Sample records for frequency separation variations

  1. Formant-frequency variation and its effects on across-formant grouping in speech perception.

    PubMed

    Roberts, Brian; Summers, Robert J; Bailey, Peter J

    2013-01-01

    How speech is separated perceptually from other speech remains poorly understood. In a series of experiments, perceptual organisation was probed by presenting three-formant (F1+F2+F3) analogues of target sentences dichotically, together with a competitor for F2 (F2C), or for F2+F3, which listeners must reject to optimise recognition. To control for energetic masking, the competitor was always presented in the opposite ear to the corresponding target formant(s). Sine-wave speech was used initially, and different versions of F2C were derived from F2 using separate manipulations of its amplitude and frequency contours. F2Cs with time-varying frequency contours were highly effective competitors, whatever their amplitude characteristics, whereas constant-frequency F2Cs were ineffective. Subsequent studies used synthetic-formant speech to explore the effects of manipulating the rate and depth of formant-frequency change in the competitor. Competitor efficacy was not tuned to the rate of formant-frequency variation in the target sentences; rather, the reduction in intelligibility increased with competitor rate relative to the rate for the target sentences. Therefore, differences in speech rate may not be a useful cue for separating the speech of concurrent talkers. Effects of competitors whose depth of formant-frequency variation was scaled by a range of factors were explored using competitors derived either by inverting the frequency contour of F2 about its geometric mean (plausibly speech-like pattern) or by using a regular and arbitrary frequency contour (triangle wave, not plausibly speech-like) matched to the average rate and depth of variation for the inverted F2C. Competitor efficacy depended on the overall depth of frequency variation, not depth relative to that for the other formants. Furthermore, the triangle-wave competitors were as effective as their more speech-like counterparts. Overall, the results suggest that formant-frequency variation is critical for

  2. Development of a frequency-separated knob with variable change rates by rotation speed.

    PubMed

    Kim, Huhn; Ham, Dong-Han

    2014-11-01

    The principle of frequency separation is a design method to display different information or feedback in accordance with the frequency of interaction between users and systems. This principle can be usefully applied to the design of knobs. Particularly, their rotation speed can be a meaningful criterion for applying the principle. Hence a knob can be developed, which shows change rates varying depending on its rotation speed. Such a knob would be more efficient than conventional knobs with constant change rate. We developed a prototype of frequency-separated knobs that has different combinations of the number of rotation speed steps and the size of the variation of change rate. With this prototype, we conducted an experiment to examine whether a speed frequency-separated knob enhances users' task performance. The results showed that the newly designed knob was effective in enhancing task performance, and that task efficiency was the best when its change rate increases exponentially and its rotation speed has three steps. We conducted another experiment to investigate how a more rapid exponential increase of change rate and a more number of steps of rotation speed influence users' task performance. The results showed that merely increasing both the size of the variation of change rates and the number of speed steps did not result in better task performance. Although two experimental results cannot easily be generalized to other contexts, they still offer practical information useful for designing a speed frequency-separated knob in various consumer electronics and control panels of industrial systems. Copyright © 2014 Elsevier Ltd and The Ergonomics Society. All rights reserved.

  3. Separation of musical instruments based on amplitude and frequency comodulation

    NASA Astrophysics Data System (ADS)

    Jacobson, Barry D.; Cauwenberghs, Gert; Quatieri, Thomas F.

    2002-05-01

    In previous work, amplitude comodulation was investigated as a basis for monaural source separation. Amplitude comodulation refers to similarities in amplitude envelopes of individual spectral components emitted by particular types of sources. In many types of musical instruments, amplitudes of all resonant modes rise/fall, and start/stop together during the course of normal playing. We found that under certain well-defined conditions, a mixture of constant frequency, amplitude comodulated sources can unambiguously be decomposed into its constituents on the basis of these similarities. In this work, system performance was improved by relaxing the constant frequency requirement. String instruments, for example, which are normally played with vibrato, are both amplitude and frequency comodulated sources, and could not be properly tracked under the constant frequency assumption upon which our original algorithm was based. Frequency comodulation refers to similarities in frequency variations of individual harmonics emitted by these types of sources. The analytical difficulty is in defining a representation of the source which properly tracks frequency varying components. A simple, fixed filter bank can only track an individual spectral component for the duration in which it is within the passband of one of the filters. Alternatives are therefore explored which are amenable to real-time implementation.

  4. Vocalization frequency and duration are coded in separate hindbrain nuclei.

    PubMed

    Chagnaud, Boris P; Baker, Robert; Bass, Andrew H

    2011-06-14

    Temporal patterning is an essential feature of neural networks producing precisely timed behaviours such as vocalizations that are widely used in vertebrate social communication. Here we show that intrinsic and network properties of separate hindbrain neuronal populations encode the natural call attributes of frequency and duration in vocal fish. Intracellular structure/function analyses indicate that call duration is encoded by a sustained membrane depolarization in vocal prepacemaker neurons that innervate downstream pacemaker neurons. Pacemaker neurons, in turn, encode call frequency by rhythmic, ultrafast oscillations in their membrane potential. Pharmacological manipulations show prepacemaker activity to be independent of pacemaker function, thus accounting for natural variation in duration which is the predominant feature distinguishing call types. Prepacemaker neurons also innervate key hindbrain auditory nuclei thereby effectively serving as a call-duration corollary discharge. We propose that premotor compartmentalization of neurons coding distinct acoustic attributes is a fundamental trait of hindbrain vocal pattern generators among vertebrates.

  5. Vocalization frequency and duration are coded in separate hindbrain nuclei

    PubMed Central

    Chagnaud, Boris P.; Baker, Robert; Bass, Andrew H.

    2011-01-01

    Temporal patterning is an essential feature of neural networks producing precisely timed behaviours such as vocalizations that are widely used in vertebrate social communication. Here we show that intrinsic and network properties of separate hindbrain neuronal populations encode the natural call attributes of frequency and duration in vocal fish. Intracellular structure/function analyses indicate that call duration is encoded by a sustained membrane depolarization in vocal prepacemaker neurons that innervate downstream pacemaker neurons. Pacemaker neurons, in turn, encode call frequency by rhythmic, ultrafast oscillations in their membrane potential. Pharmacological manipulations show prepacemaker activity to be independent of pacemaker function, thus accounting for natural variation in duration which is the predominant feature distinguishing call types. Prepacemaker neurons also innervate key hindbrain auditory nuclei thereby effectively serving as a call-duration corollary discharge. We propose that premotor compartmentalization of neurons coding distinct acoustic attributes is a fundamental trait of hindbrain vocal pattern generators among vertebrates. PMID:21673667

  6. Physics of systematic frequency variations in hydrogen masers

    NASA Technical Reports Server (NTRS)

    Mattison, Edward M.

    1990-01-01

    The frequency stability of hydrogen masers for intervals longer that 10(exp 4) seconds is limited at present by systematic processes. Researchers discuss the physics of frequency-determining mechanisms internal to the maser that are susceptible to systematic variations, and the connections between these internal mechanisms and external environmental factors. Based upon estimates of the magnitudes of systematic effects, they find that the primary internal mechanisms currently limiting long-term maser frequency stability are cavity pulling, at the level parts in 10(exp 15) per day, and wall shift variations, at the level of parts in 10(exp 16) to parts in 10(exp 15) per day. They discuss strategies for reducing systematic frequency variations.

  7. Physics of systematic frequency variations in hydrogen masers

    NASA Technical Reports Server (NTRS)

    Mattison, Edward M.

    1992-01-01

    The frequency stability of hydrogen masers for intervals longer than 10 exp 4 s is currently limited by systematic processes. The physics of frequency-determining mechanisms internal to the maser that are susceptible to systematic variations, and the connections between these internal mechanisms and external environmental factors are discussed. From estimates of the magnitudes of systematic effects, it is found that the primary internal mechanisms limiting long-term maser frequency stability are cavity pulling, at the level of parts in 1015 per day, and wall shift variations, at the level of parts in 10 exp 16 to parts in 10 exp 15 per day. Strategies for reducing systematic frequency variations are discussed.

  8. Advances in high frequency ultrasound separation of particulates from biomass.

    PubMed

    Juliano, Pablo; Augustin, Mary Ann; Xu, Xin-Qing; Mawson, Raymond; Knoerzer, Kai

    2017-03-01

    In recent years the use of high frequency ultrasound standing waves (megasonics) for droplet or cell separation from biomass has emerged beyond the microfluidics scale into the litre to industrial scale 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 scale transducers have been characterised with sonochemiluminescence and hydrophones to enable better reactor designs. High frequency enhanced separation technology has been demonstrated at industrial scale for oil recovery in the palm oil industry and at litre scale to assist olive oil, coconut oil and milk fat separation. Other applications include algal cell dewatering and milk fat globule fractionation. Frequency selection depends on the material properties and structure in the biomass mixture. Higher frequencies (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.

  9. 47 CFR 76.612 - Cable television frequency separation standards.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ... frequency separation standards. All cable television systems which operate in the frequency bands 108-137... kHz bandwidth in any 160 microsecond period must operate at frequencies offset from certain frequencies which may be used by aeronautical radio services operated by Commission licensees or by the United...

  10. When Does Frequency-Independent Selection Maintain Genetic Variation?

    PubMed

    Novak, Sebastian; Barton, Nicholas H

    2017-10-01

    Frequency-independent selection is generally considered as a force that acts to reduce the genetic variation in evolving populations, yet rigorous arguments for this idea are scarce. When selection fluctuates in time, it is unclear whether frequency-independent selection may maintain genetic polymorphism without invoking additional mechanisms. We show that constant frequency-independent selection with arbitrary epistasis on a well-mixed haploid population eliminates genetic variation if we assume linkage equilibrium between alleles. To this end, we introduce the notion of frequency-independent selection at the level of alleles, which is sufficient to prove our claim and contains the notion of frequency-independent selection on haploids. When selection and recombination are weak but of the same order, there may be strong linkage disequilibrium; numerical calculations show that stable equilibria are highly unlikely. Using the example of a diallelic two-locus model, we then demonstrate that frequency-independent selection that fluctuates in time can maintain stable polymorphism if linkage disequilibrium changes its sign periodically. We put our findings in the context of results from the existing literature and point out those scenarios in which the possible role of frequency-independent selection in maintaining genetic variation remains unclear. Copyright © 2017 by the Genetics Society of America.

  11. 46 CFR 111.01-17 - Voltage and frequency variations.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ....01-17 Shipping COAST GUARD, DEPARTMENT OF HOMELAND SECURITY (CONTINUED) ELECTRICAL ENGINEERING ELECTRIC SYSTEMS-GENERAL REQUIREMENTS General § 111.01-17 Voltage and frequency variations. Unless otherwise stated, electrical equipment must function at variations of at least ±5 percent of rated frequency...

  12. 46 CFR 111.01-17 - Voltage and frequency variations.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ....01-17 Shipping COAST GUARD, DEPARTMENT OF HOMELAND SECURITY (CONTINUED) ELECTRICAL ENGINEERING ELECTRIC SYSTEMS-GENERAL REQUIREMENTS General § 111.01-17 Voltage and frequency variations. Unless otherwise stated, electrical equipment must function at variations of at least ±5 percent of rated frequency...

  13. 46 CFR 111.01-17 - Voltage and frequency variations.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ....01-17 Shipping COAST GUARD, DEPARTMENT OF HOMELAND SECURITY (CONTINUED) ELECTRICAL ENGINEERING ELECTRIC SYSTEMS-GENERAL REQUIREMENTS General § 111.01-17 Voltage and frequency variations. Unless otherwise stated, electrical equipment must function at variations of at least ±5 percent of rated frequency...

  14. 46 CFR 111.01-17 - Voltage and frequency variations.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ....01-17 Shipping COAST GUARD, DEPARTMENT OF HOMELAND SECURITY (CONTINUED) ELECTRICAL ENGINEERING ELECTRIC SYSTEMS-GENERAL REQUIREMENTS General § 111.01-17 Voltage and frequency variations. Unless otherwise stated, electrical equipment must function at variations of at least ±5 percent of rated frequency...

  15. 46 CFR 111.01-17 - Voltage and frequency variations.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ....01-17 Shipping COAST GUARD, DEPARTMENT OF HOMELAND SECURITY (CONTINUED) ELECTRICAL ENGINEERING ELECTRIC SYSTEMS-GENERAL REQUIREMENTS General § 111.01-17 Voltage and frequency variations. Unless otherwise stated, electrical equipment must function at variations of at least ±5 percent of rated frequency...

  16. Dual-band frequency selective surface with large band separation and stable performance

    NASA Astrophysics Data System (ADS)

    Zhou, Hang; Qu, Shao-Bo; Peng, Wei-Dong; Lin, Bao-Qin; Wang, Jia-Fu; Ma, Hua; Zhang, Jie-Qiu; Bai, Peng; Wang, Xu-Hua; Xu, Zhuo

    2012-05-01

    A new technique of designing a dual-band frequency selective surface with large band separation is presented. This technique is based on a delicately designed topology of L- and Ku-band microwave filters. The two band-pass responses are generated by a capacitively-loaded square-loop frequency selective surface and an aperture-coupled frequency selective surface, respectively. A Faraday cage is located between the two frequency selective surface structures to eliminate undesired couplings. Based on this technique, a dual-band frequency selective surface with large band separation is designed, which possesses large band separation, high selectivity, and stable performance under various incident angles and different polarizations.

  17. The functional spectrum of low-frequency coding variation.

    PubMed

    Marth, Gabor T; Yu, Fuli; Indap, Amit R; Garimella, Kiran; Gravel, Simon; Leong, Wen Fung; Tyler-Smith, Chris; Bainbridge, Matthew; Blackwell, Tom; Zheng-Bradley, Xiangqun; Chen, Yuan; Challis, Danny; Clarke, Laura; Ball, Edward V; Cibulskis, Kristian; Cooper, David N; Fulton, Bob; Hartl, Chris; Koboldt, Dan; Muzny, Donna; Smith, Richard; Sougnez, Carrie; Stewart, Chip; Ward, Alistair; Yu, Jin; Xue, Yali; Altshuler, David; Bustamante, Carlos D; Clark, Andrew G; Daly, Mark; DePristo, Mark; Flicek, Paul; Gabriel, Stacey; Mardis, Elaine; Palotie, Aarno; Gibbs, Richard

    2011-09-14

    Rare coding variants constitute an important class of human genetic variation, but are underrepresented in current databases that are based on small population samples. Recent studies show that variants altering amino acid sequence and protein function are enriched at low variant allele frequency, 2 to 5%, but because of insufficient sample size it is not clear if the same trend holds for rare variants below 1% allele frequency. The 1000 Genomes Exon Pilot Project has collected deep-coverage exon-capture data in roughly 1,000 human genes, for nearly 700 samples. Although medical whole-exome projects are currently afoot, this is still the deepest reported sampling of a large number of human genes with next-generation technologies. According to the goals of the 1000 Genomes Project, we created effective informatics pipelines to process and analyze the data, and discovered 12,758 exonic SNPs, 70% of them novel, and 74% below 1% allele frequency in the seven population samples we examined. Our analysis confirms that coding variants below 1% allele frequency show increased population-specificity and are enriched for functional variants. This study represents a large step toward detecting and interpreting low frequency coding variation, clearly lays out technical steps for effective analysis of DNA capture data, and articulates functional and population properties of this important class of genetic variation.

  18. Multibeam single frequency synthetic aperture radar processor for imaging separate range swaths

    NASA Technical Reports Server (NTRS)

    Jain, A. (Inventor)

    1982-01-01

    A single-frequency multibeam synthetic aperture radar for large swath imaging is disclosed. Each beam illuminates a separate ""footprint'' (i.e., range and azimuth interval). The distinct azimuth intervals for the separate beams produce a distinct Doppler frequency spectrum for each beam. After range correlation of raw data, an optical processor develops image data for the different beams by spatially separating the beams to place each beam of different Doppler frequency spectrum in a different location in the frequency plane as well as the imaging plane of the optical processor. Selection of a beam for imaging may be made in the frequency plane by adjusting the position of an aperture, or in the image plane by adjusting the position of a slit. The raw data may also be processed in digital form in an analogous manner.

  19. Effects of the rate of formant-frequency variation on the grouping of formants in speech perception.

    PubMed

    Summers, Robert J; Bailey, Peter J; Roberts, Brian

    2012-04-01

    How speech is separated perceptually from other speech remains poorly understood. Recent research suggests that the ability of an extraneous formant to impair intelligibility depends on the modulation of its frequency, but not its amplitude, contour. This study further examined the effect of formant-frequency variation on intelligibility by manipulating the rate of formant-frequency change. Target sentences were synthetic three-formant (F1 + F2 + F3) analogues of natural utterances. Perceptual organization was probed by presenting stimuli dichotically (F1 + F2C + F3C; F2 + F3), where F2C + F3C constitute a competitor for F2 and F3 that listeners must reject to optimize recognition. Competitors were derived using formant-frequency contours extracted from extended passages spoken by the same talker and processed to alter the rate of formant-frequency variation, such that rate scale factors relative to the target sentences were 0, 0.25, 0.5, 1, 2, and 4 (0 = constant frequencies). Competitor amplitude contours were either constant, or time-reversed and rate-adjusted in parallel with the frequency contour. Adding a competitor typically reduced intelligibility; this reduction increased with competitor rate until the rate was at least twice that of the target sentences. Similarity in the results for the two amplitude conditions confirmed that formant amplitude contours do not influence across-formant grouping. The findings indicate that competitor efficacy is not tuned to the rate of the target sentences; most probably, it depends primarily on the overall rate of frequency variation in the competitor formants. This suggests that, when segregating the speech of concurrent talkers, differences in speech rate may not be a significant cue for across-frequency grouping of formants.

  20. The use of extrapolation concepts to augment the Frequency Separation Technique

    NASA Astrophysics Data System (ADS)

    Alexiou, Spiros

    2015-03-01

    The Frequency Separation Technique (FST) is a general method formulated to improve the speed and/or accuracy of lineshape calculations, including strong overlapping collisions, as is the case for ion dynamics. It should be most useful when combined with ultrafast methods, that, however have significant difficulties when the impact regime is approached. These difficulties are addressed by the Frequency Separation Technique, in which the impact limit is correctly recovered. The present work examines the possibility of combining the Frequency Separation Technique with the addition of extrapolation to improve results and minimize errors resulting from the neglect of fast-slow coupling and thus obtain the exact result with a minimum of extra effort. To this end the adequacy of one such ultrafast method, the Frequency Fluctuation Method (FFM) for treating the nonimpact part is examined. It is found that although the FFM is unable to reproduce the nonimpact profile correctly, its coupling with the FST correctly reproduces the total profile.

  1. Low-frequency dynamics of pressure-induced turbulent separation bubbles

    NASA Astrophysics Data System (ADS)

    Weiss, Julien; Mohammed-Taifour, Abdelouahab; Lefloch, Arnaud

    2017-11-01

    We experimentally investigate a pressure-induced turbulent separation bubble (TSB), which is generated on a flat test surface through a combination of adverse and favorable pressure gradients imposed on a nominally two-dimensional, incompressible, turbulent boundary layer. We probe the flow using piezo-resistive pressure transducers, MEMS shear-stress sensors, and high-speed, 2D-2C, PIV measurements. Through the use of Fourier analysis of the wall-pressure fluctuations and Proper Orthogonal Decomposition of the velocity fields, we show that this type of flow is characterized by a self-induced, low-frequency contraction and expansion - called breathing - of the TSB. The dominant Strouhal number of this motion, based on the TSB length and the incoming velocity in the potential flow, is of the order of 0.01. We compare this motion to the low-frequency dynamics observed in laminar separation bubbles (LSBs), geometry-induced TSBs, and shock-induced separated flows.

  2. Formant-Frequency Variation and Informational Masking of Speech by Extraneous Formants: Evidence Against Dynamic and Speech-Specific Acoustical Constraints

    PubMed Central

    2014-01-01

    How speech is separated perceptually from other speech remains poorly understood. Recent research indicates that the ability of an extraneous formant to impair intelligibility depends on the variation of its frequency contour. This study explored the effects of manipulating the depth and pattern of that variation. Three formants (F1+F2+F3) constituting synthetic analogues of natural sentences were distributed across the 2 ears, together with a competitor for F2 (F2C) that listeners must reject to optimize recognition (left = F1+F2C; right = F2+F3). The frequency contours of F1 − F3 were each scaled to 50% of their natural depth, with little effect on intelligibility. Competitors were created either by inverting the frequency contour of F2 about its geometric mean (a plausibly speech-like pattern) or using a regular and arbitrary frequency contour (triangle wave, not plausibly speech-like) matched to the average rate and depth of variation for the inverted F2C. Adding a competitor typically reduced intelligibility; this reduction depended on the depth of F2C variation, being greatest for 100%-depth, intermediate for 50%-depth, and least for 0%-depth (constant) F2Cs. This suggests that competitor impact depends on overall depth of frequency variation, not depth relative to that for the target formants. The absence of tuning (i.e., no minimum in intelligibility for the 50% case) suggests that the ability to reject an extraneous formant does not depend on similarity in the depth of formant-frequency variation. Furthermore, triangle-wave competitors were as effective as their more speech-like counterparts, suggesting that the selection of formants from the ensemble also does not depend on speech-specific constraints. PMID:24842068

  3. Gravitational dynamos and the low-frequency geomagnetic secular variation.

    PubMed

    Olson, P

    2007-12-18

    Self-sustaining numerical dynamos are used to infer the sources of low-frequency secular variation of the geomagnetic field. Gravitational dynamo models powered by compositional convection in an electrically conducting, rotating fluid shell exhibit several regimes of magnetic field behavior with an increasing Rayleigh number of the convection, including nearly steady dipoles, chaotic nonreversing dipoles, and chaotic reversing dipoles. The time average dipole strength and dipolarity of the magnetic field decrease, whereas the dipole variability, average dipole tilt angle, and frequency of polarity reversals increase with Rayleigh number. Chaotic gravitational dynamos have large-amplitude dipole secular variation with maximum power at frequencies corresponding to a few cycles per million years on Earth. Their external magnetic field structure, dipole statistics, low-frequency power spectra, and polarity reversal frequency are comparable to the geomagnetic field. The magnetic variability is driven by the Lorentz force and is characterized by an inverse correlation between dynamo magnetic and kinetic energy fluctuations. A constant energy dissipation theory accounts for this inverse energy correlation, which is shown to produce conditions favorable for dipole drift, polarity reversals, and excursions.

  4. Gravitational dynamos and the low-frequency geomagnetic secular variation

    PubMed Central

    Olson, P.

    2007-01-01

    Self-sustaining numerical dynamos are used to infer the sources of low-frequency secular variation of the geomagnetic field. Gravitational dynamo models powered by compositional convection in an electrically conducting, rotating fluid shell exhibit several regimes of magnetic field behavior with an increasing Rayleigh number of the convection, including nearly steady dipoles, chaotic nonreversing dipoles, and chaotic reversing dipoles. The time average dipole strength and dipolarity of the magnetic field decrease, whereas the dipole variability, average dipole tilt angle, and frequency of polarity reversals increase with Rayleigh number. Chaotic gravitational dynamos have large-amplitude dipole secular variation with maximum power at frequencies corresponding to a few cycles per million years on Earth. Their external magnetic field structure, dipole statistics, low-frequency power spectra, and polarity reversal frequency are comparable to the geomagnetic field. The magnetic variability is driven by the Lorentz force and is characterized by an inverse correlation between dynamo magnetic and kinetic energy fluctuations. A constant energy dissipation theory accounts for this inverse energy correlation, which is shown to produce conditions favorable for dipole drift, polarity reversals, and excursions. PMID:18048345

  5. Instantaneous and Frequency-Warped Signal Processing Techniques for Auditory Source Separation.

    NASA Astrophysics Data System (ADS)

    Wang, Avery Li-Chun

    This thesis summarizes several contributions to the areas of signal processing and auditory source separation. The philosophy of Frequency-Warped Signal Processing is introduced as a means for separating the AM and FM contributions to the bandwidth of a complex-valued, frequency-varying sinusoid p (n), transforming it into a signal with slowly-varying parameters. This transformation facilitates the removal of p (n) from an additive mixture while minimizing the amount of damage done to other signal components. The average winding rate of a complex-valued phasor is explored as an estimate of the instantaneous frequency. Theorems are provided showing the robustness of this measure. To implement frequency tracking, a Frequency-Locked Loop algorithm is introduced which uses the complex winding error to update its frequency estimate. The input signal is dynamically demodulated and filtered to extract the envelope. This envelope may then be remodulated to reconstruct the target partial, which may be subtracted from the original signal mixture to yield a new, quickly-adapting form of notch filtering. Enhancements to the basic tracker are made which, under certain conditions, attain the Cramer -Rao bound for the instantaneous frequency estimate. To improve tracking, the novel idea of Harmonic -Locked Loop tracking, using N harmonically constrained trackers, is introduced for tracking signals, such as voices and certain musical instruments. The estimated fundamental frequency is computed from a maximum-likelihood weighting of the N tracking estimates, making it highly robust. The result is that harmonic signals, such as voices, can be isolated from complex mixtures in the presence of other spectrally overlapping signals. Additionally, since phase information is preserved, the resynthesized harmonic signals may be removed from the original mixtures with relatively little damage to the residual signal. Finally, a new methodology is given for designing linear-phase FIR filters

  6. 47 CFR 76.612 - Cable television frequency separation standards.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ... 47 Telecommunication 4 2011-10-01 2011-10-01 false Cable television frequency separation standards. 76.612 Section 76.612 Telecommunication FEDERAL COMMUNICATIONS COMMISSION (CONTINUED) BROADCAST RADIO SERVICES MULTICHANNEL VIDEO AND CABLE TELEVISION SERVICE Technical Standards § 76.612 Cable television...

  7. Seasonal variations of volcanic eruption frequencies

    NASA Technical Reports Server (NTRS)

    Stothers, Richard B.

    1989-01-01

    Do volcanic eruptions have a tendency to occur more frequently in the months of May and June? Some past evidence suggests that they do. The present study, based on the new eruption catalog of Simkin et al.(1981), investigates the monthly statistics of the largest eruptions, grouped according to explosive magnitude, geographical latitude, and year. At the 2-delta level, no month-to-month variations in eruption frequency are found to be statistically significant. Examination of previously published month-to-month variations suggests that they, too, are not statistically significant. It is concluded that volcanism, at least averaged over large portions of the globe, is probably not periodic on a seasonal or annual time scale.

  8. Os incae: variation in frequency in major human population groups

    PubMed Central

    HANIHARA, TSUNEHIKO; ISHIDA, HAJIME

    2001-01-01

    The variation in frequency of the Inca bone was examined in major human populations around the world. The New World populations have generally high frequencies of the Inca bone, whereas lower frequencies occur in northeast Asians and Australians. Tibetan/Nepalese and Assam/Sikkim populations in northeast India have more Inca bones than do neighbouring populations. Among modern populations originally derived from eastern Asian population stock, the frequencies are highest in some of the marginal isolated groups. In Central and West Asia as well as in Europe, frequency of the Inca bone is relatively low. The incidence of the complete Inca bone is, moreover, very low in the western hemisphere of the Old World except for Subsaharan Africa. Subsaharan Africans show as a whole a second peak in the occurrence of the Inca bone. Geographical and ethnographical patterns of the frequency variation of the Inca bone found in this study indicate that the possible genetic background for the occurrence of this bone cannot be completely excluded. Relatively high frequencies of the Inca bone in Subsaharan Africans indicate that this trait is not a uniquely eastern Asian regional character. PMID:11273039

  9. Vela X-1 pulse timing. II - Variations in pulse frequency

    NASA Technical Reports Server (NTRS)

    Deeter, J. E.; Boynton, P. E.; Lamb, F. K.; Zylstra, G.

    1989-01-01

    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 frequency are identified on time scales from 2 to 2600 days; the lower nine octaves are characterized as white noise (or random walk in pulse frequency), while the longer-period variations are attributed to changes in neutron-star rotation rates.

  10. System identification through nonstationary data using Time-Frequency Blind Source Separation

    NASA Astrophysics Data System (ADS)

    Guo, Yanlin; Kareem, Ahsan

    2016-06-01

    Classical output-only system identification (SI) methods are based on the assumption of stationarity of the system response. However, measured response of buildings and bridges is usually non-stationary due to strong winds (e.g. typhoon, and thunder storm etc.), earthquakes and time-varying vehicle motions. Accordingly, the response data may have time-varying frequency contents and/or overlapping of modal frequencies due to non-stationary colored excitation. This renders traditional methods problematic for modal separation and identification. To address these challenges, a new SI technique based on Time-Frequency Blind Source Separation (TFBSS) is proposed. By selectively utilizing "effective" information in local regions of the time-frequency plane, where only one mode contributes to energy, the proposed technique can successfully identify mode shapes and recover modal responses from the non-stationary response where the traditional SI methods often encounter difficulties. This technique can also handle response with closely spaced modes which is a well-known challenge for the identification of large-scale structures. Based on the separated modal responses, frequency and damping can be easily identified using SI methods based on a single degree of freedom (SDOF) system. In addition to the exclusive advantage of handling non-stationary data and closely spaced modes, the proposed technique also benefits from the absence of the end effects and low sensitivity to noise in modal separation. The efficacy of the proposed technique is demonstrated using several simulation based studies, and compared to the popular Second-Order Blind Identification (SOBI) scheme. It is also noted that even some non-stationary response data can be analyzed by the stationary method SOBI. This paper also delineates non-stationary cases where SOBI and the proposed scheme perform comparably and highlights cases where the proposed approach is more advantageous. Finally, the performance of the

  11. Separation of Intercepted Multi-Radar Signals Based on Parameterized Time-Frequency Analysis

    NASA Astrophysics Data System (ADS)

    Lu, W. L.; Xie, J. W.; Wang, H. M.; Sheng, C.

    2016-09-01

    Modern radars use complex waveforms to obtain high detection performance and low probabilities of interception and identification. Signals intercepted from multiple radars overlap considerably in both the time and frequency domains and are difficult to separate with primary time parameters. Time-frequency analysis (TFA), as a key signal-processing tool, can provide better insight into the signal than conventional methods. In particular, among the various types of TFA, parameterized time-frequency analysis (PTFA) has shown great potential to investigate the time-frequency features of such non-stationary signals. In this paper, we propose a procedure for PTFA to separate overlapped radar signals; it includes five steps: initiation, parameterized time-frequency analysis, demodulating the signal of interest, adaptive filtering and recovering the signal. The effectiveness of the method was verified with simulated data and an intercepted radar signal received in a microwave laboratory. The results show that the proposed method has good performance and has potential in electronic reconnaissance applications, such as electronic intelligence, electronic warfare support measures, and radar warning.

  12. Analysis of all-frequency variational behavior of the Kirchhoff approximation for a classic surface-scattering model

    NASA Technical Reports Server (NTRS)

    Bird, J. F.

    1985-01-01

    In testing a stochastic variational principle at high frequencies by using a Kirchhoffean trial function in an idealized model for surface scattering - a randomly embossed plane - we have found not only the predicted high-frequency improvement but also an unexpected low-frequency improvement in the calculated scattering amplitudes. To investigate systematically the all-frequency variational behavior, we consider here the deterministic one-boss case - Rayleigh's classic model whose exact solution is available for comparison - over all wavelengths, polarizations, and configurations of incidence and scattering. We examine analytically in particular the long-wave limit of the variational-Kirchhoff amplitudes; the results demonstrate improvements in both wavelength and angle depedence for horizontal (TM) polarization and some variational improvements for vertical (TE) polarization. This low-frequency behavior in tandem with the foreseen high-frequency improvement leads to good variational-Kirchhoff results through the intermediate resonance-frequency regime for this model.

  13. Time-frequency approach to underdetermined blind source separation.

    PubMed

    Xie, Shengli; Yang, Liu; Yang, Jun-Mei; Zhou, Guoxu; Xiang, Yong

    2012-02-01

    This paper presents a new time-frequency (TF) underdetermined blind source separation approach based on Wigner-Ville distribution (WVD) and Khatri-Rao product to separate N non-stationary sources from M(M <; N) mixtures. First, an improved method is proposed for estimating the mixing matrix, where the negative value of the auto WVD of the sources is fully considered. Then after extracting all the auto-term TF points, the auto WVD value of the sources at every auto-term TF point can be found out exactly with the proposed approach no matter how many active sources there are as long as N ≤ 2M-1. Further discussion about the extraction of auto-term TF points is made and finally the numerical simulation results are presented to show the superiority of the proposed algorithm by comparing it with the existing ones.

  14. Time-frequency analysis of time-varying modulated signals based on improved energy separation by iterative generalized demodulation

    NASA Astrophysics Data System (ADS)

    Feng, Zhipeng; Chu, Fulei; Zuo, Ming J.

    2011-03-01

    Energy separation algorithm is good at tracking instantaneous changes in frequency and amplitude of modulated signals, but it is subject to the constraints of mono-component and narrow band. In most cases, time-varying modulated vibration signals of machinery consist of multiple components, and have so complicated instantaneous frequency trajectories on time-frequency plane that they overlap in frequency domain. For such signals, conventional filters fail to obtain mono-components of narrow band, and their rectangular decomposition of time-frequency plane may split instantaneous frequency trajectories thus resulting in information loss. Regarding the advantage of generalized demodulation method in decomposing multi-component signals into mono-components, an iterative generalized demodulation method is used as a preprocessing tool to separate signals into mono-components, so as to satisfy the requirements by energy separation algorithm. By this improvement, energy separation algorithm can be generalized to a broad range of signals, as long as the instantaneous frequency trajectories of signal components do not intersect on time-frequency plane. Due to the good adaptability of energy separation algorithm to instantaneous changes in signals and the mono-component decomposition nature of generalized demodulation, the derived time-frequency energy distribution has fine resolution and is free from cross term interferences. The good performance of the proposed time-frequency analysis is illustrated by analyses of a simulated signal and the on-site recorded nonstationary vibration signal of a hydroturbine rotor during a shut-down transient process, showing that it has potential to analyze time-varying modulated signals of multi-components.

  15. Refractivity variations and propagation at Ultra High Frequency

    NASA Astrophysics Data System (ADS)

    Alam, I.; Najam-Ul-Islam, M.; Mujahid, U.; Shah, S. A. A.; Ul Haq, Rizwan

    Present framework is established to deal with the refractivity variations normally affected the radio waves propagation at different frequencies, ranges and different environments. To deal such kind of effects, many researchers proposed several methodologies. One method is to use the parameters from meteorology to investigate these effects of variations in refractivity on propagation. These variations are region specific and we have selected a region of one kilometer height over the English Channel. We have constructed different modified refractivity profiles based on the local meteorological data. We have recorded more than 48 million received signal strength from a communication links of 50 km operating at 2015 MHz in the Ultra High Frequency band giving path loss between transmitting and receiving stations of the experimental setup. We have used parabolic wave equation method to simulate an hourly value of signal strength and compared the obtained simulated loss to the experimental loss. The analysis is made to compute refractivity distribution of standard (STD) and ITU (International Telecommunication Union) refractivity profiles for various evaporation ducts. It is found that a standard refractivity profile is better than the ITU refractivity profiles for the region at 2015 MHz. Further, it is inferred from the analysis of results that 10 m evaporation duct height is the dominant among all evaporation duct heights considered in the research.

  16. Determinants of echolocation call frequency variation in the Formosan lesser horseshoe bat (Rhinolophus monoceros)

    PubMed Central

    Chen, Shiang-Fan; Jones, Gareth; Rossiter, Stephen J.

    2009-01-01

    The origin and maintenance of intraspecific variation in vocal signals is important for population divergence and speciation. Where vocalizations are transmitted by vertical cultural inheritance, similarity will reflect co-ancestry, and thus vocal divergence should reflect genetic structure. Horseshoe bats are characterized by echolocation calls dominated by a constant frequency component that is partly determined by maternal imprinting. Although previous studies showed that constant frequency calls are also influenced by some non-genetic factors, it is not known how frequency relates to genetic structure. To test this, we related constant frequency variation to genetic and non-genetic variables in the Formosan lesser horseshoe bat (Rhinolophus monoceros). Recordings of bats from across Taiwan revealed that females called at higher frequencies than males; however, we found no effect of environmental or morphological factors on call frequency. By comparison, variation showed clear population structure, with frequencies lower in the centre and east, and higher in the north and south. Within these regions, frequency divergence was directional and correlated with geographical distance, suggesting that call frequencies are subject to cultural drift. However, microsatellite clustering analysis showed that broad differences in constant frequency among populations corresponded to discontinuities in allele frequencies resulting from vicariant events. Our results provide evidence that the processes shaping genetic subdivision have concomitant consequences for divergence in echolocation call frequency. PMID:19692399

  17. SENSITIVITY OF CONDITIONAL-DISCRIMINATION PERFORMANCE TO WITHIN-SESSION VARIATION OF REINFORCER FREQUENCY

    PubMed Central

    Ward, Ryan D; Odum, Amy L

    2008-01-01

    The present experiment developed a methodology for assessing sensitivity of conditional-discrimination performance to within-session variation of reinforcer frequency. Four pigeons responded under a multiple schedule of matching-to-sample components in which the ratio of reinforcers for correct S1 and S2 responses was varied across components within session. Initially, five components, each arranging a different reinforcer-frequency ratio (from 1∶9 to 9∶1), were presented randomly within a session. Under this condition, sensitivity to reinforcer frequency was low. Sensitivity failed to improve after extended exposure to this condition, and under a condition in which only three reinforcer-frequency ratios were varied within session. In a later condition, three reinforcer-frequency ratios were varied within session, but the reinforcer-frequency ratio in effect was differentially signaled within each component. Under this condition, values of sensitivity were similar to those traditionally obtained when reinforcer-frequency ratios for correct responses are varied across conditions. The effects of signaled vs. unsignaled reinforcer-frequency ratios were replicated in two subsequent conditions. The present procedure could provide a practical alternative to parametric variation of reinforcer frequency across conditions and may be useful in characterizing the effects of a variety of manipulations on steady-state sensitivity to reinforcer frequency. PMID:19070338

  18. The Radio Frequency Fragment Separator for Rare Isotope Beams at the NSCL

    NASA Astrophysics Data System (ADS)

    Stoker, Joshua; Andreev, Vladimir; Bazin, Daniel; Becerril, Ana; Doleans, Marc; Gorelov, Dimitry; Glennon, Patrick; Grimm, Terry; Lawton, Don; Mantica, Paul; Marti, Felix; Ottarson, Jack; Schatz, Hendrik; Vincent, John; Wagner, Jim; Wu, Xiaoyu; Zeller, Al

    2006-10-01

    Secondary beams at the National Superconducting Cyclotron Laboratory (NSCL) are separated through a combined application of magnetic rigidity and energy loss filtering. Design and construction of a Radio Frequency Fragment Separator (RFFS) for further beam purification is underway. The RFFS will apply a time-varying electromagnetic field to induce transverse beam separation. This method relies on velocity differences of the beam species to selectivey apply separation to unwanted fragments. The technical design of the RFFS and the expected purification of exotic beams are shown in detail[1]. [1] Gorelev, D. et al., ``RF Kicker System for Secondary Beams at the NSCL'' Proc of Part Accel Conf 2005, Knoxville, TN

  19. Low-Frequency Flow Oscillations on Stalled Wings Exhibiting Cellular Separation Topology

    NASA Astrophysics Data System (ADS)

    Disotell, Kevin James

    One of the most pervasive threats to aircraft controllability is wing stall, a condition associated with loss of lift due to separation of air flow from the wing surface at high angles of attack. A recognized need for improved upset recovery training in extended-envelope flight simulators is a physical understanding of the post-stall aerodynamic environment, particularly key flow phenomena which influence the vehicle trajectory. Large-scale flow structures known as stall cells, which scale with the wing chord and are spatially-periodic along the span, have been previously observed on post-stall airfoils with trailing-edge separation present. Despite extensive documentation of stall cells in the literature, the physical mechanisms behind their formation and evolution have proven to be elusive. The undertaken study has sought to characterize the inherently turbulent separated flow existing above the wing surface with cell formation present. In particular, the question of how the unsteady separated flow may interact with the wing to produce time-averaged cellular surface patterns is considered. Time-resolved, two-component particle image velocimetry measurements were acquired at the plane of symmetry of a single stall cell formed on an extruded NACA 0015 airfoil model at chord Reynolds number of 560,000 to obtain insight into the time-dependent flow structure. The evolution of flow unsteadiness was analyzed over a static angle-of-attack range covering the narrow post-stall regime in which stall cells have been observed. Spectral analysis of velocity fields acquired near the stall angle confirmed a low-frequency flow oscillation previously detected in pointwise surface measurements by Yon and Katz (1998), corresponding to a Strouhal number of 0.042 based on frontal projected chord height. Probability density functions of the streamwise velocity component were used to estimate the convective speed of this mode at approximately half the free-stream velocity, in agreement

  20. Blind source separation based on time-frequency morphological characteristics for rigid acoustic scattering by underwater objects

    NASA Astrophysics Data System (ADS)

    Yang, Yang; Li, Xiukun

    2016-06-01

    Separation of the components of rigid acoustic scattering by underwater objects is essential in obtaining the structural characteristics of such objects. To overcome the problem of rigid structures appearing to have the same spectral structure in the time domain, time-frequency Blind Source Separation (BSS) can be used in combination with image morphology to separate the rigid scattering components of different objects. Based on a highlight model, the separation of the rigid scattering structure of objects with time-frequency distribution is deduced. Using a morphological filter, different characteristics in a Wigner-Ville Distribution (WVD) observed for single auto term and cross terms can be simplified to remove any cross-term interference. By selecting time and frequency points of the auto terms signal, the accuracy of BSS can be improved. An experimental simulation has been used, with changes in the pulse width of the transmitted signal, the relative amplitude and the time delay parameter, in order to analyzing the feasibility of this new method. Simulation results show that the new method is not only able to separate rigid scattering components, but can also separate the components when elastic scattering and rigid scattering exist at the same time. Experimental results confirm that the new method can be used in separating the rigid scattering structure of underwater objects.

  1. Time-Frequency Masking for Speech Separation and Its Potential for Hearing Aid Design

    PubMed Central

    Wang, DeLiang

    2008-01-01

    A new approach to the separation of speech from speech-in-noise mixtures is the use of time-frequency (T-F) masking. Originated in the field of computational auditory scene analysis, T-F masking performs separation in the time-frequency domain. This article introduces the T-F masking concept and reviews T-F masking algorithms that separate target speech from either monaural or binaural mixtures, as well as microphone-array recordings. The review emphasizes techniques that are promising for hearing aid design. This article also surveys recent studies that evaluate the perceptual effects of T-F masking techniques, particularly their effectiveness in improving human speech recognition in noise. An assessment is made of the potential benefits of T-F masking methods for the hearing impaired in light of the processing constraints of hearing aids. Finally, several issues pertinent to T-F masking are discussed. PMID:18974204

  2. Ion mobility spectrometer using frequency-domain separation

    DOEpatents

    Martin, S.J.; Butler, M.A.; Frye, G.C.; Schubert, W.K.

    1998-08-04

    An apparatus and method are provided for separating and analyzing chemical species in an ion mobility spectrometer using a frequency-domain technique wherein the ions generated from the chemical species are selectively transported through an ion flow channel having a moving electrical potential therein. The moving electrical potential allows the ions to be selected according to ion mobility, with certain of the ions being transported to an ion detector and other of the ions being effectively discriminated against. The apparatus and method have applications for sensitive chemical detection and analysis for monitoring of exhaust gases, hazardous waste sites, industrial processes, aerospace systems, non-proliferation, and treaty verification. The apparatus can be formed as a microelectromechanical device (i.e. a micromachine). 6 figs.

  3. Ion mobility spectrometer using frequency-domain separation

    DOEpatents

    Martin, Stephen J.; Butler, Michael A.; Frye, Gregory C.; Schubert, W. Kent

    1998-01-01

    An apparatus and method is provided for separating and analyzing chemical species in an ion mobility spectrometer using a frequency-domain technique wherein the ions generated from the chemical species are selectively transported through an ion flow channel having a moving electrical potential therein. The moving electrical potential allows the ions to be selected according to ion mobility, with certain of the ions being transported to an ion detector and other of the ions being effectively discriminated against. The apparatus and method have applications for sensitive chemical detection and analysis for monitoring of exhaust gases, hazardous waste sites, industrial processes, aerospace systems, non-proliferation, and treaty verification. The apparatus can be formed as a microelectromechanical device (i.e. a micromachine).

  4. Spatial pattern separation of chemicals and frequency-independent components by terahertz spectroscopic imaging

    NASA Astrophysics Data System (ADS)

    Watanabe, Yuuki; Kawase, Kodo; Ikari, Tomofumi; Ito, Hiromasa; Ishikawa, Youichi; Minamide, Hiroaki

    2003-10-01

    We separated the component spatial patterns of frequency-dependent absorption in chemicals and frequency-independent components such as plastic, paper, and measurement noise in terahertz (THz) spectroscopic images, using known spectral curves. Our measurement system, which uses a widely tunable coherent THz-wave parametric oscillator source, can image at a specific frequency in the range 1-2 THz. The component patterns of chemicals can easily be extracted by use of the frequency-independent components. This method could be successfully used for nondestructive inspection for the detection of illegal drugs and devices of bioterrorism concealed, e.g., inside mail and packages.

  5. High-performance radio frequency transistors based on diameter-separated semiconducting carbon nanotubes

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

    Cao, Yu; Che, Yuchi; Zhou, Chongwu, E-mail: chongwuz@usc.edu

    In this paper, we report the high-performance radio-frequency transistors based on the single-walled semiconducting carbon nanotubes with a refined average diameter of ∼1.6 nm. These diameter-separated carbon nanotube transistors show excellent transconductance of 55 μS/μm and desirable drain current saturation with an output resistance of ∼100 KΩ μm. An exceptional radio-frequency performance is also achieved with current gain and power gain cut-off frequencies of 23 GHz and 20 GHz (extrinsic) and 65 GHz and 35 GHz (intrinsic), respectively. These radio-frequency metrics are among the highest reported for the carbon nanotube thin-film transistors. This study provides demonstration of radio frequency transistors based on carbon nanotubes with tailoredmore » diameter distributions, which will guide the future application of carbon nanotubes in radio-frequency electronics.« less

  6. Separation of O/X Polarization Modes on Oblique Ionospheric Soundings

    NASA Astrophysics Data System (ADS)

    Harris, T. J.; Cervera, M. A.; Pederick, L. H.; Quinn, A. D.

    2017-12-01

    The oblique-incidence sounder (OIS) is a well-established instrument for determining the state of the ionosphere, with several advantages over vertical-incidence sounders (VIS). However, the processing and interpretation of OIS ionograms is more complicated than that of VIS ionograms. Due to the Earth's magnetic field, the ionosphere is birefringent at radio frequencies and a VIS or OIS will typically see two distinct ionospheric returns, known as the O and X modes. The separation of these two modes on a VIS, using a polarimetric receive antenna, is a well-established technique. However, this process is more complicated on an OIS due to a variable separation in the phase difference between the two modes, as measured between the two arms of a polarimetric antenna. Using a polarimetric antenna that can be rotated and tilted, we show that this variation in phase separation within an ionogram is caused by the variation in incidence angle, with some configurations leading to greater variation in phase separation. We then develop an algorithm for separating O and X modes in oblique ionograms that can account for the variation in phase separation, and we demonstrate successful separation even in relatively difficult cases. The variation in phase separation can also be exploited to estimate the incident elevation, a technique which may be useful for other applications of HF radio.

  7. Time Variation of the Distance Separating Bomb and Dive Bomber Subsequent to Bomb Release

    NASA Technical Reports Server (NTRS)

    Mathews, Charles W.

    1952-01-01

    A study has been made of the variation of the distance separating bomb and aircraft with time after release as applied to dive-bombing operations, Separation distances determined from this study are presented in terms of two variables only, dive angle and maximum airplane accelerometer reading; the values of separation distance include the effects of delay in initiation of the pull-out and lag in attainment of the maximum normal acceleration.Contains analysis and calculations of the separation distances between bomb and dive bomber following bomb release, Separation distances as determined by the dive angle and the maximum airplane accelerometer reading are presented in a single chart.

  8. Relative importance of precipitation frequency and intensity in inter-annual variation of precipitation in Singapore during 1980-2013

    NASA Astrophysics Data System (ADS)

    Li, Xin; Babovic, Vladan

    2017-04-01

    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 frequency and intensity, understanding of the relative importance of frequency 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 frequency 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 frequency 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, frequency and intensity at both annual and seasonal time scales. Then, the relative importance of precipitation frequency 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, frequency and intensity at annual time scale, 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 scale 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 frequency. These results have

  9. High-frequency counter-flow plasma synthetic jet actuator and its application in suppression of supersonic flow separation

    NASA Astrophysics Data System (ADS)

    Wang, Hongyu; Li, Jun; Jin, Di; Tang, Mengxiao; Wu, Yun; Xiao, Lianghua

    2018-01-01

    We come up with a control strategy for suppression of supersonic flow separation based on high-frequency Counter-flow Plasma Synthetic Jet Actuator (CPSJA). The main purpose of this investigation is to verify if its control authority can be enhanced by the jet/shock interaction. We use a blunt nose to generate a bow shock, a step on a flat plate to introduce a massive separation in a Mach 2 wind tunnel, and the CPSJA to generate Plasma Synthetic Jet (PSJ). In this study, pulsed capacitive discharge is provided for an array of CPSJAs, which makes the actuation (discharge) frequency f1 = 1 kHz, f2 = 2 kHz and f3 = 3 kHz. We use the high-speed schlieren imaging and fast response pressure transducers as well as a numerical simulation to investigate the quiescent PSJ properties, the interaction between the jet and bow shock, and its disturbance effect on the downstream separated region. The schlieren images show that PSJ is characterized by a succession of vortex rings; the jet strength weakens with the increase of frequency. A 4.5 mN jet thrust is found for all the frequencies. The simulation results show that jet/shock interaction produces vorticity in the vortex ring of the jet, enhancing turbulent mixing in PSJ so that a great deal of momentum is produced into the flow. We found the downstream flow is significantly disturbed by the enhanced actuation. Actuation with frequency of f2, f3 which is close to the natural frequency fn of the separation bubble suppresses the separation with the upstream laminar boundary layer being periodically attenuated, which has a better control effect than f1. The control effect is sensitive to the position where PSJ interacts with the shear layer, but the amount of energy deposited in one pulse is not crucial in a separation reduction in the experiment.

  10. Wide Angle, Single Screen, Gridded Square-Loop Frequency Selective Surface for Diplexing Two Closely Separated Frequency Bands

    NASA Technical Reports Server (NTRS)

    Wu, Te-Kao (Inventor)

    1996-01-01

    The design and performance of a wide angle, single screen, frequency selective surface (FSS) with gridded square-loop path elements are described for diplexing closely separated signal bands, for example, X- and Ku-band signals in an Orbiting Very Long Baseline Interferometer (OVLBI) earth station reflector antenna system, as well as other applications such as military and commercial communications via satellites. Excellent agreement is obtained between the predicted and measured results of this FSS design using the gridded square-loop patch elements sandwiched between 0.0889 cm thick tetrafluoroethylene fluorocarbon polymer (PTFE) slabs. Resonant frequency drift is reduced by 1 GHz with an incidence angle from 0 deg normal to 40 deg from normal.

  11. Intra-individual and inter-individual variations in sperm aneuploidy frequencies in normal men.

    PubMed

    Tempest, Helen G; Ko, Evelyn; Rademaker, Alfred; Chan, Peter; Robaire, Bernard; Martin, Renée H

    2009-01-01

    To investigate whether there are intra-individual and/or inter-individual variations in sperm aneuploidy frequencies within the normal male population, and, if this is the case, whether they are sporadic or time-stable variants. Prospective study. University research laboratory. Ten men aged 18-32 years. None. Fluorescence in situ hybridization was used to investigate sperm aneuploidy frequencies for chromosomes X, Y, 13, and 21 in serial semen samples collected over a period of 12-18 months. Intra-individual and inter-individual variations were investigated by comparing serial samples from the same donor and by comparing the donors with each other, respectively. Intra-individual variations were found in all 10 donors for at least one investigated chromosome; variations tended to be sporadic events affecting only one time point. Inter-individual variations were found for all chromosomes (except XX and YY disomy and disomy 21), with three men identified as stable variants, consistently producing higher levels of aneuploidy for at least one of the following aneuploidies: sex chromosome nullisomy; disomy 13, or diploidy. These results suggest that there are a number of factors and mechanisms that have the potential to sporadically or consistently affect sperm aneuploidy.

  12. Production frequency effects in perception of phonological variation

    NASA Astrophysics Data System (ADS)

    Connine, Cynthia M.; Ranbom, Larissa J.

    2004-05-01

    Two experiments were conducted that investigated the relationship between phonological variant occurrence frequency (based on a corpus analysis of conversational speech) and auditory word recognition. The variant investigated was an alternation between the presence of [nt] and a nasal flap (e.g., center, cen'er). The corpus analysis showed that 80% of productions are nasal flaps, with wide variability across words (from 0% for ``enter'' to 100% for ``twenty''). In a production goodness rating experiment, listeners rated [nt] productions as better than their nasal flap counterparts. For individual items, a strong positive correlation was found between nasal flap frequency and goodness ratings: words typically produced with nasal flaps were rated as better productions. A lexical decision experiment showed that nasal flap variants were recognized more slowly and less accurately than [nt] versions. The rated quality of the nasal-flapped production was strongly correlated with the results of the lexical decision task: nasal-flapped words considered highly acceptable were recognized more quickly and accurately than words rated as poor nasal flap productions. The results demonstrate a strong relationship between experienced variant frequency and auditory word recognition and suggest that phonological variation is explicitly represented in the mental lexicon.

  13. Genetic variation among the Mapuche Indians from the Patagonian region of Argentina: mitochondrial DNA sequence variation and allele frequencies of several nuclear genes.

    PubMed

    Ginther, C; Corach, D; Penacino, G A; Rey, J A; Carnese, F R; Hutz, M H; Anderson, A; Just, J; Salzano, F M; King, M C

    1993-01-01

    DNA samples from 60 Mapuche Indians, representing 39 maternal lineages, were genetically characterized for (1) nucleotide sequences of the mtDNA control region; (2) presence or absence of a nine base duplication in mtDNA region V; (3) HLA loci DRB1 and DQA1; (4) variation at three nuclear genes with short tandem repeats; and (5) variation at the polymorphic marker D2S44. The genetic profile of the Mapuche population was compared to other Amerinds and to worldwide populations. Two highly polymorphic portions of the mtDNA control region, comprising 650 nucleotides, were amplified by the polymerase chain reaction (PCR) and directly sequenced. The 39 maternal lineages were defined by two or three generation families identified by the Mapuches. These 39 lineages included 19 different mtDNA sequences that could be grouped into four classes. The same classes of sequences appear in other Amerinds from North, Central, and South American populations separated by thousands of miles, suggesting that the origin of the mtDNA patterns predates the migration to the Americas. The mtDNA sequence similarity between Amerind populations suggests that the migration throughout the Americas occurred rapidly relative to the mtDNA mutation rate. HLA DRB1 alleles 1602 and 1402 were frequent among the Mapuches. These alleles also occur at high frequency among other Amerinds in North and South America, but not among Spanish, Chinese or African-American populations. The high frequency of these alleles throughout the Americas, and their specificity to the Americas, supports the hypothesis that Mapuches and other Amerind groups are closely related.(ABSTRACT TRUNCATED AT 250 WORDS)

  14. High Frequency Variations of Earth Rotation Parameters from GPS and GLONASS Observations

    PubMed Central

    Wei, Erhu; Jin, Shuanggen; Wan, Lihua; Liu, Wenjie; Yang, Yali; Hu, Zhenghong

    2015-01-01

    The Earth's rotation undergoes changes with the influence of geophysical factors, such as Earth's surface fluid mass redistribution of the atmosphere, ocean and hydrology. However, variations of Earth Rotation Parameters (ERP) are still not well understood, particularly the short-period variations (e.g., diurnal and semi-diurnal variations) and their causes. In this paper, the hourly time series of Earth Rotation Parameters are estimated using Global Positioning System (GPS), Global Navigation Satellite System (GLONASS), and combining GPS and GLONASS data collected from nearly 80 sites from 1 November 2012 to 10 April 2014. These new observations with combining different satellite systems can help to decorrelate orbit biases and ERP, which improve estimation of ERP. The high frequency variations of ERP are analyzed using a de-trending method. The maximum of total diurnal and semidiurnal variations are within one milli-arcseconds (mas) in Polar Motion (PM) and 0.5 milli-seconds (ms) in UT1-UTC. The semidiurnal and diurnal variations are mainly related to the ocean tides. Furthermore, the impacts of satellite orbit and time interval used to determinate ERP on the amplitudes of tidal terms are analyzed. We obtain some small terms that are not described in the ocean tide model of the IERS Conventions 2010, which may be caused by the strategies and models we used or the signal noises as well as artifacts. In addition, there are also small differences on the amplitudes between our results and IERS convention. This might be a result of other geophysical excitations, such as the high-frequency variations in atmospheric angular momentum (AAM) and hydrological angular momentum (HAM), which needs more detailed analysis with more geophysical data in the future. PMID:25635416

  15. Effects of variations of stage and flux at different frequencies on the estimates using river stage tomography

    NASA Astrophysics Data System (ADS)

    Wang, Y. L.; Yeh, T. C. J.; Wen, J. C.

    2017-12-01

    This study is to investigate the ability of river stage tomography to estimate the spatial distribution of hydraulic transmissivity (T), storage coefficient (S), and diffusivity (D) in groundwater basins using information of groundwater level variations induced by periodic variations of stream stage, and infiltrated flux from the stream boundary. In order to accomplish this objective, the sensitivity and correlation of groundwater heads with respect to the hydraulic properties is first conducted to investigate the spatial characteristics of groundwater level in response to the stream variations at different frequencies. Results of the analysis show that the spatial distributions of the sensitivity of heads at an observation well in response to periodic river stage variations are highly correlated despite different frequencies. On the other hand, the spatial patterns of the sensitivity of the observed head to river flux boundaries at different frequencies are different. Specifically, the observed head is highly correlated with T at the region between the stream and observation well when the high-frequency periodic flux is considered. On the other hand, it is highly correlated with T at the region between monitoring well and the boundary opposite to the stream when the low-frequency periodic flux is prescribed to the stream. We also find that the spatial distributions of the sensitivity of observed head to S variation are highly correlated with all frequencies in spite of heads or fluxes stream boundary. Subsequently, the differences of the spatial correlations of the observed heads to the hydraulic properties under the head and flux boundary conditions are further investigated by an inverse model (i.e., successive stochastic linear estimator). This investigation uses noise-free groundwater and stream data of a synthetic aquifer, where aquifer heterogeneity is known exactly. The ability of river stage tomography is then tested with these synthetic data sets to

  16. Seasonal Variations of the James Webb Space Telescope Orbital Dynamics

    NASA Technical Reports Server (NTRS)

    Brown, Jonathan; Peterson, Jeremy; Villac, Benjamin; Yu, Wayne

    2015-01-01

    LV separation state is fixed ECEF, so inertial states vary with hourly, daily, monthly, and yearly frequencies The net effect of all frequencies leads to significant variations in orbit geometry Injection states can be matched with invariant manifolds of periodic orbits in the CR3BP to explain observed final orbit.

  17. Ecological drivers of variation in tool-use frequency across sea otter populations

    USGS Publications Warehouse

    Fujii, Jessica; Ralls, Katherine; Tinker, M. Tim

    2015-01-01

    Sea otters are well-known tool users, employing objects such as rocks or shells to break open hard-shelled invertebrate prey. However, little is known about how the frequency of tool use varies among sea otter populations and the factors that drive these differences. We examined 17 years of observational data on prey capture and tool use from 8 sea otter populations ranging from southern California to the Aleutian Islands in Alaska. There were significant differences in the diets of these populations as well as variation in the frequency of tool use. Sea otters at Amchitka Island, Alaska, used tools on less than 1% of dives that resulted in the capture of prey compared with approximately 16% in Monterey, California. The percentage of individuals in the population that used tools ranged from 10% to 93%. In all populations, marine snails and thick-shelled bivalves were most likely to be associated with tool use, whereas soft-bodied prey items such as worms and sea stars were the least likely. The probability that a tool would be used on a given prey type varied across populations. The morphology of the prey item being handled and the prevalence of various types of prey in local diets were major ecological drivers of tool use: together they accounted for about 64% of the variation in tool-use frequency among populations. The remaining variation may be related to changes in the relative costs and benefits to an individual otter of learning to use tools effectively under differing ecological circumstances.

  18. Rapid variations in fluid chemistry constrain hydrothermal phase separation at the Main Endeavour Field

    NASA Astrophysics Data System (ADS)

