, P.; Staveley-Smith, L.; Wayth, R.; Wu, C.; Zheng, Q.

    2017-04-01

    We present a search for transient and highly variable sources at low radio frequencies (150-200 MHz) that explores long time-scales of 1-3 yr. We conducted this search by comparing the TIFR GMRT Sky Survey Alternative Data Release 1 (TGSS ADR1) and the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey catalogues. To account for the different completeness thresholds in the individual surveys, we searched for compact GLEAM sources above a flux density limit of 100 mJy that were not present in the TGSS ADR1; and also for compact TGSS ADR1 sources above a flux density limit of 200 mJy that had no counterpart in GLEAM. From a total sample of 234 333 GLEAM sources and 275 612 TGSS ADR1 sources in the overlap region between the two surveys, there were 99 658 GLEAM sources and 38 978 TGSS ADR sources that passed our flux density cut-off and compactness criteria. Analysis of these sources resulted in three candidate transient sources. Further analysis ruled out two candidates as imaging artefacts. We analyse the third candidate and show it is likely to be real, with a flux density of 182 ± 26 mJy at 147.5 MHz. This gives a transient surface density of ρ = (6.2 ± 6) × 10-5 deg-2. We present initial follow-up observations and discuss possible causes for this candidate. The small number of spurious sources from this search demonstrates the high reliability of these two new low-frequency radio catalogues.

  16. Development of a scale to measure symptoms of anxiety and depression in the general UK population: the psychiatric symptom frequency scale.

    PubMed Central

    Lindelow, M; Hardy, R; Rodgers, B

    1997-01-01

    OBJECTIVES: The psychiatric symptom frequency (PSF) scale was developed to assess symptoms of anxiety and depression (i.e. affective symptoms) experienced over the past year in the general population. This study aimed to examine the distribution of PSF scores, internal consistency, and factor structure and to investigate relationships between total scores for this scale and other indicators of poor mental health. PARTICIPANTS: The Medical Research Council national survey of health and development, a class stratified cohort study of men and women followed up from birth in 1946, with the most recent interview at age 43 when the PSF scale was administered. MAIN RESULTS: The PSF scale showed high internal consistency between the 18 items (Cronbach's alpha = 0.88). Ratings on items of the scale reflected one predominant factor, incorporating both depression and anxiety, and two additional factors of less statistical importance, one reflecting sleep problems and the other panic and situational anxiety. Total scores were calculated by adding 18 items of the scale, and high total scores were found to be strongly associated with reports of contact with a doctor or other health professional and use of prescribed medication for "nervous or emotional trouble or depression," and with suicidal ideas. CONCLUSIONS: The PSF is a useful and valid scale for evaluating affective symptoms in the general population. It is appropriate for administration by lay interviewers with minimal training, is relatively brief, and generates few missing data. The total score is a flexible measure which can be used in continuous or binary form to suit the purposes of individual investigations, and provides discrimination at lower as well as upper levels of symptom severity. PMID:9425466

  17. Climatic Signals from Intra-annual Density Fluctuation Frequency in Mediterranean Pines at a Regional Scale

    PubMed Central

    Zalloni, Enrica; de Luis, Martin; Campelo, Filipe; Novak, Klemen; De Micco, Veronica; Di Filippo, Alfredo; Vieira, Joana; Nabais, Cristina; Rozas, Vicente; Battipaglia, Giovanna

    2016-01-01

    Tree rings provide information about the climatic conditions during the growing season by recording them in different anatomical features, such as intra-annual density fluctuations (IADFs). IADFs are intra-annual changes of wood density appearing as latewood-like cells within earlywood, or earlywood-like cells within latewood. The occurrence of IADFs is dependent on the age and size of the tree, and it is triggered by climatic drivers. The variations of IADF frequency of different species and their dependence on climate across a wide geographical range have still to be explored. The objective of this study is to investigate the effect of age, tree-ring width and climate on IADF formation and frequency at a regional scale across the Mediterranean Basin in Pinus halepensis Mill., Pinus pinaster Ait., and Pinus pinea L. The analyzed tree-ring network was composed of P. pinea trees growing at 10 sites (2 in Italy, 4 in Spain, and 4 in Portugal), P. pinaster from 19 sites (2 in Italy, 13 in Spain, and 4 in Portugal), and P. halepensis from 38 sites in Spain. The correlations between IADF frequency and monthly minimum, mean and maximum temperatures, as well as between IADF frequency and total precipitation, were analyzed. A significant negative relationship between IADF frequency and tree-ring age was found for the three Mediterranean pines. Moreover, IADFs were more frequent in wider rings than in narrower ones, although the widest rings showed a reduced IADF frequency. Wet conditions during late summer/early autumn triggered the formation of IADFs in the three species. Our results suggest the existence of a common climatic driver for the formation of IADFs in Mediterranean pines, highlighting the potential use of IADF frequency as a proxy for climate reconstructions with geographical resolution. PMID:27200052

  18. Fusion of infrared and visible images based on saliency scale-space in frequency domain

    NASA Astrophysics Data System (ADS)

    Chen, Yanfei; Sang, Nong; Dan, Zhiping

    2015-12-01

    A fusion algorithm of infrared and visible images based on saliency scale-space in the frequency domain was proposed. Focus of human attention is directed towards the salient targets which interpret the most important information in the image. For the given registered infrared and visible images, firstly, visual features are extracted to obtain the input hypercomplex matrix. Secondly, the Hypercomplex Fourier Transform (HFT) is used to obtain the salient regions of the infrared and visible images respectively, the convolution of the input hypercomplex matrix amplitude spectrum with a low-pass Gaussian kernel of an appropriate scale which is equivalent to an image saliency detector are done. The saliency maps are obtained by reconstructing the 2D signal using the original phase and the amplitude spectrum, filtered at a scale selected by minimizing saliency map entropy. Thirdly, the salient regions are fused with the adoptive weighting fusion rules, and the nonsalient regions are fused with the rule based on region energy (RE) and region sharpness (RS), then the fused image is obtained. Experimental results show that the presented algorithm can hold high spectrum information of the visual image, and effectively get the thermal targets information at different scales of the infrared image.

  19. A novel scaling law relating the geometrical dimensions of a photocathode radio frequency gun to its radio frequency properties

    NASA Astrophysics Data System (ADS)

    Lal, Shankar; Pant, K. K.; Krishnagopal, S.

    2011-12-01

    Developing a photocathode RF gun with the desired RF properties of the π-mode, such as field balance (eb) ˜1, resonant frequency fπ = 2856 MHz, and waveguide-to-cavity coupling coefficient βπ ˜1, requires precise tuning of the resonant frequencies of the independent full- and half-cells (ff and fh), and of the waveguide-to-full-cell coupling coefficient (βf). While contemporary electromagnetic codes and precision machining capability have made it possible to design and tune independent cells of a photocathode RF gun for desired RF properties, thereby eliminating the need for tuning, access to such computational resources and quality of machining is not very widespread. Therefore, many such structures require tuning after machining by employing conventional tuning techniques that are iterative in nature. Any procedure that improves understanding of the tuning process and consequently reduces the number of iterations and the associated risks in tuning a photocathode gun would, therefore, be useful. In this paper, we discuss a method devised by us to tune a photocathode RF gun for desired RF properties under operating conditions. We develop and employ a simple scaling law that accounts for inter-dependence between frequency of independent cells and waveguide-to-cavity coupling coefficient, and the effect of brazing clearance for joining of the two cells. The method has been employed to successfully develop multiple 1.6 cell BNL/SLAC/UCLA type S-band photocathode RF guns with the desired RF properties, without the need to tune them by a tiresome cut-and-measure process. Our analysis also provides a physical insight into how the geometrical dimensions affect the RF properties of the photo-cathode RF gun.

  20. A simple frequency-scaling rule for animal communication

    NASA Astrophysics Data System (ADS)

    Fletcher, Neville H.

    2004-05-01

    Different animals use widely different frequencies for sound communication, and it is reasonable to assume that evolution has adapted these frequencies to give greatest conspecific communication distance for a given vocal effort. Acoustic analysis shows that the optimal communication frequency is inversely proportional to about the 0.4 power of the animal's body mass. Comparison with observational data indicates that this prediction is well supported in practice. For animals of a given class, for example mammals, the maximum communication distance varies about as the 0.6 power of the animal's mass. There is, however, a wide spread of observed results because of the different emphasis placed upon vocal effort in the evolution of different animal species.

  1. Use of the Morlet mother wavelet in the frequency-scale domain decomposition technique for the modal identification of ambient vibration responses

    NASA Astrophysics Data System (ADS)

    Le, Thien-Phu

    2017-10-01

    The frequency-scale domain decomposition technique has recently been proposed for operational modal analysis. The technique is based on the Cauchy mother wavelet. In this paper, the approach is extended to the Morlet mother wavelet, which is very popular in signal processing due to its superior time-frequency localization. Based on the regressive form and an appropriate norm of the Morlet mother wavelet, the continuous wavelet transform of the power spectral density of ambient responses enables modes in the frequency-scale domain to be highlighted. Analytical developments first demonstrate the link between modal parameters and the local maxima of the continuous wavelet transform modulus. The link formula is then used as the foundation of the proposed modal identification method. Its practical procedure, combined with the singular value decomposition algorithm, is presented step by step. The proposition is finally verified using numerical examples and a laboratory test.

  2. Theoretical Characterization of Visual Signatures and Calculation of Approximate Global Harmonic Frequency Scaling Factors

    NASA Astrophysics Data System (ADS)

    Kashinski, D. O.; Nelson, R. G.; Chase, G. M.; di Nallo, O. E.; Byrd, E. F. C.

    2016-05-01

    We are investigating the accuracy of theoretical models used to predict the visible, ultraviolet, and infrared spectra, as well as other properties, of product materials ejected from the muzzle of currently fielded systems. Recent advances in solid propellants has made the management of muzzle signature (flash) a principle issue in weapons development across the calibers. A priori prediction of the electromagnetic spectra of formulations will allow researchers to tailor blends that yield desired signatures and determine spectrographic detection ranges. Quantum chemistry methods at various levels of sophistication have been employed to optimize molecular geometries, compute unscaled harmonic frequencies, and determine the optical spectra of specific gas-phase species. Electronic excitations are being computed using Time Dependent Density Functional Theory (TD-DFT). Calculation of approximate global harmonic frequency scaling factors for specific DFT functionals is also in progress. A full statistical analysis and reliability assessment of computational results is currently underway. Work supported by the ARL, DoD-HPCMP, and USMA.

  3. The meaning of vaguely quantified frequency response options on a quality of life scale depends on respondents’ medical status and age

    PubMed Central

    Schneider, Stefan; Stone, Arthur A.

    2017-01-01

    Purpose Self-report items in quality of life (QoL) scales commonly use vague quantifiers like “sometimes” or “often” to measure the frequency of health-related experiences. This study examined whether the meaning of such vaguely quantified response options differs depending on people’s medical status and age, which may undermine the validity of QoL group comparisons. Methods Respondents (n = 600) rated the frequency of positive and negative QoL experiences using vague quantifiers (never, rarely, sometimes, often, always) and provided open-ended numeric frequency counts for the same items. Negative binomial regression analyses examined whether the numeric frequencies associated with each vague quantifier differed between medical status (no vs. one or more medical conditions) and age (18–40 years vs. 60+ years) groups. Results Compared to respondents without a chronic condition, those with a medical condition assigned a higher numeric frequency to the same vague quantifiers for negative QoL experiences; this effect was not evident for positive QoL experiences. Older respondents’ numeric frequencies were more extreme (i.e., lower at the low end and somewhat higher at the high end of the response range) than those of younger respondents. After adjusting for these effects, differences in QoL became somewhat more pronounced between medical status groups, but not between age groups. Conclusions The results suggest that people with different medical backgrounds and age do not interpret vague frequency quantifiers on a QoL scale in the same way. Open-ended numeric frequency reports may be useful to detect and potentially correct for differences in the meaning of vague quantifiers. PMID:27071685

  4. NEON: High Frequency Monitoring Network for Watershed-Scale Processes and Aquatic Ecology

    NASA Astrophysics Data System (ADS)

    Vance, J. M.; Fitzgerald, M.; Parker, S. M.; Roehm, C. L.; Goodman, K. J.; Bohall, C.; Utz, R.

    2014-12-01

    Networked high frequency hydrologic and water quality measurements needed to investigate physical and biogeochemical processes at the watershed scale and create robust models are limited and lacking standardization. Determining the drivers and mechanisms of ecological changes in aquatic systems in response to natural and anthropogenic pressures is challenging due to the large amounts of terrestrial, aquatic, atmospheric, biological, chemical, and physical data it requires at varied spatiotemporal scales. The National Ecological Observatory Network (NEON) is a continental-scale infrastructure project designed to provide data to address the impacts of climate change, land-use, and invasive species on ecosystem structure and function. Using a combination of standardized continuous in situ measurements and observational sampling, the NEON Aquatic array will produce over 200 data products across its spatially-distributed field sites for 30 years to facilitate spatiotemporal analysis of the drivers of ecosystem change. Three NEON sites in Alabama were chosen to address linkages between watershed-scale processes and ecosystem changes along an eco-hydrological gradient within the Tombigbee River Basin. The NEON Aquatic design, once deployed, will include continuous measurements of surface water physical, chemical, and biological parameters, groundwater level, temperature and conductivity and local meteorology. Observational sampling will include bathymetry, water chemistry and isotopes, and a suite of organismal sampling from microbes to macroinvertebrates to vertebrates. NEON deployed a buoy to measure the temperature profile of the Black Warrior River from July - November, 2013 to determine the spatiotemporal variability across the water column from a daily to seasonal scale. In July 2014 a series of water quality profiles were performed to assess the contribution of physical and biogeochemical drivers over a diurnal cycle. Additional river transects were performed

  5. Source conductance scaling for high frequency superconducting quasiparticle receivers

    NASA Technical Reports Server (NTRS)

    Ke, Qing; Feldman, M. J.

    1992-01-01

    It has been suggested that the optimum source conductance G(sub s) for the superconductor-insulator-superconductor (SIS) quasiparticle mixer should have a l/f dependence. This would imply that the critical current density of SIS junctions used for mixing should increase as frequency squared, a stringent constraint on the design of submillimeter SIS mixers, rather than in simple proportion to frequency as previously believed. We have used Tucker's quantum theory of mixing for extensive numerical calculations to determine G(sub s) for an optimized SIS receiver. We find that G(sub s) is very roughly independent of frequency (except for the best junctions at low frequency), and discuss the implications of our results for the design of submillimeter SIS mixers.

  6. Dual-Frequency VLBI Study of Centaurus A on Sub-Parsec Scales: The Highest-Resolution View of an Extragalactic Jet

    NASA Technical Reports Server (NTRS)

    Mueller, C.; Kadler, M.; Ojha, R.; Wilms, J.; Boeck, M.; Edwards, P.; Fromm, C. M.; Hase, H.; Horiuchi, S.; Katz, U.; hide

    2011-01-01

    Centaurus A is the closest active galactic nucleus. High resolution imaging using Very Long Baseline Interferometry (VLBI) enables us to study the spectral and kinematic behavior of the radio jet-<:ounterjet system on sub-parsec scales, providing essential information for jet emission and formation models. Aims. Our aim is to study the structure and spectral shape of the emission from the central-parsec region of Cen A. Methods. As a target of the Southern Hemisphere VLBI monitoring program TANAMI (Tracking Active Galactic Nuclei with Millliarcsecond Interferometry), VLBI observations of Cen A are made regularly at 8.4 and 22.3 GHz with the Australian Long Baseline Array (LBA) and associated telescopes in Antarctica, Chile, and South Africa. Results. The first dual-frequency images of this source are presented along with the resulting spectral index map. An angular resolution of 0.4 mas x 0.7 mas is achieved at 8.4 GHz, corresponding to a linear scale of less than 0.013 pc. Hence, we obtain the highest resolution VLBI image of Cen A, comparable to previous space-VLBI observations. By combining with the 22.3 GHz image, we present the corresponding dual-frequency spectral index distribution along the sub-parsec scale jet revealing the putative emission regions for recently detected y-rays from the core region by Fermi/LAT. Conclusions. We resolve the innermost structure of the milliarcsecond scale jet and counter jet system of Cen A into discrete components. The simultaneous observations at two frequencies provide the highest resolved spectral index map of an AGN jet allowing us to identify up to four possible sites as the origin of the high energy emission. Key words. galaxies: active galaxies: individual (Centaurus A, NGC 5128) - galaxies: jets - techniques: high angular resolution

  7. Linking Low-Frequency Large-Scale Circulation Patterns to Cold Air Outbreak Formation in the Northeastern North Atlantic

    NASA Astrophysics Data System (ADS)

    Papritz, L.; Grams, C. M.

    2018-03-01

    The regional variability of wintertime marine cold air outbreaks (CAOs) in the northeastern North Atlantic is studied focusing on the role of weather regimes in modulating the large-scale circulation. Each regime is characterized by a typical CAO frequency anomaly pattern and a corresponding imprint in air-sea heat fluxes. Cyclonically dominated regimes, Greenland blocking and the Atlantic ridge regime are found to provide favorable conditions for CAO formation in at least one major sea of the study region; CAO occurrence is suppressed, however, by blocked regimes whose associated anticyclones are centered over northern Europe (European / Scandinavian blocking). Kinematic trajectories reveal that strength and location of the storm tracks are closely linked to the pathways of CAO air masses and, thus, CAO occurrence. Finally, CAO frequencies are also linked to the strength of the stratospheric polar vortex, which is understood in terms of associated variations in the frequency of weather regimes.

  8. Frequency and zero-point vibrational energy scale factors for double-hybrid density functionals (and other selected methods): can anharmonic force fields be avoided?

    PubMed

    Kesharwani, Manoj K; Brauer, Brina; Martin, Jan M L

    2015-03-05

    We have obtained uniform frequency scaling factors λ(harm) (for harmonic frequencies), λ(fund) (for fundamentals), and λ(ZPVE) (for zero-point vibrational energies (ZPVEs)) for the Weigend-Ahlrichs and other selected basis sets for MP2, SCS-MP2, and a variety of DFT functionals including double hybrids. For selected levels of theory, we have also obtained scaling factors for true anharmonic fundamentals and ZPVEs obtained from quartic force fields. For harmonic frequencies, the double hybrids B2PLYP, B2GP-PLYP, and DSD-PBEP86 clearly yield the best performance at RMSD = 10-12 cm(-1) for def2-TZVP and larger basis sets, compared to 5 cm(-1) at the CCSD(T) basis set limit. For ZPVEs, again, the double hybrids are the best performers, reaching root-mean-square deviations (RMSDs) as low as 0.05 kcal/mol, but even mainstream functionals like B3LYP can get down to 0.10 kcal/mol. Explicitly anharmonic ZPVEs only are marginally more accurate. For fundamentals, however, simple uniform scaling is clearly inadequate.

  9. Determination of Black Hole Mass in Cyg X-1 by Scaling of Spectral Index-QPO Frequency Correlation

    NASA Technical Reports Server (NTRS)

    Shaposhnikov, Nickolai; Titarchuk, Lev

    2007-01-01

    It is well established that timing and spectral properties of Galactic Black Hole (BH) X-ray binaries (XRB) are strongly correlated. In particular, it has been shown that low frequency Quasi-Periodic Oscillation (QPO) nu(sub low) - photon index GAMMA correlation curves have a specific pattern. In a number of the sources studied the shape of the index-low frequency QPO correlations are self-similar with a position offset in the nu(sub low) - GAMMA plane determined by a BH mass M(sub BH). Specifically, Titarchuk & Fiorito (2004) gave strong theoretical and observational arguments that the QPO frequency values in this nu(sub low) - GAMMA correlation should be inversely proportional to M(sub BH). A simple translation of the correlation for a given source along frequency axis leads to the observed correlation for another source. As a result of this translation one can obtain a scaling factor which is simply a BH mass ratio for these particular sources. This property of the correlations offers a fundamentally new method for BH mass determination in XRBs. Here we use the observed QPO-index correlations observed in three BH sources: GRO J1655-40, GRS 1915+105 and Cyg X-1. The BH mass of (6.3 plus or minus 0.5) solar mass in GRO J1655-40 is obtained using optical observations. RXTE observations during the recent 2005 outburst yielded sufficient data to establish the correlation pattern during both rise and decay of the event. We use GRO J1655-40 as a standard reference source to measure the BH mass in Cyg X-1. We also revisit the GRS 1915+105 data as a further test of our scaling method. We obtain the BH mass in Cyg X-1 in the range 7.6-9.9.

  10. On Frequency Combs in Monolithic Resonators

    NASA Astrophysics Data System (ADS)

    Savchenkov, A. A.; Matsko, A. B.; Maleki, L.

    2016-06-01

    Optical frequency combs have become indispensable in astronomical measurements, biological fingerprinting, optical metrology, and radio frequency photonic signal generation. Recently demonstrated microring resonator-based Kerr frequency combs point the way towards chip scale optical frequency comb generator retaining major properties of the lab scale devices. This technique is promising for integrated miniature radiofrequency and microwave sources, atomic clocks, optical references and femtosecond pulse generators. Here we present Kerr frequency comb development in a historical perspective emphasizing its similarities and differences with other physical phenomena. We elucidate fundamental principles and describe practical implementations of Kerr comb oscillators, highlighting associated solved and unsolved problems.

  11. Evaluation of the Problem Behavior Frequency Scale-Teacher Report Form for Assessing Behavior in a Sample of Urban Adolescents.

    PubMed

    Farrell, Albert D; Goncy, Elizabeth A; Sullivan, Terri N; Thompson, Erin L

    2018-02-01

    This study evaluated the structure and validity of the Problem Behavior Frequency Scale-Teacher Report Form (PBFS-TR) for assessing students' frequency of specific forms of aggression and victimization, and positive behavior. Analyses were conducted on two waves of data from 727 students from two urban middle schools (Sample 1) who were rated by their teachers on the PBFS-TR and the Social Skills Improvement System (SSIS), and on data collected from 1,740 students from three urban middle schools (Sample 2) for whom data on both the teacher and student report version of the PBFS were obtained. Confirmatory factor analyses supported first-order factors representing 3 forms of aggression (physical, verbal, and relational), 3 forms of victimization (physical, verbal and relational), and 2 forms of positive behavior (prosocial behavior and effective nonviolent behavior), and higher-order factors representing aggression, victimization, and positive behavior. Strong measurement invariance was established over gender, grade, intervention condition, and time. Support for convergent validity was found based on correlations between corresponding scales on the PBFS-TR and teacher ratings on the SSIS in Sample 1. Significant correlations were also found between teacher ratings on the PBFS-TR and student ratings of their behavior on the Problem Behavior Frequency Scale-Adolescent Report (PBFS-AR) and a measure of nonviolent behavioral intentions in Sample 2. Overall the findings provided support for the PBFS-TR and suggested that teachers can provide useful data on students' aggressive and prosocial behavior and victimization experiences within the school setting. (PsycINFO Database Record (c) 2018 APA, all rights reserved).

  12. Strategies for Energy Efficient Resource Management of Hybrid Programming Models

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

    Li, Dong; Supinski, Bronis de; Schulz, Martin

    2013-01-01

    Many scientific applications are programmed using hybrid programming models that use both message-passing and shared-memory, due to the increasing prevalence of large-scale systems with multicore, multisocket nodes. Previous work has shown that energy efficiency can be improved using software-controlled execution schemes that consider both the programming model and the power-aware execution capabilities of the system. However, such approaches have focused on identifying optimal resource utilization for one programming model, either shared-memory or message-passing, in isolation. The potential solution space, thus the challenge, increases substantially when optimizing hybrid models since the possible resource configurations increase exponentially. Nonetheless, with the accelerating adoptionmore » of hybrid programming models, we increasingly need improved energy efficiency in hybrid parallel applications on large-scale systems. In this work, we present new software-controlled execution schemes that consider the effects of dynamic concurrency throttling (DCT) and dynamic voltage and frequency scaling (DVFS) in the context of hybrid programming models. Specifically, we present predictive models and novel algorithms based on statistical analysis that anticipate application power and time requirements under different concurrency and frequency configurations. We apply our models and methods to the NPB MZ benchmarks and selected applications from the ASC Sequoia codes. Overall, we achieve substantial energy savings (8.74% on average and up to 13.8%) with some performance gain (up to 7.5%) or negligible performance loss.« less

  13. The System Power Control Unit Based on the On-Chip Wireless Communication System

    PubMed Central

    Li, Tiefeng; Ma, Caiwen; Li, WenHua

    2013-01-01

    Currently, the on-chip wireless communication system (OWCS) includes 2nd-generation (2G), 3rd-generation (3G), and long-term evolution (LTE) communication subsystems. To improve the power consumption of OWCS, a typical architecture design of system power control unit (SPCU) is given in this paper, which can not only make a 2G, a 3G, and an LTE subsystems enter sleep mode, but it can also wake them up from sleep mode via the interrupt. During the sleep mode period, either the real-time sleep timer or the global system for mobile (GSM) communication sleep timer can be used individually to arouse the corresponding subsystem. Compared to previous sole voltage supplies on the OWCS, a 2G, a 3G, or an LTE subsystem can be independently configured with three different voltages and frequencies in normal work mode. In the meantime, the voltage supply monitor, which is an important part in the SPCU, can significantly guard the voltage of OWCS in real time. Finally, the SPCU may implement dynamic voltage and frequency scaling (DVFS) for a 2G, a 3G, or an LTE subsystem, which is automatically accomplished by the hardware. PMID:23818835

  14. The system power control unit based on the on-chip wireless communication system.

    PubMed

    Li, Tiefeng; Ma, Caiwen; Li, WenHua

    2013-01-01

    Currently, the on-chip wireless communication system (OWCS) includes 2nd-generation (2G), 3rd-generation (3G), and long-term evolution (LTE) communication subsystems. To improve the power consumption of OWCS, a typical architecture design of system power control unit (SPCU) is given in this paper, which can not only make a 2G, a 3G, and an LTE subsystems enter sleep mode, but it can also wake them up from sleep mode via the interrupt. During the sleep mode period, either the real-time sleep timer or the global system for mobile (GSM) communication sleep timer can be used individually to arouse the corresponding subsystem. Compared to previous sole voltage supplies on the OWCS, a 2G, a 3G, or an LTE subsystem can be independently configured with three different voltages and frequencies in normal work mode. In the meantime, the voltage supply monitor, which is an important part in the SPCU, can significantly guard the voltage of OWCS in real time. Finally, the SPCU may implement dynamic voltage and frequency scaling (DVFS) for a 2G, a 3G, or an LTE subsystem, which is automatically accomplished by the hardware.

  15. Nonlinear Filtering Effects of Reservoirs on Flood Frequency Curves at the Regional Scale: RESERVOIRS FILTER FLOOD FREQUENCY CURVES

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

    Wang, Wei; Li, Hong-Yi; Leung, L. Ruby

    Anthropogenic activities, e.g., reservoir operation, may alter the characteristics of Flood Frequency Curve (FFC) and challenge the basic assumption of stationarity used in flood frequency analysis. This paper presents a combined data-modeling analysis of the nonlinear filtering effects of reservoirs on the FFCs over the contiguous United States. A dimensionless Reservoir Impact Index (RII), defined as the total upstream reservoir storage capacity normalized by the annual streamflow volume, is used to quantify reservoir regulation effects. Analyses are performed for 388 river stations with an average record length of 50 years. The first two moments of the FFC, mean annual maximummore » flood (MAF) and coefficient of variations (CV), are calculated for the pre- and post-dam periods and compared to elucidate the reservoir regulation effects as a function of RII. It is found that MAF generally decreases with increasing RII but stabilizes when RII exceeds a threshold value, and CV increases with RII until a threshold value beyond which CV decreases with RII. The processes underlying the nonlinear threshold behavior of MAF and CV are investigated using three reservoir models with different levels of complexity. All models capture the non-linear relationships of MAF and CV with RII, suggesting that the basic flood control function of reservoirs is key to the non-linear relationships. The relative roles of reservoir storage capacity, operation objectives, available storage prior to a flood event, and reservoir inflow pattern are systematically investigated. Our findings may help improve flood-risk assessment and mitigation in regulated river systems at the regional scale.« less

  16. Modulating action of low frequency oscillations on high frequency instabilities in Hall thrusters

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

    Liqiu, Wei, E-mail: weiliqiu@gmail.com, E-mail: weiliqiu@hit.edu.cn; Liang, Han; Ziyi, Yang

    2015-02-07

    It is found that the low frequency oscillations have modulating action on high frequency instabilities in Hall thrusters. The physical mechanism of this modulation is discussed and verified by numerical simulations. Theoretical analyses indicate that the wide-range fluctuations of plasma density and electric field associated with the low frequency oscillations affect the electron drift velocity and anomalous electron transport across the magnetic field. The amplitude and frequency of high frequency oscillations are modulated by low frequency oscillations, which show the periodic variation in the time scale of low frequency oscillations.

  17. IRIS Arrays: Observing Wavefields at Multiple Scales and Frequencies

    NASA Astrophysics Data System (ADS)

    Sumy, D. F.; Woodward, R.; Frassetto, A.

    2014-12-01

    The Incorporated Research Institutions for Seismology (IRIS) provides instruments for creating and operating seismic arrays at a wide range of scales. As an example, for over thirty years the IRIS PASSCAL program has provided instruments to individual Principal Investigators to deploy arrays of all shapes and sizes on every continent. These arrays have ranged from just a few sensors to hundreds or even thousands of sensors, covering areas with dimensions of meters to thousands of kilometers. IRIS also operates arrays directly, such as the USArray Transportable Array (TA) as part of the EarthScope program. Since 2004, the TA has rolled across North America, at any given time spanning a swath of approximately 800 km by 2,500 km, and thus far sampling 2% of the Earth's surface. This achievement includes all of the lower-48 U.S., southernmost Canada, and now parts of Alaska. IRIS has also facilitated specialized arrays in polar environments and on the seafloor. In all cases, the data from these arrays are freely available to the scientific community. As the community of scientists who use IRIS facilities and data look to the future they have identified a clear need for new array capabilities. In particular, as part of its Wavefields Initiative, IRIS is exploring new technologies that can enable large, dense array deployments to record unaliased wavefields at a wide range of frequencies. Large-scale arrays might utilize multiple sensor technologies to best achieve observing objectives and optimize equipment and logistical costs. Improvements in packaging and power systems can provide equipment with reduced size, weight, and power that will reduce logistical constraints for large experiments, and can make a critical difference for deployments in harsh environments or other situations where rapid deployment is required. We will review the range of existing IRIS array capabilities with an overview of previous and current deployments and examples of data and results. We

  18. Model of the Radio Frequency (RF) Excitation Response from Monopole and Dipole Antennas in a Large Scale Tank

    NASA Technical Reports Server (NTRS)

    Wilson, Jeffrey D.; Zimmerli, Gregory A.

    2012-01-01

    Good antenna-mode coupling is needed for determining the amount of propellant in a tank through the method of radio frequency mass gauging (RFMG). The antenna configuration and position in a tank are important factors in coupling the antenna to the natural electromagnetic modes. In this study, different monopole and dipole antenna mounting configurations and positions were modeled and responses simulated in a full-scale tank model with the transient solver of CST Microwave Studio (CST Computer Simulation Technology of America, Inc.). The study was undertaken to qualitatively understand the effect of antenna design and placement within a tank on the resulting radio frequency (RF) tank spectrum.

  19. Experimental observation of multi-scale interactions among kink /tearing modes and high-frequency fluctuations in the HL-2A core NBI plasmas

    NASA Astrophysics Data System (ADS)

    Chen, W.; Jiang, M.; Xu, Y.; Shi, P. W.; Yu, L. M.; Ding, X. T.; Shi, Z. B.; Ji, X. Q.; Yu, D. L.; Li, Y. G.; Yang, Z. C.; Zhong, W. L.; Qiu, Z. Y.; Li, J. Q.; Dong, J. Q.; Yang, Q. W.; Liu, Yi.; Yan, L. W.; Xu, M.; Duan, X. R.

    2017-11-01

    Multi-scale interactions have been observed recently in the HL-2A core NBI plasmas, including the synchronous coupling between m/n=1/1 kink mode and m/n=2/1 tearing mode, nonlinear couplings of TAE/BAE and m/n=2/1 TM near q=2 surface, AITG/KBM/BAE and m/n=1/1 kink mode near q=1 surface, and between m/n=1/1 kink mode and high-frequency turbulence. Experimental results suggest that several couplings can exist simultaneously, Alfvenic fluctuations have an important contribution to the high-frequency turbulence spectra, and the couplings reveal the electromagnetic character. Multi-scale interactions via the nonlinear modulation process maybe enhance plasma transport and trigger sawtooth-crash onset.

  20. Interpretations of Frequency Domain Analyses of Neural Entrainment: Periodicity, Fundamental Frequency, and Harmonics.

    PubMed

    Zhou, Hong; Melloni, Lucia; Poeppel, David; Ding, Nai

    2016-01-01

    Brain activity can follow the rhythms of dynamic sensory stimuli, such as speech and music, a phenomenon called neural entrainment. It has been hypothesized that low-frequency neural entrainment in the neural delta and theta bands provides a potential mechanism to represent and integrate temporal information. Low-frequency neural entrainment is often studied using periodically changing stimuli and is analyzed in the frequency domain using the Fourier analysis. The Fourier analysis decomposes a periodic signal into harmonically related sinusoids. However, it is not intuitive how these harmonically related components are related to the response waveform. Here, we explain the interpretation of response harmonics, with a special focus on very low-frequency neural entrainment near 1 Hz. It is illustrated why neural responses repeating at f Hz do not necessarily generate any neural response at f Hz in the Fourier spectrum. A strong neural response at f Hz indicates that the time scales of the neural response waveform within each cycle match the time scales of the stimulus rhythm. Therefore, neural entrainment at very low frequency implies not only that the neural response repeats at f Hz but also that each period of the neural response is a slow wave matching the time scale of a f Hz sinusoid.

  1. Anomalous volatility scaling in high frequency financial data

    NASA Astrophysics Data System (ADS)

    Nava, Noemi; Di Matteo, T.; Aste, Tomaso

    2016-04-01

    Volatility of intra-day stock market indices computed at various time horizons exhibits a scaling behaviour that differs from what would be expected from fractional Brownian motion (fBm). We investigate this anomalous scaling by using empirical mode decomposition (EMD), a method which separates time series into a set of cyclical components at different time-scales. By applying the EMD to fBm, we retrieve a scaling law that relates the variance of the components to a power law of the oscillating period. In contrast, when analysing 22 different stock market indices, we observe deviations from the fBm and Brownian motion scaling behaviour. We discuss and quantify these deviations, associating them to the characteristics of financial markets, with larger deviations corresponding to less developed markets.

  2. The development of small-scale mechanization means positioning algorithm using radio frequency identification technology in industrial plants

    NASA Astrophysics Data System (ADS)

    Astafiev, A.; Orlov, A.; Privezencev, D.

    2018-01-01

    The article is devoted to the development of technology and software for the construction of positioning and control systems for small mechanization in industrial plants based on radio frequency identification methods, which will be the basis for creating highly efficient intelligent systems for controlling the product movement in industrial enterprises. The main standards that are applied in the field of product movement control automation and radio frequency identification are considered. The article reviews modern publications and automation systems for the control of product movement developed by domestic and foreign manufacturers. It describes the developed algorithm for positioning of small-scale mechanization means in an industrial enterprise. Experimental studies in laboratory and production conditions have been conducted and described in the article.

  3. Large Scale Assessment of Radio Frequency Interference Signatures in L-band SAR Data

    NASA Astrophysics Data System (ADS)

    Meyer, F. J.; Nicoll, J.

    2011-12-01

    Imagery of L-band Synthetic Aperture Radar (SAR) systems such as the PALSAR sensor on board the Advanced Land Observing Satellite (ALOS) has proven to be a valuable tool for observing environmental changes around the globe. Besides offering 24/7 operability, the L-band frequency provides improved interferometric coherence, and L-band polarimetric data has shown great potential for vegetation monitoring, sea ice classification, and the observation of glaciers and ice sheets. To maximize the benefit of missions such as ALOS PALSAR for environmental monitoring, data consistency and calibration are vital. Unfortunately, radio frequency interference (RFI) signatures from ground-based radar systems regularly impair L-band SAR data quality and consistency. With this study we present a large-scale analysis of typical RFI signatures that are regularly observed in L-band SAR data over the Americas. Through a study of the vast archive of L-band SAR data in the US Government Research Consortium (USGRC) data pool at the Alaska Satellite Facility (ASF) we were able to address the following research goals: 1. Assessment of RFI Signatures in L-band SAR data and their Effects on SAR Data Quality: An analysis of time-frequency properties of RFI signatures in L-band SAR data of the USGRC data pool is presented. It is shown that RFI-filtering algorithms implemented in the operational ALOS PALSAR processor are not sufficient to remove all RFI-related artifacts. In examples, the deleterious effects of RFI on SAR image quality, polarimetric signature, SAR phase, and interferometric coherence are presented. 2. Large-Scale Assessment of Severity, Spatial Distribution, and Temporal Variation of RFI Signatures in L-band SAR data: L-band SAR data in the USGRC data pool were screened for RFI using a custom algorithm. Per SAR frame, the algorithm creates geocoded frame bounding boxes that are color-coded according to RFI intensity and converted to KML files for analysis in Google Earth. From

  4. 3-D optical profilometry at micron scale with multi-frequency fringe projection using modified fibre optic Lloyd's mirror technique

    NASA Astrophysics Data System (ADS)

    Inanç, Arda; Kösoğlu, Gülşen; Yüksel, Heba; Naci Inci, Mehmet

    2018-06-01

    A new fibre optic Lloyd's mirror method is developed for extracting 3-D height distribution of various objects at the micron scale with a resolution of 4 μm. The fibre optic assembly is elegantly integrated to an optical microscope and a CCD camera. It is demonstrated that the proposed technique is quite suitable and practical to produce an interference pattern with an adjustable frequency. By increasing the distance between the fibre and the mirror with a micrometre stage in the Lloyd's mirror assembly, the separation between the two bright fringes is lowered down to the micron scale without using any additional elements as part of the optical projection unit. A fibre optic cable, whose polymer jacket is partially stripped, and a microfluidic channel are used as test objects to extract their surface topographies. Point by point sensitivity of the method is found to be around 8 μm, changing a couple of microns depending on the fringe frequency and the measured height. A straightforward calibration procedure for the phase to height conversion is also introduced by making use of the vertical moving stage of the optical microscope. The phase analysis of the acquired image is carried out by One Dimensional Continuous Wavelet Transform for which the chosen wavelet is the Morlet wavelet and the carrier removal of the projected fringe patterns is achieved by reference subtraction. Furthermore, flexible multi-frequency property of the proposed method allows measuring discontinuous heights where there are phase ambiguities like 2π by lowering the fringe frequency and eliminating the phase ambiguity.

  5. Creaming enhancement in a liter scale ultrasonic reactor at selected transducer configurations and frequencies.

    PubMed

    Juliano, Pablo; Temmel, Sandra; Rout, Manoj; Swiergon, Piotr; Mawson, Raymond; Knoerzer, Kai

    2013-01-01

    Recent research has shown that high frequency ultrasound (0.4-3 MHz), can enhance milkfat separation in small scale systems able to treat only a few milliliters of sample. In this work, the effect of ultrasonic standing waves on milkfat creaming was studied in a 6L reactor and the influence of different frequencies and transducer configurations in direct contact with the fluid was investigated. A recombined coarse milk emulsion with fat globules stained with oil-red-O dye was selected for the separation trials. Runs were performed with one or two transducers placed in vertical (parallel or perpendicular) and horizontal positions (at the reactor base) at 0.4, 1 and/or 2 MHz (specific energy 8.5 ± 0.6 kJ/kg per transducer). Creaming behavior was assessed by measuring the thickness of the separated cream layer. Other methods supporting this assessment included the measurement of fat content, backscattering, particle size distribution, and microscopy of samples taken at the bottom and top of the reactor. Most efficient creaming was found after treatment at 0.4 MHz in single and double vertical transducer configurations. Among these configurations, a higher separation rate was obtained when sonicating at 0.4 MHz in a vertical perpendicular double transducer setup. The horizontal transducer configuration promoted creaming at 2 MHz only. Fat globule size increase was observed when creaming occurred. This research highlights the potential for enhanced separation of milkfat in larger scale systems from selected transducer configurations in contact with a dairy emulsion, or emulsion splitting in general. Copyright © 2012 Elsevier B.V. All rights reserved.

  6. A Study of Acoustic Reflections in Full-Scale Rotor Low Frequency Noise Measurements Acquired in Wind Tunnels

    NASA Technical Reports Server (NTRS)

    Barbely, Natasha L.; Sim, Ben W.; Kitaplioglu, Cahit; Goulding, Pat, II

    2010-01-01

    Difficulties in obtaining full-scale rotor low frequency noise measurements in wind tunnels are addressed via residual sound reflections due to non-ideal anechoic wall treatments. Examples illustrated with the Boeing-SMART rotor test in the National Full-Scale Aerodynamics Complex (NFAC) 40- by 80-Foot Wind Tunnel facility demonstrated that these reflections introduced distortions in the measured acoustic time histories that are not representative of free-field rotor noise radiation. A simplified reflection analysis, based on the method of images, is used to examine the sound measurement quality in such "less-than-anechoic" environment. Predictions of reflection-adjusted acoustic time histories are qualitatively shown to account for some of the spurious fluctuations observed in wind tunnel noise measurements

  7. Yield Scaling of Frequency Domain Moment Tensors from Contained Chemical Explosions Detonated in Granite

    NASA Astrophysics Data System (ADS)

    MacPhail, M. D.; Stump, B. W.; Zhou, R.

    2017-12-01

    The Source Phenomenology Experiment (SPE - Arizona) was a series of nine, contained and partially contained chemical explosions within the porphyry granite at the Morenci Copper mine in Arizona. Its purpose was to detonate, record and analyze seismic waveforms from these single-fired explosions. Ground motion data from the SPE is analyzed in this study to assess the uniqueness of the time domain moment tensor source representation and its ability to quantify containment and yield scaling. Green's functions were computed for each of the explosions based on a 1D velocity model developed for the SPE. The Green's functions for the sixteen, near-source stations focused on observations from 37 to 680 m. This study analyzes the three deepest, fully contained explosions with a depth of burial of 30 m and yields of 0.77e-3, 3.08e-3 and 6.17e-3 kt. Inversions are conducted within the frequency domain and moment tensors are decomposed into deviatoric and isotropic components to evaluate the effects of containment and yield on the resulting source representation. Isotropic moments are compared to those for other contained explosions as reported by Denny and Johnson, 1991, and are in good agreement with their scaling results. The explosions in this study have isotropic moments of 1.2e12, 3.1e12 and 6.1e13 n*m. Isotropic and Mzz moment tensor spectra are compared to Mueller-Murphy, Denny-Johnson and revised Heard-Ackerman (HA) models and suggest that the larger explosions fit the HA model better. Secondary source effects resulting from free surface interactions including the effects of spallation contribute to the resulting moment tensors which include a CLVD component. Hudson diagrams, using frequency domain moment tensor data, are computed as a tool to assess how these containment scenarios affect the source representation. Our analysis suggests that, within our band of interest (2-20 Hz), as the frequency increases, the source representation becomes more explosion like

  8. Frequency scaling with miniature COmpact MIcrowave and Coaxial ion sources

    NASA Astrophysics Data System (ADS)

    Sortais, Pascal; André, Thomas; Angot, Julien; Bouat, Sophie; Jacob, Josua; Lamy, Thierry; Sole, Patrick

    2014-02-01

    We will present recent basic developments about possible extension of the COMIC (for COmpact MIcrowave and Coaxial) devices up to 5.8 GHz in place of the present 2.45 GHz operation [P. Sortais, T. Lamy, J. Médard, J. Angot, L. Latrasse, and T. Thuillier, Rev. Sci. Instrum. 81, 02B314 (2010)]. New applications associating multiple COMIC devices for thin film deposition will be described and we will explain why an increase of the current density delivered by each individual ion source could lead to the increase of the deposition rate. For this purpose, we will present results of about two devices working at 5.8 GHz. The first one is a tiny ion source, the world smallest microwave ion source, exactly similar to COMIC but operating at 5.8 GHz with a quarter wave cavity structure and a few watts microwave power consumption. We will show that the frequency scaling effect is effective inside such small machines. The second one is a more ambitious ion source designed around a three quarter wave structure that works with a few tens of watts at 5.8 GHz.

  9. Bayesian Non-Stationary Flood Frequency Estimation at Ungauged Basins Using Climate Information and a Scaling Model

    NASA Astrophysics Data System (ADS)

    Lima, C. H.; Lall, U.

    2010-12-01

    Flood frequency statistical analysis most often relies on stationary assumptions, where distribution moments (e.g. mean, standard deviation) and associated flood quantiles do not change over time. In this sense, one expects that flood magnitudes and their frequency of occurrence will remain constant as observed in the historical information. However, evidence of inter-annual and decadal climate variability and anthropogenic change as well as an apparent increase in the number and magnitude of flood events across the globe have made the stationary assumption questionable. Here, we show how to estimate flood quantiles (e.g. 100-year flood) at ungauged basins without needing to consider stationarity. A statistical model based on the well known flow-area scaling law is proposed to estimate flood flows at ungauged basins. The slope and intercept scaling law coefficients are assumed time varying and a hierarchical Bayesian model is used to include climate information and reduce parameter uncertainties. Cross-validated results from 34 streamflow gauges located in a nested Basin in Brazil show that the proposed model is able to estimate flood quantiles at ungauged basins with remarkable skills compared with data based estimates using the full record. The model as developed in this work is also able to simulate sequences of flood flows considering global climate changes provided an appropriate climate index developed from the General Circulation Model is used as a predictor. The time varying flood frequency estimates can be used for pricing insurance models, and in a forecast mode for preparations for flooding, and finally, for timing infrastructure investments and location. Non-stationary 95% interval estimation for the 100-year Flood (shaded gray region) and 95% interval for the 100-year flood estimated from data (horizontal dashed and solid lines). The average distribution of the 100-year flood is shown in green in the right side.

  10. High-frequency spectral falloff of earthquakes, fractal dimension of complex rupture, b value, and the scaling of strength on faults

    USGS Publications Warehouse

    Frankel, A.

    1991-01-01

    The high-frequency falloff ??-y of earthquake displacement spectra and the b value of aftershock sequences are attributed to the character of spatially varying strength along fault zones. I assume that the high frequency energy of a main shock is produced by a self-similar distribution of subevents, where the number of subevents with radii greater than R is proportional to R-D, D being the fractal dimension. In the model, an earthquake is composed of a hierarchical set of smaller earthquakes. The static stress drop is parameterized to be proportional to R??, and strength is assumed to be proportional to static stress drop. I find that a distribution of subevents with D = 2 and stress drop independent of seismic moment (?? = 0) produces a main shock with an ??-2 falloff, if the subevent areas fill the rupture area of the main shock. By equating subevents to "islands' of high stress of a random, self-similar stress field on a fault, I relate D to the scaling of strength on a fault, such that D = 2 - ??. Thus D = 2 corresponds to constant stress drop scaling (?? = 0) and scale-invariant fault strength. A self-similar model of aftershock rupture zones on a fault is used to determine the relationship between the b value, the size distribution of aftershock rupture zones, and the scaling of strength on a fault. -from Author

  11. Species frequency dynamics in an old-field succession: Effects of disturbance, fertilization and scale

    USGS Publications Warehouse

    Gibson, D.J.; Middleton, B.A.; Foster, K.; Honu, Y.A.K.; Hoyer, E.W.; Mathis, M.

    2005-01-01

    Question: Can patterns of species frequency in an old-field be explained within the context of a metapopulation model? Are the patterns observed related to time, spatial scale, disturbance, and nutrient availability? Location: Upland and lowland old-fields in Illinois, USA. Method: Species richness was recorded annually for seven years following plowing of an upland and lowland old-field subject to crossed fertilizer and disturbance treatments (mowing and rototilling). Species occupancy distributions were assessed with respect to the numbers of core and satellite species. Results: In both fields, species richness became higher in disturbed plots than in undisturbed plots over time, and decreased in fertilized plots irrespective of time. A bimodal pattern of species richness consistent with the Core-satellite species (CSS) hypothesis occurred in the initial seed bank and through the course of early succession. The identity of native and exotic core species (those present in > 90% of blocks) changed with time. Some core species from the seed bank became core species in the vegetation, albeit after several years. At the scale of individual plots, a bimodal fit consistent with the CSS hypothesis applied only in year 1 and rarely thereafter. Conclusions: The CSS hypothesis provides a metapopulation perspective for understanding patterns of species richness but requires the assessment of spatial and temporal scaling effects. Regional processes (e.g. propagule availability) at the largest scale have the greatest impact influencing community structure during early secondary succession. Local processes (e.g., disturbance and soil nutrients) are more important at smaller scales and place constraints on species establishment and community structure of both native and exotic species. Under the highest intensity of disturbance, exotic species may be able to use resources unavailable to, or unused by, native species. ?? IAVS; Opulus Press.

  12. Combined effect of constant high voltage electrostatic field and variable frequency pulsed electromagnetic field on the morphology of calcium carbonate scale in circulating cooling water systems.

    PubMed

    Zhao, Ju-Dong; Liu, Zhi-An; Zhao, Er-Jun

    2014-01-01

    Research on scale inhibition is of importance to improve the heat transfer efficiency of heat exchangers. The combined effect of high voltage electrostatic and variable frequency pulsed electromagnetic fields on calcium carbonate precipitation was investigated, both theoretically and experimentally. Using energy dispersive spectrum analysis, the predominant phase was found to be CaCO(3). The formed crystal phases mainly consist of calcite and aragonite, which is, in part, verified by theory. The results indicate that the setting of water flow velocity, and high voltage electrostatic and variable frequency pulsed electromagnetic fields is very important. Favorable values of these parameters can have a significant anti-scaling effect, with 68.95% of anti-scaling ratio for scale sample 13, while unfavorable values do not affect scale inhibition, but rather promoted fouling, such as scale sample 6. By using scanning electron microscopy analysis, when the anti-scaling ratio is positive, the particle size of scale was found to become smaller than that of untreated sample and the morphology became loose. The X-ray diffraction results verify that the good combined effect favors the appearance and growth of aragonite and restrains its transition to calcite. The mechanism for scale reduction is discussed.

  13. High frequency measurements of shot noise suppression in atomic-scale metal contacts

    NASA Astrophysics Data System (ADS)

    Wheeler, Patrick J.; Evans, Kenneth; Russom, Jeffrey; King, Nicholas; Natelson, Douglas

    2009-03-01

    Shot noise provides a means of assessing the number and transmission coefficients of transmitting channels in atomic- and molecular-scale junctions. Previous experiments at low temperatures in metal and semiconductor point contacts have demonstrated the expected suppression of shot noise when junction conductance is near an integer multiple of the conductance quantum, G0≡2e^2/h. Using high frequency techniques, we demonstrate the high speed acquisition of such data at room temperature in mechanical break junctions. In clean Au contacts conductance histograms with clear peaks at G0, 2G0, and 3G0 are acquired within hours, and histograms of simultaneous measurements of the shot noise show clear suppression at those conductance values. We describe the dependence of the noise on bias voltage and analyze the noise vs. conductance histograms in terms of a model that averages over transmission coefficients.

  14. A Frequency-Domain Implementation of a Sliding-Window Traffic Sign Detector for Large Scale Panoramic Datasets

    NASA Astrophysics Data System (ADS)

    Creusen, I. M.; Hazelhoff, L.; De With, P. H. N.

    2013-10-01

    In large-scale automatic traffic sign surveying systems, the primary computational effort is concentrated at the traffic sign detection stage. This paper focuses on reducing the computational load of particularly the sliding window object detection algorithm which is employed for traffic sign detection. Sliding-window object detectors often use a linear SVM to classify the features in a window. In this case, the classification can be seen as a convolution of the feature maps with the SVM kernel. It is well known that convolution can be efficiently implemented in the frequency domain, for kernels larger than a certain size. We show that by careful reordering of sliding-window operations, most of the frequency-domain transformations can be eliminated, leading to a substantial increase in efficiency. Additionally, we suggest to use the overlap-add method to keep the memory use within reasonable bounds. This allows us to keep all the transformed kernels in memory, thereby eliminating even more domain transformations, and allows all scales in a multiscale pyramid to be processed using the same set of transformed kernels. For a typical sliding-window implementation, we have found that the detector execution performance improves with a factor of 5.3. As a bonus, many of the detector improvements from literature, e.g. chi-squared kernel approximations, sub-class splitting algorithms etc., can be more easily applied at a lower performance penalty because of an improved scalability.

  15. The Frequency of Alcohol Use in Iranian Urban Population: The Results of a National Network Scale Up Survey.

    PubMed

    Nikfarjam, Ali; Hajimaghsoudi, Saiedeh; Rastegari, Azam; Haghdoost, Ali Akbar; Nasehi, Abbas Ali; Memaryan, Nadereh; Tarjoman, Terme; Baneshi, Mohammad Reza

    2016-08-17

    In Islamic countries alcohol consumption is considered as against religious values. Therefore, estimation of frequency of alcohol consumptions using direct methods is prone to different biases. In this study, we indirectly estimated the frequency of alcohol use in Iran, in network of a representative sample using network scale up (NSU) method. In a national survey, about 400 participants aged above 18 at each province, around 12 000 in total, were recruited. In a gender-match face to face interview, respondents were asked about the number of those who used alcohol (even one episode) in previous year in their active social network, classified by age and gender. The results were corrected for the level of visibility of alcohol consumption. The relative frequency of alcohol use at least once in previous year, among general population aged above 15, was estimated at 2.31% (95% CI: 2.12%, 2.53%). The relative frequency among males was about 8 times higher than females (4.13% versus 0.56%). The relative frequency among those aged 18 to 30 was 3 times higher than those aged above 30 (3.97% versus 1.36%). The relative frequency among male aged 18 to 30 was about 7%. It seems that the NSU is a feasible method to monitor the relative frequency of alcohol use in Iran, and possibly in countries with similar culture. Alcohol use was lower than non-Muslim countries, however, its relative frequency, in particular in young males, was noticeable. © 2017 The Author(s); Published by Kerman University of Medical Sciences. This is an open-access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

  16. Solar modulation of flood frequency in Central Europe during spring and summer on inter-annual to millennial time-scales

    NASA Astrophysics Data System (ADS)

    Czymzik, M.; Muscheler, R.; Brauer, A.

    2015-10-01

    Solar influences on climate variability are one of the most controversially discussed topics in climate research. We analyze solar forcing of flood frequency in Central Europe on inter-annual to millennial time-scales using daily discharge data of River Ammer (southern Germany) back to AD 1926 and revisiting the 5500 year flood layer time-series from varved sediments of the downstream Lake Ammersee. Flood frequency in the discharge record is significantly correlated to changes in solar activity during solar cycles 16-23 (r = -0.47, p < 0.0001, n = 73). Flood layer frequency (n = 1501) in the sediment record depicts distinct multi-decadal variability and significant correlations to 10Be fluxes from a Greenland ice core (r = 0.45, p < 0.0001) and 14C production rates (r =0.36, p < 0.0001), proxy records of solar activity. Flood frequency is higher when solar activity is reduced. These correlations between flood frequency and solar activity might provide empirical support for the solar top-down mechanism expected to modify the mid-latitude storm tracks over Europe by model studies. A lag of flood frequency responses in the Ammer discharge record to changes in solar activity of about one to three years could be explained by a modelled ocean-atmosphere feedback delaying the atmospheric reaction to solar activity variations up to a few years.

  17. A large-scale measurement of dielectric properties of normal and malignant colorectal tissues obtained from cancer surgeries at Larmor frequencies.

    PubMed

    Li, Zhou; Deng, Guanhua; Li, Zhe; Xin, Sherman Xuegang; Duan, Song; Lan, Maoying; Zhang, Sa; Gao, Yixin; He, Jun; Zhang, Songtao; Tang, Hongming; Wang, Weiwei; Han, Shuai; Yang, Qing X; Zhuang, Ling; Hu, Jiani; Liu, Feng

    2016-11-01

    Knowledge of dielectric properties of malignant human tissues is necessary for the recently developed magnetic resonance (MR) technique called MR electrical property tomography. This technique may be used in early tumor detection based on the obvious differentiation of the dielectric properties between normal and malignant tissues. However, the dielectric properties of malignant human tissues in the scale of the Larmor frequencies are not completely available in the literature. In this study, the authors focused only on the dielectric properties of colorectal tumor tissue. The dielectric properties of 504 colorectal malignant samples excised from 85 patients in the scale of the Larmor frequencies were measured using the precision open-ended coaxial probe method. The obtained complex-permittivity data were fitted to the single-pole Cole-Cole model. The median permittivity and conductivity for the malignant tissue sample were 79.3 and 0.881 S/m at 128 MHz, which were 14.6% and 17.0% higher, respectively, than those of normal tissue samples. Significant differences between normal and malignant tissues were found for the dielectric properties (p < 0.05). Experimental results indicated that the dielectric properties were significantly different between normal and malignant tissues for colorectal tissue. This large-scale clinical measurement provides more subtle base data to validate the technique of MR electrical property tomography.

  18. Increased fire frequency promotes stronger spatial genetic structure and natural selection at regional and local scales in Pinus halepensis Mill.

    PubMed

    Budde, Katharina B; González-Martínez, Santiago C; Navascués, Miguel; Burgarella, Concetta; Mosca, Elena; Lorenzo, Zaida; Zabal-Aguirre, Mario; Vendramin, Giovanni G; Verdú, Miguel; Pausas, Juli G; Heuertz, Myriam

    2017-04-01

    The recurrence of wildfires is predicted to increase due to global climate change, resulting in severe impacts on biodiversity and ecosystem functioning. Recurrent fires can drive plant adaptation and reduce genetic diversity; however, the underlying population genetic processes have not been studied in detail. In this study, the neutral and adaptive evolutionary effects of contrasting fire regimes were examined in the keystone tree species Pinus halepensis Mill. (Aleppo pine), a fire-adapted conifer. The genetic diversity, demographic history and spatial genetic structure were assessed at local (within-population) and regional scales for populations exposed to different crown fire frequencies. Eight natural P. halepensis stands were sampled in the east of the Iberian Peninsula, five of them in a region exposed to frequent crown fires (HiFi) and three of them in an adjacent region with a low frequency of crown fires (LoFi). Samples were genotyped at nine neutral simple sequence repeats (SSRs) and at 251 single nucleotide polymorphisms (SNPs) from coding regions, some of them potentially important for fire adaptation. Fire regime had no effects on genetic diversity or demographic history. Three high-differentiation outlier SNPs were identified between HiFi and LoFi stands, suggesting fire-related selection at the regional scale. At the local scale, fine-scale spatial genetic structure (SGS) was overall weak as expected for a wind-pollinated and wind-dispersed tree species. HiFi stands displayed a stronger SGS than LoFi stands at SNPs, which probably reflected the simultaneous post-fire recruitment of co-dispersed related seeds. SNPs with exceptionally strong SGS, a proxy for microenvironmental selection, were only reliably identified under the HiFi regime. An increasing fire frequency as predicted due to global change can promote increased SGS with stronger family structures and alter natural selection in P. halepensis and in plants with similar life history traits

  19. Increased fire frequency promotes stronger spatial genetic structure and natural selection at regional and local scales in Pinus halepensis Mill

    PubMed Central

    González-Martínez, Santiago C.; Navascués, Miguel; Burgarella, Concetta; Mosca, Elena; Lorenzo, Zaida; Zabal-Aguirre, Mario; Vendramin, Giovanni G.; Verdú, Miguel; Pausas, Juli G.

    2017-01-01

    Background and Aims The recurrence of wildfires is predicted to increase due to global climate change, resulting in severe impacts on biodiversity and ecosystem functioning. Recurrent fires can drive plant adaptation and reduce genetic diversity; however, the underlying population genetic processes have not been studied in detail. In this study, the neutral and adaptive evolutionary effects of contrasting fire regimes were examined in the keystone tree species Pinus halepensis Mill. (Aleppo pine), a fire-adapted conifer. The genetic diversity, demographic history and spatial genetic structure were assessed at local (within-population) and regional scales for populations exposed to different crown fire frequencies. Methods Eight natural P. halepensis stands were sampled in the east of the Iberian Peninsula, five of them in a region exposed to frequent crown fires (HiFi) and three of them in an adjacent region with a low frequency of crown fires (LoFi). Samples were genotyped at nine neutral simple sequence repeats (SSRs) and at 251 single nucleotide polymorphisms (SNPs) from coding regions, some of them potentially important for fire adaptation. Key Results Fire regime had no effects on genetic diversity or demographic history. Three high-differentiation outlier SNPs were identified between HiFi and LoFi stands, suggesting fire-related selection at the regional scale. At the local scale, fine-scale spatial genetic structure (SGS) was overall weak as expected for a wind-pollinated and wind-dispersed tree species. HiFi stands displayed a stronger SGS than LoFi stands at SNPs, which probably reflected the simultaneous post-fire recruitment of co-dispersed related seeds. SNPs with exceptionally strong SGS, a proxy for microenvironmental selection, were only reliably identified under the HiFi regime. Conclusions An increasing fire frequency as predicted due to global change can promote increased SGS with stronger family structures and alter natural selection in P

  20. Low-frequency climate anomalies, changes in synoptic scale circulation patterns and statistics of extreme events over south-east Poland during the Last Millennium

    NASA Astrophysics Data System (ADS)

    Slawinska, J. M.; Bartoszek, K.; Gabriel, C. J.

    2016-12-01

    Long-term predictions of changes in extreme event frequency are of utmost importance due to their high societal and economic impact. Yet, current projections are of limited skills as they rely on satellite records that are relatively short compared to the timescale of interest, and also due to the presence of a significant anthropogenic trend superimposed onto other low-frequency variabilities. Novel simulations of past climates provide unique opportunity to separate external perturbations from internal climate anomalies and to attribute the latter to systematic changes in different types of synoptic scale circulation and distributions of high-frequency events. Here we study such changes by employing the Last Millennium Ensemble of climate simulations carried out with the Community Earth System Model (CESM) at the U.S. National Center for Atmospheric Research, focusing in particular on decadal changes in frequency of extreme precipitation events over south-east Poland. We analyze low-frequency modulations of dominant patterns of synoptic scale circulations over Europe and their dependence on the Atlantic Meridional Overturning Circulation, along with their coupling with the North Atlantic Oscillation. Moreover, we examine whether some decades of persistently anomalous statistics of extreme events can be attributed to externally forced (e.g., via volcanic eruptions) perturbations of the North Atlantic climate. In the end, we discuss the possible linkages and physical mechanisms connecting volcanic eruptions, low-frequency variabilities of North Atlantic climate and changes in statistics of high impact weather, and compare briefly our results with some historical and paleontological records.

  1. Assessment of motivation to control alcohol use: The motivational thought frequency and state motivation scales for alcohol control.

    PubMed

    Robinson, Nicole; Kavanagh, David; Connor, Jason; May, Jon; Andrade, Jackie

    2016-08-01

    The Elaborated Intrusion Theory of Desire holds that desires for functional and dysfunctional goals share a common form. Both are embodied cognitive events, characterised by affective intensity and frequency. Accordingly, we developed scales to measure motivational cognitions for functional goals (Motivational Thought Frequency, MTF; State Motivation, SM), based on the existing Craving Experience Questionnaire (CEQ). When applied to increasing exercise, MTF and SM showed the same three-factor structure as the CEQ (Intensity, Imagery, Availability). The current study tested the internal structure and concurrent validity of the MTF and SM Scales when applied to control of alcohol consumption (MTF-A; SM-A). Participants (N=417) were adult tertiary students, staff or community members who had recently engaged in high-risk drinking or were currently trying to control alcohol consumption. They completed an online survey comprising the MTF-A, SM-A, Alcohol Use Disorders Identification Test (AUDIT), Readiness to Change Questionnaire (RCQ) and demographics. Confirmatory Factor Analysis gave acceptable fit for the MTF-A, but required the loss of one SM-A item, and was improved by intercorrelations of error terms. Higher scores were associated with more severe problems on the AUDIT and with higher Contemplation and Action scores on the RCQ. The MTF-A and SM-A show potential as measures of motivation to control drinking. Future research will examine their predictive validity and sensitivity to change. The scales' application to both increasing functional and decreasing dysfunctional behaviours is consistent with EI Theory's contention that both goal types operate in similar ways. Copyright © 2016 Elsevier Ltd. All rights reserved.

  2. Influence of 2D electrostatic effects on the high-frequency noise behavior of sub-100-nm scaled MOSFETs

    NASA Astrophysics Data System (ADS)

    Rengel, Raul; Pardo, Daniel; Martin, Maria J.

    2004-05-01

    In this work, we have performed an investigation of the consequences of dowscaling the bulk MOSFET beyond the 100 nm range by means of a particle-based Monte Carlo simulator. Taking a 250 nm gate-length ideal structure as the starting point, the constant field scaling rules (also known as "classical" scaling) are considered and the high-frequency dynamic and noise performance of transistors with 130 nm, 90 nm and 60 nm gate-lengths are studied in depth. The analysis of internal quantities such as electric fields, velocity and energy of carriers or conduction band profiles shows the increasing importance of electrostatic two-dimensional effects due to the proximity of source and drain regions even when the most ideal bias conditions are imposed. As a consequence, a loss of the transistor action for the smallest MOSFET and the degradation of the most important high-frequency figures of merit is observed. Whereas the comparative values of intrinsic noise sources (SID, SIG) are improved when reducing the dimensions and the bias voltages, the poor dynamic performance yields an overall worse noise behaviour than expected (especially for Rn and Gass), limiting at the same time the useful bias ranges and conditions for a proper low-noise configuration.

  3. Results from sudden loss of vacuum on scaled superconducting radio frequency cryomodule experiment

    NASA Astrophysics Data System (ADS)

    Dalesandro, Andrew A.; Dhuley, Ram C.; Theilacker, Jay C.; Van Sciver, Steven W.

    2014-01-01

    Superconducting radio frequency (SRF) cavities for particle accelerators are at risk of failure due to sudden loss of vacuum (SLV) adjacent to liquid helium (LHe) spaces. To better understand this failure mode and its associated risks an experiment is designed to test the longitudinal effects of SLV within the beam tube of a scaled SRF cryomodule that has considerable length relative to beam tube cross section. The scaled cryomodule consists of six individual SRF cavities each roughly 350 mm long, initially cooled to 2 K by a superfluid helium bath and a beam tube pumped to vacuum. A fast-acting solenoid valve is used to simulate SLV on the beam tube, from which point it takes over 3 s for the beam tube pressure to equalize with atmosphere, and 30 s for the helium space to reach the relief pressure of 4 bara. A SLV longitudinal effect in the beam tube is evident in both pressure and temperature data, but interestingly the temperatures responds more quickly to SLV than do the pressures. It takes 500 ms (roughly 100 ms per cavity) for the far end of the 2 m long beam tube to respond to a pressure increase compared to 300 ms for temperature (approximately 50 ms per cavity). The paper expands upon these and other results to better understand the longitudinal effect for SRF cryomodules due to SLV.

  4. Validation of a short qualitative food frequency list used in several German large scale surveys.

    PubMed

    Winkler, G; Döring, A

    1998-09-01

    Our study aimed to test the validity of a short, qualitative food frequency list (FFL) used in several German large scale surveys. In the surveys of the MONICA project Augsburg, the FFL was used in randomly selected adults. In 1984/85, a dietary survey with 7-day records (DR) was conducted within the subsample of men aged 45 to 64 (response 70%). The 899 DR were used to validate the FFL. Mean weekly food intake frequency and mean daily food intake were compared and Spearman rank order correlation coefficients and classification into tertiles with values of the statistic Kappa were calculated. Spearman correlations range between 0.15 for the item "Other sweets (candies, compote)" and 0.60 for the items "Curds, yoghurt, sour milk", "Milk including butter milk" and "Mineral water"; values for statistic Kappa vary between 0.04 ("White bread, brown bread, crispbread") and 0.41 ("Flaked oats, muesli, cornflakes" and "milk including butter milk"). With the exception of two items, FFL data can be used for analysis on group level. Analysis on individual level should be done with caution. It seems, as if some food groups are generally easier to ask for in FFL than others.

  5. 4D Cone-beam CT reconstruction using a motion model based on principal component analysis

    PubMed Central

    Staub, David; Docef, Alen; Brock, Robert S.; Vaman, Constantin; Murphy, Martin J.

    2011-01-01

    Purpose: To provide a proof of concept validation of a novel 4D cone-beam CT (4DCBCT) reconstruction algorithm and to determine the best methods to train and optimize the algorithm. Methods: The algorithm animates a patient fan-beam CT (FBCT) with a patient specific parametric motion model in order to generate a time series of deformed CTs (the reconstructed 4DCBCT) that track the motion of the patient anatomy on a voxel by voxel scale. The motion model is constrained by requiring that projections cast through the deformed CT time series match the projections of the raw patient 4DCBCT. The motion model uses a basis of eigenvectors that are generated via principal component analysis (PCA) of a training set of displacement vector fields (DVFs) that approximate patient motion. The eigenvectors are weighted by a parameterized function of the patient breathing trace recorded during 4DCBCT. The algorithm is demonstrated and tested via numerical simulation. Results: The algorithm is shown to produce accurate reconstruction results for the most complicated simulated motion, in which voxels move with a pseudo-periodic pattern and relative phase shifts exist between voxels. The tests show that principal component eigenvectors trained on DVFs from a novel 2D/3D registration method give substantially better results than eigenvectors trained on DVFs obtained by conventionally registering 4DCBCT phases reconstructed via filtered backprojection. Conclusions: Proof of concept testing has validated the 4DCBCT reconstruction approach for the types of simulated data considered. In addition, the authors found the 2D/3D registration approach to be our best choice for generating the DVF training set, and the Nelder-Mead simplex algorithm the most robust optimization routine. PMID:22149852

  6. Impacts of short-time scale water column variability on broadband high-frequency acoustic wave propagation

    NASA Astrophysics Data System (ADS)

    Eickmeier, Justin

    Acoustical oceanography is one way to study the ocean, its internal layers, boundaries and all processes occurring within using underwater acoustics. Acoustical sensing techniques allows for the measurement of ocean processes from within that logistically or financially preclude traditional in-situ measurements. Acoustic signals propagate as pressure wavefronts from a source to a receiver through an ocean medium with variable physical parameters. The water column physical parameters that change acoustic wave propagation in the ocean include temperature, salinity, current, surface roughness, seafloor bathymetry, and vertical stratification over variable time scales. The impacts of short-time scale water column variability on acoustic wave propagation include coherent and incoherent surface reflections, wavefront arrival time delay, focusing or defocusing of the intensity of acoustic beams and refraction of acoustic rays. This study focuses on high-frequency broadband acoustic waves, and examines the influence of short-time scale water column variability on broadband high-frequency acoustics, wavefronts, from 7 to 28 kHz, in shallow water. Short-time scale variability is on the order of seconds to hours and the short-spatial scale variability is on the order of few centimeters. Experimental results were collected during an acoustic experiment along 100 m isobaths and data analysis was conducted using available acoustic wave propagation models. Three main topics are studied to show that acoustic waves are viable as a remote sensing tool to measure oceanographic parameters in shallow water. First, coherent surface reflections forming striation patterns, from multipath receptions, through rough surface interaction of broadband acoustic signals with the dynamic sea surface are analyzed. Matched filtered results of received acoustic waves are compared with a ray tracing numerical model using a sea surface boundary generated from measured water wave spectra at the time of

  7. Time Correlations and the Frequency Spectrum of Sound Radiated by Turbulent Flows

    NASA Technical Reports Server (NTRS)

    Rubinstein, Robert; Zhou, Ye

    1997-01-01

    Theories of turbulent time correlations are applied to compute frequency spectra of sound radiated by isotropic turbulence and by turbulent shear flows. The hypothesis that Eulerian time correlations are dominated by the sweeping action of the most energetic scales implies that the frequency spectrum of the sound radiated by isotropic turbulence scales as omega(exp 4) for low frequencies and as omega(exp -3/4) for high frequencies. The sweeping hypothesis is applied to an approximate theory of jet noise. The high frequency noise again scales as omega(exp -3/4), but the low frequency spectrum scales as omega(exp 2). In comparison, a classical theory of jet noise based on dimensional analysis gives omega(exp -2) and omega(exp 2) scaling for these frequency ranges. It is shown that the omega(exp -2) scaling is obtained by simplifying the description of turbulent time correlations. An approximate theory of the effect of shear on turbulent time correlations is developed and applied to the frequency spectrum of sound radiated by shear turbulence. The predicted steepening of the shear dominated spectrum appears to be consistent with jet noise measurements.

  8. Diagnostics of a large-scale irregularity in the electron density near the boundary of the radio transparency frequency range of the ionosphere

    NASA Astrophysics Data System (ADS)

    Afanasiev, N. T.; Markov, V. P.

