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Showing papers by "University of New Hampshire published in 2013"


Journal ArticleDOI
TL;DR: The Electric and Magnetic Field Instrument and Integrated Science (EMFISIS) investigation on the NASA Radiation Belt Storm Probes (now named the Van Allen Probes) mission provides key wave and very low frequency magnetic field measurements to understand radiation belt acceleration, loss, and transport.
Abstract: The Electric and Magnetic Field Instrument and Integrated Science (EMFISIS) investigation on the NASA Radiation Belt Storm Probes (now named the Van Allen Probes) mission provides key wave and very low frequency magnetic field measurements to understand radiation belt acceleration, loss, and transport. The key science objectives and the contribution that EMFISIS makes to providing measurements as well as theory and modeling are described. The key components of the instruments suite, both electronics and sensors, including key functional parameters, calibration, and performance, demonstrate that EMFISIS provides the needed measurements for the science of the RBSP mission. The EMFISIS operational modes and data products, along with online availability and data tools provide the radiation belt science community with one the most complete sets of data ever collected.

1,060 citations


Journal ArticleDOI
J. Aasi1, J. Abadie1, B. P. Abbott1, R. Abbott1  +745 moreInstitutions (73)
TL;DR: In this article, the authors inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz.
Abstract: Nearly a century after Einstein first predicted the existence of gravitational waves, a global network of Earth-based gravitational wave observatories1, 2, 3, 4 is seeking to directly detect this faint radiation using precision laser interferometry. Photon shot noise, due to the quantum nature of light, imposes a fundamental limit on the attometre-level sensitivity of the kilometre-scale Michelson interferometers deployed for this task. Here, we inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz, critically important for several astrophysical sources, with no deterioration of performance observed at any frequency. With the injection of squeezed states, this LIGO detector demonstrated the best broadband sensitivity to gravitational waves ever achieved, with important implications for observing the gravitational-wave Universe with unprecedented sensitivity.

805 citations


Journal ArticleDOI
TL;DR: Few significant changes could be detected in rates since an equivalent survey in 2008, but declines were documented in peer flashing, school bomb threats, juvenile sibling assault, and robbery and total property victimization.
Abstract: Importance Because exposure to violence, crime, and abuse has been shown to have serious consequences on child development, physicians and policymakers need to know the kinds of exposure that occur at various developmental stages. Objectives To provide updated estimates of and trends for childhood exposure to a broad range of violence, crime, and abuse victimizations. Design The National Survey of Children’s Exposure to Violence was based on a cross-sectional, US national telephone survey conducted in 2011. Setting Interviews by telephone. Participants The experiences of 4503 children and youth aged 1 month to 17 years were assessed by interviews with caregivers and with youth in the case of those aged 10 to 17 years. Results Two-fifths (41.2%) of children and youth experienced a physical assault in the last year, and 1 in 10 (10.1%) experienced an assault-related injury. Two percent experienced sexual assault or sexual abuse in the last year, but the rate was 10.7% for girls aged 14 to 17 years. More than 1 in 10 (13.7%) experienced maltreatment by a caregiver, including 3.7% who experienced physical abuse. Few significant changes could be detected in rates since an equivalent survey in 2008, but declines were documented in peer flashing, school bomb threats, juvenile sibling assault, and robbery and total property victimization. Conclusions and Relevance The variety and scope of children’s exposure to violence, crime, and abuse suggest the need for better and more comprehensive tools in clinical and research settings for identifying these experiences and their effects.

693 citations


Journal ArticleDOI
19 Dec 2013-Nature
TL;DR: High-resolution electron observations obtained during the 9 October storm are reported and chorus scattering explains the temporal evolution of both the energy and angular distribution of the observed relativistic electron flux increase, and detailed modelling demonstrates the remarkable efficiency of wave acceleration in the Earth's outer radiation belt.
Abstract: Recent analysis of satellite data obtained during the 9 October 2012 geomagnetic storm identified the development of peaks in electron phase space density, which are compelling evidence for local electron acceleration in the heart of the outer radiation belt, but are inconsistent with acceleration by inward radial diffusive transport. However, the precise physical mechanism responsible for the acceleration on 9 October was not identified. Previous modelling has indicated that a magnetospheric electromagnetic emission known as chorus could be a potential candidate for local electron acceleration, but a definitive resolution of the importance of chorus for radiation-belt acceleration was not possible because of limitations in the energy range and resolution of previous electron observations and the lack of a dynamic global wave model. Here we report high-resolution electron observations obtained during the 9 October storm and demonstrate, using a two-dimensional simulation performed with a recently developed time-varying data-driven model, that chorus scattering explains the temporal evolution of both the energy and angular distribution of the observed relativistic electron flux increase. Our detailed modelling demonstrates the remarkable efficiency of wave acceleration in the Earth's outer radiation belt, and the results presented have potential application to Jupiter, Saturn and other magnetized astrophysical objects.

