Influence of upstream solar wind on magnetic field distribution in the Martian nightside ionosphere
Influence of upstream solar wind on magnetic field distribution in the Martian nightside ionosphere
摘要
关键词
Martian magnetic field/external magnetic field/upstream solar wind drivers/IMF penetration altitude/magnetic field activity indicesKey words
Martian magnetic field/external magnetic field/upstream solar wind drivers/IMF penetration altitude/magnetic field activity indices引用本文复制引用
JiaWei Gao,ZhaoJin Rong,Qi Zhang,Anna Mittelholz,Chi Zhang,Yong Wei..Influence of upstream solar wind on magnetic field distribution in the Martian nightside ionosphere[J].地球与行星物理（英文）,2024,8(5):728-741,14.基金项目
This work is supported by the National Natural Science Foundation of China(Grant No.42304186),China Postdoctoral Science Foun-dation(2023M743466),the Key Research Program of Chinese Academy of Sciences(Grant No.ZDBS-SSW-TLC00103),the Key Research Program of the Institute of Geology & Geophysics,CAS(Grant No.s IGGCAS-201904,IGGCAS-202102).This research was also supported by the International Space Science Institute(ISSI)in Bern and Beijing,through ISSI/ISSI-BJ International Team project"Understanding the Mars Space Environment through Multi-Spacecraft Measurements"(ISSI Team project #23-582 （Grant No.42304186）
ISSI-BJ Team project #58).We would like to thank the entire MAVEN team and instrument leaders for access to data and support.We thank Yongxin Pan for helpful language assistance. （）
