24 results on '"Scott England"'
Search Results
2. Climatology of Dayside E‐Region Zonal Neutral Wind Shears From ICON‐MIGHTI Observations
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Minjing Li, Yue Deng, Brian J. Harding, and Scott England
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Meteorology. Climatology ,QC851-999 ,Astrophysics ,QB460-466 - Abstract
Abstract Large vertical shears in the E‐region neutral zonal winds can lead to ion convergences and contribute to plasma irregularities, but climatological studies of vertical shears of horizontal winds in a global scale are lacking due to the limitations of data coverage. The Ionospheric Connection Explorer (ICON) Michelson Interferometer for Global High‐resolution Thermospheric Imaging (MIGHTI) has provided neutral wind observations with an unprecedented spatial coverage. In this study, the climatology of dayside E‐region neutral wind shears has been examined using 2‐years’ data (2020–2021). Specifically, the study focuses on large wind shears with a magnitude larger than 20 m/s/km, since large wind shears are more likely to cause significant perturbation in the ionosphere‐thermosphere (I‐T) system. The results show that the probability of occurrence of large shears is strongly dependent on the altitude, with the vertical profile varying with shear direction, latitude, season, and local time. In general, below 110 km altitude, large negative shears of the eastward wind are most likely to happen during summer at 8–10 LT in 25°N–40°N latitudes, showing a high probability across nearly all longitudes. Meanwhile, large positive shears tend to occur in 10°S–10°N latitudes, with peak probabilities exhibiting roughly consistent longitudinal structures across 8–10 LT in all seasons. The discrepancies between positive and negative large shear distributions underlie different global tidal influences. The large‐shear occurrence probabilities above 110 km are generally small, except in latitudes above 25°N during the winter for positive shears.
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- 2024
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3. Patchy Proton Aurora at Mars: A Global View of Solar Wind Precipitation Across the Martian Dayside From EMM/EMUS
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Michael S. Chaffin, Christopher M. Fowler, Justin Deighan, Sonal Jain, Greg Holsclaw, Andréa Hughes, Robin Ramstad, Yaxue Dong, Dave Brain, Hoor AlMazmi, Krishnaprasad Chirakkil, John Correira, Scott England, J. Scott Evans, Matt Fillingim, Rob Lillis, Fatma Lootah, Susarla Raghuram, Jim McFadden, Jasper Halekas, Jared Espley, Nick Schneider, Majd Mayyasi, Christina O. Lee, Shannon Curry, and Hessa AlMatroushi
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Mars ,aurora ,radial IMF ,Geophysics. Cosmic physics ,QC801-809 - Abstract
Abstract Proton aurora at Mars are thought to form indirectly, as a result of solar wind proton charge exchange with planetary coronal hydrogen upstream of the bow shock. This charge exchange produces beamed energetic neutral atoms that bypass the induced magnetosphere and cause spatially uniform auroral emission when they collide with the thermosphere. Here we report multiple definitive observations of spatially localized “patchy” proton aurora at Mars using the Emirates Mars Ultraviolet Spectrometer on the Emirates Mars Mission, and characterize the plasma environment during these events using contemporaneous Mars Atmosphere and Volatile EvolutioN mission measurements. Multiple mechanisms are required to explain these observations, including at times the direct deposition of solar wind plasma into the thermosphere, particularly during radial interplanetary magnetic field conditions. Much future work will be needed to assess these mechanisms and understand the impact of these auroral events on Mars atmospheric evolution.