665 citations


Journal ArticleDOI
TL;DR: Analyses of the assembly indicate that two whole-genome duplications likely occurred before the divergence of ancestral lamprey and gnathostome lineages, and help define key evolutionary events within vertebrate lineages.
Abstract: Lampreys are representatives of an ancient vertebrate lineage that diverged from our own ∼500 million years ago. By virtue of this deeply shared ancestry, the sea lamprey (P. marinus) genome is uniquely poised to provide insight into the ancestry of vertebrate genomes and the underlying principles of vertebrate biology. Here, we present the first lamprey whole-genome sequence and assembly. We note challenges faced owing to its high content of repetitive elements and GC bases, as well as the absence of broad-scale sequence information from closely related species. Analyses of the assembly indicate that two whole-genome duplications likely occurred before the divergence of ancestral lamprey and gnathostome lineages. Moreover, the results help define key evolutionary events within vertebrate lineages, including the origin of myelin-associated proteins and the development of appendages. The lamprey genome provides an important resource for reconstructing vertebrate origins and the evolutionary events that have shaped the genomes of extant organisms.

596 citations


Journal ArticleDOI
TL;DR: In this paper, the authors describe the Magnetic Electron Ion Spectrometer (MagEIS) instruments aboard the RBSP spacecraft from an instrumentation and engineering point of view, including four magnetic spectrometers.
Abstract: This paper describes the Magnetic Electron Ion Spectrometer (MagEIS) instruments aboard the RBSP spacecraft from an instrumentation and engineering point of view. There are four magnetic spectrometers aboard each of the two spacecraft, one low-energy unit (20–240 keV), two medium-energy units (80–1200 keV), and a high-energy unit (800–4800 keV). The high unit also contains a proton telescope (55 keV–20 MeV).

582 citations


Journal ArticleDOI
TL;DR: In this paper, the authors measured the temperature response of microbial efficiency in soils amended with substrates varying in lability, and found that the efficiency with which soil microorganisms use organic matter is dependent on both temperature and substrate quality, with efficiency declining with increasing temperatures for more recalcitrant substrates.
Abstract: Soils are the largest repository of organic carbon in the terrestrial biosphere. Nevertheless, relatively little is known about the factors controlling the efficiency with which microbial communities utilize carbon, and its effect on soil–atmosphere CO2 exchange. Now research using long-term experimental plots suggests that climate warming could alter the decay dynamics of more stable organic-matter compounds with implications for carbon storage in soils and ultimately climate warming. Soils are the largest repository of organic carbon (C) in the terrestrial biosphere and represent an important source of carbon dioxide (CO2) to the atmosphere, releasing 60–75 Pg C annually through microbial decomposition of organic materials1,2. A primary control on soil CO2 flux is the efficiency with which the microbial community uses C. Despite its critical importance to soil–atmosphere CO2 exchange, relatively few studies have examined the factors controlling soil microbial efficiency. Here, we measured the temperature response of microbial efficiency in soils amended with substrates varying in lability. We also examined the temperature sensitivity of microbial efficiency in response to chronic soil warming in situ. We find that the efficiency with which soil microorganisms use organic matter is dependent on both temperature and substrate quality, with efficiency declining with increasing temperatures for more recalcitrant substrates. However, the utilization efficiency of a more recalcitrant substrate increased at higher temperatures in soils exposed to almost two decades of warming 5 °C above ambient. Our work suggests that climate warming could alter the decay dynamics of more stable organic matter compounds, thereby having a positive feedback to climate that is attenuated by a shift towards a more efficient microbial community in the longer term.