    2011-08-01

    Approximate functional relationships for the calculation of a disturbed transionogram with a trace deformation caused by the influence of a large-scale irregularity in the electron density are obtained. Numerical and asymptotic modeling of disturbed transionograms at various positions of a spacecraft relative to a ground-based observation point is performed. A possibility of the determination of the intensity and dimensions of a single large-scale irregularity near the boundary of the radio transparency frequency range of the ionosphere is demonstrated.

  9. Advances in time-scale algorithms

    NASA Technical Reports Server (NTRS)

    Stein, S. R.

    1993-01-01

    The term clock is usually used to refer to a device that counts a nearly periodic signal. A group of clocks, called an ensemble, is often used for time keeping in mission critical applications that cannot tolerate loss of time due to the failure of a single clock. The time generated by the ensemble of clocks is called a time scale. The question arises how to combine the times of the individual clocks to form the time scale. One might naively be tempted to suggest the expedient of averaging the times of the individual clocks, but a simple thought experiment demonstrates the inadequacy of this approach. Suppose a time scale is composed of two noiseless clocks having equal and opposite frequencies. The mean time scale has zero frequency. However if either clock fails, the time-scale frequency immediately changes to the frequency of the remaining clock. This performance is generally unacceptable and simple mean time scales are not used. First, previous time-scale developments are reviewed and then some new methods that result in enhanced performance are presented. The historical perspective is based upon several time scales: the AT1 and TA time scales of the National Institute of Standards and Technology (NIST), the A.1(MEAN) time scale of the US Naval observatory (USNO), the TAI time scale of the Bureau International des Poids et Measures (BIPM), and the KAS-1 time scale of the Naval Research laboratory (NRL). The new method was incorporated in the KAS-2 time scale recently developed by Timing Solutions Corporation. The goal is to present time-scale concepts in a nonmathematical form with as few equations as possible. Many other papers and texts discuss the details of the optimal estimation techniques that may be used to implement these concepts.

  10. The effect of large-scale model time step and multiscale coupling frequency on cloud climatology, vertical structure, and rainfall extremes in a superparameterized GCM

    DOE PAGES

    Yu, Sungduk; Pritchard, Michael S.

    2015-12-17

    The effect of global climate model (GCM) time step—which also controls how frequently global and embedded cloud resolving scales are coupled—is examined in the Superparameterized Community Atmosphere Model ver 3.0. Systematic bias reductions of time-mean shortwave cloud forcing (~10 W/m 2) and longwave cloud forcing (~5 W/m 2) occur as scale coupling frequency increases, but with systematically increasing rainfall variance and extremes throughout the tropics. An overarching change in the vertical structure of deep tropical convection, favoring more bottom-heavy deep convection as a global model time step is reduced may help orchestrate these responses. The weak temperature gradient approximation ismore » more faithfully satisfied when a high scale coupling frequency (a short global model time step) is used. These findings are distinct from the global model time step sensitivities of conventionally parameterized GCMs and have implications for understanding emergent behaviors of multiscale deep convective organization in superparameterized GCMs. Lastly, the results may also be useful for helping to tune them.« less

  11. The effect of large-scale model time step and multiscale coupling frequency on cloud climatology, vertical structure, and rainfall extremes in a superparameterized GCM

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

    Yu, Sungduk; Pritchard, Michael S.

    The effect of global climate model (GCM) time step—which also controls how frequently global and embedded cloud resolving scales are coupled—is examined in the Superparameterized Community Atmosphere Model ver 3.0. Systematic bias reductions of time-mean shortwave cloud forcing (~10 W/m 2) and longwave cloud forcing (~5 W/m 2) occur as scale coupling frequency increases, but with systematically increasing rainfall variance and extremes throughout the tropics. An overarching change in the vertical structure of deep tropical convection, favoring more bottom-heavy deep convection as a global model time step is reduced may help orchestrate these responses. The weak temperature gradient approximation ismore » more faithfully satisfied when a high scale coupling frequency (a short global model time step) is used. These findings are distinct from the global model time step sensitivities of conventionally parameterized GCMs and have implications for understanding emergent behaviors of multiscale deep convective organization in superparameterized GCMs. Lastly, the results may also be useful for helping to tune them.« less

  12. In Situ Polymerization and Characterization of Highly Conducting Polypyrrole Fish Scales for High-Frequency Applications

    NASA Astrophysics Data System (ADS)

    Velhal, Ninad B.; Patil, Narayan D.; Puri, Vijaya R.

    2015-12-01

    Polypyrrole (Ppy) thin films on alumina were synthesized by an in situ chemical oxidative polymerization method at 300 K with equal monomer-to-oxidant ratio. Fourier transform infrared spectroscopy (FTIR) and FT-Raman spectroscopy confirmed the formation of Ppy. A thickness-dependent change from cauliflower to fish-scale morphology was observed. Microwave properties such as transmission, reflection, shielding effectiveness, permittivity, and microwave conductivity are reported in the frequency range from 8 GHz to 12 GHz. The direct-current (DC) conductivity varied from 9.45 × 10-3 S/cm to 17.29 × 10-3 S/cm, whereas the microwave conductivity varied from 63.07 S/cm to 349.08 S/cm. The shielding effectiveness varied between 6.18 dB and 10.39 dB.

  13. Modeling of viscoelastic properties of nonpermeable porous rocks saturated with highly viscous fluid at seismic frequencies at the core scale

    NASA Astrophysics Data System (ADS)