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- 2022
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4. Emirates Mars Ultraviolet Spectrometer's (EMUS) Observation of Argon in the Martian Thermosphere
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Fatma Hussain Lootah, Justin Deighan, Matthew Fillingim, Sonal Jain, J. Scott Evans, Hessa Al Matroushi, Michael Chaffin, Gregory Holsclaw, Robert Lillis, Hour Al Mazmi, John Correira, and Scott England
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Geophysics. Cosmic physics ,QC801-809 - Abstract
Abstract The Emirates Mars Ultraviolet Spectrometer (EMUS) is a far ultraviolet spectrometer on‐board the Emirates Mars Mission's (EMM) which arrived at Mars on 9 February 2021. EMUS is designed to observe key neutral species in the Martian thermosphere (100–200 km) and exosphere (≥200 km). EMUS has observed two neutral argon (Ar) emission lines, Ar I 104.8 nm and Ar I 106.6 nm, in the thermosphere. Our interest in these emissions stem from argon's non‐reactiveness, making it a tracer for transport between the upper and lower atmosphere. We report average argon disk brightness measured by EMUS and compare them to measurements from Earth orbiting observatories. For the first time, this work investigates the variability of Ar I 106.6 nm brightness due to emission angles, solar zenith angles, solar longitudes, local times and latitudes. To contrast the behavior of inert argon we compare these results with the photochemically reactive oxygen 135.6 nm.
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- 2022
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5. EMM EMUS Observations of Hot Oxygen Corona at Mars: Radial Distribution and Temporal Variability
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Krishnaprasad Chirakkil, Justin Deighan, Michael S. Chaffin, Sonal K. Jain, Robert J. Lillis, Susarla Raghuram, Greg Holsclaw, David A. Brain, Ed Thiemann, Phil Chamberlin, Matthew O. Fillingim, J. Scott Evans, Scott England, Hessa AlMatroushi, Hoor AlMazmi, Frank Eparvier, Marko Gacesa, Nayla El‐Kork, and Shannon M. Curry
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- 2024
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6. On the Variation of Column Density Ratio ΣO/N2 in the Upper Atmosphere Using Principal Component Analysis in 2‐Dimensional Images
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Divyam Goel, Yen‐Jung J. Wu, Brian J. Harding, Colin C. Triplett, Thomas J. Immel, Chihoko Cullens, and Scott England
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- 2023
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7. Tidal Effects on the Longitudinal Structures of the Martian Thermosphere and Topside Ionosphere Observed by MAVEN
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Xiaohua Fang, Jeffrey M Forbes, Quan Gan, Guiping Liu, Scott Thaller, Stephen Bougher, Laila Andersson, Mehdi Benna, Francis Eparvier, Yingjuan Ma, David Pawlowski, Scott England, and Bruce Jakosky
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Earth Resources And Remote Sensing - Abstract
Longitudinal structures in the Martian thermosphere and topside ionosphere between 150 and 200 km altitudes are studied using in situ electron and neutral measurements from the NASA Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. Four time intervals are selected for comparison, during which MAVEN sampled similar local time (9.3–10.3 h) and latitude (near 20°S) regions but at different solar longitude positions (two near northern summer solstice, one each at northern vernal and autumnal equinoxes). Persistent and pronounced tidal oscillations characterize the ionosphere and thermosphere, whose longitudinal variations in density are generally in-phase with each other. Our analysis of simultaneous and collocated neutral and electron data provides direct observational evidence for thermosphere-ionosphere coupling through atmospheric tides. We conclude that the ionosphere is subject to modulation by upward-propagating thermal tides, via both tide-induced vertical displacement and photochemical reactions. Atmospheric tides constitute a ubiquitous and significant perturbation source to the ionospheric electron density, up to ∼15% near 200 km.
