bluuebunny/crossref_metadata_2025_split huggingface dataset:
Preparing for a Foreign Animal Disease Outbreak Using a Novel Tabletop Exercise
Authors: Linskens Eric J. , Neu Abby E. , Walz Emily J. , St. Charles Kaitlyn M. , Culhane Marie R. , Ssematimba Amos , Goldsmith Timothy J. , Halvorson David A. , Cardona Carol J. 
Published: September 2018

AbstractIntroductionForeign animal disease (FAD) outbreaks can have devastating impacts, but they occur infrequently in any specific sector anywhere in the United States (US). Training to proactively discuss implementation of control and prevention strategies are beneficial in that they provide stakeholders with the practical information and educational experience they will need to respond effectively to an FAD. Such proactive approaches are the mission of the Secure Food System (SFS; University of Minnesota; St. Paul, Minnesota USA).MethodsThe SFS exercises were designed as educational activities based on avian influenza (AI) outbreaks in commercial poultry scenarios. These scenarios were created by subject matter experts and were based on epidemiology reports, risk pathway analyses, local industry practices, and site-specific circumstances. Target audiences of an exercise were the groups involved in FAD control: animal agriculture industry members; animal health regulators; and diagnosticians. Groups of industry participants seated together at tables represented fictional poultry premises and were guided by a moderator to respond to an on-farm situation within a simulated outbreak. The impact of SFS exercises was evaluated through interviews with randomized industry participants and selected table moderators. Descriptive statistics and qualitative analyses were performed on interview feedback.ResultsEleven SFS exercises occurred from December 2016 through October 2017 in multiple regions of the US. Exercises were conducted as company-wide, state-wide, or regional trainings. Nine were based on highly pathogenic avian influenza (HPAI) outbreaks and two focused on outbreaks of co-circulating HPAI and low pathogenicity avian influenza (LPAI). Poultry industry participants interviewed generally found attending an SFS exercise to be useful. The most commonly identified benefits of participation were its value to people without prior outbreak experience and knowledge gained about Continuity of Business (COB)-permitted movement. After completing an exercise, most participants evaluated their preparedness to respond to an outbreak as somewhat to very ready, and more than one-half reported their respective company or farms had discussions or changed actions due to participation.Conclusion:Evaluation feedback suggests the SFS exercises were an effective training method to supplement preparedness efforts for an AI outbreak. The concept of using multi-faceted scenarios and multiple education strategies during a tabletop exercise may be translatable to other emergency preparedness needs.LinskensEJ, NeuAE, WalzEJ, St. CharlesKM, CulhaneMR, SsematimbaA, GoldsmithTJ, HalvorsonDA, CardonaCJ. Preparing for a foreign animal disease outbreak using a novel tabletop exercise. Prehosp Disaster Med. 2018;33(6):640–646.
Impact of Patients Presenting with Alcohol and/or Drug Intoxication on In-Event Health Care Services at Mass-Gathering Events: An Integrative Literature Review
Authors: Bullock Makayla , Ranse Jamie , Hutton Alison 
Published: September 2018

AbstractBackgroundThere is a growing body of literature relating to mass-gathering events. A common thread amongst this literature, particularly the literature relating to music festivals, is the incidence of patients presenting with substance and/or alcohol intoxication. However, the impact of alcohol and/or drugs on the provision of in-event health care services has not been explored in detail.AimThe goal of this review was to develop an understanding of the impact of alcohol and/or drugs on in-event health care services at mass-gathering events.MethodThis paper used integrative review as a methodology. The articles included in this literature review were sourced by searching databases inclusive of Medline (Ovid; US National Library of Medicine, National Institutes of Health; Bethesda, Maryland USA), Scopus (Elsevier; Amsterdam, Netherlands), PsycINFO (Ovid; American Psychological Association; Washington DC, USA), and Pub Med (National Center for Biotechnology Information, National Institutes of Health; Bethesda, Maryland USA). Identified manuscripts that met the inclusion criteria were thematically analyzed.ResultsIn total, 12 manuscripts met the inclusion criteria for this review. A thematic analysis of these manuscripts identified three main themes: (i) predictive factors, (ii) patient presentation rates, and (iii) levels of care.Conclusion:Substance use and/or intoxication can place a strain on in-event medical services at mass-gathering events. Of the various types of mass-gathering events, music festivals appear to be the most affected by substance use and intoxication.BullockM, RanseJ, HuttonA.Impact of patients presenting with alcohol and/or drug intoxication on in-event health care services at mass-gathering events: an integrative literature review. Prehosp Disaster Med. 2018;33(5):539–542.
Compact ultra-wideband bandpass-response power divider with high-frequency selectivity
Authors: Guo Song , Song Kaijun , Zhou Yedi , Fan Yong 
Published: September 2018