    Wang, Zizhen; Schmitt, Douglas R.; Wang, Ruihe

    2017-08-01

    A core scale modeling method for viscoelastic properties of rocks saturated with viscous fluid at low frequencies is developed based on the stress-strain method. The elastic moduli dispersion of viscous fluid is described by the Maxwell's spring-dash pot model. Based on this modeling method, we numerically test the effects of frequency, fluid viscosity, porosity, pore size, and pore aspect ratio on the storage moduli and the stress-strain phase lag of saturated rocks. And we also compared the modeling results to the Hashin-Shtrikman bounds and the coherent potential approximation (CPA). The dynamic moduli calculated from the modeling are lower than the predictions of CPA, and both of these fall between the Hashin-Shtrikman bounds. The modeling results indicate that the frequency and the fluid viscosity have similar effects on the dynamic moduli dispersion of fully saturated rocks. We observed the Debye peak in the phase lag variation with the change of frequency and viscosity. The pore structure parameters, such as porosity, pore size, and aspect ratio affect the rock frame stiffness and result in different viscoelastic behaviors of the saturated rocks. The stress-strain phase lags are larger with smaller stiffness contrasts between the rock frame and the pore fluid. The viscoelastic properties of saturated rocks are more sensitive to aspect ratio compared to other pore structure parameters. The results suggest that significant seismic dispersion (at about 50-200 Hz) might be expected for both compressional and shear waves passing through rocks saturated with highly viscous fluids.Plain Language SummaryWe develop a core <span class="hlt">scale</span> modeling method to simulate the viscoelastic properties of rocks saturated with viscous fluid at low <span class="hlt">frequencies</span> based on the stress-strain method. The elastic moduli dispersion of viscous fluid is described by the Maxwell's spring-dash pot model. By using this modeling method, we numerically test</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA374244','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA374244"><span>Power <span class="hlt">Scaling</span> and <span class="hlt">Frequency</span> Stabilization of an Injection-Locked Laser</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2000-05-01</p> <p>In Chapter 4,1 alter the well -documented theory of locking a laser to a Fabry- Perot by performing the PDH error signal derivation in a new manner...the well -documented modulation transfer scheme to lock the <span class="hlt">frequency</span>-doubled NPRO to a hyperfine component of an electronic transition in I2. 33 I...generally true at very low noise <span class="hlt">frequencies</span>, well within the feedback loop bandwidth. However, when G0L(V„) « 1 and thus GCL(vn) « 1, Equation 3.9</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=gender+AND+spectrum&pg=5&id=EJ1029479','ERIC'); return false;" href="https://eric.ed.gov/?q=gender+AND+spectrum&pg=5&id=EJ1029479"><span>Influences of Fundamental <span class="hlt">Frequency</span>, Formant <span class="hlt">Frequencies</span>, Aperiodicity, and Spectrum Level on the Perception of Voice Gender</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Skuk, Verena G.; Schweinberger, Stefan R.</p> <p>2014-01-01</p> <p>Purpose: To determine the relative importance of acoustic parameters (fundamental <span class="hlt">frequency</span> [F0], formant <span class="hlt">frequencies</span> [FFs], aperiodicity, and spectrum level [SL]) on voice gender perception, the authors used a novel parameter-morphing approach that, unlike spectral envelope shifting, allows the application of nonuniform <span class="hlt">scale</span> factors to transform…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28679272','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28679272"><span>The <span class="hlt">frequency</span>-difference and <span class="hlt">frequency</span>-sum acoustic-field autoproducts.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Worthmann, Brian M; Dowling, David R</p> <p>2017-06-01</p> <p>The <span class="hlt">frequency</span>-difference and <span class="hlt">frequency</span>-sum autoproducts are quadratic products of solutions of the Helmholtz equation at two different <span class="hlt">frequencies</span> (ω + and ω - ), and may be constructed from the Fourier transform of any time-domain acoustic field. Interestingly, the autoproducts may carry wave-field information at the difference (ω + - ω - ) and sum (ω + + ω - ) <span class="hlt">frequencies</span> even though these <span class="hlt">frequencies</span> may not be present in the original acoustic field. This paper provides analytical and simulation results that justify and illustrate this possibility, and indicate its limitations. The analysis is based on the inhomogeneous Helmholtz equation and its solutions while the simulations are for a point source in a homogeneous half-space bounded by a perfectly reflecting surface. The analysis suggests that the autoproducts have a spatial phase structure similar to that of a true acoustic field at the difference and sum <span class="hlt">frequencies</span> if the in-band acoustic field is a plane or spherical wave. For multi-ray-path environments, this phase structure similarity persists in portions of the autoproduct fields that are not suppressed by bandwidth averaging. Discrepancies between the bandwidth-averaged autoproducts and true out-of-band acoustic fields (with potentially modified boundary conditions) <span class="hlt">scale</span> inversely with the product of the bandwidth and ray-path arrival time differences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EPJST.225.1997N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EPJST.225.1997N"><span>Time-dependent <span class="hlt">scaling</span> patterns in high <span class="hlt">frequency</span> financial data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nava, Noemi; Di Matteo, Tiziana; Aste, Tomaso</p> <p>2016-10-01</p> <p>We measure the influence of different time-<span class="hlt">scales</span> on the intraday dynamics of financial markets. This is obtained by decomposing financial time series into simple oscillations associated with distinct time-<span class="hlt">scales</span>. We propose two new time-varying measures of complexity: 1) an amplitude <span class="hlt">scaling</span> exponent and 2) an entropy-like measure. We apply these measures to intraday, 30-second sampled prices of various stock market indices. Our results reveal intraday trends where different time-horizons contribute with variable relative amplitudes over the course of the trading day. Our findings indicate that the time series we analysed have a non-stationary multifractal nature with predominantly persistent behaviour at the middle of the trading session and anti-persistent behaviour at the opening and at the closing of the session. We demonstrate that these patterns are statistically significant, robust, reproducible and characteristic of each stock market. We argue that any modelling, analytics or trading strategy must take into account these non-stationary intraday <span class="hlt">scaling</span> patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ThApC.131..573C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ThApC.131..573C"><span>On the consideration of <span class="hlt">scaling</span> properties of extreme rainfall in Madrid (Spain) for developing a generalized intensity-duration-<span class="hlt">frequency</span> equation and assessing probable maximum precipitation estimates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Casas-Castillo, M. Carmen; Rodríguez-Solà, Raúl; Navarro, Xavier; Russo, Beniamino; Lastra, Antonio; González, Paula; Redaño, Angel</p> <p>2018-01-01</p> <p>The fractal behavior of extreme rainfall intensities registered between 1940 and 2012 by the Retiro Observatory of Madrid (Spain) has been examined, and a simple <span class="hlt">scaling</span> regime ranging from 25 min to 3 days of duration has been identified. Thus, an intensity-duration-<span class="hlt">frequency</span> (IDF) master equation of the location has been constructed in terms of the simple <span class="hlt">scaling</span> formulation. The <span class="hlt">scaling</span> behavior of probable maximum precipitation (PMP) for durations between 5 min and 24 h has also been verified. For the statistical estimation of the PMP, an envelope curve of the <span class="hlt">frequency</span> factor ( k m ) based on a total of 10,194 station-years of annual maximum rainfall from 258 stations in Spain has been developed. This curve could be useful to estimate suitable values of PMP at any point of the Iberian Peninsula from basic statistical parameters (mean and standard deviation) of its rainfall series. [Figure not available: see fulltext.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29219606','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29219606"><span>Achieving Optimal Quantum Acceleration of <span class="hlt">Frequency</span> Estimation Using Adaptive Coherent Control.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Naghiloo, M; Jordan, A N; Murch, K W</p> <p>2017-11-03</p> <p>Precision measurements of <span class="hlt">frequency</span> are critical to accurate time keeping and are fundamentally limited by quantum measurement uncertainties. While for time-independent quantum Hamiltonians the uncertainty of any parameter <span class="hlt">scales</span> at best as 1/T, where T is the duration of the experiment, recent theoretical works have predicted that explicitly time-dependent Hamiltonians can yield a 1/T^{2} <span class="hlt">scaling</span> of the uncertainty for an oscillation <span class="hlt">frequency</span>. This quantum acceleration in precision requires coherent control, which is generally adaptive. We experimentally realize this quantum improvement in <span class="hlt">frequency</span> sensitivity with superconducting circuits, using a single transmon qubit. With optimal control pulses, the theoretically ideal <span class="hlt">frequency</span> precision <span class="hlt">scaling</span> is reached for times shorter than the decoherence time. This result demonstrates a fundamental quantum advantage for <span class="hlt">frequency</span> estimation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29044047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29044047"><span><span class="hlt">Scaling</span> and the <span class="hlt">frequency</span> dependence of Nyquist plot maxima of the electrical impedance of the human thigh.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shiffman, Carl</p> <p>2017-11-30</p> <p>To define and elucidate the properties of reduced-variable Nyquist plots. Non-invasive measurements of the electrical impedance of the human thigh. A retrospective analysis of the electrical impedances of 154 normal subjects measured over the past decade shows that '<span class="hlt">scaling</span>' of the Nyquist plots for human thigh muscles is a property shared by healthy thigh musculature, irrespective of subject and the length of muscle segment. Here the term <span class="hlt">scaling</span> signifies the near and sometimes 'perfect' coalescence of the separate X versus R plots into one 'reduced' Nyquist plot by the simple expedient of dividing R and X by X m , the value of X at the reactance maximum. To the extent allowed by noise levels one can say that there is one 'universal' reduced Nyquist plot for the thigh musculature of healthy subjects. There is one feature of the Nyquist curves which is not 'universal', however, namely the <span class="hlt">frequency</span> f m at which the maximum in X is observed. That is found to vary from 10 to 100 kHz. depending on subject and segment length. Analysis shows, however, that the mean value of 1/f m is an accurately linear function of segment length, though there is a small subject-to-subject random element as well. Also, following the recovery of an otherwise healthy victim of ankle fracture demonstrates the clear superiority of measurements above about 800 kHz, where <span class="hlt">scaling</span> is not observed, in contrast to measurements below about 400 kHz, where <span class="hlt">scaling</span> is accurately obeyed. The ubiquity of '<span class="hlt">scaling</span>' casts new light on the interpretation of impedance results as they are used in electrical impedance myography and bioelectric impedance analysis.</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('https://ntrs.nasa.gov/search.jsp?R=19910044054&hterms=Increased+entropy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DIncreased%2Bentropy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910044054&hterms=Increased+entropy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DIncreased%2Bentropy"><span>Implications of solar p-mode <span class="hlt">frequency</span> shifts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Goldreich, Peter; Murray, Norman; Willette, Gregory; Kumar, Pawan</p> <p>1991-01-01</p> <p>An expression is derived that relates solar p-mode <span class="hlt">frequency</span> shifts to changes in the entropy and magnetic field of the sun. The <span class="hlt">frequency</span> variations result from changes in path length and propagation speed. Path length changes dominate for entropy perturbations, and propagation speed changes dominate for most types of magnetic field peturbations. The p-mode <span class="hlt">frequencies</span> increased along with solar activity between 1986 and 1989; these <span class="hlt">frequency</span> shifts exhibited a rapid rise with increasing <span class="hlt">frequency</span> followed by a precipitous drop. The positive component of the shifts can be accounted for by variations of the mean square magnetic field strength in the vicinity of the photosphere. The magnetic stress perturbation decays above the top of the convection zone on a length <span class="hlt">scale</span> comparable to the pressure <span class="hlt">scale</span> height and grows gradually with depth below. The presence of a resonance in the chromospheric cavity means that the transition layer maintains enough coherence to partially reflect acoustic waves even near cycle maximum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1033047','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1033047"><span>Nano-<span class="hlt">Scale</span> Devices for <span class="hlt">Frequency</span>-Based Magnetic Biosensing</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-01-31</p> <p>UNLIMITED: PB Public Release 13.  SUPPLEMENTARY NOTES 14.  ABSTRACT We demonstrate via experiment and simulation that the magnetic-field-dependent <span class="hlt">frequency</span>...Stirling Highway, Crawley WA 6009; +61 8 6488 7015; Fax. Period of Performance: 06/05/2015 – 11/04/2016 Abstract: We demonstrate via experiment ...particle-induced changes to the ( quasi -)static magnetization within the active layer of the device 2 . This project however focuses on particle-induced</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3743071','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3743071"><span>How High <span class="hlt">Frequency</span> Trading Affects a Market Index</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kenett, Dror Y.; Ben-Jacob, Eshel; Stanley, H. Eugene; gur-Gershgoren, Gitit</p> <p>2013-01-01</p> <p>The relationship between a market index and its constituent stocks is complicated. While an index is a weighted average of its constituent stocks, when the investigated time <span class="hlt">scale</span> is one day or longer the index has been found to have a stronger effect on the stocks than vice versa. We explore how this interaction changes in short time <span class="hlt">scales</span> using high <span class="hlt">frequency</span> data. Using a correlation-based analysis approach, we find that in short time <span class="hlt">scales</span> stocks have a stronger influence on the index. These findings have implications for high <span class="hlt">frequency</span> trading and suggest that the price of an index should be published on shorter time <span class="hlt">scales</span>, as close as possible to those of the actual transaction time <span class="hlt">scale</span>. PMID:23817553</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/7555114','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/7555114"><span>Noise measurements during high-<span class="hlt">frequency</span> oscillatory and conventional mechanical ventilation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Berens, R J; Weigle, C G</p> <p>1995-10-01</p> <p>To evaluate the noise levels with high-<span class="hlt">frequency</span> oscillatory ventilation and conventional mechanical ventilation. An observational, prospective study. Pediatric intensive care unit. The caretakers and environment of the pediatric intensive care unit. High-<span class="hlt">frequency</span> oscillatory and conventional mechanical ventilation. Caretakers evaluated noise using a visual analog <span class="hlt">scale</span>. Noise was measured with a decibel meter and an octave band <span class="hlt">frequency</span> filter. There was twice as much noise perceived by the caretakers and as measured on the decibel A <span class="hlt">scale</span>. All measures showed significantly greater noise, especially at low <span class="hlt">frequencies</span>, with high-<span class="hlt">frequency</span> oscillatory ventilation. High-<span class="hlt">frequency</span> oscillatory ventilation exposes the patient to twice as much noise as does the use of conventional mechanical ventilation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040075044','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040075044"><span>A Method for Estimating Noise from Full-<span class="hlt">Scale</span> Distributed Exhaust Nozzles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kinzie, Kevin W.; Schein, David B.</p> <p>2004-01-01</p> <p>A method to estimate the full-<span class="hlt">scale</span> noise suppression from a <span class="hlt">scale</span> model distributed exhaust nozzle (DEN) is presented. For a conventional <span class="hlt">scale</span> model exhaust nozzle, Strouhal number <span class="hlt">scaling</span> using a <span class="hlt">scale</span> factor related to the nozzle exit area is typically applied that shifts model <span class="hlt">scale</span> <span class="hlt">frequency</span> in proportion to the geometric <span class="hlt">scale</span> factor. However, model <span class="hlt">scale</span> DEN designs have two inherent length <span class="hlt">scales</span>. One is associated with the mini-nozzles, whose size do not change in going from model <span class="hlt">scale</span> to full <span class="hlt">scale</span>. The other is associated with the overall nozzle exit area which is much smaller than full size. Consequently, lower <span class="hlt">frequency</span> energy that is generated by the coalesced jet plume should <span class="hlt">scale</span> to lower <span class="hlt">frequency</span>, but higher <span class="hlt">frequency</span> energy generated by individual mini-jets does not shift <span class="hlt">frequency</span>. In addition, jet-jet acoustic shielding by the array of mini-nozzles is a significant noise reduction effect that may change with DEN model size. A technique has been developed to <span class="hlt">scale</span> laboratory model spectral data based on the premise that high and low <span class="hlt">frequency</span> content must be treated differently during the <span class="hlt">scaling</span> process. The model-<span class="hlt">scale</span> distributed exhaust spectra are divided into low and high <span class="hlt">frequency</span> regions that are then adjusted to full <span class="hlt">scale</span> separately based on different physics-based <span class="hlt">scaling</span> laws. The regions are then recombined to create an estimate of the full-<span class="hlt">scale</span> acoustic spectra. These spectra can then be converted to perceived noise levels (PNL). The paper presents the details of this methodology and provides an example of the estimated noise suppression by a distributed exhaust nozzle compared to a round conic nozzle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030063912','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030063912"><span>Acoustic Treatment Design <span class="hlt">Scaling</span> Methods. Phase 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Clark, L. (Technical Monitor); Parrott, T. (Technical Monitor); Jones, M. (Technical Monitor); Kraft, R. E.; Yu, J.; Kwan, H. W.; Beer, B.; Seybert, A. F.; Tathavadekar, P.</p> <p>2003-01-01</p> <p>The ability to design, build and test miniaturized acoustic treatment panels on <span class="hlt">scale</span> model fan rigs representative of full <span class="hlt">scale</span> engines provides not only cost-savings, but also an opportunity to optimize the treatment by allowing multiple tests. To use <span class="hlt">scale</span> model treatment as a design tool, the impedance of the sub-<span class="hlt">scale</span> liner must be known with confidence. This study was aimed at developing impedance measurement methods for high <span class="hlt">frequencies</span>. A normal incidence impedance tube method that extends the upper <span class="hlt">frequency</span> range to 25,000 Hz. without grazing flow effects was evaluated. The free field method was investigated as a potential high <span class="hlt">frequency</span> technique. The potential of the two-microphone in-situ impedance measurement method was evaluated in the presence of grazing flow. Difficulties in achieving the high <span class="hlt">frequency</span> goals were encountered in all methods. Results of developing a time-domain finite difference resonator impedance model indicated that a re-interpretation of the empirical fluid mechanical models used in the <span class="hlt">frequency</span> domain model for nonlinear resistance and mass reactance may be required. A <span class="hlt">scale</span> model treatment design that could be tested on the Universal Propulsion Simulator vehicle was proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2562758','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2562758"><span>Low-<span class="hlt">frequency</span> and high-<span class="hlt">frequency</span> distortion product otoacoustic emission suppression in humans</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gorga, Michael P.; Neely, Stephen T.; Dierking, Darcia M.; Kopun, Judy; Jolkowski, Kristin; Groenenboom, Kristin; Tan, Hongyang; Stiegemann, Bettina</p> <p>2008-01-01</p> <p>Distortion product otoacoustic emission suppression (quantified as decrements) was measured for f2=500 and 4000 Hz, for a range of primary levels (L2), suppressor <span class="hlt">frequencies</span> (f3), and suppressor levels (L3) in 19 normal-hearing subjects. Slopes of decrement-versus-L3 functions were similar at both f2 <span class="hlt">frequencies</span>, and decreased as f3 increased. Suppression tuning curves, constructed from decrement functions, were used to estimate (1) suppression for on- and low-<span class="hlt">frequency</span> suppressors, (2) tip-to-tail differences, (3) QERB, and (4) best <span class="hlt">frequency</span>. Compression, estimated from the slope of functions relating suppression “threshold” to L2 for off-<span class="hlt">frequency</span> suppressors, was similar for 500 and 4000 Hz. Tip-to-tail differences, QERB, and best <span class="hlt">frequency</span> decreased as L2 increased for both <span class="hlt">frequencies</span>. However, tip-to-tail difference (an estimate of cochlear-amplifier gain) was 20 dB greater at 4000 Hz, compared to 500 Hz. QERB decreased to a greater extent with L2 when f2=4000 Hz, but, on an octave <span class="hlt">scale</span>, best <span class="hlt">frequency</span> shifted more with level when f2=500 Hz. These data indicate that, at both <span class="hlt">frequencies</span>, cochlear processing is nonlinear. Response growth and compression are similar at the two <span class="hlt">frequencies</span>, but gain is greater at 4000 Hz and spread of excitation is greater at 500 Hz. PMID:18397024</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/411718-time-frequency-analysis-electric-motors','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/411718-time-frequency-analysis-electric-motors"><span>Time-<span class="hlt">frequency</span> analysis of electric motors</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>Bentley, C.L.; Dunn, M.E.; Mattingly, J.K.</p> <p>1995-12-31</p> <p>Physical signals such as the current of an electric motor become nonstationary as a consequence of degraded operation and broken parts. In this instance, their power spectral densities become time dependent, and time-<span class="hlt">frequency</span> analysis techniques become the appropriate tools for signal analysis. The first among these techniques, generally called the short-time Fourier transform (STFT) method, is the Gabor transform 2 (GT) of a signal S(t), which decomposes the signal into time-local <span class="hlt">frequency</span> modes: where the window function, {Phi}(t-{tau}), is a normalized Gaussian. Alternatively, one can decompose the signal into its multi-resolution representation at different levels of magnification. This representation ismore » achieved by the continuous wavelet transform (CWT) where the function g(t) is a kernel of zero average belonging to a family of <span class="hlt">scaled</span> and shifted wavelet kernels. The CWT can be interpreted as the action of a microscope that locates the signal by the shift parameter b and adjusts its magnification by changing the <span class="hlt">scale</span> parameter a. The Fourier-transformed CWT, W,{sub g}(a, {omega}), acts as a filter that places the high-<span class="hlt">frequency</span> content of a signal into the lower end of the <span class="hlt">scale</span> spectrum and vice versa for the low <span class="hlt">frequencies</span>. Signals from a motor in three different states were analyzed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S51A0588L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S51A0588L"><span>Multi-<span class="hlt">scale</span> Slip Inversion Based on Simultaneous Spatial and Temporal Domain Wavelet Transform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, W.; Yao, H.; Yang, H. Y.</p> <p>2017-12-01</p> <p>Finite fault inversion is a widely used method to study earthquake rupture processes. Some previous studies have proposed different methods to implement finite fault inversion, including time-domain, <span class="hlt">frequency</span>-domain, and wavelet-domain methods. Many previous studies have found that different <span class="hlt">frequency</span> bands show different characteristics of the seismic rupture (e.g., Wang and Mori, 2011; Yao et al., 2011, 2013; Uchide et al., 2013; Yin et al., 2017). Generally, lower <span class="hlt">frequency</span> waveforms correspond to larger-<span class="hlt">scale</span> rupture characteristics while higher <span class="hlt">frequency</span> data are representative of smaller-<span class="hlt">scale</span> ones. Therefore, multi-<span class="hlt">scale</span> analysis can help us understand the earthquake rupture process thoroughly from larger <span class="hlt">scale</span> to smaller <span class="hlt">scale</span>. By the use of wavelet transform, the wavelet-domain methods can analyze both the time and <span class="hlt">frequency</span> information of signals in different <span class="hlt">scales</span>. Traditional wavelet-domain methods (e.g., Ji et al., 2002) implement finite fault inversion with both lower and higher <span class="hlt">frequency</span> signals together to recover larger-<span class="hlt">scale</span> and smaller-<span class="hlt">scale</span> characteristics of the rupture process simultaneously. Here we propose an alternative strategy with a two-step procedure, i.e., firstly constraining the larger-<span class="hlt">scale</span> characteristics with lower <span class="hlt">frequency</span> signals, and then resolving the smaller-<span class="hlt">scale</span> ones with higher <span class="hlt">frequency</span> signals. We have designed some synthetic tests to testify our strategy and compare it with the traditional one. We also have applied our strategy to study the 2015 Gorkha Nepal earthquake using tele-seismic waveforms. Both the traditional method and our two-step strategy only analyze the data in different temporal <span class="hlt">scales</span> (i.e., different <span class="hlt">frequency</span> bands), while the spatial distribution of model parameters also shows multi-<span class="hlt">scale</span> characteristics. A more sophisticated strategy is to transfer the slip model into different spatial <span class="hlt">scales</span>, and then analyze the smooth slip distribution (larger <span class="hlt">scales</span>) with lower <span class="hlt">frequency</span> data firstly and more</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4111839','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4111839"><span>An initial study on the estimation of time-varying volumetric treatment images and 3D tumor localization from single MV cine EPID images</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mishra, Pankaj; Li, Ruijiang; Mak, Raymond H.; Rottmann, Joerg; Bryant, Jonathan H.; Williams, Christopher L.; Berbeco, Ross I.; Lewis, John H.</p> <p>2014-01-01</p> <p>Purpose: In this work the authors develop and investigate the feasibility of a method to estimate time-varying volumetric images from individual MV cine electronic portal image device (EPID) images. Methods: The authors adopt a two-step approach to time-varying volumetric image estimation from a single cine EPID image. In the first step, a patient-specific motion model is constructed from 4DCT. In the second step, parameters in the motion model are tuned according to the information in the EPID image. The patient-specific motion model is based on a compact representation of lung motion represented in displacement vector fields (<span class="hlt">DVFs</span>). <span class="hlt">DVFs</span> are calculated through deformable image registration (DIR) of a reference 4DCT phase image (typically peak-exhale) to a set of 4DCT images corresponding to different phases of a breathing cycle. The salient characteristics in the <span class="hlt">DVFs</span> are captured in a compact representation through principal component analysis (PCA). PCA decouples the spatial and temporal components of the <span class="hlt">DVFs</span>. Spatial information is represented in eigenvectors and the temporal information is represented by eigen-coefficients. To generate a new volumetric image, the eigen-coefficients are updated via cost function optimization based on digitally reconstructed radiographs and projection images. The updated eigen-coefficients are then multiplied with the eigenvectors to obtain updated <span class="hlt">DVFs</span> that, in turn, give the volumetric image corresponding to the cine EPID image. Results: The algorithm was tested on (1) Eight digital eXtended CArdiac-Torso phantom datasets based on different irregular patient breathing patterns and (2) patient cine EPID images acquired during SBRT treatments. The root-mean-squared tumor localization error is (0.73 ± 0.63 mm) for the XCAT data and (0.90 ± 0.65 mm) for the patient data. Conclusions: The authors introduced a novel method of estimating volumetric time-varying images from single cine EPID images and a PCA-based lung motion model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22409568-initial-study-estimation-time-varying-volumetric-treatment-images-tumor-localization-from-single-mv-cine-epid-images','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22409568-initial-study-estimation-time-varying-volumetric-treatment-images-tumor-localization-from-single-mv-cine-epid-images"><span>An initial study on the estimation of time-varying volumetric treatment images and 3D tumor localization from single MV cine EPID images</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>Mishra, Pankaj, E-mail: pankaj.mishra@varian.com; Mak, Raymond H.; Rottmann, Joerg</p> <p>2014-08-15</p> <p>Purpose: In this work the authors develop and investigate the feasibility of a method to estimate time-varying volumetric images from individual MV cine electronic portal image device (EPID) images. Methods: The authors adopt a two-step approach to time-varying volumetric image estimation from a single cine EPID image. In the first step, a patient-specific motion model is constructed from 4DCT. In the second step, parameters in the motion model are tuned according to the information in the EPID image. The patient-specific motion model is based on a compact representation of lung motion represented in displacement vector fields (<span class="hlt">DVFs</span>). <span class="hlt">DVFs</span> are calculatedmore » through deformable image registration (DIR) of a reference 4DCT phase image (typically peak-exhale) to a set of 4DCT images corresponding to different phases of a breathing cycle. The salient characteristics in the <span class="hlt">DVFs</span> are captured in a compact representation through principal component analysis (PCA). PCA decouples the spatial and temporal components of the <span class="hlt">DVFs</span>. Spatial information is represented in eigenvectors and the temporal information is represented by eigen-coefficients. To generate a new volumetric image, the eigen-coefficients are updated via cost function optimization based on digitally reconstructed radiographs and projection images. The updated eigen-coefficients are then multiplied with the eigenvectors to obtain updated <span class="hlt">DVFs</span> that, in turn, give the volumetric image corresponding to the cine EPID image. Results: The algorithm was tested on (1) Eight digital eXtended CArdiac-Torso phantom datasets based on different irregular patient breathing patterns and (2) patient cine EPID images acquired during SBRT treatments. The root-mean-squared tumor localization error is (0.73 ± 0.63 mm) for the XCAT data and (0.90 ± 0.65 mm) for the patient data. Conclusions: The authors introduced a novel method of estimating volumetric time-varying images from single cine EPID images and a PCA-based lung</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Nanot..28V5203F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Nanot..28V5203F"><span><span class="hlt">Scaling</span> of graphene field-effect transistors supported on hexagonal boron nitride: radio-<span class="hlt">frequency</span> stability as a limiting factor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feijoo, Pedro C.; Pasadas, Francisco; Iglesias, José M.; Martín, María J.; Rengel, Raúl; Li, Changfeng; Kim, Wonjae; Riikonen, Juha; Lipsanen, Harri; Jiménez, David</p> <p>2017-12-01</p> <p>The quality of graphene in nanodevices has increased hugely thanks to the use of hexagonal boron nitride as a supporting layer. This paper studies to which extent hBN together with channel length <span class="hlt">scaling</span> can be exploited in graphene field-effect transistors (GFETs) to get a competitive radio-<span class="hlt">frequency</span> (RF) performance. Carrier mobility and saturation velocity were obtained from an ensemble Monte Carlo simulator that accounted for the relevant scattering mechanisms (intrinsic phonons, scattering with impurities and defects, etc). This information is fed into a self-consistent simulator, which solves the drift-diffusion equation coupled with the two-dimensional Poisson’s equation to take full account of short channel effects. Simulated GFET characteristics were benchmarked against experimental data from our fabricated devices. Our simulations show that scalability is supposed to bring to RF performance an improvement that is, however, highly limited by instability. Despite the possibility of a lower performance, a careful choice of the bias point can avoid instability. Nevertheless, maximum oscillation <span class="hlt">frequencies</span> are still achievable in the THz region for channel lengths of a few hundreds of nanometers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ESD.....9..757N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESD.....9..757N"><span>Recent trends in the <span class="hlt">frequency</span> and duration of global floods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Najibi, Nasser; Devineni, Naresh</p> <p>2018-06-01</p> <p><span class="hlt">Frequency</span> and duration of floods are analyzed using the global flood database of the Dartmouth Flood Observatory (DFO) to explore evidence of trends during 1985-2015 at global and latitudinal <span class="hlt">scales</span>. Three classes of flood duration (i.e., short: 1-7, moderate: 8-20, and long: 21 days and above) are also considered for this analysis. The nonparametric Mann-Kendall trend analysis is used to evaluate three hypotheses addressing potential monotonic trends in the <span class="hlt">frequency</span> of flood, moments of duration, and <span class="hlt">frequency</span> of specific flood duration types. We also evaluated if trends could be related to large-<span class="hlt">scale</span> atmospheric teleconnections using a generalized linear model framework. Results show that flood <span class="hlt">frequency</span> and the tails of the flood duration (long duration) have increased at both the global and the latitudinal <span class="hlt">scales</span>. In the tropics, floods have increased 4-fold since the 2000s. This increase is 2.5-fold in the north midlatitudes. However, much of the trend in <span class="hlt">frequency</span> and duration of the floods can be placed within the long-term climate variability context since the Atlantic Multidecadal Oscillation, North Atlantic Oscillation, and Pacific Decadal Oscillation were the main atmospheric teleconnections explaining this trend. There is no monotonic trend in the <span class="hlt">frequency</span> of short-duration floods across all the global and latitudinal <span class="hlt">scales</span>. There is a significant increasing trend in the annual median of flood durations globally and each latitudinal belt, and this trend is not related to these teleconnections. While the DFO data come with a certain level of epistemic uncertainty due to imprecision in the estimation of floods, overall, the analysis provides insights for understanding the <span class="hlt">frequency</span> and persistence in hydrologic extremes and how they relate to changes in the climate, organization of global and local dynamical systems, and country-<span class="hlt">scale</span> socioeconomic factors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MeScT..28k5004Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MeScT..28k5004Y"><span>JY1 time <span class="hlt">scale</span>: a new Kalman-filter time <span class="hlt">scale</span> designed at NIST</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yao, Jian; Parker, Thomas E.; Levine, Judah</p> <p>2017-11-01</p> <p>We report on a new Kalman-filter hydrogen-maser time <span class="hlt">scale</span> (i.e. JY1 time <span class="hlt">scale</span>) designed at the National Institute of Standards and Technology (NIST). The JY1 time <span class="hlt">scale</span> is composed of a few hydrogen masers and a commercial Cs clock. The Cs clock is used as a reference clock to ease operations with existing data. Unlike other time <span class="hlt">scales</span>, the JY1 time <span class="hlt">scale</span> uses three basic time-<span class="hlt">scale</span> equations, instead of only one equation. Also, this time <span class="hlt">scale</span> can detect a clock error (i.e. time error, <span class="hlt">frequency</span> error, or <span class="hlt">frequency</span> drift error) automatically. These features make the JY1 time <span class="hlt">scale</span> stiff and less likely to be affected by an abnormal clock. Tests show that the JY1 time <span class="hlt">scale</span> deviates from the UTC by less than  ±5 ns for ~100 d, when the time <span class="hlt">scale</span> is initially aligned to the UTC and then is completely free running. Once the time <span class="hlt">scale</span> is steered to a Cs fountain, it can maintain the time with little error even if the Cs fountain stops working for tens of days. This can be helpful when we do not have a continuously operated fountain or when the continuously operated fountain accidentally stops, or when optical clocks run occasionally.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27217305','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27217305"><span>Advances in high <span class="hlt">frequency</span> ultrasound separation of particulates from biomass.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Juliano, Pablo; Augustin, Mary Ann; Xu, Xin-Qing; Mawson, Raymond; Knoerzer, Kai</p> <p>2017-03-01</p> <p>In recent years the use of high <span class="hlt">frequency</span> ultrasound standing waves (megasonics) for droplet or cell separation from biomass has emerged beyond the microfluidics <span class="hlt">scale</span> into the litre to industrial <span class="hlt">scale</span> applications. The principle for this separation technology relies on the differential positioning of individual droplets or particles across an ultrasonic standing wave field within the reactor and subsequent biomass material predisposition for separation via rapid droplet agglomeration or coalescence into larger entities. Large <span class="hlt">scale</span> transducers have been characterised with sonochemiluminescence and hydrophones to enable better reactor designs. High <span class="hlt">frequency</span> enhanced separation technology has been demonstrated at industrial <span class="hlt">scale</span> for oil recovery in the palm oil industry and at litre <span class="hlt">scale</span> to assist olive oil, coconut oil and milk fat separation. Other applications include algal cell dewatering and milk fat globule fractionation. <span class="hlt">Frequency</span> selection depends on the material properties and structure in the biomass mixture. Higher <span class="hlt">frequencies</span> (1 and 2MHz) have proven preferable for better separation of materials with smaller sized droplets such as milk fat globules. For palm oil and olive oil, separation has been demonstrated within the 400-600kHz region, which has high radical production, without detectable impact on product quality. Crown Copyright © 2016. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10562518','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10562518"><span><span class="hlt">Scaling</span> of echolocation call parameters in bats.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jones, G</p> <p>1999-12-01</p> <p>I investigated the <span class="hlt">scaling</span> of echolocation call parameters (<span class="hlt">frequency</span>, duration and repetition rate) in bats in a functional context. Low-duty-cycle bats operate with search phase cycles of usually less than 20 %. They process echoes in the time domain and are therefore intolerant of pulse-echo overlap. High-duty-cycle (>30 %) species use Doppler shift compensation, and they separate pulse and echo in the <span class="hlt">frequency</span> domain. Call <span class="hlt">frequency</span> <span class="hlt">scales</span> negatively with body mass in at least five bat families. Pulse duration <span class="hlt">scales</span> positively with mass in low-duty-cycle quasi-constant-<span class="hlt">frequency</span> (QCF) species because the large aerial-hawking species that emit these signals fly fast in open habitats. They therefore detect distant targets and experience pulse-echo overlap later than do smaller bats. Pulse duration also <span class="hlt">scales</span> positively with mass in the Hipposideridae, which show at least partial Doppler shift compensation. Pulse repetition rate corresponds closely with wingbeat <span class="hlt">frequency</span> in QCF bat species that fly relatively slowly. Larger, fast-flying species often skip pulses when detecting distant targets. There is probably a trade-off between call intensity and repetition rate because 'whispering' bats (and hipposiderids) produce several calls per predicted wingbeat and because batches of calls are emitted per wingbeat during terminal buzzes. Severe atmospheric attenuation at high <span class="hlt">frequencies</span> limits the range of high-<span class="hlt">frequency</span> calls. Low-duty-cycle bats that call at high <span class="hlt">frequencies</span> must therefore use short pulses to avoid pulse-echo overlap. Rhinolophids escape this constraint by Doppler shift compensation and, importantly, can exploit advantages associated with the emission of both high-<span class="hlt">frequency</span> and long-duration calls. Low <span class="hlt">frequencies</span> are unsuited for the detection of small prey, and low repetition rates may limit prey detection rates. Echolocation parameters may therefore constrain maximum body size in aerial-hawking bats.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1338078-multiple-harmonic-frequencies-resonant-cavity-design-half-scale-prototype-measurements-fast-kicker','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1338078-multiple-harmonic-frequencies-resonant-cavity-design-half-scale-prototype-measurements-fast-kicker"><span>Multiple harmonic <span class="hlt">frequencies</span> resonant cavity design and half-<span class="hlt">scale</span> prototype measurements for a fast kicker</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Huang, Yulu; Wang, Haipeng; Wang, Shaoheng; ...</p> <p>2016-12-09</p> <p>Quarter wavelength resonator (QWR) based deflecting cavities with the capability of supporting multiple odd-harmonic modes have been developed for an ultrafast periodic kicker system in the proposed Jefferson Lab Electron Ion Collider (JLEIC, formerly MEIC). Previous work on the kicking pulse synthesis and the transverse beam dynamics tracking simulations show that a flat-top kicking pulse can be generated with minimal emittance growth during injection and circulation of the cooling electron bunches. This flat-top kicking pulse can be obtained when a DC component and 10 harmonic modes with appropriate amplitude and phase are combined together. To support 10 such harmonic modes,more » four QWR cavities are used with 5, 3, 1, and 1 modes, respectively. In the multiple-mode cavities, several slightly tapered segments of the inner conductor are introduced to tune the higher order deflecting modes to be harmonic, and stub tuners are used to fine tune each <span class="hlt">frequency</span> to compensate for potential errors. In this paper, we summarize the electromagnetic design of the five-mode cavity, including the geometry optimization to get high transverse shunt impedance, the <span class="hlt">frequency</span> tuning and sensitivity analysis, and the single loop coupler design for coupling to all of the harmonic modes. In particular we report on the design and fabrication of a half-<span class="hlt">scale</span> copper prototype of this proof-of-principle five-odd-mode cavity, as well as the rf bench measurements. Lastly, we demonstrate mode superposition in this cavity experimentally, which illustrates the kicking pulse generation concept.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1015592','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1015592"><span>Systems and methods for process and user driven dynamic voltage and <span class="hlt">frequency</span> <span class="hlt">scaling</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Mallik, Arindam [Evanston, IL; Lin, Bin [Hillsboro, OR; Memik, Gokhan [Evanston, IL; Dinda, Peter [Evanston, IL; Dick, Robert [Evanston, IL</p> <p>2011-03-22</p> <p>Certain embodiments of the present invention provide a method for power management including determining at least one of an operating <span class="hlt">frequency</span> and an operating voltage for a processor and configuring the processor based on the determined at least one of the operating <span class="hlt">frequency</span> and the operating voltage. The operating <span class="hlt">frequency</span> is determined based at least in part on direct user input. The operating voltage is determined based at least in part on an individual profile for processor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.U62A..09J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.U62A..09J"><span>Earthquake <span class="hlt">Scaling</span> Relations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jordan, T. H.; Boettcher, M.; Richardson, E.</p> <p>2002-12-01</p> <p>Using <span class="hlt">scaling</span> relations to understand nonlinear geosystems has been an enduring theme of Don Turcotte's research. In particular, his studies of <span class="hlt">scaling</span> in active fault systems have led to a series of insights about the underlying physics of earthquakes. This presentation will review some recent progress in developing <span class="hlt">scaling</span> relations for several key aspects of earthquake behavior, including the inner and outer <span class="hlt">scales</span> of dynamic fault rupture and the energetics of the rupture process. The proximate observations of mining-induced, friction-controlled events obtained from in-mine seismic networks have revealed a lower seismicity cutoff at a seismic moment Mmin near 109 Nm and a corresponding upper <span class="hlt">frequency</span> cutoff near 200 Hz, which we interpret in terms of a critical slip distance for frictional drop of about 10-4 m. Above this cutoff, the apparent stress <span class="hlt">scales</span> as M1/6 up to magnitudes of 4-5, consistent with other near-source studies in this magnitude range (see special session S07, this meeting). Such a relationship suggests a damage model in which apparent fracture energy <span class="hlt">scales</span> with the stress intensity factor at the crack tip. Under the assumption of constant stress drop, this model implies an increase in rupture velocity with seismic moment, which successfully predicts the observed variation in corner <span class="hlt">frequency</span> and maximum particle velocity. Global observations of oceanic transform faults (OTFs) allow us to investigate a situation where the outer <span class="hlt">scale</span> of earthquake size may be controlled by dynamics (as opposed to geologic heterogeneity). The seismicity data imply that the effective area for OTF moment release, AE, depends on the thermal state of the fault but is otherwise independent of fault's average slip rate; i.e., AE ~ AT, where AT is the area above a reference isotherm. The data are consistent with β = 1/2 below an upper cutoff moment Mmax that increases with AT and yield the interesting <span class="hlt">scaling</span> relation Amax ~ AT1/2. Taken together, the OTF</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4972500','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4972500"><span>Respiratory motion correction in 4D-PET by simultaneous motion estimation and image reconstruction (SMEIR)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kalantari, Faraz; Li, Tianfang; Jin, Mingwu; Wang, Jing</p> <p>2016-01-01</p> <p>In conventional 4D positron emission tomography (4D-PET), images from different frames are reconstructed individually and aligned by registration methods. Two issues that arise with this approach are as follows: 1) the reconstruction algorithms do not make full use of projection statistics; and 2) the registration between noisy images can result in poor alignment. In this study, we investigated the use of simultaneous motion estimation and image reconstruction (SMEIR) methods for motion estimation/correction in 4D-PET. A modified ordered-subset expectation maximization algorithm coupled with total variation minimization (OSEM-TV) was used to obtain a primary motion-compensated PET (pmc-PET) from all projection data, using Demons derived deformation vector fields (<span class="hlt">DVFs</span>) as initial motion vectors. A motion model update was performed to obtain an optimal set of <span class="hlt">DVFs</span> in the pmc-PET and other phases, by matching the forward projection of the deformed pmc-PET with measured projections from other phases. The OSEM-TV image reconstruction was repeated using updated <span class="hlt">DVFs</span>, and new <span class="hlt">DVFs</span> were estimated based on updated images. A 4D-XCAT phantom with typical FDG biodistribution was generated to evaluate the performance of the SMEIR algorithm in lung and liver tumors with different contrasts and different diameters (10 to 40 mm). The image quality of the 4D-PET was greatly improved by the SMEIR algorithm. When all projections were used to reconstruct 3D-PET without motion compensation, motion blurring artifacts were present, leading up to 150% tumor size overestimation and significant quantitative errors, including 50% underestimation of tumor contrast and 59% underestimation of tumor uptake. Errors were reduced to less than 10% in most images by using the SMEIR algorithm, showing its potential in motion estimation/correction in 4D-PET. PMID:27385378</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/2016PMB....61.5639K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PMB....61.5639K"><span>Respiratory motion correction in 4D-PET by simultaneous motion estimation and image reconstruction (SMEIR)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kalantari, Faraz; Li, Tianfang; Jin, Mingwu; Wang, Jing</p> <p>2016-08-01</p> <p>In conventional 4D positron emission tomography (4D-PET), images from different frames are reconstructed individually and aligned by registration methods. Two issues that arise with this approach are as follows: (1) the reconstruction algorithms do not make full use of projection statistics; and (2) the registration between noisy images can result in poor alignment. In this study, we investigated the use of simultaneous motion estimation and image reconstruction (SMEIR) methods for motion estimation/correction in 4D-PET. A modified ordered-subset expectation maximization algorithm coupled with total variation minimization (OSEM-TV) was used to obtain a primary motion-compensated PET (pmc-PET) from all projection data, using Demons derived deformation vector fields (<span class="hlt">DVFs</span>) as initial motion vectors. A motion model update was performed to obtain an optimal set of <span class="hlt">DVFs</span> in the pmc-PET and other phases, by matching the forward projection of the deformed pmc-PET with measured projections from other phases. The OSEM-TV image reconstruction was repeated using updated <span class="hlt">DVFs</span>, and new <span class="hlt">DVFs</span> were estimated based on updated images. A 4D-XCAT phantom with typical FDG biodistribution was generated to evaluate the performance of the SMEIR algorithm in lung and liver tumors with different contrasts and different diameters (10-40 mm). The image quality of the 4D-PET was greatly improved by the SMEIR algorithm. When all projections were used to reconstruct 3D-PET without motion compensation, motion blurring artifacts were present, leading up to 150% tumor size overestimation and significant quantitative errors, including 50% underestimation of tumor contrast and 59% underestimation of tumor uptake. Errors were reduced to less than 10% in most images by using the SMEIR algorithm, showing its potential in motion estimation/correction in 4D-PET.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251896-distance-preserving-rigidity-penalty-deformable-image-registration-multiple-skeletal-components-neck','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251896-distance-preserving-rigidity-penalty-deformable-image-registration-multiple-skeletal-components-neck"><span>Distance-preserving rigidity penalty on deformable image registration of multiple skeletal components in the neck</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kim, Jihun, E-mail: jihun@umich.edu; Saitou, Kazuhiro; Matuszak, Martha M.</p> <p></p> <p>Purpose: This study aims at developing and testing a novel rigidity penalty suitable for the deformable registration of tightly located skeletal components in the head and neck from planning computed tomography (CT) and daily cone-beam CT (CBCT) scans of patients undergoing radiotherapy. Methods: The proposed rigidity penalty is designed to preserve intervoxel distances within each bony structure. This penalty was tested in the intensity-based B-spline deformable registration of five cervical vertebral bodies (C1–C5). The displacement vector fields (<span class="hlt">DVFs</span>) from the registrations were compared to the <span class="hlt">DVFs</span> generated by using rigid body motions of the cervical vertebrae, measured by the surfacemore » registration of vertebrae delineated on CT and CBCT images. Twenty five pairs of planning CT (reference) and treatment CBCTs (target) from five patients were aligned without and with the penalty. An existing penalty based on the orthonormality of the deformation gradient tensor was also tested and the effects of the penalties compared. Results: The mean magnitude of the maximum registration error with the proposed distance-preserving penalty was (0.86, 1.12, 1.33) mm compared to (2.11, 2.49, 2.46) without penalty and (1.53, 1.64, 1.64) with the existing orthonormality-based penalty. The improvement in the accuracy of the deformable image registration was also verified by comparing the Procrustes distance between the <span class="hlt">DVFs</span>. With the proposed penalty, the average distance was 0.11 (σ 0.03 mm) which is smaller than 0.53 (0.1 mm) without penalty and 0.28 (0.04 mm) with the orthonormality-based penalty. Conclusions: The accuracy of aligning multiple bony elements was improved by using the proposed distance-preserving rigidity penalty. The voxel-based statistical analysis of the registration error shows that the proposed penalty improved the integrity of the <span class="hlt">DVFs</span> within the vertebral bodies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251451-distance-preserving-rigidity-penalty-deformable-image-registration-multiple-skeletal-components-neck','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251451-distance-preserving-rigidity-penalty-deformable-image-registration-multiple-skeletal-components-neck"><span>Distance-preserving rigidity penalty on deformable image registration of multiple skeletal components in the neck</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kim, Jihun, E-mail: jihun@umich.edu; Saitou, Kazuhiro; Matuszak, Martha M.</p> <p>2013-12-15</p> <p>Purpose: This study aims at developing and testing a novel rigidity penalty suitable for the deformable registration of tightly located skeletal components in the head and neck from planning computed tomography (CT) and daily cone-beam CT (CBCT) scans of patients undergoing radiotherapy. Methods: The proposed rigidity penalty is designed to preserve intervoxel distances within each bony structure. This penalty was tested in the intensity-based B-spline deformable registration of five cervical vertebral bodies (C1–C5). The displacement vector fields (<span class="hlt">DVFs</span>) from the registrations were compared to the <span class="hlt">DVFs</span> generated by using rigid body motions of the cervical vertebrae, measured by the surfacemore » registration of vertebrae delineated on CT and CBCT images. Twenty five pairs of planning CT (reference) and treatment CBCTs (target) from five patients were aligned without and with the penalty. An existing penalty based on the orthonormality of the deformation gradient tensor was also tested and the effects of the penalties compared. Results: The mean magnitude of the maximum registration error with the proposed distance-preserving penalty was (0.86, 1.12, 1.33) mm compared to (2.11, 2.49, 2.46) without penalty and (1.53, 1.64, 1.64) with the existing orthonormality-based penalty. The improvement in the accuracy of the deformable image registration was also verified by comparing the Procrustes distance between the <span class="hlt">DVFs</span>. With the proposed penalty, the average distance was 0.11 (σ 0.03 mm) which is smaller than 0.53 (0.1 mm) without penalty and 0.28 (0.04 mm) with the orthonormality-based penalty. Conclusions: The accuracy of aligning multiple bony elements was improved by using the proposed distance-preserving rigidity penalty. The voxel-based statistical analysis of the registration error shows that the proposed penalty improved the integrity of the <span class="hlt">DVFs</span> within the vertebral bodies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2878725','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2878725"><span>The temporal structures and functional significance of <span class="hlt">scale</span>-free brain activity</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>He, Biyu J.; Zempel, John M.; Snyder, Abraham Z.; Raichle, Marcus E.</p> <p>2010-01-01</p> <p>SUMMARY <span class="hlt">Scale</span>-free dynamics, with a power spectrum following P ∝ f-β, are an intrinsic feature of many complex processes in nature. In neural systems, <span class="hlt">scale</span>-free activity is often neglected in electrophysiological research. Here, we investigate <span class="hlt">scale</span>-free dynamics in human brain and show that it contains extensive nested <span class="hlt">frequencies</span>, with the phase of lower <span class="hlt">frequencies</span> modulating the amplitude of higher <span class="hlt">frequencies</span> in an upward progression across the <span class="hlt">frequency</span> spectrum. The functional significance of <span class="hlt">scale</span>-free brain activity is indicated by task performance modulation and regional variation, with β being larger in default network and visual cortex and smaller in hippocampus and cerebellum. The precise patterns of nested <span class="hlt">frequencies</span> in the brain differ from other <span class="hlt">scale</span>-free dynamics in nature, such as earth seismic waves and stock market fluctuations, suggesting system-specific generative mechanisms. Our findings reveal robust temporal structures and behavioral significance of <span class="hlt">scale</span>-free brain activity and should motivate future study on its physiological mechanisms and cognitive implications. PMID:20471349</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/wri994232/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/wri994232/"><span>Depth-Duration <span class="hlt">Frequency</span> of Precipitation for Oklahoma</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tortorelli, Robert L.; Rea, Alan; Asquith, William H.</p> <p>1999-01-01</p> <p>A regional <span class="hlt">frequency</span> analysis was conducted to estimate the depth-duration <span class="hlt">frequency</span> of precipitation for 12 durations in Oklahoma (15, 30, and 60 minutes; 1, 2, 3, 6, 12, and 24 hours; and 1, 3, and 7 days). Seven selected <span class="hlt">frequencies</span>, expressed as recurrence intervals, were investigated (2, 5, 10, 25, 50, 100, and 500 years). L-moment statistics were used to summarize depth-duration data and to determine the appropriate statistical distributions. Three different rain-gage networks provided the data (15minute, 1-hour, and 1-day). The 60-minute, and 1-hour; and the 24-hour, and 1-day durations were analyzed separately. Data were used from rain-gage stations with at least 10-years of record and within Oklahoma or about 50 kilometers into bordering states. Precipitation annual maxima (depths) were determined from the data for 110 15-minute, 141 hourly, and 413 daily stations. The L-moment statistics for depths for all durations were calculated for each station using unbiased L-mo-ment estimators for the mean, L-<span class="hlt">scale</span>, L-coefficient of variation, L-skew, and L-kur-tosis. The relation between L-skew and L-kurtosis (L-moment ratio diagram) and goodness-of-fit measures were used to select the <span class="hlt">frequency</span> distributions. The three-parameter generalized logistic distribution was selected to model the <span class="hlt">frequencies</span> of 15-, 30-, and 60-minute annual maxima; and the three-parameter generalized extreme-value distribution was selected to model the <span class="hlt">frequencies</span> of 1-hour to 7-day annual maxima. The mean for each station and duration was corrected for the bias associated with fixed interval recording of precipitation amounts. The L-<span class="hlt">scale</span> and spatially averaged L-skew statistics were used to compute the location, <span class="hlt">scale</span>, and shape parameters of the selected distribution for each station and duration. The three parameters were used to calculate the depth-duration-<span class="hlt">frequency</span> relations for each station. The precipitation depths for selected <span class="hlt">frequencies</span> were contoured from weighted depth</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27760490','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27760490"><span>The word <span class="hlt">frequency</span> effect during sentence reading: A linear or nonlinear effect of log <span class="hlt">frequency</span>?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>White, Sarah J; Drieghe, Denis; Liversedge, Simon P; Staub, Adrian</p> <p>2016-10-20</p> <p>The effect of word <span class="hlt">frequency</span> on eye movement behaviour during reading has been reported in many experimental studies. However, the vast majority of these studies compared only two levels of word <span class="hlt">frequency</span> (high and low). Here we assess whether the effect of log word <span class="hlt">frequency</span> on eye movement measures is linear, in an experiment in which a critical target word in each sentence was at one of three approximately equally spaced log <span class="hlt">frequency</span> levels. Separate analyses treated log <span class="hlt">frequency</span> as a categorical or a continuous predictor. Both analyses showed only a linear effect of log <span class="hlt">frequency</span> on the likelihood of skipping a word, and on first fixation duration. Ex-Gaussian analyses of first fixation duration showed similar effects on distributional parameters in comparing high- and medium-<span class="hlt">frequency</span> words, and medium- and low-<span class="hlt">frequency</span> words. Analyses of gaze duration and the probability of a refixation suggested a nonlinear pattern, with a larger effect at the lower end of the log <span class="hlt">frequency</span> <span class="hlt">scale</span>. However, the nonlinear effects were small, and Bayes Factor analyses favoured the simpler linear models for all measures. The possible roles of lexical and post-lexical factors in producing nonlinear effects of log word <span class="hlt">frequency</span> during sentence reading are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1710193P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1710193P"><span>Eddy-driven low-<span class="hlt">frequency</span> variability: physics and observability through altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Penduff, Thierry; Sérazin, Guillaume; Arbic, Brian; Mueller, Malte; Richman, James G.; Shriver, Jay F.; Morten, Andrew J.; Scott, Robert B.</p> <p>2015-04-01</p> <p>Model studies have revealed the propensity of the eddying ocean circulation to generate strong low-<span class="hlt">frequency</span> variability (LFV) intrinsically, i.e. without low-<span class="hlt">frequency</span> atmospheric variability. In the present study, gridded satellite altimeter products, idealized quasi-geostrophic (QG) turbulent simulations, and realistic high-resolution global ocean simulations are used to study the spontaneous tendency of mesoscale (relatively high <span class="hlt">frequency</span> and high wavenumber) kinetic energy to non-linearly cascade towards larger time and space <span class="hlt">scales</span>. The QG model reveals that large-<span class="hlt">scale</span> variability, arising from the well-known spatial inverse cascade, is associated with low <span class="hlt">frequencies</span>. Low-<span class="hlt">frequency</span>, low-wavenumber energy is maintained primarily by nonlinearities in the QG model, with forcing (by large-<span class="hlt">scale</span> shear) and friction playing secondary roles. In realistic simulations, nonlinearities also generally drive kinetic energy to low <span class="hlt">frequencies</span> and low wavenumbers. In some, but not all, regions of the gridded altimeter product, surface kinetic energy is also found to cascade toward low <span class="hlt">frequencies</span>. Exercises conducted with the realistic model suggest that the spatial and temporal filtering inherent in the construction of gridded satellite altimeter maps may contribute to the discrepancies seen in some regions between the direction of <span class="hlt">frequency</span> cascade in models versus gridded altimeter maps. Finally, the range of <span class="hlt">frequencies</span> that are highly energized and engaged these cascades appears much greater than the range of highly energized and engaged wavenumbers. Global eddying simulations, performed in the context of the CHAOCEAN project in collaboration with the CAREER project, provide estimates of the range of timescales that these oceanic nonlinearities are likely to feed without external variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S21E..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S21E..01A"><span>A Moment Rate Function Deduced from Peak Ground Motions from M 3.3-5.3 Earthquakes: Implications for <span class="hlt">Scaling</span>, Corner <span class="hlt">Frequency</span> and Stress Drop</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Archuleta, R. J.; Ji, C.</p> <p>2016-12-01</p> <p>Based on 3827 records of peak horizontal ground motions in the NGA-West2 database we computed linear regressions for Log PGA, Log PGV and the ratio PGA/2πPGV (which we call dominant <span class="hlt">frequency</span>, DomF) versus moment magnitude for M 3.3-5.3 earthquakes. The slopes are nearly one for Log PGA and Log PGV and negative one for PGA/PGV. For magnitudes 5.3 and smaller the source can be treated as a point source. Using these regressions and an expression between the half peak-to-peak amplitude of Wood Anderson records (PWA) and moment magnitude, we have deduced an `apparent' moment rate function (aMRF) that increases quadratically in time until it reaches its maximum at time tp after which it decays linearly until a final duration td. For t*=0.054 s and with parameters tp and td <span class="hlt">scaling</span> with seismic moment, tp(M0) = 0.03[M0/ M0(M=3.3)]1/7.0 and td(M0) = 0.31[M0/ M0(M=3.3)]1/3.3 . all the magnitude dependence within M 3.3-5.3 can be explained. The Fourier amplitude spectrum (FAS) of the aMRF has two corner <span class="hlt">frequencies</span> connected by an intermediate slope of f-1. The smaller corner <span class="hlt">frequency</span> fC 1/ td, i.e., a corner <span class="hlt">frequency</span> related to the full duration. Stress drop associated with the average over the fault <span class="hlt">scales</span> weakly with seismic moment Δσ M00.09. The larger corner <span class="hlt">frequency</span> is proportional to 1/ tp. We also find that DomF ≈ 1/[2.2(tp(M0) + t*)], thus there is a strong tradeoff between tp and t*. The higher corner <span class="hlt">frequency</span> and the intermediate slope in the spectrum could be completely obscured by t* for t* 0.04-0.06 s, producing a Brune-type spectrum. If so, it will be practically impossible to retrieve the true spectrum. Because the fC derived from the spectrum is controlled by td while PGA and PGV are controlled mostly by the time <span class="hlt">scale</span> tp, this aMRF could explain the difference in uncertainty of the mean stress drop inferred from peak ground motion data and that inferred from displacement amplitude spectra. This aMRF is consistent with a rupture that initiates from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1971d0026X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1971d0026X"><span><span class="hlt">Frequency</span> control of wind turbine in power system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Huawei</p> <p>2018-06-01</p> <p>In order to improve the stability of the overall <span class="hlt">frequency</span> of the power system, automatic power generation control and secondary <span class="hlt">frequency</span> adjustment were applied. Automatic power generation control was introduced into power generation planning. A dual-fed wind generator power regulation model suitable for secondary <span class="hlt">frequency</span> regulation was established. The results showed that this method satisfied the basic requirements of <span class="hlt">frequency</span> regulation control of large-<span class="hlt">scale</span> wind power access power systems and improved the stability and reliability of power system operation. Therefore, this system <span class="hlt">frequency</span> control method and strategy is relatively simple. The effect is significant. The system <span class="hlt">frequency</span> can quickly reach a steady state. It is worth applying and promoting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AIPC.1434.1567D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AIPC.1434.1567D"><span>Experiment for transient effects of sudden catastrophic loss of vacuum on a <span class="hlt">scaled</span> superconducting radio <span class="hlt">frequency</span> cryomodule</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dalesandro, Andrew A.; Theilacker, Jay; Van Sciver, Steven</p> <p>2012-06-01</p> <p>Safe operation of superconducting radio <span class="hlt">frequency</span> (SRF) cavities require design consideration of a sudden catastrophic loss of vacuum (SCLV) adjacent with liquid helium (LHe) vessels and subsequent dangers. An experiment is discussed to test the longitudinal effects of SCLV along the beam line of a string of <span class="hlt">scaled</span> SRF cavities. Each <span class="hlt">scaled</span> cavity includes one segment of beam tube within a LHe vessel containing 2 K saturated LHe, and a riser pipe connecting the LHe vessel to a common gas header. At the beam tube inlet is a fast acting solenoid valve to simulate SCLV and a high/low range orifice plate flow-meter to measure air influx to the cavity. The gas header exit also has an orifice plate flow-meter to measure helium venting the system at the relief pressure of 0.4 MPa. Each cavity is instrumented with Validyne pressure transducers and Cernox thermometers. The purpose of this experiment is to quantify the time required to spoil the beam vacuum and the effects of transient heat and mass transfer on the helium system. Heat transfer data is expected to reveal a longitudinal effect due to the geometry of the experiment. Details of the experimental design criteria and objectives are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001PhyA..289..249G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001PhyA..289..249G"><span><span class="hlt">Scaling</span> properties of foreign exchange volatility</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gençay, Ramazan; Selçuk, Faruk; Whitcher, Brandon</p> <p>2001-01-01</p> <p>In this paper, we investigate the <span class="hlt">scaling</span> properties of foreign exchange volatility. Our methodology is based on a wavelet multi-<span class="hlt">scaling</span> approach which decomposes the variance of a time series and the covariance between two time series on a <span class="hlt">scale</span> by <span class="hlt">scale</span> basis through the application of a discrete wavelet transformation. It is shown that foreign exchange rate volatilities follow different <span class="hlt">scaling</span> laws at different horizons. Particularly, there is a smaller degree of persistence in intra-day volatility as compared to volatility at one day and higher <span class="hlt">scales</span>. Therefore, a common practice in the risk management industry to convert risk measures calculated at shorter horizons into longer horizons through a global <span class="hlt">scaling</span> parameter may not be appropriate. This paper also demonstrates that correlation between the foreign exchange volatilities is the lowest at the intra-day <span class="hlt">scales</span> but exhibits a gradual increase up to a daily <span class="hlt">scale</span>. The correlation coefficient stabilizes at <span class="hlt">scales</span> one day and higher. Therefore, the benefit of currency diversification is the greatest at the intra-day <span class="hlt">scales</span> and diminishes gradually at higher <span class="hlt">scales</span> (lower <span class="hlt">frequencies</span>). The wavelet cross-correlation analysis also indicates that the association between two volatilities is stronger at lower <span class="hlt">frequencies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25873359','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25873359"><span><span class="hlt">Scaling</span> of graphene integrated circuits.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bianchi, Massimiliano; Guerriero, Erica; Fiocco, Marco; Alberti, Ruggero; Polloni, Laura; Behnam, Ashkan; Carrion, Enrique A; Pop, Eric; Sordan, Roman</p> <p>2015-05-07</p> <p>The influence of transistor size reduction (<span class="hlt">scaling</span>) on the speed of realistic multi-stage integrated circuits (ICs) represents the main performance metric of a given transistor technology. Despite extensive interest in graphene electronics, <span class="hlt">scaling</span> efforts have so far focused on individual transistors rather than multi-stage ICs. Here we study the <span class="hlt">scaling</span> of graphene ICs based on transistors from 3.3 to 0.5 μm gate lengths and with different channel widths, access lengths, and lead thicknesses. The shortest gate delay of 31 ps per stage was obtained in sub-micron graphene ROs oscillating at 4.3 GHz, which is the highest oscillation <span class="hlt">frequency</span> obtained in any strictly low-dimensional material to date. We also derived the fundamental Johnson limit, showing that <span class="hlt">scaled</span> graphene ICs could be used at high <span class="hlt">frequencies</span> in applications with small voltage swing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAG...153..113C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAG...153..113C"><span>Multi-<span class="hlt">scale</span> signed envelope inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Guo-Xin; Wu, Ru-Shan; Wang, Yu-Qing; Chen, Sheng-Chang</p> <p>2018-06-01</p> <p>Envelope inversion based on modulation signal mode was proposed to reconstruct large-<span class="hlt">scale</span> structures of underground media. In order to solve the shortcomings of conventional envelope inversion, multi-<span class="hlt">scale</span> envelope inversion was proposed using new envelope Fréchet derivative and multi-<span class="hlt">scale</span> inversion strategy to invert strong contrast models. In multi-<span class="hlt">scale</span> envelope inversion, amplitude demodulation was used to extract the low <span class="hlt">frequency</span> information from envelope data. However, only to use amplitude demodulation method will cause the loss of wavefield polarity information, thus increasing the possibility of inversion to obtain multiple solutions. In this paper we proposed a new demodulation method which can contain both the amplitude and polarity information of the envelope data. Then we introduced this demodulation method into multi-<span class="hlt">scale</span> envelope inversion, and proposed a new misfit functional: multi-<span class="hlt">scale</span> signed envelope inversion. In the numerical tests, we applied the new inversion method to the salt layer model and SEG/EAGE 2-D Salt model using low-cut source (<span class="hlt">frequency</span> components below 4 Hz were truncated). The results of numerical test demonstrated the effectiveness of this method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhyA..444..828Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhyA..444..828Y"><span>Randomness versus specifics for word-<span class="hlt">frequency</span> distributions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Xiaoyong; Minnhagen, Petter</p> <p>2016-02-01</p> <p>The text-length-dependence of real word-<span class="hlt">frequency</span> distributions can be connected to the general properties of a random book. It is pointed out that this finding has strong implications, when deciding between two conceptually different views on word-<span class="hlt">frequency</span> distributions, i.e. the specific 'Zipf's-view' and the non-specific 'Randomness-view', as is discussed. It is also noticed that the text-length transformation of a random book does have an exact <span class="hlt">scaling</span> property precisely for the power-law index γ = 1, as opposed to the Zipf's exponent γ = 2 and the implication of this exact <span class="hlt">scaling</span> property is discussed. However a real text has γ > 1 and as a consequence γ increases when shortening a real text. The connections to the predictions from the RGF (Random Group Formation) and to the infinite length-limit of a meta-book are also discussed. The difference between 'curve-fitting' and 'predicting' word-<span class="hlt">frequency</span> distributions is stressed. It is pointed out that the question of randomness versus specifics for the distribution of outcomes in case of sufficiently complex systems has a much wider relevance than just the word-<span class="hlt">frequency</span> example analyzed in the present work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3457083','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3457083"><span>Using the Daydreaming <span class="hlt">Frequency</span> <span class="hlt">Scale</span> to Investigate the Relationships between Mind-Wandering, Psychological Well-Being, and Present-Moment Awareness</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Stawarczyk, David; Majerus, Steve; Van der Linden, Martial; D’Argembeau, Arnaud</p> <p>2012-01-01</p> <p>Recent findings have shown that mind-wandering – the occurrence of stimulus-independent and task-unrelated thoughts – is associated with negative affect and lower psychological well-being. However, it remains unclear whether this relationship is due to the occurrence of mind-wandering per se or to the fact that people who mind wander more tend to be generally less attentive to present-moment experience. In three studies, we first validate a French translation of a retrospective self-report questionnaire widely used to assess the general occurrence of mind-wandering in daily life – the Daydreaming <span class="hlt">Frequency</span> <span class="hlt">Scale</span>. Using this questionnaire, we then show that the relationship between mind-wandering <span class="hlt">frequency</span> and psychological distress is fully accounted for by individual differences in dispositional mindful awareness and encoding style. These findings suggest that it may not be mind-wandering per se that is responsible for psychological distress, but rather the general tendency to be less aware and attentive to the present-moment. Thus, although mind-wandering and present-moment awareness are related constructs, they are not reducible to one another, and are distinguishable in terms of their relationship with psychological well-being. PMID:23055995</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.S12A..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.S12A..01M"><span>The origin of high <span class="hlt">frequency</span> radiation in earthquakes and the geometry of faulting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Madariaga, R.</p> <p>2004-12-01</p> <p>In a seminal paper of 1967 Kei Aki discovered the <span class="hlt">scaling</span> law of earthquake spectra and showed that, among other things, the high <span class="hlt">frequency</span> decay was of type omega-squared. This implies that high <span class="hlt">frequency</span> displacement amplitudes are proportional to a characteristic length of the fault, and radiated energy <span class="hlt">scales</span> with the cube of the fault dimension, just like seismic moment. Later in the seventies, it was found out that a simple explanation for this <span class="hlt">frequency</span> dependence of spectra was that high <span class="hlt">frequencies</span> were generated by stopping phases, waves emitted by changes in speed of the rupture front as it propagates along the fault, but this did not explain the <span class="hlt">scaling</span> of high <span class="hlt">frequency</span> waves with fault length. Earthquake energy balance is such that, ignoring attenuation, radiated energy is the change in strain energy minus energy released for overcoming friction. Until recently the latter was considered to be a material property that did not <span class="hlt">scale</span> with fault size. Yet, in another classical paper Aki and Das estimated in the late 70s that energy release rate also <span class="hlt">scaled</span> with earthquake size, because earthquakes were often stopped by barriers or changed rupture speed at them. This observation was independently confirmed in the late 90s by Ide and Takeo and Olsen et al who found that energy release rates for Kobe and Landers were in the order of a MJ/m2, implying that Gc necessarily <span class="hlt">scales</span> with earthquake size, because if this was a material property, small earthquakes would never occur. Using both simple analytical and numerical models developed by Addia-Bedia and Aochi and Madariaga, we examine the consequence of these observations for the <span class="hlt">scaling</span> of high <span class="hlt">frequency</span> waves with fault size. We demonstrate using some classical results by Kostrov, Husseiny and Freund that high <span class="hlt">frequency</span> energy flow measures energy release rate and is generated when ruptures change velocity (both direction and speed) at fault kinks or jogs. Our results explain why super shear ruptures are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009fsm..conf.....M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009fsm..conf.....M"><span><span class="hlt">Frequency</span> Standards and Metrology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maleki, Lute</p> <p>2009-04-01</p> <p> over 172 KM of installed fiber / S. Crane -- pt. X. Miniature systems. Chip-<span class="hlt">scale</span> atomic devices: precision atomic instruments based on MEMS (Invited) / J. Kitching ... [et al.]. CSAC - the chip-<span class="hlt">scale</span> atomic clock (Invited) / R. Lutwak ... [et al.]. Reaching a few 10[symbol] stability level with a compact cold atom clock / F. X. Esnault ... [et al.]. Evaluation of Lin||Lin CPT for compact and high performance <span class="hlt">frequency</span> standard / E. Breschi ... [et al.] -- pt. XI. Time <span class="hlt">scales</span>. Atomic time <span class="hlt">scales</span> TAI and TI(BIPM): present status and prospects (Invited) / G. Petit. Weight functions for biases in atomic <span class="hlt">frequency</span> standards / J. H. Shirley -- pt. XII. Interferometers. Definition and construction of noise budget in atom interferometry (Invited) / E. D'Ambriosio. Characterization of a cold atom gyroscope (Invited) / A. Landragin ... [et al.]. A mobile atom interferometer for high precision measurements of local gravity / M. Schmidt ... [et al.]. Demonstration of atom interferometer comprised of geometric beam splitters / Hiromitsu Imai and Atsuo Morinaga -- pt. XIII. New directions. Active optical clocks (Invited) / J. Chen. Prospects for a nuclear optical <span class="hlt">frequency</span> standard based on Thorium-229 (Invited) / E. Peik ... [et al.]. Whispering gallery mode oscillators and optical comb generators (Invited) / A. B. Matsko ... [et al.]. <span class="hlt">Frequency</span> comparison using energy-time entangled photons / A. Stefanov -- List of participants.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25e3102E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25e3102E"><span>Cascaded chirped photon acceleration for efficient <span class="hlt">frequency</span> conversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, Matthew R.; Qu, Kenan; Jia, Qing; Mikhailova, Julia M.; Fisch, Nathaniel J.</p> <p>2018-05-01</p> <p>A cascaded sequence of photon acceleration stages using the instantaneous creation of a plasma density gradient by flash ionization allows the generation of coherent and chirped ultraviolet and x-ray pulses with independently tunable <span class="hlt">frequency</span> and bandwidth. The efficiency of the cascaded process <span class="hlt">scales</span> with 1/ω in energy, and multiple stages produce significant <span class="hlt">frequency</span> up-conversion with gas-density plasmas. Chirping permits subsequent pulse compression to few-cycle durations, and output <span class="hlt">frequencies</span> are not limited to integer harmonics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14971883','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14971883"><span>Is there any correlation between the ATS, BTS, ERS and GOLD COPD's severity <span class="hlt">scales</span> and the <span class="hlt">frequency</span> of hospital admissions?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tsoumakidou, Maria; Tzanakis, Nikolaos; Voulgaraki, Olga; Mitrouska, Ioanna; Chrysofakis, Georgios; Samiou, Maria; Siafakas, Nikolaos M</p> <p>2004-02-01</p> <p>Disagreement exists between different COPD guidelines considering classification of severity of the disease. The aim of our study was to determine whether there is any correlation between severity <span class="hlt">scales</span> of various COPD guidelines (ATS, BTS, ERS and GOLD) and the <span class="hlt">frequency</span> of hospitalisations for COPD exacerbation. A cohort of 67 COPD patients (65 male 2 female, 45 ex-smokers, 22 current smokers, aged (69.4 +/- 1.1)) was recruited from those admitted in the pulmonary clinic of the University Hospital of Heraklion, Crete for an acute exacerbation. Lung function tests and arterial blood gases analyses were performed during stable conditions at a scheduled visit 2 months after discharge. The patients were stratified using the FEV1 percent-predicted measurement of this visit into mild, moderate and severe in accordance to the ATS, BTS, ERS and GOLD <span class="hlt">scales</span> of severity. The number of hospitalisations for acute exacerbation was recorded for the following 18 months. A total of 165 exacerbations were recorded. The correlation between the severity of COPD and the number of hospitalisations per year was statistically significant using the GOLD classification system of severity (P = 0.02 and r = 0.294). A weak correlation was also found between the number of hospitalisations and the ERS classification system (P = 0.05 and r = 0.24). No statistically significant correlation was found between the number of hospitalisations and the ATS or BTS severity <span class="hlt">scales</span>. In conclusion the GOLD and ERS classification systems of severity of COPD correlated to exacerbations causing hospitalisation. The same was not true for the ATS and BTS severity <span class="hlt">scales</span>. Better correlation was achieved with the GOLD <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5883185','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5883185"><span><span class="hlt">Frequency</span>-Specific Fractal Analysis of Postural Control Accounts for Control Strategies</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gilfriche, Pierre; Deschodt-Arsac, Véronique; Blons, Estelle; Arsac, Laurent M.</p> <p>2018-01-01</p> <p>Diverse indicators of postural control in Humans have been explored for decades, mostly based on the trajectory of the center-of-pressure. Classical approaches focus on variability, based on the notion that if a posture is too variable, the subject is not stable. Going deeper, an improved understanding of underlying physiology has been gained from studying variability in different <span class="hlt">frequency</span> ranges, pointing to specific short-loops (proprioception), and long-loops (visuo-vestibular) in neural control. More recently, fractal analyses have proliferated and become useful additional metrics of postural control. They allowed identifying two <span class="hlt">scaling</span> phenomena, respectively in short and long timescales. Here, we show that one of the most widely used methods for fractal analysis, Detrended Fluctuation Analysis, could be enhanced to account for <span class="hlt">scalings</span> on specific <span class="hlt">frequency</span> ranges. By computing and filtering a bank of synthetic fractal signals, we established how <span class="hlt">scaling</span> analysis can be focused on specific <span class="hlt">frequency</span> components. We called the obtained method <span class="hlt">Frequency</span>-specific Fractal Analysis (FsFA) and used it to associate the two <span class="hlt">scaling</span> phenomena of postural control to proprioceptive-based control loop and visuo-vestibular based control loop. After that, convincing arguments of method validity came from an application on the study of unaltered vs. altered postural control in athletes. Overall, the analysis suggests that at least two timescales contribute to postural control: a velocity-based control in short timescales relying on proprioceptive sensors, and a position-based control in longer timescales with visuo-vestibular sensors, which is a brand-new vision of postural control. <span class="hlt">Frequency</span>-specific <span class="hlt">scaling</span> exponents are promising markers of control strategies in Humans. PMID:29643816</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('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=9319&keyword=jones+AND+index&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=9319&keyword=jones+AND+index&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span><span class="hlt">SCALE</span> PROBLEMS IN REPORTING LANDSCAPE PATTERN AT THE REGIONAL <span class="hlt">SCALE</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Remotely sensed data for Southeastern United States (Standard Federal Region 4) are used to examine the <span class="hlt">scale</span> problems involved in reporting landscape pattern for a large, heterogeneous region. <span class="hlt">Frequency</span> distributions of landscape indices illustrate problems associated with the g...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFD.R4007O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFD.R4007O"><span>Micro-<span class="hlt">Scale</span> Thermoacoustics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Offner, Avshalom; Ramon, Guy Z.</p> <p>2016-11-01</p> <p>Thermoacoustic phenomena - conversion of heat to acoustic oscillations - may be harnessed for construction of reliable, practically maintenance-free engines and heat pumps. Specifically, miniaturization of thermoacoustic devices holds great promise for cooling of micro-electronic components. However, as devices size is pushed down to micro-meter <span class="hlt">scale</span> it is expected that non-negligible slip effects will exist at the solid-fluid interface. Accordingly, new theoretical models for thermoacoustic engines and heat pumps were derived, accounting for a slip boundary condition. These models are essential for the design process of micro-<span class="hlt">scale</span> thermoacoustic devices that will operate under ultrasonic <span class="hlt">frequencies</span>. Stability curves for engines - representing the onset of self-sustained oscillations - were calculated with both no-slip and slip boundary conditions, revealing improvement in the performance of engines with slip at the resonance <span class="hlt">frequency</span> range applicable for micro-<span class="hlt">scale</span> devices. Maximum achievable temperature differences curves for thermoacoustic heat pumps were calculated, revealing the negative effect of slip on the ability to pump heat up a temperature gradient. The authors acknowledge the support from the Nancy and Stephen Grand Technion Energy Program (GTEP).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGE....15..658L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGE....15..658L"><span>SNR enhancement for downhole microseismic data based on <span class="hlt">scale</span> classification shearlet transform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Juan; Ji, Shuo; Li, Yue; Qian, Zhihong; Lu, Weili</p> <p>2018-06-01</p> <p>Shearlet transform (ST) can be effective in 2D signal processing, due to its parabolic <span class="hlt">scaling</span>, high directional sensitivity, and optimal sparsity. ST combined with thresholding has been successfully applied to suppress random noise. However, because of the low magnitude and high <span class="hlt">frequency</span> of a downhole microseismic signal, the coefficient values of valid signals and noise are similar in the shearlet domain. As a result, it is difficult to use for denoising. In this paper, we present a <span class="hlt">scale</span> classification ST to solve this problem. The ST is used to decompose noisy microseismic data into serval <span class="hlt">scales</span>. By analyzing the spectrum and energy distribution of the shearlet coefficients of microseismic data, we divide the <span class="hlt">scales</span> into two types: low-<span class="hlt">frequency</span> <span class="hlt">scales</span> which contain less useful signal and high-<span class="hlt">frequency</span> <span class="hlt">scales</span> which contain more useful signal. After classification, we use two different methods to deal with the coefficients on different <span class="hlt">scales</span>. For the low-<span class="hlt">frequency</span> <span class="hlt">scales</span>, the noise is attenuated using a thresholding method. As for the high-<span class="hlt">frequency</span> <span class="hlt">scales</span>, we propose to use a generalized Gauss distribution model based a non-local means filter, which takes advantage of the temporal and spatial similarity of microseismic data. The experimental results on both synthetic records and field data illustrate that our proposed method preserves the useful components and attenuates the noise well.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015LatJP..52a..52A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015LatJP..52a..52A"><span><span class="hlt">Frequency</span> Arrangement For 700 MHz Band</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ancans, G.; Bobrovs, V.; Ivanovs, G.</p> <p>2015-02-01</p> <p>The 694-790 MHz (700 MHz) band was allocated by the 2012 World Radiocommunication Conference (WRC-12) in ITU Region 1 (Europe included), to the mobile service on a co-primary basis with other services to which this band was allocated on the primary basis and identified for the International Mobile Telecommunications (IMT). At the same time, the countries of Region 1 will be able also to continue using these <span class="hlt">frequencies</span> for their broadcasting services if necessary. This allocation will be effective immediately after 2015 World Radiocommunication Conference (WRC-15). In order to make the best possible use of this <span class="hlt">frequency</span> band for mobile service, a worldwide harmonized <span class="hlt">frequency</span> arrangement is to be prepared to allow for large economies of <span class="hlt">scale</span> and international roaming as well as utilizing the available spectrum in the best possible way, minimizing possible interference between services, facilitating deployment and cross-border coordination. The authors analyze different possible <span class="hlt">frequency</span> arrangements and conclude on the <span class="hlt">frequency</span> arrangement most suitable for Europe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/29189','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/29189"><span>Cross-<span class="hlt">scale</span> analysis of fire regimes</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Donald A. Falk; Carol Miller; Donald McKenzie; Anne E. Black</p> <p>2007-01-01</p> <p>Cross-<span class="hlt">scale</span> spatial and temporal perspectives are important for studying contagious landscape disturbances such as fire, which are controlled by myriad processes operating at different <span class="hlt">scales</span>. We examine fire regimes in forests of western North America, focusing on how observed patterns of fire <span class="hlt">frequency</span> change across spatial <span class="hlt">scales</span>. To quantify changes in fire...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22608639-eulerian-frequency-analysis-structural-vibrations-from-high-speed-video','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22608639-eulerian-frequency-analysis-structural-vibrations-from-high-speed-video"><span>Eulerian <span class="hlt">frequency</span> analysis of structural vibrations from high-speed video</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>Venanzoni, Andrea; Siemens Industry Software NV, Interleuvenlaan 68, B-3001 Leuven; De Ryck, Laurent</p> <p></p> <p>An approach for the analysis of the <span class="hlt">frequency</span> content of structural vibrations from high-speed video recordings is proposed. The techniques and tools proposed rely on an Eulerian approach, that is, using the time history of pixels independently to analyse structural motion, as opposed to Lagrangian approaches, where the motion of the structure is tracked in time. The starting point is an existing Eulerian motion magnification method, which consists in decomposing the video frames into a set of spatial <span class="hlt">scales</span> through a so-called Laplacian pyramid [1]. Each <span class="hlt">scale</span> — or level — can be amplified independently to reconstruct a magnified motionmore » of the observed structure. The approach proposed here provides two analysis tools or pre-amplification steps. The first tool provides a representation of the global <span class="hlt">frequency</span> content of a video per pyramid level. This may be further enhanced by applying an angular filter in the spatial <span class="hlt">frequency</span> domain to each frame of the video before the Laplacian pyramid decomposition, which allows for the identification of the <span class="hlt">frequency</span> content of the structural vibrations in a particular direction of space. This proposed tool complements the existing Eulerian magnification method by amplifying selectively the levels containing relevant motion information with respect to their <span class="hlt">frequency</span> content. This magnifies the displacement while limiting the noise contribution. The second tool is a holographic representation of the <span class="hlt">frequency</span> content of a vibrating structure, yielding a map of the predominant <span class="hlt">frequency</span> components across the structure. In contrast to the global <span class="hlt">frequency</span> content representation of the video, this tool provides a local analysis of the periodic gray <span class="hlt">scale</span> intensity changes of the frame in order to identify the vibrating parts of the structure and their main <span class="hlt">frequencies</span>. Validation cases are provided and the advantages and limits of the approaches are discussed. The first validation case consists of the <span class="hlt">frequency</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/542939-frequency-constant-unity-disorder','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/542939-frequency-constant-unity-disorder"><span><span class="hlt">Frequency</span>-constant Q, unity and disorder</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>Hargreaves, N.D.</p> <p>1995-12-31</p> <p>In exploration geophysics we obtain information about the earth by observing its response to different types of applied force. The response can cover the full range of possible Q values (where Q, the quality factor, is a measure of energy dissipation), from close to infinity in the case of deep crustal seismic to close to 0 in the case of many electromagnetic methods. When Q is <span class="hlt">frequency</span>-constant, however, the various types of response have a common <span class="hlt">scaling</span> behavior and can be described as being self-affine. The wave-equation then takes on a generalised form, changing from the standard wave-equation at Qmore » = {infinity} to the diffusion equation at Q = 0, via lossy, diffusive, propagation at intermediate Q values. Solutions of this wave-diffusion equation at any particular Q value can be converted to an equivalent set of results for any other Q value. In particular it is possible to convert from diffusive to wave propagation by a mapping from Q < {infinity} to Q = {infinity}. In the context of seismic sounding this is equivalent to applying inverse Q-filtering; in a more general context the mapping integrates different geophysical observations by referencing them to the common result at Q = {infinity}. The self-affinity of the observations for <span class="hlt">frequency</span>-constant Q is an expression of <span class="hlt">scale</span> invariance in the fundamental physical properties of the medium of propagation, this being the case whether the mechanism of diffusive propagation is scattering of intrinsic attenuation. <span class="hlt">Scale</span> invariance, or fractal <span class="hlt">scaling</span>, is a general property of disordered systems; the assumption of <span class="hlt">frequency</span>-constant Q not only implies a unity between different geophysical observations, but also suggests that it is the disordered nature of the earth`s sub-surface that is the unifying factor.