    Love, Brooke; Lilley, Marvin; Butterfield, David; Olson, Eric; Larson, Benjamin

    2017-02-01

    Previous work at the Main Endeavour Field (MEF) has shown that chloride concentration in high-temperature vent fluids has not exceeded 510 mmol/kg (94% of seawater), which is consistent with brine condensation and loss at depth, followed by upward flow of a vapor phase toward the seafloor. Magmatic and seismic events have been shown to affect fluid temperature and composition and these effects help narrow the possibilities for sub-surface processes. However, chloride-temperature data alone are insufficient to determine details of phase separation in the upflow zone. Here we use variation in chloride and gas content in a set of fluid samples collected over several days from one sulfide chimney structure in the MEF to constrain processes of mixing and phase separation. The combination of gas (primarily magmatic CO2 and seawater-derived Ar) and chloride data, indicate that neither variation in the amount of brine lost, nor mixing of the vapor phase produced at depth with variable quantities of (i) brine or (ii) altered gas rich seawater that has not undergone phase separation, can explain the co-variation of gas and chloride content. The gas-chloride data require additional phase separation of the ascending vapor-like fluid. Mixing and gas partitioning calculations show that near-critical temperature and pressure conditions can produce the fluid compositions observed at Sully vent as a vapor-liquid conjugate pair or as vapor-liquid pair with some remixing, and that the gas partition coefficients implied agree with theoretically predicted values.Plain Language SummaryWhen the chemistry of fluids from deep sea hot springs changes over a short time span, it allows us to narrow down the conditions and processes that created those fluids. This gives us a better idea what is happening under the seafloor where the water is interacting with hot rocks and minerals, boiling, and taking on the character it will have when it emerges at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JASTP.100...24I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JASTP.100...24I"><span><span class="hlt">Variation</span> of saturation effect in the ionospheric F2 critical <span class="hlt">frequency</span> at low latitude</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ikubanni, S. O.; Adeniyi, J. O.</p> <p>2013-08-01</p> <p>Saturation in the dependence of foF2 on solar flux is a phenomenon more pronounced in the equatorial ionization anomaly region. The phenomenon was observed in the relationship between the F2 critical <span class="hlt">frequency</span> (foF2) and any solar indices. Using a two-segmented regression fit on data from an African low latitude station (Geographical Latitude 12.4°N; Geomagnetic latitude 3.5°N), saturation features from the dependence of foF2 on solar radio flux (F10.7) was studied. Diurnal and seasonal <span class="hlt">variation</span> were studied for the first time in this low latitude region of the African sector. Significant <span class="hlt">variations</span> were observed, especially in the solstices. It was observed that saturation effect is closely related to the hourly F2 critical <span class="hlt">frequency</span> and these results were compared with those from Asian, Australian and the American sectors. The diurnal and seasonal <span class="hlt">variations</span> find their explanations in the photo-ionization process, the fountain effect, and the pre-reversal enhancement while the seasonal <span class="hlt">variation</span> was attributed to both the ion drift and thermospheric circulation. Future work with larger volume of data is expected to validate the observations from this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5706677','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5706677"><span>Testing the Sensory Drive Hypothesis: Geographic <span class="hlt">variation</span> in echolocation <span class="hlt">frequencies</span> of Geoffroy's horseshoe bat (Rhinolophidae: Rhinolophus clivosus)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Catto, Sarah; Mutumi, Gregory L.; Finger, Nikita; Webala, Paul W.</p> <p>2017-01-01</p> <p>Geographic <span class="hlt">variation</span> in sensory traits is usually influenced by adaptive processes because these traits are involved in crucial life-history aspects including orientation, communication, lineage recognition and mate choice. Studying this <span class="hlt">variation</span> can therefore provide insights into lineage diversification. According to the Sensory Drive Hypothesis, lineage diversification may be driven by adaptation of sensory systems to local environments. It predicts that acoustic signals vary in association with local climatic conditions so that atmospheric attenuation is minimized and transmission of the signals maximized. To test this prediction, we investigated the influence of climatic factors (specifically relative humidity and temperature) on geographic <span class="hlt">variation</span> in the resting <span class="hlt">frequencies</span> of the echolocation pulses of Geoffroy’s horseshoe bat, Rhinolophus clivosus. If the evolution of phenotypic <span class="hlt">variation</span> in this lineage tracks climate <span class="hlt">variation</span>, human induced climate change may lead to decreases in detection volumes and a reduction in foraging efficiency. A complex non-linear interaction between relative humidity and temperature affects atmospheric attenuation of sound and principal components composed of these correlated variables were, therefore, used in a linear mixed effects model to assess their contribution to observed <span class="hlt">variation</span> in resting <span class="hlt">frequencies</span>. A principal component composed predominantly of mean annual temperature (factor loading of -0.8455) significantly explained a proportion of the <span class="hlt">variation</span> in resting <span class="hlt">frequency</span> across sites (P < 0.05). Specifically, at higher relative humidity (around 60%) prevalent across the distribution of R. clivosus, increasing temperature had a strong negative effect on resting <span class="hlt">frequency</span>. Climatic factors thus strongly influence acoustic signal divergence in this lineage, supporting the prediction of the Sensory Drive Hypothesis. The predicted future increase in temperature due to climate change is likely to decrease the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29186147','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29186147"><span>Testing the Sensory Drive Hypothesis: Geographic <span class="hlt">variation</span> in echolocation <span class="hlt">frequencies</span> of Geoffroy's horseshoe bat (Rhinolophidae: Rhinolophus clivosus).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jacobs, David S; Catto, Sarah; Mutumi, Gregory L; Finger, Nikita; Webala, Paul W</p> <p>2017-01-01</p> <p>Geographic <span class="hlt">variation</span> in sensory traits is usually influenced by adaptive processes because these traits are involved in crucial life-history aspects including orientation, communication, lineage recognition and mate choice. Studying this <span class="hlt">variation</span> can therefore provide insights into lineage diversification. According to the Sensory Drive Hypothesis, lineage diversification may be driven by adaptation of sensory systems to local environments. It predicts that acoustic signals vary in association with local climatic conditions so that atmospheric attenuation is minimized and transmission of the signals maximized. To test this prediction, we investigated the influence of climatic factors (specifically relative humidity and temperature) on geographic <span class="hlt">variation</span> in the resting <span class="hlt">frequencies</span> of the echolocation pulses of Geoffroy's horseshoe bat, Rhinolophus clivosus. If the evolution of phenotypic <span class="hlt">variation</span> in this lineage tracks climate <span class="hlt">variation</span>, human induced climate change may lead to decreases in detection volumes and a reduction in foraging efficiency. A complex non-linear interaction between relative humidity and temperature affects atmospheric attenuation of sound and principal components composed of these correlated variables were, therefore, used in a linear mixed effects model to assess their contribution to observed <span class="hlt">variation</span> in resting <span class="hlt">frequencies</span>. A principal component composed predominantly of mean annual temperature (factor loading of -0.8455) significantly explained a proportion of the <span class="hlt">variation</span> in resting <span class="hlt">frequency</span> across sites (P < 0.05). Specifically, at higher relative humidity (around 60%) prevalent across the distribution of R. clivosus, increasing temperature had a strong negative effect on resting <span class="hlt">frequency</span>. Climatic factors thus strongly influence acoustic signal divergence in this lineage, supporting the prediction of the Sensory Drive Hypothesis. The predicted future increase in temperature due to climate change is likely to decrease the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22622203-frequency-independent-approach-calculate-physical-optics-radiations-quadratic-concave-phase-variations','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22622203-frequency-independent-approach-calculate-physical-optics-radiations-quadratic-concave-phase-variations"><span><span class="hlt">Frequency</span>-independent approach to calculate physical optics radiations with the quadratic concave phase <span class="hlt">variations</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>Wu, Yu Mao, E-mail: yumaowu@fudan.edu.cn; Teng, Si Jia, E-mail: sjteng12@fudan.edu.cn</p> <p></p> <p>In this work, we develop the numerical steepest descent path (NSDP) method to calculate the physical optics (PO) radiations with the quadratic concave phase <span class="hlt">variations</span>. With the surface integral equation method, the physical optics (PO) scattered fields are formulated and further reduced to the surface integrals. The high <span class="hlt">frequency</span> physical critical points contributions, including the stationary phase points, the boundary resonance points and the vertex points are comprehensively studied via the proposed NSDP method. The key contributions of this work are twofold. One is that together with the PO integrals taking the quadratic parabolic and hyperbolic phase terms, this workmore » makes the NSDP theory be complete for treating the PO integrals with quadratic phase <span class="hlt">variations</span>. Another is that, in order to illustrate the transition effect of the high <span class="hlt">frequency</span> physical critical points, in this work, we consider and further extend the NSDP method to calculate the PO integrals with the coalescence of the high <span class="hlt">frequency</span> critical points. Numerical results for the highly oscillatory PO integral with the coalescence of the critical points are given to verify the efficiency of the proposed NSDP method. The NSDP method could achieve the <span class="hlt">frequency</span> independent computational workload and error controllable accuracy in all the numerical experiments, especially for the case of the coalescence of the high <span class="hlt">frequency</span> critical points.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000056935','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000056935"><span>Hg(+) <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>Prestage, John D.; Tjoelker, Robert L.; Maleki, Lute</p> <p>2000-01-01</p> <p>In this paper we review the development of Hg(+) microwave <span class="hlt">frequency</span> standards for use in high reliability and continuous operation applications. In recent work we have demonstrated short-term <span class="hlt">frequency</span> stability of 3 x 10(exp -14)/nu(sub tau) when a cryogenic oscillator of stability 2-3 x 10(exp 15) was used a the local oscillator. The trapped ion <span class="hlt">frequency</span> standard employs a Hg-202 discharge lamp to optically pump the trapped Hg(+)-199 clock ions and a helium buffer gas to cool the ions to near room temperature. We describe a small Hg(+) ion trap based <span class="hlt">frequency</span> standard with an extended linear ion trap (LITE) architecture which <span class="hlt">separates</span> the optical state selection region from the clock resonance region. This <span class="hlt">separation</span> allows the use of novel trap configurations in the resonance region since no optical pumping is carried out there. A method for measuring the size of an ion cloud inside a linear trap with a 12-rod trap is currently being investigated. At approx. 10(exp -12), the 2nd order Doppler shift for trapped mercury ion <span class="hlt">frequency</span> standards is one of the largest <span class="hlt">frequency</span> offsets and its measurement to the 1% level would represent an advance in insuring the very long-term stability of these standards to the 10(exp -14) or better level. Finally, we describe atomic clock comparison experiments that can probe for a time <span class="hlt">variation</span> of the fine structure constant, alpha = e(exp 2)/2(pi)hc, at the level of 10(exp -20)/year as predicted in some Grand Unified String Theories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930009777','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930009777"><span><span class="hlt">Variations</span> of the Milankovitch <span class="hlt">frequencies</span> in time</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Loutre, Marie-France; Berger, A.</p> <p>1992-01-01</p> <p>The sensitivity of the amplitudes and <span class="hlt">frequencies</span> in the development of the Earth's orbital and rotational elements involved in the astronomical theory of paleoclimates (eccentricity, obliquity, and climate precession), to the Earth-Moon distance and consequently to the length of the day and to the dynamical ellipticity of the Earth has been discussed for the last billions of years. The shortening of the Earth-Moon distance and of the length of the day, as well as the lengthening of the dynamical ellipticity of the Earth back in time induce a shortening of the fundamental astronomical periods for precession and obliquity. At the same time, the amplitudes of the different terms in the development of the obliquity are undergoing a relative enlargement of about 50 percent at 2 x 10(exp 9) yr BP but the independent term is increasing very weakly (less than 0.1 percent). In other words, the value of the obliquity, which lies within a range of 21.7 to 24.9 deg over the Quarternary was restricted to a range of 22.5 to 24.1 deg at 2 x 10(exp 9) yr BP. On the other hand, the amplitudes in the development of the climatic precession do not change. Moreover, these changes in the <span class="hlt">frequencies</span> and amplitudes for both obliquity and climatic precession are larger for longer period terms. Finally, the periods in the eccentricity development are not influenced by the <span class="hlt">variation</span> of the lunar distance. But the motion of the solar system, especially of the inner planets, was shown to be chaotic. It means that it is impossible to compute the exact motion of the planets over more than about 100 Myr, and the fundamental <span class="hlt">frequencies</span> of the systems are not fixed quantities, but are slowly varying with time. As long as we consider the most important terms, the maximum deviation from the present-day value of the 19-kyr precessional period due to the chaotic motion of the solar system only does not reach more than a few tens of years around 80 Myr BP. Therefore the shortening of the obliquity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SeScT..33e5007L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SeScT..33e5007L"><span>Thermal phase <span class="hlt">separation</span> of ZrSiO4 thin films and <span class="hlt">frequency</span>- dependent electrical characteristics of the Al/ZrSiO4/p-Si/Al MOS capacitors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lok, R.; Kaya, S.; Yilmaz, E.</p> <p>2018-05-01</p> <p>In this work, the thermal phase <span class="hlt">separation</span> and annealing optimization of ZrSiO4 thin films have been carried out. Following annealing optimization, the <span class="hlt">frequency</span>-dependent electrical characteristics of the Al/ZrSiO4/p-Si/Al MOS capacitors were investigated in detail. The chemical evolution of the films under various annealing temperatures was determined by Fourier transform infrared spectroscopy (FTIR) measurements. The phase <span class="hlt">separation</span> was determined by x-ray diffraction (XRD) measurements. The electrical parameters were determined via the capacitance–voltage (C–V), conductance–voltage (G/ω) and leakage-current–voltage (Ig–Vg ). The results demonstrate that zirconium silicate formations are present at 1000 °C annealing with the SiO2 interfacial layer. The film was in amorphous form after annealing at 250 °C. The tetragonal phases of ZrO2 were obtained after annealing at 500 °C. When the temperature approaches 750 °C, transitions from the tetragonal phase to the monoclinic phase were observed. The obtained XRD peaks after 1000 °C annealing matched the crystalline peaks of ZrSiO4. This means that the crystalline zirconium dioxide in the structure has been converted into a crystalline silicate phase. The interface states increased to 5.71 × 1010 and the number of border traps decreased to 7.18 × 1010 cm‑2 with the increasing temperature. These results indicate that an excellent ZrSiO4/Si interface has been fabricated. The order of the leakage current varied from 10‑9 Acm‑2 to 10‑6 Acm‑2. The MOS capacitor fabricated with the films annealed at 1000 °C shows better behavior in terms of its structural, chemical and electrical properties. Hence, detailed <span class="hlt">frequency</span>-dependent electrical characteristics were performed for the ZrSiO4 thin film annealed at 1000 °C. Very slight capacitance <span class="hlt">variations</span> were observed under the <span class="hlt">frequency</span> <span class="hlt">variations</span>. This shows that the density of <span class="hlt">frequency</span>-dependent charges is very low at the ZrSiO4/Si interface. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/4652882','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/4652882"><span>Maintenance of genetic <span class="hlt">variation</span> with a <span class="hlt">frequency</span>-dependent selection model as compared to the overdominant model.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hedrick, P W</p> <p>1972-12-01</p> <p>A <span class="hlt">frequency</span>-dependent selection model proposed by Huang, Singh and Kojima (1971) was found to be more effective at maintaining genetic <span class="hlt">variation</span> in a finite population than the overdominant model. The fourth moment parameter of the distribution of unfixed states showed that there was a more platykurtic distribution for the <span class="hlt">frequency</span>-dependent model. This agreed well with the expected gene <span class="hlt">frequency</span> change found for an infinite population.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920068598&hterms=Age+earth&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAge%2Bearth','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920068598&hterms=Age+earth&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAge%2Bearth"><span><span class="hlt">Frequency</span> <span class="hlt">variations</span> of the earth's obliquity and the 100-kyr ice-age cycles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, Han-Shou</p> <p>1992-01-01</p> <p>Changes in the earth's climate are induced by <span class="hlt">variations</span> in the earth's orbital parameters which modulate the seasonal distribution of solar radiation. Periodicities in the geological climate record with cycles of 100, 41, and 23 kyr have been linked with changes in obliquity, eccentricity, and precession of the equinoxes. The effect of <span class="hlt">variations</span> of eccentricity during a 100 kyr period is weak relative to the signals from obliquity and precession <span class="hlt">variations</span> and it may therefore be expected that the 100 kyr signal in the climate record would be of low intensity. However, this signal dominates the climate record and internal nonlinear processes within the climate system have previously been proposed to account for this fact. The author shows that <span class="hlt">variations</span> in the <span class="hlt">frequency</span> of the obliquity cycle can give rise to strong 100-kyr forcing of climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JIMTW..37..944P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JIMTW..37..944P"><span>A Tri-Band <span class="hlt">Frequency</span> Selective Surface (FSS) to Diplex Widely <span class="hlt">Separated</span> Bands for Millimeter Wave Remote Sensing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poojali, Jayaprakash; Ray, Shaumik; Pesala, Bala; Chitti, Krishnamurthy V.; Arunachalam, Kavitha</p> <p>2016-10-01</p> <p>A substrate-backed <span class="hlt">frequency</span> selective surface (FSS) is presented for diplexing the widely <span class="hlt">separated</span> <span class="hlt">frequency</span> spectrum centered at 55, 89, and 183 GHz with varying bandwidth for spatial <span class="hlt">separation</span> in the quasi-optical feed network of the millimeter wave sounder. A unit cell composed of a crossed dipole integrated with a circular ring and loaded inside a square ring is optimized for tri-band <span class="hlt">frequency</span> response with transmission window at 89 GHz and rejection windows at 55 and 183 GHz. The reflection and transmission losses predicted for the optimized unit cell (728 μm × 728 μm) composed of dissimilar resonant shapes is less than 0.5 dB for transverse electric (TE) and transverse magnetic (TM) polarizations and wide angle of incidence (0°-45°). The FSS is fabricated on a 175-μm-thick quartz substrate using microfabrication techniques. The transmission characteristics measured with continuous wave (CW) terahertz transmit receive system are in good agreement with the numerical simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1212870','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1212870"><span>Maintenance of Genetic <span class="hlt">Variation</span> with a <span class="hlt">Frequency</span>-Dependent Selection Model as Compared to the Overdominant Model</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hedrick, Philip W.</p> <p>1972-01-01</p> <p>A <span class="hlt">frequency</span>-dependent selection model proposed by Huang, Singh and Kojima (1971) was found to be more effective at maintaining genetic <span class="hlt">variation</span> in a finite population than the overdominant model. The fourth moment parameter of the distribution of unfixed states showed that there was a more platykurtic distribution for the <span class="hlt">frequency</span>-dependent model. This agreed well with the expected gene <span class="hlt">frequency</span> change found for an infinite population. PMID:4652882</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ApJ...765....5D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ApJ...765....5D"><span>Periodic <span class="hlt">Variations</span> in the O - C Diagrams of Five Pulsation <span class="hlt">Frequencies</span> of the DB White Dwarf EC 20058-5234</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dalessio, J.; Sullivan, D. J.; Provencal, J. L.; Shipman, H. L.; Sullivan, T.; Kilkenny, D.; Fraga, L.; Sefako, R.</p> <p>2013-03-01</p> <p><span class="hlt">Variations</span> in the pulsation arrival time of five independent pulsation <span class="hlt">frequencies</span> of the DB white dwarf EC 20058-5234 individually imitate the effects of reflex motion induced by a planet or companion but are inconsistent when considered in unison. The pulsation <span class="hlt">frequencies</span> vary periodically in a 12.9 year cycle and undergo secular changes that are inconsistent with simple neutrino plus photon-cooling models. The magnitude of the periodic and secular <span class="hlt">variations</span> increases with the period of the pulsations, possibly hinting that the corresponding physical mechanism is located near the surface of the star. The phase of the periodic <span class="hlt">variations</span> appears coupled to the sign of the secular <span class="hlt">variations</span>. The standards for pulsation-timing-based detection of planetary companions around pulsating white dwarfs, and possibly other variables such as subdwarf B stars, should be re-evaluated. The physical mechanism responsible for this surprising result may involve a redistribution of angular momentum or a magnetic cycle. Additionally, <span class="hlt">variations</span> in a supposed combination <span class="hlt">frequency</span> are shown to match the sum of the <span class="hlt">variations</span> of the parent <span class="hlt">frequencies</span> to remarkable precision, an expected but unprecedented confirmation of theoretical predictions. Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the US National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25828030','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25828030"><span>Top down and bottom up selection drives <span class="hlt">variations</span> in <span class="hlt">frequency</span> and form of a visual signal.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yeh, Chien-Wei; Blamires, Sean J; Liao, Chen-Pan; Tso, I-Min</p> <p>2015-03-30</p> <p>The <span class="hlt">frequency</span> and form of visual signals can be shaped by selection from predators, prey or both. When a signal simultaneously attracts predators and prey selection may favour a strategy that minimizes risks while attracting prey. Accordingly, varying the <span class="hlt">frequency</span> and form of the silken decorations added to their web may be a way that Argiope spiders minimize predation while attracting prey. Nonetheless, the role of extraneous factors renders the influences of top down and bottom up selection on decoration <span class="hlt">frequency</span> and form <span class="hlt">variation</span> difficult to discern. Here we used dummy spiders and decorations to simulate four possible strategies that the spider Argiope aemula may choose and measured the prey and predator attraction consequences for each in the field. The strategy of decorating at a high <span class="hlt">frequency</span> with a variable form attracted the most prey, while that of decorating at a high <span class="hlt">frequency</span> with a fixed form attracted the most predators. These results suggest that mitigating the cost of attracting predators while maintaining prey attraction drives the use of <span class="hlt">variation</span> in decoration form by many Argiope spp. when decorating frequently. Our study highlights the importance of considering top-down and bottom up selection pressure when devising evolutionary ecology experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.476.2704M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.476.2704M"><span>Low-<span class="hlt">frequency</span> pulse profile <span class="hlt">variation</span> in PSR B2217+47: evidence for echoes from the interstellar medium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michilli, D.; Hessels, J. W. T.; Donner, J. Y.; Grießmeier, J.-M.; Serylak, M.; Shaw, B.; Stappers, B. W.; Verbiest, J. P. W.; Deller, A. T.; Driessen, L. N.; Stinebring, D. R.; Bondonneau, L.; Geyer, M.; Hoeft, M.; Karastergiou, A.; Kramer, M.; Osłowski, S.; Pilia, M.; Sanidas, S.; Weltevrede, P.</p> <p>2018-05-01</p> <p>We have observed a complex and continuous change in the integrated pulse profile of PSR B2217+47, manifested as additional components trailing the main peak. These transient components are detected over 6 yr at 150 MHz using the LOw <span class="hlt">Frequency</span> ARray (LOFAR), but they are not seen in contemporaneous Lovell observations at 1.5 GHz. We argue that propagation effects in the ionized interstellar medium (IISM) are the most likely cause. The putative structures in the IISM causing the profile <span class="hlt">variation</span> are roughly half-way between the pulsar and the Earth and have transverse radii R ˜ 30 au. We consider different models for the structures. Under the assumption of spherical symmetry, their implied average electron density is \\overline{n}_e ˜ 100 cm-3. Since PSR B2217+47 is more than an order of magnitude brighter than the average pulsar population visible to LOFAR, similar profile <span class="hlt">variations</span> would not have been identified in most pulsars, suggesting that subtle profile <span class="hlt">variations</span> in low-<span class="hlt">frequency</span> profiles might be more common than we have observed to date. Systematic studies of these <span class="hlt">variations</span> at low <span class="hlt">frequencies</span> can provide a new tool to investigate the proprieties of the IISM and the limits to the precision of pulsar timing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030112522','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030112522"><span><span class="hlt">Frequency</span> Reuse, Cell <span class="hlt">Separation</span>, and Capacity Analysis of VHF Digital Link Mode 3 TDMA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shamma, Mohammed A.; Nguyen, Thanh C.; Apaza, Rafael D.</p> <p>2003-01-01</p> <p>The most recent studies by the Federal Aviation Administration (FAA) and the aviation industry have indicated that it has become increasingly difficult to make new VHF <span class="hlt">frequency</span> or channel assignments to meet the aviation needs for air-ground communications. FAA has planned for several aggressive improvement measures to the existing systems, but these measures would not meet the projected voice communications needs beyond 2009. FAA found that since 1974 there has been, on the average, a 4 percent annual increase in the number of channel assignments needed to satisfy the air-ground communication traffic (approximately 300 new channel assignments per year). With the planned improvement measures, the channel assignments are expected to reach a maximum number of 16615 channels by about 2010. Hence, the FAA proposed the use of VDL Mode 3 as a new integrated digital voice and data communications systems to meet the future air traffic demand. This paper presents analytical results of <span class="hlt">frequency</span> reuse; cell <span class="hlt">separation</span> and capacity estimation of VDL Mode 3 TDMA systems that FAA has planned to implement the future VHF air-ground communications system by the year 2010. For TDMA, it is well understood that the <span class="hlt">frequency</span> reuse factor is a crucial parameter for capacity estimation. Formulation of this <span class="hlt">frequency</span> reuse factor is shown, taking into account the limitation imposed by the requirement to have a sufficient Signal to Co-Channel Interference Ratio. Several different values for the Signal to Co-Channel Interference Ratio were utilized corresponding to the current analog VHF DSB-AM systems, and the future digital VDL Mode 3. The required <span class="hlt">separation</span> of Co-Channel cells is computed for most of the <span class="hlt">Frequency</span> Protected Service Volumes (FPSV's) currently in use by the FAA. Additionally, the ideal cell capacity for each FPSV is presented. Also, using actual traffic for the Detroit air space, a FPSV traffic distribution model is used to generate a typical cell for channel capacity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011ClDy...36..957K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011ClDy...36..957K"><span>Multidecadal changes in winter circulation-climate relationship in Europe: <span class="hlt">frequency</span> <span class="hlt">variations</span>, within-type modifications, and long-term trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Küttel, Marcel; Luterbacher, Jürg; Wanner, Heinz</p> <p>2011-03-01</p> <p>Using pressure fields classified by the SANDRA algorithm, this study investigates the changes in the relationship between North Atlantic/European sea level pressure (SLP) and gridded European winter (DJF) temperature and precipitation back to 1750. Important changes in the <span class="hlt">frequency</span> of the SLP clusters are found, though none of them indicating significant long-term trends. However, for the majority of the SLP clusters a tendency toward overall warmer and partly wetter winter conditions is found, most pronounced over the last decades. This suggests important within-type <span class="hlt">variations</span>, i.e. the temperature and precipitation fields related to a particular SLP pattern change their characteristics over time. Using a decomposition scheme we find for temperature and precipitation that within-type-related <span class="hlt">variations</span> dominate over those due to changed <span class="hlt">frequencies</span> of the SLP clusters: Approximately 70% (60%) of European winter temperature (precipitation) <span class="hlt">variations</span> can be explained by within-type changes, most strongly expressed over Eastern Europe and Scandinavia. This indicates that the current European winter warming cannot be explained by changed <span class="hlt">frequencies</span> of the SLP patterns alone, but to a larger degree by changed characteristics of the patterns themselves. Potential sources of within-type <span class="hlt">variations</span> are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080023303','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080023303"><span>Spectral <span class="hlt">Separation</span> of the Turbofan Engine Coherent Combustion Noise Component</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miles, Jeffrey Hilton</p> <p>2008-01-01</p> <p>The core noise components of a dual spool turbofan engine (Honeywell TECH977) were <span class="hlt">separated</span> by the use of a coherence function. A source location technique based on adjusting the time delay between the combustor pressure sensor signal and the far-field microphone signal to maximize the coherence and remove as much <span class="hlt">variation</span> of the phase angle with <span class="hlt">frequency</span> as possible was used. While adjusting the time delay to maximize the coherence and minimize the cross spectrum phase angle <span class="hlt">variation</span> with <span class="hlt">frequency</span>, the discovery was made that for the 130 microphone a 90.027 ms time shift worked best for the <span class="hlt">frequency</span> band from 0 to 200 Hz while a 86.975 ms time shift worked best for the <span class="hlt">frequency</span> band from 200 to 400 Hz. Since the 0 to 200 Hz band signal took more time to travel the same distance, it is slower than the 200 to 400 Hz band signal. This suggests the 0 to 200 Hz coherent cross spectral density band is partly due to indirect combustion noise attributed to hot spots interacting with the turbine. The signal in the 200 to 400 Hz <span class="hlt">frequency</span> band is attributed mostly to direct combustion noise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4406052','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4406052"><span>Top down and bottom up selection drives <span class="hlt">variations</span> in <span class="hlt">frequency</span> and form of a visual signal</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yeh, Chien-Wei; Blamires, Sean J.; Liao, Chen-Pan; Tso, I.-Min</p> <p>2015-01-01</p> <p>The <span class="hlt">frequency</span> and form of visual signals can be shaped by selection from predators, prey or both. When a signal simultaneously attracts predators and prey, selection may favour a strategy that minimizes risks while attracting prey. Accordingly, varying the <span class="hlt">frequency</span> and form of the silken decorations added to their web may be a way that Argiope spiders minimize predation while attracting prey. Nonetheless, the role of extraneous factors renders the influences of top down and bottom up selection on decoration <span class="hlt">frequency</span> and form <span class="hlt">variation</span> difficult to discern. Here we used dummy spiders and decorations to simulate four possible strategies that the spider Argiope aemula may choose and measured the prey and predator attraction consequences for each in the field. The strategy of decorating at a high <span class="hlt">frequency</span> with a variable form attracted the most prey, while that of decorating at a high <span class="hlt">frequency</span> with a fixed form attracted the most predators. These results suggest that mitigating the cost of attracting predators while maintaining prey attraction drives the use of <span class="hlt">variation</span> in decoration form by many Argiope spp. when decorating frequently. Our study highlights the importance of considering top-down and bottom up selection pressure when devising evolutionary ecology experiments. PMID:25828030</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7159875','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/7159875"><span>Systems for controlling the intensity <span class="hlt">variations</span> in a laser beam and for <span class="hlt">frequency</span> conversion thereof</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Skupsky, S.; Craxton, R.S.; Soures, J.</p> <p>1990-10-02</p> <p>In order to control the intensity of a laser beam so that its intensity varies uniformly and provides uniform illumination of a target, such as a laser fusion target, a broad bandwidth laser pulse is spectrally dispersed spatially so that the <span class="hlt">frequency</span> components thereof are spread apart. A disperser (grating) provides an output beam which varies spatially in wavelength in at least one direction transverse to the direction of propagation of the beam. Temporal spread (time delay) across the beam is corrected by using a phase delay device (a time delay compensation echelon). The dispersed beam may be amplified with laser amplifiers and <span class="hlt">frequency</span> converted (doubled, tripled or quadrupled in <span class="hlt">frequency</span>) with nonlinear optical elements (birefringent crystals). The spectral <span class="hlt">variation</span> across the beam is compensated by varying the angle of incidence on one of the crystals with respect to the crystal optical axis utilizing a lens which diverges the beam. Another lens after the <span class="hlt">frequency</span> converter may be used to recollimate the beam. The <span class="hlt">frequency</span> converted beam is recombined so that portions of different <span class="hlt">frequency</span> interfere and, unlike interference between waves of the same wavelength, there results an intensity pattern with rapid temporal oscillations which average out rapidly in time thereby producing uniform illumination on target. A distributed phase plate (also known as a random phase mask), through which the spectrally dispersed beam is passed and then focused on a target, is used to provide the interference pattern which becomes nearly modulation free and uniform in intensity in the direction of the spectral <span class="hlt">variation</span>. 16 figs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/867546','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/867546"><span>Systems for controlling the intensity <span class="hlt">variations</span> in a laser beam and for <span class="hlt">frequency</span> conversion thereof</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Skupsky, Stanley; Craxton, R. Stephen; Soures, John</p> <p>1990-01-01</p> <p>In order to control the intensity of a laser beam so that its intensity varies uniformly and provides uniform illumination of a target, such as a laser fusion target, a broad bandwidth laser pulse is spectrally dispersed spatially so that the <span class="hlt">frequency</span> components thereof are spread apart. A disperser (grating) provides an output beam which varies spatially in wavelength in at least one direction transverse to the direction of propagation of the beam. Temporal spread (time delay) across the beam is corrected by using a phase delay device (a time delay compensation echelon). The dispersed beam may be amplified with laser amplifiers and <span class="hlt">frequency</span> converted (doubled, tripled or quadrupled in <span class="hlt">frequency</span>) with nonlinear optical elements (birefringent crystals). The spectral <span class="hlt">variation</span> across the beam is compensated by varying the angle of incidence on one of the crystals with respect to the crystal optical axis utilizing a lens which diverges the beam. Another lens after the <span class="hlt">frequency</span> converter may be used to recollimate the beam. The <span class="hlt">frequency</span> converted beam is recombined so that portions of different <span class="hlt">frequency</span> interfere and, unlike interference between waves of the same wavelength, there results an intensity pattern with rapid temoral oscillations which average out rapidly in time thereby producing uniform illumination on target. A distributed phase plate (also known as a random phase mask), through which the spectrally dispersed beam is passed and then focused on a target, is used to provide the interference pattern which becomes nearly modulation free and uniform in intensity in the direction of the spectral <span class="hlt">variation</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20407068','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20407068"><span>Read distance performance and <span class="hlt">variation</span> of 5 low-<span class="hlt">frequency</span> radio <span class="hlt">frequency</span> identification panel transceiver manufacturers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ryan, S E; Blasi, D A; Anglin, C O; Bryant, A M; Rickard, B A; Anderson, M P; Fike, K E</p> <p>2010-07-01</p> <p>Use of electronic animal identification technologies by livestock managers is increasing, but performance of these technologies can be variable when used in livestock production environments. This study was conducted to determine whether 1) read distance of low-<span class="hlt">frequency</span> radio <span class="hlt">frequency</span> identification (RFID) transceivers is affected by type of transponder being interrogated; 2) read distance <span class="hlt">variation</span> of low-<span class="hlt">frequency</span> RFID transceivers is affected by transceiver manufacturer; and 3) read distance of various transponder-transceiver manufacturer combinations meet the 2004 United States Animal Identification Plan (USAIP) bovine standards subcommittee minimum read distance recommendation of 60 cm. Twenty-four transceivers (n = 5 transceivers per manufacturer for Allflex, Boontech, Farnam, and Osborne; n = 4 transceivers for Destron Fearing) were tested with 60 transponders [n = 10 transponders per type for Allflex full duplex B (FDX-B), Allflex half duplex (HDX), Destron Fearing FDX-B, Farnam FDX-B, and Y-Tex FDX-B; n = 6 for Temple FDX-B (EM Microelectronic chip); and n = 4 for Temple FDX-B (HiTag chip)] presented in the parallel orientation. All transceivers and transponders met International Organization for Standardization 11784 and 11785 standards. Transponders represented both one-half duplex and full duplex low-<span class="hlt">frequency</span> air interface technologies. Use of a mechanical trolley device enabled the transponders to be presented to the center of each transceiver at a constant rate, thereby reducing human error. Transponder and transceiver manufacturer interacted (P < 0.0001) to affect read distance, indicating that transceiver performance was greatly dependent upon the transponder type being interrogated. Twenty-eight of 30 combinations of transceivers and transponders evaluated met the minimum recommended USAIP read distance. The mean read distance across all 30 combinations was 45.1 to 129.4 cm. Transceiver manufacturer and transponder type interacted to affect read</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1429744','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1429744"><span>Drought Conditions Maximize the Impact of High-<span class="hlt">Frequency</span> Flow <span class="hlt">Variations</span> on Thermal Regimes and Biogeochemical Function in the Hyporheic Zone.</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>None, None</p> <p></p> <p>Anthropogenic activities, such as dam operations, often induce larger and more frequent stage fluctuations than those occurring in natural rivers. However, the long-term impact of such flow <span class="hlt">variations</span> on thermal and biogeochemical dynamics of the associated hyporheic zone (HZ) is poorly understood. A heterogeneous, two-dimensional thermo-hydro-biogeochemical model revealed an important interaction between high-<span class="hlt">frequency</span> flow <span class="hlt">variations</span> and watershed-scale hydrology. High-<span class="hlt">frequency</span> stage fluctuations had their strongest thermal and biogeochemical impacts when the mean river stage was low during fall and winter. An abnormally thin snowpack in 2015, however, created a low river stage during summer and early fall, whereby high <span class="hlt">frequency</span> stagemore » fluctuations caused the HZ to be warmer than usual. This study provided the scientific basis to assess the potential ecological consequences of the high-<span class="hlt">frequency</span> flow <span class="hlt">variations</span> in a regulated river, as well as guidance on how to maximize the potential benefits—or minimize the drawbacks—of river regulation to river ecosystems.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EEEV...14..715K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EEEV...14..715K"><span>Analysis of <span class="hlt">frequency</span> shifting in seismic signals using Gabor-Wigner transform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Roshan; Sumathi, P.; Kumar, Ashok</p> <p>2015-12-01</p> <p>A hybrid time-<span class="hlt">frequency</span> method known as Gabor-Wigner transform (GWT) is introduced in this paper for examining the time-<span class="hlt">frequency</span> patterns of earthquake damaged buildings. GWT is developed by combining the Gabor transform (GT) and Wigner-Ville distribution (WVD). GT and WVD have been used <span class="hlt">separately</span> on synthetic and recorded earthquake data to identify <span class="hlt">frequency</span> shifting due to earthquake damages, but GT is prone to windowing effect and WVD involves ambiguity function. Hence to obtain better clarity and to remove the cross terms (<span class="hlt">frequency</span> interference), GT and WVD are judiciously combined and the resultant GWT used to identify <span class="hlt">frequency</span> shifting. Synthetic seismic response of an instrumented building and real-time earthquake data recorded on the building were investigated using GWT. It is found that GWT offers good accuracy for even slow <span class="hlt">variations</span> in <span class="hlt">frequency</span>, good time-<span class="hlt">frequency</span> resolution, and localized response. Presented results confirm the efficacy of GWT when compared with GT and WVD used <span class="hlt">separately</span>. Simulation results were quantified by the Renyi entropy measures and GWT shown to be an adequate technique in identifying localized response for structural damage detection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EPSC....8.1025G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EPSC....8.1025G"><span>International Deep Planet Survey, 317 stars to determine the wide-<span class="hlt">separated</span> planet <span class="hlt">frequency</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Galicher, R.; Marois, C.; Macintosh, B.; Zuckerman, B.; Song, I.; Barman, T.; Patience, J.</p> <p>2013-09-01</p> <p>Since 2000, more than 300 nearby young stars were observed for the International Deep Planet Survey with adaptive optics systems at Gemini (NIRI/NICI), Keck (Nirc2), and VLT (Naco). Massive young AF stars were included in our sample whereas they have generally been neglected in first generation surveys because the contrast and target distances are less favorable to image substellar companions. The most significant discovery of the campaign is the now well-known HR 8799 multi-planet system. This remarkable finding allows, for the first time, an estimate of the Jovians planet population at large <span class="hlt">separations</span> (further than a few AUs) instead of deriving upper limits. During my presentation, I will present the survey showing images of multiple stars and planets. I will then propose a statistic study of the observed stars deriving constraints on the Jupiter-like planet <span class="hlt">frequency</span> at large <span class="hlt">separations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2007/5091/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2007/5091/"><span>Amplitude <span class="hlt">Variation</span> of Bottom Simulating Reflection with Respect to <span class="hlt">Frequency</span> - Transitional Base or Attenuation?</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lee, Myung W.</p> <p>2007-01-01</p> <p>The amplitude of a bottom simulating reflection (BSR), which occurs near the phase boundary between gas hydrate-bearing sediments and underlying gas-filled sediments, strongly depends on the <span class="hlt">frequency</span> content of a seismic signal, as well as the impedance contrast across the phase boundary. A strong-amplitude BSR, detectable in a conventional seismic profile, is a good indicator of the presence of free gas beneath the phase boundary. However, the BSR as observed in low-<span class="hlt">frequency</span> multichannel seismic data is generally difficult to identify in high-<span class="hlt">frequency</span>, single-channel seismic data. To investigate the <span class="hlt">frequency</span> dependence of BSR amplitudes, single-channel seismic data acquired with an air gun source at Blake Ridge, which is located off the shore of South Carolina, were analyzed in the <span class="hlt">frequency</span> range of 10-240 Hz. The <span class="hlt">frequency</span>-dependent impedance contrast caused by the velocity dispersion in partially gas saturated sediments is important to accurately analyze BSR amplitude. Analysis indicates that seismic attenuation of gas hydrate-bearing sediments, velocity dispersion, and a transitional base all contribute to the <span class="hlt">frequency</span>-dependent BSR amplitude <span class="hlt">variation</span> in the <span class="hlt">frequency</span> range of 10-500 Hz. When velocity dispersion is incorporated into the BSR amplitude analysis, the <span class="hlt">frequency</span>-dependent BSR amplitude at Blake Ridge can be explained with gas hydrate-bearing sediments having a quality factor of about 250 and a transitional base with a thickness of about 1 meter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGeod..90.1237M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGeod..90.1237M"><span>High-<span class="hlt">frequency</span> Earth rotation <span class="hlt">variations</span> deduced from altimetry-based ocean tides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Madzak, Matthias; Schindelegger, Michael; Böhm, Johannes; Bosch, Wolfgang; Hagedoorn, Jan</p> <p>2016-11-01</p> <p>A model of diurnal and semi-diurnal <span class="hlt">variations</span> in Earth rotation parameters (ERP) is constructed based on altimetry-measured tidal heights from a multi-mission empirical ocean tide solution. Barotropic currents contributing to relative angular momentum changes are estimated for nine major tides in a global inversion algorithm that solves the two-dimensional momentum equations on a regular 0.5° grid with a heavily weighted continuity constraint. The influence of 19 minor tides is accounted for by linear admittance interpolation of ocean tidal angular momentum, although the assumption of smooth admittance <span class="hlt">variations</span> with <span class="hlt">frequency</span> appears to be a doubtful concept for semi-diurnal mass terms in particular. A validation of the newly derived model based on post-fit corrections to polar motion and universal time (Δ UT1) from the analysis of Very Long Baseline Interferometry (VLBI) observations shows a variance reduction for semi-diurnal Δ UT1 residuals that is significant at the 0.05 level with respect to the conventional ERP model. Improvements are also evident for the explicitly modeled K_1, Q_1, and K_2 tides in individual ERP components, but large residuals of more than 15 μ as remain at the principal lunar <span class="hlt">frequencies</span> of O_1 and M_2. We attribute these shortcomings to uncertainties in the inverted relative angular momentum changes and, to a minor extent, to violation of mass conservation in the empirical ocean tide solution. Further dedicated hydrodynamic modeling efforts of these anomalous constituents are required to meet the accuracy standards of modern space geodesy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19821115','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19821115"><span>Droplet-based magnetically activated cell <span class="hlt">separation</span>: analysis of <span class="hlt">separation</span> efficiency based on the <span class="hlt">variation</span> of flow-induced circulation in a pendent drop.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Youngho; Lee, Sang Ho; Kim, Byungkyu</p> <p>2009-12-01</p> <p>Under the assumption that <span class="hlt">separation</span> efficiencies are mainly affected by the velocity of flow-induced circulation due to buffer injection in a pendent drop, this paper describes an analysis of the <span class="hlt">separation</span> efficiency of a droplet-based magnetically activated cell <span class="hlt">separation</span> (DMACS) system. To investigate the velocity of the flow-induced circulation, we supposed that numerous flows in a pendent drop could be considered as a "theoretically normalized" flow (or conceptually normalized flow, CNF) based on the Cauchy-Goursat theorem. With the morphological characteristics (length and duration time) of a pendent drop depending on the initial volume, we obtained the velocities of the CNF. By measuring the <span class="hlt">separation</span> efficiencies for different initial volumes and by analyzing the <span class="hlt">separation</span> efficiency in terms of the velocity of the CNF, we found that the <span class="hlt">separation</span> efficiencies (in the case of a low rate of buffer injection; 5 and 15 microl x min(-1)) are mainly affected by the velocity of the CNF. Moreover, we confirmed that the phenomenological features of a pendent drop cause a fluctuation of its <span class="hlt">separation</span> efficiencies over a range of specific volumes (initial volumes ranging from 40 to 80 microl), because of the "sweeping-off" phenomenon, that is, positive cells gathered into the positive fraction are forced to move away from the magnetic side by flow-induced circulation due to buffer injection. In addition, from the <span class="hlt">variation</span> of the duration time, that is, the interval between the beginning of injection of the buffer solution and the time at which a pendent drop detaches, it could also be confirmed that a shorter duration time leads to decrease of the number of positive cells in negative fraction regardless of the rate of buffer injection (5, 15, and 50 microl x min(-1)). Therefore, if a DMACS system is operated with a 15 microl x min(-1) buffer injection flow rate and an initial volume of 80 microl or more, we would have the best efficiency of <span class="hlt">separation</span> in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006SSEle..50.1156H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006SSEle..50.1156H"><span>Gate line edge roughness amplitude and <span class="hlt">frequency</span> <span class="hlt">variation</span> effects on intra die MOS device characteristics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamadeh, Emad; Gunther, Norman G.; Niemann, Darrell; Rahman, Mahmud</p> <p>2006-06-01</p> <p>Random fluctuations in fabrication process outcomes such as gate line edge roughness (LER) give rise to corresponding fluctuations in scaled down MOS device characteristics. A thermodynamic-<span class="hlt">variational</span> model is presented to study the effects of LER on threshold voltage and capacitance of sub-50 nm MOS devices. Conceptually, we treat the geometric definition of the MOS devices on a die as consisting of a collection of gates. In turn, each of these gates has an area, A, and a perimeter, P, defined by nominally straight lines subject to random process outcomes producing roughness. We treat roughness as being deviations from straightness consisting of both transverse amplitude and longitudinal wavelength each having lognormal distribution. We obtain closed-form expressions for variance of threshold voltage ( Vth), and device capacitance ( C) at Onset of Strong Inversion (OSI) for a small device. Using our <span class="hlt">variational</span> model, we characterized the device electrical properties such as σ and σC in terms of the statistical parameters of the roughness amplitude and spatial <span class="hlt">frequency</span>, i.e., inverse roughness wavelength. We then verified our model with numerical analysis of Vth roll-off for small devices and σ due to dopant fluctuation. Our model was also benchmarked against TCAD of σ as a function of LER. We then extended our analysis to predict <span class="hlt">variations</span> in σ and σC versus average LER spatial <span class="hlt">frequency</span> and amplitude, and oxide-thickness. Given the intuitive expectation that LER of very short wavelengths must also have small amplitude, we have investigated the case in which the amplitude mean is inversely related to the <span class="hlt">frequency</span> mean. We compare with the situation in which amplitude and <span class="hlt">frequency</span> mean are unrelated. Given also that the gate perimeter may consist of different LER signature for each side, we have extended our analysis to the case when the LER statistical difference between gate sides is moderate, as well as when it is significantly large.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080007433','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080007433"><span>Active noise control using noise source having adaptive resonant <span class="hlt">frequency</span> tuning through stiffness <span class="hlt">variation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rajiyah, Harindra (Inventor); Hedeen, Robert A. (Inventor); Pla, Frederic G. (Inventor); Renshaw, Anthony A. (Inventor)</p> <p>1995-01-01</p> <p>A noise source for an aircraft engine active noise cancellation system in which the resonant <span class="hlt">frequency</span> of a noise radiating element is tuned to permit noise cancellation over a wide range of <span class="hlt">frequencies</span>. The resonant <span class="hlt">frequency</span> of the noise radiating element is tuned by a plurality of force transmitting mechanisms which contact the noise radiating element. Each one of the force transmitting mechanisms includes an expandable element and a spring in contact with the noise radiating element so that excitation of the element varies the spring force applied to the noise radiating element. The elements are actuated by a controller which receives input of a signal proportional to displacement of the noise radiating element and a signal corresponding to the blade passage <span class="hlt">frequency</span> of the engine's fan. In response, the controller determines a control signal which is sent to the elements and causes the spring force applied to the noise radiating element to be varied. The force transmitting mechanisms can be arranged to either produce bending or linear stiffness <span class="hlt">variations</span> in the noise radiating element.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28464617','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28464617"><span>A blind source <span class="hlt">separation</span> approach for humpback whale song <span class="hlt">separation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Zhenbin; White, Paul R</p> <p>2017-04-01</p> <p>Many marine mammal species are highly social and are frequently encountered in groups or aggregations. When conducting passive acoustic monitoring in such circumstances, recordings commonly contain vocalizations of multiple individuals which overlap in time and <span class="hlt">frequency</span>. This paper considers the use of blind source <span class="hlt">separation</span> as a method for processing these recordings to <span class="hlt">separate</span> the calls of individuals. The example problem considered here is that of the songs of humpback whales. The high levels of noise and long impulse responses can make source <span class="hlt">separation</span> in underwater contexts a challenging proposition. The approach present here is based on time-<span class="hlt">frequency</span> masking, allied to a noise reduction process. The technique is assessed using simulated and measured data sets, and the results demonstrate the effectiveness of the method for <span class="hlt">separating</span> humpback whale songs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/3070622','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/3070622"><span>Psychophysiological effects of self-regulation method: EEG <span class="hlt">frequency</span> analysis and contingent negative <span class="hlt">variations</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ikemi, A</p> <p>1988-01-01</p> <p>Experiments were conducted to investigate the psychophysiological effects of self-regulation method (SRM), a newly developed method of self-control, using EEG <span class="hlt">frequency</span> analysis and contingent negative <span class="hlt">variations</span> (CNV). The results of the EEG <span class="hlt">frequency</span> analysis showed that there is a significant increase in the percentage (power) of the theta-band and a significant decrease in the percentage (power) of the beta-band during SRM. Moreover, the results of an identical experiment conducted on subjects in a drowsy state showed that the changes in EEG <span class="hlt">frequencies</span> during SRM can be differentiated from those of a drowsy state. Furthermore, experiments using CNV showed that there is a significant reduction of CNV amplitude during SRM. Despite the reduced amplitude during SRM, the number of errors in a task to evoke the CNV was reduced significantly without significant delay of reaction time. When an identical experiment was conducted in a drowsy state, CNV amplitude was reduced significantly, but reaction time and errors increased. From these experiments, the state of vigilance during SRM was discussed as a state of 'relaxed alertness'.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5982401','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5982401"><span>Unsupervised Learning for Monaural Source <span class="hlt">Separation</span> Using Maximization–Minimization Algorithm with Time–<span class="hlt">Frequency</span> Deconvolution †</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bouridane, Ahmed; Ling, Bingo Wing-Kuen</p> <p>2018-01-01</p> <p>This paper presents an unsupervised learning algorithm for sparse nonnegative matrix factor time–<span class="hlt">frequency</span> deconvolution with optimized fractional β-divergence. The β-divergence is a group of cost functions parametrized by a single parameter β. The Itakura–Saito divergence, Kullback–Leibler divergence and Least Square distance are special cases that correspond to β=0, 1, 2, respectively. This paper presents a generalized algorithm that uses a flexible range of β that includes fractional values. It describes a maximization–minimization (MM) algorithm leading to the development of a fast convergence multiplicative update algorithm with guaranteed convergence. The proposed model operates in the time–<span class="hlt">frequency</span> domain and decomposes an information-bearing matrix into two-dimensional deconvolution of factor matrices that represent the spectral dictionary and temporal codes. The deconvolution process has been optimized to yield sparse temporal codes through maximizing the likelihood of the observations. The paper also presents a method to estimate the fractional β value. The method is demonstrated on <span class="hlt">separating</span> audio mixtures recorded from a single channel. The paper shows that the extraction of the spectral dictionary and temporal codes is significantly more efficient by using the proposed algorithm and subsequently leads to better source <span class="hlt">separation</span> performance. Experimental tests and comparisons with other factorization methods have been conducted to verify its efficacy. PMID:29702629</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70180688','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70180688"><span>Genetic <span class="hlt">variation</span> in steelhead of Oregon and northern California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reisenbichler, R.R.; McIntyre, J.D.; Solazzi, M.F.; Landino, S.W</p> <p>1992-01-01</p> <p>Steelhead Oncorhynchus mykiss from various sites between the Columbia River and the Mad River, California, were genetically characterized at 10 protein-coding loci or pairs of loci by starch gel electrophoresis. Fish from coastal streams differed from fish east of the Cascade Mountains and from fish of the Willamette River (a tributary of the Columbia River, west of the Cascade Mountains). Coastal steelhead from the northern part of the study area differed from those in the southern part. Genetic differentiation within and among drainages was not statistically significant; however, gene diversity analysis and the life history of steelhead suggested that fish from different drainages should be considered as <span class="hlt">separate</span> populations. Genetic <span class="hlt">variation</span> among fish in <span class="hlt">separate</span> drainages was similar to that reported in northwestern Washington and less than that reported in British Columbia. Allele <span class="hlt">frequencies</span> varied significantly among year-classes. Genetic <span class="hlt">variation</span> within samples accounted for 98.3% of the total genetic <span class="hlt">variation</span> observed in this study. Most hatchery populations differed from wild populations, suggesting that conservation of genetic diversity among and within wild populations could be facilitated by altering hatchery programs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27917394','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27917394"><span>A Deep Ensemble Learning Method for Monaural Speech <span class="hlt">Separation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Xiao-Lei; Wang, DeLiang</p> <p>2016-03-01</p> <p>Monaural speech <span class="hlt">separation</span> is a fundamental problem in robust speech processing. Recently, deep neural network (DNN)-based speech <span class="hlt">separation</span> methods, which predict either clean speech or an ideal time-<span class="hlt">frequency</span> mask, have demonstrated remarkable performance improvement. However, a single DNN with a given window length does not leverage contextual information sufficiently, and the differences between the two optimization objectives are not well understood. In this paper, we propose a deep ensemble method, named multicontext networks, to address monaural speech <span class="hlt">separation</span>. The first multicontext network averages the outputs of multiple DNNs whose inputs employ different window lengths. The second multicontext network is a stack of multiple DNNs. Each DNN in a module of the stack takes the concatenation of original acoustic features and expansion of the soft output of the lower module as its input, and predicts the ratio mask of the target speaker; the DNNs in the same module employ different contexts. We have conducted extensive experiments with three speech corpora. The results demonstrate the effectiveness of the proposed method. We have also compared the two optimization objectives systematically and found that predicting the ideal time-<span class="hlt">frequency</span> mask is more efficient in utilizing clean training speech, while predicting clean speech is less sensitive to SNR <span class="hlt">variations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790011946','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790011946"><span>Theory of low <span class="hlt">frequency</span> noise transmission through turbines</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Matta, R. K.; Mani, R.</p> <p>1979-01-01</p> <p>Improvements of the existing theory of low <span class="hlt">frequency</span> noise transmission through turbines and development of a working prediction tool are described. The existing actuator-disk model and a new finite-chord model were utilized in an analytical study. The interactive effect of adjacent blade rows, higher order spinning modes, blade-passage shocks, and duct area <span class="hlt">variations</span> were considered <span class="hlt">separately</span>. The improved theory was validated using the data acquired in an earlier NASA program. Computer programs incorporating the improved theory were produced for transmission loss prediction purposes. The programs were exercised parametrically and charts constructed to define approximately the low <span class="hlt">frequency</span> noise transfer through turbines. The loss through the exhaust nozzle and flow(s) was also considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027606','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027606"><span>Response of a hydrothermal system to magmatic heat inferred from temporal <span class="hlt">variations</span> in the complex <span class="hlt">frequencies</span> of long-period events at Kusatsu-Shirane Volcano, Japan</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakano, M.; Kumagai, H.</p> <p>2005-01-01</p> <p>We investigate temporal <span class="hlt">variations</span> in the complex <span class="hlt">frequencies</span> (<span class="hlt">frequency</span> and quality factor Q) of long-period (LP) events that occurred at Kusatsu-Shirane Volcano, central Japan. We analyze LP waveforms observed at this volcano in the period between 1988 and 1995, which covers a seismically active period between 1989 and 1993. Systematic temporal <span class="hlt">variations</span> in the complex <span class="hlt">frequencies</span> are observed in October-November 1989, July-October 1991, and September 1992-January 1993. We use acoustic properties of a crack filled with hydrothermal fluids to interpret the observed temporal <span class="hlt">variations</span> in the complex <span class="hlt">frequencies</span>. The temporal <span class="hlt">variations</span> in October-November 1989 can be divided into two periods, which are explained by a gradual decrease and increase of a gas-volume fraction in a water-steam mixture in a crack, respectively. The temporal <span class="hlt">variations</span> in July-October 1991 can be also divided into two periods. These <span class="hlt">variations</span> in the first and second periods are similar to those observed in November 1989 and in September-November 1992, respectively, and are interpreted as drying of a water-steam mixture and misty gas in a crack, respectively. The repeated nature of the temporal <span class="hlt">variations</span> observed in similar seasons between July and November suggests the existence of seasonality in the occurrence of LP events. This may be caused by a seasonally variable meteoritic water supply to a hydrothermal system, which may have been heated by the flux of volcanic gases from magma beneath this volcano. ?? 2005 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010APS..DFD.GP003O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010APS..DFD.GP003O"><span>Long Chain DNA <span class="hlt">Separation</span> in a Sparse Nanopost Array</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ou, Jia; Joswiak, Mark; Dorfman, Kevin</p> <p>2010-11-01</p> <p>Long chain DNA <span class="hlt">separation</span> is a challenge for gel lectrophoresis. Our previous DNA <span class="hlt">separation</span> experiments and simulations demonstrated that a sparse micro post array can <span class="hlt">separate</span> large DNA. However, the smaller DNA are not well resolved. We hypothesized that smaller posts will increase the collision <span class="hlt">frequency</span> of the smaller DNA and thus the resolution. We successfully fabricated a hexagonal array of 350 nm diameter posts with a 3 μm spacing using an oxygen plasma etching method. Under an electric field of 10 V/cm, the mobilities of different species ranging from 10-48.5 kilobasepair (kbp) were normalized by the mobility of λ DNA (48.5 kbp), which was included in all experiments as a standard to correct for day-to-day <span class="hlt">variations</span> in electroosmotic flow. The resolution of these DNA is markedly improved when compared with a 1 μm diameter micropost array. We demonstrate the robustness of the device by using the calibration curve to identify the peaks in a <span class="hlt">separation</span> of the λ DNA-Mono Cut mix.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26561972','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26561972"><span>Effects of <span class="hlt">Frequency</span> <span class="hlt">Separation</span> and Diotic/Dichotic Presentations on the Alternation <span class="hlt">Frequency</span> Limits in Audition Derived from a Temporal Phase Discrimination Task.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kanaya, Shoko; Fujisaki, Waka; Nishida, Shin'ya; Furukawa, Shigeto; Yokosawa, Kazuhiko</p> <p>2015-02-01</p> <p>Temporal phase discrimination is a useful psychophysical task to evaluate how sensory signals, synchronously detected in parallel, are perceptually bound by human observers. In this task two stimulus sequences synchronously alternate between two states (say, A-B-A-B and X-Y-X-Y) in either of two temporal phases (ie A and B are respectively paired with X and Y, or vice versa). The critical alternation <span class="hlt">frequency</span> beyond which participants cannot discriminate the temporal phase is measured as an index characterizing the temporal property of the underlying binding process. This task has been used to reveal the mechanisms underlying visual and cross-modal bindings. To directly compare these binding mechanisms with those in another modality, this study used the temporal phase discrimination task to reveal the processes underlying auditory bindings. The two sequences were alternations between two pitches. We manipulated the distance between the two sequences by changing intersequence <span class="hlt">frequency</span> <span class="hlt">separation</span>, or presentation ears (diotic vs dichotic). Results showed that the alternation <span class="hlt">frequency</span> limit ranged from 7 to 30 Hz, becoming higher as the intersequence distance decreased, as is the case with vision. However, unlike vision, auditory phase discrimination limits were higher and more variable across participants. © 2015 SAGE Publications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20377573','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20377573"><span>Does infectious disease cause global <span class="hlt">variation</span> in the <span class="hlt">frequency</span> of intrastate armed conflict and civil war?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Letendre, Kenneth; Fincher, Corey L; Thornhill, Randy</p> <p>2010-08-01</p> <p>Geographic and cross-national <span class="hlt">variation</span> in the <span class="hlt">frequency</span> of intrastate armed conflict and civil war is a subject of great interest. Previous theory on this <span class="hlt">variation</span> has focused on the influence on human behaviour of climate, resource competition, national wealth, and cultural characteristics. We present the parasite-stress model of intrastate conflict, which unites previous work on the correlates of intrastate conflict by linking <span class="hlt">frequency</span> of the outbreak of such conflict, including civil war, to the intensity of infectious disease across countries of the world. High intensity of infectious disease leads to the emergence of xenophobic and ethnocentric cultural norms. These cultures suffer greater poverty and deprivation due to the morbidity and mortality caused by disease, and as a result of decreased investment in public health and welfare. Resource competition among xenophobic and ethnocentric groups within a nation leads to increased <span class="hlt">frequency</span> of civil war. We present support for the parasite-stress model with regression analyses. We find support for a direct effect of infectious disease on intrastate armed conflict, and support for an indirect effect of infectious disease on the incidence of civil war via its negative effect on national wealth. We consider the entanglements of feedback of conflict into further reduced wealth and increased incidence of disease, and discuss implications for international warfare and global patterns of wealth and imperialism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22489096-coupling-tuning-modal-frequencies-direct-current-biased-microelectromechanical-systems-arrays','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22489096-coupling-tuning-modal-frequencies-direct-current-biased-microelectromechanical-systems-arrays"><span>Coupling and tuning of modal <span class="hlt">frequencies</span> in direct current biased microelectromechanical systems arrays</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>Kambali, Prashant N.; Swain, Gyanadutta; Pandey, Ashok Kumar, E-mail: ashok@iith.ac.in</p> <p>2015-08-10</p> <p>Understanding the coupling of different modal <span class="hlt">frequencies</span> and their tuning mechanisms has become essential to design multi-<span class="hlt">frequency</span> MEMS devices. In this work, we fabricate a MEMS beam with fixed boundaries <span class="hlt">separated</span> from two side electrodes and a bottom electrode. Subsequently, we perform experiments to obtain the <span class="hlt">frequency</span> <span class="hlt">variation</span> of in-plane and out-of-plane mechanical modes of the microbeam with respect to both DC bias and laser heating. We show that the <span class="hlt">frequencies</span> of the two modes coincide at a certain DC bias, which in turn can also be varied due to temperature. Subsequently, we develop a theoretical model to predict themore » <span class="hlt">variation</span> of the two modes and their coupling due to a variable gap between the microbeam and electrodes, initial tension, and fringing field coefficients. Finally, we discuss the influence of <span class="hlt">frequency</span> tuning parameters in arrays of 3, 33, and 40 microbeams, respectively. It is also found that the <span class="hlt">frequency</span> bandwidth of a microbeam array can be increased to as high as 25 kHz for a 40 microbeam array with a DC bias of 80 V.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28086892','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28086892"><span>Pressure ulcer image segmentation technique through synthetic <span class="hlt">frequencies</span> generation and contrast <span class="hlt">variation</span> using toroidal geometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>David, Ortiz P; Sierra-Sosa, Daniel; Zapirain, Begoña García</p> <p>2017-01-06</p> <p>Pressure ulcers have become subject of study in recent years due to the treatment high costs and decreased life quality from patients. These chronic wounds are related to the global life expectancy increment, being the geriatric and physical disable patients the principal affected by this condition. Injuries diagnosis and treatment usually takes weeks or even months by medical personel. Using non-invasive techniques, such as image processing techniques, it is possible to conduct an analysis from ulcers and aid in its diagnosis. This paper proposes a novel technique for image segmentation based on contrast changes by using synthetic <span class="hlt">frequencies</span> obtained from the grayscale value available in each pixel of the image. These synthetic <span class="hlt">frequencies</span> are calculated using the model of energy density over an electric field to describe a relation between a constant density and the image amplitude in a pixel. A toroidal geometry is used to decompose the image into different contrast levels by <span class="hlt">variating</span> the synthetic <span class="hlt">frequencies</span>. Then, the decomposed image is binarized applying Otsu's threshold allowing for obtaining the contours that describe the contrast <span class="hlt">variations</span>. Morphological operations are used to obtain the desired segment of the image. The proposed technique is evaluated by synthesizing a Data Base with 51 images of pressure ulcers, provided by the Centre IGURCO. With the segmentation of these pressure ulcer images it is possible to aid in its diagnosis and treatment. To provide evidences of technique performance, digital image correlation was used as a measure, where the segments obtained using the methodology are compared with the real segments. The proposed technique is compared with two benchmarked algorithms. The results over the technique present an average correlation of 0.89 with a <span class="hlt">variation</span> of ±0.1 and a computational time of 9.04 seconds. The methodology presents better segmentation results than the benchmarked algorithms using less computational time and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22673411','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22673411"><span>Variables <span class="hlt">separation</span> of the spectral BRDF for better understanding color <span class="hlt">variation</span> in special effect pigment coatings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ferrero, Alejandro; Rabal, Ana María; Campos, Joaquín; Pons, Alicia; Hernanz, María Luisa</p> <p>2012-06-01</p> <p>A type of representation of the spectral bidirectional reflectance distribution function (BRDF) is proposed that distinctly <span class="hlt">separates</span> the spectral variable (wavelength) from the geometrical variables (spherical coordinates of the irradiation and viewing directions). Principal components analysis (PCA) is used in order to decompose the spectral BRDF in decorrelated spectral components, and the weight that they have at every geometrical configuration of irradiation/viewing is established. This method was applied to the spectral BRDF measurement of a special effect pigment sample, and four principal components with relevant variance were identified. These four components are enough to reproduce the great diversity of spectral reflectances observed at different geometrical configurations. Since this representation is able to <span class="hlt">separate</span> spectral and geometrical variables, it facilitates the interpretation of the color <span class="hlt">variation</span> of special effect pigments coatings versus the geometrical configuration of irradiation/viewing.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRD..120.4600Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRD..120.4600Z"><span>Studies of the <span class="hlt">variations</span> of the first Schumann resonance <span class="hlt">frequency</span> during the solar flare on 7 March 2012</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, Hongjuan; Qiao, Xiaolin</p> <p>2015-05-01</p> <p>The ELF measurements at the YS station in China during the X5.4 solar flare on 7 March 2012 are examined. The first modal Schumann resonance (SR) <span class="hlt">frequencies</span> of the horizontal magnetic field components were found to increase by 0.1-0.2 Hz during the X-ray burst. During the enhancement of the proton flux, the first modal <span class="hlt">frequency</span> of the east-west magnetic field component decreases by approximately 0.6 Hz at most, while the <span class="hlt">variation</span> in the north-south magnetic field component is less well defined. The mechanisms of the <span class="hlt">variations</span> are simulated with a finite difference time domain technique by modeling the perturbed conductivity profile in the day-night asymmetric Earth-ionosphere cavity and modeling the global lightning source with the raw flash data measured by satellites. The simulated varying trends of the SR <span class="hlt">frequencies</span> observed near the ground with the altitudes of the conductivity perturbations are nearly the same as those previously reported and are interpreted by the two characteristic height model first proposed by Greifinger and Greifinger. It is concluded that the SR <span class="hlt">frequencies</span> increase for enhanced conductivity above the altitude of 60-70 km because of the lowered magnetic height and decrease for enhanced conductivity below this altitude due to the lowered electric height. This finding can explain the opposite behaviors of the SR <span class="hlt">frequencies</span> during X-ray bursts and strong solar proton events (SPEs). The simulation model in this work proved to be effective, with the simulated shifts in the values of SR <span class="hlt">frequencies</span> during X-ray bursts and SPEs being close to the practical measurements.</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 <span class="hlt">separate</span> 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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160012469','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160012469"><span>Complex Signal Kurtosis and Independent Component Analysis for Wideband Radio <span class="hlt">Frequency</span> Interference Detection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schoenwald, Adam; Mohammed, Priscilla; Bradley, Damon; Piepmeier, Jeffrey; Wong, Englin; Gholian, Armen</p> <p>2016-01-01</p> <p>Radio-<span class="hlt">frequency</span> interference (RFI) has negatively implicated scientific measurements across a wide <span class="hlt">variation</span> passive remote sensing satellites. This has been observed in the L-band radiometers SMOS, Aquarius and more recently, SMAP [1, 2]. RFI has also been observed at higher <span class="hlt">frequencies</span> such as K band [3]. Improvements in technology have allowed wider bandwidth digital back ends for passive microwave radiometry. A complex signal kurtosis radio <span class="hlt">frequency</span> interference detector was developed to help identify corrupted measurements [4]. This work explores the use of ICA (Independent Component Analysis) as a blind source <span class="hlt">separation</span> technique to pre-process radiometric signals for use with the previously developed real and complex signal kurtosis detectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27661929','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27661929"><span>Origin of terminal voltage <span class="hlt">variations</span> due to self-mixing in terahertz <span class="hlt">frequency</span> quantum cascade lasers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grier, Andrew; Dean, Paul; Valavanis, Alexander; Keeley, James; Kundu, Iman; Cooper, Jonathan D; Agnew, Gary; Taimre, Thomas; Lim, Yah Leng; Bertling, Karl; Rakić, Aleksandar D; Li, Lianhe H; Harrison, Paul; Linfield, Edmund H; Ikonić, Zoran; Davies, A Giles; Indjin, Dragan</p> <p>2016-09-19</p> <p>We explain the origin of voltage <span class="hlt">variations</span> due to self-mixing in a terahertz (THz) <span class="hlt">frequency</span> quantum cascade laser (QCL) using an extended density matrix (DM) approach. Our DM model allows calculation of both the current-voltage (I-V) and optical power characteristics of the QCL under optical feedback by changing the cavity loss, to which the gain of the active region is clamped. The <span class="hlt">variation</span> of intra-cavity field strength necessary to achieve gain clamping, and the corresponding change in bias required to maintain a constant current density through the heterostructure is then calculated. Strong enhancement of the self-mixing voltage signal due to non-linearity of the (I-V) characteristics is predicted and confirmed experimentally in an exemplar 2.6 THz bound-to-continuum QCL.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27382482','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27382482"><span>Path loss <span class="hlt">variation</span> of on-body UWB channel in the <span class="hlt">frequency</span> bands of IEEE 802.15.6 standard.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Goswami, Dayananda; Sarma, Kanak C; Mahanta, Anil</p> <p>2016-06-01</p> <p>The wireless body area network (WBAN) has gaining tremendous attention among researchers and academicians for its envisioned applications in healthcare service. Ultra wideband (UWB) radio technology is considered as excellent air interface for communication among body area network devices. Characterisation and modelling of channel parameters are utmost prerequisite for the development of reliable communication system. The path loss of on-body UWB channel for each <span class="hlt">frequency</span> band defined in IEEE 802.15.6 standard is experimentally determined. The parameters of path loss model are statistically determined by analysing measurement data. Both the line-of-sight and non-line-of-sight channel conditions are considered in the measurement. <span class="hlt">Variations</span> of parameter values with the size of human body are analysed along with the <span class="hlt">variation</span> of parameter values with the surrounding environments. It is observed that the parameters of the path loss model vary with the <span class="hlt">frequency</span> band as well as with the body size and surrounding environment. The derived parameter values are specific to the particular <span class="hlt">frequency</span> bands of IEEE 802.15.6 standard, which will be useful for the development of efficient UWB WBAN system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3718373','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3718373"><span>A Mechanism for <span class="hlt">Frequency</span> Modulation in Songbirds Shared with 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>Margoliash, Daniel</p> <p>2013-01-01</p> <p>In most animals that vocalize, control of fundamental <span class="hlt">frequency</span> is a key element for effective communication. In humans, subglottal pressure controls vocal intensity but also influences fundamental <span class="hlt">frequency</span> during phonation. Given the underlying similarities in the biomechanical mechanisms of vocalization in humans and songbirds, songbirds offer an attractive opportunity to study <span class="hlt">frequency</span> modulation by pressure. Here, we present a novel technique for dynamic control of subsyringeal pressure in zebra finches. By regulating the opening of a custom-built fast valve connected to the air sac system, we achieved partial or total silencing of specific syllables, and could modify syllabic acoustics through more complex manipulations of air sac pressure. We also observed that more nuanced pressure <span class="hlt">variations</span> over a limited interval during production of a syllable concomitantly affected the <span class="hlt">frequency</span> of that syllable segment. These results can be explained in terms of a mathematical model for phonation that incorporates a nonlinear description for the vocal source capable of generating the observed <span class="hlt">frequency</span> modulations induced by pressure <span class="hlt">variations</span>. We conclude that the observed interaction between pressure and <span class="hlt">frequency</span> was a feature of the source, not a result of feedback control. Our results indicate that, beyond regulating phonation or its absence, regulation of pressure is important for control of fundamental <span class="hlt">frequencies</span> of vocalizations. Thus, although there are <span class="hlt">separate</span> brainstem pathways for syringeal and respiratory control of song production, both can affect airflow and <span class="hlt">frequency</span>. We hypothesize that the control of pressure and <span class="hlt">frequency</span> is combined holistically at higher levels of the vocalization pathways. PMID:23825417</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23825417','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23825417"><span>A mechanism for <span class="hlt">frequency</span> modulation in songbirds shared with humans.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Amador, Ana; Margoliash, Daniel</p> <p>2013-07-03</p> <p>In most animals that vocalize, control of fundamental <span class="hlt">frequency</span> is a key element for effective communication. In humans, subglottal pressure controls vocal intensity but also influences fundamental <span class="hlt">frequency</span> during phonation. Given the underlying similarities in the biomechanical mechanisms of vocalization in humans and songbirds, songbirds offer an attractive opportunity to study <span class="hlt">frequency</span> modulation by pressure. Here, we present a novel technique for dynamic control of subsyringeal pressure in zebra finches. By regulating the opening of a custom-built fast valve connected to the air sac system, we achieved partial or total silencing of specific syllables, and could modify syllabic acoustics through more complex manipulations of air sac pressure. We also observed that more nuanced pressure <span class="hlt">variations</span> over a limited interval during production of a syllable concomitantly affected the <span class="hlt">frequency</span> of that syllable segment. These results can be explained in terms of a mathematical model for phonation that incorporates a nonlinear description for the vocal source capable of generating the observed <span class="hlt">frequency</span> modulations induced by pressure <span class="hlt">variations</span>. We conclude that the observed interaction between pressure and <span class="hlt">frequency</span> was a feature of the source, not a result of feedback control. Our results indicate that, beyond regulating phonation or its absence, regulation of pressure is important for control of fundamental <span class="hlt">frequencies</span> of vocalizations. Thus, although there are <span class="hlt">separate</span> brainstem pathways for syringeal and respiratory control of song production, both can affect airflow and <span class="hlt">frequency</span>. We hypothesize that the control of pressure and <span class="hlt">frequency</span> is combined holistically at higher levels of the vocalization pathways.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRA..123..567S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRA..123..567S"><span><span class="hlt">Variations</span> of High-Latitude Geomagnetic Pulsation <span class="hlt">Frequencies</span>: A Comparison of Time-of-Flight Estimates and IMAGE Magnetometer Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sandhu, J. K.; Yeoman, T. K.; James, M. K.; Rae, I. J.; Fear, R. C.</p> <p>2018-01-01</p> <p>The fundamental eigenfrequencies of standing Alfvén waves on closed geomagnetic field lines are estimated for the region spanning 5.9≤L < 9.5 over all MLT (Magnetic Local Time). The T96 magnetic field model and a realistic empirical plasma mass density model are employed using the time-of-flight approximation, refining previous calculations that assumed a relatively simplistic mass density model. An assessment of the implications of using different mass density models in the time-of-flight calculations is presented. The calculated <span class="hlt">frequencies</span> exhibit dependences on field line footprint magnetic latitude and MLT, which are attributed to both magnetic field configuration and spatial <span class="hlt">variations</span> in mass density. In order to assess the validity of the time-of-flight calculated <span class="hlt">frequencies</span>, the estimates are compared to observations of FLR (Field Line Resonance) <span class="hlt">frequencies</span>. Using IMAGE (International Monitor for Auroral Geomagnetic Effects) ground magnetometer observations obtained between 2001 and 2012, an automated FLR identification method is developed, based on the cross-phase technique. The average FLR <span class="hlt">frequency</span> is determined, including <span class="hlt">variations</span> with footprint latitude and MLT, and compared to the time-of-flight analysis. The results show agreement in the latitudinal and local time dependences. Furthermore, with the use of the realistic mass density model in the time-of-flight calculations, closer agreement with the observed FLR <span class="hlt">frequencies</span> is obtained. The study is limited by the latitudinal coverage of the IMAGE magnetometer array, and future work will aim to extend the ground magnetometer data used to include additional magnetometer arrays.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhyA..392.4279S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhyA..392.4279S"><span>Irreversibility and entropy production in transport phenomena, IV: Symmetry, integrated intermediate processes and <span class="hlt">separated</span> <span class="hlt">variational</span> principles for multi-currents</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suzuki, Masuo</p> <p>2013-10-01</p> <p>The mechanism of entropy production in transport phenomena is discussed again by emphasizing the role of symmetry of non-equilibrium states and also by reformulating Einstein’s theory of Brownian motion to derive entropy production from it. This yields conceptual reviews of the previous papers [M. Suzuki, Physica A 390 (2011) 1904; 391 (2012) 1074; 392 (2013) 314]. <span class="hlt">Separated</span> <span class="hlt">variational</span> principles of steady states for multi external fields {Xi} and induced currents {Ji} are proposed by extending the principle of minimum integrated entropy production found by the present author for a single external field. The basic strategy of our theory on steady states is to take in all the intermediate processes from the equilibrium state to the final possible steady states in order to study the irreversible physics even in the steady states. As an application of this principle, Gransdorff-Prigogine’s evolution criterion inequality (or stability condition) dXP≡∫dr∑iJidXi≤0 is derived in the stronger form dQi≡∫drJidXi≤0 for individual force Xi and current Ji even in nonlinear responses which depend on all the external forces {Xk} nonlinearly. This is called “<span class="hlt">separated</span> evolution criterion”. Some explicit demonstrations of the present general theory to simple electric circuits with multi external fields are given in order to clarify the physical essence of our new theory and to realize the condition of its validity concerning the existence of the solutions of the simultaneous equations obtained by the <span class="hlt">separated</span> <span class="hlt">variational</span> principles. It is also instructive to compare the two results obtained by the new <span class="hlt">variational</span> theory and by the old scheme based on the instantaneous entropy production. This seems to be suggestive even to the energy problem in the world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007ACPD....712417B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007ACPD....712417B"><span>Assessment of high to low <span class="hlt">frequency</span> <span class="hlt">variations</span> of isoprene emission rates using a neural network approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boissard, C.; Chervier, F.; Dutot, A. L.</p> <p>2007-08-01</p> <p>Using a statistical approach based on artificial neural networks, an emission algorithm (ISO_LF) accounting for high (instantaneous) to low (seasonal) <span class="hlt">frequency</span> <span class="hlt">variations</span> was developed for isoprene. ISO_LF was optimised using an isoprene emission data base (ISO-DB) specifically designed for this work. ISO-DB consists of 1321 emission rates collected in the literature, together with 34 environmental variables, measured or assessed using NCDC (National Climatic Data Center) or NCEP (National Centers for Environmental Predictions) meteorological databases. ISO-DB covers a large variety of emitters (25 species) and environmental conditions (10° S to 60° N). When only instantaneous environmental regressors (air temperature and photosynthetic active radiation, PAR) were used, a maximum of 60% of the overall isoprene variability was assessed and the highest emissions were underestimated. Considering a total of 9 high (instantaneous) to low (up to 3 weeks) <span class="hlt">frequency</span> regressors, ISO_LF accounts for up to 91% of the isoprene emission variability, whatever the emission range, species or climate. Diurnal and seasonal <span class="hlt">variations</span> are correctly reproduced for textit{Ulex europaeus} with a maximum factor of discrepancy of 4. ISO-LF was found to be mainly sensitive to air temperature cumulated over 3 weeks T21 and to instantaneous light L0 and air temperature T0 <span class="hlt">variations</span>. T21, T0 and L0 only accounts for 76% of the overall variability. The use of ISO-LF for non stored monoterpene emissions was shown to give poor results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15664226','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15664226"><span>Ethnic <span class="hlt">variations</span> in UK asthma <span class="hlt">frequency</span>, morbidity, and health-service use: a systematic review and meta-analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Netuveli, Gopalakrishnan; Hurwitz, Brian; Levy, Mark; Fletcher, Monica; Barnes, Greta; Durham, Stephen R; Sheikh, Aziz</p> <p></p> <p>The <span class="hlt">frequency</span> of asthma varies between countries, and may also vary between ethnic groups in more geographically confined areas. We sought evidence of such ethnic <span class="hlt">variations</span> in the UK for asthma <span class="hlt">frequency</span>, morbidity, and health-services use, and to understand possible reasons for any differences. We searched MEDLINE, EMBASE, CINAHL, PSYCHInfo, PREMEDLINE, HEALTHSTAR, Cambridge Register of Conference Abstracts, the Dissertation and Thesis Database, and the National Registry of Research. Additionally, we searched the bibliographies of reports identified and websites of health authorities, and contacted experts in this discipline. Our main outcomes were comparisons of asthma rate, morbidity, and health-services use. We did meta-analyses using random-effects models. 13 studies contained relevant data. All prevalence studies were of children and showed that south Asian children had a lower <span class="hlt">frequency</span> of symptoms suggestive of asthma compared with black and white children (pooled rate of history of wheeze in the previous 12 months: south Asians 9.6% [95%CI 8.0-11.2%], black people 16.2% [12.8-19.6%], white people 14.6% [11.5-17.8%]). The pooled <span class="hlt">frequency</span> of clinician-diagnosed asthma in children followed a similar pattern (south Asians 7.6% [3.7-11.4%], black people 15.0% [3.5-26.5%], white people 10.6% [4.6-16.7%]. However, relative to white people, the risk of admission for asthma in children and adults was higher for south Asians (odds ratio 2.9 [2.4-3.4]) and black people (2.1 [1.8-2.5]). The differences in admission are not explained by differences in asthma <span class="hlt">frequency</span> between groups; they could relate to ethnic <span class="hlt">variations</span> in asthma severity, differences in health-seeking behaviour, or difficulties in accessing high-quality primary care services.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830026125','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830026125"><span><span class="hlt">Separability</span> of agricultural crops with airborne scatterometry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mehta, N. C.</p> <p>1983-01-01</p> <p>Backscattering measurements were acquired with airborne scatterometers over a site in Cass County, North Dakota on four days in the 1981 crop growing season. Data were acquired at three <span class="hlt">frequencies</span> (L-, C- and Ku-bands), two polarizations (like and cross) and ten incidence angles (5 degrees to 50 degrees in 5 degree steps). Crop <span class="hlt">separability</span> is studied in an hierarchical fashion. A two-class <span class="hlt">separability</span> measure is defined, which compares within-class to between-class variability, to determine crop <span class="hlt">separability</span>. The scatterometer channels with the best potential for crop <span class="hlt">separability</span> are determined, based on this <span class="hlt">separability</span> measure. Higher <span class="hlt">frequencies</span> are more useful for discriminating small grains, while lower <span class="hlt">frequencies</span> tend to <span class="hlt">separate</span> non-small grains better. Some crops are more <span class="hlt">separable</span> when row direction is taken into account. The effect of pixel purity is to increase the <span class="hlt">separability</span> between all crops while not changing the order of useful scatterometer channels. Crude estimates of <span class="hlt">separability</span> errors are calculated based on these analyses. These results are useful in selecting the parameters of active microwave systems in agricultural remote sensing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004ASAJ..116.1656F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ASAJ..116.1656F"><span>Auditory stream segregation in monkey auditory cortex: effects of <span class="hlt">frequency</span> <span class="hlt">separation</span>, presentation rate, and tone duration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fishman, Yonatan I.; Arezzo, Joseph C.; Steinschneider, Mitchell</p> <p>2004-09-01</p> <p>Auditory stream segregation refers to the organization of sequential sounds into ``perceptual streams'' reflecting individual environmental sound sources. In the present study, sequences of alternating high and low tones, ``...ABAB...,'' similar to those used in psychoacoustic experiments on stream segregation, were presented to awake monkeys while neural activity was recorded in primary auditory cortex (A1). Tone <span class="hlt">frequency</span> <span class="hlt">separation</span> (ΔF), tone presentation rate (PR), and tone duration (TD) were systematically varied to examine whether neural responses correlate with effects of these variables on perceptual stream segregation. ``A'' tones were fixed at the best <span class="hlt">frequency</span> of the recording site, while ``B'' tones were displaced in <span class="hlt">frequency</span> from ``A'' tones by an amount=ΔF. As PR increased, ``B'' tone responses decreased in amplitude to a greater extent than ``A'' tone responses, yielding neural response patterns dominated by ``A'' tone responses occurring at half the alternation rate. Increasing TD facilitated the differential attenuation of ``B'' tone responses. These findings parallel psychoacoustic data and suggest a physiological model of stream segregation whereby increasing ΔF, PR, or TD enhances spatial differentiation of ``A'' tone and ``B'' tone responses along the tonotopic map in A1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123j4903L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123j4903L"><span>Radio-<span class="hlt">frequency</span> characteristic <span class="hlt">variation</span> of interdigital capacitor having multilayer graphene of various widths</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Hee-Jo; Hong, Young-Pyo</p> <p>2018-03-01</p> <p>In this paper, a radio-<span class="hlt">frequency</span> circuit model of an interdigital capacitor (IDC) with a multilayer graphene (MLG) width <span class="hlt">variation</span> is proposed. The circuit model with three sample configurations, i.e., a bare IDC, IDC-MLG with a width of 5 μm, and IDC-MLG with a width of 20 μm, is constructed via a fitted method based on the measured samples. The simulated results of the circuit model are validated through the RF characteristics, e.g., the capacitance and the self-resonance <span class="hlt">frequency</span>, of the measured samples. From the circuit model, all samples show not only a similar capacitance behavior but also an identical self-resonance <span class="hlt">frequency</span> of 10 GHz. Moreover, the R, L, and C values of MLG with a 5 μm width (MLG with a 20 μm width) alone are approximately 0.8 kΩ (0.5 kΩ), 0.5 nH (0.9 nH), and 0.3 pF (0.1 pF), respectively. As a result, we find that the simulated results are in good agreement with RF characteristics of the measured samples. In the future, we expect that the proposed circuit model of an IDC with MLG will offer assistance with performance predictions of diverse IDC-based 2D material applications, such as biosensors and gas sensors, as well as supercapacitors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29312060','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29312060"><span>Fundamental <span class="hlt">Frequency</span> <span class="hlt">Variation</span> of Neonatal Spontaneous Crying Predicts Language Acquisition in Preterm and Term Infants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shinya, Yuta; Kawai, Masahiko; Niwa, Fusako; Imafuku, Masahiro; Myowa, Masako</p> <p>2017-01-01</p> <p>Spontaneous cries of infants exhibit rich melodic features (i.e., time <span class="hlt">variation</span> of fundamental <span class="hlt">frequency</span> [ F 0 ]) even during the neonatal period, and the development of these characteristics might provide an essential base for later expressive prosody in language. However, little is known about the melodic features of spontaneous cries in preterm infants, who have a higher risk of later language-related problems. Thus, the present study investigated how preterm birth influenced melodic features of spontaneous crying at term-equivalent age as well as how these melodic features related to language outcomes at 18 months of corrected age in preterm and term infants. At term, moderate-to-late preterm (MLP) infants showed spontaneous cries with significantly higher F 0 <span class="hlt">variation</span> and melody complexity than term infants, while there were no significant differences between very preterm (VP) and term infants. Furthermore, larger F 0 <span class="hlt">variation</span> within cry series at term was significantly related to better language and cognitive outcomes, particularly expressive language skills, at 18 months. On the other hand, no other melodic features at term predicted any developmental outcomes at 18 months. The present results suggest that the additional postnatal vocal experience of MLP preterm infants increased F 0 <span class="hlt">variation</span> and the complexity of spontaneous cries at term. Additionally, the increases in F 0 <span class="hlt">variation</span> may partly reflect the development of voluntary vocal control, which, in turn, contributes to expressive language in infancy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19893303','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19893303"><span>Human <span class="hlt">frequency</span>-following response to speech-like sounds: correlates of off-<span class="hlt">frequency</span> masking.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krishnan, Ananthanarayan; Agrawal, Smita</p> <p>2010-01-01</p> <p>Off-<span class="hlt">frequency</span> masking of the second formant by energy at the first formant has been shown to influence both identification and discrimination of the second formant in normal-hearing and hearing-impaired listeners. While both excitatory spread and two-tone suppression have been implicated in this simultaneous masking, their relative contribution has been shown to depend on both the level of the masker and the <span class="hlt">frequency</span> <span class="hlt">separation</span> between the probe and the masker. Off-<span class="hlt">frequency</span> masking effects were evaluated in 10 normal-hearing human adults using the <span class="hlt">frequency</span>-following response (FFR) to two two-tone approximations of vowel stimuli (/a/ and /u/). In the first experiment, the masking effect of F(1) on F(2) was evaluated by attenuating the level of F(1) relative to a fixed F(2) level. In the second experiment, the masking effect was evaluated by increasing the <span class="hlt">frequency</span> <span class="hlt">separation</span> between F(1) and F(2) using F(2) <span class="hlt">frequency</span> as the variable. Results revealed that both attenuation of the F(1) level, and increasing the <span class="hlt">frequency</span> <span class="hlt">separation</span> between F(1) and F(2) increased the magnitude of the FFR component at F(2). These results are consistent with a release from off-<span class="hlt">frequency</span> masking. Given that the results presented here are for high signal and masker levels and for relatively smaller <span class="hlt">frequency</span> <span class="hlt">separation</span> between the masker and the probe, it is possible that both suppression and excitatory spread contributed to the masking effects observed in our data. Copyright2009 S. Karger AG, Basel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Tectp.615....1E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Tectp.615....1E"><span>Spatiotemporal <span class="hlt">variations</span> in the b-value of earthquake magnitude-<span class="hlt">frequency</span> distributions: Classification and causes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>El-Isa, Z. H.; Eaton, David W.