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[期刊论文] 作者：MengHao Fu,Jun Cui,XiaoShu Wu,,
来源：地球与行星物理:英文版 年份：2020
The exobase is defined as the interface between the strongly collisional and the collisionless parts of an atmosphere. Although in reality the exobase is a tran...
Photoelectron pitch angle distribution near Mars and implications on cross terminator magnetic field
[期刊论文] 作者：YuTian Cao,Jun Cui,XiaoShu Wu,,
来源：地球与行星物理:英文版 年份：2020
The photoelectron peak at 22 27 eV, a distinctive feature of the energetic electron distribution in the dayside Martian ionosphere, is a useful diagnostic of so...
[期刊论文] 作者：MeiJuan Yao,Jun Cui,XiaoShu Wu,
来源：地球与行星物理:英文版 年份：2019
The Martian ionosphere is produced by a number of controlling processes, including solar extreme ultraviolet radiation (EUV) and X-ray ionization, impact ioniza...
[期刊论文] 作者：XiaoShu Wu,Jun Cui,YuTian Cao,,
来源：地球与行星物理:英文版 年份：2020
An important population of the dayside Martian ionosphere are photoelectrons that are produced by solar Extreme Ultraviolet and X-ray ionization of atmospheric...
[期刊论文] 作者：XiaoShu Wu,Jun Cui,Jiang Yu,Li,
来源：地球与行星物理:英文版 年份：2019
Photoelectrons are produced by solar Extreme Ultraviolet radiation and contribute significantly to the local ionization and heat balances in planetary upper atm...
[期刊论文] 作者：XiaoShu Wu,Jun Cui,Jiang Yu,LiJuan Liu,ZhenJun Zhou,
来源：黑龙江科技信息 年份：2019
本文通过对荣华二采区10...
Is Solar Wind electron precipitation a source of neutral heating in the nightside Martian upper atmo
[期刊论文] 作者：LongKang Dai,Jun Cui,DanDan Niu,Hao Gu,YuTian Cao,XiaoShu Wu,HaiRong Lai,
来源：地球与行星物理（英文） 年份：2021
Solar Wind (SW) electron precipitation is able to deposit a substantial amount of energy in the nightside Martian upperatmosphere, potentially exerting an influ...
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