AbstractThe ultra-wideband bandpass-response power divider with high-frequency selectivity is presented in this paper. This power divider consists of an impedance transformer, a filter network, and two isolation resistors. In order to realize the ultra-wideband filtering performance, parallel coupling lines and parallel open-circuit branches are applied to the second impedance converter. A resistor is added to the ends of the coupling lines to achieve good isolation and output return loss. The equivalent-circuit method is employed to analyze the presented power divider. The power divider, working at 3.45–8.29 GHz, is designed and fabricated. Two transmission zeros are generated at 2.8 and 9 GHz, respectively, and the out-of-band suppression is >13 dB. The measured results are in good agreement with the simulation ones.
Decline in Surface Melt Duration on Larsen C Ice Shelf Revealed by The Advanced Scatterometer (ASCAT)
Authors: Bevan Suzanne Louise , Luckman Adrian John , Kuipers Munneke Peter , Hubbard Bryn , Kulessa Bernd , Ashmore David William 
Published: September 2018

Surface melting has been contributing to the surface lowering and loss of firn air content on Larsen C Ice Shelf since at least the mid‐1990s. Where the amount of melting and refreezing is significant, the firn can become impermeable and begin to support ponds of surface meltwater such as have been implicated in ice shelf collapse. Although meteorological station data indicated an increase in melt on the Antarctic Peninsula over the second half of the 20th century, the existing Ku‐band Quick Scatterometer (QuikSCAT) time series is too short (1999–2009) to detect any significant 21st century trends. Here we investigate a longer 21st century period by extending the time series to 2017 using the C‐band Advanced Scatterometer (ASCAT). We validate our recent observations with in situ weather station data and, using a firn percolation model, explore the sensitivity of scatterometry to water at varying depths in the firn. We find that active microwave C‐band (5.6‐cm wavelength) instruments can detect water at depths of up to 0.75 m below a frozen firn layer. Our longer scatterometry time series reveals that Larsen C Ice Shelf has experienced a decrease in melt season length of 1–2 days per year over the past 18 years consistent with decreasing summer air temperatures. Only in western inlets, where föhn winds drive melt, has the annual melt duration increased during this period.
Radiation Belt Slot Region Filling Events: Sustained Energetic Precipitation Into the Mesosphere
Authors: Kavanagh Andrew J. , Cobbett Neil , Kirsch Peter 
Published: September 2018

AbstractPrecipitation of energetic electrons to the atmosphere is both a loss mechanism for radiation belt particles and a means by which the geospace environment influences the Earth's atmosphere; thus, it is important to fully understand the extent of this precipitation. A set of polar orbiting satellites have been used to identify periods when energetic charged particles fill the slot region between the inner and outer radiation belts. These suggest that electrons with energies >30 keV penetrate this region, even under levels of modest geomagnetic activity. Those events with sufficient fluxes of particles produce enough ionization to be detected by a ground‐based radar in Antarctica; this precipitation lasts for ~10 days on average. Analysis of these data reveals that the average precipitation penetrates to the stratopause (~55‐km altitude). For some (if not all) of these events, the likely cause of the most energetic precipitation is an interaction between (relativistic) electrons and plasmaspheric hiss leading to little, if no, local time variation in precipitation. This does not preclude a longitudinal effect given that all radar measurements are fixed in longitude. During winter months the radar is under the stable southern polar atmospheric vortex. This transports atmospheric species to lower altitudes including the ozone destroying chemicals that are produced by energetic precipitation. Thus, the precipitation from the slot region in the Southern Hemisphere will likely contribute to the destruction of ozone and changes to atmospheric heat balance and chemistry; more work is required to determine the true impact of these events.
Recent Developments in Our Knowledge of Inner Magnetosphere‐Ionosphere Convection
Authors: Kunduri B. S. R. , Baker J. B. H. , Ruohoniemi J. M. , Sazykin S. , Oksavik K. , Maimaiti M. , Chi P. J. , Engebretson M. J. 
Published: September 2018