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18447548','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18447548"><span>High <span class="hlt">frequency</span> pressure oscillator for microcryocoolers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vanapalli, S; ter Brake, H J M; Jansen, H V; Zhao, Y; Holland, H J; Burger, J F; Elwenspoek, M C</p> <p>2008-04-01</p> <p>Microminiature pulse tube cryocoolers should operate at a <span class="hlt">frequency</span> of an order higher than the conventional macro ones because the pulse tube cryocooler operating <span class="hlt">frequency</span> <span class="hlt">scales</span> inversely with the square of the pulse tube diameter. In this paper, the design and experiments of a high <span class="hlt">frequency</span> pressure oscillator is presented with the aim to power a micropulse tube cryocooler operating between 300 and 80 K, delivering a cooling power of 10 mW. Piezoelectric actuators operate efficiently at high <span class="hlt">frequencies</span> and have high power density making them good candidates as drivers for high <span class="hlt">frequency</span> pressure oscillator. The pressure oscillator described in this work consists of a membrane driven by a piezoelectric actuator. A pressure ratio of about 1.11 was achieved with a filling pressure of 2.5 MPa and compression volume of about 22.6 mm(3) when operating the actuator with a peak-to-peak sinusoidal voltage of 100 V at a <span class="hlt">frequency</span> of 1 kHz. The electrical power input was 2.73 W. The high pressure ratio and low electrical input power at high <span class="hlt">frequencies</span> would herald development of microminiature cryocoolers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008RScI...79d5103V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008RScI...79d5103V"><span>High <span class="hlt">frequency</span> pressure oscillator for microcryocoolers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vanapalli, S.; ter Brake, H. J. M.; Jansen, H. V.; Zhao, Y.; Holland, H. J.; Burger, J. F.; Elwenspoek, M. C.</p> <p>2008-04-01</p> <p>Microminiature pulse tube cryocoolers should operate at a <span class="hlt">frequency</span> of an order higher than the conventional macro ones because the pulse tube cryocooler operating <span class="hlt">frequency</span> <span class="hlt">scales</span> inversely with the square of the pulse tube diameter. In this paper, the design and experiments of a high <span class="hlt">frequency</span> pressure oscillator is presented with the aim to power a micropulse tube cryocooler operating between 300 and 80K, delivering a cooling power of 10mW. Piezoelectric actuators operate efficiently at high <span class="hlt">frequencies</span> and have high power density making them good candidates as drivers for high <span class="hlt">frequency</span> pressure oscillator. The pressure oscillator described in this work consists of a membrane driven by a piezoelectric actuator. A pressure ratio of about 1.11 was achieved with a filling pressure of 2.5MPa and compression volume of about 22.6mm3 when operating the actuator with a peak-to-peak sinusoidal voltage of 100V at a <span class="hlt">frequency</span> of 1kHz. The electrical power input was 2.73W. The high pressure ratio and low electrical input power at high <span class="hlt">frequencies</span> would herald development of microminiature cryocoolers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26469577','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26469577"><span>Power and efficiency <span class="hlt">scaling</span> of diode pumped Cr:LiSAF lasers: 770-1110 nm tuning range and <span class="hlt">frequency</span> doubling to 387-463 nm.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Demirbas, Umit; Baali, Ilyes</p> <p>2015-10-15</p> <p>We report significant average power and efficiency <span class="hlt">scaling</span> of diode-pumped Cr:LiSAF lasers in continuous-wave (cw), cw <span class="hlt">frequency</span>-doubled, and mode-locked regimes. Four single-emitter broad-area laser diodes around 660 nm were used as the pump source, which provided a total pump power of 7.2 W. To minimize thermal effects, a 20 mm long Cr:LiSAF sample with a relatively low Cr-concentration (0.8%) was used as the gain medium. In cw laser experiments, 2.4 W of output power, a slope efficiency of 50%, and a tuning range covering the 770-1110 nm region were achieved. Intracavity <span class="hlt">frequency</span> doubling with beta-barium borate (BBO) crystals generated up to 1160 mW of blue power and a record tuning range in the 387-463 nm region. When mode locked with a saturable absorber mirror, the laser produced 195 fs pulses with 580 mW of average power around 820 nm at a 100.3 MHz repetition rate. The optical-to-optical conversion efficiency of the system was 33% in cw, 16% in cw <span class="hlt">frequency</span>-doubled, and 8% in cw mode-locked regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17950029','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17950029"><span><span class="hlt">Scale</span>-free dynamics of the synchronization between sleep EEG power bands and the high <span class="hlt">frequency</span> component of heart rate variability in normal men and patients with sleep apnea-hypopnea syndrome.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dumont, Martine; Jurysta, Fabrice; Lanquart, Jean-Pol; Noseda, André; van de Borne, Philippe; Linkowski, Paul</p> <p>2007-12-01</p> <p>To investigate the dynamics of the synchronization between heart rate variability and sleep electroencephalogram power spectra and the effect of sleep apnea-hypopnea syndrome. Heart rate and sleep electroencephalogram signals were recorded in controls and patients with sleep apnea-hypopnea syndrome that were matched for age, gender, sleep parameters, and blood pressure. Spectral analysis was applied to electrocardiogram and electroencephalogram sleep recordings to obtain power values every 20s. Synchronization likelihood was computed between time series of the normalized high <span class="hlt">frequency</span> spectral component of RR-intervals and all electroencephalographic <span class="hlt">frequency</span> bands. Detrended fluctuation analysis was applied to the synchronizations in order to qualify their dynamic behaviors. For all sleep bands, the fluctuations of the synchronization between sleep EEG and heart activity appear <span class="hlt">scale</span> free and the <span class="hlt">scaling</span> exponent is close to one as for 1/f noise. We could not detect any effect due to sleep apnea-hypopnea syndrome. The synchronizations between the high <span class="hlt">frequency</span> component of heart rate variability and all sleep power bands exhibited robust fluctuations characterized by self-similar temporal behavior of 1/f noise type. No effects of sleep apnea-hypopnea syndrome were observed in these synchronizations. Sleep apnea-hypopnea syndrome does not affect the interdependence between the high <span class="hlt">frequency</span> component of heart rate variability and all sleep power bands as measured by synchronization likelihood.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24704802','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24704802"><span>Practice and transfer of the <span class="hlt">frequency</span> structures of continuous isometric force.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>King, Adam C; Newell, Karl M</p> <p>2014-04-01</p> <p>The present study examined the learning, retention and transfer of task outcome and the <span class="hlt">frequency</span>-dependent properties of isometric force output dynamics. During practice participants produced isometric force to a moderately irregular target pattern either under a constant or variable presentation. Immediate and delayed retention tests examined the persistence of practice-induced changes of force output dynamics and transfer tests investigated performance to novel (low and high) irregular target patterns. The results showed that both constant and variable practice conditions exhibited similar reductions in task error but that the <span class="hlt">frequency</span>-dependent properties were differentially modified across the entire bandwidth (0-12Hz) of force output dynamics as a function of practice. Task outcome exhibited persistent properties on the delayed retention test whereas the retention of faster time <span class="hlt">scales</span> processes (i.e., 4-12Hz) of force output was mediated as a function of <span class="hlt">frequency</span> structure. The structure of the force <span class="hlt">frequency</span> components during early practice and following a rest interval was characterized by an enhanced emphasis on the slow time <span class="hlt">scales</span> related to perceptual-motor feedback. The findings support the proposition that there are different time <span class="hlt">scales</span> of learning at the levels of task outcome and the adaptive <span class="hlt">frequency</span> bandwidths of force output dynamics. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SCPMA..60e7301H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SCPMA..60e7301H"><span>Radio-<span class="hlt">frequency</span> measurement in semiconductor quantum computation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, TianYi; Chen, MingBo; Cao, Gang; Li, HaiOu; Xiao, Ming; Guo, GuoPing</p> <p>2017-05-01</p> <p>Semiconductor quantum dots have attracted wide interest for the potential realization of quantum computation. To realize efficient quantum computation, fast manipulation and the corresponding readout are necessary. In the past few decades, considerable progress of quantum manipulation has been achieved experimentally. To meet the requirements of high-speed readout, radio-<span class="hlt">frequency</span> (RF) measurement has been developed in recent years, such as RF-QPC (radio-<span class="hlt">frequency</span> quantum point contact) and RF-DGS (radio-<span class="hlt">frequency</span> dispersive gate sensor). Here we specifically demonstrate the principle of the radio-<span class="hlt">frequency</span> reflectometry, then review the development and applications of RF measurement, which provides a feasible way to achieve high-bandwidth readout in quantum coherent control and also enriches the methods to study these artificial mesoscopic quantum systems. Finally, we prospect the future usage of radio-<span class="hlt">frequency</span> reflectometry in <span class="hlt">scaling</span>-up of the quantum computing models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........97W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........97W"><span>Multi-<span class="hlt">Scale</span> Scattering Transform in Music Similarity Measuring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Ruobai</p> <p></p> <p>Scattering transform is a Mel-<span class="hlt">frequency</span> spectrum based, time-deformation stable method, which can be used in evaluating music similarity. Compared with Dynamic time warping, it has better performance in detecting similar audio signals under local time-<span class="hlt">frequency</span> deformation. Multi-<span class="hlt">scale</span> scattering means to combine scattering transforms of different window lengths. This paper argues that, multi-<span class="hlt">scale</span> scattering transform is a good alternative of dynamic time warping in music similarity measuring. We tested the performance of multi-<span class="hlt">scale</span> scattering transform against other popular methods, with data designed to represent different conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028557','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028557"><span>Alongshore wind forcing of coastal sea level as a function of <span class="hlt">frequency</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>Ryan, H.F.; Noble, M.A.</p> <p>2006-01-01</p> <p>The amplitude of the <span class="hlt">frequency</span> response function between coastal alongshore wind stress and adjusted sea level anomalies along the west coast of the United States increases linearly as a function of the logarithm (log10) of the period for time <span class="hlt">scales</span> up to at least 60, and possibly 100, days. The amplitude of the <span class="hlt">frequency</span> response function increases even more rapidly at longer periods out to at least 5 yr. At the shortest periods, the amplitude of the <span class="hlt">frequency</span> response function is small because sea level is forced only by the local component of the wind field. The regional wind field, which controls the wind-forced response in sea level for periods between 20 and 100 days, not only has much broader spatial <span class="hlt">scales</span> than the local wind, but also propagates along the coast in the same direction as continental shelf waves. Hence, it has a stronger coupling to and an increased <span class="hlt">frequency</span> response for sea level. At periods of a year or more, observed coastal sea level fluctuations are not only forced by the regional winds, but also by joint correlations among the larger-<span class="hlt">scale</span> climatic patterns associated with El Nin??o. Therefore, the amplitude of the <span class="hlt">frequency</span> response function is large, despite the fact that the energy in the coastal wind field is relatively small. These data show that the coastal sea level response to wind stress forcing along the west coast of the United States changes in a consistent and predictable pattern over a very broad range of <span class="hlt">frequencies</span> with time <span class="hlt">scales</span> from a few days to several years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22098718-dosimetric-effect-reduction-inverse-consistency-transitivity-errors-deformable-image-registration-dose-accumulation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22098718-dosimetric-effect-reduction-inverse-consistency-transitivity-errors-deformable-image-registration-dose-accumulation"><span>On the dosimetric effect and reduction of inverse consistency and transitivity errors in deformable image registration for dose accumulation</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>Bender, Edward T.; Hardcastle, Nicholas; Tome, Wolfgang A.</p> <p>2012-01-15</p> <p>Purpose: Deformable image registration (DIR) is necessary for accurate dose accumulation between multiple radiotherapy image sets. DIR algorithms can suffer from inverse and transitivity inconsistencies. When using deformation vector fields (<span class="hlt">DVFs</span>) that exhibit inverse-inconsistency and are nontransitive, dose accumulation on a given image set via different image pathways will lead to different accumulated doses. The purpose of this study was to investigate the dosimetric effect of and propose a postprocessing solution to reduce inverse consistency and transitivity errors. Methods: Four MVCT images and four phases of a lung 4DCT, each with an associated calculated dose, were selected for analysis. DVFsmore » between all four images in each data set were created using the Fast Symmetric Demons algorithm. Dose was accumulated on the fourth image in each set using DIR via two different image pathways. The two accumulated doses on the fourth image were compared. The inverse consistency and transitivity errors in the <span class="hlt">DVFs</span> were then reduced. The dose accumulation was repeated using the processed <span class="hlt">DVFs</span>, the results of which were compared with the accumulated dose from the original <span class="hlt">DVFs</span>. To evaluate the influence of the postprocessing technique on DVF accuracy, the original and processed DVF accuracy was evaluated on the lung 4DCT data on which anatomical landmarks had been identified by an expert. Results: Dose accumulation to the same image via different image pathways resulted in two different accumulated dose results. After the inverse consistency errors were reduced, the difference between the accumulated doses diminished. The difference was further reduced after reducing the transitivity errors. The postprocessing technique had minimal effect on the accuracy of the DVF for the lung 4DCT images. Conclusions: This study shows that inverse consistency and transitivity errors in DIR have a significant dosimetric effect in dose accumulation; Depending on the image pathway</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22570116-we-ab-respiratory-motion-correction-pet-simultaneous-motion-estimation-image-reconstruction-smeir','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22570116-we-ab-respiratory-motion-correction-pet-simultaneous-motion-estimation-image-reconstruction-smeir"><span>WE-AB-204-09: Respiratory Motion Correction in 4D-PET by Simultaneous Motion Estimation and Image Reconstruction (SMEIR)</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>Kalantari, F; Wang, J; Li, T</p> <p>2015-06-15</p> <p>Purpose: In conventional 4D-PET, images from different frames are reconstructed individually and aligned by registration methods. Two issues with these approaches are: 1) Reconstruction algorithms do not make full use of all projections statistics; and 2) Image registration between noisy images can Result in poor alignment. In this study we investigated the use of simultaneous motion estimation and image reconstruction (SMEIR) method for cone beam CT for motion estimation/correction in 4D-PET. Methods: Modified ordered-subset expectation maximization algorithm coupled with total variation minimization (OSEM- TV) is used to obtain a primary motion-compensated PET (pmc-PET) from all projection data using Demons derivedmore » deformation vector fields (<span class="hlt">DVFs</span>) as initial. Motion model update is done to obtain an optimal set of <span class="hlt">DVFs</span> between the pmc-PET and other phases by matching the forward projection of the deformed pmc-PET and measured projections of other phases. Using updated <span class="hlt">DVFs</span>, OSEM- TV image reconstruction is repeated and new <span class="hlt">DVFs</span> are estimated based on updated images. 4D XCAT phantom with typical FDG biodistribution and a 10mm diameter tumor was used to evaluate the performance of the SMEIR algorithm. Results: Image quality of 4D-PET is greatly improved by the SMEIR algorithm. When all projections are used to reconstruct a 3D-PET, motion blurring artifacts are present, leading to a more than 5 times overestimation of the tumor size and 54% tumor to lung contrast ratio underestimation. This error reduced to 37% and 20% for post reconstruction registration methods and SMEIR respectively. Conclusion: SMEIR method can be used for motion estimation/correction in 4D-PET. The statistics is greatly improved since all projection data are combined together to update the image. The performance of the SMEIR algorithm for 4D-PET is sensitive to smoothness control parameters in the DVF estimation step.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22626761-su-regularized-pca-can-model-treatment-related-changes-head-neck-patients-using-daily-cbcts','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22626761-su-regularized-pca-can-model-treatment-related-changes-head-neck-patients-using-daily-cbcts"><span>SU-F-R-41: Regularized PCA Can Model Treatment-Related Changes in Head and Neck Patients Using Daily CBCTs</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>Chetvertkov, M; Henry Ford Health System, Detroit, MI; Siddiqui, F</p> <p>2016-06-15</p> <p>Purpose: To use daily cone beam CTs (CBCTs) to develop regularized principal component analysis (PCA) models of anatomical changes in head and neck (H&N) patients, to guide replanning decisions in adaptive radiation therapy (ART). Methods: Known deformations were applied to planning CT (pCT) images of 10 H&N patients to model several different systematic anatomical changes. A Pinnacle plugin was used to interpolate systematic changes over 35 fractions, generating a set of 35 synthetic CTs for each patient. Deformation vector fields (<span class="hlt">DVFs</span>) were acquired between the pCT and synthetic CTs and random fraction-to-fraction changes were superimposed on the <span class="hlt">DVFs</span>. Standard non-regularizedmore » and regularized patient-specific PCA models were built using the <span class="hlt">DVFs</span>. The ability of PCA to extract the known deformations was quantified. PCA models were also generated from clinical CBCTs, for which the deformations and <span class="hlt">DVFs</span> were not known. It was hypothesized that resulting eigenvectors/eigenfunctions with largest eigenvalues represent the major anatomical deformations during the course of treatment. Results: As demonstrated with quantitative results in the supporting document regularized PCA is more successful than standard PCA at capturing systematic changes early in the treatment. Regularized PCA is able to detect smaller systematic changes against the background of random fraction-to-fraction changes. To be successful at guiding ART, regularized PCA should be coupled with models of when anatomical changes occur: early, late or throughout the treatment course. Conclusion: The leading eigenvector/eigenfunction from the both PCA approaches can tentatively be identified as a major systematic change during radiotherapy course when systematic changes are large enough with respect to random fraction-to-fraction changes. In all cases the regularized PCA approach appears to be more reliable at capturing systematic changes, enabling dosimetric consequences to be projected once trends</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3625286','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3625286"><span>Universal distribution of component <span class="hlt">frequencies</span> in biological and technological 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>Pang, Tin Yau; Maslov, Sergei</p> <p>2013-01-01</p> <p>Bacterial genomes and large-<span class="hlt">scale</span> computer software projects both consist of a large number of components (genes or software packages) connected via a network of mutual dependencies. Components can be easily added or removed from individual systems, and their use <span class="hlt">frequencies</span> vary over many orders of magnitude. We study this <span class="hlt">frequency</span> distribution in genomes of ∼500 bacterial species and in over 2 million Linux computers and find that in both cases it is described by the same <span class="hlt">scale</span>-free power-law distribution with an additional peak near the tail of the distribution corresponding to nearly universal components. We argue that the existence of a power law distribution of <span class="hlt">frequencies</span> of components is a general property of any modular system with a multilayered dependency network. We demonstrate that the <span class="hlt">frequency</span> of a component is positively correlated with its dependency degree given by the total number of upstream components whose operation directly or indirectly depends on the selected component. The observed <span class="hlt">frequency</span>/dependency degree distributions are reproduced in a simple mathematically tractable model introduced and analyzed in this study. PMID:23530195</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4764863','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4764863"><span><span class="hlt">Frequency</span> comb transferred by surface plasmon resonance</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Geng, Xiao Tao; Chun, Byung Jae; Seo, Ji Hoon; Seo, Kwanyong; Yoon, Hana; Kim, Dong-Eon; Kim, Young-Jin; Kim, Seungchul</p> <p>2016-01-01</p> <p><span class="hlt">Frequency</span> combs, millions of narrow-linewidth optical modes referenced to an atomic clock, have shown remarkable potential in time/<span class="hlt">frequency</span> metrology, atomic/molecular spectroscopy and precision LIDARs. Applications have extended to coherent nonlinear Raman spectroscopy of molecules and quantum metrology for entangled atomic qubits. <span class="hlt">Frequency</span> combs will create novel possibilities in nano-photonics and plasmonics; however, its interrelation with surface plasmons is unexplored despite the important role that plasmonics plays in nonlinear spectroscopy and quantum optics through the manipulation of light on a subwavelength <span class="hlt">scale</span>. Here, we demonstrate that a <span class="hlt">frequency</span> comb can be transformed to a plasmonic comb in plasmonic nanostructures and reverted to the original <span class="hlt">frequency</span> comb without noticeable degradation of <6.51 × 10−19 in absolute position, 2.92 × 10−19 in stability and 1 Hz in linewidth. The results indicate that the superior performance of a well-defined <span class="hlt">frequency</span> comb can be applied to nanoplasmonic spectroscopy, quantum metrology and subwavelength photonic circuits. PMID:26898307</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('https://www.osti.gov/biblio/22413442-toward-adaptive-radiotherapy-head-neck-patients-uncertainties-dose-warping-due-choice-deformable-registration-algorithm','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22413442-toward-adaptive-radiotherapy-head-neck-patients-uncertainties-dose-warping-due-choice-deformable-registration-algorithm"><span>Toward adaptive radiotherapy for head and neck patients: Uncertainties in dose warping due to the choice of deformable registration algorithm</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>Veiga, Catarina, E-mail: catarina.veiga.11@ucl.ac.uk; Royle, Gary; Lourenço, Ana Mónica</p> <p>2015-02-15</p> <p>Purpose: The aims of this work were to evaluate the performance of several deformable image registration (DIR) algorithms implemented in our in-house software (NiftyReg) and the uncertainties inherent to using different algorithms for dose warping. Methods: The authors describe a DIR based adaptive radiotherapy workflow, using CT and cone-beam CT (CBCT) imaging. The transformations that mapped the anatomy between the two time points were obtained using four different DIR approaches available in NiftyReg. These included a standard unidirectional algorithm and more sophisticated bidirectional ones that encourage or ensure inverse consistency. The forward (CT-to-CBCT) deformation vector fields (<span class="hlt">DVFs</span>) were used tomore » propagate the CT Hounsfield units and structures to the daily geometry for “dose of the day” calculations, while the backward (CBCT-to-CT) <span class="hlt">DVFs</span> were used to remap the dose of the day onto the planning CT (pCT). Data from five head and neck patients were used to evaluate the performance of each implementation based on geometrical matching, physical properties of the <span class="hlt">DVFs</span>, and similarity between warped dose distributions. Geometrical matching was verified in terms of dice similarity coefficient (DSC), distance transform, false positives, and false negatives. The physical properties of the <span class="hlt">DVFs</span> were assessed calculating the harmonic energy, determinant of the Jacobian, and inverse consistency error of the transformations. Dose distributions were displayed on the pCT dose space and compared using dose difference (DD), distance to dose difference, and dose volume histograms. Results: All the DIR algorithms gave similar results in terms of geometrical matching, with an average DSC of 0.85 ± 0.08, but the underlying properties of the <span class="hlt">DVFs</span> varied in terms of smoothness and inverse consistency. When comparing the doses warped by different algorithms, we found a root mean square DD of 1.9% ± 0.8% of the prescribed dose (pD) and that an average of 9% ± 4</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT.........1Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT.........1Q"><span>Scheduling for energy and reliability management on multiprocessor real-time systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qi, Xuan</p> <p></p> <p>Scheduling algorithms for multiprocessor real-time systems have been studied for years with many well-recognized algorithms proposed. However, it is still an evolving research area and many problems remain open due to their intrinsic complexities. With the emergence of multicore processors, it is necessary to re-investigate the scheduling problems and design/develop efficient algorithms for better system utilization, low scheduling overhead, high energy efficiency, and better system reliability. Focusing cluster schedulings with optimal global schedulers, we study the utilization bound and scheduling overhead for a class of cluster-optimal schedulers. Then, taking energy/power consumption into consideration, we developed energy-efficient scheduling algorithms for real-time systems, especially for the proliferating embedded systems with limited energy budget. As the commonly deployed energy-saving technique (e.g. dynamic voltage <span class="hlt">frequency</span> <span class="hlt">scaling</span> (<span class="hlt">DVFS</span>)) will significantly affect system reliability, we study schedulers that have intelligent mechanisms to recuperate system reliability to satisfy the quality assurance requirements. Extensive simulation is conducted to evaluate the performance of the proposed algorithms on reduction of scheduling overhead, energy saving, and reliability improvement. The simulation results show that the proposed reliability-aware power management schemes could preserve the system reliability while still achieving substantial energy saving.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1436855','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1436855"><span>Fast Grid <span class="hlt">Frequency</span> Support from Distributed Inverter-Based Resources</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>Hoke, Anderson F</p> <p></p> <p>This presentation summarizes power hardware-in-the-loop testing performed to evaluate the ability of distributed inverter-coupled generation to support grid <span class="hlt">frequency</span> on the fastest time <span class="hlt">scales</span>. The research found that distributed PV inverters and other DERs can effectively support the grid on sub-second time <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMNG51A1652L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMNG51A1652L"><span>Do GCM's Predict the Climate.... Or the Low <span class="hlt">Frequency</span> Weather?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lovejoy, S.; Varon, D.; Schertzer, D. J.</p> <p>2011-12-01</p> <p>Over twenty-five years ago, a three-regime <span class="hlt">scaling</span> model was proposed describing the statistical variability of the atmosphere over time <span class="hlt">scales</span> ranging from weather <span class="hlt">scales</span> out to ≈ 100 kyrs. Using modern in situ data reanalyses, monthly surface series (at 5ox5o), 8 "multiproxy" (yearly) series of the Northern hemisphere from 1500- 1980, and GRIP and Vostok paleotemperatures at 5.2 and ≈ 100 year resolutions (over the past 91-420 kyrs), we refine the model and show how it can be understood with the help of new developments in nonlinear dynamics, especially multifractals and cascades. In a <span class="hlt">scaling</span> range, mean fluctuations in state variables such as temperature ΔT ≈ ΔtH the where Δt is the duration. At small (weather) <span class="hlt">scales</span> the fluctuation exponents are generally H>0; they grow with <span class="hlt">scale</span>. At longer <span class="hlt">scales</span> Δt >τw (≈ 10 days) they change sign, the fluctuations decrease with <span class="hlt">scale</span>; this is the low variability, "low <span class="hlt">frequency</span> weather" regime the spectrum is a relatively flat "plateau", it's variability is that of the usual idea of "long term weather statistics". Finally for longer times, Δt>τc ≈ 10 - 100 years, again H>0, the variability again increases with <span class="hlt">scale</span>. This is the true climate regime. These <span class="hlt">scaling</span> regimes allow us to objectively define the weather as fluctuations over periods <τw, "climate states", as fluctuations at <span class="hlt">scale</span> τc and "climate change" as the fluctuations at longer periods >τc). We show that the intermediate regime is the result of the weather regime undergoing a "dimensional transition": at temporal <span class="hlt">scales</span> longer than the typical lifetime of planetary structures (τw), the spatial degrees of freedom are rapidly quenched, only the temporal degrees of freedom are important. This low <span class="hlt">frequency</span> weather regime has statistical properties well reproduced not only by weather cascade models, but also by control runs (i.e. without climate forcing) of GCM's (including IPSL and ECHAM GCM's). In order for GCM's to go beyond simply</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70160573','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70160573"><span>Quantifying watershed-<span class="hlt">scale</span> groundwater loading and in-stream fate of nitrate using high-<span class="hlt">frequency</span> water quality data</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, Matthew P.; Tesoriero, Anthony J.; Capel, Paul D.; Pellerin, Brian A.; Hyer, Kenneth E.; Burns, Douglas A.</p> <p>2016-01-01</p> <p>We describe a new approach that couples hydrograph separation with high-<span class="hlt">frequency</span> nitrate data to quantify time-variable groundwater and runoff loading of nitrate to streams, and the net in-stream fate of nitrate at the watershed-<span class="hlt">scale</span>. The approach was applied at three sites spanning gradients in watershed size and land use in the Chesapeake Bay watershed. Results indicate that 58-73% of the annual nitrate load to the streams was groundwater-discharged nitrate. Average annual first order nitrate loss rate constants (k) were similar to those reported in both modelling and in-stream process-based studies, and were greater at the small streams (0.06 and 0.22 d-1) than at the large river (0.05 d-1), but 11% of the annual loads were retained/lost in the small streams, compared with 23% in the large river. Larger streambed area to water volume ratios in small streams result in greater loss rates, but shorter residence times in small streams result in a smaller fraction of nitrate loads being removed than in larger streams. A seasonal evaluation of k values suggests that nitrate was retained/lost at varying rates during the growing season. Consistent with previous studies, streamflow and nitrate concentration were inversely related to k. This new approach for interpreting high-<span class="hlt">frequency</span> nitrate data and the associated findings furthers our ability to understand, predict, and mitigate nitrate impacts on streams and receiving waters by providing insights into temporal nitrate dynamics that would be difficult to obtain using traditional field-based studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDG30007A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDG30007A"><span>Stabilizing Effect of Sweep on Low-<span class="hlt">Frequency</span> STBLI Unsteadiness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adler, Michael; Gaitonde, Datta</p> <p>2017-11-01</p> <p>A Large-Eddy Simulation database is generated to examine unsteady shock/turbulent boundary-layer-interaction (STBLI) mechanisms in a Mach 2 swept-compression-corner. Such interactions exhibit open separation, with separation relief from the sweep, and lack the closed mean recirculation found in spanwise-homogeneous STBLIs. We find that the swept interaction lacks the low-<span class="hlt">frequency</span> coherent shock unsteadiness, two-decades below incoming turbulent boundary layer <span class="hlt">scales</span>, that is a principal feature of comparable closed separation STBLIs. Rather, the prominent unsteady content is a mid-<span class="hlt">frequency</span> regime that develops in the separated shear layer and <span class="hlt">scales</span> weakly with the local separation length. Additionally, a linear perturbation analysis of the unsteady flow indicates that the feedback pathway (associated with an absolute instability in spanwise-homogeneous interactions) is absent in swept-compression-corner interactions. This suggests that 1) the linear oscillator is an essential component of low-<span class="hlt">frequency</span> unsteadiness in interactions with closed separation. 2) Low-<span class="hlt">frequency</span> control efforts should be focused on disrupting this oscillator. 3) Introduction of 3D effects constitute one mechanism to disrupt the oscillator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865919','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865919"><span>Low <span class="hlt">frequency</span> AC waveform generator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bilharz, Oscar W.</p> <p>1986-01-01</p> <p>Low <span class="hlt">frequency</span> sine, cosine, triangle and square waves are synthesized in circuitry which allows variation in the waveform amplitude and <span class="hlt">frequency</span> while exhibiting good stability and without requiring significant stabilization time. A triangle waveform is formed by a ramped integration process controlled by a saturation amplifier circuit which produces the necessary hysteresis for the triangle waveform. The output of the saturation circuit is tapped to produce the square waveform. The sine waveform is synthesized by taking the absolute value of the triangular waveform, raising this absolute value to a predetermined power, multiplying the raised absolute value of the triangle wave with the triangle wave itself and properly <span class="hlt">scaling</span> the resultant waveform and subtracting it from the triangular waveform itself. The cosine is synthesized by squaring the triangular waveform, raising the triangular waveform to a predetermined power and adding the squared waveform raised to the predetermined power with a DC reference and subtracting the squared waveform therefrom, with all waveforms properly <span class="hlt">scaled</span>. The resultant waveform is then multiplied with a square wave in order to correct the polarity and produce the resultant cosine waveform.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6736140','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6736140"><span>Low <span class="hlt">frequency</span> ac waveform generator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bilharz, O.W.</p> <p>1983-11-22</p> <p>Low <span class="hlt">frequency</span> sine, cosine, triangle and square waves are synthesized in circuitry which allows variation in the waveform amplitude and <span class="hlt">frequency</span> while exhibiting good stability and without requiring significant stablization time. A triangle waveform is formed by a ramped integration process controlled by a saturation amplifier circuit which produces the necessary hysteresis for the triangle waveform. The output of the saturation circuit is tapped to produce the square waveform. The sine waveform is synthesized by taking the absolute value of the triangular waveform, raising this absolute value to a predetermined power, multiplying the raised absolute value of the triangle wave with the triangle wave itself and properly <span class="hlt">scaling</span> the resultant waveform and subtracting it from the triangular waveform to a predetermined power and adding the squared waveform raised to the predetermined power with a DC reference and subtracting the squared waveform therefrom, with all waveforms properly <span class="hlt">scaled</span>. The resultant waveform is then multiplied with a square wave in order to correct the polarity and produce the resultant cosine waveform.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413219L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413219L"><span>Do GCM's predict the climate.... Or the low <span class="hlt">frequency</span> weather?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lovejoy, S.; Schertzer, D.; Varon, D.</p> <p>2012-04-01</p> <p>Over twenty-five years ago, a three-regime <span class="hlt">scaling</span> model was proposed describing the statistical variability of the atmosphere over time <span class="hlt">scales</span> ranging from weather <span class="hlt">scales</span> out to ≈ 100 kyrs. Using modern in situ data reanalyses, monthly surface series (at 5ox5o), 8 "multiproxy" (yearly) series of the Northern hemisphere from 1500 - 1980, and GRIP and Vostok paleotemperatures at 5.2 and ≈ 100 year resolutions (over the past 91-420 kyrs), we refine the model and show how it can be understood with the help of new developments in nonlinear dynamics, especially multifractals and cascades. In a <span class="hlt">scaling</span> range, mean fluctuations in state variables such as temperature ΔT vary in power law manners ≈ Δt**H the where Δt is the duration. At small (weather) <span class="hlt">scales</span> the fluctuation exponents are generally H>0; they grow with <span class="hlt">scale</span> (Δt). At longer <span class="hlt">scales</span> Δt >τw (≈ 10 days) H changes sign, the fluctuations decrease with <span class="hlt">scale</span>; this is the low variability, "low <span class="hlt">frequency</span> weather" regime. In this regime, the spectrum is a relatively flat "plateau", it's variability is low, stable, corresponding to our usual idea of "long term weather statistics". Finally for longer times, Δt>τc ≈ 10 - 100 years, once again H>0, so that the variability increases with <span class="hlt">scale</span>: the true climate regime. These <span class="hlt">scaling</span> regimes allow us to objectively define the weather as fluctuations over periods <τw, to define "climate states" as fluctuations at <span class="hlt">scale</span> τc and then "climate change" as the fluctuations at longer periods (Δt>τc). We show that the intermediate low <span class="hlt">frequency</span> weather regime is the result of the weather regime undergoing a "dimensional transition": at temporal <span class="hlt">scales</span> longer than the typical lifetime of planetary structures (τw), the spatial degrees of freedom are rapidly quenched so that only the temporal degrees of freedom are important. This low <span class="hlt">frequency</span> weather regime has statistical properties well reproduced not only by stochastic cascade models of weather, but also by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940026151','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940026151"><span>Accuracy metrics for judging time <span class="hlt">scale</span> algorithms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Douglas, R. J.; Boulanger, J.-S.; Jacques, C.</p> <p>1994-01-01</p> <p>Time <span class="hlt">scales</span> have been constructed in different ways to meet the many demands placed upon them for time accuracy, <span class="hlt">frequency</span> accuracy, long-term stability, and robustness. Usually, no single time <span class="hlt">scale</span> is optimum for all purposes. In the context of the impending availability of high-accuracy intermittently-operated cesium fountains, we reconsider the question of evaluating the accuracy of time <span class="hlt">scales</span> which use an algorithm to span interruptions of the primary standard. We consider a broad class of calibration algorithms that can be evaluated and compared quantitatively for their accuracy in the presence of <span class="hlt">frequency</span> drift and a full noise model (a mixture of white PM, flicker PM, white FM, flicker FM, and random walk FM noise). We present the analytic techniques for computing the standard uncertainty for the full noise model and this class of calibration algorithms. The simplest algorithm is evaluated to find the average-<span class="hlt">frequency</span> uncertainty arising from the noise of the cesium fountain's local oscillator and from the noise of a hydrogen maser transfer-standard. This algorithm and known noise sources are shown to permit interlaboratory <span class="hlt">frequency</span> transfer with a standard uncertainty of less than 10(exp -15) for periods of 30-100 days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6853H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6853H"><span>Decadal predictability of winter windstorm <span class="hlt">frequency</span> in Eastern Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Höschel, Ines; Grieger, Jens; Ulbrich, Uwe</p> <p>2017-04-01</p> <p>Winter windstorms are one of the most impact relevant extreme-weather events in Europe. This study is focussed on windstorm <span class="hlt">frequency</span> in Eastern Europe at multi-year time <span class="hlt">scale</span>. Individual storms are identified by using 6-hourly 10m-wind-fields. The impact-oriented tracking algorithm is based on the exceedance of the local 98 percentile of wind speed and a minimum duration of 18 hours. Here, storm <span class="hlt">frequency</span> is the number of 1000km-footprints of identified windstorms touching the location during extended boreal winter from October to March. The temporal development of annual storm <span class="hlt">frequencies</span> in Eastern Europe shows variations on a six to fifteen years period. Higher than normal windstorm <span class="hlt">frequency</span> occurred end of the 1950s and in beginning of the seventies, while lower than normal <span class="hlt">frequency</span> were around 1960 and in the forties, for example. The correlation between bandpass filtered storm <span class="hlt">frequency</span> and North Atlantic sea surface temperature shows a significant pattern with a positive correlation in the subtropical East Atlantic and significant negative correlations in the Gulfstream region. The relationship between these multi-year variations and predictability on decadal time <span class="hlt">scales</span> is discussed. The resulting skill of winter wind storms in the German decadal prediction system MiKlip, based on the numerical earth system model MPI-ESM, will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhRvA..94d3411T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhRvA..94d3411T"><span>Spatiotemporal interference of photoelectron wave packets and the time <span class="hlt">scale</span> of nonadiabatic transitions in the high-<span class="hlt">frequency</span> regime</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toyota, Koudai</p> <p>2016-10-01</p> <p>The method of the envelope Hamiltonian [K. Toyota, U. Saalmann, and J. M. Rost, New J. Phys. 17, 073005 (2015), 10.1088/1367-2630/17/7/073005] is applied to further study a detachment dynamics of a model negative ion in one dimension in the high-<span class="hlt">frequency</span> regime. This method is based on the Floquet approach, but the time dependency of an envelope function is explicitly kept for arbitrary pulse durations. Therefore, it is capable of describing not only a photon absorption or emission, but also a nonadiabatic transition which is induced by the time-varying envelope of the pulse. It was shown that the envelope Hamiltonian accurately retrieves the results obtained by the time-dependent Schrödinger equation, and the underlying physics were well understood by the adiabatic approximation based on the envelope Hamiltonian. In this paper, we explore two more aspects of the detachment dynamics, which were not considered in our previous work. First, we determine the features of both a spatial and temporal interference of photoelectron wave packets in a photon-absorption process. We conclude that both of the interference mechanisms are universal in ionization dynamics in the high-<span class="hlt">frequency</span> regime. Second, we extract a pulse duration which maximizes a yield of the nonadiabatic transition as a function of a pulse duration. It is shown that it becomes maximum when the pulse duration is comparable to a time <span class="hlt">scale</span> of an electron.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28166429','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28166429"><span>Comparison of Rating <span class="hlt">Scales</span> in the Development of Patient-Reported Outcome Measures for Children with Eye Disorders.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hatt, Sarah R; Leske, David A; Wernimont, Suzanne M; Birch, Eileen E; Holmes, Jonathan M</p> <p>2017-03-01</p> <p>A rating <span class="hlt">scale</span> is a critical component of patient-reported outcome instrument design, but the optimal rating <span class="hlt">scale</span> format for pediatric use has not been investigated. We compared rating <span class="hlt">scale</span> performance when administering potential questionnaire items to children with eye disorders and their parents. Three commonly used rating <span class="hlt">scales</span> were evaluated: <span class="hlt">frequency</span> (never, sometimes, often, always), severity (not at all, a little, some, a lot), and difficulty (not difficult, a little difficult, difficult, very difficult). Ten patient-derived items were formatted for each rating <span class="hlt">scale</span>, and rating <span class="hlt">scale</span> testing order was randomized. Both child and parent were asked to comment on any problems with, or a preference for, a particular <span class="hlt">scale</span>. Any confusion about options or inability to answer was recorded. Twenty-one children, aged 5-17 years, with strabismus, amblyopia, or refractive error were recruited, each with one of their parents. Of the first 10 children, 4 (40%) had problems using the difficulty <span class="hlt">scale</span>, compared with 1 (10%) using <span class="hlt">frequency</span>, and none using severity. The difficulty <span class="hlt">scale</span> was modified, replacing the word "difficult" with "hard." Eleven additional children (plus parents) then completed all 3 questionnaires. No children had problems using any <span class="hlt">scale</span>. Four (36%) parents had problems using the difficulty ("hard") <span class="hlt">scale</span> and 1 (9%) with <span class="hlt">frequency</span>. Regarding preference, 6 (55%) of 11 children and 5 (50%) of 10 parents preferred using the <span class="hlt">frequency</span> <span class="hlt">scale</span>. Children and parents found the <span class="hlt">frequency</span> <span class="hlt">scale</span> and question format to be the most easily understood. Children and parents also expressed preference for the <span class="hlt">frequency</span> <span class="hlt">scale</span>, compared with the difficulty and severity <span class="hlt">scales</span>. We recommend <span class="hlt">frequency</span> rating <span class="hlt">scales</span> for patient-reported outcome measures in pediatric populations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28663563','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28663563"><span>A low-<span class="hlt">frequency</span> chip-<span class="hlt">scale</span> optomechanical oscillator with 58 kHz mechanical stiffening and more than 100th-order stable harmonics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huang, Yongjun; Flores, Jaime Gonzalo Flor; Cai, Ziqiang; Yu, Mingbin; Kwong, Dim-Lee; Wen, Guangjun; Churchill, Layne; Wong, Chee Wei</p> <p>2017-06-29</p> <p>For the sensitive high-resolution force- and field-sensing applications, the large-mass microelectromechanical system (MEMS) and optomechanical cavity have been proposed to realize the sub-aN/Hz 1/2 resolution levels. In view of the optomechanical cavity-based force- and field-sensors, the optomechanical coupling is the key parameter for achieving high sensitivity and resolution. Here we demonstrate a chip-<span class="hlt">scale</span> optomechanical cavity with large mass which operates at ≈77.7 kHz fundamental mode and intrinsically exhibiting large optomechanical coupling of 44 GHz/nm or more, for both optical resonance modes. The mechanical stiffening range of ≈58 kHz and a more than 100 th -order harmonics are obtained, with which the free-running <span class="hlt">frequency</span> instability is lower than 10 -6 at 100 ms integration time. Such results can be applied to further improve the sensing performance of the optomechanical inspired chip-<span class="hlt">scale</span> sensors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhFl...30e5103T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30e5103T"><span><span class="hlt">Scale</span> interaction and arrangement in a turbulent boundary layer perturbed by a wall-mounted cylindrical element</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tang, Zhanqi; Jiang, Nan</p> <p>2018-05-01</p> <p>This study reports the modifications of <span class="hlt">scale</span> interaction and arrangement in a turbulent boundary layer perturbed by a wall-mounted circular cylinder. Hot-wire measurements were executed at multiple streamwise and wall-normal wise locations downstream of the cylindrical element. The streamwise fluctuating signals were decomposed into large-, small-, and dissipative-<span class="hlt">scale</span> signatures by corresponding cutoff filters. The <span class="hlt">scale</span> interaction under the cylindrical perturbation was elaborated by comparing the small- and dissipative-<span class="hlt">scale</span> amplitude/<span class="hlt">frequency</span> modulation effects downstream of the cylinder element with the results observed in the unperturbed case. It was obtained that the large-<span class="hlt">scale</span> fluctuations perform a stronger amplitude modulation on both the small and dissipative <span class="hlt">scales</span> in the near-wall region. At the wall-normal positions of the cylinder height, the small-<span class="hlt">scale</span> amplitude modulation coefficients are redistributed by the cylinder wake. The similar observation was noted in small-<span class="hlt">scale</span> <span class="hlt">frequency</span> modulation; however, the dissipative-<span class="hlt">scale</span> <span class="hlt">frequency</span> modulation seems to be independent of the cylindrical perturbation. The phase-relationship observation indicated that the cylindrical perturbation shortens the time shifts between both the small- and dissipative-<span class="hlt">scale</span> variations (amplitude and <span class="hlt">frequency</span>) and large-<span class="hlt">scale</span> fluctuations. Then, the integral time <span class="hlt">scale</span> dependence of the phase-relationship between the small/dissipative <span class="hlt">scales</span> and large <span class="hlt">scales</span> was also discussed. Furthermore, the discrepancy of small- and dissipative-<span class="hlt">scale</span> time shifts relative to the large-<span class="hlt">scale</span> motions was examined, which indicates that the small-<span class="hlt">scale</span> amplitude/<span class="hlt">frequency</span> leads the dissipative <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003328','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003328"><span>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harrington, Kathleen; Marriage, Tobias; Ali, Aamir; Appel, John; Bennett, Charles; Boone, Fletcher; Brewer, Michael; Chan, Manwei; Chuss, David T.; Colazo, Felipe; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170003328'); toggleEditAbsImage('author_20170003328_show'); toggleEditAbsImage('author_20170003328_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170003328_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170003328_hide"></p> <p>2016-01-01</p> <p>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) is a four telescope array designed to characterize relic primordial gravitational waves from inflation and the optical depth to reionization through a measurement of the polarized cosmic microwave background (CMB) on the largest angular <span class="hlt">scales</span>. The <span class="hlt">frequencies</span> of the four CLASS telescopes, one at 38 GHz, two at 93 GHz, and one dichroic system at 145217 GHz, are chosen to avoid spectral regions of high atmospheric emission and span the minimum of the polarized Galactic foregrounds: synchrotron emission at lower <span class="hlt">frequencies</span> and dust emission at higher <span class="hlt">frequencies</span>. Low-noise transition edge sensor detectors and a rapid front-end polarization modulator provide a unique combination of high sensitivity, stability, and control of systematics. The CLASS site, at 5200 m in the Chilean Atacama desert, allows for daily mapping of up to 70% of the sky and enables the characterization of CMB polarization at the largest angular <span class="hlt">scales</span>. Using this combination of a broad <span class="hlt">frequency</span> range, large sky coverage, control over systematics, and high sensitivity, CLASS will observe the reionization and recombination peaks of the CMB E- and B-mode power spectra. CLASS will make a cosmic variance limited measurement of the optical depth to reionization and will measure or place upper limits on the tensor-to-scalar ratio, r, down to a level of 0.01 (95% C.L.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9914E..1KH','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9914E..1KH"><span>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harrington, Kathleen; Marriage, Tobias; Ali, Aamir; Appel, John W.; Bennett, Charles L.; Boone, Fletcher; Brewer, Michael; Chan, Manwei; Chuss, David T.; Colazo, Felipe; Dahal, Sumit; Denis, Kevin; Dünner, Rolando; Eimer, Joseph; Essinger-Hileman, Thomas; Fluxa, Pedro; Halpern, Mark; Hilton, Gene; Hinshaw, Gary F.; Hubmayr, Johannes; Iuliano, Jeffrey; Karakla, John; McMahon, Jeff; Miller, Nathan T.; Moseley, Samuel H.; Palma, Gonzalo; Parker, Lucas; Petroff, Matthew; Pradenas, Bastián.; Rostem, Karwan; Sagliocca, Marco; Valle, Deniz; Watts, Duncan; Wollack, Edward; Xu, Zhilei; Zeng, Lingzhen</p> <p>2016-07-01</p> <p>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) is a four telescope array designed to characterize relic primordial gravitational waves from in ation and the optical depth to reionization through a measurement of the polarized cosmic microwave background (CMB) on the largest angular <span class="hlt">scales</span>. The <span class="hlt">frequencies</span> of the four CLASS telescopes, one at 38 GHz, two at 93 GHz, and one dichroic system at 145/217 GHz, are chosen to avoid spectral regions of high atmospheric emission and span the minimum of the polarized Galactic foregrounds: synchrotron emission at lower <span class="hlt">frequencies</span> and dust emission at higher <span class="hlt">frequencies</span>. Low-noise transition edge sensor detectors and a rapid front-end polarization modulator provide a unique combination of high sensitivity, stability, and control of systematics. The CLASS site, at 5200 m in the Chilean Atacama desert, allows for daily mapping of up to 70% of the sky and enables the characterization of CMB polarization at the largest angular <span class="hlt">scales</span>. Using this combination of a broad <span class="hlt">frequency</span> range, large sky coverage, control over systematics, and high sensitivity, CLASS will observe the reionization and recombination peaks of the CMB E- and B-mode power spectra. CLASS will make a cosmic variance limited measurement of the optical depth to reionization and will measure or place upper limits on the tensor-to-scalar ratio, r, down to a level of 0.01 (95% C.L.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950054632&hterms=solar+intensity+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dsolar%2Bintensity%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950054632&hterms=solar+intensity+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dsolar%2Bintensity%2Bmeasurement"><span>Measurement of high-degree solar oscillation <span class="hlt">frequencies</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bachmann, K. T.; Duvall, T. L., Jr.; Harvey, J. W.; Hill, F.</p> <p>1995-01-01</p> <p>We present m-averaged solar p- and f-mode oscillation <span class="hlt">frequencies</span> over the <span class="hlt">frequency</span> range nu greater than 1.8 and less than 5.0 mHz and the spherical harmonic degree range l greater than or equal to 100 and less than or equal to 1200 from full-disk, 1000 x 1024 pixel, Ca II intensity images collected 1993 June 22-25 with a temporal cadence of 60 s. We itemize the sources and magnitudes of statistical and systematic uncertainties and of small <span class="hlt">frequency</span> corrections, and we show that our <span class="hlt">frequencies</span> represent an improvement in accuracy and coverage over previous measurements. Our <span class="hlt">frequencies</span> agree at the 2 micro Hz level with Mount Wilson <span class="hlt">frequencies</span> determined for l less than or equal to 600 from full-disk images, and we find systematic offsets of 10-20 micro Hz with respect to <span class="hlt">frequencies</span> measured from Big Bear and La Palma observations. We give evidence that these latter offsets are indicative of spatial <span class="hlt">scaling</span> uncertainties associated with the analysis of partial-disk images. In comparison with theory, our p-mode <span class="hlt">frequencies</span> agree within 10 micro Hz of <span class="hlt">frequencies</span> predicted by the Los Alamos model but are as much as 100 micro Hz smaller than <span class="hlt">frequencies</span> predicted by the Denmark and Yale models at degrees near 1000. We also find systematic differences between our n = 0 <span class="hlt">frequencies</span> and the <span class="hlt">frequencies</span> closely agreed upon by all three models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CG....102...45L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CG....102...45L"><span>A multi-<span class="hlt">frequency</span> receiver function inversion approach for crustal velocity structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Xuelei; Li, Zhiwei; Hao, Tianyao; Wang, Sheng; Xing, Jian</p> <p>2017-05-01</p> <p>In order to constrain the crustal velocity structures better, we developed a new nonlinear inversion approach based on multi-<span class="hlt">frequency</span> receiver function waveforms. With the global optimizing algorithm of Differential Evolution (DE), low-<span class="hlt">frequency</span> receiver function waveforms can primarily constrain large-<span class="hlt">scale</span> velocity structures, while high-<span class="hlt">frequency</span> receiver function waveforms show the advantages in recovering small-<span class="hlt">scale</span> velocity structures. Based on the synthetic tests with multi-<span class="hlt">frequency</span> receiver function waveforms, the proposed approach can constrain both long- and short-wavelength characteristics of the crustal velocity structures simultaneously. Inversions with real data are also conducted for the seismic stations of KMNB in southeast China and HYB in Indian continent, where crustal structures have been well studied by former researchers. Comparisons of inverted velocity models from previous and our studies suggest good consistency, but better waveform fitness with fewer model parameters are achieved by our proposed approach. Comprehensive tests with synthetic and real data suggest that the proposed inversion approach with multi-<span class="hlt">frequency</span> receiver function is effective and robust in inverting the crustal velocity structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22663459-wavelet-based-characterization-small-scale-solar-emission-features-low-radio-frequencies','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22663459-wavelet-based-characterization-small-scale-solar-emission-features-low-radio-frequencies"><span>Wavelet-based Characterization of Small-<span class="hlt">scale</span> Solar Emission Features at Low Radio <span class="hlt">Frequencies</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Suresh, A.; Sharma, R.; Oberoi, D.</p> <p></p> <p>Low radio <span class="hlt">frequency</span> solar observations using the Murchison Widefield Array have recently revealed the presence of numerous weak short-lived narrowband emission features, even during moderately quiet solar conditions. These nonthermal features occur at rates of many thousands per hour in the 30.72 MHz observing bandwidth, and hence necessarily require an automated approach for their detection and characterization. Here, we employ continuous wavelet transform using a mother Ricker wavelet for feature detection from the dynamic spectrum. We establish the efficacy of this approach and present the first statistically robust characterization of the properties of these features. In particular, we examine distributionsmore » of their peak flux densities, spectral spans, temporal spans, and peak <span class="hlt">frequencies</span>. We can reliably detect features weaker than 1 SFU, making them, to the best of our knowledge, the weakest bursts reported in literature. The distribution of their peak flux densities follows a power law with an index of −2.23 in the 12–155 SFU range, implying that they can provide an energetically significant contribution to coronal and chromospheric heating. These features typically last for 1–2 s and possess bandwidths of about 4–5 MHz. Their occurrence rate remains fairly flat in the 140–210 MHz <span class="hlt">frequency</span> range. At the time resolution of the data, they appear as stationary bursts, exhibiting no perceptible <span class="hlt">frequency</span> drift. These features also appear to ride on a broadband background continuum, hinting at the likelihood of them being weak type-I bursts.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2016EL....11668004Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EL....11668004Z"><span><span class="hlt">Scaling</span> for hard-sphere colloidal glasses near jamming</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zargar, Rojman; DeGiuli, Eric; Bonn, Daniel</p> <p>2016-12-01</p> <p>Hard-sphere colloids are model systems in which to study the glass transition and universal properties of amorphous solids. Using covariance matrix analysis to determine the vibrational modes, we experimentally measure here the <span class="hlt">scaling</span> behavior of the density of states, shear modulus, and mean-squared displacement (MSD) in a hard-sphere colloidal glass. <span class="hlt">Scaling</span> the <span class="hlt">frequency</span> with the boson-peak <span class="hlt">frequency</span>, we find that the density of states at different volume fractions all collapse on a single master curve, which obeys a power law in terms of the <span class="hlt">scaled</span> <span class="hlt">frequency</span>. Below the boson peak, the exponent is consistent with theoretical results obtained by real-space and phase-space approaches to understanding amorphous solids. We find that the shear modulus and the MSD are nearly inversely proportional, and show a singular power-law dependence on the distance from random close packing. Our results are in very good agreement with the theoretical predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.5700G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.5700G"><span>Declining <span class="hlt">frequency</span> of summertime local-<span class="hlt">scale</span> precipitation over eastern China from 1970 to 2010 and its potential link to aerosols</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Jianping; Su, Tianning; Li, Zhanqing; Miao, Yucong; Li, Jing; Liu, Huan; Xu, Hui; Cribb, Maureen; Zhai, Panmao</p> <p>2017-06-01</p> <p>Summer precipitation plays critical roles in the energy balance and the availability of fresh water over eastern China. However, little is known regarding the trend in local-<span class="hlt">scale</span> precipitation (LSP). Here we developed a novel method to determine LSP events in the summer afternoon throughout eastern China from 1970 to 2010 based on hourly gauge measurements. The LSP occurrence hours decrease at an annual rate of 0.25%, which varies considerably by region, ranging from 0.14% over the Yangtze River Delta to 0.56% over the Pearl River Delta. This declining <span class="hlt">frequency</span> of LSP is generally accompanied by an increase in rain rate of LSP but a decrease in visibility, whose linkage to LSP events was investigated. In particular, more LSP events tended to form when the atmosphere was slightly polluted. Afterward, LSP was suppressed. These findings have important implications for improving our understanding of the climatology of daytime precipitation at local <span class="hlt">scales</span>.<abstract type="synopsis"><title type="main">Plain Language SummarySummer precipitation plays critical roles in the energy balance and the availability of fresh water over eastern China. However, the knowledge remains poorly understood regarding the trend of local-<span class="hlt">scale</span> precipitation (LSP). Long-term hourly gauge data in the summer afternoon throughout eastern China for 1970 to 2010 reveal that LSP occurrence hours decrease at an annual rate of 0.25%, which differs greatly by region, ranging from 0.14% over the Yangtze River Delta to 0.56% over the Pearl River Delta. In contrast, large-<span class="hlt">scale</span> precipitation events do not show significant increasing/decreasing trends over most regions. Further, concurrent visibility observations exhibit a decreasing trend, whose linkage to declining LSP is investigated. In particular, more LSP events tend to form as the atmosphere is slightly polluted. Afterward, LSP is suppressed. The findings provide deep insight into how precipitation changes over long term from a perspective of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24682580','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24682580"><span><span class="hlt">Frequency</span> and correlates of suicidal ideation in pediatric obsessive-compulsive disorder.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Storch, Eric A; Bussing, Regina; Jacob, Marni L; Nadeau, Joshua M; Crawford, Erika; Mutch, P Jane; Mason, Dana; Lewin, Adam B; Murphy, Tanya K</p> <p>2015-02-01</p> <p>This study examined the <span class="hlt">frequency</span> and sociodemographic and clinical correlates of suicidal ideation in a sample of children and adolescents with obsessive-compulsive disorder (OCD). Fifty-four youth with OCD and their parent(s) were administered the Schedule for Affective Disorders and Schizophrenia for School-Age Children-Present and Lifetime, Children's Yale-Brown Obsessive Compulsive <span class="hlt">Scale</span>, and Children's Depression Rating <span class="hlt">Scale</span>-Revised. Children completed the Suicidal Ideation Questionnaire-Junior (SIQ-JR), Child Obsessive Compulsive Impact <span class="hlt">Scale</span>-Child, and Multidimensional Anxiety <span class="hlt">Scale</span> for Children; parents completed the Child Obsessive Compulsive Impact <span class="hlt">Scale</span>-Parent, Swanson, Nolan, and Pelham-IV Parent <span class="hlt">Scale</span>, and Young Mania Rating <span class="hlt">Scale</span>-Parent Version. Seven youth endorsed clinically significant levels of suicidal ideation on the SIQ-JR. Suicidal ideation was significantly related to clinician-rated depressive symptoms, age, child-rated impairment and anxiety symptoms, and symmetry, sexuality/religiosity and miscellaneous symptom dimensions. There was no significant association between suicidal ideation and obsessive-compulsive symptom severity, comorbidity patterns, or several parent-rated indices (e.g., impairment, impulsivity). These results provide initial information regarding the <span class="hlt">frequency</span> and correlates of suicidal ideation in treatment-seeking youth with OCD. Clinical implications are discussed, as well as directions for future research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21805988','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21805988"><span>High-<span class="hlt">frequency</span> graphene voltage amplifier.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, Shu-Jen; Jenkins, Keith A; Valdes Garcia, Alberto; Franklin, Aaron D; Bol, Ageeth A; Haensch, Wilfried</p> <p>2011-09-14</p> <p>While graphene transistors have proven capable of delivering gigahertz-range cutoff <span class="hlt">frequencies</span>, applying the devices to RF circuits has been largely hindered by the lack of current saturation in the zero band gap graphene. Herein, the first high-<span class="hlt">frequency</span> voltage amplifier is demonstrated using large-area chemical vapor deposition grown graphene. The graphene field-effect transistor (GFET) has a 6-finger gate design with gate length of 500 nm. The graphene common-source amplifier exhibits ∼5 dB low <span class="hlt">frequency</span> gain with the 3 dB bandwidth greater than 6 GHz. This first AC voltage gain demonstration of a GFET is attributed to the clear current saturation in the device, which is enabled by an ultrathin gate dielectric (4 nm HfO(2)) of the embedded gate structures. The device also shows extrinsic transconductance of 1.2 mS/μm at 1 V drain bias, the highest for graphene FETs using large-<span class="hlt">scale</span> graphene reported to date.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22410175-large-scale-magnetic-shield-sup-damping-millihertz-frequencies','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22410175-large-scale-magnetic-shield-sup-damping-millihertz-frequencies"><span>A large-<span class="hlt">scale</span> magnetic shield with 10{sup 6} damping at millihertz <span class="hlt">frequencies</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Altarev, I.; Bales, M.; Fierlinger, K.</p> <p></p> <p>We present a magnetically shielded environment with a damping factor larger than 1 × 10{sup 6} at the mHz <span class="hlt">frequency</span> regime and an extremely low field and gradient over an extended volume. This extraordinary shielding performance represents an improvement of the state-of-the-art in the difficult regime of damping very low-<span class="hlt">frequency</span> distortions by more than an order of magnitude. This technology enables a new generation of high-precision measurements in fundamental physics and metrology, including searches for new physics far beyond the reach of accelerator-based experiments. We discuss the technical realization of the shield with its improvements in design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25866071','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25866071"><span>Waveform selectivity at the same <span class="hlt">frequency</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wakatsuchi, Hiroki; Anzai, Daisuke; Rushton, Jeremiah J; Gao, Fei; Kim, Sanghoon; Sievenpiper, Daniel F</p> <p>2015-04-13</p> <p>Electromagnetic properties depend on the composition of materials, i.e. either angstrom <span class="hlt">scales</span> of molecules or, for metamaterials, subwavelength periodic structures. Each material behaves differently in accordance with the <span class="hlt">frequency</span> of an incoming electromagnetic wave due to the <span class="hlt">frequency</span> dispersion or the resonance of the periodic structures. This indicates that if the <span class="hlt">frequency</span> is fixed, the material always responds in the same manner unless it has nonlinearity. However, such nonlinearity is controlled by the magnitude of the incoming wave or other bias. Therefore, it is difficult to distinguish different incoming waves at the same <span class="hlt">frequency</span>. Here we present a new concept of circuit-based metasurfaces to selectively absorb or transmit specific types of waveforms even at the same <span class="hlt">frequency</span>. The metasurfaces, integrated with schottky diodes as well as either capacitors or inductors, selectively absorb short or long pulses, respectively. The two types of circuit elements are then combined to absorb or transmit specific waveforms in between. This waveform selectivity gives us another degree of freedom to control electromagnetic waves in various fields including wireless communications, as our simulation reveals that the metasurfaces are capable of varying bit error rates in response to different waveforms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11504012','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11504012"><span>Subjective <span class="hlt">frequency</span> estimates for 2,938 monosyllabic words.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Balota, D A; Pilotti, M; Cortese, M J</p> <p>2001-06-01</p> <p>Subjective <span class="hlt">frequency</span> estimates for large sample of monosyllabic English words were collected from 574 young adults (undergraduate students) and from a separate group of 1,590 adults of varying ages and educational backgrounds. Estimates from the latter group were collected via the internet. In addition, 90 healthy older adults provided estimates for a random sample of 480 of these words. All groups rated words with respect to the estimated <span class="hlt">frequency</span> of encounters of each word on a 7-point <span class="hlt">scale</span>, ranging from never encountered to encountered several times a day. The young and older groups also rated each word with respect to the <span class="hlt">frequency</span> of encounters in different perceptual domains (e.g., reading, hearing, writing, or speaking). The results of regression analyses indicated that objective log <span class="hlt">frequency</span> and meaningfulness accounted for most of the variance in subjective <span class="hlt">frequency</span> estimates, whereas neighborhood size accounted for the least amount of variance in the ratings. The predictive power of log <span class="hlt">frequency</span> and meaningfulness were dependent on the level of subjective <span class="hlt">frequency</span> estimates. Meaningfulness was a better predictor of subjective <span class="hlt">frequency</span> for uncommon words, whereas log <span class="hlt">frequency</span> was a better predictor of subjective <span class="hlt">frequency</span> for common words. Our discussion focuses on the utility of subjective <span class="hlt">frequency</span> estimates compared with other estimates of familiarity. The raw subjective <span class="hlt">frequency</span> data for all words are available at http://www.artsci.wustl.edu/dbalota/labpub.html.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.S31A2032T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.S31A2032T"><span>Regional difference in small-<span class="hlt">scale</span> heterogeneities in the crust and upper mantle in Japan derived by the analysis of high-<span class="hlt">frequency</span> P-wave</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takemura, S.; Furumura, T.</p> <p>2010-12-01</p> <p>In order to understand distribution properties of small-<span class="hlt">scale</span> heterogeneities in the crust and upper mantle structure, we analyze three-component seismograms recorded by Hi-net in Japan. We examined relative strength of the P-wave in the transverse (T) component and its change as a function of <span class="hlt">frequency</span> and propagation distances, which is strongly relating to the strength of seismic wave scattering in the lithosphere. We analyzed 53,220 Hi-net record from 310 shallow (h<30km) crustal earthquakes with MJMA =2.0-5.3. The three-component seismograms are firstly applied by band-pass filter with pass band <span class="hlt">frequency</span> of f=1-2, 2-4, 4-8, 8-16, 16-32 Hz and then the Hilbert transform is used to synthesize envelope of each component. Then, the energy partition (EP) of P wave in the T component relative to total P-wave energy is evaluated around the P wave in 3-sec time window. The estimated EP value is almost constant 0.2 in high-<span class="hlt">frequencies</span> (8-16 Hz) at shorter distance, while it is 0.07 in low-<span class="hlt">frequencies</span> (1-2 Hz). We found clearly <span class="hlt">frequency</span>-change property of EP value. But at larger distance over 150 km, EP values gradually increase with increasing distance. In high-<span class="hlt">frequencies</span> (8-16, 16-32 Hz), especially EP values asymptotically reach from 0.2 to 0.33, equi-partitioning of P-wave energy into three components. This may because Pn-phase dominates in larger hypocentral distances. In order to examine difference in the EP in each area of Japan which would be relating to the strength of crustal heterogeneities in each area we divided the area of Japan into three regions, fore-arc side of Tohoku, back-arc side of Tohoku and Chugoku-Shikoku area. The difference in EP value in each area is clearly found in the high-<span class="hlt">frequency</span> (4-8 Hz) band, where larger EP (0.2) was obtained at back-arc side of Tohoku relative to smaller EP (0.1) at fore-arc side of Tohoku and Chugoku-Shikoku. This is consistent with the results of Carcole and Sato (2009) who estimated the strength of crustal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/5380','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/5380"><span><span class="hlt">Scale</span> problems in reporting landscape pattern at the regional <span class="hlt">scale</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>R.V. O' Neill; C.T. Hunsaker; S.P. Timmins; B.L. Jackson; K.B. Jones; Kurt H. Riitters; James D. Wickham</p> <p>1996-01-01</p> <p>Remotely sensed data for Southeastern United States (Standard Federal Region 4) are used to examine the <span class="hlt">scale</span> problems involved in reporting landscape pattern for a large, heterogeneous region. <span class="hlt">Frequency</span> distribu-tions of landscape indices illustrate problems associated with the grain or resolution of the data. Grain should be 2 to 5 times smaller than the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Theories+AND+bullying&pg=6&id=EJ959631','ERIC'); return false;" href="https://eric.ed.gov/?q=Theories+AND+bullying&pg=6&id=EJ959631"><span>Validation of the Perceived School Bullying Severity <span class="hlt">Scale</span></span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Chen, Li Ming; Liu, Kun Shia; Cheng, Ying Yao</p> <p>2012-01-01</p> <p>Research on school bullying has tended to focus on its prevalence or <span class="hlt">frequency</span> while ignoring its perceived severity. This study attempted to construct a perceived School Bullying Severity <span class="hlt">Scale</span> (SBSS). The original 24-item instrument, revised from the Victim <span class="hlt">Scale</span> of the School Bullying <span class="hlt">Scales</span>, covered the four categories of physical, verbal,…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhyA..337..231K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhyA..337..231K"><span>Time <span class="hlt">scales</span> involved in emergent market coherence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kwapień, J.; Drożdż, S.; Speth, J.</p> <p>2004-06-01</p> <p>In addressing the question of the time <span class="hlt">scales</span> characteristic for the market formation, we analyze high-<span class="hlt">frequency</span> tick-by-tick data from the NYSE and from the German market. By using returns on various time <span class="hlt">scales</span> ranging from seconds or minutes up to 2 days, we compare magnitude of the largest eigenvalue of the correlation matrix for the same set of securities but for different time <span class="hlt">scales</span>. For various sets of stocks of different capitalization (and the average trading <span class="hlt">frequency</span>), we observe a significant elevation of the largest eigenvalue with increasing time <span class="hlt">scale</span>. Our results from the correlation matrix study can be considered as a manifestation of the so-called Epps effect. There is no unique explanation of this effect and it seems that many different factors play a role here. One of such factors is randomness in transaction moments for different stocks. Another interesting conclusion to be drawn from our results is that in the contemporary markets the emergence of significant correlations occurs on time <span class="hlt">scales</span> much smaller than in the more distant history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ASAJ..113.2299J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ASAJ..113.2299J"><span>Tempo and <span class="hlt">scale</span> of biogenic effects on high-<span class="hlt">frequency</span> acoustic propagation near the marine sediment-water interface in shallow water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jumars, Peter</p> <p>2003-04-01</p> <p>Organisms have natural <span class="hlt">scales</span>, such as lifetimes, body sizes, <span class="hlt">frequencies</span> of movement to new locations, and residence times of material in digestive systems, and each <span class="hlt">scale</span> has potential implications for acoustic effects. The effects of groups of organisms, like organisms themselves, aggregate in space and time. This review, including an assortment of unpublished information, examines examples of such aggregations, many of them documented acoustically. Light synchronizes many activities. Macroscopic animals forage primarily under cover of darkness. This phasing applies both to animals that extend appendages above the sediment-water interface and to animals that leave the seabed at night. Whereas their bottom-modifying activities are concentrated in nocturnal or crepuscular fashion, the bottom-modifying activities of the visual feeders follow a different phasing and often dominate the rate of change in acoustic backscatter from the interface. Light also acts through its effects on primary production, often concentrated in a very thin surficial layer atop the seabed. The supersaturation of oxygen does, and microbubble nucleation may, result. Where tidal velocities are large, light-set patterns are often tidally modulated. Activities of animals living below the seabed, however, remain a mystery, whose primary hope for solution is acoustic. [Work supported by ONR and DEPSCoR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880014164','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880014164"><span>Acoustic characteristics of 1/20-<span class="hlt">scale</span> model helicopter rotors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shenoy, Rajarama K.; Kohlhepp, Fred W.; Leighton, Kenneth P.</p> <p>1986-01-01</p> <p>A wind tunnel test to study the effects of geometric <span class="hlt">scale</span> on acoustics and to investigate the applicability of very small <span class="hlt">scale</span> models for the study of acoustic characteristics of helicopter rotors was conducted in the United Technologies Research Center Acoustic Research Tunnel. The results show that the Reynolds number effects significantly alter the Blade-Vortex-Interaction (BVI) Noise characteristics by enhancing the lower <span class="hlt">frequency</span> content and suppressing the higher <span class="hlt">frequency</span> content. In the time domain this is observed as an inverted thickness noise impulse rather than the typical positive-negative impulse of BVI noise. At higher advance ratio conditions, in the absence of BVI, the 1/20 <span class="hlt">scale</span> model acoustic trends with Mach number follow those of larger <span class="hlt">scale</span> models. However, the 1/20 <span class="hlt">scale</span> model acoustic trends appear to indicate stall at higher thrust and advance ratio conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160010539&hterms=cosmology&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcosmology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160010539&hterms=cosmology&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcosmology"><span>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harrington, Kathleen; Marriange, Tobias; Aamir, Ali; Appel, John W.; Bennett, Charles L.; Boone, Fletcher; Brewer, Michael; Chan, Manwei; Chuss, David T.; Colazo, Felipe; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160010539'); toggleEditAbsImage('author_20160010539_show'); toggleEditAbsImage('author_20160010539_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160010539_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160010539_hide"></p> <p>2016-01-01</p> <p>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) is a four telescope array designed to characterize relic primordial gravitational waves from in ation and the optical depth to reionization through a measurement of the polarized cosmic microwave background (CMB) on the largest angular <span class="hlt">scales</span>. The <span class="hlt">frequencies</span> of the four CLASS telescopes, one at 38 GHz, two at 93 GHz, and one dichroic system at 145/217 GHz, are chosen to avoid spectral regions of high atmospheric emission and span the minimum of the polarized Galactic foregrounds: synchrotron emission at lower <span class="hlt">frequencies</span> and dust emission at higher <span class="hlt">frequencies</span>. Low-noise transition edge sensor detectors and a rapid front-end polarization modulator provide a unique combination of high sensitivity, stability, and control of systematics. The CLASS site, at 5200 m in the Chilean Atacama desert, allows for daily mapping of up to 70% of the sky and enables the characterization of CMB polarization at the largest angular <span class="hlt">scales</span>. Using this combination of a broad <span class="hlt">frequency</span> range, large sky coverage, control over systematics, and high sensitivity, CLASS will observe the reionization and recombination peaks of the CMB E- and B-mode power spectra. CLASS will make a cosmic variance limited measurement of the optical depth to reionization and will measure or place upper limits on the tensor-to-scalar ratio, r, down to a level of 0.01 (95% C.L.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT.........6V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT.........6V"><span>Statistical modeling of interfractional tissue deformation and its application in radiation therapy planning</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vile, Douglas J.</p> <p></p> <p>In radiation therapy, interfraction organ motion introduces a level of geometric uncertainty into the planning process. Plans, which are typically based upon a single instance of anatomy, must be robust against daily anatomical variations. For this problem, a model of the magnitude, direction, and likelihood of deformation is useful. In this thesis, principal component analysis (PCA) is used to statistically model the 3D organ motion for 19 prostate cancer patients, each with 8-13 fractional computed tomography (CT) images. Deformable image registration and the resultant displacement vector fields (<span class="hlt">DVFs</span>) are used to quantify the interfraction systematic and random motion. By applying the PCA technique to the random <span class="hlt">DVFs</span>, principal modes of random tissue deformation were determined for each patient, and a method for sampling synthetic random <span class="hlt">DVFs</span> was developed. The PCA model was then extended to describe the principal modes of systematic and random organ motion for the population of patients. A leave-one-out study tested both the systematic and random motion model's ability to represent PCA training set <span class="hlt">DVFs</span>. The random and systematic DVF PCA models allowed the reconstruction of these data with absolute mean errors between 0.5-0.9 mm and 1-2 mm, respectively. To the best of the author's knowledge, this study is the first successful effort to build a fully 3D statistical PCA model of systematic tissue deformation in a population of patients. By sampling synthetic systematic and random errors, organ occupancy maps were created for bony and prostate-centroid patient setup processes. By thresholding these maps, PCA-based planning target volume (PTV) was created and tested against conventional margin recipes (van Herk for bony alignment and 5 mm fixed [3 mm posterior] margin for centroid alignment) in a virtual clinical trial for low-risk prostate cancer. Deformably accumulated delivered dose served as a surrogate for clinical outcome. For the bony landmark setup</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4386880','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4386880"><span>An Adaptive MR-CT Registration Method for MRI-guided Prostate Cancer Radiotherapy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhong, Hualiang; Wen, Ning; Gordon, James; Elshaikh, Mohamed A; Movsas, Benjamin; Chetty, Indrin J.</p> <p>2015-01-01</p> <p>Magnetic Resonance images (MRI) have superior soft tissue contrast compared with CT images. Therefore, MRI might be a better imaging modality to differentiate the prostate from surrounding normal organs. Methods to accurately register MRI to simulation CT images are essential, as we transition the use of MRI into the routine clinic setting. In this study, we present a finite element method (FEM) to improve the performance of a commercially available, B-spline-based registration algorithm in the prostate region. Specifically, prostate contours were delineated independently on ten MRI and CT images using the Eclipse treatment planning system. Each pair of MRI and CT images was registered with the B-spline-based algorithm implemented in the VelocityAI system. A bounding box that contains the prostate volume in the CT image was selected and partitioned into a tetrahedral mesh. An adaptive finite element method was then developed to adjust the displacement vector fields (<span class="hlt">DVFs</span>) of the B-spline-based registrations within the box. The B-spline and FEM-based registrations were evaluated based on the variations of prostate volume and tumor centroid, the unbalanced energy of the generated <span class="hlt">DVFs</span>, and the clarity of the reconstructed anatomical structures. The results showed that the volumes of the prostate contours warped with the B-spline-based <span class="hlt">DVFs</span> changed 10.2% on average, relative to the volumes of the prostate contours on the original MR images. This discrepancy was reduced to 1.5% for the FEM-based <span class="hlt">DVFs</span>. The average unbalanced energy was 2.65 and 0.38 mJ/cm3, and the prostate centroid deviation was 0.37 and 0.28 cm, for the B-spline and FEM-based registrations, respectively. Different from the B-spline-warped MR images, the FEM-warped MR images have clear boundaries between prostates and bladders, and their internal prostatic structures are consistent with those of the original MR images. In summary, the developed adaptive FEM method preserves the prostate volume during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PMB....60.2837Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PMB....60.2837Z"><span>An adaptive MR-CT registration method for MRI-guided prostate cancer radiotherapy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhong, Hualiang; Wen, Ning; Gordon, James J.; Elshaikh, Mohamed A.; Movsas, Benjamin; Chetty, Indrin J.</p> <p>2015-04-01</p> <p>Magnetic Resonance images (MRI) have superior soft tissue contrast compared with CT images. Therefore, MRI might be a better imaging modality to differentiate the prostate from surrounding normal organs. Methods to accurately register MRI to simulation CT images are essential, as we transition the use of MRI into the routine clinic setting. In this study, we present a finite element method (FEM) to improve the performance of a commercially available, B-spline-based registration algorithm in the prostate region. Specifically, prostate contours were delineated independently on ten MRI and CT images using the Eclipse treatment planning system. Each pair of MRI and CT images was registered with the B-spline-based algorithm implemented in the VelocityAI system. A bounding box that contains the prostate volume in the CT image was selected and partitioned into a tetrahedral mesh. An adaptive finite element method was then developed to adjust the displacement vector fields (<span class="hlt">DVFs</span>) of the B-spline-based registrations within the box. The B-spline and FEM-based registrations were evaluated based on the variations of prostate volume and tumor centroid, the unbalanced energy of the generated <span class="hlt">DVFs</span>, and the clarity of the reconstructed anatomical structures. The results showed that the volumes of the prostate contours warped with the B-spline-based <span class="hlt">DVFs</span> changed 10.2% on average, relative to the volumes of the prostate contours on the original MR images. This discrepancy was reduced to 1.5% for the FEM-based <span class="hlt">DVFs</span>. The average unbalanced energy was 2.65 and 0.38 mJ cm-3, and the prostate centroid deviation was 0.37 and 0.28 cm, for the B-spline and FEM-based registrations, respectively. Different from the B-spline-warped MR images, the FEM-warped MR images have clear boundaries between prostates and bladders, and their internal prostatic structures are consistent with those of the original MR images. In summary, the developed adaptive FEM method preserves the prostate volume</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26084736','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26084736"><span>High-<span class="hlt">frequency</span> - Spinal Cord Stimulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rapcan, R; Mlaka, J; Venglarcik, M; Vinklerova, V; Gajdos, M; Illes, R</p> <p>2015-01-01</p> <p>Our clinical experience with high - <span class="hlt">frequency</span> SCS for FBSS in patients with predominant low back pain is presented. After a trial period, 100 % (21 out of 21) of patients with FBSS with predominant low back pain reported a significant improvement in visual analog <span class="hlt">scale</span> (VAS) pain score and underwent permanent implantation of the high - <span class="hlt">frequency</span> SCS system. SCS trials lasted 7-14 days (median 9 days). SCS leads were mostly positioned at the T8-10 or T8-12 vertebral levels . We used both single and dual lead placement. VAS, patient satisfaction, patient performance status, opioid consumption and complication rate were assessed for the period of 12 months. The mean VAS score before implantation (8.7) compared to VAS 12 months after implantation (4.0) was significantly lower (CI95[3.9-5.4], p < 0.001). There was a significant improvement in performance status when comparing PS before implantation (3.0) and 12 months after implantation (1.8) (CI95[0.9-1.6], p < 0.001). The mean patient satisfaction scores (PSS) did not differ throughout the whole one year follow-up period. Our group of 21 patients with implanted high - <span class="hlt">frequency</span> SCS systems reported significant low back pain and leg pain relief within the period of 12 months as well as significant improvement in their performance status. We had a special subgroup of 5 patients with regular change of <span class="hlt">frequencies</span> between high <span class="hlt">frequency</span> and conventional <span class="hlt">frequency</span> (with paresthesia) also with significant leg and low back pain relief (Tab. 2, Fig. 1, Ref. 8). Text in PDF www.elis.sk.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880046303&hterms=centaurus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dcentaurus','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880046303&hterms=centaurus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dcentaurus"><span>The very low <span class="hlt">frequency</span> power spectrum of Centaurus X-3</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gruber, D. E.</p> <p>1988-01-01</p> <p>The long-term variability of Cen X-3 on time <span class="hlt">scales</span> ranging from days to years has been examined by combining data obtained by the HEAO 1 A-4 instrument with data from Vela 5B. A simple interpretation of the data is made in terms of the standard alpha-disk model of accretion disk structure and dynamics. Assuming that the low-<span class="hlt">frequency</span> variance represents the inherent variability of the mass transfer from the companion, the decline in power at higher <span class="hlt">frequencies</span> results from the leveling of radial structure in the accretion disk through viscous mixing. The shape of the observed power spectrum is shown to be in excellent agreement with a calculation based on a simplified form of this model. The observed low-<span class="hlt">frequency</span> power spectrum of Cen X-3 is consistent with a disk in which viscous mixing occurs about as rapidly as possible and on the largest <span class="hlt">scale</span> possible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1017065','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1017065"><span>Low-<span class="hlt">frequency</span> fluid waves in fractures and pipes</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>Korneev, Valeri</p> <p>2010-09-01</p> <p>Low-<span class="hlt">frequency</span> analytical solutions have been obtained for phase velocities of symmetrical fluid waves within both an infinite fracture and a pipe filled with a viscous fluid. Three different fluid wave regimes can exist in such objects, depending on the various combinations of parameters, such as fluid density, fluid viscosity, walls shear modulus, channel thickness, and <span class="hlt">frequency</span>. Equations for velocities of all these regimes have explicit forms and are verified by comparisons with the exact solutions. The dominant role of fractures in rock permeability at field <span class="hlt">scales</span> and the strong amplitude and <span class="hlt">frequency</span> effects of Stoneley guided waves suggest the importancemore » of including these wave effects into poroelastic theories.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2015AGUFMSA31F2386S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSA31F2386S"><span>Ionospheric Coherence Bandwidth Measurements in the Lower VHF <span class="hlt">Frequency</span> Range</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suszcynsky, D. M.; Light, M. E.; Pigue, M. J.</p> <p>2015-12-01</p> <p>The United States Department of Energy's Radio <span class="hlt">Frequency</span> Propagation (RFProp) experiment consists of a satellite-based radio receiver suite to study various aspects of trans-ionospheric signal propagation and detection in four <span class="hlt">frequency</span> bands, 2 - 55 MHz, 125 - 175 MHz, 365 - 415 MHz and 820 - 1100 MHz. In this paper, we present simultaneous ionospheric coherence bandwidth and S4 scintillation index measurements in the 32 - 44 MHz <span class="hlt">frequency</span> range collected during the ESCINT equatorial scintillation experiment. 40-MHz continuous wave (CW) and 32 - 44 MHz swept <span class="hlt">frequency</span> signals were transmitted simultaneously to the RFProp receiver suite from the Reagan Test Site at Kwajalein Atoll in the Marshall Islands (8.7° N, 167.7° E) in three separate campaigns during the 2014 and 2015 equinoxes. Results show coherence bandwidths as small as ~ 1 kHz for strong scintillation (S4 > 0.7) and indicate a high degree of ionospheric variability and irregularity on 10-m spatial <span class="hlt">scales</span>. Spread-Doppler clutter effects arising from preferential ray paths to the satellite due to refraction off of isolated density irregularities are also observed and are dominant at low elevation angles. The results are compared to previous measurements and available <span class="hlt">scaling</span> laws.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1983JSV....88..145N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983JSV....88..145N"><span>Parametrically excited multidegree-of-freedom systems with repeated <span class="hlt">frequencies</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nayfeh, A. H.</p> <p>1983-05-01</p> <p>An analysis is presented of the linear response of multidegree-of-freedom systems with a repeated <span class="hlt">frequency</span> of order three to a harmonic parametric excitation. The method of multiple <span class="hlt">scales</span> is used to determine the modulation of the amplitudes and phases for two cases: fundamental resonance of the modes with the repeated <span class="hlt">frequency</span> and combination resonance involving these modes and another mode. Conditions are then derived for determining the stability of the motion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.S41A2364C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.S41A2364C"><span>A Multi-<span class="hlt">scale</span> Finite-<span class="hlt">frequency</span> Approach to the Inversion of Reciprocal Travel Times for 3-D Velocity Structure beneath Taiwan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Y.; Hung, S.; Kuo, B.; Kuochen, H.