571 citations


Journal ArticleDOI
30 Aug 2013-Science
TL;DR: Measurements from NASA’s Van Allen Radiation Belt Storm Probes are reported that clearly distinguish between the two types of acceleration, and the observed radial profiles of phase space density are characteristic of local acceleration in the heart of the radiation belts and are inconsistent with a predominantly radial acceleration process.
Abstract: The Van Allen radiation belts contain ultrarelativistic electrons trapped in Earth's magnetic field. Since their discovery in 1958, a fundamental unanswered question has been how electrons can be accelerated to such high energies. Two classes of processes have been proposed: transport and acceleration of electrons from a source population located outside the radiation belts (radial acceleration) or acceleration of lower-energy electrons to relativistic energies in situ in the heart of the radiation belts (local acceleration). We report measurements from NASA's Van Allen Radiation Belt Storm Probes that clearly distinguish between the two types of acceleration. The observed radial profiles of phase space density are characteristic of local acceleration in the heart of the radiation belts and are inconsistent with a predominantly radial acceleration process.

495 citations


Journal ArticleDOI
TL;DR: In this article, the authors examined whether stream nitrogen concentrations in forested reference catchments have changed over time and if patterns were consistent across the USA, synthesized up to 44 yr of data collected from 22 catchments at seven USDA Forest Service Experimental Forests.
Abstract: To examine whether stream nitrogen concentrations in forested reference catchments have changed over time and if patterns were consistent across the USA, we synthesized up to 44 yr of data collected from 22 catchments at seven USDA Forest Service Experimental Forests. Trends in stream nitrogen presented high spatial variability both among catchments at a site and among sites across the USA. We found both increasing and decreasing trends in monthly flow-weighted stream nitrate and ammonium concentrations. At a subset of the catchments, we found that the length and period of analysis influenced whether trends were positive, negative or non-significant. Trends also differed among neighboring catchments within several Experimental Forests, suggesting the importance of catchment-specific factors in determining nutrient exports. Over the longest time periods, trends were more consistent among catchments within sites, although there are fewer long-term records for analysis. These findings highlight the critical value of long-term, uninterrupted stream chemistry monitoring at a network of sites across the USA to elucidate patterns of change in nutrient concentrations at minimally disturbed forested sites.

494 citations


Journal ArticleDOI
TL;DR: The Radiation Belt Storm Probes (RBSP)-Energetic Particle, Composition, and Thermal Plasma (ECT) suite contains an innovative complement of particle instruments to ensure the highest quality measurements ever made in the inner magnetosphere and radiation belts as mentioned in this paper.
Abstract: The Radiation Belt Storm Probes (RBSP)-Energetic Particle, Composition, and Thermal Plasma (ECT) suite contains an innovative complement of particle instruments to ensure the highest quality measurements ever made in the inner magnetosphere and radiation belts. The coordinated RBSP-ECT particle measurements, analyzed in combination with fields and waves observations and state-of-the-art theory and modeling, are necessary for understanding the acceleration, global distribution, and variability of radiation belt electrons and ions, key science objectives of NASA’s Living With a Star program and the Van Allen Probes mission. The RBSP-ECT suite consists of three highly-coordinated instruments: the Magnetic Electron Ion Spectrometer (MagEIS), the Helium Oxygen Proton Electron (HOPE) sensor, and the Relativistic Electron Proton Telescope (REPT). Collectively they cover, continuously, the full electron and ion spectra from one eV to 10’s of MeV with sufficient energy resolution, pitch angle coverage and resolution, and with composition measurements in the critical energy range up to 50 keV and also from a few to 50 MeV/nucleon. All three instruments are based on measurement techniques proven in the radiation belts. The instruments use those proven techniques along with innovative new designs, optimized for operation in the most extreme conditions in order to provide unambiguous separation of ions and electrons and clean energy responses even in the presence of extreme penetrating background environments. The design, fabrication and operation of ECT spaceflight instrumentation in the harsh radiation belt environment ensure that particle measurements have the fidelity needed for closure in answering key mission science questions. ECT instrument details are provided in companion papers in this same issue.