</p> <p>2014-03-01</p> <p>Interpretation of the b-value of earthquake <span class="hlt">frequency</span>-magnitude distributions has received considerable attention in recent decades. This paper provides a comprehensive review of previous investigations of spatial and temporal <span class="hlt">variations</span> in b-value, including their classification and possible causes. Based on least-squares regression of seismicity data compiled from the NEIC, IRIS and ISC catalogs, we find an average value of 1.02 ± 0.03 for the whole Earth and its two hemispheres, consistent with the general view that in seismically active regions the long-term average value is close to unity. Nevertheless, wide-ranging b-<span class="hlt">variations</span> (0.3 ≤ b ≤ 2.5) have been reported in the literature. This variability has been interpreted to arise from one or more of the following factors: prevailing stress state, crustal heterogeneity, focal depth, pore pressure, geothermal gradient, tectonic setting, petrological/environmental/geophysical characteristics, clustering of events, incomplete catalog data, and/or method of calculation. Excluding the latter, all of these factors appear to be linked, directly or indirectly, with the effective state of stress. Although time-dependent changes in b-value are well documented, conflicting observations reveal either a precursory increase or decrease in b value before major earthquakes. Our compilation of published analyses suggests that statistically significant b-<span class="hlt">variations</span> occur globally on various timescales, including annual, monthly and perhaps diurnal. Taken together, our review suggests that b-<span class="hlt">variations</span> are most plausibly linked with changes in effective stress.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27207643','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27207643"><span>In situ cardiac perfusion reveals interspecific <span class="hlt">variation</span> of intraventricular flow <span class="hlt">separation</span> in reptiles.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Joyce, William; Axelsson, Michael; Altimiras, Jordi; Wang, Tobias</p> <p>2016-07-15</p> <p>The ventricles of non-crocodilian reptiles are incompletely divided and provide an opportunity for mixing of oxygen-poor blood and oxygen-rich blood (intracardiac shunting). However, both cardiac morphology and in vivo shunting patterns exhibit considerable interspecific <span class="hlt">variation</span> within reptiles. In the present study, we develop an in situ double-perfused heart approach to characterise the propensity and capacity for shunting in five reptile species: the turtle Trachemys scripta, the rock python Python sebae, the yellow anaconda Eunectes notaeus, the varanid lizard Varanus exanthematicus and the bearded dragon Pogona vitticeps To simulate changes in vascular bed resistance, pulmonary and systemic afterloads were independently manipulated and changes in blood flow distribution amongst the central outflow tracts were monitored. As previously demonstrated in Burmese pythons, rock pythons and varanid lizards exhibited pronounced intraventricular flow <span class="hlt">separation</span>. As pulmonary or systemic afterload was raised, flow in the respective circulation decreased. However, flow in the other circulation, where afterload was constant, remained stable. This correlates with the convergent evolution of intraventricular pressure <span class="hlt">separation</span> and the large intraventricular muscular ridge, which compartmentalises the ventricle, in these species. Conversely, in the three other species, the pulmonary and systemic flows were strongly mutually dependent, such that the decrease in pulmonary flow in response to elevated pulmonary afterload resulted in redistribution of perfusate to the systemic circuit (and vice versa). Thus, in these species, the muscular ridge appeared labile and blood could readily transverse the intraventricular cava. We conclude that relatively minor structural differences between non-crocodilian reptiles result in the fundamental changes in cardiac function. Further, our study emphasises that functionally similar intracardiac flow <span class="hlt">separation</span> evolved independently in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23382536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23382536"><span>Single molecule molecular inversion probes for targeted, high-accuracy detection of low-<span class="hlt">frequency</span> <span class="hlt">variation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hiatt, Joseph B; Pritchard, Colin C; Salipante, Stephen J; O'Roak, Brian J; Shendure, Jay</p> <p>2013-05-01</p> <p>The detection and quantification of genetic heterogeneity in populations of cells is fundamentally important to diverse fields, ranging from microbial evolution to human cancer genetics. However, despite the cost and throughput advances associated with massively parallel sequencing, it remains challenging to reliably detect mutations that are present at a low relative abundance in a given DNA sample. Here we describe smMIP, an assay that combines single molecule tagging with multiplex targeted capture to enable practical and highly sensitive detection of low-<span class="hlt">frequency</span> or subclonal <span class="hlt">variation</span>. To demonstrate the potential of the method, we simultaneously resequenced 33 clinically informative cancer genes in eight cell line and 45 clinical cancer samples. Single molecule tagging facilitated extremely accurate consensus calling, with an estimated per-base error rate of 8.4 × 10(-6) in cell lines and 2.6 × 10(-5) in clinical specimens. False-positive mutations in the single molecule consensus base-calls exhibited patterns predominantly consistent with DNA damage, including 8-oxo-guanine and spontaneous deamination of cytosine. Based on mixing experiments with cell line samples, sensitivity for mutations above 1% <span class="hlt">frequency</span> was 83% with no false positives. At clinically informative sites, we identified seven low-<span class="hlt">frequency</span> point mutations (0.2%-4.7%), including BRAF p.V600E (melanoma, 0.2% alternate allele <span class="hlt">frequency</span>), KRAS p.G12V (lung, 0.6%), JAK2 p.V617F (melanoma, colon, two lung, 0.3%-1.4%), and NRAS p.Q61R (colon, 4.7%). We anticipate that smMIP will be broadly adoptable as a practical and effective method for accurately detecting low-<span class="hlt">frequency</span> mutations in both research and clinical settings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10164E..2VK','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10164E..2VK"><span>Development of flow <span class="hlt">separation</span> control system to reduce the vibration of wind turbine blades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Ho-Young; Kim, Ho-Hyun; Han, Jong-Seob; Han, Jae-Hung</p> <p>2017-04-01</p> <p>The size of wind turbine blade has been continuously increased. Large-scale wind turbine blades induce loud noise, vibration; and maintenance difficulty is also increased. It causes the eventual increases of the cost of energy. The vibration of wind turbine blade is caused by several reasons such as a blade rotation, tower shadow, wind shear, and flow <span class="hlt">separation</span> of a wind turbine blade. This wind speed <span class="hlt">variation</span> changes in local angle of attack of the blades and create the vibration. The <span class="hlt">variation</span> of local angle of attack influences the lift coefficient and causes the large change of the lift. In this study, we focus on the lift coefficient control using a flow control device to reduce the vibration. DU35-A15 airfoil was employed as baseline model. A plasma actuator was installed to generate the upwind jet in order to control the lift coefficient. Wind tunnel experiment was performed to demonstrate of the performance of the plasma actuator. The results show the plasma actuator can induce the flow <span class="hlt">separation</span> compared with the baseline model. In addition, the actuator can delay the flow <span class="hlt">separation</span> depending on the input AC <span class="hlt">frequency</span> with the same actuator configuration.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21731056','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21731056"><span>Data-driven approach to detect common copy-number <span class="hlt">variations</span> and <span class="hlt">frequency</span> profiles in a population-based Korean cohort.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Moon, Sanghoon; Kim, Young Jin; Hong, Chang Bum; Kim, Dong-Joon; Lee, Jong-Young; Kim, Bong-Jo</p> <p>2011-11-01</p> <p>To date, hundreds of thousands of copy-number <span class="hlt">variation</span> (CNV) data have been reported using various platforms. The proportion of Asians in these data is, however, relatively small as compared with that of other ethnic groups, such as Caucasians and Yorubas. Because of limitations in platform resolution and the high noise level in signal intensity, in most CNV studies (particularly those using single nucleotide polymorphism arrays), the average number of CNVs in an individual is less than the number of known CNVs. In this study, we ascertained reliable, common CNV regions (CNVRs) and identified actual <span class="hlt">frequency</span> rates in the Korean population to provide more CNV information. We performed two-stage analyses for detecting structural <span class="hlt">variations</span> with two platforms. We discovered 576 common CNVRs (88 CNV segments on average in an individual), and 87% (501 of 576) of these CNVRs overlapped by ≥1 bp with previously validated CNV events. Interestingly, from the <span class="hlt">frequency</span> analysis of CNV profiles, 52 of 576 CNVRs had a <span class="hlt">frequency</span> rate of <1% in the 8842 individuals. Compared with other common CNV studies, this study found six common CNVRs that were not reported in previous CNV studies. In conclusion, we propose the data-driven detection approach to discover common CNVRs including those of unreported in the previous Korean CNV study while minimizing false positives. Through our approach, we successfully discovered more common CNVRs than previous Korean CNV study and conducted <span class="hlt">frequency</span> analysis. These results will be a valuable resource for the effective level of CNVs in the Korean population.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JOUC...11..267W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JOUC...11..267W"><span>Diagnosis of seasonal <span class="hlt">variations</span> of tropical cyclogenesis over the South China Sea using a genesis potential index</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Lei; Pan, Xiumei</p> <p>2012-09-01</p> <p>This study examines the seasonal <span class="hlt">variations</span> of tropical cyclogenesis over the South China Sea (SCS) using a genesis potential (GP) index developed by Emanuel and Nolan. How different environmental factors (including low-level vorticity, mid-level relative humidity, vertical wind shear, and potential intensity) contribute to these <span class="hlt">variations</span> is investigated. Composite anomalies of the GP index are produced for the summer and winter monsoons <span class="hlt">separately</span>. These composites replicate the observed seasonal <span class="hlt">variations</span> of the observed <span class="hlt">frequency</span> and location of tropical cyclogenesis over the SCS. The degree of contribution by each factor in different regions is determined quantitatively by producing composites of modified indices in which only one of the contributing factors varies, with the others set to climatology. Over the northern SCS, potential intensity makes the largest contributions to the seasonal <span class="hlt">variations</span> in tropical cyclogenesis. Over the southern SCS, the low-level relative vorticity plays the primary role in the seasonal modulation of tropical cyclone (TC) genesis <span class="hlt">frequency</span>, and the vertical wind shear plays the secondary role. Thermodynamic factors play more important roles for the seasonal <span class="hlt">variations</span> in tropical cyclogenesis over the northern SCS, while dynamic factors are more important in the seasonal modulation of TC genesis <span class="hlt">frequency</span> over the southern SCS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4929657','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4929657"><span>Artificial neural networks for retrieving absorption and reduced scattering spectra from <span class="hlt">frequency</span>-domain diffuse reflectance spectroscopy at short source-detector <span class="hlt">separation</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>Chen, Yu-Wen; Chen, Chien-Chih; Huang, Po-Jung; Tseng, Sheng-Hao</p> <p>2016-01-01</p> <p>Diffuse reflectance spectroscopy (DRS) based on the <span class="hlt">frequency</span>-domain (FD) technique has been employed to investigate the optical properties of deep tissues such as breast and brain using source to detector <span class="hlt">separation</span> up to 40 mm. Due to the modeling and system limitations, efficient and precise determination of turbid sample optical properties from the FD diffuse reflectance acquired at a source-detector <span class="hlt">separation</span> (SDS) of around 1 mm has not been demonstrated. In this study, we revealed that at SDS of 1 mm, acquiring FD diffuse reflectance at multiple <span class="hlt">frequencies</span> is necessary for alleviating the influence of inevitable measurement uncertainty on the optical property recovery accuracy. Furthermore, we developed artificial neural networks (ANNs) trained by Monte Carlo simulation generated databases that were capable of efficiently determining FD reflectance at multiple <span class="hlt">frequencies</span>. The ANNs could work in conjunction with a least-square optimization algorithm to rapidly (within 1 second), accurately (within 10%) quantify the sample optical properties from FD reflectance measured at SDS of 1 mm. In addition, we demonstrated that incorporating the steady-state apparatus into the FD DRS system with 1 mm SDS would enable obtaining broadband absorption and reduced scattering spectra of turbid samples in the wavelength range from 650 to 1000 nm. PMID:27446671</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4406589','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4406589"><span>Extreme Recombination <span class="hlt">Frequencies</span> Shape Genome <span class="hlt">Variation</span> and Evolution in the Honeybee, Apis mellifera</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wallberg, Andreas; Glémin, Sylvain; Webster, Matthew T.</p> <p>2015-01-01</p> <p>Meiotic recombination is a fundamental cellular process, with important consequences for evolution and genome integrity. However, we know little about how recombination rates vary across the genomes of most species and the molecular and evolutionary determinants of this <span class="hlt">variation</span>. The honeybee, Apis mellifera, has extremely high rates of meiotic recombination, although the evolutionary causes and consequences of this are unclear. Here we use patterns of linkage disequilibrium in whole genome resequencing data from 30 diploid honeybees to construct a fine-scale map of rates of crossing over in the genome. We find that, in contrast to vertebrate genomes, the recombination landscape is not strongly punctate. Crossover rates strongly correlate with levels of genetic <span class="hlt">variation</span>, but not divergence, which indicates a pervasive impact of selection on the genome. Germ-line methylated genes have reduced crossover rate, which could indicate a role of methylation in suppressing recombination. Controlling for the effects of methylation, we do not infer a strong association between gene expression patterns and recombination. The site <span class="hlt">frequency</span> spectrum is strongly skewed from neutral expectations in honeybees: rare variants are dominated by AT-biased mutations, whereas GC-biased mutations are found at higher <span class="hlt">frequencies</span>, indicative of a major influence of GC-biased gene conversion (gBGC), which we infer to generate an allele fixation bias 5 – 50 times the genomic average estimated in humans. We uncover further evidence that this repair bias specifically affects transitions and favours fixation of CpG sites. Recombination, via gBGC, therefore appears to have profound consequences on genome evolution in honeybees and interferes with the process of natural selection. These findings have important implications for our understanding of the forces driving molecular evolution. PMID:25902173</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005ASAJ..117.2390M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005ASAJ..117.2390M"><span>The impact of <span class="hlt">variation</span> in low-<span class="hlt">frequency</span> interaural cross correlation on auditory spatial imagery in stereophonic loudspeaker reproduction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martens, William</p> <p>2005-04-01</p> <p>Several attributes of auditory spatial imagery associated with stereophonic sound reproduction are strongly modulated by <span class="hlt">variation</span> in interaural cross correlation (IACC) within low <span class="hlt">frequency</span> bands. Nonetheless, a standard practice in bass management for two-channel and multichannel loudspeaker reproduction is to mix low-<span class="hlt">frequency</span> musical content to a single channel for reproduction via a single driver (e.g., a subwoofer). This paper reviews the results of psychoacoustic studies which support the conclusion that reproduction via multiple drivers of decorrelated low-<span class="hlt">frequency</span> signals significantly affects such important spatial attributes as auditory source width (ASW), auditory source distance (ASD), and listener envelopment (LEV). A variety of methods have been employed in these tests, including forced choice discrimination and identification, and direct ratings of both global dissimilarity and distinct attributes. Contrary to assumptions that underlie industrial standards established in 1994 by ITU-R. Recommendation BS.775-1, these findings imply that substantial stereophonic spatial information exists within audio signals at <span class="hlt">frequencies</span> below the 80 to 120 Hz range of prescribed subwoofer cutoff <span class="hlt">frequencies</span>, and that loudspeaker reproduction of decorrelated signals at <span class="hlt">frequencies</span> as low as 50 Hz can have an impact upon auditory spatial imagery. [Work supported by VRQ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28689084','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28689084"><span>Regional <span class="hlt">variations</span> in <span class="hlt">frequency</span> of glycosylated hemoglobin (HbA1c) monitoring in Korea: A multilevel analysis of nationwide data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yoo, Kyoung-Hun; Shin, Dong-Wook; Cho, Mi-Hee; Kim, Sang-Hyuck; Bahk, Hyun-Jung; Kim, Shin-Hye; Jeong, Su-Min; Yun, Jae-Moon; Park, Jin-Ho; Kim, Heesun; Cho, BeLong</p> <p>2017-09-01</p> <p>Suboptimal <span class="hlt">frequency</span> of glycosylated hemoglobin (HbA1c) monitoring is associated with poor diabetes control. We aimed to analyze compliance to HbA1c testing guidelines and explore associated individual and area-level determinants, focusing on regional <span class="hlt">variation</span>. This cross-sectional study between the period of 2012-2013 was conducted by using the Korean National Health Insurance Research Database, and included 45,634 patients diagnosed with diabetes mellitus, who were prescribed any anti-diabetic medications, including insulin. We calculated the proportion of each HbA1c testing <span class="hlt">frequency</span> (≥1, ≥2, or ≥4 times per year) stratified by 17 administrative regions. Multilevel and multivariate logistic analyses were performed with regional (proportion of farmer population) and individual characteristics (age, sex, income level, duration of diabetes, and most visited medical institution). Overall, 67.3% of the patients received≥1 HbA1c test per year; 37.8% and 6.1% received ≥2 and ≥4 tests per year, respectively. Those managed in secondary-level hospitals or clinics and those living in rural areas were less likely to receive HbA1c testing. Even after adjusting for individual and regional level characteristics, significant area level <span class="hlt">variation</span> was observed (variance participant coefficients were 7.91%, 9.58%, and 14.43% for testing <span class="hlt">frequencies</span> of ≥1, ≥2, and ≥4 times a year, respectively). The <span class="hlt">frequency</span> of HbA1c monitoring is suboptimal in Korea, especially in rural areas. Moreover, significant regional <span class="hlt">variation</span> was observed, implying a contextual effect. This suggests the need for developing policy actions to improve HbA1c monitoring. In particular, access to HbA1c testing in rural primary care clinics must be improved. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27814533','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27814533"><span>Temporal and spatial <span class="hlt">variations</span> in road traffic noise for different <span class="hlt">frequency</span> components in metropolitan Taichung, Taiwan.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Ven-Shing; Lo, Ei-Wen; Liang, Chih-Hsiang; Chao, Keh-Ping; Bao, Bo-Ying; Chang, Ta-Yuan</p> <p>2016-12-01</p> <p>Road traffic noise exposure has been associated with auditory and non-auditory health effects, but few studies report noise characteristics. This study determines 24-h noise levels and analyzes their <span class="hlt">frequency</span> components to investigate associations between seasons, meteorology, land-use types, and traffic. We set up 50 monitoring stations covering ten different land-use types and conducted measurements at three times of the year to obtain 24-h-average A-weighted equivalent noise levels (L Aeq , 24h ) and <span class="hlt">frequency</span> analyses from 2013 to 2014 in Taichung, Taiwan. Information on land-use types, road parameters, traffic flow rates, and meteorological variables was also collected for analysis with the annual averages of road traffic noise and its <span class="hlt">frequency</span> components. The annual average L Aeq , 24h in Taichung was 66.4 ± 4.7 A-weighed decibels (dBA). Significant differences in L Aeq , 24h and <span class="hlt">frequency</span> components were observed between land-use types (all p-values < 0.001), but not between seasons, with the highest two noise levels of 71.2 ± 1.0 dBA and 70.0 ± 2.6 dBA measured in stream-channel and commercial areas, with the highest component being 61.4 ± 5.3 dBA at 1000 Hz. Road width, traffic flow rates, and land-use types were significantly associated with annual average L Aeq , 24h (all p-values < 0.050). Noise levels at 125 Hz had the highest correlation with total traffic (Spearman's coefficient = 0.795) and the highest prediction in the multiple linear regression (R 2  = 0.803; adjusted R 2  = 0.765). These findings reveal the spatial <span class="hlt">variation</span> in road traffic noise exposure in Taichung. The highest correlation and predictive capacity was observed between this <span class="hlt">variation</span> and noise levels at 125 Hz. We recommend that governmental agencies should take actions to reduce noise levels from traffic vehicles. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28783163','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28783163"><span><span class="hlt">Frequency</span> of mononuclear diploid cardiomyocytes underlies natural <span class="hlt">variation</span> in heart regeneration.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Patterson, Michaela; Barske, Lindsey; Van Handel, Ben; Rau, Christoph D; Gan, Peiheng; Sharma, Avneesh; Parikh, Shan; Denholtz, Matt; Huang, Ying; Yamaguchi, Yukiko; Shen, Hua; Allayee, Hooman; Crump, J Gage; Force, Thomas I; Lien, Ching-Ling; Makita, Takako; Lusis, Aldons J; Kumar, S Ram; Sucov, Henry M</p> <p>2017-09-01</p> <p>Adult mammalian cardiomyocyte regeneration after injury is thought to be minimal. Mononuclear diploid cardiomyocytes (MNDCMs), a relatively small subpopulation in the adult heart, may account for the observed degree of regeneration, but this has not been tested. We surveyed 120 inbred mouse strains and found that the <span class="hlt">frequency</span> of adult mononuclear cardiomyocytes was surprisingly variable (>7-fold). Cardiomyocyte proliferation and heart functional recovery after coronary artery ligation both correlated with pre-injury MNDCM content. Using genome-wide association, we identified Tnni3k as one gene that influences <span class="hlt">variation</span> in this composition and demonstrated that Tnni3k knockout resulted in elevated MNDCM content and increased cardiomyocyte proliferation after injury. Reciprocally, overexpression of Tnni3k in zebrafish promoted cardiomyocyte polyploidization and compromised heart regeneration. Our results corroborate the relevance of MNDCMs in heart regeneration. Moreover, they imply that intrinsic heart regeneration is not limited nor uniform in all individuals, but rather is a variable trait influenced by multiple genes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28035792','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28035792"><span>Novel microfluidic device for the continuous <span class="hlt">separation</span> of cancer cells using dielectrophoresis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alazzam, Anas; Mathew, Bobby; Alhammadi, Falah</p> <p>2017-03-01</p> <p>We describe the design, microfabrication, and testing of a microfluidic device for the <span class="hlt">separation</span> of cancer cells based on dielectrophoresis. Cancer cells, specifically green fluorescent protein-labeled MDA-MB-231, are successfully <span class="hlt">separated</span> from a heterogeneous mixture of the same and normal blood cells. MDA-MB-231 cancer cells are <span class="hlt">separated</span> with an accuracy that enables precise detection and counting of circulating tumor cells present among normal blood cells. The <span class="hlt">separation</span> is performed using a set of planar interdigitated transducer electrodes that are deposited on the surface of a glass wafer and slightly protrude into the <span class="hlt">separation</span> microchannel at one side. The device includes two parts, namely, a glass wafer and polydimethylsiloxane element. The device is fabricated using standard microfabrication techniques. All experiments are conducted with low conductivity sucrose-dextrose isotonic medium. The <span class="hlt">variation</span> in response between MDA-MB-231 cancer cells and normal cells to a certain band of alternating-current <span class="hlt">frequencies</span> is used for continuous <span class="hlt">separation</span> of cells. The fabrication of the microfluidic device, preparation of cells and medium, and flow conditions are detailed. The proposed microdevice can be used to detect and <span class="hlt">separate</span> malignant cells from heterogeneous mixture of cells for the purpose of early screening for cancer. © 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3638140','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3638140"><span>Single molecule molecular inversion probes for targeted, high-accuracy detection of low-<span class="hlt">frequency</span> <span class="hlt">variation</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>Hiatt, Joseph B.; Pritchard, Colin C.; Salipante, Stephen J.; O'Roak, Brian J.; Shendure, Jay</p> <p>2013-01-01</p> <p>The detection and quantification of genetic heterogeneity in populations of cells is fundamentally important to diverse fields, ranging from microbial evolution to human cancer genetics. However, despite the cost and throughput advances associated with massively parallel sequencing, it remains challenging to reliably detect mutations that are present at a low relative abundance in a given DNA sample. Here we describe smMIP, an assay that combines single molecule tagging with multiplex targeted capture to enable practical and highly sensitive detection of low-<span class="hlt">frequency</span> or subclonal <span class="hlt">variation</span>. To demonstrate the potential of the method, we simultaneously resequenced 33 clinically informative cancer genes in eight cell line and 45 clinical cancer samples. Single molecule tagging facilitated extremely accurate consensus calling, with an estimated per-base error rate of 8.4 × 10−6 in cell lines and 2.6 × 10−5 in clinical specimens. False-positive mutations in the single molecule consensus base-calls exhibited patterns predominantly consistent with DNA damage, including 8-oxo-guanine and spontaneous deamination of cytosine. Based on mixing experiments with cell line samples, sensitivity for mutations above 1% <span class="hlt">frequency</span> was 83% with no false positives. At clinically informative sites, we identified seven low-<span class="hlt">frequency</span> point mutations (0.2%–4.7%), including BRAF p.V600E (melanoma, 0.2% alternate allele <span class="hlt">frequency</span>), KRAS p.G12V (lung, 0.6%), JAK2 p.V617F (melanoma, colon, two lung, 0.3%–1.4%), and NRAS p.Q61R (colon, 4.7%). We anticipate that smMIP will be broadly adoptable as a practical and effective method for accurately detecting low-<span class="hlt">frequency</span> mutations in both research and clinical settings. PMID:23382536</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1204006','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1204006"><span><span class="hlt">Frequency</span>-Dependent Selection: The High Potential for Permanent Genetic <span class="hlt">Variation</span> in the Diallelic, Pairwise Interaction Model</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Asmussen, M. A.; Basnayake, E.</p> <p>1990-01-01</p> <p>A detailed analytic and numerical study is made of the potential for permanent genetic <span class="hlt">variation</span> in <span class="hlt">frequency</span>-dependent models based on pairwise interactions among genotypes at a single diallelic locus. The full equilibrium structure and qualitative gene-<span class="hlt">frequency</span> dynamics are derived analytically for a symmetric model, in which pairwise fitnesses are chiefly determined by the genetic similarity of the individuals involved. This is supplemented by an extensive numerical investigation of the general model, the symmetric model, and nine other special cases. Together the results show that there is a high potential for permanent genetic diversity in the pairwise interaction model, and provide insight into the extent to which various forms of genotypic interactions enhance or reduce this potential. Technically, although two stable polymorphic equilibria are possible, the increased likelihood of maintaining both alleles, and the poor performance of protected polymorphism conditions as a measure of this likelihood, are primarily due to a greater variety and <span class="hlt">frequency</span> of equilibrium patterns with one stable polymorphic equilibrium, in conjunction with a disproportionately large domain of attraction for stable internal equilibria. PMID:2341034</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1005582-self-assembly-amorphous-biophotonic-nanostructures-phase-separation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1005582-self-assembly-amorphous-biophotonic-nanostructures-phase-separation"><span>Self-assembly of amorphous biophotonic nanostructures by phase <span class="hlt">separation</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>Dufresne, Eric R.; Noh, Heeso; Saranathan, Vinodkumar</p> <p>2009-04-23</p> <p>Some of the most vivid colors in the animal kingdom are created not by pigments, but by wavelength-selective scattering of light from nanostructures. Here we investigate quasi-ordered nanostructures of avian feather barbs which produce vivid non-iridescent colors. These {beta}-keratin and air nanostructures are found in two basic morphologies: tortuous channels and amorphous packings of spheres. Each class of nanostructure is isotropic and has a pronounced characteristic length scale of <span class="hlt">variation</span> in composition. These local structural correlations lead to strong backscattering over a narrow range of optical <span class="hlt">frequencies</span> and little <span class="hlt">variation</span> with angle of incidence. Such optical properties play important rolesmore » in social and sexual communication. To be effective, birds need to precisely control the development of these nanoscale structures, yet little is known about how they grow. We hypothesize that multiple lineages of birds have convergently evolved to exploit phase <span class="hlt">separation</span> and kinetic arrest to self-assemble spongy color-producing nanostructures in feather barbs. Observed avian nanostructures are strikingly similar to those self-assembled during the phase <span class="hlt">separation</span> of fluid mixtures; the channel and sphere morphologies are characteristic of phase <span class="hlt">separation</span> by spinodal decomposition and nucleation and growth, respectively. These unstable structures are locked-in by the kinetic arrest of the {beta}-keratin matrix, likely through the entanglement or cross-linking of supermolecular {beta}-keratin fibers. Using the power of self-assembly, birds can robustly realize a diverse range of nanoscopic morphologies with relatively small physical and chemical changes during feather development.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMNS41B1685K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMNS41B1685K"><span>Development of a new medium <span class="hlt">frequency</span> EM device: Mapping soil water content <span class="hlt">variations</span> using electrical conductivity and dielectric permittivity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kessouri, P.; Buvat, S.; Tabbagh, A.</p> <p>2012-12-01</p> <p>Both electrical conductivity and dielectric permittivity of soil are influenced by its water content. Dielectric permittivity is usually measured in the high <span class="hlt">frequency</span> range, using GPR or TDR, where the sensitivity to water content is high. However, its evaluation is limited by a low investigation depth, especially for clay rich soils. Electrical conductivity is closely related not only to soil water content, but also to clay content and soil structure. A simultaneous estimation of these electrical parameters can allow the mapping of soil water content <span class="hlt">variations</span> for an investigation depth close to 1m. In order to estimate simultaneously both soil electrical conductivity and dielectric permittivity, an electromagnetic device working in the medium <span class="hlt">frequency</span> range (between 100 kHz and 10 MHz) has been designed. We adopted Slingram geometry for the EM prototype: its PERP configuration (vertical transmission loop Tx and horizontal measuring loop Rx) was defined using 1D ground models. As the required investigation depth is around 1m, the coil spacing was fixed to 1.2m. This prototype works in a <span class="hlt">frequency</span> range between 1 and 5 MHz. After calibration, we tested the response of prototype to objects with known properties. The first in situ measurements were led on experimental sites with different types of soils and different water content <span class="hlt">variations</span> (artificially created or natural): sandy alluvium on a plot of INRA (French National Institute for Agricultural Research) in Orléans (Centre, France), a clay-loam soil on an experimental site in Estrée-Mons (Picardie, France) and fractured limestone at the vicinity of Grand (Vosges, France). In the case of the sandy alluvium, the values of dielectric permittivity measured are close to those of HF permittivity and allow the use of existing theoretical models to determine the soil water content. For soils containing higher amount of clay, the coupled information brought by the electrical conductivity and the dielectric</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDA17007C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDA17007C"><span>Control of flow <span class="hlt">separation</span> in a turbulent boundary layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, Minjeong; Choi, Sangho; Choi, Haecheon</p> <p>2015-11-01</p> <p>Towards the development of successful control methods for <span class="hlt">separation</span> delay in a turbulent boundary layer, we adopt a model flow field, in which a turbulent <span class="hlt">separation</span> occurs above a flat plate (Na and Moin 1998 JFM), and apply controls to this flow for reducing the size of the <span class="hlt">separation</span> bubble and investigating the interaction between the forcing and flow near the <span class="hlt">separation</span> bubble. We provide a single-<span class="hlt">frequency</span> forcing with zero net mass flow rate at the upstream of the <span class="hlt">separation</span> bubble. At low forcing <span class="hlt">frequencies</span>, spanwise vortices are generated and travel downstream, bringing high momentum toward the wall and reducing the size of the <span class="hlt">separation</span> bubble. Also, these vortices cause the <span class="hlt">separation</span> and reattachment points to travel downstream. On the other hand, at high forcing <span class="hlt">frequencies</span>, the size of the <span class="hlt">separation</span> bubble becomes smaller and larger in time, respectively, due to the pressure gradient alternating favorably and adversely in time. Supported by NRF-2011-0028032 and 2014048162.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/862448','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/862448"><span>Product <span class="hlt">separator</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Welsh, Robert A.; Deurbrouck, Albert W.</p> <p>1976-01-20</p> <p>A secondary light sensitive photoelectric product <span class="hlt">separator</span> for use with a primary product <span class="hlt">separator</span> that concentrates a material so that it is visually distinguishable from adjacent materials. The concentrate <span class="hlt">separation</span> is accomplished first by feeding the material onto a vibratory inclined surface with a liquid flow, such as a wet concentrating table. Vibrations generally perpendicular to the stream direction of flow cause the concentrate to <span class="hlt">separate</span> from its mixture according to its color. When the concentrate and its surrounding stream reach the recovery end of the table, a detecting device notes the line of color demarcation and triggers a signal if it differs from a normal condition. If no difference is noted nothing moves on the second <span class="hlt">separator</span>. However, if a difference is detected in the constant monitoring of the color line's location, a product splitter and recovery unit normally positioned near the color line at the recovery end, moves to a new position. In this manner the selected <span class="hlt">separated</span> concentrate is recovered at a maximum rate regardless of <span class="hlt">variations</span> in the flow stream or other conditions present.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A13G0313M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A13G0313M"><span>Regional <span class="hlt">frequency</span> analysis to asses wind resource spatial and temporal <span class="hlt">variations</span> in Washington State</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mortuza, M.; Demissie, D.</p> <p>2013-12-01</p> <p>According to the U.S. Department of Energy's annual wind technologies market report, the wind power capacity in the country grew from 2.5 gigawatts in early 2000 to 60 gigawatts in 2012, making it one of the largest new sources of electric capacity additions in the U.S. in recent years. With over 2.8 gigawatts of current capacity (eighth largest in the nation), Washington State plays a significant role in this rapidly increasing energy resource. To further expand and/or optimize these capacities, assessment of wind resource and its spatial and temporal <span class="hlt">variations</span> are important. However, since at-site <span class="hlt">frequency</span> analysis using meteorological data is not adequate for extending wind <span class="hlt">frequency</span> to locations with no data, longer return period, and heterogeneous topography and surface, a regional <span class="hlt">frequency</span> analysis based on L-moment method is adopted in this study to estimate regional wind speed patterns and return periods in Washington State using hourly mean wind speed data from 1979 - 2010. The analysis applies the k-means, hierarchical and self-organizing map clustering techniques to explore potential clusters or regions; statistical tests are then applied to identify homogeneous regions and appropriate probability distribution models. The result from the analysis is expected to provide essential knowledge about the areas with potential capacity of constructing wind power plants, which can also be readily extended to assist decisions on their daily operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CRGeo.345..350F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CRGeo.345..350F"><span>Estimating <span class="hlt">variation</span> in stomatal <span class="hlt">frequency</span> at intra-individual, intra-site, and inter-taxonomic levels in populations of the Leonardoxa africana (Fabaceae) complex over environmental gradients in Cameroon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finsinger, Walter; Dos Santos, Thibaut; McKey, Doyle</p> <p>2013-07-01</p> <p><span class="hlt">Variation</span> of stomatal <span class="hlt">frequency</span> (stomatal density and stomatal index) includes genetically-based, potentially-adaptive <span class="hlt">variation</span>, and <span class="hlt">variation</span> due to phenotypic plasticity, the degree of which may be fundamental to the ability to maintain high water-use efficiency and thus to deal with environmental change. We analysed stomatal <span class="hlt">frequency</span> and morphology (pore length, pore width) in leaves from several individuals from nine populations of four sub-species of the Leonardoxa africana complex. The dataset represents a hierarchical sampling wherein factors are nested within each level (leaves in individuals, individuals in sites, etc.), allowing estimation of the contribution of different levels to overall <span class="hlt">variation</span>, using variance-component analysis. SI showed significant <span class="hlt">variation</span> among sites ("site" is largely confounded with "sub-species"), being highest in the sub-species localized in the highest-elevation site. However, most of the observed variance was accounted for at intra-site and intra-individual levels. This variance could reflect great phenotypic plasticity, presumably in response to highly local <span class="hlt">variation</span> in micro-environmental conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MeScT..28g5004G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MeScT..28g5004G"><span>Mode <span class="hlt">separation</span> in <span class="hlt">frequency</span>-wavenumber domain through compressed sensing of far-field Lamb waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gao, Fei; Zeng, Liang; Lin, Jing; Luo, Zhi</p> <p>2017-07-01</p> <p>This method based on Lamb waves shows great potential for long-range damage detection. Mode superposition resulting from multi-modal and dispersive characteristics makes signal interpretation and damage feature extraction difficult. Mode <span class="hlt">separation</span> in the <span class="hlt">frequency</span>-wavenumber (f-k) domain using a 1D sparse sensing array is a promising solution. However, due to the lack of prior knowledge about damage location, this method based on 1D linear measurement, for the mode extraction of arbitrary reflections caused by defects that are not in line with the sensor array, is restricted. In this paper, an improved compressed sensing method under the far-field assumption is established, which is beneficial to the reconstruction of reflections in the f-k domain. Hence, multiple components consisting of structure and damage features could be recovered via a limited number of measurements. Subsequently, a mode sweeping process based on theoretical dispersion curves has been designed for mode characterization and direction of arrival estimation. Moreover, 2D f-k filtering and inverse transforms are applied to the reconstructed f-k distribution in order to extract the purified mode of interest. As a result, overlapping waveforms can be <span class="hlt">separated</span> and the direction of defects can be estimated. A uniform linear sensor array consisting of 16 laser excitations is finally employed for experimental investigations and the results demonstrate the efficiency of the proposed method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10509388','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10509388"><span>[<span class="hlt">Variation</span> in mycoses <span class="hlt">frequency</span> in Mexico].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Méndez Tovar, L J; López Martínez, R; Macotela Ruiz, E; Manzano Gayosso, P; Serrano Jaén, L; Carmona Castañón, A; Mondragón Gonźalez, R</p> <p>1999-01-01</p> <p>We show the records about diagnosed mycoses in a hospital in Mexico City in two periods of time: from 1967 to 1977 and from 1993 to 1997. In the former 15,429 patients were studied and in the latter, 5,998. Striking differences among <span class="hlt">frequency</span>, etiological agents and clinical outcome, were observed. The most frequent infections in both lapses were the superficial ones, however the most recent scores showed a notorious increase in opportunistic infections. We diagnosed only one histoplasmosis case during the period from 1993 to 1997. Etiological agents have also changed, dermatophytes <span class="hlt">frequency</span> like Trichophyton mentagrophytes and T. tonsurans have diminished while T. rubrum increased from 60% to 80% of the whole dermatophytoses cases. Even though Criptococcus neoformans used to be the only agent causing criptococosis, in the most recent report we found that C. laurentii, C. terreus and C. unigutulatus were also isolated. Another important difference was mortality in rhinocerebral mucormicosis: twenty years ago it was fairly 80%, nowadays it has decreased to 20%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5157949','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5157949"><span>Mutation Rate <span class="hlt">Variation</span> is a Primary Determinant of the Distribution of Allele <span class="hlt">Frequencies</span> 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>Pritchard, Jonathan K.</p> <p>2016-01-01</p> <p>The site <span class="hlt">frequency</span> spectrum (SFS) has long been used to study demographic history and natural selection. Here, we extend this summary by examining the SFS conditional on the alleles found at the same site in other species. We refer to this extension as the “phylogenetically-conditioned SFS” or cSFS. Using recent large-sample data from the Exome Aggregation Consortium (ExAC), combined with primate genome sequences, we find that human variants that occurred independently in closely related primate lineages are at higher <span class="hlt">frequencies</span> in humans than variants with parallel substitutions in more distant primates. We show that this effect is largely due to sites with elevated mutation rates causing significant departures from the widely-used infinite sites mutation model. Our analysis also suggests substantial <span class="hlt">variation</span> in mutation rates even among mutations involving the same nucleotide changes. In summary, we show that variable mutation rates are key determinants of the SFS in humans. PMID:27977673</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT.......183H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT.......183H"><span>Experimental investigation on the effects of non-cyclical <span class="hlt">frequency</span> and amplitude <span class="hlt">variation</span> on dynamic stall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heintz, Kyle C.</p> <p></p> <p>An experimental study of a cambered airfoil undergoing non-cyclical, transient pitch trajectories and the resulting effects on the dynamic stall phenomenon is presented. Surface pressure measurements and airfoil incidence angle are acquired simultaneously to resolve instantaneous aerodynamic load coefficients at Mach numbers ranging from 0.2 to 0.4. Derived from these coefficients are various formulations of the aerodynamic damping factor, referred to copiously throughout. Using a two-motor mechanism, each providing independent <span class="hlt">frequency</span> and amplitude input to the airfoil, unique pitch motions can be implemented by actively controlling the phase between inputs. This work primarily focuses on three pitch motion schemas, the first of which is a "chirp" style trajectory featuring concurrent exponential <span class="hlt">frequency</span> growth and amplitude decay. Second, these parameters are tested <span class="hlt">separately</span> to determine their individual contributions. Lastly, a novel dual harmonic pitch motion is devised which rapidly traverses dynamic stall regimes on an inter-cycle basis by modulating the static-stall penetration angle. Throughout all results presented, there is evidence that for consecutive pitch-cycles, the process of dynamic stall is affected when prior oscillations prior have undergone deeper stall-penetration angles. In other words when stall-penetration is descending, retreating from a regime of light or deep stall, statistics of load coefficients, such as damping coefficient, maximum lift, minimum quarter-chord moment, and their phase relationships, do not match the values seen when stall-penetration was growing. The outcomes herein suggest that the airfoil retains some memory of previous flow <span class="hlt">separation</span> which has the potential to change the influence of the dynamic stall vortex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17360212','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17360212"><span>Interannual <span class="hlt">variations</span> in feeding <span class="hlt">frequencies</span> and food quality of greater flamingo chicks (Phoenicopterus roseus): evidence from plasma chemistry and effects on body condition.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Amat, Juan A; Hortas, Francisco; Arroyo, Gonzalo M; Rendón, Miguel A; Ramírez, José M; Rendón-Martos, Manuel; Pérez-Hurtado, Alejandro; Garrido, Araceli</p> <p>2007-06-01</p> <p>Greater flamingos in southern Spain foraged in areas distant from a breeding site, spending 4-6 days in foraging areas between successive visits to the colony to feed their chicks. During four years, we took blood samples from chicks to ascertain whether there were interannual <span class="hlt">variations</span> in several blood parameters, indicative of food quality and feeding <span class="hlt">frequencies</span>. When the chicks were captured, 20-31% of them had their crops empty, indicating that not all chicks were fed daily. Additional evidence of <span class="hlt">variations</span> in feeding <span class="hlt">frequencies</span> was obtained from a principal component analysis (PCA) on plasma chemistry values, which also indicated that there were annual <span class="hlt">variations</span> in the quality of food received by chicks. The association of cholesterol and glucose with some PC axes indicated that some chicks were experiencing fasting periods. Of all plasma metabolites considered, cholesterol was the best one to predict body condition. Greater flamingo chicks experiencing longer fasting intervals, as suggested by higher plasma levels of cholesterol, were in lower body condition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15525061','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15525061"><span>Limit on the present temporal <span class="hlt">variation</span> of the fine structure constant.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peik, E; Lipphardt, B; Schnatz, H; Schneider, T; Tamm, Chr; Karshenboim, S G</p> <p>2004-10-22</p> <p>The comparison of different atomic transition <span class="hlt">frequencies</span> over time can be used to determine the present value of the temporal derivative of the fine structure constant alpha in a model-independent way without assumptions on constancy or variability of other parameters, allowing tests of the consequences of unification theories. We have measured an optical transition <span class="hlt">frequency</span> at 688 THz in 171Yb+ with a cesium atomic clock at 2 times <span class="hlt">separated</span> by 2.8 yr and find a value for the fractional <span class="hlt">variation</span> of the <span class="hlt">frequency</span> ratio f(Yb)/f(Cs) of (-1.2+/-4.4)x10(-15) yr(-1), consistent with zero. Combined with recently published values for the constancy of other transition <span class="hlt">frequencies</span> this measurement sets an upper limit on the present variability of alpha at the level of 2.0x10(-15) yr(-1) (1sigma), corresponding so far to the most stringent limit from laboratory experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/24061','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/24061"><span>Cover/<span class="hlt">Frequency</span> (CF)</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>John F. Caratti</p> <p>2006-01-01</p> <p>The FIREMON Cover/<span class="hlt">Frequency</span> (CF) method is used to assess changes in plant species cover and <span class="hlt">frequency</span> for a macroplot. This method uses multiple quadrats to sample within-plot <span class="hlt">variation</span> and quantify statistically valid changes in plant species cover, height, and <span class="hlt">frequency</span> over time. Because it is difficult to estimate cover in quadrats for larger plants, this method...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B33F0260T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B33F0260T"><span>Process Inference from High <span class="hlt">Frequency</span> Temporal <span class="hlt">Variations</span> in Dissolved Organic Carbon (DOC) Dynamics Across Nested Spatial Scales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tunaley, C.; Tetzlaff, D.; Lessels, J. S.; Soulsby, C.</p> <p>2014-12-01</p> <p>In order to understand aquatic ecosystem functioning it is critical to understand the processes that control the spatial and temporal <span class="hlt">variations</span> in DOC. DOC concentrations are highly dynamic, however, our understanding at short, high <span class="hlt">frequency</span> timescales is still limited. Optical sensors which act as a proxy for DOC provide the opportunity to investigate near-continuous DOC <span class="hlt">variations</span> 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 <span class="hlt">frequency</span> 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 <span class="hlt">frequency</span> 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 <span class="hlt">frequency</span> 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</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050215216','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050215216"><span>Impulsive Injection for Compressor Stator <span class="hlt">Separation</span> Control</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Culley, Dennis E.; Braunscheidel, Edward P.; Bright, Michelle M.</p> <p>2005-01-01</p> <p>Flow control using impulsive injection from the suction surface of a stator vane has been applied in a low speed axial compressor. Impulsive injection is shown to significantly reduce <span class="hlt">separation</span> relative to steady injection for vanes that were induced to <span class="hlt">separate</span> by an increase in vane stagger angle of 4 degrees. Injected flow was applied to the airfoil suction surface using spanwise slots pitched in the streamwise direction. Injection was limited to the near-hub region, from 10 to 36 percent of span, to affect the dominant loss due to hub leakage flow. Actuation was provided externally using high-speed solenoid valves closely coupled to the vane tip. <span class="hlt">Variations</span> in injected mass, <span class="hlt">frequency</span>, and duty cycle are explored. The local corrected total pressure loss across the vane at the lower span region was reduced by over 20 percent. Additionally, low momentum fluid migrating from the hub region toward the tip was effectively suppressed resulting in an overall benefit which reduced corrected area averaged loss through the passage by 4 percent. The injection mass fraction used for impulsive actuation was typically less than 0.1 percent of the compressor through flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7205091','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/7205091"><span>Light beam <span class="hlt">frequency</span> comb generator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Priatko, G.J.; Kaskey, J.A.</p> <p>1992-11-24</p> <p>A light beam <span class="hlt">frequency</span> comb generator uses an acousto-optic modulator to generate a plurality of light beams with <span class="hlt">frequencies</span> which are uniformly <span class="hlt">separated</span> and possess common noise and drift characteristics. A well collimated monochromatic input light beam is passed through this modulator to produce a set of both <span class="hlt">frequency</span> shifted and unshifted optical beams. An optical system directs one or more <span class="hlt">frequency</span> shifted beams along a path which is parallel to the path of the input light beam such that the <span class="hlt">frequency</span> shifted beams are made incident on the modulator proximate to but <span class="hlt">separated</span> from the point of incidence of the input light beam. After the beam is thus returned to and passed through the modulator repeatedly, a plurality of mutually parallel beams are generated which are <span class="hlt">frequency</span>-shifted different numbers of times and possess common noise and drift characteristics. 2 figs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/868558','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/868558"><span>Light beam <span class="hlt">frequency</span> comb generator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Priatko, Gordon J.; Kaskey, Jeffrey A.</p> <p>1992-01-01</p> <p>A light beam <span class="hlt">frequency</span> comb generator uses an acousto-optic modulator to generate a plurality of light beams with <span class="hlt">frequencies</span> which are uniformly <span class="hlt">separated</span> and possess common noise and drift characteristics. A well collimated monochromatic input light beam is passed through this modulator to produce a set of both <span class="hlt">frequency</span> shifted and unshifted optical beams. An optical system directs one or more <span class="hlt">frequency</span> shifted beams along a path which is parallel to the path of the input light beam such that the <span class="hlt">frequency</span> shifted beams are made incident on the modulator proximate to but <span class="hlt">separated</span> from the point of incidence of the input light beam. After the beam is thus returned to and passed through the modulator repeatedly, a plurality of mutually parallel beams are generated which are <span class="hlt">frequency</span>-shifted different numbers of times and possess common noise and drift characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22607811','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22607811"><span>Intraspecific <span class="hlt">variations</span> of Dekkera/Brettanomyces bruxellensis genome studied by capillary electrophoresis <span class="hlt">separation</span> of the intron splice site profiles.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vigentini, Ileana; De Lorenzis, Gabriella; Picozzi, Claudia; Imazio, Serena; Merico, Annamaria; Galafassi, Silvia; Piškur, Jure; Foschino, Roberto</p> <p>2012-06-15</p> <p>In enology, "Brett" character refers to the wine spoilage caused by the yeast Dekkera/Brettanomyces bruxellensis and its production of volatile phenolic off-flavours. However, the spoilage potential of this yeast is strain-dependent. Therefore, a rapid and reliable recognition at the strain level is a key point to avoid serious economic losses. The present work provides an operative tool to assess the genetic intraspecific <span class="hlt">variation</span> in this species through the use of introns as molecular targets. Firstly, the available partial D./B. bruxellensis genome sequence was investigated in order to build primers annealing to introns 5' splice site sequence (ISS). This analysis allowed the detection of a non-random vocabulary flanking the site and, exploiting this feature, the creation of specific probes for strain discrimination. Secondly, the <span class="hlt">separation</span> of the intron splice site PCR fragments was obtained throughout the set up of a capillary electrophoresis protocol, giving a 94% repeatability threshold in our experimental conditions. The comparison of results obtained with ISS-PCR/CE versus the ones performed by mtDNA RFLP revealed that the former protocol is more discriminating and allowed a reliable identification at strain level. Actually sixty D./B. bruxellensis isolates were recognised as unique strains, showing a level of similarity below 79% and confirming the high genetic polymorphism existing within the species. Two main clusters were grouped at similarity levels of about 46% and 47%, respectively, showing a poor correlation with the geographic area of isolation. Moreover, from the evolutionary point of view, the proposed technique could determine the <span class="hlt">frequency</span> of the genome rearrangements that can occur in D./B. bruxellesis populations. Copyright © 2012 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT........71S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT........71S"><span>Optimal Control of Airfoil Flow <span class="hlt">Separation</span> using Fluidic Excitation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shahrabi, Arireza F.</p> <p></p> <p> as well as F+ were evaluated and discussed. The computational model predictions showed good agreement with the experimental data. It was observed that different angles of attack and flap angles have different requirements for the minimum value of the momentum coefficient, Cμ, in order for the SJA to be effective for control of <span class="hlt">separation</span>. It was also found that the <span class="hlt">variation</span> of F + noticeably affects the lift and drag forces acting on the airfoil. The optimum values of parameters during open loop control simulations have been applied in order to introduce the optimal open loop control outcome. An innovative approach has been implemented to formulate optimal <span class="hlt">frequencies</span> and momentum ratios of vortex shedding which depends on angle of attack and static pressure of the <span class="hlt">separation</span> zone in the upper chord. Optimal open loop results have been compared with the optimal closed loop results. Cumulative case studies in the matter of angle of attacks, flap angles, Re, Cμ and F+ provide a convincing collection of evidence to the following conclusion. An improvement of a direct closed loop control was demonstrated, and an analytical formula describing the properties of a <span class="hlt">separated</span> flow and vortex shedding was proposed. Best AFC solutions are offered by providing optimal <span class="hlt">frequencies</span> and momentum ratios at a variety of flow conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A31E0112Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A31E0112Y"><span>Decadal <span class="hlt">Variation</span>'s Offset of Global Warming in Recent Tropical Pacific Climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yeo, S. R.; Yeh, S. W.; Kim, K. Y.; Kim, W.</p> <p>2015-12-01</p> <p>Despite the increasing greenhouse gas concentration, there is no significant warming in the sea surface temperature (SST) over the tropical eastern Pacific since about 2000. This counterintuitive observation has generated substantial interest in the role of low-<span class="hlt">frequency</span> <span class="hlt">variation</span> over the Pacific Ocean such as Pacific Decadal Oscillation (PDO) or Interdecadal Pacific Oscillation (IPO). Therefore, it is necessary to appropriately <span class="hlt">separate</span> low-<span class="hlt">frequency</span> variability and global warming from SST records. Here we present three primary modes of global SST as a secular warming trend, a low-<span class="hlt">frequency</span> variability, and a biennial oscillation through the use of novel statistical method. By analyzing temporal behavior of the three-mode, it is found that the opposite contributions of secular warming trend and cold phase of low-<span class="hlt">frequency</span> variability since 1999 account for the warming hiatus in the tropical eastern Pacific. This result implies that the low-<span class="hlt">frequency</span> variability modulates the manifestation of global warming signal in the tropical Pacific SST. Furthermore, if the low-<span class="hlt">frequency</span> variability turns to a positive phase, warming in the tropical eastern Pacific will be amplified and also strong El Niño events will occur more frequently in the near future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15797412','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15797412"><span>Lateral <span class="hlt">separation</span> of colloids or cells by dielectrophoresis augmented by AC electroosmosis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhou, Hao; White, Lee R; Tilton, Robert D</p> <p>2005-05-01</p> <p>Colloidal particles and biological cells are patterned and <span class="hlt">separated</span> laterally adjacent to a micropatterned electrode array by applying AC electric fields that are principally oriented normally to the electrode array. This is demonstrated for yeast cells, red blood cells, and colloidal polystyrene particles of different sizes and zeta-potentials. The <span class="hlt">separation</span> mechanism is observed experimentally to depend on the applied field <span class="hlt">frequency</span> and voltage. At high <span class="hlt">frequencies</span>, particles position themselves in a manner that is consistent with dielectrophoresis, while at low <span class="hlt">frequencies</span>, the positioning is explained in terms of a strong coupling between gravity, the vertical component of the dielectrophoretic force, and the Stokes drag on particles induced by AC electroosmotic flow. Compared to high <span class="hlt">frequency</span> dielectrophoretic <span class="hlt">separations</span>, the low <span class="hlt">frequency</span> <span class="hlt">separations</span> are faster and require lower applied voltages. Furthermore, the AC electroosmosis coupling with dielectrophoresis may enable cell <span class="hlt">separations</span> that are not feasible based on dielectrophoresis alone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010PhDT.......269M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010PhDT.......269M"><span>Turbulent transition behavior in a <span class="hlt">separated</span> and attached-flow low pressure turbine passage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Memory, Curtis L.</p> <p></p> <p>Various time accurate numerical simulations were conducted on the aft-loaded L1A low pressure turbine airfoil operating at Reynolds numbers presenting with fully-stalled, non-reattaching laminar <span class="hlt">separation</span>. The numerical solver TURBO was modified from its annular gas turbine simulation configuration to conduct simulations based on a linear cascade wind tunnel facility. Simulation results for the fully <span class="hlt">separated</span> flow fields revealed various turbulent decay mechanisms. <span class="hlt">Separated</span> shear layer decay, in the form of vortices forming between the shear layer and the blade wall, was shown to agree with experimental particle image velocimetry (PIV) data in terms of decay vortex size and core vorticity levels. These vortical structures eventually mix into a large recirculation zone which dominates the blade wake. Turbulent wake ex- tent and time-averaged velocity distributions agreed with PIV data. Steady-blowing vortex generating jet (VGJ) flow control was then applied to the flow fields. VGJ-induced streamwise vorticity was only present at blowing ratios above 1.5. VGJs actuated at the point of flow <span class="hlt">separation</span> on the blade wall were more effective than those actuated downstream, within the <span class="hlt">separation</span> zone. Pulsed-blowing VGJs at the upstream blade wall position were then actuated at various pulsing <span class="hlt">frequencies</span>, duty cycles, and blowing ratios. These condition <span class="hlt">variations</span> yielded differing levels of <span class="hlt">separation</span> zone mitigation. Pulsed VGJs were shown to be more effective than steady blowing VGJs at conditions of high blowing ratio, high <span class="hlt">frequency</span>, or high duty cycle, where blowing ratio had the highest level of influence on pulsed jet efficacy. The characteristic "calm zone" following the end of a given VGJ pulse was observed in simulations exhibiting high levels of <span class="hlt">separation</span> zone mitigation. Numerical velocity fields near the blade wall during this calm zone was shown to be similar to velocity fields observed in PIV data. Instantaneous numerical vorticity fields indicated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22413033-modulating-action-low-frequency-oscillations-high-frequency-instabilities-hall-thrusters','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22413033-modulating-action-low-frequency-oscillations-high-frequency-instabilities-hall-thrusters"><span>Modulating action of low <span class="hlt">frequency</span> oscillations on high <span class="hlt">frequency</span> instabilities in Hall thrusters</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>Liqiu, Wei, E-mail: weiliqiu@gmail.com, E-mail: weiliqiu@hit.edu.cn; Liang, Han; Ziyi, Yang</p> <p>2015-02-07</p> <p>It is found that the low <span class="hlt">frequency</span> oscillations have modulating action on high <span class="hlt">frequency</span> 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 <span class="hlt">frequency</span> oscillations affect the electron drift velocity and anomalous electron transport across the magnetic field. The amplitude and <span class="hlt">frequency</span> of high <span class="hlt">frequency</span> oscillations are modulated by low <span class="hlt">frequency</span> oscillations, which show the periodic <span class="hlt">variation</span> in the time scale of low <span class="hlt">frequency</span> oscillations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982PhDT........90G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982PhDT........90G"><span>A Analysis of the Low <span class="hlt">Frequency</span> Sound Field in Non-Rectangular Enclosures Using the Finite Element Method.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geddes, Earl Russell</p> <p></p> <p>The details of the low <span class="hlt">frequency</span> sound field for a rectangular room can be studied by the use of an established analytic technique--<span class="hlt">separation</span> of variables. The solution is straightforward and the results are well-known. A non -rectangular room has boundary conditions which are not <span class="hlt">separable</span> and therefore other solution techniques must be used. This study shows that the finite element method can be adapted for use in the study of sound fields in arbitrary shaped enclosures. The finite element acoustics problem is formulated and the modification of a standard program, which is necessary for solving acoustic field problems, is examined. The solution of the semi-non-rectangular room problem (one where the floor and ceiling remain parallel) is carried out by a combined finite element/<span class="hlt">separation</span> of variables approach. The solution results are used to construct the Green's function for the low <span class="hlt">frequency</span> sound field in five rooms (or data cases): (1) a rectangular (Louden) room; (2) The smallest wall of the Louden room canted 20 degrees from normal; (3) The largest wall of the Louden room canted 20 degrees from normal; (4) both the largest and the smallest walls are canted 20 degrees; and (5) a five-sided room <span class="hlt">variation</span> of Case 4. Case 1, the rectangular room was calculated using both the finite element method and the <span class="hlt">separation</span> of variables technique. The results for the two methods are compared in order to access the accuracy of the finite element method models. The modal damping coefficient are calculated and the results examined. The statistics of the source and receiver average normalized RMS P('2) responses in the 80 Hz, 100 Hz, and 125 Hz one-third octave bands are developed. The receiver averaged pressure response is developed to determine the effect of the source locations on the response. Twelve source locations are examined and the results tabulated for comparison. The effect of a finite sized source is looked at briefly. Finally, the standard deviation of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24386006','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24386006"><span>Cardiorespiratory dynamic response to mental stress: a multivariate time-<span class="hlt">frequency</span> analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Widjaja, Devy; Orini, Michele; Vlemincx, Elke; Van Huffel, Sabine</p> <p>2013-01-01</p> <p>Mental stress is a growing problem in our society. In order to deal with this, it is important to understand the underlying stress mechanisms. In this study, we aim to determine how the cardiorespiratory interactions are affected by mental arithmetic stress and attention. We conduct cross time-<span class="hlt">frequency</span> (TF) analyses to assess the cardiorespiratory coupling. In addition, we introduce partial TF spectra to <span class="hlt">separate</span> <span class="hlt">variations</span> in the RR interval series that are linearly related to respiration from RR interval <span class="hlt">variations</span> (RRV) that are not related to respiration. The performance of partial spectra is evaluated in two simulation studies. Time-varying parameters, such as instantaneous powers and <span class="hlt">frequencies</span>, are derived from the computed spectra. Statistical analysis is carried out continuously in time to evaluate the dynamic response to mental stress and attention. The results show an increased heart and respiratory rate during stress and attention, compared to a resting condition. Also a fast reduction in vagal activity is noted. The partial TF analysis reveals a faster reduction of RRV power related to (3 s) than unrelated to (30 s) respiration, demonstrating that the autonomic response to mental stress is driven by mechanisms characterized by different temporal scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12822811','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12822811"><span><span class="hlt">Variation</span> in humpback whale (Megaptera novaeangliae) song length in relation to low-<span class="hlt">frequency</span> sound broadcasts.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fristrup, Kurt M; Hatch, Leila T; Clark, Christopher W</p> <p>2003-06-01</p> <p>Humpback whale song lengths were measured from recordings made off the west coast of the island of Hawai'i in March 1998 in relation to acoustic broadcasts ("pings") from the U.S. Navy SURTASS Low <span class="hlt">Frequency</span> Active sonar system. Generalized additive models were used to investigate the relationships between song length and time of year, time of day, and broadcast factors. There were significant seasonal and diurnal effects. The seasonal factor was associated with changes in the density of whales sighted near shore. The diurnal factor was associated with changes in surface social activity. Songs that ended within a few minutes of the most recent ping tended to be longer than songs sung during control periods. Many songs that were overlapped by pings, and songs that ended several minutes after the most recent ping, did not differ from songs sung in control periods. The longest songs were sung between 1 and 2 h after the last ping. Humpbacks responded to louder broadcasts with longer songs. The fraction of <span class="hlt">variation</span> in song length that could be attributed to broadcast factors was low. Much of the <span class="hlt">variation</span> in humpback song length remains unexplained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ASAJ..113.3411F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ASAJ..113.3411F"><span><span class="hlt">Variation</span> in humpback whale (Megaptera novaeangliae) song length in relation to low-<span class="hlt">frequency</span> sound broadcasts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fristrup, Kurt M.; Hatch, Leila T.; Clark, Christopher W.</p> <p>2003-06-01</p> <p>Humpback whale song lengths were measured from recordings made off the west coast of the island of Hawai'i in March 1998 in relation to acoustic broadcasts (``pings'') from the U.S. Navy SURTASS Low <span class="hlt">Frequency</span> Active sonar system. Generalized additive models were used to investigate the relationships between song length and time of year, time of day, and broadcast factors. There were significant seasonal and diurnal effects. The seasonal factor was associated with changes in the density of whales sighted near shore. The diurnal factor was associated with changes in surface social activity. Songs that ended within a few minutes of the most recent ping tended to be longer than songs sung during control periods. Many songs that were overlapped by pings, and songs that ended several minutes after the most recent ping, did not differ from songs sung in control periods. The longest songs were sung between 1 and 2 h after the last ping. Humpbacks responded to louder broadcasts with longer songs. The fraction of <span class="hlt">variation</span> in song length that could be attributed to broadcast factors was low. Much of the <span class="hlt">variation</span> in humpback song length remains unexplained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20015460-synthesis-amplitude-versus-offset-variations-ground-penetrating-radar-data','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20015460-synthesis-amplitude-versus-offset-variations-ground-penetrating-radar-data"><span>Synthesis of amplitude-versus-offset <span class="hlt">variations</span> in ground-penetrating radar data</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>Zeng, X.; McMechan, G.A.; Xu, T.</p> <p>2000-02-01</p> <p>To evaluate the importance of amplitude-versus-offset information in the interpretation of ground-penetrating radar (GPR) data, GPR reflections are synthesized as a function of antenna <span class="hlt">separation</span> using a 2.5-D Finite-difference solution of Maxwell's equations. The conductivity, the complex dielectric permittivity,and the complex magnetic permeability are varied systematically in nine suites of horizontally layered models. The source used is a horizontal transverse-electric dipole situated at the air-earth interface. Cole-Cole relaxation mechanisms define the <span class="hlt">frequency</span> dependence of the media. Reflection magnitudes and their <span class="hlt">variations</span> with antenna <span class="hlt">separation</span> differ substantially, depending on the contrast in electromagnetic properties that caused the reflection. The spectral charactermore » of the dielectric and magnetic relaxations produces only second-order <span class="hlt">variations</span> in reflection coefficients compared with those associated with contrasts in permittivity, conductivity, and permeability, so they may not be <span class="hlt">separable</span> even when they are detected. In typical earth materials, attenuation of propagating GPR waves is influenced most strongly by conductivity, followed by dielectric relaxation, followed by magnetic relaxation. A pervasive feature of the simulated responses is locally high amplitude associated with the critical incident angle at the air-earth interface in the antenna radiation pattern. Full wavefield simulations of two field data sets from a fluvial/eolian environment are able to reproduce the main amplitude behaviors observed in the data.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MSSP...96..303Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MSSP...96..303Y"><span>Noise source <span class="hlt">separation</span> of diesel engine by combining binaural sound localization method and blind source <span class="hlt">separation</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>Yao, Jiachi; Xiang, Yang; Qian, Sichong; Li, Shengyang; Wu, Shaowei</p> <p>2017-11-01</p> <p>In order to <span class="hlt">separate</span> and identify the combustion noise and the piston slap noise of a diesel engine, a noise source <span class="hlt">separation</span> and identification method that combines a binaural sound localization method and blind source <span class="hlt">separation</span> method is proposed. During a diesel engine noise and vibration test, because a diesel engine has many complex noise sources, a lead covering method was carried out on a diesel engine to isolate other interference noise from the No. 1-5 cylinders. Only the No. 6 cylinder parts were left bare. Two microphones that simulated the human ears were utilized to measure the radiated noise signals 1 m away from the diesel engine. First, a binaural sound localization method was adopted to <span class="hlt">separate</span> the noise sources that are in different places. Then, for noise sources that are in the same place, a blind source <span class="hlt">separation</span> method is utilized to further <span class="hlt">separate</span> and identify the noise sources. Finally, a coherence function method, continuous wavelet time-<span class="hlt">frequency</span> analysis method, and prior knowledge of the diesel engine are combined to further identify the <span class="hlt">separation</span> results. The results show that the proposed method can effectively <span class="hlt">separate</span> and identify the combustion noise and the piston slap noise of a diesel engine. The <span class="hlt">frequency</span> of the combustion noise and the piston slap noise are respectively concentrated at 4350 Hz and 1988 Hz. Compared with the blind source <span class="hlt">separation</span> method, the proposed method has superior <span class="hlt">separation</span> and identification effects, and the <span class="hlt">separation</span> results have fewer interference components from other noise.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhRvE..70c1915S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhRvE..70c1915S"><span>Double-wavelet approach to study <span class="hlt">frequency</span> and amplitude modulation in renal autoregulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sosnovtseva, O. V.; Pavlov, A. N.; Mosekilde, E.; Holstein-Rathlou, N.-H.; Marsh, D. J.</p> <p>2004-09-01</p> <p>Biological time series often display complex oscillations with several interacting rhythmic components. Renal autoregulation, for instance, involves at least two <span class="hlt">separate</span> mechanisms both of which can produce oscillatory <span class="hlt">variations</span> in the pressures and flows of the individual nephrons. Using double-wavelet analysis we propose a method to examine how the instantaneous <span class="hlt">frequency</span> and amplitude of a fast mode is modulated by the presence of a slower mode. Our method is applied both to experimental data from normotensive and hypertensive rats showing different oscillatory patterns and to simulation results obtained from a physiologically based model of the nephron pressure and flow control. We reveal a nonlinear interaction between the two mechanisms that regulate the renal blood flow in the form of <span class="hlt">frequency</span> and amplitude modulation of the myogenic oscillations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29227912','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29227912"><span>Annual <span class="hlt">variations</span> in sexual hormones and births' <span class="hlt">frequency</span> in female stump-tailed macaques (Macaca arctoides).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mondragón-Ceballos, R; García-Granados, M D; Matamoros-Trejo, G; Hernández-López, L E</p> <p>2018-03-01</p> <p>Although the breeding seasonality in Macaca arctoides have been studied over a long period of time, it is still controversial whether reproduction in this primate tend to increase during certain months of the year as it happens in most of the macaque species. Many authors have classified Macaca arctoides as not being seasonal species. Nonetheless, there were no reports, about seasonal <span class="hlt">variations</span> of female sexual hormones to demonstrate that asseveration. Therefore, in the present study we collect 1611 fecal samples from June 2009 to November 2010 from 10 female stump-tailed macaques to measure 17β-estradiol and progesterone concentrations. Also, we included the birth <span class="hlt">frequency</span> per year, in order to identify if sexual hormones peaked at a certain period of the year, thus, births would be occurring six months later according to the gestation length of stump-tailed macaques. Our results indicate two mating seasons per year in stump-tailed macaques: one in July-August and a second one in November. The distribution of the birth <span class="hlt">frequency</span>, throughout the year support these results. We conclude that stump-tail macaques have a discrete seasonality no different than most of macaques' species. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JLTP..191..153W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JLTP..191..153W"><span>Morphological Simulation of Phase <span class="hlt">Separation</span> Coupled Oscillation Shear and Varying Temperature Fields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Heping; Li, Xiaoguang; Lin, Kejun; Geng, Xingguo</p> <p>2018-05-01</p> <p>This paper explores the effect of the shear <span class="hlt">frequency</span> and Prandtl number ( Pr) on the procedure and pattern formation of phase <span class="hlt">separation</span> in symmetric and asymmetric systems. For the symmetric system, the periodic shear significantly prolongs the spinodal decomposition stage and enlarges the <span class="hlt">separated</span> domain in domain growth stage. By adjusting the Pr and shear <span class="hlt">frequency</span>, the number and orientation of <span class="hlt">separated</span> steady layer structures can be controlled during domain stretch stage. The numerical results indicate that the increase in Pr and decrease in the shear <span class="hlt">frequency</span> can significantly increase in the layer number of the lamellar structure, which relates to the decrease in domain size. Furthermore, the lamellar orientation parallel to the shear direction is altered into that perpendicular to the shear direction by further increasing the shear <span class="hlt">frequency</span>, and also similar results for larger systems. For asymmetric system, the quantitative analysis shows that the decrease in the shear <span class="hlt">frequency</span> enlarges the size of <span class="hlt">separated</span> minority phases. These numerical results provide guidance for setting the optimum condition for the phase <span class="hlt">separation</span> under periodic shear and slow cooling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Metro..55...11D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Metro..55...11D"><span>Study of the GPS inter-<span class="hlt">frequency</span> calibration of timing receivers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Defraigne, P.; Huang, W.; Bertrand, B.; Rovera, D.</p> <p>2018-02-01</p> <p>When calibrating Global Positioning System (GPS) stations dedicated to timing, the hardware delays of P1 and P2, the P(Y)-codes on <span class="hlt">frequencies</span> L1 and L2, are determined <span class="hlt">separately</span>. In the international atomic time (TAI) network the GPS stations of the time laboratories are calibrated relatively against reference stations. This paper aims at determining the consistency between the P1 and P2 hardware delays (called dP1 and dP2) of these reference stations, and to look at the stability of the inter-signal hardware delays dP1-dP2 of all the stations in the network. The method consists of determining the dP1-dP2 directly from the GPS pseudorange measurements corrected for the <span class="hlt">frequency</span>-dependent antenna phase center and the <span class="hlt">frequency</span>-dependent ionosphere corrections, and then to compare these computed dP1-dP2 to the calibrated values. Our results show that the differences between the computed and calibrated dP1-dP2 are well inside the expected combined uncertainty of the two quantities. Furthermore, the consistency between the calibrated time transfer solution obtained from either single-<span class="hlt">frequency</span> P1 or dual-<span class="hlt">frequency</span> P3 for reference laboratories is shown to be about 1.0 ns, well inside the 2.1 ns uB uncertainty of a time transfer link based on GPS P3 or Precise Point Positioning. This demonstrates the good consistency between the P1 and P2 hardware delays of the reference stations used for calibration in the TAI network. The long-term stability of the inter-signal hardware delays is also analysed from the computed dP1-dP2. It is shown that only <span class="hlt">variations</span> larger than 2 ns can be detected for a particular station, while <span class="hlt">variations</span> of 200 ps can be detected when differentiating the results between two stations. Finally, we also show that in the differential calibration process as used in the TAI network, using the same antenna phase center or using different positions for L1 and L2 signals gives maximum differences of 200 ps on the hardware delays of the <span class="hlt">separate</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT.........4I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT.........4I"><span>Towards Enhanced Underwater Lidar Detection via Source <span class="hlt">Separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Illig, David W.</p> <p></p> <p>Interest in underwater optical sensors has grown as technologies enabling autonomous underwater vehicles have been developed. Propagation of light through water is complicated by the dual challenges of absorption and scattering. While absorption can be reduced by operating in the blue-green region of the visible spectrum, reducing scattering is a more significant challenge. Collection of scattered light negatively impacts underwater optical ranging, imaging, and communications applications. This thesis concentrates on the ranging application, where scattering reduces operating range as well as range accuracy. The focus of this thesis is on the problem of backscatter, which can create a "clutter" return that may obscure submerged target(s) of interest. The main contributions of this thesis are explorations of signal processing approaches to increase the <span class="hlt">separation</span> between the target and backscatter returns. Increasing this <span class="hlt">separation</span> allows detection of weak targets in the presence of strong scatter, increasing both operating range and range accuracy. Simulation and experimental results will be presented for a variety of approaches as functions of water clarity and target position. This work provides several novel contributions to the underwater lidar field: 1. Quantification of temporal <span class="hlt">separation</span> approaches: While temporal <span class="hlt">separation</span> has been studied extensively, this work provides a quantitative assessment of the extent to which both high <span class="hlt">frequency</span> modulation and spatial filter approaches improve the <span class="hlt">separation</span> between target and backscatter. 2. Development and assessment of <span class="hlt">frequency</span> <span class="hlt">separation</span>: This work includes the first <span class="hlt">frequency</span>-based <span class="hlt">separation</span> approach for underwater lidar, in which the channel <span class="hlt">frequency</span> response is measured with a wideband waveform. Transforming to the time-domain gives a channel impulse response, in which target and backscatter returns may appear in unique range bins and thus be <span class="hlt">separated</span>. 3. Development and assessment of statistical</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 <span class="hlt">separation</span>, with <span class="hlt">separation</span> 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 scales, that is a principal feature of comparable closed <span class="hlt">separation</span> STBLIs. Rather, the prominent unsteady content is a mid-<span class="hlt">frequency</span> regime that develops in the <span class="hlt">separated</span> shear layer and scales weakly with the local <span class="hlt">separation</span> 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 <span class="hlt">separation</span>. 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('http://adsabs.harvard.edu/abs/2018JAESc.154..419P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAESc.154..419P"><span>Natural time analysis on the ultra-low <span class="hlt">frequency</span> magnetic field <span class="hlt">variations</span> prior to the 2016 Kumamoto (Japan) earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Potirakis, Stelios M.; Schekotov, Alexander; Asano, Tomokazu; Hayakawa, Masashi</p> <p>2018-04-01</p> <p>On 15 April 2016 a very strong and shallow earthquake (EQ) (MW = 7.0 , depth ∼ 10 km) occurred in Southwest Japan under the city of Kumamoto, while two very strong foreshocks (MW = 6.2 and MW = 6.0) preceded by about one day. The Kumamoto EQs being very catastrophic, have already attracted much attention among the scientific community in a quest for understanding the generation mechanism, as well as for reporting any preseismic anomalies in various observables and assessing the effectivity of the current early warning systems. In the present article we report precursory behavior of the ground-based observed ultra-low <span class="hlt">frequency</span> (ULF) magnetic field <span class="hlt">variations</span> before the Kumamoto EQs. By analyzing specific ULF magnetic field characteristics in terms of the recently introduced natural time (NT) analysis method, we identified that ULF magnetic field <span class="hlt">variations</span> presented critical features from 2 weeks up to 1 month before the Kumamoto EQs. Specifically, the ULF magnetic field characteristics Fh , Fz , Dh and δDep were analyzed. The first two represent <span class="hlt">variations</span> of the horizontal and vertical components of the geomagnetic field. The third and fourth characteristics correspond to the depression (decrease) and a relative depression of the horizontal magnetic field <span class="hlt">variations</span>, respectively. The latter depends on the degree of ionospheric disturbance. All of them were found to reach criticality before the Kumamoto EQs; however, in different time periods for each characteristic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998APS..DFD..JB02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998APS..DFD..JB02D"><span>Vortex Formation During Unsteady Boundary-Layer <span class="hlt">Separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, Debopam; Arakeri, Jaywant H.</p> <p>1998-11-01</p> <p>Unsteady laminar boundary-layer <span class="hlt">separation</span> is invariably accompanied by the formation of vortices. The aim of the present work is to study the vortex formation mechanism(s). An adverse pressure gradient causing a <span class="hlt">separation</span> can be decomposed into a spatial component ( spatial <span class="hlt">variation</span> of the velocity external to the boundary layer ) and a temporal component ( temporal <span class="hlt">variation</span> of the external velocity ). Experiments were conducted in a piston driven 2-D water channel, where the spatial component could be be contolled by geometry and the temporal component by the piston motion. We present results for three divergent channel geometries. The piston motion consists of three phases: constant acceleration from start, contant velocity, and constant deceleration to stop. Depending on the geometry and piston motion we observe different types of unsteady <span class="hlt">separation</span> and vortex formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDQ27003Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDQ27003Y"><span>Using resolvent analysis for the design of <span class="hlt">separation</span> control on a NACA 0012 airfoil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yeh, Chi-An; Taira, Kunihiko</p> <p>2017-11-01</p> <p>A combined effort based on large-eddy simulation and resolvent analysis on the <span class="hlt">separated</span> flow over a NACA 0012 airfoil is conducted to design active flow control for suppression of <span class="hlt">separation</span>. This study considers the the airfoil at 6 deg. angle-of-attack and Reynolds number of 23000. The response mode obtained from the resolvent analysis about the baseline turbulent mean flow reveals modal structures that can be categorized into three families when sweeping through the resonant <span class="hlt">frequency</span>: (1) von Karman wake structure for low <span class="hlt">frequency</span>; (2) Kelvin-Helmholtz structure in the <span class="hlt">separation</span> bubble for high <span class="hlt">frequency</span>; (3) blended structure of (1) and (2) for the intermediate <span class="hlt">frequency</span>. Leveraging the insights from resolvent analysis, unsteady thermal actuation is introduced to the flow near the leading-edge to examine the use of the <span class="hlt">frequencies</span> from three families for <span class="hlt">separation</span> control in LES. As indicated by the resolvent response modes, we find that the use of intermediate <span class="hlt">frequencies</span> are most effective in suppressing the flow <span class="hlt">separation</span>, since the shear layer over the <span class="hlt">separation</span> bubble and the wake are both receptive to the perturbation at the these <span class="hlt">frequencies</span>. The resolvent-analysis-based control strategy achieves 35% drag reduction and 9% lift increase with effective <span class="hlt">frequency</span>. This work was supported by Office of Naval Research (N00014-15-R-FO13) and Army Research Office (W911NF-14-1-0224).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25831332','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25831332"><span><span class="hlt">Frequency</span>-agile dual-<span class="hlt">frequency</span> lidar for integrated coherent radar-lidar architectures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vercesi, Valeria; Onori, Daniel; Laghezza, Francesco; Scotti, Filippo; Bogoni, Antonella; Scaffardi, Mirco</p> <p>2015-04-01</p> <p>We propose a novel architecture for implementing a dual-<span class="hlt">frequency</span> lidar (DFL) exploiting differential Doppler shift measurement. The two <span class="hlt">frequency</span> tones, needed for target velocity measurements, are selected from the spectrum of a mode-locked laser operating in the C-band. The tones' <span class="hlt">separation</span> is easily controlled by using a programmable wavelength selective switch, thus allowing for a dynamic trade-off among robustness to atmospheric turbulence and sensitivity. Speed measurements for different tone <span class="hlt">separations</span> equal to 10, 40, 80, and 160 GHz are demonstrated, proving the system's capability of working in different configurations. Thanks to the acquisition system based on an analog-to-digital converter and digital-signal processing, real-time velocity measurements are demonstrated. The MLL-based proposed architecture enables the integration of the DFL with a photonic-based radar that exploits the same laser for generating and receiving radio-<span class="hlt">frequency</span> signal with high performance, thus allowing for simultaneous or complementary target observations by exploiting the advantages of both radar and lidar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PlST...20e4016Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PlST...20e4016Y"><span>Characterization and comprehension of corona partial discharge in air under power <span class="hlt">frequency</span> to very low <span class="hlt">frequency</span> voltage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yuanxiang, ZHOU; Zhongliu, ZHOU; Ling, ZHANG; Yunxiao, ZHANG; Yajun, MO; Jiantao, SUN</p> <p>2018-05-01</p> <p>For the partial discharge test of electrical equipment with large capacitance, the use of low-<span class="hlt">frequency</span> voltage instead of power <span class="hlt">frequency</span> voltage can effectively reduce the capacity requirements of test power supply. However, the validity of PD test under low <span class="hlt">frequency</span> voltage needs to be evaluated. In order to investigate the influence of voltage <span class="hlt">frequency</span> on corona discharge in the air, the discharge test of the tip-plate electrode under the <span class="hlt">frequency</span> from 50 to 0.1 Hz is carried out based on the impulse current method. The results show that some of the main features of corona under low <span class="hlt">frequency</span> do not change. The magnitude of discharge in a positive half cycle is obviously larger than that in a negative cycle. The magnitude of discharge and interval in positive cycle are random, while that in negative cycle are regular. With the decrease of <span class="hlt">frequency</span>, the inception voltage increases. The <span class="hlt">variation</span> trend of maximum and average magnitude and repetition rate of the discharge in positive and negative half cycle with the <span class="hlt">variation</span> of voltage <span class="hlt">frequency</span> and magnitude is demonstrated, with discussion and interpretation from the aspects of space charge transportation, effective discharge time and transition of discharge modes. There is an obvious difference in the phase resolved pattern of partial discharge and characteristic parameters of discharge patterns between power and low <span class="hlt">frequency</span>. The experimental results can be the reference for mode identification of partial discharge under low <span class="hlt">frequency</span> tests. The trend of the measured parameters with the <span class="hlt">variation</span> of <span class="hlt">frequency</span> provides more information about the insulation defect than traditional measurements under a single <span class="hlt">frequency</span> (usually 50 Hz). Also it helps to understand the mechanism of corona discharge with an explanation of the characteristics under different <span class="hlt">frequencies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OSJ....53....1C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OSJ....53....1C"><span>Interannual <span class="hlt">Variation</span> of Surface Circulation in the Japan/East Sea due to External Forcings and Intrinsic Variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choi, Byoung-Ju; Cho, Seong Hun; Jung, Hee Seok; Lee, Sang-Ho; Byun, Do-Seong; Kwon, Kyungman</p> <p>2018-03-01</p> <p>The interannual <span class="hlt">variation</span> of surface ocean currents can be as large as seasonal <span class="hlt">variation</span> in the Japan/East Sea (JES). To identify the major factors that cause such interannual variability of surface ocean circulation in the JES, surface circulation was simulated from 1998 to 2009 using a three-dimensional model. Contributions of atmospheric forcing (ATM), open boundary data (OBC), and intrinsic variability (ITV) of the surface flow in the JES on the interannual variability of surface ocean circulation were <span class="hlt">separately</span> examined using numerical simulations. Variability in surface circulation was quantified in terms of variance in sea surface height, 100-m depth water temperature, and surface currents. ITV was found to be the dominant factor that induced interannual variabilities of surface circulation, the main path of the East Korea Warm Current (EKWC), and surface kinetic energy on a time scale of 2-4 years. OBC and ATM were secondary factors contributing to the interannual <span class="hlt">variation</span> of surface circulation. Interannual <span class="hlt">variation</span> of ATM changed the <span class="hlt">separation</span> latitude of EKWC and increased the variability of surface circulation in the Ulleung Basin. Interannual <span class="hlt">variation</span> of OBC enhanced low-<span class="hlt">frequency</span> changes in surface circulation and eddies in the Yamato Basin. It also modulated basin-wide uniform oscillations of sea level. This study suggests that precise estimation of initial conditions using data assimilation is essential for long-term prediction of surface circulation in the JES.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21732149','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21732149"><span>[Correlation of pure tone thresholds and hearing loss for numbers. Comparison of three calculation <span class="hlt">variations</span> for plausibility checking in expertise].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Braun, T; Dochtermann, S; Krause, E; Schmidt, M; Schorn, K; Hempel, J M</p> <p>2011-09-01</p> <p>The present study analyzes the best combination of <span class="hlt">frequencies</span> for the calculation of mean hearing loss in pure tone threshold audiometry for correlation with hearing loss for numbers in speech audiometry, since the literature describes different calculation <span class="hlt">variations</span> for plausibility checking in expertise. Three calculation <span class="hlt">variations</span>, A (250, 500 and 1000 Hz), B (500 and 1000 Hz) and C (500, 1000 and 2000 Hz), were compared. Audiograms in 80 patients with normal hearing, 106 patients with hearing loss and 135 expertise patients were analyzed in a retrospective manner. Differences between mean pure tone audiometry thresholds and hearing loss for numbers were calculated and statistically compared <span class="hlt">separately</span> for the right and the left ear in the three patient collectives. We found the calculation <span class="hlt">variation</span> A to be the best combination of <span class="hlt">frequencies</span>, since it yielded the smallest standard deviations while being statistically different to calculation <span class="hlt">variations</span> B and C. The 1- and 2.58-fold standard deviation (representing 68.3% and 99.0% of all values) was ±4.6 and ±11.8 dB for calculation <span class="hlt">variation</span> A in patients with hearing loss, respectively. For plausibility checking in expertise, the mean threshold from the <span class="hlt">frequencies</span> 250, 500 and 1000 Hz should be compared to the hearing loss for numbers. The common recommendation reported by the literature to doubt plausibility when the difference of these values exceeds ±5 dB is too strict as shown by this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3246290','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3246290"><span>Partial differential equation transform — <span class="hlt">Variational</span> formulation and Fourier analysis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Yang; Wei, Guo-Wei; Yang, Siyang</p> <p>2011-01-01</p> <p>Nonlinear partial differential equation (PDE) models are established approaches for image/signal processing, data analysis and surface construction. Most previous geometric PDEs are utilized as low-pass filters which give rise to image trend information. In an earlier work, we introduced mode decomposition evolution equations (MoDEEs), which behave like high-pass filters and are able to systematically provide intrinsic mode functions (IMFs) of signals and images. Due to their tunable time-<span class="hlt">frequency</span> localization and perfect reconstruction, the operation of MoDEEs is called a PDE transform. By appropriate selection of PDE transform parameters, we can tune IMFs into trends, edges, textures, noise etc., which can be further utilized in the secondary processing for various purposes. This work introduces the <span class="hlt">variational</span> formulation, performs the Fourier analysis, and conducts biomedical and biological applications of the proposed PDE transform. The <span class="hlt">variational</span> formulation offers an algorithm to incorporate two image functions and two sets of low-pass PDE operators in the total energy functional. Two low-pass PDE operators have different signs, leading to energy disparity, while a coupling term, acting as a relative fidelity of two image functions, is introduced to reduce the disparity of two energy components. We construct <span class="hlt">variational</span> PDE transforms by using Euler-Lagrange equation and artificial time propagation. Fourier analysis of a simplified PDE transform is presented to shed light on the filter properties of high order PDE transforms. Such an analysis also offers insight on the parameter selection of the PDE transform. The proposed PDE transform algorithm is validated by numerous benchmark tests. In one selected challenging example, we illustrate the ability of PDE transform to <span class="hlt">separate</span> two adjacent <span class="hlt">frequencies</span> of sin(x) and sin(1.1x). Such an ability is due to PDE transform’s controllable <span class="hlt">frequency</span> localization obtained by adjusting the order of PDEs. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4116343','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/4116343"><span>AUTOMATIC <span class="hlt">FREQUENCY</span> CONTROL SYSTEM</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Hansen, C.F.; Salisbury, J.D.</p> <p>1961-01-10</p> <p>A control is described for automatically matching the <span class="hlt">frequency</span> of a resonant cavity to that of a driving oscillator. The driving oscillator is disconnected from the cavity and a secondary oscillator is actuated in which the cavity is the <span class="hlt">frequency</span> determining element. A low <span class="hlt">frequency</span> is mixed with the output of the driving oscillator and the resultant lower and upper sidebands are <span class="hlt">separately</span> derived. The <span class="hlt">frequencies</span> of the sidebands are compared with the secondary oscillator <span class="hlt">frequency</span>. deriving a servo control signal to adjust a tuning element in the cavity and matching the cavity <span class="hlt">frequency</span> to that of the driving oscillator. The driving oscillator may then be connected to the cavity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...613A..70S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...613A..70S"><span>Study of a sample of faint Be stars in the exofield of CoRoT. II. Pulsation and outburst events: Time series analysis of photometric <span class="hlt">variations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Semaan, T.; Hubert, A. M.; Zorec, J.; Gutiérrez-Soto, J.; Frémat, Y.; Martayan, C.; Fabregat, J.; Eggenberger, P.</p> <p>2018-06-01</p> <p>Context. The class of Be stars are the epitome of rapid rotators in the main sequence. These stars are privileged candidates for studying the incidence of rotation on the stellar internal structure and on non-radial pulsations. Pulsations are considered possible mechanisms to trigger mass-ejection phenomena required to build up the circumstellar disks of Be stars. Aims: Time series analyses of the light curves of 15 faint Be stars observed with the CoRoT satellite were performed to obtain the distribution of non-radial pulsation (NRP) <span class="hlt">frequencies</span> in their power spectra at epochs with and without light outbursts and to discriminate pulsations from rotation-related photometric <span class="hlt">variations</span>. Methods: Standard Fourier techniques were employed to analyze the CoRoT light curves. Fundamental parameters corrected for rapid-rotation effects were used to study the power spectrum as a function of the stellar location in the instability domains of the Hertzsprung-Russell (H-R) diagram. Results: <span class="hlt">Frequencies</span> are concentrated in <span class="hlt">separate</span> groups as predicted for g-modes in rapid B-type rotators, except for the two stars that are outside the H-R instability domain. In five objects the <span class="hlt">variations</span> in the power spectrum are correlated with the time-dependent outbursts characteristics. Time-<span class="hlt">frequency</span> analysis showed that during the outbursts the amplitudes of stable main <span class="hlt">frequencies</span> within 0.03 c d-1 intervals strongly change, while transients and/or <span class="hlt">frequencies</span> of low amplitude appear <span class="hlt">separated</span> or not <span class="hlt">separated</span> from the stellar <span class="hlt">frequencies</span>. The <span class="hlt">frequency</span> patterns and activities depend on evolution phases: (i) the average <span class="hlt">separations</span> between groups of <span class="hlt">frequencies</span> are larger in the zero-age main sequence (ZAMS) than in the terminal age main sequence (TAMS) and are the largest in the middle of the MS phase; (ii) a poor <span class="hlt">frequency</span> spectrum with f ≲ 1 cd-1 of low amplitude characterizes the stars beyond the TAMS; and (iii) outbursts are seen in stars hotter than B4 spectral type and in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20436544','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20436544"><span><span class="hlt">Frequency</span> and seasonal <span class="hlt">variation</span> of ophthalmology-related internet searches.