</p> <p>2012-12-01</p> <p>Taiwan is one of the archetypical places for studying the active orogenic process in the world, where the Luzon arc has obliquely collided into the southwest China continental margin since 5 Ma ago. Because of the lack of convincing evidence for the structure in the lithospheric mantle and at even greater depths, several competing models have been proposed for the Taiwan mountain-building process. With the deployment of ocean-bottom seismometers (OBSs) on the seafloor around Taiwan from the TAIGER (TAiwan Integrated GEodynamic Research) and IES seismic experiments, the aperture of the seismic network is greatly extended to improve the depth resolution of tomographic imaging, which is critical to illuminate the nature of the arc-continent collision and accretion in Taiwan. In this study, we use relative travel-time residuals between a collection of teleseismic body wave arrivals to tomographically image the velocity structure beneath Taiwan. In addition to those from common distant earthquakes observed across an array of stations, we take advantage of dense seismicity in the vicinity of Taiwan and the source and receiver reciprocity to augment the data coverage from clustered earthquakes recorded by global stations. As waveforms are dependent of source mechanisms, we carry out the cluster analysis to group the phase arrivals with similar waveforms into clusters and simultaneously determine relative travel-time anomalies in the same cluster accurately by a cross correlation method. The combination of these two datasets would particularly enhance the resolvability of the tomographic models offshore of eastern Taiwan, where the two subduction systems of opposite polarity are taking place and have primarily shaped the present tectonic framework of Taiwan. On the other hand, our inversion adopts an innovation that invokes wavelet-based, multi-<span class="hlt">scale</span> parameterization and finite-<span class="hlt">frequency</span> theory. Not only does this approach make full use of <span class="hlt">frequency</span>-dependent travel</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ERL....11d4003Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ERL....11d4003Y"><span>Contribution of large-<span class="hlt">scale</span> circulation anomalies to changes in extreme precipitation <span class="hlt">frequency</span> in the United States</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Lejiang; Zhong, Shiyuan; Pei, Lisi; Bian, Xindi; Heilman, Warren E.</p> <p>2016-04-01</p> <p>The mean global climate has warmed as a result of the increasing emission of greenhouse gases induced by human activities. This warming is considered the main reason for the increasing number of extreme precipitation events in the US. While much attention has been given to extreme precipitation events occurring over several days, which are usually responsible for severe flooding over a large region, little is known about how extreme precipitation events that cause flash flooding and occur at sub-daily time <span class="hlt">scales</span> have changed over time. Here we use the observed hourly precipitation from the North American Land Data Assimilation System Phase 2 forcing datasets to determine trends in the <span class="hlt">frequency</span> of extreme precipitation events of short (1 h, 3 h, 6 h, 12 h and 24 h) duration for the period 1979-2013. The results indicate an increasing trend in the central and eastern US. Over most of the western US, especially the Southwest and the Intermountain West, the trends are generally negative. These trends can be largely explained by the interdecadal variability of the Pacific Decadal Oscillation and Atlantic Multidecadal Oscillation (AMO), with the AMO making a greater contribution to the trends in both warm and cold seasons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAG...150....1P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAG...150....1P"><span>Insight into large-<span class="hlt">scale</span> topography on analysis of high-<span class="hlt">frequency</span> Rayleigh waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ping, Ping; Chu, Risheng; Chong, Jiajun; Ni, Sidao; Zhang, Yu</p> <p>2018-03-01</p> <p>The dispersion of surface waves could be biased in regions where topography is comparable to the wavelength. We investigate the effects on high-<span class="hlt">frequency</span> Rayleigh waves propagating in a typical massif model through numerical simulations. High-<span class="hlt">frequency</span> Rayleigh waves have relatively higher signal-to-noise ratios (SNR) using the Q component in the LQT coordinate system, perpendicular to the local free surface in these topographic models. When sources and stations are located at different sides of the massif, the conventional dispersion image overestimates phase velocities of Rayleigh waves, as much as 25% with topographic height/width ratio (H/r) > 0.5. The dispersion perturbation is more distinctive for fundamental modes. Using a two-layer model, the thickness deviation (ΔD/D) may be significant in surface-wave inversion due to the variation of H/r and the thickness of the first layer. These phenomena cannot be ignored in surface-wave interpretations, nevertheless they are trivial for the source and stations located at the same side of the massif.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=research+AND+analysis+AND+rosenberg+AND+self-esteem+AND+scale&pg=4&id=ED198570','ERIC'); return false;" href="https://eric.ed.gov/?q=research+AND+analysis+AND+rosenberg+AND+self-esteem+AND+scale&pg=4&id=ED198570"><span>Personality as a Determinate of Response Dimension <span class="hlt">Scaling</span> for Likert Rating Categories.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Hensley, Wayne E.; Sanford, David L.</p> <p></p> <p>A study was designed to evaluate the use of summated rating (Likert) <span class="hlt">scales</span> of agreement, evaluation, and <span class="hlt">frequency</span>. The subjects, 58 female and 45 male college students, rank ordered the descriptive adjectives for the areas of agreement, evaluation, and <span class="hlt">frequency</span> on a <span class="hlt">scale</span> of 1 to 100. They also completed the Personal Report of Communication…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25577229','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25577229"><span>An Ethical Issue <span class="hlt">Scale</span> for Community Pharmacy Setting (EISP): Development and Validation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Crnjanski, Tatjana; Krajnovic, Dusanka; Tadic, Ivana; Stojkov, Svetlana; Savic, Mirko</p> <p>2016-04-01</p> <p>Many problems that arise when providing pharmacy services may contain some ethical components and the aims of this study were to develop and validate a <span class="hlt">scale</span> that could assess difficulties of ethical issues, as well as the <span class="hlt">frequency</span> of those occurrences in everyday practice of community pharmacists. Development and validation of the <span class="hlt">scale</span> was conducted in three phases: (1) generating items for the initial survey instrument after qualitative analysis; (2) defining the design and format of the instrument; (3) validation of the instrument. The constructed Ethical Issue <span class="hlt">scale</span> for community pharmacy setting has two parts containing the same 16 items for assessing the difficulty and <span class="hlt">frequency</span> thereof. The results of the 171 completely filled out <span class="hlt">scales</span> were analyzed (response rate 74.89%). The Cronbach's α value of the part of the instrument that examines difficulties of the ethical situations was 0.83 and for the part of the instrument that examined <span class="hlt">frequency</span> of the ethical situations was 0.84. Test-retest reliability for both parts of the instrument was satisfactory with all Interclass correlation coefficient (ICC) values above 0.6, (for the part that examines severity ICC = 0.809, for the part that examines <span class="hlt">frequency</span> ICC = 0.929). The 16-item <span class="hlt">scale</span>, as a self assessment tool, demonstrated a high degree of content, criterion, and construct validity and test-retest reliability. The results support its use as a research tool to asses difficulty and <span class="hlt">frequency</span> of ethical issues in community pharmacy setting. The validated <span class="hlt">scale</span> needs to be further employed on a larger sample of pharmacists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PMB....58.6481L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PMB....58.6481L"><span>Voxel-based statistical analysis of uncertainties associated with deformable image registration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Shunshan; Glide-Hurst, Carri; Lu, Mei; Kim, Jinkoo; Wen, Ning; Adams, Jeffrey N.; Gordon, James; Chetty, Indrin J.; Zhong, Hualiang</p> <p>2013-09-01</p> <p>Deformable image registration (DIR) algorithms have inherent uncertainties in their displacement vector fields (<span class="hlt">DVFs</span>).The purpose of this study is to develop an optimal metric to estimate DIR uncertainties. Six computational phantoms have been developed from the CT images of lung cancer patients using a finite element method (FEM). The FEM generated <span class="hlt">DVFs</span> were used as a standard for registrations performed on each of these phantoms. A mechanics-based metric, unbalanced energy (UE), was developed to evaluate these registration <span class="hlt">DVFs</span>. The potential correlation between UE and DIR errors was explored using multivariate analysis, and the results were validated by landmark approach and compared with two other error metrics: DVF inverse consistency (IC) and image intensity difference (ID). Landmark-based validation was performed using the POPI-model. The results show that the Pearson correlation coefficient between UE and DIR error is rUE-error = 0.50. This is higher than rIC-error = 0.29 for IC and DIR error and rID-error = 0.37 for ID and DIR error. The Pearson correlation coefficient between UE and the product of the DIR displacements and errors is rUE-error × DVF = 0.62 for the six patients and rUE-error × DVF = 0.73 for the POPI-model data. It has been demonstrated that UE has a strong correlation with DIR errors, and the UE metric outperforms the IC and ID metrics in estimating DIR uncertainties. The quantified UE metric can be a useful tool for adaptive treatment strategies, including probability-based adaptive treatment planning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11367799','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11367799"><span>Interdigital pair bonding for high <span class="hlt">frequency</span> (20-50 MHz) ultrasonic composite transducers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, R; Harasiewicz, K A; Foster, F S</p> <p>2001-01-01</p> <p>Interdigital pair bonding is a novel methodology that enables the fabrication of high <span class="hlt">frequency</span> piezoelectric composites with high volume fractions of the ceramic phase. This enhancement in ceramic volume fraction significantly reduces the dimensional <span class="hlt">scale</span> of the epoxy phase and increases the related effective physical parameters of the composite, such as dielectric constant and the longitudinal sound velocity, which are major concerns in the development of high <span class="hlt">frequency</span> piezoelectric composites. In this paper, a method called interdigital pair bonding (IPB) is used to prepare 1-3 piezoelectric composite with a pitch of 40 microns, a kerf of 4 microns, and a ceramic volume fraction of 81%. The composites prepared in this fashion exhibited a very pure thickness-mode resonance up to a <span class="hlt">frequency</span> of 50 MHz. Unlike the 2-2 piezoelectric composites with the same ceramic and epoxy <span class="hlt">scales</span> developed earlier, the anticipated lateral modes between 50 to 100 MHz were not observed in the current 1-3 composites. The mechanisms for the elimination of the lateral modes at high <span class="hlt">frequency</span> are discussed. The effective electromechanical coupling coefficient of the composite was 0.72 at a <span class="hlt">frequency</span> of 50 MHz. The composites showed a high longitudinal sound velocity of 4300 m/s and a high clamped dielectric constant of 1111 epsilon 0, which will benefit the development of high <span class="hlt">frequency</span> ultrasonic transducers and especially high <span class="hlt">frequency</span> transducer arrays for medical imaging.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.osti.gov/sciencecinema/biblio/987708','SCIGOVIMAGE-SCICINEMA'); return false;" href="http://www.osti.gov/sciencecinema/biblio/987708"><span><span class="hlt">Scales</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/sciencecinema/">ScienceCinema</a></p> <p>Murray Gibson</p> <p>2017-12-09</p> <p>Musical <span class="hlt">scales</span> involve notes that, sounded simultaneously (chords), sound good together. The result is the left brain meeting the right brain — a Pythagorean interval of overlapping notes. This synergy would suggest less difference between the working of the right brain and the left brain than common wisdom would dictate. The pleasing sound of harmony comes when two notes share a common harmonic, meaning that their <span class="hlt">frequencies</span> are in simple integer ratios, such as 3/2 (G/C) or 5/4 (E/C).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019868','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019868"><span><span class="hlt">Scaling</span> laws from geomagnetic time series</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Voros, Z.; Kovacs, P.; Juhasz, A.; Kormendi, A.; Green, A.W.</p> <p>1998-01-01</p> <p>The notion of extended self-similarity (ESS) is applied here for the X - component time series of geomagnetic field fluctuations. Plotting nth order structure functions against the fourth order structure function we show that low-<span class="hlt">frequency</span> geomagnetic fluctuations up to the order n = 10 follow the same <span class="hlt">scaling</span> laws as MHD fluctuations in solar wind, however, for higher <span class="hlt">frequencies</span> (f > l/5[h]) a clear departure from the expected universality is observed for n > 6. ESS does not allow to make an unambiguous statement about the non triviality of <span class="hlt">scaling</span> laws in "geomagnetic" turbulence. However, we suggest to use higher order moments as promising diagnostic tools for mapping the contributions of various remote magnetospheric sources to local observatory data. Copyright 1998 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987AmJPh..55..223H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987AmJPh..55..223H"><span>A numerical exercise in musical <span class="hlt">scales</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hartmann, George C.</p> <p>1987-03-01</p> <p>This paper investigates why the 12-note <span class="hlt">scale</span>, having equal intervals, seems to be the best representation of <span class="hlt">scales</span> constructed from purely harmonic intervals. Is it possible that other equal temperament <span class="hlt">scales</span> with more or less than 12 notes would serve just as well? The investigation is done by displaying the difference between a set of harmonic notes and <span class="hlt">scales</span> with equal intervals having n notes per octave. The difference is small when n is equal to 12, but also when n equals 19 and 29. The number density of notes per unit <span class="hlt">frequency</span> intervals is also investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28839169','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28839169"><span><span class="hlt">Frequency</span>, moisture content, and temperature dependent dielectric properties of potato starch related to drying with radio-<span class="hlt">frequency</span>/microwave energy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhu, Zhuozhuo; Guo, Wenchuan</p> <p>2017-08-24</p> <p>To develop advanced drying methods using radio-<span class="hlt">frequency</span> (RF) or microwave (MW) energy, dielectric properties of potato starch were determined using an open-ended coaxial-line probe and network analyzer at <span class="hlt">frequencies</span> between 20 and 4,500 MHz, moisture contents between 15.1% and 43.1% wet basis (w.b.), and temperatures between 25 and 75 °C. The results showed that both dielectric constant (ε') and loss factor (ε″) were dependent on <span class="hlt">frequency</span>, moisture content, and temperature. ε' decreased with increasing <span class="hlt">frequency</span> at a given moisture content or temperature. At low moisture contents (≤25.4% w.b.) or low temperatures (≤45 °C), ε″ increased with increasing <span class="hlt">frequency</span>. However, ε″ changed from decrease to increase with increasing <span class="hlt">frequency</span> at high moisture contents or temperatures. At low temperatures (25-35 °C), both ε' and ε″ increased with increasing moisture content. At low moisture contents (15.1-19.5% w.b.), they increased with increasing temperature. The change trends of ε' and ε″ were different and dependent on temperature and moisture content at their high levels. The penetration depth (d p ) decreased with increasing <span class="hlt">frequency</span>. RF treatments may provide potential large-<span class="hlt">scale</span> industrial drying application for potato starch. This research offers useful information on dielectric properties of potato starch related to drying with electromagnetic energy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CNSNS..60...50L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CNSNS..60...50L"><span>Identifying the <span class="hlt">scale</span>-dependent motifs in atmospheric surface layer by ordinal pattern analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Qinglei; Fu, Zuntao</p> <p>2018-07-01</p> <p>Ramp-like structures in various atmospheric surface layer time series have been long studied, but the presence of motifs with the finer <span class="hlt">scale</span> embedded within larger <span class="hlt">scale</span> ramp-like structures has largely been overlooked in the reported literature. Here a novel, objective and well-adapted methodology, the ordinal pattern analysis, is adopted to study the finer-<span class="hlt">scaled</span> motifs in atmospheric boundary-layer (ABL) time series. The studies show that the motifs represented by different ordinal patterns take clustering properties and 6 dominated motifs out of the whole 24 motifs account for about 45% of the time series under particular <span class="hlt">scales</span>, which indicates the higher contribution of motifs with the finer <span class="hlt">scale</span> to the series. Further studies indicate that motif statistics are similar for both stable conditions and unstable conditions at larger <span class="hlt">scales</span>, but large discrepancies are found at smaller <span class="hlt">scales</span>, and the <span class="hlt">frequencies</span> of motifs "1234" and/or "4321" are a bit higher under stable conditions than unstable conditions. Under stable conditions, there are great changes for the occurrence <span class="hlt">frequencies</span> of motifs "1234" and "4321", where the occurrence <span class="hlt">frequencies</span> of motif "1234" decrease from nearly 24% to 4.5% with the <span class="hlt">scale</span> factor increasing, and the occurrence <span class="hlt">frequencies</span> of motif "4321" change nonlinearly with the <span class="hlt">scale</span> increasing. These great differences of dominated motifs change with <span class="hlt">scale</span> can be taken as an indicator to quantify the flow structure changes under different stability conditions, and motif entropy can be defined just by only 6 dominated motifs to quantify this time-<span class="hlt">scale</span> independent property of the motifs. All these results suggest that the defined <span class="hlt">scale</span> of motifs with the finer <span class="hlt">scale</span> should be carefully taken into consideration in the interpretation of turbulence coherent structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MARK27005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MARK27005S"><span>Carbon nanotube transistor based high-<span class="hlt">frequency</span> electronics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schroter, Michael</p> <p></p> <p>At the nanoscale carbon nanotubes (CNTs) have higher carrier mobility and carrier velocity than most incumbent semiconductors. Thus CNT based field-effect transistors (FETs) are being considered as strong candidates for replacing existing MOSFETs in digital applications. In addition, the predicted high intrinsic transit <span class="hlt">frequency</span> and the more recent finding of ways to achieve highly linear transfer characteristics have inspired investigations on analog high-<span class="hlt">frequency</span> (HF) applications. High linearity is extremely valuable for an energy efficient usage of the <span class="hlt">frequency</span> spectrum, particularly in mobile communications. Compared to digital applications, the much more relaxed constraints for CNT placement and lithography combined with already achieved operating <span class="hlt">frequencies</span> of at least 10 GHz for fabricated devices make an early entry in the low GHz HF market more feasible than in large-<span class="hlt">scale</span> digital circuits. Such a market entry would be extremely beneficial for funding the development of production CNTFET based process technology. This talk will provide an overview on the present status and feasibility of HF CNTFET technology will be given from an engineering point of view, including device modeling, experimental results, and existing roadblocks. Carbon nanotube transistor based high-<span class="hlt">frequency</span> electronics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016isms.confETC06L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016isms.confETC06L"><span>Mid-Infrared <span class="hlt">Frequency</span>-Agile Dual-Comb Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Pei-Ling; Yan, Ming; Iwakuni, Kana; Millot, Guy; Hänsch, Theodor W.; Picqué, Nathalie</p> <p>2016-06-01</p> <p>We demonstrate a new approach to mid-infrared dual-comb spectroscopy. It opens up new opportunities for accurate real-time spectroscopic diagnostics and it significantly simplifies the technique of dual-comb spectroscopy. Two mid-infrared <span class="hlt">frequency</span> combs of slightly different repetition <span class="hlt">frequencies</span> and moderate, but rapidly tunable, spectral span are generated in the 2800-3200 cm-1 region. The generators rely on electro-optic modulators, nonlinear fibers for spectral broadening and difference <span class="hlt">frequency</span> generation and do not involve mode-locked lasers. Flat-top <span class="hlt">frequency</span> combs span up to 10 cm-1 with a comb line spacing of 100 MHz (3×10-3 cm-1). The performance of the spectrometer without any phase-lock electronics or correction scheme is illustrated with spectra showing resolved comb lines and Doppler-limited spectra of methane. High precision on the spectroscopic parameter (line positions and intensities) determination is demonstrated for spectra measured on a millisecond time <span class="hlt">scale</span> and it is validated with comparison with literature data. G. Millot, S. Pitois, M. Yan, T. Hovannysyan, A. Bendahmane, T.W. Hänsch, N. Picqué, <span class="hlt">Frequency</span>-agile dual-comb spectroscopy, Nature Photonics 10, 27-30 (2016).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29877427','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29877427"><span>Coherent multi-heterodyne spectroscopy using acousto-optic <span class="hlt">frequency</span> combs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Durán, Vicente; Schnébelin, Cȏme; Guillet de Chatellus, Hugues</p> <p>2018-05-28</p> <p>We propose and characterize experimentally a new source of optical <span class="hlt">frequency</span> combs for performing multi-heterodyne spectrometry. This comb modality is based on a <span class="hlt">frequency</span>-shifting loop seeded with a continuous-wave (CW) monochromatic laser. The comb lines are generated by successive passes of the CW laser through an acousto-optic <span class="hlt">frequency</span> shifter. We report the generation of <span class="hlt">frequency</span> combs with more than 1500 mutually coherent lines, without resorting to non-linear broadening phenomena or external electronic modulation. The comb line spacing is easily reconfigurable from tens of MHz down to the kHz region. We first use a single acousto-optic <span class="hlt">frequency</span> comb to conduct self-heterodyne interferometry with a high <span class="hlt">frequency</span> resolution (500 kHz). By increasing the line spacing to 80 MHz, we demonstrate molecular spectroscopy on the sub-millisecond time <span class="hlt">scale</span>. In order to reduce the detection bandwidth, we subsequently implement an acousto-optic dual-comb spectrometer with the aid of two mutually coherent <span class="hlt">frequency</span> shifting loops. In each architecture, the potentiality of acousto-optic <span class="hlt">frequency</span> combs for spectroscopy is validated by spectral measurements of hydrogen cyanide in the near-infrared region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OExpr..2613800D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OExpr..2613800D"><span>Coherent multi-heterodyne spectroscopy using acousto-optic <span class="hlt">frequency</span> combs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durán, Vicente; Schnébelin, Cȏme; Guillet de Chatellus, Hugues</p> <p>2018-05-01</p> <p>We propose and characterize experimentally a new source of optical <span class="hlt">frequency</span> combs for performing multi-heterodyne spectrometry. This comb modality is based on a <span class="hlt">frequency</span> shifting loop seeded with a CW monochromatic laser. The comb lines are generated by successive passes of the CW laser through an acousto-optic <span class="hlt">frequency</span> shifter. We report the generation of <span class="hlt">frequency</span> combs with more than 1500 mutually coherent lines, without resorting to non-linear broadening phenomena or external electronic modulation. The comb line spacing is easily reconfigurable from tens of MHz down to the kHz region. We first use a single acousto-optic <span class="hlt">frequency</span> comb to conduct self-heterodyne interferometry with a high <span class="hlt">frequency</span> resolution (500 kHz). By increasing the line spacing to 80 MHz, we demonstrate molecular spectroscopy on the sub-millisecond time <span class="hlt">scale</span>. In order to reduce the detection bandwidth, we subsequently implement an acousto-optic dual-comb spectrometer with the aid of two mutually coherent <span class="hlt">frequency</span> shifting loops. In each architecture, the potentiality of acousto-optic <span class="hlt">frequency</span> combs for spectroscopy is validated by spectral measurements of hydrogen cyanide in the near-infrared region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080007193','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080007193"><span>Small <span class="hlt">Scale</span> Response and Modeling of Periodically Forced Turbulence</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bos, Wouter; Clark, Timothy T.; Rubinstein, Robert</p> <p>2007-01-01</p> <p>The response of the small <span class="hlt">scales</span> of isotropic turbulence to periodic large <span class="hlt">scale</span> forcing is studied using two-point closures. The <span class="hlt">frequency</span> response of the turbulent kinetic energy and dissipation rate, and the phase shifts between production, energy and dissipation are determined as functions of Reynolds number. It is observed that the amplitude and phase of the dissipation exhibit nontrivial <span class="hlt">frequency</span> and Reynolds number dependence that reveals a filtering effect of the energy cascade. Perturbation analysis is applied to understand this behavior which is shown to depend on distant interactions between widely separated <span class="hlt">scales</span> of motion. Finally, the extent to which finite dimensional models (standard two-equation models and various generalizations) can reproduce the observed behavior is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=%22flapping+flight%22+OR+%22flapping+wing%22+OR+%22bird+flight%22&id=EJ260300','ERIC'); return false;" href="https://eric.ed.gov/?q=%22flapping+flight%22+OR+%22flapping+wing%22+OR+%22bird+flight%22&id=EJ260300"><span>Fundamentals of Zoological <span class="hlt">Scaling</span>.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Lin, Herbert</p> <p>1982-01-01</p> <p>The following animal characteristics are considered to determine how properties and characteristics of various systems change with system size (<span class="hlt">scaling</span>): skeletal weight, speed of running, height and range of jumping, food consumption, heart rate, lifetime, locomotive efficiency, <span class="hlt">frequency</span> of wing-flapping, and maximum sizes of flying and hovering…</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/2018OptL...43.2406G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptL...43.2406G"><span>Terabit optical OFDM superchannel transmission via coherent carriers of a hybrid chip-<span class="hlt">scale</span> soliton <span class="hlt">frequency</span> comb</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geng, Yong; Huang, Xiatao; Cui, Wenwen; Ling, Yun; Xu, Bo; Zhang, Jin; Yi, Xingwen; Wu, Baojian; Huang, Shu-Wei; Qiu, Kun; Wong, Chee Wei; Zhou, Heng</p> <p>2018-05-01</p> <p>We demonstrate seamless channel multiplexing and high bitrate superchannel transmission of coherent optical orthogonal-<span class="hlt">frequency</span>-division-multiplexing (CO-OFDM) data signals utilizing a dissipative Kerr soliton (DKS) <span class="hlt">frequency</span> comb generated in an on-chip microcavity. Aided by comb line multiplication through Nyquist pulse modulation, the high stability and mutual coherence among mode-locked Kerr comb lines are exploited for the first time to eliminate the guard intervals between communication channels and achieve full spectral density bandwidth utilization. Spectral efficiency as high as 2.625 bit/Hz/s is obtained for 180 CO-OFDM bands encoded with 12.75 Gbaud 8-QAM data, adding up to total bitrate of 6.885 Tb/s within 2.295 THz <span class="hlt">frequency</span> comb bandwidth. Our study confirms that high coherence is the key superiority of Kerr soliton <span class="hlt">frequency</span> combs over independent laser diodes, as a multi-spectral coherent laser source for high-bandwidth high-spectral-density transmission networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JChPh.141l4504M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JChPh.141l4504M"><span><span class="hlt">Frequency</span> analysis of stress relaxation dynamics in model asphalts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Masoori, Mohammad; Greenfield, Michael L.</p> <p>2014-09-01</p> <p>Asphalt is an amorphous or semi-crystalline material whose mechanical performance relies on viscoelastic responses to applied strain or stress. Chemical composition and its effect on the viscoelastic properties of model asphalts have been investigated here by computing complex modulus from molecular dynamics simulation results for two different model asphalts whose compositions each resemble the Strategic Highway Research Program AAA-1 asphalt in different ways. For a model system that contains smaller molecules, simulation results for storage and loss modulus at 443 K reach both the low and high <span class="hlt">frequency</span> <span class="hlt">scaling</span> limits of the Maxwell model. Results for a model system composed of larger molecules (molecular weights 300-900 g/mol) with longer branches show a quantitatively higher complex modulus that decreases significantly as temperature increases over 400-533 K. Simulation results for its loss modulus approach the low <span class="hlt">frequency</span> <span class="hlt">scaling</span> limit of the Maxwell model at only the highest temperature simulated. A Black plot or van Gurp-Palman plot of complex modulus vs. phase angle for the system of larger molecules suggests some overlap among results at different temperatures for less high <span class="hlt">frequencies</span>, with an interdependence consistent with the empirical Christensen-Anderson-Marasteanu model. Both model asphalts are thermorheologically complex at very high <span class="hlt">frequencies</span>, where they show a loss peak that appears to be independent of temperature and density.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1691825','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1691825"><span>Tuning of Strouhal number for high propulsive efficiency accurately predicts how wingbeat <span class="hlt">frequency</span> and stroke amplitude relate and <span class="hlt">scale</span> with size and flight speed in birds.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Nudds, Robert L.; Taylor, Graham K.; Thomas, Adrian L. R.</p> <p>2004-01-01</p> <p>The wing kinematics of birds vary systematically with body size, but we still, after several decades of research, lack a clear mechanistic understanding of the aerodynamic selection pressures that shape them. Swimming and flying animals have recently been shown to cruise at Strouhal numbers (St) corresponding to a regime of vortex growth and shedding in which the propulsive efficiency of flapping foils peaks (St approximately fA/U, where f is wingbeat <span class="hlt">frequency</span>, U is cruising speed and A approximately bsin(theta/2) is stroke amplitude, in which b is wingspan and theta is stroke angle). We show that St is a simple and accurate predictor of wingbeat <span class="hlt">frequency</span> in birds. The Strouhal numbers of cruising birds have converged on the lower end of the range 0.2 < St < 0.4 associated with high propulsive efficiency. Stroke angle <span class="hlt">scales</span> as theta approximately 67b-0.24, so wingbeat <span class="hlt">frequency</span> can be predicted as f approximately St.U/bsin(33.5b-0.24), with St0.21 and St0.25 for direct and intermittent fliers, respectively. This simple aerodynamic model predicts wingbeat <span class="hlt">frequency</span> better than any other relationship proposed to date, explaining 90% of the observed variance in a sample of 60 bird species. Avian wing kinematics therefore appear to have been tuned by natural selection for high aerodynamic efficiency: physical and physiological constraints upon wing kinematics must be reconsidered in this light. PMID:15451698</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.tmp..215M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.tmp..215M"><span>Field-<span class="hlt">scale</span> comparison of <span class="hlt">frequency</span>- and time-domain spectral induced polarization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maurya, P. K.; Fiandaca, G.; Christiansen, A. V.; Auken, E.</p> <p>2018-05-01</p> <p>In this paper we present a comparison study of the time-domain (TD) and <span class="hlt">frequency</span>-domain (FD) spectral induced polarization (IP) methods in terms of acquisition time, data quality, and spectral information retrieved from inversion. We collected TDIP and FDIP surface measurements on three profiles with identical electrode setups, at two different field sites with different lithology. In addition, TDIP data were collected in two boreholes using the El-Log drilling technique, in which apparent formation resistivity and chargeability values are measured during drilling using electrodes integrated within the stem auger.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JVGR..128..201J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JVGR..128..201J"><span>Modelling the time-dependent <span class="hlt">frequency</span> content of low-<span class="hlt">frequency</span> volcanic earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jousset, Philippe; Neuberg, Jürgen; Sturton, Susan</p> <p>2003-11-01</p> <p>Low-<span class="hlt">frequency</span> volcanic earthquakes and tremor have been observed on seismic networks at a number of volcanoes, including Soufrière Hills volcano on Montserrat. Single events have well known characteristics, including a long duration (several seconds) and harmonic spectral peaks (0.2-5 Hz). They are commonly observed in swarms, and can be highly repetitive both in waveforms and amplitude spectra. As the time delay between them decreases, they merge into tremor, often preceding critical volcanic events like dome collapses or explosions. Observed amplitude spectrograms of long-period volcanic earthquake swarms may display gliding lines which reflect a time dependence in the <span class="hlt">frequency</span> content. Using a magma-filled dyke embedded in a solid homogeneous half-space as a simplified volcanic structure, we employ a 2D finite-difference method to compute the propagation of seismic waves in the conduit and its vicinity. We successfully replicate the seismic wave field of a single low-<span class="hlt">frequency</span> event, as well as the occurrence of events in swarms, their highly repetitive characteristics, and the time dependence of their spectral content. We use our model to demonstrate that there are two modes of conduit resonance, leading to two types of interface waves which are recorded at the free surface as surface waves. We also demonstrate that reflections from the top and the bottom of a conduit act as secondary sources that are recorded at the surface as repetitive low-<span class="hlt">frequency</span> events with similar waveforms. We further expand our modelling to account for gradients in physical properties across the magma-solid interface. We also expand it to account for time dependence of magma properties, which we implement by changing physical properties within the conduit during numerical computation of wave propagation. We use our expanded model to investigate the amplitude and time <span class="hlt">scales</span> required for modelling gliding lines, and show that changes in magma properties, particularly changes in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AeoRe..30...97M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AeoRe..30...97M"><span>High-<span class="hlt">frequency</span> measurements of aeolian saltation flux: Field-based methodology and applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, Raleigh L.; Kok, Jasper F.; Hugenholtz, Chris H.; Barchyn, Thomas E.; Chamecki, Marcelo; Ellis, Jean T.</p> <p>2018-02-01</p> <p>Aeolian transport of sand and dust is driven by turbulent winds that fluctuate over a broad range of temporal and spatial <span class="hlt">scales</span>. However, commonly used aeolian transport models do not explicitly account for such fluctuations, likely contributing to substantial discrepancies between models and measurements. Underlying this problem is the absence of accurate sand flux measurements at the short time <span class="hlt">scales</span> at which wind speed fluctuates. Here, we draw on extensive field measurements of aeolian saltation to develop a methodology for generating high-<span class="hlt">frequency</span> (up to 25 Hz) time series of total (vertically-integrated) saltation flux, namely by calibrating high-<span class="hlt">frequency</span> (HF) particle counts to low-<span class="hlt">frequency</span> (LF) flux measurements. The methodology follows four steps: (1) fit exponential curves to vertical profiles of saltation flux from LF saltation traps, (2) determine empirical calibration factors through comparison of LF exponential fits to HF number counts over concurrent time intervals, (3) apply these calibration factors to subsamples of the saltation count time series to obtain HF height-specific saltation fluxes, and (4) aggregate the calibrated HF height-specific saltation fluxes into estimates of total saltation fluxes. When coupled to high-<span class="hlt">frequency</span> measurements of wind velocity, this methodology offers new opportunities for understanding how aeolian saltation dynamics respond to variability in driving winds over time <span class="hlt">scales</span> from tens of milliseconds to days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860003112','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860003112"><span>Rapid estimation of <span class="hlt">frequency</span> response functions by close-range photogrammetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tripp, J. S.</p> <p>1985-01-01</p> <p>The accuracy of a rapid method which estimates the <span class="hlt">frequency</span> response function from stereoscopic dynamic data is computed. It is shown that reversal of the order of the operations of coordinate transformation and Fourier transformation, which provides a significant increase in computational speed, introduces error. A portion of the error, proportional to the perturbation components normal to the camera focal planes, cannot be eliminated. The remaining error may be eliminated by proper <span class="hlt">scaling</span> of <span class="hlt">frequency</span> data prior to coordinate transformation. Methods are developed for least squares estimation of the full 3x3 <span class="hlt">frequency</span> response matrix for a three dimensional structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22399371-repetition-frequency-scaling-all-polarization-maintaining-erbium-doped-mode-locked-fiber-laser-based-carbon-nanotubes-saturable-absorber','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22399371-repetition-frequency-scaling-all-polarization-maintaining-erbium-doped-mode-locked-fiber-laser-based-carbon-nanotubes-saturable-absorber"><span>Repetition <span class="hlt">frequency</span> <span class="hlt">scaling</span> of an all-polarization maintaining erbium-doped mode-locked fiber laser based on carbon nanotubes saturable absorber</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>Sotor, J., E-mail: jaroslaw.sotor@pwr.edu.pl; Sobon, G.; Abramski, K. M.</p> <p></p> <p>We demonstrate an all-polarization maintaining (PM), mode-locked erbium (Er)-doped fiber laser based on a carbon nanotubes (CNT) saturable absorber (SA). The laser resonator was maximally simplified by using only one passive hybrid component and a pair of fiber connectors with deposited CNTs. The repetition <span class="hlt">frequency</span> (F{sub rep}) of such a cost-effective and self-starting mode-locked laser was <span class="hlt">scaled</span> from 54.3 MHz to 358.6 MHz. The highest F{sub rep} was obtained when the total cavity length was shortened to 57 cm. The laser allows ultrashort pulse generation with the duration ranging from 240 fs to 550 fs. Because the laser components were based on PMmore » fibers the laser was immune to the external perturbations and generated laniary polarized light with the degree of polarization (DOP) of 98.7%.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...611A..72K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...611A..72K"><span>CHANG-ES. IX. Radio <span class="hlt">scale</span> heights and <span class="hlt">scale</span> lengths of a consistent sample of 13 spiral galaxies seen edge-on and their correlations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krause, Marita; Irwin, Judith; Wiegert, Theresa; Miskolczi, Arpad; Damas-Segovia, Ancor; Beck, Rainer; Li, Jiang-Tao; Heald, George; Müller, Peter; Stein, Yelena; Rand, Richard J.; Heesen, Volker; Walterbos, Rene A. M.; Dettmar, Ralf-Jürgen; Vargas, Carlos J.; English, Jayanne; Murphy, Eric J.</p> <p>2018-03-01</p> <p>Aim. The vertical halo <span class="hlt">scale</span> height is a crucial parameter to understand the transport of cosmic-ray electrons (CRE) and their energy loss mechanisms in spiral galaxies. Until now, the radio <span class="hlt">scale</span> height could only be determined for a few edge-on galaxies because of missing sensitivity at high resolution. Methods: We developed a sophisticated method for the <span class="hlt">scale</span> height determination of edge-on galaxies. With this we determined the <span class="hlt">scale</span> heights and radial <span class="hlt">scale</span> lengths for a sample of 13 galaxies from the CHANG-ES radio continuum survey in two <span class="hlt">frequency</span> bands. Results: The sample average values for the radio <span class="hlt">scale</span> heights of the halo are 1.1 ± 0.3 kpc in C-band and 1.4 ± 0.7 kpc in L-band. From the <span class="hlt">frequency</span> dependence analysis of the halo <span class="hlt">scale</span> heights we found that the wind velocities (estimated using the adiabatic loss time) are above the escape velocity. We found that the halo <span class="hlt">scale</span> heights increase linearly with the radio diameters. In order to exclude the diameter dependence, we defined a normalized <span class="hlt">scale</span> height h˜ which is quite similar for all sample galaxies at both <span class="hlt">frequency</span> bands and does not depend on the star formation rate or the magnetic field strength. However, h˜ shows a tight anticorrelation with the mass surface density. Conclusions: The sample galaxies with smaller <span class="hlt">scale</span> lengths are more spherical in the radio emission, while those with larger <span class="hlt">scale</span> lengths are flatter. The radio <span class="hlt">scale</span> height depends mainly on the radio diameter of the galaxy. The sample galaxies are consistent with an escape-dominated radio halo with convective cosmic ray propagation, indicating that galactic winds are a widespread phenomenon in spiral galaxies. While a higher star formation rate or star formation surface density does not lead to a higher wind velocity, we found for the first time observational evidence of a gravitational deceleration of CRE outflow, e.g. a lowering of the wind velocity from the galactic disk.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MAR.M1375S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MAR.M1375S"><span>Carbon nanotube transistor based high-<span class="hlt">frequency</span> electronics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schroter, Michael</p> <p></p> <p>At the nanoscale carbon nanotubes (CNTs) have higher carrier mobility and carrier velocity than most incumbent semiconductors. Thus CNT based field-effect transistors (FETs) are being considered as strong candidates for replacing existing MOSFETs in digital applications. In addition, the predicted high intrinsic transit <span class="hlt">frequency</span> and the more recent finding of ways to achieve highly linear transfer characteristics have inspired investigations on analog high-<span class="hlt">frequency</span> (HF) applications. High linearity is extremely valuable for an energy efficient usage of the <span class="hlt">frequency</span> spectrum, particularly in mobile communications. Compared to digital applications, the much more relaxed constraints for CNT placement and lithography combined with already achieved operating <span class="hlt">frequencies</span> of at least 10 GHz for fabricated devices make an early entry in the low GHz HF market more feasible than in large-<span class="hlt">scale</span> digital circuits. Such a market entry would be extremely beneficial for funding the development of production CNTFET based process technology. This talk will provide an overview on the present status and feasibility of HF CNTFET technology will be given from an engineering point of view, including device modeling, experimental results, and existing roadblocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28951158','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28951158"><span>Cortical feedback signals generalise across different spatial <span class="hlt">frequencies</span> of feedforward inputs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Revina, Yulia; Petro, Lucy S; Muckli, Lars</p> <p>2017-09-22</p> <p>Visual processing in cortex relies on feedback projections contextualising feedforward information flow. Primary visual cortex (V1) has small receptive fields and processes feedforward information at a fine-grained spatial <span class="hlt">scale</span>, whereas higher visual areas have larger, spatially invariant receptive fields. Therefore, feedback could provide coarse information about the global scene structure or alternatively recover fine-grained structure by targeting small receptive fields in V1. We tested if feedback signals generalise across different spatial <span class="hlt">frequencies</span> of feedforward inputs, or if they are tuned to the spatial <span class="hlt">scale</span> of the visual scene. Using a partial occlusion paradigm, functional magnetic resonance imaging (fMRI) and multivoxel pattern analysis (MVPA) we investigated whether feedback to V1 contains coarse or fine-grained information by manipulating the spatial <span class="hlt">frequency</span> of the scene surround outside an occluded image portion. We show that feedback transmits both coarse and fine-grained information as it carries information about both low (LSF) and high spatial <span class="hlt">frequencies</span> (HSF). Further, feedback signals containing LSF information are similar to feedback signals containing HSF information, even without a large overlap in spatial <span class="hlt">frequency</span> bands of the HSF and LSF scenes. Lastly, we found that feedback carries similar information about the spatial <span class="hlt">frequency</span> band across different scenes. We conclude that cortical feedback signals contain information which generalises across different spatial <span class="hlt">frequencies</span> of feedforward inputs. Copyright © 2017 The Authors. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995PhDT........48P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995PhDT........48P"><span>Characterization of Defects in <span class="hlt">Scaled</span> Mis Dielectrics with Variable <span class="hlt">Frequency</span> Charge Pumping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paulsen, Ronald Eugene</p> <p>1995-01-01</p> <p>Historically, the interface trap has been extensively investigated to determine the effects on device performance. Recently, much attention has been paid to trapping in near-interface oxide traps. Performance of high precision analog circuitry is affected by charge trapping in near-interface oxide traps which produces hysteresis, charge redistribution errors, and dielectric relaxation effects. In addition, the performance of low power digital circuitry, with reduced noise margins, may be drastically affected by the threshold voltage shifts associated with charge trapping in near -interface oxide traps. Since near-interface oxide traps may substantially alter the performance of devices, complete characterization of these defects is necessary. In this dissertation a new characterization technique, variable <span class="hlt">frequency</span> charge pumping, is introduced which allows charge trapped at the interface to be distinguished from the charge trapped within the oxide. The new experimental technique is an extension of the charge pumping technique to low <span class="hlt">frequencies</span> such that tunneling may occur from interface traps to near-interface oxide traps. A generalized charge pumping model, based on Shockley-Read-Hall statistics and trap-to-trap tunneling theory, has been developed which allows a more complete characterization of near-interface oxide traps. A pair of coupled differential equations governing the rate of change of occupied interface and near-interface oxide traps have been developed. Due to the experimental conditions in the charge pumping technique the equations may be decoupled, leading to an equation governing the rate of change of occupied interface traps and an equation governing the rate of change of occcupied near-interface oxide traps. Solving the interface trap equation and applying non-steady state charge dynamics leads to an interface trap component of the charge pumping current. In addition, solution to the near-interface oxide trap equation leads to an additional</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4745A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4745A"><span>Long-term, high-<span class="hlt">frequency</span> water quality monitoring in an agricultural catchment: insights from spectral analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aubert, Alice; Kirchner, James; Faucheux, Mikael; Merot, Philippe; Gascuel-Odoux, Chantal</p> <p>2013-04-01</p> <p>The choice of sampling <span class="hlt">frequency</span> is a key issue in the design and operation of environmental observatories. The choice of sampling <span class="hlt">frequency</span> creates a spectral window (or temporal filter) that highlights some timescales and processes, and de-emphasizes others (1). New online measurement technologies can monitor surface water quality almost continuously, allowing the creation of very rich time series. The question of how best to analyze such detailed temporal datasets is an important issue in environmental monitoring. In the present work, we studied water quality data from the AgrHys long-term hydrological observatory (located at Kervidy-Naizin, Western France) sampled at daily and 20-minute time <span class="hlt">scales</span>. Manual sampling has provided 12 years of daily measurements of nitrate, dissolved organic carbon (DOC), chloride and sulfate (2), and 3 years of daily measurements of about 30 other solutes. In addition, a UV-spectrometry probe (Spectrolyser) provides one year of 20-minute measurements for nitrate and DOC. Spectral analysis of the daily water quality time series reveals that our intensively farmed catchment exhibits universal 1/f <span class="hlt">scaling</span> (power spectrum slope of -1) for a large number of solutes, confirming and extending the earlier discovery of universal 1/f <span class="hlt">scaling</span> in the relatively pristine Plynlimon catchment (3). 1/f time series confound conventional methods for assessing the statistical significance of trends. Indeed, conventional methods assume that there is a clear separation of <span class="hlt">scales</span> between the signal (the trend line) and the noise (the scatter around the line). This is not true for 1/f noise, since it overestimates the occurrence of significant trends. Our results raise the possibility that 1/f <span class="hlt">scaling</span> is widespread in water quality time series, thus posing fundamental challenges to water quality trend analysis. Power spectra of the 20-minute nitrate and DOC time series show 1/f <span class="hlt">scaling</span> at <span class="hlt">frequencies</span> below 1/day, consistent with the longer-term daily</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvE..95d2202B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvE..95d2202B"><span><span class="hlt">Scaling</span> dependence and synchronization of forced mercury beating heart systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Biswas, Animesh; Das, Dibyendu; Parmananda, P.</p> <p>2017-04-01</p> <p>We perform experiments on a nonautonomous Mercury beating heart system, which is forced to pulsate using an external square wave potential. At suitable <span class="hlt">frequencies</span> and volumes, the drop exhibits pulsation with polygonal shapes having n corners. We find the <span class="hlt">scaling</span> dependence of the forcing <span class="hlt">frequency</span> νn on the volume V of the drop and establish the relationship νn∝n/√{V } . It is shown that the geometrical shape of substrate is important for obtaining closer match to these <span class="hlt">scaling</span> relationships. Furthermore, we study synchronization of two nonidentical drops driven by the same <span class="hlt">frequency</span> and establish that synchrony happens when the relationship n2/n1=√{V2/V1 } is satisfied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19760016541','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19760016541"><span>Vibration characteristics of 1/8-<span class="hlt">scale</span> dynamic models of the space-shuttle solid-rocket boosters</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Leadbetter, S. A.; Stephens, W.; Sewall, J. L.; Majka, J. W.; Barret, J. R.</p> <p>1976-01-01</p> <p>Vibration tests and analyses of six 1/8 <span class="hlt">scale</span> models of the space shuttle solid rocket boosters are reported. Natural vibration <span class="hlt">frequencies</span> and mode shapes were obtained for these aluminum shell models having internal solid fuel configurations corresponding to launch, midburn (maximum dynamic pressure), and near endburn (burnout) flight conditions. Test results for longitudinal, torsional, bending, and shell vibration <span class="hlt">frequencies</span> are compared with analytical predictions derived from thin shell theory and from finite element plate and beam theory. The lowest analytical longitudinal, torsional, bending, and shell vibration <span class="hlt">frequencies</span> were within + or - 10 percent of experimental values. The effects of damping and asymmetric end skirts on natural vibration <span class="hlt">frequency</span> were also considered. The analytical <span class="hlt">frequencies</span> of an idealized full <span class="hlt">scale</span> space shuttle solid rocket boosted structure are computed with and without internal pressure and are compared with the 1/8 <span class="hlt">scale</span> model results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NJPh...20e3009H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NJPh...20e3009H"><span>Fundamental limits to <span class="hlt">frequency</span> estimation: a comprehensive microscopic perspective</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haase, J. F.; Smirne, A.; Kołodyński, J.; Demkowicz-Dobrzański, R.; Huelga, S. F.</p> <p>2018-05-01</p> <p>We consider a metrology scenario in which qubit-like probes are used to sense an external field that affects their energy splitting in a linear fashion. Following the <span class="hlt">frequency</span> estimation approach in which one optimizes the state and sensing time of the probes to maximize the sensitivity, we provide a systematic study of the attainable precision under the impact of noise originating from independent bosonic baths. Specifically, we invoke an explicit microscopic derivation of the probe dynamics using the spin-boson model with weak coupling of arbitrary geometry. We clarify how the secular approximation leads to a phase-covariant (PC) dynamics, where the noise terms commute with the field Hamiltonian, while the inclusion of non-secular contributions breaks the PC. Moreover, unless one restricts to a particular (i.e., Ohmic) spectral density of the bath modes, the noise terms may contain relevant information about the <span class="hlt">frequency</span> to be estimated. Thus, by considering general evolutions of a single probe, we study regimes in which these two effects have a non-negligible impact on the achievable precision. We then consider baths of Ohmic spectral density yet fully accounting for the lack of PC, in order to characterize the ultimate attainable <span class="hlt">scaling</span> of precision when N probes are used in parallel. Crucially, we show that beyond the semigroup (Lindbladian) regime the Zeno limit imposing the 1/N 3/2 <span class="hlt">scaling</span> of the mean squared error, recently derived assuming PC, generalises to any dynamics of the probes, unless the latter are coupled to the baths in the direction perfectly transversal to the <span class="hlt">frequency</span> encoding—when a novel <span class="hlt">scaling</span> of 1/N 7/4 arises. As our microscopic approach covers all classes of dissipative dynamics, from semigroup to non-Markovian ones (each of them potentially non-phase-covariant), it provides an exhaustive picture, in which all the different asymptotic <span class="hlt">scalings</span> of precision naturally emerge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11051501','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11051501"><span>Application of a finite-element model to low-<span class="hlt">frequency</span> sound insulation in dwellings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Maluski, S P; Gibbs, B M</p> <p>2000-10-01</p> <p>The sound transmission between adjacent rooms has been modeled using a finite-element method. Predicted sound-level difference gave good agreement with experimental data using a full-<span class="hlt">scale</span> and a quarter-<span class="hlt">scale</span> model. Results show that the sound insulation characteristics of a party wall at low <span class="hlt">frequencies</span> strongly depend on the modal characteristics of the sound field of both rooms and of the partition. The effect of three edge conditions of the separating wall on the sound-level difference at low <span class="hlt">frequencies</span> was examined: simply supported, clamped, and a combination of clamped and simply supported. It is demonstrated that a clamped partition provides greater sound-level difference at low <span class="hlt">frequencies</span> than a simply supported. It also is confirmed that the sound-pressure level difference is lower in equal room than in unequal room configurations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhyA..413...25A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhyA..413...25A"><span>Permutation approach, high <span class="hlt">frequency</span> trading and variety of micro patterns in financial time series</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aghamohammadi, Cina; Ebrahimian, Mehran; Tahmooresi, Hamed</p> <p>2014-11-01</p> <p>Permutation approach is suggested as a method to investigate financial time series in micro <span class="hlt">scales</span>. The method is used to see how high <span class="hlt">frequency</span> trading in recent years has affected the micro patterns which may be seen in financial time series. Tick to tick exchange rates are considered as examples. It is seen that variety of patterns evolve through time; and that the <span class="hlt">scale</span> over which the target markets have no dominant patterns, have decreased steadily over time with the emergence of higher <span class="hlt">frequency</span> trading.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG21A0122C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG21A0122C"><span>Wave-field decay rate estimate from the wavenumber-<span class="hlt">frequency</span> spectra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Comisel, H.; Narita, Y.; Voros, Z.</p> <p>2017-12-01</p> <p>Observational data for wave or turbulent fields are conveniently analyzed and interpreted in the Fourier domain spanning the <span class="hlt">frequencies</span> and the wavenumbers. If a wave field has not only oscillatory components (characterized by real parts of <span class="hlt">frequency</span>) but also temporally decaying components (characterized by imaginary parts of <span class="hlt">frequency</span>), the energy spectrum shows a <span class="hlt">frequency</span> broadening around the peak due to the imaginary parts of <span class="hlt">frequency</span> (or the decay rate). The mechanism of the <span class="hlt">frequency</span> broadening is the same as that of the Breit-Wigner spectrum in nuclear resonance phenomena. We show that the decay rate can observationally and directly be estimated once multi-point data are available, and apply the method to Cluster four-point magnetometer data in the solar wind on a spatial <span class="hlt">scale</span> of about 1000 km. The estimated decay rate is larger than the eddy turnover time, indicating that the decay profile of solar wind turbulence is more plasma physical such as excitation of whistler waves and other modes rather than hydrodynamic turbulence behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780051462&hterms=Cambridge+Law&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DCambridge%2BLaw','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780051462&hterms=Cambridge+Law&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DCambridge%2BLaw"><span>A simplified Mach number <span class="hlt">scaling</span> law for helicopter rotor noise</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aravamudan, K. S.; Lee, A.; Harris, W. L.</p> <p>1978-01-01</p> <p>Mach number <span class="hlt">scaling</span> laws are derived for the rotational and the high-<span class="hlt">frequency</span> broadband noise from helicopter rotors. The rotational <span class="hlt">scaling</span> law is obtained directly from the theory of Lowson and Ollerhead (1969) by exploiting the properties of the dominant terms in the expression for the complex Fourier coefficients of sound radiation from a point source. The <span class="hlt">scaling</span> law for the high-<span class="hlt">frequency</span> broadband noise is obtained by assuming that the noise sources are acoustically compact and computing the instantaneous pressure due to an element on an airfoil where vortices are shed. Experimental results on the correlation lengths for stationary airfoils are extended to rotating airfoils. On the assumption that the correlation length varies as the boundary layer displacement thickness, it is found that the Mach number <span class="hlt">scaling</span> law contains a factor of Mach number raised to the exponent 5.8. Both <span class="hlt">scaling</span> laws were verified by model tests.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4630940','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4630940"><span>Notched-noise embedded <span class="hlt">frequency</span> specific chirps for objective audiometry using auditory brainstem responses</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Corona-Strauss, Farah I.; Schick, Bernhard; Delb, Wolfgang; Strauss, Daniel J.</p> <p>2012-01-01</p> <p>It has been shown recently that chirp-evoked auditory brainstem responses (ABRs) show better performance than click stimulations, especially at low intensity levels. In this paper we present the development, test, and evaluation of a series of notched-noise embedded <span class="hlt">frequency</span> specific chirps. ABRs were collected in healthy young control subjects using the developed stimuli. Results of the analysis of the corresponding ABRs using a time-<span class="hlt">scale</span> phase synchronization stability (PSS) measure are also reported. The resultant wave V amplitude and latency measures showed a similar behavior as for values reported in literature. The PSS of <span class="hlt">frequency</span> specific chirp-evoked ABRs reflected the presence of the wave V for all stimulation intensities. The <span class="hlt">scales</span> that resulted in higher PSS are in line with previous findings, where ABRs evoked by broadband chirps were analyzed, and which stated that low <span class="hlt">frequency</span> channels are better for the recognition and analysis of chirp-evoked ABRs. We conclude that the development and test of the series of notched-noise embedded <span class="hlt">frequency</span> specific chirps allowed the assessment of <span class="hlt">frequency</span> specific ABRs, showing an identifiable wave V for different intensity levels. Future work may include the development of a faster automatic recognition scheme for these <span class="hlt">frequency</span> specific ABRs. PMID:26557336</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DFD.L6005L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DFD.L6005L"><span>Flight testing of live Monarch butterflies to determine the aerodynamic benefit of butterfly <span class="hlt">scales</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lang, Amy; Cranford, Jacob; Conway, Jasmine; Slegers, Nathan; Dechello, Nicole; Wilroy, Jacob</p> <p>2014-11-01</p> <p>Evolutionary adaptations in the morphological structure of butterfly <span class="hlt">scales</span> (0.1 mm in size) to develop a unique micro-patterning resulting in a surface drag alteration, stem from a probable aerodynamic benefit of minimizing the energy requirement to fly a very lightweight body with comparably large surface area in a low Re flow regime. Live Monarch butterflies were tested at UAHuntsville's Autonomous Tracking and Optical Measurement (ATOM) Laboratory, which uses 22 Vicon T40 cameras that allow for millimeter level tracking of reflective markers at 515 fps over a 4 m × 6 m × 7 m volume. Data recorded included the flight path as well as the wing flapping angle and wing-beat <span class="hlt">frequency</span>. Insects were first tested with their <span class="hlt">scales</span> intact, and then again with the <span class="hlt">scales</span> carefully removed. Differences in flapping <span class="hlt">frequency</span> and/or energy obtained during flight due to the removal of the <span class="hlt">scales</span> will be discussed. Initial data analysis indicates that <span class="hlt">scale</span> removal in some specimens leads to increased flapping <span class="hlt">frequencies</span> for similar energetic flight or reduced flight speed for similar flapping <span class="hlt">frequencies</span>. Both results point to the <span class="hlt">scales</span> providing an aerodynamic benefit, which is hypothesized to be linked to leading-edge vortex formation and induced drag. Funding from the National Science Foundation (CBET and REU) is gratefully acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=bullied&pg=2&id=EJ1069572','ERIC'); return false;" href="https://eric.ed.gov/?q=bullied&pg=2&id=EJ1069572"><span>Self-Reported <span class="hlt">Frequency</span> and Perceived Severity of Being Bullied among Elementary School Students</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Chen, Li-Ming</p> <p>2015-01-01</p> <p>Background: This study reports students' perspectives on the <span class="hlt">frequency</span> and perceived severity of being bullied. Methods: A sample of 1816 elementary school students completed self-report surveys of perceived severity and <span class="hlt">frequency</span> of being bullied. A Rasch technique aligned different victimized behaviors on interval logit <span class="hlt">scales</span>. A 4-fold schema…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17164633','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17164633"><span>Examining the uniqueness of <span class="hlt">frequency</span> and intensity symptom ratings in posttraumatic stress disorder assessment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Elhai, Jon D; Lindsay, Brenda M; Gray, Matt J; Grubaugh, Anouk L; North, Terry C; Frueh, B Christopher</p> <p>2006-12-01</p> <p>Data from two studies are presented, investigating the relative effectiveness of posttraumatic stress disorder (PTSD) symptom <span class="hlt">frequency</span> and intensity rating dimensions, in assessing overall PTSD severity and diagnosis. We assessed <span class="hlt">frequency</span> and intensity ratings using 1) the Modified PTSD Symptom <span class="hlt">Scale</span> with 298 trauma-exposed college students, and 2) the Clinician-Administered PTSD <span class="hlt">Scale</span> with 130 combat-exposed military veterans. Results demonstrated little empirical justification for separating <span class="hlt">frequency</span> and intensity ratings when measuring PTSD. Large overlaps in variance were evidenced between the dimensions (suggesting construct redundancy), with little meaningful contribution to diagnosing PTSD using one dimension over the other. Implications for future PTSD clinical and research assessment are discussed, including the potential to decrease administration time for these commonly used PTSD measures, given their time-consuming nature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ASAJ..114Q2336G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ASAJ..114Q2336G"><span>Effects of <span class="hlt">frequency</span> shifts and visual gender information on vowel category judgments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Glidden, Catherine; Assmann, Peter F.</p> <p>2003-10-01</p> <p>Visual morphing techniques were used together with a high-quality vocoder to study the audiovisual contribution of talker gender to the identification of <span class="hlt">frequency</span>-shifted vowels. A nine-step continuum ranging from ``bit'' to ``bet'' was constructed from natural recorded syllables spoken by an adult female talker. Upward and downward <span class="hlt">frequency</span> shifts in spectral envelope (<span class="hlt">scale</span> factors of 0.85 and 1.0) were applied in combination with shifts in fundamental <span class="hlt">frequency</span>, F0 (<span class="hlt">scale</span> factors of 0.5 and 1.0). Downward <span class="hlt">frequency</span> shifts generally resulted in malelike voices whereas upward shifts were perceived as femalelike. Two separate nine-step visual continua from ``bit'' to ``bet'' were also constructed, one from a male face and the other a female face, each producing the end-point words. Each step along the two visual continua was paired with the corresponding step on the acoustic continuum, creating natural audiovisual utterances. Category boundary shifts were found for both acoustic cues (F0 and formant <span class="hlt">frequency</span> shifts) and visual cues (visual gender). The visual gender effect was larger when acoustic and visual information were matched appropriately. These results suggest that visual information provided by the speech signal plays an important supplemental role in talker normalization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43F1135C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43F1135C"><span>Large-<span class="hlt">Scale</span> Atmospheric Teleconnection Patterns Associated with the Interannual Variability of Heatwaves in East Asia and Its Decadal Changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choi, N.; Lee, M. I.; Lim, Y. K.; Kim, K. M.</p> <p>2017-12-01</p> <p>Heatwave is an extreme hot weather event which accompanies fatal damage to human health. The heatwave has a strong relationship with the large-<span class="hlt">scale</span> atmospheric teleconnection patterns. In this study, we examine the spatial pattern of heatwave in East Asia by using the EOF analysis and the relationship between heatwave <span class="hlt">frequency</span> and large-<span class="hlt">scale</span> atmospheric teleconnection patterns. We also separate the time <span class="hlt">scale</span> of heatwave <span class="hlt">frequency</span> as the time <span class="hlt">scale</span> longer than a decade and the interannual time <span class="hlt">scale</span>. The long-term variation of heatwave <span class="hlt">frequency</span> in East Asia shows a linkage with the sea surface temperature (SST) variability over the North Atlantic with a decadal time <span class="hlt">scale</span> (a.k.a. the Atlantic Multidecadal Oscillation; AMO). On the other hands, the interannual variation of heatwave <span class="hlt">frequency</span> is linked with the two dominant spatial patterns associated with the large-<span class="hlt">scale</span> teleconnection patterns mimicking the Scandinavian teleconnection (SCAND-like) pattern and the circumglobal teleconnection (CGT-like) pattern, respectively. It is highlighted that the interannual variation of heatwave <span class="hlt">frequency</span> in East Asia shows a remarkable change after mid-1990s. While the heatwave <span class="hlt">frequency</span> was mainly associated with the CGT-like pattern before mid-1990s, the SCAND-like pattern becomes the most dominant one after mid-1990s, making the CGT-like pattern as the second. This study implies that the large-<span class="hlt">scale</span> atmospheric teleconnection patterns play a key role in developing heatwave events in East Asia. This study further discusses possible mechanisms for the decadal change in the linkage between heatwave <span class="hlt">frequency</span> and the large-<span class="hlt">scale</span> teleconnection patterns in East Asia such as early melting of snow cover and/or weakening of East Asian jet stream due to global warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017FlDyR..49f5510K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017FlDyR..49f5510K"><span>Time-<span class="hlt">frequency</span> analysis of submerged synthetic jet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Abhay; Saha, Arun K.; Panigrahi, P. K.</p> <p>2017-12-01</p> <p>The coherent structures transport the finite body of fluid mass through rolling which plays an important role in heat transfer, boundary layer control, mixing, cooling, propulsion and other engineering applications. A synthetic jet in the form of a train of vortex rings having coherent structures of different length <span class="hlt">scales</span> is expected to be useful in these applications. The propagation and sustainability of these coherent structures (vortex rings) in downstream direction characterize the performance of synthetic jet. In the present study, the velocity signal acquired using the S-type hot-film probe along the synthetic jet centerline has been taken for the spectral analysis. One circular and three rectangular orifices of aspect ratio 1, 2 and 4 actuating at 1, 6 and 18 Hz <span class="hlt">frequency</span> have been used for creating different synthetic jets. The laser induced fluorescence images are used to study the flow structures qualitatively and help in explaining the velocity signal for detection of coherent structures. The study depicts four regions as vortex rollup and suction region (X/D h ≤ 3), steadily translating region (X/D h ≤ 3-8), vortex breakup region (X/Dh ≤ 4-8) and dissipation of small-<span class="hlt">scale</span> vortices (X/D h ≤ 8-15). The presence of coherent structures localized in physical and temporal domain is analyzed for the characterization of synthetic jet. Due to pulsatile nature of synthetic jet, analysis of velocity time trace or signal in time, <span class="hlt">frequency</span> and combined time-<span class="hlt">frequency</span> domain assist in characterizing the signatures of coherent structures. It has been observed that the maximum energy is in the first harmonic of actuation <span class="hlt">frequency</span>, which decreases slowly in downstream direction at 6 Hz compared to 1 and 18 Hz of actuation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1953i0077B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1953i0077B"><span>Polaronic conductivity and <span class="hlt">scaling</span> behavior of lithium iron phosphate glass</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banday, Azeem; Murugavel, Sevi</p> <p>2018-05-01</p> <p>Charge transport properties of the Lithium Iron Phosphate (LFP) glass has been investigated in a wide <span class="hlt">frequency</span> and temperature range by means of broadband dielectric spectroscopy. The conductivity spectra has been studied on the basis of Jonscher power law for characterizing the hopping dynamics of charge carriers. The ac conductivity and <span class="hlt">scaling</span> behavior of the LFP glass has been studied in the temperature range from 333K to 573K and <span class="hlt">frequency</span> range from 100 mHz to 1 MHz. The conductivity isotherms of LFP glass do not superimpose upon each other by using Summerfield <span class="hlt">scaling</span>. The structural peculiarities in the material could result in different conduction pathways giving rise to the deviation from Summerfield <span class="hlt">scaling</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5014860','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5014860"><span>A New Measure of Reading Habit: Going Beyond Behavioral <span class="hlt">Frequency</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>Schmidt, Fabian T. C.; Retelsdorf, Jan</p> <p>2016-01-01</p> <p>Reading habit is considered an important construct in reading research as it serves as a significant predictor of reading achievement. However, there is still no consensus on how to best measure reading habit. In recent research, it has mostly been measured as behavioral <span class="hlt">frequency</span>; this approach neglects the fact that repeated behavior does not cover the broad content of habitual behavior—such as automaticity and the expression of one’s identity. In this study, we aimed to adapt a 10-item <span class="hlt">scale</span> on the basis of the Self-Report Habit Index by Verplanken and Orbell (2003) that is comprehensive but still economical for measuring reading habit. It was tested by drawing on a sample of N = 1,418 upper secondary school students. The <span class="hlt">scale</span> showed good psychometric properties and the internal and external validity was supported. Moreover, the <span class="hlt">scale</span> predicted reading achievement and decoding speed over and above reading <span class="hlt">frequency</span>. The implications of an elaborated but still economical way of measuring reading habit are discussed giving new impetus on research on reading habit, challenging conventional approaches of traditional measures. PMID:27660619</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120001768','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120001768"><span>Ares I <span class="hlt">Scale</span> Model Acoustic Test Instrumentation for Acoustic and Pressure Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vargas, Magda B.; Counter, Douglas</p> <p>2011-01-01</p> <p>Ares I <span class="hlt">Scale</span> Model Acoustic Test (ASMAT) is a 5% <span class="hlt">scale</span> model test of the Ares I vehicle, launch pad and support structures conducted at MSFC to verify acoustic and ignition environments and evaluate water suppression systems Test design considerations 5% measurements must be <span class="hlt">scaled</span> to full <span class="hlt">scale</span> requiring high <span class="hlt">frequency</span> measurements Users had different <span class="hlt">frequencies</span> of interest Acoustics: 200 - 2,000 Hz full <span class="hlt">scale</span> equals 4,000 - 40,000 Hz model <span class="hlt">scale</span> Ignition Transient: 0 - 100 Hz full <span class="hlt">scale</span> equals 0 - 2,000 Hz model <span class="hlt">scale</span> Environment exposure Weather exposure: heat, humidity, thunderstorms, rain, cold and snow Test environments: Plume impingement heat and pressure, and water deluge impingement Several types of sensors were used to measure the environments Different instrument mounts were used according to the location and exposure to the environment This presentation addresses the observed effects of the selected sensors and mount design on the acoustic and pressure measurements</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27410083','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27410083"><span>Scattering effects and high-spatial-<span class="hlt">frequency</span> nanostructures on ultrafast laser irradiated surfaces of zirconium metallic alloys with nano-<span class="hlt">scaled</span> topographies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Chen; Cheng, Guanghua; Sedao, Xxx; Zhang, Wei; Zhang, Hao; Faure, Nicolas; Jamon, Damien; Colombier, Jean-Philippe; Stoian, Razvan</p> <p>2016-05-30</p> <p>The origin of high-spatial-<span class="hlt">frequency</span> laser-induced periodic surface structures (HSFL) driven by incident ultrafast laser fields, with their ability to achieve structure resolutions below λ/2, is often obscured by the overlap with regular ripples patterns at quasi-wavelength periodicities. We experimentally demonstrate here employing defined surface topographies that these structures are intrinsically related to surface roughness in the nano-<span class="hlt">scale</span> domain. Using Zr-based bulk metallic glass (Zr-BMG) and its crystalline alloy (Zr-CA) counterpart formed by thermal annealing from its glassy precursor, we prepared surfaces showing either smooth appearances on thermoplastic BMG or high-density nano-protuberances from randomly distributed embedded nano-crystallites with average sizes below 200 nm on the recrystallized alloy. Upon ultrashort pulse irradiation employing linearly polarized 50 fs, 800 nm laser pulses, the surfaces show a range of nanoscale organized features. The change of topology was then followed under multiple pulse irradiation at fluences around and below the single pulse threshold. While the former material (Zr-BMG) shows a specific high quality arrangement of standard ripples around the laser wavelength, the latter (Zr-CA) demonstrates strong predisposition to form high spatial <span class="hlt">frequency</span> rippled structures (HSFL). We discuss electromagnetic scenarios assisting their formation based on near-field interaction between particles and field-enhancement leading to structure linear growth. Finite-difference-time-domain simulations outline individual and collective effects of nanoparticles on electromagnetic energy modulation and the feedback processes in the formation of HSFL structures with correlation to regular ripples (LSFL).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28167573','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28167573"><span>Reynolds number trend of hierarchies and <span class="hlt">scale</span> interactions in turbulent boundary layers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baars, W J; Hutchins, N; Marusic, I</p> <p>2017-03-13</p> <p>Small-<span class="hlt">scale</span> velocity fluctuations in turbulent boundary layers are often coupled with the larger-<span class="hlt">scale</span> motions. Studying the nature and extent of this <span class="hlt">scale</span> interaction allows for a statistically representative description of the small <span class="hlt">scales</span> over a time <span class="hlt">scale</span> of the larger, coherent <span class="hlt">scales</span>. In this study, we consider temporal data from hot-wire anemometry at Reynolds numbers ranging from Re τ ≈2800 to 22 800, in order to reveal how the <span class="hlt">scale</span> interaction varies with Reynolds number. Large-<span class="hlt">scale</span> conditional views of the representative amplitude and <span class="hlt">frequency</span> of the small-<span class="hlt">scale</span> turbulence, relative to the large-<span class="hlt">scale</span> features, complement the existing consensus on large-<span class="hlt">scale</span> modulation of the small-<span class="hlt">scale</span> dynamics in the near-wall region. Modulation is a type of <span class="hlt">scale</span> interaction, where the amplitude of the small-<span class="hlt">scale</span> fluctuations is continuously proportional to the near-wall footprint of the large-<span class="hlt">scale</span> velocity fluctuations. Aside from this amplitude modulation phenomenon, we reveal the influence of the large-<span class="hlt">scale</span> motions on the characteristic <span class="hlt">frequency</span> of the small <span class="hlt">scales</span>, known as <span class="hlt">frequency</span> modulation. From the wall-normal trends in the conditional averages of the small-<span class="hlt">scale</span> properties, it is revealed how the near-wall modulation transitions to an intermittent-type <span class="hlt">scale</span> arrangement in the log-region. On average, the amplitude of the small-<span class="hlt">scale</span> velocity fluctuations only deviates from its mean value in a confined temporal domain, the duration of which is fixed in terms of the local Taylor time <span class="hlt">scale</span>. These concentrated temporal regions are centred on the internal shear layers of the large-<span class="hlt">scale</span> uniform momentum zones, which exhibit regions of positive and negative streamwise velocity fluctuations. With an increasing <span class="hlt">scale</span> separation at high Reynolds numbers, this interaction pattern encompasses the features found in studies on internal shear layers and concentrated vorticity fluctuations in high-Reynolds-number wall turbulence.This article is part of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PMB....61.5335S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PMB....61.5335S"><span>Image-driven, model-based 3D abdominal motion estimation for MR-guided radiotherapy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stemkens, Bjorn; Tijssen, Rob H. N.; de Senneville, Baudouin Denis; Lagendijk, Jan J. W.; van den Berg, Cornelis A. T.</p> <p>2016-07-01</p> <p>Respiratory motion introduces substantial uncertainties in abdominal radiotherapy for which traditionally large margins are used. The MR-Linac will open up the opportunity to acquire high resolution MR images just prior to radiation and during treatment. However, volumetric MRI time series are not able to characterize 3D tumor and organ-at-risk motion with sufficient temporal resolution. In this study we propose a method to estimate 3D deformation vector fields (<span class="hlt">DVFs</span>) with high spatial and temporal resolution based on fast 2D imaging and a subject-specific motion model based on respiratory correlated MRI. In a pre-beam phase, a retrospectively sorted 4D-MRI is acquired, from which the motion is parameterized using a principal component analysis. This motion model is used in combination with fast 2D cine-MR images, which are acquired during radiation, to generate full field-of-view 3D <span class="hlt">DVFs</span> with a temporal resolution of 476 ms. The geometrical accuracies of the input data (4D-MRI and 2D multi-slice acquisitions) and the fitting procedure were determined using an MR-compatible motion phantom and found to be 1.0-1.5 mm on average. The framework was tested on seven healthy volunteers for both the pancreas and the kidney. The calculated motion was independently validated using one of the 2D slices, with an average error of 1.45 mm. The calculated 3D <span class="hlt">DVFs</span> can be used retrospectively for treatment simulations, plan evaluations, or to determine the accumulated dose for both the tumor and organs-at-risk on a subject-specific basis in MR-guided radiotherapy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27362636','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27362636"><span>Image-driven, model-based 3D abdominal motion estimation for MR-guided radiotherapy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stemkens, Bjorn; Tijssen, Rob H N; de Senneville, Baudouin Denis; Lagendijk, Jan J W; van den Berg, Cornelis A T</p> <p>2016-07-21</p> <p>Respiratory motion introduces substantial uncertainties in abdominal radiotherapy for which traditionally large margins are used. The MR-Linac will open up the opportunity to acquire high resolution MR images just prior to radiation and during treatment. However, volumetric MRI time series are not able to characterize 3D tumor and organ-at-risk motion with sufficient temporal resolution. In this study we propose a method to estimate 3D deformation vector fields (<span class="hlt">DVFs</span>) with high spatial and temporal resolution based on fast 2D imaging and a subject-specific motion model based on respiratory correlated MRI. In a pre-beam phase, a retrospectively sorted 4D-MRI is acquired, from which the motion is parameterized using a principal component analysis. This motion model is used in combination with fast 2D cine-MR images, which are acquired during radiation, to generate full field-of-view 3D <span class="hlt">DVFs</span> with a temporal resolution of 476 ms. The geometrical accuracies of the input data (4D-MRI and 2D multi-slice acquisitions) and the fitting procedure were determined using an MR-compatible motion phantom and found to be 1.0-1.5 mm on average. The framework was tested on seven healthy volunteers for both the pancreas and the kidney. The calculated motion was independently validated using one of the 2D slices, with an average error of 1.45 mm. The calculated 3D <span class="hlt">DVFs</span> can be used retrospectively for treatment simulations, plan evaluations, or to determine the accumulated dose for both the tumor and organs-at-risk on a subject-specific basis in MR-guided radiotherapy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15196186','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15196186"><span>Nurse competence <span class="hlt">scale</span>: development and psychometric testing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Meretoja, Riitta; Isoaho, Hannu; Leino-Kilpi, Helena</p> <p>2004-07-01</p> <p>Self-assessment assists nurses to maintain and improve their practice by identifying their strengths and areas that may need to be further developed. Professional competence profiles encourage them to take an active part in the learning process of continuing education. Although competence recognition offers a way to motivate practising nurses to produce quality care, few measuring tools are available for this purpose. This paper describes the development and testing of the Nurse Competence <span class="hlt">Scale</span>, an instrument with which the level of nurse competence can be assessed in different hospital work environments. The categories of the Nurse Competence <span class="hlt">Scale</span> were derived from Benner's From Novice to Expert competency framework. A seven-step approach, including literature review and six expert groups, was used to identify and validate the indicators of nurse competence. After a pilot test, psychometric testing of the Nurse Competence <span class="hlt">Scale</span> (content, construct and concurrent validity, and internal consistency) was undertaken with 498 nurses. The 73-item <span class="hlt">scale</span> consists of seven categories, with responses on a visual analogy <span class="hlt">scale</span> format. The <span class="hlt">frequency</span> of using competencies was additionally tested with a four-point <span class="hlt">scale</span>. Self-assessed overall scores indicated a high level of competence across categories. The Nurse Competence <span class="hlt">Scale</span> data were normally distributed. The higher the <span class="hlt">frequency</span> of using competencies, the higher was the self-assessed level of competence. Age and length of work experience had a positive but not very strong correlation with level of competence. According to the item analysis, the categories of the Nurse Competence <span class="hlt">Scale</span> showed good internal consistency. The results provide strong evidence of the reliability and validity of the Nurse Competence <span class="hlt">Scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24857683','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24857683"><span>Coupling between high-<span class="hlt">frequency</span> ultrasound and solar photo-Fenton at pilot <span class="hlt">scale</span> for the treatment of organic contaminants: an initial approach.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Papoutsakis, Stefanos; Miralles-Cuevas, Sara; Gondrexon, Nicolas; Baup, Stéphane; Malato, Sixto; Pulgarin, César</p> <p>2015-01-01</p> <p>This study aims to evaluate the performance of a novel pilot-<span class="hlt">scale</span> coupled system consisting of a high <span class="hlt">frequency</span> ultrasonic reactor (400kHz) and a compound parabolic collector (CPC). The benefits of the concurrent application of ultrasound and the photo-Fenton process were studied in regard to the degradation behavior of a series of organic pollutants. Three compounds (phenol, bisphenol A and diuron) with different physicochemical properties have been chosen in order to identify possible synergistic effects and to obtain a better estimate of the general feasibility of such a system at field <span class="hlt">scale</span> (10L). Bisphenol A and diuron were specifically chosen due to their high hydrophobicity, and thus their assumed higher affinity towards the cavitation bubble. Experiments were conducted under ultrasonic, photo-Fenton and combined treatments. Enhanced degradation kinetics were observed during the coupled treatment and synergy factors clearly in excess of 1 have been calculated for phenol as well as for saturated solutions of bisphenol A and diuron. Although the relatively high cost of ultrasound compared to photo-Fenton still presents a significant challenge towards mainstream industrial application, the observed behavior suggests that its prudent use has the potential to significantly benefit the photo-Fenton process, via the decrease of both treatment time and H2O2 consumption. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994ptti.meet..523A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994ptti.meet..523A"><span>Russian national time <span class="hlt">scale</span> long-term stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alshina, A. P.; Gaigerov, B. A.; Koshelyaevsky, N. B.; Pushkin, S. B.</p> <p>1994-05-01</p> <p>The Institute of Metrology for Time and Space NPO 'VNIIFTRI' generates the National Time <span class="hlt">Scale</span> (NTS) of Russia -- one of the most stable time <span class="hlt">scales</span> in the world. Its striking feature is that it is based on a free ensemble of H-masers only. During last two years the estimations of NTS longterm stability based only on H-maser intercomparison data gives a flicker floor of about (2 to 3) x 10(exp -15) for averaging times from 1 day to 1 month. Perhaps the most significant feature for a time laboratory is an extremely low possible <span class="hlt">frequency</span> drift -- it is too difficult to estimate it reliably. The other estimations, free from possible inside the ensemble correlation phenomena, are available based on the time comparison of NTS relative to the stable enough time <span class="hlt">scale</span> of outer laboratories. The data on NTS comparison relative to the time <span class="hlt">scale</span> of secondary time and <span class="hlt">frequency</span> standards at Golitzino and Irkutsk in Russia and relative to NIST, PTB and USNO using GLONASS and GPS time transfer links gives stability estimations which are close to that based on H-maser intercomparisons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940026174','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940026174"><span>Russian national time <span class="hlt">scale</span> long-term stability</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Alshina, A. P.; Gaigerov, B. A.; Koshelyaevsky, N. B.; Pushkin, S. B.</p> <p>1994-01-01</p> <p>The Institute of Metrology for Time and Space NPO 'VNIIFTRI' generates the National Time <span class="hlt">Scale</span> (NTS) of Russia -- one of the most stable time <span class="hlt">scales</span> in the world. Its striking feature is that it is based on a free ensemble of H-masers only. During last two years the estimations of NTS longterm stability based only on H-maser intercomparison data gives a flicker floor of about (2 to 3) x 10(exp -15) for averaging times from 1 day to 1 month. Perhaps the most significant feature for a time laboratory is an extremely low possible <span class="hlt">frequency</span> drift -- it is too difficult to estimate it reliably. The other estimations, free from possible inside the ensemble correlation phenomena, are available based on the time comparison of NTS relative to the stable enough time <span class="hlt">scale</span> of outer laboratories. The data on NTS comparison relative to the time <span class="hlt">scale</span> of secondary time and <span class="hlt">frequency</span> standards at Golitzino and Irkutsk in Russia and relative to NIST, PTB and USNO using GLONASS and GPS time transfer links gives stability estimations which are close to that based on H-maser intercomparisons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S51E..07T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S51E..07T"><span><span class="hlt">Frequency</span>-dependent moment release of very low <span class="hlt">frequency</span> earthquakes in the Cascadia subduction zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takeo, A.; Houston, H.</p> <p>2014-12-01</p> <p>Episodic tremor and slip (ETS) has been observed in Cascadia subduction zone at two different time <span class="hlt">scales</span>: tremor at a high-<span class="hlt">frequency</span> range of 2-8 Hz and slow slip events at a geodetic time-<span class="hlt">scale</span> of days-months. The intermediate time <span class="hlt">scale</span> is needed to understand the source spectrum of slow earthquakes. Ghosh et al. (2014, IRIS abs) recently reported the presence of very low <span class="hlt">frequency</span> earthquakes (VLFEs) in Cascadia. In southwest Japan, VLFEs are usually observed at a period range around 20-50 s, and coincide with tremors (e.g., Ito et al. 2007). In this study, we analyzed VLFEs in and around the Olympic Peninsula to confirm their presence and estimate their moment release. We first detected VLFE events by using broadband seismograms with a band-pass filter of 20-50 s. The preliminary result shows that there are at least 16 VLFE events with moment magnitudes of 3.2-3.7 during the M6.8 2010 ETS. The focal mechanisms are consistent with the thrust earthquakes at the subducting plate interface. To detect signals of VLFEs below noise level, we further stacked long-period waveforms at the peak timings of tremor amplitudes for tremors within a 10-15 km radius by using tremor catalogs in 2006-2010, and estimated the focal mechanisms for each tremor source region as done in southwest Japan (Takeo et al. 2010 GRL). As a result, VLFEs could be detected for almost the entire tremor source region at a period range of 20-50 s with average moment magnitudes in each 5-min tremor window of 2.4-2.8. Although the region is limited, we could also detect VLFEs at a period range of 50-100 s with average moment magnitudes of 3.0-3.2. The moment release at 50-100 s is 4-8 times larger than that at 20-50 s, roughly consistent with an omega-squared spectral model. Further study including tremor, slow slip events and characteristic activities, such as rapid tremor reversal and tremor streaks, will reveal the source spectrum of slow earthquakes in a broader time <span class="hlt">scale</span> from 0.1 s to days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4043862','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4043862"><span>Interplay between Functional Connectivity and <span class="hlt">Scale</span>-Free Dynamics in Intrinsic fMRI Networks</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ciuciu, Philippe; Abry, Patrice; He, Biyu J.</p> <p>2014-01-01</p> <p>Studies employing functional connectivity-type analyses have established that spontaneous fluctuations in functional magnetic resonance imaging (fMRI) signals are organized within large-<span class="hlt">scale</span> brain networks. Meanwhile, fMRI signals have been shown to exhibit 1/f-type power spectra – a hallmark of <span class="hlt">scale</span>-free dynamics. We studied the interplay between functional connectivity and <span class="hlt">scale</span>-free dynamics in fMRI signals, utilizing the fractal connectivity framework – a multivariate extension of the univariate fractional Gaussian noise model, which relies on a wavelet formulation for robust parameter estimation. We applied this framework to fMRI data acquired from healthy young adults at rest and performing a visual detection task. First, we found that <span class="hlt">scale</span>-invariance existed beyond univariate dynamics, being present also in bivariate cross-temporal dynamics. Second, we observed that <span class="hlt">frequencies</span> within the <span class="hlt">scale</span>-free range do not contribute evenly to inter-regional connectivity, with a systematically stronger contribution of the lowest <span class="hlt">frequencies</span>, both at rest and during task. Third, in addition to a decrease of the Hurst exponent and inter-regional correlations, task performance modified cross-temporal dynamics, inducing a larger contribution of the highest <span class="hlt">frequencies</span> within the <span class="hlt">scale</span>-free range to global correlation. Lastly, we found that across individuals, a weaker task modulation of the <span class="hlt">frequency</span> contribution to inter-regional connectivity was associated with better task performance manifesting as shorter and less variable reaction times. These findings bring together two related fields that have hitherto been studied separately – resting-state networks and <span class="hlt">scale</span>-free dynamics, and show that <span class="hlt">scale</span>-free dynamics of human brain activity manifest in cross-regional interactions as well. PMID:24675649</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://www.dtic.mil/docs/citations/ADA492115','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA492115"><span>Special Issue on Time <span class="hlt">Scale</span> Algorithms</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2008-01-01</p> <p>are currently Two Way Satellite Time and <span class="hlt">Frequency</span> Transfer ( TWSTFT ) and GPS carrier phase time transfer. The interest in time <span class="hlt">scale</span> algorithms and...laboratory-specific innovations and practices, GNSS applications, UTC generation, TWSTFT applications, GPS applications, small-ensemble applications</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ApPhL.105b3902L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ApPhL.105b3902L"><span>On the natural <span class="hlt">frequency</span> of tidal current power systems—A discussion of sea testing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Ye; Yi, Jin-Hak; Song, Huimin; Wang, Qi; Yang, Zhaoqing; Kelley, Neil D.; Lee, Kwang-Soo</p> <p>2014-07-01</p> <p>To study the wet natural <span class="hlt">frequency</span> (in water) and dry natural <span class="hlt">frequency</span> (in air) of a tidal current turbine, we conducted a two-year measurement campaign by deploying a full-<span class="hlt">scale</span> prototype of the system. In this article, a theoretical model is developed and validated with the <span class="hlt">frequency</span> measurements. It reveals the measured wet natural <span class="hlt">frequency</span> of the system could approach half that of the dry one. The measurements also show that inflow turbulence is very important in the excitation of system resonances that can lead to system failure. We also briefly discuss how the wet <span class="hlt">frequency</span> varies over a long period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70187987','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70187987"><span>Doubling of coastal flooding <span class="hlt">frequency</span> within decades due to sea-level rise</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vitousek, Sean; Barnard, Patrick L.; Fletcher, Charles H.; Frazer, Neil; Erikson, Li; Storlazzi, Curt D.