492 citations


Journal ArticleDOI
TL;DR: The HOPE mass spectrometer of the Radiation Belt Storm Probes (RBSP) mission is designed to measure the in situ plasma ion and electron fluxes over 4π sr at each RBSP spacecraft within the terrestrial radiation belts.
Abstract: The HOPE mass spectrometer of the Radiation Belt Storm Probes (RBSP) mission (renamed the Van Allen Probes) is designed to measure the in situ plasma ion and electron fluxes over 4π sr at each RBSP spacecraft within the terrestrial radiation belts. The scientific goal is to understand the underlying physical processes that govern the radiation belt structure and dynamics. Spectral measurements for both ions and electrons are acquired over 1 eV to 50 keV in 36 log-spaced steps at an energy resolution ΔE FWHM/E≈15 %. The dominant ion species (H+, He+, and O+) of the magnetosphere are identified using foil-based time-of-flight (TOF) mass spectrometry with channel electron multiplier (CEM) detectors. Angular measurements are derived using five polar pixels coplanar with the spacecraft spin axis, and up to 16 azimuthal bins are acquired for each polar pixel over time as the spacecraft spins. Ion and electron measurements are acquired on alternate spacecraft spins. HOPE incorporates several new methods to minimize and monitor the background induced by penetrating particles in the harsh environment of the radiation belts. The absolute efficiencies of detection are continuously monitored, enabling precise, quantitative measurements of electron and ion fluxes and ion species abundances throughout the mission. We describe the engineering approaches for plasma measurements in the radiation belts and present summaries of HOPE measurement strategy and performance.


Journal ArticleDOI
17 Jan 2013-Cell
TL;DR: The crystal structure of MDA5 bound to dsRNA is reported, which shows how, using the same domain architecture, MDA5 recognizes the internal duplex structure, whereas RIG-I recognizes the terminus of ds RNA.

Journal ArticleDOI
TL;DR: This paper reviewed studies concerned with abusive supervision and provided a constructive revision of Tepper's 2007 model and added additional variables and casual paths to increase its explanatory potential, emphasizing the importance of subordinates' individual differences such as attribution style, negative affectivity, and implicit work theories to account for significant variability in subordinates' perceptions of abuse.
Abstract: This paper reviews studies concerned with abusive supervision and provides a constructive revision of Tepper’s 2007 model. As a result of our review of the recent research, we revised the 2007 Tepper model and added additional variables and casual paths to increase its explanatory potential. The model we propose distinguishes between abusive supervisory behavior and abusive supervisory perceptions, suggesting that each of these variables needs to be studied separately until we know more about how they are related. The revised model also explicitly recognizes possibilities for reverse causation and stresses the importance of subordinates’ individual differences such as attribution style, negative affectivity, and implicit work theories, which have the potential to account for significant variability in subordinates’ perceptions of abuse. Suggestions for future research based on the original relationships identified by the Tepper review as well as the variables and causal paths suggested in the revised model are provided.

Journal ArticleDOI
TL;DR: The Relativistic Electron-Proton Telescope (REPT) as mentioned in this paper was designed for the Radiation Belt Storm Probe (RBSP) pair of spacecraft to measure high-energy electrons (up to ∼20 MeV) with excellent sensitivity and also measured magnetospheric and solar protons to energies well above E=100 MeV.
Abstract: Particle acceleration and loss in the million electron Volt (MeV) energy range (and above) is the least understood aspect of radiation belt science. In order to measure cleanly and separately both the energetic electron and energetic proton components, there is a need for a carefully designed detector system. The Relativistic Electron-Proton Telescope (REPT) on board the Radiation Belt Storm Probe (RBSP) pair of spacecraft consists of a stack of high-performance silicon solid-state detectors in a telescope configuration, a collimation aperture, and a thick case surrounding the detector stack to shield the sensors from penetrating radiation and bremsstrahlung. The instrument points perpendicular to the spin axis of the spacecraft and measures high-energy electrons (up to ∼20 MeV) with excellent sensitivity and also measures magnetospheric and solar protons to energies well above E=100 MeV. The instrument has a large geometric factor (g=0.2 cm2 sr) to get reasonable count rates (above background) at the higher energies and yet will not saturate at the lower energy ranges. There must be fast enough electronics to avert undue dead-time limitations and chance coincidence effects. The key goal for the REPT design is to measure the directional electron intensities (in the range 10−2–106 particles/cm2 s sr MeV) and energy spectra (ΔE/E∼25 %) throughout the slot and outer radiation belt region. Present simulations and detailed laboratory calibrations show that an excellent design has been attained for the RBSP needs. We describe the engineering design, operational approaches, science objectives, and planned data products for REPT.