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Leffler, Christopher T; Davenport, Byrd; Chan, Dana</p> <p>2010-06-01</p> <p>To use internet search activity to reveal the intensity of public interest and seasonal <span class="hlt">variation</span> in ophthalmology-related diseases, symptoms, and treatments. Time-series analysis of internet search data. Google trend data for ophthalmology terms for the United States, the United Kingdom, Canada, and Australia from 2004 through 2008 were studied. Mean population-weighted temperature and fraction of schools in session were estimated from databases, and relative potential sunlight intensity was calculated. Multivariable linear regression was used to predict search term <span class="hlt">frequency</span> based on environmental variables. Relative to diabetes searches (100%), common US eye-related searches were: "glasses" (44%), "Lasik" (16%), "contact lenses" (12.4%), "pink eye" (9.5%), "glaucoma" (5.9%), "cataract" (4.1%), "dry eyes" (2.1%), "eye twitching" (1.9%), and "eye pain" (1.9%). Seasonal nature was high for "conjunctivitis" (r(2) = 0.37), "pink eye" (r(2) = 0.32), "eye floaters" (r2 = 0.26), and "stye" (r(2) = 0.19), moderate for "glaucoma" (r(2) = 0.09) and "eye twitching" (r(2) = 0.06), and low for "uveitis" (r(2) = 0.02) and "macular degeneration" (r(2) < 0.01). Heat was associated with "stye" and cold was associated with "pink eye," "conjunctivitis," and "glaucoma" (all p < 0.002). Sunlight intensity was associated with "dry eyes" and "eye floaters" (p < 0.01). School sessions were associated positively with "eye twitching" (p >= 0.001) and negatively with "eyeglasses." "Eye allergy," "itchy eyes," and "watery eyes" were highly seasonal (r(2) = 0.75-0.38) and associated with "pollen" searches. Internet ophthalmology searches relate (in decreasing order) to refractive correction, eye diseases, and eye symptoms. Search study reveals the seasonality and environmental associations of interest in health terms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.4484B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.4484B"><span>Microscopic Electron <span class="hlt">Variations</span> Measured Simultaneously By The Cluster Spacecraft</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buckley, A. M.; Carozzi, T. D.; Gough, M. P.; Beloff, N.</p> <p></p> <p>Data is used from the Particle Correlator experiments running on each of the four Cluster spacecraft so as to determine common microscopic behaviour in the elec- tron population observed over the macroscopic Cluster <span class="hlt">separations</span>. The Cluster par- ticle correlator experiments operate by forming on board Auto Correlation Functions (ACFs) generated from short time series of electron counts obtained, as a function of electron energy, from the PEACE HEEA sensor. The information on the microscopic <span class="hlt">variation</span> of the electron flux covers the <span class="hlt">frequency</span> range DC up to 41 kHz (encom- passing typical electron plasma <span class="hlt">frequencies</span> and electron gyro <span class="hlt">frequencies</span> and their harmonics), the electron energy range is that covered by the PEACE HEEA sensor (within the range 1 eV to 26 keV). Results are presented of coherent electron struc- tures observed simultaneously by the four spacecraft in the differing plasma interac- tion regions and boundaries encountered by Cluster. As an aid to understanding the plasma interactions, use is made of numerical simulations which model both the un- derlying statistical properties of the electrons and also the manner in which particle correlator experiments operate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000025187&hterms=Reynolds+numbers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DReynolds%2Bnumbers','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000025187&hterms=Reynolds+numbers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DReynolds%2Bnumbers"><span>Dynamics of Active <span class="hlt">Separation</span> Control at High Reynolds Numbers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pack, LaTunia G.; Seifert, Avi</p> <p>2000-01-01</p> <p>A series of active flow control experiments were recently conducted at high Reynolds numbers on a generic <span class="hlt">separated</span> configuration. The model simulates the upper surface of a 20% thick Glauert-Goldschmied type airfoil at zero angle of attack. The flow is fully turbulent since the tunnel sidewall boundary layer flows over the model. The main motivation for the experiments is to generate a comprehensive data base for validation of unsteady numerical simulation as a first step in the development of a CFD design tool, without which it would not be possible to effectively utilize the great potential of unsteady flow control. This paper focuses on the dynamics of several key features of the baseline as well as the controlled flow. It was found that the thickness of the upstream boundary layer has a negligible effect on the flow dynamics. It is speculated that <span class="hlt">separation</span> is caused mainly by the highly convex surface while viscous effects are less important. The two-dimensional <span class="hlt">separated</span> flow contains unsteady waves centered on a reduced <span class="hlt">frequency</span> of 0.9, while in the three dimensional <span class="hlt">separated</span> flow, <span class="hlt">frequencies</span> around a reduced <span class="hlt">frequency</span> of 0.3 and 1 are active. Several scenarios of resonant wave interaction take place at the <span class="hlt">separated</span> shear-layer and in the pressure recovery region. The unstable reduced <span class="hlt">frequency</span> bands for periodic excitation are centered on 1.5 and 5, but these reduced <span class="hlt">frequencies</span> are based on the length of the baseline bubble that shortens due to the excitation. The conventional works well for the coherent wave features. Reproduction of these dynamic effects by a numerical simulation would provide benchmark validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000021448','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000021448"><span>Dynamics of Active <span class="hlt">Separation</span> Control at High Reynolds Numbers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pack, LaTunia G.; Seifert, Avi</p> <p>2000-01-01</p> <p>A series of active flow control experiments were recently conducted at high Reynolds numbers on a generic <span class="hlt">separated</span> configuration. The model simulates the upper surface of a 20% thick Glauert-Goldschmied type airfoil at zero angle of attack. The flow is fully turbulent since the tunnel sidewall boundary layer flows over the model. The main motivation for the experiments is to generate a comprehensive data base for validation of unsteady numerical simulation as a first step in the development of a CFD design tool, without which it would not be possible to effectively utilize the great potential of unsteady flow control. This paper focuses on the dynamics of several key features of the baseline as well as the controlled flow. It was found that the thickness of the upstream boundary layer has a negligible effect on the flow dynamics. It is speculated that <span class="hlt">separation</span> is caused mainly by the highly convex surface while viscous effects are less important. The two-dimensional <span class="hlt">separated</span> flow contains unsteady waves centered on a reduced <span class="hlt">frequency</span> of 0.8, while in the three dimensional <span class="hlt">separated</span> flow, <span class="hlt">frequencies</span> around a reduced <span class="hlt">frequency</span> of 0.3 and 1 are active. Several scenarios of resonant wave interaction take place at the <span class="hlt">separated</span> shear-layer and in the pressure recovery region. The unstable reduced <span class="hlt">frequency</span> bands for periodic excitation are centered on 1.5 and 5, but these reduced <span class="hlt">frequencies</span> are based on the length of the baseline bubble that shortens due to the excitation. The conventional swept wing-scaling works well for the coherent wave features. Reproduction of these dynamic effects by a numerical simulation would provide benchmark validation.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22492970-multi-frequency-inversion-charge-pumping-charge-separation-mobility-analysis-high-ingaas-metal-oxide-semiconductor-field-effect-transistors','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22492970-multi-frequency-inversion-charge-pumping-charge-separation-mobility-analysis-high-ingaas-metal-oxide-semiconductor-field-effect-transistors"><span>Multi-<span class="hlt">frequency</span> inversion-charge pumping for charge <span class="hlt">separation</span> and mobility analysis in high-k/InGaAs metal-oxide-semiconductor field-effect transistors</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>Djara, V.; Cherkaoui, K.; Negara, M. A.</p> <p>2015-11-28</p> <p>An alternative multi-<span class="hlt">frequency</span> inversion-charge pumping (MFICP) technique was developed to directly <span class="hlt">separate</span> the inversion charge density (N{sub inv}) from the trapped charge density in high-k/InGaAs metal-oxide-semiconductor field-effect transistors (MOSFETs). This approach relies on the fitting of the <span class="hlt">frequency</span> response of border traps, obtained from inversion-charge pumping measurements performed over a wide range of <span class="hlt">frequencies</span> at room temperature on a single MOSFET, using a modified charge trapping model. The obtained model yielded the capture time constant and density of border traps located at energy levels aligned with the InGaAs conduction band. Moreover, the combination of MFICP and pulsed I{sub d}-V{sub g}more » measurements enabled an accurate effective mobility vs N{sub inv} extraction and analysis. The data obtained using the MFICP approach are consistent with the most recent reports on high-k/InGaAs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770000169&hterms=Separation+Techniques&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DSeparation%2BTechniques','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770000169&hterms=Separation+Techniques&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DSeparation%2BTechniques"><span>Radioactive-gas <span class="hlt">separation</span> technique</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Haney, R.; King, K. J.; Nellis, D. O.; Nisson, R. S.; Robling, P.; Womack, W.</p> <p>1977-01-01</p> <p>Cryogenic technique recovers gases inexpensively. Method uses differences in vapor pressures, melting points, and boiling points of components in gaseous mixture. Series of temperature and pressure <span class="hlt">variations</span> converts gases independently to solid and liquid states, thereby simplifying <span class="hlt">separation</span>. Apparatus uses readily available cryogen and does not require expensive refrigeration equipment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PASP..129k5001R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PASP..129k5001R"><span>Multiple Spatial <span class="hlt">Frequencies</span> Pyramid WaveFront Sensing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ragazzoni, Roberto; Vassallo, Daniele; Dima, Marco; Portaluri, Elisa; Bergomi, Maria; Greggio, Davide; Viotto, Valentina; Gullieuszik, Marco; Biondi, Federico; Carolo, Elena; Chinellato, Simonetta; Farinato, Jacopo; Magrin, Demetrio; Marafatto, Luca</p> <p>2017-11-01</p> <p>A modification of the pyramid wavefront sensor is described. In this conceptually new class of devices, the perturbations are split at the level of the focal plane depending upon their spatial <span class="hlt">frequencies</span>, and then measured <span class="hlt">separately</span>. The aim of this approach is to increase the accuracy in the determination of some range of spatial <span class="hlt">frequency</span> perturbations, or a certain classes of modes, disentangling them from the noise associated to the Poissonian fluctuations of the light coming from the perturbations outside of the range of interest or from the background in the pupil planes; the latter case specifically when the pyramid wavefront sensor is used with a large modulation. While the limits and the effectiveness of this approach should be further investigated, a number of <span class="hlt">variations</span> on the concept are shown, including a generalization of the spatial filtering in the point-diffraction wavefront sensor. The simplest application, a generalization to the pyramid of the well-known spatially filtering in wavefront sensing, is showing promise as a significant limiting magnitude advance. Applications are further speculated in the area of extreme adaptive optics and when serving spectroscopic instrumentation where “light in the bucket” rather than Strehl performance is required.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050182046','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050182046"><span>Unsteady Aerodynamic Response of a Linear Cascade of Airfoils in <span class="hlt">Separated</span> Flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Capece, Vincent R.; Ford, Christopher; Bone, Christopher; Li, Rui</p> <p>2004-01-01</p> <p>The overall objective of this research program was to investigate methods to modify the leading edge <span class="hlt">separation</span> region, which could lead to an improvement in aeroelastic stability of advanced airfoil designs. The airfoil section used is representative of current low aspect ratio fan blade tip sections. The experimental potion of this study investigated <span class="hlt">separated</span> zone boundary layer from removal through suction slots. Suction applied to a cavity in the vicinity of the <span class="hlt">separation</span> onset point was found to be the most effective location. The computational study looked into the influence of front camber on flutter stability. To assess the influence of the change in airfoil shape on stability the work-per-cycle was evaluated for torsion mode oscillations. It was shown that the front camberline shape can be an important factor for stabilizing the predicted work-per-cycle and reducing the predicted extent of the <span class="hlt">separation</span> zone. In addition, data analysis procedures are discussed for reducing data acquired in experiments that involve periodic unsteady data. This work was conducted in support of experiments being conducted in the NASA Glenn Research Center Transonic Flutter Cascade. The spectral block averaging method is presented. This method is shown to be able to account for <span class="hlt">variations</span> in airfoil oscillation <span class="hlt">frequency</span> that can occur in experiments that force oscillate the airfoils to simulate flutter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1708C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1708C"><span>Steepest Ascent Low/Non-Low-<span class="hlt">Frequency</span> Ratio in Empirical Mode Decomposition to <span class="hlt">Separate</span> Deterministic and Stochastic Velocities From a Single Lagrangian Drifter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chu, Peter C.</p> <p>2018-03-01</p> <p>SOund Fixing And Ranging (RAFOS) floats deployed by the Naval Postgraduate School (NPS) in the California Current system from 1992 to 2001 at depth between 150 and 600 m (http://www.oc.nps.edu/npsRAFOS/) are used to study 2-D turbulent characteristics. Each drifter trajectory is adaptively decomposed using the empirical mode decomposition (EMD) into a series of intrinsic mode functions (IMFs) with corresponding specific scale for each IMF. A new steepest ascent low/non-low-<span class="hlt">frequency</span> ratio is proposed in this paper to <span class="hlt">separate</span> a Lagrangian trajectory into low-<span class="hlt">frequency</span> (nondiffusive, i.e., deterministic) and high-<span class="hlt">frequency</span> (diffusive, i.e., stochastic) components. The 2-D turbulent (or called eddy) diffusion coefficients are calculated on the base of the classical turbulent diffusion with mixing length theory from stochastic component of a single drifter. Statistical characteristics of the calculated 2-D turbulence length scale, strength, and diffusion coefficients from the NPS RAFOS data are presented with the mean values (over the whole drifters) of the 2-D diffusion coefficients comparable to the commonly used diffusivity tensor method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013A%26A...549A.104L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013A%26A...549A.104L"><span>Low-<span class="hlt">frequency</span> <span class="hlt">variations</span> of unknown origin in the Kepler δ Scuti star KIC 5988140 = HD 188774</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lampens, P.; Tkachenko, A.; Lehmann, H.; Debosscher, J.; Aerts, C.; Beck, P. G.; Bloemen, S.; Kochiashvili, N.; Derekas, A.; Smith, J. C.; Tenenbaum, P.; Twicken, J. D.</p> <p>2013-01-01</p> <p>Context. The NASA exoplanet search mission Kepler is currently providing a wealth of light curves of ultra-high quality from space. Aims: We used high-quality Kepler photometry and spectroscopic data to investigate the Kepler target and binary candidate KIC 5988140. We aim to interpret the observed <span class="hlt">variations</span> of KIC 5988140 considering three possible scenarios: binarity, co-existence of δ Sct- and γ Dor-type oscillations, and rotational modulation caused by an asymmetric surface intensity distribution. Methods: We used the spectrum synthesis method to derive the fundamental parameters Teff, log g, [M/H], and v sin i from the newly obtained high-resolution, high S/N spectra. <span class="hlt">Frequency</span> analyses of both the photometric and the spectroscopic data were performed. Results: The star has a spectral type of A7.5 IV-III and a metallicity slightly lower than that of the Sun. Both Fourier analyses reveal the same two dominant <span class="hlt">frequencies</span> F1 = 2F2 = 0.688 and F2 = 0.344 d-1. We also detected in the photometry the signal of nine more, significant <span class="hlt">frequencies</span> located in the typical range of δ Sct pulsation. The light and radial velocity curves follow a similar, stable double-wave pattern which are not exactly in anti-phase but show a relative phase shift of about 0.1 period between the moment of minimum velocity and that of maximum light. Conclusions: Such findings are incompatible with the star being a binary system. We next show that, for all possible (limit) configurations of a spotted surface, the predicted light-to-velocity amplitude ratio is almost two orders larger than the observed value, which pleads against rotational modulation. The same argument also invalidates the explanation in terms of pulsations of type γ Dor (i.e. hybrid pulsations). We confirm the occurrence of various independent δ Sct-type pressure modes in the Kepler light curve. With respect to the low-<span class="hlt">frequency</span> content, however, we argue that the physical cause of the remaining light and radial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4314442','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4314442"><span>The Tracking Study: Description of a randomized controlled trial of <span class="hlt">variations</span> on weight tracking <span class="hlt">frequency</span> in a behavioral weight loss program</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Linde, Jennifer A.; Jeffery, Robert W.; Crow, Scott J.; Brelje, Kerrin L.; Pacanowski, Carly R.; Gavin, Kara L.; Smolenski, Derek J.</p> <p>2014-01-01</p> <p>Observational evidence from behavioral weight control trials and community studies suggests that greater <span class="hlt">frequency</span> of weighing oneself, or tracking weight, is associated with better weight outcomes. Conversely, it has also been suggested that frequent weight tracking may have a negative impact on mental health and outcomes during weight loss, but there are minimal experimental data that address this concern in the context of an active weight loss program. To achieve the long-term goal of strengthening behavioral weight loss programs, the purpose of this randomized controlled trial (the Tracking Study) is to test <span class="hlt">variations</span> on <span class="hlt">frequency</span> of self-weighing during a behavioral weight loss program, and to examine psychosocial and mental health correlates of weight tracking and weight loss outcomes. Three hundred thirty-nine overweight and obese adults were recruited and randomized to one of three <span class="hlt">variations</span> on weight tracking <span class="hlt">frequency</span> during a 12-month weight loss program with a 12-month follow-up: daily weight tracking, weekly weight tracking, or no weight tracking. The primary outcome is weight in kilograms at 24 months. The weight loss program integrates each weight tracking instruction with standard behavioral weight loss techniques (goal setting, self-monitoring, stimulus control, dietary and physical activity enhancements, lifestyle modifications); participants in weight tracking conditions were provided with wireless Internet technology (Wi-Fi-enabled digital scales and touchscreen personal devices) to facilitate weight tracking during the study. This paper describes the study design, intervention features, recruitment, and baseline characteristics of participants enrolled in the Tracking Study. PMID:25533727</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24111326','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24111326"><span>A <span class="hlt">frequency</span> domain analysis of respiratory <span class="hlt">variations</span> in the seismocardiogram signal.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pandia, Keya; Inan, Omer T; Kovacs, Gregory T A</p> <p>2013-01-01</p> <p>The seismocardiogram (SCG) signal traditionally measured using a chest-mounted accelerometer contains low-<span class="hlt">frequency</span> (0-100 Hz) cardiac vibrations that can be used to derive diagnostically relevant information about cardiovascular and cardiopulmonary health. This work is aimed at investigating the effects of respiration on the <span class="hlt">frequency</span> domain characteristics of SCG signals measured from 18 healthy subjects. Toward this end, the 0-100 Hz SCG signal bandwidth of interest was sub-divided into 5 Hz and 10 Hz <span class="hlt">frequency</span> bins to compare the spectral energy in corresponding <span class="hlt">frequency</span> bins of the SCG signal measured during three key conditions of respiration--inspiration, expiration, and apnea. Statistically significant differences were observed between the power in ensemble averaged inspiratory and expiratory SCG beats and between ensemble averaged inspiratory and apneaic beats across the 18 subjects for multiple <span class="hlt">frequency</span> bins in the 10-40 Hz <span class="hlt">frequency</span> range. Accordingly, the spectral analysis methods described in this paper could provide complementary and improved classification of respiratory modulations in the SCG signal over and above time-domain SCG analysis methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27781469','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27781469"><span><span class="hlt">Frequency</span> spirals.</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>2016-09-01</p> <p>We study the dynamics of coupled phase oscillators on a two-dimensional Kuramoto lattice with periodic boundary conditions. For coupling strengths just below the transition to global phase-locking, we find localized spatiotemporal patterns that we call "<span class="hlt">frequency</span> spirals." These patterns cannot be seen under time averaging; they become visible only when we examine the spatial <span class="hlt">variation</span> of the oscillators' instantaneous <span class="hlt">frequencies</span>, where they manifest themselves as two-armed rotating spirals. In the more familiar phase representation, they appear as wobbly periodic patterns surrounding a phase vortex. Unlike the stationary phase vortices seen in magnetic spin systems, or the rotating spiral waves seen in reaction-diffusion systems, <span class="hlt">frequency</span> spirals librate: the phases of the oscillators surrounding the central vortex move forward and then backward, executing a periodic motion with zero winding number. We construct the simplest <span class="hlt">frequency</span> spiral and characterize its properties using analytical and numerical methods. Simulations show that <span class="hlt">frequency</span> spirals in large lattices behave much like this simple prototype.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMSA51B2075C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMSA51B2075C"><span>Detection of Traveling Ionospheric Disturbances by Medium <span class="hlt">Frequency</span> Doppler Sounding Using AM Radio Transmissions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chilcote, M. A.; Labelle, J. W.; Lind, F. D.; Coster, A. J.; Galkin, I. A.; Miller, E.; Weatherwax, A. T.</p> <p>2013-12-01</p> <p>Nighttime traveling ionosphere disturbances (TIDs) propagating in the lower F region of the ionosphere were detected from time <span class="hlt">variations</span> in the Doppler shifts of commercial AM radio broadcast stations. Three <span class="hlt">separately</span> deployed receivers, components of the Intercepted Signals for Ionospheric Science (ISIS) Array software radio instrumentation network, recorded signals from two radio stations during eleven nights in March-April, 2012. Combining these measurements established that <span class="hlt">variations</span> in the <span class="hlt">frequencies</span> of the received signals, with amplitudes up to a few tenths of a Hertz, resulted from Doppler shifts produced by the ionosphere. At times, TIDs were detected as large amplitude <span class="hlt">variations</span> in the Doppler shift with approximately 40-minute period correlated across the array. For one study interval, 0000-0400 UT on April 13, 2012, simultaneous GPS-TEC, digisonde, and superDARN coherent backscatter radar measurements confirmed the detection of TIDs with the same period. Detection of the AM signals at widely spaced receivers allowed the phase velocity and wavelength of the TIDs to be inferred, with some limitations due to differing reflection heights for the different <span class="hlt">frequencies</span>. These measurements will be compared to phase velocities and wavelengths determined from combining an array of GPS receivers; discrepancies due to the altitude sensitivity of the techniques or other effects will be discussed. These results demonstrate that AM radio signals can be used for detection of nighttime TIDs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23297925','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23297925"><span>Multi-component <span class="hlt">separation</span> and analysis of bat echolocation calls.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>DiCecco, John; Gaudette, Jason E; Simmons, James A</p> <p>2013-01-01</p> <p>The vast majority of animal vocalizations contain multiple <span class="hlt">frequency</span> modulated (FM) components with varying amounts of non-linear modulation and harmonic instability. This is especially true of biosonar sounds where precise time-<span class="hlt">frequency</span> templates are essential for neural information processing of echoes. Understanding the dynamic waveform design by bats and other echolocating animals may help to improve the efficacy of man-made sonar through biomimetic design. Bats are known to adapt their call structure based on the echolocation task, proximity to nearby objects, and density of acoustic clutter. To interpret the significance of these changes, a method was developed for component <span class="hlt">separation</span> and analysis of biosonar waveforms. Techniques for imaging in the time-<span class="hlt">frequency</span> plane are typically limited due to the uncertainty principle and interference cross terms. This problem is addressed by extending the use of the fractional Fourier transform to isolate each non-linear component for <span class="hlt">separate</span> analysis. Once <span class="hlt">separated</span>, empirical mode decomposition can be used to further examine each component. The Hilbert transform may then successfully extract detailed time-<span class="hlt">frequency</span> information from each isolated component. This multi-component analysis method is applied to the sonar signals of four species of bats recorded in-flight by radiotelemetry along with a comparison of other common time-<span class="hlt">frequency</span> representations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910010057','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910010057"><span>Turbulent boundary layer <span class="hlt">separation</span> over a rearward facing ramp and its control through mechanical excitation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mckinzie, Daniel J., Jr.</p> <p>1991-01-01</p> <p>A vane oscillating about a fixed point at the inlet to a two-dimensional 20 degree rearward facing ramp has proven effective in delaying the <span class="hlt">separation</span> of a turbulent boundary layer. Measurements of the ramp surface static pressure coefficient obtained under the condition of vane oscillation and constant inlet velocity revealed that two different effects occurred with surface distance along the ramp. In the vicinity of the oscillating vane, the pressure coefficients varied as a negative function of the vane's trailing edge rms velocity; the independent variable on which the rms velocity depends are the vane's oscillation <span class="hlt">frequency</span> and its displacement amplitude. From a point downstream of the vane to the exit of the ramp; however, the pressure coefficient varied as a more complex function of the two independent variables. That is, it was found to vary as a function of the vane's oscillation <span class="hlt">frequency</span> throughout the entire range of <span class="hlt">frequencies</span> covered during the test, but over only a limited range of the trailing edge displacement amplitudes covered. More specifically, the value of the pressure coefficient was independent of increases in the vane's displacement amplitude above approximately 35 inner wall units of the boundary layer. Below this specific amplitude it varied as a function of the vane's trailing edge rms velocity. This height is close to the upper limit of the buffer layer. A parametric study was made to determine the <span class="hlt">variation</span> of the maximum static pressure recovery as a function of the vane's oscillation <span class="hlt">frequency</span>, for several ramp inlet velocities and a constant displacement amplitude of the vane's trailing edge. The results indicate that the phenomenon producing the optimum delay of <span class="hlt">separation</span> may be Strouhal number dependent. Corona anemometer measurements obtained in the inner wall regions of the boundary layer for the excited case reveal a large range of unsteadiness in the local velocities. These measurements imply the existence of inflections</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22408129-ionospheric-very-low-frequency-transmitter','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22408129-ionospheric-very-low-frequency-transmitter"><span>Ionospheric very low <span class="hlt">frequency</span> transmitter</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>Kuo, Spencer P.</p> <p>2015-02-15</p> <p>The theme of this paper is to establish a reliable ionospheric very low <span class="hlt">frequency</span> (VLF) transmitter, which is also broad band. Two approaches are studied that generate VLF waves in the ionosphere. The first, classic approach employs a ground-based HF heater to directly modulate the high latitude ionospheric, or auroral electrojet. In the classic approach, the intensity-modulated HF heater induces an alternating current in the electrojet, which serves as a virtual antenna to transmit VLF waves. The spatial and temporal <span class="hlt">variations</span> of the electrojet impact the reliability of the classic approach. The second, beat-wave approach also employs a ground-based HFmore » heater; however, in this approach, the heater operates in a continuous wave mode at two HF <span class="hlt">frequencies</span> <span class="hlt">separated</span> by the desired VLF <span class="hlt">frequency</span>. Theories for both approaches are formulated, calculations performed with numerical model simulations, and the calculations are compared to experimental results. Theory for the classic approach shows that an HF heater wave, intensity-modulated at VLF, modulates the electron temperature dependent electrical conductivity of the ionospheric electrojet, which, in turn, induces an ac electrojet current. Thus, the electrojet becomes a virtual VLF antenna. The numerical results show that the radiation intensity of the modulated electrojet decreases with an increase in VLF radiation <span class="hlt">frequency</span>. Theory for the beat wave approach shows that the VLF radiation intensity depends upon the HF heater intensity rather than the electrojet strength, and yet this approach can also modulate the electrojet when present. HF heater experiments were conducted for both the intensity modulated and beat wave approaches. VLF radiations were generated and the experimental results confirm the numerical simulations. Theory and experimental results both show that in the absence of the electrojet, VLF radiation from the F-region is generated via the beat wave approach. Additionally, the beat wave</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/862972','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/862972"><span>Method for isotope <span class="hlt">separation</span> by photodeflection</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bernhardt, Anthony F.</p> <p>1977-01-01</p> <p>In the method of <span class="hlt">separating</span> isotopes wherein a desired isotope species is selectively deflected out of a beam of mixed isotopes by irradiating the beam with a directed beam of light of narrowly defined <span class="hlt">frequency</span> which is selectively absorbed by the desired species, the improvement comprising irradiating the deflected beam with light from other light sources whose <span class="hlt">frequencies</span> are selected to cause the depopulation of any metastable excited states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22837794','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22837794"><span>School-Based Racial and Gender Discrimination among African American Adolescents: Exploring Gender <span class="hlt">Variation</span> in <span class="hlt">Frequency</span> and Implications for Adjustment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cogburn, Courtney D; Chavous, Tabbye M; Griffin, Tiffany M</p> <p>2011-01-03</p> <p>The present study examined school-based racial and gender discrimination experiences among African American adolescents in Grade 8 (n = 204 girls; n = 209 boys). A primary goal was exploring gender <span class="hlt">variation</span> in <span class="hlt">frequency</span> of both types of discrimination and associations of discrimination with academic and psychological functioning among girls and boys. Girls and boys did not vary in reported racial discrimination <span class="hlt">frequency</span>, but boys reported more gender discrimination experiences. Multiple regression analyses within gender groups indicated that among girls and boys, racial discrimination and gender discrimination predicted higher depressive symptoms and school importance and racial discrimination predicted self-esteem. Racial and gender discrimination were also negatively associated with grade point average among boys but were not significantly associated in girls' analyses. Significant gender discrimination X racial discrimination interactions resulted in the girls' models predicting psychological outcomes and in boys' models predicting academic achievement. Taken together, findings suggest the importance of considering gender- and race-related experiences in understanding academic and psychological adjustment among African American adolescents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910877S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910877S"><span>Full waveform inversion in the <span class="hlt">frequency</span> domain using classified time-domain residual wavefields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Son, Woohyun; Koo, Nam-Hyung; Kim, Byoung-Yeop; Lee, Ho-Young; Joo, Yonghwan</p> <p>2017-04-01</p> <p>We perform the acoustic full waveform inversion in the <span class="hlt">frequency</span> domain using residual wavefields that have been <span class="hlt">separated</span> in the time domain. We sort the residual wavefields in the time domain according to the order of absolute amplitudes. Then, the residual wavefields are <span class="hlt">separated</span> into several groups in the time domain. To analyze the characteristics of the residual wavefields, we compare the residual wavefields of conventional method with those of our residual <span class="hlt">separation</span> method. From the residual analysis, the amplitude spectrum obtained from the trace before <span class="hlt">separation</span> appears to have little energy at the lower <span class="hlt">frequency</span> bands. However, the amplitude spectrum obtained from our strategy is regularized by the <span class="hlt">separation</span> process, which means that the low-<span class="hlt">frequency</span> components are emphasized. Therefore, our method helps to emphasize low-<span class="hlt">frequency</span> components of residual wavefields. Then, we generate the <span class="hlt">frequency</span>-domain residual wavefields by taking the Fourier transform of the <span class="hlt">separated</span> time-domain residual wavefields. With these wavefields, we perform the gradient-based full waveform inversion in the <span class="hlt">frequency</span> domain using back-propagation technique. Through a comparison of gradient directions, we confirm that our <span class="hlt">separation</span> method can better describe the sub-salt image than the conventional approach. The proposed method is tested on the SEG/EAGE salt-dome model. The inversion results show that our algorithm is better than the conventional gradient based waveform inversion in the <span class="hlt">frequency</span> domain, especially for deeper parts of the velocity model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004ASAJ..116.1710A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ASAJ..116.1710A"><span>Flow <span class="hlt">separation</span> in a computational oscillating vocal fold model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alipour, Fariborz; Scherer, Ronald C.</p> <p>2004-09-01</p> <p>A finite-volume computational model that solves the time-dependent glottal airflow within a forced-oscillation model of the glottis was employed to study glottal flow <span class="hlt">separation</span>. Tracheal input velocity was independently controlled with a sinusoidally varying parabolic velocity profile. Control parameters included flow rate (Reynolds number), oscillation <span class="hlt">frequency</span> and amplitude of the vocal folds, and the phase difference between the superior and inferior glottal margins. Results for static divergent glottal shapes suggest that velocity increase caused glottal <span class="hlt">separation</span> to move downstream, but reduction in velocity increase and velocity decrease moved the <span class="hlt">separation</span> upstream. At the fixed <span class="hlt">frequency</span>, an increase of amplitude of the glottal walls moved the <span class="hlt">separation</span> further downstream during glottal closing. Increase of Reynolds number caused the flow <span class="hlt">separation</span> to move upstream in the glottis. The flow <span class="hlt">separation</span> cross-sectional ratio ranged from approximately 1.1 to 1.9 (average of 1.47) for the divergent shapes. Results suggest that there may be a strong interaction of rate of change of airflow, inertia, and wall movement. Flow <span class="hlt">separation</span> appeared to be ``delayed'' during the vibratory cycle, leading to movement of the <span class="hlt">separation</span> point upstream of the glottal end only after a significant divergent angle was reached, and to persist upstream into the convergent phase of the cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ExFl...58...66S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ExFl...58...66S"><span>Inspection of the dynamic properties of laminar <span class="hlt">separation</span> bubbles: free-stream turbulence intensity effects for different Reynolds numbers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Simoni, Daniele; Lengani, Davide; Ubaldi, Marina; Zunino, Pietro; Dellacasagrande, Matteo</p> <p>2017-06-01</p> <p>The effects of free-stream turbulence intensity (FSTI) on the transition process of a pressure-induced laminar <span class="hlt">separation</span> bubble have been studied for different Reynolds numbers (Re) by means of time-resolved (TR) PIV. Measurements have been performed along a flat plate installed within a double-contoured test section, designed to produce an adverse pressure gradient typical of ultra-high-lift turbine blade profiles. A test matrix spanning 3 FSTI levels and 3 Reynolds numbers has been considered allowing estimation of cross effects of these parameters on the instability mechanisms driving the <span class="hlt">separated</span> flow transition process. Boundary layer integral parameters, spatial growth rate and saturation level of velocity fluctuations are discussed for the different cases in order to characterize the base flow response as well as the time-mean properties of the Kelvin-Helmholtz instability. The inspection of the instantaneous velocity vector maps highlights the dynamics of the large-scale structures shed near the bubble maximum displacement, as well as the low-<span class="hlt">frequency</span> motion of the fore part of the <span class="hlt">separated</span> shear layer. Proper Orthogonal Decomposition (POD) has been implemented to reduce the large amount of data for each condition allowing a rapid evaluation of the group velocity, spatial wavelength and dominant <span class="hlt">frequency</span> of the vortex shedding process. The dimensionless shedding wave number parameter makes evident that the modification of the shear layer thickness at <span class="hlt">separation</span> due to Reynolds number <span class="hlt">variation</span> mainly drives the length scale of the rollup vortices, while higher FSTI levels force the onset of the shedding phenomenon to occur upstream due to the higher velocity fluctuations penetrating into the <span class="hlt">separating</span> boundary layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AdAtS..35..423C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AdAtS..35..423C"><span><span class="hlt">Variations</span> in High-<span class="hlt">frequency</span> Oscillations of Tropical Cyclones over the Western North Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Shumin; Li, Weibiao; Wen, Zhiping; Zhou, Mingsen; Lu, Youyu; Qian, Yu-Kun; Liu, Haoya; Fang, Rong</p> <p>2018-04-01</p> <p><span class="hlt">Variations</span> in the high-<span class="hlt">frequency</span> oscillations of tropical cyclones (TCs) over the western North Pacific (WNP) are studied in numerical model simulations. Power spectrum analysis of maximum wind speeds at 10 m (MWS10) from an ensemble of 15 simulated TCs shows that oscillations are significant for all TCs. The magnitudes of oscillations in MWS10 are similar in the WNP and South China Sea (SCS); however, the mean of the averaged significant periods in the SCS (1.93 h) is shorter than that in the open water of the WNP (2.83 h). The shorter period in the SCS is examined through an ensemble of simulations, and a case simulation as well as a sensitivity experiment in which the continent is replaced by ocean for Typhoon Hagupit (2008). The analysis of the convergence efficiency within the boundary layer suggests that the shorter periods in the SCS are possibly due to the stronger terrain effect, which intensifies convergence through greater friction. The enhanced convergence strengthens the disturbance of the gradient and thermal wind balances, and then contributes to the shorter oscillation periods in the SCS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RScI...89e5007A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RScI...89e5007A"><span>Polydyne displacement interferometer using <span class="hlt">frequency</span>-modulated light</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arablu, Masoud; Smith, Stuart T.</p> <p>2018-05-01</p> <p>A radio-<span class="hlt">frequency</span> <span class="hlt">Frequency</span>-Modulated (FM) signal is used to diffract a He-Ne laser beam through an Acousto-Optic Modulator (AOM). Due to the modulation of the FM signal, the measured spectra of the diffracted beams comprise a series of phase-synchronized harmonics that have exact integer <span class="hlt">frequency</span> <span class="hlt">separation</span>. The first diffraction side-beam emerging from the AOM is selected by a slit to be used in a polydyne displacement interferometer in a Michelson interferometer topology. The displacement measurement is derived from the phase measurement of selected modulation harmonic pairs. Individual harmonic <span class="hlt">frequency</span> amplitudes are measured using discrete Fourier transform applied to the signal from a single photodetector. Phase signals are derived from the changes in the amplitudes of different harmonic pairs (typically odd-even pairs) with the phase being extracted using a standard quadrature method. In this study, two different modulation <span class="hlt">frequencies</span> of 5 and 10 kHz are used at different modulation depths. The measured displacements by different harmonic pairs are compared with a commercial heterodyne interferometer being used as a reference for these studies. Measurements obtained from five different harmonic pairs when the moving mirror of the interferometer is scanned over ranges up to 10 μm all show differences of less than 50 nm from the reference interferometer measurements. A drift test was also used to evaluate the differences between the polydyne interferometer and reference measurements that had different optical path lengths of approximately 25 mm and 50 mm, respectively. The drift test results indicate that about half of the differences can be attributed to temperature, pressure, and humidity <span class="hlt">variations</span>. Other influences include Abbe and thermal expansion effects. Rough magnitude estimates using simple models for these two effects can account for remaining observed deviations.</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://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5698618','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5698618"><span><span class="hlt">Variation</span> in recombination <span class="hlt">frequency</span> and distribution across eukaryotes: patterns and processes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Feulner, Philine G. D.; Johnston, Susan E.; Santure, Anna W.; Smadja, Carole M.</p> <p>2017-01-01</p> <p>Recombination, the exchange of DNA between maternal and paternal chromosomes during meiosis, is an essential feature of sexual reproduction in nearly all multicellular organisms. While the role of recombination in the evolution of sex has received theoretical and empirical attention, less is known about how recombination rate itself evolves and what influence this has on evolutionary processes within sexually reproducing organisms. Here, we explore the patterns of, and processes governing recombination in eukaryotes. We summarize patterns of <span class="hlt">variation</span>, integrating current knowledge with an analysis of linkage map data in 353 organisms. We then discuss proximate and ultimate processes governing recombination rate <span class="hlt">variation</span> and consider how these influence evolutionary processes. Genome-wide recombination rates (cM/Mb) can vary more than tenfold across eukaryotes, and there is large <span class="hlt">variation</span> in the distribution of recombination events across closely related taxa, populations and individuals. We discuss how <span class="hlt">variation</span> in rate and distribution relates to genome architecture, genetic and epigenetic mechanisms, sex, environmental perturbations and variable selective pressures. There has been great progress in determining the molecular mechanisms governing recombination, and with the continued development of new modelling and empirical approaches, there is now also great opportunity to further our understanding of how and why recombination rate varies. This article is part of the themed issue ‘Evolutionary causes and consequences of recombination rate <span class="hlt">variation</span> in sexual organisms’. PMID:29109219</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22596658-frequency-spirals','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22596658-frequency-spirals"><span><span class="hlt">Frequency</span> spirals</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>Ottino-Löffler, Bertrand; Strogatz, Steven H., E-mail: strogatz@cornell.edu</p> <p>2016-09-15</p> <p>We study the dynamics of coupled phase oscillators on a two-dimensional Kuramoto lattice with periodic boundary conditions. For coupling strengths just below the transition to global phase-locking, we find localized spatiotemporal patterns that we call “<span class="hlt">frequency</span> spirals.” These patterns cannot be seen under time averaging; they become visible only when we examine the spatial <span class="hlt">variation</span> of the oscillators' instantaneous <span class="hlt">frequencies</span>, where they manifest themselves as two-armed rotating spirals. In the more familiar phase representation, they appear as wobbly periodic patterns surrounding a phase vortex. Unlike the stationary phase vortices seen in magnetic spin systems, or the rotating spiral waves seenmore » in reaction-diffusion systems, <span class="hlt">frequency</span> spirals librate: the phases of the oscillators surrounding the central vortex move forward and then backward, executing a periodic motion with zero winding number. We construct the simplest <span class="hlt">frequency</span> spiral and characterize its properties using analytical and numerical methods. Simulations show that <span class="hlt">frequency</span> spirals in large lattices behave much like this simple prototype.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JHyd..553..486Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JHyd..553..486Q"><span>Assessing the ecohydrological <span class="hlt">separation</span> hypothesis and seasonal <span class="hlt">variations</span> in water use by Ginkgo biloba L. in a subtropical riparian area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qian, Jin; Zheng, Hao; Wang, Peifang; Liao, Xiaolin; Wang, Chao; Hou, Jun; Ao, Yanhui; Shen, Mengmeng; Liu, Jingjing; Li, Kun</p> <p>2017-10-01</p> <p>In this study we used a dual stable isotope approach (δ18O and δ2H) to assess the ecohydrological <span class="hlt">separation</span> hypothesis and to identify the seasonal <span class="hlt">variation</span> in water sources of Ginkgo biloba L. in the riparian zone in the Taihu Lake basin, China. Three study sites located at 5, 10, and 30 m from a river bank were established. From August 2014 to July 2015, samples of rainwater, river water, groundwater, bulk soil water at five soil depths (i.e. 0-30, 30-60, 60-90, 90-120, 120-150 cm), and xylem water of G. biloba, were collected and their δ18O and δ2H values were measured. Generally, the δ18O and δ2H values for xylem water, groundwater, and soil water clustered together and <span class="hlt">separated</span> from those of river water, suggesting the possible occurrence of ecohydrological <span class="hlt">separation</span>. However, the line-conditioned excess (lc-excess) values of most xylem water were positive, indicating a mixture of different water sources. Significant correlations were observed between the contributions of precipitation, soil water, and groundwater to water uptake by G. biloba, further supporting ecohydrological connectivity rather than ecohydrological <span class="hlt">separation</span>. G. biloba switched its major water sources from soil water at 0-60 cm depth and precipitation in the wet summer, to soil water from >90 cm depth and groundwater in the dry winter. The river water was a minor water source for G. biloba, but its contribution was comparatively greater at the site closest to the river bank. Our findings contribute to understanding of plant-soil-water relationships and the water balance, and may provide important information for investigations of nutrient sources and sinks in riparian zones. The present study suggests the need to rethink the application of ecohydrological connectivity and <span class="hlt">separation</span> in different biomes, especially where river water and groundwater recharge each other over time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993RaSc...28..203C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993RaSc...28..203C"><span>Spaced antenna diversity in temperate latitude meteor burst systems operating near 40 MHz - <span class="hlt">Variation</span> of signal cross-correlation coefficients with antenna <span class="hlt">separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cannon, Paul S.; Shukla, Anil K.; Lester, Mark</p> <p>1993-04-01</p> <p>We have studied 37-MHz signals received over an 800-km temperate latitude path using 400-W continuous wave transmissions. Signals collected during a 9-day period in February 1990 on two antennas at <span class="hlt">separations</span> of 5, 10, and 20 lambda were analyzed. Three signal categories were identified (overdense, underdense, and not known (NK)) and cross-correlation coefficients between the signals received by the two antennas were calculated for each signal category. No spatial <span class="hlt">variation</span>, and in particular no decrease, in average cross-correlation coefficient was observed for underdense or NK signals as the antenna spacing was increased from 5 to 20 lambda. At each antenna <span class="hlt">separation</span> the cross-correlation coefficients of these two categories were strongly dependent on time. Overdense signals, however, showed no cross-correlation time dependency at 5 and 10 lambda, but there was a strong time dependency at 20 lambda. Recommendations are made in regard to the optimum antenna spacing for a meteor burst communication system using spaced antenna diversity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3675855','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3675855"><span><span class="hlt">Variation</span> in Nephrologist Visits to Patients on Hemodialysis across Dialysis Facilities and Geographic Locations</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tan, Kelvin B.; Winkelmayer, Wolfgang C.; Chertow, Glenn M.; Bhattacharya, Jay</p> <p>2013-01-01</p> <p>Summary Background and objectives Geographic and other <span class="hlt">variations</span> in medical practices lead to differences in medical costs, often without a clear link to health outcomes. This work examined <span class="hlt">variation</span> in the <span class="hlt">frequency</span> of physician visits to patients receiving hemodialysis to measure the relative importance of provider practice patterns (including those patterns linked to geographic region) and patient health in determining visit <span class="hlt">frequency</span>. Design, setting, participants, & measurements This work analyzed a nationally representative 2006 database of patients receiving hemodialysis in the United States. A <span class="hlt">variation</span> decomposition analysis of the relative importance of facility, geographic region, and patient characteristics—including demographics, socioeconomic status, and indicators of health status—in explaining physician visit <span class="hlt">frequency</span> <span class="hlt">variation</span> was conducted. Finally, the associations between facility, geographic and patient characteristics, and provider visit <span class="hlt">frequency</span> were measured using multivariable regression. Results Patient characteristics accounted for only 0.9% of the total visit <span class="hlt">frequency</span> <span class="hlt">variation</span>. Accounting for case-mix differences, patients’ hemodialysis facilities explained about 24.9% of visit <span class="hlt">frequency</span> <span class="hlt">variation</span>, of which 9.3% was explained by geographic region. Visit <span class="hlt">frequency</span> was more closely associated with many facility and geographic characteristics than indicators of health status. More recent dialysis initiation and recent hospitalization were associated with decreased visit <span class="hlt">frequency</span>. Conclusions In hemodialysis, provider visit <span class="hlt">frequency</span> depends more on geography and facility location and characteristics than patients’ health status or acuity of illness. The magnitude of <span class="hlt">variation</span> unrelated to patient health suggests that provider visit <span class="hlt">frequency</span> practices do not reflect optimal management of patients on dialysis. PMID:23430207</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790002207','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790002207"><span>Methods of <span class="hlt">separation</span> of variables in turbulence theory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tsuge, S.</p> <p>1978-01-01</p> <p>Two schemes of closing turbulent moment equations are proposed both of which make double correlation equations <span class="hlt">separated</span> into single-point equations. The first is based on neglected triple correlation, leading to an equation differing from small perturbed gasdynamic equations where the <span class="hlt">separation</span> constant appears as the <span class="hlt">frequency</span>. Grid-produced turbulence is described in this light as time-independent, cylindrically-isotropic turbulence. Application to wall turbulence guided by a new asymptotic method for the Orr-Sommerfeld equation reveals a neutrally stable mode of essentially three dimensional nature. The second closure scheme is based on an assumption of identity of the <span class="hlt">separated</span> variables through which triple and quadruple correlations are formed. The resulting equation adds, to its equivalent of the first scheme, an integral of nonlinear convolution in the <span class="hlt">frequency</span> describing a role due to triple correlation of direct energy-cascading.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AcAau.133..158X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AcAau.133..158X"><span>Experimental study on the flow <span class="hlt">separation</span> and self-excited oscillation phenomenon in a rectangular duct</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiong, Bing; Wang, Zhen-Guo; Fan, Xiao-Qiang; Wang, Yi</p> <p>2017-04-01</p> <p>To study the characteristics of flow <span class="hlt">separation</span> and self-excited oscillation of a shock train in a rectangular duct, a simple test case has been conducted and analyzed. The high-speed Schlieren technique and high-<span class="hlt">frequency</span> pressure measurements have been adopted to collect the data. The experimental results show that there are two <span class="hlt">separation</span> modes in the duct under M3 incoming condition. The <span class="hlt">separation</span> mode switch has great effects on the flow effects, such as the pressure distribution, the standard deviation distribution and so on. The <span class="hlt">separation</span> mode switch can be judged by the history of pressure standard deviation. When it comes to the self-excited oscillation of a shock train, the <span class="hlt">frequency</span> contents in the undisturbed region, the intermittent region, and the <span class="hlt">separated</span> bubble have been compared. It was found that the low-<span class="hlt">frequency</span> disturbance induced by the upstream shock foot motions can travel downstream and the <span class="hlt">frequency</span> will be magnified by the <span class="hlt">separation</span> bubble. The oscillation of the small shock foot and the oscillation of the large shock foot are associated with each other rather than oscillating independently.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12347392','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12347392"><span>Spousal-residence <span class="hlt">separation</span> among Chinese young couples.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ma, Z; Liaw K-l; Zeng, Y</p> <p>1996-05-01</p> <p>The factors affecting the residential <span class="hlt">separation</span> of spouses in China are examined. "Based on the microdata of the 1987 National Population Survey, we find that the <span class="hlt">variation</span> in spousal-residence <span class="hlt">separations</span> among Chinese young couples in the mid-1980s is well explained by personal and household factors within a multivariate model. The <span class="hlt">separations</span> were aggravated by migrations for the reasons of employment or education. Although marriage migrations reduced the number of <span class="hlt">separations</span>, those who had been married for a short period of time...were more prone to be <span class="hlt">separated</span>. It is ironic that the higher a person's level of education, the greater the tendency for them to suffer the pain of spousal-residence <span class="hlt">separation</span>. Household status could also be a very important factor: the lower the household status of a married individual, the more likely that he (or she) would be <span class="hlt">separated</span> from their spouse." excerpt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2896409','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2896409"><span>The role of off-<span class="hlt">frequency</span> masking in binaural hearing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Buss, Emily; Hall, Joseph W.</p> <p>2010-01-01</p> <p>The present studies examined the binaural masking level difference (MLD) for off-<span class="hlt">frequency</span> masking. It has been shown previously that the MLD decreases steeply with increasing spectral <span class="hlt">separation</span> between a pure tone signal and a 10-Hz wide band of masking noise. Data collected here show that this reduction in the off-<span class="hlt">frequency</span> MLD as a function of signal∕masker <span class="hlt">separation</span> is comparable at 250 and 2500 Hz, indicating that neither interaural phase cues nor <span class="hlt">frequency</span> resolution are critical to this finding. The MLD decreases more gradually with spectral <span class="hlt">separation</span> when the masker is a 250-Hz-wide band of noise, a result that implicates the rate of inherent amplitude modulation of the masker. Thresholds were also measured for a brief signal presented coincident with a local masker modulation minimum or maximum. Sensitivity was better in the minima for all NoSπ and off-<span class="hlt">frequency</span> NoSo conditions, with little or no effect of signal position for on-<span class="hlt">frequency</span> NoSo conditions. Taken together, the present results indicate that the steep reduction in the off-<span class="hlt">frequency</span> MLD for a narrowband noise masker is due at least in part to envelope cues in the NoSo conditions. There was no evidence of a reduction in binaural cue quality for off-<span class="hlt">frequency</span> masking. PMID:20550265</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990028208','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990028208"><span>[Low-<span class="hlt">Frequency</span> Flow Oscillation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bragg, Michael B.</p> <p>1997-01-01</p> <p>The results of the research conducted under this grant are presented in detail in three Master theses, by Heinrich, Balow, and Broeren. Additional analysis of the experimental data can be found in two AIAA Journal articles and two conference papers. Citations for all of the studies' publications can be found in the bibliography which is attached. The objective of Heinrich's study was to document the low-<span class="hlt">frequency</span> flow oscillation on the LRN-1007 airfoil, which had been previously observed at low Reynolds number, to determine its origin, and explore the phenomenon at higher Reynolds number. Heinrich performed detailed flow visualization on the airfoil using surface fluorescent oil and laser-sheet off-body visualization. A large leading-edge <span class="hlt">separation</span> bubble and trailing-edge <span class="hlt">separation</span> was identified on the airfoil just prior to the onset of the unsteady stall flow oscillation. From the laser-sheet data, the unsteady flow appeared as a massive boundary-layer <span class="hlt">separation</span> followed by flow reattachment. Hot-wire data were taken in the wake to identify the presence of the flow oscillation and the dominant <span class="hlt">frequency</span>. The oscillation was found in the flow from a Reynolds number of 0.3 to 1.3 x 10 exp 6. The Strouhal number based on airfoil projected height was nominally 0.02 and increased slightly with increasing Reynolds number and significantly with increasing airfoil angle of attack. Balow focused his research on the leading-edge <span class="hlt">separation</span> bubble which was hypothesized to be the origin of the low-<span class="hlt">frequency</span> oscillation. Initially, experimental measurements in the bubble at the onset of the low-<span class="hlt">frequency</span> oscillation were attempted to study the characteristics of the bubble and explain possible relationships to the shear-layer-flapping phenomena. Unfortunately, the bubble proved to be extremely sensitive to the probe interference and it drastically reduced the size of the bubble. These detailed measurements were then abandoned by Balow. However, this led to a series of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5790043','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5790043"><span>Genetic <span class="hlt">variation</span> in resistance to blast (Pyricularia oryzae Cavara) in rice (Oryza sativa L.) germplasms of Bangladesh</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Khan, Mohammad Ashik Iqbal; Latif, Mohammad Abdul; Khalequzzaman, Mohammad; Tomita, Asami; Ali, Mohammad Ansar; Fukuta, Yoshimichi</p> <p>2017-01-01</p> <p>Genetic <span class="hlt">variation</span> in blast resistance was clarified in 334 Bangladesh rice accessions from 4 major ecotypes (Aus, Aman, Boro and Jhum). Cluster analysis of polymorphism data of 74 SSR markers <span class="hlt">separated</span> these accessions into cluster I (corresponding to the Japonica Group) and cluster II (corresponding to the Indica Group). Cluster II accessions were represented with high <span class="hlt">frequency</span> in all ecotypes. Cluster II was further subdivided into subclusters IIa and IIb. Subcluster IIa accessions were represented with high <span class="hlt">frequency</span> in only Aus and Jhum ecotypes. Cluster I accessions were more frequent in the Aman ecotype than in other ecotypes. Distinct <span class="hlt">variations</span> in resistance were found, and accessions were classified into 4 groups (A1, A2, B1 and B2) based on their reactions to standard differential blast isolates. The most susceptible group was A2 (which included susceptible variety Lijiangxintuanheigu, most of the differential varieties, and a few Bangladesh accessions), followed in order by A1, B2 and B1 (the most resistant). Accessions from 4 ecotypes fell with different <span class="hlt">frequencies</span> into each of these resistance groups. These results demonstrated that Japonica Group accessions were found mainly in Aman, and Indica Group accessions were distributed across all ecotypes. Susceptible accessions were limited in Aus and Aman. PMID:29398943</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28760406','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28760406"><span>The <span class="hlt">variation</span> in <span class="hlt">frequency</span> locations in Doppler ultrasound spectra for maximum blood flow velocities in narrowed vessels.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Yingyun; Zhang, Yufeng; Gao, Lian; Deng, Li; Hu, Xiao; Zhang, Kexin; Li, Haiyan</p> <p>2017-11-01</p> <p>This study assessed the <span class="hlt">variation</span> in the <span class="hlt">frequency</span> locations in the Doppler ultrasound spectra for the maximum blood flow velocities of in vessels with different degrees of bilaterally axisymmetric stenosis. This was done by comparing the relationship between the velocity distributions and corresponding Doppler power spectra. First, a geometric vessel model with axisymmetric stenosis was established. This made it possible to obtain the blood flow velocity distributions for different degrees of stenosis from the solutions of the Navier-Stokes equations. Then, the Doppler spectra were calculated for the entire segment of the vessel that was covered by the sound field. Finally, the maximum <span class="hlt">frequency</span> locations for the spectra were determined based on the intersections of the maximum values chosen from the calculated blood flow velocity distributions and their corresponding spectra. The computational analysis showed that the maximum <span class="hlt">frequencies</span>, which corresponded to the maximum blood flow velocities for different degrees of stenosis, were located at different positions along the spectral falling edges. The location for a normal (stenosis free) vessel was in the middle of the falling edge. For vessels with increasing degrees of stenosis, this location shifted approximately linearly downward along the falling edge. For 40% stenosis, the location reached a position at the falling edge of 0.32. Results obtained using the Field II simulation tool demonstrated the validity of the theoretical analysis and calculations, and may help to improve the maximum velocity estimation accuracy for Doppler blood flow spectra in stenosed vessels. Copyright © 2017 IPEM. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993ElL....29.1441M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993ElL....29.1441M"><span>Single-layer dual <span class="hlt">frequency</span> patch antenna</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maci, S.; Gentili, G. B.; Avitabile, G.</p> <p>1993-08-01</p> <p>A configuration for a slotted patch antenna is introduced which allows two <span class="hlt">separate</span> operating <span class="hlt">frequencies</span>. Both of these <span class="hlt">frequencies</span> are associated with a radiating mode almost identical to that of a standard patch. The two resonances are related to the patch width and the slot/patch length, respectively.</p> </li> <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> <span class="hlt">variations</span> 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 <span class="hlt">variations</span> 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 scale comparable to the pressure scale 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('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 <span class="hlt">separately</span>. 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-scale, L-coefficient of <span class="hlt">variation</span>, 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-scale and spatially averaged L-skew statistics were used to compute the location, scale, 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/1179219','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/1179219"><span>Binaural beats at high <span class="hlt">frequencies</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McFadden, D; Pasanen, E G</p> <p>1975-10-24</p> <p>Binaural beats have long been believed to be audible only at low <span class="hlt">frequencies</span>, but an interaction reminiscent of a binaural beat can sometimes be heard when different two-tone complexes of high <span class="hlt">frequency</span> are presented to the two ears. The primary requirement is that the <span class="hlt">frequency</span> <span class="hlt">separation</span> in the complex at one ear be slightly different from that in the other--that is, that there be a small interaural difference in the envelope periodicities. This finding is in accord with other recent demonstrations that the auditory system is not deaf to interaural time differences at high <span class="hlt">frequencies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..163a2036B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..163a2036B"><span>Single-phase <span class="hlt">frequency</span> converter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baciu, I.; Cunţan, C. D.</p> <p>2017-01-01</p> <p>The paper presents a continuous voltage inverter - AC (12V / 230V) made with IGBT and two-stage voltage transformer. The sequence control transistors is achieved using a ring counter whose clock signal is obtained with a monostable circuit LM 555. The <span class="hlt">frequency</span> of the clock signal can be adjustment with a potentiometer that modifies the charging current of the capacitor which causes constant monostable circuit time. Command sequence consists of 8 intervals of which 6 are assigned to command four transistors and two for the period break at the beginning and end of the sequence control. To obtain an alternation consisting of two different voltage level, two transistors will be comanded, connected to different windings of the transformer and the one connected to the winding providing lower voltage must be comanded twice. The output of the numerator goes through an inverter type MOS and a current amplifier with bipolar transistor.To achieve galvanic <span class="hlt">separation</span>, an optocoupler will be used for each IGBT transistor, while protection is achieved with resistance and diode circuit. At the end there is connected an LC filter for smoothing voltage <span class="hlt">variations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ExFl...58..106S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ExFl...58..106S"><span><span class="hlt">Separation</span> control with fluidic oscillators in water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, H.-J.; Woszidlo, R.; Nayeri, C. N.; Paschereit, C. O.</p> <p>2017-08-01</p> <p>The present study assesses the applicability of fluidic oscillators for <span class="hlt">separation</span> control in water. The first part of this work evaluates the properties of the fluidic oscillators including <span class="hlt">frequency</span>, cavitation effects, and exerted thrust. Derived from the governing internal dynamics, the oscillation <span class="hlt">frequency</span> is found to scale directly with the jet's exit velocity and the size of the fluidic oscillator independent of the working fluid. <span class="hlt">Frequency</span> data from various experiments collapse onto a single curve. The occurrence of cavitation is examined by visual inspection and hydrophone measurements. The oscillation <span class="hlt">frequency</span> is not affected by cavitation because it does not occur inside the oscillators. The spectral information obtained with the hydrophone provide a reliable indicator for the onset of cavitation at the exit. The performance of the fluidic oscillators for <span class="hlt">separation</span> control on a bluff body does not seem to be affected by the presence of cavitation. The thrust exerted by an array of fluidic oscillators with water as the working fluid is measured to be even larger than theoretically estimated values. The second part of the presented work compares the performance of fluidic oscillators for <span class="hlt">separation</span> control in water with previous results in air. The array of fluidic oscillators is installed into the rear end of a bluff body model. The drag improvements based on force balance measurements agree well with previous wind tunnel experiments on the same model. The flow field is examined by pressure measurements and with particle image velocimetry. Similar performance and flow field characteristics are observed in both water and air.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.G43B0748F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.G43B0748F"><span><span class="hlt">Separation</span> of GRACE geoid time-<span class="hlt">variations</span> using Independent Component Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frappart, F.; Ramillien, G.; Maisongrande, P.; Bonnet, M.</p> <p>2009-12-01</p> <p>Independent Component Analysis (ICA) is a blind <span class="hlt">separation</span> method based on the simple assumptions of the independence of the sources and the non-Gaussianity of the observations. An approach based on this numerical method is used here to extract hydrological signals over land and oceans from the polluting striping noise due to orbit repetitiveness and present in the GRACE global mass anomalies. We took advantage of the availability of monthly Level-2 solutions from three official providers (i.e., CSR, JPL and GFZ) that can be considered as different observations of the same phenomenon. The efficiency of the methodology is first demonstrated on a synthetic case. Applied to one month of GRACE solutions, it allows to clearly <span class="hlt">separate</span> the total water storage change from the meridional-oriented spurious gravity signals on the continents but not on the oceans. This technique gives results equivalent as the destriping method for continental water storage for the hydrological patterns with less smoothing. This methodology is then used to filter the complete series of the 2002-2009 GRACE solutions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=ethnic+AND+variations&id=EJ879236','ERIC'); return false;" href="https://eric.ed.gov/?q=ethnic+AND+variations&id=EJ879236"><span>Ethnic <span class="hlt">Variations</span> in the Connection between Work-Induced Family <span class="hlt">Separation</span> and Turnover Intent</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>Behnke, Andrew O.; MacDermid, Shelley M.; Anderson, James C.; Weiss, Howard M.</p> <p>2010-01-01</p> <p>Using conservation of resources theory, this study examines the role of resources in the relationship between work-induced family <span class="hlt">separation</span> and workers' intentions to leave their employment and how these relationships vary across ethnic groups. Analyses of a large representative sample of military members reveal that family <span class="hlt">separation</span> is…</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JFS....45...50E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JFS....45...50E"><span>Tangential synthetic jets for <span class="hlt">separation</span> control</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esmaeili Monir, H.; Tadjfar, M.; Bakhtian, A.</p> <p>2014-02-01</p> <p>A numerical study of <span class="hlt">separation</span> control has been made to investigate aerodynamic characteristics of a NACA23012 airfoil with a tangential synthetic jet. Simulations are carried out at the chord Reynolds number of Re=2.19×106. The present approach relies on solving the Unsteady Reynolds-Averaged Navier-Stokes (URANS) equations. The turbulence model used in the present computation is the Spalart-Allmaras one-equation model. All computations are performed with a finite volume based code. Stall characteristics are significantly improved by controlling the formation of <span class="hlt">separation</span> vortices in the flow. We placed the synthetic jet at the 12% chord, xj=0.12c, where we expected the <span class="hlt">separation</span> to occur. Two distinct jet oscillating <span class="hlt">frequencies</span>: Fj+=0.159 and Fj+=1 were considered. We studied the effect of blowing ratio, Vj/U∞, where it was varied from 0 to 5. The inclined angle of the synthetic jet was varied from αj=0° up to αj=83°. For the non-zero inclined angles, the local maximum in the aerodynamic performance, Cl/Cd, of 6.89 was found for the inclined angle of about 43°. In the present method, by means of creating a dent on the airfoil, linear momentum is transferred to the flow system in tangential direction to the airfoil surface. Thus the absolute maximum of 11.19 was found for the tangential synthetic jet at the inclined angle of the jet of 0°. The mechanisms involved for a tangential jet appear to behave linearly, as by multiplying the activation <span class="hlt">frequency</span> of the jet by a factor produces the same multiplication factor in the resulting <span class="hlt">frequency</span> in the flow. However, the mechanisms involved in the non-zero inclined angle cases behave nonlinearly when the activation <span class="hlt">frequency</span> is multiplied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110011849','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110011849"><span>Round-Trip System Available to Measure Path Length <span class="hlt">Variation</span> in Korea VLBI System for Geodesy</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Oh, Hongjong; Kondo, Tetsuro; Lee, Jinoo; Kim, Tuhwan; Kim, Myungho; Kim, Suchul; Park, Jinsik; Ju, Hyunhee</p> <p>2010-01-01</p> <p>The construction project of Korea Geodetic VLBI officially started in October 2008. The construction of all systems will be completed by the end of 2011. The project was named Korea VLBI system for Geodesy (KVG), and its main purpose is to maintain the Korea Geodetic Datum. In case of the KVG system, an observation room with an H-maser <span class="hlt">frequency</span> standard is located in a building <span class="hlt">separated</span> from the antenna by several tens of meters. Therefore KVG system will adopt a so-called round-trip system to transmit reference signals to the antenna with reduction of the effect of path length <span class="hlt">variations</span>. KVG s round-trip system is designed not only to use either metal or optical fiber cables, but also to measure path length <span class="hlt">variations</span> directly. We present this unique round trip system for KVG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28428539','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28428539"><span><span class="hlt">Separating</span> decadal global water cycle variability from sea level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hamlington, B D; Reager, J T; Lo, M-H; Karnauskas, K B; Leben, R R</p> <p>2017-04-20</p> <p>Under a warming climate, amplification of the water cycle and changes in precipitation patterns over land are expected to occur, subsequently impacting the terrestrial water balance. On global scales, such changes in terrestrial water storage (TWS) will be reflected in the water contained in the ocean and can manifest as global sea level <span class="hlt">variations</span>. Naturally occurring climate-driven TWS variability can temporarily obscure the long-term trend in sea level rise, in addition to modulating the impacts of sea level rise through natural periodic undulation in regional and global sea level. The internal variability of the global water cycle, therefore, confounds both the detection and attribution of sea level rise. Here, we use a suite of observations to quantify and map the contribution of TWS variability to sea level variability on decadal timescales. In particular, we find that decadal sea level variability centered in the Pacific Ocean is closely tied to low <span class="hlt">frequency</span> variability of TWS in key areas across the globe. The unambiguous identification and clean <span class="hlt">separation</span> of this component of variability is the missing step in uncovering the anthropogenic trend in sea level and understanding the potential for low-<span class="hlt">frequency</span> modulation of future TWS impacts including flooding and drought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090029265','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090029265"><span>Dual-Polarization, Sideband-<span class="hlt">Separating</span>, Balanced Receiver for 1.5 THz</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chattopadhyay, Goutman; Ward, John; Manohara, Harish; Siegel, Peter</p> <p>2009-01-01</p> <p>A proposed heterodyne receiver would be capable of detecting electromagnetic radiation in both of two orthogonal linear polarizations, <span class="hlt">separating</span> sidebands, and providing balanced outputs in a <span class="hlt">frequency</span> band centered at 1.5 THz with a fractional bandwidth greater than 40 percent. Dual polarization, sideband-<span class="hlt">separating</span>, and balanced-output receivers are well-known and have been used extensively at <span class="hlt">frequencies</span> up to about 100 GHz; and there was an earlier proposal for such a receiver for <span class="hlt">frequencies</span> up to 900 GHz. However, the present proposal represents the first realistic design concept for such a receiver capable of operating above 1 THz. The proposed receiver is intended to be a prototype of mass-producible receiver units, operating at <span class="hlt">frequencies</span> up to 6 THz, that would be incorporated into highly sensitive heterodyne array instruments to be used in astronomical spectroscopic and imaging studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1038967','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1038967"><span>Signal Identification and Isolation Utilizing Radio <span class="hlt">Frequency</span> Photonics</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-09-01</p> <p>analyzers can measure the <span class="hlt">frequency</span> of signals and filters can be used to <span class="hlt">separate</span> the signals apart from one another. This report will review...different techniques for spectrum analysis and isolation. 15. SUBJECT TERMS radio <span class="hlt">frequency</span>, photonics, spectrum analyzer, filters 16. SECURITY CLASSIFICATION...Analyzers .......................................................................................... 3 3.2 <span class="hlt">Frequency</span> Identification using Filters</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3403690','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3403690"><span>School-Based Racial and Gender Discrimination among African American Adolescents: Exploring Gender <span class="hlt">Variation</span> in <span class="hlt">Frequency</span> and Implications for Adjustment</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chavous, Tabbye M.; Griffin, Tiffany M.</p> <p>2012-01-01</p> <p>The present study examined school-based racial and gender discrimination experiences among African American adolescents in Grade 8 (n = 204 girls; n = 209 boys). A primary goal was exploring gender <span class="hlt">variation</span> in <span class="hlt">frequency</span> of both types of discrimination and associations of discrimination with academic and psychological functioning among girls and boys. Girls and boys did not vary in reported racial discrimination <span class="hlt">frequency</span>, but boys reported more gender discrimination experiences. Multiple regression analyses within gender groups indicated that among girls and boys, racial discrimination and gender discrimination predicted higher depressive symptoms and school importance and racial discrimination predicted self-esteem. Racial and gender discrimination were also negatively associated with grade point average among boys but were not significantly associated in girls’ analyses. Significant gender discrimination X racial discrimination interactions resulted in the girls’ models predicting psychological outcomes and in boys’ models predicting academic achievement. Taken together, findings suggest the importance of considering gender- and race-related experiences in understanding academic and psychological adjustment among African American adolescents. PMID:22837794</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23290479','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23290479"><span>Water-fat <span class="hlt">separation</span> with parallel imaging based on BLADE.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weng, Dehe; Pan, Yanli; Zhong, Xiaodong; Zhuo, Yan</p> <p>2013-06-01</p> <p>Uniform suppression of fat signal is desired in clinical applications. Based on phase differences introduced by different chemical shift <span class="hlt">frequencies</span>, Dixon method and its <span class="hlt">variations</span> are used as alternatives of fat saturation methods, which are sensitive to B0 inhomogeneities. Iterative Decomposition of water and fat with Echo Asymmetry and Least squares estimation (IDEAL) <span class="hlt">separates</span> water and fat images with flexible echo shifting. Periodically Rotated Overlapping ParallEL Lines with Enhanced Reconstruction (PROPELLER, alternatively termed as BLADE), in conjunction with IDEAL, yields Turboprop IDEAL (TP-IDEAL) and allows for decomposition of water and fat signal with motion correction. However, the flexibility of its parameter setting is limited, and the related phase correction is complicated. To address these problems, a novel method, BLADE-Dixon, is proposed in this study. This method used the same polarity readout gradients (fly-back gradients) to acquire in-phase and opposed-phases images, which led to less complicated phase correction and more flexible parameter setting compared to TP-IDEAL. Parallel imaging and undersampling were integrated to reduce scan time. Phantom, orbit, neck and knee images were acquired with BLADE-Dixon. Water-fat <span class="hlt">separation</span> results were compared to those measured with conventional turbo spin echo (TSE) Dixon and TSE with fat saturation, respectively, to demonstrate the performance of BLADE-Dixon. Copyright © 2013 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22280581','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22280581"><span>Time-<span class="hlt">frequency</span> analysis of the bistatic acoustic scattering from a spherical elastic shell.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Anderson, Shaun D; Sabra, Karim G; Zakharia, Manell E; Sessarego, Jean-Pierre</p> <p>2012-01-01</p> <p>The development of low-<span class="hlt">frequency</span> sonar systems, using, for instance, a network of autonomous systems in unmanned vehicles, provides a practical means for bistatic measurements (i.e., when the source and receiver are widely <span class="hlt">separated</span>) allowing for multiple viewpoints of the target of interest. Time-<span class="hlt">frequency</span> analysis, in particular, Wigner-Ville analysis, takes advantage of the evolution time dependent aspect of the echo spectrum to differentiate a man-made target, such as an elastic spherical shell, from a natural object of the similar shape. A key energetic feature of fluid-loaded and thin spherical shell is the coincidence pattern, also referred to as the mid-<span class="hlt">frequency</span> enhancement (MFE), that results from antisymmetric Lamb-waves propagating around the circumference of the shell. This article investigates numerically the bistatic <span class="hlt">variations</span> of the MFE with respect to the monostatic configuration using the Wigner-Ville analysis. The observed time-<span class="hlt">frequency</span> shifts of the MFE are modeled using a previously derived quantitative ray theory by Zhang et al. [J. Acoust. Soc. Am. 91, 1862-1874 (1993)] for spherical shell's scattering. Additionally, the advantage of an optimal array beamformer, based on joint time delays and <span class="hlt">frequency</span> shifts is illustrated for enhancing the detection of the MFE recorded across a bistatic receiver array when compared to a conventional time-delay beamformer. © 2012 Acoustical Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040088046&hterms=pacemaker&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dpacemaker','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040088046&hterms=pacemaker&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dpacemaker"><span><span class="hlt">Separation</span> of circadian and wake duration-dependent modulation of EEG activation during wakefulness</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cajochen, C.; Wyatt, J. K.; Czeisler, C. A.; Dijk, D. J.</p> <p>2002-01-01</p> <p>The <span class="hlt">separate</span> contribution of circadian rhythmicity and elapsed time awake on electroencephalographic (EEG) activity during wakefulness was assessed. Seven men lived in an environmental scheduling facility for 4 weeks and completed fourteen 42.85-h 'days', each consisting of an extended (28.57-h) wake episode and a 14.28-h sleep opportunity. The circadian rhythm of plasma melatonin desynchronized from the 42.85-h day. This allowed quantification of the <span class="hlt">separate</span> contribution of circadian phase and elapsed time awake to <span class="hlt">variation</span> in EEG power spectra (1-32 Hz). EEG activity during standardized behavioral conditions was markedly affected by both circadian phase and elapsed time awake in an EEG <span class="hlt">frequency</span>- and derivation-specific manner. The nadir of the circadian rhythm in alpha (8-12 Hz) activity in both fronto-central and occipito-parietal derivations occurred during the biological night, close to the crest of the melatonin rhythm. The nadir of the circadian rhythm of theta (4.5-8 Hz) and beta (20-32 Hz) activity in the fronto-central derivation was located close to the onset of melatonin secretion, i.e. during the wake maintenance zone. As time awake progressed, delta <span class="hlt">frequency</span> (1-4.5 Hz) and beta (20-32 Hz) activity rose monotonically in frontal derivations. The interaction between the circadian and wake-dependent increase in frontal delta was such that the intrusion of delta was minimal when sustained wakefulness coincided with the biological day, but pronounced during the biological night. Our data imply that the circadian pacemaker facilitates frontal EEG activation during the wake maintenance zone, by generating an arousal signal that prevents the intrusion of low-<span class="hlt">frequency</span> EEG components, the propensity for which increases progressively during wakefulness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JFS....40..233D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JFS....40..233D"><span>Unsteady <span class="hlt">separation</span> and vortex shedding from a laminar <span class="hlt">separation</span> bubble over a bluff body</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, S. P.; Srinivasan, U.; Arakeri, J. H.</p> <p>2013-07-01</p> <p>Boundary layers are subject to favorable and adverse pressure gradients because of both the temporal and spatial components of the pressure gradient. The adverse pressure gradient may cause the flow to <span class="hlt">separate</span>. In a closed loop unsteady tunnel we have studied the initiation of <span class="hlt">separation</span> in unsteady flow past a constriction (bluff body) in a channel. We have proposed two important scalings for the time when boundary layer <span class="hlt">separates</span>. One is based on the local pressure gradient and the other is a convective time scale based on boundary layer parameters. The flow visualization using a dye injection technique shows the flow structure past the body. Nondimensional shedding <span class="hlt">frequency</span> (Strouhal number) is calculated based on boundary layer and momentum thicknesses. Strouhal number based on the momentum thickness shows a close agreement with that for flat plate and circular cylinder.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880014582','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880014582"><span>Acoustic emission <span class="hlt">frequency</span> discrimination</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sugg, Frank E. (Inventor); Graham, Lloyd J. (Inventor)</p> <p>1988-01-01</p> <p>In acoustic emission nondestructive testing, broadband <span class="hlt">frequency</span> noise is distinguished from narrow banded acoustic emission signals, since the latter are valid events indicative of structural flaws in the material being examined. This is accomplished by <span class="hlt">separating</span> out those signals which contain <span class="hlt">frequency</span> components both within and beyond (either above or below) the range of valid acoustic emission events. Application to acoustic emission monitoring during nondestructive bond verification and proof loading of undensified tiles on the Space Shuttle Orbiter is considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JASTP..66.1179P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JASTP..66.1179P"><span>Diurnal, seasonal and inter-annual <span class="hlt">variations</span> in the Schumann resonance parameters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Price, Colin; Melnikov, Alexander</p> <p>2004-09-01</p> <p>The Schumann resonances (SR) represent an electromagnetic phenomenon in the Earth's atmosphere related to global lightning activity. The spectral characteristics of the SR modes are defined by their resonant mode amplitude, center <span class="hlt">frequency</span> and half-width (Q-factor). Long-term (4 years) diurnal and seasonal <span class="hlt">variations</span> of these parameters are presented based on measurements at a field site in the Negev desert, Israel. <span class="hlt">Variations</span> of the different modes (8, 14 and 20Hz) and the different electromagnetic components (Hns, Hew and Ez) are presented. The power <span class="hlt">variations</span> of the various modes and components show three dominant maxima in the diurnal cycle related to lightning activity in south-east Asia (0800UT), Africa (1400UT) and South America (2000UT). The largest global lightning activity occurs during the northern hemisphere summer (JJA) with the southern hemisphere summer (DJF) having the least lightning around the globe. The <span class="hlt">frequency</span> and half-width (Q-factor) <span class="hlt">variations</span> of the different modes and SR components are fairly complicated in structure, and will need additional theoretical work to explain their <span class="hlt">variations</span>. However, the <span class="hlt">frequency</span> <span class="hlt">variations</span> are in excellent agreement with previous studies, implying that the <span class="hlt">frequency</span> <span class="hlt">variations</span> are robust features of the SR. The inter-annual variability of global lightning activity is shown to vary differently for each of the three major source regions of global lightning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI11B..01P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI11B..01P"><span>Local <span class="hlt">Variations</span> in the Upper-Mantle Transition Zone Structure From a Novel Approach Using High-<span class="hlt">Frequency</span> Triplication Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, S.; Ishii, M.</p> <p>2017-12-01</p> <p>Constraining elastic properties of the 410- and 660-km discontinuities is vital for understanding the mantle composition and dynamics. One approach to study the transition zone is to use the "triplicated" arrivals of seismic data. These arrivals consist of three seismic phases that are sensitive to seismic structure slightly above, at, and below the discontinuity. Therefore, these data provide powerful constraints on the depth, width, and magnitude of velocity jump of the discontinuities with consequences for the studies of mantle composition, relevant phase transitions, and dynamics. Nevertheless, one of the most challenging aspects of using the triplication data is to identify the three individual phases that arrive close in time. In order to <span class="hlt">separate</span> the three phases, we apply Radon transform to short-period seismograms recorded by a dense array of stations. This approach unwraps the triplication pattern, and brings out the high-<span class="hlt">frequency</span> information that is not easily accessible in the original form of data. This method is applied to study the transition zone around the Kuril subduction zone, a region northeast of Japan. We take advantage of the High-Sensitivity Seismograph Network in Japan comprised of more than 700 stations whose dense sampling in distance allows us to capture the triplication pattern. The data are processed to obtain the <span class="hlt">variations</span> in wave speeds around the discontinuities, i.e., at 410±100 and 660±100 km, resulting in models of topography and sharpness of discontinuities at various sampling locations. Both discontinuities exhibit local topography undulations consistent with the temperature effect; the 410- and 660-km discontinuities become shallower and deeper, respectively, nearer to the slab. Additional discontinuities around 660 km are also detected, which may be attributed to the garnet transitions occurring at similar depths as the post-spinel transition. The 410-km discontinuity is observed to be more diffuse than 660-km</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29067977','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29067977"><span>Genetic <span class="hlt">variations</span> in the Dravidian population of South West coast of India: Implications in designing case-control studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>D'Cunha, Anitha; Pandit, Lekha; Malli, Chaithra</p> <p>2017-06-01</p> <p>Indian data have been largely missing from genome-wide databases that provide information on genetic <span class="hlt">variations</span> in different populations. This hinders association studies for complex disorders in India. This study was aimed to determine whether the complex genetic structure and endogamy among Indians could potentially influence the design of case-control studies for autoimmune disorders in the south Indian population. A total of 12 single nucleotide <span class="hlt">variations</span> (SNVs) related to genes associated with autoimmune disorders were genotyped in 370 healthy individuals belonging to six different caste groups in southern India. Allele <span class="hlt">frequencies</span> were estimated; genetic divergence and phylogenetic relationship within the various caste groups and other HapMap populations were ascertained. Allele <span class="hlt">frequencies</span> for all genotyped SNVs did not vary significantly among the different groups studied. Wright's FSTwas 0.001 per cent among study population and 0.38 per cent when compared with Gujarati in Houston (GIH) population on HapMap data. The analysis of molecular variance results showed a 97 per cent <span class="hlt">variation</span> attributable to differences within the study population and <1 per cent <span class="hlt">variation</span> due to differences between castes. Phylogenetic analysis showed a <span class="hlt">separation</span> of Dravidian population from other HapMap populations and particularly from GIH population. Despite the complex genetic origins of the Indian population, our study indicated a low level of genetic differentiation among Dravidian language-speaking people of south India. Case-control studies of association among Dravidians of south India may not require stratification based on language and caste.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001fmce.conf..249R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001fmce.conf..249R"><span>Optical <span class="hlt">Frequency</span> Measurements Relying on a Mid-Infrared <span class="hlt">Frequency</span> Standard</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rovera, G. Daniele; Acef, Ouali</p> <p></p> <p>Only a small number of groups are capable of measuring optical <span class="hlt">frequencies</span> throughout the world. In this contribution we present some of the underlying philosophy of such <span class="hlt">frequency</span> measurement systems, including some important theoretical hints. In particular, we concentrate on the approach that has been used with the BNM-LPTF <span class="hlt">frequency</span> chain, where a <span class="hlt">separate</span> secondary <span class="hlt">frequency</span> standard in the mid-infrared has been used. The low-<span class="hlt">frequency</span> section of the chain is characterized by a measurement of the phase noise spectral density Sφ at 716GHz.Most of the significant measurements performed in the last decade are briefly presented, together with a report on the actual stability and reproducibility of the <!- MATH CO_2 / OsO_4 -> CO2/ OsO4 <span class="hlt">frequency</span> standard.Measuring the <span class="hlt">frequency</span> of an optical <span class="hlt">frequency</span> standard by direct comparison with the signal available at the output of a primary <span class="hlt">frequency</span> standard (usually between 5MHz and 100MHz) requires a multiplication factor greater than 107. A number of possible configurations, using harmonic generation, sum or difference <span class="hlt">frequency</span> generation, have been proposed and realized in the past [1,2,3,4,5,6] and in more recent times [7]. A new technique, employing a femtosecond laser, is presently giving its first impressive results [8].All of the classical <span class="hlt">frequency</span> chains require a large amount of manpower, together with a great deal of simultaneously operating hardware. This has the consequence that only a very few systems are actually in an operating condition throughout the world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA541675','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA541675"><span>Modeling and <span class="hlt">Frequency</span> Tracking of Marine Mammal Whistle Calls</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2009-02-01</p> <p>retrieve em- bedded information from watermarked synthetic whistle calls. Different fundamental <span class="hlt">frequency</span> watermarking schemes are proposed b&𔃽ed on...unmodified <span class="hlt">frequency</span> contour is relatively constant, there is little <span class="hlt">frequency</span> <span class="hlt">separation</span> between information bits, and watermark retrieval requires...UHYLHZLQJWKHFROOHFWLRQRILQIRUPDWLRQ6HQGFRPPHQWVUHJDUGLQJWKLVEXUGHQHVWLPDWH RU DQ\\RWKHUDVSHFWRIWKLVFROOHFWLRQ RI LQIRUPDWLRQ LQFOXGLQJ</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24558468','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24558468"><span>Modelling of human low <span class="hlt">frequency</span> sound localization acuity demonstrates dominance of spatial <span class="hlt">variation</span> of interaural time difference and suggests uniform just-noticeable differences in interaural time difference.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Smith, Rosanna C G; Price, Stephen R</p> <p>2014-01-01</p> <p>Sound source localization is critical to animal survival and for identification of auditory objects. We investigated the acuity with which humans localize low <span class="hlt">frequency</span>, pure tone sounds using timing differences between the ears. These small differences in time, known as interaural time differences or ITDs, are identified in a manner that allows localization acuity of around 1° at the midline. Acuity, a relative measure of localization ability, displays a non-linear <span class="hlt">variation</span> as sound sources are positioned more laterally. All species studied localize sounds best at the midline and progressively worse as the sound is located out towards the side. To understand why sound localization displays this <span class="hlt">variation</span> with azimuthal angle, we took a first-principles, systemic, analytical approach to model localization acuity. We calculated how ITDs vary with sound <span class="hlt">frequency</span>, head size and sound source location for humans. This allowed us to model ITD <span class="hlt">variation</span> for previously published experimental acuity data and determine the distribution of just-noticeable differences in ITD. Our results suggest that the best-fit model is one whereby just-noticeable differences in ITDs are identified with uniform or close to uniform sensitivity across the physiological range. We discuss how our results have several implications for neural ITD processing in different species as well as development of the auditory system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28690505','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28690505"><span>Evidence for <span class="hlt">Separate</span> Contributions of High and Low Spatial <span class="hlt">Frequencies</span> during Visual Word Recognition.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Winsler, Kurt; Holcomb, Phillip J; Midgley, Katherine J; Grainger, Jonathan</p> <p>2017-01-01</p> <p>Previous studies have shown that different spatial <span class="hlt">frequency</span> information processing streams interact during the recognition of visual stimuli. However, it is a matter of debate as to the contributions of high and low spatial <span class="hlt">frequency</span> (HSF and LSF) information for visual word recognition. This study examined the role of different spatial <span class="hlt">frequencies</span> in visual word recognition using event-related potential (ERP) masked priming. EEG was recorded from 32 scalp sites in 30 English-speaking adults in a go/no-go semantic categorization task. Stimuli were white characters on a neutral gray background. Targets were uppercase five letter words preceded by a forward-mask (#######) and a 50 ms lowercase prime. Primes were either the same word (repeated) or a different word (un-repeated) than the subsequent target and either contained only high, only low, or full spatial <span class="hlt">frequency</span> information. Additionally within each condition, half of the prime-target pairs were high lexical <span class="hlt">frequency</span>, and half were low. In the full spatial <span class="hlt">frequency</span> condition, typical ERP masked priming effects were found with an attenuated N250 (sub-lexical) and N400 (lexical-semantic) for repeated compared to un-repeated primes. For HSF primes there was a weaker N250 effect which interacted with lexical <span class="hlt">frequency</span>, a significant reversal of the effect around 300 ms, and an N400-like effect for only high lexical <span class="hlt">frequency</span> word pairs. LSF primes did not produce any of the classic ERP repetition priming effects, however they did elicit a distinct early effect around 200 ms in the opposite direction of typical repetition effects. HSF information accounted for many of the masked repetition priming ERP effects and therefore suggests that HSFs are more crucial for word recognition. However, LSFs did produce their own pattern of priming effects indicating that larger scale information may still play a role in word recognition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRA..122.7698S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRA..122.7698S"><span>Modeling of temporal <span class="hlt">variation</span> of very low <span class="hlt">frequency</span> radio waves over long paths as observed from Indian Antarctic stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sasmal, Sudipta; Basak, Tamal; Chakraborty, Suman; Palit, Sourav; Chakrabarti, Sandip K.</p> <p>2017-07-01</p> <p>Characteristics of very low <span class="hlt">frequency</span> (VLF) signal depends on solar illumination across the propagation path. For a long path, solar zenith angle varies widely over the path and this has a significant influence on the propagation characteristics. To study the effect, Indian Centre for Space Physics participated in the 27th and 35th Scientific Expedition to Antarctica. VLF signals transmitted from the transmitters, namely, VTX (18.2 kHz), Vijayanarayanam, India, and NWC (19.8 kHz), North West Cape, Australia, were recorded simultaneously at Indian permanent stations Maitri and Bharati having respective geographic coordinates 70.75°S, 11.67°E, and 69.4°S, 76.17°E. A very stable diurnal <span class="hlt">variation</span> of the signal has been obtained from both the stations. We reproduced the signal <span class="hlt">variations</span> of VLF signal using solar zenith angle model coupled with long wavelength propagation capability (LWPC) code. We divided the whole path into several segments and computed the solar zenith angle (χ) profile. We assumed a linear relationship between the Wait's exponential model parameters effective reflection height (h'), steepness parameter (β), and solar zenith angle. The h' and β values were later used in the LWPC code to obtain the VLF signal amplitude at a particular time. The same procedure was repeated to obtain the whole day signal. Nature of the whole day signal <span class="hlt">variation</span> from the theoretical modeling is also found to match with our observation to some extent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880001649','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880001649"><span>Grace DAKASEP alkaline battery <span class="hlt">separator</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Giovannoni, R. T.; Lundquist, J. T.; Choi, W. M.</p> <p>1987-01-01</p> <p>The Grace DAKASEP <span class="hlt">separator</span> was originally developed as a wicking layer for nickel-zinc alkaline batteries. The DAKASEP is a filled non-woven <span class="hlt">separator</span> which is flexible and heat sealable. Through modification of formulation and processing variables, products with a variety of properties can be produced. <span class="hlt">Variations</span> of DAKASEP were tested in Ni-H2, Ni-Zn, Ni-Cd, and primary alkaline batteries with good results. The properties of DAKASEP which are optimized for Hg-Zn primary batteries are shown in tabular form. This <span class="hlt">separator</span> has high tensile strength, 12 micron average pore size, relatively low porosity at 46-48 percent, and consequently moderately high resistivity. Versions were produced with greater than 70 percent porosity and resistivities in 33 wt percent KOH as low as 3 ohm cm. Performance data for Hg-Zn E-1 size cells containing DAKASEP with the properties shown in tabular form, are more reproducible than data obtained with a competitive polypropylene non-woven <span class="hlt">separator</span>. In addition, utilization of active material is in general considerably improved.