</p> <p>2017-01-01</p> <p>Global climate change drives sea-level rise, increasing the <span class="hlt">frequency</span> of coastal flooding. In most coastal regions, the amount of sea-level rise occurring over years to decades is significantly smaller than normal ocean-level fluctuations caused by tides, waves, and storm surge. However, even gradual sea-level rise can rapidly increase the <span class="hlt">frequency</span> and severity of coastal flooding. So far, global-<span class="hlt">scale</span> estimates of increased coastal flooding due to sea-level rise have not considered elevated water levels due to waves, and thus underestimate the potential impact. Here we use extreme value theory to combine sea-level projections with wave, tide, and storm surge models to estimate increases in coastal flooding on a continuous global <span class="hlt">scale</span>. We find that regions with limited water-level variability, i.e., short-tailed flood-level distributions, located mainly in the Tropics, will experience the largest increases in flooding <span class="hlt">frequency</span>. The 10 to 20 cm of sea-level rise expected no later than 2050 will more than double the <span class="hlt">frequency</span> of extreme water-level events in the Tropics, impairing the developing economies of equatorial coastal cities and the habitability of low-lying Pacific island nations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H33I..07K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H33I..07K"><span>Groundwater/Seawater Exchange over Multiple Time <span class="hlt">Scales</span>: Two Years of High-<span class="hlt">Frequency</span> Data from the Coastal Seabed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karam, H. N.; Mulligan, A. E.; Abarca, E.; Gardner, A.; Hemond, H.; Harvey, C. F.</p> <p>2013-12-01</p> <p>We present time series of vertical pressure gradients in the sea floor at Waquoit Bay, MA, collected along a transect of locations perpendicular to shore, with a 10-minute resolution over two years. The custom-made instruments used for data collection measure pressure differences with an accuracy of 0.5 mm freshwater head, and record pore water and surface water salinities, allowing a robust calculation of the direction and magnitude of flux across the sediment-water interface given an estimate of sediment permeability. Distinct processes of seawater circulation in the subsurface driven by different forcings, including storms, tides, variations in fresh groundwater head, and salinity gradients in coastal groundwater, are manifest as different <span class="hlt">frequency</span> components in the time series. We characterize the relative contributions of these different forcings to seafloor fluxes at our site, as a function of the time of year and the distance from shore. We find that: 1) Sea level variations drive variations in seafloor flux at time <span class="hlt">scales</span> of hours to weeks, around a mean flux that is produced by processes with longer time <span class="hlt">scales</span>, including the seasonal cycle in fresh groundwater head and the density-driven circulation of seawater through the coastal aquifer. 2) Seafloor flux responds non-linearly to shifts in seawater level. Furthermore, this response is asymmetric, with very low tides producing an amplified response in submarine groundwater discharge relative to the recharge produced by equivalently high tides. 3) The amplitude of seafloor pressure gradients shows a three-fold increase during winters relative to summers. We present a model to explain this effect based on the increase in shallow pore water viscosity at colder temperatures. We generalize our findings to help guide the design of sampling studies of seafloor fluxes at other sites. Finally, we present the distribution of subsurface residence times for seawater in Waquoit Bay, derived from our pressure gradient</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DFDH21003R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DFDH21003R"><span>End-effects-regime in full <span class="hlt">scale</span> and lab <span class="hlt">scale</span> rocket nozzles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rojo, Raymundo; Tinney, Charles; Baars, Woutijn; Ruf, Joseph</p> <p>2014-11-01</p> <p>Modern rockets utilize a thrust-optimized parabolic-contour design for their nozzles for its high performance and reliability. However, the evolving internal flow structures within these high area ratio rocket nozzles during start up generate a powerful amount of vibro-acoustic loads that act on the launch vehicle. Modern rockets must be designed to accommodate for these heavy loads or else risk a catastrophic failure. This study quantifies a particular moment referred to as the ``end-effects regime,'' or the largest source of vibro-acoustic loading during start-up [Nave & Coffey, AIAA Paper 1973-1284]. Measurements from full <span class="hlt">scale</span> ignitions are compared with aerodynamically <span class="hlt">scaled</span> representations in a fully anechoic chamber. Laboratory <span class="hlt">scale</span> data is then matched with both static and dynamic wall pressure measurements to capture the associating shock structures within the nozzle. The event generated during the ``end-effects regime'' was successfully reproduced in the both the lab-<span class="hlt">scale</span> models, and was characterized in terms of its mean, variance and skewness, as well as the spectral properties of the signal obtained by way of time-<span class="hlt">frequency</span> analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27415267','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27415267"><span>Kuramoto model with uniformly spaced <span class="hlt">frequencies</span>: Finite-N asymptotics of the locking threshold.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ottino-Löffler, Bertrand; Strogatz, Steven H</p> <p>2016-06-01</p> <p>We study phase locking in the Kuramoto model of coupled oscillators in the special case where the number of oscillators, N, is large but finite, and the oscillators' natural <span class="hlt">frequencies</span> are evenly spaced on a given interval. In this case, stable phase-locked solutions are known to exist if and only if the <span class="hlt">frequency</span> interval is narrower than a certain critical width, called the locking threshold. For infinite N, the exact value of the locking threshold was calculated 30 years ago; however, the leading corrections to it for finite N have remained unsolved analytically. Here we derive an asymptotic formula for the locking threshold when N≫1. The leading correction to the infinite-N result <span class="hlt">scales</span> like either N^{-3/2} or N^{-1}, depending on whether the <span class="hlt">frequencies</span> are evenly spaced according to a midpoint rule or an end-point rule. These <span class="hlt">scaling</span> laws agree with numerical results obtained by Pazó [D. Pazó, Phys. Rev. E 72, 046211 (2005)PLEEE81539-375510.1103/PhysRevE.72.046211]. Moreover, our analysis yields the exact prefactors in the <span class="hlt">scaling</span> laws, which also match the numerics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3045111','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3045111"><span>Speech Enhancement Using Gaussian <span class="hlt">Scale</span> Mixture Models</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hao, Jiucang; Lee, Te-Won; Sejnowski, Terrence J.</p> <p>2011-01-01</p> <p>This paper presents a novel probabilistic approach to speech enhancement. Instead of a deterministic logarithmic relationship, we assume a probabilistic relationship between the <span class="hlt">frequency</span> coefficients and the log-spectra. The speech model in the log-spectral domain is a Gaussian mixture model (GMM). The <span class="hlt">frequency</span> coefficients obey a zero-mean Gaussian whose covariance equals to the exponential of the log-spectra. This results in a Gaussian <span class="hlt">scale</span> mixture model (GSMM) for the speech signal in the <span class="hlt">frequency</span> domain, since the log-spectra can be regarded as <span class="hlt">scaling</span> factors. The probabilistic relation between <span class="hlt">frequency</span> coefficients and log-spectra allows these to be treated as two random variables, both to be estimated from the noisy signals. Expectation-maximization (EM) was used to train the GSMM and Bayesian inference was used to compute the posterior signal distribution. Because exact inference of this full probabilistic model is computationally intractable, we developed two approaches to enhance the efficiency: the Laplace method and a variational approximation. The proposed methods were applied to enhance speech corrupted by Gaussian noise and speech-shaped noise (SSN). For both approximations, signals reconstructed from the estimated <span class="hlt">frequency</span> coefficients provided higher signal-to-noise ratio (SNR) and those reconstructed from the estimated log-spectra produced lower word recognition error rate because the log-spectra fit the inputs to the recognizer better. Our algorithms effectively reduced the SSN, which algorithms based on spectral analysis were not able to suppress. PMID:21359139</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvD..97b5005C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvD..97b5005C"><span>Low-<span class="hlt">frequency</span> analogue Hawking radiation: The Korteweg-de Vries model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coutant, Antonin; Weinfurtner, Silke</p> <p>2018-01-01</p> <p>We derive analytic expressions for the low-<span class="hlt">frequency</span> properties of the analogue Hawking radiation in a general weak-dispersive medium. A thermal low-<span class="hlt">frequency</span> part of the spectrum is expected even when dispersive effects become significant. We consider the two most common class of weak-dispersive media and investigate all possible anomalous scattering processes due inhomogeneous background flows. We first argue that under minimal assumptions, the scattering processes in near-critical flows are well described by a linearized Korteweg-de Vries equation. Within our theoretical model grey-body factors are neglected, that is, the mode comoving with the flow decouples from the other ones. We also exhibit a flow example with an exact expression for the effective temperature. We see that this temperature coincides with the Hawking one only when the dispersive length <span class="hlt">scale</span> is much smaller than the flow gradient <span class="hlt">scale</span>. We apply the same method in inhomogeneous flows without an analogue horizon. In this case, the spectrum coefficients decrease with decreasing <span class="hlt">frequencies</span>. Our findings are in agreement with previous numerical works, generalizing their findings to arbitrary flow profiles. Our analytical expressions provide estimates to guide ongoing experimental efforts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29900957','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29900957"><span>High <span class="hlt">Frequency</span> of Fibromyalgia in Patients With Acne Vulgaris.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yazmalar, Levent; Çelepkolu, Tahsin; Batmaz, İbrahim; Sariyildiz, Mustafa Akif; Sula, Bilal; Alpayci, Mahmut; An, İsa; Burkan, Yahya Kemal; Uçak, Haydar; Çevik, Remzi</p> <p>2016-06-01</p> <p>This study aims to investigate the <span class="hlt">frequency</span> of fibromyalgia syndrome and to specify fibromyalgia syndrome-associated clinical symptoms in patients with acne vulgaris. Eighty-eight patients (28 males, 60 females; mean age 23.2±5.1 years; range 18 to 40 years) with acne vulgaris and age, sex- and body mass index-similar 76 healthy controls (14 males, 62 females; mean age 24.5±2.9 years; range 18 to 35 years) were included. Acne vulgaris was evaluated by using the Global Acne <span class="hlt">Scale</span>, while Hospital Anxiety and Depression <span class="hlt">Scale</span> was used to evaluate anxiety. Fibromyalgia-associated pain, sleep disturbance, anxiety, and menstrual cycle disturbance were significantly more frequent in patients with acne vulgaris than controls. Also, the severity of anxiety and the number of tender points were significantly higher in the acne vulgaris patients than controls. This study indicates that patients with acne vulgaris have increased <span class="hlt">frequency</span> of fibromyalgia syndrome than healthy controls (21.6% versus 5.3%, respectively).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017626','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017626"><span>The Atacama Cosmology Telescope: Likelihood for Small-<span class="hlt">Scale</span> CMB Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dunkley, J.; Calabrese, E.; Sievers, J.; Addison, G. E.; Battaglia, N.; Battistelli, E. S.; Bond, J. R.; Das, S.; Devlin, M. J.; Dunner, R.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140017626'); toggleEditAbsImage('author_20140017626_show'); toggleEditAbsImage('author_20140017626_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140017626_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140017626_hide"></p> <p>2013-01-01</p> <p>The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute <span class="hlt">scales</span> at <span class="hlt">frequencies</span> of 148 and 218 GHz, from three seasons of data. At small <span class="hlt">scales</span> the fluctuations in the primordial Cosmic Microwave Background (CMB) become increasingly obscured by extragalactic foregounds and secondary CMB signals. We present results from a nine-parameter model describing these secondary effects, including the thermal and kinematic Sunyaev-Zel'dovich (tSZ and kSZ) power; the clustered and Poisson-like power from Cosmic Infrared Background (CIB) sources, and their <span class="hlt">frequency</span> <span class="hlt">scaling</span>; the tSZ-CIB correlation coefficient; the extragalactic radio source power; and thermal dust emission from Galactic cirrus in two different regions of the sky. In order to extract cosmological parameters, we describe a likelihood function for the ACT data, fitting this model to the multi-<span class="hlt">frequency</span> spectra in the multipole range 500 < l < 10000. We extend the likelihood to include spectra from the South Pole Telescope at <span class="hlt">frequencies</span> of 95, 150, and 220 GHz. Accounting for different radio source levels and Galactic cirrus emission, the same model provides an excellent fit to both datasets simultaneously, with ?2/dof= 675/697 for ACT, and 96/107 for SPT. We then use the multi-<span class="hlt">frequency</span> likelihood to estimate the CMB power spectrum from ACT in bandpowers, marginalizing over the secondary parameters. This provides a simplified 'CMB-only' likelihood in the range 500 < l < 3500 for use in cosmological parameter estimation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23995148','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23995148"><span>Monitoring meso-<span class="hlt">scale</span> ordering of cellulose in intact plant cell walls using sum <span class="hlt">frequency</span> generation spectroscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Park, Yong Bum; Lee, Christopher M; Koo, Bon-Wook; Park, Sunkyu; Cosgrove, Daniel J; Kim, Seong H</p> <p>2013-10-01</p> <p>Sum <span class="hlt">frequency</span> generation (SFG) vibration spectroscopy can selectively detect crystalline cellulose without spectral interference from cell wall matrix components. Here, we show that the cellulose SFG spectrum is sensitive to cellulose microfibril alignment and packing within the cell wall. SFG intensity at 2,944 cm(-1) correlated well with crystalline cellulose contents of various regions of the Arabidopsis (Arabidopsis thaliana) inflorescence, while changes in the 3,320/2,944 cm(-1) intensity ratio suggest subtle changes in cellulose ordering as tissues mature. SFG analysis of two cellulose synthase mutants (irx1/cesa8 and irx3/cesa7) indicates a reduction in cellulose content without evidence of altered cellulose structure. In primary cell walls of Arabidopsis, cellulose exhibited a characteristic SFG peak at 2,920 and 3,320 cm(-1), whereas in secondary cell walls, it had peaks at 2,944 and 3,320 cm(-1). Starch (amylose) gave an SFG peak at 2,904 cm(-1) (CH methine) whose intensity increased with light exposure prior to harvest. Selective removal of matrix polysaccharides from primary cell walls by acid hydrolysis resulted in an SFG spectrum resembling that of secondary wall cellulose. Our results show that SFG spectroscopy is sensitive to the ordering of cellulose microfibrils in plant cell walls at the meso <span class="hlt">scale</span> (nm to μm) that is important for cell wall architecture but cannot be probed by other spectroscopic or diffraction techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4439524','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4439524"><span>Neural tuning matches <span class="hlt">frequency</span>-dependent time differences between the ears</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Benichoux, Victor; Fontaine, Bertrand; Franken, Tom P; Karino, Shotaro; Joris, Philip X; Brette, Romain</p> <p>2015-01-01</p> <p>The time it takes a sound to travel from source to ear differs between the ears and creates an interaural delay. It varies systematically with spatial direction and is generally modeled as a pure time delay, independent of <span class="hlt">frequency</span>. In acoustical recordings, we found that interaural delay varies with <span class="hlt">frequency</span> at a fine <span class="hlt">scale</span>. In physiological recordings of midbrain neurons sensitive to interaural delay, we found that preferred delay also varies with sound <span class="hlt">frequency</span>. Similar observations reported earlier were not incorporated in a functional framework. We find that the <span class="hlt">frequency</span> dependence of acoustical and physiological interaural delays are matched in key respects. This suggests that binaural neurons are tuned to acoustical features of ecological environments, rather than to fixed interaural delays. Using recordings from the nerve and brainstem we show that this tuning may emerge from neurons detecting coincidences between input fibers that are mistuned in <span class="hlt">frequency</span>. DOI: http://dx.doi.org/10.7554/eLife.06072.001 PMID:25915620</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhyA..344..252P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhyA..344..252P"><span>A comparison of high-<span class="hlt">frequency</span> cross-correlation measures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Precup, Ovidiu V.; Iori, Giulia</p> <p>2004-12-01</p> <p>On a high-<span class="hlt">frequency</span> <span class="hlt">scale</span> the time series are not homogeneous, therefore standard correlation measures cannot be directly applied to the raw data. There are two ways to deal with this problem. The time series can be homogenised through an interpolation method (An Introduction to High-<span class="hlt">Frequency</span> Finance, Academic Press, NY, 2001) (linear or previous tick) and then the Pearson correlation statistic computed. Recently, methods that can handle raw non-synchronous time series have been developed (Int. J. Theor. Appl. Finance 6(1) (2003) 87; J. Empirical Finance 4 (1997) 259). This paper compares two traditional methods that use interpolation with an alternative method applied directly to the actual time series.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AdAtS..34.1346L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AdAtS..34.1346L"><span>Impact of the time <span class="hlt">scale</span> of model sensitivity response on coupled model parameter estimation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Chang; Zhang, Shaoqing; Li, Shan; Liu, Zhengyu</p> <p>2017-11-01</p> <p>That a model has sensitivity responses to parameter uncertainties is a key concept in implementing model parameter estimation using filtering theory and methodology. Depending on the nature of associated physics and characteristic variability of the fluid in a coupled system, the response time <span class="hlt">scales</span> of a model to parameters can be different, from hourly to decadal. Unlike state estimation, where the update <span class="hlt">frequency</span> is usually linked with observational <span class="hlt">frequency</span>, the update <span class="hlt">frequency</span> for parameter estimation must be associated with the time <span class="hlt">scale</span> of the model sensitivity response to the parameter being estimated. Here, with a simple coupled model, the impact of model sensitivity response time <span class="hlt">scales</span> on coupled model parameter estimation is studied. The model includes characteristic synoptic to decadal <span class="hlt">scales</span> by coupling a long-term varying deep ocean with a slow-varying upper ocean forced by a chaotic atmosphere. Results show that, using the update <span class="hlt">frequency</span> determined by the model sensitivity response time <span class="hlt">scale</span>, both the reliability and quality of parameter estimation can be improved significantly, and thus the estimated parameters make the model more consistent with the observation. These simple model results provide a guideline for when real observations are used to optimize the parameters in a coupled general circulation model for improving climate analysis and prediction initialization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27077467','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27077467"><span>Harvesting Low-<span class="hlt">Frequency</span> (<5 Hz) Irregular Mechanical Energy: A Possible Killer Application of Triboelectric Nanogenerator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zi, Yunlong; Guo, Hengyu; Wen, Zhen; Yeh, Min-Hsin; Hu, Chenguo; Wang, Zhong Lin</p> <p>2016-04-26</p> <p>Electromagnetic generators (EMGs) and triboelectric nanogenerators (TENGs) are the two most powerful approaches for harvesting ambient mechanical energy, but the effectiveness of each depends on the triggering <span class="hlt">frequency</span>. Here, after systematically comparing the performances of EMGs and TENGs under low-<span class="hlt">frequency</span> motion (<5 Hz), we demonstrated that the output performance of EMGs is proportional to the square of the <span class="hlt">frequency</span>, while that of TENGs is approximately in proportion to the <span class="hlt">frequency</span>. Therefore, the TENG has a much better performance than that of the EMG at low <span class="hlt">frequency</span> (typically 0.1-3 Hz). Importantly, the extremely small output voltage of the EMG at low <span class="hlt">frequency</span> makes it almost inapplicable to drive any electronic unit that requires a certain threshold voltage (∼0.2-4 V), so that most of the harvested energy is wasted. In contrast, a TENG has an output voltage that is usually high enough (>10-100 V) and independent of <span class="hlt">frequency</span> so that most of the generated power can be effectively used to power the devices. Furthermore, a TENG also has advantages of light weight, low cost, and easy <span class="hlt">scale</span> up through advanced structure designs. All these merits verify the possible killer application of a TENG for harvesting energy at low <span class="hlt">frequency</span> from motions such as human motions for powering small electronics and possibly ocean waves for large-<span class="hlt">scale</span> blue energy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CNSNS..59..306Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CNSNS..59..306Z"><span>Interpreting Popov criteria in Lure´ systems with complex <span class="hlt">scaling</span> stability analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, J.</p> <p>2018-06-01</p> <p>The paper presents a novel <span class="hlt">frequency</span>-domain interpretation of Popov criteria for absolute stability in Lure´ systems by means of what we call complex <span class="hlt">scaling</span> stability analysis. The complex <span class="hlt">scaling</span> technique is developed for exponential/asymptotic stability in LTI feedback systems, which dispenses open-loop poles distribution, contour/locus orientation and prior <span class="hlt">frequency</span> sweeping. Exploiting the technique for alternatively revealing positive realness of transfer functions, re-interpreting Popov criteria is explicated. More specifically, the suggested <span class="hlt">frequency</span>-domain stability conditions are conformable both in scalar and multivariable cases, and can be implemented either graphically with locus plotting or numerically without; in particular, the latter is suitable as a design tool with auxiliary parameter freedom. The interpretation also reveals further <span class="hlt">frequency</span>-domain facts about Lure´ systems. Numerical examples are included to illustrate the main results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA532070','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA532070"><span>Direct CFD Predictions of Low <span class="hlt">Frequency</span> Sounds Generated by a Helicopter Main Rotor</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-05-01</p> <p>modeling and grid constraints. NOTATION α Shaft tilt (corrected) or tip-path-plane angle BPF Blade passing <span class="hlt">frequency</span> CT/σ Thrust coefficient to rotor...cyclic pitch angle, deg. LFSPL Low <span class="hlt">frequency</span> sound metric (1st-6th BPF ), dB MFSPL Mid <span class="hlt">frequency</span> sound metric (> 6th BPF ), dB OASPL Overall sound metric...Tunnel of the National Full- <span class="hlt">Scale</span> Aerodynamic Complex (NFAC) at NASA Ames Research Center in 2008 (Fig. 2a), as a guide for prediction validation. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22508898','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22508898"><span>Admissible Diffusion Wavelets and Their Applications in Space-<span class="hlt">Frequency</span> Processing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hou, Tingbo; Qin, Hong</p> <p>2013-01-01</p> <p>As signal processing tools, diffusion wavelets and biorthogonal diffusion wavelets have been propelled by recent research in mathematics. They employ diffusion as a smoothing and <span class="hlt">scaling</span> process to empower multiscale analysis. However, their applications in graphics and visualization are overshadowed by nonadmissible wavelets and their expensive computation. In this paper, our motivation is to broaden the application scope to space-<span class="hlt">frequency</span> processing of shape geometry and scalar fields. We propose the admissible diffusion wavelets (ADW) on meshed surfaces and point clouds. The ADW are constructed in a bottom-up manner that starts from a local operator in a high <span class="hlt">frequency</span>, and dilates by its dyadic powers to low <span class="hlt">frequencies</span>. By relieving the orthogonality and enforcing normalization, the wavelets are locally supported and admissible, hence facilitating data analysis and geometry processing. We define the novel rapid reconstruction, which recovers the signal from multiple bands of high <span class="hlt">frequencies</span> and a low-<span class="hlt">frequency</span> base in full resolution. It enables operations localized in both space and <span class="hlt">frequency</span> by manipulating wavelet coefficients through space-<span class="hlt">frequency</span> filters. This paper aims to build a common theoretic foundation for a host of applications, including saliency visualization, multiscale feature extraction, spectral geometry processing, etc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AAS...21113304W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AAS...21113304W"><span>The Importance of High <span class="hlt">Frequency</span> Observations for the SKA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Welch, William J.</p> <p>2007-12-01</p> <p>The plan for the Square Kilometer Array (SKA) is one or more very large arrays operating in two or more contiguous <span class="hlt">frequency</span> bands: roughly 15 - 90 MHz, 120 - 500 MHz, and 500 MHz - 25 GHz. The last band may be further divided into roughly 500 MHz - 1.5 GHz and 1.5 - 25 GHz. Construction costs may delay or forgo one or more of these bands. We argue that the entire high <span class="hlt">frequency</span> band is of special importance for astronomy both in the local universe and at great distances and early times. One of the Key Science Projects, the Cradle of Life, requires high sensitivity and resolution at <span class="hlt">frequencies</span> up to 20 GHz for the study of forming disks around new stars with disk opacities too great for millimeter wave observations. The larger issue of star formation, a poorly understood area, will also benefit from high sensitivity observations at short cm wavelengths. Magnetic field measurements through the Zeeman effect in the densest star forming gas are best done using tracers such as CCS at <span class="hlt">frequencies</span> of 11 and 22 GHz. The wide <span class="hlt">frequency</span> range of the SKA permits the observation of multiple rotational transitions of long chain molecules, providing accurate measures of both gas densities and temperatures. The wide field of view will permit large <span class="hlt">scale</span> surveys of entire star forming clouds revealing, at high resolution, the formation of clusters of pre-protostellar stars and class 0-2 protostars in line radiation. The continuum cm wave radiation will reveal the growth of grains in disks. On the larger <span class="hlt">scale</span>, observations of CO at high redshifts will trace the evolution of star formation and the formation of metals back to the Epic of Reionization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850006243&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850006243&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsonar"><span>Color and Grey <span class="hlt">Scale</span> in Sonar Displays</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kraiss, K. F.; Kuettelwesch, K. H.</p> <p>1984-01-01</p> <p>In spite of numerous publications 1 it is still rather unclear, whether color is of any help in sonar displays. The work presented here deals with a particular type of sonar data, i.e., LOFAR-grams (low <span class="hlt">frequency</span> analysing and recording) where acoustic sensor data are continuously written as a time-<span class="hlt">frequency</span> plot. The question to be answered quantitatively is, whether color coding does improve target detection when compared with a grey <span class="hlt">scale</span> code. The data show significant differences in receiver-operating characteristics performance for the selected codes. In addition it turned out, that the background noise level affects the performance dramatically for some color codes, while others remain stable or even improve. Generally valid rules are presented on how to generate useful color <span class="hlt">scales</span> for this particular application.</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/2018SPIE10512E..2AP','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10512E..2AP"><span>200-W single <span class="hlt">frequency</span> laser based on short active double clad tapered fiber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pierre, Christophe; Guiraud, Germain; Yehouessi, Jean-Paul; Santarelli, Giorgio; Boullet, Johan; Traynor, Nicholas; Vincont, Cyril</p> <p>2018-02-01</p> <p>High power single <span class="hlt">frequency</span> lasers are very attractive for a wide range of applications such as nonlinear conversion, gravitational wave sensing or atom trapping. Power <span class="hlt">scaling</span> in single <span class="hlt">frequency</span> regime is a challenging domain of research. In fact, nonlinear effect as stimulated Brillouin scattering (SBS) is the primary power limitation in single <span class="hlt">frequency</span> amplifiers. To mitigate SBS, different well-known techniques has been improved. These techniques allow generation of several hundred of watts [1]. Large mode area (LMA) fibers, transverse acoustically tailored fibers [2], coherent beam combining and also tapered fiber [3] seem to be serious candidates to continue the power <span class="hlt">scaling</span>. We have demonstrated the generation of stable 200W output power with nearly diffraction limited output, and narrow linewidth (Δν<30kHz) by using a tapered Yb-doped fiber which allow an adiabatic transition from a small purely single mode input to a large core output.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15550622','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15550622"><span>United time-<span class="hlt">frequency</span> spectroscopy for dynamics and global structure.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marian, Adela; Stowe, Matthew C; Lawall, John R; Felinto, Daniel; Ye, Jun</p> <p>2004-12-17</p> <p>Ultrashort laser pulses have thus far been used in two distinct modes. In the time domain, the pulses have allowed probing and manipulation of dynamics on a subpicosecond time <span class="hlt">scale</span>. More recently, phase stabilization has produced optical <span class="hlt">frequency</span> combs with absolute <span class="hlt">frequency</span> reference across a broad bandwidth. Here we combine these two applications in a spectroscopic study of rubidium atoms. A wide-bandwidth, phase-stabilized femtosecond laser is used to monitor the real-time dynamic evolution of population transfer. Coherent pulse accumulation and quantum interference effects are observed and well modeled by theory. At the same time, the narrow linewidth of individual comb lines permits a precise and efficient determination of the global energy-level structure, providing a direct connection among the optical, terahertz, and radio-<span class="hlt">frequency</span> domains. The mechanical action of the optical <span class="hlt">frequency</span> comb on the atomic sample is explored and controlled, leading to precision spectroscopy with an appreciable reduction in systematic errors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A42C..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A42C..07W"><span>Atmospheric River <span class="hlt">Frequency</span> and Intensity Changes in CMIP5 Climate Model Projections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Warner, M.; Mass, C.; Salathe, E. P., Jr.</p> <p>2012-12-01</p> <p>Most extreme precipitation events that occur along the North American west coast are associated with narrow plumes of above-average water vapor concentration that stretch from the tropics or subtropics to the West Coast. These events generally occur during the wet season (October-March) and are referred to as atmospheric rivers (AR). ARs can cause major river management problems, damage from flooding or landslides, and loss of life. It is currently unclear how these events will change in <span class="hlt">frequency</span> and intensity as a result of climate change in the coming century. While climate model global mean precipitation match observations reasonably well in historical runs, precipitation <span class="hlt">frequency</span> and intensity is generally poorly represented at local <span class="hlt">scales</span>; however, synoptic-<span class="hlt">scale</span> features are more realistically simulated by climate models, and AR events can be identified by extremely high values of integrated water vapor flux at points near the West Coast. There have been many recent studies indicating changes in synoptic-<span class="hlt">scale</span> features under climate change that could have meaningful impacts on the <span class="hlt">frequency</span> and intensity of ARs. In this study, a suite of CMIP5 models are used to analyze predicted changes in <span class="hlt">frequency</span> and intensity of AR events impacting the West Coast from the contemporary period (1970-1999) to the end of this century (2070-2099). Generally, integrated water vapor is predicted to increase in these models (both the mean and extremes) while low-level wind decreases and upper-level wind increases. This study aims to determine the influence of these changes on precipitation intensity in AR events in future climate simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21258918','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21258918"><span>Velocity perception for sounds moving in <span class="hlt">frequency</span> space.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Henry, Molly J; McAuley, J Devin</p> <p>2011-01-01</p> <p>In three experiments, we considered the relative contribution of <span class="hlt">frequency</span> change (Δf) and time change (Δt) to perceived velocity (Δf/Δt) for sounds that moved either continuously in <span class="hlt">frequency</span> space (Experiment 1) or in discrete steps (Experiments 2 and 3). In all the experiments, participants estimated "how quickly stimuli changed in pitch" on a <span class="hlt">scale</span> ranging from 0 (not changing at all) to 100 (changing very quickly). Objective <span class="hlt">frequency</span> velocity was specified in terms of semitones per second (ST/s), with ascending and descending stimuli presented on each trial at one of seven velocities (2, 4, 6, 8, 10, 12, and 14 ST/s). Separate contributions of <span class="hlt">frequency</span> change (Δf) and time change (Δt) to perceived velocity were assessed by holding total Δt constant and varying Δf or vice versa. For tone glides that moved continuously in <span class="hlt">frequency</span> space, both Δf and Δt cues contributed approximately equally to perceived velocity. For tone sequences, in contrast, perceived velocity was based almost entirely on Δt, with surprisingly little contribution from Δf. Experiment 3 considered separate judgments about Δf and Δt in order to rule out the possibility that the results of Experiment 2 were due to the inability to judge <span class="hlt">frequency</span> change in tone sequences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060031759&hterms=reliability+standards&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dreliability%2Bstandards','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060031759&hterms=reliability+standards&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dreliability%2Bstandards"><span>Optical <span class="hlt">frequency</span> standard development in support of NASA's gravity-mapping missions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Klipstein, W. M.; Seidel, D. J.; White, J. A.; Young, B. C.</p> <p>2001-01-01</p> <p>We intend to combine the exquisite performance over short time <span class="hlt">scales</span> coming from a cavity reference with the long-term stability of an atomic <span class="hlt">frequency</span> standard with an eye towards reliability in a spaceflight application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070031548','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070031548"><span>Radio <span class="hlt">Frequency</span> Mass Gauging of Propellants</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zimmerli, Gregory A.; Vaden, Karl R.; Herlacher, Michael D.; Buchanan, David A.; VanDresar, Neil T.</p> <p>2007-01-01</p> <p>A combined experimental and computer simulation effort was conducted to measure radio <span class="hlt">frequency</span> (RF) tank resonance modes in a dewar partially filled with liquid oxygen, and compare the measurements with numerical simulations. The goal of the effort was to demonstrate that computer simulations of a tank's electromagnetic eigenmodes can be used to accurately predict ground-based measurements, thereby providing a computational tool for predicting tank modes in a low-gravity environment. Matching the measured resonant <span class="hlt">frequencies</span> of several tank modes with computer simulations can be used to gauge the amount of liquid in a tank, thus providing a possible method to gauge cryogenic propellant tanks in low-gravity. Using a handheld RF spectrum analyzer and a small antenna in a 46 liter capacity dewar for experimental measurements, we have verified that the four lowest transverse magnetic eigenmodes can be accurately predicted as a function of liquid oxygen fill level using computer simulations. The input to the computer simulations consisted of tank dimensions, and the dielectric constant of the fluid. Without using any adjustable parameters, the calculated and measured <span class="hlt">frequencies</span> agree such that the liquid oxygen fill level was gauged to within 2 percent full <span class="hlt">scale</span> uncertainty. These results demonstrate the utility of using electromagnetic simulations to form the basis of an RF mass gauging technology with the power to simulate tank resonance <span class="hlt">frequencies</span> from arbitrary fluid configurations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatPh..13..771R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatPh..13..771R"><span>High-<span class="hlt">frequency</span> microrheology reveals cytoskeleton dynamics in living cells</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rigato, Annafrancesca; Miyagi, Atsushi; Scheuring, Simon; Rico, Felix</p> <p>2017-08-01</p> <p>Living cells are viscoelastic materials, dominated by an elastic response on timescales longer than a millisecond. On shorter timescales, the dynamics of individual cytoskeleton filaments are expected to emerge, but active microrheology measurements on cells accessing this regime are scarce. Here, we develop high-<span class="hlt">frequency</span> microrheology experiments to probe the viscoelastic response of living cells from 1 Hz to 100 kHz. We report the viscoelasticity of different cell types under cytoskeletal drug treatments. On previously inaccessible short timescales, cells exhibit rich viscoelastic responses that depend on the state of the cytoskeleton. Benign and malignant cancer cells revealed remarkably different <span class="hlt">scaling</span> laws at high <span class="hlt">frequencies</span>, providing a unique mechanical fingerprint. Microrheology over a wide dynamic range--up to the <span class="hlt">frequency</span> characterizing the molecular components--provides a mechanistic understanding of cell mechanics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28463745','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28463745"><span><span class="hlt">Frequency</span> selection for coda wave interferometry in concrete structures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fröjd, Patrik; Ulriksen, Peter</p> <p>2017-09-01</p> <p>This study contributes to the establishment of <span class="hlt">frequency</span> recommendations for use in coda wave interferometry structural health monitoring (SHM) systems for concrete structures. To this end, codas with widely different central <span class="hlt">frequencies</span> were used to detect boreholes with different diameters in a large concrete floor slab, and to track increasing damage in a small concrete beam subjected to bending loads. SHM results were obtained for damage that can be simulated by drilled holes on the <span class="hlt">scale</span> of a few mm or microcracks due to bending. These results suggest that signals in the range of 50-150kHz are suitable in large concrete structures where it is necessary to account for the high attenuation of high-<span class="hlt">frequency</span> signals. Copyright © 2017 The Authors. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24261042','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24261042"><span>Landscape-<span class="hlt">scale</span> forest disturbance regimes in southern Peruvian Amazonia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boyd, Doreen S; Hill, Ross A; Hopkinson, Chris; Baker, Timothy R</p> <p>2013-10-01</p> <p>Landscape-<span class="hlt">scale</span> gap-size <span class="hlt">frequency</span> distributions in tropical forests are a poorly studied but key ecological variable. Currently, a <span class="hlt">scale</span> gap currently exists between local-<span class="hlt">scale</span> field-based studies and those employing regional-<span class="hlt">scale</span> medium-resolution satellite data. Data at landscape <span class="hlt">scales</span> but of fine resolution would, however, facilitate investigation into a range of ecological questions relating to gap dynamics. These include whether canopy disturbances captured in permanent sample plots (PSPs) are representative of those in their surrounding landscape, and whether disturbance regimes vary with forest type. Here, therefore, we employ airborne LiDAR data captured over 142.5 km2 of mature, swamp, and regenerating forests in southeast Peru to assess the landscape-<span class="hlt">scale</span> disturbance at a sampling resolution of up to 2 m. We find that this landscape is characterized by large numbers of small gaps; large disturbance events are insignificant and infrequent. Of the total number of gaps that are 2 m2 or larger in area, just 0.45% were larger than 100 m2, with a power-law exponent (alpha) value of the gap-size <span class="hlt">frequency</span> distribution of 2.22. However, differences in disturbance regimes are seen among different forest types, with a significant difference in the alpha value of the gap-size <span class="hlt">frequency</span> distribution observed for the swamp/regenerating forests compared with the mature forests at higher elevations. Although a relatively small area of the total forest of this region was investigated here, this study presents an unprecedented assessment of this landscape with respect to its gap dynamics. This is particularly pertinent given the range of forest types present in the landscape and the differences observed. The coupling of detailed insights into forest properties and growth provided by PSPs with the broader statistics of disturbance events using remote sensing is recommended as a strong basis for <span class="hlt">scaling</span>-up estimates of landscape and regional-<span class="hlt">scale</span> carbon balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhRvL.102i8701G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhRvL.102i8701G"><span>Cross-Modulated Amplitudes and <span class="hlt">Frequencies</span> Characterize Interacting Components in Complex Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gans, Fabian; Schumann, Aicko Y.; Kantelhardt, Jan W.; Penzel, Thomas; Fietze, Ingo</p> <p>2009-03-01</p> <p>The dynamics of complex systems is characterized by oscillatory components on many time <span class="hlt">scales</span>. To study the interactions between these components we analyze the cross modulation of their instantaneous amplitudes and <span class="hlt">frequencies</span>, separating synchronous and antisynchronous modulation. We apply our novel technique to brain-wave oscillations in the human electroencephalogram and show that interactions between the α wave and the δ or β wave oscillators as well as spatial interactions can be quantified and related with physiological conditions (e.g., sleep stages). Our approach overcomes the limitation to oscillations with similar <span class="hlt">frequencies</span> and enables us to quantify directly nonlinear effects such as positive or negative <span class="hlt">frequency</span> modulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1236332-case-application-oblivious-energy-efficient-mpi-runtime','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1236332-case-application-oblivious-energy-efficient-mpi-runtime"><span>A Case for Application Oblivious Energy-Efficient MPI Runtime</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>Venkatesh, Akshay; Vishnu, Abhinav; Hamidouche, Khaled</p> <p></p> <p>Power has become the major impediment in designing large <span class="hlt">scale</span> high-end systems. Message Passing Interface (MPI) is the {\\em de facto} communication interface used as the back-end for designing applications, programming models and runtime for these systems. Slack --- the time spent by an MPI process in a single MPI call --- provides a potential for energy and power savings, if an appropriate power reduction technique such as core-idling/Dynamic Voltage and <span class="hlt">Frequency</span> <span class="hlt">Scaling</span> (<span class="hlt">DVFS</span>) can be applied without perturbing application's execution time. Existing techniques that exploit slack for power savings assume that application behavior repeats across iterations/executions. However, an increasingmore » use of adaptive, data-dependent workloads combined with system factors (OS noise, congestion) makes this assumption invalid. This paper proposes and implements Energy Aware MPI (EAM) --- an application-oblivious energy-efficient MPI runtime. EAM uses a combination of communication models of common MPI primitives (point-to-point, collective, progress, blocking/non-blocking) and an online observation of slack for maximizing energy efficiency. Each power lever incurs time overhead, which must be amortized over slack to minimize degradation. When predicted communication time exceeds a lever overhead, the lever is used {\\em as soon as possible} --- to maximize energy efficiency. When mis-prediction occurs, the lever(s) are used automatically at specific intervals for amortization. We implement EAM using MVAPICH2 and evaluate it on ten applications using up to 4096 processes. Our performance evaluation on an InfiniBand cluster indicates that EAM can reduce energy consumption by 5--41\\% in comparison to the default approach, with negligible (less than 4\\% in all cases) performance loss.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSM.H11C..02T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSM.H11C..02T"><span>Assessment of Multi-<span class="hlt">frequency</span> Electromagnetic Induction for Determining Soil Moisture Patterns at the Hillslope <span class="hlt">Scale</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tromp-van Meerveld, I.; McDonnell, J.</p> <p>2009-05-01</p> <p>We present an assessment of electromagnetic induction (EM) as a potential rapid and non-invasive method to map soil moisture patterns at the Panola (GA, USA) hillslope. We address the following questions regarding the applicability of EM measurements for hillslope hydrological investigations: (1) Can EM be used for soil moisture measurements in areas with shallow soils?; (2) Can EM represent the temporal and spatial patterns of soil moisture throughout the year?; and (3) can multiple <span class="hlt">frequencies</span> be used to extract additional information content from the EM approach and explain the depth profile of soil moisture? We found that the apparent conductivity measured with the multi-<span class="hlt">frequency</span> GEM-300 was linearly related to soil moisture measured with an Aqua-pro capacitance sensor below a threshold conductivity and represented the temporal patterns in soil moisture well. During spring rainfall events that wetted only the surface soil layers the apparent conductivity measurements explained the soil moisture dynamics at depth better than the surface soil moisture dynamics. All four EM <span class="hlt">frequencies</span> (7290, 9090, 11250, and 14010 Hz) were highly correlated and linearly related to each other and could be used to predict soil moisture. This limited our ability to use the four different EM <span class="hlt">frequencies</span> to obtain a soil moisture profile with depth. The apparent conductivity patterns represented the observed spatial soil moisture patterns well when the individually fitted relationships between measured soil moisture and apparent conductivity were used for each measurement point. However, when the same (master) relationship was used for all measurement locations, the soil moisture patterns were smoothed and did not resemble the observed soil moisture patterns very well. In addition, the range in calculated soil moisture values was reduced compared to observed soil moisture. Part of the smoothing was likely due to the much larger measurement area of the GEM-300 compared to the Aqua</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29263383','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29263383"><span>Inter-annual and decadal changes in teleconnections drive continental-<span class="hlt">scale</span> synchronization of tree reproduction.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ascoli, Davide; Vacchiano, Giorgio; Turco, Marco; Conedera, Marco; Drobyshev, Igor; Maringer, Janet; Motta, Renzo; Hacket-Pain, Andrew</p> <p>2017-12-20</p> <p>Climate teleconnections drive highly variable and synchronous seed production (masting) over large <span class="hlt">scales</span>. Disentangling the effect of high-<span class="hlt">frequency</span> (inter-annual variation) from low-<span class="hlt">frequency</span> (decadal trends) components of climate oscillations will improve our understanding of masting as an ecosystem process. Using century-long observations on masting (the MASTREE database) and data on the Northern Atlantic Oscillation (NAO), we show that in the last 60 years both high-<span class="hlt">frequency</span> summer and spring NAO, and low-<span class="hlt">frequency</span> winter NAO components are highly correlated to continent-wide masting in European beech and Norway spruce. Relationships are weaker (non-stationary) in the early twentieth century. This finding improves our understanding on how climate variation affects large-<span class="hlt">scale</span> synchronization of tree masting. Moreover, it supports the connection between proximate and ultimate causes of masting: indeed, large-<span class="hlt">scale</span> features of atmospheric circulation coherently drive cues and resources for masting, as well as its evolutionary drivers, such as pollination efficiency, abundance of seed dispersers, and natural disturbance regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGeod..86.1165B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGeod..86.1165B"><span>High-<span class="hlt">frequency</span> signal and noise estimates of CSR GRACE RL04</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonin, Jennifer A.; Bettadpur, Srinivas; Tapley, Byron D.</p> <p>2012-12-01</p> <p>A sliding window technique is used to create daily-sampled Gravity Recovery and Climate Experiment (GRACE) solutions with the same background processing as the official CSR RL04 monthly series. By estimating over shorter time spans, more frequent solutions are made using uncorrelated data, allowing for higher <span class="hlt">frequency</span> resolution in addition to daily sampling. Using these data sets, high-<span class="hlt">frequency</span> GRACE errors are computed using two different techniques: assuming the GRACE high-<span class="hlt">frequency</span> signal in a quiet area of the ocean is the true error, and computing the variance of differences between multiple high-<span class="hlt">frequency</span> GRACE series from different centers. While the signal-to-noise ratios prove to be sufficiently high for confidence at annual and lower <span class="hlt">frequencies</span>, at <span class="hlt">frequencies</span> above 3 cycles/year the signal-to-noise ratios in the large hydrological basins looked at here are near 1.0. Comparisons with the GLDAS hydrological model and high <span class="hlt">frequency</span> GRACE series developed at other centers confirm CSR GRACE RL04's poor ability to accurately and reliably measure hydrological signal above 3-9 cycles/year, due to the low power of the large-<span class="hlt">scale</span> hydrological signal typical at those <span class="hlt">frequencies</span> compared to the GRACE errors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H23J1709N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H23J1709N"><span>On Flood <span class="hlt">Frequency</span> in Urban Areas under Changing Conditions and Implications on Stormwater Infrastructure Planning and Design</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norouzi, A.; Habibi, H.; Nazari, B.; Noh, S.; Seo, D. J.; Zhang, Y.</p> <p>2016-12-01</p> <p>With urbanization and climate change, many areas in the US and abroad face increasing threats of flash flooding. Due to nonstationarities arising from changes in land cover and climate, however, it is not readily possible to project how such changes may modify flood <span class="hlt">frequency</span>. In this work, we describe a simple spatial stochastic model for rainfall-to-areal runoff in urban areas, evaluate climatological mean and variance of mean areal runoff (MAR) over a range of catchment <span class="hlt">scale</span>, translate them into runoff <span class="hlt">frequency</span>, which is used as a proxy for flood <span class="hlt">frequency</span>, and assess its sensitivity to precipitation, imperviousness and soil, and their changes as a function of catchment <span class="hlt">scale</span> and magnitude of precipitation. The findings indicate that, due to large sensitivity of <span class="hlt">frequency</span> of MAR to multiple hydrometeorological and physiographic factors, estimation of flood <span class="hlt">frequency</span> for urban catchments is inherently more uncertain. The approach used in this work is useful in developing bounds for flood <span class="hlt">frequencies</span> in urban areas under nonstationary conditions arising from urbanization and climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4179999','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4179999"><span><span class="hlt">Frequency</span> and Correlates of Suicidal Ideation in Pediatric Obsessive-Compulsive Disorder</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Storch, Eric A.; Bussing, Regina; Jacob, Marni L.; Nadeau, Joshua M.; Crawford, Erika; Mutch, P. Jane; Mason, Dana; Lewin, Adam B.; Murphy, Tanya K.</p> <p>2014-01-01</p> <p>This study examined the <span class="hlt">frequency</span> and sociodemographic and clinical correlates of suicidal ideation in a sample of children and adolescents with obsessive-compulsive disorder (OCD). Fifty-four youth with OCD and their parent(s) were administered the Schedule for Affective Disorders and Schizophrenia for School-Age Children-Present and Lifetime, Children’s Yale-Brown Obsessive Compulsive <span class="hlt">Scale</span>, and Children’s Depression Rating <span class="hlt">Scale</span>-Revised. Children completed the Suicidal Ideation Questionnaire - Junior, Child Obsessive Compulsive Impact Scale–Child, and Multidimensional Anxiety <span class="hlt">Scale</span> for Children; parents completed the Child Obsessive Compulsive Impact Scale–Parent, Swanson, Nolan, and Pelham–IV Parent <span class="hlt">Scale</span>, and Young Mania Rating Scale–Parent Version. Seven youth endorsed clinically significant levels of suicidal ideation on the Suicidal Ideation Questionnaire - Junior. Suicidal ideation was significantly related to clinician-rated depressive symptoms, age, child-rated impairment and anxiety symptoms, and symmetry, sexuality/religiosity and miscellaneous symptom dimensions. There was no significant association between suicidal ideation and obsessive-compulsive symptom severity, comorbidity patterns, or several parent-rated indices (e.g., impairment, impulsivity). These results provide initial information regarding the <span class="hlt">frequency</span> and correlates of suicidal ideation in treatment-seeking youth with OCD. Clinical implications are discussed, as well as directions for future research. PMID:24682580</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BoLMe.166...69C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BoLMe.166...69C"><span>High-<span class="hlt">Frequency</span> Response of the Atmospheric Electric Potential Gradient Under Strong and Dry Boundary-Layer Convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Conceição, Ricardo; Silva, Hugo Gonçalves; Bennett, Alec; Salgado, Rui; Bortoli, Daniele; Costa, Maria João; Collares Pereira, Manuel</p> <p>2018-01-01</p> <p>The spectral response of atmospheric electric potential gradient gives important information about phenomena affecting this gradient at characteristic time <span class="hlt">scales</span> ranging from years (e.g., solar modulation) to fractions of a second (e.g., turbulence). While long-term time <span class="hlt">scales</span> have been exhaustively explored, short-term <span class="hlt">scales</span> have received less attention. At such <span class="hlt">frequencies</span>, space-charge transport inside the planetary boundary layer becomes a sizeable contribution to the potential gradient variability. For the first time, co-located (Évora, Portugal) measurements of boundary-layer backscatter profiles and the 100-Hz potential gradient are reported. Five campaign days are analyzed, providing evidence for a relation between high-<span class="hlt">frequency</span> response of the potential gradient and strong dry convection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/486/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/486/"><span>High-<span class="hlt">Frequency</span>, Crosswell Radar Data Collected in a Laboratory Tank</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Peters, Bas; Moulton, Craig W.; Ellefsen, Karl J.; Horton, Robert J.; McKenna, Jason R.</p> <p>2010-01-01</p> <p>Crosswell radar data were collected among three wells in a laboratory tank filled with dry sand. Embedded within the sand was a long plastic box, which was the target for the data collection. Two datasets were collected between each pair of wells, making a total of six datasets. The <span class="hlt">frequencies</span> in the data ranged from 0.5 to 1.5 gigahertz, and the peak <span class="hlt">frequency</span> was 0.9 gigahertz. The data are well suited for evaluating various processing algorithms, and the data linearly <span class="hlt">scale</span> to typical field conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890035332&hterms=rate+change+frequency&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Drate%2Bchange%2Bfrequency','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890035332&hterms=rate+change+frequency&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Drate%2Bchange%2Bfrequency"><span>Vela X-1 pulse timing. II - Variations in pulse <span class="hlt">frequency</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Deeter, J. E.; Boynton, P. E.; Lamb, F. K.; Zylstra, G.</p> <p>1989-01-01</p> <p>The pulsed X-ray emission of Vela X-1 during May 1978 and December-January 1978-1979 is investigated analytically on the basis of published satellite observations. The data are compiled in tables and graphs and discussed in detail, with reference to data for the entire 1975-1982 period. Variations in pulse <span class="hlt">frequency</span> are identified on time <span class="hlt">scales</span> from 2 to 2600 days; the lower nine octaves are characterized as white noise (or random walk in pulse <span class="hlt">frequency</span>), while the longer-period variations are attributed to changes in neutron-star rotation rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27557196','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27557196"><span>Dissemination of optical-comb-based ultra-broadband <span class="hlt">frequency</span> reference through a fiber network.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nagano, Shigeo; Kumagai, Motohiro; Li, Ying; Ido, Tetsuya; Ishii, Shoken; Mizutani, Kohei; Aoki, Makoto; Otsuka, Ryohei; Hanado, Yuko</p> <p>2016-08-22</p> <p>We disseminated an ultra-broadband optical <span class="hlt">frequency</span> reference based on a femtosecond (fs)-laser optical comb through a kilometer-<span class="hlt">scale</span> fiber link. Its spectrum ranged from 1160 nm to 2180 nm without additional fs-laser combs at the end of the link. By employing a fiber-induced phase noise cancellation technique, the linewidth and fractional <span class="hlt">frequency</span> instability attained for all disseminated comb modes were of order 1 Hz and 10<sup>-18</sup> in a 5000 s averaging time. The ultra-broad optical <span class="hlt">frequency</span> reference, for which absolute <span class="hlt">frequency</span> is traceable to Japan Standard Time, was applied in the <span class="hlt">frequency</span> stabilization of an injection-seeded Q-switched 2051 nm pulse laser for a coherent light detection and ranging LIDAR system.</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/2011EnOp...43..813C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011EnOp...43..813C"><span>Optimizing a realistic large-<span class="hlt">scale</span> <span class="hlt">frequency</span> assignment problem using a new parallel evolutionary approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chaves-González, José M.; Vega-Rodríguez, Miguel A.; Gómez-Pulido, Juan A.; Sánchez-Pérez, Juan M.</p> <p>2011-08-01</p> <p>This article analyses the use of a novel parallel evolutionary strategy to solve complex optimization problems. The work developed here has been focused on a relevant real-world problem from the telecommunication domain to verify the effectiveness of the approach. The problem, known as <span class="hlt">frequency</span> assignment problem (FAP), basically consists of assigning a very small number of <span class="hlt">frequencies</span> to a very large set of transceivers used in a cellular phone network. Real data FAP instances are very difficult to solve due to the NP-hard nature of the problem, therefore using an efficient parallel approach which makes the most of different evolutionary strategies can be considered as a good way to obtain high-quality solutions in short periods of time. Specifically, a parallel hyper-heuristic based on several meta-heuristics has been developed. After a complete experimental evaluation, results prove that the proposed approach obtains very high-quality solutions for the FAP and beats any other result published.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhPl...22a2901K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhPl...22a2901K"><span>Ionospheric modifications in high <span class="hlt">frequency</span> heating experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuo, Spencer P.</p> <p>2015-01-01</p> <p>Featured observations in high-<span class="hlt">frequency</span> (HF) heating experiments conducted at Arecibo, EISCAT, and high <span class="hlt">frequency</span> active auroral research program are discussed. These phenomena appearing in the F region of the ionosphere include high-<span class="hlt">frequency</span> heater enhanced plasma lines, airglow enhancement, energetic electron flux, artificial ionization layers, artificial spread-F, ionization enhancement, artificial cusp, wideband absorption, short-<span class="hlt">scale</span> (meters) density irregularities, and stimulated electromagnetic emissions, which were observed when the O-mode HF heater waves with <span class="hlt">frequencies</span> below foF2 were applied. The implication and associated physical mechanism of each observation are discussed and explained. It is shown that these phenomena caused by the HF heating are all ascribed directly or indirectly to the excitation of parametric instabilities which instigate anomalous heating. Formulation and analysis of parametric instabilities are presented. The results show that oscillating two stream instability and parametric decay instability can be excited by the O-mode HF heater waves, transmitted from all three heating facilities, in the regions near the HF reflection height and near the upper hybrid resonance layer. The excited Langmuir waves, upper hybrid waves, ion acoustic waves, lower hybrid waves, and field-aligned density irregularities set off subsequent wave-wave and wave-electron interactions, giving rise to the observed phenomena.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4924066','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4924066"><span>Crash <span class="hlt">Frequency</span> Modeling Using Real-Time Environmental and Traffic Data and Unbalanced Panel Data Models</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chen, Feng; Chen, Suren; Ma, Xiaoxiang</p> <p>2016-01-01</p> <p>Traffic and environmental conditions (e.g., weather conditions), which frequently change with time, have a significant impact on crash occurrence. Traditional crash <span class="hlt">frequency</span> models with large temporal <span class="hlt">scales</span> and aggregated variables are not sufficient to capture the time-varying nature of driving environmental factors, causing significant loss of critical information on crash <span class="hlt">frequency</span> modeling. This paper aims at developing crash <span class="hlt">frequency</span> models with refined temporal <span class="hlt">scales</span> for complex driving environments, with such an effort providing more detailed and accurate crash risk information which can allow for more effective and proactive traffic management and law enforcement intervention. Zero-inflated, negative binomial (ZINB) models with site-specific random effects are developed with unbalanced panel data to analyze hourly crash <span class="hlt">frequency</span> on highway segments. The real-time driving environment information, including traffic, weather and road surface condition data, sourced primarily from the Road Weather Information System, is incorporated into the models along with site-specific road characteristics. The estimation results of unbalanced panel data ZINB models suggest there are a number of factors influencing crash <span class="hlt">frequency</span>, including time-varying factors (e.g., visibility and hourly traffic volume) and site-varying factors (e.g., speed limit). The study confirms the unique significance of the real-time weather, road surface condition and traffic data to crash <span class="hlt">frequency</span> modeling. PMID:27322306</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24677370','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24677370"><span>Nanoliter-droplet acoustic streaming via ultra high <span class="hlt">frequency</span> surface acoustic waves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shilton, Richie J; Travagliati, Marco; Beltram, Fabio; Cecchini, Marco</p> <p>2014-08-06</p> <p>The relevant length <span class="hlt">scales</span> in sub-nanometer amplitude surface acoustic wave-driven acoustic streaming are demonstrated. We demonstrate the absence of any physical limitations preventing the downscaling of SAW-driven internal streaming to nanoliter microreactors and beyond by extending SAW microfluidics up to operating <span class="hlt">frequencies</span> in the GHz range. This method is applied to nanoliter <span class="hlt">scale</span> fluid mixing. © 2014 The Authors. Published by WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23134714H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23134714H"><span>Probing the Jet Turnover <span class="hlt">Frequency</span> Dependence on Mass and Mass Accretion Rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hammerstein, Erica; Gültekin, Kayhan; King, Ashley</p> <p>2018-01-01</p> <p>We have examined a sample of 15 sub-Eddington supermassive black holes (SMBHs) in a variety of galaxy classifications to further understand the proposed fundamental plane of black hole activity and <span class="hlt">scaling</span> relations between black hole masses and their radio and X-ray luminosities. This plane describes black holes from stellar-mass to supermassive. The physics probed by these sub-Eddington systems is thought to be a radiatively inefficient, jet-dominated accretion flow. By studying black holes in this regime, we can learn important information on the disk-jet connection for accreting black holes.A key factor in studying the fundamental plane is the turnover <span class="hlt">frequency</span> — the <span class="hlt">frequency</span> at which emission transitions from optically thick at lower <span class="hlt">frequencies</span> to optically thin at higher <span class="hlt">frequencies</span>. This turnover point can be measured by observing the source in both radio and X-ray. Our project aims to test the dependence of the turnover <span class="hlt">frequency</span> on mass and mass accretion rate.Radio observations of the sample were obtained using the Karl G. Jansky Very Large Array (VLA) in the range of 5-40 GHz across four different <span class="hlt">frequency</span> bands in A configuration to give the highest spatial resolution to focus on the core emission. Our carefully chosen sample of SMBHs with dynamically measured masses consists of two sub-samples: those with approximately constant mass accretion rate (LX/LEdd ~ 10‑7) and those with approximately constant mass (MBH ~ 108 Msun). X-ray data were obtained from archival Chandra observations. To find the turnover <span class="hlt">frequency</span>, we used Markov Chain Monte Carlo methods to fit two power laws to the radio data and the archival X-ray data. The intersection of the radio and X-ray fits is the turnover <span class="hlt">frequency</span>.We present the results for both subsamples of SMBHs and their relationship between the turnover <span class="hlt">frequency</span> and X-ray luminosity, which we take to <span class="hlt">scale</span> with mass accretion rate, and jet power derived from both radio and X-ray properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26832546','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26832546"><span>Experimental demonstration of deep <span class="hlt">frequency</span> modulation interferometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Isleif, Katharina-Sophie; Gerberding, Oliver; Schwarze, Thomas S; Mehmet, Moritz; Heinzel, Gerhard; Cervantes, Felipe Guzmán</p> <p>2016-01-25</p> <p>Experiments for space and ground-based gravitational wave detectors often require a large dynamic range interferometric position readout of test masses with 1 pm/√Hz precision over long time <span class="hlt">scales</span>. Heterodyne interferometer schemes that achieve such precisions are available, but they require complex optical set-ups, limiting their scalability for multiple channels. This article presents the first experimental results on deep <span class="hlt">frequency</span> modulation interferometry, a new technique that combines sinusoidal laser <span class="hlt">frequency</span> modulation in unequal arm length interferometers with a non-linear fit algorithm. We have tested the technique in a Michelson and a Mach-Zehnder Interferometer topology, respectively, demonstrated continuous phase tracking of a moving mirror and achieved a performance equivalent to a displacement sensitivity of 250 pm/Hz at 1 mHz between the phase measurements of two photodetectors monitoring the same optical signal. By performing time series fitting of the extracted interference signals, we measured that the linearity of the laser <span class="hlt">frequency</span> modulation is on the order of 2% for the laser source used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25013277','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25013277"><span>Effects of Low-<span class="hlt">frequency</span> Current Sacral Dermatome Stimulation on Idiopathic Slow Transit Constipation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Jin-Seop; Yi, Seung-Ju</p> <p>2014-06-01</p> <p>[Purpose] This study aimed to determine whether low-<span class="hlt">frequency</span> current therapy can be used to reduce the symptoms of idiopathic slow transit constipation (ISTC). [Subjects] Fifteen patients (ten male and five female) with idiopathic slow transit constipation were enrolled in the present study. [Results] Bowel movements per day, bowel movements per week, and constipation assessment <span class="hlt">scale</span> scores significantly improved after low-<span class="hlt">frequency</span> current simulation of S2-S3. [Conclusion] Our results show that stimulation with low-<span class="hlt">frequency</span> current of the sacral dermatomes may offer therapeutic benefits for a subject of patients with ISTC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23383910','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23383910"><span>Ion kinetic <span class="hlt">scale</span> in the solar wind observed.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Śafránková, Jana; Němeček, Zdeněk; Přech, Lubomír; Zastenker, Georgy N</p> <p>2013-01-11</p> <p>This Letter shows the first results from the solar wind monitor onboard the Spektr-R spacecraft which measures plasma moments with a time resolution of 31 ms. This high-time resolution allows us to make direct observations of solar wind turbulence below ion kinetic length <span class="hlt">scales</span>. We present examples of the <span class="hlt">frequency</span> spectra of the density, velocity, and thermal velocity. Our study reveals that although these parameters exhibit the same behavior at the magnetohydrodynamic <span class="hlt">scale</span>, their spectra are remarkably different at the kinetic <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RRPRA..22....7K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RRPRA..22....7K"><span>I. S. Shklovsky and Low-<span class="hlt">Frequency</span> Radio Astronomy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konovalenko, A. A.</p> <p>2017-03-01</p> <p>Purpose: Proving of the high astrophysical significance of the low-<span class="hlt">frequency</span> radio astronomy (decameter and adjacent hectometer and meter wavelengths), demonstration of the priority results of the Ukrainian low-<span class="hlt">frequency</span> radio astronomy as well as significant contribution of I. S. Shklovsky to its development. Design/methodology/approach: The requirements to characteristics of high efficiency radio telescopes UTR-2, URAN, GURT and to sensitive and interference immune observational methods at low <span class="hlt">frequencies</span> are formulated by using the theoretical analysis and astrophysical predictions including those I. S. Shklovsky’s. Findings: New generation radio telescopes UTR-2, URAN, GURT are created and modernized. New observational methods at low <span class="hlt">frequencies</span> are introduced. Large-<span class="hlt">scale</span> investigations of the Solar system, Galaxy and Methagalaxy are carried out. They have allowed to detect new objects and phenomena for the continuum, monochromatic, pulse and sporadic cosmic radio emission. The role of I. S. Shklovsky in the development of many low-<span class="hlt">frequency</span> radio astronomy directions is noted, too. Conclusions: The unique possibilities of the low-<span class="hlt">frequency</span> radio astronomy which gives new information about the Universe, inaccessible with the other astrophysical methods, are shown. The progress of the low-<span class="hlt">frequency</span> radio astronomy opens the impressive possibilities for the future. It includes modernization of the largest radio telescopes UTR-2, URAN, NDA and creation of new instruments GURT, NenuFAR, LOFAR, LWA, MWA, SKA as well as making multi-antenna and ground-space experiments. The contribution of outstanding astrophysicist of the XX century I. S. Shklovsky to this part of actual astronomical science is evident, claiming for attention and will never be forgotten.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29955064','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29955064"><span>Zero-static power radio-<span class="hlt">frequency</span> switches based on MoS2 atomristors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Myungsoo; Ge, Ruijing; Wu, Xiaohan; Lan, Xing; Tice, Jesse; Lee, Jack C; Akinwande, Deji</p> <p>2018-06-28</p> <p>Recently, non-volatile resistance switching or memristor (equivalently, atomristor in atomic layers) effect was discovered in transitional metal dichalcogenides (TMD) vertical devices. Owing to the monolayer-thin transport and high crystalline quality, ON-state resistances below 10 Ω are achievable, making MoS 2 atomristors suitable as energy-efficient radio-<span class="hlt">frequency</span> (RF) switches. MoS 2 RF switches afford zero-hold voltage, hence, zero-static power dissipation, overcoming the limitation of transistor and mechanical switches. Furthermore, MoS 2 switches are fully electronic and can be integrated on arbitrary substrates unlike phase-change RF switches. High-<span class="hlt">frequency</span> results reveal that a key figure of merit, the cutoff <span class="hlt">frequency</span> (f c ), is about 10 THz for sub-μm 2 switches with favorable <span class="hlt">scaling</span> that can afford f c above 100 THz for nanoscale devices, exceeding the performance of contemporary switches that suffer from an area-invariant <span class="hlt">scaling</span>. These results indicate a new electronic application of TMDs as non-volatile switches for communication platforms, including mobile systems, low-power internet-of-things, and THz beam steering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhBio..15b6009B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhBio..15b6009B"><span>ProteinAC: a <span class="hlt">frequency</span> domain technique for analyzing protein dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bozkurt Varolgunes, Yasemin; Demir, Alper</p> <p>2018-03-01</p> <p>It is widely believed that the interactions of proteins with ligands and other proteins are determined by their dynamic characteristics as opposed to only static, time-invariant processes. We propose a novel computational technique, called ProteinAC (PAC), that can be used to analyze small <span class="hlt">scale</span> functional protein motions as well as interactions with ligands directly in the <span class="hlt">frequency</span> domain. PAC was inspired by a <span class="hlt">frequency</span> domain analysis technique that is widely used in electronic circuit design, and can be applied to both coarse-grained and all-atom models. It can be considered as a generalization of previously proposed static perturbation-response methods, where the <span class="hlt">frequency</span> of the perturbation becomes the key. We discuss the precise relationship of PAC to static perturbation-response schemes. We show that the <span class="hlt">frequency</span> of the perturbation may be an important factor in protein dynamics. Perturbations at different <span class="hlt">frequencies</span> may result in completely different response behavior while magnitude and direction are kept constant. Furthermore, we introduce several novel <span class="hlt">frequency</span> dependent metrics that can be computed via PAC in order to characterize response behavior. We present results for the ferric binding protein that demonstrate the potential utility of the proposed techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20632593','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20632593"><span>Real-time volumetric image reconstruction and 3D tumor localization based on a single x-ray projection image for lung cancer radiotherapy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Ruijiang; Jia, Xun; Lewis, John H; Gu, Xuejun; Folkerts, Michael; Men, Chunhua; Jiang, Steve B</p> <p>2010-06-01</p> <p>To develop an algorithm for real-time volumetric image reconstruction and 3D tumor localization based on a single x-ray projection image for lung cancer radiotherapy. Given a set of volumetric images of a patient at N breathing phases as the training data, deformable image registration was performed between a reference phase and the other N-1 phases, resulting in N-1 deformation vector fields (<span class="hlt">DVFs</span>). These <span class="hlt">DVFs</span> can be represented efficiently by a few eigenvectors and coefficients obtained from principal component analysis (PCA). By varying the PCA coefficients, new <span class="hlt">DVFs</span> can be generated, which, when applied on the reference image, lead to new volumetric images. A volumetric image can then be reconstructed from a single projection image by optimizing the PCA coefficients such that its computed projection matches the measured one. The 3D location of the tumor can be derived by applying the inverted DVF on its position in the reference image. The algorithm was implemented on graphics processing units (GPUs) to achieve real-time efficiency. The training data were generated using a realistic and dynamic mathematical phantom with ten breathing phases. The testing data were 360 cone beam projections corresponding to one gantry rotation, simulated using the same phantom with a 50% increase in breathing amplitude. The average relative image intensity error of the reconstructed volumetric images is 6.9% +/- 2.4%. The average 3D tumor localization error is 0.8 +/- 0.5 mm. On an NVIDIA Tesla C1060 GPU card, the average computation time for reconstructing a volumetric image from each projection is 0.24 s (range: 0.17 and 0.35 s). The authors have shown the feasibility of reconstructing volumetric images and localizing tumor positions in 3D in near real-time from a single x-ray image.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1014478','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1014478"><span>Radio <span class="hlt">frequency</span> detection assembly and method for detecting radio <span class="hlt">frequencies</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Cown, Steven H.; Derr, Kurt Warren</p> <p>2010-03-16</p> <p>A radio <span class="hlt">frequency</span> detection assembly is described and which includes a radio <span class="hlt">frequency</span> detector which detects a radio <span class="hlt">frequency</span> emission produced by a radio <span class="hlt">frequency</span> emitter from a given location which is remote relative to the radio <span class="hlt">frequency</span> detector; a location assembly electrically coupled with the radio <span class="hlt">frequency</span> detector and which is operable to estimate the location of the radio <span class="hlt">frequency</span> emitter from the radio <span class="hlt">frequency</span> emission which has been received; and a radio <span class="hlt">frequency</span> transmitter electrically coupled with the radio <span class="hlt">frequency</span> detector and the location assembly, and which transmits a radio <span class="hlt">frequency</span> signal which reports the presence of the radio <span class="hlt">frequency</span> emitter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSV...420..174H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSV...420..174H"><span>Multi-<span class="hlt">Scale</span> Stochastic Resonance Spectrogram for fault diagnosis of rolling element bearings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>He, Qingbo; Wu, Enhao; Pan, Yuanyuan</p> <p>2018-04-01</p> <p>It is not easy to identify incipient defect of a rolling element bearing by analyzing the vibration data because of the disturbance of background noise. The weak and unrecognizable transient fault signal of a mechanical system can be enhanced by the stochastic resonance (SR) technique that utilizes the noise in the system. However, it is challenging for the SR technique to identify sensitive fault information in non-stationary signals. This paper proposes a new method called multi-<span class="hlt">scale</span> SR spectrogram (MSSRS) for bearing defect diagnosis. The new method considers the non-stationary property of the defective bearing vibration signals, and treats every <span class="hlt">scale</span> of the time-<span class="hlt">frequency</span> distribution (TFD) as a modulation system. Then the SR technique is utilized on each modulation system according to each <span class="hlt">frequencies</span> in the TFD. The SR results are sensitive to the defect information because the energy of transient vibration is distributed in a limited <span class="hlt">frequency</span> band in the TFD. Collecting the spectra of the SR outputs at all <span class="hlt">frequency</span> <span class="hlt">scales</span> then generates the MSSRS. The proposed MSSRS is able to well deal with the non-stationary transient signal, and can highlight the defect-induced <span class="hlt">frequency</span> component corresponding to the impulse information. Experimental results with practical defective bearing vibration data have shown that the proposed method outperforms the former SR methods and exhibits a good application prospect in rolling element bearing fault diagnosis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4704029','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4704029"><span>High-<span class="hlt">frequency</span> chaotic dynamics enabled by optical phase-conjugation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mercier, Émeric; Wolfersberger, Delphine; Sciamanna, Marc</p> <p>2016-01-01</p> <p>Wideband chaos is of interest for applications such as random number generation or encrypted communications, which typically use optical feedback in a semiconductor laser. Here, we show that replacing conventional optical feedback with phase-conjugate feedback improves the chaos bandwidth. In the range of achievable phase-conjugate mirror reflectivities, the bandwidth increase reaches 27% when compared with feedback from a conventional mirror. Experimental measurements of the time-resolved <span class="hlt">frequency</span> dynamics on nanosecond time-<span class="hlt">scales</span> show that the bandwidth enhancement is related to the onset of self-pulsing solutions at harmonics of the external-cavity <span class="hlt">frequency</span>. In the observed regime, the system follows a chaotic itinerancy among these destabilized high-<span class="hlt">frequency</span> external-cavity modes. The recorded features are unique to phase-conjugate feedback and distinguish it from the long-standing problem of time-delayed feedback dynamics. PMID:26739806</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SMaS...26i5008Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SMaS...26i5008Y"><span>Internal resonance and low <span class="hlt">frequency</span> vibration energy harvesting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Wei; Towfighian, Shahrzad</p> <p>2017-09-01</p> <p>A nonlinear vibration energy harvester with internal resonance is presented. The proposed harvester consists of two cantilevers, each with a permanent magnet on its tip. One cantilever has a piezoelectric layer at its base. When magnetic force is applied this two degrees-of-freedom nonlinear vibration system shows the internal resonance phenomenon that broadens the <span class="hlt">frequency</span> bandwidth compared to a linear system. Three coupled partial differential equations are obtained to predict the dynamic behavior of the nonlinear energy harvester. The perturbation method of multiple <span class="hlt">scales</span> is used to solve equations. Results from experiments done at different vibration levels with varying distances between the magnets validate the mathematical model. Experiments and simulations show the design outperforms the linear system by doubling the <span class="hlt">frequency</span> bandwidth. Output voltage for <span class="hlt">frequency</span> response is studied for different system parameters. The optimal load resistance is obtained for the maximum power in the internal resonance case. The results demonstrate that a design combining internal resonance and magnetic nonlinearity improves the efficiency of energy harvesting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1356284','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1356284"><span>GMLC Hawaii Regional Partnership: Distributed Inverter-Based Grid <span class="hlt">Frequency</span> Support</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>Nelson, Austin; Hoke, Andy</p> <p></p> <p>This presentation is part of a panel session at the IEEE ISGT conference on Grid Modernization Initiative projects. This segment of the panel session provides a brief overview of a Hawaii Regional Partnership project focusing grid <span class="hlt">frequency</span> support from distributed resources on the fastest time <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23284815','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23284815"><span>Long-term tinnitus suppression with linear octave <span class="hlt">frequency</span> transposition hearing AIDS.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peltier, Elisabeth; Peltier, Cedric; Tahar, Stephanie; Alliot-Lugaz, Evelyne; Cazals, Yves</p> <p>2012-01-01</p> <p>Over the last three years of hearing aid dispensing, it was observed that among 74 subjects fitted with a linear octave <span class="hlt">frequency</span> transposition (LOFT) hearing aid, 60 reported partial or complete tinnitus suppression during day and night, an effect still lasting after several months or years of daily use. We report in more details on 38 subjects from whom we obtained quantified measures of tinnitus suppression through visual analog <span class="hlt">scaling</span> and several additional psychoacoustic and audiometric measures. The long-term suppression seems independent of subject age, and of duration and subjective localization of tinnitus. A small but significant correlation was found with audiogram losses but not with high <span class="hlt">frequency</span> loss slope. Long-term tinnitus suppression was observed for different etiologies, but with a low success rate for sudden deafness. It should be noted that a majority of subjects (23) had a history of noise exposure. Tinnitus suppression started after a few days of LOFT hearing aid use and reached a maximum after a few weeks of daily use. For nine subjects different amounts of <span class="hlt">frequency</span> shifting were tried and found more or less successful for long-term tinnitus suppression, no correlation was found with tinnitus pitch. When the use of the LOFT hearing aid was stopped tinnitus reappeared within a day, and after re-using the LOFT aid it disappeared again within a day. For about one third of the 38 subjects a classical amplification or a non linear <span class="hlt">frequency</span> compression aid was also tried, and no such tinnitus suppression was observed. Besides improvements in audiometric sensitivity to high <span class="hlt">frequencies</span> and in speech discrimination scores, LOFT can be considered as a remarkable opportunity to suppress tinnitus over a long time <span class="hlt">scale</span>. From a pathophysiological viewpoint these observations seem to fit with a possible re-attribution of activity to previously deprived cerebral areas corresponding to high <span class="hlt">frequency</span> coding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IAUGA..2248188P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IAUGA..2248188P"><span>The <span class="hlt">frequency</span> of stellar X-ray flares from a large-<span class="hlt">scale</span> XMM-Newton sample</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pye, John P.; Rosen, Simon</p> <p>2015-08-01</p> <p>We present a uniform, large-<span class="hlt">scale</span> survey of X-ray flare emission, with emphasis on the corrections needed to arrive at estimates of flare occurrence rates. The XMM-Newton Serendipitous Source Catalogue has been used as the basis for a survey of X-ray flares from late-type (i.e. spectral type F-M) stars in the Hipparcos Tycho catalogue. The XMM catalogue and its associated data products provide an excellent basis for a comprehensive and sensitive survey of stellar flares - both from targeted active stars and from those observed serendipitously in the half-degree diameter field-of-view of each observation. Our sample contains ~130 flares with well-observed profiles; they range in duration from ~103 to ~104s, have peak X-ray fluxes from ~10-13 to ~10-11 erg cm-2 s-1, peak X-ray luminosities from ~1029 to ~1032 erg s-1 and X-ray energy output from ~1032 to ~1035 erg. Most of the serendipitously-observed stars have little previously reported information. We present flare <span class="hlt">frequency</span> distributions from both target and serendipitous observations. The latter provide an unbiased (with respect to stellar activity) study of flare energetics. The serendipitous sample demonstrates the need for care when calculating flaring rates, especially when normalising the number of flares to a total exposure time, where it is important to consider both the stars seen to flare and those measured as non-variable, since in our survey, the latter outnumber the former by more than a factor ten. The serendipitous variable and non-variable stars appear very similar in terms of the distributions of general properties such as quiescent X-ray luminosity; from the available data, it is unclear whether the distinction by flaring is due to an additional, intrinsic property such as intra-system interactions in a close binary system, or is simply the result of limited observations of a random flaring process, with no real difference between the two samples. We discuss future observations and analyses</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820063958&hterms=Electromagnetic+Spectrum&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DElectromagnetic%2BSpectrum','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820063958&hterms=Electromagnetic+Spectrum&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DElectromagnetic%2BSpectrum"><span>Two-<span class="hlt">frequency</span> /Delta k/ microwave scatterometer measurements of ocean wave spectra from an aircraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johnson, J. W.; Jones, W. L.; Weissman, D. E.</p> <p>1981-01-01</p> <p>A technique for remotely sensing the large-<span class="hlt">scale</span> gravity wave spectrum on the ocean surface using a two <span class="hlt">frequency</span> (Delta k) microwave scatterometer has been demonstrated from stationary platforms and proposed from moving platforms. This measurement takes advantage of Bragg type resonance matching between the electromagnetic wavelength at the difference <span class="hlt">frequency</span> and the length of the large-<span class="hlt">scale</span> surface waves. A prominent resonance appears in the cross product power spectral density (PSD) of the two backscattered signals. Ku-Band aircraft scatterometer measurements were conducted by NASA in the North Sea during the 1979 Maritime Remote Sensing (MARSEN) experiment. Typical examples of cross product PSD's computed from the MARSEN data are presented. They demonstrate strong resonances whose <span class="hlt">frequency</span> and bandwidth agree with the surface characteristics and the theory. Directional modulation spectra of the surface reflectivity are compared to the gravity wave spectrum derived from surface truth measurements.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ResPh...8.1068A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ResPh...8.1068A"><span>Multiple time <span class="hlt">scale</span> analysis of pressure oscillations in solid rocket motors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahmed, Waqas; Maqsood, Adnan; Riaz, Rizwan</p> <p>2018-03-01</p> <p>In this study, acoustic pressure oscillations for single and coupled longitudinal acoustic modes in Solid Rocket Motor (SRM) are investigated using Multiple Time <span class="hlt">Scales</span> (MTS) method. Two independent time <span class="hlt">scales</span> are introduced. The oscillations occur on fast time <span class="hlt">scale</span> whereas the amplitude and phase changes on slow time <span class="hlt">scale</span>. Hopf bifurcation is employed to investigate the properties of the solution. The supercritical bifurcation phenomenon is observed for linearly unstable system. The amplitude of the oscillations result from equal energy gain and loss rates of longitudinal acoustic modes. The effect of linear instability and <span class="hlt">frequency</span> of longitudinal modes on amplitude and phase of oscillations are determined for both single and coupled modes. For both cases, the maximum amplitude of oscillations decreases with the <span class="hlt">frequency</span> of acoustic mode and linear instability of SRM. The comparison of analytical MTS results and numerical simulations demonstrate an excellent agreement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9970E..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9970E..04S"><span>New prototype of acousto-optical radio-wave spectrometer with parallel <span class="hlt">frequency</span> processing for astrophysical applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shcherbakov, Alexandre S.; Chavez Dagostino, Miguel; Arellanes, Adan O.; Aguirre Lopez, Arturo</p> <p>2016-09-01</p> <p>We develop a multi-band spectrometer with a few spatially parallel optical arms for the combined processing of their data flow. Such multi-band capability has various applications in astrophysical scenarios at different <span class="hlt">scales</span>: from objects in the distant universe to planetary atmospheres in the Solar system. Each optical arm exhibits original performances to provide parallel multi-band observations with different <span class="hlt">scales</span> simultaneously. Similar possibility is based on designing each optical arm individually via exploiting different materials for acousto-optical cells operating within various regimes, <span class="hlt">frequency</span> ranges and light wavelengths from independent light sources. Individual beam shapers provide both the needed incident light polarization and the required apodization to increase the dynamic range of a system. After parallel acousto-optical processing, data flows are united by the joint CCD matrix on the stage of the combined electronic data processing. At the moment, the prototype combines still three bands, i.e. includes three spatial optical arms. The first low-<span class="hlt">frequency</span> arm operates at the central <span class="hlt">frequencies</span> 60-80 MHz with <span class="hlt">frequency</span> bandwidth 40 MHz. The second arm is oriented to middle-<span class="hlt">frequencies</span> 350-500 MHz with <span class="hlt">frequency</span> bandwidth 200-300 MHz. The third arm is intended for ultra-high-<span class="hlt">frequency</span> radio-wave signals about 1.0-1.5 GHz with <span class="hlt">frequency</span> bandwidth <300 MHz. To-day, this spectrometer has the following preliminary performances. The first arm exhibits <span class="hlt">frequency</span> resolution 20 KHz; while the second and third arms give the resolution 150-200 KHz. The numbers of resolvable spots are 1500- 2000 depending on the regime of operation. The fourth optical arm at the <span class="hlt">frequency</span> range 3.5 GHz is currently under construction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ChA%26A..41..430Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ChA%26A..41..430Y"><span>Ensemble Pulsar Time <span class="hlt">Scale</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yin, Dong-shan; Gao, Yu-ping; Zhao, Shu-hong</p> <p>2017-07-01</p> <p>Millisecond pulsars can generate another type of time <span class="hlt">scale</span> that is totally independent of the atomic time <span class="hlt">scale</span>, because the physical mechanisms of the pulsar time <span class="hlt">scale</span> and the atomic time <span class="hlt">scale</span> are quite different from each other. Usually the pulsar timing observations are not evenly sampled, and the internals between two data points range from several hours to more than half a month. Further more, these data sets are sparse. All this makes it difficult to generate an ensemble pulsar time <span class="hlt">scale</span>. Hence, a new algorithm to calculate the ensemble pulsar time <span class="hlt">scale</span> is proposed. Firstly, a cubic spline interpolation is used to densify the data set, and make the intervals between data points uniform. Then, the Vondrak filter is employed to smooth the data set, and get rid of the high-<span class="hlt">frequency</span> noises, and finally the weighted average method is adopted to generate the ensemble pulsar time <span class="hlt">scale</span>. The newly released NANOGRAV (North American Nanohertz Observatory for Gravitational Waves) 9-year data set is used to generate the ensemble pulsar time <span class="hlt">scale</span>. This data set includes the 9-year observational data of 37 millisecond pulsars observed by the 100-meter Green Bank telescope and the 305-meter Arecibo telescope. It is found that the algorithm used in this paper can reduce effectively the influence caused by the noises in pulsar timing residuals, and improve the long-term stability of the ensemble pulsar time <span class="hlt">scale</span>. Results indicate that the long-term (> 1 yr) stability of the ensemble pulsar time <span class="hlt">scale</span> is better than 3.4 × 10-15.