Journal ArticleDOI
TL;DR: Their understanding of the most harmful childhood adversities is still incomplete because of complex interrelationships among them, but the authors know enough to proceed to interventional studies to determine whether prevention and remediation can improve long-term outcomes.
Abstract: Objective To test and improve upon the list of adverse childhood experiences from the Adverse Childhood Experiences (ACE) Study scale by examining the ability of a broader range to correlate with mental health symptoms. Design Nationally representative sample of children and adolescents. Setting and Participants Telephone interviews with a nationally representative sample of 2030 youth aged 10 to 17 years who were asked about lifetime adversities and current distress symptoms. Main Outcome Measures Lifetime adversities and current distress symptoms. Results The adversities from the original ACE scale items were associated with mental health symptoms among the participants, but the association was significantly improved (from R 2 = 0.21 to R 2 = 0.34) by removing some of the original ACE scale items and adding others in the domains of peer rejection, peer victimization, community violence exposure, school performance, and socioeconomic status. Conclusions Our understanding of the most harmful childhood adversities is still incomplete because of complex interrelationships among them, but we know enough to proceed to interventional studies to determine whether prevention and remediation can improve long-term outcomes.


Journal ArticleDOI
TL;DR: In this article, the authors explore the hybrid phenomenon of social business, that is, both a form of organization and a practice that deliberately harnesses market dynamics to address deeply rooted social issues through the design and implementation of a core product or service.
Abstract: This article explores the hybrid phenomenon of social business, that is, both a form of organization and a practice that deliberately harnesses market dynamics to address deeply rooted social issues through the design and implementation of a core product or service. This new form of hybrid venture melds the social purpose traditionally associated with non-profit organizations with the economic purpose and market-based methods traditionally associated with for-profit firms. This exploratory research inductively explores the process by which social businesses are designed. The result suggests that clear intentionality around social purpose drives the design of these ventures and their associated missions and business models such that they can creatively synthesize competing paradigms (economic and social purpose) within one venture. The tight coupling of mission, method, and operationalization allows for the multi-stakeholder promise of the business model to be fulfilled.

Journal ArticleDOI
TL;DR: The International Bathymetric Chart of the Southern Ocean (IBCSO) Version 1.0 is a new digital bathymetric model (DBM) portraying the seafloor of the circum-Antarctic waters south of 60 degrees S as discussed by the authors.
Abstract: The International Bathymetric Chart of the Southern Ocean (IBCSO) Version 1.0 is a new digital bathymetric model (DBM) portraying the seafloor of the circum-Antarctic waters south of 60 degrees S. ...

Journal ArticleDOI
TL;DR: The theoretical basis of GIOP is described, a preliminary default configuration for GIOP (GIOP-DC) is proposed, and its comparable performance to other popular SAAs is presented and the sensitivities of their output to their parameterization are quantified.
Abstract: Ocean color measured from satellites provides daily, global estimates of marine inherent optical properties (IOPs). Semi-analytical algorithms (SAAs) provide one mechanism for inverting the color of the water observed by the satellite into IOPs. While numerous SAAs exist, most are similarly constructed and few are appropriately parameterized for all water masses for all seasons. To initiate community-wide discussion of these limitations, NASA organized two workshops that deconstructed SAAs to identify similarities and uniqueness and to progress toward consensus on a unified SAA. This effort resulted in the development of the generalized IOP (GIOP) model software that allows for the construction of different SAAs at runtime by selection from an assortment of model parameterizations. As such, GIOP permits isolation and evaluation of specific modeling assumptions, construction of SAAs, development of regionally tuned SAAs, and execution of ensemble inversion modeling. Working groups associated with the workshops proposed a preliminary default configuration for GIOP (GIOP-DC), with alternative model parameterizations and features defined for subsequent evaluation. In this paper, we: (1) describe the theoretical basis of GIOP; (2) present GIOP-DC and verify its comparable performance to other popular SAAs using both in situ and synthetic data sets; and, (3) quantify the sensitivities of their output to their parameterization. We use the latter to develop a hierarchical sensitivity of SAAs to various model parameterizations, to identify components of SAAs that merit focus in future research, and to provide material for discussion on algorithm uncertainties and future emsemble applications.