AbstractPlasma convection in the coupled inner magnetosphere‐ionosphere is influenced by different factors such as neutral winds, penetration electric fields, and polarization electric fields. Several crucial insights about the dynamics in the region have been derived by interpreting observations in conjunction with numerical simulations, and recent expansion in ground‐ and space‐based measurements in the region along with improvements in theoretical modeling has fueled renewed interest in the subject. In this paper we present a comprehensive review of the literature with an emphasis on studies since 2012 relevant to the National Science Foundation Geospace Environment Modeling program. We cover four specific areas: (1) the subauroral polarization stream, (2) penetration electric fields, (3) the disturbance dynamo, and (4) quiet time subauroral convection. We summarize new observations and resulting insights relevant to each of these topics and discuss various outstanding issues and unanswered questions.
Multiscale Analysis of Spatiotemporal Relationship Between Injection and Seismicity in Oklahoma
Authors: Haffener Jackson , Chen Xiaowei , Murray Kyle 
Published: September 2018

AbstractMany previous studies have suggested that wastewater disposal is the most probable factor affecting increased seismicity in Oklahoma since 2009. While this relationship is clear at the state scale, a systematic quantitative analysis of the spatiotemporal relationships between injection and seismicity is needed. We first apply multiscale analyses to assess the temporal correlation between injection rate and seismicity rate at a range of different grid sizes, which demonstrate clear temporal correlations within the two main seismic regions at variable time delays. The time delay variability decreases with larger grid sizes, whereby the average time delay ranges from 150 to 220 days. The average time delay at large scales is consistent with inferred large‐scale diffusive migration away from areas of high injection rates with diffusivities of 0.5 to 2.0 m2/s. The inferred large‐scale diffusivities are consistent with an expected range of diffusivity within the Arbuckle Group where wastewater disposals are occurring. However, individual earthquake clusters have diffusivities that are about one to two orders lower than the large‐scale models. We interpret this as a manifestation of a two‐layered diffusion model with high diffusivity within the injection layer above basement, which facilitates stress transfer at a larger spatial footprint, triggering seismic slip at multiple seismogenic faults within the crystalline basement with low diffusivity, similar to fluid‐driven clusters in other tectonic regions.
Time Dependence of Passive Degassing at Volcán Popocatépetl, Mexico, From Infrared Measurements: Implications for Gas Pressure Distribution and Lava Dome Stability
Authors: Hyman David M. , Bursik Marcus I. , Legorreta Paulín Gabriel 
Published: September 2018

