On the variations of protons during the magnetospheric substorm at Earth and Mercury in the near-tail: A comparative study
Weijie Sun1, James A Slavin2, Ryan M. Dewey3, Jim M Raines3, Suiyan Fu4, Yong Wei5, Tomas Karlsson6, Gangkai Poh7, Xianzhe Jia8, Daniel J Gershman9, Qiugang Zong4, Weixing Wan10, Quanqi Shi11, Zuyin Pu4 and Duo Zhao12, (1)University of California Berkeley, Space Science Laboratory, Berkeley, CA, United States, (2)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (3)University of Michigan, Ann Arbor, United States, (4)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (5)Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China, (6)Royal Institute of Technology, Stockholm, Sweden, (7)Catholic University of America, Dept. of Physics, Maryland, United States, (8)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States, (9)NASA Goddard Space Flight Center, Greenbelt, United States, (10)University of the Chinese Academy of Sciences, Beijing, China, (11)Shandong University at Weihai, Weihai, China, (12)Peking University, SchoolofEarthandSpaceSciences, Beijing, China
