Martian ion currents and escape driven by interplanetary magnetic field orientation based on hybrid simulationsOA
Martian ion currents and escape driven by interplanetary magnetic field orientation based on hybrid simulations
HengLe Du;BinBin Ni;Xiao-Dong Wang;Shahab Fatemi;Xing Cao
School of Earth and Space Science and Technology,Wuhan University,Wuhan 430074,China||Solar System Physics and Space Technology Programme,Swedish Institute of Space Physics,SE-981 92 Kiruna,SwedenSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430074,ChinaSolar System Physics and Space Technology Programme,Swedish Institute of Space Physics,SE-981 92 Kiruna,SwedenDepartment of Physics,Umeå University,SE-901 87 Umeå,SwedenSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430074,China
Martian spaceion currention escapeinterplanetary magnetic field orientation
Martian spaceion currention escapeinterplanetary magnetic field orientation
《地球与行星物理（英文）》 2026 (3)
417-426,10
This work was supported by the National Natural Science Foundation of China(Grant Nos.42188101,42025404,42374193,and 42578012),the National Key R&D Program of China(Grant Nos.2022YFF0503700 and 2022YFF0503900),the Natural Science Foundation of Hubei Province,China(Grant 2025AFA030),the Fengyun Application Pioneering Project(FY-APP),and the Tencent X-plorer prize.This work was also supported by a special scholarship provided through the Graduate Student Exchange Program at Wuhan University,China.The Amitis simulations were performed using computational resources provided by the High Performance Computing Center North(HPC2N),Umeå University,Sweden.These resources were partly sponsored by Kempestiftelserna(Grant Nos.JCSMK25-0057 and JCK22-0035).
评论