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- 2020
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8. MOSAIC: A Satellite Constellation to Enable Groundbreaking Mars Climate System Science and Prepare for Human Exploration
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Robert J. Lillis, David Mitchell, Luca Montabone, Nicholas Heavens, Tanya Harrison, Cassie Stuurman, Scott Guzewich, Scott England, Paul Withers, Mike Chaffin, Shannon Curry, Chi Ao, Steven Matousek, Nathan Barba, Ryan Woolley, Isaac Smith, Gordon R. Osinski, Armin Kleinböhl, Leslie Tamppari, Michael Mischna, David Kass, Michael Smith, Michael Wolff, Melinda Kahre, Aymeric Spiga, François Forget, Bruce Cantor, Justin Deighan, Amanda Brecht, Stephen Bougher, Christopher M. Fowler, David Andrews, Martin Patzold, Kerstin Peter, Silvia Tellmann, Mark Lester, Beatriz Sánchez-Cano, Janet Luhmann, François Leblanc, Jasper Halekas, David Brain, Xiaohua Fang, Jared Espley, Hermann Opgenoorth, Oleg Vaisberg, David Hinson, Sami Asmar, Joshua Vander Hook, Ozgur Karatekin, Aroh Barjatya, and Abhishek Tripathi
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- 2021
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9. Geophysical Research Letters
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Sonal K. Jain, Justin Deighan, Mike Chaffin, Greg Holsclaw, Rob Lillis, Matt Fillingim, J. Scott Evans, John Correira, Hessa AlMatroushi, Fatma Lootah, Scott England, Hoor AlMazmi, Ed Thiemann, Phil Chamberlin, and Frank Eparvier
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Geophysics ,Spectrometer experiment ,General Earth and Planetary Sciences ,upper-atmosphere - Abstract
We present the first continuous observations of the extreme and far ultraviolet (EUV and FUV) dayglow emissions measured by Emirates Mars Ultraviolet Spectrometer (EMUS) onboard the Emirates Mars Mission. We found excellent agreement between the previous observations from the Hopkins Ultraviolet Telescope and recent observations by EMUS both in shape and magnitude. We presented the average disk brightness of major EUV and FUV emissions for about 10 months of data from April 2021 to February 2022. The solar activity was mild/minimum during the first half of the period presented in this study, but we noticed significant day-to-day variations in the major dayglow emissions independent of solar activity, indicating possible coupling from the lower atmosphere via waves/tides. The solar activity increased significantly during the second half of the study period. Our analysis showed that all major EUV and FUV emissions are highly correlated with solar forcing as well as seasonal changes. UAE government; NASA Published version Funding for the development of the Emirates Mars Mission mission was provided by the UAE government, and to co-authors outside of the UAE by MBRSC. Ed Thiemann, Phil Chamberlin, and Frank Eparvier are supported by NASA through the MAVEN project.
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- 2022
10. First Synoptic Images of FUV Discrete Aurora and Discovery of Sinuous Aurora at Mars by EMM EMUS
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Robert J. Lillis, Justin Deighan, David Brain, Matthew Fillingim, Sonal Jain, Michael Chaffin, Scott England, Greg Holsclaw, Krishnaprasad Chirakkil, Hessa Al Matroushi, Fatma Lootah, Hoor Al Mazmi, Ed Thiemann, Frank Eparvier, Nick Schneider, and Shannon Curry
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Geophysics ,General Earth and Planetary Sciences - Published
- 2022
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11. Combined Analysis of Hydrogen and Oxygen 102.6 nm Emission at Mars
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Michael S. Chaffin, Justin Deighan, Sonal Jain, Greg Holsclaw, Hoor AlMazmi, Krishnaprasad Chirakkil, John Correira, Scott England, J. Scott Evans, Matt Fillingim, Rob Lillis, Fatma Lootah, Susarla Raghuram, Frank Eparvier, Ed Thiemann, Shannon Curry, and Hessa AlMatroushi
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Geophysics ,ultraviolet ,aeronomy ,Mars ,General Earth and Planetary Sciences - Abstract
Water is lost from the Mars upper atmosphere to space as hydrogen and oxygen, both of which can be observed in scattered ultraviolet sunlight at 102.6 nm. We present Emirates Mars Mission Emirates Mars Ultraviolet Spectrometer (EMM/EMUS) insertion orbit observations of this airglow, resolving the independent altitude contributions of H and O for the first time. We present the first airglow modeling of the complete H and O 102.6 nm system and the first 3D azimuthally symmetric modeling of the O emission, retrieving temperatures and densities typical of northern spring. Our model reproduces the emission well above 200 km, but does not incorporate partial frequency redistribution needed to reproduce the observed O brightness at lower altitudes and on the disk. These results support future EMM/EMUS science orbit retrievals of H loss and the use of 102.6 nm observations to constrain planetary atmospheres across the solar system. UAE government; EMM/MBRSC; NASA through the MAVEN mission; KU-CU-LASP Space Sci. [8474000332] Published version Funding for development of the EMM mission was provided by the UAE government, and to co-authors outside of the UAE by MBRSC. Funding for the development of the radiative transfer model was provided by EMM/MBRSC and by NASA through the MAVEN mission. SR and KC are supported by the grant 8474000332-KU-CU-LASP Space Sci.