Journal ArticleDOI
TL;DR: Joint spatial analysis of stressors and ecosystem services can provide a critical foundation for maximizing social and ecological benefits from restoration investments and find that many important areas for fisheries and recreation are subject to high stress, indicating that ecosystem degradation could be threatening key services.
Abstract: With increasing pressure placed on natural systems by growing human populations, both scientists and resource managers need a better understanding of the relationships between cumulative stress from human activities and valued ecosystem services. Societies often seek to mitigate threats to these services through large-scale, costly restoration projects, such as the over one billion dollar Great Lakes Restoration Initiative currently underway. To help inform these efforts, we merged high-resolution spatial analyses of environmental stressors with mapping of ecosystem services for all five Great Lakes. Cumulative ecosystem stress is highest in near-shore habitats, but also extends offshore in Lakes Erie, Ontario, and Michigan. Variation in cumulative stress is driven largely by spatial concordance among multiple stressors, indicating the importance of considering all stressors when planning restoration activities. In addition, highly stressed areas reflect numerous different combinations of stressors rather than a single suite of problems, suggesting that a detailed understanding of the stressors needing alleviation could improve restoration planning. We also find that many important areas for fisheries and recreation are subject to high stress, indicating that ecosystem degradation could be threatening key services. Current restoration efforts have targeted high-stress sites almost exclusively, but generally without knowledge of the full range of stressors affecting these locations or differences among sites in service provisioning. Our results demonstrate that joint spatial analysis of stressors and ecosystem services can provide a critical foundation for maximizing social and ecological benefits from restoration investments.

Journal ArticleDOI
TL;DR: In this article, a set of seven global hydrological models (GHMs) were used to quantify the impact of projected global climate change on IWD on currently irrigated areas by the end of this century, and the resulting uncertainties arising from both theGHMs and climate projections.
Abstract: Crop irrigation is responsible for 70% of humanity’swater demand. Since the late 1990s, the expansion ofirrigated areas has been tapering off, and this trend isexpected to continue in the future. Future irrigation waterdemand (IWD) is, however, subject to large uncertaintiesdue to anticipated climate change. Here, we use a set ofseven global hydrological models (GHMs) to quantify theimpact of projected global climate change on IWD oncurrently irrigated areas by the end of this century, and toassess the resulting uncertainties arising from both theGHMs and climate projections. The resulting ensembleprojections generally show an increasing trend in futureIWD, but the increase varies substantially depending onthe degree of global warming and associated regionalprecipitation changes. Under the highest greenhouse gasemission scenario (RCP8.5), IWD will considerably increaseduring the summer in the Northern Hemisphere (>20% by2100), and the present peak IWD is projected to shift onemonth or more over regions where ≥80% of the globalirrigated areas exist and 4 billion people currently live.Uncertaint ies arising from GHMs and global climatemodels (GCMs) are large, with GHM uncertainty dominatingthroughout the century and with GCM uncertaintysubstantially increasing from the midcentury, indicating thechoice of GHM outweighing by far the uncertainty arisingfrom the choi ce of GCM and associated emission scenario.


Journal ArticleDOI
12 Apr 2013-Science
TL;DR: In situ energy-specific and temporally resolved spacecraft observations reveal an isolated third ring, or torus, of high-energy electrons that formed on 2 September 2012 and persisted largely unchanged in the geocentric radial range of 3.0 to ~3.5 Earth radii for more than 4 weeks before being disrupted (and virtually annihilated) by a powerful interplanetary shock wave passage.
Abstract: Since their discovery more than 50 years ago, Earth’s Van Allen radiation belts have been considered to consist of two distinct zones of trapped, highly energetic charged particles. The outer zone is composed predominantly of megaelectron volt (MeV) electrons that wax and wane in intensity on time scales ranging from hours to days, depending primarily on external forcing by the solar wind. The spatially separated inner zone is composed of commingled high-energy electrons and very energetic positive ions (mostly protons), the latter being stable in intensity levels over years to decades. In situ energy-specific and temporally resolved spacecraft observations reveal an isolated third ring, or torus, of high-energy (>2 MeV) electrons that formed on 2 September 2012 and persisted largely unchanged in the geocentric radial range of 3.0 to ~3.5 Earth radii for more than 4 weeks before being disrupted (and virtually annihilated) by a powerful interplanetary shock wave passage.