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112p3902Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112p3902Z"><span><span class="hlt">Frequency</span> up-converted piezoelectric energy harvester for ultralow-<span class="hlt">frequency</span> and ultrawide-<span class="hlt">frequency</span>-range operation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Xiyang; Gao, Shiqiao; Li, Dongguang; Jin, Lei; Wu, Qinghe; Liu, Feng</p> <p>2018-04-01</p> <p>At present, <span class="hlt">frequency</span> up-converted piezoelectric energy harvesters are disadvantaged by their narrow range of operating <span class="hlt">frequencies</span> and low efficiency at ultralow-<span class="hlt">frequency</span> excitation. To address these shortcomings, we propose herein an impact-driven <span class="hlt">frequency</span> up-converted piezoelectric energy harvester composed of two driving beams and a generating beam. We find experimentally that the proposed device offers efficient energy output over an ultrawide-<span class="hlt">frequency</span>-range and performs very well in the ultralow-<span class="hlt">frequency</span> excitation. A maximum peak power of 29.3 mW is achieved under 0.5g acceleration at the excitation <span class="hlt">frequency</span> of 12.7 Hz. The performance of the energy harvester can be adjusted and optimized by adjusting the spacing between the driving and generating beams. The results show that the proposed harvester has the potential to power miniaturized portable devices and wireless sensor nodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDG39006T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDG39006T"><span>LES-based generation of high-<span class="hlt">frequency</span> fluctuation in wind turbulence obtained by meteorological model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamura, Tetsuro; Kawaguchi, Masaharu; Kawai, Hidenori; Tao, Tao</p> <p>2017-11-01</p> <p>The connection between a meso-<span class="hlt">scale</span> model and a micro-<span class="hlt">scale</span> large eddy simulation (LES) is significant to simulate the micro-<span class="hlt">scale</span> meteorological problem such as strong convective events due to the typhoon or the tornado using LES. In these problems the mean velocity profiles and the mean wind directions change with time according to the movement of the typhoons or tornadoes. Although, a fine grid micro-<span class="hlt">scale</span> LES could not be connected to a coarse grid meso-<span class="hlt">scale</span> WRF directly. In LES when the grid is suddenly refined at the interface of nested grids which is normal to the mean advection the resolved shear stresses decrease due to the interpolation errors and the delay of the generation of smaller <span class="hlt">scale</span> turbulence that can be resolved on the finer mesh. For the estimation of wind gust disaster the peak wind acting on buildings and structures has to be correctly predicted. In the case of meteorological model the velocity fluctuations have a tendency of diffusive variation without the high <span class="hlt">frequency</span> component due to the numerically filtering effects. In order to predict the peak value of wind velocity with good accuracy, this paper proposes a LES-based method for generating the higher <span class="hlt">frequency</span> components of velocity and temperature fields obtained by meteorological model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.717..193K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.717..193K"><span>Interactions of multi-<span class="hlt">scale</span> heterogeneity in the lithosphere: Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kennett, B. L. N.; Yoshizawa, K.; Furumura, T.</p> <p>2017-10-01</p> <p>Understanding the complex heterogeneity of the continental lithosphere involves a wide variety of spatial <span class="hlt">scales</span> and the synthesis of multiple classes of information. Seismic surface waves and multiply reflected body waves provide the main constraints on broad-<span class="hlt">scale</span> structure, and bounds on the extent of the lithosphere-asthenosphere transition (LAT) can be found from the vertical gradients of S wavespeed. Information on finer-<span class="hlt">scale</span> structures comes through body wave studies, including detailed seismic tomography and P-wave reflectivity extracted from stacked autocorrelograms of continuous component records. With the inclusion of deterministic large-<span class="hlt">scale</span> structure and realistic medium-<span class="hlt">scale</span> stochastic features fine-<span class="hlt">scale</span> variations are subdued. The resulting multi-<span class="hlt">scale</span> heterogeneity model for the Australian region gives a good representation of the character of observed seismograms and their geographic variations and matches the observations of P-wave reflectivity. P reflections in the 0.5-3.0 Hz band in the uppermost mantle suggest variations on vertical <span class="hlt">scales</span> of a few hundred metres with amplitudes of the order of 1%. Interference of waves reflected or converted at sequences of such modest variations in physical properties produce relatively simple behaviour for lower <span class="hlt">frequencies</span>, which can suggest simpler structures than are actually present. Vertical changes in the character of fine-<span class="hlt">scale</span> heterogeneity can produce apparent discontinuities. In Central Australia a 'mid-lithospheric discontinuity' can be tracked via changes in <span class="hlt">frequency</span> content of station reflectivity, with links to the broad-<span class="hlt">scale</span> pattern of wavespeed gradients and, in particular, the gradients of radial anisotropy. Comparisons with xenolith results from southeastern Australia indicate a strong tie between geochemical stratification and P-wave reflectivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhyU...59.1091G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhyU...59.1091G"><span>Dynamic properties of ionospheric plasma turbulence driven by high-power high-<span class="hlt">frequency</span> radiowaves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grach, S. M.; Sergeev, E. N.; Mishin, E. V.; Shindin, A. V.</p> <p>2016-11-01</p> <p>A review is given of the current state-of-the-art of experimental studies and the theoretical understanding of nonlinear phenomena that occur in the ionospheric F-layer irradiated by high-power high-<span class="hlt">frequency</span> ground-based transmitters. The main focus is on the dynamic features of high-<span class="hlt">frequency</span> turbulence (plasma waves) and low-<span class="hlt">frequency</span> turbulence (density irregularities of various <span class="hlt">scales</span>) that have been studied in experiments at the Sura and HAARP heating facilities operated in temporal and <span class="hlt">frequency</span> regimes specially designed with consideration of the characteristic properties of nonlinear processes in the perturbed ionosphere using modern radio receivers and optical instruments. Experimental results are compared with theoretical turbulence models for a magnetized collisional plasma in a high-<span class="hlt">frequency</span> electromagnetic field, allowing the identification of the processes responsible for the observed features of artificial ionospheric turbulence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvE..91a2916N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvE..91a2916N"><span><span class="hlt">Frequency</span> adjustment and synchrony in networks of delayed pulse-coupled oscillators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nishimura, Joel</p> <p>2015-01-01</p> <p>We introduce a system of pulse-coupled oscillators that can change both their phases and <span class="hlt">frequencies</span> and prove that when there is a separation of time <span class="hlt">scales</span> between phase and <span class="hlt">frequency</span> adjustment the system converges to exact synchrony on strongly connected graphs with time delays. The analysis involves decomposing the network into a forest of tree-like structures that capture causality. These results provide a robust method of sensor net synchronization as well as demonstrate a new avenue of possible pulse-coupled oscillator research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003PhRvE..67c1903S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003PhRvE..67c1903S"><span>Detecting <span class="hlt">scaling</span> in the period dynamics of multimodal signals: Application to Parkinsonian tremor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sapir, Nir; Karasik, Roman; Havlin, Shlomo; Simon, Ely; Hausdorff, Jeffrey M.</p> <p>2003-03-01</p> <p>Patients with Parkinson’s disease exhibit tremor, involuntary movement of the limbs. The <span class="hlt">frequency</span> spectrum of tremor typically has broad peaks at “harmonic” <span class="hlt">frequencies</span>, much like that seen in other physical processes. In general, this type of harmonic structure in the <span class="hlt">frequency</span> domain may be due to two possible mechanisms: a nonlinear oscillation or a superposition of (multiple) independent modes of oscillation. A broad peak spectrum generally indicates that a signal is semiperiodic with a fluctuating period. These fluctuations may posses intrinsic order that can be quantified using <span class="hlt">scaling</span> analysis. We propose a method to extract the correlation (<span class="hlt">scaling</span>) properties in the period dynamics of multimodal oscillations, in order to distinguish between a nonlinear oscillation and a superposition of individual modes of oscillation. The method is based on our finding that the information content of the temporal correlations in a fluctuating period of a single oscillator is contained in a finite <span class="hlt">frequency</span> band in the power spectrum, allowing for decomposition of modes by bandpass filtering. Our simulations for a nonlinear oscillation show that harmonic modes possess the same <span class="hlt">scaling</span> properties. In contrast, when the method is applied to tremor records from patients with Parkinson’s disease, the first two modes of oscillations yield different <span class="hlt">scaling</span> patterns, suggesting that these modes may not be simple harmonics, as might be initially assumed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22522255-frequency-shifts-resonant-modes-sun-due-near-surface-convective-scattering','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22522255-frequency-shifts-resonant-modes-sun-due-near-surface-convective-scattering"><span><span class="hlt">FREQUENCY</span> SHIFTS OF RESONANT MODES OF THE SUN DUE TO NEAR-SURFACE CONVECTIVE SCATTERING</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>Bhattacharya, J.; Hanasoge, S.; Antia, H. M.</p> <p></p> <p>Measurements of oscillation <span class="hlt">frequencies</span> of the Sun and stars can provide important independent constraints on their internal structure and dynamics. Seismic models of these oscillations are used to connect structure and rotation of the star to its resonant <span class="hlt">frequencies</span>, which are then compared with observations, the goal being that of minimizing the difference between the two. Even in the case of the Sun, for which structure models are highly tuned, observed <span class="hlt">frequencies</span> show systematic deviations from modeled <span class="hlt">frequencies</span>, a phenomenon referred to as the “surface term.” The dominant source of this systematic effect is thought to be vigorous near-surface convection,more » which is not well accounted for in both stellar modeling and mode-oscillation physics. Here we bring to bear the method of homogenization, applicable in the asymptotic limit of large wavelengths (in comparison to the correlation <span class="hlt">scale</span> of convection), to characterize the effect of small-<span class="hlt">scale</span> surface convection on resonant-mode <span class="hlt">frequencies</span> in the Sun. We show that the full oscillation equations, in the presence of temporally stationary three-dimensional (3D) flows, can be reduced to an effective “quiet-Sun” wave equation with altered sound speed, Brünt–Väisäla <span class="hlt">frequency</span>, and Lamb <span class="hlt">frequency</span>. We derive the modified equation and relations for the appropriate averaging of 3D flows and thermal quantities to obtain the properties of this effective medium. Using flows obtained from 3D numerical simulations of near-surface convection, we quantify their effect on solar oscillation <span class="hlt">frequencies</span> and find that they are shifted systematically and substantially. We argue therefore that consistent interpretations of resonant <span class="hlt">frequencies</span> must include modifications to the wave equation that effectively capture the impact of vigorous hydrodynamic convection.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21300935-abelian-higgs-cosmic-strings-small-scale-structure-loops','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21300935-abelian-higgs-cosmic-strings-small-scale-structure-loops"><span>Abelian Higgs cosmic strings: Small-<span class="hlt">scale</span> structure and loops</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>Hindmarsh, Mark; Stuckey, Stephanie; Bevis, Neil</p> <p>2009-06-15</p> <p>Classical lattice simulations of the Abelian Higgs model are used to investigate small-<span class="hlt">scale</span> structure and loop distributions in cosmic string networks. Use of the field theory ensures that the small-<span class="hlt">scale</span> physics is captured correctly. The results confirm analytic predictions of Polchinski and Rocha 29 for the two-point correlation function of the string tangent vector, with a power law from length <span class="hlt">scales</span> of order the string core width up to horizon <span class="hlt">scale</span>. An analysis of the size distribution of string loops gives a very low number density, of order 1 per horizon volume, in contrast with Nambu-Goto simulations. Further, our loopmore » distribution function does not support the detailed analytic predictions for loop production derived by Dubath et al. 30. Better agreement to our data is found with a model based on loop fragmentation 32, coupled with a constant rate of energy loss into massive radiation. Our results show a strong energy-loss mechanism, which allows the string network to <span class="hlt">scale</span> without gravitational radiation, but which is not due to the production of string width loops. From evidence of small-<span class="hlt">scale</span> structure we argue a partial explanation for the <span class="hlt">scale</span> separation problem of how energy in the very low <span class="hlt">frequency</span> modes of the string network is transformed into the very high <span class="hlt">frequency</span> modes of gauge and Higgs radiation. We propose a picture of string network evolution, which reconciles the apparent differences between Nambu-Goto and field theory simulations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940011555','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940011555"><span>Similarity and <span class="hlt">scale</span> in catchment storm response</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wood, Eric F.; Sivapalan, Murugesu; Beven, Keith</p> <p>1993-01-01</p> <p>Until recently, very little progress had been made in understanding the relationship between small-<span class="hlt">scale</span> variability of topography, soil, and rainfalls and the storm response seen at the catchment <span class="hlt">scale</span>. The work reviewed here represents the first attempt at a systematic theoretical framework for such understanding in the context of surface runoff generation by different processes. The parameterization of hydrological processes over a range of <span class="hlt">scales</span> is examined, and the concept of the 'representative elementary area' (REA) is introduced. The REA is a fundamental <span class="hlt">scale</span> for catchment modeling at which continuum assumptions can be applied for the spatially variable controls and parameters, and spatial patterns no longer have to be considered explicitly. The investigation of <span class="hlt">scale</span> leads into the concept of hydrologic similarity in which the effects of the environmental controls on runoff generation and flood <span class="hlt">frequency</span> response be investigated independently of catchment <span class="hlt">scale</span>. The paper reviews the authors' initial results and hopefully will motivate others to also investigate the issues of hydrologic <span class="hlt">scale</span> and similarity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRD..118.3259L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRD..118.3259L"><span>Linking snowflake microstructure to multi-<span class="hlt">frequency</span> radar observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leinonen, J.; Moisseev, D.; Nousiainen, T.</p> <p>2013-04-01</p> <p>Spherical or spheroidal particle shape models are commonly used to calculate numerically the radar backscattering properties of aggregate snowflakes. A more complicated and computationally intensive approach is to use detailed models of snowflake structure together with numerical scattering models that can operate on arbitrary particle shapes. Recent studies have shown that there can be significant differences between the results of these approaches. In this paper, an analytical model, based on the Rayleigh-Gans scattering theory, is formulated to explain this discrepancy in terms of the effect of discrete ice crystals that constitute the snowflake. The ice crystals cause small-<span class="hlt">scale</span> inhomogeneities whose effects can be understood through the density autocorrelation function of the particle mass, which the Rayleigh-Gans theory connects to the function that gives the radar reflectivity as a function of <span class="hlt">frequency</span>. The derived model is a weighted sum of two Gaussian functions. A term that corresponds to the average shape of the particle, similar to that given by the spheroidal shape model, dominates at low <span class="hlt">frequencies</span>. At high <span class="hlt">frequencies</span>, that term vanishes and is gradually replaced by the effect of the ice crystal monomers. The autocorrelation-based description of snowflake microstructure appears to be sufficient for multi-<span class="hlt">frequency</span> radar studies. The link between multi-<span class="hlt">frequency</span> radar observations and the particle microstructure can thus be used to infer particle properties from the observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3861400','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3861400"><span>Large-<span class="hlt">scale</span> cortical correlation structure of spontaneous oscillatory activity</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hipp, Joerg F.; Hawellek, David J.; Corbetta, Maurizio; Siegel, Markus; Engel, Andreas K.</p> <p>2013-01-01</p> <p>Little is known about the brain-wide correlation of electrophysiological signals. Here we show that spontaneous oscillatory neuronal activity exhibits <span class="hlt">frequency</span>-specific spatial correlation structure in the human brain. We developed an analysis approach that discounts spurious correlation of signal power caused by the limited spatial resolution of electrophysiological measures. We applied this approach to source estimates of spontaneous neuronal activity reconstructed from magnetoencephalography (MEG). Overall, correlation of power across cortical regions was strongest in the alpha to beta <span class="hlt">frequency</span> range (8–32 Hz) and correlation patterns depended on the underlying oscillation <span class="hlt">frequency</span>. Global hubs resided in the medial temporal lobe in the theta <span class="hlt">frequency</span> range (4–6 Hz), in lateral parietal areas in the alpha to beta <span class="hlt">frequency</span> range (8–23 Hz), and in sensorimotor areas for higher <span class="hlt">frequencies</span> (32–45 Hz). Our data suggest that interactions in various large-<span class="hlt">scale</span> cortical networks may be reflected in <span class="hlt">frequency</span> specific power-envelope correlations. PMID:22561454</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27822664','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27822664"><span>Assessment of Motivational Cognitions in Diabetes Self-Care: the Motivation Thought <span class="hlt">Frequency</span> <span class="hlt">Scales</span> for Glucose Testing, Physical Activity and Healthy Eating.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Parham, Sophie C; Kavanagh, David J; Gericke, Christian A; King, Neil; May, Jon; Andrade, Jackie</p> <p>2017-06-01</p> <p>There is a need for improved measurement of motivation for diabetes self-care. The Elaborated Intrusion Theory of Desire offers a coherent framework for understanding and identifying the cognitive-affective events that constitute the subjective experience of motivation and may therefore inform the development of such an instrument. Recent research has shown the resultant Motivation Thought <span class="hlt">Frequency</span> <span class="hlt">scale</span> (MTF) to have a stable factor structure (Intensity, Incentives Imagery, Self-Efficacy Imagery, Availability) when applied to physical activity, excessive snacking or alcohol use in the general population. The current study aimed to confirm the four-factor structure of the MTF for glucose testing, physical activity and healthy eating in people with type 2 diabetes. Associations with self-reports of concurrent diabetic self-care behaviours were also examined. Confirmatory factor analyses tested the internal structure, and multiple regressions assessed the <span class="hlt">scale</span>'s relationship with concurrent self-care behaviours. The MTF was completed by 340 adults with type 2 diabetes, and 237 from that sample also reported self-care behaviours. Separate MTFs assessed motivation for glucose testing, physical activity and healthy eating. Self-care was assessed using questions from the Summary of Diabetes Self-Care Activities. The MTF for each goal achieved an acceptable fit on all indices after selected errors within factors were allowed to intercorrelate. Intensity and Self-Efficacy Imagery provided the strongest and most consistent correlations with relevant self-care behaviours. Results provide preliminary support for the MTF in a diabetes sample. Testing of its sensitivity to change and its predictive utility over time is needed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=6016299','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=6016299"><span>Efficacy of dietary supplement with nutraceutical composed combined with extremely-low-<span class="hlt">frequency</span> electromagnetic fields in carpal tunnel syndrome</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Paolucci, Teresa; Piccinini, Giulia; Nusca, Sveva Maria; Marsilli, Gabriella; Mannocci, Alice; La Torre, Giuseppe; Saraceni, Vincenzo Maria; Vulpiani, Maria Chiara; Villani, Ciro</p> <p>2018-01-01</p> <p>[Purpose] The aim of this study was to investigate the clinical effects of a nutraceutical composed (Xinepa®) combined with extremely-low-<span class="hlt">frequency</span> electromagnetic fields in the carpal tunnel syndrome. [Subjects and Methods] Thirty-one patients with carpal tunnel syndrome were randomized into group 1-A (N=16) (nutraceutical + extremely-low-<span class="hlt">frequency</span> electromagnetic fields) and group 2-C (n=15) (placebo + extremely-low-<span class="hlt">frequency</span> electromagnetic fields). The dietary supplement with nutraceutical was twice daily for one month in the 1-A group and both groups received extremely-low-<span class="hlt">frequency</span> electromagnetic fields at the level of the carpal tunnel 3 times per week for 12 sessions. The Visual Analogue <span class="hlt">Scale</span> for pain, the Symptoms Severity <span class="hlt">Scale</span> and Functional Severity <span class="hlt">Scale</span> of the Boston Carpal Tunnel Questionnaire were used at pre-treatment (T0), after the end of treatment (T1) and at 3 months post-treatment (T2). [Results] At T1 and T2 were not significant differences in outcome measures between the two groups. In group 1-A a significant improvement in the <span class="hlt">scales</span> were observed at T1 and T2. In group 2-C it was observed only at T1. [Conclusion] Significant clinical effects from pre-treatment to the end of treatment were shown in both groups. Only in group 1-A they were maintained at 3 months post-treatment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009IEITF..92..681L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009IEITF..92..681L"><span>Neural Network Compensation for <span class="hlt">Frequency</span> Cross-Talk in Laser Interferometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Wooram; Heo, Gunhaeng; You, Kwanho</p> <p></p> <p>The heterodyne laser interferometer acts as an ultra-precise measurement apparatus in semiconductor manufacture. However the periodical nonlinearity property caused from <span class="hlt">frequency</span> cross-talk is an obstacle to improve the high measurement accuracy in nanometer <span class="hlt">scale</span>. In order to minimize the nonlinearity error of the heterodyne interferometer, we propose a <span class="hlt">frequency</span> cross-talk compensation algorithm using an artificial intelligence method. The feedforward neural network trained by back-propagation compensates the nonlinearity error and regulates to minimize the difference with the reference signal. With some experimental results, the improved accuracy is proved through comparison with the position value from a capacitive displacement sensor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H11G1276R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H11G1276R"><span><span class="hlt">Frequency</span> Dependent Macro-dispersion Induced by Oscillatory Inputs and Spatial Heterogeneity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rajabi, F.; Battiato, I.</p> <p>2017-12-01</p> <p>Elucidating flow and transport processes at the pore <span class="hlt">scale</span> is the cornerstone of most hydrologic studies in the subsurface. This becomes even more imperative when the system is subject to a cyclic forcing. Such temporal variations with evolving heterogeneity of time <span class="hlt">scales</span> spanning from days to years can influence transport phenomena at the pore level, e.g. yearly freeze/thaw in the thin active layer of soil above permafrost zone whose thickness increases throughout the thaw season. Moreover, understanding the interactions of different physical phenomena at the pore <span class="hlt">scale</span> is key to predict the behavior at the continuum <span class="hlt">scale</span>. Yet, the connection between periodic inputs at the pore <span class="hlt">scale</span> and macrotransport is to a great extent unknown. In the spirit of homogenization technique, we derived a macrotime continuum-<span class="hlt">scale</span> equation as well as expressions for the effective transport coefficients. The macrodispersion arises from contributions of molecular diffusion, spatial heterogeneity and time-dependent fluctuations. Moreover, we have quantified the solute spreading by effective dispersion in terms of dimensionless numbers (Pe, Da, and Strouhal), i.e. expressing the interplay of molecular diffusion, advection, reaction and signal <span class="hlt">frequency</span>. Yet, as every macroscopic model, spatiotemporally averaged models can breakdown when certain criteria are violated. This makes the continuum <span class="hlt">scale</span> equation a poor approximation for the processes at the pore <span class="hlt">scale</span>. To this end, we also provide the conditions under which the space-time averaged equations accurately describe pore-<span class="hlt">scale</span> processes. In addition, this study gives a robust evidence that transverse mixing can in fact benefit from fluctuating boundary forcing due to the interaction of temporal fluctuations and molecular diffusion. Furthermore, it provides a robust quantitative foundation for designing the desired systems since the interplay of geometry and external forcing has been directly connected to each other in terms of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830027084','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830027084"><span>Influence of modulation <span class="hlt">frequency</span> in rubidium cell <span class="hlt">frequency</span> standards</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Audoin, C.; Viennet, J.; Cyr, N.; Vanier, J.</p> <p>1983-01-01</p> <p>The error signal which is used to control the <span class="hlt">frequency</span> of the quartz crystal oscillator of a passive rubidium cell <span class="hlt">frequency</span> standard is considered. The value of the slope of this signal, for an interrogation <span class="hlt">frequency</span> close to the atomic transition <span class="hlt">frequency</span> is calculated and measured for various phase (or <span class="hlt">frequency</span>) modulation waveforms, and for several values of the modulation <span class="hlt">frequency</span>. A theoretical analysis is made using a model which applies to a system in which the optical pumping rate, the relaxation rates and the RF field are homogeneous. Results are given for sine-wave phase modulation, square-wave <span class="hlt">frequency</span> modulation and square-wave phase modulation. The influence of the modulation <span class="hlt">frequency</span> on the slope of the error signal is specified. It is shown that the modulation <span class="hlt">frequency</span> can be chosen as large as twice the non-saturated full-width at half-maximum without a drastic loss of the sensitivity to an offset of the interrogation <span class="hlt">frequency</span> from center line, provided that the power saturation factor and the amplitude of modulation are properly adjusted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5075946','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5075946"><span><span class="hlt">Scale</span>-Free Neural and Physiological Dynamics in Naturalistic Stimuli Processing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lin, Amy</p> <p>2016-01-01</p> <p>Abstract Neural activity recorded at multiple spatiotemporal <span class="hlt">scales</span> is dominated by arrhythmic fluctuations without a characteristic temporal periodicity. Such activity often exhibits a 1/f-type power spectrum, in which power falls off with increasing <span class="hlt">frequency</span> following a power-law function: P(f)∝1/fβ, which is indicative of <span class="hlt">scale</span>-free dynamics. Two extensively studied forms of <span class="hlt">scale</span>-free neural dynamics in the human brain are slow cortical potentials (SCPs)—the low-<span class="hlt">frequency</span> (<5 Hz) component of brain field potentials—and the amplitude fluctuations of α oscillations, both of which have been shown to carry important functional roles. In addition, <span class="hlt">scale</span>-free dynamics characterize normal human physiology such as heartbeat dynamics. However, the exact relationships among these <span class="hlt">scale</span>-free neural and physiological dynamics remain unclear. We recorded simultaneous magnetoencephalography and electrocardiography in healthy subjects in the resting state and while performing a discrimination task on <span class="hlt">scale</span>-free dynamical auditory stimuli that followed different <span class="hlt">scale</span>-free statistics. We observed that long-range temporal correlation (captured by the power-law exponent β) in SCPs positively correlated with that of heartbeat dynamics across time within an individual and negatively correlated with that of α-amplitude fluctuations across individuals. In addition, across individuals, long-range temporal correlation of both SCP and α-oscillation amplitude predicted subjects’ discrimination performance in the auditory task, albeit through antagonistic relationships. These findings reveal interrelations among different <span class="hlt">scale</span>-free neural and physiological dynamics and initial evidence for the involvement of <span class="hlt">scale</span>-free neural dynamics in the processing of natural stimuli, which often exhibit <span class="hlt">scale</span>-free dynamics. PMID:27822495</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/2013PhDT.......361B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......361B"><span>Whispering gallery mode resonators for <span class="hlt">frequency</span> metrology applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baumgartel, Lukas</p> <p></p> <p>This dissertation describes an investigation into the use of whispering gallery mode (WGM) resonators for applications towards <span class="hlt">frequency</span> reference and metrology. Laser stabilization and the measurement of optical <span class="hlt">frequencies</span> have enabled myriad technologies of both academic and commercial interest. A technology which seems to span both motivations is optical atomic clocks. These devices are virtually unimaginable without the ultra stable lasers plus <span class="hlt">frequency</span> measurement and down-conversion afforded by Fabry Perot (FP) cavities and model-locked laser combs, respectively. However, WGM resonators can potentially perform both of these tasks while having the distinct advantages of compactness and simplicity. This work represents progress towards understanding and mitigating the performance limitations of WGM cavities for such applications. A system for laser <span class="hlt">frequency</span> stabilization to a the cavity via the Pound-Drever-Hall (PDH) method is described. While the laser lock itself is found to perform at the level of several parts in 1015, a variety of fundamental and technical mechanisms destabilize the WGM <span class="hlt">frequency</span> itself. Owing to the relatively large thermal expansion coefficients in optical crystals, environmental temperature drifts set the stability limit at time <span class="hlt">scales</span> greater than the thermal relaxation time of the crystal. Uncompensated, these drifts pull WGM <span class="hlt">frequencies</span> about 3 orders of magnitude more than they would in an FP cavity. Thus, two temperature compensation schemes are developed. An active scheme measures and stabilizes the mode volume temperature to the level of several nK, reducing the effective temperature coefficient of the resonator to 1.7x10-7 K-1; simulations suggest that the value could eventually be as low as 3.5x10-8 K-1, on par with the aforementioned FP cavities. A second, passive scheme is also described, which employs a heterogeneous resonator structure that capitalizes on the thermo-mechanical properties of one material and the optical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4085202','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4085202"><span>Effects of Low-<span class="hlt">frequency</span> Current Sacral Dermatome Stimulation on Idiopathic Slow Transit Constipation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kim, Jin-Seop; Yi, Seung-Ju</p> <p>2014-01-01</p> <p>[Purpose] This study aimed to determine whether low-<span class="hlt">frequency</span> current therapy can be used to reduce the symptoms of idiopathic slow transit constipation (ISTC). [Subjects] Fifteen patients (ten male and five female) with idiopathic slow transit constipation were enrolled in the present study. [Results] Bowel movements per day, bowel movements per week, and constipation assessment <span class="hlt">scale</span> scores significantly improved after low-<span class="hlt">frequency</span> current simulation of S2-S3. [Conclusion] Our results show that stimulation with low-<span class="hlt">frequency</span> current of the sacral dermatomes may offer therapeutic benefits for a subject of patients with ISTC. PMID:25013277</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014WRR....50.7590M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014WRR....50.7590M"><span>Estimating porosity and solid dielectric permittivity in the Miami Limestone using high-<span class="hlt">frequency</span> ground penetrating radar (GPR) measurements at the laboratory <span class="hlt">scale</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mount, Gregory J.; Comas, Xavier</p> <p>2014-10-01</p> <p>Subsurface water flow in South Florida is largely controlled by the heterogeneous nature of the karst limestone in the Biscayne aquifer and its upper formation, the Miami Limestone. These heterogeneities are amplified by dissolution structures that induce changes in the aquifer's material and physical properties (i.e., porosity and dielectric permittivity) and create preferential flow paths. Understanding such patterns are critical for the development of realistic groundwater flow models, particularly in the Everglades, where restoration of hydrological conditions is intended. In this work, we used noninvasive ground penetrating radar (GPR) to estimate the spatial variability in porosity and the dielectric permittivity of the solid phase of the limestone at centimeter-<span class="hlt">scale</span> resolution to evaluate the potential for field-based GPR studies. A laboratory setup that included high-<span class="hlt">frequency</span> GPR measurements under completely unsaturated and saturated conditions was used to estimate changes in electromagnetic wave velocity through Miami Limestone samples. The Complex Refractive Index Model was used to derive estimates of porosity and dielectric permittivity of the solid phase of the limestone. Porosity estimates of the samples ranged between 45.2 and 66.0% and showed good correspondence with estimates of porosity using analytical and digital image techniques. Solid dielectric permittivity values ranged between 7.0 and 13.0. This study shows the ability of GPR to image the spatial variability of porosity and dielectric permittivity in the Miami Limestone and shows potential for expanding these results to larger <span class="hlt">scales</span> and other karst aquifers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21331462','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21331462"><span><span class="hlt">Scaling</span> analysis of bilateral hand tremor movements in essential tremor patients.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Blesic, S; Maric, J; Dragasevic, N; Milanovic, S; Kostic, V; Ljubisavljevic, Milos</p> <p>2011-08-01</p> <p>Recent evidence suggests that the dynamic-<span class="hlt">scaling</span> behavior of the time-series of signals extracted from separate peaks of tremor spectra may reveal existence of multiple independent sources of tremor. Here, we have studied dynamic characteristics of the time-series of hand tremor movements in essential tremor (ET) patients using the detrended fluctuation analysis method. Hand accelerometry was recorded with (500 g) and without weight loading under postural conditions in 25 ET patients and 20 normal subjects. The time-series comprising peak-to-peak (PtP) intervals were extracted from regions around the first three main <span class="hlt">frequency</span> components of power spectra (PwS) of the recorded tremors. The data were compared between the load and no-load condition on dominant (related to tremor severity) and non-dominant tremor side and with the normal (physiological) oscillations in healthy subjects. Our analysis shows that, in ET, the dynamic characteristics of the main <span class="hlt">frequency</span> component of recorded tremors exhibit <span class="hlt">scaling</span> behavior. Furthermore, they show that the two main components of ET tremor <span class="hlt">frequency</span> spectra, otherwise indistinguishable without load, become significantly different after inertial loading and that they differ between the tremor sides (related to tremor severity). These results show that <span class="hlt">scaling</span>, a time-domain analysis, helps revealing tremor features previously not revealed by <span class="hlt">frequency</span>-domain analysis and suggest that distinct oscillatory central circuits may generate the tremor in ET patients.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940026163','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940026163"><span>An algorithm for the Italian atomic time <span class="hlt">scale</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cordara, F.; Vizio, G.; Tavella, P.; Pettiti, V.</p> <p>1994-01-01</p> <p>During the past twenty years, the time <span class="hlt">scale</span> at the IEN has been realized by a commercial cesium clock, selected from an ensemble of five, whose rate has been continuously steered towards UTC to maintain a long term agreement within 3 x 10(exp -13). A time <span class="hlt">scale</span> algorithm, suitable for a small clock ensemble and capable of improving the medium and long term stability of the IEN time <span class="hlt">scale</span>, has been recently designed taking care of reducing the effects of the seasonal variations and the sudden <span class="hlt">frequency</span> anomalies of the single cesium clocks. The new time <span class="hlt">scale</span>, TA(IEN), is obtained as a weighted average of the clock ensemble computed once a day from the time comparisons between the local reference UTC(IEN) and the single clocks. It is foreseen to include in the computation also ten cesium clocks maintained in other Italian laboratories to further improve its reliability and its long term stability. To implement this algorithm, a personal computer program in Quick Basic has been prepared and it has been tested at the IEN time and <span class="hlt">frequency</span> laboratory. Results obtained using this algorithm on the real clocks data relative to a period of about two years are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16822148','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16822148"><span>The low-<span class="hlt">frequency</span> encoding disadvantage: Word <span class="hlt">frequency</span> affects processing demands.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Diana, Rachel A; Reder, Lynne M</p> <p>2006-07-01</p> <p>Low-<span class="hlt">frequency</span> words produce more hits and fewer false alarms than high-<span class="hlt">frequency</span> words in a recognition task. The low-<span class="hlt">frequency</span> hit rate advantage has sometimes been attributed to processes that operate during the recognition test (e.g., L. M. Reder et al., 2000). When tasks other than recognition, such as recall, cued recall, or associative recognition, are used, the effects seem to contradict a low-<span class="hlt">frequency</span> advantage in memory. Four experiments are presented to support the claim that in addition to the advantage of low-<span class="hlt">frequency</span> words at retrieval, there is a low-<span class="hlt">frequency</span> disadvantage during encoding. That is, low-<span class="hlt">frequency</span> words require more processing resources to be encoded episodically than high-<span class="hlt">frequency</span> words. Under encoding conditions in which processing resources are limited, low-<span class="hlt">frequency</span> words show a larger decrement in recognition than high-<span class="hlt">frequency</span> words. Also, studying items (pictures and words of varying <span class="hlt">frequencies</span>) along with low-<span class="hlt">frequency</span> words reduces performance for those stimuli. Copyright 2006 APA, all rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3440596','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3440596"><span>Telerobotic-assisted bone-drilling system using bilateral control with feed operation <span class="hlt">scaling</span> and cutting force <span class="hlt">scaling</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>Kasahara, Yusuke; Kawana, Hiromasa; Usuda, Shin; Ohnishi, Kouhei</p> <p>2012-01-01</p> <p>Background Drilling is used in the medical field, especially in oral surgery and orthopaedics. In recent years, oral surgery involving dental implants has become more common. However, the risky drilling process causes serious accidents. To prevent these accidents, supporting systems such as robotic drilling systems are required. Methods A telerobotic-assisted drilling system is proposed. An acceleration-based four-channel bilateral control system is implemented in linear actuators in a master–slave system for drill feeding. A reaction force observer is used instead of a force sensor for measuring cutting force. Cutting force transmits from a cutting material to a surgeon, who may feel a static cutting resistance force and vigorous cutting vibrations, via the master–slave system. Moreover, position <span class="hlt">scaling</span> and force <span class="hlt">scaling</span> are achieved. <span class="hlt">Scaling</span> functions are used to achieve precise drilling and hazard detection via force sensation. Results Cutting accuracy and reproducibility of the cutting force were evaluated by angular velocity/position error and <span class="hlt">frequency</span> analysis of the cutting force, respectively, and errors were > 2.0 rpm and > 0.2 mm, respectively. Spectrum peaks of the cutting vibration were at the theoretical vibration <span class="hlt">frequencies</span> of 30, 60 and 90 Hz. Conclusions The proposed telerobotic-assisted drilling system achieved precise manipulation of the drill feed and vivid feedback from the cutting force. Copyright © 2012 John Wiley & Sons, Ltd. PMID:22271710</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5794059','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5794059"><span>A novel optogenetically tunable <span class="hlt">frequency</span> modulating oscillator</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2018-01-01</p> <p>Synthetic biology has enabled the creation of biological reconfigurable circuits, which perform multiple functions monopolizing a single biological machine; Such a system can switch between different behaviours in response to environmental cues. Previous work has demonstrated switchable dynamical behaviour employing reconfigurable logic gate genetic networks. Here we describe a computational framework for reconfigurable circuits in E.coli using combinations of logic gates, and also propose the biological implementation. The proposed system is an oscillator that can exhibit tunability of <span class="hlt">frequency</span> and amplitude of oscillations. Further, the <span class="hlt">frequency</span> of operation can be changed optogenetically. Insilico analysis revealed that two-component light systems, in response to light within a <span class="hlt">frequency</span> range, can be used for modulating the <span class="hlt">frequency</span> of the oscillator or stopping the oscillations altogether. Computational modelling reveals that mixing two colonies of E.coli oscillating at different <span class="hlt">frequencies</span> generates spatial beat patterns. Further, we show that these oscillations more robustly respond to input perturbations compared to the base oscillator, to which the proposed oscillator is a modification. Compared to the base oscillator, the proposed system shows faster synchronization in a colony of cells for a larger region of the parameter space. Additionally, the proposed oscillator also exhibits lesser synchronization error in the transient period after input perturbations. This provides a strong basis for the construction of synthetic reconfigurable circuits in bacteria and other organisms, which can be <span class="hlt">scaled</span> up to perform functions in the field of time dependent drug delivery with tunable dosages, and sets the stage for further development of circuits with synchronized population level behaviour. PMID:29389936</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29389936','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29389936"><span>A novel optogenetically tunable <span class="hlt">frequency</span> modulating oscillator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mahajan, Tarun; Rai, Kshitij</p> <p>2018-01-01</p> <p>Synthetic biology has enabled the creation of biological reconfigurable circuits, which perform multiple functions monopolizing a single biological machine; Such a system can switch between different behaviours in response to environmental cues. Previous work has demonstrated switchable dynamical behaviour employing reconfigurable logic gate genetic networks. Here we describe a computational framework for reconfigurable circuits in E.coli using combinations of logic gates, and also propose the biological implementation. The proposed system is an oscillator that can exhibit tunability of <span class="hlt">frequency</span> and amplitude of oscillations. Further, the <span class="hlt">frequency</span> of operation can be changed optogenetically. Insilico analysis revealed that two-component light systems, in response to light within a <span class="hlt">frequency</span> range, can be used for modulating the <span class="hlt">frequency</span> of the oscillator or stopping the oscillations altogether. Computational modelling reveals that mixing two colonies of E.coli oscillating at different <span class="hlt">frequencies</span> generates spatial beat patterns. Further, we show that these oscillations more robustly respond to input perturbations compared to the base oscillator, to which the proposed oscillator is a modification. Compared to the base oscillator, the proposed system shows faster synchronization in a colony of cells for a larger region of the parameter space. Additionally, the proposed oscillator also exhibits lesser synchronization error in the transient period after input perturbations. This provides a strong basis for the construction of synthetic reconfigurable circuits in bacteria and other organisms, which can be <span class="hlt">scaled</span> up to perform functions in the field of time dependent drug delivery with tunable dosages, and sets the stage for further development of circuits with synchronized population level behaviour.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032036','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032036"><span>Map <span class="hlt">scale</span> effects on estimating the number of undiscovered mineral 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>Singer, D.A.; Menzie, W.D.</p> <p>2008-01-01</p> <p>Estimates of numbers of undiscovered mineral deposits, fundamental to assessing mineral resources, are affected by map <span class="hlt">scale</span>. Where consistently defined deposits of a particular type are estimated, spatial and <span class="hlt">frequency</span> distributions of deposits are linked in that some <span class="hlt">frequency</span> distributions can be generated by processes randomly in space whereas others are generated by processes suggesting clustering in space. Possible spatial distributions of mineral deposits and their related <span class="hlt">frequency</span> distributions are affected by map <span class="hlt">scale</span> and associated inclusions of non-permissive or covered geological settings. More generalized map <span class="hlt">scales</span> are more likely to cause inclusion of geologic settings that are not really permissive for the deposit type, or that include unreported cover over permissive areas, resulting in the appearance of deposit clustering. Thus, overly generalized map <span class="hlt">scales</span> can cause deposits to appear clustered. We propose a model that captures the effects of map <span class="hlt">scale</span> and the related inclusion of non-permissive geologic settings on numbers of deposits estimates, the zero-inflated Poisson distribution. Effects of map <span class="hlt">scale</span> as represented by the zero-inflated Poisson distribution suggest that the appearance of deposit clustering should diminish as mapping becomes more detailed because the number of inflated zeros would decrease with more detailed maps. Based on observed worldwide relationships between map <span class="hlt">scale</span> and areas permissive for deposit types, mapping at a <span class="hlt">scale</span> with twice the detail should cut permissive area size of a porphyry copper tract to 29% and a volcanic-hosted massive sulfide tract to 50% of their original sizes. Thus some direct benefits of mapping an area at a more detailed <span class="hlt">scale</span> are indicated by significant reductions in areas permissive for deposit types, increased deposit density and, as a consequence, reduced uncertainty in the estimate of number of undiscovered deposits. Exploration enterprises benefit from reduced areas requiring</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28062901','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28062901"><span>Changes in Soil Fungal Community Structure with Increasing Disturbance <span class="hlt">Frequency</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cho, Hyunjun; Kim, Mincheol; Tripathi, Binu; Adams, Jonathan</p> <p>2017-07-01</p> <p>Although disturbance is thought to be important in many ecological processes, responses of fungal communities to soil disturbance have been little studied experimentally. We subjected a soil microcosm to physical disturbance, at a range of <span class="hlt">frequencies</span> designed to simulate ecological disturbance events. We analyzed the fungal community structure using Illumina HiSeq sequencing of the ITS1 region. Fungal diversity was found to decline with the increasing disturbance <span class="hlt">frequencies</span>, with no sign of the "humpback" pattern found in many studies of larger sedentary organisms. There is thus no evidence of an effect of release from competition resulting from moderate disturbance-which suggests that competition and niche overlap may not be important in limiting soil fungal diversity. Changing disturbance <span class="hlt">frequency</span> also led to consistent differences in community composition. There were clear differences in OTU-level composition, with different disturbance treatments each having distinct fungal communities. The functional profile of fungal groups (guilds) was changed by the level of disturbance <span class="hlt">frequency</span>. These predictable differences in community composition suggest that soil fungi can possess different niches in relation to disturbance <span class="hlt">frequency</span>, or time since last disturbance. Fungi appear to be most abundant relative to bacteria at intermediate disturbance <span class="hlt">frequencies</span>, on the time <span class="hlt">scale</span> we studied here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.4309K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4309K"><span>A Development of Nonstationary Regional <span class="hlt">Frequency</span> Analysis Model with Large-<span class="hlt">scale</span> Climate Information: Its Application to Korean Watershed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Jin-Young; Kwon, Hyun-Han; Kim, Hung-Soo</p> <p>2015-04-01</p> <p>The existing regional <span class="hlt">frequency</span> analysis has disadvantages in that it is difficult to consider geographical characteristics in estimating areal rainfall. In this regard, this study aims to develop a hierarchical Bayesian model based nonstationary regional <span class="hlt">frequency</span> analysis in that spatial patterns of the design rainfall with geographical information (e.g. latitude, longitude and altitude) are explicitly incorporated. This study assumes that the parameters of Gumbel (or GEV distribution) are a function of geographical characteristics within a general linear regression framework. Posterior distribution of the regression parameters are estimated by Bayesian Markov Chain Monte Carlo (MCMC) method, and the identified functional relationship is used to spatially interpolate the parameters of the distributions by using digital elevation models (DEM) as inputs. The proposed model is applied to derive design rainfalls over the entire Han-river watershed. It was found that the proposed Bayesian regional <span class="hlt">frequency</span> analysis model showed similar results compared to L-moment based regional <span class="hlt">frequency</span> analysis. In addition, the model showed an advantage in terms of quantifying uncertainty of the design rainfall and estimating the area rainfall considering geographical information. Finally, comprehensive discussion on design rainfall in the context of nonstationary will be presented. KEYWORDS: Regional <span class="hlt">frequency</span> analysis, Nonstationary, Spatial information, Bayesian Acknowledgement This research was supported by a grant (14AWMP-B082564-01) from Advanced Water Management Research Program funded by Ministry of Land, Infrastructure and Transport of Korean government.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70140708','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70140708"><span>Characterizing riverbed sediment using high-<span class="hlt">frequency</span> acoustics 1: spectral properties of scattering</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Buscombe, Daniel D.; Grams, Paul E.; Kaplinski, Matt A.</p> <p>2014-01-01</p> <p>Bed-sediment classification using high-<span class="hlt">frequency</span> hydro-acoustic instruments is challenging when sediments are spatially heterogeneous, which is often the case in rivers. The use of acoustic backscatter to classify sediments is an attractive alternative to analysis of topography because it is potentially sensitive to grain-<span class="hlt">scale</span> roughness. Here, a new method is presented which uses high-<span class="hlt">frequency</span> acoustic backscatter from multibeam sonar to classify heterogeneous riverbed sediments by type (sand, gravel,rock) continuously in space and at small spatial resolution. In this, the first of a pair of papers that examine the scattering signatures from a heterogeneous riverbed, methods are presented to construct spatially explicit maps of spectral properties from geo-referenced point clouds of geometrically and radiometrically corrected echoes. Backscatter power spectra are computed to produce <span class="hlt">scale</span> and amplitude metrics that collectively characterize the length <span class="hlt">scales</span> of stochastic measures of riverbed scattering, termed ‘stochastic geometries’. Backscatter aggregated over small spatial <span class="hlt">scales</span> have spectra that obey a power-law. This apparently self-affine behavior could instead arise from morphological- and grain-<span class="hlt">scale</span> roughnesses over multiple overlapping <span class="hlt">scales</span>, or riverbed scattering being transitional between Rayleigh and geometric regimes. Relationships exist between stochastic geometries of backscatter and areas of rough and smooth sediments. However, no one parameter can uniquely characterize a particular substrate, nor definitively separate the relative contributions of roughness and acoustic impedance (hardness). Combinations of spectral quantities do, however, have the potential to delineate riverbed sediment patchiness, in a data-driven approach comparing backscatter with bed-sediment observations (which is the subject of part two of this manuscript).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24465918','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24465918"><span>Liquidity spillover in international stock markets through distinct time <span class="hlt">scales</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Righi, Marcelo Brutti; Vieira, Kelmara Mendes</p> <p>2014-01-01</p> <p>This paper identifies liquidity spillovers through different time <span class="hlt">scales</span> based on a wavelet multiscaling method. We decompose daily data from U.S., British, Brazilian and Hong Kong stock markets indices in order to calculate the <span class="hlt">scale</span> correlation between their illiquidities. The sample is divided in order to consider non-crisis, sub-prime crisis and Eurozone crisis. We find that there are changes in correlations of distinct <span class="hlt">scales</span> and different periods. Association in finest <span class="hlt">scales</span> is smaller than in coarse <span class="hlt">scales</span>. There is a rise on associations in periods of crisis. In <span class="hlt">frequencies</span>, there is predominance for significant distinctions involving the coarsest <span class="hlt">scale</span>, while for crises periods there is predominance for distinctions on the finest <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3896460','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3896460"><span>Liquidity Spillover in International Stock Markets through Distinct Time <span class="hlt">Scales</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>Righi, Marcelo Brutti; Vieira, Kelmara Mendes</p> <p>2014-01-01</p> <p>This paper identifies liquidity spillovers through different time <span class="hlt">scales</span> based on a wavelet multiscaling method. We decompose daily data from U.S., British, Brazilian and Hong Kong stock markets indices in order to calculate the <span class="hlt">scale</span> correlation between their illiquidities. The sample is divided in order to consider non-crisis, sub-prime crisis and Eurozone crisis. We find that there are changes in correlations of distinct <span class="hlt">scales</span> and different periods. Association in finest <span class="hlt">scales</span> is smaller than in coarse <span class="hlt">scales</span>. There is a rise on associations in periods of crisis. In <span class="hlt">frequencies</span>, there is predominance for significant distinctions involving the coarsest <span class="hlt">scale</span>, while for crises periods there is predominance for distinctions on the finest <span class="hlt">scale</span>. PMID:24465918</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..118a2024B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..118a2024B"><span>What do we know about Indonesian tropical lakes? Insights from high <span class="hlt">frequency</span> measurement</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Budi Santoso, Arianto; Triwisesa, Endra; Fakhrudin, Muh.; Harsono, Eko; Agita Rustini, Hadiid</p> <p>2018-02-01</p> <p>When measuring ecological variables in lakes, sampling <span class="hlt">frequency</span> is critical in capturing an environmental pattern. Discrete sampling of traditional monitoring programs is likely to result in vital knowledge gaps in understanding any processes particularly those with fine temporal <span class="hlt">scale</span> characteristics. The development of high <span class="hlt">frequency</span> measurements offer a sophisticated range of information in recording any events in lakes at a finer time <span class="hlt">scale</span>. We present physical indices of a tropical deep Lake Maninjau arrayed from OnLine Monitoring System (OLM). It is revealed that Lake Maninjau mostly has a diurnal thermal stratification pattern. The calculated lake stability (Schmidt stability), however, follows a seasonal pattern; low in December-January and around August, and high in May and September. Using a 3D numerical model simulation (ELCOM), we infer how wind and solar radiation intensity control lake’s temperature profiles. In this review, we highlight the needs of high <span class="hlt">frequency</span> measurement establishment in Indonesian tropical lakes to better understand the unique processes and to support the authorities’ decision making in maximizing the provision of ecosystem services supplied by lakes and reservoirs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010CompM..45..637D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010CompM..45..637D"><span>Two-time <span class="hlt">scale</span> fatigue modelling: application to damage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Devulder, Anne; Aubry, Denis; Puel, Guillaume</p> <p>2010-05-01</p> <p>A temporal multiscale modelling applied to fatigue damage evolution in cortical bone is presented. Microdamage accumulation in cortical bone, ensued from daily activities, leads to impaired mechanical properties, in particular by reducing the bone stiffness and inducing fatigue. However, bone damage is also known as a stimulus to bone remodelling, whose aim is to repair and generate new bone, adapted to its environment. This biological process by removing fatigue damage seems essential to the skeleton lifetime. As daily activities induce high <span class="hlt">frequency</span> cycles (about 10,000 cycles a day), identifying two-time <span class="hlt">scale</span> is very fruitful: a fast one connected with the high <span class="hlt">frequency</span> cyclic loading and a slow one related to a quasi-static loading. A <span class="hlt">scaling</span> parameter is defined between the intrinsic time (bone lifetime of several years) and the high <span class="hlt">frequency</span> loading (few seconds). An asymptotic approach allows to decouple the two <span class="hlt">scales</span> and to take into account history effects (Guennouni and Aubry in CR Acad Sci Paris Ser II 20:1765-1767, 1986). The method is here applied to a simple case of fatigue damage and a real cortical bone microstructure. A significant reduction in the amount of computation time in addition to a small computational error between time homogenized and non homogenized models are obtained. This method seems thus to give new perspectives to assess fatigue damage and, with regard to bone, to give a better understanding of bone remodelling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913842L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913842L"><span>Relative importance of precipitation <span class="hlt">frequency</span> and intensity in inter-annual variation of precipitation in Singapore during 1980-2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Xin; Babovic, Vladan</p> <p>2017-04-01</p> <p>Observed studies on inter-annual variation of precipitation provide insight into the response of precipitation to anthropogenic climate change and natural climate variability. Inter-annual variation of precipitation results from the concurrent variations of precipitation <span class="hlt">frequency</span> and intensity, understanding of the relative importance of <span class="hlt">frequency</span> and intensity in the variability of precipitation can help fathom its changing properties. Investigation of the long-term changes of precipitation schemes has been extensively carried out in many regions across the world, however, detailed studies of the relative importance of precipitation <span class="hlt">frequency</span> and intensity in inter-annual variation of precipitation are still limited, especially in the tropics. Therefore, this study presents a comprehensive framework to investigate the inter-annual variation of precipitation and the dominance of precipitation <span class="hlt">frequency</span> and intensity in a tropical urban city-state, Singapore, based on long-term (1980-2013) daily precipitation series from 22 rain gauges. First, an iterative Mann-Kendall trend test method is applied to detect long-term trends in precipitation total, <span class="hlt">frequency</span> and intensity at both annual and seasonal time <span class="hlt">scales</span>. Then, the relative importance of precipitation <span class="hlt">frequency</span> and intensity in inducing the inter-annual variation of wet-day precipitation total is analyzed using a dominance analysis method based on linear regression. The results show statistically significant upward trends in wet-day precipitation total, <span class="hlt">frequency</span> and intensity at annual time <span class="hlt">scale</span>, however, these trends are not evident during the monsoon seasons. The inter-annual variation of wet-day precipitation is mainly dominated by precipitation intensity for most of the stations at annual time <span class="hlt">scale</span> and during the Northeast monsoon season. However, during the Southwest monsoon season, the inter-annual variation of wet-day precipitation is mainly dominated by precipitation <span class="hlt">frequency</span>. These results have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112a3503P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112a3503P"><span>Synchronization of electrically coupled micromechanical oscillators with a <span class="hlt">frequency</span> ratio of 3:1</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pu, Dong; Wei, Xueyong; Xu, Liu; Jiang, Zhuangde; Huan, Ronghua</p> <p>2018-01-01</p> <p>In this Letter, synchronization of micromechanical oscillators with a <span class="hlt">frequency</span> ratio of 3:1 is reported. Two electrically coupled piezoresistive micromechanical oscillators are built for the study, and their oscillation <span class="hlt">frequencies</span> are tuned via the Joule heating effect to find out the synchronization region. Experimental results show that the larger coupling strength or bias driving voltage is applied and a wider synchronization region is obtained. Interestingly, however, the oscillator's <span class="hlt">frequency</span> tunability is dramatically reduced from -809.1 Hz/V to -23.1 Hz/V when synchronization is reached. A nearly 10-fold improvement of <span class="hlt">frequency</span> stability at 1 s is observed from one of the synchronized oscillators, showing a comparable performance of the other. The stable high order synchronization of micromechanical oscillators is helpful to design high performance resonant sensors with a better <span class="hlt">frequency</span> resolution and a larger <span class="hlt">scale</span> factor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001ExFl...30..202H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001ExFl...30..202H"><span>An experimental study of large-<span class="hlt">scale</span> vortices over a blunt-faced flat plate in pulsating flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hwang, K. S.; Sung, H. J.; Hyun, J. M.</p> <p></p> <p>Laboratory measurements are made of flow over a blunt flat plate of finite thickness, which is placed in a pulsating free stream, U=Uo(1+Aocos 2πfpt). Low turbulence-intensity wind tunnel experiments are conducted in the ranges of Stp<=1.23 and Ao<=0.118 at ReH=560. Pulsation is generated by means of a woofer speaker. Variations of the time-mean reattachment length xR as functions of Stp and Ao are scrutinized by using the forward-time fraction and surface pressure distributions (Cp). The shedding <span class="hlt">frequency</span> of large-<span class="hlt">scale</span> vortices due to pulsation is measured. Flow visualizations depict the behavior of large-<span class="hlt">scale</span> vortices. The results for non-pulsating flows (Ao=0) are consistent with the published data. In the lower range of Ao, as Stp increases, xR attains a minimum value at a particular pulsation <span class="hlt">frequency</span>. For large Ao, the results show complicated behaviors of xR. For Stp>=0.80, changes in xR are insignificant as Ao increases. The shedding <span class="hlt">frequency</span> of large-<span class="hlt">scale</span> vortices is locked-in to the pulsation <span class="hlt">frequency</span>. A vortex-pairing process takes place between two neighboring large-<span class="hlt">scale</span> vortices in the separated shear layer.</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/2017PhRvD..96j3502Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvD..96j3502Y"><span>Generalized Doppler and aberration kernel for <span class="hlt">frequency</span>-dependent cosmological observables</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yasini, Siavash; Pierpaoli, Elena</p> <p>2017-11-01</p> <p>We introduce a <span class="hlt">frequency</span>-dependent Doppler and aberration transformation kernel for the harmonic multipoles of a general cosmological observable with spin weight s , Doppler weight d and arbitrary <span class="hlt">frequency</span> spectrum. In the context of cosmic microwave background (CMB) studies, the <span class="hlt">frequency</span>-dependent formalism allows to correct for the motion-induced aberration and Doppler effects on individual <span class="hlt">frequency</span> maps with different masks. It also permits to deboost background radiations with non-blackbody <span class="hlt">frequency</span> spectra, like extragalactic foregrounds and CMB spectra with primordial spectral distortions. The formalism can also be used to correct individual E and B polarization modes and account for motion-induced E/B mixing of polarized observables with d ≠1 at different <span class="hlt">frequencies</span>. We apply the generalized aberration kernel on polarized and unpolarized specific intensity at 100 and 217 GHz and show that the motion-induced effects typically increase with the <span class="hlt">frequency</span> of observation. In all-sky CMB experiments, the <span class="hlt">frequency</span>-dependence of the motion-induced effects for a blackbody spectrum are overall negligible. However in a cut-sky analysis, ignoring the <span class="hlt">frequency</span> dependence can lead to percent level error in the polarized and unpolarized power spectra over all angular <span class="hlt">scales</span>. In the specific cut-sky used in our analysis (b >4 5 ° ,fsky≃14 % ), and for the dipole-inferred velocity β =0.00123 typically attributed to our peculiar motion, the Doppler and aberration effects can change polarized and unpolarized power spectra of specific intensity in the CMB rest frame by 1 - 2 % , but we find the polarization cross-leakage between E and B modes to be negligible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080040697','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080040697"><span>A Revised Method of Presenting Wavenumber-<span class="hlt">Frequency</span> Power Spectrum Diagrams That Reveals the Asymmetric Nature of Tropical Large-<span class="hlt">scale</span> Waves</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chao, Winston C.; Yang, Bo; Fu, Xiouhua</p> <p>2007-01-01</p> <p>The popular method of presenting wavenumber-<span class="hlt">frequency</span> power spectrum diagrams for studying tropical large-<span class="hlt">scale</span> waves in the literature is shown to give an incomplete presentation of these waves. The so-called "convectively-coupled Kelvin (mixed Rossby-gravity) waves" are presented as existing only in the symmetric (antisymmetric) component of the diagrams. This is obviously not consistent with the published composite/regression studies of "convectively-coupled Kelvin waves," which illustrate the asymmetric nature of these waves. The cause of this inconsistency is revealed in this note and a revised method of presenting the power spectrum diagrams is proposed. When this revised method is used, "convectively-coupled Kelvin waves" do show anti-symmetric components, and "convectively-coupled mixed Rossby-gravity waves (also known as Yanai waves)" do show a hint of symmetric components. These results bolster a published proposal that these waves be called "chimeric Kelvin waves," "chimeric mixed Rossby-gravity waves," etc. This revised method of presenting power spectrum diagrams offers a more rigorous means of comparing the General Circulation Models (GCM) output with observations by calling attention to the capability of GCMs in correctly simulating the asymmetric characteristics of the equatorial waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4552601','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4552601"><span>The <span class="hlt">Frequency</span> of Involuntary Autobiographical Memories and Future Thoughts in Relation to Daydreaming, Emotional Distress, and Age</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Berntsen, Dorthe; Rubin, David C.; Salgado, Sinue</p> <p>2015-01-01</p> <p>We introduce a new <span class="hlt">scale</span>, the Involuntary Autobiographical Memory Inventory (IAMI), for measuring the <span class="hlt">frequency</span> of involuntary autobiographical memories and involuntary future thoughts. Using the <span class="hlt">scale</span> in relation to other psychometric and demographic measures provided three important, novel findings. First, the <span class="hlt">frequency</span> of involuntary and voluntary memories and future thoughts are similarly related to general measures of emotional distress. This challenges the idea that the involuntary mode is uniquely associated with emotional distress. Second, the <span class="hlt">frequency</span> of involuntary autobiographical remembering does not decline with age, whereas measures of daydreaming, suppression of unwanted thoughts and dissociative experiences all do. Thus, involuntary autobiographical remembering relates differently to aging than daydreaming and other forms of spontaneous and uncontrollable thoughts. Third, unlike involuntary autobiographical remembering, the <span class="hlt">frequency</span> of future thoughts does decrease with age. This finding underscores the need for examining past and future mental time travel in relation to aging and life span development. PMID:26241025</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27650130','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27650130"><span>Effect of turning <span class="hlt">frequency</span> on co-composting pig manure and fungus residue.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jiang-Ming, Zhou</p> <p>2017-03-01</p> <p>Composting of agricultural wastes not only can reduce environmental pollution caused by improper disposal, but also can recycle agricultural wastes and transform them into highly valuable products, such as fertilizers or soil conditioners, for agricultural applications. However, the composting process and final product are easily affected by the limited oxygen supply that results from insufficient aeration, especially in the center of a large-<span class="hlt">scale</span> windrow. Hence, a pilot-<span class="hlt">scale</span> experiment was conducted to investigate the effects of the turning <span class="hlt">frequency</span> on the composting efficiency and compost quality of used pig manure and fungus residue. Physical and chemical characteristics were measured over the course of 63 days of composting. The data indicate that higher temperatures and more rapid moisture removal generally result from a turning treatment of once every 2-4 days than in fewer, or no, turning treatments. The total nitrogen, total phosphorus, and total potassium contents increased in all windrows as the organic matter content decreased, but both the increases and decrease were greater in windrows that were turned more frequently. The reduction of the organic matter mass by 53.7-66.0% for a turning of once every 2-8 days is significantly higher than that for the static windrow (39.1%). Although there is an increase in nitrogen mass loss with an increased turning <span class="hlt">frequency</span>, lower nitrogen mass losses (12.7-25.7%) in all treatments were noted compared with previous studies. A final compost product with less moisture, less weight, higher nutrient content (N, P, and K), and greater stability was obtained in windrows with turning <span class="hlt">frequencies</span> of once every 2-4 days, which is recommended when composting pig manure and fungus residue. Composting of agricultural wastes not only can reduce environmental pollution caused by improper disposal, but recycling of agricultural wastes transforms them into highly valuable products, such as fertilizers or soil conditioners, for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MSSP...54...41L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MSSP...54...41L"><span>Adaptive noise cancelling and time-<span class="hlt">frequency</span> techniques for rail surface defect detection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, B.; Iwnicki, S.; Ball, A.; Young, A. E.</p> <p>2015-03-01</p> <p>Adaptive noise cancelling (ANC) is a technique which is very effective to remove additive noises from the contaminated signals. It has been widely used in the fields of telecommunication, radar and sonar signal processing. However it was seldom used for the surveillance and diagnosis of mechanical systems before late of 1990s. As a promising technique it has gradually been exploited for the purpose of condition monitoring and fault diagnosis. Time-<span class="hlt">frequency</span> analysis is another useful tool for condition monitoring and fault diagnosis purpose as time-<span class="hlt">frequency</span> analysis can keep both time and <span class="hlt">frequency</span> information simultaneously. This paper presents an ANC and time-<span class="hlt">frequency</span> application for railway wheel flat and rail surface defect detection. The experimental results from a <span class="hlt">scaled</span> roller test rig show that this approach can significantly reduce unwanted interferences and extract the weak signals from strong background noises. The combination of ANC and time-<span class="hlt">frequency</span> analysis may provide us one of useful tools for condition monitoring and fault diagnosis of railway vehicles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4684220','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4684220"><span><span class="hlt">Scaling</span> in Free-Swimming Fish and Implications for Measuring Size-at-Time in the Wild</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Broell, Franziska; Taggart, Christopher T.</p> <p>2015-01-01</p> <p>This study was motivated by the need to measure size-at-age, and thus growth rate, in fish in the wild. We postulated that this could be achieved using accelerometer tags based first on early isometric <span class="hlt">scaling</span> models that hypothesize that similar animals should move at the same speed with a stroke <span class="hlt">frequency</span> that <span class="hlt">scales</span> with length-1, and second on observations that the speed of primarily air-breathing free-swimming animals, presumably swimming ‘efficiently’, is independent of size, confirming that stroke <span class="hlt">frequency</span> <span class="hlt">scales</span> as length-1. However, such <span class="hlt">scaling</span> relations between size and swimming parameters for fish remain mostly theoretical. Based on free-swimming saithe and sturgeon tagged with accelerometers, we introduce a species-specific <span class="hlt">scaling</span> relationship between dominant tail beat <span class="hlt">frequency</span> (TBF) and fork length. Dominant TBF was proportional to length-1 (r2 = 0.73, n = 40), and estimated swimming speed within species was independent of length. Similar <span class="hlt">scaling</span> relations accrued in relation to body mass-0.29. We demonstrate that the dominant TBF can be used to estimate size-at-time and that accelerometer tags with onboard processing may be able to provide size-at-time estimates among free-swimming fish and thus the estimation of growth rate (change in size-at-time) in the wild. PMID:26673777</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080022352','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080022352"><span>Pressure and Thrust Measurements of a High-<span class="hlt">Frequency</span> Pulsed-Detonation Actuator</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nguyen, Namtran C.; Cutler, Andrew D.</p> <p>2008-01-01</p> <p>This paper describes the development of a small-<span class="hlt">scale</span>, high-<span class="hlt">frequency</span> pulsed detonation actuator. The device utilized a fuel mixture of H2 and air, which was injected into the device at <span class="hlt">frequencies</span> of up to 1200 Hz. Pulsed detonations were demonstrated in an 8-inch long combustion volume, at approx.600 Hz, for the lambda/4 mode. The primary objective of this experiment was to measure the generated thrust. A mean value of thrust was measured up to 6.0 lb, corresponding to specific impulse of 2611 s. This value is comparable to other H2-fueled pulsed detonation engines (PDEs) experiments. The injection and detonation <span class="hlt">frequency</span> for this new experimental case was approx.600 Hz, and was much higher than typical PDEs, where <span class="hlt">frequencies</span> are usually less than 100 Hz. The compact size of the model and high <span class="hlt">frequency</span> of detonation yields a thrust-per-unit-volume of approximately 2.0 lb/cu in, and compares favorably with other experiments, which typically have thrust-per-unit-volume values of approximately 0.01 lb/cu in.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10089E..0HI','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10089E..0HI"><span>Velocity measurement using <span class="hlt">frequency</span> domain interferometer and chirped pulse laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ishii, K.; Nishimura, Y.; Mori, Y.; Hanayama, R.; Kitagawa, Y.; Sekine, T.; Sato, N.; Kurita, T.; Kawashima, T.; Sunahara, A.; Sentoku, Y.; Miura, E.; Iwamoto, A.; Sakagami, H.</p> <p>2017-02-01</p> <p>An ultra-intense short pulse laser induces a shock wave in material. The pressure of shock compression is stronger than a few tens GPa. To characterize shock waves, time-resolved velocity measurement in nano- or pico-second time <span class="hlt">scale</span> is needed. <span class="hlt">Frequency</span> domain interferometer and chirped pulse laser provide single-shot time-resolved measurement. We have developed a laser-driven shock compression system and <span class="hlt">frequency</span> domain interferometer with CPA laser. In this paper, we show the principle of velocity measurement using a <span class="hlt">frequency</span> domain interferometer and a chirped pulse laser. Next, we numerically calculated spectral interferograms and show the time-resolved velocity measurement can be done from the phase analysis of spectral interferograms. Moreover we conduct the laser driven shock generation and shock velocity measurement. From the spectral fringes, we analyze the velocities of the sample and shockwaves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19740054880&hterms=Exciter&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DExciter','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19740054880&hterms=Exciter&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DExciter"><span>Satellite observations of type III solar radio bursts at low <span class="hlt">frequencies</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fainberg, J.; Stone, R. G.</p> <p>1974-01-01</p> <p>Type III solar radio bursts have been observed from 10 MHz to 10 kHz by satellite experiments above the terrestrial plasmasphere. Solar radio emission in this <span class="hlt">frequency</span> range results from excitation of the interplanetary plasma by energetic particles propagating outward along open field lines over distances from 5 earth radii to at least 1 AU from the sun. This review summarizes the morphology, characteristics, and analysis of individual as well as storms of bursts. Substantial evidence is available to show that the radio emission is observed at the second harmonic instead of the fundamental of the plasma <span class="hlt">frequency</span>. This brings the density <span class="hlt">scale</span> derived by radio observations into better agreement with direct solar wind density measurements at 1 AU and relaxes the requirement for type III propagation along large density-enhanced regions. This density <span class="hlt">scale</span> with the measured direction of arrival of the radio burst allows the trajectory of the exciter path to be determined from 10 earth radii to 1 AU.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ExFl...47..613V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ExFl...47..613V"><span>An Eulerian time filtering technique to study large-<span class="hlt">scale</span> transient flow phenomena</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vanierschot, Maarten; Persoons, Tim; van den Bulck, Eric</p> <p>2009-10-01</p> <p>Unsteady fluctuating velocity fields can contain large-<span class="hlt">scale</span> periodic motions with <span class="hlt">frequencies</span> well separated from those of turbulence. Examples are the wake behind a cylinder or the processing vortex core in a swirling jet. These turbulent flow fields contain large-<span class="hlt">scale</span>, low-<span class="hlt">frequency</span> oscillations, which are obscured by turbulence, making it impossible to identify them. In this paper, we present an Eulerian time filtering (ETF) technique to extract the large-<span class="hlt">scale</span> motions from unsteady statistical non-stationary velocity fields or flow fields with multiple phenomena that have sufficiently separated spectral content. The ETF method is based on non-causal time filtering of the velocity records in each point of the flow field. It is shown that the ETF technique gives good results, similar to the ones obtained by the phase-averaging method. In this paper, not only the influence of the temporal filter is checked, but also parameters such as the cut-off <span class="hlt">frequency</span> and sampling <span class="hlt">frequency</span> of the data are investigated. The technique is validated on a selected set of time-resolved stereoscopic particle image velocimetry measurements such as the initial region of an annular jet and the transition between flow patterns in an annular jet. The major advantage of the ETF method in the extraction of large <span class="hlt">scales</span> is that it is computationally less expensive and it requires less measurement time compared to other extraction methods. Therefore, the technique is suitable in the startup phase of an experiment or in a measurement campaign where several experiments are needed such as parametric studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040139910','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040139910"><span>Transient Modeling of Hybrid Rocket Low <span class="hlt">Frequency</span> Instabilities</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Karabeyoglu, M. Arif; DeZilwa, Shane; Cantwell, Brian; Zilliac, Greg</p> <p>2003-01-01</p> <p>A comprehensive dynamic model of a hybrid rocket has been developed in order to understand and predict the transient behavior including instabilities. A linearized version of the transient model predicted the low-<span class="hlt">frequency</span> chamber pressure oscillations that are commonly observed in hybrids. The source of the instabilities is based on a complex coupling of thermal transients in the solid fuel, wall heat transfer blocking due to fuel regression rate and the transients in the boundary layer that forms on the fuel surface. The oscillation <span class="hlt">frequencies</span> predicted by the linearized theory are in very good agreement with 43 motor test results obtained from the hybrid propulsion literature. The motor test results used in the comparison cover a very wide spectrum of parameters including: 1) four separate research and development programs, 2) three different oxidizers (LOX, GOX, N2O), 3) a wide range of motor dimensions (i.e. from 5 inch diameter to 72 inch diameter) and operating conditions and 4) several fuel formulations. A simple universal <span class="hlt">scaling</span> formula for the <span class="hlt">frequency</span> of the primary oscillation mode is suggested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26953172','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26953172"><span>Sparse time-<span class="hlt">frequency</span> decomposition based on dictionary adaptation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hou, Thomas Y; Shi, Zuoqiang</p> <p>2016-04-13</p> <p>In this paper, we propose a time-<span class="hlt">frequency</span> analysis method to obtain instantaneous <span class="hlt">frequencies</span> and the corresponding decomposition by solving an optimization problem. In this optimization problem, the basis that is used to decompose the signal is not known a priori. Instead, it is adapted to the signal and is determined as part of the optimization problem. In this sense, this optimization problem can be seen as a dictionary adaptation problem, in which the dictionary is adaptive to one signal rather than a training set in dictionary learning. This dictionary adaptation problem is solved by using the augmented Lagrangian multiplier (ALM) method iteratively. We further accelerate the ALM method in each iteration by using the fast wavelet transform. We apply our method to decompose several signals, including signals with poor <span class="hlt">scale</span> separation, signals with outliers and polluted by noise and a real signal. The results show that this method can give accurate recovery of both the instantaneous <span class="hlt">frequencies</span> and the intrinsic mode functions. © 2016 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GMS...216...31S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GMS...216...31S"><span>Low-<span class="hlt">Frequency</span> Waves in HF Heating of the Ionosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharma, A. S.; Eliasson, B.; Milikh, G. M.; Najmi, A.; Papadopoulos, K.; Shao, X.; Vartanyan, A.</p> <p>2016-02-01</p> <p>Ionospheric heating experiments have enabled an exploration of the ionosphere as a large-<span class="hlt">scale</span> natural laboratory for the study of many plasma processes. These experiments inject high-<span class="hlt">frequency</span> (HF) radio waves using high-power transmitters and an array of ground- and space-based diagnostics. This chapter discusses the excitation and propagation of low-<span class="hlt">frequency</span> waves in HF heating of the ionosphere. The theoretical aspects and the associated models and simulations, and the results from experiments, mostly from the HAARP facility, are presented together to provide a comprehensive interpretation of the relevant plasma processes. The chapter presents the plasma model of the ionosphere for describing the physical processes during HF heating, the numerical code, and the simulations of the excitation of low-<span class="hlt">frequency</span> waves by HF heating. It then gives the simulations of the high-latitude ionosphere and mid-latitude ionosphere. The chapter also briefly discusses the role of kinetic processes associated with wave generation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930018563','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930018563"><span>Quasi-optical antenna-mixer-array design for terahertz <span class="hlt">frequencies</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Guo, Yong; Potter, Kent A.; Rutledge, David B.</p> <p>1992-01-01</p> <p>A new quasi-optical antenna-mixer-array design for terahertz <span class="hlt">frequencies</span> is presented. In the design, antenna and mixer are combined into an entity, based on the technology in which millimeter-wave horn antenna arrays have been fabricated in silicon wafers. It consists of a set of forward- and backward-looking horns made with a set of silicon wafers. The front side is used to receive incoming signal, and the back side is used to feed local oscillator signal. Intermediate <span class="hlt">frequency</span> is led out from the side of the array. Signal received by the horn array is picked up by antenna probes suspended on thin silicon-oxynitride membranes inside the horns. Mixer diodes will be located on the membranes inside the horns. Modeling of such an antenna-mixer-array design is done on a <span class="hlt">scaled</span> model at microwave <span class="hlt">frequencies</span>. The impedance matching, RF and LO isolation, and patterns of the array have been tested and analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...611A..10S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...611A..10S"><span>High <span class="hlt">frequency</span> generation in the corona: Resonant cavities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santamaria, I. C.; Van Doorsselaere, T.</p> <p>2018-03-01</p> <p>Aims: Null points are prominent magnetic field singularities in which the magnetic field strength strongly decreases in very small spatial <span class="hlt">scales</span>. Around null points, predicted to be ubiquitous in the solar chromosphere and corona, the wave behavior changes considerably. Null points are also responsible for driving very energetic phenomena, and for contributing to chromospheric and coronal heating. In previous works we demonstrated that slow magneto-acoustic shock waves were generated in the chromosphere propagate through the null point, thereby producing a train of secondary shocks escaping along the field lines. A particular combination of the shock wave speeds generates waves at a <span class="hlt">frequency</span> of 80 MHz. The present work aims to investigate this high <span class="hlt">frequency</span> region around a coronal null point to give a plausible explanation to its generation at that particular <span class="hlt">frequency</span>. Methods: We carried out a set of two-dimensional numerical simulations of wave propagation in the neighborhood of a null point located in the corona. We varied both the amplitude of the driver and the atmospheric properties to investigate the sensitivity of the high <span class="hlt">frequency</span> waves to these parameters. Results: We demonstrate that the wave <span class="hlt">frequency</span> is sensitive to the atmospheric parameters in the corona, but it is independent of the strength of the driver. Thus, the null point behaves as a resonant cavity generating waves at specific <span class="hlt">frequencies</span> that depend on the background equilibrium model. Moreover, we conclude that the high <span class="hlt">frequency</span> wave train generated at the null point is not necessarily a result of the interaction between the null point and a shock wave. This wave train can be also developed by the interaction between the null point and fast acoustic-like magneto-acoustic waves, that is, this interaction within the linear regime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3400A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3400A"><span><span class="hlt">Scaling</span> A Moment-Rate Function For Small To Large Magnitude Events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Archuleta, Ralph; Ji, Chen</p> <p>2017-04-01</p> <p>Since the 1980's seismologists have recognized that peak ground acceleration (PGA) and peak ground velocity (PGV) <span class="hlt">scale</span> differently with magnitude for large and moderate earthquakes. In a recent paper (Archuleta and Ji, GRL 2016) we introduced an apparent moment-rate function (aMRF) that accurately predicts the <span class="hlt">scaling</span> with magnitude of PGA, PGV, PWA (Wood-Anderson Displacement) and the ratio PGA/2πPGV (dominant <span class="hlt">frequency</span>) for earthquakes 3.3 ≤ M ≤ 5.3. This apparent moment-rate function is controlled by two temporal parameters, tp and td, which are related to the time for the moment-rate function to reach its peak amplitude and the total duration of the earthquake, respectively. These two temporal parameters lead to a Fourier amplitude spectrum (FAS) of displacement that has two corners in between which the spectral amplitudes decay as 1/f, f denotes <span class="hlt">frequency</span>. At higher or lower <span class="hlt">frequencies</span>, the FAS of the aMRF looks like a single-corner Aki-Brune omega squared spectrum. However, in the presence of attenuation the higher corner is almost certainly masked. Attempting to correct the spectrum to an Aki-Brune omega-squared spectrum will produce an "apparent" corner <span class="hlt">frequency</span> that falls between the double corner <span class="hlt">frequency</span> of the aMRF. We reason that the two corners of the aMRF are the reason that seismologists deduce a stress drop (e.g., Allmann and Shearer, JGR 2009) that is generally much smaller than the stress parameter used to produce ground motions from stochastic simulations (e.g., Boore, 2003 Pageoph.). The presence of two corners for the smaller magnitude earthquakes leads to several questions. Can deconvolution be successfully used to determine <span class="hlt">scaling</span> from small to large earthquakes? Equivalently will large earthquakes have a double corner? If large earthquakes are the sum of many smaller magnitude earthquakes, what should the displacement FAS look like for a large magnitude earthquake? Can a combination of such a double-corner spectrum and random</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2352A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2352A"><span>Contributions of Dynamic and Thermodynamic <span class="hlt">Scaling</span> in Subdaily Precipitation Extremes in India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ali, Haider; Mishra, Vimal</p> <p>2018-03-01</p> <p>Despite the importance of subdaily precipitation extremes for urban areas, the role of dynamic and thermodynamic <span class="hlt">scaling</span> in changes in precipitation extremes in India remains poorly constrained. Here we estimate contributions from thermodynamic and dynamic <span class="hlt">scaling</span> on changes in subdaily precipitation extremes for 23 urban locations in India. Subdaily precipitation extremes have become more intense during the last few decades. Moreover, we find a twofold rise in the <span class="hlt">frequency</span> of subdaily precipitation extremes during 1979-2015, which is faster than the increase in daily precipitation extremes. The contribution of dynamic <span class="hlt">scaling</span> in this rise in the <span class="hlt">frequency</span> and intensity of subdaily precipitation extremes is higher than the thermodynamic <span class="hlt">scaling</span>. Moreover, half-hourly precipitation extremes show higher contributions from the both thermodynamic ( 10%/K) and dynamic ( 15%/K) <span class="hlt">scaling</span> than daily (6%/K and 9%/K, respectively) extremes indicating the role of warming on the rise in the subdaily precipitation extremes in India. Our findings have implications for better understanding the dynamic response of precipitation extremes under the warming climate over India.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990052767','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990052767"><span>Acoustic Treatment Design <span class="hlt">Scaling</span> Methods. Volume 5; Analytical and Experimental Data Correlation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chien, W. E.; Kraft, R. E.; Syed, A. A.</p> <p>1999-01-01</p> <p>The primary purpose of the study presented in this volume is to present the results and data analysis of in-duct transmission loss measurements. Transmission loss testing was performed on full-<span class="hlt">scale</span>, 1/2-<span class="hlt">scale</span>, and 115-<span class="hlt">scale</span> treatment panel samples. The objective of the study was to compare predicted and measured transmission loss for full-<span class="hlt">scale</span> and subscale panels in an attempt to evaluate the variations in suppression between full- and subscale panels which were ostensibly of equivalent design. Generally, the results indicated an unsatisfactory agreement between measurement and prediction, even for full-<span class="hlt">scale</span>. This was attributable to difficulties encountered in obtaining sufficiently accurate test results, even with extraordinary care in calibrating the instrumentation and performing the test. Test difficulties precluded the ability to make measurements at <span class="hlt">frequencies</span> high enough to be representative of subscale liners. It is concluded that transmission loss measurements without ducts and data acquisition facilities specifically designed to operate with the precision and complexity required for high subscale <span class="hlt">frequency</span> ranges are inadequate for evaluation of subscale treatment effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvL.120n4301L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvL.120n4301L"><span>Double <span class="hlt">Scaling</span> in the Relaxation Time in the β -Fermi-Pasta-Ulam-Tsingou Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lvov, Yuri V.; Onorato, Miguel</p> <p>2018-04-01</p> <p>We consider the original β -Fermi-Pasta-Ulam-Tsingou system; numerical simulations and theoretical arguments suggest that, for a finite number of masses, a statistical equilibrium state is reached independently of the initial energy of the system. Using ensemble averages over initial conditions characterized by different Fourier random phases, we numerically estimate the time <span class="hlt">scale</span> of equipartition and we find that for very small nonlinearity it matches the prediction based on exact wave-wave resonant interaction theory. We derive a simple formula for the nonlinear <span class="hlt">frequency</span> broadening and show that when the phenomenon of overlap of <span class="hlt">frequencies</span> takes place, a different <span class="hlt">scaling</span> for the thermalization time <span class="hlt">scale</span> is observed. Our result supports the idea that the Chirikov overlap criterion identifies a transition region between two different relaxation time <span class="hlt">scalings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=%22frequency+list%22&id=EJ1056039','ERIC'); return false;" href="https://eric.ed.gov/?q=%22frequency+list%22&id=EJ1056039"><span>Parametric Effects of Word <span class="hlt">Frequency</span> in Memory for Mixed <span class="hlt">Frequency</span> Lists</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Lohnas, Lynn J.; Kahana, Michael J.