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- 2022
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12. MAVEN Observations of the Effects of Crustal Magnetic Fields on Electron Density and Temperature in the Martian Dayside Ionosphere
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Casey L. Flynn, Marissa F. Vogt, Paul Withers, Laila Andersson, Scott England, and Guiping Liu
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- 2017
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13. Contributors
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Ercha Aa, Shane Coyle, Tong Dang, Yue Deng, Kshitija B. Deshpande, Yakov S. Dimant, Mark J. Engebretson, Scott England, Xiaohua Fang, Evgeny N. Fedorov, Alex Glocer, Lindsay V. Goodwin, Christine Gabrielse, Bea Gallardo-Lacourt, Michael D. Hartinger, Michael Hirsch, Mingwu Jin, Stephen R. Kaeppler, Hyosub Kil, Liam M. Kilcommons, Naritoshi Kitamura, Delores J. Knipp, Leslie Lamarche, Woo Kyoung Lee, Jiuhou Lei, Cissi Y. Lin, Chaoqun Liu, Huixin Liu, William J. Longley, Gang Lu, Larry R. Lyons, Yukitoshi Nishimura, Meers M. Oppenheim, Larry J. Paxton, Vyacheslav A. Pilipenko, Gareth W. Perry, Mark Redden, Cheng Sheng, Andres Spicher, Olga P. Verkhoglyadova, Chih-Ping Wang, Matthew A. Young, Yiqun Yu, Matthew D. Zettergren, Weijia Zhan, Shun-Rong Zhang, and Qingyu Zhu
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- 2022
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14. Emirates Mars Mission Characterization of Mars Atmosphere Dynamics and Processes
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Hessa Almatroushi, Hoor AlMazmi, Noora AlMheiri, Mariam AlShamsi, Eman AlTunaiji, Khalid Badri, Robert J. Lillis, Fatma Lootah, Maryam Yousuf, Sarah Amiri, David A. Brain, Michael Chaffin, Justin Deighan, Christopher S. Edwards, Francois Forget, Michael D. Smith, Michael J. Wolff, Philip R. Christensen, Scott England, Matthew Fillingim, Gregory M. Holsclaw, Sonal Jain, Andrew R. Jones, Mikki Osterloo, Bruce M. Jakosky, Janet G. Luhmann, and Roland M. B. Young
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Space and Planetary Science ,Astronomy and Astrophysics - Abstract
The Emirates Mars Mission (EMM) – Hope Probe – was developed to understand Mars atmospheric circulation, dynamics, and processes through characterization of the Mars atmosphere layers and its interconnections enabled by a unique high-altitude (19,970 km periapse and 42,650 km apoapse) low inclination orbit that will offer an unprecedented local and seasonal time coverage over most of the planet. EMM has three scientific objectives to (A) characterize the state of the Martian lower atmosphere on global scales and its geographic, diurnal and seasonal variability, (B) correlate rates of thermal and photochemical atmospheric escape with conditions in the collisional Martian atmosphere, and (C) characterize the spatial structure and variability of key constituents in the Martian exosphere. The EMM data products include a variety of spectral and imaging data from three scientific instruments measuring Mars at visible, ultraviolet, and infrared wavelengths and contemporaneously and globally sampled on both diurnal and seasonal timescale. Here, we describe our strategies for addressing each objective with these data in addition to the complementary science data, tools, and physical models that will facilitate our understanding. The results will also fill a unique role by providing diagnostics of the physical processes driving atmospheric structure and dynamics, the connections between the lower and upper atmospheres, and the influences of these on atmospheric escape.
