SM51A:
Processes That Couple Inner Magnetospheric Plasma Populations II Posters
Submit an Abstract to this Session
Session ID#: 22666
Session Description:
The Earth’s inner magnetosphere has three primary plasma populations: the “thermal" particles in the eV energy range, the “hot” particles in the keV energy range, and the “energetic” particles in the MeV range. These populations are not isolated but rather continually interact with each other. The hot plasma dominates the particle pressure and therefore the electric and magnetic distortions, not only the large-scale field configuration but also the free energy for plasma wave excitation. The thermal plasma dominates the plasma mass density and therefore sets the underlying conditions for wave excitation and propagation. Because of their fast drift periods, the energetic particles are excellent tracers of coupling, providing a diagnostic measurement that integrates all processes around their drift path. This session welcomes presentations of research on the processes that couple inner magnetospheric plasma populations, including data analysis studies, numerical assessments, theoretical examinations, and any combination of these methods.
Primary Convener: Michael Warren Liemohn, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
Conveners: Yiqun Yu, Beihang University, Beijing, China, Colby Lemon, The Aerospace Corporation, El Segundo, United States and Jichun Zhang, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States
Chairs: Jichun Zhang, University of New Hampshire, Durham, NH, United States and Colby Lemon, The Aerospace Corporation, El Segundo, United States
OSPA Liaison: Yiqun Yu, Beihang University, Beijing, China
Abstracts Submitted to this Session:
Shichen Bai1, Quanqi Shi2, Anmin Tian1, Motoharu Nowada3, Alex W Degeling2, Xu-Zhi Zhou4, Qiugang Zong5, Jonathan Rae6, Suiyan Fu5, Hui Zhang7, Zuyin Pu5 and Andrew Neil Fazakerley8, (1)Shandong University at Weihai, Institute of Space Science, Weihai, China, (2)Shandong University at Weihai, Weihai, China, (3)Tucson, AZ, United States, (4)Peking University, Institute of space physics and applied technology, Beijing, China, (5)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (6)University College London, Mullard Space Science Laboratory, London, United Kingdom, (7)University of Alaska Fairbanks, Physics Department & Geophysical Institute, Fairbanks, AK, United States, (8)Mullard Space Science Lab., Dorking, United Kingdom
Katsuki Nishi, Nagoya University, Nagoya, Japan and Shiokawa Kazuo, ISEE, Nagoya University, Nagoya, Japan
Nikita Aseev1, Yuri Shprits2, Alexander Drozdov3, Adam C Kellerman4 and Dedong Wang2, (1)German Research Centre for Geosciences, Potsdam, Germany, (2)GFZ German Research Centre for Geosciences, Potsdam, Germany, (3)University of California Los Angeles, Los Angeles, United States, (4)University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States
Junhyun Lee1, Ensang Lee2, Khan-Hyuk Kim2, Dong-Hun Lee3, Jaejin Lee4 and Junga Hwang4, (1)Kyung Hee University, School of Space Research, Yongin, Korea, Republic of (South), (2)Kyung Hee University, School of Space Research, Yongin, South Korea, (3)Kyung Hee University, Yongin, Korea, Republic of (South), (4)KASI Korea Astronomy and Space Science Institute, Daejeon, South Korea
Cristian Ferradas1, Geoffrey D Reeves2, Jichun Zhang3, Harlan E Spence4, Lynn M Kistler5, Brian Larsen2, Ruth M. Skoug6 and Herbert O Funsten2, (1)New Mexico Consortium, Los Alamos, United States, (2)Los Alamos National Laboratory, Los Alamos, NM, United States, (3)University of New Hampshire, Durham, NH, United States, (4)Solar System Exploration Research Virtual Institute, NASA Ames Research Center, Moffett Field, CA, United States, (5)Univ New Hampshire, Durham, United States, (6)Los Alamos National Laboratory, Los Alamos, United States
Elizabeth Carlisle, Eric Donovan and Brian J Jackel, University of Calgary, Calgary, AB, Canada
Forrest Mozer1, Oleksiy V Agapitov2, Arthur Jean Hull3, Solene Lejosne1 and Ivan Vasko4, (1)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of California Berkeley, Berkeley, CA, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (4)Space Science Lab, UC Berkeley, Berkeley, CA, United States
Konstantin V Gamayunov, Florida Institute of Technology, Department of Aerospace, Physics and Space Sciences, Melbourne, FL, United States, Jichun Zhang, University of New Hampshire, Durham, NH, United States, Anthony Saikin, University of New Hampshire, Durham, United States and Hamid K Rassoul, Florida Inst Tech, Department of Aerospace Physics and Space Science, Melbourne, United States
Sam Bingham, University of New Hampshire Main Campus, Durham, NH, United States, Christopher Mouikis, UNH, New Hampshire, United States, Lynn M Kistler, Univ New Hampshire, Durham, United States, Charles J Farrugia, New hampshire university, Durham, NH, United States, Kristoff W Paulson, University of New Hampshire, Chelmsford, United States, Chia-Lin Huang, University of New Hampshire, Durham, NH, United States, Alex Boyd, New Mexico Consortium, Los Alamos, NM, United States, Harlan E Spence, Solar System Exploration Research Virtual Institute, NASA Ames Research Center, Moffett Field, CA, United States and Craig Kletzing, University of Iowa, Physics and Astronomy, Iowa City, United States
Ashanthi Shanika Maxworth, University of Colorado Denver, Denver, CO, United States, Mark Golkowski, University of Colorado Denver, Denver, United States, David Malaspina, Univ Colorado, Boulder, CO, United States and Allison N Jaynes, University of Iowa, Iowa City, IA, United States
