SM14A:
Dayside Magnetosphere Interactions II
Submit an Abstract to this Session
Session ID#: 60861
Session Description:
The Earth's magnetosphere can be significantly affected by transient solar wind features. Important energy transfer and transport will occur during the interaction of transient solar wind features with the Geospace system. Solar energy in various forms can propagate into the magnetosphere and ionosphere. Charged particle energy can be transformed to electromagnetic energy and vice versa. In-depth understanding of how the magnetosphere responds to transient solar wind features will enhance our knowledge on the solar wind - magnetosphere –ionosphere coupling.
This special session will address the processes by which solar wind mass, momentum, and energy enter the magnetosphere. Regions of interest include the foreshock, bow shock, magnetosheath, magnetopause, and cusps, the dayside magnetosphere, and both the dayside polar and equatorial ionosphere. This special session will provide a forum to present the latest results from in-situ spacecraft observations, ground-based observations, and global simulations. Coordinated multi-point observations are especially encouraged.
Primary Convener: Qiugang Zong, Peking University, Institute of Space Physics and Applied Technology, Beijing, China
Convener: Hui Zhang, University of Alaska Fairbanks, Physics Department & Geophysical Institute, Fairbanks, AK, United States
Primary Liaison: Qiugang Zong, Peking University, Institute of Space Physics and Applied Technology, Beijing, China
Chairs: Hui Zhang, University of Alaska Fairbanks, Physics Department & Geophysical Institute, Fairbanks, AK, United States and Quanqi Shi, Shandong University at Weihai, Institute of Space Science, Weihai, China
OSPA Liaison: Hui Zhang, University of Alaska Fairbanks, Physics Department & Geophysical Institute, Fairbanks, AK, United States
Abstracts Submitted to this Session:
Daniel N Baker, University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, United States
Guan Le, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Peter J Chi, University of California Los Angeles, Department of Earth Planetary and Space Sciences, Los Angeles, California, United States, Robert J Strangeway, Univ California, Los Angeles, CA, United States, Christopher T Russell, University of California Los Angeles, Los Angeles, United States, James A Slavin, University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, Brian J Anderson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Rumi Nakamura, Austrian Academy of Sciences, Space Research Institute, Graz, Austria, Ferdinand Plaschke, IWF ÖAW, Graz, Austria and Roy B Torbert, University of New Hampshire, Durham, United States
Ennio R Sanchez, SRI International Menlo Park, Menlo Park, CA, United States and Jesper W Gjerloev, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Bruce Tsurutani, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and The Relativistic Electron Decrease (RED) Scientific Team
Qiugang Zong, Peking University, Institute of Space Physics and Applied Technology, Beijing, China
J. F. Fennell, Aerospace Corporation Los Angeles, Space Science Applications Laboratory, Los Angeles, CA, United States, Drew L. Turner, The Aerospace Corporation, Los Angeles, CA, United States, Colby Lemon, The Aerospace Corporation, Space Science Applications Laboratory, El Segundo, United States, Shiva Kavosi, University of New Hampshire, Durham, United States, Harlan E Spence, University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, Trevor W Leonard, University of New Hampshire, Durham, NH, United States, Allison N Jaynes, University of Iowa, Iowa City, IA, United States, J Bernard Blake, Aerospace Corporation Arlington, Arlington, VA, United States, James H. Clemmons, The Aerospace Corp, Los Angeles, CA, United States, Daniel N Baker, University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, United States, Barry Mauk, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Ian J Cohen, Johns Hopkins University Applied Physics Laboratory, Laurel, United States
Robert Rankin1, Yongfu Wang2, Alex W Degeling3, Qiugang Zong4 and Xuzhi Zhou4, (1)University of Alberta, Department of Physics, Edmonton, AB, Canada, (2)Peking University, School of Earth and Space Sciences, Beijing, China, (3)Shandong University at Weihai, Weihai, China, (4)Peking University, Institute of Space Physics and Applied Technology, Beijing, China
Jie Ren1, Q. -G. Zong2, Xuzhi Zhou3, Robert Rankin4, Yong Fu Wang1 and Yifan Zhu1, (1)Peking University, Beijing, China, (2)Peking University, Institute of space physics and applied technology, Beijing, China, (3)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (4)University of Alberta, Department of Physics, Edmonton, AB, Canada