AbstractThe transport and storage of gas within lava domes is critical to their stability or explosivity. To analyze gas flow through these systems, degassing from Volcán Popocatépetl, Mexico, is studied here. Short‐duration (hours) passive degassing at Popocatépetl is dominated by oscillating components with periods between 100 and 1,000 s in agreement with similar measurements across a range of other volcanic systems. Over these timescales, porous gas flow through an idealized dome obeys a nonlinear diffusion equation. Approximate solutions contain series of diffusive pressure waves which decay to a steep boundary layer near the dome surface. Wave behavior is governed by the oscillation period and dome rock permeability, acting as a low‐pass filter on flux oscillations. This may explain the weakness of higher‐frequency (>0.01 Hz) oscillations in the Popocatépetl degassing data. These waves are shown to significantly modify the dome effective strength. For ∼100‐m‐radius domes, the pore pressure is comparable to the overburden, and the total strength of the dome is dominated by tensile strength. The pressure in smaller domes (≪100 m) dominates and may induce failure. This may explain observations of extrusion and destruction cycling during dome‐producing eruptions. The difference between pore pressure and overburden exhibits a shallow (outermost 5–25%), high‐pressure layer which changes in size, shape, and overpressure magnitude throughout oscillations. Linear governing equations assumed by previous studies underestimate the pore pressure distribution and do not capture this shallow layer. Recognition of this layer allows for better understanding of the destabilization or explosion of pressurized lava domes.
Magnetic Mineral Diagenesis in a High Temperature and Deep Methanic Zone in Izu Rear Arc Marine Sediments, Northwest Pacific Ocean
Authors: Kars Myriam , Musgrave Robert J. , Hoshino Tatsuhiko , Jonas Ann‐Sophie , Bauersachs Thorsten , Inagaki Fumio , Kodama Kazuto 
Published: September 2018

AbstractMagnetic mineral diagenesis is an important process in sediments that is responsible for the partial or total destruction of records of Earth's magnetic field variations and also plays an important part in iron and sulfur cycling. A rock magnetic study has been carried out at International Ocean Discovery Program Expedition 350 Site U1437 in the Izu Bonin rear arc to investigate magnetic mineral diagenesis in deeply buried sediments from ~775 to ~1,002 m below sea floor (mbsf) with burial temperatures ranging from ~67 to 85 °C. Nonsteady state geochemical environments occur within an unusual deep methanic zone (below 850 mbsf) because of a release of sulfate below the shallow sulfate reduction zone. A drastic decline in magnetic susceptibility and remanence is observed at ~850 mbsf due to a decrease in ferrimagnetic iron oxide contents. Reduction of (titano)‐magnetite and pyritization occur at this inferred deep sulfate‐methane transition zone. Below ~850 mbsf, lower magnetic mineral contents coincide with further methane release. Geochemical analyses support a change in redox conditions and secondary precipitation of iron sulfides and carbonates in the methane‐rich zone. Magnetic mineral alteration is enhanced in zones where methane accumulates underneath low porosity intervals that act as seals. Although geochemical processes due to methane occurrence are likely dominant, more than one mechanism, possibly involving microbial activity, is probably responsible for the observed magnetic mineral assemblage changes.
A Transfer Function Between Line‐of‐Sight Gravity Difference and GRACE Intersatellite Ranging Data and an Application to Hydrological Surface Mass Variation
Authors: Ghobadi‐Far Khosro , Han Shin‐Chan , Weller Steven , Loomis Bryant D. , Luthcke Scott B. , Mayer‐Gürr Torsten , Behzadpour Saniya 
Published: September 2018

AbstractWe develop a transfer function to determine in situ line‐of‐sight gravity difference (LGD) directly from Gravity Recovery and Climate Experiment (GRACE) range‐acceleration measurements. We first reduce GRACE data to form residual range‐acceleration referenced to dynamic orbit computed with a reference gravity field and nonconservative force data. Thus, the residuals and the corresponding LGD data reflect time‐variable gravity signals. A transfer function is designed based on correlation‐admittance spectral analysis. The correlation spectrum shows that residual range‐acceleration and LGD are near‐perfectly correlated for frequencies >5 cycles‐per‐revolution. The admittance spectrum quantifies that the LGD response to range‐acceleration is systematically larger at lower frequencies, due to the increased contribution of centrifugal acceleration. We find that the correlation and admittance spectra are stationary (i.e., are independent of time, satellite altitude, and gravity strength) and, therefore, can be determined a priori with high fidelity. We determine the spectral transfer function and the equivalent time domain filter. Using both synthetic and actual GRACE data, we demonstrate that in situ LGD can be estimated via the transfer function with an estimation error of 0.15 nm/s2, whereas the actual GRACE data error is around 1.0 nm/s2. We present an application of LGD data to surface water storage changes in large basins such as Amazon, Congo, Parana, and Mississippi by processing 11 years of GRACE data. Runoff routing models are calibrated directly using LGD data. Our technique demonstrates a new way of using GRACE data by forward modeling of various geophysical models and in‐orbit comparison with such GRACE in situ data.
Moment Tensors of Induced Microearthquakes in The Geysers Geothermal Reservoir From Broadband Seismic Recordings: Implications for Faulting Regime, Stress Tensor, and Fluid Pressure
Authors: Yu Changpeng , Vavryčuk Václav , Adamová Petra , Bohnhoff Marco 
Published: September 2018