Journal ArticleDOI
Anushka Udara Abeysekara1, Ruben Alfaro2, C. Alvarez, J. D. Álvarez3, R. Arceo, J.C. Arteaga-Velázquez3, H. A. Ayala Solares4, A. S. Barber5, B. M. Baughman6, N. Bautista-Elivar7, E. Belmont2, Segev BenZvi8, D. Berley6, M. Bonilla Rosales9, J. Braun6, R. A. Caballero-Lopez2, A. Carraminana9, M. Castillo10, U. Cotti3, Jorge Cotzomi10, E. De la Fuente11, C. De León3, Tyce DeYoung12, R. Diaz Hernandez9, Juan Carlos Diaz-Velez8, Brenda Dingus13, Michael DuVernois8, R. W. Ellsworth6, R. W. Ellsworth14, A. Fernandez10, D. W. Fiorino8, Nissim Illich Fraija2, A. Galindo9, Jose Luis García-Luna11, Guillermo Garcia-Torales11, Fernando Garfias2, Luis Xavier Gonzalez2, Maria Magdalena González2, J. A. Goodman6, V. Grabski2, M. Gussert15, Z. Hampel-Arias8, C. M. Hui4, Petra Hüntemeyer4, A. Imran13, Arturo Iriarte2, P. Karn16, David Kieda5, Gerd J. Kunde13, Alejandro Lara2, R. J. Lauer17, William H. Lee2, Dirk Lennarz18, H. León Vargas2, E. C. Linares3, J. T. Linnemann1, M. Longo15, R. Luna-García19, A. Marinelli2, O. Martinez10, Jesús Martínez-Castro19, J. A. Matthews17, Pedro Miranda-Romagnoli9, Pedro Miranda-Romagnoli20, E. Moreno10, Miguel Mostafá15, J. Nava9, Lukas Nellen2, Michael Newbold5, R. Noriega-Papaqui20, T. Oceguera-Becerra2, T. Oceguera-Becerra11, B. Patricelli2, R. Pelayo10, E. G. Pérez-Pérez7, J. Pretz13, Colas Rivière2, James M. Ryan21, Daniel Rosa-Gonzalez9, Humberto Ibarguen Salazar10, F. Salesa15, A. Sandoval2, Elton J. G. Santos, Michael Schneider22, S. Silich9, G. Sinnis13, A. J. Smith6, K. Sparks12, R. W. Springer5, I. Taboada18, P. A. Toale23, Kirsten Tollefson1, I. Torres9, T. N. Ukwatta1, L. Villaseñor3, Thomas Weisgarber8, S. Westerhoff8, I. G. Wisher8, Joshua Wood6, G. B. Yodh16, P. W. Younk13, D. Zaborov12, Arnulfo Zepeda24, Hao Zhou4 
TL;DR: The High Altitude Water Cherenkov (HAWC) observatory as mentioned in this paper is an array of large water-cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band between 100 GeV and 100 TeV.

Journal ArticleDOI
TL;DR: In this article, it was shown that the fluctuations well below the proton scale are predominantly kinetic Alfven turbulence, and if present at all, the whistler fluctuations make up only a small fraction of the total energy.
Abstract: The nature of subproton scale fluctuations in the solar wind is an open question, partly because two similar types of electromagnetic turbulence can occur: kinetic Alfven turbulence and whistler turbulence. These two possibilities, however, have one key qualitative difference: whistler turbulence, unlike kinetic Alfven turbulence, has negligible power in density fluctuations. In this Letter, we present new observational data, as well as analytical and numerical results, to investigate this difference. These results show, for the first time, that the fluctuations well below the proton scale are predominantly kinetic Alfven turbulence, and, if present at all, the whistler fluctuations make up only a small fraction of the total energy.

Journal ArticleDOI
06 Dec 2013-Science
TL;DR: Observations from boreholes drilled by the Integrated Ocean Drilling Program Expedition 343 and 343T show a single major plate-boundary fault accommodated the large slip of the Tohoku-Oki earthquake rupture, as well as nearly all the cumulative interplate motion at the drill site.
Abstract: The mechanics of great subduction earthquakes are influenced by the frictional properties, structure, and composition of the plate-boundary fault. We present observations of the structure and composition of the shallow source fault of the 2011 Tohoku-Oki earthquake and tsunami from boreholes drilled by the Integrated Ocean Drilling Program Expedition 343 and 343T. Logging-while-drilling and core-sample observations show a single major plate-boundary fault accommodated the large slip of the Tohoku-Oki earthquake rupture, as well as nearly all the cumulative interplate motion at the drill site. The localization of deformation onto a limited thickness (less than 5 meters) of pelagic clay is the defining characteristic of the shallow earthquake fault, suggesting that the pelagic clay may be a regionally important control on tsunamigenic earthquakes.