</p> <p>2013-01-01</p> <p>The "word <span class="hlt">frequency</span> paradox" refers to the finding that low <span class="hlt">frequency</span> words are better recognized than high <span class="hlt">frequency</span> words yet high <span class="hlt">frequency</span> words are better recalled than low <span class="hlt">frequency</span> words. Rather than comparing separate groups of low and high <span class="hlt">frequency</span> words, we sought to quantify the functional relation between word <span class="hlt">frequency</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_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3995693','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3995693"><span>Exploring Empirical Rank-<span class="hlt">Frequency</span> Distributions Longitudinally through a Simple Stochastic Process</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Finley, Benjamin J.; Kilkki, Kalevi</p> <p>2014-01-01</p> <p>The frequent appearance of empirical rank-<span class="hlt">frequency</span> laws, such as Zipf’s law, in a wide range of domains reinforces the importance of understanding and modeling these laws and rank-<span class="hlt">frequency</span> distributions in general. In this spirit, we utilize a simple stochastic cascade process to simulate several empirical rank-<span class="hlt">frequency</span> distributions longitudinally. We focus especially on limiting the process’s complexity to increase accessibility for non-experts in mathematics. The process provides a good fit for many empirical distributions because the stochastic multiplicative nature of the process leads to an often observed concave rank-<span class="hlt">frequency</span> distribution (on a log-log <span class="hlt">scale</span>) and the finiteness of the cascade replicates real-world finite size effects. Furthermore, we show that repeated trials of the process can roughly simulate the longitudinal variation of empirical ranks. However, we find that the empirical variation is often less that the average simulated process variation, likely due to longitudinal dependencies in the empirical datasets. Finally, we discuss the process limitations and practical applications. PMID:24755621</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24755621','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24755621"><span>Exploring empirical rank-<span class="hlt">frequency</span> distributions longitudinally through a simple stochastic process.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Finley, Benjamin J; Kilkki, Kalevi</p> <p>2014-01-01</p> <p>The frequent appearance of empirical rank-<span class="hlt">frequency</span> laws, such as Zipf's law, in a wide range of domains reinforces the importance of understanding and modeling these laws and rank-<span class="hlt">frequency</span> distributions in general. In this spirit, we utilize a simple stochastic cascade process to simulate several empirical rank-<span class="hlt">frequency</span> distributions longitudinally. We focus especially on limiting the process's complexity to increase accessibility for non-experts in mathematics. The process provides a good fit for many empirical distributions because the stochastic multiplicative nature of the process leads to an often observed concave rank-<span class="hlt">frequency</span> distribution (on a log-log <span class="hlt">scale</span>) and the finiteness of the cascade replicates real-world finite size effects. Furthermore, we show that repeated trials of the process can roughly simulate the longitudinal variation of empirical ranks. However, we find that the empirical variation is often less that the average simulated process variation, likely due to longitudinal dependencies in the empirical datasets. Finally, we discuss the process limitations and practical applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5560622','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5560622"><span>Impact of Non-Suicidal Self-Injury <span class="hlt">Scale</span>: Initial Psychometric Validation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Burke, Taylor A.; Ammerman, Brooke A.; Hamilton, Jessica L.; Alloy, Lauren B.</p> <p>2017-01-01</p> <p>The current study examined the psychometric properties of the Impact of Non-Suicidal Self-Injury <span class="hlt">Scale</span> (INS), a <span class="hlt">scale</span> developed to assess the social, behavioral, and emotional consequences of engaging in non-suicidal self-injury (NSSI). University students (N=128) who endorsed a history of NSSI were administered the INS, as well as measures of hypothesized convergent and divergent validity. Results suggested that the INS is best conceptualized as a one-factor <span class="hlt">scale</span>, and internal consistency analyses indicated excellent reliability. The INS was significantly correlated with well-known measures of NSSI severity (i.e., NSSI <span class="hlt">frequency</span>, NSSI recency), and measures of suicide attempt history and emotional reactivity. Logistic regression analyses indicated that the INS contributed unique variance to the prediction of physical disfigurement (i.e., NSSI scarring) and clinically significant social anxiety, even after taking into account NSSI <span class="hlt">frequency</span>. Furthermore, the INS demonstrated divergent validity. Implications for research on NSSI disorder and clinical practice are discussed. PMID:28824214</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1983srai.reptQ....G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983srai.reptQ....G"><span>Semiconductor materials for high <span class="hlt">frequency</span> solid state sources</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grubin, H. L.</p> <p>1983-03-01</p> <p>The broad goal of the subject contract is to suggest candidate materials for high <span class="hlt">frequency</span> device operation. During the initial phase of the study, attention has been focused on defining the general role of the band structure and associated scattering processes in determining the response of semiconductors to transient high-speed electrical signals. Moments of the Boltzmann transport equation form the basis of the study, and the scattering rates define the semiconductor under study. The selection of semiconductor materials proceeds from a set of simple, yet significant, set of <span class="hlt">scaling</span> principles. During the first quarter <span class="hlt">scaling</span> was associated with what can formally be identified as velocity invariants, but which in more practical terms identifies the relative speed advantages of e.g., InP over GaAs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1817216C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1817216C"><span>Atmospheric Electric Field Measurements at 100 Hz and High <span class="hlt">Frequency</span> Electric Phenomena</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Conceição, Ricardo; Gonçalves da Silva, Hugo; Matthews, James; Bennett, Alec; Chubb, John</p> <p>2016-04-01</p> <p>Spectral response of Atmospheric Electric Potential Gradient (PG), symmetric to the Atmospheric Electric Field, gives important information about phenomena affecting these measurements with characteristic time-<span class="hlt">scales</span> that appear in the spectra as specific periodicities. This is the case of urban pollution that has a clear weekly dependence and reveals itself on PG measurements by a ~7 day periodicity (Silva et al., 2014). While long-term time-<span class="hlt">scales</span> (low <span class="hlt">frequencies</span>) have been exhaustively explored in literature, short-term time-<span class="hlt">scales</span> (high <span class="hlt">frequencies</span>), above 1 Hz, have comparatively received much less attention (Anisimov et al., 1999). This is mainly because of the technical difficulties related with the storage of such a huge amount of data (for 100 Hz sampling two days of data uses a ~1 Gb file) and the response degradation of the field-meters at such <span class="hlt">frequencies</span>. Nevertheless, important Electric Phenomena occurs for <span class="hlt">frequencies</span> above 1 Hz that are worth pursuing, e.g. the Schumann Resonances have a signature of worldwide thunderstorm activity at <span class="hlt">frequencies</span> that go from ~8 up to ~40 Hz. To that end the present work shows preliminary results on PG measurements at 100 Hz that took place on two clear-sky days (17th and 18th June 2015) on the South of Portugal, Évora (38.50° N, 7.91° W). The field-mill used is a JCI 131F installed in the University of Évora campus (at 2 m height) with a few trees and two buildings in its surroundings (~50 m away). This device was developed by John Chubb (Chubb, 2014) and manufactured by Chilworth (UK). It was calibrated in December 2013 and recent work by the author (who is honored in this study for his overwhelming contribution to atmospheric electricity) reveals basically a flat spectral response of the device up to <span class="hlt">frequencies</span> of 100 Hz (Chubb, 2015). This makes this device suitable for the study of High <span class="hlt">Frequency</span> Electric Phenomena. Anisimov, S.V., et al. (1999). On the generation and evolution of aeroelectric structures</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JaJAP..49i6601P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JaJAP..49i6601P"><span>Improvement of <span class="hlt">Frequency</span> Locking Algorithm for Atomic <span class="hlt">Frequency</span> Standards</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Young-Ho; Kang, Hoonsoo; Heyong Lee, Soo; Eon Park, Sang; Lee, Jong Koo; Lee, Ho Seong; Kwon, Taeg Yong</p> <p>2010-09-01</p> <p>The authors describe a novel method of <span class="hlt">frequency</span> locking algorithm for atomic <span class="hlt">frequency</span> standards. The new algorithm for locking the microwave <span class="hlt">frequency</span> to the Ramsey resonance is compared with the old one that had been employed in the cesium atomic beam <span class="hlt">frequency</span> standards such as NIST-7 and KRISS-1. Numerical simulations for testing the performance of the algorithm show that the new method has a noise filtering performance superior to the old one by a factor of 1.2 for the flicker signal noise and 1.4 for random-walk signal noise. The new algorithm can readily be used to enhance the <span class="hlt">frequency</span> stability for a digital servo employing the slow square wave <span class="hlt">frequency</span> modulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1026057','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1026057"><span>Cross-Layer Modeling Framework for Energy-Efficient Resilience</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-04-01</p> <p>functional block diagram of the software architecture of PEARL, which stands for: Power Efficient and Resilient Embedded Processing with Real - Time ... <span class="hlt">DVFS</span> ). The goal of the run- time manager is to minimize power consumption, while maintaining system resilience targets (on average) and meeting... real - time performance targets. The integrated performance, power and resilience models are nothing but the analytical modeling toolkit described in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15169131','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15169131"><span>Generation of zonal magnetic fields by low-<span class="hlt">frequency</span> dispersive electromagnetic waves in a nonuniform dusty magnetoplasma.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shukla, P K</p> <p>2004-04-01</p> <p>It is shown that zonal magnetic fields can be parametrically excited by low-<span class="hlt">frequency</span> dispersive driftlike compressional electromagnetic (DDCEM) modes in a nonuniform dusty magnetoplasma. For this purpose, we derive a pair of coupled equations which exhibits the nonlinear coupling between DDCEM modes and zonal magnetic fields. The coupled mode equations are Fourier analyzed to derive a nonlinear dispersion relation. The latter depicts that zonal magnetic fields are nonlinearly generated at the expense of the low-<span class="hlt">frequency</span> DDCEM wave energy. The relevance of our investigation to the transfer of energy from short <span class="hlt">scale</span> DDCEM waves to long <span class="hlt">scale</span> zonal magnetic field structures in dark molecular clouds is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148t4507M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148t4507M"><span>Atomistic interpretation of the ac-dc crossover <span class="hlt">frequency</span> in crystalline and glassy ionic conductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marple, M. A. T.; Avila-Paredes, H.; Kim, S.; Sen, S.</p> <p>2018-05-01</p> <p>A comprehensive analysis of the ionic dynamics in a wide variety of crystalline and glassy ionic conductors, obtained in recent studies using a combination of electrochemical impedance and nuclear magnetic resonance spectroscopic techniques, is presented. These results demonstrate that the crossover <span class="hlt">frequency</span>, between the <span class="hlt">frequency</span>-independent dc conductivity and the <span class="hlt">frequency</span>-dependent ac conductivity, corresponds to the time <span class="hlt">scale</span> of "successful" diffusive hops of the mobile ions between the trapping sites in the structure. These inter-site hops are typically compound in nature and consist of several elementary hops in the intervening region between the neighboring trapping sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29865839','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29865839"><span>Atomistic interpretation of the ac-dc crossover <span class="hlt">frequency</span> in crystalline and glassy ionic conductors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marple, M A T; Avila-Paredes, H; Kim, S; Sen, S</p> <p>2018-05-28</p> <p>A comprehensive analysis of the ionic dynamics in a wide variety of crystalline and glassy ionic conductors, obtained in recent studies using a combination of electrochemical impedance and nuclear magnetic resonance spectroscopic techniques, is presented. These results demonstrate that the crossover <span class="hlt">frequency</span>, between the <span class="hlt">frequency</span>-independent dc conductivity and the <span class="hlt">frequency</span>-dependent ac conductivity, corresponds to the time <span class="hlt">scale</span> of "successful" diffusive hops of the mobile ions between the trapping sites in the structure. These inter-site hops are typically compound in nature and consist of several elementary hops in the intervening region between the neighboring trapping sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28177924','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28177924"><span>Adapted wavelet transform improves time-<span class="hlt">frequency</span> representations: a study of auditory elicited P300-like event-related potentials in rats.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Richard, Nelly; Laursen, Bettina; Grupe, Morten; Drewes, Asbjørn M; Graversen, Carina; Sørensen, Helge B D; Bastlund, Jesper F</p> <p>2017-04-01</p> <p>Active auditory oddball paradigms are simple tone discrimination tasks used to study the P300 deflection of event-related potentials (ERPs). These ERPs may be quantified by time-<span class="hlt">frequency</span> analysis. As auditory stimuli cause early high <span class="hlt">frequency</span> and late low <span class="hlt">frequency</span> ERP oscillations, the continuous wavelet transform (CWT) is often chosen for decomposition due to its multi-resolution properties. However, as the conventional CWT traditionally applies only one mother wavelet to represent the entire spectrum, the time-<span class="hlt">frequency</span> resolution is not optimal across all <span class="hlt">scales</span>. To account for this, we developed and validated a novel method specifically refined to analyse P300-like ERPs in rats. An adapted CWT (aCWT) was implemented to preserve high time-<span class="hlt">frequency</span> resolution across all <span class="hlt">scales</span> by commissioning of multiple wavelets operating at different <span class="hlt">scales</span>. First, decomposition of simulated ERPs was illustrated using the classical CWT and the aCWT. Next, the two methods were applied to EEG recordings obtained from prefrontal cortex in rats performing a two-tone auditory discrimination task. While only early ERP <span class="hlt">frequency</span> changes between responses to target and non-target tones were detected by the CWT, both early and late changes were successfully described with strong accuracy by the aCWT in rat ERPs. Increased frontal gamma power and phase synchrony was observed particularly within theta and gamma <span class="hlt">frequency</span> bands during deviant tones. The study suggests superior performance of the aCWT over the CWT in terms of detailed quantification of time-<span class="hlt">frequency</span> properties of ERPs. Our methodological investigation indicates that accurate and complete assessment of time-<span class="hlt">frequency</span> components of short-time neural signals is feasible with the novel analysis approach which may be advantageous for characterisation of several types of evoked potentials in particularly rodents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JNEng..14b6012R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JNEng..14b6012R"><span>Adapted wavelet transform improves time-<span class="hlt">frequency</span> representations: a study of auditory elicited P300-like event-related potentials in rats</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Richard, Nelly; Laursen, Bettina; Grupe, Morten; Drewes, Asbjørn M.; Graversen, Carina; Sørensen, Helge B. D.; Bastlund, Jesper F.</p> <p>2017-04-01</p> <p>Objective. Active auditory oddball paradigms are simple tone discrimination tasks used to study the P300 deflection of event-related potentials (ERPs). These ERPs may be quantified by time-<span class="hlt">frequency</span> analysis. As auditory stimuli cause early high <span class="hlt">frequency</span> and late low <span class="hlt">frequency</span> ERP oscillations, the continuous wavelet transform (CWT) is often chosen for decomposition due to its multi-resolution properties. However, as the conventional CWT traditionally applies only one mother wavelet to represent the entire spectrum, the time-<span class="hlt">frequency</span> resolution is not optimal across all <span class="hlt">scales</span>. To account for this, we developed and validated a novel method specifically refined to analyse P300-like ERPs in rats. Approach. An adapted CWT (aCWT) was implemented to preserve high time-<span class="hlt">frequency</span> resolution across all <span class="hlt">scales</span> by commissioning of multiple wavelets operating at different <span class="hlt">scales</span>. First, decomposition of simulated ERPs was illustrated using the classical CWT and the aCWT. Next, the two methods were applied to EEG recordings obtained from prefrontal cortex in rats performing a two-tone auditory discrimination task. Main results. While only early ERP <span class="hlt">frequency</span> changes between responses to target and non-target tones were detected by the CWT, both early and late changes were successfully described with strong accuracy by the aCWT in rat ERPs. Increased frontal gamma power and phase synchrony was observed particularly within theta and gamma <span class="hlt">frequency</span> bands during deviant tones. Significance. The study suggests superior performance of the aCWT over the CWT in terms of detailed quantification of time-<span class="hlt">frequency</span> properties of ERPs. Our methodological investigation indicates that accurate and complete assessment of time-<span class="hlt">frequency</span> components of short-time neural signals is feasible with the novel analysis approach which may be advantageous for characterisation of several types of evoked potentials in particularly rodents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1340286','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1340286"><span>Multimachine data–based prediction of high-<span class="hlt">frequency</span> sensor signal noise for resistive wall mode control in ITER</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Liu, Yueqiang; Sabbagh, S. A.; Chapman, I. T.</p> <p></p> <p>The high-<span class="hlt">frequency</span> noise measured by magnetic sensors, at levels above the typical <span class="hlt">frequency</span> of resistive wall modes, is analyzed across a range of present tokamak devices including DIII-D, JET, MAST, ASDEX Upgrade, JT-60U, and NSTX. A high-pass filter enables identification of the noise component with Gaussian-like statistics that shares certain common characteristics in all devices considered. A conservative prediction is made for ITER plasma operation of the high-<span class="hlt">frequency</span> noise component of the sensor signals, to be used for resistive wall mode feedback stabilization, based on the multimachine database. The predicted root-mean-square n = 1 (n is the toroidal mode number)more » noise level is 10 4 to 10 5 G/s for the voltage signal, and 0.1 to 1 G for the perturbed magnetic field signal. The lower cutoff <span class="hlt">frequency</span> of the Gaussian pickup noise <span class="hlt">scales</span> linearly with the sampling <span class="hlt">frequency</span>, with a <span class="hlt">scaling</span> coefficient of about 0.1. As a result, these basic noise characteristics should be useful for the modeling-based design of the feedback control system for the resistive wall mode in ITER.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1340286-multimachine-databased-prediction-high-frequency-sensor-signal-noise-resistive-wall-mode-control-iter','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1340286-multimachine-databased-prediction-high-frequency-sensor-signal-noise-resistive-wall-mode-control-iter"><span>Multimachine data–based prediction of high-<span class="hlt">frequency</span> sensor signal noise for resistive wall mode control in ITER</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Liu, Yueqiang; Sabbagh, S. A.; Chapman, I. T.; ...</p> <p>2017-03-27</p> <p>The high-<span class="hlt">frequency</span> noise measured by magnetic sensors, at levels above the typical <span class="hlt">frequency</span> of resistive wall modes, is analyzed across a range of present tokamak devices including DIII-D, JET, MAST, ASDEX Upgrade, JT-60U, and NSTX. A high-pass filter enables identification of the noise component with Gaussian-like statistics that shares certain common characteristics in all devices considered. A conservative prediction is made for ITER plasma operation of the high-<span class="hlt">frequency</span> noise component of the sensor signals, to be used for resistive wall mode feedback stabilization, based on the multimachine database. The predicted root-mean-square n = 1 (n is the toroidal mode number)more » noise level is 10 4 to 10 5 G/s for the voltage signal, and 0.1 to 1 G for the perturbed magnetic field signal. The lower cutoff <span class="hlt">frequency</span> of the Gaussian pickup noise <span class="hlt">scales</span> linearly with the sampling <span class="hlt">frequency</span>, with a <span class="hlt">scaling</span> coefficient of about 0.1. As a result, these basic noise characteristics should be useful for the modeling-based design of the feedback control system for the resistive wall mode in ITER.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26427063','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26427063"><span>Intrinsic Multi-<span class="hlt">Scale</span> Dynamic Behaviors of Complex Financial Systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ouyang, Fang-Yan; Zheng, Bo; Jiang, Xiong-Fei</p> <p>2015-01-01</p> <p>The empirical mode decomposition is applied to analyze the intrinsic multi-<span class="hlt">scale</span> dynamic behaviors of complex financial systems. In this approach, the time series of the price returns of each stock is decomposed into a small number of intrinsic mode functions, which represent the price motion from high <span class="hlt">frequency</span> to low <span class="hlt">frequency</span>. These intrinsic mode functions are then grouped into three modes, i.e., the fast mode, medium mode and slow mode. The probability distribution of returns and auto-correlation of volatilities for the fast and medium modes exhibit similar behaviors as those of the full time series, i.e., these characteristics are rather robust in multi time <span class="hlt">scale</span>. However, the cross-correlation between individual stocks and the return-volatility correlation are time <span class="hlt">scale</span> dependent. The structure of business sectors is mainly governed by the fast mode when returns are sampled at a couple of days, while by the medium mode when returns are sampled at dozens of days. More importantly, the leverage and anti-leverage effects are dominated by the medium mode.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4591268','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4591268"><span>Intrinsic Multi-<span class="hlt">Scale</span> Dynamic Behaviors of Complex Financial 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>Ouyang, Fang-Yan; Zheng, Bo; Jiang, Xiong-Fei</p> <p>2015-01-01</p> <p>The empirical mode decomposition is applied to analyze the intrinsic multi-<span class="hlt">scale</span> dynamic behaviors of complex financial systems. In this approach, the time series of the price returns of each stock is decomposed into a small number of intrinsic mode functions, which represent the price motion from high <span class="hlt">frequency</span> to low <span class="hlt">frequency</span>. These intrinsic mode functions are then grouped into three modes, i.e., the fast mode, medium mode and slow mode. The probability distribution of returns and auto-correlation of volatilities for the fast and medium modes exhibit similar behaviors as those of the full time series, i.e., these characteristics are rather robust in multi time <span class="hlt">scale</span>. However, the cross-correlation between individual stocks and the return-volatility correlation are time <span class="hlt">scale</span> dependent. The structure of business sectors is mainly governed by the fast mode when returns are sampled at a couple of days, while by the medium mode when returns are sampled at dozens of days. More importantly, the leverage and anti-leverage effects are dominated by the medium mode. PMID:26427063</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1423976-efficient-multiscale-finite-element-method-frequency-domain-seismic-wave-propagation','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1423976-efficient-multiscale-finite-element-method-frequency-domain-seismic-wave-propagation"><span>An Efficient Multiscale Finite-Element Method for <span class="hlt">Frequency</span>-Domain Seismic Wave Propagation</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Gao, Kai; Fu, Shubin; Chung, Eric T.</p> <p>2018-02-13</p> <p>The <span class="hlt">frequency</span>-domain seismic-wave equation, that is, the Helmholtz equation, has many important applications in seismological studies, yet is very challenging to solve, particularly for large geological models. Iterative solvers, domain decomposition, or parallel strategies can partially alleviate the computational burden, but these approaches may still encounter nontrivial difficulties in complex geological models where a sufficiently fine mesh is required to represent the fine-<span class="hlt">scale</span> heterogeneities. We develop a novel numerical method to solve the <span class="hlt">frequency</span>-domain acoustic wave equation on the basis of the multiscale finite-element theory. We discretize a heterogeneous model with a coarse mesh and employ carefully constructed high-order multiscalemore » basis functions to form the basis space for the coarse mesh. Solved from medium- and <span class="hlt">frequency</span>-dependent local problems, these multiscale basis functions can effectively capture themedium’s fine-<span class="hlt">scale</span> heterogeneity and the source’s <span class="hlt">frequency</span> information, leading to a discrete system matrix with a much smaller dimension compared with those from conventional methods.We then obtain an accurate solution to the acoustic Helmholtz equation by solving only a small linear system instead of a large linear system constructed on the fine mesh in conventional methods.We verify our new method using several models of complicated heterogeneities, and the results show that our new multiscale method can solve the Helmholtz equation in complex models with high accuracy and extremely low computational costs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1423976-efficient-multiscale-finite-element-method-frequency-domain-seismic-wave-propagation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1423976-efficient-multiscale-finite-element-method-frequency-domain-seismic-wave-propagation"><span>An Efficient Multiscale Finite-Element Method for <span class="hlt">Frequency</span>-Domain Seismic Wave Propagation</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>Gao, Kai; Fu, Shubin; Chung, Eric T.</p> <p></p> <p>The <span class="hlt">frequency</span>-domain seismic-wave equation, that is, the Helmholtz equation, has many important applications in seismological studies, yet is very challenging to solve, particularly for large geological models. Iterative solvers, domain decomposition, or parallel strategies can partially alleviate the computational burden, but these approaches may still encounter nontrivial difficulties in complex geological models where a sufficiently fine mesh is required to represent the fine-<span class="hlt">scale</span> heterogeneities. We develop a novel numerical method to solve the <span class="hlt">frequency</span>-domain acoustic wave equation on the basis of the multiscale finite-element theory. We discretize a heterogeneous model with a coarse mesh and employ carefully constructed high-order multiscalemore » basis functions to form the basis space for the coarse mesh. Solved from medium- and <span class="hlt">frequency</span>-dependent local problems, these multiscale basis functions can effectively capture themedium’s fine-<span class="hlt">scale</span> heterogeneity and the source’s <span class="hlt">frequency</span> information, leading to a discrete system matrix with a much smaller dimension compared with those from conventional methods.We then obtain an accurate solution to the acoustic Helmholtz equation by solving only a small linear system instead of a large linear system constructed on the fine mesh in conventional methods.We verify our new method using several models of complicated heterogeneities, and the results show that our new multiscale method can solve the Helmholtz equation in complex models with high accuracy and extremely low computational costs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24872925','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24872925"><span><span class="hlt">Frequency</span> Preference Response to Oscillatory Inputs in Two-dimensional Neural Models: A Geometric Approach to Subthreshold Amplitude and Phase Resonance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rotstein, Horacio G</p> <p>2014-01-01</p> <p>We investigate the dynamic mechanisms of generation of subthreshold and phase resonance in two-dimensional linear and linearized biophysical (conductance-based) models, and we extend our analysis to account for the effect of simple, but not necessarily weak, types of nonlinearities. Subthreshold resonance refers to the ability of neurons to exhibit a peak in their voltage amplitude response to oscillatory input currents at a preferred non-zero (resonant) <span class="hlt">frequency</span>. Phase-resonance refers to the ability of neurons to exhibit a zero-phase (or zero-phase-shift) response to oscillatory input currents at a non-zero (phase-resonant) <span class="hlt">frequency</span>. We adapt the classical phase-plane analysis approach to account for the dynamic effects of oscillatory inputs and develop a tool, the envelope-plane diagrams, that captures the role that conductances and time <span class="hlt">scales</span> play in amplifying the voltage response at the resonant <span class="hlt">frequency</span> band as compared to smaller and larger <span class="hlt">frequencies</span>. We use envelope-plane diagrams in our analysis. We explain why the resonance phenomena do not necessarily arise from the presence of imaginary eigenvalues at rest, but rather they emerge from the interplay of the intrinsic and input time <span class="hlt">scales</span>. We further explain why an increase in the time-<span class="hlt">scale</span> separation causes an amplification of the voltage response in addition to shifting the resonant and phase-resonant <span class="hlt">frequencies</span>. This is of fundamental importance for neural models since neurons typically exhibit a strong separation of time <span class="hlt">scales</span>. We extend this approach to explain the effects of nonlinearities on both resonance and phase-resonance. We demonstrate that nonlinearities in the voltage equation cause amplifications of the voltage response and shifts in the resonant and phase-resonant <span class="hlt">frequencies</span> that are not predicted by the corresponding linearized model. The differences between the nonlinear response and the linear prediction increase with increasing levels of the time <span class="hlt">scale</span> separation between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750003212','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750003212"><span>Digital <span class="hlt">frequency</span> control of satellite <span class="hlt">frequency</span> standards. [Defense Navigation Satellites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nichols, S. A.</p> <p>1973-01-01</p> <p>In the <span class="hlt">Frequency</span> and Time Standard Development Program of the TIMATION System, a new miniaturized rubidium vapor <span class="hlt">frequency</span> standard has been tested and analyzed for possible use on the TIMATION 3A launch, as part of the Defense Navigation Satellite Development Program. The design and construction of a digital <span class="hlt">frequency</span> control was required to remotely control this rubidium vapor <span class="hlt">frequency</span> standard as well as the quartz oscillator in current use. This control must be capable of accepting commands from a satellite telemetry system, verify that the correct commands have been sent and control the <span class="hlt">frequency</span> to the requirements of the system. Several modifications must be performed to the rubidium vapor <span class="hlt">frequency</span> standard to allow it to be compatible with the digital <span class="hlt">frequency</span> control. These include the addition of a varactor to voltage tune the coarse range of the flywheel oscillator, and a modification to supply the C field current externally. The digital <span class="hlt">frequency</span> control for the rubidium vapor <span class="hlt">frequency</span> standard has been successfully tested in prototype form.</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('https://ntrs.nasa.gov/search.jsp?R=20040081284&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbackground%2Bwind','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040081284&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dbackground%2Bwind"><span>Towards a High Temporal <span class="hlt">Frequency</span> Grass Canopy Thermal IR Model for Background Signatures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ballard, Jerrell R., Jr.; Smith, James A.; Koenig, George G.</p> <p>2004-01-01</p> <p>In this paper, we present our first results towards understanding high temporal <span class="hlt">frequency</span> thermal infrared response from a dense plant canopy and compare the application of our model, driven both by slowly varying, time-averaged meteorological conditions and by high <span class="hlt">frequency</span> measurements of local and within canopy profiles of relative humidity and wind speed, to high <span class="hlt">frequency</span> thermal infrared observations. Previously, we have employed three-dimensional ray tracing to compute the intercepted and scattered radiation fluxes and for final scene rendering. For the turbulent fluxes, we employed simple resistance models for latent and sensible heat with one-dimensional profiles of relative humidity and wind speed. Our modeling approach has proven successful in capturing the directional and diurnal variation in background thermal infrared signatures. We hypothesize that at these <span class="hlt">scales</span>, where the model is typically driven by time-averaged, local meteorological conditions, the primary source of thermal variance arises from the spatial distribution of sunlit and shaded foliage elements within the canopy and the associated radiative interactions. In recent experiments, we have begun to focus on the high temporal <span class="hlt">frequency</span> response of plant canopies in the thermal infrared at 1 second to 5 minute intervals. At these <span class="hlt">scales</span>, we hypothesize turbulent mixing plays a more dominant role. Our results indicate that in the high <span class="hlt">frequency</span> domain, the vertical profile of temperature change is tightly coupled to the within canopy wind speed In the results reported here, the canopy cools from the top down with increased wind velocities and heats from the bottom up at low wind velocities. .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24618529','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24618529"><span>Ultrasonic pilot-<span class="hlt">scale</span> reactor for enzymatic bleaching of cotton fabrics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gonçalves, Idalina; Herrero-Yniesta, Victor; Perales Arce, Iratxe; Escrigas Castañeda, Monica; Cavaco-Paulo, Artur; Silva, Carla</p> <p>2014-07-01</p> <p>The potential of ultrasound-assisted technology has been demonstrated by several laboratory <span class="hlt">scale</span> studies. However, their successful industrial <span class="hlt">scaling</span>-up is still a challenge due to the limited pilot and commercial sonochemical reactors. In this work, a pilot reactor for laccase-hydrogen peroxide cotton bleaching assisted by ultrasound was <span class="hlt">scaled</span>-up. For this purpose, an existing dyeing machine was transformed and adapted by including piezoelectric ultrasonic devices. Laboratory experiments demonstrated that both low <span class="hlt">frequency</span>, high power (22 kHz, 2100 W) and high <span class="hlt">frequency</span>, low power ultrasounds (850 kHz, 400 W) were required to achieve satisfactory results. Standard half (4 g/L H2O2 at 90 °C for 60 min) and optical (8 g/L H2O2 at 103 °C for 40 min) cotton bleaching processes were used as references. Two sequential stages were established for cotton bleaching: (1) laccase pretreatment assisted by high <span class="hlt">frequency</span> ultrasound (850 kHz, 400 W) and (2) bleaching using high power ultrasound (22 kHz, 2100 W). When compared with conventional methods, combined laccase-hydrogen peroxide cotton bleaching with ultrasound energy improved the whitening effectiveness. Subsequently, less energy (temperature) and chemicals (hydrogen peroxide) were needed for cotton bleaching thus resulting in costs reduction. This technology allowed the combination of enzyme and hydrogen peroxide treatment in a continuous process. The developed pilot-<span class="hlt">scale</span> reactor offers an enhancement of the cotton bleaching process with lower environmental impact as well as a better performance of further finishing operations. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160007357&hterms=cosmology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcosmology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160007357&hterms=cosmology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcosmology"><span>Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) Focal Plane Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chuss, D. T.; Ali, A.; Amiri, M.; Appel, J.; Bennett, C. L.; Colazo, F.; Denis, K. L.; Dunner, R.; Essinger-Hileman, T.; Eimer, J.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160007357'); toggleEditAbsImage('author_20160007357_show'); toggleEditAbsImage('author_20160007357_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160007357_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160007357_hide"></p> <p>2015-01-01</p> <p>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) will measure the polarization of the Cosmic Microwave Background to search for and characterize the polarized signature of inflation. CLASS will operate from the Atacama Desert and observe approx.70% of the sky. A variable-delay polarization modulator provides modulation of the polarization at approx.10Hz to suppress the 1/f noise of the atmosphere and enable the measurement of the large angular <span class="hlt">scale</span> polarization modes. The measurement of the inflationary signal across angular <span class="hlt">scales</span> that spans both the recombination and reionization features allows a test of the predicted shape of the polarized angular power spectra in addition to a measurement of the energy <span class="hlt">scale</span> of inflation. CLASS is an array of telescopes covering <span class="hlt">frequencies</span> of 38, 93, 148, and 217 GHz. These <span class="hlt">frequencies</span> straddle the foreground minimum and thus allow the extraction of foregrounds from the primordial signal. Each focal plane contains feedhorn-coupled transition-edge sensors that simultaneously detect two orthogonal linear polarizations. The use of single-crystal silicon as the dielectric for the on-chip transmission lines enables both high efficiency and uniformity in fabrication. Integrated band definition has been implemented that both controls the bandpass of the single-mode transmission on the chip and prevents stray light from coupling to the detectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JLTP..184..759C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JLTP..184..759C"><span>Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) Focal Plane Development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuss, D. T.; Ali, A.; Amiri, M.; Appel, J.; Bennett, C. L.; Colazo, F.; Denis, K. L.; Dünner, R.; Essinger-Hileman, T.; Eimer, J.; Fluxa, P.; Gothe, D.; Halpern, M.; Harrington, K.; Hilton, G.; Hinshaw, G.; Hubmayr, J.; Iuliano, J.; Marriage, T. A.; Miller, N.; Moseley, S. H.; Mumby, G.; Petroff, M.; Reintsema, C.; Rostem, K.; U-Yen, K.; Watts, D.; Wagner, E.; Wollack, E. J.; Xu, Z.; Zeng, L.</p> <p>2016-08-01</p> <p>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) will measure the polarization of the Cosmic Microwave Background to search for and characterize the polarized signature of inflation. CLASS will operate from the Atacama Desert and observe ˜ 70 % of the sky. A variable-delay polarization modulator provides modulation of the polarization at ˜ 10 Hz to suppress the 1/ f noise of the atmosphere and enable the measurement of the large angular <span class="hlt">scale</span> polarization modes. The measurement of the inflationary signal across angular <span class="hlt">scales</span> that spans both the recombination and reionization features allows a test of the predicted shape of the polarized angular power spectra in addition to a measurement of the energy <span class="hlt">scale</span> of inflation. CLASS is an array of telescopes covering <span class="hlt">frequencies</span> of 38, 93, 148, and 217 GHz. These <span class="hlt">frequencies</span> straddle the foreground minimum and thus allow the extraction of foregrounds from the primordial signal. Each focal plane contains feedhorn-coupled transition-edge sensors that simultaneously detect two orthogonal linear polarizations. The use of single-crystal silicon as the dielectric for the on-chip transmission lines enables both high efficiency and uniformity in fabrication. Integrated band definition has been implemented that both controls the bandpass of the single-mode transmission on the chip and prevents stray light from coupling to the detectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4272385','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4272385"><span>Solution pH change in non-uniform alternating current electric fields at <span class="hlt">frequencies</span> above the electrode charging <span class="hlt">frequency</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>An, Ran; Massa, Katherine</p> <p>2014-01-01</p> <p>AC Faradaic reactions have been reported as a mechanism inducing non-ideal phenomena such as flow reversal and cell deformation in electrokinetic microfluidic systems. Prior published work described experiments in parallel electrode arrays below the electrode charging <span class="hlt">frequency</span> (fc), the <span class="hlt">frequency</span> for electrical double layer charging at the electrode. However, 2D spatially non-uniform AC electric fields are required for applications such as in plane AC electroosmosis, AC electrothermal pumps, and dielectrophoresis. Many microscale experimental applications utilize AC <span class="hlt">frequencies</span> around or above fc. In this work, a pH sensitive fluorescein sodium salt dye was used to detect [H+] as an indicator of Faradaic reactions in aqueous solutions within non-uniform AC electric fields. Comparison experiments with (a) parallel (2D uniform fields) electrodes and (b) organic media were employed to deduce the electrode charging mechanism at 5 kHz (1.5fc). Time dependency analysis illustrated that Faradaic reactions exist above the theoretically predicted electrode charging <span class="hlt">frequency</span>. Spatial analysis showed [H+] varied spatially due to electric field non-uniformities and local pH changed at length <span class="hlt">scales</span> greater than 50 μm away from the electrode surface. Thus, non-uniform AC fields yielded spatially varied pH gradients as a direct consequence of ion path length differences while uniform fields did not yield pH gradients; the latter is consistent with prior published data. <span class="hlt">Frequency</span> dependence was examined from 5 kHz to 12 kHz at 5.5 Vpp potential, and voltage dependency was explored from 3.5 to 7.5 Vpp at 5 kHz. Results suggest that Faradaic reactions can still proceed within electrochemical systems in the absence of well-established electrical double layers. This work also illustrates that in microfluidic systems, spatial medium variations must be considered as a function of experiment time, initial medium conditions, electric signal potential, <span class="hlt">frequency</span>, and spatial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919159T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919159T"><span>Evaluation of Hydrologic and Meteorological Impacts on Dengue Fever Incidences in Southern Taiwan using Time- <span class="hlt">Frequency</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>Tsai, Christina; Yeh, Ting-Gu</p> <p>2017-04-01</p> <p>Extreme weather events are occurring more frequently as a result of climate change. Recently dengue fever has become a serious issue in southern Taiwan. It may have characteristic temporal <span class="hlt">scales</span> that can be identified. Some researchers have hypothesized that dengue fever incidences are related to climate change. This study applies time-<span class="hlt">frequency</span> analysis to time series data concerning dengue fever and hydrologic and meteorological variables. Results of three time-<span class="hlt">frequency</span> analytical methods - the Hilbert Huang transform (HHT), the Wavelet Transform (WT) and the Short Time Fourier Transform (STFT) are compared and discussed. A more effective time-<span class="hlt">frequency</span> analysis method will be identified to analyze relevant time series data. The most influential time <span class="hlt">scales</span> of hydrologic and meteorological variables that are associated with dengue fever are determined. Finally, the linkage between hydrologic/meteorological factors and dengue fever incidences can be established.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPhL.110p1909C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPhL.110p1909C"><span>Implementation of acoustic demultiplexing with membrane-type metasurface in low <span class="hlt">frequency</span> range</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Xing; Liu, Peng; Hou, Zewei; Pei, Yongmao</p> <p>2017-04-01</p> <p>Wavelength division multiplexing technology, adopted to increase the information density, plays a significant role in optical communication. However, in acoustics, a similar function can be hardly implemented due to the weak dispersion in natural acoustic materials. Here, an acoustic demultiplexer, based on the concept of metasurfaces, is proposed for splitting acoustic waves and propagating along different trajectories in a low <span class="hlt">frequency</span> range. An acoustic metasurface, containing multiple resonant units, is designed with various phase profiles for different <span class="hlt">frequencies</span>. Originating from the highly dispersive properties, the resonant units are independent and merely work in the vicinity of their resonant <span class="hlt">frequencies</span>. Therefore, by combing multiple resonant units appropriately, the phenomena of anomalous reflection, acoustic focusing, and acoustic wave bending can occur in different <span class="hlt">frequencies</span>. The proposed acoustic demultiplexer has advantages on the subwavelength <span class="hlt">scale</span> and the versatility in wave control, providing a strategy for separating acoustic waves with different Fourier components.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26134588','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26134588"><span>Radio <span class="hlt">Frequency</span> Transistors and Circuits Based on CVD MoS2.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sanne, Atresh; Ghosh, Rudresh; Rai, Amritesh; Yogeesh, Maruthi Nagavalli; Shin, Seung Heon; Sharma, Ankit; Jarvis, Karalee; Mathew, Leo; Rao, Rajesh; Akinwande, Deji; Banerjee, Sanjay</p> <p>2015-08-12</p> <p>We report on the gigahertz radio <span class="hlt">frequency</span> (RF) performance of chemical vapor deposited (CVD) monolayer MoS2 field-effect transistors (FETs). Initial DC characterizations of fabricated MoS2 FETs yielded current densities exceeding 200 μA/μm and maximum transconductance of 38 μS/μm. A contact resistance corrected low-field mobility of 55 cm(2)/(V s) was achieved. Radio <span class="hlt">frequency</span> FETs were fabricated in the ground-signal-ground (GSG) layout, and standard de-embedding techniques were applied. Operating at the peak transconductance, we obtain short-circuit current-gain intrinsic cutoff <span class="hlt">frequency</span>, fT, of 6.7 GHz and maximum intrinsic oscillation <span class="hlt">frequency</span>, fmax, of 5.3 GHz for a device with a gate length of 250 nm. The MoS2 device afforded an extrinsic voltage gain Av of 6 dB at 100 MHz with voltage amplification until 3 GHz. With the as-measured <span class="hlt">frequency</span> performance of CVD MoS2, we provide the first demonstration of a common-source (CS) amplifier with voltage gain of 14 dB and an active <span class="hlt">frequency</span> mixer with conversion gain of -15 dB. Our results of gigahertz <span class="hlt">frequency</span> performance as well as analog circuit operation show that large area CVD MoS2 may be suitable for industrial-<span class="hlt">scale</span> electronic applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995AAS...187.2403C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995AAS...187.2403C"><span>Large-<span class="hlt">Scale</span> Outflows in Seyfert Galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colbert, E. J. M.; Baum, S. A.</p> <p>1995-12-01</p> <p>\\catcode`\\@=11 \\ialign{m @th#1hfil ##hfil \\crcr#2\\crcr\\sim\\crcr}}} \\catcode`\\@=12 Highly collimated outflows extend out to Mpc <span class="hlt">scales</span> in many radio-loud active galaxies. In Seyfert galaxies, which are radio-quiet, the outflows extend out to kpc <span class="hlt">scales</span> and do not appear to be as highly collimated. In order to study the nature of large-<span class="hlt">scale</span> (>~1 kpc) outflows in Seyferts, we have conducted optical, radio and X-ray surveys of a distance-limited sample of 22 edge-on Seyfert galaxies. Results of the optical emission-line imaging and spectroscopic survey imply that large-<span class="hlt">scale</span> outflows are present in >~{{1} /{4}} of all Seyferts. The radio (VLA) and X-ray (ROSAT) surveys show that large-<span class="hlt">scale</span> radio and X-ray emission is present at about the same <span class="hlt">frequency</span>. Kinetic luminosities of the outflows in Seyferts are comparable to those in starburst-driven superwinds. Large-<span class="hlt">scale</span> radio sources in Seyferts appear diffuse, but do not resemble radio halos found in some edge-on starburst galaxies (e.g. M82). We discuss the feasibility of the outflows being powered by the active nucleus (e.g. a jet) or a circumnuclear starburst.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5477P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5477P"><span>How to measure the thickness of dirty, wet Himalayan glaciers with low-<span class="hlt">frequency</span> radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pritchard, Hamish; Mayer, Christoph; Lambrecht, Astrid</p> <p>2017-04-01</p> <p>High Mountain Asia holds 90,000 glaciers of which only around ten have any ice thickness measurements at all, and on any one glacier these tend to be sparsely distributed and not well suited to calculating glacier ice volume. Existing regional ice volume estimates come from indirect methods (based on area-volume <span class="hlt">scaling</span> or modelled ice flux) that are poorly constrained in this region and so have a wide spread (e.g., 1670 to 6500 km3 (Bolch et al., 2012; Huss and Faranotti, 2012)). Sufficiently extensive measurements of ice thickness can be used to calculate ice volumes directly, or can be used to calibrate and hence improve the indirect estimates. Unfortunately, measuring ice thickness on such glaciers on a useful <span class="hlt">scale</span> is difficult. They are often remote with very rough, water-logged and debris-covered ablation areas, a lossy environment for radar and quite different to clean and cold polar glaciers that lend themselves well to rapid radar surveying by snowmobile or aeroplane. A possible solution is to develop a low-<span class="hlt">frequency</span>, helicopter-borne radar that can access remote mountain valleys and penetrate to the beds of the thickest of these mountain glaciers. But the lower the <span class="hlt">frequency</span>, the longer the dipole and the more cumbersome the radar: what <span class="hlt">frequency</span> do we need to detect the bed? Here we report results from pilot studies on the ground in the Langtang Valley and on Ngozumpa, Nepal's largest glacier, that show how bed detectability depends on <span class="hlt">frequency</span> both in terms of signal attenuation and clutter, and what this means for a planned regional-<span class="hlt">scale</span> glacier thickness surveys.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRB..112.3204M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRB..112.3204M"><span>Poroelastic finite difference modeling of seismic attenuation and dispersion due to mesoscopic-<span class="hlt">scale</span> heterogeneity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Masson, Y. J.; Pride, S. R.</p> <p>2007-03-01</p> <p>Seismic attenuation and dispersion are numerically determined for computer-generated porous materials that contain arbitrary amounts of mesoscopic-<span class="hlt">scale</span> heterogeneity in the porous continuum properties. The local equations used to determine the poroelastic response within such materials are those of Biot (1962). Upon applying a step change in stress to samples containing mesoscopic-<span class="hlt">scale</span> heterogeneity, the poroelastic response is determined using finite difference modeling, and the average strain throughout the sample computed, along with the effective complex and <span class="hlt">frequency</span>-dependent elastic moduli of the sample. The ratio of the imaginary and real parts of these moduli determines the attenuation as a function of <span class="hlt">frequency</span> associated with the modes of applied stress (pure compression and pure shear). By having a wide range of heterogeneity present, there exists a wide range of relaxation <span class="hlt">frequencies</span> in the response with the result that the curves of attenuation as a function of <span class="hlt">frequency</span> are broader than in existing analytical theories based on a single relaxation <span class="hlt">frequency</span>. Analytical explanations are given for the various high-<span class="hlt">frequency</span> and low-<span class="hlt">frequency</span> asymptotic behavior observed in the numerical simulations. It is also shown that the overall level of attenuation of a given sample is proportional to the square of the incompressibility contrasts locally present.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT.......105M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT.......105M"><span>A multi-<span class="hlt">scale</span> model for geared transmission aero-thermodynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McIntyre, Sean M.</p> <p></p> <p>A multi-<span class="hlt">scale</span>, multi-physics computational tool for the simulation of high-per- formance gearbox aero-thermodynamics was developed and applied to equilibrium and pathological loss-of-lubrication performance simulation. The physical processes at play in these systems include multiphase compressible ow of the air and lubricant within the gearbox, meshing kinematics and tribology, as well as heat transfer by conduction, and free and forced convection. These physics are coupled across their representative space and time <span class="hlt">scales</span> in the computational framework developed in this dissertation. These <span class="hlt">scales</span> span eight orders of magnitude, from the thermal response of the full gearbox O(100 m; 10 2 s), through effects at the tooth passage time <span class="hlt">scale</span> O(10-2 m; 10-4 s), down to tribological effects on the meshing gear teeth O(10-6 m; 10-6 s). Direct numerical simulation of these coupled physics and <span class="hlt">scales</span> is intractable. Accordingly, a <span class="hlt">scale</span>-segregated simulation strategy was developed by partitioning and treating the contributing physical mechanisms as sub-problems, each with associated space and time <span class="hlt">scales</span>, and appropriate coupling mechanisms. These are: (1) the long time <span class="hlt">scale</span> thermal response of the system, (2) the multiphase (air, droplets, and film) aerodynamic flow and convective heat transfer within the gearbox, (3) the high-<span class="hlt">frequency</span>, time-periodic thermal effects of gear tooth heating while in mesh and its subsequent cooling through the rest of rotation, (4) meshing effects including tribology and contact mechanics. The overarching goal of this dissertation was to develop software and analysis procedures for gearbox loss-of-lubrication performance. To accommodate these four physical effects and their coupling, each is treated in the CFD code as a sub problem. These physics modules are coupled algorithmically. Specifically, the high- <span class="hlt">frequency</span> conduction analysis derives its local heat transfer coefficient and near-wall air temperature boundary conditions from a quasi</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1339504-frequency-support-pmsg-wtg-based-improved-inertial-control','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1339504-frequency-support-pmsg-wtg-based-improved-inertial-control"><span><span class="hlt">Frequency</span> Support of PMSG-WTG Based on Improved Inertial Control</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>Wu, Z.; Wang, X.; Gao, W.</p> <p>2016-11-14</p> <p>With increasing integrations of large-<span class="hlt">scale</span> systems based on permanent magnet synchronous generator wind turbine generators (PMSG-WTGs), the overall inertial response of a power system will tend to deteriorate as a result of the decoupling of rotor speed and grid <span class="hlt">frequency</span> through the power converter as well as the scheduled retirement of conventional synchronous generators. Thus, PMSG-WTGs can provide value to an electric grid by contributing to the system's inertial response by utilizing the inherent kinetic energy stored in their rotating masses and fast power control. In this work, an improved inertial control method based on the maximum power point trackingmore » operation curve is introduced to enhance the overall <span class="hlt">frequency</span> support capability of PMSG-WTGs in the case of large supply-demand imbalances. Moreover, this method is implemented in the CART2-PMSG integrated model in MATLAB/Simulink to investigate its impact on the wind turbine's structural loads during the inertial response process. Simulation results indicate that the proposed method can effectively reduce the <span class="hlt">frequency</span> nadir, arrest the rate of change of <span class="hlt">frequency</span>, and mitigate the secondary <span class="hlt">frequency</span> drop while imposing no negative impact on the major mechanical components of the wind turbine.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Nanot..27t5501M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Nanot..27t5501M"><span>Sustaining GHz oscillation of carbon nanotube based oscillators via a MHz <span class="hlt">frequency</span> excitation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Motevalli, Benyamin; Taherifar, Neda; Zhe Liu, Jefferson</p> <p>2016-05-01</p> <p>There have been intensive studies to investigate the properties of gigahertz nano-oscillators based on multi-walled carbon nanotubes (MWCNTs). Many of these studies, however, revealed that the unique telescopic translational oscillations in such devices would damp quickly due to various energy dissipation mechanisms. This challenge remains the primary obstacle against its practical applications. Herein, we propose a design concept in which a GHz oscillation could be re-excited by a MHz mechanical motion. This design involves a triple-walled CNT, in which sliding of the longer inner tube at a MHz <span class="hlt">frequency</span> can re-excite and sustain a GHz oscillation of the shorter middle tube. Our molecular dynamics (MD) simulations prove this design concept at ˜10 nm <span class="hlt">scale</span>. A mathematical model is developed to explore the feasibility at a larger size <span class="hlt">scale</span>. As an example, in an oscillatory system with the CNT’s length above 100 nm, the high oscillatory <span class="hlt">frequency</span> range of 1.8-3.3 GHz could be excited by moving the inner tube at a much lower <span class="hlt">frequency</span> of 53.4 MHz. This design concept together with the mechanical model could energize the development of GHz nano-oscillators in miniaturized electro-mechanical devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24260117','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24260117"><span><span class="hlt">Scale</span> effects between body size and limb design in quadrupedal mammals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kilbourne, Brandon M; Hoffman, Louwrens C</p> <p>2013-01-01</p> <p>Recently the metabolic cost of swinging the limbs has been found to be much greater than previously thought, raising the possibility that limb rotational inertia influences the energetics of locomotion. Larger mammals have a lower mass-specific cost of transport than smaller mammals. The <span class="hlt">scaling</span> of the mass-specific cost of transport is partly explained by decreasing stride <span class="hlt">frequency</span> with increasing body size; however, it is unknown if limb rotational inertia also influences the mass-specific cost of transport. Limb length and inertial properties--limb mass, center of mass (COM) position, moment of inertia, radius of gyration, and natural <span class="hlt">frequency</span>--were measured in 44 species of terrestrial mammals, spanning eight taxonomic orders. Limb length increases disproportionately with body mass via positive allometry (length ∝ body mass(0.40)); the positive allometry of limb length may help explain the <span class="hlt">scaling</span> of the metabolic cost of transport. When <span class="hlt">scaled</span> against body mass, forelimb inertial properties, apart from mass, <span class="hlt">scale</span> with positive allometry. Fore- and hindlimb mass <span class="hlt">scale</span> according to geometric similarity (limb mass ∝ body mass(1.0)), as do the remaining hindlimb inertial properties. The positive allometry of limb length is largely the result of absolute differences in limb inertial properties between mammalian subgroups. Though likely detrimental to locomotor costs in large mammals, <span class="hlt">scale</span> effects in limb inertial properties appear to be concomitant with <span class="hlt">scale</span> effects in sensorimotor control and locomotor ability in terrestrial mammals. Across mammals, the forelimb's potential for angular acceleration <span class="hlt">scales</span> according to geometric similarity, whereas the hindlimb's potential for angular acceleration <span class="hlt">scales</span> with positive allometry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3832634','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3832634"><span><span class="hlt">Scale</span> Effects between Body Size and Limb Design in Quadrupedal Mammals</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kilbourne, Brandon M.; Hoffman, Louwrens C.</p> <p>2013-01-01</p> <p>Recently the metabolic cost of swinging the limbs has been found to be much greater than previously thought, raising the possibility that limb rotational inertia influences the energetics of locomotion. Larger mammals have a lower mass-specific cost of transport than smaller mammals. The <span class="hlt">scaling</span> of the mass-specific cost of transport is partly explained by decreasing stride <span class="hlt">frequency</span> with increasing body size; however, it is unknown if limb rotational inertia also influences the mass-specific cost of transport. Limb length and inertial properties – limb mass, center of mass (COM) position, moment of inertia, radius of gyration, and natural <span class="hlt">frequency</span> – were measured in 44 species of terrestrial mammals, spanning eight taxonomic orders. Limb length increases disproportionately with body mass via positive allometry (length ∝ body mass0.40); the positive allometry of limb length may help explain the <span class="hlt">scaling</span> of the metabolic cost of transport. When <span class="hlt">scaled</span> against body mass, forelimb inertial properties, apart from mass, <span class="hlt">scale</span> with positive allometry. Fore- and hindlimb mass <span class="hlt">scale</span> according to geometric similarity (limb mass ∝ body mass1.0), as do the remaining hindlimb inertial properties. The positive allometry of limb length is largely the result of absolute differences in limb inertial properties between mammalian subgroups. Though likely detrimental to locomotor costs in large mammals, <span class="hlt">scale</span> effects in limb inertial properties appear to be concomitant with <span class="hlt">scale</span> effects in sensorimotor control and locomotor ability in terrestrial mammals. Across mammals, the forelimb's potential for angular acceleration <span class="hlt">scales</span> according to geometric similarity, whereas the hindlimb's potential for angular acceleration <span class="hlt">scales</span> with positive allometry. PMID:24260117</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=work+AND+stress+AND+affect+AND+health&pg=3&id=EJ749292','ERIC'); return false;" href="https://eric.ed.gov/?q=work+AND+stress+AND+affect+AND+health&pg=3&id=EJ749292"><span>The Positive Event <span class="hlt">Scale</span>: Measuring Uplift <span class="hlt">Frequency</span> and Intensity in an Adult Sample</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Maybery, D. J.; Jones-Ellis, Jenny; Neale, Jason; Arentz, Alexandra</p> <p>2006-01-01</p> <p>Of the limited number of studies employing positive event (uplift) measures none have published detailed psychometric information about the <span class="hlt">scale</span> that was used (Maybery and Graham, 2001, Stress and Health 17, pp. 91-104). Building on previous work with university students and employing conceptually distinct measurement strategies (i.e. measuring…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25844315','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25844315"><span>Low-<span class="hlt">frequency</span> connectivity is associated with mild traumatic brain injury.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dunkley, B T; Da Costa, L; Bethune, A; Jetly, R; Pang, E W; Taylor, M J; Doesburg, S M</p> <p>2015-01-01</p> <p>Mild traumatic brain injury (mTBI) occurs from a closed-head impact. Often referred to as concussion, about 20% of cases complain of secondary psychological sequelae, such as disorders of attention and memory. Known as post-concussive symptoms (PCS), these problems can severely disrupt the patient's quality of life. Changes in local spectral power, particularly low-<span class="hlt">frequency</span> amplitude increases and/or peak alpha slowing have been reported in mTBI, but large-<span class="hlt">scale</span> connectivity metrics based on inter-regional amplitude correlations relevant for integration and segregation in functional brain networks, and their association with disorders in cognition and behaviour, remain relatively unexplored. Here, we used non-invasive neuroimaging with magnetoencephalography to examine functional connectivity in a resting-state protocol in a group with mTBI (n = 20), and a control group (n = 21). We observed a trend for atypical slow-wave power changes in subcortical, temporal and parietal regions in mTBI, as well as significant long-range increases in amplitude envelope correlations among deep-source, temporal, and frontal regions in the delta, theta, and alpha bands. Subsequently, we conducted an exploratory analysis of patterns of connectivity most associated with variability in secondary symptoms of mTBI, including inattention, anxiety, and depression. Differential patterns of altered resting state neurophysiological network connectivity were found across <span class="hlt">frequency</span> bands. This indicated that multiple network and <span class="hlt">frequency</span> specific alterations in large <span class="hlt">scale</span> brain connectivity may contribute to overlapping cognitive sequelae in mTBI. In conclusion, we show that local spectral power content can be supplemented with measures of correlations in amplitude to define general networks that are atypical in mTBI, and suggest that certain cognitive difficulties are mediated by disturbances in a variety of alterations in network interactions which are differentially expressed across</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SSRv..214...66N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SSRv..214...66N"><span>Very Long Baseline Interferometry: Dependencies on <span class="hlt">Frequency</span> Stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nothnagel, Axel; Nilsson, Tobias; Schuh, Harald</p> <p>2018-04-01</p> <p>Very Long Baseline Interferometry (VLBI) is a differential technique observing radiation of compact extra-galactic radio sources with pairs of radio telescopes. For these observations, the <span class="hlt">frequency</span> standards at the telescopes need to have very high stability. In this article we discuss why this is, and we investigate exactly how precise the <span class="hlt">frequency</span> standards need to be. Four areas where good clock performance is needed are considered: coherence, geodetic parameter estimation, correlator synchronization, and UT1 determination. We show that in order to ensure the highest accuracy of VLBI, stability similar to that of a hydrogen maser is needed for time-<span class="hlt">scales</span> up to a few hours. In the article, we are considering both traditional VLBI where extra-galactic radio sources are observed, as well as observation of man-made artificial radio sources emitted by satellites or spacecrafts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=aggressive&pg=2&id=EJ1147803','ERIC'); return false;" href="https://eric.ed.gov/?q=aggressive&pg=2&id=EJ1147803"><span>An Independent Investigation into the Psychometric Properties of the Adult <span class="hlt">Scale</span> of Hostility and Aggression (A-SHARP)</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Rojahn, Johannes; Rick-Betancourt, Brittney; Barnard-Brak, Lucy; Moore, Linda</p> <p>2017-01-01</p> <p>Background: The Adult <span class="hlt">Scale</span> of Hostility and Aggression (A-SHARP) rating <span class="hlt">scale</span> assesses the <span class="hlt">frequency</span>/severity (problem <span class="hlt">scale</span>) and the reactive-proactive motivation (provocation <span class="hlt">scale</span>) of aggressive behaviors in adults with intellectual disabilities (ID). Items are assigned to five subscales (Verbal Aggression, Physical Aggression, Hostile Affect,…</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('https://www.ncbi.nlm.nih.gov/pubmed/27572284','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27572284"><span>Knowledge discovery from high-<span class="hlt">frequency</span> stream nitrate concentrations: hydrology and biology contributions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aubert, Alice H; Thrun, Michael C; Breuer, Lutz; Ultsch, Alfred</p> <p>2016-08-30</p> <p>High-<span class="hlt">frequency</span>, in-situ monitoring provides large environmental datasets. These datasets will likely bring new insights in landscape functioning and process <span class="hlt">scale</span> understanding. However, tailoring data analysis methods is necessary. Here, we detach our analysis from the usual temporal analysis performed in hydrology to determine if it is possible to infer general rules regarding hydrochemistry from available large datasets. We combined a 2-year in-stream nitrate concentration time series (time resolution of 15 min) with concurrent hydrological, meteorological and soil moisture data. We removed the low-<span class="hlt">frequency</span> variations through low-pass filtering, which suppressed seasonality. We then analyzed the high-<span class="hlt">frequency</span> variability component using Pareto Density Estimation, which to our knowledge has not been applied to hydrology. The resulting distribution of nitrate concentrations revealed three normally distributed modes: low, medium and high. Studying the environmental conditions for each mode revealed the main control of nitrate concentration: the saturation state of the riparian zone. We found low nitrate concentrations under conditions of hydrological connectivity and dominant denitrifying biological processes, and we found high nitrate concentrations under hydrological recession conditions and dominant nitrifying biological processes. These results generalize our understanding of hydro-biogeochemical nitrate flux controls and bring useful information to the development of nitrogen process-based models at the landscape <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19736969','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19736969"><span>Parametric nanomechanical amplification at very high <span class="hlt">frequency</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Karabalin, R B; Feng, X L; Roukes, M L</p> <p>2009-09-01</p> <p>Parametric resonance and amplification are important in both fundamental physics and technological applications. Here we report very high <span class="hlt">frequency</span> (VHF) parametric resonators and mechanical-domain amplifiers based on nanoelectromechanical systems (NEMS). Compound mechanical nanostructures patterned by multilayer, top-down nanofabrication are read out by a novel scheme that parametrically modulates longitudinal stress in doubly clamped beam NEMS resonators. Parametric pumping and signal amplification are demonstrated for VHF resonators up to approximately 130 MHz and provide useful enhancement of both resonance signal amplitude and quality factor. We find that Joule heating and reduced thermal conductance in these nanostructures ultimately impose an upper limit to device performance. We develop a theoretical model to account for both the parametric response and nonequilibrium thermal transport in these composite nanostructures. The results closely conform to our experimental observations, elucidate the <span class="hlt">frequency</span> and threshold-voltage <span class="hlt">scaling</span> in parametric VHF NEMS resonators and sensors, and establish the ultimate sensitivity limits of this approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23306722','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23306722"><span>The Spanish version of the Emotional Labour <span class="hlt">Scale</span> (ELS): a validation study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Picardo, Juan M; López-Fernández, Consuelo; Hervás, María José Abellán</p> <p>2013-10-01</p> <p>To validate the Spanish version of the Emotional Labour <span class="hlt">Scale</span> (ELS), an instrument widely used to understand how professionals working with people face emotional labor in their daily job. An observational, cross-sectional and multicenter survey was used. Nursing students and their clinical tutors (n=211) completed the self-reported ELS when the clinical practice period was over. First order and second order Confirmatory Factor Analyses (CFA) were estimated in order to test the factor structure of the <span class="hlt">scale</span>. The results of the CFA confirm a factor structure of the <span class="hlt">scale</span> with six first order factors (duration, <span class="hlt">frequency</span>, intensity, variety, surface acting and deep acting) and two larger second order factors named Demands (duration, <span class="hlt">frequency</span>, intensity and variety) and Acting (surface acting and deep acting) establishing the validity of the Spanish version of the ELS. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26138146','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26138146"><span>Multi-<span class="hlt">scale</span> analysis of neural activity in humans: Implications for micro-<span class="hlt">scale</span> electrocorticography.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kellis, Spencer; Sorensen, Larry; Darvas, Felix; Sayres, Conor; O'Neill, Kevin; Brown, Richard B; House, Paul; Ojemann, Jeff; Greger, Bradley</p> <p>2016-01-01</p> <p>Electrocorticography grids have been used to study and diagnose neural pathophysiology for over 50 years, and recently have been used for various neural prosthetic applications. Here we provide evidence that micro-<span class="hlt">scale</span> electrodes are better suited for studying cortical pathology and function, and for implementing neural prostheses. This work compares dynamics in space, time, and <span class="hlt">frequency</span> of cortical field potentials recorded by three types of electrodes: electrocorticographic (ECoG) electrodes, non-penetrating micro-ECoG (μECoG) electrodes that use microelectrodes and have tighter interelectrode spacing; and penetrating microelectrodes (MEA) that penetrate the cortex to record single- or multiunit activity (SUA or MUA) and local field potentials (LFP). While the finest spatial <span class="hlt">scales</span> are found in LFPs recorded intracortically, we found that LFP recorded from μECoG electrodes demonstrate <span class="hlt">scales</span> of linear similarity (i.e., correlation, coherence, and phase) closer to the intracortical electrodes than the clinical ECoG electrodes. We conclude that LFPs can be recorded intracortically and epicortically at finer <span class="hlt">scales</span> than clinical ECoG electrodes are capable of capturing. Recorded with appropriately <span class="hlt">scaled</span> electrodes and grids, field potentials expose a more detailed representation of cortical network activity, enabling advanced analyses of cortical pathology and demanding applications such as brain-computer interfaces. Copyright © 2015 International Federation of Clinical Neurophysiology. Published by Elsevier Ireland Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29109246','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29109246"><span><span class="hlt">Scale</span>-dependent climatic drivers of human epidemics in ancient China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tian, Huidong; Yan, Chuan; Xu, Lei; Büntgen, Ulf; Stenseth, Nils C; Zhang, Zhibin</p> <p>2017-12-05</p> <p>A wide range of climate change-induced effects have been implicated in the prevalence of infectious diseases. Disentangling causes and consequences, however, remains particularly challenging at historical time <span class="hlt">scales</span>, for which the quality and quantity of most of the available natural proxy archives and written documentary sources often decline. Here, we reconstruct the spatiotemporal occurrence patterns of human epidemics for large parts of China and most of the last two millennia. Cold and dry climate conditions indirectly increased the prevalence of epidemics through the influences of locusts and famines. Our results further reveal that low-<span class="hlt">frequency</span>, long-term temperature trends mainly contributed to negative associations with epidemics, while positive associations of epidemics with droughts, floods, locusts, and famines mainly coincided with both higher and lower <span class="hlt">frequency</span> temperature variations. Nevertheless, unstable relationships between human epidemics and temperature changes were observed on relatively smaller time <span class="hlt">scales</span>. Our study suggests that an intertwined, direct, and indirect array of biological, ecological, and societal responses to different aspects of past climatic changes strongly depended on the <span class="hlt">frequency</span> domain and study period chosen.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhFl...29k5107Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhFl...29k5107Z"><span>Experimental investigation on <span class="hlt">frequency</span> characteristics of plasma synthetic jets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zong, Haohua; Kotsonis, Marios</p> <p>2017-11-01</p> <p>The performance of a two-electrode plasma synthetic jet actuator (PSJA) is investigated for a wide range of dimensionless actuation <span class="hlt">frequencies</span> ( f*) using high-speed phase-locked particle imaging velocimetry measurements. The jet-induced velocity fields in the axisymmetric plane are measured during both transient and steady working stages of the PSJA. When f* increases, the jet duration time (Tjet) is reduced, while the peak suction velocity (Us) increases consistently. Three integral parameters including the total expelled gas mass, impulse, and issued mechanical energy also decline considerably with increasing <span class="hlt">frequency</span>, which is shown to relate to both the reduced cavity density and the decreasing jet duration. Theoretical analysis reveals that the mean cavity density decreases monotonically with the square root of the discharge <span class="hlt">frequency</span>. The decreasing rate is inversely proportional to a thermal cut-off <span class="hlt">frequency</span> ( fc, 210 Hz for the current study), which <span class="hlt">scales</span> with the convective heat transfer coefficient between the actuator cavity walls and the cavity gas, as well as the area of the cavity internal surface. In the time-averaged velocity fields, the jet centreline velocity (U¯ c) exhibits a local maximum in the axial coordinate. The nondimensional maximum centreline velocity reduces with increasing <span class="hlt">frequency</span> of operation. The jet spreading rate of the plasma synthetic jets (PSJs) decreases from 0.14 to 0.09 with increasing <span class="hlt">frequency</span>. During the transient working stage of a PSJ, the exit velocity trace elapses 20 successive actuation cycles to stabilize. In contrast to the exit velocity, approximately 130 cycles are needed for the mean cavity density/temperature to reach steady values.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914812B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914812B"><span>Conditional flood <span class="hlt">frequency</span> and catchment state: a simulation approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brettschneider, Marco; Bourgin, François; Merz, Bruno; Andreassian, Vazken; Blaquiere, Simon</p> <p>2017-04-01</p> <p>Catchments have memory and the conditional flood <span class="hlt">frequency</span> distribution for a time period ahead can be seen as non-stationary: it varies with the catchment state and climatic factors. From a risk management perspective, understanding the link of conditional flood <span class="hlt">frequency</span> to catchment state is a key to anticipate potential periods of higher flood risk. Here, we adopt a simulation approach to explore the link between flood <span class="hlt">frequency</span> obtained by continuous rainfall-runoff simulation and the initial state of the catchment. The simulation chain is based on i) a three state rainfall generator applied at the catchment <span class="hlt">scale</span>, whose parameters are estimated for each month, and ii) the GR4J lumped rainfall-runoff model, whose parameters are calibrated with all available data. For each month, a large number of stochastic realizations of the continuous rainfall generator for the next 12 months are used as inputs for the GR4J model in order to obtain a large number of stochastic realizations for the next 12 months. This process is then repeated for 50 different initial states of the soil moisture reservoir of the GR4J model and for all the catchments. Thus, 50 different conditional flood <span class="hlt">frequency</span> curves are obtained for the 50 different initial catchment states. We will present an analysis of the link between the catchment states, the period of the year and the strength of the conditioning of the flood <span class="hlt">frequency</span> compared to the unconditional flood <span class="hlt">frequency</span>. A large sample of diverse catchments in France will be used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=poisson+AND+process&id=EJ183716','ERIC'); return false;" href="https://eric.ed.gov/?q=poisson+AND+process&id=EJ183716"><span><span class="hlt">Frequency</span>-Rank Distributions</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Brookes, Bertram C.; Griffiths, Jose M.</p> <p>1978-01-01</p> <p><span class="hlt">Frequency</span>, rank, and <span class="hlt">frequency</span> rank distributions are defined. Extensive discussion on several aspects of <span class="hlt">frequency</span> rank distributions includes the Poisson process as a means of exploring the stability of ranks; the correlation of <span class="hlt">frequency</span> rank distributions; and the transfer coefficient, a new measure in <span class="hlt">frequency</span> rank distribution. (MBR)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ClDy...33..843C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ClDy...33..843C"><span>A revised method of presenting wavenumber-<span class="hlt">frequency</span> power spectrum diagrams that reveals the asymmetric nature of tropical large-<span class="hlt">scale</span> waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chao, Winston C.; Yang, Bo; Fu, Xiouhua</p> <p>2009-11-01</p> <p>The popular method of presenting wavenumber-<span class="hlt">frequency</span> power spectrum diagrams for studying tropical large-<span class="hlt">scale</span> waves in the literature is shown to give an incomplete presentation of these waves. The so-called “convectively coupled Kelvin (mixed Rossby-gravity) waves” are presented as existing only in the symmetric (anti-symmetric) component of the diagrams. This is obviously not consistent with the published composite/regression studies of “convectively coupled Kelvin waves,” which illustrate the asymmetric nature of these waves. The cause of this inconsistency is revealed in this note and a revised method of presenting the power spectrum diagrams is proposed. When this revised method is used, “convectively coupled Kelvin waves” do show anti-symmetric components, and “convectively coupled mixed Rossby-gravity waves (also known as Yanai waves)” do show a hint of symmetric components. These results bolster a published proposal that these waves should be called “chimeric Kelvin waves,” “chimeric mixed Rossby-gravity waves,” etc. This revised method of presenting power spectrum diagrams offers an additional means of comparing the GCM output with observations by calling attention to the capability of GCMs to correctly simulate the asymmetric characteristics of equatorial waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23826188','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23826188"><span>Are all types of expertise created equal? Car experts use different spatial <span class="hlt">frequency</span> <span class="hlt">scales</span> for subordinate categorization of cars and faces.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harel, Assaf; Bentin, Shlomo</p> <p>2013-01-01</p> <p>A much-debated question in object recognition is whether expertise for faces and expertise for non-face objects utilize common perceptual information. We investigated this issue by assessing the diagnostic information required for different types of expertise. Specifically, we asked whether face categorization and expert car categorization at the subordinate level relies on the same spatial <span class="hlt">frequency</span> (SF) <span class="hlt">scales</span>. Fifteen car experts and fifteen novices performed a category verification task with spatially filtered images of faces, cars, and airplanes. Images were categorized based on their basic (e.g. "car") and subordinate level (e.g. "Japanese car") identity. The effect of expertise was not evident when objects were categorized at the basic level. However, when the car experts categorized faces and cars at the subordinate level, the two types of expertise required different kinds of SF information. Subordinate categorization of faces relied on low SFs more than on high SFs, whereas subordinate expert car categorization relied on high SFs more than on low SFs. These findings suggest that expertise in the recognition of objects and faces do not utilize the same type of information. Rather, different types of expertise require different types of diagnostic visual information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3691146','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3691146"><span>Are All Types of Expertise Created Equal? Car Experts Use Different Spatial <span class="hlt">Frequency</span> <span class="hlt">Scales</span> for Subordinate Categorization of Cars and Faces</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Harel, Assaf; Bentin, Shlomo</p> <p>2013-01-01</p> <p>A much-debated question in object recognition is whether expertise for faces and expertise for non-face objects utilize common perceptual information. We investigated this issue by assessing the diagnostic information required for different types of expertise. Specifically, we asked whether face categorization and expert car categorization at the subordinate level relies on the same spatial <span class="hlt">frequency</span> (SF) <span class="hlt">scales</span>. Fifteen car experts and fifteen novices performed a category verification task with spatially filtered images of faces, cars, and airplanes. Images were categorized based on their basic (e.g. “car”) and subordinate level (e.g. “Japanese car”) identity. The effect of expertise was not evident when objects were categorized at the basic level. However, when the car experts categorized faces and cars at the subordinate level, the two types of expertise required different kinds of SF information. Subordinate categorization of faces relied on low SFs more than on high SFs, whereas subordinate expert car categorization relied on high SFs more than on low SFs. These findings suggest that expertise in the recognition of objects and faces do not utilize the same type of information. Rather, different types of expertise require different types of diagnostic visual information. PMID:23826188</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4340971','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4340971"><span>Tuning In to Sound: <span class="hlt">Frequency</span>-Selective Attentional Filter in Human Primary Auditory Cortex</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Da Costa, Sandra; van der Zwaag, Wietske; Miller, Lee M.; Clarke, Stephanie</p> <p>2013-01-01</p> <p>Cocktail parties, busy streets, and other noisy environments pose a difficult challenge to the auditory system: how to focus attention on selected sounds while ignoring others? Neurons of primary auditory cortex, many of which are sharply tuned to sound <span class="hlt">frequency</span>, could help solve this problem by filtering selected sound information based on <span class="hlt">frequency</span>-content. To investigate whether this occurs, we used high-resolution fMRI at 7 tesla to map the fine-<span class="hlt">scale</span> <span class="hlt">frequency</span>-tuning (1.5 mm isotropic resolution) of primary auditory areas A1 and R in six human participants. Then, in a selective attention experiment, participants heard low (250 Hz)- and high (4000 Hz)-<span class="hlt">frequency</span> streams of tones presented at the same time (dual-stream) and were instructed to focus attention onto one stream versus the other, switching back and forth every 30 s. Attention to low-<span class="hlt">frequency</span> tones enhanced neural responses within low-<span class="hlt">frequency</span>-tuned voxels relative to high, and when attention switched the pattern quickly reversed. Thus, like a radio, human primary auditory cortex is able to tune into attended <span class="hlt">frequency</span> channels and can switch channels on demand. PMID:23365225</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ApPhA.tmp..233M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ApPhA.tmp..233M"><span>AC conductivity <span class="hlt">scaling</span> behavior in grain and grain boundary response regime of fast lithium ionic conductors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mariappan, C. R.</p> <p>2014-05-01</p> <p>AC conductivity spectra of Li-analogues NASICON-type Li1.5Al0.5Ge1.5P3O12 (LAGP), Li-Al-Ti-P-O (LATP) glass-ceramics and garnet-type Li7La2Ta2O13 (LLTO) ceramic are analyzed by universal power law and Summerfield <span class="hlt">scaling</span> approaches. The activation energies and pre-exponential factors of total and grain conductivities are following the Meyer-Neldel (M-N) rule for NASICON-type materials. However, the garnet-type LLTO material deviates from the M-N rule line of NASICON-type materials. The <span class="hlt">frequency</span>- and temperature-dependent conductivity spectra of LAGP and LLTO are superimposed by Summerfield <span class="hlt">scaling</span>. The <span class="hlt">scaled</span> conductivity curves of LATP are not superimposed at the grain boundary response region. The superimposed conductivity curves are observed at cross-over <span class="hlt">frequencies</span> of grain boundary response region for LATP by incorporating the exp ( {{{ - (EAt - EAg )} {{{ - (EAt - EAg )} {kT}}} ) factor along with Summerfield <span class="hlt">scaling</span> factors on the <span class="hlt">frequency</span> axis, where EAt and EAg are the activation energies of total and grain conductivities, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1417425-ghz-spaced-comb-high-dimensional-frequency-bin-entangled-photons-from-chip-silicon-nitride-microresonator','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1417425-ghz-spaced-comb-high-dimensional-frequency-bin-entangled-photons-from-chip-silicon-nitride-microresonator"><span>50-GHz-spaced comb of high-dimensional <span class="hlt">frequency</span>-bin entangled photons from an on-chip silicon nitride microresonator</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>Imany, Poolad; Jaramillo-Villegas, Jose A.; Odele, Ogaga D.</p> <p></p> <p>Quantum <span class="hlt">frequency</span> combs from chip-<span class="hlt">scale</span> integrated sources are promising candidates for scalable and robust quantum information processing (QIP). However, to use these quantum combs for <span class="hlt">frequency</span> domain QIP, demonstration of entanglement in the <span class="hlt">frequency</span> basis, showing that the entangled photons are in a coherent superposition of multiple <span class="hlt">frequency</span> bins, is required. We present a verification of qubit and qutrit <span class="hlt">frequency</span>-bin entanglement using an on-chip quantum <span class="hlt">frequency</span> comb with 40 mode pairs, through a two-photon interference measurement that is based on electro-optic phase modulation. Our demonstrations provide an important contribution in establishing integrated optical microresonators as a source for high-dimensional <span class="hlt">frequency</span>-binmore » encoded quantum computing, as well as dense quantum key distribution.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1417425-ghz-spaced-comb-high-dimensional-frequency-bin-entangled-photons-from-chip-silicon-nitride-microresonator','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1417425-ghz-spaced-comb-high-dimensional-frequency-bin-entangled-photons-from-chip-silicon-nitride-microresonator"><span>50-GHz-spaced comb of high-dimensional <span class="hlt">frequency</span>-bin entangled photons from an on-chip silicon nitride microresonator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Imany, Poolad; Jaramillo-Villegas, Jose A.; Odele, Ogaga D.; ...</p> <p>2018-01-18</p> <p>Quantum <span class="hlt">frequency</span> combs from chip-<span class="hlt">scale</span> integrated sources are promising candidates for scalable and robust quantum information processing (QIP). However, to use these quantum combs for <span class="hlt">frequency</span> domain QIP, demonstration of entanglement in the <span class="hlt">frequency</span> basis, showing that the entangled photons are in a coherent superposition of multiple <span class="hlt">frequency</span> bins, is required. We present a verification of qubit and qutrit <span class="hlt">frequency</span>-bin entanglement using an on-chip quantum <span class="hlt">frequency</span> comb with 40 mode pairs, through a two-photon interference measurement that is based on electro-optic phase modulation. Our demonstrations provide an important contribution in establishing integrated optical microresonators as a source for high-dimensional <span class="hlt">frequency</span>-binmore » encoded quantum computing, as well as dense quantum key distribution.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160008995','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160008995"><span>An Investigation of High <span class="hlt">Frequency</span> Motions in the Tropical Tropopause Layer near Convection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pfister, Leonhard; Bui, T. P.; Dean-Day, Jon; Lim, Boon; Lawson, Paul</p> <p>2016-01-01</p> <p>Indirect evidence indicates a role for vertical mixing in the Tropical Tropopause Layer (TTL). In the past 20 years, high altitude NASA aircraft such as the ER-2, WB-57, and GLobal Hawk have been making 20hz measurements of vertical velocity and other meteorological parameters in the Upper Tropospere-Lower Stratosphere region, many in the tropics, most recently in connection with the Airborne Tropical TRopopause EXperiment (ATTREX). In the stable environment of the UTLS, high <span class="hlt">frequency</span> activity occurs in bursts, presumably in connection with nearby convection or strong vertical shear associated with larger <span class="hlt">scale</span> gravity waves. This paper examines tropical high <span class="hlt">frequency</span> aircraft data to obtain some basic information about the distribution and character of high <span class="hlt">frequency</span> activity in vertical velocity in the TTL. In particular, we focus on relating the high <span class="hlt">frequency</span> activity to nearby tropical convection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10512E..19F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10512E..19F"><span>High-energy 100-ns single-<span class="hlt">frequency</span> all-fiber laser at 1064 nm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fu, Shijie; Shi, Wei; Tang, Zhao; Shi, Chaodu; Bai, Xiaolei; Sheng, Quan; Chavez-Pirson, Arturo; Peyghambarian, N.; Yao, Jianquan</p> <p>2018-02-01</p> <p>A high-energy, single-<span class="hlt">frequency</span> fiber laser with long pulse duration of 100 ns has been experimentally investigated in an all-fiber architecture. Only 34-cm long heavily Yb-doped phosphate fiber was employed in power <span class="hlt">scaling</span> stage to efficiently suppress the Stimulated Brillouin effect (SBS). In the experiment, 0.47 mJ single pulse energy was achieved in power <span class="hlt">scaling</span> stage at the pump power of 16 W. The pre-shaped pulse was gradually broadened from 103 to 140 ns during the amplification without shape distortion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=279471','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=279471"><span>Ecosystem resilience despite large-<span class="hlt">scale</span> altered hydro climatic conditions</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Climate change is predicted to increase both drought <span class="hlt">frequency</span> and duration, and when coupled with substantial warming, will establish a new hydroclimatological paradigm for many regions. Large-<span class="hlt">scale</span>, warm droughts have recently impacted North America, Africa, Europe, Amazonia, and Australia result...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140007513','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140007513"><span>The Cosmology Large Angular <span class="hlt">Scale</span> Surveyor (CLASS) Telescope Architecture</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chuss, David T.; Ali, Aamir; Amiri, Mandana; Appel, John W.; Araujo, Derek; Bennett, Charles L.; Boone, Fletcher; Chan, Manwei; Cho, Hsiao-Mei; Colazo, Felipe; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140007513'); toggleEditAbsImage('author_20140007513_show'); toggleEditAbsImage('author_20140007513_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140007513_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140007513_hide"></p> <p>2014-01-01</p> <p>We describe the instrument architecture of the Johns Hopkins University-led CLASS instrument, a groundbased cosmic microwave background (CMB) polarimeter that will measure the large-<span class="hlt">scale</span> polarization of the CMB in several <span class="hlt">frequency</span> bands to search for evidence of inflation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820060297&hterms=time+synchronization&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dtime%2Bsynchronization','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820060297&hterms=time+synchronization&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dtime%2Bsynchronization"><span><span class="hlt">Frequency</span> synchronization of a <span class="hlt">frequency</span>-hopped MFSK communication system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Huth, G. K.; Polydoros, A.; Simon, M. K.</p> <p>1981-01-01</p> <p>This paper presents the performance of fine-<span class="hlt">frequency</span> synchronization. The performance degradation due to imperfect <span class="hlt">frequency</span> synchronization is found in terms of the effect on bit error probability as a function of full-band or partial-band noise jamming levels and of the number of <span class="hlt">frequency</span> hops used in the estimator. The effect of imperfect fine-time synchronization is also included in the calculation of fine-<span class="hlt">frequency</span> synchronization performance to obtain the overall performance degradation due to synchronization errors.</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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