The Energetic Oxygen Ion Beams in the Martian Magnetotail Current Sheets: Hints From the Comparisons Between Two Types of Current Sheets
Chi Zhang, Zhaojin Rong, Xinzhou Li, M. Fräenz, H. Nilsson, R. Järvinen, Moa Persson, Yoshifumi Futaana, Chuanfei Dong, M. Yamauchi, Jiawei Gao, Yi‐Jia Zhou, Lei Wang, Zhen Shi, Yong Wei, Fei He, Mats Holmström, S. Barabash
Abstract
Abstract Using data from the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission, we explore the plasma properties of Martian magnetotail current sheets (CS), to further understand the solar wind interaction with Mars and ion escape. There are some CS exhibit energetic oxygen ions that show narrow beam structures in the energy spectrum, which primarily occurs in the hemisphere where the solar wind electric field ( Esw ) is directed away from the planet. On average, these CS have a higher escaping flux than that of the CS without energetic oxygen ion beams, suggesting different roles in ion escape. The CS with energetic oxygen ion beams exhibits different proton and electron properties to the CS without energetic oxygen ion beams, indicating their different origins. Our analysis suggests that the CS with energetic oxygen ion beams may result from the interaction between the penetrated solar wind and localized oxygen ion plumes.