SH44A:
Novel Instrument Techniques for Space Plasma: In Situ and Remote Sensing
Submit an Abstract to this Session
Session ID#: 31370
Session Description:
This session will focus on novel instrument techniques to observe space plasmas in a wide variety of regions in the field of Heliophysics and Planetary sciences. Challenging science targets have been advanced by emerging technologies throughout the space era, and recent technological advances provide low-cost, low-power, light-weight, high-resolution, high-accuracy, and wide-dynamic-range investigations that can enhance the technical capabilities and scientific closure of next generation missions. Abstracts are solicited that investigate and develop instruments for in-situ studies of particles (thermal, suprathermal to energetic plasmas ranging eV to MeV, and neutral gas including bulk features and mass spectrometry) and fields (electric and magnetic fields from low to high frequencies), and remote studies of energetic neutral atoms and photons (from the near infrared to x-rays).
Primary Convener: Keiichi Ogasawara, Southwest Research Institute, San Antonio, TX, United States
Conveners: John W Bonnell, University of California Berkeley, Berkeley, CA, United States, Jason A Gilbert, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States and Eric Quemerais, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France
Chairs: Jason A Gilbert, University of Michigan, Ann Arbor, MI, United States, John W Bonnell, University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States, Keiichi Ogasawara, Southwest Research Institute, San Antonio, TX, United States and Eric Quemerais, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France
OSPA Liaison: Keiichi Ogasawara, Southwest Research Institute, San Antonio, TX, United States
Abstracts Submitted to this Session:
Christopher M Cully1, Dain Galts1, Matthew Patrick1, Cooper Duffin1, April Catherine Jang1, Jared Pitzel1, Tiana Trumpour1, Michael McCarthy2 and David K Milling3, (1)University of Calgary, Calgary, AB, Canada, (2)University of Washington, Department of Earth and Space Sciences, Seattle, United States, (3)University of Alberta, Department of Physics, Edmonton, AB, Canada
Kazuo Yoshioka1, Go Murakami2, Atsushi Yamazaki2, Fuminori Tsuchiya3, Masato Kagitani4, Tomoki Kimura5 and Ichiro Yoshikawa1, (1)The University of Tokyo, Tokyo, Japan, (2)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (3)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (4)PPARC, Tohoku University, Sendai, Japan, (5)Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai, Japan
Joe H Westlake1, Ralph L McNutt Jr2, Justin Christophe Kasper3, Corina Battista1, Anthony W Case3, Corey Cochrane4, Matthew Grey1, Xianzhe Jia5, Margaret Kivelson6, Cindy Kim1, Haje Korth2, Krishan K Khurana7, Norbert Krupp8, Carol S Paty9, Elias Roussos10, Abigail M Rymer1, Michael Louis Stevens3, James A Slavin11, Howard Todd Smith2, Joachim Saur12 and David Coren13, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (5)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (6)UCLA, Los Angeles, United States, (7)University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States, (8)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (9)University of Oregon, Earth Sciences, Eugene, OR, United States, (10)Max Planck Institute for Solar System Research, Göttingen, Germany, (11)University of Michigan, Ann Arbor, MI, United States, (12)University of Cologne, Cologne, Germany, (13)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
Hui-Kuan Fang1, Alfred Bing-Chih Chen2, Charles Lin3, Ting-Jhou Wu3, Ke-Shen Liu3 and Chia-Wen Chuang3, (1)NCKU National Cheng Kung University, Tainan City, Taiwan, (2)NCKU National Cheng Kung University, Department of Physics, Tainan, Taiwan, (3)NCKU National Cheng Kung University, Tainan, Taiwan
Matthieu Berthomier, Laboratoire de Physique des Plasmas, Saint-Maur Des Fossés Cedex, France and Jean-Denis Techer, Laboratoire De Physique Des Plasmas, Paris, France
Amy R Winebarger1, Sabrina L Savage2, Ken Kobayashi2, Patrick R. Champey1, David E. McKenzie1, Leon Golub3, Paola Testa3, Katharine Reeves3, Peter Cheimets3, Jonathan W Cirtain1, Robert William Walsh4, Stephen J. Bradshaw5, Harry P Warren6, Helen E Mason7 and Giulio Del Zanna8, (1)NASA Marshall Space Flight Center, Huntsville, AL, United States, (2)NASA Marshall Space Flight Center, Huntsville, United States, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (4)University of Central Lancashire, Preston, United Kingdom, (5)Rice University, Department of Physics and Astronomy, Houston, United States, (6)Naval Research Laboratory, Washington, DC, United States, (7)University of Cambridge, Department of Applied Mathematics and Theoretical Physics, Cambridge, United Kingdom, (8)University of Cambridge, DAMTP, Cambridge, United Kingdom
Steven Christe1, Albert Y Shih1, Sam Krucker2, Lindsay Glesener3, Pascal Saint-Hilaire4, Amir Caspi5, Joel C Allred6, Marina Battaglia7, Bin Chen8, James Frederick Drake9, Dale E Gary10, Keith Goetz11, Szymon Gburek12, Brian Grefenstette13, Iain G Hannah14, Gordon Holman15, Hugh S Hudson16, Andrew R Inglis17, Jack Ireland18, Shin-nosuke Ishikawa19, James A Klimchuk6, Eduard Kontar20, Adam F Kowalski21, Anna Maria Massone22, Michele Piana23, Brian Ramsey24, Richard Schwartz15, Marek Steslicki12, Paul Turin25, Daniel Ryan15, Alexander Warmuth26, Astrid Veronig27, Nicole Vilmer28, Stephen M White29, Thomas N Woods30 and FOXSI Science Working Group, (1)NASA GSFC, Solar Physics Lab, Greenbelt, United States, (2)Space Sciences Laboratory, Berkeley, United States, (3)University of Minnesota Twin Cities, Minneapolis, United States, (4)UC Berkeley, Space Science Lab, Berkeley, United States, (5)Southwest Research Institute, Boulder, CO, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)University of Applied Sciences Northwestern Switzerland, Windisch, Switzerland, (8)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Edison, NJ, United States, (9)University of California Berkeley, Berkeley, CA, United States, (10)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (11)University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, United States, (12)Space Research Centre, Polish Academy of Sciences, Wrocław, Poland, (13)California Institute of Technology, Pasadena, United States, (14)University of Glasgow, Glasgow, United Kingdom, (15)NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States, (16)Space Sciences Laboratory, Berkeley, CA, United States, (17)Catholic University of America, Washington, United States, (18)ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States, (19)ISAS Institute of Space and Astronautical Science, Kanagawa, Japan, (20)University of Glasgow, Glasgow, G12, United Kingdom, (21)NASA Goddard Space Flight Center, Greenbelt, United States, (22)University of Genoa, Department of Mathematics, Genova, Italy, (23)University of Genoa, Department of Mathematics, Genoa, Italy, (24)NASA Marshall Space Flight Center, Huntsville, AL, United States, (25)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (26)Leibniz Institute for Astrophysics Potsdam, Potsdam, Germany, (27)University of Graz, Institute of Physics, Graz, Austria, (28)Observatoire Paris, Meudon, France, (29)Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States, (30)Laboratory for Atmospheric and Space Physics, Boulder, United States