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- 2021
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15. Modeling Occupational Fingernail Onycholysis Disorders in the Population of US Astronauts Who Have Engaged in Extravehicular Activity
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Christopher R, Reid, Jacqueline M, Charvat, Shane M, Mcfarland, Jason R, Norcross, Elizabeth, Benson, Scott, England, and Sudhakar, Rajulu
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Behavioral Neuroscience ,Human Factors and Ergonomics ,Applied Psychology - Abstract
Objectives Spacesuits are designed to be reliable personal spacecraft that preserve the life and well-being of the astronaut from the extremes of space. However, materials, operating pressures, and suit design requirements often result in a risk of musculoskeletal discomfort and injury to various areas of the body. In particular, this investigation looked at fingernails and their risk of developing onycholysis. Methods An onycholysis literature review was followed by a retrospective analysis of injury characteristics, astronaut suited training and spaceflight events, hand anthropometry, glove sizing, and astronaut demographics. Multiple logistic regression was used to assess the likelihood of onycholysis occurrence by testing potential risk variables against the dataset compiled from the retrospective data mining. Results The duration of event exposure, type of glove used, distance (delta) between the fingertip and the tip of the glove, sex, and age were found to be significantly related to occurrence of onycholysis (whether protective or injurious). Conclusion An initial risk formula (model) for onycholysis was developed as a result of this investigation. In addition to validation through a future study, further improvement to this onycholysis equation and spacesuit discomfort and injury in general can be aided by future investigations that lead to better definition of the threshold between safe and risky exposure for each type of risk factor. Application This work described a potential method that can be used for EVA spacesuit glove onycholysis injury risk analysis for either iterative glove design or between glove comparisons, such as during a product downselect process.
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- 2021
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16. Is distance learning really a substitute for on-site learning? Perceptions of faculty who teach undergraduate economics using both formats
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Dawn Richards Elliott, Timothy A. Wunder, and Scott England
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Cooperative learning ,Blended learning ,Computer science ,Teaching and learning center ,Pedagogy ,Active learning ,Mathematics education ,Educational technology ,Open learning ,Experiential learning ,Learning sciences ,Education - Abstract
This study draws from the divergent conclusions found in distance learning studies in general compared to those done within economics. Most studies of distance learning report no difference in learning outcomes compared to in class instruction. This is challenged by controlled studies within economics which report a negative difference in distance learning. Economics faculties who have taught the same undergraduate courses using both methods were surveyed. They perceive a learning advantage in onsite learning but not in learning outcomes. What explains this anomaly and what does it suggest about the growing use of distance learning in higher education? The survey suggests that differences in learning outcomes may reflect differences in evaluative techniques. This implies that distance and onsite learning are not perfect substitutes and suggests that learning tradeoffs must be managed. One example relates to faculty training on the importance of standardizing evaluative techniques.
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- 2013
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17. Application of Strength Requirements to Complex Loading Scenarios
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Sudhakar Rajulu and Scott England
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Flexibility (engineering) ,Engineering ,Bionics ,business.industry ,media_common.quotation_subject ,Human spaceflight ,Fidelity ,Human factors integration ,Space (commercial competition) ,Range (aeronautics) ,Systems engineering ,business ,Contingency ,Simulation ,media_common - Abstract
NASA’s endeavors in human spaceflight rely on extensive volumes of human-systems integration requirements to ensure mission success. These requirements protect space hardware accommodation for the full range of potential crewmembers, but cannot cover every possible action and contingency in detail. This study was undertaken in response to questions from various strength requirement users who were unclear how to apply idealized strength requirements that did not map well to the complex loading scenarios that crewmembers would encounter. Three of the most commonly occurring questions from stakeholders were selected to be investigated by human testing and human modeling. Preliminary findings indicate that deviation from nominal postures can affect compliance with strength requirements positively or negatively, depending on the nature of the deviation. Human modeling offers some avenues for quickly addressing requirement verification questions, but is limited by the fidelity of the model and environment.