AbstractFull moment tensors of 1,421 microearthquakes in The Geysers geothermal field were calculated using waveform data from a field‐wide broadband network and the approach based on the principal component analysis. Spatial characteristics of faulting regime, stress tensor and the isotropic component (ISO) of moment tensors were investigated. The studied events form different clusters dominated by normal faults (NF) and strike‐slip (SS) faults, respectively. The SS‐dominated clusters are related to the SS stress state observed in the southwestern side of the field where two NW‐SE trending fault zones exist. Increasing proportions of SS faults were observed near the shallow and deep parts of the NF‐dominated clusters. Temperature differences between the upper and lower parts of the reservoir do not change the overall stress states of clusters. The stress ratios in the NW part are much smaller than in the SE part of the field. The retrieved ISOs range between −5% and 25% for 96% of events. The average percentages of positive ISOs are correlated with the average injection rates in different clusters, and keep an increasing trend with depth below the main injection interval. Only 10% of events show negative ISO and are mainly constrained within the depth range of steam extraction. The proportion of events with negative ISO suggests much weaker seismic responses of the steam extraction than the water injection. The spatial variations of the ISO percentage do not follow the seismicity variations as the ISO is more sensitive to the pressure changes related to the fluid injection and migration.
Grid Mapping the Northern Plains of Mars: A New Overview of Recent Water‐ and Ice‐Related Landforms in Acidalia Planitia
Authors: Orgel Csilla , Hauber Ernst , van Gasselt Stephan , Reiss Dennis , Johnsson Andreas , Ramsdale Jason D. , Smith Isaac , Swirad Zuzanna M. , Séjourné Antoine , Wilson Jack T. , Balme Matthew R. , Conway Susan J. , Costard Francois , Eke Vince R. , Gallagher Colman , Kereszturi Ákos , Łosiak Anna , Massey Richard J. , Platz Thomas , Skinner James A. , Teodoro Luis F. A. 
Published: September 2018

AbstractWe used a grid‐mapping technique to analyze the distribution of 13 water‐ and ice‐related landforms in Acidalia Planitia as part of a joint effort to study the three main basins in the northern lowlands of Mars, that is, Acidalia, Utopia, and Arcadia Planitiae. The landforms were mapped at full Context Camera resolution along a 300‐km‐wide strip from 20°N to 84°N. We identified four landform assemblages: (1) Geologically recent polar cap (massive ice), which superposes the latitude‐dependent mantle (LDM) (LA1); (2) ice‐related landforms, such as LDM, textured terrain, small‐scale polygons, scalloped terrain, large‐scale viscous flow features, and gullies, which have an overlapping distribution (LA2); (3) surface features possibly related to water and subsurface sediment mobilization (LA3; kilometer‐scale polygons, large pitted mounds, small pitted mounds, thumbprint terrain); and (4) irregularly shaped pits with raised rims on equator‐facing slopes. Pits are likely the result of an energetic release of volatiles (H2O, CO2, and CH4), rather than impact‐, volcanism‐, or wind‐related processes. LDM occurs ubiquitously from 44°N to 78°N in Acidalia Planitia. Various observations suggest an origin of air fall deposition of LDM, which contains less ice in the uppermost tens of meters in Acidalia Planitia than in Arcadia and Utopia Planitiae. However, LDM may be thicker and more extended in the past in Acidalia Planitia. The transition between LDM‐free terrain and LDM is situated further north than in Utopia and Arcadia Planitiae, suggesting different past and/or present climatic conditions among the main basins in the northern lowlands.