</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('https://www.ncbi.nlm.nih.gov/pubmed/18238499','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18238499"><span>Use of GPS ASHTECH Z12T receivers for accurate time and <span class="hlt">frequency</span> comparisons.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Petit, G; Thomas, C; Jiang, Z; Uhrich, P; Taris, F</p> <p>1999-01-01</p> <p>The GPS phase measurements described in this paper were obtained using two similar multichannel GPS ASHTECH Z12T receivers belonging to the Bureau International des Poids et Mesures, BIPM, and the Laboratoire Primaire du Temps et des <span class="hlt">Frequences</span>, BNM-LPTF. These receivers are based on the conventional geodetic ASHTECH Z12 unit, which has been modified to meet the stability requirements of time and <span class="hlt">frequency</span> comparisons. Comparison of the two receivers operated side by side in different antenna configurations shows typical short-term noise of 1.1 to 3.5 ps. Longer term <span class="hlt">variations</span> indicate a temperature sensitivity in the equipment, which limits the performance of the GPS phase method. One of the receivers was successfully operated using a temperature-stabilized antenna TSA from 3S Navigation, and the ASHTECH antenna, which feeds the second receiver, was placed in a home-built oven maintained at a constant temperature. These precautions made it possible to reduce a number of systematic effects. A <span class="hlt">separate</span> study of <span class="hlt">frequency</span> comparison was carried out between two hydrogen-masers located at the BNM-LPTF (Paris, France) and the PTB (Braunschweig, Germany) using receivers similar to ASHTECH Z12T receivers. The relative <span class="hlt">frequency</span> stability obtained was about 3.3x10(-15) for an average time of 15 000 s, an interesting result comparable with the outstanding performance of new ultrastable <span class="hlt">frequency</span> standards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090032090','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090032090"><span>Estimating Transmitted-Signal Phase <span class="hlt">Variations</span> for Uplink Array Antennas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Paal, Leslie; Mukai, Ryan; Vilntrotter, Victor; Cornish, Timothy; Lee, Dennis</p> <p>2009-01-01</p> <p>A method of estimating phase drifts of microwave signals distributed to, and transmitted by, antennas in an array involves the use of the signals themselves as phase references. The method was conceived as part of the solution of the problem of maintaining precise phase calibration required for proper operation of an array of Deep Space Network (DSN) antennas on Earth used for communicating with distant spacecraft at <span class="hlt">frequencies</span> between 7 and 8 GHz. The method could also be applied to purely terrestrial phased-array radar and other radio antenna array systems. In the DSN application, the electrical lengths (effective signal-propagation path lengths) of the various branches of the system for distributing the transmitted signals to the antennas are not precisely known, and they vary with time. The <span class="hlt">variations</span> are attributable mostly to thermal expansion and contraction of fiber-optic and electrical signal cables and to a variety of causes associated with aging of signal-handling components. The <span class="hlt">variations</span> are large enough to introduce large phase drifts at the signal <span class="hlt">frequency</span>. It is necessary to measure and correct for these phase drifts in order to maintain phase calibration of the antennas. A prior method of measuring phase drifts involves the use of reference-<span class="hlt">frequency</span> signals <span class="hlt">separate</span> from the transmitted signals. A major impediment to accurate measurement of phase drifts over time by the prior method is the fact that although DSN reference-<span class="hlt">frequency</span> sources <span class="hlt">separate</span> from the transmitting signal sources are stable and accurate enough for most DSN purposes, they are not stable enough for use in maintaining phase calibrations, as required, to within a few degrees over times as long as days or possibly even weeks. By eliminating reliance on the reference-<span class="hlt">frequency</span> subsystem, the present method overcomes this impediment. In a DSN array to which the present method applies (see figure), the microwave signals to be transmitted are generated by exciters in a signal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100036538','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100036538"><span>Robust Optimization Design Algorithm for High-<span class="hlt">Frequency</span> TWTs</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wilson, Jeffrey D.; Chevalier, Christine T.</p> <p>2010-01-01</p> <p>Traveling-wave tubes (TWTs), such as the Ka-band (26-GHz) model recently developed for the Lunar Reconnaissance Orbiter, are essential as communication amplifiers in spacecraft for virtually all near- and deep-space missions. This innovation is a computational design algorithm that, for the first time, optimizes the efficiency and output power of a TWT while taking into account the effects of dimensional tolerance <span class="hlt">variations</span>. Because they are primary power consumers and power generation is very expensive in space, much effort has been exerted over the last 30 years to increase the power efficiency of TWTs. However, at <span class="hlt">frequencies</span> higher than about 60 GHz, efficiencies of TWTs are still quite low. A major reason is that at higher <span class="hlt">frequencies</span>, dimensional tolerance <span class="hlt">variations</span> from conventional micromachining techniques become relatively large with respect to the circuit dimensions. When this is the case, conventional design- optimization procedures, which ignore dimensional <span class="hlt">variations</span>, provide inaccurate designs for which the actual amplifier performance substantially under-performs that of the design. Thus, this new, robust TWT optimization design algorithm was created to take account of and ameliorate the deleterious effects of dimensional <span class="hlt">variations</span> and to increase efficiency, power, and yield of high-<span class="hlt">frequency</span> TWTs. This design algorithm can help extend the use of TWTs into the terahertz <span class="hlt">frequency</span> regime of 300-3000 GHz. Currently, these <span class="hlt">frequencies</span> are under-utilized because of the lack of efficient amplifiers, thus this regime is known as the "terahertz gap." The development of an efficient terahertz TWT amplifier could enable breakthrough applications in space science molecular spectroscopy, remote sensing, nondestructive testing, high-resolution "through-the-wall" imaging, biomedical imaging, and detection of explosives and toxic biochemical agents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004ASAJ..115..324B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ASAJ..115..324B"><span><span class="hlt">Separation</span> of concurrent broadband sound sources by human listeners</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Best, Virginia; van Schaik, André; Carlile, Simon</p> <p>2004-01-01</p> <p>The effect of spatial <span class="hlt">separation</span> on the ability of human listeners to resolve a pair of concurrent broadband sounds was examined. Stimuli were presented in a virtual auditory environment using individualized outer ear filter functions. Subjects were presented with two simultaneous noise bursts that were either spatially coincident or <span class="hlt">separated</span> (horizontally or vertically), and responded as to whether they perceived one or two source locations. Testing was carried out at five reference locations on the audiovisual horizon (0°, 22.5°, 45°, 67.5°, and 90° azimuth). Results from experiment 1 showed that at more lateral locations, a larger horizontal <span class="hlt">separation</span> was required for the perception of two sounds. The reverse was true for vertical <span class="hlt">separation</span>. Furthermore, it was observed that subjects were unable to <span class="hlt">separate</span> stimulus pairs if they delivered the same interaural differences in time (ITD) and level (ILD). These findings suggested that the auditory system exploited differences in one or both of the binaural cues to resolve the sources, and could not use monaural spectral cues effectively for the task. In experiments 2 and 3, <span class="hlt">separation</span> of concurrent noise sources was examined upon removal of low-<span class="hlt">frequency</span> content (and ITDs), onset/offset ITDs, both of these in conjunction, and all ITD information. While onset and offset ITDs did not appear to play a major role, differences in ongoing ITDs were robust cues for <span class="hlt">separation</span> under these conditions, including those in the envelopes of high-<span class="hlt">frequency</span> channels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4590873','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4590873"><span>Seasonal <span class="hlt">Variation</span> and <span class="hlt">Frequency</span> Distribution of Ectoparasites in Crossbreed Cattle in Southeastern Brazil</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ferraz da Costa, Maria do Socorro; Guimarães, Marcos Pezzi; Lima, Walter dos Santos; Ferraz da Costa, Ana Julia; Facury Filho, Elias Jorge; Araujo, Ricardo Nascimento</p> <p>2014-01-01</p> <p>The aims of this study were to evaluate the seasonal <span class="hlt">variation</span> and <span class="hlt">frequency</span> distribution of Rhipicephalus (Boophilus) microplus, Haematobia irritans, and Dermatobia hominis on crossbred heifers under field conditions in the northeast of Minas Gerais state, southeastern Brazil. From November 2007 to September 2009 (23 months), 40 heifers aged 16.6 ± 2.4 months were divided into groups A (1/4 Holstein × 3/4 Gir) and B (1/2 Holstein × 1/2 Gir) and had the monthly infestation estimated along with the climatic conditions. The mean maximum and minimum temperatures were 28.5 and 19°C, respectively. The ectoparasites were present on animals in all months of the year. The levels of ticks on the animals were low (3.0 ± 0.2 ticks/animal), with the highest density in midwinter. The temperature was the climatic factor that most influenced the tick levels. The population of H. irritans (13.9 ± 0.3 flies/animal) and D. hominis (1.5 ± 0.2 larvae/animal) on heifers was more influenced by rainfall and exhibited two population peaks during the year. 1/2 Holstein heifers harbored significantly more H. irritans and D. hominis than 1/4 Holstein heifers. The results are discussed considering the most appropriate periods to apply ectoparasiticides and the genetic make-up of the animals. PMID:26464941</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ArtSa..52...19F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ArtSa..52...19F"><span><span class="hlt">Variation</span> of Static-PPP Positioning Accuracy Using GPS-Single <span class="hlt">Frequency</span> Observations (Aswan, Egypt)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farah, Ashraf</p> <p>2017-06-01</p> <p>Precise Point Positioning (PPP) is a technique used for position computation with a high accuracy using only one GNSS receiver. It depends on highly accurate satellite position and clock data rather than broadcast ephemeries. PPP precision varies based on positioning technique (static or kinematic), observations type (single or dual <span class="hlt">frequency</span>) and the duration of collected observations. PPP-(dual <span class="hlt">frequency</span> receivers) offers comparable accuracy to differential GPS. PPP-single <span class="hlt">frequency</span> receivers has many applications such as infrastructure, hydrography and precision agriculture. PPP using low cost GPS single-<span class="hlt">frequency</span> receivers is an area of great interest for millions of users in developing countries such as Egypt. This research presents a study for the variability of single <span class="hlt">frequency</span> static GPS-PPP precision based on different observation durations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840027015','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840027015"><span>The calculation of molecular Eigen-<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>Lindemann, F. A.</p> <p>1984-01-01</p> <p>A method of determining molecular eigen-<span class="hlt">frequencies</span> based on the function of Einstein expressing the <span class="hlt">variation</span> of the atomic heat of various elements is proposed. It is shown that the same equation can be utilized to calculate both atomic heat and optically identifiably eigen-<span class="hlt">frequencies</span> - at least to an order of magnitude - suggesting that in both cases the same oscillating structure is responsible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1514246J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1514246J"><span>High <span class="hlt">frequency</span> <span class="hlt">variations</span> of the main magnetic field: convergence of observations and theory (Petrus Peregrinus Medal Lecture)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jault, Dominique</p> <p>2013-04-01</p> <p>Understanding the main magnetic field <span class="hlt">variations</span> has been hindered by the discrepancy between the periods (from months to years) of the simplest linear wave phenomena and the relatively long time intervals (10 to 100 years) over which magnetic field changes can be confidently monitored. A theoretical description of short-period waves within the Earth's fluid core is at hand. Quasi-geostrophic inertial waves (akin to Rossby waves in the atmosphere) are slightly modified in the presence of magnetic fields and torsional oscillations consist of differential motion between coaxial rigid cylindrical annuli. Torsional oscillations are sensitive to the whole magnetic field that they shear in the course of their propagation. From their modelling, we have thus gained an estimate for the magnetic field strength in the core interior. There is now ongoing work to extend the theoretical framework to longer times. Furthermore, data collected from the Swarm constellation of three satellites to be launched this year by ESA will permit to better <span class="hlt">separate</span> the internal and external magnetic signals. We may thus dream to detect quasi-geostrophic inertial waves. As the spectral ranges of theoretical models and observations begin to overlap, we can now go beyond the understanding of the magnetic field <span class="hlt">variations</span> as the juxtaposition of partial models, arranged as a set of nested Matryoshka dolls. This talk will give illustrations for this statement, among which the question of induction in the lower mantle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2752304','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2752304"><span>High-speed polarization sensitive optical <span class="hlt">frequency</span> domain imaging with <span class="hlt">frequency</span> multiplexing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yun, S.H.; Vakoc, B.J.; Shishkov, M.; Desjardins, A.E.; Park, B.H.; de Boer, J.F.; Tearney, G.J.; Bouma, B.E.</p> <p>2009-01-01</p> <p>Polarization sensitive optical coherence tomography (PS-OCT) provides a cross-sectional image of birefringence in biological samples that is complementary in many applications to the standard reflectance-based image. Recent ex vivo studies have demonstrated that birefringence mapping enables the characterization of collagen and smooth muscle concentration and distribution in vascular tissues. Instruments capable of applying these measurements percutaneously in vivo may provide new insights into coronary atherosclerosis and acute myocardial infarction. We have developed a polarization sensitive optical <span class="hlt">frequency</span> domain imaging (PS-OFDI) system that enables high-speed intravascular birefringence imaging through a fiber-optic catheter. The novel design of this system utilizes <span class="hlt">frequency</span> multiplexing to simultaneously measure reflectance of two incident polarization states, overcoming concerns regarding temporal <span class="hlt">variations</span> of the catheter fiber birefringence and spatial <span class="hlt">variations</span> in the birefringence of the sample. We demonstrate circular cross-sectional birefringence imaging of a human coronary artery ex vivo through a flexible fiber-optic catheter with an A-line rate of 62 kHz and a ranging depth of 6.2 mm. PMID:18542183</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830001865','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830001865"><span>Polyvinyl alcohol membranes as alkaline battery <span class="hlt">separators</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sheibley, D. W.; Gonzalez-Sanabria, O.; Manzo, M. A.</p> <p>1982-01-01</p> <p>Polyvinly alcohol (PVA) cross-linked with aldehyde reagents yields membranes that demonstrate properties that make them suitable for use as alkaline battery <span class="hlt">separators</span>. Film properties can be controlled by the choice of cross-linker, cross-link density and the method of cross-linking. Three methods of cross-linking and their effects on film properties are discussed. Film properties can also be modified by using a copolymer of vinyl alcohol and acrylic acid as the base for the <span class="hlt">separator</span> and cross-linking it similarly to the PVA. Fillers can be incorporated into the films to further modify film properties. Results of <span class="hlt">separator</span> screening tests and cell tests for several <span class="hlt">variations</span> of PBA films are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/864305','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/864305"><span><span class="hlt">Frequency</span> regulator for synchronous generators</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Karlicek, Robert F.</p> <p>1982-01-01</p> <p>The present invention is directed to a novel <span class="hlt">frequency</span> regulator which controls a generator output <span class="hlt">frequency</span> for <span class="hlt">variations</span> in both the input power to the generator and the power supplied to an uncontrolled external load. The present invention further includes over current and current balance protection devices which are relatively inexpensive to manufacture, which may be encapsulated to provide protection from the operating environment and which respond more quickly than previously known electromechanical devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.16002013S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.16002013S"><span>On the relation between activity-related <span class="hlt">frequency</span> shifts and the sunspot distribution over the solar cycle 23</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santos, Ângela R. G.; Cunha, Margarida S.; Avelino, Pedro P.; Chaplin, William J.; Campante, Tiago L.</p> <p>2017-10-01</p> <p>The activity-related <span class="hlt">variations</span> in the solar acoustic <span class="hlt">frequencies</span> have been known for 30 years. However, the importance of the different contributions is still not well established. With this in mind, we developed an empirical model to estimate the spot-induced <span class="hlt">frequency</span> shifts, which takes into account the sunspot properties, such as area and latitude. The comparison between the model <span class="hlt">frequency</span> shifts obtained from the daily sunspot records and those observed suggests that the contribution from a stochastic component to the total <span class="hlt">frequency</span> shifts is about 30%. The remaining 70% is related to a global, long-term <span class="hlt">variation</span>. We also propose a new observable to investigate the short-and mid-term <span class="hlt">variations</span> of the <span class="hlt">frequency</span> shifts, which is insensitive to the long-term <span class="hlt">variations</span> contained in the data. On the shortest time scales the <span class="hlt">variations</span> in the <span class="hlt">frequency</span> shifts are strongly correlated with the <span class="hlt">variations</span> in the total area covered by sunspots. However, a significant loss of correlation is still found, which cannot be fully explained by ignoring the invisible side of the Sun when accounting for the total sunspot area. We also verify that the times when the <span class="hlt">frequency</span> shifts and the sunspot areas do not vary in a similar way tend to coincide with the times of the maximum amplitude of the quasi-biennial <span class="hlt">variations</span> found in the seismic data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AIPC.1703i0002S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AIPC.1703i0002S"><span>High-<span class="hlt">frequency</span> tone-pip-evoked otoacoustic emissions in chinchillas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siegel, Jonathan H.; Charaziak, Karolina K.</p> <p>2015-12-01</p> <p>We measured otoacoustic emissions in anesthetized chinchillas evoked by short (1 ms) high-<span class="hlt">frequency</span> (4 kHz) tone-pips (TEOAE) using either a compression or suppression method to <span class="hlt">separate</span> the stimulus from the emission. Both methods revealed consistent features of the TEOAEs. The main spectral band of the emission generally corresponded to the spectrum of the stimulus, exhibiting a group delay similar to that of SFOAEs [9]. However, a second spectral band below 1.5 kHz, clearly <span class="hlt">separated</span> from the low-<span class="hlt">frequency</span> cut-off <span class="hlt">frequency</span> of the stimulus spectrum, corresponded to an amplitude modulation of the waveform of the TEOAE. The group delay of this low-<span class="hlt">frequency</span> band was similar to that of the main band near the probe <span class="hlt">frequency</span>. The average level and group delay of the main band declined monotonically when revealed as the suppressor <span class="hlt">frequency</span> was raised above the probe. The low-<span class="hlt">frequency</span> band was more sensitive than the main band to shifts in compound action potential thresholds near the probe <span class="hlt">frequency</span> induced by acute exposure to intense tones. Taken together, the experiments indicate that both the main and low-<span class="hlt">frequency</span> bands of the TEOAE are generated primarily near the cochlear region maximally stimulated by the probe, but that significant contributions arise over a large region even more basal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016A%26A...594A..25P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016A%26A...594A..25P"><span>Planck 2015 results. XXV. Diffuse low-<span class="hlt">frequency</span> Galactic foregrounds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Planck Collaboration; Ade, P. A. R.; Aghanim, N.; Alves, M. I. R.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartlett, J. G.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoît, A.; Benoit-Lévy, A.; Bernard, J.-P.; Bersanelli, M.; Bielewicz, P.; Bock, J. J.; Bonaldi, A.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bucher, M.; Burigana, C.; Butler, R. C.; Calabrese, E.; Cardoso, J.-F.; Catalano, A.; Challinor, A.; Chamballu, A.; Chary, R.-R.; Chiang, H. C.; Christensen, P. R.; Colombi, S.; Colombo, L. P. L.; Combet, C.; Couchot, F.; Coulais, A.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J.; Delouis, J.-M.; Désert, F.-X.; Dickinson, C.; Diego, J. M.; Dole, H.; Donzelli, S.; Doré, O.; Douspis, M.; Ducout, A.; Dupac, X.; Efstathiou, G.; Elsner, F.; Enßlin, T. A.; Eriksen, H. K.; Falgarone, E.; Fergusson, J.; Finelli, F.; Forni, O.; Frailis, M.; Fraisse, A. A.; Franceschi, E.; Frejsel, A.; Galeotta, S.; Galli, S.; Ganga, K.; Ghosh, T.; Giard, M.; Giraud-Héraud, Y.; Gjerløw, E.; González-Nuevo, J.; Górski, K. M.; Gratton, S.; Gregorio, A.; Gruppuso, A.; Gudmundsson, J. E.; Hansen, F. K.; Hanson, D.; Harrison, D. L.; Helou, G.; Henrot-Versillé, S.; Hernández-Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hornstrup, A.; Hovest, W.; Huffenberger, K. M.; Hurier, G.; Jaffe, A. H.; Jaffe, T. R.; Jones, W. C.; Juvela, M.; Keihänen, E.; Keskitalo, R.; Kisner, T. S.; Kneissl, R.; Knoche, J.; Kunz, M.; Kurki-Suonio, H.; Lagache, G.; Lähteenmäki, A.; Lamarre, J.-M.; Lasenby, A.; Lattanzi, M.; Lawrence, C. R.; Leahy, J. P.; Leonardi, R.; Lesgourgues, J.; Levrier, F.; Liguori, M.; Lilje, P. B.; Linden-Vørnle, M.; López-Caniego, M.; Lubin, P. M.; Macías-Pérez, J. F.; Maggio, G.; Maino, D.; Mandolesi, N.; Mangilli, A.; Maris, M.; Marshall, D. J.; Martin, P. G.; Martínez-González, E.; Masi, S.; Matarrese, S.; McGehee, P.; Meinhold, P. R.; Melchiorri, A.; Mendes, L.; Mennella, A.; Migliaccio, M.; Mitra, S.; Miville-Deschênes, M.-A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Moss, A.; Munshi, D.; Murphy, J. A.; Nati, F.; Natoli, P.; Netterfield, C. B.; Nørgaard-Nielsen, H. U.; Noviello, F.; Novikov, D.; Novikov, I.; Orlando, E.; Oxborrow, C. A.; Paci, F.; Pagano, L.; Pajot, F.; Paladini, R.; Paoletti, D.; Partridge, B.; Pasian, F.; Patanchon, G.; Pearson, T. J.; Peel, M.; Perdereau, O.; Perotto, L.; Perrotta, F.; Pettorino, V.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Pratt, G. W.; Prézeau, G.; Prunet, S.; Puget, J.-L.; Rachen, J. P.; Reach, W. T.; Rebolo, R.; Reinecke, M.; Remazeilles, M.; Renault, C.; Renzi, A.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Rossetti, M.; Roudier, G.; Rubiño-Martín, J. A.; Rusholme, B.; Sandri, M.; Santos, D.; Savelainen, M.; Savini, G.; Scott, D.; Seiffert, M. D.; Shellard, E. P. S.; Spencer, L. D.; Stolyarov, V.; Stompor, R.; Strong, A. W.; Sudiwala, R.; Sunyaev, R.; Sutton, D.; Suur-Uski, A.-S.; Sygnet, J.-F.; Tauber, J. A.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Tristram, M.; Tucci, M.; Tuovinen, J.; Umana, G.; Valenziano, L.; Valiviita, J.; Van Tent, F.; Vidal, M.; Vielva, P.; Villa, F.; Wade, L. A.; Wandelt, B. D.; Watson, R.; Wehus, I. K.; Wilkinson, A.; Yvon, D.; Zacchei, A.; Zonca, A.</p> <p>2016-09-01</p> <p>We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas the polarized intensity is dominated by synchrotron emission. The Commander component-<span class="hlt">separation</span> tool has been used to <span class="hlt">separate</span> the various astrophysical processes in total intensity. Comparison with radio recombination line templates verifies the recovery of the free-free emission along the Galactic plane. Comparison of the high-latitude Hα emission with our free-free map shows residuals that correlate with dust optical depth, consistent with a fraction (≈30%) of Hα having been scattered by high-latitude dust. We highlight a number of diffuse spinning dust morphological features at high latitude. There is substantial spatial <span class="hlt">variation</span> in the spinning dust spectrum, with the emission peak (in Iν) ranging from below 20 GHz to more than 50 GHz. There is a strong tendency for the spinning dust component near many prominent H II regions to have a higher peak <span class="hlt">frequency</span>, suggesting that this increase in peak <span class="hlt">frequency</span> is associated with dust in the photo-dissociation regions around the nebulae. The emissivity of spinning dust in these diffuse regions is of the same order as previous detections in the literature. Over the entire sky, the Commander solution finds more anomalous microwave emission (AME) than the WMAP component maps, at the expense of synchrotron and free-free emission. This can be explained by the difficulty in <span class="hlt">separating</span> multiple broadband components with a limited number of <span class="hlt">frequency</span> maps. Future surveys, particularly at 5-20 GHz, will greatly improve the <span class="hlt">separation</span> by constraining the synchrotron spectrum. We combine Planck and WMAP data to make the highest signal-to-noise ratio maps yet of the intensity of the all-sky polarized synchrotron emission at <span class="hlt">frequencies</span> above a few GHz. Most of the high-latitude polarized emission is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1398405-planck-results-xxv-diffuse-low-frequency-galactic-foregrounds','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1398405-planck-results-xxv-diffuse-low-frequency-galactic-foregrounds"><span>Planck 2015 results: XXV. Diffuse low-<span class="hlt">frequency</span> Galactic foregrounds</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ade, P. A. R.; Aghanim, N.; Alves, M. I. R.; ...</p> <p>2016-09-20</p> <p>In this paper, we discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas the polarized intensity is dominated by synchrotron emission. The Commander component-<span class="hlt">separation</span> tool has been used to <span class="hlt">separate</span> the various astrophysical processes in total intensity. Comparison with radio recombination line templates verifies the recovery of the free-free emission along the Galactic plane. Comparison of the high-latitude Hα emission with our free-free map shows residuals that correlate with dust optical depth, consistent withmore » a fraction (≈30%) of Hα having been scattered by high-latitude dust. We highlight a number of diffuse spinning dust morphological features at high latitude. There is substantial spatial <span class="hlt">variation</span> in the spinning dust spectrum, with the emission peak (in I ν) ranging from below 20 GHz to more than 50 GHz. There is a strong tendency for the spinning dust component near many prominent H ii regions to have a higher peak <span class="hlt">frequency</span>, suggesting that this increase in peak <span class="hlt">frequency</span> is associated with dust in the photo-dissociation regions around the nebulae. The emissivity of spinning dust in these diffuse regions is of the same order as previous detections in the literature. Over the entire sky, the Commander solution finds more anomalous microwave emission (AME) than the WMAP component maps, at the expense of synchrotron and free-free emission. This can be explained by the difficulty in <span class="hlt">separating</span> multiple broadband components with a limited number of <span class="hlt">frequency</span> maps. Future surveys, particularly at 5–20 GHz, will greatly improve the <span class="hlt">separation</span> by constraining the synchrotron spectrum. We combine Planck and WMAP data to make the highest signal-to-noise ratio maps yet of the intensity of the all-sky polarized synchrotron emission at <span class="hlt">frequencies</span> above a few GHz. Most of the high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1398405','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1398405"><span>Planck 2015 results: XXV. Diffuse low-<span class="hlt">frequency</span> Galactic foregrounds</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>Ade, P. A. R.; Aghanim, N.; Alves, M. I. R.</p> <p></p> <p>In this paper, we discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas the polarized intensity is dominated by synchrotron emission. The Commander component-<span class="hlt">separation</span> tool has been used to <span class="hlt">separate</span> the various astrophysical processes in total intensity. Comparison with radio recombination line templates verifies the recovery of the free-free emission along the Galactic plane. Comparison of the high-latitude Hα emission with our free-free map shows residuals that correlate with dust optical depth, consistent withmore » a fraction (≈30%) of Hα having been scattered by high-latitude dust. We highlight a number of diffuse spinning dust morphological features at high latitude. There is substantial spatial <span class="hlt">variation</span> in the spinning dust spectrum, with the emission peak (in I ν) ranging from below 20 GHz to more than 50 GHz. There is a strong tendency for the spinning dust component near many prominent H ii regions to have a higher peak <span class="hlt">frequency</span>, suggesting that this increase in peak <span class="hlt">frequency</span> is associated with dust in the photo-dissociation regions around the nebulae. The emissivity of spinning dust in these diffuse regions is of the same order as previous detections in the literature. Over the entire sky, the Commander solution finds more anomalous microwave emission (AME) than the WMAP component maps, at the expense of synchrotron and free-free emission. This can be explained by the difficulty in <span class="hlt">separating</span> multiple broadband components with a limited number of <span class="hlt">frequency</span> maps. Future surveys, particularly at 5–20 GHz, will greatly improve the <span class="hlt">separation</span> by constraining the synchrotron spectrum. We combine Planck and WMAP data to make the highest signal-to-noise ratio maps yet of the intensity of the all-sky polarized synchrotron emission at <span class="hlt">frequencies</span> above a few GHz. Most of the high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA639435','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA639435"><span>Compensated Fiber-Optic <span class="hlt">Frequency</span> Distribution Equipment</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-11-01</p> <p>fiber optic links have been developed and deployed, providing stability sufficient to transfer hydrogen maser-derived <span class="hlt">frequency</span> references in intra...effectively compensate for the added noise and instability of an inter-facility fiber - optic <span class="hlt">frequency</span> distribution link , it is important to understand the...dispersion (the <span class="hlt">variation</span> in group velocity as a function of optical wavelength) may also affect the performance of the fiber optic link , when link</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27557262','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27557262"><span><span class="hlt">Frequency</span> comb SFG: a new approach to multiplex detection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kearns, Patrick M; Sohrabpour, Zahra; Massari, Aaron M</p> <p>2016-08-22</p> <p>Determination of molecular orientation at interfaces by vibrational sum <span class="hlt">frequency</span> generation spectroscopy (VSFG) requires measurements using at least two different polarization combinations of the incoming visible, IR, and generated SFG beams. We present a new method for the simultaneous collection of different VSFG polarization outputs by use of a modified 4f pulseshaper to create a simple <span class="hlt">frequency</span> comb. Via the <span class="hlt">frequency</span> comb, two visible pulses are <span class="hlt">separated</span> spectrally but aligned in space and time to interact at the sample with mixed polarization IR light. This produces two different VSFG outputs that are <span class="hlt">separated</span> by their <span class="hlt">frequencies</span> at the monochromator rather than their polarizations. Spectra were collected from organic thin films with different polarization combinations to show the reliability of the method. The results show that the optical arrangement is immune to fluctuations in laser power, beam pointing, and IR spectral shape.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880035237&hterms=Agarwal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DAgarwal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880035237&hterms=Agarwal&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DAgarwal"><span>Features of <span class="hlt">separating</span> turbulent boundary layers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nagabushana, K. A.; Agarwal, Naval K.; Simpson, Roger L.</p> <p>1988-01-01</p> <p>In the present study of two strong adverse pressure gradient flows, mean flow and turbulence characteristics are measured, together with <span class="hlt">frequency</span> spectra, using hot-wire and laser anemometry. In these <span class="hlt">separating</span> flows, reattachment occurs over a shorter distance than <span class="hlt">separation</span>. It is noted that the outer flow variables form a unique set of scaling parameters for streamwise power spectra in adverse pressure gradient flows. The inner flow scaling of Perry et al. (1985) for streamwise spectra does not hold in the backflow region unless the value of the downstream-upstream intermittency in the flow is unity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7156946','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/7156946"><span><span class="hlt">Frequency</span> regulator for synchronous generators</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Karlicek, R.F.</p> <p>1982-08-10</p> <p>The present invention is directed to a novel <span class="hlt">frequency</span> regulator which controls a generator output <span class="hlt">frequency</span> for <span class="hlt">variations</span> in both the input power to the generator and the power supplied to an uncontrolled external load. The present invention further includes over current and current balance protection devices which are relatively inexpensive to manufacture, which may be encapsulated to provide protection from the operating environment and which respond more quickly than previously known electromechanical devices. 11 figs.</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('https://www.ncbi.nlm.nih.gov/pubmed/9473911','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9473911"><span><span class="hlt">Separation</span>/divorce and child and adolescent completed suicide.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gould, M S; Shaffer, D; Fisher, P; Garfinkel, R</p> <p>1998-02-01</p> <p>To investigate factors that may modify the effect of <span class="hlt">separation</span>/divorce on youth suicide. A case-control, psychological autopsy study of 120 of 170 consecutive suicides younger than age 20 and 147 community age-, sex-, and ethnic group-matched controls living in the greater New York area was conducted. Fifty-eight suicide victims and 49 community controls came from nonintact families of origin, indicating the permanent <span class="hlt">separation</span>/divorce of the biological parents. Potential modifiers of <span class="hlt">separation</span>/divorce include youth's age at <span class="hlt">separation</span>, custodial parent's remarriage, nonresidential parent's <span class="hlt">frequency</span> of contact, parent-child relationships, and parental psychopathology. The relatively small impact of <span class="hlt">separation</span>/divorce was further diminished after accounting for parental psychopathology. An interaction of <span class="hlt">separation</span>/divorce and the father-child relationship emerged. The dramatic increase in youth suicide during the past three decades seems unlikely to be attributable to the increase in divorce rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3797851','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3797851"><span>High-<span class="hlt">Frequency</span> Subband Compressed Sensing MRI Using Quadruplet Sampling</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Sung, Kyunghyun; Hargreaves, Brian A</p> <p>2013-01-01</p> <p>Purpose To presents and validates a new method that formalizes a direct link between k-space and wavelet domains to apply <span class="hlt">separate</span> undersampling and reconstruction for high- and low-spatial-<span class="hlt">frequency</span> k-space data. Theory and Methods High- and low-spatial-<span class="hlt">frequency</span> regions are defined in k-space based on the <span class="hlt">separation</span> of wavelet subbands, and the conventional compressed sensing (CS) problem is transformed into one of localized k-space estimation. To better exploit wavelet-domain sparsity, CS can be used for high-spatial-<span class="hlt">frequency</span> regions while parallel imaging can be used for low-spatial-<span class="hlt">frequency</span> regions. Fourier undersampling is also customized to better accommodate each reconstruction method: random undersampling for CS and regular undersampling for parallel imaging. Results Examples using the proposed method demonstrate successful reconstruction of both low-spatial-<span class="hlt">frequency</span> content and fine structures in high-resolution 3D breast imaging with a net acceleration of 11 to 12. Conclusion The proposed method improves the reconstruction accuracy of high-spatial-<span class="hlt">frequency</span> signal content and avoids incoherent artifacts in low-spatial-<span class="hlt">frequency</span> regions. This new formulation also reduces the reconstruction time due to the smaller problem size. PMID:23280540</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28886652','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28886652"><span>Linear and nonlinear <span class="hlt">frequency</span>- and time-domain spectroscopy with multiple <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>Bennett, Kochise; Rouxel, Jeremy R; Mukamel, Shaul</p> <p>2017-09-07</p> <p>Two techniques that employ equally spaced trains of optical pulses to map an optical high <span class="hlt">frequency</span> into a low <span class="hlt">frequency</span> modulation of the signal that can be detected in real time are compared. The development of phase-stable optical <span class="hlt">frequency</span> combs has opened up new avenues to metrology and spectroscopy. The ability to generate a series of <span class="hlt">frequency</span> spikes with precisely controlled <span class="hlt">separation</span> permits a fast, highly accurate sampling of the material response. Recently, pairs of <span class="hlt">frequency</span> combs with slightly different repetition rates have been utilized to down-convert material susceptibilities from the optical to microwave regime where they can be recorded in real time. We show how this one-dimensional dual comb technique can be extended to multiple dimensions by using several combs. We demonstrate how nonlinear susceptibilities can be quickly acquired using this technique. In a second class of techniques, sequences of ultrafast mode locked laser pulses are used to recover pathways of interactions contributing to nonlinear susceptibilities by using a photo-acoustic modulation varying along the sequences. We show that these techniques can be viewed as a time-domain analog of the multiple <span class="hlt">frequency</span> comb scheme.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11572429','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11572429"><span><span class="hlt">Variation</span> of consumer contact with household products: a preliminary investigation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weegels, M E; van Veen, M P</p> <p>2001-06-01</p> <p>Little information is available on product use by consumers, which severely hampers exposure estimation for consumer products. This article describes actual contact with several consumer products, specifically dishwashing detergents, cleaning products, and hair styling products. How and where products are handled, as well as the duration, <span class="hlt">frequency</span>, and amount of use were studied by means of diaries, in-home observations, and measurements. This study addressed the question, "To what extent are <span class="hlt">frequency</span>, duration, and amount of use associated?" Findings showed that there was a large intra- as well as interindividual <span class="hlt">variation</span> in <span class="hlt">frequency</span>, duration, and amount of use, with the interindividual <span class="hlt">variation</span> being considerably larger. At the same time, results showed that, for a given activity, users tended to follow their own routine. Few relations were found among <span class="hlt">frequency</span>, duration, and amount of use. It was concluded that among persons, <span class="hlt">frequency</span>, duration, and amount of product act in practice as independent parameters. Diaries appear to be quite suitable for gaining insight into frequently used products. Observations of usage, recorded on video, were indispensable for obtaining particular information on product use. In addition, home visits enabled the collection of specific measurements. Although diaries and home visits are time-consuming, the combination provided insight into <span class="hlt">variation</span> as well as relations among <span class="hlt">frequency</span>, duration, and amount of use.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10466E..4ST','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10466E..4ST"><span>Verification of the effects of Schumann <span class="hlt">frequency</span> range electromagnetic fields on the human cardiovascular system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tuzhilkin, D. A.; Borodin, A. S.</p> <p>2017-11-01</p> <p>The results of the study of <span class="hlt">variations</span> in the electromagnetic background parameters of the Schumann resonator <span class="hlt">frequency</span> range and the variability indices of the human heart period during its free activity are presented on the basis of 24-hour synchronous monitoring data. It is shown that the integral evaluation of the conjugacy of the heart rate variability indices from the Schumann resonance parameters is extremely weak. In this case, the differential evaluation of this dependence with <span class="hlt">separation</span> into characteristic time intervals of the day, characterized by different motor activity of the subjects, becomes significantly higher. The number of volunteers whose conjugacy is characterized by a strong correlation in some cases reaches 35 percent of the sample.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24981085','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24981085"><span>Two-dimensional numerical modeling for <span class="hlt">separation</span> of deformable cells using dielectrophoresis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ye, Ting; Li, Hua; Lam, K Y</p> <p>2015-02-01</p> <p>In this paper, we numerically explore the possibility of <span class="hlt">separating</span> two groups of deformable cells, by a very small dielectrophoretic (DEP) microchip with the characteristic length of several cell diameters. A 2D two-fluid model is developed to describe the <span class="hlt">separation</span> process, where three types of forces are considered, the aggregation force for cell-cell interaction, the deformation force for cell deformation, and the DEP force for cell dielectrophoresis. As a model validation, we calculate the levitation height of a cell subject to DEP force, and compare it with the experimental data. After that, we simulate the <span class="hlt">separation</span> of two groups of cells with different dielectric properties at high and low <span class="hlt">frequencies</span>, respectively. The simulation results show that the deformable cells can be <span class="hlt">separated</span> successfully by a very small DEP microchip, according to not only their different permittivities at the high <span class="hlt">frequency</span>, but also their different conductivities at the low <span class="hlt">frequency</span>. In addition, both two groups of cells have a shape deformation from an original shape to a lopsided slipper shape during the <span class="hlt">separation</span> process. It is found that the cell motion is mainly determined by the DEP force arising from the electric field, causing the cells to deviate from the centerline of microchannel. However, the cell deformation is mainly determined by the deformation force arising from the fluid flow, causing the deviated cells to undergo an asymmetric motion with the deformation of slipper shape. © 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <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 scale) 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 <span class="hlt">variation</span> of empirical ranks. However, we find that the empirical <span class="hlt">variation</span> is often less that the average simulated process <span class="hlt">variation</span>, 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 scale) 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 <span class="hlt">variation</span> of empirical ranks. However, we find that the empirical <span class="hlt">variation</span> is often less that the average simulated process <span class="hlt">variation</span>, 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('http://adsabs.harvard.edu/abs/2018AIPC.1931c0044F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1931c0044F"><span>Experimental study of <span class="hlt">separator</span> effect and shift angle on crossflow wind turbine performance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fahrudin, Tjahjana, Dominicus Danardono Dwi Prija; Santoso, Budi</p> <p>2018-02-01</p> <p>This paper present experimental test results of <span class="hlt">separator</span> and shift angle influence on Crossflow vertical axis wind turbine. Modification by using a <span class="hlt">separator</span> and shift angle is expected to improve the thrust on the blade so as to improve the efficiency. The design of the wind turbine is tested at different wind speeds. There are 2 <span class="hlt">variations</span> of crossflow turbine design which will be analyzed using an experimental test scheme that is, 3 stage crossflow and 2 stage crossflow with the shift angle. Maximum power coefficient obtained as Cpmax = 0.13 at wind speed 4.05 m/s for 1 <span class="hlt">separator</span> and Cpmax = 0.12 for 12° shear angle of wind speed 4.05 m/s. In this study, power characteristics of the crossflow rotor with <span class="hlt">separator</span> and shift angle have been tested. The experimental data was collected by <span class="hlt">variation</span> of 2 <span class="hlt">separator</span> and shift angle 0°, 6°, 12° and wind speed 3.01 - 4.85 m/s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2567358','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2567358"><span>A Fundamental Relationship Between Genotype <span class="hlt">Frequencies</span> and Fitnesses</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lachance, Joseph</p> <p>2008-01-01</p> <p>The set of possible postselection genotype <span class="hlt">frequencies</span> in an infinite, randomly mating population is found. Geometric mean heterozygote <span class="hlt">frequency</span> divided by geometric mean homozygote <span class="hlt">frequency</span> equals two times the geometric mean heterozygote fitness divided by geometric mean homozygote fitness. The ratio of genotype <span class="hlt">frequencies</span> provides a measure of genetic <span class="hlt">variation</span> that is independent of allele <span class="hlt">frequencies</span>. When this ratio does not equal two, either selection or population structure is present. Within-population HapMap data show population-specific patterns, while pooled data show an excess of homozygotes. PMID:18780726</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110000842','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110000842"><span>Multiple <span class="hlt">frequency</span> optical mixer and demultiplexer and apparatus for remote sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chen, Jeffrey R. (Inventor)</p> <p>2010-01-01</p> <p>A pulsed laser system includes a modulator module configured to provide pulsed electrical signals and a plurality of solid-state seed sources coupled to the modulator module and configured to operate, responsive to the pulsed electrical signals, in a pulse mode. Each of the plurality of solid-state seed sources is tuned to a different <span class="hlt">frequency</span> channel <span class="hlt">separated</span> from any adjacent <span class="hlt">frequency</span> channel by a <span class="hlt">frequency</span> offset. The pulsed laser system also includes a combiner that combines outputs from each of the solid state seed sources into a single optical path and an optical doubler and demultiplexer coupled to the single optical path and providing each doubled seed <span class="hlt">frequency</span> on a <span class="hlt">separate</span> output path.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50.4507L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50.4507L"><span>Modulation of the atmospheric quasi-biweekly oscillation on the diurnal <span class="hlt">variation</span> of the occurrence <span class="hlt">frequency</span> of the Tibetan Plateau vortices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Lun; Zhang, Renhe; Wen, Min</p> <p>2018-06-01</p> <p>In this study, modulation of the atmospheric quasi-biweekly oscillation (QBWO) on diurnal <span class="hlt">variation</span> of the occurrence <span class="hlt">frequency</span> of Tibetan Plateau vortices (TPVs) during May-August of 2000-2009 was investigated. The diurnal <span class="hlt">variations</span> of the occurrence <span class="hlt">frequency</span> of the TPVs (OFTPVs) and the related dynamic and thermodynamic features in the positive and negative phases of QBWO were compared. In both the positive and negative phases, the OFTPVs reaches the maximum from evening to midnight (18-00 LT, LT indicates the local time), and minimum from early morning to noon (06-12 LT). At 18 LT, there is strongest convergence at 500 hPa and ascending motion, as well as the most abundant net water vapor budget over the Tibetan Plateau, which is in favor of the precipitation and the related condensation latent heat release, corresponding to the maximum of OFTPVs in 18-00 LT. On the contrary, in the early morning at 06 LT, the conditions are most unfavorable for genesis of TPVs in 06-12 LT. QBWO leads to stronger convergence at 500 hPa, ascending motion as well as more massive water vapor in the positive phases than those in the negative phases, resulting in larger numbers of TPVs occur in all of the four periods of a day (00-06 LT, 06-12 LT, 12-18 LT, and 18-00 LT) in the former. The TPVs generating from the early morning to noon (06-12 LT) are weaker and more sensitive and fragile to the disadvantageous background, while the TPVs occurring from evening to midnight (18-00 LT) are stronger and seem to be well tolerated, leading to more remarkable contrast between the OFTPVs in the negative and positive phases in 06-12 LT than in 18-00 LT.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997jena.confE.119C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997jena.confE.119C"><span>On the short term periodic light <span class="hlt">variations</span> of the flare star BY Drac</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Contadakis, M. E.</p> <p></p> <p>The analysis of a homogeneous set of photometric UBV data of the flare star BY Drac for the time interval between 1974 and 1980 indicates that BY Drac exhibits intervals of periodic light <span class="hlt">variations</span> with amplitudes up to 0.1 magnitude and period of 3d.8285. The duration of these active periods is suggested to be of the order of one or two months and are <span class="hlt">separated</span> by calm periods. The photometrically active periods coincide either with periods of relatively high flare activity or with periods during which Ha emission is present in the spectrum either of the primary or of the secondary. The phasing of the light minima are in good agreement with the phasing of the flare <span class="hlt">frequency</span> for the period of relatively high flare activity, ie July 1974. These results are in favour of a starspot modulated light <span class="hlt">variation</span> model of the star which rotates with a period of 3d.8285. The starspot lifetime should be comparable to that of the sunspot and the longitudinal location of the starspot area should be mobil.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3515628','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3515628"><span>Learned Vocal <span class="hlt">Variation</span> Is Associated with Abrupt Cryptic Genetic Change in a Parrot Species Complex</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ribot, Raoul F. H.; Buchanan, Katherine L.; Endler, John A.; Joseph, Leo; Bennett, Andrew T. D.; Berg, Mathew L.</p> <p>2012-01-01</p> <p>Contact zones between subspecies or closely related species offer valuable insights into speciation processes. A typical feature of such zones is the presence of clinal <span class="hlt">variation</span> in multiple traits. The nature of these traits and the concordance among clines are expected to influence whether and how quickly speciation will proceed. Learned signals, such as vocalizations in species having vocal learning (e.g. humans, many birds, bats and cetaceans), can exhibit rapid change and may accelerate reproductive isolation between populations. Therefore, particularly strong concordance among clines in learned signals and population genetic structure may be expected, even among continuous populations in the early stages of speciation. However, empirical evidence for this pattern is often limited because differences in vocalisations between populations are driven by habitat differences or have evolved in allopatry. We tested for this pattern in a unique system where we may be able to <span class="hlt">separate</span> effects of habitat and evolutionary history. We studied geographic <span class="hlt">variation</span> in the vocalizations of the crimson rosella (Platycercus elegans) parrot species complex. Parrots are well known for their life-long vocal learning and cognitive abilities. We analysed contact calls across a ca 1300 km transect encompassing populations that differed in neutral genetic markers and plumage colour. We found steep clinal changes in two acoustic variables (fundamental <span class="hlt">frequency</span> and peak <span class="hlt">frequency</span> position). The positions of the two clines in vocal traits were concordant with a steep cline in microsatellite-based genetic <span class="hlt">variation</span>, but were discordant with the steep clines in mtDNA, plumage and habitat. Our study provides new evidence that vocal <span class="hlt">variation</span>, in a species with vocal learning, can coincide with areas of restricted gene flow across geographically continuous populations. Our results suggest that traits that evolve culturally can be strongly associated with reduced gene flow between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1683611','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1683611"><span>Amerindian mitochondrial DNAs have rare Asian mutations at high <span class="hlt">frequencies</span>, suggesting they derived from four primary maternal lineages.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Schurr, T G; Ballinger, S W; Gan, Y Y; Hodge, J A; Merriwether, D A; Lawrence, D N; Knowler, W C; Weiss, K M; Wallace, D C</p> <p>1990-01-01</p> <p>The mitochondrial DNA (mtDNA) sequence <span class="hlt">variation</span> of the South American Ticuna, the Central American Maya, and the North American Pima was analyzed by restriction-endonuclease digestion and oligonucleotide hybridization. The analysis revealed that Amerindian populations have high <span class="hlt">frequencies</span> of mtDNAs containing the rare Asian RFLP HincII morph 6, a rare HaeIII site gain, and a unique AluI site gain. In addition, the Asian-specific deletion between the cytochrome c oxidase subunit II (COII) and tRNA(Lys) genes was also prevalent in both the Pima and the Maya. These data suggest that Amerindian mtDNAs derived from at least four primary maternal lineages, that new tribal-specific variants accumulated as these mtDNAs became distributed throughout the Americas, and that some genetic <span class="hlt">variation</span> may have been lost when the progenitors of the Ticuna <span class="hlt">separated</span> from the North and Central American populations. Images Figure 1 PMID:1968708</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24158281','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24158281"><span>High-resolution <span class="hlt">frequency</span> measurement method with a wide-<span class="hlt">frequency</span> range based on a quantized phase step law.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Du, Baoqiang; Dong, Shaofeng; Wang, Yanfeng; Guo, Shuting; Cao, Lingzhi; Zhou, Wei; Zuo, Yandi; Liu, Dan</p> <p>2013-11-01</p> <p>A wide-<span class="hlt">frequency</span> and high-resolution <span class="hlt">frequency</span> measurement method based on the quantized phase step law is presented in this paper. Utilizing a <span class="hlt">variation</span> law of the phase differences, the direct different <span class="hlt">frequency</span> phase processing, and the phase group synchronization phenomenon, combining an A/D converter and the adaptive phase shifting principle, a counter gate is established in the phase coincidences at one-group intervals, which eliminates the ±1 counter error in the traditional <span class="hlt">frequency</span> measurement method. More importantly, the direct phase comparison, the measurement, and the control between any periodic signals have been realized without <span class="hlt">frequency</span> normalization in this method. Experimental results show that sub-picosecond resolution can be easily obtained in the <span class="hlt">frequency</span> measurement, the <span class="hlt">frequency</span> standard comparison, and the phase-locked control based on the phase quantization processing technique. The method may be widely used in navigation positioning, space techniques, communication, radar, astronomy, atomic <span class="hlt">frequency</span> standards, and other high-tech fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23436439','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23436439"><span>Continuous <span class="hlt">separation</span> of colloidal particles using dielectrophoresis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yunus, Nurul Amziah Md; Nili, Hossein; Green, Nicolas G</p> <p>2013-04-01</p> <p>Dielectrophoresis is the movement of particles in nonuniform electric fields and has been of interest for application to manipulation and <span class="hlt">separation</span> at and below the microscale. This technique has the advantages of being noninvasive, nondestructive, and noncontact, with the movement of particle achieved by means of electric fields generated by miniaturized electrodes and microfluidic systems. Although the majority of applications have been above the microscale, there is increasing interest in application to colloidal particles around a micron and smaller. This paper begins with a review of colloidal and nanoscale dielectrophoresis with specific attention paid to <span class="hlt">separation</span> applications. An innovative design of integrated microelectrode array and its application to flow-through, continuous <span class="hlt">separation</span> of colloidal particles is then presented. The details of the angled chevron microelectrode array and the test microfluidic system are then discussed. The <span class="hlt">variation</span> in device operation with applied signal voltage is presented and discussed in terms of <span class="hlt">separation</span> efficiency, demonstrating 99.9% <span class="hlt">separation</span> of a mixture of colloidal latex spheres. © 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/816440','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/816440"><span>High-Throughput Genetic Analysis and Combinatorial Chiral <span class="hlt">Separations</span> Based on Capillary Electrophoresis</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>Zhong, Wenwan</p> <p>2003-01-01</p> <p>Capillary electrophoresis (CE) offers many advantages over conventional analytical methods, such as speed, simplicity, high resolution, low cost, and small sample consumption, especially for the <span class="hlt">separation</span> of enantiomers. However, chiral method developments still can be time consuming and tedious. They designed a comprehensive enantioseparation protocol employing neutral and sulfated cyclodextrins as chiral selectors for common basic, neutral, and acidic compounds with a 96-capillary array system. By using only four judiciously chosen <span class="hlt">separation</span> buffers, successful enantioseparations were achieved for 49 out of 54 test compounds spanning a large variety of pKs and structures. Therefore, unknown compounds can be screened in thismore » manner to identify optimal enantioselective conditions in just one rn. In addition to superior <span class="hlt">separation</span> efficiency for small molecules, CE is also the most powerful technique for DNA <span class="hlt">separations</span>. Using the same multiplexed capillary system with UV absorption detection, the sequence of a short DNA template can be acquired without any dye-labels. Two internal standards were utilized to adjust the migration time <span class="hlt">variations</span> among capillaries, so that the four electropherograms for the A, T, C, G Sanger reactions can be aligned and base calling can be completed with a high level of confidence. the CE <span class="hlt">separation</span> of DNA can be applied to study differential gene expression as well. Combined with pattern recognition techniques, small <span class="hlt">variations</span> among electropherograms obtained by the <span class="hlt">separation</span> of cDNA fragments produced from the total RNA samples of different human tissues can be revealed. These <span class="hlt">variations</span> reflect the differences in total RNA expression among tissues. Thus, this Ce-based approach can serve as an alternative to the DNA array techniques in gene expression analysis.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..294a2033B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..294a2033B"><span>Natural <span class="hlt">frequencies</span> of thin rectangular plates clamped on contour using the Finite Element Method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>(Barboni Haţiegan, L.; Haţiegan, C.; Gillich, G. R.; Hamat, C. O.; Vasile, O.; Stroia, M. D.</p> <p>2018-01-01</p> <p>This paper presents the determining of natural <span class="hlt">frequencies</span> of plates without and with damages using the finite element method of SolidWorks program. The first thirty natural <span class="hlt">frequencies</span> obtained for thin rectangular rectangular plates clamped on contour without and with central damages a for different dimensions. The relative <span class="hlt">variation</span> of natural <span class="hlt">frequency</span> was determined and the obtained results by the finite element method (FEM) respectively relative <span class="hlt">variation</span> of natural <span class="hlt">frequency</span>, were graphically represented according to their vibration natural modes. Finally, the obtained results were compared.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19308360','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19308360"><span><span class="hlt">Separation</span> of malignant human breast cancer epithelial cells from healthy epithelial cells using an advanced dielectrophoresis-activated cell sorter (DACS).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>An, Jaemin; Lee, Jangwon; Lee, Sang Ho; Park, Jungyul; Kim, Byungkyu</p> <p>2009-06-01</p> <p>In this paper, we successfully <span class="hlt">separated</span> malignant human breast cancer epithelial cells (MCF 7) from healthy breast cells (MCF 10A) and analyzed the main parameters that influence the <span class="hlt">separation</span> efficiency with an advanced dielectrophoresis (DEP)-activated cell sorter (DACS). Using the efficient DACS, the malignant cancer cells (MCF 7) were isolated successfully by noninvasive methods from normal cells with similar cell size distributions (MCF 10A), depending on differences between their material properties such as conductivity and permittivity, because our system was able to discern the subtle differences in the properties by generating continuously changed electrical field gradients. In order to evaluate the <span class="hlt">separation</span> performance without considering size <span class="hlt">variations</span>, the cells collected from each outlet were divided into size-dependent groups and counted statistically. Following that, the quantitative relative ratio of numbers between MCF 7 and MCF 10A cells in each size-dependent group <span class="hlt">separated</span> by the DEP were compared according to applied <span class="hlt">frequencies</span> in the range 48, 51, and 53 MHz with an applied amplitude of 8 V(pp). Finally, under the applied voltage of 48 MHz-8 V(pp) and a flow rate of 290 microm/s, MCF 7 and MCF 10A cells were <span class="hlt">separated</span> with a maximum efficiency of 86.67% and 98.73% respectively. Therefore, our suggested system shows it can be used for detection and <span class="hlt">separation</span> of cancerous epithelial cells from noncancerous cells in clinical applications.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850022892','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850022892"><span>Self-Tuning Adaptive-Controller Using Online <span class="hlt">Frequency</span> Identification</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chiang, W. W.; Cannon, R. H., Jr.</p> <p>1985-01-01</p> <p>A real time adaptive controller was designed and tested successfully on a fourth order laboratory dynamic system which features very low structural damping and a noncolocated actuator sensor pair. The controller, implemented in a digital minicomputer, consists of a state estimator, a set of state feedback gains, and a <span class="hlt">frequency</span> locked loop (FLL) for real time parameter identification. The FLL can detect the closed loop natural <span class="hlt">frequency</span> of the system being controlled, calculate the mismatch between a plant parameter and its counterpart in the state estimator, and correct the estimator parameter in real time. The adaptation algorithm can correct the controller error and stabilize the system for more than 50% <span class="hlt">variation</span> in the plant natural <span class="hlt">frequency</span>, compared with a 10% stability margin in <span class="hlt">frequency</span> <span class="hlt">variation</span> for a fixed gain controller having the same performance at the nominal plant condition. After it has locked to the correct plant <span class="hlt">frequency</span>, the adaptive controller works as well as the fixed gain controller does when there is no parameter mismatch. The very rapid convergence of this adaptive system is demonstrated experimentally, and can also be proven with simple root locus methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4959233','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4959233"><span>Mycoplasma agalactiae Secretion of β-(1→6)-Glucan, a Rare Polysaccharide in Prokaryotes, Is Governed by High-<span class="hlt">Frequency</span> Phase <span class="hlt">Variation</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>Baranowski, E.; Pau-Roblot, C.; Sagné, E.; Citti, C.</p> <p>2016-01-01</p> <p>ABSTRACT Mycoplasmas are minimal, wall-less bacteria but have retained the ability to secrete complex carbohydrate polymers that constitute a glycocalyx. In members of the Mycoplasma mycoides cluster, which are important ruminant pathogens, the glycocalyx includes both cell-attached and cell-free polysaccharides. This report explores the potential secretion of polysaccharides by M. agalactiae, another ruminant pathogen that belongs to a distant phylogenetic group. Comparative genomic analyses showed that M. agalactiae possesses all the genes required for polysaccharide secretion. Notably, a putative synthase gene (gsmA) was identified, by in silico reconstruction of the biosynthetic pathway, that could be involved in both polymerization and export of the carbohydrate polymers. M. agalactiae polysaccharides were then purified in vitro and found to be mainly cell attached, with a linear β-(1→6)-glucopyranose structure [β-(1→6)-glucan]. Secretion of β-(1→6)-glucan was further shown to rely on the presence of a functional gsmA gene, whose expression is subjected to high-<span class="hlt">frequency</span> phase <span class="hlt">variation</span>. This event is governed by the spontaneous intraclonal <span class="hlt">variation</span> in length of a poly(G) tract located in the gsmA coding sequence and was shown to occur in most of the M. agalactiae clinical isolates tested in this study. M. agalactiae susceptibility to serum-killing activity appeared to be dictated by ON/OFF switching of β-(1→6)-glucan secretion, suggesting a role of this phenomenon in survival of the pathogen when it invades the host bloodstream. Finally, β-(1→6)-glucan secretion was not restricted to M. agalactiae but was detected also in M. mycoides subsp. capri PG3T, another pathogen of small ruminants. IMPORTANCE Many if not all bacteria are able to secrete polysaccharides, either attached to the cell surface or exported unbound into the extracellular environment. Both types of polysaccharides can play a role in bacterium-host interactions. Mycoplasmas are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1949k0006K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1949k0006K"><span>Model based optimization of driver-pickup <span class="hlt">separation</span> for eddy current measurement of gap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klein, G.; Morelli, J.; Krause, T. W.</p> <p>2018-04-01</p> <p>The fuel channels in CANDU® (CANada Deuterium Uranium) nuclear reactors consist of a pressure tube (PT) contained within a larger diameter calandria tube (CT). The <span class="hlt">separation</span> between the tubes, known as the PT-CT gap, ensures PT hydride blisters, which could lead to potential cracking of the PT, do not develop. Therefore, accurate measurements are required to confirm that contact between PT and CT is not imminent. Gap measurement uses an eddy current probe. However this probe is sensitive to lift-off <span class="hlt">variations</span>, which can adversely affect estimated gap. A validated analytical flat plate model of eddy current response to gap was used to examine the effect of driver-pickup spacing on lift-off and response to gap at a <span class="hlt">frequency</span> of 4 kHz, which is used for in-reactor measurements. This model was compared against, and shown to have good agreement with, a COMSOL® finite element method (FEM) model. The optimum coil <span class="hlt">separation</span>, which included the constraint of coil size, was found to be 11 mm, resulting in a phase response between lift-off and response to change in gap of 66°. This work demonstrates the advantages of using analytical models for optimizing coil designs for measurement of parameters that may negatively influence the outcome of an inspection measurement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27846291','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27846291"><span>Geographic <span class="hlt">Variation</span> in Festuca rubra L. Ploidy Levels and Systemic Fungal Endophyte <span class="hlt">Frequencies</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dirihan, Serdar; Helander, Marjo; Väre, Henry; Gundel, Pedro E; Garibaldi, Lucas A; Irisarri, J Gonzalo N; Saloniemi, Irma; Saikkonen, Kari</p> <p>2016-01-01</p> <p>Polyploidy and symbiotic Epichloë fungal endophytes are common and heritable characteristics that can facilitate environmental range expansion in grasses. Here we examined geographic patterns of polyploidy and the <span class="hlt">frequency</span> of fungal endophyte colonized plants in 29 Festuca rubra L. populations from eight geographic sites across latitudes from Spain to northernmost Finland and Greenland. Ploidy seemed to be positively and negatively correlated with latitude and productivity, respectively. However, the correlations were nonlinear; 84% of the plants were hexaploids (2n = 6x = 42), and the positive correlation between ploidy level and latitude is the result of only four populations skewing the data. In the southernmost end of the gradient 86% of the plants were tetraploids (2n = 4x = 28), whereas in the northernmost end of the gradient one population had only octoploid plants (2n = 8x = 56). Endophytes were detected in 22 out of the 29 populations. Endophyte <span class="hlt">frequencies</span> varied among geographic sites, and populations and habitats within geographic sites irrespective of ploidy, latitude or productivity. The highest overall endophyte <span class="hlt">frequencies</span> were found in the southernmost end of the gradient, Spain, where 69% of plants harbored endophytes. In northern Finland, endophytes were detected in 30% of grasses but endophyte <span class="hlt">frequencies</span> varied among populations from 0% to 75%, being higher in meadows compared to riverbanks. The endophytes were detected in 36%, 30% and 27% of the plants in Faroe Islands, Iceland and Switzerland, respectively. Practically all examined plants collected from southern Finland and Greenland were endophyte-free, whereas in other geographic sites endophyte <span class="hlt">frequencies</span> were highly variable among populations. Common to all populations with high endophyte <span class="hlt">frequencies</span> is heavy vertebrate grazing. We propose that the detected endophyte <span class="hlt">frequencies</span> and ploidy levels mirror past distribution history of F. rubra after the last glaciation period, and local</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5112939','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5112939"><span>Geographic <span class="hlt">Variation</span> in Festuca rubra L. Ploidy Levels and Systemic Fungal Endophyte <span class="hlt">Frequencies</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>Dirihan, Serdar; Helander, Marjo; Väre, Henry; Gundel, Pedro E.; Garibaldi, Lucas A.; Irisarri, J. Gonzalo N.; Saloniemi, Irma; Saikkonen, Kari</p> <p>2016-01-01</p> <p>Polyploidy and symbiotic Epichloë fungal endophytes are common and heritable characteristics that can facilitate environmental range expansion in grasses. Here we examined geographic patterns of polyploidy and the <span class="hlt">frequency</span> of fungal endophyte colonized plants in 29 Festuca rubra L. populations from eight geographic sites across latitudes from Spain to northernmost Finland and Greenland. Ploidy seemed to be positively and negatively correlated with latitude and productivity, respectively. However, the correlations were nonlinear; 84% of the plants were hexaploids (2n = 6x = 42), and the positive correlation between ploidy level and latitude is the result of only four populations skewing the data. In the southernmost end of the gradient 86% of the plants were tetraploids (2n = 4x = 28), whereas in the northernmost end of the gradient one population had only octoploid plants (2n = 8x = 56). Endophytes were detected in 22 out of the 29 populations. Endophyte <span class="hlt">frequencies</span> varied among geographic sites, and populations and habitats within geographic sites irrespective of ploidy, latitude or productivity. The highest overall endophyte <span class="hlt">frequencies</span> were found in the southernmost end of the gradient, Spain, where 69% of plants harbored endophytes. In northern Finland, endophytes were detected in 30% of grasses but endophyte <span class="hlt">frequencies</span> varied among populations from 0% to 75%, being higher in meadows compared to riverbanks. The endophytes were detected in 36%, 30% and 27% of the plants in Faroe Islands, Iceland and Switzerland, respectively. Practically all examined plants collected from southern Finland and Greenland were endophyte-free, whereas in other geographic sites endophyte <span class="hlt">frequencies</span> were highly variable among populations. Common to all populations with high endophyte <span class="hlt">frequencies</span> is heavy vertebrate grazing. We propose that the detected endophyte <span class="hlt">frequencies</span> and ploidy levels mirror past distribution history of F. rubra after the last glaciation period, and local</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. <span class="hlt">Separate</span> 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> scale. 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/2018Tectp.722..235B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.722..235B"><span>Regional <span class="hlt">variation</span> of coda Q in Kopili fault zone of northeast India and its implications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bora, Nilutpal; Biswas, Rajib; Dobrynina, Anna A.</p> <p>2018-01-01</p> <p>Kopili fault has been experiencing higher seismic and tectonic activity during the recent years. These kind of active tectonics can be inspected by examining coda-wave attenuation and its dependence with <span class="hlt">frequency</span>. Exploiting single back-scattering model, we have endeavored to measure coda Q and its associated parameters such as <span class="hlt">frequency</span> dependent factor (n) and attenuation coefficient (γ) covering seven lapse-time windows spanning from 30 to 90 s and central <span class="hlt">frequencies</span> 1.5, 3.5, 6, 9 and 12 Hz. The average estimated values of QC increases with <span class="hlt">frequency</span> and lapse time window from 114 at <span class="hlt">frequency</span> 1.5 Hz to 1563 at <span class="hlt">frequency</span> 12 Hz for 30 s window length, and from 305 at <span class="hlt">frequency</span> 1.5 Hz to 2135 at <span class="hlt">frequency</span> 12 Hz for 90 s window length. The values of Q0 and n are also estimated for the entire Kopili fault zone. For this study region, the Q0 values vary from 62 to 348 and n varies from 0.57 to 1.51 within the <span class="hlt">frequency</span> range 1.5 to 12 Hz. Furthermore, depth <span class="hlt">variation</span> of attenuation of this region reveals that there is velocity anomaly at depth 210-220 km as there arises sharp changes in γ and n which are supported by available data, reported by other researcher for this region. Finally, we have tried to <span class="hlt">separate</span> the intrinsic and scattering attenuation for this area. It is observed that the entire region is dominated by mainly scattering attenuation, but we can see an increase in intrinsic attenuation with depths in two stations namely TZR and BKD. Furthermore, the obtained results are comparable with the available global data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28596934','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28596934"><span>Gel performance in rheology and profile control under low-<span class="hlt">frequency</span> vibration: coupling application of physical and chemical EOR techniques.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zheng, Li Ming; Pu, Chun Sheng; Liu, Jing; Ma, Bo; Khan, Nasir</p> <p>2017-01-01</p> <p>Flowing gel plugging and low-<span class="hlt">frequency</span> vibration oil extraction technology have been widely applied in low-permeability formation. High probability of overlapping in action spheres of two technologies might lead to poor operating efficiency during gel injection. Study on flowing gel rheological properties under low-<span class="hlt">frequency</span> vibration was essential, which was carried out indoor with viscosity measurement. Potential dynamic mechanisms were analyzed for the rheological <span class="hlt">variation</span>. Under low-<span class="hlt">frequency</span> vibration, gel rheological properties were found to be obviously influenced, with vibration delaying gel cross-linking in induction period, causing a two-stage gel viscosity change in acceleration period, and decreasing gel strength in stable period. Surface of gel system under vibration presented different fluctuating phenomenon from initial harmonic vibrating to heterogeneous fluctuating (droplet <span class="hlt">separation</span> might appear) to final harmonic vibrating again. Dynamic displacement in unconsolidated sand pack revealed that low-<span class="hlt">frequency</span> vibration during gel injection might be a measure to achieve deep profile control, with the gel injection depth increased by 65.8 % compared with the vibration-free sample. At last, suggestions for field test were given in the paper to achieve lower injection friction and better gel plugging efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930018268','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930018268"><span>Discrete-vortex simulation of pulsating flow on a turbulent leading-edge <span class="hlt">separation</span> bubble</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sung, Hyung Jin; Rhim, Jae Wook; Kiya, Masaru</p> <p>1992-01-01</p> <p>Studies are made of the turbulent <span class="hlt">separation</span> bubble in a two-dimensional semi-infinite blunt plate aligned to a uniform free stream with a pulsating component. The discrete-vortex method is applied to simulate this flow situation because this approach is effective for representing the unsteady motions of the turbulent shear layer and the effect of viscosity near the solid surface. The numerical simulation provides reasonable predictions when compared with the experimental results. A particular <span class="hlt">frequency</span> with a minimum reattachment is related to the drag reduction. The most effective <span class="hlt">frequency</span> is dependent on the amplified shedding <span class="hlt">frequency</span>. The turbulent flow structure is scrutinized. This includes the time-mean and fluctuations of the velocity and the surface pressure, together with correlations between the fluctuating components. A comparison between the pulsating flow and the non-pulsating flow at the particular <span class="hlt">frequency</span> of the minimum reattachment length of the <span class="hlt">separation</span> bubble suggests that the large-scale vortical structure is associated with the shedding <span class="hlt">frequency</span> and the flow instabilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770012598&hterms=Your+Mother&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DYour%2BMother','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770012598&hterms=Your+Mother&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DYour%2BMother"><span>Low <span class="hlt">frequency</span> electric field <span class="hlt">variations</span> during HF transmissions on a mother-daughter rocket</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rosenberg, T. J.; Maynard, M. C.; Holtet, J. A.; Karlsen, N. O.; Egeland, A.; Moe, T. E.; Troim, J.</p> <p>1977-01-01</p> <p>HF wave propagation experiments were conducted on Mother-Daughter rockets in the polar ionosphere. Swept <span class="hlt">frequency</span> transmissions from the Mother, nominally covering the range from 0.5 to 5 MHz in both CW and pulse modes, are received by the Daughter. In the most recent rocket of the series, the Mother also contained an AC electric field spectrometer covering the <span class="hlt">frequency</span> range from 10 Hz to 100 kHz in four decade bands. The low <span class="hlt">frequency</span> response of the ionosphere with respect to waves emitted from the onboard HF transmitter is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EaSci..26..301E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EaSci..26..301E"><span>Continuous-cyclic <span class="hlt">variations</span> in the b-value of the earthquake <span class="hlt">frequency</span>-magnitude distribution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>El-Isa, Z. H.</p> <p>2013-10-01</p> <p>Seismicity of the Earth ( M ≥ 4.5) was compiled from NEIC, IRIS and ISC catalogues and used to compute b-value based on various time windows. It is found that continuous cyclic b-<span class="hlt">variations</span> occur on both long and short time scales, the latter being of much higher value and sometimes in excess of 0.7 of the absolute b-value. These <span class="hlt">variations</span> occur not only yearly or monthly, but also daily. Before the occurrence of large earthquakes, b-values start increasing with variable gradients that are affected by foreshocks. In some cases, the gradient is reduced to zero or to a negative value a few days before the earthquake occurrence. In general, calculated b-values attain maxima 1 day before large earthquakes and minima soon after their occurrence. Both linear regression and maximum likelihood methods give correlatable, but variable results. It is found that an expanding time window technique from a fixed starting point is more effective in the study of b-<span class="hlt">variations</span>. The calculated b-<span class="hlt">variations</span> for the whole Earth, its hemispheres, quadrants and the epicentral regions of some large earthquakes are of both local and regional character, which may indicate that in such cases, the geodynamic processes acting within a certain region have a much regional effect within the Earth. The b-<span class="hlt">variations</span> have long been known to vary with a number of local and regional factors including tectonic stresses. The results reported here indicate that geotectonic stress remains the most significant factor that controls b-<span class="hlt">variations</span>. It is found that for earthquakes with M w ≥ 7, an increase of about 0.20 in the b-value implies a stress increase that will result in an earthquake with a magnitude one unit higher.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014RaSc...49..753O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014RaSc...49..753O"><span>Spatial distribution and temporal <span class="hlt">variations</span> of occurrence <span class="hlt">frequency</span> of lightning whistlers observed by VLF/WBA onboard Akebono</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oike, Yuta; Kasahara, Yoshiya; Goto, Yoshitaka</p> <p>2014-09-01</p> <p>We statistically analyzed lightning whistlers detected from the analog waveform data below 15 kHz observed by the VLF instruments onboard Akebono. We examined the large amount of data obtained at Uchinoura Space Center in Japan for 22 years from 1989 to 2010. The lightning whistlers were mainly observed inside the L shell region below 2. Seasonal dependence of the occurrence <span class="hlt">frequency</span> of lightning whistlers has two peaks around July to August and December to January. As lightning is most active in summer, in general, these two peaks correspond to summer in the Northern and Southern Hemispheres, respectively. Diurnal <span class="hlt">variation</span> of the occurrence <span class="hlt">frequency</span> showed that lightning whistlers begin to increase in the early evening and remain at a high-occurrence level through the night with a peak around 21 in magnetic local time (MLT). This peak shifts toward nightside compared with lightning activity, which begins to rise around noon and peaks in the late afternoon. This trend is supposed to be caused by attenuation of VLF wave in the ionosphere in the daytime. Comparison study with the ground-based observation revealed consistent results, except that the peak of the ground-based observation appeared after midnight while our measurements obtained by Akebono was around 21 in MLT. This difference is explained qualitatively in terms that lightning whistlers measured at the ground station passed through the ionosphere twice above both source region and the ground station. These facts provide an important clue to evaluate quantitatively the absorption effect of lightning whistler in the ionosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27076394','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27076394"><span>Investigating lipids as a source of chemical exchange-induced MRI <span class="hlt">frequency</span> shifts.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shmueli, K; Dodd, S J; van Gelderen, P; Duyn, J H</p> <p>2017-04-01</p> <p>While magnetic susceptibility is a major contributor to NMR resonance <span class="hlt">frequency</span> <span class="hlt">variations</span> in the human brain, a substantial contribution may come from the chemical exchange of protons between water and other molecules. Exchange-induced <span class="hlt">frequency</span> shifts f e have been measured in tissue and protein solutions, but relatively lipid-rich white matter (WM) has a larger f e than gray matter, suggesting that lipids could contribute. Galactocerebrosides (GC) are a prime candidate as they are abundant in WM and susceptible to exchange. To investigate this, f e was measured in a model of WM lipid membranes in the form of multilamellar vesicles (MLVs), consisting of a 1:2 molar ratio of GC and phospholipids (POPC), and in MLVs with POPC only. Chemical shift imaging with 15% volume fraction of dioxane, an internal reference whose protons are assumed not to undergo chemical exchange, was used to remove susceptibility-induced <span class="hlt">frequency</span> shifts in an attempt to measure f e in MLVs at several lipid concentrations. Initial analysis of these measurements indicated a necessity to correct for small unexpected <span class="hlt">variations</span> in dioxane concentration due to its effect on the water <span class="hlt">frequency</span> shift. To achieve this, the actual dioxane concentration was inferred from spectral analysis and its additional contribution to f e was removed through <span class="hlt">separate</span> experiments which showed that the water-dioxane <span class="hlt">frequency</span> shift depended linearly on the dioxane concentration at low concentrations with a proportionality constant of -0.021 ± 0.002 ppb/mM in agreement with published experiments. Contrary to expectations and uncorrected results, for GC + POPC vesicles, the dependence of the corrected f e on GC concentration was insignificant (0.023 ± 0.037 ppb/mM; r 2  = 0.085, p > 0.57), whereas for the POPC-only vesicles a small but significant linear increase with POPC concentration was found: 0.044 ± 0.008 ppb/mM (r 2  = 0.877, p < 0.01). These findings suggest that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGeod..91.1099W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGeod..91.1099W"><span>Group delay <span class="hlt">variations</span> of GPS transmitting and receiving antennas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wanninger, Lambert; Sumaya, Hael; Beer, Susanne</p> <p>2017-09-01</p> <p>GPS code pseudorange measurements exhibit group delay <span class="hlt">variations</span> at the transmitting and the receiving antenna. We calibrated C1 and P2 delay <span class="hlt">variations</span> with respect to dual-<span class="hlt">frequency</span> carrier phase observations and obtained nadir-dependent corrections for 32 satellites of the GPS constellation in early 2015 as well as elevation-dependent corrections for 13 receiving antenna models. The combined delay <span class="hlt">variations</span> reach up to 1.0 m (3.3 ns) in the ionosphere-free linear combination for specific pairs of satellite and receiving antennas. Applying these corrections to the code measurements improves code/carrier single-<span class="hlt">frequency</span> precise point positioning, ambiguity fixing based on the Melbourne-Wübbena linear combination, and determination of ionospheric total electron content. It also affects fractional cycle biases and differential code biases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037400','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037400"><span>Rayleigh-wave mode <span class="hlt">separation</span> by high-resolution linear radon transform</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Luo, Y.; Xia, J.; Miller, R.D.; Xu, Y.; Liu, J.; Liu, Q.</p> <p>2009-01-01</p> <p>Multichannel analysis of surface waves (MASW) method is an effective tool for obtaining vertical shear wave profiles from a single non-invasive measurement. One key step of the MASW method is generation of a dispersion image and extraction of a reliable dispersion curve from raw multichannel shot records. Because different Rayleigh-wave modes normally interfere with each other in the time and space domain, it is necessary to perform mode <span class="hlt">separation</span> and reconstruction to increase the accuracy of phase velocities determined from a dispersion image. In this paper, we demonstrate the effectiveness of high-resolution linear Radon transform (LRT) as a means of <span class="hlt">separating</span> and reconstructing multimode, dispersive Rayleigh-wave energy. We first introduce high-resolution LRT methods and Rayleigh-wave mode <span class="hlt">separation</span> using high-resolution LRT. Next, we use synthetic data and a real-world example to demonstrate the effectiveness of Rayleigh-wave mode <span class="hlt">separation</span> using high-resolution LRT. Our synthetic and real-world results demonstrate that (1) high-resolution LRT successfully <span class="hlt">separates</span> and reconstructs multimode dispersive Rayleigh-wave energy with high resolution allowing the multimode energy to be more accurately determined. The horizontal resolution of the Rayleigh-wave method can be increased by extraction of dispersion curves from a pair of traces in the mode-<span class="hlt">separated</span> shot gather and (2) multimode <span class="hlt">separation</span> and reconstruction expand the usable <span class="hlt">frequency</span> range of higher mode dispersive energy, which increases the depth of investigation and provides a means for accurately determining cut-off <span class="hlt">frequencies</span>. ?? 2009 The Authors Journal compilation ?? 2009 RAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19128839','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19128839"><span><span class="hlt">Separation</span> as a suicide risk factor.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wyder, Marianne; Ward, Patrick; De Leo, Diego</p> <p>2009-08-01</p> <p>Marital <span class="hlt">separation</span> (as distinct from divorce) is rarely researched in the suicidological literature. Studies usually report on the statuses of '<span class="hlt">separated</span>' and 'divorced' as a combined category, possibly because demographic registries are not able to identify <span class="hlt">separation</span> reliably. However, in most countries divorce only happens once the process of <span class="hlt">separation</span> has settled which, in most cases, occurs a long time after the initial break-up. It has been hypothesised that <span class="hlt">separation</span> might carry a far greater risk of suicide than divorce. The present study investigates the impact of <span class="hlt">separation</span> on suicide risk by taking into account the effects of age and gender. The incidence of suicide associated with marital status, age and gender was determined by comparing the Queensland Suicide Register (a large dataset of all suicides in Queensland from 1994 to 2004) with the QLD population through two different census datasets: the Registered Marital Status and the Social Marital Status. These two registries permit the isolation of the variable '<span class="hlt">separated</span>' with great reliability. During the examined period, 6062 persons died by suicide in QLD (an average of 551 cases per year), with males outnumbering females by four to one. For both males and females <span class="hlt">separation</span> created a risk of suicide at least 4 times higher than any other marital status. The risk was particularly high for males aged 15 to 24 (RR 91.62). This study highlights a great <span class="hlt">variation</span> in the incidence of suicide by marital status, age and gender, which suggests that these variables should not be studied in isolation. Furthermore, particularly in younger males, <span class="hlt">separation</span> appears to be strongly associated with the risk of suicide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860011197','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860011197"><span>Automatic oscillator <span class="hlt">frequency</span> control system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, S. F. (Inventor)</p> <p>1985-01-01</p> <p>A <span class="hlt">frequency</span> control system makes an initial correction of the <span class="hlt">frequency</span> of its own timing circuit after comparison against a <span class="hlt">frequency</span> of known accuracy and then sequentially checks and corrects the <span class="hlt">frequencies</span> of several voltage controlled local oscillator circuits. The timing circuit initiates the machine cycles of a central processing unit which applies a <span class="hlt">frequency</span> index to an input register in a modulo-sum <span class="hlt">frequency</span> divider stage and enables a multiplexer to clock an accumulator register in the divider stage with a cyclical signal derived from the oscillator circuit being checked. Upon expiration of the interval, the processing unit compares the remainder held as the contents of the accumulator against a stored zero error constant and applies an appropriate correction word to a correction stage to shift the <span class="hlt">frequency</span> of the oscillator being checked. A signal from the accumulator register may be used to drive a phase plane ROM and, with periodic shifts in the applied <span class="hlt">frequency</span> index, to provide <span class="hlt">frequency</span> shift keying of the resultant output signal. Interposition of a phase adder between the accumulator register and phase plane ROM permits phase shift keying of the output signal by periodic <span class="hlt">variation</span> in the value of a phase index applied to one input of the phase adder.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050019217','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050019217"><span><span class="hlt">Frequency</span> Bandwidth Optimization of Left-Handed Metamaterial</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chevalier, Christine T.; Wilson, Jeffrey D.</p> <p>2004-01-01</p> <p>Recently, left-handed metamaterials (LHM s) have been demonstrated with an effective negative index of refraction and with antiparallel group and phase velocities for microwave radiation over a narrow <span class="hlt">frequency</span> bandwidth. In order to take advantage of these characteristics for practical applications, it will be beneficial to develop LHM s with increased <span class="hlt">frequency</span> bandwidth response and lower losses. In this paper a commercial three-dimensional electromagnetic simulation code is used to explore the effects of geometry parameter <span class="hlt">variations</span> on the <span class="hlt">frequency</span> bandwidth of a LHM at microwave <span class="hlt">frequencies</span>. Utilizing an optimizing routine in the code, a geometry was generated with a bandwidth more than twice as large as the original geometry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830000283&hterms=frequency+modulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dfrequency%2Bmodulation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830000283&hterms=frequency+modulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dfrequency%2Bmodulation"><span>Radio-<span class="hlt">Frequency</span> and Wideband Modulation Arraying</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Brockman, M. H.</p> <p>1984-01-01</p> <p>Summing network receives coherent signals from all receivers in array. Method sums narrow-band radio-<span class="hlt">frequency</span> (RF) carrier powers and wide-band spectrum powers of array of <span class="hlt">separate</span> antenna/receiver systems designed for phase-locked-loop or suppressed-carrier operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AIPC.1391..350G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AIPC.1391..350G"><span>Time-<span class="hlt">Frequency</span> Approach for Stochastic Signal Detection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghosh, Ripul; Akula, Aparna; Kumar, Satish; Sardana, H. K.</p> <p>2011-10-01</p> <p>The detection of events in a stochastic signal has been a subject of great interest. One of the oldest signal processing technique, Fourier Transform of a signal contains information regarding <span class="hlt">frequency</span> content, but it cannot resolve the exact onset of changes in the <span class="hlt">frequency</span>, all temporal information is contained in the phase of the transform. On the other hand, Spectrogram is better able to resolve temporal evolution of <span class="hlt">frequency</span> content, but has a trade-off in time resolution versus <span class="hlt">frequency</span> resolution in accordance with the uncertainty principle. Therefore, time-<span class="hlt">frequency</span> representations are considered for energetic characterisation of the non-stationary signals. Wigner Ville Distribution (WVD) is the most prominent quadratic time-<span class="hlt">frequency</span> signal representation and used for analysing <span class="hlt">frequency</span> <span class="hlt">variations</span> in signals.WVD allows for instantaneous <span class="hlt">frequency</span> estimation at each data point, for a typical temporal resolution of fractions of a second. This paper through simulations describes the way time <span class="hlt">frequency</span> models are applied for the detection of event in a stochastic signal.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/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 scale 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). <span class="hlt">Separate</span> 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 <span class="hlt">separate</span> 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('http://adsabs.harvard.edu/abs/2018SPIE10697E..58H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10697E..58H"><span>Emitter signal <span class="hlt">separation</span> method based on multi-level digital channelization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, Xun; Ping, Yifan; Wang, Sujun; Feng, Ying; Kuang, Yin; Yang, Xinquan</p> <p>2018-02-01</p> <p>To solve the problem of emitter <span class="hlt">separation</span> under complex electromagnetic environment, a signal <span class="hlt">separation</span> method based on multi-level digital channelization is proposed in this paper. A two-level structure which can divide signal into different channel is designed first, after that, the peaks of different channels are tracked using the track filter and the coincident signals in time domain are <span class="hlt">separated</span> in time-<span class="hlt">frequency</span> domain. Finally, the time domain waveforms of different signals are acquired by reverse transformation. The validness of the proposed method is proved by experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29733288','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29733288"><span>Low-Temperature <span class="hlt">Variation</span> of Acoustic Velocity in PDMS for High-<span class="hlt">Frequency</span> Applications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Streque, Jeremy; Rouxel, Didier; Talbi, Abdelkrim; Thomassey, Matthieu; Vincent, Brice</p> <p>2018-05-01</p> <p>Polydimethylsiloxane (PDMS) and other related silicon-based polymers are among the most widely employed elastomeric materials in microsystems, owing to their physical and chemical properties. Meanwhile, surface acoustic wave (SAW) and bulk acoustic wave (BAW) sensors and filters have been vastly explored for sensing and wireless applications. Many fields could benefit from the combined use of acoustic wave devices, and polydimethylsiloxane-based soft-substrates, microsystems, or packaging elements. The mechanical constants of PDMS strongly depend on <span class="hlt">frequency</span>, similar to rubber materials. This brings to the exploration of the specific mechanical properties of PDMS encountered at high <span class="hlt">frequency</span>, required for its exploitation in SAW or BAW devices. First, low-<span class="hlt">frequency</span> mechanical behavior is confirmed from stress strain measurements, remaining useful for the exploitation of PDMS as a soft substrate or packaging material. The study, then, proposes a temperature-dependent, high-<span class="hlt">frequency</span> mechanical study of PDMS based on Brillouin spectroscopy to determine the evolution of the longitudinal acoustic velocity in this material, which constitutes the main mechanical parameter for the design of acoustic wave devices. The PDMS glass transition is then retrieved by differential scanning calorimetry in order to confirm the observations made by Brillouin spectroscopy. This paper validates Brillouin spectroscopy as a very suitable characterization technique for the retrieval of longitudinal mechanical properties at low temperature, as a preliminary investigation for the design of acoustic wave devices coupled with soft materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5006941','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5006941"><span>Perceptual Qualities of Ethanol Depend on Concentration, and <span class="hlt">Variation</span> in These Percepts Associates with Drinking <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>Nolden, Alissa A.</p> <p>2016-01-01</p> <p>Introduction Ethanol, the pharmaceutically active ingredient in all alcoholic beverages, elicits multiple percepts including sweet, bitter, drying, and burning. However, quality-specific perceptual dose-response functions have not been previously reported. Also, individual differences in ethanol perception may associate with differences in alcoholic beverage use. Here, we describe the chemosensory profile of ethanol across concentrations in a convenience sample of mixed-age adults; secondarily, we explore whether individual differences in various qualities from ethanol associate with alcohol use behaviors. Methods Participants (n=100, 33 men) aged 21 to 55 (mean 33 years) tasted ethanol in water (4, 8, 16, 32, and 48 % v/v) and rated sweetness, bitterness, drying, and burning/tingling on four general Labeled Magnitude Scales. Demographic question and alcohol use measures (years drinking and reported <span class="hlt">frequency</span> of drinking occasions) were also collected. Results Intensity of most qualities increased as a function of ethanol concentration, although the dominant sensation differed with concentration. The dominant sensation for 8 and 16 % ethanol was bitterness (7.4±1.0; 13.5±1.4), whereas for 32 and 48 % ethanol, burning/tingling was the dominant sensation (29.7±2.1; 44.7±2.4). <span class="hlt">Variation</span> in quality-specific intensities of sampled ethanol explained variability in the reported intake <span class="hlt">frequency</span> for beer, wine, straight spirits, and number of drinking occasions. The number of years reported drinking (grand mean 10.5±0.8) was not significantly associated with perceptual ratings for sampled ethanol. Conclusions In a convenience sample of mixed-aged adults, the sensations from suprathreshold ethanol varied by concentration: bitterness dominated at lower concentrations, while burn dominated at higher concentrations. Exploratory analyses also suggest that differences in chemosensory responses across participants may associate with measures of alcohol use. PMID:27594968</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3331741','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3331741"><span>Deep Resequencing Unveils Genetic Architecture of ADIPOQ and Identifies a Novel Low-<span class="hlt">Frequency</span> Variant Strongly Associated With Adiponectin <span class="hlt">Variation</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>Warren, Liling L.; Li, Li; Nelson, Matthew R.; Ehm, Margaret G.; Shen, Judong; Fraser, Dana J.; Aponte, Jennifer L.; Nangle, Keith L.; Slater, Andrew J.; Woollard, Peter M.; Hall, Matt D.; Topp, Simon D.; Yuan, Xin; Cardon, Lon R.; Chissoe, Stephanie L.; Mooser, Vincent; Morris, Andrew D.; Palmer, Colin N.A.; Perry, John R.; Frayling, Timothy M.; Whittaker, John C.; Waterworth, Dawn M.</p> <p>2012-01-01</p> <p>Increased adiponectin levels have been shown to be associated with a lower risk of type 2 diabetes. To understand the relations between genetic <span class="hlt">variation</span> at the adiponectin-encoding gene, ADIPOQ, and adiponectin levels, and subsequently its role in disease, we conducted a deep resequencing experiment of ADIPOQ in 14,002 subjects, including 12,514 Europeans, 594 African Americans, and 567 Indian Asians. We identified 296 single nucleotide polymorphisms (SNPs), including 30 amino acid changes, and carried out association analyses in a subset of 3,665 subjects from two independent studies. We confirmed multiple genome-wide association study findings and identified a novel association between a low-<span class="hlt">frequency</span> SNP (rs17366653) and adiponectin levels (P = 2.2E–17). We show that seven SNPs exert independent effects on adiponectin levels. Together, they explained 6% of adiponectin <span class="hlt">variation</span> in our samples. We subsequently assessed association between these SNPs and type 2 diabetes in the Genetics of Diabetes Audit and Research in Tayside Scotland (GO-DARTS) study, comprised of 5,145 case and 6,374 control subjects. No evidence of association with type 2 diabetes was found, but we were also unable to exclude the possibility of substantial effects (e.g., odds ratio 95% CI for rs7366653 [0.91–1.58]). Further investigation by large-scale and well-powered Mendelian randomization studies is warranted. PMID:22403302</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21315395','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21315395"><span>Regional price differences and food consumption <span class="hlt">frequency</span> among elementary school children.