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- 2016
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18. The Effects of Extravehicular Activity (EVA) Glove Pressure on Tactility
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Miranda Mesloh, Sudhakar Rajulu, Scott England, Elizabeth Benson, and Shelby Thompson
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Colloid and Surface Chemistry ,Materials science ,InformationSystems_INFORMATIONINTERFACESANDPRESENTATION(e.g.,HCI) ,law ,Acoustics ,Space suit ,Extravehicular Mobility Unit ,Physical and Theoretical Chemistry ,Load cell ,GeneralLiterature_MISCELLANEOUS ,Simulation ,Tactile stimuli ,law.invention - Abstract
The purpose of the current study was to quantify finger tactility, while wearing a Phase VI Extravehicular Activity (EVA) glove. Subjects were fully suited in an Extravehicular Mobility Unit (EMU) suit. Data was collected under three conditions: bare-handed, gloved at 0 psi, and gloved at 4.3 psi. In order to test tactility, a series of 30 tactile stimuli (bumps) were created that varied in both height and width. With the hand obscured, subjects applied pressure to each bump until detected tactilely. The amount of force needed to detect each bump was recorded using load cells located under a force-plate. The amount of force needed to detect a bump was positively related to width, but inversely related to height. In addition, as the psi of the glove increased, more force was needed to detect the bump. In terms of application, it was possible to determine the optimal width and height a bump needs to be for a specific amount of force applied for tactility.
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- 2011
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19. Fact Based Economic Education
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Scott England, Thomas Kemp, and Timothy A. Wunder
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Economics and Econometrics ,media_common.quotation_subject ,Information literacy ,Field (Bourdieu) ,Economics education ,Economic literacy ,General Business, Management and Accounting ,Literacy ,Critical literacy ,Work (electrical) ,ComputingMilieux_COMPUTERSANDEDUCATION ,Mathematics education ,Criticism ,Sociology ,Social science ,media_common - Abstract
Current economic literacy tests focus on theory while almost totally ignoring the economy itself. This study analyzes how well we are teaching students empirical facts. Most agree that economic literacy is a laudable goal and current literacy pedagogy is centered on teaching students how to "think like economists." The authors do not intend to imply criticism to current literacy campaigns; rather this work is intended to open a discussion within the field about the need to also introduce students to some basic economic facts. This study is based upon surveys given to several hundred introductory economics students and tabulates some preliminary observations about their level of fact attainment.
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- 2009
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20. Urban and regional distinctions for aggregating time series data
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Scott England, Harvey Cutler, and Stephan Weiler
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Cointegration ,Economies of agglomeration ,Geography, Planning and Development ,Monetary policy ,Econometrics ,Economics ,Pairwise comparison ,Optimal distinctiveness theory ,Economic geography ,Environmental Science (miscellaneous) ,Time series ,North American Industry Classification System - Abstract
This article argues that using either the SIC or NAICS one-digit classifications as a method of aggregating two- and three-digit time series data can ignore important regional characteristics. We present a pairwise cointegration approach of aggregation where the aggregated sectors can vary widely across regions. By systematically constructing region-specific sectors from more detailed industries, we find that the level of agglomeration across rural and urban areas can affect the composition and number of local sectors in a region. We use the results pointing to rural/urban geographic distinctiveness to further consider the Carlino and Defina (1998, 1999) finding that monetary policy has disparate effects across regions in the U.S.
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- 2007
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21. Determining Regional Structure through Cointegration
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Stephan Weiler, Harvey Cutler, and Scott England
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Structure (mathematical logic) ,Cointegration ,Process (engineering) ,Geography, Planning and Development ,Aggregate (data warehouse) ,Metropolitan area ,Regional ,Core (game theory) ,jel:R32 ,Economics ,Econometrics ,Pairwise comparison ,jel:R11 ,Earth-Surface Processes - Abstract
Evaluating regional industrial structures remains an inexact process as traditional aggregation schemes often lump superficially similar but behaviorally distinct industries together. We use pairwise cointegration methods to apply econometric criteria to aggregate detailed industries into behaviorally similar sectors. Based on these aggregations, cointegration guides the proper specification of a regional system to analyze the export versus local nature of core sectors. These methodologies are applied to Denver metropolitan data to demonstrate their utility. The findings indicate previous aggregation schemes are statistically inferior to those generated by this paper’s approach.
