The siphonic energy transfer between hot solar wind and cold martian ionosphere through open magnetic flux rope

The siphonic energy transfer between hot solar wind and cold martian ionosphere through open magnetic flux rope

A mechanism for energy transfer from the solar wind to the Martian ionosphere through open magnetic flux rope is proposed based on the observations by Mars Atmosphere and Volatile EvolutioN (MAVEN). The satellite was located in the dayside magnetosheath at an altitude of about 700 km above the north...

Full description

Bibliographic Details
Main Authors: Xiaojun Xu, Lou-Chuang Lee, Qi Xu, Qing Chang, Jing Wang, Ming Wang, Shaosui Xu, Christian Möstl, Charles J. Farrugia, Xing Wang, Yudong Ye, Zilu Zhou, Lei Luo, Peishan He, Shaoguan Cheng
Format: Article
Language:English
Published: KeAi Communications Co. Ltd. 2024-07-01
Series:Fundamental Research
Subjects:
Mars
Flux rope
Solar wind
Ionosphere
Ion loss
Online Access:http://www.sciencedirect.com/science/article/pii/S2667325822001959

Internet

http://www.sciencedirect.com/science/article/pii/S2667325822001959

Similar Items