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sturm, R; Datar, A</p> <p>2011-03-01</p> <p>Food prices may affect diet and weight gain among youth and lead to geographic disparities in obesity. This paper examines the association between regional prices and consumption <span class="hlt">frequency</span> of fruit/vegetables and snack items among elementary school children in the USA. Observational study using individual-level survey data of fifth-grade children (average age 11 years) and regional food prices based on store visits in 2004. Dependent variables are self-reported consumption <span class="hlt">frequency</span> in fifth grade; primary explanatory variables are metropolitan area food prices relative to cost of living. Multivariate regression analysis. Price <span class="hlt">variation</span> across metropolitan areas exists, and lower real prices for vegetables and fruits predict significantly higher intake <span class="hlt">frequency</span>. Higher dairy prices predict lower <span class="hlt">frequency</span> of milk consumption, while higher meat prices predict increased milk consumption. Similar price effects were not found for fast food or soft drink consumption. The geographic <span class="hlt">variation</span> in food prices across the USA is sufficiently large to affect dietary patterns among youth for fruit, vegetables and milk. The price <span class="hlt">variation</span> is either too small to affect children's consumption <span class="hlt">frequency</span> of fast food or soft drinks, or the consumption of these foods is less price sensitive. Copyright © 2010 The Royal Society for Public Health. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3073594','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3073594"><span>Regional price differences and food consumption <span class="hlt">frequency</span> among elementary school children</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Sturm, R.; Datar, A.</p> <p>2010-01-01</p> <p>SUMMARY Objective Food prices may affect diet and weight gain among youth and lead to geographic disparities in obesity. This paper examines the association between regional prices and consumption <span class="hlt">frequency</span> of fruit/vegetables and snack items among elementary school children in the USA. Study design Observational study using individual-level survey data of fifth-grade children (average age 11 years) and regional food prices based on store visits in 2004. Methods Dependent variables are self-reported consumption <span class="hlt">frequency</span> in fifth grade; primary explanatory variables are metropolitan area food prices relative to cost of living. Multivariate regression analysis. Results Price <span class="hlt">variation</span> across metropolitan areas exists, and lower real prices for vegetables and fruits predict significantly higher intake <span class="hlt">frequency</span>. Higher dairy prices predict lower <span class="hlt">frequency</span> of milk consumption, while higher meat prices predict increased milk consumption. Similar price effects were not found for fast food or soft drink consumption. Discussion The geographic <span class="hlt">variation</span> in food prices across the USA is sufficiently large to affect dietary patterns among youth for fruit, vegetables and milk. This suggests that either the price <span class="hlt">variation</span> is too small to affect children’s consumption <span class="hlt">frequency</span> of fast food or soft drinks, or that the consumption of these foods is less price sensitive. PMID:21315395</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22483216-chaotic-attractors-separated-scrolls','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22483216-chaotic-attractors-separated-scrolls"><span>Chaotic attractors with <span class="hlt">separated</span> scrolls</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>Bouallegue, Kais, E-mail: kais-bouallegue@yahoo.fr</p> <p>2015-07-15</p> <p>This paper proposes a new behavior of chaotic attractors with <span class="hlt">separated</span> scrolls while combining Julia's process with Chua's attractor and Lorenz's attractor. The main motivation of this work is the ability to generate a set of <span class="hlt">separated</span> scrolls with different behaviors, which in turn allows us to choose one or many scrolls combined with modulation (amplitude and <span class="hlt">frequency</span>) for secure communication or synchronization. This set seems a new class of hyperchaos because each element of this set looks like a simple chaotic attractor with one positive Lyapunov exponent, so the cardinal of this set is greater than one. This newmore » approach could be used to generate more general higher-dimensional hyperchaotic attractor for more potential application. Numerical simulations are given to show the effectiveness of the proposed theoretical results.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ASPC..499..361M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ASPC..499..361M"><span>ALMA High <span class="hlt">Frequency</span> Techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, J. D.; Mason, B.; Impellizzeri, V.; Kameno, S.; Fomalont, E.; Chibueze, J.; Takahashi, S.; Remijan, A.; Wilson, C.; ALMA Science Team</p> <p>2015-12-01</p> <p>The purpose of the ALMA High <span class="hlt">Frequency</span> Campaign is to improve the quality and efficiency of science observing in Bands 8, 9, and 10 (385-950 GHz), the highest <span class="hlt">frequencies</span> available to the ALMA project. To this end, we outline observing modes which we have demonstrated to improve high <span class="hlt">frequency</span> calibration for the 12m array and the ACA, and we present the calibration of the total power antennas at these <span class="hlt">frequencies</span>. Band-to-band (B2B) transfer and bandwidth switching (BWSW), techniques which improve the speed and accuracy of calibration at the highest <span class="hlt">frequencies</span>, are most necessary in Bands 8, 9, and 10 due to the rarity of strong calibrators. These techniques successfully enable increased signal-to-noise on the calibrator sources (and better calibration solutions) by measuring the calibrators at lower <span class="hlt">frequencies</span> (B2B) or in wider bandwidths (BWSW) compared to the science target. We have also demonstrated the stability of the bandpass shape to better than 2.4% for 1 hour, hidden behind random noise, in Band 9. Finally, total power observing using the dual sideband receivers in Bands 9 and 10 requires the <span class="hlt">separation</span> of the two sidebands; this procedure has been demonstrated in Band 9 and is undergoing further testing in Band 10.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AJ....135.2526C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AJ....135.2526C"><span>The Evolution of the Multiplicity of Embedded Protostars. II. Binary <span class="hlt">Separation</span> Distribution and Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Connelley, Michael S.; Reipurth, Bo; Tokunaga, Alan T.</p> <p>2008-06-01</p> <p>We present the Class I protostellar binary <span class="hlt">separation</span> distribution based on the data tabulated in a companion paper. We verify the excess of Class I binary stars over solar-type main-sequence stars in the <span class="hlt">separation</span> range from 500 AU to 4500 AU. Although our sources are in nearby star-forming regions distributed across the entire sky (including Orion), none of our objects are in a high stellar density environment. A log-normal function, used by previous authors to fit the main-sequence and T Tauri binary <span class="hlt">separation</span> distributions, poorly fits our data, and we determine that a log-uniform function is a better fit. Our observations show that the binary <span class="hlt">separation</span> distribution changes significantly during the Class I phase, and that the binary <span class="hlt">frequency</span> at <span class="hlt">separations</span> greater than 1000 AU declines steadily with respect to spectral index. Despite these changes, the binary <span class="hlt">frequency</span> remains constant until the end of the Class I phase, when it drops sharply. We propose a scenario to account for the changes in the Class I binary <span class="hlt">separation</span> distribution. This scenario postulates that a large number of companions with a <span class="hlt">separation</span> greater than ~1000 AU were ejected during the Class 0 phase, but remain gravitationally bound due to the significant mass of the Class I envelope. As the envelope dissipates, these companions become unbound and the binary <span class="hlt">frequency</span> at wide <span class="hlt">separations</span> declines. Circumstellar and circumbinary disks are expected to play an important role in the orbital evolution at closer <span class="hlt">separations</span>. This scenario predicts that a large number of Class 0 objects should be non-hierarchical multiple systems, and that many Class I young stellar objects (YSOs) with a widely <span class="hlt">separated</span> companion should also have a very close companion. We also find that Class I protostars are not dynamically pristine, but have experienced dynamical evolution before they are visible as Class I objects. Our analysis shows that the Class I binary <span class="hlt">frequency</span> and the binary <span class="hlt">separation</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.G32B..03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.G32B..03W"><span>High <span class="hlt">Frequency</span> <span class="hlt">Variations</span> in Earth Orientation Derived From GNSS Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weber, R.; Englich, S.; Snajdrova, K.; Boehm, J.</p> <p>2006-12-01</p> <p>Current observations gained by the space geodetic techniques, especially VLBI, GPS and SLR, allow for the determination of Earth Orientation Parameters (EOPs - polar motion, UT1/LOD, nutation offsets) with unprecedented accuracy and temporal resolution. This presentation focuses on contributions to the EOP recovery provided by satellite navigation systems (primarily GPS). The IGS (International GNSS Service), for example, currently provides daily polar motion with an accuracy of less than 0.1mas and LOD estimates with an accuracy of a few microseconds. To study more rapid <span class="hlt">variations</span> in polar motion and LOD we established in a first step a high resolution (hourly resolution) ERP-time series from GPS observation data of the IGS network covering the period from begin of 2005 till March 2006. The calculations were carried out by means of the Bernese GPS Software V5.0 considering observations from a subset of 79 fairly stable stations out of the IGb00 reference frame sites. From these ERP time series the amplitudes of the major diurnal and semidiurnal <span class="hlt">variations</span> caused by ocean tides are estimated. After correcting the series for ocean tides the remaining geodetic observed excitation is compared with <span class="hlt">variations</span> of atmospheric excitation (AAM). To study the sensitivity of the estimates with respect to the applied mapping function we applied both the widely used NMF (Niell Mapping Function) and the VMF1 (Vienna Mapping Function 1). In addition, based on computations covering two months in 2005, the potential improvement due to the use of additional GLONASS data will be discussed. Finally, satellite techniques are also able to provide nutation offset rates with respect to the most recent nutation model. Based on GPS observations from 2005 we established nutation rate time series and subsequently derived the amplitudes of several nutation waves with periods less than 30 days. The results are compared to VLBI estimates processed by means of the OCCAM 6.1 software.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5499255','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5499255"><span>Genetic <span class="hlt">Variation</span> and Its Reflection on Posttranslational Modifications in <span class="hlt">Frequency</span> Clock and Mating Type a-1 Proteins in Sordaria fimicola</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Arif, Rabia; Akram, Faiza; Jamil, Tazeen; Lee, Siu Fai</p> <p>2017-01-01</p> <p>Posttranslational modifications (PTMs) occur in all essential proteins taking command of their functions. There are many domains inside proteins where modifications take place on side-chains of amino acids through various enzymes to generate different species of proteins. In this manuscript we have, for the first time, predicted posttranslational modifications of <span class="hlt">frequency</span> clock and mating type a-1 proteins in Sordaria fimicola collected from different sites to see the effect of environment on proteins or various amino acids pickings and their ultimate impact on consensus sequences present in mating type proteins using bioinformatics tools. Furthermore, we have also measured and walked through genomic DNA of various Sordaria strains to determine genetic diversity by genotyping the short sequence repeats (SSRs) of wild strains of S. fimicola collected from contrasting environments of two opposing slopes (harsh and xeric south facing slope and mild north facing slope) of Evolution Canyon (EC), Israel. Based on the whole genome sequence of S. macrospora, we targeted 20 genomic regions in S. fimicola which contain short sequence repeats (SSRs). Our data revealed genetic <span class="hlt">variations</span> in strains from south facing slope and these findings assist in the hypothesis that genetic <span class="hlt">variations</span> caused by stressful environments lead to evolution. PMID:28717646</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28717646','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28717646"><span>Genetic <span class="hlt">Variation</span> and Its Reflection on Posttranslational Modifications in <span class="hlt">Frequency</span> Clock and Mating Type a-1 Proteins in Sordaria fimicola.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Arif, Rabia; Akram, Faiza; Jamil, Tazeen; Mukhtar, Hamid; Lee, Siu Fai; Saleem, Muhammad</p> <p>2017-01-01</p> <p>Posttranslational modifications (PTMs) occur in all essential proteins taking command of their functions. There are many domains inside proteins where modifications take place on side-chains of amino acids through various enzymes to generate different species of proteins. In this manuscript we have, for the first time, predicted posttranslational modifications of <span class="hlt">frequency</span> clock and mating type a-1 proteins in Sordaria fimicola collected from different sites to see the effect of environment on proteins or various amino acids pickings and their ultimate impact on consensus sequences present in mating type proteins using bioinformatics tools. Furthermore, we have also measured and walked through genomic DNA of various Sordaria strains to determine genetic diversity by genotyping the short sequence repeats (SSRs) of wild strains of S. fimicola collected from contrasting environments of two opposing slopes (harsh and xeric south facing slope and mild north facing slope) of Evolution Canyon (EC), Israel. Based on the whole genome sequence of S. macrospora , we targeted 20 genomic regions in S. fimicola which contain short sequence repeats (SSRs). Our data revealed genetic <span class="hlt">variations</span> in strains from south facing slope and these findings assist in the hypothesis that genetic <span class="hlt">variations</span> caused by stressful environments lead to evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120007494','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120007494"><span><span class="hlt">Frequency</span> to Voltage Converter Analog Front-End Prototype</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mata, Carlos; Raines, Matthew</p> <p>2012-01-01</p> <p>The <span class="hlt">frequency</span> to voltage converter analog front end evaluation prototype (F2V AFE) is an evaluation board designed for comparison of different methods of accurately extracting the <span class="hlt">frequency</span> of a sinusoidal input signal. A configurable input stage is routed to one or several of five <span class="hlt">separate</span>, configurable filtering circuits, and then to a configurable output stage. Amplifier selection and gain, filter corner <span class="hlt">frequencies</span>, and comparator hysteresis and voltage reference are all easily configurable through the use of jumpers and potentiometers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26978944','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26978944"><span>High-<span class="hlt">Frequency</span> Observation of Water Spectrum and Its Application in Monitoring of Dynamic <span class="hlt">Variation</span> of Suspended Materials in the Hangzhou Bay.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dai, Qian; Pan, De-lu; He, Xian-qiang; Zhu, Qian-kun; Gong, Fang; Huang, Hai-qing</p> <p>2015-11-01</p> <p>In situ measurement of water spectrum is the basis of the validation of the ocean color remote sensing. The traditional method to obtain the water spectrum is based on the shipboard measurement at limited stations, which is difficult to meet the requirement of validation of ocean color remote sensing in the highly dynamic coastal waters. To overcome this shortage, continuously observing systems of water spectrum have been developed in the world. However, so far, there are still few high-<span class="hlt">frequency</span> observation systems of the water spectrum in coastal waters, especially in the highly turbid and high-dynamic waters. Here, we established a high-<span class="hlt">frequency</span> water-spectrum observing system based on tower in the Hangzhou Bay. The system measures the water spectrum at a step of 3 minutes, which can fully match the satellite observation. In this paper, we primarily developed a data processing method for the tower-based high-<span class="hlt">frequency</span> water spectrum data, to realize automatic judgment of clear sky, sun glint, platform shadow, and weak illumination, etc. , and verified the processing results. The results show that the normalized water-leaving radiance spectra obtained through tower observation have relatively high consistency with the shipboard measurement results, with correlation coefficient of more than 0. 99, and average relative error of 9.96%. In addition, the long-term observation capability of the tower-based high-<span class="hlt">frequency</span> water-spectrum observing system was evaluated, and the results show that although the system has run for one year, the normalized water-leaving radiance obtained by this system have good consistency with the synchronously measurement by Portable spectrometer ASD in respect of spectral shape and value, with correlation coefficient of more than 0.90 and average relative error of 6.48%. Moreover, the water spectra from high-<span class="hlt">frequency</span> observation by the system can be used to effectively monitor the rapid dynamic <span class="hlt">variation</span> in concentration of suspended</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21364687-decoherence-collisional-frequency-shifts-trapped-bosons-fermions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21364687-decoherence-collisional-frequency-shifts-trapped-bosons-fermions"><span>Decoherence and Collisional <span class="hlt">Frequency</span> Shifts of Trapped Bosons and Fermions</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>Gibble, Kurt; LNE-SYRTE, Observatoire de Paris, 75014 Paris</p> <p>2009-09-11</p> <p>We perform exact calculations of collisional <span class="hlt">frequency</span> shifts for several fermions or bosons using a singlet and triplet basis for pairs of particles. The 'factor of 2 controversy' for bosons becomes clear - the factor is always 2. Decoherence is described by singlet states and they are unaffected by spatially uniform clock fields. Spatial <span class="hlt">variations</span> are critical, especially for fermions which were previously thought to be immune to collision shifts. The spatial <span class="hlt">variations</span> lead to decoherence and a novel <span class="hlt">frequency</span> shift that is not proportional to the partial density of internal states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ApJ...783...89B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ApJ...783...89B"><span>Evidence of Resonant Mode Coupling and the Relationship between Low and High <span class="hlt">Frequencies</span> in a Rapidly Rotating a Star</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Breger, M.; Montgomery, M. H.</p> <p>2014-03-01</p> <p>In the theory of resonant mode coupling, the parent and child modes are directly related in <span class="hlt">frequency</span> and phase. The oscillations present in the fast rotating δ Sct star KIC 8054146 allow us to test the most general and generic aspects of such a theory. The only direct way to <span class="hlt">separate</span> the parent and coupled (child) modes is to examine the correlations in amplitude variability between the different <span class="hlt">frequencies</span>. For the dominant family of related <span class="hlt">frequencies</span>, only a single mode and a triplet are the origins of nine dominant <span class="hlt">frequency</span> peaks ranging from 2.93 to 66.30 cycles day-1 (as well as dozens of small-amplitude combination modes and a predicted and detected third high-<span class="hlt">frequency</span> triplet). The mode-coupling model correctly predicts the large amplitude <span class="hlt">variations</span> of the coupled modes as a product of the amplitudes of the parent modes, while the phase changes are also correctly modeled. This differs from the behavior of "normal" combination <span class="hlt">frequencies</span> in that the amplitudes are three orders of magnitude larger and may exceed even the amplitudes of the parent modes. We show that two dominant low <span class="hlt">frequencies</span> at 5.86 and 2.93 cycles day-1 in the gravity-mode region are not harmonics of each other, and their properties follow those of the almost equidistant high-<span class="hlt">frequency</span> triplet. We note that the previously puzzling situation of finding two strong peaks in the low-<span class="hlt">frequency</span> region related by nearly a factor of two in <span class="hlt">frequency</span> has been seen in other δ Sct stars as well.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25281310','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25281310"><span>CNV amplitude as a neural correlate for stuttering <span class="hlt">frequency</span>: A case report of acquired stuttering.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vanhoutte, Sarah; Van Borsel, John; Cosyns, Marjan; Batens, Katja; van Mierlo, Pieter; Hemelsoet, Dimitri; Van Roost, Dirk; Corthals, Paul; De Letter, Miet; Santens, Patrick</p> <p>2014-11-01</p> <p>A neural hallmark of developmental stuttering is abnormal articulatory programming. One of the neurophysiological substrates of articulatory preparation is the contingent negative <span class="hlt">variation</span> (CNV). Unfortunately, CNV tasks are rarely performed in persons who stutter and mainly focus on the effect of task <span class="hlt">variation</span> rather than on interindividual <span class="hlt">variation</span> in stutter related variables. However, <span class="hlt">variations</span> in motor programming seem to be related to <span class="hlt">variation</span> in stuttering <span class="hlt">frequency</span>. The current study presents a case report of acquired stuttering following stroke and stroke related surgery in the left superior temporal gyrus. A speech related CNV task was administered at four points in time with differences in stuttering severity and <span class="hlt">frequency</span>. Unexpectedly, CNV amplitudes at electrode sites approximating bilateral motor and left inferior frontal gyrus appeared to be inversely proportional to stuttering <span class="hlt">frequency</span>. The higher the stuttering <span class="hlt">frequency</span>, the lower the activity for articulatory preparation. Thus, the amount of disturbance in motor programming seems to determine stuttering <span class="hlt">frequency</span>. At right frontal electrodes, a relative increase in CNV amplitude was seen at the test session with most severe stuttering. Right frontal overactivation is cautiously suggested to be a compensation strategy. In conclusion, late CNV amplitude elicited by a relatively simple speech task seems to be able to provide an objective, neural correlate of stuttering <span class="hlt">frequency</span>. The present case report supports the hypothesis that motor preparation has an important role in stuttering. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4985177','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4985177"><span>Highly-Efficient Charge <span class="hlt">Separation</span> and Polaron Delocalization in Polymer-Fullerene Bulk-Heterojunctions: A Comparative Multi-<span class="hlt">Frequency</span> EPR & DFT Study</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Niklas, Jens; Mardis, Kristy L.; Banks, Brian P.; Grooms, Gregory M.; Sperlich, Andreas; Dyakonov, Vladimir; Beaupré, Serge; Leclerc, Mario; Xu, Tao; Yu, Luping; Poluektov, Oleg G.</p> <p>2016-01-01</p> <p>The ongoing depletion of fossil fuels has led to an intensive search for additional renewable energy sources. Solar-based technologies could provide sufficient energy to satisfy the global economic demands in the near future. Photovoltaic (PV) cells are the most promising man-made devices for direct solar energy utilization. Understanding the charge <span class="hlt">separation</span> and charge transport in PV materials at a molecular level is crucial for improving the efficiency of the solar cells. Here, we use light-induced EPR spectroscopy combined with DFT calculations to study the electronic structure of charge <span class="hlt">separated</span> states in blends of polymers (P3HT, PCDTBT, and PTB7) and fullerene derivatives (C60-PCBM and C70-PCBM). Solar cells made with the same composites as active layers show power conversion efficiencies of 3.3% (P3HT), 6.1% (PCDTBT), and 7.3% (PTB7), respectively. Under illumination of these composites, two paramagnetic species are formed due to photo-induced electron transfer between the conjugated polymer and the fullerene. They are the positive, P+, and negative, P-, polarons on the polymer backbone and fullerene cage, respectively, and correspond to radical cations and radical anions. Using the high spectral resolution of high-<span class="hlt">frequency</span> EPR (130 GHz), the EPR spectra of these species were resolved and principal components of the g-tensors were assigned. Light-induced pulsed ENDOR spectroscopy allowed the determination of 1H hyperfine coupling constants of photogenerated positive and negative polarons. The experimental results obtained for the different polymer-fullerene composites have been compared with DFT calculations, revealing that in all three systems the positive polaron is distributed over distances of 40 - 60 Å on the polymer chain. This corresponds to about 15 thiophene units for P3HT, approximately three units PCDTBT, and about three to four units for PTB7. No spin density delocalization between neighboring fullerene molecules was detected by EPR. Strong</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JPhCS.574a2120M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JPhCS.574a2120M"><span>Cluster analysis of word <span class="hlt">frequency</span> dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maslennikova, Yu S.; Bochkarev, V. V.; Belashova, I. A.</p> <p>2015-01-01</p> <p>This paper describes the analysis and modelling of word usage <span class="hlt">frequency</span> time series. During one of previous studies, an assumption was put forward that all word usage <span class="hlt">frequencies</span> have uniform dynamics approaching the shape of a Gaussian function. This assumption can be checked using the <span class="hlt">frequency</span> dictionaries of the Google Books Ngram database. This database includes 5.2 million books published between 1500 and 2008. The corpus contains over 500 billion words in American English, British English, French, German, Spanish, Russian, Hebrew, and Chinese. We clustered time series of word usage <span class="hlt">frequencies</span> using a Kohonen neural network. The similarity between input vectors was estimated using several algorithms. As a result of the neural network training procedure, more than ten different forms of time series were found. They describe the dynamics of word usage <span class="hlt">frequencies</span> from birth to death of individual words. Different groups of word forms were found to have different dynamics of word usage <span class="hlt">frequency</span> <span class="hlt">variations</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5400112','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5400112"><span>Graph <span class="hlt">Frequency</span> Analysis of Brain Signals</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huang, Weiyu; Goldsberry, Leah; Wymbs, Nicholas F.; Grafton, Scott T.; Bassett, Danielle S.; Ribeiro, Alejandro</p> <p>2016-01-01</p> <p>This paper presents methods to analyze functional brain networks and signals from graph spectral perspectives. The notion of <span class="hlt">frequency</span> and filters traditionally defined for signals supported on regular domains such as discrete time and image grids has been recently generalized to irregular graph domains, and defines brain graph <span class="hlt">frequencies</span> associated with different levels of spatial smoothness across the brain regions. Brain network <span class="hlt">frequency</span> also enables the decomposition of brain signals into pieces corresponding to smooth or rapid <span class="hlt">variations</span>. We relate graph <span class="hlt">frequency</span> with principal component analysis when the networks of interest denote functional connectivity. The methods are utilized to analyze brain networks and signals as subjects master a simple motor skill. We observe that brain signals corresponding to different graph <span class="hlt">frequencies</span> exhibit different levels of adaptability throughout learning. Further, we notice a strong association between graph spectral properties of brain networks and the level of exposure to tasks performed, and recognize the most contributing and important <span class="hlt">frequency</span> signatures at different levels of task familiarity. PMID:28439325</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017A%26A...597A.131W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017A%26A...597A.131W"><span>Monopole and dipole estimation for multi-<span class="hlt">frequency</span> sky maps by linear regression</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wehus, I. K.; Fuskeland, U.; Eriksen, H. K.; Banday, A. J.; Dickinson, C.; Ghosh, T.; Górski, K. M.; Lawrence, C. R.; Leahy, J. P.; Maino, D.; Reich, P.; Reich, W.</p> <p>2017-01-01</p> <p>We describe a simple but efficient method for deriving a consistent set of monopole and dipole corrections for multi-<span class="hlt">frequency</span> sky map data sets, allowing robust parametric component <span class="hlt">separation</span> with the same data set. The computational core of this method is linear regression between pairs of <span class="hlt">frequency</span> maps, often called T-T plots. Individual contributions from monopole and dipole terms are determined by performing the regression locally in patches on the sky, while the degeneracy between different <span class="hlt">frequencies</span> is lifted whenever the dominant foreground component exhibits a significant spatial spectral index <span class="hlt">variation</span>. Based on this method, we present two different, but each internally consistent, sets of monopole and dipole coefficients for the nine-year WMAP, Planck 2013, SFD 100 μm, Haslam 408 MHz and Reich & Reich 1420 MHz maps. The two sets have been derived with different analysis assumptions and data selection, and provide an estimate of residual systematic uncertainties. In general, our values are in good agreement with previously published results. Among the most notable results are a relative dipole between the WMAP and Planck experiments of 10-15μK (depending on <span class="hlt">frequency</span>), an estimate of the 408 MHz map monopole of 8.9 ± 1.3 K, and a non-zero dipole in the 1420 MHz map of 0.15 ± 0.03 K pointing towards Galactic coordinates (l,b) = (308°,-36°) ± 14°. These values represent the sum of any instrumental and data processing offsets, as well as any Galactic or extra-Galactic component that is spectrally uniform over the full sky.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27627739','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27627739"><span>Morphological <span class="hlt">variation</span> among the inner ears of extinct and extant baleen whales (Cetacea: Mysticeti).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ekdale, Eric G</p> <p>2016-12-01</p> <p>Living mysticetes (baleen whales) and odontocetes (toothed whales) differ significantly in auditory function in that toothed whales are sensitive to high-<span class="hlt">frequency</span> and ultrasonic sound vibrations and mysticetes to low-<span class="hlt">frequency</span> and infrasonic noises. Our knowledge of the evolution and phylogeny of cetaceans, and mysticetes in particular, is at a point at which we can explore morphological and physiological changes within the baleen whale inner ear. Traditional comparative anatomy and landmark-based 3D-geometric morphometric analyses were performed to investigate the anatomical diversity of the inner ears of extinct and extant mysticetes in comparison with other cetaceans. Principal component analyses (PCAs) show that the cochlear morphospace of odontocetes is tangential to that of mysticetes, but odontocetes are completely <span class="hlt">separated</span> from mysticetes when semicircular canal landmarks are combined with the cochlear data. The cochlea of the archaeocete Zygorhiza kochii and early diverging extinct mysticetes plot within the morphospace of crown mysticetes, suggesting that mysticetes possess ancestral cochlear morphology and physiology. The PCA results indicate <span class="hlt">variation</span> among mysticete species, although no major patterns are recovered to suggest <span class="hlt">separate</span> hearing or locomotor regimes. Phylogenetic signal was detected for several clades, including crown Cetacea and crown Mysticeti, with the most clades expressing phylogenetic signal in the semicircular canal dataset. Brownian motion could not be excluded as an explanation for the signal, except for analyses combining cochlea and semicircular canal datasets for Balaenopteridae. J. Morphol. 277:1599-1615, 2016. © 2016 Wiley Periodicals, Inc. © 2016 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...5E9071T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...5E9071T"><span>Morphology of human sweat ducts observed by optical coherence tomography and their <span class="hlt">frequency</span> of resonance in the terahertz <span class="hlt">frequency</span> region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tripathi, Saroj R.; Miyata, Eisuke; Ishai, Paul Ben; Kawase, Kodo</p> <p>2015-03-01</p> <p>It is crucial to understand the various biological effects induced by terahertz (THz) electromagnetic waves with the rapid development of electronic and photonic devices operating in the THz <span class="hlt">frequency</span> region. The presence of sweat glands plays an important role in THz wave interactions with human skin. We investigated the morphological features of sweat ducts using optical coherence tomography (OCT) to further understand such phenomena. We observed remarkable features of the ducts, such as their clear helical structure. The intersubject and intrasubject <span class="hlt">variations</span> in the diameter of sweat ducts were considerably smaller than the <span class="hlt">variations</span> in other structural parameters, such as length and number of turns. Based on the sweat duct dimensions and THz dielectric properties of skin measured using terahertz time-domain spectroscopy (THz-TDS), we calculated the resonating <span class="hlt">frequency</span> of the sweat duct under the assumption of it functioning as a helical antenna. Here, we show that the resonance <span class="hlt">frequency</span> in the axial mode of operation lies in the THz wave region with a centre <span class="hlt">frequency</span> of 0.44 +/- 0.07 THz. We expect that these findings will further our understanding of the various health consequences of the interaction of THz waves with human beings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=267220','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=267220"><span>HILIC <span class="hlt">separation</span> mechanisms of tetracyclines on amino bonded silica column</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>Effects of mobile phase <span class="hlt">variations</span> on the chromatographic <span class="hlt">separation</span> on amino bonded silica column in hydrophilic interaction chromatography (HILIC) were investigated for four zwitterionic tetracyclines (TCs): oxytetracycline, doxycycline, chlortetracycline and tetracycline. A mixed-mode retention m...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27060816','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27060816"><span>Effect of ultrasound-enhanced fat <span class="hlt">separation</span> on whey powder phospholipid composition and stability.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Torkamani, Amir E; Juliano, Pablo; Fagan, Peter; Jiménez-Flores, Rafael; Ajlouni, Said; Singh, Tanoj K</p> <p>2016-06-01</p> <p>Fat from freshly pasteurized liquid whey was partially <span class="hlt">separated</span> by gravity for 5, 10, and 30min, with and without simultaneous application of ultrasound. Ultrasound treatments were carried out at 400 and 1,000 kHz at different specific energy inputs (23-390 kJ/kg). The fat-enriched top layers (L1) and the fat-depleted bottom layers (L2) were <span class="hlt">separately</span> removed and freeze-dried. Nonsonicated and sonicated L2 powders were stored for 14d at ambient temperature to assess their oxidative stability. Creaming was enhanced at both <span class="hlt">frequencies</span> and fat <span class="hlt">separation</span> increased with higher ultrasonic energy, extended sonication, or both. The oxidative volatile compound content decreased in defatted whey powders below published odor detection threshold values for all cases. Sonication had a minor influence on the partitioning of phospholipids with fat <span class="hlt">separation</span>. The current study suggested that ultrasonication at high <span class="hlt">frequency</span> enhanced fat <span class="hlt">separation</span> from freshly pasteurized whey while improving whey powder oxidative stability. Copyright © 2016 American Dairy Science Association. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ChPhB..24e5201W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ChPhB..24e5201W"><span>Low-<span class="hlt">frequency</span> oscillations in Hall thrusters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wei, Li-Qiu; Han, Liang; Yu, Da-Ren; Guo, Ning</p> <p>2015-05-01</p> <p>In this paper, we summarize the research development of low-<span class="hlt">frequency</span> oscillations in the last few decades. The findings of physical mechanism, characteristics and stabilizing methods of low-<span class="hlt">frequency</span> oscillations are discussed. It shows that it is unreasonable and incomplete to model an ionization region <span class="hlt">separately</span> to analyze the physical mechanism of low-<span class="hlt">frequency</span> oscillations. Electro-dynamics as well as the formation conditions of ionization distribution play an important role in characteristics and stabilizing of low-<span class="hlt">frequency</span> oscillations. Understanding the physical mechanism and characteristics of low- <span class="hlt">frequency</span> oscillations thoroughly and developing a feasible method stabilizing this instability are still important research subjects. Project supported by the National Natural Science Foundation of China (Grant No. 51477035), the Fundamental Research Funds for the Central Universities, China (Grant No. HIT.NSRIF 2015064), and the Open Research Fund Program of State Key Laboratory of Cryogenic Vacuum Technology and Physics, China (Grant No. ZDK201304).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4738879','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4738879"><span>Kinematic Analysis of Four Plyometric Push-Up <span class="hlt">Variations</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>MOORE, LAURA H.; TANKOVICH, MICHAEL J.; RIEMANN, BRYAN L.; DAVIES, GEORGE J.</p> <p>2012-01-01</p> <p>Plyometric research in the upper extremity is limited, with the effects of open-chain plyometric exercises being studied most. Kinematic and ground reaction force data concerning closed-chain upper extremity plyometrics has yet to be examined. Twenty-one recreationally active male subjects performed four <span class="hlt">variations</span> of plyometric push-ups in a counterbalanced order. These included box drop push-ups from 3.8 cm, 7.6 cm, 11.4 cm heights, and clap push-ups. Kinematics of the trunk, dominant extremity and both hands were collected to examine peak flight, elbow flexion at ground contact, elbow displacement, and hand <span class="hlt">separation</span>. Additionally peak vertical ground reaction force was measured under the dominant extremity. The 11.4 cm and clap push-ups had significantly higher peak flight than the other <span class="hlt">variations</span> (P<.001). At ground contact, the elbow was in significantly greater flexion for the 3.8 cm and clap push-up compared to the other <span class="hlt">variations</span> (P<.001). The clap push-up had significantly more elbow displacement than the other <span class="hlt">variations</span> (P<.001) while hand <span class="hlt">separation</span> was not significantly different between <span class="hlt">variations</span> (P=.129). Peak vertical ground reaction force was significantly greater for the clap push-ups than for all other <span class="hlt">variations</span> (P< .001). Despite similar flight heights between the 11.4 cm and clap push-ups, the greater peak vertical ground reaction force and elbow displacement of the clap push-ups indicates the clap push-up is the most intense of the <span class="hlt">variations</span> examined. Understanding the kinematic variables involved will aid in the creation of a closed chain upper-extremity plyometric progression. PMID:27182390</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28414369','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28414369"><span><span class="hlt">Frequency</span> comb calibrated <span class="hlt">frequency</span>-sweeping interferometry for absolute group refractive index measurement of air.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Lijun; Wu, Xuejian; Wei, Haoyun; Li, Yan</p> <p>2017-04-10</p> <p>The absolute group refractive index of air at 194061.02 GHz is measured in real time using <span class="hlt">frequency</span>-sweeping interferometry calibrated by an optical <span class="hlt">frequency</span> comb. The group refractive index of air is calculated from the calibration peaks of the laser <span class="hlt">frequency</span> <span class="hlt">variation</span> and the interference signal of the two beams passing through the inner and outer regions of a vacuum cell when the <span class="hlt">frequency</span> of a tunable external cavity diode laser is scanned. We continuously measure the refractive index of air for 2 h, which shows that the difference between measured results and Ciddor's equation is less than 9.6×10<sup>-8</sup>, and the standard deviation of that difference is 5.9×10<sup>-8</sup>. The relative uncertainty of the measured refractive index of air is estimated to be 8.6×10<sup>-8</sup>. The data update rate is 0.2 Hz, making it applicable under conditions in which air refractive index fluctuates fast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25838754','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25838754"><span>Effects of Parkinson's Disease on Fundamental <span class="hlt">Frequency</span> Variability in Running Speech.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bowen, Leah K; Hands, Gabrielle L; Pradhan, Sujata; Stepp, Cara E</p> <p>2013-09-01</p> <p>In Parkinson's Disease (PD), qualitative speech changes such as decreased <span class="hlt">variation</span> in pitch and loudness are common, but quantitative vocal changes are not well documented. The variability of fundamental <span class="hlt">frequency</span> (F0) in 32 individuals (23 male) with PD both ON and OFF levodopa medication was compared with 32 age-matched healthy controls (23 male). Participants read a single paragraph and estimates of fundamental <span class="hlt">frequency</span> (F0) variability were determined for the entire reading passage as well as for the first and last sentences of the passage <span class="hlt">separately</span>. F0 variability was significantly increased in controls relative to both PD groups and PD patients showed significantly higher F0 variability while ON medication relative to OFF. No significant effect of group was seen in the change in F0 variability from the beginning to the end of the reading passage. Female speakers were found to have higher F0 variability than males. F0 variability was both significantly reduced in PD relative to controls and significantly increased in patients with PD during use of dopaminergic medications. F0 variability changes over the course of reading a paragraph may not be indicative of PD but rather dependent on non-disease factors such as the linguistic characteristics of the text.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2894800','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2894800"><span>Ensembl <span class="hlt">variation</span> resources</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>2010-01-01</p> <p>Background The maturing field of genomics is rapidly increasing the number of sequenced genomes and producing more information from those previously sequenced. Much of this additional information is <span class="hlt">variation</span> data derived from sampling multiple individuals of a given species with the goal of discovering new variants and characterising the population <span class="hlt">frequencies</span> of the variants that are already known. These data have immense value for many studies, including those designed to understand evolution and connect genotype to phenotype. Maximising the utility of the data requires that it be stored in an accessible manner that facilitates the integration of <span class="hlt">variation</span> data with other genome resources such as gene annotation and comparative genomics. Description The Ensembl project provides comprehensive and integrated <span class="hlt">variation</span> resources for a wide variety of chordate genomes. This paper provides a detailed description of the sources of data and the methods for creating the Ensembl <span class="hlt">variation</span> databases. It also explores the utility of the information by explaining the range of query options available, from using interactive web displays, to online data mining tools and connecting directly to the data servers programmatically. It gives a good overview of the <span class="hlt">variation</span> resources and future plans for expanding the <span class="hlt">variation</span> data within Ensembl. Conclusions <span class="hlt">Variation</span> data is an important key to understanding the functional and phenotypic differences between individuals. The development of new sequencing and genotyping technologies is greatly increasing the amount of <span class="hlt">variation</span> data known for almost all genomes. The Ensembl <span class="hlt">variation</span> resources are integrated into the Ensembl genome browser and provide a comprehensive way to access this data in the context of a widely used genome bioinformatics system. All Ensembl data is freely available at http://www.ensembl.org and from the public MySQL database server at ensembldb.ensembl.org. PMID:20459805</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140007321','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140007321"><span>Drop Size Distribution - Based <span class="hlt">Separation</span> of Stratiform and Convective Rain</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thurai, Merhala; Gatlin, Patrick; Williams, Christopher</p> <p>2014-01-01</p> <p>For applications in hydrology and meteorology, it is often desirable to <span class="hlt">separate</span> regions of stratiform and convective rain from meteorological radar observations, both from ground-based polarimetric radars and from space-based dual <span class="hlt">frequency</span> radars. In a previous study by Bringi et al. (2009), dual <span class="hlt">frequency</span> profiler and dual polarization radar (C-POL) observations in Darwin, Australia, had shown that stratiform and convective rain could be <span class="hlt">separated</span> in the log10(Nw) versus Do domain, where Do is the mean volume diameter and Nw is the scaling parameter which is proportional to the ratio of water content to the mass weighted mean diameter. Note, Nw and Do are two of the main drop size distribution (DSD) parameters. In a later study, Thurai et al (2010) confirmed that both the dual-<span class="hlt">frequency</span> profiler based stratiform-convective rain <span class="hlt">separation</span> and the C-POL radar based <span class="hlt">separation</span> were consistent with each other. In this paper, we test this <span class="hlt">separation</span> method using DSD measurements from a ground based 2D video disdrometer (2DVD), along with simultaneous observations from a collocated, vertically-pointing, X-band profiling radar (XPR). The measurements were made in Huntsville, Alabama. One-minute DSDs from 2DVD are used as input to an appropriate gamma fitting procedure to determine Nw and Do. The fitted parameters - after averaging over 3-minutes - are plotted against each other and compared with a predefined <span class="hlt">separation</span> line. An index is used to determine how far the points lie from the <span class="hlt">separation</span> line (as described in Thurai et al. 2010). Negative index values indicate stratiform rain and positive index indicate convective rain, and, moreover, points which lie somewhat close to the <span class="hlt">separation</span> line are considered 'mixed' or 'transition' type precipitation. The XPR observations are used to evaluate/test the 2DVD data-based classification. A 'bright-band' detection algorithm was used to classify each vertical reflectivity profile as either stratiform or convective</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25360934','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25360934"><span>Class-A dual-<span class="hlt">frequency</span> VECSEL at telecom wavelength.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>De, Syamsundar; Baili, Ghaya; Alouini, Mehdi; Harmand, Jean-Christophe; Bouchoule, Sophie; Bretenaker, Fabien</p> <p>2014-10-01</p> <p>We report class-A dual-<span class="hlt">frequency</span> oscillation at 1.55 μm in a vertical external cavity surface emitting laser with more than 100 mW optical power. The two orthogonal linear polarizations of different <span class="hlt">frequencies</span> oscillate simultaneously as their nonlinear coupling is reduced below unity by spatially <span class="hlt">separating</span> them inside the active medium. The spectral behavior of the radio <span class="hlt">frequency</span> beatnote obtained by optically mixing two polarizations and the phase noise of the beatnote have been explored for different coupling strengths between the lasing modes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhFl...25b2002W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhFl...25b2002W"><span><span class="hlt">Frequency</span> dependence and <span class="hlt">frequency</span> control of microbubble streaming flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Cheng; Rallabandi, Bhargav; Hilgenfeldt, Sascha</p> <p>2013-02-01</p> <p>Steady streaming from oscillating microbubbles is a powerful actuating mechanism in microfluidics, enjoying increased use due to its simplicity of manufacture, ease of integration, low heat generation, and unprecedented control over the flow field and particle transport. As the streaming flow patterns are caused by oscillations of microbubbles in contact with walls of the set-up, an understanding of the bubble dynamics is crucial. Here we experimentally characterize the oscillation modes and the <span class="hlt">frequency</span> response spectrum of such cylindrical bubbles, driven by a pressure <span class="hlt">variation</span> resulting from ultrasound in the range of 1 kHz raisebox {-.9ex{stackrel{textstyle <}{˜ }} }f raisebox {-.9ex{stackrel{textstyle <}{˜ }} } 100 kHz. We find that (i) the appearance of 2D streaming flow patterns is governed by the relative amplitudes of bubble azimuthal surface modes (normalized by the volume response), (ii) distinct, robust resonance patterns occur independent of details of the set-up, and (iii) the position and width of the resonance peaks can be understood using an asymptotic theory approach. This theory describes, for the first time, the shape oscillations of a pinned cylindrical bubble at a wall and gives insight into necessary mode couplings that shape the response spectrum. Having thus correlated relative mode strengths and observed flow patterns, we demonstrate that the performance of a bubble micromixer can be optimized by making use of such flow <span class="hlt">variations</span> when modulating the driving <span class="hlt">frequency</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23443553','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23443553"><span>Human haemodynamic <span class="hlt">frequency</span> harmonics regulate the inflammatory phenotype of vascular endothelial cells.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Feaver, Ryan E; Gelfand, Bradley D; Blackman, Brett R</p> <p>2013-01-01</p> <p>Haemodynamic <span class="hlt">variations</span> are inherent to blood vessel geometries (such as bifurcations) and correlate with regional development of inflammation and atherosclerosis. However, the complex <span class="hlt">frequency</span> spectrum characteristics from these haemodynamics have never been exploited to test whether <span class="hlt">frequency</span> <span class="hlt">variations</span> are critical determinants of endothelial inflammatory phenotype. Here we utilize an experimental Fourier transform analysis to systematically manipulate individual <span class="hlt">frequency</span> harmonics from human carotid shear stress waveforms applied in vitro to human endothelial cells. The <span class="hlt">frequency</span> spectrum, specifically the 0 th and 1st harmonics, is a significant regulator of inflammation, including NF-κB activity and downstream inflammatory phenotype. Further, a harmonic-based regression-model predicts eccentric NF-κB activity observed in the human internal carotid artery. Finally, short interfering RNA-knockdown of the mechanosensor PECAM-1 reverses <span class="hlt">frequency</span>-dependent regulation of NF-κB activity. Thus, PECAM-1 may have a critical role in the endothelium's exquisite sensitivity to complex shear stress <span class="hlt">frequency</span> harmonics and provide a mechanism for the focal development of vascular inflammation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JAG...107...25Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JAG...107...25Z"><span>Time-<span class="hlt">frequency</span> domain SNR estimation and its application in seismic data processing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Yan; Liu, Yang; Li, Xuxuan; Jiang, Nansen</p> <p>2014-08-01</p> <p>Based on an approach estimating <span class="hlt">frequency</span> domain signal-to-noise ratio (FSNR), we propose a method to evaluate time-<span class="hlt">frequency</span> domain signal-to-noise ratio (TFSNR). This method adopts short-time Fourier transform (STFT) to estimate instantaneous power spectrum of signal and noise, and thus uses their ratio to compute TFSNR. Unlike FSNR describing the <span class="hlt">variation</span> of SNR with <span class="hlt">frequency</span> only, TFSNR depicts the <span class="hlt">variation</span> of SNR with time and <span class="hlt">frequency</span>, and thus better handles non-stationary seismic data. By considering TFSNR, we develop methods to improve the effects of inverse Q filtering and high <span class="hlt">frequency</span> noise attenuation in seismic data processing. Inverse Q filtering considering TFSNR can better solve the problem of amplitude amplification of noise. The high <span class="hlt">frequency</span> noise attenuation method considering TFSNR, different from other de-noising methods, distinguishes and suppresses noise using an explicit criterion. Examples of synthetic and real seismic data illustrate the correctness and effectiveness of the proposed methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1449628','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1449628"><span>Patterned <span class="hlt">variation</span> in prehistoric chiefdoms</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Drennan, Robert D.; Peterson, Christian E.</p> <p>2006-01-01</p> <p>Comparative study of early complex societies (chiefdoms) conjures visions of a cultural evolutionary emphasis on similarities and societal typology. <span class="hlt">Variation</span> within the group has not been as systematically examined but offers an even more productive avenue of approach to fundamental principles of organization and change. Three widely <span class="hlt">separated</span> trajectories of early chiefdom development are compared here: the Valley of Oaxaca (Mexico), the Alto Magdalena (Colombia), and Northeast China. Archaeological data from all three regions are analyzed with the same tools to reveal <span class="hlt">variation</span> in human activities, relationships, and interactions as these change in the emergence of chiefly communities. Patterning in this <span class="hlt">variation</span> suggests the operation of underlying general principles, which are offered as hypotheses that merit further investigation and evaluation in comparative study of a much larger number of cases. PMID:16473941</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22429772-separative-analyses-chromatographic-column-packed-core-shell-adsorbent-lithium-isotope-separation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22429772-separative-analyses-chromatographic-column-packed-core-shell-adsorbent-lithium-isotope-separation"><span><span class="hlt">Separative</span> analyses of a chromatographic column packed with a core-shell adsorbent for lithium isotope <span class="hlt">separation</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>Sugiyama, T.; Sugura, K.; Enokida, Y.</p> <p>2015-03-15</p> <p>Lithium-6 is used as a blanket material for sufficient tritium production in DT fueled fusion reactors. A core-shell type adsorbent was proposed for lithium isotope <span class="hlt">separation</span> by chromatography. The mass transfer model in a chromatographic column consisted of 4 steps, such as convection and dispersion in the column, transfer through liquid films, intra-particle diffusion and and adsorption or desorption at the local adsorption sites. A model was developed and concentration profiles and time <span class="hlt">variation</span> in the column were numerically simulated. It became clear that core-shell type adsorbents with thin porous shell were saturated rapidly relatively to fully porous one andmore » established a sharp edge of adsorption band. This is very important feature because lithium isotope <span class="hlt">separation</span> requires long-distance development of adsorption band. The values of HETP (Height Equivalent of a Theoretical Plate) for core-shell adsorbent packed column were estimated by statistical moments of the step response curve. The value of HETP decreased with the thickness of the porous shell. A core-shell type adsorbent is, then, useful for lithium isotope <span class="hlt">separation</span>. (authors)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17236416','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17236416"><span>The long-term evolution of multilocus traits under <span class="hlt">frequency</span>-dependent disruptive selection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>van Doorn, G Sander; Dieckmann, Ulf</p> <p>2006-11-01</p> <p><span class="hlt">Frequency</span>-dependent disruptive selection is widely recognized as an important source of genetic <span class="hlt">variation</span>. Its evolutionary consequences have been extensively studied using phenotypic evolutionary models, based on quantitative genetics, game theory, or adaptive dynamics. However, the genetic assumptions underlying these approaches are highly idealized and, even worse, predict different consequences of <span class="hlt">frequency</span>-dependent disruptive selection. Population genetic models, by contrast, enable genotypic evolutionary models, but traditionally assume constant fitness values. Only a minority of these models thus addresses <span class="hlt">frequency</span>-dependent selection, and only a few of these do so in a multilocus context. An inherent limitation of these remaining studies is that they only investigate the short-term maintenance of genetic <span class="hlt">variation</span>. Consequently, the long-term evolution of multilocus characters under <span class="hlt">frequency</span>-dependent disruptive selection remains poorly understood. We aim to bridge this gap between phenotypic and genotypic models by studying a multilocus version of Levene's soft-selection model. Individual-based simulations and deterministic approximations based on adaptive dynamics theory provide insights into the underlying evolutionary dynamics. Our analysis uncovers a general pattern of polymorphism formation and collapse, likely to apply to a wide variety of genetic systems: after convergence to a fitness minimum and the subsequent establishment of genetic polymorphism at multiple loci, genetic <span class="hlt">variation</span> becomes increasingly concentrated on a few loci, until eventually only a single polymorphic locus remains. This evolutionary process combines features observed in quantitative genetics and adaptive dynamics models, and it can be explained as a consequence of changes in the selection regime that are inherent to <span class="hlt">frequency</span>-dependent disruptive selection. Our findings demonstrate that the potential of <span class="hlt">frequency</span>-dependent disruptive selection to maintain polygenic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830008400','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830008400"><span>Experimental measurements of unsteady turbulent boundary layers near <span class="hlt">separation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Simpson, R. L.</p> <p>1982-01-01</p> <p>Investigations conducted to document the behavior of turbulent boundary layers on flat surfaces that <span class="hlt">separate</span> due to adverse pressure gradients are reported. Laser and hot wire anemometers measured turbulence and flow structure of a steady free stream <span class="hlt">separating</span> turbulent boundary layer produced on the flow of a wind tunnel section. The effects of sinusoidal and unsteadiness of the free stream velocity on this <span class="hlt">separating</span> turbulent boundary layer at a reduced <span class="hlt">frequency</span> were determined. A friction gage and a thermal tuft were developed and used to measure the surface skin friction and the near wall fraction of time the flow moves downstream for several cases. Abstracts are provided of several articles which discuss the effects of the periodic free stream unsteadiness on the structure or <span class="hlt">separating</span> turbulent boundary layers.</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://hdl.handle.net/2060/19960003235','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960003235"><span>High-<span class="hlt">frequency</span> <span class="hlt">variations</span> in Earth rotation and the planetary momentum budget</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rosen, Richard D.</p> <p>1995-01-01</p> <p>The major focus of the subject contract was on helping to resolve one of the more notable discrepancies still existing in the axial momentum budget of the solid Earth-atmosphere system, namely the disappearance of coherence between length-of-day (l.o.d.) and atmospheric angular momentum (AAM) at periods shorter than about a fortnight. Recognizing the importance of identifying the source of the high-<span class="hlt">frequency</span> momentum budget anomaly, the scientific community organized two special measurement campaigns (SEARCH '92 and CONT '94) to obtain the best possible determinations of l.o.d. and AAM. An additional goal was to analyze newly developed estimates of the torques that transfer momentum between the atmosphere and its underlying surface to determine whether the ocean might be a reservoir of momentum on short time scales. Discrepancies between AAM and l.o.d. at sub-fortnightly periods have been attributed to either measurement errors in these quantities or the need to incorporate oceanic angular momentum into the planetary budget. Results from the SEARCH '92 and CONT '94 campaigns suggest that when special attention is paid to the quality of the measurements, better agreement between l.o.d. and AAM at high <span class="hlt">frequencies</span> can be obtained. The mechanism most responsible for the high-<span class="hlt">frequency</span> changes observed in AAM during these campaigns involves a direct coupling to the solid Earth, i.e, the mountain torque, thereby obviating a significant oceanic role.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080014213','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080014213"><span>Active Control of <span class="hlt">Separation</span> From the Flap of a Supercritical Airfoil</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Melton, LaTunia Pack; Yao, Chung-Sheng; Seifert, Avi</p> <p>2006-01-01</p> <p>Zero-mass-flux periodic excitation was applied at several regions on a simplified high-lift system to delay the occurrence of flow <span class="hlt">separation</span>. The NASA Energy Efficient Transport (EET) supercritical airfoil was equipped with a 15% chord simply hinged leading edge flap and a 25% chord simply hinged trailing edge flap. Detailed flow features were measured in an attempt to identify optimal actuator placement. The measurements included steady and unsteady model and tunnel wall pressures, wake surveys, arrays of surface hot-films, flow visualization, and particle image velocimetry (PIV). The current paper describes the application of active <span class="hlt">separation</span> control at several locations on the deflected trailing edge flap. High <span class="hlt">frequency</span> (F(+) approximately equal to 10) and low <span class="hlt">frequency</span> amplitude modulation (F(+) sub AM approximately equal to 1) of the high <span class="hlt">frequency</span> excitation were used for control. It was noted that the same performance gains were obtained with amplitude modulation and required only 30% of the momentum input required by pure sine excitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030063166','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030063166"><span>Active Control of <span class="hlt">Separation</span> From the Flap of a Supercritical Airfoil</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Melton, La Tunia Pack; Yao, Chung-Sheng; Seifert, Avi</p> <p>2003-01-01</p> <p>Active flow control in the form of periodic zero-mass-flux excitation was applied at several regions on the leading edge and trailing edge flaps of a simplified high-lift system t o delay flow <span class="hlt">separation</span>. The NASA Energy Efficient Transport (EET) supercritical airfoil was equipped with a 15% chord simply hinged leading edge flap and a 25% chord simply hinged trailing edge flap. Detailed flow features were measured in an attempt to identify optimal actuator placement. The measurements included steady and unsteady model and tunnel wall pressures, wake surveys, arrays of surface hot-films, flow visualization, and particle image velocimetry (PIV). The current paper describes the application of active <span class="hlt">separation</span> control at several locations on the deflected trailing edge flap. High <span class="hlt">frequency</span> (F(+) approx.= 10) and low <span class="hlt">frequency</span> amplitude modulation (F(+)AM approx.= 1) of the high <span class="hlt">frequency</span> excitation were used for control. Preliminary efforts to combine leading and trailing edge flap excitations are also reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010MNRAS.401.1602D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010MNRAS.401.1602D"><span>Impact of calibration errors on CMB component <span class="hlt">separation</span> using FastICA and ILC</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dick, Jason; Remazeilles, Mathieu; Delabrouille, Jacques</p> <p>2010-01-01</p> <p>The <span class="hlt">separation</span> of emissions from different astrophysical processes is an important step towards the understanding of observational data. This topic of component <span class="hlt">separation</span> is of particular importance in the observation of the relic cosmic microwave background (CMB) radiation, as performed by the Wilkinson Microwave Anisotropy Probe satellite and the more recent Planck mission, launched on 2009 May 14 from Kourou and currently taking data. When performing any sort of component <span class="hlt">separation</span>, some assumptions about the components must be used. One assumption that many techniques typically use is knowledge of the <span class="hlt">frequency</span> scaling of one or more components. This assumption may be broken in the presence of calibration errors. Here we compare, in the context of imperfect calibration, the recovery of a clean map of emission of the CMB from observational data with two methods: FastICA (which makes no assumption of the <span class="hlt">frequency</span> scaling of the components) and an `Internal Linear Combination' (ILC), which explicitly extracts a component with a given <span class="hlt">frequency</span> scaling. We find that even in the presence of small calibration errors (less than 1 per cent) with a Planck-style mission, the ILC method can lead to inaccurate CMB reconstruction in the high signal-to-noise ratio regime, because of partial cancellation of the CMB emission in the recovered map. While there is no indication that the failure of the ILC will translate to other foreground cleaning or component <span class="hlt">separation</span> techniques, we propose that all methods which assume knowledge of the <span class="hlt">frequency</span> scaling of one or more components be careful to estimate the effects of calibration errors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........35M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........35M"><span>Active Flow Control and Global Stability Analysis of <span class="hlt">Separated</span> Flow Over a NACA 0012 Airfoil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Munday, Phillip M.</p> <p></p> <p> definition of the coefficient of momentum, which successfully characterizes suppression of <span class="hlt">separation</span> and lift enhancement. The effect of angular momentum is incorporated into the modified coefficient of momentum by introducing a characteristic swirling jet velocity based on the non-dimensional swirl number. With the modified coefficient of momentum, this single value is able to categorize controlled flows into <span class="hlt">separated</span>, transitional, and attached flows. With inadequate control input (<span class="hlt">separated</span> flow regime), lift decreased compared to the baseline flow. Increasing the modified coefficient of momentum, flow transitions from <span class="hlt">separated</span> to attached and accordingly results in improved aerodynamic forces. Modifying the spanwise spacing, it is shown that the minimum modified coefficient of momentum input required to begin transitioning the flow is dependent on actuator spacing. The growth (or decay) of perturbations can facilitate or inhibit the influence of flow control inputs. Biglobal stability analysis is considered to further analyze the behavior of control inputs on <span class="hlt">separated</span> flow over a symmetric airfoil. Assuming a spanwise periodic waveform for the perturbations, the eigenvalues and eigenvectors about a base flow are solved to understand the influence of spanwise <span class="hlt">variation</span> on the development of the flow. Two algorithms are developed and validated to solve for the eigenvalues of the flow: an algebraic eigenvalue solver (matrix based) and a time-stepping algorithm. The matrix based approach is formulated without ever storing the matrices, creating a computationally memory efficient algorithm. Increasing the Reynolds number to Re = 23,000 over a NACA 0012 airfoil, the time-stepper method is implemented due to rising computational cost of the matrix-based method. Stability analysis about the time-averaged flow is performed for spanwise wavenumbers of beta = 1/c, 10pi/ c and 20pi/c, which the latter two wavenumbers are representative of the spanwise spacing between the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007APS..DFD.NK005T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007APS..DFD.NK005T"><span>Corner <span class="hlt">separation</span> and the onset of stall in an axial compressor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thiam, Aicha; Whittlesey, Robert; Wark, Candace; Williams, David</p> <p>2007-11-01</p> <p>Axial compressor performance is limited by the onset of stall between the diffusing passageways of the rotors and stators. The flow physics responsible for the stall depends on the blade geometry of the machine, and in this experiment stall develops from a blade-hub corner <span class="hlt">separation</span>. The 1.5 stage axial compressor consists of inlet guide vanes, a rotor and stator section. <span class="hlt">Separate</span> motors drive the downstream fan and rotor, which makes it possible to change the compressor pressure ratio and flow coefficient by changing either the wheel speed or the bulk flow rate through the machine. Detailed maps of the flow behind the stators and in front of the rotors were obtained using a Kulite stagnation pressure probe. Mean pressure measurements show the growth of the corner flow <span class="hlt">separation</span> and divergence of the ``through flow'' toward the outer casing. Spectra show a sensitivity of the <span class="hlt">separated</span> region to small amplitude external disturbances, in this case originating from the downstream fan. The onset of rotating stall appears as the first subharmonic of the rotor <span class="hlt">frequency</span>, 0.5 fr, then shifts to a slightly lower <span class="hlt">frequency</span> 0.45 fr as the flow coefficient is decreased.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5871668','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5871668"><span>Ploidy <span class="hlt">Variation</span> in Kluyveromyces marxianus <span class="hlt">Separates</span> Dairy and Non-dairy Isolates</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ortiz-Merino, Raúl A.; Varela, Javier A.; Coughlan, Aisling Y.; Hoshida, Hisashi; da Silveira, Wendel B.; Wilde, Caroline; Kuijpers, Niels G. A.; Geertman, Jan-Maarten; Wolfe, Kenneth H.; Morrissey, John P.</p> <p>2018-01-01</p> <p>Kluyveromyces marxianus is traditionally associated with fermented dairy products, but can also be isolated from diverse non-dairy environments. Because of thermotolerance, rapid growth and other traits, many different strains are being developed for food and industrial applications but there is, as yet, little understanding of the genetic diversity or population genetics of this species. K. marxianus shows a high level of phenotypic <span class="hlt">variation</span> but the only phenotype that has been clearly linked to a genetic polymorphism is lactose utilisation, which is controlled by <span class="hlt">variation</span> in the LAC12 gene. The genomes of several strains have been sequenced in recent years and, in this study, we sequenced a further nine strains from different origins. Analysis of the Single Nucleotide Polymorphisms (SNPs) in 14 strains was carried out to examine genome structure and genetic diversity. SNP diversity in K. marxianus is relatively high, with up to 3% DNA sequence divergence between alleles. It was found that the isolates include haploid, diploid, and triploid strains, as shown by both SNP analysis and flow cytometry. Diploids and triploids contain long genomic tracts showing loss of heterozygosity (LOH). All six isolates from dairy environments were diploid or triploid, whereas 6 out 7 isolates from non-dairy environment were haploid. This also correlated with the presence of functional LAC12 alleles only in dairy haplotypes. The diploids were hybrids between a non-dairy and a dairy haplotype, whereas triploids included three copies of a dairy haplotype. PMID:29619042</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvF...3c3901S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvF...3c3901S"><span>Effect of synthetic jet modulation schemes on the reduction of a laminar <span class="hlt">separation</span> bubble</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seo, J. H.; Cadieux, F.; Mittal, R.; Deem, E.; Cattafesta, L.</p> <p>2018-03-01</p> <p>The response of a laminar <span class="hlt">separation</span> bubble to synthetic jet forcing with various modulation schemes is investigated via direct numerical simulations. A simple sinusoidal waveform is considered as a reference case, and various amplitude modulation schemes, including the square-wave "burst" modulation, are employed in the simulations. The results indicate that burst modulation is less effective at reducing the length of the flow <span class="hlt">separation</span> than the sinusoidal forcing primarily because burst modulation is associated with a broad spectrum of input <span class="hlt">frequencies</span> that are higher than the target <span class="hlt">frequency</span> for the flow control. It is found that such high-<span class="hlt">frequency</span> forcing delays vortex roll-up and promotes vortex pairing and merging, which have an adverse effect on reducing the <span class="hlt">separation</span> bubble length. A commonly used amplitude modulation scheme is also found to have reduced effectiveness due to its spectral content. A new amplitude modulation scheme which is tailored to impart more energy at the target <span class="hlt">frequency</span> is proposed and shown to be more effective than the other modulation schemes. Experimental measurements confirm that modulation schemes can be preserved through the actuator and used to enhance the energy content at the target modulation <span class="hlt">frequency</span>. The present study therefore suggests that the effectiveness of synthetic jet-based flow control could be improved by carefully designing the spectral content of the modulation scheme.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/866594','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/866594"><span>Liquid-phase thermal diffusion isotope <span class="hlt">separation</span> apparatus and method having tapered column</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Rutherford, William M.</p> <p>1988-05-24</p> <p>A thermal diffusion counterflow method and apparatus for <span class="hlt">separating</span> isotopes in solution in which the solution is confined in a long, narrow, vertical slit which tapers from bottom to top. The <span class="hlt">variation</span> in the width of the slit permits maintenance of a stable concentration distribution with relatively long columns, thus permitting isotopic <span class="hlt">separation</span> superior to that obtainable in the prior art.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6666538','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6666538"><span>Liquid-phase thermal diffusion isotope <span class="hlt">separation</span> apparatus and method having tapered column</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Rutherford, W.M.</p> <p>1985-12-04</p> <p>A thermal diffusion counterflow method and apparatus for <span class="hlt">separating</span> isotopes in solution in which the solution is confined in a long, narrow, vertical slit which tapers from bottom to top. The <span class="hlt">variation</span> in the width of the slit permits maintenance of a stable concentration distribution with relatively long columns, thus permitting isotopic <span class="hlt">separation</span> superior to that obtained in the prior art.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26674035','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26674035"><span>Seasonally adjusted birth <span class="hlt">frequencies</span> follow the Poisson distribution.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barra, Mathias; Lindstrøm, Jonas C; Adams, Samantha S; Augestad, Liv A</p> <p>2015-12-15</p> <p><span class="hlt">Variations</span> in birth <span class="hlt">frequencies</span> have an impact on activity planning in maternity wards. Previous studies of this phenomenon have commonly included elective births. A Danish study of spontaneous births found that birth <span class="hlt">frequencies</span> were well modelled by a Poisson process. Somewhat unexpectedly, there were also weekly <span class="hlt">variations</span> in the <span class="hlt">frequency</span> of spontaneous births. Another study claimed that birth <span class="hlt">frequencies</span> follow the Benford distribution. Our objective was to test these results. We analysed 50,017 spontaneous births at Akershus University Hospital in the period 1999-2014. To investigate the Poisson distribution of these births, we plotted their variance over a sliding average. We specified various Poisson regression models, with the number of births on a given day as the outcome variable. The explanatory variables included various combinations of years, months, days of the week and the digit sum of the date. The relationship between the variance and the average fits well with an underlying Poisson process. A Benford distribution was disproved by a goodness-of-fit test (p < 0.01). The fundamental model with year and month as explanatory variables is significantly improved (p < 0.001) by adding day of the week as an explanatory variable. Altogether 7.5% more children are born on Tuesdays than on Sundays. The digit sum of the date is non-significant as an explanatory variable (p = 0.23), nor does it increase the explained variance. INERPRETATION: Spontaneous births are well modelled by a time-dependent Poisson process when monthly and day-of-the-week <span class="hlt">variation</span> is included. The <span class="hlt">frequency</span> is highest in summer towards June and July, Friday and Tuesday stand out as particularly busy days, and the activity level is at its lowest during weekends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21612017-time-frequency-approach-stochastic-signal-detection','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21612017-time-frequency-approach-stochastic-signal-detection"><span>Time-<span class="hlt">Frequency</span> Approach for Stochastic Signal Detection</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>Ghosh, Ripul; Akula, Aparna; Kumar, Satish</p> <p>2011-10-20</p> <p>The detection of events in a stochastic signal has been a subject of great interest. One of the oldest signal processing technique, Fourier Transform of a signal contains information regarding <span class="hlt">frequency</span> content, but it cannot resolve the exact onset of changes in the <span class="hlt">frequency</span>, all temporal information is contained in the phase of the transform. On the other hand, Spectrogram is better able to resolve temporal evolution of <span class="hlt">frequency</span> content, but has a trade-off in time resolution versus <span class="hlt">frequency</span> resolution in accordance with the uncertainty principle. Therefore, time-<span class="hlt">frequency</span> representations are considered for energetic characterisation of the non-stationary signals. Wigner Villemore » Distribution (WVD) is the most prominent quadratic time-<span class="hlt">frequency</span> signal representation and used for analysing <span class="hlt">frequency</span> <span class="hlt">variations</span> in signals.WVD allows for instantaneous <span class="hlt">frequency</span> estimation at each data point, for a typical temporal resolution of fractions of a second. This paper through simulations describes the way time <span class="hlt">frequency</span> models are applied for the detection of event in a stochastic signal.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17358752','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17358752"><span>Limit on the temporal <span class="hlt">variation</span> of the fine-structure constant using atomic dysprosium.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cingöz, A; Lapierre, A; Nguyen, A-T; Leefer, N; Budker, D; Lamoreaux, S K; Torgerson, J R</p> <p>2007-01-26</p> <p>Over 8 months, we monitored transition <span class="hlt">frequencies</span> between nearly degenerate, opposite-parity levels in two isotopes of atomic dysprosium (Dy). These <span class="hlt">frequencies</span> are sensitive to <span class="hlt">variation</span> of the fine-structure constant (alpha) due to relativistic corrections of opposite sign for the opposite-parity levels. In this unique system, in contrast to atomic-clock comparisons, the difference of the electronic energies of the opposite-parity levels can be monitored directly utilizing a rf electric-dipole transition between them. Our measurements show that the <span class="hlt">frequency</span> <span class="hlt">variation</span> of the 3.1-MHz transition in (163)Dy and the 235-MHz transition in (162)Dy are 9.0+/-6.7 Hz/yr and -0.6+/-6.5 Hz/yr, respectively. These results provide a rate of fractional <span class="hlt">variation</span> of alpha of (-2.7+/-2.6) x 10(-15) yr(-1) (1 sigma) without assumptions on constancy of other fundamental constants, indicating absence of significant <span class="hlt">variation</span> at the present level of sensitivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26916103','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26916103"><span>Anatomic <span class="hlt">variation</span> and orgasm: Could <span class="hlt">variations</span> in anatomy explain differences in orgasmic success?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Emhardt, E; Siegel, J; Hoffman, L</p> <p>2016-07-01</p> <p>Though the public consciousness is typically focused on factors such as psychology, penis size, and the presence of the "G-spot," there are other anatomical and neuro-anatomic differences that could play an equal, or more important, role in the <span class="hlt">frequency</span> and intensity of orgasms. Discovering these <span class="hlt">variations</span> could direct further medical or procedural management to improve sexual satisfaction. The aim of this study is to review the available literature of anatomical sexual <span class="hlt">variation</span> and to explain why this <span class="hlt">variation</span> may predispose some patients toward a particular sexual experience. In this review, we explored the available literature on sexual anatomy and neuro-anatomy. We used PubMed and OVID Medline for search terms, including orgasm, penile size <span class="hlt">variation</span>, clitoral <span class="hlt">variation</span>, Grafenberg spot, and benefits of orgasm. First we review the basic anatomy and innervation of the reproductive organs. Then we describe several anatomical <span class="hlt">variations</span> that likely play a superior role to popular known <span class="hlt">variation</span> (penis size, presence of g-spot, etc). For males, the delicate play between the parasympathetic and sympathetic nervous systems is vital to achieve orgasm. For females, the autonomic component is more complex. The clitoris is the primary anatomical feature for female orgasm, including its migration toward the anterior vaginal wall. In conclusions, orgasms are complex phenomena involving psychological, physiological, and anatomic <span class="hlt">variation</span>. While these <span class="hlt">variations</span> predispose people to certain sexual function, future research should explore how to surgically or medically alter these. Clin. Anat. 29:665-672, 2016. © 2016 Wiley Periodicals, Inc. © 2016 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5137703','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5137703"><span>Statistics of natural reverberation enable perceptual <span class="hlt">separation</span> of sound and space</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Traer, James; McDermott, Josh H.</p> <p>2016-01-01</p> <p>In everyday listening, sound reaches our ears directly from a source as well as indirectly via reflections known as reverberation. Reverberation profoundly distorts the sound from a source, yet humans can both identify sound sources and distinguish environments from the resulting sound, via mechanisms that remain unclear. The core computational challenge is that the acoustic signatures of the source and environment are combined in a single signal received by the ear. Here we ask whether our recognition of sound sources and spaces reflects an ability to <span class="hlt">separate</span> their effects and whether any such <span class="hlt">separation</span> is enabled by statistical regularities of real-world reverberation. To first determine whether such statistical regularities exist, we measured impulse responses (IRs) of 271 spaces sampled from the distribution encountered by humans during daily life. The sampled spaces were diverse, but their IRs were tightly constrained, exhibiting exponential decay at <span class="hlt">frequency</span>-dependent rates: Mid <span class="hlt">frequencies</span> reverberated longest whereas higher and lower <span class="hlt">frequencies</span> decayed more rapidly, presumably due to absorptive properties of materials and air. To test whether humans leverage these regularities, we manipulated IR decay characteristics in simulated reverberant audio. Listeners could discriminate sound sources and environments from these signals, but their abilities degraded when reverberation characteristics deviated from those of real-world environments. Subjectively, atypical IRs were mistaken for sound sources. The results suggest the brain <span class="hlt">separates</span> sound into contributions from the source and the environment, constrained by a prior on natural reverberation. This <span class="hlt">separation</span> process may contribute to robust recognition while providing information about spaces around us. PMID:27834730</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27834730','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27834730"><span>Statistics of natural reverberation enable perceptual <span class="hlt">separation</span> of sound and space.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Traer, James; McDermott, Josh H</p> <p>2016-11-29</p> <p>In everyday listening, sound reaches our ears directly from a source as well as indirectly via reflections known as reverberation. Reverberation profoundly distorts the sound from a source, yet humans can both identify sound sources and distinguish environments from the resulting sound, via mechanisms that remain unclear. The core computational challenge is that the acoustic signatures of the source and environment are combined in a single signal received by the ear. Here we ask whether our recognition of sound sources and spaces reflects an ability to <span class="hlt">separate</span> their effects and whether any such <span class="hlt">separation</span> is enabled by statistical regularities of real-world reverberation. To first determine whether such statistical regularities exist, we measured impulse responses (IRs) of 271 spaces sampled from the distribution encountered by humans during daily life. The sampled spaces were diverse, but their IRs were tightly constrained, exhibiting exponential decay at <span class="hlt">frequency</span>-dependent rates: Mid <span class="hlt">frequencies</span> reverberated longest whereas higher and lower <span class="hlt">frequencies</span> decayed more rapidly, presumably due to absorptive properties of materials and air. To test whether humans leverage these regularities, we manipulated IR decay characteristics in simulated reverberant audio. Listeners could discriminate sound sources and environments from these signals, but their abilities degraded when reverberation characteristics deviated from those of real-world environments. Subjectively, atypical IRs were mistaken for sound sources. The results suggest the brain <span class="hlt">separates</span> sound into contributions from the source and the environment, constrained by a prior on natural reverberation. This <span class="hlt">separation</span> process may contribute to robust recognition while providing information about spaces around us.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002PhyU...45..719I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002PhyU...45..719I"><span>REVIEWS OF TOPICAL PROBLEMS: Periodic weather and climate <span class="hlt">variations</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivanov, Vladimir V.</p> <p>2002-07-01</p> <p><span class="hlt">Variations</span> in meteorological parameters are largely due to periodic processes and can be forecast for several years. Many such processes are related to astronomical factors such as the gravitational influences of the Moon and the Sun, and the modulation of solar irradiance by lunar and planetary motion. The Moon, Jupiter, and Venus have the strongest effect. These influences produce lines in the spectra of meteorological <span class="hlt">variations</span>, which are combinations of the harmonics of the <span class="hlt">frequencies</span> of revolution of the planets, the Earth, and the Moon around the Sun with the harmonics of the lunar revolution around the Earth. Due to <span class="hlt">frequency</span> differences between the orbital and radial motions, fine spectral features of three types appear: line splitting, line-profile complications due to radial oscillations, and additional lines due to the combination of radial-oscillation <span class="hlt">frequencies</span> with perturbation harmonics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9584088','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9584088"><span>Inherited and environmentally induced differences in mutation <span class="hlt">frequencies</span> between wild strains of Sordaria fimicola from "Evolution Canyon".</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lamb, B C; Saleem, M; Scott, W; Thapa, N; Nevo, E</p> <p>1998-05-01</p> <p>We have studied whether there is natural genetic <span class="hlt">variation</span> for mutation <span class="hlt">frequencies</span>, and whether any such <span class="hlt">variation</span> is environment-related. Mutation <span class="hlt">frequencies</span> differed significantly between wild strains of the fungus Sordaria fimicola isolated from a harsher or a milder microscale environment in "Evolution Canyon," Israel. Strains from the harsher, drier, south-facing slope had higher <span class="hlt">frequencies</span> of new spontaneous mutations and of accumulated mutations than strains from the milder, lusher, north-facing slope. Collective total mutation <span class="hlt">frequencies</span> over many loci for ascospore pigmentation were 2.3, 3.5 and 4.4% for three strains from the south-facing slope, and 0.9, 1.1, 1.2, 1.3 and 1.3% for five strains from the north-facing slope. Some of this between-slope difference was inherited through two generations of selfing, with average spontaneous mutation <span class="hlt">frequencies</span> of 1.9% for south-facing slope strains and 0.8% for north-facing slope strains. The remainder was caused by different <span class="hlt">frequencies</span> of mutations arising in the original environments. There was also significant heritable genetic <span class="hlt">variation</span> in mutation <span class="hlt">frequencies</span> within slopes. Similar between-slope differences were found for ascospore germination-resistance to acriflavine, with much higher <span class="hlt">frequencies</span> in strains from the south-facing slope. Such inherited <span class="hlt">variation</span> provides a basis for natural selection for optimum mutation rates in each environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1460149','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1460149"><span>Inherited and environmentally induced differences in mutation <span class="hlt">frequencies</span> between wild strains of Sordaria fimicola from "Evolution Canyon".</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lamb, B C; Saleem, M; Scott, W; Thapa, N; Nevo, E</p> <p>1998-01-01</p> <p>We have studied whether there is natural genetic <span class="hlt">variation</span> for mutation <span class="hlt">frequencies</span>, and whether any such <span class="hlt">variation</span> is environment-related. Mutation <span class="hlt">frequencies</span> differed significantly between wild strains of the fungus Sordaria fimicola isolated from a harsher or a milder microscale environment in "Evolution Canyon," Israel. Strains from the harsher, drier, south-facing slope had higher <span class="hlt">frequencies</span> of new spontaneous mutations and of accumulated mutations than strains from the milder, lusher, north-facing slope. Collective total mutation <span class="hlt">frequencies</span> over many loci for ascospore pigmentation were 2.3, 3.5 and 4.4% for three strains from the south-facing slope, and 0.9, 1.1, 1.2, 1.3 and 1.3% for five strains from the north-facing slope. Some of this between-slope difference was inherited through two generations of selfing, with average spontaneous mutation <span class="hlt">frequencies</span> of 1.9% for south-facing slope strains and 0.8% for north-facing slope strains. The remainder was caused by different <span class="hlt">frequencies</span> of mutations arising in the original environments. There was also significant heritable genetic <span class="hlt">variation</span> in mutation <span class="hlt">frequencies</span> within slopes. Similar between-slope differences were found for ascospore germination-resistance to acriflavine, with much higher <span class="hlt">frequencies</span> in strains from the south-facing slope. Such inherited <span class="hlt">variation</span> provides a basis for natural selection for optimum mutation rates in each environment. PMID:9584088</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22395493-accurate-formula-dissipative-interaction-frequency-modulation-atomic-force-microscopy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22395493-accurate-formula-dissipative-interaction-frequency-modulation-atomic-force-microscopy"><span>Accurate formula for dissipative interaction in <span class="hlt">frequency</span> modulation atomic force microscopy</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>Suzuki, Kazuhiro; Matsushige, Kazumi; Yamada, Hirofumi</p> <p>2014-12-08</p> <p>Much interest has recently focused on the viscosity of nano-confined liquids. <span class="hlt">Frequency</span> modulation atomic force microscopy (FM-AFM) is a powerful technique that can detect <span class="hlt">variations</span> in the conservative and dissipative forces between a nanometer-scale tip and a sample surface. We now present an accurate formula to convert the dissipation power of the cantilever measured during the experiment to damping of the tip-sample system. We demonstrated the conversion of the dissipation power versus tip-sample <span class="hlt">separation</span> curve measured using a colloidal probe cantilever on a mica surface in water to the damping curve, which showed a good agreement with the theoretical curve.more » Moreover, we obtained the damping curve from the dissipation power curve measured on the hydration layers on the mica surface using a nanometer-scale tip, demonstrating that the formula allows us to quantitatively measure the viscosity of a nano-confined liquid using FM-AFM.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=separation+AND+parents&pg=5&id=EJ748474','ERIC'); return false;" href="https://eric.ed.gov/?q=separation+AND+parents&pg=5&id=EJ748474"><span>Factors Moderating Children's Adjustment to Parental <span class="hlt">Separation</span>: Findings from a Community Study in England</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>Cheng, Helen; Dunn, Judy; O'Connor, Thomas G.; Golding, Jean</p> <p>2006-01-01</p> <p>Research findings show that there is marked variability in children's response to parental <span class="hlt">separation</span>, but few studies identify the sources of this <span class="hlt">variation</span>. This prospective longitudinal study examines the factors modifying children's adjustment to parental <span class="hlt">separation</span> in a community sample of 5,635 families in England. Children's…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033277','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033277"><span>Application of high-resolution linear Radon transform for Rayleigh-wave dispersive energy imaging and mode <span class="hlt">separating</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>Luo, Y.; Xia, J.; Miller, R.D.; Liu, J.; Xu, Y.; Liu, Q.</p> <p>2008-01-01</p> <p>Multichannel Analysis of Surface Waves (MASW) analysis is an efficient tool to obtain the vertical shear-wave profile. One of the key steps in the MASW method is to generate an image of dispersive energy in the <span class="hlt">frequency</span>-velocity domain, so dispersion curves can be determined by picking peaks of dispersion energy. In this paper, we image Rayleigh-wave dispersive energy and <span class="hlt">separate</span> multimodes from a multichannel record by high-resolution linear Radon transform (LRT). We first introduce Rayleigh-wave dispersive energy imaging by high-resolution LRT. We then show the process of Rayleigh-wave mode <span class="hlt">separation</span>. Results of synthetic and real-world examples demonstrate that (1) compared with slant stacking algorithm, high-resolution LRT can improve the resolution of images of dispersion energy by more than 50% (2) high-resolution LRT can successfully <span class="hlt">separate</span> multimode dispersive energy of Rayleigh waves with high resolution; and (3) multimode <span class="hlt">separation</span> and reconstruction expand <span class="hlt">frequency</span> ranges of higher mode dispersive energy, which not only increases the investigation depth but also provides a means to accurately determine cut-off <span class="hlt">frequencies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27992653','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27992653"><span><span class="hlt">Frequency</span> Distribution in Domestic Microwave Ovens and Its Influence on Heating Pattern.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Luan, Donglei; Wang, Yifen; Tang, Juming; Jain, Deepali</p> <p>2017-02-01</p> <p>In this study, snapshots of operating <span class="hlt">frequency</span> profiles of domestic microwave ovens were collected to reveal the extent of microwave <span class="hlt">frequency</span> <span class="hlt">variations</span> under different operation conditions. A computer simulation model was developed based on the finite difference time domain method to analyze the influence of the shifting <span class="hlt">frequency</span> on heating patterns of foods in a microwave oven. The results showed that the operating <span class="hlt">frequencies</span> of empty and loaded domestic microwave ovens varied widely even among ovens of the same model purchased on the same date. Each microwave oven had its unique characteristic operating <span class="hlt">frequencies</span>, which were also affected by the location and shape of the load. The simulated heating patterns of a gellan gel model food when heated on a rotary plate agreed well with the experimental results, which supported the reliability of the developed simulation model. Simulation indicated that the heating patterns of a stationary model food load changed with the varying operating <span class="hlt">frequency</span>. However, the heating pattern of a rotary model food load was not sensitive to microwave <span class="hlt">frequencies</span> due to the severe edge heating overshadowing the effects of the <span class="hlt">frequency</span> <span class="hlt">variations</span>. © 2016 Institute of Food Technologists®.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..249a2013H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..249a2013H"><span>Measurement of corner <span class="hlt">separation</span> zone response on a compression ramp to plasma actuation within the hypersonic boundary layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hedlund, Brock E.; Houpt, Alec W.; Gordeyev, Stanislav V.; Leonov, Sergey B.</p> <p>2017-10-01</p> <p>This study was performed to characterize the dominant <span class="hlt">frequencies</span> present in the boundary layer uptsream of and in the corner <span class="hlt">separation</span> zone of a compression surface in Mach 4.5 flow and to determine a control effect of transient plasma actuation on the boundary layer. Schlieren imaging was used to distinguish the corner <span class="hlt">separation</span> zone for 20°, 25°, and 30° compression ramps mounted on flat plates. Spectra of the natural disturbances present in the boundary layer and <span class="hlt">separation</span> zone were gathered using a high-speed Shack-Hartmann wavefront sensor and surface mounted PCBTM pressure sensors while varying flow parameters by adjusting total pressure, temperature, and ramp angle. Shallow cavity discharge plasma actuators were used as a high-<span class="hlt">frequency</span> localized thermal forcing mechanism of the boundary layer. The plasma effect was negligible for forcing <span class="hlt">frequencies</span> (50 kHz) below the natural dominant <span class="hlt">frequency</span> (~55-80 kHz). High <span class="hlt">frequency</span> perturbations that can promote the transition to turbulence were amplified when the plasma forcing <span class="hlt">frequency</span> (100 kHz) was higher than the natural dominant <span class="hlt">frequency</span> (~55-80 kHz). This technique can potentially be used for active control of hypersonic boundary layer transition and the supersonic flow structure on the compression surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.S43D1914S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.S43D1914S"><span>Seismic noise level <span class="hlt">variation</span> in South Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sheen, D.; Shin, J.</p> <p>2008-12-01</p> <p>The <span class="hlt">variations</span> of seismic background noise in South Korea have been investigated by means of power spectral analysis. The Korea Institute of Geoscience and Mineral Resources (KIGAM) and the Korea Meteorological Administation (KMA) have national wide seismic networks in South Korea, and, in the end of 2007, there are 30 broadband stations which have been operating for more than a year. In this study, we have estimated the power spectral density of seismic noise for 30 broadband stations from 2005 to 2007. Since we estimate PSDs from a large dataset of continuous waveform in this study, a robust PSD estimate of McNamara and Buland (2004) is used. In the <span class="hlt">frequency</span> range 1-5 Hz, the diurnal <span class="hlt">variations</span> of noise are observed at most of stations, which are especially larger at coastal stations and at insular than at inland. Some stations shows daily difference of diurnal <span class="hlt">variations</span>, which represents that cultural activities contribute to the noise level of a station. The <span class="hlt">variation</span> of number of triggered stations, however, shows that cultural noise has little influence on the detection capability of seismic network in South Korea. Seasonal <span class="hlt">variations</span> are observed well in the range 0.1-0.5 Hz, while much less found in the <span class="hlt">frequency</span> range 1-5 Hz. We observed that strong peaks in the range 0.1-0.5 Hz occur at the summer when Pacific typhoons are close to the Korean Peninsula.</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 scale. 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 <span class="hlt">variations</span> 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 <span class="hlt">variations</span> and predictability on decadal time scales 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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3094178','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3094178"><span><span class="hlt">Separability</span> of stimulus parameter encoding by on-off directionally selective rabbit retinal ganglion cells</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Nowak, Przemyslaw; Dobbins, Allan C.; Gawne, Timothy J.; Grzywacz, Norberto M.</p> <p>2011-01-01</p> <p>The ganglion cell output of the retina constitutes a bottleneck in sensory processing in that ganglion cells must encode multiple stimulus parameters in their responses. Here we investigate encoding strategies of On-Off directionally selective retinal ganglion cells (On-Off DS RGCs) in rabbits, a class of cells dedicated to representing motion. The exquisite axial discrimination of these cells to preferred vs. null direction motion is well documented: it is invariant with respect to speed, contrast, spatial configuration, spatial <span class="hlt">frequency</span>, and motion extent. However, these cells have broad direction tuning curves and their responses also vary as a function of other parameters such as speed and contrast. In this study, we examined whether the <span class="hlt">variation</span> in responses across multiple stimulus parameters is systematic, that is the same for all cells, and <span class="hlt">separable</span>, such that the response to a stimulus is a product of the effects of each stimulus parameter alone. We extracellularly recorded single On-Off DS RGCs in a superfused eyecup preparation while stimulating them with moving bars. We found that spike count responses of these cells scaled as independent functions of direction, speed, and luminance. Moreover, the speed and luminance functions were common across the whole sample of cells. Based on these findings, we developed a model that accurately predicted responses of On-Off DS RGCs as products of <span class="hlt">separable</span> functions of direction, speed, and luminance (r = 0.98; P < 0.0001). Such a multiplicatively <span class="hlt">separable</span> encoding strategy may simplify the decoding of these cells' outputs by the higher visual centers. PMID:21325684</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22351595-evidence-resonant-mode-coupling-relationship-between-low-high-frequencies-rapidly-rotating-star','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22351595-evidence-resonant-mode-coupling-relationship-between-low-high-frequencies-rapidly-rotating-star"><span>Evidence of resonant mode coupling and the relationship between low and high <span class="hlt">frequencies</span> in a rapidly rotating a star</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>Breger, M.; Montgomery, M. H.</p> <p></p> <p>In the theory of resonant mode coupling, the parent and child modes are directly related in <span class="hlt">frequency</span> and phase. The oscillations present in the fast rotating δ Sct star KIC 8054146 allow us to test the most general and generic aspects of such a theory. The only direct way to <span class="hlt">separate</span> the parent and coupled (child) modes is to examine the correlations in amplitude variability between the different <span class="hlt">frequencies</span>. For the dominant family of related <span class="hlt">frequencies</span>, only a single mode and a triplet are the origins of nine dominant <span class="hlt">frequency</span> peaks ranging from 2.93 to 66.30 cycles day{sup –1} (asmore » well as dozens of small-amplitude combination modes and a predicted and detected third high-<span class="hlt">frequency</span> triplet). The mode-coupling model correctly predicts the large amplitude <span class="hlt">variations</span> of the coupled modes as a product of the amplitudes of the parent modes, while the phase changes are also correctly modeled. This differs from the behavior of 'normal' combination <span class="hlt">frequencies</span> in that the amplitudes are three orders of magnitude larger and may exceed even the amplitudes of the parent modes. We show that two dominant low <span class="hlt">frequencies</span> at 5.86 and 2.93 cycles day{sup –1} in the gravity-mode region are not harmonics of each other, and their properties follow those of the almost equidistant high-<span class="hlt">frequency</span> triplet. We note that the previously puzzling situation of finding two strong peaks in the low-<span class="hlt">frequency</span> region related by nearly a factor of two in <span class="hlt">frequency</span> has been seen in other δ Sct stars as well.