- Published
- 2003
22. Use of Traditional and Novel Methods to Evaluate the Influence of an EVA Glove on Hand Performance
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Elizabeth Benson, Sudhakar ajulu, Shelby Thompson, Miranda Mesloh, and Scott England
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Engineering ,InformationSystems_INFORMATIONINTERFACESANDPRESENTATION(e.g.,HCI) ,law ,business.industry ,Space suit ,Thermal Micrometeoroid Garment ,business ,GeneralLiterature_MISCELLANEOUS ,Simulation ,law.invention - Abstract
The gloved hand is one of an astronaut s primary means of interacting with the environment, and any restrictions imposed by the glove can strongly affect performance during extravehicular activity (EVA). Glove restrictions have been the subject of study for decades, yet previous studies have generally been unsuccessful in quantifying glove mobility and tactility. Past studies have tended to focus on the dexterity, strength, and functional performance of the gloved hand; this provides only a circumspect analysis of the impact of each type of restriction on the glove s overall capability. The aim of this study was to develop novel capabilities to provide metrics for mobility and tactility that can be used to assess the performance of a glove in a way that could enable designers and engineers to improve their current designs. A series of evaluations were performed to compare unpressurized and pressurized (4.3 psi) gloved conditions with the ungloved condition. A second series of evaluations were performed with the Thermal Micrometeoroid Garment (TMG) removed. This series of tests provided interesting insight into how much of an effect the TMG has on gloved mobility - in some cases, the presence of the TMG restricted glove mobility as much as pressurization did. Previous hypotheses had assumed that the TMG would have a much lower impact on mobility, but these results suggest that an improvement in the design of the TMG could have a significant impact on glove performance. Tactility testing illustrated the effect of glove pressurization, provided insight into the design of hardware that interfaces with the glove, and highlighted areas of concern. The metrics developed in this study served to benchmark the Phase VI EVA glove and to develop requirements for the next-generation glove for the Constellation program.
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- 2010
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23. The Effects of Extravehicular Activity (EVA) Glove Pressure on Hand Strength
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Miranda Mesloh, Scott England, Elizabeth Benson, Shelby Thompson, and Sudhakar Rajulu
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- 2010
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24. Functional Mobility Testing: A Novel Method To Establish Human-System Interface Design Requirements
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Elizabeth Benson, Sudhakar Rajulu, and Scott England
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Data processing ,Engineering ,business.industry ,Space suit ,Space Shuttle ,Type design ,Space (commercial competition) ,Space exploration ,law.invention ,law ,International Space Station ,Systems engineering ,System integration ,business ,Simulation - Abstract
Across all fields of human-system interface design it is vital to posses a sound methodology dictating the constraints on the system based on the capabilities of the human user. These limitations may be based on strength, mobility, dexterity, cognitive ability, etc. and combinations thereof. Data collected in an isolated environment to determine, for example, maximal strength or maximal range of motion would indeed be adequate for establishing not-to-exceed type design limitations, however these restraints on the system may be excessive over what is basally needed. Resources may potentially be saved by having a technique to determine the minimum measurements a system must accommodate. This paper specifically deals with the creation of a novel methodology for establishing mobility requirements for a new generation of space suit design concepts. Historically, the Space Shuttle and the International Space Station vehicle and space hardware design requirements documents such as the Man-Systems Integration Standards and International Space Station Flight Crew Integration Standard explicitly stated that the designers should strive to provide the maximum joint range of motion capabilities exhibited by a minimally clothed human subject. In the course of developing the Human-Systems Integration Requirements (HSIR) for the new space exploration initiative (Constellation), an effort was made to redefine the mobility requirements in the interest of safety and cost. Systems designed for manned space exploration can receive compounded gains from simplified designs that are both initially less expensive to produce and lighter, thereby, cheaper to launch.
- Published
- 2008
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