Electromagnetic Fields, Plasma Distributions, and Energy Conversion in Mars’ Induced Magnetosphere
Electromagnetic Fields, Plasma Distributions, and Energy Conversion in Mars’ Induced Magnetosphere
Chi Zhang1, Chuanfei Dong2, Hongyang Zhou2, Jiawei Gao1, Dr. Xinmin Li2, Hans Nilsson3, Xiao-dong Wang4, Jasper S Halekas5, Yuki Harada6, Han-Wen Shen7, Christian Xavier Mazelle8, Robin Ramstad9, Liang Wang2, Shaosui Xu10, Abigail Tadlock11, Kathleen Gwen Hanley12, Shannon Curry13 and David Mitchell12, (1)Boston University, Center for Space Physics and Department of Astronomy, Boston, United States, (2)Boston University, Boston, United States, (3)IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, (4)IRF, Kiruna, Sweden, (5)University of Iowa, Physics and Astronomy, Iowa City, United States, (6)Kyoto University, Kyoto, Japan, (7)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (8)IRAP, CNRS-UPS, Toulouse, France, (9)Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (10)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (11)Boston University, Boston, MA, United States, (12)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (13)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States