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5820S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5820S"><span>High <span class="hlt">frequency</span> noise studies at the Hartousov mofette area (CZE)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Andreas; Flores-Estrella, Hortencia; Pommerencke, Julia; Umlauft, Josefine</p> <p>2014-05-01</p> <p>Ambient noise analysis has been used as a reliable tool to investigate sub-surface structures at seismological quiet regions with none or less specific seismic events. Here, we consider the acoustic signals from a single mofette at the Hartoušov area (CZE) as a noise-like high <span class="hlt">frequency</span> source caused by multiple near surface degassing processes in a restricted location. From this assumption we have used different array geometries for recording at least one hour of continuous noise. We installed triangular arrays with 3 component geophones: the first deployment consisted on two co-centric triangles with side length of 30 and 50 m with the mofette in the center; the second deployment consisted on two triangular arrays, both with side length of 30 m, co-directional to the mofette. Furthermore, we also installed profiles with 24 channels and vertical geophones locating them in different positions with respect to the mofette. In this work, we present preliminary results from the data analysis dependent on the geometry, to show the characteristics of the noise wave-field referring to <span class="hlt">frequency</span> content and propagation features, such as directionality and surface wave velocity. The spectral analysis shows that the energy is concentrated in a <span class="hlt">frequency</span> band among 10 and 40 Hz. However, in this interval there is no evidence of any exclusive fundamental <span class="hlt">frequencies</span>. From this, man-induced influences can be identified as intermittent signal peaks in narrow <span class="hlt">frequency</span> bands and can be <span class="hlt">separated</span> to receive the revised mofette wave-field record. The inversion of dispersive surface waves, that were detected by interferometric methods, provides a velocity model down to 12 m with an S-wave velocity between 160 and 180 m/s on the uppermost layer. Furthermore, the interferometric signal properties indicate that it is not possible to characterize the mofette as a punctual source, but rather as a conglomerate of multiple sources with time and location <span class="hlt">variations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017A%26A...601A.130R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017A%26A...601A.130R"><span><span class="hlt">Frequency</span> regularities of acoustic modes and multi-colour mode identification in rapidly rotating stars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reese, D. R.; Lignières, F.; Ballot, J.; Dupret, M.-A.; Barban, C.; van't Veer-Menneret, C.; MacGregor, K. B.</p> <p>2017-05-01</p> <p>Context. Mode identification has remained a major obstacle in the interpretation of pulsation spectra in rapidly rotating stars. This has motivated recent work on calculating realistic multi-colour mode visibilities in this type of star. Aims: We would like to test mode identification methods and seismic diagnostics in rapidly rotating stars, using oscillation spectra that are based on these new theoretical predictions. Methods: We investigate the auto-correlation function and Fourier transform of theoretically calculated <span class="hlt">frequency</span> spectra, in which modes are selected according to their visibilities. Given that intrinsic mode amplitudes are determined by non-linear saturation and cannot currently be theoretically predicted, we experimented with various ad-hoc prescriptions for setting the mode amplitudes, including using random values. Furthermore, we analyse the ratios between mode amplitudes observed in different photometric bands to see up to what extent they can identify modes. Results: When non-random intrinsic mode amplitudes are used, our results show that it is possible to extract a mean value for the large <span class="hlt">frequency</span> <span class="hlt">separation</span> or half its value and, sometimes, twice the rotation rate, from the auto-correlation of the <span class="hlt">frequency</span> spectra. Furthermore, the Fourier transforms are mostly sensitive to the large <span class="hlt">frequency</span> <span class="hlt">separation</span> or half its value. The combination of the two methods may therefore measure and distinguish the two types of <span class="hlt">separations</span>. When the intrinsic mode amplitudes include random factors, which seems more representative of real stars, the results are far less favourable. It is only when the large <span class="hlt">separation</span> or half its value coincides with twice the rotation rate, that it might be possible to detect the signature of a <span class="hlt">frequency</span> regularity. We also find that amplitude ratios are a good way of grouping together modes with similar characteristics. By analysing the <span class="hlt">frequencies</span> of these groups, it is possible to constrain mode identification, as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15764212','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15764212"><span>Effect on LTAS of vocal loudness <span class="hlt">variation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nordenberg, Maria; Sundberg, Johan</p> <p>2004-01-01</p> <p>Long-term-average spectrum (LTAS) is an efficient method for voice analysis, revealing both voice source and formant characteristics. However, the LTAS contour is non-uniformly affected by vocal loudness. This <span class="hlt">variation</span> was analyzed in 15 male and 16 female untrained voices reading a text 7 times at different degrees of vocal loudness, mean change in overall equivalent sound level (Leq) amounting to 27.9 dB and 28.4 dB for the female and male subjects. For all <span class="hlt">frequency</span> values up to 4 kHz, spectrum level was strongly and linearly correlated with Leq for each subject. The gain factor, that is to say, the rate of level increase, varied with <span class="hlt">frequency</span>, from about 0.5 at low <span class="hlt">frequencies</span> to about 1.5 in the <span class="hlt">frequency</span> range 1.5-3 kHz. Using the gain factors for a subject, LTAS contours could be predicted at any Leq within the measured range, with an average accuracy of 2-3 dB below 4 kHz. Mean LTAS calculated for an Leq of 70 dB for each subject showed considerable individual <span class="hlt">variation</span> for both males and females, SD of the level varying between 7 dB and 4 dB depending on <span class="hlt">frequency</span>. On the other hand, the results also suggest that meaningful comparisons of LTAS, recorded for example before and after voice therapy, can be made, provided that the documentation includes a set of recordings at different loudness levels from one recording session.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JSV...210..461Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JSV...210..461Y"><span>STICK-SLIP-<span class="hlt">SEPARATION</span> Analysis and Non-Linear Stiffness and Damping Characterization of Friction Contacts Having Variable Normal Load</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, B. D.; Chu, M. L.; Menq, C. H.</p> <p>1998-03-01</p> <p>Mechanical systems in which moving components are mutually constrained through contacts often lead to complex contact kinematics involving tangential and normal relative motions. A friction contact model is proposed to characterize this type of contact kinematics that imposes both friction non-linearity and intermittent <span class="hlt">separation</span> non-linearity on the system. The stick-slip friction phenomenon is analyzed by establishing analytical criteria that predict the transition between stick, slip, and <span class="hlt">separation</span> of the interface. The established analytical transition criteria are particularly important to the proposed friction contact model for the transition conditions of the contact kinematics are complicated by the effect of normal load <span class="hlt">variation</span> and possible interface <span class="hlt">separation</span>. With these transition criteria, the induced friction force on the contact plane and the variable normal load perpendicular to the contact plane, can be predicted for any given cyclic relative motions at the contact interface and hysteresis loops can be produced so as to characterize the equivalent damping and stiffness of the friction contact. These-non-linear damping and stiffness methods along with the harmonic balance method are then used to predict the resonant response of a frictionally constrained two-degree-of-freedom oscillator. The predicted results are compared with those of the time integration method and the damping effect, the resonant <span class="hlt">frequency</span> shift, and the jump phenomenon are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1201825','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1201825"><span><span class="hlt">Frequencies</span> of Null Alleles at Enzyme Loci in Natural Populations of Ponderosa and Red Pine</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Allendorf, Fred W.; Knudsen, Kathy L.; Blake, George M.</p> <p>1982-01-01</p> <p>Pinus ponderosa and P. resinosa population samples have mean <span class="hlt">frequencies</span> of enzymatically inactive alleles of 0.0031 and 0.0028 at 29 and 27 enzyme loci, respectively. Such alleles are rare and are apparently maintained by selection-mutation balance. Ponderosa pine have much higher amounts of allozymic and polygenic phenotypic <span class="hlt">variation</span> than red pine, yet both species have similar <span class="hlt">frequencies</span> of null alleles. Thus, null alleles apparently do not contribute to polygenic <span class="hlt">variation</span>, as has been suggested. The concordance between allozymic and polygenic <span class="hlt">variation</span> adds support to the view that allozyme studies may be valuable in predicting the relative amount of polygenic <span class="hlt">variation</span> in populations. PMID:17246067</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26547390','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26547390"><span>Areas V1 and V2 show microsaccade-related 3-4-Hz covariation in gamma power and <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>Lowet, E; Roberts, M J; Bosman, C A; Fries, P; De Weerd, P</p> <p>2016-05-01</p> <p>Neuronal gamma-band synchronization (25-80 Hz) in visual cortex appears sustained and stable during prolonged visual stimulation when investigated with conventional averages across trials. However, recent studies in macaque visual cortex have used single-trial analyses to show that both power and <span class="hlt">frequency</span> of gamma oscillations exhibit substantial moment-by-moment <span class="hlt">variation</span>. This has raised the question of whether these apparently random <span class="hlt">variations</span> might limit the functional role of gamma-band synchronization for neural processing. Here, we studied the moment-by-moment <span class="hlt">variation</span> in gamma oscillation power and <span class="hlt">frequency</span>, as well as inter-areal gamma synchronization, by simultaneously recording local field potentials in V1 and V2 of two macaque monkeys. We additionally analyzed electrocorticographic V1 data from a third monkey. Our analyses confirm that gamma-band synchronization is not stationary and sustained but undergoes moment-by-moment <span class="hlt">variations</span> in power and <span class="hlt">frequency</span>. However, those <span class="hlt">variations</span> are neither random and nor a possible obstacle to neural communication. Instead, the gamma power and <span class="hlt">frequency</span> <span class="hlt">variations</span> are highly structured, shared between areas and shaped by a microsaccade-related 3-4-Hz theta rhythm. Our findings provide experimental support for the suggestion that cross-<span class="hlt">frequency</span> coupling might structure and facilitate the information flow between brain regions. © 2015 Federation of European Neuroscience Societies and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27328784','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27328784"><span>An overview of maternal <span class="hlt">separation</span> effects on behavioural outcomes in mice: Evidence from a four-stage methodological systematic review.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tractenberg, Saulo G; Levandowski, Mateus L; de Azeredo, Lucas Araújo; Orso, Rodrigo; Roithmann, Laura G; Hoffmann, Emerson S; Brenhouse, Heather; Grassi-Oliveira, Rodrigo</p> <p>2016-09-01</p> <p>Early life stress (ELS) developmental effects have been widely studied by preclinical researchers. Despite the growing body of evidence from ELS models, such as the maternal <span class="hlt">separation</span> paradigm, the reported results have marked inconsistencies. The maternal <span class="hlt">separation</span> model has several methodological pitfalls that could influence the reliability of its results. Here, we critically review 94 mice studies that addressed the effects of maternal <span class="hlt">separation</span> on behavioural outcomes. We also discuss methodological issues related to the heterogeneity of <span class="hlt">separation</span> protocols and the quality of reporting methods. Our findings indicate a lack of consistency in maternal <span class="hlt">separation</span> effects: major studies of behavioural and biological phenotypes failed to find significant deleterious effects. Furthermore, we identified several specific <span class="hlt">variations</span> in <span class="hlt">separation</span> methodological procedures. These methodological <span class="hlt">variations</span> could contribute to the inconsistency of maternal <span class="hlt">separation</span> effects by producing different degrees of stress exposure in maternal <span class="hlt">separation</span>-reared pups. These methodological problems, together with insufficient reporting, might lead to inaccurate and unreliable effect estimates in maternal <span class="hlt">separation</span> studies. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910057123&hterms=Waterfall+model&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DWaterfall%2Bmodel','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910057123&hterms=Waterfall+model&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DWaterfall%2Bmodel"><span>Space Shuttle Redesigned Solid Rocket Motor nozzle natural <span class="hlt">frequency</span> <span class="hlt">variations</span> with burn time</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lui, C. Y.; Mason, D. R.</p> <p>1991-01-01</p> <p>The effects of erosion and thermal degradation on the Space Shuttle Redesigned Solid Rocket Motor (RSRM) nozzle's structural dynamic characteristics were analytically evaluated. Also considered was stiffening of the structure due to internal pressurization. A detailed NASTRAN finite element model of the nozzle was developed and used to evaluate the influence of these effects at several discrete times during motor burn. Methods were developed for treating erosion and thermal degradation, and a procedure was developed to account for internal pressure stiffening using differential stiffness matrix techniques. Results were verified using static firing test accelerometer data. Fast Fourier Transform and Maximum Entropy Method techniques were applied to the data to generate waterfall plots which track modal <span class="hlt">frequencies</span> with burn time. Results indicate that the lower <span class="hlt">frequency</span> nozzle 'vectoring' modes are only slightly affected by erosion, thermal effects and internal pressurization. The higher <span class="hlt">frequency</span> shell modes of the nozzle are, however, significantly reduced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080007426','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080007426"><span>Active noise control using noise source having adaptive resonant <span class="hlt">frequency</span> tuning through stress <span class="hlt">variation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pla, Frederic G. (Inventor); Renshaw, Anthony A. (Inventor); Rajiyah, Harindra (Inventor); Hedeen, Robert A. (Inventor)</p> <p>1995-01-01</p> <p>A noise source for an aircraft engine active noise cancellation system in which the resonant <span class="hlt">frequency</span> of a noise radiating element is tuned to permit noise cancellation over a wide range of <span class="hlt">frequencies</span>. The resonant <span class="hlt">frequency</span> of the noise radiating element is tuned by an expandable ring embedded in the noise radiating element. Excitation of the ring causes expansion or contraction of the ring, thereby varying the stress in the noise radiating element. The ring is actuated by a controller which receives input of a feedback signal proportional to displacement of the noise radiating element and a signal corresponding to the blade passage <span class="hlt">frequency</span> of the engine's fan. In response, the controller determines a control signal which is sent to the ring, causing the ring to expand or contract. Instead of a single ring embedded in the noise radiating panel, a first expandable ring can be bonded to one side of the noise radiating element, and a second expandable ring can be bonded to the other side.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110013126','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110013126"><span>System and method for tuning adjusting the central <span class="hlt">frequency</span> of a laser while maintaining <span class="hlt">frequency</span> stabilization to an external reference</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Livas, Jeffrey (Inventor); Thorpe, James I. (Inventor); Numata, Kenji (Inventor)</p> <p>2011-01-01</p> <p>A method and system for stabilizing a laser to a <span class="hlt">frequency</span> reference with an adjustable offset. The method locks a sideband signal generated by passing an incoming laser beam through the phase modulator to a <span class="hlt">frequency</span> reference, and adjusts a carrier <span class="hlt">frequency</span> relative to the locked sideband signal by changing a phase modulation <span class="hlt">frequency</span> input to the phase modulator. The sideband signal can be a single sideband (SSB), dual sideband (DSB), or an electronic sideband (ESB) signal. Two <span class="hlt">separate</span> electro-optic modulators can produce the DSB signal. The two electro-optic modulators can be a broadband modulator and a resonant modulator. With a DSB signal, the method can introduce two sinusoidal phase modulations at the phase modulator. With ESB signals, the method can further drive the optical phase modulator with an electrical signal with nominal <span class="hlt">frequency</span> OMEGA(sub 1) that is phase modulated at a <span class="hlt">frequency</span> OMEGA(sub 2)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25d3501I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25d3501I"><span>Multipactor susceptibility on a dielectric with two carrier <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>Iqbal, Asif; Verboncoeur, John; Zhang, Peng</p> <p>2018-04-01</p> <p>This work investigates multipactor discharge on a single dielectric surface with two carrier <span class="hlt">frequencies</span> of an rf electric field. We use Monte Carlo simulations and analytical calculations to obtain susceptibility diagrams in terms of the rf electric field and normal electric field due to the residual charge on the dielectric. It is found that in contrast to the single <span class="hlt">frequency</span> case, in general, the presence of a second carrier <span class="hlt">frequency</span> of the rf electric field increases the threshold of the magnitude of the rf electric field to initiate multipactor. The effects of the relative strength and phase, and the <span class="hlt">frequency</span> <span class="hlt">separation</span> of the two carrier <span class="hlt">frequencies</span> are examined. The conditions to minimize mulitpactor are derived.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ISPAr41B1..395W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ISPAr41B1..395W"><span>Low <span class="hlt">Frequency</span> Error Analysis and Calibration for High-Resolution Optical Satellite's Uncontrolled Geometric Positioning</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Mi; Fang, Chengcheng; Yang, Bo; Cheng, Yufeng</p> <p>2016-06-01</p> <p>The low <span class="hlt">frequency</span> error is a key factor which has affected uncontrolled geometry processing accuracy of the high-resolution optical image. To guarantee the geometric quality of imagery, this paper presents an on-orbit calibration method for the low <span class="hlt">frequency</span> error based on geometric calibration field. Firstly, we introduce the overall flow of low <span class="hlt">frequency</span> error on-orbit analysis and calibration, which includes optical axis angle <span class="hlt">variation</span> detection of star sensor, relative calibration among star sensors, multi-star sensor information fusion, low <span class="hlt">frequency</span> error model construction and verification. Secondly, we use optical axis angle change detection method to analyze the law of low <span class="hlt">frequency</span> error <span class="hlt">variation</span>. Thirdly, we respectively use the method of relative calibration and information fusion among star sensors to realize the datum unity and high precision attitude output. Finally, we realize the low <span class="hlt">frequency</span> error model construction and optimal estimation of model parameters based on DEM/DOM of geometric calibration field. To evaluate the performance of the proposed calibration method, a certain type satellite's real data is used. Test results demonstrate that the calibration model in this paper can well describe the law of the low <span class="hlt">frequency</span> error <span class="hlt">variation</span>. The uncontrolled geometric positioning accuracy of the high-resolution optical image in the WGS-84 Coordinate Systems is obviously improved after the step-wise calibration.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2141928','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2141928"><span>CRITICAL ILLUMINATION AND FLICKER <span class="hlt">FREQUENCY</span> IN RELATED FISHES</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Crozier, W. J.; Wolf, E.; Zerrahn-Wolf, Gertrud</p> <p>1937-01-01</p> <p>Flicker response curves have been obtained at 21.5°C. for three genera of fresh water teleosts: Enneacanthus (sunfish), Xiphophorus (swordtail), Platypoecilius (Platy), by the determination of mean critical intensities for response at fixed flicker <span class="hlt">frequencies</span>, and for a certain homogeneous group of backcross hybrids of swordtail x Platy (Black Helleri). The curves exhibit marked differences in form and proportions. The same type of analysis is applicable to each, however. A low intensity rod-governed section has added to it a more extensive cone portion. Each part is accurately described by the equation F = Fmax./(1 + e -p log-p logI/Ii), where F = flicker <span class="hlt">frequency</span>, I = associated mean critical intensity, and Ii is the intensity at the inflection point of the sigmoid curve relating F to log I. There is no correlation between quantitative features of the rod and cone portions. Threshold intensities, p, Ii, and Fmax. are <span class="hlt">separately</span> and independently determined. The hybrid Black Helleri show quantitative agreement with the Xiphophorus parental stock in the values of p for rods and cones, and in the cone Fmax.; the rod Fmax. is very similar to that for the Platy stock; the general level of effective intensities is rather like that of the Platy form. This provides, among other things, a new kind of support for the duplicity doctrine. Various races of Platypoecilius maculatus, and P. variatus, give closely agreeing values of Im at different flicker <span class="hlt">frequencies</span>; and two species of sunfish also agree. The effect of cross-breeding is thus not a superficial thing. It indicates the possibility of further genetic investigation. The variability of the critical intensity for response to flicker follows the rules previously found to hold for other forms. The <span class="hlt">variation</span> is the expression of a property of the tested organism. It is shown that, on the assumption of a <span class="hlt">frequency</span> distribution of receptor element thresholds as a function of log I, with fluctuation in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27894294','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27894294"><span>Appropriate threshold levels of cardiac beat-to-beat <span class="hlt">variation</span> in semi-automatic analysis of equine ECG recordings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Flethøj, Mette; Kanters, Jørgen K; Pedersen, Philip J; Haugaard, Maria M; Carstensen, Helena; Olsen, Lisbeth H; Buhl, Rikke</p> <p>2016-11-28</p> <p>Although premature beats are a matter of concern in horses, the interpretation of equine ECG recordings is complicated by a lack of standardized analysis criteria and a limited knowledge of the normal beat-to-beat <span class="hlt">variation</span> of equine cardiac rhythm. The purpose of this study was to determine the appropriate threshold levels of maximum acceptable deviation of RR intervals in equine ECG analysis, and to evaluate a novel two-step timing algorithm by quantifying the <span class="hlt">frequency</span> of arrhythmias in a cohort of healthy adult endurance horses. Beat-to-beat <span class="hlt">variation</span> differed considerably with heart rate (HR), and an adaptable model consisting of three different HR ranges with <span class="hlt">separate</span> threshold levels of maximum acceptable RR deviation was consequently defined. For resting HRs <60 beats/min (bpm) the threshold level of RR deviation was set at 20%, for HRs in the intermediate range between 60 and 100 bpm the threshold was 10%, and for exercising HRs >100 bpm, the threshold level was 4%. Supraventricular premature beats represented the most prevalent arrhythmia category with varying <span class="hlt">frequencies</span> in seven horses at rest (median 7, range 2-86) and six horses during exercise (median 2, range 1-24). Beat-to-beat <span class="hlt">variation</span> of equine cardiac rhythm varies according to HR, and threshold levels in equine ECG analysis should be adjusted accordingly. Standardization of the analysis criteria will enable comparisons of studies and follow-up examinations of patients. A small number of supraventricular premature beats appears to be a normal finding in endurance horses. Further studies are required to validate the findings and determine the clinical significance of premature beats in horses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RaSc...52.1534H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RaSc...52.1534H"><span>A Robust Automatic Ionospheric O/X Mode <span class="hlt">Separation</span> Technique for Vertical Incidence Sounders</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harris, T. J.; Pederick, L. H.</p> <p>2017-12-01</p> <p>The sounding of the ionosphere by a vertical incidence sounder (VIS) is the oldest and most common technique for determining the state of the ionosphere. The automatic extraction of relevant ionospheric parameters from the ionogram image, referred to as scaling, is important for the effective utilization of data from large ionospheric sounder networks. Due to the Earth's magnetic field, the ionosphere is birefringent at radio <span class="hlt">frequencies</span>, so a VIS will typically see two distinct returns for each <span class="hlt">frequency</span>. For the automatic scaling of ionograms, it is highly desirable to be able to <span class="hlt">separate</span> the two modes. Defence Science and Technology Group has developed a new VIS solution which is based on direct digital receiver technology and includes an algorithm to <span class="hlt">separate</span> the O and X modes. This algorithm can provide high-quality <span class="hlt">separation</span> even in difficult ionospheric conditions. In this paper we describe the algorithm and demonstrate its consistency and reliability in successfully <span class="hlt">separating</span> 99.4% of the ionograms during a 27 day experimental campaign under sometimes demanding ionospheric conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDKP1123K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDKP1123K"><span>Microparticle <span class="hlt">Separation</span> by Cyclonic <span class="hlt">Separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karback, Keegan; Leith, Alexander</p> <p>2017-11-01</p> <p>The ability to <span class="hlt">separate</span> particles based on their size has wide ranging applications from the industrial to the medical. Currently, cyclonic <span class="hlt">separators</span> are primarily used in agriculture and manufacturing to syphon out contaminates or products from an air supply. This has led us to believe that cyclonic <span class="hlt">separation</span> has more applications than the agricultural and industrial. Using the OpenFoam computational package, we were able to determine the flow parameters of a vortex in a cyclonic <span class="hlt">separator</span> in order to segregate dust particles to a cutoff size of tens of nanometers. To test the model, we constructed an experiment to <span class="hlt">separate</span> a test dust of various sized particles. We filled a chamber with Arizona test dust and utilized an acoustic suspension technique to segregate particles finer than a coarse cutoff size and introduce them into the cyclonic <span class="hlt">separation</span> apparatus where they were further <span class="hlt">separated</span> via a vortex following our computational model. The size of the particles <span class="hlt">separated</span> from this experiment will be used to further refine our model. Metropolitan State University of Denver, Colorado University of Denver, Dr. Randall Tagg, Dr. Richard Krantz.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RaSc...53..577B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RaSc...53..577B"><span>Solar Influences on the Return Direction of High-<span class="hlt">Frequency</span> Radar Backscatter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burrell, Angeline G.; Perry, Gareth W.; Yeoman, Timothy K.; Milan, Stephen E.; Stoneback, Russell</p> <p>2018-04-01</p> <p>Coherent-scatter, high-<span class="hlt">frequency</span>, phased-array radars create narrow beams through the use of constructive and destructive interference patterns. This formation method leads to the creation of a secondary beam, or lobe, that is sent out behind the radar. This study investigates the relative importance of the beams in front of and behind the high-<span class="hlt">frequency</span> radar located in Hankasalmi, Finland, using observations taken over a solar cycle, as well as coincident observations from Hankasalmi and the Enhanced Polar Outflow Probe Radio Receiver Instrument. These observations show that the relative strength of the front and rear beams is <span class="hlt">frequency</span> dependent, with the relative amount of power sent to the front lobe increasing with increasing <span class="hlt">frequency</span>. At the range of <span class="hlt">frequencies</span> used by Hankasalmi, both front and rear beams are always present, though the main beam is always stronger than the rear lobe. Because signals are always transmitted to the front and rear of the radar, it is always possible to receive backscatter from both return directions. Examining the return direction as a function of local time, season, and solar cycle shows that the dominant return direction depends primarily on the local ionospheric structure. Diurnal changes in plasma density typically cause an increase in the amount of groundscatter returning from the rear lobe at night, though the strength of this <span class="hlt">variation</span> has a seasonal dependence. Solar cycle <span class="hlt">variations</span> are also seen in the groundscatter return direction, modifying the existing local time and seasonal <span class="hlt">variations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865621','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865621"><span><span class="hlt">Frequency</span> shift measurement in shock-compressed materials</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Moore, David S.; Schmidt, Stephen C.</p> <p>1985-01-01</p> <p>A method for determining molecular vibrational <span class="hlt">frequencies</span> in shock-compressed transparent materials. A single laser beam pulse is directed into a sample material while the material is shock-compressed from a direction opposite that of the incident laser beam. A Stokes beam produced by stimulated Raman scattering is emitted back along the path of the incident laser beam, that is, in the opposite direction to that of the incident laser beam. The Stokes beam is <span class="hlt">separated</span> from the incident beam and its <span class="hlt">frequency</span> measured. The difference in <span class="hlt">frequency</span> between the Stokes beam and the incident beam is representative of the characteristic <span class="hlt">frequency</span> of the Raman active mode of the sample. Both the incident beam and the Stokes beam pass perpendicularly through the shock front advancing through the sample, thereby minimizing adverse effects of refraction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27761740','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27761740"><span>Aftereffects of Intense Low-<span class="hlt">Frequency</span> Sound on Spontaneous Otoacoustic Emissions: Effect of <span class="hlt">Frequency</span> and Level.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jeanson, Lena; Wiegrebe, Lutz; Gürkov, Robert; Krause, Eike; Drexl, Markus</p> <p>2017-02-01</p> <p>The presentation of intense, low-<span class="hlt">frequency</span> (LF) sound to the human ear can cause very slow, sinusoidal oscillations of cochlear sensitivity after LF sound offset, coined the "Bounce" phenomenon. Changes in level and <span class="hlt">frequency</span> of spontaneous otoacoustic emissions (SOAEs) are a sensitive measure of the Bounce. Here, we investigated the effect of LF sound level and <span class="hlt">frequency</span> on the Bounce. Specifically, the level of SOAEs was tracked for minutes before and after a 90-s LF sound exposure. Trials were carried out with several LF sound levels (93 to 108 dB SPL corresponding to 47 to 75 phons at a fixed <span class="hlt">frequency</span> of 30 Hz) and different LF sound <span class="hlt">frequencies</span> (30, 60, 120, 240 and 480 Hz at a fixed loudness level of 80 phons). At an LF sound <span class="hlt">frequency</span> of 30 Hz, a minimal sound level of 102 dB SPL (64 phons) was sufficient to elicit a significant Bounce. In some subjects, however, 93 dB SPL (47 phons), the lowest level used, was sufficient to elicit the Bounce phenomenon and actual thresholds could have been even lower. Measurements with different LF sound <span class="hlt">frequencies</span> showed a mild reduction of the Bounce phenomenon with increasing LF sound <span class="hlt">frequency</span>. This indicates that the strength of the Bounce not only is a simple function of the spectral <span class="hlt">separation</span> between SOAE and LF sound <span class="hlt">frequency</span> but also depends on absolute LF sound <span class="hlt">frequency</span>, possibly related to the magnitude of the AC component of the outer hair cell receptor potential.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017FlDyR..49c5509A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017FlDyR..49c5509A"><span>Use of a rotating cylinder to induce laminar and turbulent <span class="hlt">separation</span> over a flat plate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Afroz, F.; Lang, A.; Jones, E.</p> <p>2017-06-01</p> <p>An innovative and easy technique using a rotating cylinder system has been implemented in a water tunnel experiment to generate an adverse pressure gradient (APG). The strength of the APG was varied through adjustment in the rotation speed and location of the cylinder. Then the technique was used for inducing a laminar <span class="hlt">separation</span> bubble (LSB) and turbulent boundary layer (TBL) <span class="hlt">separation</span> over a flat plate. A theoretical model to predict the pressure <span class="hlt">variation</span> induced on the plate consists of an inviscid flow over a reverse doublet-like configuration of two counter rotating cylinders. This model quantified the pressure distribution with changes of cylinder speed and location. The dimensionless velocity ratio (VR) of the cylinder rotation rate to the mainstream velocity and gap to diameter ratio \\tfrac{G}{D} were chosen as the two main ways of varying the strength of the APG, which affects the nature and extent of the LSB as well as TBL <span class="hlt">separation</span>. The experimental parametric study, using time-resolved digital particle image velocimetry, was then conducted in a water tunnel. The <span class="hlt">variation</span> in height (h), length (l), and the <span class="hlt">separation</span> point (S) of the LSB was documented due to the <span class="hlt">variation</span> in the APG. The similar type of experimental parametric study was used to explore the unsteady, turbulent <span class="hlt">separation</span> bubble in a 2D plane aligned with the flow and perpendicular to the plate. The mean detachment locations of TBL <span class="hlt">separation</span> are determined by two different definitions: (i) back-flow coefficient (χ) = 50%, and (ii) location of start of negative mean skin friction coefficient (C f). They are in good agreement and <span class="hlt">separation</span> bubble characteristics agreed well with results obtained using different methods thus proving the validity of the technique.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFD.R5005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFD.R5005S"><span><span class="hlt">Separation</span> control in a hypersonic shock wave / turbulent boundary-layer interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schreyer, Anne-Marie; Bermejo-Moreno, Ivan; Kim, Jeonglae; Urzay, Javier</p> <p>2016-11-01</p> <p>Hypersonic vehicles play a key role for affordable access to space. The associated flow fields are strongly affected by shock wave/turbulent boundary-layer interactions, and the inherent <span class="hlt">separation</span> causes flow distortion and low-<span class="hlt">frequency</span> unsteadiness. Microramp sub-boundary layer vortex generators are a promising means to control <span class="hlt">separation</span> and diminish associated detrimental effects. We investigate the effect of a microramp on the low-<span class="hlt">frequency</span> unsteadiness in a fully <span class="hlt">separated</span> interaction. A large eddy simulation of a 33 ∘ -compression-ramp interaction was performed for an inflow Mach number of 7.2 and a Reynolds number based on momentum thickness of Reθ = 3500 , matching the experiment of Schreyer et al. (2011). For the control case, we introduced a counter-rotating vortex pair, as induced by a single microramp, into the boundary layer through the inflow conditions. We applied a dynamic mode decomposition (DMD) on both cases to identify coherent structures that are responsible for the dynamic behavior. Based on the DMD, we discuss the reduction of the <span class="hlt">separation</span> zone and the stabilization of the shock motion achieved by the microramp, and contribute to the description of the governing mechanisms. Pursued during the 2016 CTR Summer Program at Stanford University.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1391856-frequency-analysis-uncertain-structures-using-imprecise-probability','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1391856-frequency-analysis-uncertain-structures-using-imprecise-probability"><span><span class="hlt">Frequency</span> analysis of uncertain structures using imprecise probability</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>Modares, Mehdi; Bergerson, Joshua</p> <p>2015-01-01</p> <p>Two new methods for finite element based <span class="hlt">frequency</span> analysis of a structure with uncertainty are developed. An imprecise probability formulation based on enveloping p-boxes is used to quantify the uncertainty present in the mechanical characteristics of the structure. For each element, independent <span class="hlt">variations</span> are considered. Using the two developed methods, P-box <span class="hlt">Frequency</span> Analysis (PFA) and Interval Monte-Carlo <span class="hlt">Frequency</span> Analysis (IMFA), sharp bounds on natural circular <span class="hlt">frequencies</span> at different probability levels are obtained. These methods establish a framework for handling incomplete information in structural dynamics. Numerical example problems are presented that illustrate the capabilities of the new methods along with discussionsmore » on their computational efficiency.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1467808','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1467808"><span>Os zygomaticum bipartitum: <span class="hlt">frequency</span> distribution in major human populations</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>HANIHARA, TSUNEHIKO; ISHIDA, HAJIME; DODO, YUKIO</p> <p>1998-01-01</p> <p>The <span class="hlt">frequency</span> of the Os zygomaticum bipartitum was examined in major human populations around the world. Eastern Asians have a higher <span class="hlt">frequency</span> of the bipartite zygomatic bone than any other geographical groups. The arctic peoples, Amerindians and the Oceanians, who all may have derived from eastern Asian population stocks, have a considerably low <span class="hlt">frequency</span> of this trait. The <span class="hlt">frequency</span> distribution from East/Southeast Asia to Africa and Europe through South/Central/West Asia suggests some clinality for the bipartite zygomatic bone. The second peak in the <span class="hlt">frequency</span> is seen in Subsaharan Africa. The clinal <span class="hlt">variation</span> with no identifiable regulation by subsistence patterns and environmental factors suggested a genetic background for the occurrence of the Os zygomaticum bipartitum. PMID:9723981</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21709334','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21709334"><span>Onsager's <span class="hlt">variational</span> principle in soft matter.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Doi, Masao</p> <p>2011-07-20</p> <p>In the celebrated paper on the reciprocal relation for the kinetic coefficients in irreversible processes, Onsager (1931 Phys. Rev. 37 405) extended Rayleigh's principle of the least energy dissipation to general irreversible processes. In this paper, I shall show that this <span class="hlt">variational</span> principle gives us a very convenient framework for deriving many established equations which describe the nonlinear and non-equilibrium phenomena in soft matter, such as phase <span class="hlt">separation</span> kinetics in solutions, gel dynamics, molecular modeling for viscoelasticity nemato-hydrodynamics, etc. Onsager's <span class="hlt">variational</span> principle can therefore be regarded as a solid general basis for soft matter physics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17928860','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17928860"><span><span class="hlt">Frequency</span> of word-use predicts rates of lexical evolution throughout Indo-European history.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pagel, Mark; Atkinson, Quentin D; Meade, Andrew</p> <p>2007-10-11</p> <p>Greek speakers say "omicronupsilonrho", Germans "schwanz" and the French "queue" to describe what English speakers call a 'tail', but all of these languages use a related form of 'two' to describe the number after one. Among more than 100 Indo-European languages and dialects, the words for some meanings (such as 'tail') evolve rapidly, being expressed across languages by dozens of unrelated words, while others evolve much more slowly--such as the number 'two', for which all Indo-European language speakers use the same related word-form. No general linguistic mechanism has been advanced to explain this striking <span class="hlt">variation</span> in rates of lexical replacement among meanings. Here we use four large and divergent language corpora (English, Spanish, Russian and Greek) and a comparative database of 200 fundamental vocabulary meanings in 87 Indo-European languages to show that the <span class="hlt">frequency</span> with which these words are used in modern language predicts their rate of replacement over thousands of years of Indo-European language evolution. Across all 200 meanings, frequently used words evolve at slower rates and infrequently used words evolve more rapidly. This relationship holds <span class="hlt">separately</span> and identically across parts of speech for each of the four language corpora, and accounts for approximately 50% of the <span class="hlt">variation</span> in historical rates of lexical replacement. We propose that the <span class="hlt">frequency</span> with which specific words are used in everyday language exerts a general and law-like influence on their rates of evolution. Our findings are consistent with social models of word change that emphasize the role of selection, and suggest that owing to the ways that humans use language, some words will evolve slowly and others rapidly across all languages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22380151','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22380151"><span>Operation of the CAPRICE electron cyclotron resonance ion source applying <span class="hlt">frequency</span> tuning and double <span class="hlt">frequency</span> heating.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Maimone, F; Tinschert, K; Celona, L; Lang, R; Mäder, J; Rossbach, J; Spädtke, P</p> <p>2012-02-01</p> <p>The properties of the electromagnetic waves heating the electrons of the ECR ion sources (ECRIS) plasma affect the features of the extracted ion beams such as the emittance, the shape, and the current, in particular for higher charge states. The electron heating methods such as the <span class="hlt">frequency</span> tuning effect and the double <span class="hlt">frequency</span> heating are widely used for enhancing the performances of ECRIS or even for the routine operation during the beam production. In order to better investigate these effects the CAPRICE ECRIS has been operated using these techniques. The ion beam properties for highly charged ions have been measured with beam diagnostic tools. The reason of the observed <span class="hlt">variations</span> of this performance can be related to the different electromagnetic field patterns, which are changing inside the plasma chamber when the <span class="hlt">frequency</span> is varying.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27091582','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27091582"><span>Correlated inter-regional <span class="hlt">variations</span> in low <span class="hlt">frequency</span> local field potentials and resting state BOLD signals within S1 cortex of monkeys.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wilson, George H; Yang, Pai-Feng; Gore, John C; Chen, Li Min</p> <p>2016-08-01</p> <p>The hypothesis that specific <span class="hlt">frequency</span> components of the spontaneous local field potentials (LFPs) underlie low <span class="hlt">frequency</span> fluctuations of resting state fMRI (rsfMRI) signals was tested. The previous analyses of rsfMRI signals revealed differential inter-regional correlations among areas 3a, 3b, and 1 of primary somatosensory cortex (S1) in anesthetized monkeys (Wang et al. [2013]: Neuron 78:1116-1126). Here LFP band(s) which correlated between S1 regions, and how these inter-regional correlation differences covaried with rsfMRI signals were examined. LFP signals were filtered into seven bands (delta, theta, alpha, beta, gamma low, gamma high, and gamma very high), and then a Hilbert transformation was applied to obtain measures of instantaneous amplitudes and temporal lags between regions of interest (ROI) digit-digit pairs (areas 3b-area 1, area 3a-area 1, area 3a-area 3b) and digit-face pairs (area 3b-face, area 1-face, and area 3a-face). It was found that <span class="hlt">variations</span> in the inter-regional correlation strengths between digit-digit and digit-face pairs in the delta (1-4 Hz), alpha (9-14 Hz), beta (15-30 Hz), and gamma (31-50 Hz) bands parallel those of rsfMRI signals to varying degrees. Temporal lags between digit-digit area pairs varied across LFP bands, with area 3a mostly leading areas 1/2 and 3b. In summary, the data demonstrates that the low and middle <span class="hlt">frequency</span> range (1-50 Hz) of spontaneous LFP signals similarly covary with the low <span class="hlt">frequency</span> fluctuations of rsfMRI signals within local circuits of S1, supporting a neuronal electrophysiological basis of rsfMRI signals. Inter-areal LFP temporal lag differences provided novel insights into the directionality of information flow among S1 areas at rest. Hum Brain Mapp 37:2755-2766, 2016. © 2016 Wiley Periodicals, Inc. © 2016 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011APS..DFDL16001V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011APS..DFDL16001V"><span>Effect of wakes from moving upstream rods on boundary layer <span class="hlt">separation</span> from a high lift airfoil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volino, Ralph J.</p> <p>2011-11-01</p> <p>Highly loaded airfoils in turbines allow power generation using fewer airfoils. High loading, however, can cause boundary layer <span class="hlt">separation</span>, resulting in reduced lift and increased aerodynamic loss. <span class="hlt">Separation</span> is affected by the interaction between rotating blades and stationary vanes. Wakes from upstream vanes periodically impinge on downstream blades, and can reduce <span class="hlt">separation</span>. The wakes include elevated turbulence, which can induce transition, and a velocity deficit, which results in an impinging flow on the blade surface known as a ``negative jet.'' In the present study, flow through a linear cascade of very high lift airfoils is studied experimentally. Wakes are produced with moving rods which cut through the flow upstream of the airfoils, simulating the effect of upstream vanes. Pressure and velocity fields are documented. Wake spacing and velocity are varied. At low Reynolds numbers without wakes, the boundary layer <span class="hlt">separates</span> and does not reattach. At high wake passing <span class="hlt">frequencies</span> <span class="hlt">separation</span> is largely suppressed. At lower <span class="hlt">frequencies</span>, ensemble averaged velocity results show intermittent <span class="hlt">separation</span> and reattachment during the wake passing cycle. Supported by NASA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......419M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......419M"><span>Novel Waveguide Structures in the Terahertz <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>Mbonye, Marx</p> <p></p> <p>Over the last decade, considerable research interest has peaked in realizing an efficient Terahertz (THz) waveguide for potential applications in imaging, sensing, and communications applications. Two of the promising candidates are the two-wire waveguide and the parallel-plate waveguide (PPWG). I present theoretical and experimental evidence that show that the two-wire waveguide supports low loss terahertz pulse propagation, and illustrate that the mode pattern at the end of the waveguide resembles that of a dipole. In comparison to the weakly guided Sommerfeld wave of a single wire waveguide, this two-wire structure exhibits much lower bending losses. I also observe that a commercial 300-Ohm two-wire TVantenna cable can be used for guiding <span class="hlt">frequency</span> components of up to 0.2 THz, although these cables are generally designed to operate only up to about 800 MHz. The parallel-plate waveguide is another promising candidate that would make an efficient THz waveguide, since it has relatively low Ohmic losses. The transverse electromagnetic mode (TEM) of this waveguide has been generally preferred since it has no cutoff <span class="hlt">frequency</span>, and therefore no group velocity dispersion. Utilizing this TEM mode, I study the reflection of THz radiation at the end of a PPWG, due to the impedance mismatch between the propagating transverse-electromagnetic mode and the free-space background. I find that for a PPWG with uniformly spaced plates, the reflection coefficient at the output face increases as the plate <span class="hlt">separation</span> decreases, consistent with predictions by early low <span class="hlt">frequency</span> ray optical theory. I observe this same trend in tapered PPWGs, when the input <span class="hlt">separation</span> is fixed, and the output <span class="hlt">separation</span> is varied. In another study, I investigate how to minimize diffraction losses in PPWGs by using plates with slightly concave surfaces. Using a simple "bouncing plane wave" analysis, I demonstrate how to determine an ideal radius of curvature for a waveguide operating at a given THz</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990064427','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990064427"><span>Studying the Fine Structure and Temporal <span class="hlt">Variations</span> of the Zodiacal Cloud and Asteroidal Dust Bands Using the 3-Year Near-IR COBE-DIRBE Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jayaraman, Sumita</p> <p>1999-01-01</p> <p>The report presents the results of the data analyses of the DIRBE-COBE data set to study the structure of the zodiacal cloud in the near-infrared wavebands at 1.2, 2.2, and 3.4 microns. The cloud has been divided into two components which have been analyzed and studied <span class="hlt">separately</span>. The annual <span class="hlt">variation</span> of the flux in the smooth or low <span class="hlt">frequency</span> component has been measured in all three bands and the presence of any asymmetries due to the Earth's resonant ring have been studied. The high <span class="hlt">frequency</span> component which primarily consisted of the asteroidal dust bands. Extensive and careful co-addition was done to extract the central bands in all three wavebands. The ten-degree bands are present in the 1.2 and 2.2 microns but not in the 3.4 micron waveband.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/863597','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/863597"><span>Isotope <span class="hlt">separation</span> apparatus</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Arnush, Donald; MacKenzie, Kenneth R.; Wuerker, Ralph F.</p> <p>1980-01-01</p> <p>Isotope <span class="hlt">separation</span> apparatus consisting of a plurality of cells disposed adjacent to each other in an evacuated container. A common magnetic field is established extending through all of the cells. A source of energetic electrons at one end of the container generates electrons which pass through the cells along the magnetic field lines. Each cell includes an array of collector plates arranged in parallel or in tandem within a common magnetic field. Sets of collector plates are disposed adjacent to each other in each cell. Means are provided for differentially energizing ions of a desired isotope by applying energy at the cyclotron resonant <span class="hlt">frequency</span> of the desired isotope. As a result, the energized desired ions are preferentially collected by the collector plates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JSV...340...22H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JSV...340...22H"><span>Experimental and analytical study of secondary path <span class="hlt">variations</span> in active engine mounts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hausberg, Fabian; Scheiblegger, Christian; Pfeffer, Peter; Plöchl, Manfred; Hecker, Simon; Rupp, Markus</p> <p>2015-03-01</p> <p>Active engine mounts (AEMs) provide an effective solution to further improve the acoustic and vibrational comfort of passenger cars. Typically, adaptive feedforward control algorithms, e.g., the filtered-x-least-mean-squares (FxLMS) algorithm, are applied to cancel disturbing engine vibrations. These algorithms require an accurate estimate of the AEM active dynamic characteristics, also known as the secondary path, in order to guarantee control performance and stability. This paper focuses on the experimental and theoretical study of secondary path <span class="hlt">variations</span> in AEMs. The impact of three major influences, namely nonlinearity, change of preload and component temperature, on the AEM active dynamic characteristics is experimentally analyzed. The obtained test results are theoretically investigated with a linear AEM model which incorporates an appropriate description for elastomeric components. A special experimental set-up extends the model validation of the active dynamic characteristics to higher <span class="hlt">frequencies</span> up to 400 Hz. The theoretical and experimental results show that significant secondary path <span class="hlt">variations</span> are merely observed in the <span class="hlt">frequency</span> range of the AEM actuator's resonance <span class="hlt">frequency</span>. These <span class="hlt">variations</span> mainly result from the change of the component temperature. As the stability of the algorithm is primarily affected by the actuator's resonance <span class="hlt">frequency</span>, the findings of this paper facilitate the design of AEMs with simpler adaptive feedforward algorithms. From a practical point of view it may further be concluded that algorithmic countermeasures against instability are only necessary in the <span class="hlt">frequency</span> range of the AEM actuator's resonance <span class="hlt">frequency</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2004ASAJ..115.2609F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ASAJ..115.2609F"><span>Fundamental <span class="hlt">frequency</span> perturbation indicates perceived health and age in male and female speakers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feinberg, David R.</p> <p>2004-05-01</p> <p>There is strong support for the idea that healthy vocal chords are able to produce fundamental <span class="hlt">frequencies</span> (F0) with minimal perturbation. Measures of F0 perturbation have been shown to discriminate pathological versus healthy populations. In addition to measuring vocal chord health, F0 perturbation is a correlate of real and perceived age. Here, the role of jitter (periodic <span class="hlt">variation</span> in F0) and shimmer (periodic <span class="hlt">variation</span> in amplitude of F0) in perceived health and age in a young adult (males aged 18-33, females aged 18-26), nondysphonic population was investigated. Voices were assessed for health and age by peer aged, opposite-sex raters. Jitter and shimmer were measured with Praat software (www.praat.org) using various algorithms (jitter: DDP, local, local absolute, PPQ5, and RAP; shimmer: DDA, local, local absolute, APQ3, APQ5, APQ11) to reduce measurement error, and to ascertain the robustness of the findings. Male and female voices were analyzed <span class="hlt">separately</span>. In both sexes, ratings of health and age were significantly correlated. Measures of jitter and shimmer correlated negatively with perceived health, and positively with perceived age. Further analysis revealed that these effects were independent in male voices. Implications of this finding are that attributions of vocal health and age may reflect actual underlying condition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptEn..56c6114C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptEn..56c6114C"><span>Accuracy enhanced distance measurement system using double-sideband modulated <span class="hlt">frequency</span> scanning interferometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Xilun; Wang, Xiangchuan; Pan, Shilong</p> <p>2017-03-01</p> <p>An implementation of a distance measurement system using double-sideband with suppressed carrier modulation (DSB-SC) <span class="hlt">frequency</span> scanning interferometry is proposed to reduce the <span class="hlt">variations</span> in the optical path and improve the measurement accuracy. In this proposed system, the electro-optic DSB-SC is used to create dual-swept signals with opposite scanning directions. For each swept signal, the relative distance between the reference arm and the measuring arm is determined by the beat <span class="hlt">frequency</span> of signals from two arms. By multiplying both beat signals, measurement errors caused by <span class="hlt">variations</span> in the optical path can be greatly reduced. As an experimental demonstration, a vibration was introduced in the optical path length. The experimental results show that the <span class="hlt">variations</span> can be suppressed for over 19.9 dB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850036090&hterms=IOTA&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DIOTA','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850036090&hterms=IOTA&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DIOTA"><span>Copernicus observations of Iota Herculis velocity <span class="hlt">variations</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rogerson, J. B., Jr.</p> <p>1984-01-01</p> <p>Observations of Iota Her at 109.61-109.67 nm obtained with the U1 channel of the Copernicus spectrophotometer at resolution 5 pm during 3.6 days in May, 1979, are reported. Radial-velocity <span class="hlt">variations</span> are detected and analyzed as the sum of two sinusoids with <span class="hlt">frequencies</span> 0.660 and 0.618 cycles/day and amplitudes 9.18 and 8.11 km/s, respectively. Weak evidence supporting the 13.9-h periodicity seen in line-profile <span class="hlt">variations</span> by Smith (1978) is found.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25811421','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25811421"><span>Freely Chosen Index Finger Tapping <span class="hlt">Frequency</span> Is Increased in Repeated Bouts of Tapping.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hansen, Ernst Albin; Ebbesen, Brian Duborg; Dalsgaard, Ane; Mora-Jensen, Mark Holten; Rasmussen, Jakob</p> <p>2015-01-01</p> <p>Healthy individuals (n = 40) performed index finger tapping at freely chosen <span class="hlt">frequency</span> during repeated bouts and before and after near-maximal muscle action consisting of 3 intense flexions of the index finger metacarpal phalangeal joint. One experiment showed, unexpectedly, that a bout of tapping increased the tapping <span class="hlt">frequency</span> in the subsequent bout. Thus, a cumulating increase of 8.2 ± 5.4% (p < .001) occurred across 4 bouts, which were all <span class="hlt">separated</span> by 10 min rest periods. Follow-up experiments revealed that tapping <span class="hlt">frequency</span> was still increased in consecutive bouts when rest periods were extended to 20 min. Besides, near-maximal muscle activation, followed by 5 min rest, did not affect the tapping <span class="hlt">frequency</span>. In conclusion, freely chosen tapping <span class="hlt">frequency</span> was increased in repeated bouts of tapping, which were <span class="hlt">separated</span> by 10-20 min rest periods. The observed phenomenon is suggested to be termed repeated bout rate enhancement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EJASP2014...27M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EJASP2014...27M"><span>Perceptually controlled doping for audio source <span class="hlt">separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mahé, Gaël; Nadalin, Everton Z.; Suyama, Ricardo; Romano, João MT</p> <p>2014-12-01</p> <p>The <span class="hlt">separation</span> of an underdetermined audio mixture can be performed through sparse component analysis (SCA) that relies however on the strong hypothesis that source signals are sparse in some domain. To overcome this difficulty in the case where the original sources are available before the mixing process, the informed source <span class="hlt">separation</span> (ISS) embeds in the mixture a watermark, which information can help a further <span class="hlt">separation</span>. Though powerful, this technique is generally specific to a particular mixing setup and may be compromised by an additional bitrate compression stage. Thus, instead of watermarking, we propose a `doping' method that makes the time-<span class="hlt">frequency</span> representation of each source more sparse, while preserving its audio quality. This method is based on an iterative decrease of the distance between the distribution of the signal and a target sparse distribution, under a perceptual constraint. We aim to show that the proposed approach is robust to audio coding and that the use of the sparsified signals improves the source <span class="hlt">separation</span>, in comparison with the original sources. In this work, the analysis is made only in instantaneous mixtures and focused on voice sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28831962','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28831962"><span>Effects of feed delivery <span class="hlt">frequency</span> in different environmental conditions on time budget of lactating dairy cows.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mattachini, Gabriele; Bava, Luciana; Sandrucci, Anna; Tamburini, Alberto; Riva, Elisabetta; Provolo, Giorgio</p> <p>2017-08-01</p> <p>This study aimed to examine the influence of feed delivery <span class="hlt">frequency</span> and environmental conditions on daily time budget of lactating dairy cows. The study was carried out in two commercial dairy farms with Holstein herds. Fifty lactating dairy cows milked in automatic milking units (AMS farm) and 96 primiparous lactating dairy cows milked in a conventional milking parlour (conventional farm) were exposed to different <span class="hlt">frequencies</span> of feed delivery replicated in different periods of the year (warm and mild) that were characterized by different temperature-humidity indices (THI). On each farm, feeding treatments consisted of two different feed delivery <span class="hlt">frequencies</span> (1× and 2× on the AMS farm; 2× and 3× on the conventional farm). All behaviours of the cows were monitored for the last 8 d of each treatment period using continuous video recording. The two data sets from different farm systems were considered <span class="hlt">separately</span> for analysis. On both farms, environmental conditions expressed as THI affected time budgets and the pattern of the behavioural indices throughout the day. The <span class="hlt">variation</span> in the <span class="hlt">frequency</span> of feed delivery seems to affect the cow's time budget only in a limited way. Standing time of cows on the conventional farm and the time spent by cows in the milking waiting area on the AMS farm both increased in response to increased feeding <span class="hlt">frequency</span>. Although feed delivery <span class="hlt">frequency</span> showed limited influence on cow's time budget, the effect on standing time could be carefully considered, especially on farms equipped with AMS where the type of cow traffic system (e.g., milking first) might amplify the negative consequences of more frequent feed delivery. Further investigations are required to evaluate the effect of THI and feed delivery <span class="hlt">frequency</span> on other aspects of behavioural activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AIPC..823..845Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AIPC..823..845Q"><span>Development of a 4 K <span class="hlt">Separate</span> Two-Stage Pulse Tube Refrigerator with High Efficiency</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qiu, L. M.; He, Y. L.; Gan, Z. H.; Chen, G. B.</p> <p>2006-04-01</p> <p>Compared to the traditional 4 K cryocoolers, the <span class="hlt">separate</span> 4 K pulse tube refrigerator (PTR) consists of two independent PTRs, which are thermally connected between the cold end of the first stage and some middle position of the second stage regenerator. It is possible to use different <span class="hlt">frequency</span>, valve timing, phase shifter and even compressor for each stage for better cooling performance. A 4 K <span class="hlt">separate</span> two-stage PTR was designed and manufactured. The first stage was <span class="hlt">separately</span> optimized. A minimum temperature of 12.6 K and cooling capacity of 59.0 W at 40 K was achieved for the first stage by adding some Er3Ni at the cold part of the regenerator. An experimental investigation of valve timing effects on the cooling performance of the 4 K <span class="hlt">separate</span> two-stage PTR is reported. The experiments show that the optimization of valve timing can considerably improve the cooling performance of the PTR. Cooling capacity of 0.59 W at 4.2 K and 15.4 W at 37.0 K were achieved with an actual input power of 6.6 kW. Effect of <span class="hlt">frequency</span> on the performance of the <span class="hlt">separate</span> two-stage PTR is also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SPIE.9378E..22S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SPIE.9378E..22S"><span>Fiber-laser <span class="hlt">frequency</span> combs for the generation of tunable single-<span class="hlt">frequency</span> laser lines, mm- and THz-waves and sinc-shaped Nyquist pulses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, Thomas</p> <p>2015-03-01</p> <p>High-quality <span class="hlt">frequency</span> comb sources like femtosecond-lasers have revolutionized the metrology of fundamental physical constants. The generated comb consists of <span class="hlt">frequency</span> lines with an equidistant <span class="hlt">separation</span> over a bandwidth of several THz. This bandwidth can be broadened further to a super-continuum of more than an octave through propagation in nonlinear media. The <span class="hlt">frequency</span> <span class="hlt">separation</span> between the lines is defined by the repetition rate and the width of each comb line can be below 1 Hz, even without external stabilization. By extracting just one of these lines, an ultra-narrow linewidth, tunable laser line for applications in communications and spectroscopy can be generated. If two lines are extracted, the superposition of these lines in an appropriate photo-mixer produces high-quality millimeter- and THz-waves. The extraction of several lines can be used for the creation of almost-ideally sinc-shaped Nyquist pulses, which enable optical communications with the maximum-possible baud rate. Especially combs generated by low-cost, small-footprint fs-fiber lasers are very promising. However due to the resonator length, the comb <span class="hlt">frequencies</span> have a typical <span class="hlt">separation</span> of 80 - 100 MHz, far too narrow for the selection of single tones with standard optical filters. Here the extraction of single lines of an fs-fiber laser by polarization pulling assisted stimulated Brillouin scattering is presented. The application of these extracted lines as ultra-narrow, stable and tunable laser lines, for the generation of very high-quality mm and THz-waves with an ultra-narrow linewidth and phase noise and for the generation of sinc-shaped Nyquist pulses with arbitrary bandwidth and repetition rate is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23435049','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23435049"><span><span class="hlt">Frequency</span> noise properties of lasers for interferometry in nanometrology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hrabina, Jan; Lazar, Josef; Holá, Miroslava; Cíp, Ondřej</p> <p>2013-02-07</p> <p>In this contribution we focus on laser <span class="hlt">frequency</span> noise properties and their influence on the interferometric displacement measurements. A setup for measurement of laser <span class="hlt">frequency</span> noise is proposed and tested together with simultaneous measurement of fluctuations in displacement in the Michelson interferometer. Several laser sources, including traditional He-Ne and solid-state lasers, and their noise properties are evaluated and compared. The contribution of the laser <span class="hlt">frequency</span> noise to the displacement measurement is discussed in the context of other sources of uncertainty associated with the interferometric setup, such as, mechanics, resolution of analog-to-digital conversion, <span class="hlt">frequency</span> bandwidth of the detection chain, and <span class="hlt">variations</span> of the refractive index of air.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJP..132..452W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJP..132..452W"><span>Study on ion energy distribution in low-<span class="hlt">frequency</span> oscillation time scale of Hall thrusters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wei, Liqiu; Li, Wenbo; Ding, Yongjie; Han, Liang; Yu, Daren; Cao, Yong</p> <p>2017-11-01</p> <p>This paper reports on the dynamic characteristics of the distribution of ion energy during Hall thruster discharge in the low-<span class="hlt">frequency</span> 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-<span class="hlt">frequency</span> oscillation. The results show that the ion energy distribution exhibits a periodic change during the low-<span class="hlt">frequency</span> oscillation. Moreover, the <span class="hlt">variation</span> in the ion energy peak is opposite to that of the discharge current, and the <span class="hlt">variations</span> in width of the ion energy distribution and the ratio of high-energy ions are consistent with that of the discharge current. The <span class="hlt">variation</span> 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-<span class="hlt">frequency</span> oscillation depends on the relationship between the ionization source term and discharge potential distribution during ionization in the discharge channel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAG...149...42S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAG...149...42S"><span><span class="hlt">Frequency</span> band adjustment match filtering based on variable <span class="hlt">frequency</span> GPR antennas pairing scheme for shallow subsurface investigations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shaikh, Shahid Ali; Tian, Gang; Shi, Zhanjie; Zhao, Wenke; Junejo, S. A.</p> <p>2018-02-01</p> <p>Ground penetrating Radar (GPR) is an efficient tool for subsurface geophysical investigations, particularly at shallow depths. The non-destructiveness, cost efficiency, and data reliability are the important factors that make it an ideal tool for the shallow subsurface investigations. Present study encompasses; <span class="hlt">variations</span> in central <span class="hlt">frequency</span> of transmitting and receiving GPR antennas (Tx-Rx) have been analyzed and <span class="hlt">frequency</span> band adjustment match filters are fabricated and tested accordingly. Normally, the <span class="hlt">frequency</span> of both the antennas remains similar to each other whereas in this study we have experimentally changed the <span class="hlt">frequencies</span> of Tx-Rx and deduce the response. Instead of normally adopted three pairs, a total of nine Tx-Rx pairs were made from 50 MHz, 100 MHz, and 200 MHz antennas. The experimental data was acquired at the designated near surface geophysics test site of the Zhejiang University, Hangzhou, China. After the impulse response analysis of acquired data through conventional as well as varied Tx-Rx pairs, different swap effects were observed. The <span class="hlt">frequency</span> band and exploration depth are influenced by transmitting <span class="hlt">frequencies</span> rather than the receiving <span class="hlt">frequencies</span>. The impact of receiving <span class="hlt">frequencies</span> was noticed on the resolution; the more noises were observed using the combination of high <span class="hlt">frequency</span> transmitting with respect to low <span class="hlt">frequency</span> receiving. On the basis of above said variable results we have fabricated two <span class="hlt">frequency</span> band adjustment match filters, the constant <span class="hlt">frequency</span> transmitting (CFT) and the variable <span class="hlt">frequency</span> transmitting (VFT) <span class="hlt">frequency</span> band adjustment match filters. By the principle, the lower and higher <span class="hlt">frequency</span> components were matched and then incorporated with intermediate one. Therefore, this study reveals that a Tx-Rx combination of low <span class="hlt">frequency</span> transmitting with high <span class="hlt">frequency</span> receiving is a better choice. Moreover, both the filters provide better radargram than raw one, the result of VFT <span class="hlt">frequency</span> band adjustment filter is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JCoPh.330..981G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JCoPh.330..981G"><span>Time-dependent wave splitting and source <span class="hlt">separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grote, Marcus J.; Kray, Marie; Nataf, Frédéric; Assous, Franck</p> <p>2017-02-01</p> <p>Starting from classical absorbing boundary conditions, we propose a method for the <span class="hlt">separation</span> of time-dependent scattered wave fields due to multiple sources or obstacles. In contrast to previous techniques, our method is local in space and time, deterministic, and avoids a priori assumptions on the <span class="hlt">frequency</span> spectrum of the signal. Numerical examples in two space dimensions illustrate the usefulness of wave splitting for time-dependent scattering problems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3872487','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3872487"><span>Spatial <span class="hlt">separation</span> benefit for unaided and aided listening</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ahlstrom, Jayne B.; Horwitz, Amy R.; Dubno, Judy R.</p> <p>2013-01-01</p> <p>Consonant recognition in noise was measured at a fixed signal-to-noise ratio as a function of low-pass-cutoff <span class="hlt">frequency</span> and noise location in older adults fit with bilateral hearing aids. To quantify age-related differences, spatial benefit was assessed in younger and older adults with normal hearing. Spatial benefit was similar for all groups suggesting that older adults used interaural difference cues to improve speech recognition in noise equivalently to younger adults. Although amplification was sufficient to increase high-<span class="hlt">frequency</span> audibility with spatial <span class="hlt">separation</span>, hearing-aid benefit was minimal, suggesting that factors beyond simple audibility may be responsible for limited hearing-aid benefit. PMID:24121648</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4307689','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/4307689"><span>VELOCITY SELECTOR METHOD FOR THE <span class="hlt">SEPARATION</span> OF ISOTOPES</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Britten, R.J.</p> <p>1957-12-31</p> <p>A velocity selector apparatus is described for <span class="hlt">separating</span> and collecting an enriched fraction of the isotope of a particular element. The invention has the advantage over conventional mass spectrometers in that a magnetic field is not used, doing away with the attendant problems of magnetic field <span class="hlt">variation</span>. The apparatus <span class="hlt">separates</span> the isotopes by selectively accelerating the ionized constituents present in a beam of the polyisotopic substance that are of uniform kinetic energy, the acceleration being applied intermittently and at spaced points along the beam and in a direction normal to the direction of the propagation of the uniform energy beam whereby a transverse displacement of the isotopic constituents of different mass is obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21852715','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21852715"><span>Effect of outer wing <span class="hlt">separation</span> on lift and thrust generation in a flapping wing system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mahardika, Nanang; Viet, Nguyen Quoc; Park, Hoon Cheol</p> <p>2011-09-01</p> <p>We explore the implementation of wing feather <span class="hlt">separation</span> and lead-lagging motion to a flapping wing. A biomimetic flapping wing system with <span class="hlt">separated</span> outer wings is designed and demonstrated. The artificial wing feather <span class="hlt">separation</span> is implemented in the biomimetic wing by dividing the wing into inner and outer wings. The features of flapping, lead-lagging, and outer wing <span class="hlt">separation</span> of the flapping wing system are captured by a high-speed camera for evaluation. The performance of the flapping wing system with <span class="hlt">separated</span> outer wings is compared to that of a flapping wing system with closed outer wings in terms of forward force and downward force production. For a low flapping <span class="hlt">frequency</span> ranging from 2.47 to 3.90 Hz, the proposed biomimetic flapping wing system shows a higher thrust and lift generation capability as demonstrated by a series of experiments. For 1.6 V application (lower <span class="hlt">frequency</span> operation), the flapping wing system with <span class="hlt">separated</span> wings could generate about 56% higher forward force and about 61% less downward force compared to that with closed wings, which is enough to demonstrate larger thrust and lift production capability of the <span class="hlt">separated</span> outer wings. The experiments show that the outer parts of the <span class="hlt">separated</span> wings are able to deform, resulting in a smaller amount of drag production during the upstroke, while still producing relatively greater lift and thrust during the downstroke.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24556674','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24556674"><span>Inductive sensor performance in partial discharges and noise <span class="hlt">separation</span> by means of spectral power ratios.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ardila-Rey, Jorge Alfredo; Rojas-Moreno, Mónica Victoria; Martínez-Tarifa, Juan Manuel; Robles, Guillermo</p> <p>2014-02-19</p> <p>Partial discharge (PD) detection is a standardized technique to qualify electrical insulation in machines and power cables. Several techniques that analyze the waveform of the pulses have been proposed to discriminate noise from PD activity. Among them, spectral power ratio representation shows great flexibility in the <span class="hlt">separation</span> of the sources of PD. Mapping spectral power ratios in two-dimensional plots leads to clusters of points which group pulses with similar characteristics. The position in the map depends on the nature of the partial discharge, the setup and the <span class="hlt">frequency</span> response of the sensors. If these clusters are clearly <span class="hlt">separated</span>, the subsequent task of identifying the source of the discharge is straightforward so the distance between clusters can be a figure of merit to suggest the best option for PD recognition. In this paper, two inductive sensors with different <span class="hlt">frequency</span> responses to pulsed signals, a high <span class="hlt">frequency</span> current transformer and an inductive loop sensor, are analyzed to test their performance in detecting and <span class="hlt">separating</span> the sources of partial discharges.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3958299','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3958299"><span>Inductive Sensor Performance in Partial Discharges and Noise <span class="hlt">Separation</span> by Means of Spectral Power Ratios</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ardila-Rey, Jorge Alfredo; Rojas-Moreno, Mónica Victoria; Martínez-Tarifa, Juan Manuel; Robles, Guillermo</p> <p>2014-01-01</p> <p>Partial discharge (PD) detection is a standardized technique to qualify electrical insulation in machines and power cables. Several techniques that analyze the waveform of the pulses have been proposed to discriminate noise from PD activity. Among them, spectral power ratio representation shows great flexibility in the <span class="hlt">separation</span> of the sources of PD. Mapping spectral power ratios in two-dimensional plots leads to clusters of points which group pulses with similar characteristics. The position in the map depends on the nature of the partial discharge, the setup and the <span class="hlt">frequency</span> response of the sensors. If these clusters are clearly <span class="hlt">separated</span>, the subsequent task of identifying the source of the discharge is straightforward so the distance between clusters can be a figure of merit to suggest the best option for PD recognition. In this paper, two inductive sensors with different <span class="hlt">frequency</span> responses to pulsed signals, a high <span class="hlt">frequency</span> current transformer and an inductive loop sensor, are analyzed to test their performance in detecting and <span class="hlt">separating</span> the sources of partial discharges. PMID:24556674</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22641702','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22641702"><span>A novel encoding scheme for effective biometric discretization: Linearly <span class="hlt">Separable</span> Subcode.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lim, Meng-Hui; Teoh, Andrew Beng Jin</p> <p>2013-02-01</p> <p><span class="hlt">Separability</span> in a code is crucial in guaranteeing a decent Hamming-distance <span class="hlt">separation</span> among the codewords. In multibit biometric discretization where a code is used for quantization-intervals labeling, <span class="hlt">separability</span> is necessary for preserving distance dissimilarity when feature components are mapped from a discrete space to a Hamming space. In this paper, we examine <span class="hlt">separability</span> of Binary Reflected Gray Code (BRGC) encoding and reveal its inadequacy in tackling interclass <span class="hlt">variation</span> during the discrete-to-binary mapping, leading to a tradeoff between classification performance and entropy of binary output. To overcome this drawback, we put forward two encoding schemes exhibiting full-ideal and near-ideal <span class="hlt">separability</span> capabilities, known as Linearly <span class="hlt">Separable</span> Subcode (LSSC) and Partially Linearly <span class="hlt">Separable</span> Subcode (PLSSC), respectively. These encoding schemes convert the conventional entropy-performance tradeoff into an entropy-redundancy tradeoff in the increase of code length. Extensive experimental results vindicate the superiority of our schemes over the existing encoding schemes in discretization performance. This opens up possibilities of achieving much greater classification performance with high output entropy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1215493','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1215493"><span>Algorithm for identifying and <span class="hlt">separating</span> beats from arterial pulse records</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Treo, Ernesto F; Herrera, Myriam C; Valentinuzzi, Max E</p> <p>2005-01-01</p> <p>Background This project was designed as an epidemiological aid-selecting tool for a small country health center with the general objective of screening out possible coronary patients. Peripheral artery function can be non-invasively evaluated by impedance plethysmography. Changes in these vessels appear as good predictors of future coronary behavior. Impedance plethysmography detects volume <span class="hlt">variations</span> after simple occlusive maneuvers that may show indicative modifications in arterial/venous responses. Averaging of a series of pulses is needed and this, in turn, requires proper determination of the beginning and end of each beat. Thus, the objective here is to describe an algorithm to identify and <span class="hlt">separate</span> out beats from a plethysmographic record. A secondary objective was to compare the output given by human operators against the algorithm. Methods The identification algorithm detected the beat's onset and end on the basis of the maximum rising phase, the choice of possible ventricular systolic starting points considering cardiac <span class="hlt">frequency</span>, and the adjustment of some tolerance values to optimize the behavior. Out of 800 patients in the study, 40 occlusive records (supradiastolic- subsystolic) were randomly selected without any preliminary diagnosis. Radial impedance plethysmographic pulse and standard ECG were recorded digitizing and storing the data. Cardiac <span class="hlt">frequency</span> was estimated with the Power Density Function and, thereafter, the signal was derived twice, followed by binarization of the first derivative and rectification of the second derivative. The product of the two latter results led to a weighing signal from which the cycles' onsets and ends were established. Weighed and <span class="hlt">frequency</span> filters are needed along with the pre-establishment of their respective tolerances. Out of the 40 records, 30 seconds strands were randomly chosen to be analyzed by the algorithm and by two operators. Sensitivity and accuracy were calculated by means of the true/false and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6365630','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6365630"><span><span class="hlt">Frequency</span> shift measurement in shock-compressed materials</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Moore, D.S.; Schmidt, S.C.</p> <p>1984-02-21</p> <p>A method is disclosed for determining molecular vibrational <span class="hlt">frequencies</span> in shock-compressed transparent materials. A single laser beam pulse is directed into a sample material while the material is shock-compressed from a direction opposite that of the incident laser beam. A Stokes beam produced by stimulated Raman scattering is emitted back along the path of the incident laser beam, that is, in the opposite direction to that of the incident laser beam. The Stokes beam is <span class="hlt">separated</span> from the incident beam and its <span class="hlt">frequency</span> measured. The difference in <span class="hlt">frequency</span> between the Stokes beam and the incident beam is representative of the characteristic <span class="hlt">frequency</span> of the Raman active mode of the sample. Both the incident beam and the Stokes beam pass perpendicularly through the stock front advancing through the sample, thereby minimizing adverse effects of refraction.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1461899','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1461899"><span>Inherited differences in crossing over and gene conversion <span class="hlt">frequencies</span> between wild strains of Sordaria fimicola from "Evolution Canyon".</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Saleem, M; Lamb, B C; Nevo, E</p> <p>2001-01-01</p> <p>Recombination generates new combinations of existing genetic <span class="hlt">variation</span> and therefore may be important in adaptation and evolution. We investigated whether there was natural genetic <span class="hlt">variation</span> for recombination <span class="hlt">frequencies</span> and whether any such <span class="hlt">variation</span> was environment related and possibly adaptive. Crossing over and gene conversion <span class="hlt">frequencies</span> often differed significantly in a consistent direction between wild strains of the fungus Sordaria fimicola isolated from a harsher or a milder microscale environment in "Evolution Canyon," Israel. First- and second-generation descendants from selfing the original strains from the harsher, more variable, south-facing slope had higher <span class="hlt">frequencies</span> of crossing over in locus-centromere intervals and of gene conversion than those from the lusher north-facing slopes. There were some significant differences between strains within slopes, but these were less marked than between slopes. Such inherited <span class="hlt">variation</span> could provide a basis for natural selection for optimum recombination <span class="hlt">frequencies</span> in each environment. There were no significant differences in meiotic hybrid DNA correction <span class="hlt">frequencies</span> between strains from the different slopes. The conversion analysis was made using only conversions to wild type, because estimations of conversion to mutant were affected by a high <span class="hlt">frequency</span> of spontaneous mutation. There was no polarized segregation of chromosomes at meiosis I or of chromatids at meiosis II. PMID:11779798</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11779798','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11779798"><span>Inherited differences in crossing over and gene conversion <span class="hlt">frequencies</span> between wild strains of Sordaria fimicola from "Evolution Canyon".</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saleem, M; Lamb, B C; Nevo, E</p> <p>2001-12-01</p> <p>Recombination generates new combinations of existing genetic <span class="hlt">variation</span> and therefore may be important in adaptation and evolution. We investigated whether there was natural genetic <span class="hlt">variation</span> for recombination <span class="hlt">frequencies</span> and whether any such <span class="hlt">variation</span> was environment related and possibly adaptive. Crossing over and gene conversion <span class="hlt">frequencies</span> often differed significantly in a consistent direction between wild strains of the fungus Sordaria fimicola isolated from a harsher or a milder microscale environment in "Evolution Canyon," Israel. First- and second-generation descendants from selfing the original strains from the harsher, more variable, south-facing slope had higher <span class="hlt">frequencies</span> of crossing over in locus-centromere intervals and of gene conversion than those from the lusher north-facing slopes. There were some significant differences between strains within slopes, but these were less marked than between slopes. Such inherited <span class="hlt">variation</span> could provide a basis for natural selection for optimum recombination <span class="hlt">frequencies</span> in each environment. There were no significant differences in meiotic hybrid DNA correction <span class="hlt">frequencies</span> between strains from the different slopes. The conversion analysis was made using only conversions to wild type, because estimations of conversion to mutant were affected by a high <span class="hlt">frequency</span> of spontaneous mutation. There was no polarized segregation of chromosomes at meiosis I or of chromatids at meiosis II.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27687570','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27687570"><span>Weak low-<span class="hlt">frequency</span> electromagnetic oscillations in water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liboff, A R; Poggi, Claudio; Pratesi, Piero</p> <p>2017-01-01</p> <p>Recent observations of low-<span class="hlt">frequency</span> electromagnetic oscillations in water suggest an inductive structural component. Accordingly, we assume a helical basis enabling us to model water as an LC tuned oscillator. A proposed tetrahedral structure consisting of three water molecules and one hydronium ion is incorporated into the Boerdijk-Coxeter tetrahelix to form long water chains that are shown to have resonance <span class="hlt">frequencies</span> consistent with observation. This model also serves to explain <span class="hlt">separately</span> reported claims of ion cyclotron resonance of hydronium ions, in that the tetrahelix provides a built-in path for helical proton-hopping.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/867321','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/867321"><span>Particle <span class="hlt">separator</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Hendricks, Charles D.</p> <p>1990-01-01</p> <p>Method and apparatus (10) are provided for <span class="hlt">separating</span> and classifying particles (48,50,56) by dispersing the particles within a fluid (52) that is upwardly flowing within a cone-shaped pipe (12) that has its large end (20) above its small end (18). Particles of similar size and shape (48,50) migrate to individual levels (A,B) within the flowing fluid. As the fluid is deflected by a plate (42) at the top end of the pipe (12), the smallest particles are collected on a shelf-like flange (40). Ever larger particles are collected as the flow rate of the fluid is increased. To prevent particle sticking on the walls (14) of the pipe (12), additional fluid is caused to flow into the pipe (12) through holes (68) that are specifically provided for that purpose. Sticking is further prevented by high <span class="hlt">frequency</span> vibrators (70) that are positioned on the apparatus (10).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28619514','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28619514"><span>The <span class="hlt">frequency</span> of Th17 cells in the small intestine exhibits a day-night <span class="hlt">variation</span> dependent on circadian clock activity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thu Le, Ha Pham; Nakamura, Yuki; Oh-Oka, Kyoko; Ishimaru, Kayoko; Nakajima, Shotaro; Nakao, Atsuhito</p> <p>2017-08-19</p> <p>Interleukin-17-producing CD4 + T helper (Th17) cells are a key immune lineage that protects against bacterial and fungal infections at mucosal surfaces. At steady state, Th17 cells are abundant in the small intestinal mucosa of mice. There are several mechanisms for regulating the population of Th17 cells in the small intestine, reflecting the importance of maintaining their numbers in the correct balance. Here we demonstrate the existence of a time-of-day-dependent <span class="hlt">variation</span> in the <span class="hlt">frequency</span> of Th17 cells in the lamina propria of the small intestine in wild-type mice, which was not observed in mice with a loss-of-function mutation of the core circadian gene Clock or in mice housed under aberrant light/dark conditions. Consistent with this, expression of CCL20, a chemokine that regulates homeostatic trafficking of Th17 cells to the small intestine, exhibited circadian rhythms in the small intestine of wild-type, but not Clock-mutated, mice. In support of these observations, the magnitude of ovalbumin (OVA)-specific antibody and T-cell responses in mice sensitized with OVA plus cholera toxin, a mucosal Th17 cell-dependent adjuvant, was correlated with daily <span class="hlt">variations</span> in the proportion of Th17 cells in the small intestine. These results suggest that the proportion of Th17 cells in the small intestine exhibits a day-night <span class="hlt">variation</span> in association with CCL20 expression, which depends on circadian clock activity. The findings provide novel insight into the regulation of the Th17 cell population in the small intestine at steady state, which may have translational potential for mucosal vaccination strategies. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29155802','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29155802"><span>Investigation of common, low-<span class="hlt">frequency</span> and rare genome-wide <span class="hlt">variation</span> in anorexia nervosa.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huckins, L M; Hatzikotoulas, K; Southam, L; Thornton, L M; Steinberg, J; Aguilera-McKay, F; Treasure, J; Schmidt, U; Gunasinghe, C; Romero, A; Curtis, C; Rhodes, D; Moens, J; Kalsi, G; Dempster, D; Leung, R; Keohane, A; Burghardt, R; Ehrlich, S; Hebebrand, J; Hinney, A; Ludolph, A; Walton, E; Deloukas, P; Hofman, A; Palotie, A; Palta, P; van Rooij, F J A; Stirrups, K; Adan, R; Boni, C; Cone, R; Dedoussis, G; van Furth, E; Gonidakis, F; Gorwood, P; Hudson, J; Kaprio, J; Kas, M; Keski-Rahonen, A; Kiezebrink, K; Knudsen, G-P; Slof-Op 't Landt, M C T; Maj, M; Monteleone, A M; Monteleone, P; Raevuori, A H; Reichborn-Kjennerud, T; Tozzi, F; Tsitsika, A; van Elburg, A; Collier, D A; Sullivan, P F; Breen, G; Bulik, C M; Zeggini, E</p> <p>2018-05-01</p> <p>Anorexia nervosa (AN) is a complex neuropsychiatric disorder presenting with dangerously low body weight, and a deep and persistent fear of gaining weight. To date, only one genome-wide significant locus associated with AN has been identified. We performed an exome-chip based genome-wide association studies (GWAS) in 2158 cases from nine populations of European origin and 15 485 ancestrally matched controls. Unlike previous studies, this GWAS also probed association in low-<span class="hlt">frequency</span> and rare variants. Sixteen independent variants were taken forward for in silico and de novo replication (11 common and 5 rare). No findings reached genome-wide significance. Two notable common variants were identified: rs10791286, an intronic variant in OPCML (P=9.89 × 10 -6 ), and rs7700147, an intergenic variant (P=2.93 × 10 -5 ). No low-<span class="hlt">frequency</span> variant associations were identified at genome-wide significance, although the study was well-powered to detect low-<span class="hlt">frequency</span> variants with large effect sizes, suggesting that there may be no AN loci in this genomic search space with large effect sizes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5828108','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5828108"><span>Investigation of common, low-<span class="hlt">frequency</span> and rare genome-wide <span class="hlt">variation</span> in anorexia nervosa</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huckins, L M; Hatzikotoulas, K; Southam, L; Thornton, L M; Steinberg, J; Aguilera-McKay, F; Treasure, J; Schmidt, U; Gunasinghe, C; Romero, A; Curtis, C; Rhodes, D; Moens, J; Kalsi, G; Dempster, D; Leung, R; Keohane, A; Burghardt, R; Ehrlich, S; Hebebrand, J; Hinney, A; Ludolph, A; Walton, E; Deloukas, P; Hofman, A; Palotie, A; Palta, P; van Rooij, F J A; Stirrups, K; Adan, R; Boni, C; Cone, R; Dedoussis, G; van Furth, E; Gonidakis, F; Gorwood, P; Hudson, J; Kaprio, J; Kas, M; Keski-Rahonen, A; Kiezebrink, K; Knudsen, G-P; Slof-Op 't Landt, M C T; Maj, M; Monteleone, A M; Monteleone, P; Raevuori, A H; Reichborn-Kjennerud, T; Tozzi, F; Tsitsika, A; van Elburg, A; Adan, R A H; Alfredsson, L; Ando, T; Andreassen, O A; Aschauer, H; Baker, J H; Barrett, J C; Bencko, V; Bergen, A W; Berrettini, W H; Birgegard, A; Boni, C; Boraska Perica, V; Brandt, H; Breen, G; Bulik, C M; Carlberg, L; Cassina, M; Cichon, S; Clementi, M; Cohen-Woods, S; Coleman, J; Cone, R D; Courtet, P; Crawford, S; Crow, S; Crowley, J; Danner, U N; Davis, O S P; de Zwaan, M; Dedoussis, G; Degortes, D; DeSocio, J E; Dick, D M; Dikeos, D; Dina, C; Ding, B; Dmitrzak-Weglarz, M; Docampo, E; Duncan, L; Egberts, K; Ehrlich, S; Escaramís, G; Esko, T; Espeseth, T; Estivill, X; Favaro, A; Fernández-Aranda, F; Fichter, M M; Finan, C; Fischer, K; Floyd, J A B; Foretova, L; Forzan, M; Franklin, C S; Gallinger, S; Gambaro, G; Gaspar, H A; Giegling, I; Gonidakis, F; Gorwood, P; Gratacos, M; Guillaume, S; Guo, Y; Hakonarson, H; Halmi, K A; Hatzikotoulas, K; Hauser, J; Hebebrand, J; Helder, S; Herms, S; Herpertz-Dahlmann, B; Herzog, W; Hilliard, C E; Hinney, A; Hübel, C; Huckins, L M; Hudson, J I; Huemer, J; Inoko, H; Janout, V; Jiménez-Murcia, S; Johnson, C; Julià, A; Juréus, A; Kalsi, G; Kaminska, D; Kaplan, A S; Kaprio, J; Karhunen, L; Karwautz, A; Kas, M J H; Kaye, W; Kennedy, J L; Keski-Rahkonen, A; Kiezebrink, K; Klareskog, L; Klump, K L; Knudsen, G P S; Koeleman, B P C; Koubek, D; La Via, M C; Landén, M; Le Hellard, S; Levitan, R D; Li, D; Lichtenstein, P; Lilenfeld, L; Lissowska, J; Lundervold, A; Magistretti, P; Maj, M; Mannik, K; Marsal, S; Martin, N; Mattingsdal, M; McDevitt, S; McGuffin, P; Merl, E; Metspalu, A; Meulenbelt, I; Micali, N; Mitchell, J; Mitchell, K; Monteleone, P; Monteleone, A M; Mortensen, P; Munn-Chernoff, M A; Navratilova, M; Nilsson, I; Norring, C; Ntalla, I; Ophoff, R A; O'Toole, J K; Palotie, A; Pante, J; Papezova, H; Pinto, D; Rabionet, R; Raevuori, A; Rajewski, A; Ramoz, N; Rayner, N W; Reichborn-Kjennerud, T; Ripatti, S; Roberts, M; Rotondo, A; Rujescu, D; Rybakowski, F; Santonastaso, P; Scherag, A; Scherer, S W; Schmidt, U; Schork, N J; Schosser, A; Slachtova, L; Sladek, R; Slagboom, P E; Slof-Op 't Landt, M C T; Slopien, A; Soranzo, N; Southam, L; Steen, V M; Strengman, E; Strober, M; Sullivan, P F; Szatkiewicz, J P; Szeszenia-Dabrowska, N; Tachmazidou, I; Tenconi, E; Thornton, L M; Tortorella, A; Tozzi, F; Treasure, J; Tsitsika, A; Tziouvas, K; van Elburg, A A; van Furth, E F; Wagner, G; Walton, E; Watson, H; Wichmann, H-E; Widen, E; Woodside, D B; Yanovski, J; Yao, S; Yilmaz, Z; Zeggini, E; Zerwas, S; Zipfel, S; Collier, D A; Sullivan, P F; Breen, G; Bulik, C M; Zeggini, E</p> <p>2018-01-01</p> <p>Anorexia nervosa (AN) is a complex neuropsychiatric disorder presenting with dangerously low body weight, and a deep and persistent fear of gaining weight. To date, only one genome-wide significant locus associated with AN has been identified. We performed an exome-chip based genome-wide association studies (GWAS) in 2158 cases from nine populations of European origin and 15 485 ancestrally matched controls. Unlike previous studies, this GWAS also probed association in low-<span class="hlt">frequency</span> and rare variants. Sixteen independent variants were taken forward for in silico and de novo replication (11 common and 5 rare). No findings reached genome-wide significance. Two notable common variants were identified: rs10791286, an intronic variant in OPCML (P=9.89 × 10−6), and rs7700147, an intergenic variant (P=2.93 × 10−5). No low-<span class="hlt">frequency</span> variant associations were identified at genome-wide significance, although the study was well-powered to detect low-<span class="hlt">frequency</span> variants with large effect sizes, suggesting that there may be no AN loci in this genomic search space with large effect sizes. PMID:29155802</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AdSpR..58..326G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AdSpR..58..326G"><span>Modeling the <span class="hlt">variations</span> of reflection coefficient of Earth's lower ionosphere using very low <span class="hlt">frequency</span> radio wave data by artificial neural network</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghanbari, Keyvan; Khakian Ghomi, Mehdi; Mohammadi, Mohammad; Marbouti, Marjan; Tan, Le Minh</p> <p>2016-08-01</p> <p>The ionized atmosphere lying from 50 to 600 km above surface, known as ionosphere, contains high amount of electrons and ions. Very Low <span class="hlt">Frequency</span> (VLF) radio waves with <span class="hlt">frequencies</span> between 3 and 30 kHz are reflected from the lower ionosphere specifically D-region. A lot of applications in long range communications and navigation systems have been inspired by this characteristic of ionosphere. There are several factors which affect the ionization rate in this region, such as: time of day (presence of sun in the sky), solar zenith angle (seasons) and solar activities. Due to nonlinear response of ionospheric reflection coefficient to these factors, finding an accurate relation between these parameters and reflection coefficient is an arduous task. In order to model these kinds of nonlinear functionalities, some numerical methods are employed. One of these methods is artificial neural network (ANN). In this paper, the VLF radio wave data of 4 sudden ionospheric disturbance (SID) stations are given to a multi-layer perceptron ANN in order to simulate the <span class="hlt">variations</span> of reflection coefficient of D region ionosphere. After training, validation and testing the ANN, outputs of ANN and observed values are plotted together for 2 random cases of each station. By evaluating the results using 2 parameters of pearson correlation coefficient and root mean square error, a satisfying agreement was found between ANN outputs and real observed data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17028940','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17028940"><span>Spatial <span class="hlt">variation</span> in colour morph, spotting and allozyme <span class="hlt">frequencies</span> in the candy-stripe spider, Enoplognatha ovata (Theridiidae) on two Swedish archipelagos.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Oxford, G S; Gunnarsson, B</p> <p>2006-01-01</p> <p>The selective significance, if any, of many invertebrate visible polymorphisms is still not fully understood. Here we examine colour- and black spotting-morph <span class="hlt">frequencies</span> in the spider Enoplognatha ovata in populations on two Swedish archipelagos with respect to different spatial scales and, in one archipelago, against the background of <span class="hlt">variation</span> at four putative neutral allozyme marker loci. Every population studied was polymorphic for colour and 28 out of 30 contained all three colour morphs--lineata, redimita and ovata. We found no evidence for a breakdown in the traditional colour morph designation previously suggested for other northern European populations of this species. For colour there is no significant heterogeneity at spatial scales greater than between local populations within islands. Black spotting <span class="hlt">frequencies</span> show a similar lack of pattern over larger spatial scales except that there are significant differences between the Stockholm and Göteborg archipelagos. Measures of population differentiation (theta) within the Stockholm islands for the two visible systems show them to be significantly more differentiated than the neutral markers, suggesting local selection acting on them in a population-specific manner. On the basis of previous observations and the distribution of spotting phenotypes on a European scale, it is argued that thermal selection might operate on black spotting during the juvenile stages favouring more spots in continental climates. It is not clear what selective forces act on colour.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JTurb..18..338F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JTurb..18..338F"><span>Optimal <span class="hlt">frequency</span>-response sensitivity of compressible flow over roughness elements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fosas de Pando, Miguel; Schmid, Peter J.</p> <p>2017-04-01</p> <p>Compressible flow over a flat plate with two localised and well-<span class="hlt">separated</span> roughness elements is analysed by global <span class="hlt">frequency</span>-response analysis. This analysis reveals a sustained feedback loop consisting of a convectively unstable shear-layer instability, triggered at the upstream roughness, and an upstream-propagating acoustic wave, originating at the downstream roughness and regenerating the shear-layer instability at the upstream protrusion. A typical multi-peaked <span class="hlt">frequency</span> response is recovered from the numerical simulations. In addition, the optimal forcing and response clearly extract the components of this feedback loop and isolate flow regions of pronounced sensitivity and amplification. An efficient parametric-sensitivity framework is introduced and applied to the reference case which shows that first-order increases in Reynolds number and roughness height act destabilising on the flow, while changes in Mach number or roughness <span class="hlt">separation</span> cause corresponding shifts in the peak <span class="hlt">frequencies</span>. This information is gained with negligible effort beyond the reference case and can easily be applied to more complex flows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5482750','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5482750"><span>Long short-term memory for speaker generalization in supervised speech <span class="hlt">separation</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>Chen, Jitong; Wang, DeLiang</p> <p>2017-01-01</p> <p>Speech <span class="hlt">separation</span> can be formulated as learning to estimate a time-<span class="hlt">frequency</span> mask from acoustic features extracted from noisy speech. For supervised speech <span class="hlt">separation</span>, generalization to unseen noises and unseen speakers is a critical issue. Although deep neural networks (DNNs) have been successful in noise-independent speech <span class="hlt">separation</span>, DNNs are limited in modeling a large number of speakers. To improve speaker generalization, a <span class="hlt">separation</span> model based on long short-term memory (LSTM) is proposed, which naturally accounts for temporal dynamics of speech. Systematic evaluation shows that the proposed model substantially outperforms a DNN-based model on unseen speakers and unseen noises in terms of objective speech intelligibility. Analyzing LSTM internal representations reveals that LSTM captures long-term speech contexts. It is also found that the LSTM model is more advantageous for low-latency speech <span class="hlt">separation</span> and it, without future frames, performs better than the DNN model with future frames. The proposed model represents an effective approach for speaker- and noise-independent speech <span class="hlt">separation</span>. PMID:28679261</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980213315','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980213315"><span>Investigation of Turbulent Boundary-Layer <span class="hlt">Separation</span> Using Laser Velocimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Modarress, D.; Johnson, D. A.</p> <p>1979-01-01</p> <p>Boundary-layer measurements realized by laser velocimetry are presented for a Much 2.9, two-dimensional, shock-wave/turbulent boundary-layer interaction containing an extensive region of <span class="hlt">separated</span> flow. Mean velocity and turbulent intensity profiles were obtained from upstream of the interaction zone to downstream of the mean reattachment point. The superiority of the laser velocimeter technique over pressure sensors in turbulent <span class="hlt">separated</span> flows is demonstrated by a comparison of the laser velocimeter data with results obtained from local pilot and static pressure measurements for the same flow conditions. The locations of the mean <span class="hlt">separation</span> and reattachment points as deduced from the mean velocity measurements are compared to oil-now visualization results. Representative velocity probability density functions obtained in the <span class="hlt">separated</span> now region are also presented. Critical to the success of this investigation were: the use of Bragg cell <span class="hlt">frequency</span> shifting and artificial seeding of the now with submicron light-scattering particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S22A..05G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S22A..05G"><span>Impact of Ocean Wave Climate on Double-<span class="hlt">Frequency</span> Microseisms and Evaluation of Seismic Site Effect in Northern Mississippi, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Z.; Aydin, A.; Xue, M.