Journal ArticleDOI
TL;DR: In this paper, the authors address the question of what would have happened if this powerful interplanetary event had been Earthward directed, and they find that the 23-24 July event would certainly have produced a geomagnetic storm that was comparable to the largest events of the twentieth century.
Abstract: A key goal for space weather studies is to define severe and extreme conditions that might plausibly afflict human technology. On 23 July 2012, solar active region 1520 (approx. 141 deg W heliographic longitude) gave rise to a powerful coronal mass ejection (CME) with an initial speed that was determined to be 2500+/-500 km/s. The eruption was directed away from Earth toward 125 deg W longitude. STEREO-A sensors detected the CME arrival only about 19 h later and made in situ measurements of the solar wind and interplanetary magnetic field. In this paper, we address the question of what would have happened if this powerful interplanetary event had been Earthward directed. Using a well-proven geomagnetic storm forecast model, we find that the 23-24 July event would certainly have produced a geomagnetic storm that was comparable to the largest events of the twentieth century (Dst approx. - 500 nT). Using plausible assumptions about seasonal and time-of-day orientation of the Earth's magnetic dipole, the most extreme modeled value of storm-time disturbance would have been Dst= - 1182 nT. This is considerably larger than estimates for the famous Carrington storm of 1859. This finding has far reaching implications because it demonstrates that extreme space weather conditions such as those during March of 1989 or September of 1859 can happen even during a modest solar activity cycle such as the one presently underway. We argue that this extreme event should immediately be employed by the space weather community to model severe space weather effects on technological systems such as the electric power grid.

Journal ArticleDOI
TL;DR: In this paper, a conceptual framework is proposed to reveal interplay among various marketing and non-marketing-controlled product cues, and the results reveal theoretical and managerial implications for processing multiple-quality cues in consumers' inference-making behaviors and suggest that consumers generally aggregate perceptions in more complex ways than suggested in the prior literature.
Abstract: Consumers usually infer unobservable product quality by processing multiple-quality cues in the environment. Prior research considering the simultaneous effects of marketing cues on consumer quality perceptions is sparse. Despite the growing importance of third-party information, research examining its simultaneous effects with marketing cues on consumers’ decision making is especially absent. This research, drawing on cue-diagnosticity, cue-consistency, and negativity bias theories, proposes and tests a conceptual framework to reveal interplays among various marketing- and nonmarketing-controlled product cues. The first study examines how two- and three-way interactions of high-scope (i.e., brand reputation) and low-scope marketing cues (i.e., price and warranty) affect consumer perceptions. The second study examines a set of interaction effects between third-party quality ratings and marketing cues (i.e., price and warranty) on consumers’ perceptions. Overall, the results reveal theoretical and managerial implications for processing multiple-quality cues in consumers’ inference-making behaviors and suggest that consumers generally aggregate perceptions in more complex ways than suggested in the prior literature when making global product quality evaluations. C

Journal ArticleDOI
TL;DR: The binding energies of a range of nuclei and hypernuclei with atomic number A 4 and strangeness jsj 2, including the deuteron, di-neutron, H-dibaryon and 4 He, were calculated in the limit of avor-SU(3) symmetry at the physical strange-quark mass with quantum chromodynamics as mentioned in this paper.
Abstract: The binding energies of a range of nuclei and hypernuclei with atomic number A 4 and strangeness jsj 2, including the deuteron, di-neutron, H-dibaryon, 3 He, 3 He, 4 He, 4 He, and 4 He, are calculated in the limit of avor-SU(3) symmetry at the physical strange-quark mass with quantum chromodynamics (without electromagnetic interactions). The nuclear states are extracted from Lattice QCD calculations performed with nf = 3 dynamical light quarks using an isotropic clover discretization of the quark action in three lattice volumes of spatial extent L 3:4 fm; 4:5 fm and 6:7 fm, and with a single lattice spacing b 0:145 fm.