</p> <p>2017-12-01</p> <p>This research presents the power spectral density (PSD) of double-<span class="hlt">frequency</span> (DF) microseisms in both vertical (V) and resultant horizontal (H) directions and horizontal-to-vertical spectral ratios (HVSR) of 13 continuous single point long-term ambient noise recordings (LTR) at 5 inland and 2 coastal locations selected in Mississippi Embayment, and <span class="hlt">frequency</span> value and PSD at DF peak (PSD@DF), predominant <span class="hlt">frequency</span> (f0) and HVSR value at f0 (HVSR@f0) at 234 single point short-term ambient noise recordings (STR) over a large range of unconsolidated sediment thickness (UST) in Northern Mississippi. By correlating PSD of LTRs with the simultaneous ocean wave climate data of Atlantic Ocean and Gulf of Mexico, DF microseisms observed in Northern Mississippi were shown to be shaped by a combined impact of wave climates of both Atlantic Ocean and Gulf of Mexico. Polarization analysis conducted <span class="hlt">separately</span> for LTRs and STRs strengthen this conclusion. The LTRs show stable estimates of f0, on the other hand, time-dependent <span class="hlt">variations</span> on HVSR@f0 value. The plots of DFH-UST, rather than DFV-UST, coincide well with plots of f0-UST within area where UST is larger than 300 m, which indicates that the shear wave resonance in thick sediments modifies the DF microseisms more obviously in horizontal direction than in vertical direction. Transfer functions between HVSR@f0 and ocean data indicates that the <span class="hlt">variation</span> of HVSR@f0 is caused by <span class="hlt">variations</span> of source location and energy level of DF microseisms, i.e. ocean wave activities in Atlantic Ocean and Gulf of Mexico. Additionally, 3D microseism spectra of each LTR and those of all STRs within each 100 m-UST group are converted into spatial spectral vectors and projected on stereographic nets. Patterns of the clusters formed by these projections show that the HVSR@f0 values are related to both UST and vibration source location and energy level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23852630','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23852630"><span>A <span class="hlt">frequency</span> control method for regulating wireless power to implantable devices.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ping Si; Hu, A P; Malpas, S; Budgett, D</p> <p>2008-03-01</p> <p>This paper presents a method to regulate the power transferred over a wireless link by adjusting the resonant operating <span class="hlt">frequency</span> of the primary converter. A significant advantage of this method is that effective power regulation is maintained under <span class="hlt">variations</span> in load, coupling and circuit parameters. This is particularly important when the wireless supply is used to power implanted medical devices where substantial coupling <span class="hlt">variations</span> between internal and external systems is expected. The operating <span class="hlt">frequency</span> is changed dynamically by altering the effective tuning capacitance through soft switched phase control. A thorough analysis of the proposed system has been undertaken, and experimental results verify its functionality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JASS...23..199C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JASS...23..199C"><span>Time/<span class="hlt">Frequency</span> Analysis of Terrestrial Impack Crater Records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Heon-Young</p> <p>2006-09-01</p> <p>The terrestrial impact cratering record recently has been examined in the time domain by Chang & Moon (2005). It was found that the ˜ 26 Myr periodicity in the impact cratering rate exists over the last ˜ 250 Myrs. Such a periodicity can be found regardless of the lower limit of the diameter up to D ˜ 35 km. It immediately called pros and cons. The aim of this paper is two-fold: (1) to test if reported periodicities can be obtained with an independent method, (2) to see, as attempted earlier, if the phase is modulated. To achieve these goals we employ the time/<span class="hlt">frequency</span> analysis and for the first time apply this method to the terrestrial impact cratering records. We have confirmed that without exceptions noticeable peaks appear around ˜ 25 Myr, corresponding to a <span class="hlt">frequency</span> of ˜ 0.04 (Myr)^{-1}. We also find periodicities in the data base including small impact craters, which are longer. Though the time/<span class="hlt">frequency</span> analysis allows us to observe directly phase <span class="hlt">variations</span>, we cannot find any indications of such changes. Instead, modes display slow <span class="hlt">variations</span> of power in time. The time/<span class="hlt">frequency</span> analysis shows a nonstationary behavior of the modes. The power can grow from just above the noise level and then decrease back to its initial level in a time of order of 10 Myrs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RScI...89e3704B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RScI...89e3704B"><span>Total <span class="hlt">variation</span>-based neutron computed tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barnard, Richard C.; Bilheux, Hassina; Toops, Todd; Nafziger, Eric; Finney, Charles; Splitter, Derek; Archibald, Rick</p> <p>2018-05-01</p> <p>We perform the neutron computed tomography reconstruction problem via an inverse problem formulation with a total <span class="hlt">variation</span> penalty. In the case of highly under-resolved angular measurements, the total <span class="hlt">variation</span> penalty suppresses high-<span class="hlt">frequency</span> artifacts which appear in filtered back projections. In order to efficiently compute solutions for this problem, we implement a <span class="hlt">variation</span> of the split Bregman algorithm; due to the error-forgetting nature of the algorithm, the computational cost of updating can be significantly reduced via very inexact approximate linear solvers. We present the effectiveness of the algorithm in the significantly low-angular sampling case using synthetic test problems as well as data obtained from a high flux neutron source. The algorithm removes artifacts and can even roughly capture small features when an extremely low number of angles are used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...611A..84S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...611A..84S"><span><span class="hlt">Frequency</span> dependence of p-mode <span class="hlt">frequency</span> shifts induced by magnetic activity in Kepler solar-like stars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salabert, D.; Régulo, C.; Pérez Hernández, F.; García, R. A.</p> <p>2018-04-01</p> <p>The <span class="hlt">variations</span> of the <span class="hlt">frequencies</span> of the low-degree acoustic oscillations in the Sun induced by magnetic activity show a dependence on radial order. The <span class="hlt">frequency</span> shifts are observed to increase towards higher-order modes to reach a maximum of about 0.8 μHz over the 11-yr solar cycle. A comparable <span class="hlt">frequency</span> dependence is also measured in two other main sequence solar-like stars, the F-star HD 49933, and the young 1 Gyr-old solar analog KIC 10644253, although with different amplitudes of the shifts of about 2 μHz and 0.5 μHz, respectively. Our objective here is to extend this analysis to stars with different masses, metallicities, and evolutionary stages. From an initial set of 87 Kepler solar-like oscillating stars with known individual p-mode <span class="hlt">frequencies</span>, we identify five stars showing <span class="hlt">frequency</span> shifts that can be considered reliable using selection criteria based on Monte Carlo simulations and on the photospheric magnetic activity proxy Sph. The <span class="hlt">frequency</span> dependence of the <span class="hlt">frequency</span> shifts of four of these stars could be measured for the l = 0 and l = 1 modes individually. Given the quality of the data, the results could indicate that a physical source of perturbation different from that in the Sun is dominating in this sample of solar-like stars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26337610','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26337610"><span>Do key dimensions of seed and seedling functional trait <span class="hlt">variation</span> capture <span class="hlt">variation</span> in recruitment probability?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Larson, Julie E; Sheley, Roger L; Hardegree, Stuart P; Doescher, Paul S; James, Jeremy J</p> <p>2016-05-01</p> <p>Seedling recruitment is a critical driver of population dynamics and community assembly, yet we know little about functional traits that define different recruitment strategies. For the first time, we examined whether trait relatedness across germination and seedling stages allows the identification of general recruitment strategies which share core functional attributes and also correspond to recruitment outcomes in applied settings. We measured six seed and eight seedling traits (lab- and field-collected, respectively) for 47 varieties of dryland grasses and used principal component analysis (PCA) and cluster analysis to identify major dimensions of trait <span class="hlt">variation</span> and to isolate trait-based recruitment groups, respectively. PCA highlighted some links between seed and seedling traits, suggesting that relative growth rate and root elongation rate are simultaneously but independently associated with seed mass and initial root mass (first axis), and with leaf dry matter content, specific leaf area, coleoptile tissue density and germination rate (second axis). Third and fourth axes captured <span class="hlt">separate</span> tradeoffs between hydrothermal time and base water potential for germination, and between specific root length and root mass ratio, respectively. Cluster analysis <span class="hlt">separated</span> six recruitment types along dimensions of germination and growth rates, but classifications did not correspond to patterns of germination, emergence or recruitment in the field under either of two watering treatments. Thus, while we have begun to identify major threads of functional <span class="hlt">variation</span> across seed and seedling stages, our understanding of how this <span class="hlt">variation</span> influences demographic processes-particularly germination and emergence-remains a key gap in functional ecology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24481431','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24481431"><span>[A 35-year report of the study of group on gastrointestinal cancer in Mexico City: <span class="hlt">variations</span> in <span class="hlt">frequency</span> of different digestive tract neoplasms among different socioeconomic statuses].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Villalobos Pérez, José Jesús; Bourlon, María T; Loaeza Del Castillo, Aurora; Torres Villalobos, Gonzalo</p> <p>2014-01-01</p> <p>Since the middle of the last century, North America and occidental countries have reported <span class="hlt">variations</span> in the <span class="hlt">frequency</span> of gastrointestinal neoplasms. Several environmental factors, mainly nutritional and dietary exposure, as well as habits have contributed to these changes. We have documented these changes in Mexico during the last 35 years. To define the epidemiologic changes of gastrointestinal neoplasms during the last three decades in our population. We summarized the evidence of an observational study, registering the <span class="hlt">frequency</span> of different gastrointestinal malignancies from four institutions of socioeconomically different populations in Mexico City during 35 years. The Mexican National Academy of Medicine supported this effort. During this period, two nutritional surveys took place, letting us define the relationship between dietary changes and cancer occurrence. Replacement of gastric cancer by colorectal cancer as the leading gastrointestinal malignancy. Relationship between cancer and diet changes. Increase of esophageal adenocarcinoma in relation to epidermoid carcinoma secondary to gastroesophageal reflux and Barrett's esophagus rising incidence. Gall bladder cancer had a high <span class="hlt">frequency</span> in one institution, probably related to genetic and racial factors. This epidemiologic data should lead us to implement sanitary measures for the prevention, early diagnosis, and appropriate treatment of gastrointestinal neoplasms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......109Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......109Y"><span>Boundary layer and <span class="hlt">separation</span> control on wings at low Reynolds numbers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Shanling</p> <p></p> <p>Results on boundary layer and <span class="hlt">separation</span> control through acoustic excitation at low Re numbers are reported. The Eppler 387 profile is specifically chosen because of its pre-stall hysteresis and bi-stable state behavior in the transitional Re regime, which is a result of flow <span class="hlt">separation</span> and reattachment. External acoustic forcing on the wing yields large improvements (more than 70%) in lift-to-drag ratio and flow reattachment at forcing <span class="hlt">frequencies</span> that correlate with the measured anti-resonances in the wind tunnel. The optimum St/Re1/2 range for Re = 60,000 matches the proposed optimum range in the literature, but there is less agreement for Re = 40,000, which suggests that correct St scaling has not been determined. The correlation of aerodynamic improvements to wind tunnel resonances implies that external acoustic forcing is facility-dependent, which inhibits practical application. Therefore, internal acoustic excitation for the same wing profile is also pursued. Internal acoustic forcing is designed to be accomplished by embedding small speakers inside a custom-designed wing that contains many internal cavities and small holes in the suction surface. However, initial testing of this semi-porous wing model shows that the presence of the small holes in the suction surface completely transforms the aerodynamic performance by changing the mean chordwise <span class="hlt">separation</span> location and causing an originally <span class="hlt">separated</span>, low-lift state flow to reattach into a high-lift state. The aerodynamic improvements are not caused by the geometry of the small holes themselves, but rather by Helmholtz resonance that occurs in the cavities, which generate tones that closely match the intrinsic flow instabilities. Essentially, opening and closing holes in the suction surface of a wing, perhaps by digital control, can be used as a means of passive <span class="hlt">separation</span> control. Given the similarity of wing-embedded pressure tap systems to Helmholtz resonators, particular attention must be given to the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22408237-injection-locking-two-mode-electron-oscillator-close-frequencies','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22408237-injection-locking-two-mode-electron-oscillator-close-frequencies"><span>Injection locking of a two-mode electron oscillator with close <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>Starodubova, E. N.; Usacheva, S. A.; Ryskin, N. M.</p> <p>2015-03-15</p> <p>Theory of injection locking is developed for a two-mode electron maser with close <span class="hlt">frequencies</span>, when the driving signal affects both modes. There exist two regimes of phase locking in which either first or second mode dominates. Hard transitions between the two regimes are observed with <span class="hlt">variation</span> of the driving <span class="hlt">frequency</span>. The results of numerical simulations are presented for the case of driving by a signal with linear <span class="hlt">frequency</span> chirp, as well as by a signal with sinusoidal <span class="hlt">frequency</span> modulation. The effect of bifurcation delay is observed with the increase of chirp rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29604668','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29604668"><span>Active room compensation for sound reinforcement using sound field <span class="hlt">separation</span> techniques.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Heuchel, Franz M; Fernandez-Grande, Efren; Agerkvist, Finn T; Shabalina, Elena</p> <p>2018-03-01</p> <p>This work investigates how the sound field created by a sound reinforcement system can be controlled at low <span class="hlt">frequencies</span>. An indoor control method is proposed which actively absorbs the sound incident on a reflecting boundary using an array of secondary sources. The sound field is <span class="hlt">separated</span> into incident and reflected components by a microphone array close to the secondary sources, enabling the minimization of reflected components by means of optimal signals for the secondary sources. The method is purely feed-forward and assumes constant room conditions. Three different sound field <span class="hlt">separation</span> techniques for the modeling of the reflections are investigated based on plane wave decomposition, equivalent sources, and the Spatial Fourier transform. Simulations and an experimental validation are presented, showing that the control method performs similarly well at enhancing low <span class="hlt">frequency</span> responses with the three sound <span class="hlt">separation</span> techniques. Resonances in the entire room are reduced, although the microphone array and secondary sources are confined to a small region close to the reflecting wall. Unlike previous control methods based on the creation of a plane wave sound field, the investigated method works in arbitrary room geometries and primary source positions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFD.R5007H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFD.R5007H"><span>Characterization of the low-<span class="hlt">frequency</span> unsteadines in LES data of supersonic and hypersonic STBLI</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Helm, Clara; Martin, Pino</p> <p>2016-11-01</p> <p>In a recent study, Priebe et al. (JFM 2016) used Dynamic Mode Decomposition (DMD) to analyze DNS data of a Mach 3 ramp-generated shock and turbulent boundary layer interaction (STBLI). The authors found that the reconstructed low-<span class="hlt">frequency</span> DMD modes took on the form of Görtler-like vortices downstream of <span class="hlt">separation</span>. The five reconstructed modes reproduced the low-<span class="hlt">frequency</span> dynamics of the <span class="hlt">separation</span> bubble accurately. Martín et al. (AIAA2016-3341) and Martín et al. (APS, DFD 2016) show that the low-<span class="hlt">frequency</span> unsteadiness in STBLI results from an inviscid centrifugal instability similar to that found in <span class="hlt">separated</span> subsonic and laminar flows, and that the turbulence is modulated but passive to the global mode. In this work we further characterize the Görtler-like vortices using LES data of Mach 3 and Mach 7 <span class="hlt">separated</span> STBLIs. We find that the Görtler-like vortices are unsteady, and we quantify the wavelength, amplitude and the aperiodic development of these structures. This work is supported by the Air Force Office of Scientific Research under Grant AF9550-15-1-0284.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3649415','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3649415"><span><span class="hlt">Frequency</span> Noise Properties of Lasers for Interferometry in Nanometrology</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hrabina, Jan; Lazar, Josef; Holá, Miroslava; Číp, Ondřej</p> <p>2013-01-01</p> <p>In this contribution we focus on laser <span class="hlt">frequency</span> noise properties and their influence on the interferometric displacement measurements. A setup for measurement of laser <span class="hlt">frequency</span> noise is proposed and tested together with simultaneous measurement of fluctuations in displacement in the Michelson interferometer. Several laser sources, including traditional He-Ne and solid-state lasers, and their noise properties are evaluated and compared. The contribution of the laser <span class="hlt">frequency</span> noise to the displacement measurement is discussed in the context of other sources of uncertainty associated with the interferometric setup, such as, mechanics, resolution of analog-to-digital conversion, <span class="hlt">frequency</span> bandwidth of the detection chain, and <span class="hlt">variations</span> of the refractive index of air. PMID:23435049</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.3573C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.3573C"><span>Joint analysis of short-period <span class="hlt">variations</span> of ionospheric parameters in Siberia and the Far East and processes of the tropical cyclogenesis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chernigovskaya, M. A.; Kurkin, V. I.; Orlov, I. I.; Sharkov, E. A.; Pokrovskaya, I. V.</p> <p>2009-04-01</p> <p>In this work a possibility of manifestation of strong meteorological disturbances in the Earth lower atmosphere in <span class="hlt">variations</span> of ionospheric parameters in the zone remote from the disturbance source has been studied. The spectral analysis of short-period <span class="hlt">variations</span> (about ten minutes, hours) in maximum observed <span class="hlt">frequencies</span> (MOF) of one-skip signals of oblique sounding has been carried out. These <span class="hlt">variations</span> were induced by changes in the upper atmosphere parameters along the Magadan-Irkutsk oblique-incidence sounding path on the background of diurnal <span class="hlt">variations</span> in the parameter under study. Data on MOF measurements with off-duty factor approximately 5 min in equinoxes (September, March) of 2005-2007 were used. The analysis was made using the improved ISTP-developed technique of determining periodicities in time series. The increase of signal spectrum energy at certain <span class="hlt">frequencies</span> is interpreted as manifestation of traveling ionospheric disturbances (TID) associated with propagation of internal gravity waves in the atmosphere. The analysis revealed TIDs of temporal scales under consideration. The question concerning localization of possible sources of revealed disturbances is discussed. Troposphere meteorological disturbances giant in their energy (tropical cyclones, typhoon) are considered as potential sources of observable TIDs. The needed information on tropical cyclones that occurred in the north area of the Indian Ocean, south-west and central areas of the Pacific Ocean in 2005-2007 is taken from the electron base of satellite data on the global tropical cyclogenesis "Global-TC" (ISR RAS). In order to effectively <span class="hlt">separate</span> disturbances associated with the magnetospheric-ionospheric interaction and disturbances induced by the lower atmosphere influence on the upper atmosphere, we analyze the tropical cyclogenesis events that occurred in quiet helio-geomagnetic conditions. The study was supported by the Program of RAS Presidium N 16 (Part 3) and the RFBR Grant N 08-05-00658.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApJ...853..161C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApJ...853..161C"><span><span class="hlt">Frequency</span> Dependence of Helioseismic Measurements of the Center-to-Limb Effect and Flow-induced Travel-time Shifts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Ruizhu; Zhao, Junwei</p> <p>2018-02-01</p> <p>Time–distance helioseismology measures acoustic travel times to infer the structure and flow field of the solar interior; however, both the mean travel times and the travel-time shifts suffer systematic center-to-limb <span class="hlt">variations</span>, which complicate the interpretation and inversions of the time–distance measurements. In particular, the center-to-limb <span class="hlt">variation</span> in travel-time shifts (CtoL effect) has a significant impact on the inference of the Sun’s meridional circulation, and needs to be removed from the helioseismic measurements, although the observational properties and the physical cause of the CtoL effect have yet to be investigated. In this study, we measure the CtoL effect in the <span class="hlt">frequency</span> domain using Doppler-velocity data from the Solar Dynamics Observatory/Helioseismic and Magnetic Imager, and study its properties as a function of disk-centric distance, travel distance, and <span class="hlt">frequency</span> of acoustic waves. It is found that the CtoL effect has a significant <span class="hlt">frequency</span> dependence—it reverses sign at a <span class="hlt">frequency</span> around 5.4 mHz and reaches maximum at around 4.0 mHz before the sign reversal. The tendency of <span class="hlt">frequency</span> dependence varies with disk-centric distance in a way that both the sign-reversal <span class="hlt">frequency</span> and the maximum-value <span class="hlt">frequency</span> decrease closer to the limb. The <span class="hlt">variation</span> tendency does not change with travel distance, but the <span class="hlt">variation</span> magnitude is approximately proportional to travel distance. For comparison, the flow-induced travel-time shifts show little <span class="hlt">frequency</span> dependence. These observational properties provide more clues on the nature of the CtoL effect, and also possibly lead to new ways of effect-removal for a more robust determination of the deep meridional flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730020190','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730020190"><span>Prediction of fluctuating pressure environments associated with plume-induced <span class="hlt">separated</span> flow fields</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Plotkin, K. J.</p> <p>1973-01-01</p> <p>The <span class="hlt">separated</span> flow environment induced by underexpanded rocket plumes during boost phase of rocket vehicles has been investigated. A simple semi-empirical model for predicting the extent of <span class="hlt">separation</span> was developed. This model offers considerable computational economy as compared to other schemes reported in the literature, and has been shown to be in good agreement with limited flight data. The unsteady pressure field in plume-induced <span class="hlt">separated</span> regions was investigated. It was found that fluctuations differed from those for a rigid flare only at low <span class="hlt">frequencies</span>. The major difference between plume-induced <span class="hlt">separation</span> and flare-induced <span class="hlt">separation</span> was shown to be an increase in shock oscillation distance for the plume case. The prediction schemes were applied to PRR shuttle launch configuration. It was found that fluctuating pressures from plume-induced <span class="hlt">separation</span> are not as severe as for other fluctuating environments at the critical flight condition of maximum dynamic pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21612658-theoretical-mode-oscillation-frequencies-rapidly-rotating-delta-scuti-star-alpha-ophiuchi','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21612658-theoretical-mode-oscillation-frequencies-rapidly-rotating-delta-scuti-star-alpha-ophiuchi"><span>THEORETICAL p-MODE OSCILLATION <span class="hlt">FREQUENCIES</span> FOR THE RAPIDLY ROTATING {delta} SCUTI STAR {alpha} OPHIUCHI</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>Deupree, Robert G., E-mail: bdeupree@ap.smu.ca</p> <p>2011-11-20</p> <p>A rotating, two-dimensional stellar model is evolved to match the approximate conditions of {alpha} Oph. Both axisymmetric and nonaxisymmetric oscillation <span class="hlt">frequencies</span> are computed for two-dimensional rotating models which approximate the properties of {alpha} Oph. These computed <span class="hlt">frequencies</span> are compared to the observed <span class="hlt">frequencies</span>. Oscillation calculations are made assuming the eigenfunction can be fitted with six Legendre polynomials, but comparison calculations with eight Legendre polynomials show the <span class="hlt">frequencies</span> agree to within about 0.26% on average. The surface horizontal shape of the eigenfunctions for the two sets of assumed number of Legendre polynomials agrees less well, but all calculations show significant departuresmore » from that of a single Legendre polynomial. It is still possible to determine the large <span class="hlt">separation</span>, although the small <span class="hlt">separation</span> is more complicated to estimate. With the addition of the nonaxisymmetric modes with |m| {<=} 4, the <span class="hlt">frequency</span> space becomes sufficiently dense that it is difficult to comment on the adequacy of the fit of the computed to the observed <span class="hlt">frequencies</span>. While the nonaxisymmetric <span class="hlt">frequency</span> mode splitting is no longer uniform, the <span class="hlt">frequency</span> difference between the <span class="hlt">frequencies</span> for positive and negative values of the same m remains 2m times the rotation rate.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010BGeo....7.2739M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010BGeo....7.2739M"><span>Investigating the effect of previous treatments on wheat biomass over multiple spatial <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>Milne, A. E.; Castellanos, M. T.; Cartagena, M. C.; Tarquis, A. M.; Lark, R. M.</p> <p>2010-09-01</p> <p>In this study we use the maximum overlap discrete packet transform (MODWPT) to investigate residual effects on wheat biomass of fertigation treatments applied to a previous crop. The wheat crop covered nine subplots from a previous experiment on melon response to fertigation. Each subplot had previously received a different level of applied nitrogen. Many factors affect wheat biomass, causing it to vary at different spatial <span class="hlt">frequencies</span>. We hypothesize that these will include residual effects from fertilizer application (at relatively low spatial <span class="hlt">frequencies</span>) and the local influence of individual plants from the previous melon crop (at high <span class="hlt">frequency</span>). To test this hypothesis we use the MODWPT to identify the dominant spatial <span class="hlt">frequencies</span> of wheat biomass <span class="hlt">variation</span>, and analyse the relationship to both the previous fertilizer application and the location of individual melon plants in the previous crop. The MODWPT is particularly appropriate for this because it allows us first to identify the key spatial <span class="hlt">frequencies</span> in the wheat biomass objectively and to analyse them, and their relationship to hypothesized driving factors without any assumptions of uniformity (stationarity) of wheat-biomass <span class="hlt">variation</span>. The results showed that the applied nitrogen dominated the wheat biomass response, and that there was a noticeable component of wheat-biomass <span class="hlt">variation</span> at the spatial <span class="hlt">frequency</span> that corresponds to the melon cropping. We expected wheat biomass to be negatively correlated with the position of melons in the previous crop, due to uptake of the applied nitrogen. The MODWPT, which allows us to detect changes in correlation between variables at different <span class="hlt">frequencies</span>, showed that such a relationship was found across part of the experiment but not uniformly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4538399','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4538399"><span>Experimental realization of spatially <span class="hlt">separated</span> entanglement with continuous variables using laser pulse trains</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhang, Yun; Okubo, Ryuhi; Hirano, Mayumi; Eto, Yujiro; Hirano, Takuya</p> <p>2015-01-01</p> <p>Spatially <span class="hlt">separated</span> entanglement is demonstrated by interfering two high-repetition squeezed pulse trains. The entanglement correlation of the quadrature amplitudes between individual pulses is interrogated. It is characterized in terms of the sufficient inseparability criterion with an optimum result of in the <span class="hlt">frequency</span> domain and in the time domain. The quantum correlation is also observed when the two measurement stations are <span class="hlt">separated</span> by a physical distance of 4.5 m, which is sufficiently large to demonstrate the space-like <span class="hlt">separation</span>, after accounting for the measurement time. PMID:26278478</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JInst...9.7003G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JInst...9.7003G"><span>Field stabilization studies for a radio <span class="hlt">frequency</span> quadrupole accelerator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gaur, R.; Kumar, V.</p> <p>2014-07-01</p> <p>The Radio <span class="hlt">Frequency</span> Quadrupole (RFQ) linear accelerator is an accelerator that efficiently focuses, bunches and accelerates a high intensity DC beam from an ion source, for various applications. Unlike other conventional RF linear accelerators, the electromagnetic mode used for its operation is not the lowest <span class="hlt">frequency</span> mode supported by the structure. In a four vane type RFQ, there are several undesired electromagnetic modes having <span class="hlt">frequency</span> close to that of the operating mode. While designing an RFQ accelerator, care must be taken to ensure that the <span class="hlt">frequencies</span> of these nearby modes are sufficiently <span class="hlt">separated</span> from the operating mode. If the undesired nearby modes have <span class="hlt">frequencies</span> close to the operating mode, the electromagnetic field pattern in the presence of geometrical errors will not be stabilized to the desired field profile, and will be perturbed by the nearby modes. This will affect the beam dynamics and reduce the beam transmission. In this paper, we present a detailed study of the electromagnetic modes supported, which is followed by calculations for implementation of suitable techniques to make the desired operating mode stable against mixing with unwanted modes for an RFQ being designed for the proposed Indian Spallation Neutron Source (ISNS) project at Raja Ramanna Centre for Advanced Technology, Indore. Resonant coupling scheme, along with dipole stabilization rods has been proposed to increase the mode <span class="hlt">separation</span>. The paper discusses the details of a generalized optimization procedure that has been used for the design of mode stabilization scheme.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoJI.208..257T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoJI.208..257T"><span>Lateral <span class="hlt">variation</span> of seismic attenuation in Sikkim Himalaya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thirunavukarasu, Ajaay; Kumar, Ajay; Mitra, Supriyo</p> <p>2017-01-01</p> <p>We use data from local earthquakes (mb ≥ 3.0) recorded by the Sikkim broad-band seismograph network to study the <span class="hlt">frequency</span>-dependent attenuation of the crust and uppermost mantle. These events have been relocated using body wave phase data from local and regional seismograms. The decay of coda amplitudes at a range of central <span class="hlt">frequencies</span> (1 to 12 Hz) has been measured for 74 earthquake-receiver pairs. These measurements are combined to estimate the <span class="hlt">frequency</span>-dependent coda Q of the form Q( f) = Q0 f η. The estimated Q0 values range from 80 to 200, with an average of 123 ± 29; and η ranges from 0.92 to 1.04, with an average of 0.98 ± 0.04. To study the lateral <span class="hlt">variation</span> of Q0 and η, we regionalized the measured Q values by combining all the earthquake-receiver path measurements through a back projection algorithm. We consider a single back-scatter model for the coda waves with elliptical sampling and parametrize the sampled area using 0.2° square grids. A nine-point spatial smoothening (similar to spatial Gaussian filter) is applied to stabilize the inversion. This is done at every <span class="hlt">frequency</span> to observe the spatial <span class="hlt">variation</span> of Q( f) and subsequently combined to obtain η <span class="hlt">variations</span>. Results of our study reveal that the Sikkim Himalaya is characterized by low Q0 (80-100) compared to the foreland basin to its south (150-200) and the Nepal Himalaya to its west (140-160). The low Q and high η in Sikkim Himalaya is attributed to extrinsic scattering attenuation from structural heterogeneity and active faults within the crust, and intrinsic attenuation due to anelasticity in the hotter lithosphere beneath the actively deforming mountain belt. Similar low Q and high η values had also been observed in northwest and Garhwal-Kumaun Himalaya.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA610255','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA610255"><span>Approximate <span class="hlt">Separability</span> of Green’s Function for High <span class="hlt">Frequency</span> Helmholtz Equations</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-09-01</p> <p>is highly <span class="hlt">separable</span> (Theorem 2.8) for two disjoint domains X,Y based on a key gradient estimate by Caccioppoli inequality . The method and result can be...bounded by (17) 1 ≥< Ĝ(·,y1), Ĝ(·,y2) >X≥ K̃−2, K̃ = C(d, λ, µ) c(d, λ, µ) [ 1 + r ρ ]d−2 . Also Caccioppoli inequality gives a L2 norm bound of the...1− 2) nhk∑ m=1 λm ≥ (1− 2)cnhk . 24 BJÖRN ENGQUIST AND HONGKAI ZHAO Hence inequalities (60) is replaced by the following: (75) nhk∑ m=1 λ2m > N</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24384081','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24384081"><span>Factors influencing individual <span class="hlt">variation</span> in perceptual directional microphone benefit.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Keidser, Gitte; Dillon, Harvey; Convery, Elizabeth; Mejia, Jorge</p> <p>2013-01-01</p> <p>Large <span class="hlt">variations</span> in perceptual directional microphone benefit, which far exceed the <span class="hlt">variation</span> expected from physical performance measures of directional microphones, have been reported in the literature. The cause for the individual <span class="hlt">variation</span> has not been systematically investigated. To determine the factors that are responsible for the individual <span class="hlt">variation</span> in reported perceptual directional benefit. A correlational study. Physical performance measures of the directional microphones obtained after they had been fitted to individuals, cognitive abilities of individuals, and measurement errors were related to perceptual directional benefit scores. Fifty-nine hearing-impaired adults with varied degrees of hearing loss participated in the study. All participants were bilaterally fitted with a Motion behind-the-ear device (500 M, 501 SX, or 501 P) from Siemens according to the National Acoustic Laboratories' non-linear prescription, version two (NAL-NL2). Using the Bamford-Kowal-Bench (BKB) sentences, the perceptual directional benefit was obtained as the difference in speech reception threshold measured in babble noise (SRTn) with the devices in directional (fixed hypercardioid) and in omnidirectional mode. The SRTn measurements were repeated three times with each microphone mode. Physical performance measures of the directional microphone included the angle of the microphone ports to loudspeaker axis, the <span class="hlt">frequency</span> range dominated by amplified sound, the in situ signal-to-noise ratio (SNR), and the in situ three-dimensional, articulation-index weighted directivity index (3D AI-DI). The cognitive tests included auditory selective attention, speed of processing, and working memory. Intraparticipant <span class="hlt">variation</span> on the repeated SRTn's and the interparticipant <span class="hlt">variation</span> on the average SRTn were used to determine the effect of measurement error. A multiple regression analysis was used to determine the effect of other factors. Measurement errors explained 52% of the <span class="hlt">variation</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6267R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6267R"><span>POD and PPP with multi-<span class="hlt">frequency</span> processing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roldán, Pedro; Navarro, Pedro; Rodríguez, Daniel; Rodríguez, Irma</p> <p>2017-04-01</p> <p>Precise Orbit Determination (POD) and Precise Point Positioning (PPP) are methods for estimating the orbits and clocks of GNSS satellites and the precise positions and clocks of user receivers. These methods are traditionally based on processing the ionosphere-free combination. With this combination, the delay introduced in the signal when passing through the ionosphere is removed, taking advantage of the dependency of this delay with the square of the <span class="hlt">frequency</span>. It is also possible to process the individual <span class="hlt">frequencies</span>, but in this case it is needed to properly model the ionospheric delay. This modelling is usually very challenging, as the electron content in the ionosphere experiences important temporal and spatial <span class="hlt">variations</span>. These two options define the two main kinds of processing: the dual-<span class="hlt">frequency</span> ionosphere-free processing, typically used in the POD and in certain applications of PPP, and the single-<span class="hlt">frequency</span> processing with estimation or modelisation of the ionosphere, mostly used in the PPP processing. In magicGNSS, a software tool developed by GMV for POD and PPP, a hybrid approach has been implemented. This approach combines observations from any number of individual <span class="hlt">frequencies</span> and any number of ionosphere-free combinations of these <span class="hlt">frequencies</span>. In such a way, the observations of ionosphere-free combination allow a better estimation of positions and orbits, while the inclusion of observations from individual <span class="hlt">frequencies</span> allows to estimate the ionospheric delay and to reduce the noise of the solution. It is also possible to include other kind of combinations, such as geometry-free combination, instead of processing individual <span class="hlt">frequencies</span>. The joint processing of all the <span class="hlt">frequencies</span> for all the constellations requires both the estimation or modelisation of ionospheric delay and the estimation of inter-<span class="hlt">frequency</span> biases. The ionospheric delay can be estimated from the single-<span class="hlt">frequency</span> or dual-<span class="hlt">frequency</span> geometry-free observations, but it is also possible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MSSP..102..346S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MSSP..102..346S"><span>Gear fault diagnosis based on the structured sparsity time-<span class="hlt">frequency</span> analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Ruobin; Yang, Zhibo; Chen, Xuefeng; Tian, Shaohua; Xie, Yong</p> <p>2018-03-01</p> <p>Over the last decade, sparse representation has become a powerful paradigm in mechanical fault diagnosis due to its excellent capability and the high flexibility for complex signal description. The structured sparsity time-<span class="hlt">frequency</span> analysis (SSTFA) is a novel signal processing method, which utilizes mixed-norm priors on time-<span class="hlt">frequency</span> coefficients to obtain a fine match for the structure of signals. In order to extract the transient feature from gear vibration signals, a gear fault diagnosis method based on SSTFA is proposed in this work. The steady modulation components and impulsive components of the defective gear vibration signals can be extracted simultaneously by choosing different time-<span class="hlt">frequency</span> neighborhood and generalized thresholding operators. Besides, the time-<span class="hlt">frequency</span> distribution with high resolution is obtained by piling different components in the same diagram. The diagnostic conclusion can be made according to the envelope spectrum of the impulsive components or by the periodicity of impulses. The effectiveness of the method is verified by numerical simulations, and the vibration signals registered from a gearbox fault simulator and a wind turbine. To validate the efficiency of the presented methodology, comparisons are made among some state-of-the-art vibration <span class="hlt">separation</span> methods and the traditional time-<span class="hlt">frequency</span> analysis methods. The comparisons show that the proposed method possesses advantages in <span class="hlt">separating</span> feature signals under strong noise and accounting for the inner time-<span class="hlt">frequency</span> structure of the gear vibration signals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28986206','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28986206"><span><span class="hlt">Frequency</span> dependent hub role of the dorsal and ventral right anterior insula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Yifeng; Zhu, Lixia; Zou, Qijun; Cui, Qian; Liao, Wei; Duan, Xujun; Biswal, Bharat; Chen, Huafu</p> <p>2018-01-15</p> <p>The right anterior insula (rAI) plays a crucial role in generating adaptive behavior by orchestrating multiple brain networks. Based on functional <span class="hlt">separation</span> findings of the insula and spectral fingerprints theory of cognitive functions, we hypothesize that the hub role of the rAI is region and <span class="hlt">frequency</span> dependent. Using the Human Connectome Project dataset and backtracking approach, we segregate the rAI into dorsal and ventral parts at <span class="hlt">frequency</span> bands from slow 6 to slow 3, indicating the <span class="hlt">frequency</span> dependent functional <span class="hlt">separation</span> of the rAI. Functional connectivity analysis shows that, within lower than 0.198 Hz <span class="hlt">frequency</span> range, the dorsal and ventral parts of rAI form a complementary system to synchronize with externally and internally-oriented networks. Moreover, the relationship between the dorsal and ventral rAIs predicts the relationship between anti-correlated networks associated with the dorsal rAI at slow 6 and slow 5, suggesting a <span class="hlt">frequency</span> dependent regulation of the rAI to brain networks. These findings could improve our understanding of the rAI by supporting the region and <span class="hlt">frequency</span> dependent function of rAI and its essential role in coordinating brain systems relevant to internal and external environments. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=face+AND+recognition&pg=6&id=EJ689073','ERIC'); return false;" href="https://eric.ed.gov/?q=face+AND+recognition&pg=6&id=EJ689073"><span>Face Recognition Is Affected by Similarity in Spatial <span class="hlt">Frequency</span> Range to a Greater Degree Than Within-Category Object Recognition</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>Collin, Charles A.; Liu, Chang Hong; Troje, Nikolaus F.; McMullen, Patricia A.; Chaudhuri, Avi</p> <p>2004-01-01</p> <p>Previous studies have suggested that face identification is more sensitive to <span class="hlt">variations</span> in spatial <span class="hlt">frequency</span> content than object recognition, but none have compared how sensitive the 2 processes are to <span class="hlt">variations</span> in spatial <span class="hlt">frequency</span> overlap (SFO). The authors tested face and object matching accuracy under varying SFO conditions. Their results…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29152026','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29152026"><span>Particle <span class="hlt">separation</span> by phase modulated 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>Simon, Gergely; Andrade, Marco A B; Reboud, Julien; Marques-Hueso, Jose; Desmulliez, Marc P Y; Cooper, Jonathan M; Riehle, Mathis O; Bernassau, Anne L</p> <p>2017-09-01</p> <p>High efficiency isolation of cells or particles from a heterogeneous mixture is a critical processing step in lab-on-a-chip devices. Acoustic techniques offer contactless and label-free manipulation, preserve viability of biological cells, and provide versatility as the applied electrical signal can be adapted to various scenarios. Conventional acoustic <span class="hlt">separation</span> methods use time-of-flight and achieve <span class="hlt">separation</span> up to distances of quarter wavelength with limited <span class="hlt">separation</span> power due to slow gradients in the force. The method proposed here allows <span class="hlt">separation</span> by half of the wavelength and can be extended by repeating the modulation pattern and can ensure maximum force acting on the particles. In this work, we propose an optimised phase modulation scheme for particle <span class="hlt">separation</span> in a surface acoustic wave microfluidic device. An expression for the acoustic radiation force arising from the interaction between acoustic waves in the fluid was derived. We demonstrated, for the first time, that the expression of the acoustic radiation force differs in surface acoustic wave and bulk devices, due to the presence of a geometric scaling factor. Two phase modulation schemes are investigated theoretically and experimentally. Theoretical findings were experimentally validated for different mixtures of polystyrene particles confirming that the method offers high selectivity. A Monte-Carlo simulation enabled us to assess performance in real situations, including the effects of particle size <span class="hlt">variation</span> and non-uniform acoustic field on sorting efficiency and purity, validating the ability to <span class="hlt">separate</span> particles with high purity and high resolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29856387','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29856387"><span>FBG wavelength demodulation based on a radio <span class="hlt">frequency</span> optical true time delay method.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jin; Zhu, Wanshan; Ma, Chenyuan; Xu, Tong</p> <p>2018-06-01</p> <p>A new fiber Bragg grating (FBG) wavelength shift demodulation method based on optical true time delay microwave phase detection is proposed. We used a microwave photonic link (MPL) to transport a radio <span class="hlt">frequency</span> (RF) signal over a dispersion compensation fiber (DCF). The wavelength shift of the FBG will cause the time delay change of the optical carrier that propagates in an optical fiber with chromatic dispersion, which will result in the <span class="hlt">variation</span> of the RF signal phase. A long DCF was adopted to enlarge the RF signal phase <span class="hlt">variation</span>. An IQ mixer was used to measure the RF phase <span class="hlt">variation</span> of the RF signal propagating in the MPL, and the wavelength shift of the FBG can be obtained by the measured RF signal phase <span class="hlt">variation</span>. The experimental results showed that the wavelength shift measurement resolution is 2 pm when the group velocity dispersion of the DCF is 79.5 ps/nm and the <span class="hlt">frequency</span> of the RF signal is 18 GHz. The demodulation time is as short as 0.1 ms. The measurement resolution can be improved simply by using a higher <span class="hlt">frequency</span> of the RF signal and a longer DCF or larger chromatic dispersion value of the DCF.</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://www.ncbi.nlm.nih.gov/pubmed/26211238','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26211238"><span>[Evoked Potential Blind Extraction Based on Fractional Lower Order Spatial Time-<span class="hlt">Frequency</span> Matrix].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Long, Junbo; Wang, Haibin; Zha, Daifeng</p> <p>2015-04-01</p> <p>The impulsive electroencephalograph (EEG) noises in evoked potential (EP) signals is very strong, usually with a heavy tail and infinite variance characteristics like the acceleration noise impact, hypoxia and etc., as shown in other special tests. The noises can be described by a stable distribution model. In this paper, Wigner-Ville distribution (WVD) and pseudo Wigner-Ville distribution (PWVD) time-<span class="hlt">frequency</span> distribution based on the fractional lower order moment are presented to be improved. We got fractional lower order WVD (FLO-WVD) and fractional lower order PWVD (FLO-PWVD) time-<span class="hlt">frequency</span> distribution which could be suitable for a stable distribution process. We also proposed the fractional lower order spatial time-<span class="hlt">frequency</span> distribution matrix (FLO-STFM) concept. Therefore, combining with time-<span class="hlt">frequency</span> underdetermined blind source <span class="hlt">separation</span> (TF-UBSS), we proposed a new fractional lower order spatial time-<span class="hlt">frequency</span> underdetermined blind source <span class="hlt">separation</span> (FLO-TF-UBSS) which can work in a stable distribution environment. We used the FLO-TF-UBSS algorithm to extract EPs. Simulations showed that the proposed method could effectively extract EPs in EEG noises, and the <span class="hlt">separated</span> EPs and EEG signals based on FLO-TF-UBSS were almost the same as the original signal, but blind <span class="hlt">separation</span> based on TF-UBSS had certain deviation. The correlation coefficient of the FLO-TF-UBSS algorithm was higher than the TF-UBSS algorithm when generalized signal-to-noise ratio (GSNR) changed from 10 dB to 30 dB and a varied from 1. 06 to 1. 94, and was approximately e- qual to 1. Hence, the proposed FLO-TF-UBSS method might be better than the TF-UBSS algorithm based on second order for extracting EP signal under an EEG noise environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JaJAP..56aAF03T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JaJAP..56aAF03T"><span>Atmospheric-pressure plasma activation and surface characterization on polyethylene membrane <span class="hlt">separator</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tseng, Yu-Chien; Li, Hsiao-Ling; Huang, Chun</p> <p>2017-01-01</p> <p>The surface hydrophilic activation of a polyethylene membrane <span class="hlt">separator</span> was achieved using an atmospheric-pressure plasma jet. The surface of the atmospheric-pressure-plasma-treated membrane <span class="hlt">separator</span> was found to be highly hydrophilic realized by adjusting the plasma power input. The <span class="hlt">variations</span> in membrane <span class="hlt">separator</span> chemical structure were confirmed by Fourier transform infrared spectroscopy and X-ray photoelectron spectroscopy. Chemical analysis showed newly formed carbonyl-containing groups and high surface concentrations of oxygen-containing species on the atmospheric-pressure-plasma-treated polymeric <span class="hlt">separator</span> surface. It also showed that surface hydrophilicity primarily increased from the polar component after atmospheric-pressure plasma treatment. The surface and pore structures of the polyethylene membrane <span class="hlt">separator</span> were examined by scanning electron microscopy, revealing a slight alteration in the pore structure. As a result of the incorporation of polar functionalities by atmospheric-pressure plasma activation, the electrolyte uptake and electrochemical impedance of the atmospheric-pressure-plasma-treated membrane <span class="hlt">separator</span> improved. The investigational results show that the <span class="hlt">separator</span> surface can be controlled by atmospheric-pressure plasma surface treatment to tailor the hydrophilicity and enhance the electrochemical performance of lithium ion batteries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18470250','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18470250"><span>Analysis of PVA/AA based photopolymers at the zero spatial <span class="hlt">frequency</span> limit using interferometric methods.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gallego, Sergi; Márquez, Andrés; Méndez, David; Ortuño, Manuel; Neipp, Cristian; Fernández, Elena; Pascual, Inmaculada; Beléndez, Augusto</p> <p>2008-05-10</p> <p>One of the problems associated with photopolymers as optical recording media is the thickness <span class="hlt">variation</span> during the recording process. Different values of shrinkages or swelling are reported in the literature for photopolymers. Furthermore, these <span class="hlt">variations</span> depend on the spatial <span class="hlt">frequencies</span> of the gratings stored in the materials. Thickness <span class="hlt">variations</span> can be measured using different methods: studying the deviation from the Bragg's angle for nonslanted gratings, using MicroXAM S/N 8038 interferometer, or by the thermomechanical analysis experiments. In a previous paper, we began the characterization of the properties of a polyvinyl alcohol/acrylamide based photopolymer at the lowest end of recorded spatial <span class="hlt">frequencies</span>. In this work, we continue analyzing the thickness <span class="hlt">variations</span> of these materials using a reflection interferometer. With this technique we are able to obtain the <span class="hlt">variations</span> of the layers refractive index and, therefore, a direct estimation of the polymer refractive index.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984JFM...144...13C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984JFM...144...13C"><span>Unsteady measurements in a <span class="hlt">separated</span> and reattaching flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cherry, N. J.; Hillier, R.; Latour, M. E. M. P.</p> <p>1984-07-01</p> <p>The investigation of the unsteady <span class="hlt">separated</span>-and-reattaching flow formed by a two-dimensional rectangular leading-edge test model with a thickness of 38.1 mm is presented. Fluctuating pressures were measured with Setra 237 transducers and velocity with hot-wire visualization was performed when test Reynolds number was held in the range 3.2 x 10000 + or - 0.2 x 10000. It is shown that throughout the <span class="hlt">separation</span> bubble a low-<span class="hlt">frequency</span> motion canbe detected. This effect is dominant in the surface-pressure fluctuations near <span class="hlt">separation</span>; lateral correlation scales of this motion are less than the reattachment length; and its timescale is about equal to the characteristic timescale for the shear layer and for the bubble to change between various shedding phases which were defined by the observations. Attention is given also to the spanwise correlations of the velocity and three-dimensional effects. Previous studies are discussed and their results are compared with those presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/3386558','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/3386558"><span>A compensation scheme for tape-speed <span class="hlt">variation</span> in cassette recorders.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wodicka, G R; Aguirre, A; Burns, S K; Shannon, D C</p> <p>1988-06-01</p> <p>A scheme to reduce the data corruption caused by tape-speed <span class="hlt">variation</span> in cassette recorders used for monitoring infant apnea was developed. Low-<span class="hlt">frequency</span> timing information is recorded on the tape, under the constraints of the <span class="hlt">frequency</span> response of the recorder, simultaneously with the other signals. This information is extracted during playback and multiplied to a <span class="hlt">frequency</span> suitable for data sampling, using an electronic, phase-locked loop. Analog-to-digital conversion of the data is performed at a rate proportional to the tape speed, resulting in compensation for speed <span class="hlt">variation</span>. No direct modification of the speed-control mechanism of the recorder is required. The scheme was evaluated by comparing interval measurements of recorded timing information with and without compensation. Compensation reduced the error of the measurement by nearly an order of magnitude, which was consistent with theoretical predictions. This allows analysis of clinical value to be performed on signals recorded by systems that lack sophisticated speed-control mechanisms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23231095','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23231095"><span>Large scale modulation of high <span class="hlt">frequency</span> acoustic waves in periodic porous media.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boutin, Claude; Rallu, Antoine; Hans, Stephane</p> <p>2012-12-01</p> <p>This paper deals with the description of the modulation at large scale of high <span class="hlt">frequency</span> acoustic waves in gas saturated periodic porous media. High <span class="hlt">frequencies</span> mean local dynamics at the pore scale and therefore absence of scale <span class="hlt">separation</span> 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 <span class="hlt">separation</span> 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 <span class="hlt">frequencies</span> 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 <span class="hlt">frequency</span> waves. The significant difference between modulations of simple and multiple mode are evidenced and discussed. The features of the modulation (anisotropy, width of <span class="hlt">frequency</span> band) are also analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29424691','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29424691"><span>Pi-Pi contacts are an overlooked protein feature relevant to phase <span class="hlt">separation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vernon, Robert McCoy; Chong, Paul Andrew; Tsang, Brian; Kim, Tae Hun; Bah, Alaji; Farber, Patrick; Lin, Hong; Forman-Kay, Julie Deborah</p> <p>2018-02-09</p> <p>Protein phase <span class="hlt">separation</span> is implicated in formation of membraneless organelles, signaling puncta and the nuclear pore. Multivalent interactions of modular binding domains and their target motifs can drive phase <span class="hlt">separation</span>. However, forces promoting the more common phase <span class="hlt">separation</span> of intrinsically disordered regions are less understood, with suggested roles for multivalent cation-pi, pi-pi, and charge interactions and the hydrophobic effect. Known phase-<span class="hlt">separating</span> proteins are enriched in pi-orbital containing residues and thus we analyzed pi-interactions in folded proteins. We found that pi-pi interactions involving non-aromatic groups are widespread, underestimated by force-fields used in structure calculations and correlated with solvation and lack of regular secondary structure, properties associated with disordered regions. We present a phase <span class="hlt">separation</span> predictive algorithm based on pi interaction <span class="hlt">frequency</span>, highlighting proteins involved in biomaterials and RNA processing. © 2018, Vernon et al.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5847340','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5847340"><span>Pi-Pi contacts are an overlooked protein feature relevant to phase <span class="hlt">separation</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>Vernon, Robert McCoy; Chong, Paul Andrew; Tsang, Brian; Kim, Tae Hun; Bah, Alaji; Farber, Patrick; Lin, Hong</p> <p>2018-01-01</p> <p>Protein phase <span class="hlt">separation</span> is implicated in formation of membraneless organelles, signaling puncta and the nuclear pore. Multivalent interactions of modular binding domains and their target motifs can drive phase <span class="hlt">separation</span>. However, forces promoting the more common phase <span class="hlt">separation</span> of intrinsically disordered regions are less understood, with suggested roles for multivalent cation-pi, pi-pi, and charge interactions and the hydrophobic effect. Known phase-<span class="hlt">separating</span> proteins are enriched in pi-orbital containing residues and thus we analyzed pi-interactions in folded proteins. We found that pi-pi interactions involving non-aromatic groups are widespread, underestimated by force-fields used in structure calculations and correlated with solvation and lack of regular secondary structure, properties associated with disordered regions. We present a phase <span class="hlt">separation</span> predictive algorithm based on pi interaction <span class="hlt">frequency</span>, highlighting proteins involved in biomaterials and RNA processing. PMID:29424691</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Ap%26SS.363....9T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Ap%26SS.363....9T"><span>Density <span class="hlt">variation</span> effect on multi-ions with kinetic Alfven wave around cusp region—a kinetic approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamrakar, Radha; Varma, P.; Tiwari, M. S.</p> <p>2018-01-01</p> <p>The kinetic Alfven waves in the presence of homogeneous magnetic field plasma with multi-ions effect are investigated. The dispersion relation and normalised damping rate are derived for low-β plasma using kinetic theory. The effect of density <span class="hlt">variation</span> of H+, He+ and O+ ions is observed on <span class="hlt">frequency</span> and damping rate of the wave. The <span class="hlt">variation</span> of <span class="hlt">frequency</span> (ω) and normalised damping rate (γ / Ω_{H^{ +}} ) of the wave are studied with respect to k_{ \\bot} ρj, where k_{ \\bot} is the perpendicular wave number, ρj is the ion gyroradius and j denotes H+, He+ and O+ ions. The <span class="hlt">variation</span> with k_{ \\bot} ρj is considered over wide range. The parameters appropriate to cusp region are used for the explanation of results. It is found that with hydrogen and helium ions gyration, the <span class="hlt">frequency</span> of wave is influenced by the density <span class="hlt">variation</span> of H+ and He+ ions but remains insensitive to the change in density of O+ ions. For oxygen ion gyration, the <span class="hlt">frequency</span> of wave varies over a short range only for O+ ion density <span class="hlt">variation</span>. The wave shows damping at lower altitude due to <span class="hlt">variation</span> in density of lighter H+ and He+ ions whereas at higher altitude only heavy O+ ions contribute in wave damping. The damping of wave may be due to landau damping or energy transfer from wave to particles. The present study signifies that the both lighter and heavier ions dominate differently to change the characteristics of kinetic Alfven wave and density <span class="hlt">variation</span> is also an important parameter to understand wave phenomena in cusp region.</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 <span class="hlt">separate</span> 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 scale, 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('https://www.ncbi.nlm.nih.gov/pubmed/15717332','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15717332"><span>High-<span class="hlt">frequency</span> health data and spline functions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martín-Rodríguez, Gloria; Murillo-Fort, Carlos</p> <p>2005-03-30</p> <p>Seasonal <span class="hlt">variations</span> are highly relevant for health service organization. In general, short run movements of medical magnitudes are important features for managers in this field to make adequate decisions. Thus, the analysis of the seasonal pattern in high-<span class="hlt">frequency</span> health data is an appealing task. The aim of this paper is to propose procedures that allow the analysis of the seasonal component in this kind of data by means of spline functions embedded into a structural model. In the proposed method, useful adaptions of the traditional spline formulation are developed, and the resulting procedures are capable of capturing periodic <span class="hlt">variations</span>, whether deterministic or stochastic, in a parsimonious way. Finally, these methodological tools are applied to a series of daily emergency service demand in order to capture simultaneous seasonal <span class="hlt">variations</span> in which periods are different.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.738...51D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.738...51D"><span>Lapse time and <span class="hlt">frequency</span>-dependent coda wave attenuation for Delhi and its surrounding regions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, Rabin; Mukhopadhyay, Sagarika; Singh, Ravi Kant; Baidya, Pushap R.</p> <p>2018-07-01</p> <p>Attenuation of seismic wave energy of Delhi and its surrounding regions has been estimated using coda of local earthquakes. Estimated quality factor (Qc) values are strongly dependent on <span class="hlt">frequency</span> and lapse time. <span class="hlt">Frequency</span> dependence of Qc has been estimated from the relationship Qc(f) = Q0fn for different lapse time window lengths. Q0 and n values vary from 73 to 453 and 0.97 to 0.63 for lapse time window lengths of 15 s to 90 s respectively. Average estimated <span class="hlt">frequency</span> dependent relation is, Qc(f) = 135 ± 8f0.96±0.02 for the entire region for a window length of 30 s, where the average Qc value varies from 200 at 1.5 Hz to 1962 at 16 Hz. These values show that the region is seismically active and highly heterogeneous. The entire study region is divided into two sub-regions according to the geology of the area to investigate if there is a spatial <span class="hlt">variation</span> in attenuation characteristics in this region. It is observed that at smaller lapse time both regions have similar Qc values. However, at larger lapse times the rate of increase of Qc with <span class="hlt">frequency</span> is larger for Region 2 compared to Region 1. This is understandable, as it is closer to the tectonically more active Himalayan ranges and seismically more active compared to Region 1. The difference in <span class="hlt">variation</span> of Qc with <span class="hlt">frequencies</span> for the two regions is such that at larger lapse time and higher <span class="hlt">frequencies</span> Region 2 shows higher Qc compared to Region 1. For lower <span class="hlt">frequencies</span> the opposite situation is true. This indicates that there is a systematic <span class="hlt">variation</span> in attenuation characteristics from the south (Region 1) to the north (Region 2) in the deeper part of the study area. This <span class="hlt">variation</span> can be explained in terms of an increase in heat flow and a decrease in the age of the rocks from south to north.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750020587','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750020587"><span>Dual <span class="hlt">frequency</span> scatterometer measurement of ocean wave height</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.; Swift, C. T.; Grantham, W. L.; Weissman, D. E.</p> <p>1975-01-01</p> <p>A technique for remotely measuring wave height averaged over an area of the sea surface was developed and verified with a series of aircraft flight experiments. The measurement concept involves the cross correlation of the amplitude fluctuations of two monochromatic reflected signals with variable <span class="hlt">frequency</span> <span class="hlt">separation</span>. The signal reflected by the randomly distributed specular points on the surface is observed in the backscatter direction at nadir incidence angle. The measured correlation coefficient is equal to the square of the magnitude of the characteristic function of the specular point height from which RMS wave height can be determined. The flight scatterometer operates at 13.9 GHz and 13.9 - delta f GHz with a maximum delta f of 40 MHz. Measurements were conducted for low and moderate sea states at altitudes of 2, 5, and 10 thousand feet. The experimental results agree with the predicted decorrelation with <span class="hlt">frequency</span> <span class="hlt">separation</span> and with off-nadir incidence angle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999ApPhL..74.3410H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999ApPhL..74.3410H"><span><span class="hlt">Separation</span> of density and viscosity influence on liquid-loaded surface acoustic wave devices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Herrmann, F.; Hahn, D.; Büttgenbach, S.</p> <p>1999-05-01</p> <p>Love-mode sensors are reported for <span class="hlt">separate</span> measurement of liquid density and viscosity. They combine the general merits of Love-mode devices, e.g., ease of sensitivity adjustment and robustness, with a highly effective procedure of <span class="hlt">separate</span> determination of liquid density and viscosity. A model is proposed to describe the <span class="hlt">frequency</span> response of the devices to liquid loading. Moreover, design rules are given for further optimization and sensitivity enhancement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940006523&hterms=applied+optics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dapplied%2Boptics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940006523&hterms=applied+optics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dapplied%2Boptics"><span>A wide-band fiber optic <span class="hlt">frequency</span> distribution system employing thermally controlled phase compensation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johnson, Dean; Calhoun, Malcolm; Sydnor, Richard; Lutes, George</p> <p>1993-01-01</p> <p>An active wide-band fiber optic <span class="hlt">frequency</span> distribution system employing a thermally controlled phase compensator to stabilize phase <span class="hlt">variations</span> induced by environmental temperature changes is described. The distribution system utilizes bidirectional dual wavelength transmission to provide optical feedback of induced phase <span class="hlt">variations</span> of 100 MHz signals propagating along the distribution cable. The phase compensation considered differs from earlier narrow-band phase compensation designs in that it uses a thermally controlled fiber delay coil rather than a VCO or phase modulation to compensate for induced phase <span class="hlt">variations</span>. Two advantages of the wide-band system over earlier designs are (1) that it provides phase compensation for all transmitted <span class="hlt">frequencies</span>, and (2) the compensation is applied after the optical interface rather than electronically ahead of it as in earlier schemes. Experimental results on the first prototype shows that the thermal stabilizer reduces phase <span class="hlt">variations</span> and Allan deviation by a factor of forty over an equivalent uncompensated fiber optic distribution system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ISPAr42.3..527H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ISPAr42.3..527H"><span>On the Influence of Global Warming on Atlantic Hurricane <span class="hlt">Frequency</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hosseini, S. R.; Scaioni, M.; Marani, M.</p> <p>2018-04-01</p> <p>In this paper, the possible connection between the <span class="hlt">frequency</span> of Atlantic hurricanes to the climate change, mainly the <span class="hlt">variation</span> in the Atlantic Ocean surface temperature has been investigated. The correlation between the observed hurricane <span class="hlt">frequency</span> for different categories of hurricane's intensity and Sea Surface Temperature (SST) has been examined over the Atlantic Tropical Cyclogenesis Regions (ACR). The results suggest that in general, the <span class="hlt">frequency</span> of hurricanes have a high correlation with SST. In particular, the <span class="hlt">frequency</span> of extreme hurricanes with Category 5 intensity has the highest correlation coefficient (R = 0.82). In overall, the analyses in this work demonstrates the influence of the climate change condition on the Atlantic hurricanes and suggest a strong correlation between the <span class="hlt">frequency</span> of extreme hurricanes and SST in the ACR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4785984','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4785984"><span>Kinship as a <span class="hlt">frequency</span> dependent strategy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ji, Ting; Zheng, Xiu-Deng; He, Qiao-Qiao; Wu, Jia-Jia; Tao, Yi</p> <p>2016-01-01</p> <p>Humans divide themselves up into <span class="hlt">separate</span> cultures, which is a unique and ubiquitous characteristic of our species. Kinship norms are one of the defining features of such societies. Here we show how norms of marital residence can evolve as a <span class="hlt">frequency</span>-dependent strategy, using real-world cases from southwestern China and an evolutionary game model. The process of kinship change has occurred in the past and is also occurring now in southwestern China. Our data and models show how transitions between residence types can occur both as response to changing costs and benefits of co-residence with kin, and also due to the initial <span class="hlt">frequency</span> of the strategies adopted by others in the population: patrilocal societies can become matrilocal, and neolocal societies can become duolocal. This illustrates how <span class="hlt">frequency</span>-dependent selection plays a role both in the maintenance of group-level cultural diversity and in cultural extinction. PMID:26998333</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5606140','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5606140"><span>High-<span class="hlt">Frequency</span> EEG <span class="hlt">Variations</span> in Children with Autism Spectrum Disorder during Human Faces Visualization</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Reategui, Camille; Costa, Bruna Karen de Sousa; da Fonseca, Caio Queiroz; da Silva, Luana; Morya, Edgard</p> <p>2017-01-01</p> <p>Autism spectrum disorder (ASD) is a neuropsychiatric disorder characterized by the impairment in the social reciprocity, interaction/language, and behavior, with stereotypes and signs of sensory function deficits. Electroencephalography (EEG) is a well-established and noninvasive tool for neurophysiological characterization and monitoring of the brain electrical activity, able to identify abnormalities related to <span class="hlt">frequency</span> range, connectivity, and lateralization of brain functions. This research aims to evidence quantitative differences in the <span class="hlt">frequency</span> spectrum pattern between EEG signals of children with and without ASD during visualization of human faces in three different expressions: neutral, happy, and angry. Quantitative clinical evaluations, neuropsychological evaluation, and EEG of children with and without ASD were analyzed paired by age and gender. The results showed stronger activation in higher <span class="hlt">frequencies</span> (above 30 Hz) in frontal, central, parietal, and occipital regions in the ASD group. This pattern of activation may correlate with developmental characteristics in the children with ASD. PMID:29018811</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3923184','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3923184"><span>Monitoring of ULF (ultra-low-<span class="hlt">frequency</span>) Geomagnetic <span class="hlt">Variations</span> Associated with Earthquakes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hayakawa, Masashi; Hattori, Katsumi; Ohta, Kenji</p> <p>2007-01-01</p> <p>ULF (ultra-low-<span class="hlt">frequency</span>) electromagnetic emission is recently recognized as one of the most promising candidates for short-term earthquake prediction. This paper reviews previous convincing evidence on the presence of ULF emissions before a few large earthquakes. Then, we present our network of ULF monitoring in the Tokyo area by describing our ULF magnetic sensors and we finally present a few, latest results on seismogenic electromagnetic emissions for recent large earthquakes with the use of sophisticated signal processings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=47949','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=47949"><span>Two motion systems with common and <span class="hlt">separate</span> pathways for color and luminance.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gorea, A; Papathomas, T V; Kovacs, I</p> <p>1993-01-01</p> <p>We present psychological experiments that reveal two motion systems, a specific and an unspecific one. The specific system prevails at medium to high temporal <span class="hlt">frequencies</span>. It comprises at least two <span class="hlt">separate</span> motion pathways that are selective for color and for luminance and that do not interact until after the motion signal is extracted <span class="hlt">separately</span> in each. By contrast, the unspecific system prevails at low temporal <span class="hlt">frequencies</span> and it combines color and luminance signals at an earlier stage, before motion extraction. The successful implementation of an efficient and accurate technique for assessing equiluminance corroborates further the main findings. These results offer a general framework for understanding the nature of interactions between color and luminance signals in motion perception and suggest that previously proposed dichotomies in motion processing may be encompassed by the specific/unspecific dichotomy proposed here. Images Fig. 2 Fig. 4 PMID:8248227</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ChOpL...1..249S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ChOpL...1..249S"><span>Strong intensity <span class="hlt">variations</span> of laser feedback interferometer caused by atmospheric turbulence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Yiyi; Li, Zhiping</p> <p>2003-05-01</p> <p>The significant <span class="hlt">variation</span> of the laser output can be caused by feedback of a small part of laser beam, which is reflected or backscattered by a target at a long distance from laser source, into the laser cavity. This paper describes and analyzes theoretically and experimentally the influence of atmospheric turbulence on interference caused by laser feedback. The influence depends upon both the energy of feedback into the laser cavity and the strength of turbulence over a laser propagation path in the atmosphere. In the case of stronger energy of feedback and weak turbulence variance of fluctuation of the laser output can be enhanced by hundreds to thousands times. From our measurements and theoretical analysis it shows thatthese significant enhancements can result from the change of laser-cavity-modes which can be stimulated simultaneously and from beat oscillations between a variety of <span class="hlt">frequencies</span> of laser modes. This also can result from optical chaos inside the laser resonator because a non-<span class="hlt">separable</span> distorted external cavity can become a prerequisite for optical chaos.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5936936','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5936936"><span>Epigenetic and genetic <span class="hlt">variation</span> among three <span class="hlt">separate</span> introductions of the house sparrow (Passer domesticus) into Australia</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Schrey, A.; Ragsdale, A.; Griffith, S. C.</p> <p>2018-01-01</p> <p>Invasive populations are often associated with low levels of genetic diversity owing to population bottlenecks at the initial stages of invasion. Despite this, the ability of invasive species to adapt rapidly in response to novel environments is well documented. Epigenetic mechanisms have recently been proposed to facilitate the success of invasive species by compensating for reduced levels of genetic <span class="hlt">variation</span>. Here, we use methylation sensitive-amplification fragment length polymorphism and microsatellite analyses to compare levels of epigenetic and genetic diversity and differentiation across 15 sites in the introduced Australian house sparrow population. We find patterns of epigenetic and genetic differentiation that are consistent with historical descriptions of three distinct, introductions events. However unlike genetic differentiation, epigenetic differentiation was higher among sample sites than among invasion clusters, suggesting that patterns of epigenetic <span class="hlt">variation</span> are more strongly influenced by local environmental stimuli or sequential founder events than the initial diversity in the introduction population. Interestingly, we fail to detect correlations between pairwise site comparisons of epigenetic and genetic differentiation, suggesting that some of the observed epigenetic <span class="hlt">variation</span> has arisen independently of genetic <span class="hlt">variation</span>. We also fail to detect the potentially compensatory relationship between epigenetic and genetic diversity that has been detected in a more recent house sparrow invasion in Africa. We discuss the potential for this relationship to be obscured by recovered genetic diversity in more established populations, and highlight the importance of incorporating introduction history into population-wide epigenetic analyses. PMID:29765671</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2552L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2552L"><span><span class="hlt">Variations</span> of the critical foE-<span class="hlt">frequency</span> of the ionosphere connected with earthquakes. Evaluation of observations of the vertical sounding station "Tokyo"</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liperovskaya, Elena V.; Meister, Claudia-Veronika; Hoffmann, Dieter H. H.; Silina, Alexandra S.</p> <p>2016-04-01</p> <p>In the present work the critical <span class="hlt">frequencies</span> foE and foF2 of the ionosphere are considered as possible earthquake precursors. The statistical analysis of the critical <span class="hlt">frequencies</span> is carried out based on the data of the vertical sounding station (VSS) "Kokubunji" ("Tokyo") (ϕ = 35.7o N, λ = 139.5o E, 1957-1988) obtained every hour. Disturbances are considered on the background of seasonal, geomagnetic as well as 11-years and 27-days Solar <span class="hlt">variations</span>. Special normalized parameters E and F are introduced, which represent the almost seasonal-independent parts of foE and foF2. Days with high Solar (Wolf number > 100) and geomagnetic (ΣKp > 25) activities are excluded from the analysis. For all data (observed every hour) analysed, no correlations of the normalized parameters E and F are found. One day before the seismic shock, a positive correlation is observed. The superimposed epochs method is used to determine the temporal behaviour of E and F. It is found that E and F decrease one day before the earthquakes provided that the seismic shocks occur at distances 600 < R < 1000 km from the VSS, and that the focus of earthquakes with magnitudes M > 5.5 is situated at depths smaller than 60 km. The reliability of the effect is larger than 98 %. Possible physical mechanisms of the phenomenon are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT.......245S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT.......245S"><span>High <span class="hlt">frequency</span> acoustic propagation under variable sea surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Senne, Joseph</p> <p></p> <p> considered, with the range-dependent model varying over the same time scales as the sea surface model and the range-independent model invariant over time. The bubble-induced sound speed and attenuation fluctuations are read in by the parabolic equation model, which allows for the effects of surface roughness and sub-surface bubbles to be computed <span class="hlt">separately</span> or together. These merged acoustic models are validated using concurrently-collected acoustic and environmental information, including surface wave spectra. Data to model comparisons demonstrate that the models are able to approximate the ensemble-averaged acoustic intensity at ranges of at least a kilometer for acoustic signals of 10-20 kHz. The rough surface model is shown to capture <span class="hlt">variations</span> due to surface fluctuations occurring over time scales of less than a second to tens of seconds. The <span class="hlt">separate</span> bubble models demonstrate the abilities to account for the intermittency of bubble plumes and to determine overall effect of bubbly layers, respectively. The models are shown to capture <span class="hlt">variations</span> in the acoustic field occurring over time scales of less than a second to tens of seconds. Comparisons against data demonstrate the ability of the model to track acoustic transmissions under evolving sea surfaces. The effects of the evolving bubble field are demonstrated through the use of idealized test cases. For <span class="hlt">frequency</span> ranges important to communications, surface roughness is shown to have the more dominant effect, with bubbles having an ancillary effect.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20133037','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20133037"><span>A new visually evoked cerebral blood flow response analysis using a low-<span class="hlt">frequency</span> estimation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rey, Beatriz; Naranjo, Valery; Parkhutik, Vera; Tembl, José; Alcañiz, Mariano</p> <p>2010-03-01</p> <p>Transcranial Doppler (TCD) has been widely used to monitor cerebral blood flow velocity (BFV) during the performance of cognitive tasks compared with repose periods. Although one of its main advantages is its high temporal resolution, only some of the previous functional TCD studies have focused on the analysis of the temporal evolution of the BFV signal and none of them has performed a spectral analysis of the signal. In this study, maximum BFV data in both posterior cerebral arteries was monitored during a visual perception task (10 cycles of alternating darkness and illumination) for 23 subjects. A peak was located in the low-<span class="hlt">frequency</span> band of the spectrum of the maximum BFV of each subject both during visual stimulation and repose periods. The <span class="hlt">frequency</span> of this peak was in the range between 0.037 and 0.098Hz, depending on the subject, the vessel and the experimental condition. The component of the signal at this <span class="hlt">frequency</span>, which is associated with the slow <span class="hlt">variations</span> caused by the visual stimuli, was estimated. That way, the <span class="hlt">variations</span> in BFV caused by the experimental stimuli were isolated from the <span class="hlt">variations</span> caused by other factors. This low-<span class="hlt">frequency</span> estimation signal was used to obtain parameters about the temporal evolution and the magnitude <span class="hlt">variations</span> of the BFV in a reliable way, thus, characterizing the neurovascular coupling of the participants. Copyright 2010 World Federation for Ultrasound in Medicine & Biology. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AcAau.121..116L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AcAau.121..116L"><span>The interference aerodynamics caused by the wing elasticity during store <span class="hlt">separation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lei, Yang; Zheng-yin, Ye</p> <p>2016-04-01</p> <p>Air-launch-to-orbit is the technology that has stores carried aloft and launched the store from the plane to the orbit. The <span class="hlt">separation</span> between the aircraft and store is one of the most important and difficult phases in air-launch-to-orbit technology. There exists strong aerodynamic interference between the aircraft and the store in store <span class="hlt">separation</span>. When the aspect ratio of the aircraft is large, the elastic deformations of the wing must be considered. The main purpose of this article is to study the influence of the interference aerodynamics caused by the elastic deformations of the wing to the unsteady aerodynamics of the store. By solving the coupled functions of unsteady Navier-Stokes equations, six degrees of freedom dynamic equations and structural dynamic equations simultaneously, the store <span class="hlt">separation</span> with the elastic deformation of the aircraft considered is simulated numerically. And the interactive aerodynamic forces are analyzed. The study shows that the interference aerodynamics is obvious at earlier time during the <span class="hlt">separation</span>, and the dominant <span class="hlt">frequency</span> of the elastic wing determines the aerodynamic forces <span class="hlt">frequencies</span> of the store. Because of the effect of the interference aerodynamics, the roll angle response and pitch angle response increase. When the store is mounted under the wingtip, the additional aerodynamics caused by the wingtip vortex is obvious, which accelerate the divergence of the lateral force and the lateral-directional attitude angle of the store. This study supports some beneficial conclusions to the engineering application of the air-launch-to-orbit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20774652-variational-method-lattice-spectroscopy-ghosts','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20774652-variational-method-lattice-spectroscopy-ghosts"><span><span class="hlt">Variational</span> method for lattice spectroscopy with ghosts</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>Burch, Tommy; Hagen, Christian; Gattringer, Christof</p> <p>2006-01-01</p> <p>We discuss the <span class="hlt">variational</span> method used in lattice spectroscopy calculations. In particular we address the role of ghost contributions which appear in quenched or partially quenched simulations and have a nonstandard euclidean time dependence. We show that the ghosts can be <span class="hlt">separated</span> from the physical states. Our result is illustrated with numerical data for the scalar meson.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19720026849&hterms=frequency+modulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dfrequency%2Bmodulation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19720026849&hterms=frequency+modulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dfrequency%2Bmodulation"><span>Basic characteristics of high-<span class="hlt">frequency</span> Stark-effect modulation of CO2 lasers.</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Claspy, P. C.; Pao, Y. H.</p> <p>1971-01-01</p> <p>The molecular Stark effect and its application to the modulation of infrared laser radiation have been investigated both theoretically and experimentally. Using a density matrix approach, a quantum mechanical description of the effect of a time-varying electric field on the absorption coefficient and refractive index of a molecular gas near an absorption line has been formulated. For modulation applications a quantity known as the ?modulation depth' is of prime importance. Theoretical expressions for the <span class="hlt">frequency</span> dependence of the modulation depth show that the response to the <span class="hlt">frequency</span> of a time-varying Stark field is <span class="hlt">separated</span> into a nondispersive and a dispersive region, depending on whether the modulating <span class="hlt">frequency</span> is less than or greater than the homogeneous absorption linewidth. Experimental results showing nondispersive modulation at <span class="hlt">frequencies</span> to 30 MHz are presented. In addition it is shown that the response of modulation depth to Stark field amplitude is <span class="hlt">separated</span> into linear and nonlinear regions, the field at which nonlinearities begin being determined by the absorption spectrum of the molecule being used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9844E..0WF','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9844E..0WF"><span>Spatial tuning of a RF <span class="hlt">frequency</span> selective surface through origami</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fuchi, Kazuko; Buskohl, Philip R.; Bazzan, Giorgio; Durstock, Michael F.; Joo, James J.; Reich, Gregory W.; Vaia, Richard A.</p> <p>2016-05-01</p> <p>Origami devices have the ability to spatially reconfigure between 2D and 3D states through folding motions. The precise mapping of origami presents a novel method to spatially tune radio <span class="hlt">frequency</span> (RF) devices, including adaptive antennas, sensors, reflectors, and <span class="hlt">frequency</span> selective surfaces (FSSs). While conventional RF FSSs are designed based upon a planar distribution of conductive elements, this leaves the large design space of the out of plane dimension underutilized. We investigated this design regime through the computational study of four FSS origami tessellations with conductive dipoles. The dipole patterns showed increased resonance shift with decreased <span class="hlt">separation</span> distances, with the <span class="hlt">separation</span> in the direction orthogonal to the dipole orientations having a more significant effect. The coupling mechanisms between dipole neighbours were evaluated by comparing surface charge densities, which revealed the gain and loss of coupling as the dipoles moved in and out of alignment via folding. Collectively, these results provide a basis of origami FSS designs for experimental study and motivates the development of computational tools to systematically predict optimal fold patterns for targeted <span class="hlt">frequency</span> response and directionality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA628566','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA628566"><span>High-<span class="hlt">Frequency</span> Sound Interaction in Ocean Sediments</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2003-09-30</p> <p>results, combined with measured sediment properties, to test the validity of sediment acoustic models , and in particular the poroelastic (Biot...understanding of the dominant scatterers versus <span class="hlt">frequency</span> near the sediment surface, the potential need for poroelastic sediment models , the...work are described under a <span class="hlt">separate</span> ONR project titled “ Acoustic propagation and scattering within sand sediments: Laboratory experiments, modeling</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27916666','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27916666"><span>Rhythmic entrainment source <span class="hlt">separation</span>: Optimizing analyses of neural responses to rhythmic sensory stimulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cohen, Michael X; Gulbinaite, Rasa</p> <p>2017-02-15</p> <p>Steady-state evoked potentials (SSEPs) are rhythmic brain responses to rhythmic sensory stimulation, and are often used to study perceptual and attentional processes. We present a data analysis method for maximizing the signal-to-noise ratio of the narrow-band steady-state response in the <span class="hlt">frequency</span> and time-<span class="hlt">frequency</span> domains. The method, termed rhythmic entrainment source <span class="hlt">separation</span> (RESS), is based on denoising source <span class="hlt">separation</span> approaches that take advantage of the simultaneous but differential projection of neural activity to multiple electrodes or sensors. Our approach is a combination and extension of existing multivariate source <span class="hlt">separation</span> methods. We demonstrate that RESS performs well on both simulated and empirical data, and outperforms conventional SSEP analysis methods based on selecting electrodes with the strongest SSEP response, as well as several other linear spatial filters. We also discuss the potential confound of overfitting, whereby the filter captures noise in absence of a signal. Matlab scripts are available to replicate and extend our simulations and methods. We conclude with some practical advice for optimizing SSEP data analyses and interpreting the results. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhRvA..88f3402C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhRvA..88f3402C"><span>X-ray <span class="hlt">frequency</span> combs from optically controlled resonance fluorescence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavaletto, Stefano M.; Harman, Zoltán; Buth, Christian; Keitel, Christoph H.</p> <p>2013-12-01</p> <p>An x-ray pulse-shaping scheme is put forward for imprinting an optical <span class="hlt">frequency</span> comb onto the radiation emitted on a driven x-ray transition, thus producing an x-ray <span class="hlt">frequency</span> comb. A four-level system is used to describe the level structure of N ions driven by narrow-bandwidth x rays, an optical auxiliary laser, and an optical <span class="hlt">frequency</span> comb. By including many-particle enhancement of the emitted resonance fluorescence, a spectrum is predicted consisting of equally spaced narrow lines which are centered on an x-ray transition energy and <span class="hlt">separated</span> by the same tooth spacing as the driving optical <span class="hlt">frequency</span> comb. Given an x-ray reference <span class="hlt">frequency</span>, our comb could be employed to determine an unknown x-ray <span class="hlt">frequency</span>. While relying on the quality of the light fields used to drive the ensemble of ions, the model has validity at energies from the 100 eV to the keV range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25e2110I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25e2110I"><span>A transverse <span class="hlt">separate</span>-spin-evolution streaming instability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iqbal, Z.; Andreev, Pavel A.; Murtaza, G.</p> <p>2018-05-01</p> <p>By using the <span class="hlt">separate</span> spin evolution quantum hydrodynamical model, the instability of transverse mode due to electron streaming in a partially spin polarized magnetized degenerate plasma is studied. The electron spin polarization gives birth to a new spin-dependent wave (i.e., <span class="hlt">separate</span> spin evolution streaming driven ordinary wave) in the real wave spectrum. It is shown that the spin polarization and streaming speed significantly affect the <span class="hlt">frequency</span> of this new mode. Analyzing growth rate, it is found that the electron spin effects reduce the growth rate and shift the threshold of instability as well as its termination point towards higher values. Additionally, how the other parameters like electron streaming and Fermi pressure influence the growth rate is also investigated. Current study can help towards better understanding of the existence of new waves and streaming instability in the astrophysical plasmas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V21B2705M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V21B2705M"><span>An analytical formula for the longitudinal resonance <span class="hlt">frequencies</span> of a fluid-filled crack</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maeda, Y.; Kumagai, H.</p> <p>2013-12-01</p> <p> longitudinal mode resonances. The peak <span class="hlt">frequencies</span> computed by the FDM are well fitted by Eq. (1). The best-fit ɛmL values are different from those for 2D and depend on W/L, where W is the crack width. Eq. (1) shows that fmL is a simple analytical function of a/L and C given m and W/L. This enables simple and rapid interpretations of the source processes of LP events, including estimation of the fluid properties and crack geometries as well as identification of the resonance modes of the individual peak <span class="hlt">frequencies</span>. LP events at volcanoes often exhibit peak <span class="hlt">frequency</span> <span class="hlt">variations</span>. In such cases, the <span class="hlt">frequency</span> <span class="hlt">variations</span> can be easily converted to <span class="hlt">variations</span> in the fluid properties and crack geometries. We showed that Eq. (1) is consistent with the analytical solution for an infinite crack given by Ferrazzini and Aki (1987, JGR). Although a theoretical derivation of Eq. (1) was not obtained yet, Eq. (1) is consistent with the <span class="hlt">frequencies</span> expected from the wavelengths of the fluid pressure <span class="hlt">variation</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21967339','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21967339"><span>Recent developments in membrane-based <span class="hlt">separations</span> in biotechnology processes: review.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rathore, A S; Shirke, A</p> <p>2011-01-01</p> <p>Membrane-based <span class="hlt">separations</span> are the most ubiquitous unit operations in biotech processes. There are several key reasons for this. First, they can be used with a large variety of applications including clarification, concentration, buffer exchange, purification, and sterilization. Second, they are available in a variety of formats, such as depth filtration, ultrafiltration, diafiltration, nanofiltration, reverse osmosis, and microfiltration. Third, they are simple to operate and are generally robust toward normal <span class="hlt">variations</span> in feed material and operating parameters. Fourth, membrane-based <span class="hlt">separations</span> typically require lower capital cost when compared to other processing options. As a result of these advantages, a typical biotech process has anywhere from 10 to 20 membrane-based <span class="hlt">separation</span> steps. In this article we review the major developments that have occurred on this topic with a focus on developments in the last 5 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29401959','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29401959"><span><span class="hlt">Frequency</span> comb generation in a silicon ring resonator modulator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Demirtzioglou, Iosif; Lacava, Cosimo; Bottrill, Kyle R H; Thomson, David J; Reed, Graham T; Richardson, David J; Petropoulos, Periklis</p> <p>2018-01-22</p> <p>We report on the generation of an optical comb of highly uniform in power <span class="hlt">frequency</span> lines (<span class="hlt">variation</span> less than 0.7 dB) using a silicon ring resonator modulator. A characterization involving the measurement of the complex transfer function of the ring is presented and five <span class="hlt">frequency</span> tones with a 10-GHz spacing are produced using a dual-<span class="hlt">frequency</span> electrical input at 10 and 20 GHz. A comb shape comparison is conducted for different modulator bias voltages, indicating optimum operation at a small forward-bias voltage. A time-domain measurement confirmed that the comb signal was highly coherent, forming 20.3-ps-long pulses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS11C1655Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS11C1655Z"><span>Velocity Spectrum <span class="hlt">Variation</span> in Central Gulf of Mexico: 9Case Studies for the 2005 Hurricanes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, F.; Li, C.</p> <p>2012-12-01</p> <p>Significant near inertial oscillation caused by hurricanes is common in the ocean. The details of the vertical and temporal <span class="hlt">variations</span> of hurricane induced near inertial oscillation are usually complicated. We have done a case study of such vertical and temporal <span class="hlt">variations</span> of velocity spectrum focusing around the inertial <span class="hlt">frequency</span> for the 2005 hurricane season. Data were from a deep water mooring chain containing a series of current meters and 2 ADCPs from June to November 2005. The velocity spectrum is obtained with a 10-day sliding window at different depths for the 40-hour high-passed data to exclude the low <span class="hlt">frequency</span> Loop Current <span class="hlt">variations</span>. This gives a temporal <span class="hlt">variation</span> of the spectrum at different depths. Such <span class="hlt">variations</span> in velocity spectrum are resulted from the ocean dynamics influenced by the passage of hurricanes. Our preliminary analysis of the results show that (1) right before the center of the hurricane gets closest to the mooring site, there always exists a 2-peak feature of energy at almost all depths; while during the passage of the hurricane these two peaks will merge Into one peak which has a corresponding period of 30.3 to 25.6 hours, encompassing that corresponding to the inertial <span class="hlt">frequency</span> in this latitude; (2) after the passage of the hurricane, the decay process of energy is also complicated. It is found that the whole profile can be at least divided into 3 layers: surface to 800m, 800m to 1500m, and 1500m to the bottom, which is consistent with the stratification of the water column. It is also found that shift in the peak <span class="hlt">frequency</span> to either side of the inertial <span class="hlt">frequency</span> is very common. The main peak of energy can break into several parts during the decay stage, with blue shift and red shift.; ;</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090007955','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090007955"><span>Application of Synthetic Jets to Reduce Stator Flow <span class="hlt">Separation</span> in a Low Speed Axial Compressor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Braunscheidel, Edward P.; Culley, Dennis E.; Zaman, Khairul B.M.Q.</p> <p>2008-01-01</p> <p>Flow control using synthetic jet injection has been applied in a low speed axial compressor. The synthetic jets were applied from the suction surface of a stator vane via a span-wise row of slots pitched in the streamwise direction. Actuation was provided externally from acoustic drivers coupled to the vane tip via flexible tubing. The acoustic resonance characteristics of the system, and the resultant jet velocities were obtained. The effects on the <span class="hlt">separated</span> flow field for various jet velocities and <span class="hlt">frequencies</span> were explored. Total pressure loss reductions across the vane passage were measured. The effect of synthetic jet injection was shown to be comparable to that of pulsatory injection with mass addition for stator vanes which had <span class="hlt">separated</span> flow. While only a weak dependence of the beneficial effect was noted based on the excitation <span class="hlt">frequency</span>, a strong dependence on the amplitude was observed at all <span class="hlt">frequencies</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17503936','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17503936"><span>Lock-in amplifier error prediction and correction in <span class="hlt">frequency</span> sweep measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sonnaillon, Maximiliano Osvaldo; Bonetto, Fabian Jose</p> <p>2007-01-01</p> <p>This article proposes an analytical algorithm for predicting errors in lock-in amplifiers (LIAs) working with time-varying reference <span class="hlt">frequency</span>. Furthermore, a simple method for correcting such errors is presented. The reference <span class="hlt">frequency</span> can be swept in order to measure the <span class="hlt">frequency</span> response of a system within a given spectrum. The continuous <span class="hlt">variation</span> of the reference <span class="hlt">frequency</span> produces a measurement error that depends on three factors: the sweep speed, the LIA low-pass filters, and the <span class="hlt">frequency</span> response of the measured system. The proposed error prediction algorithm is based on the final value theorem of the Laplace transform. The correction method uses a double-sweep measurement. A mathematical analysis is presented and validated with computational simulations and experimental measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080047421','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080047421"><span><span class="hlt">Separating</span> Turbofan Engine Noise Sources Using Auto and Cross Spectra from Four Microphones</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miles, Jeffrey Hilton</p> <p>2008-01-01</p> <p>The study of core noise from turbofan engines has become more important as noise from other sources such as the fan and jet were reduced. A multiple-microphone and acoustic-source modeling method to <span class="hlt">separate</span> correlated and uncorrelated sources is discussed. The auto- and cross spectra in the <span class="hlt">frequency</span> range below 1000 Hz are fitted with a noise propagation model based on a source couplet consisting of a single incoherent monopole source with a single coherent monopole source or a source triplet consisting of a single incoherent monopole source with two coherent monopole point sources. Examples are presented using data from a Pratt& Whitney PW4098 turbofan engine. The method <span class="hlt">separates</span> the low-<span class="hlt">frequency</span> jet noise from the core noise at the nozzle exit. It is shown that at low power settings, the core noise is a major contributor to the noise. Even at higher power settings, it can be more important than jet noise. However, at low <span class="hlt">frequencies</span>, uncorrelated broadband noise and jet noise become the important factors as the engine power setting is increased.</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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