Dayside Magnetic Reconnection With Outflow Below the Mars' Escape Velocity: MAVEN Observation

Abstract Previous studies have demonstrated that magnetic reconnection can cause ionospheric ions to escape from Mars. Using data from the Mars Atmosphere and Volatile Evolution (MAVEN) mission, we observed a dayside magnetic reconnection event with a jet speed of approximately 1.1 km/s, which is below Mars' escape velocity of 5 km/s. This event, characterized by a clear Hall magnetic field between draped interplanetary magnetic fields and open crustal field lines, was detected in the dayside ionosphere of the southern hemisphere. Due to the high density of heavy ions, the inflow Alfvén speed is low, around 2 km/s. Consequently, the reconnection jet, moving approximately at the inflow Alfvén speed, cannot escape Mars despite moving towards space. However, the reconnection significantly heated the ionospheric ions. Our findings may offer valuable insights into the study of similar processes, such as failed eruptions in the solar corona.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-04-01
DOI
https://doi.org/10.1029/2024je008846
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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article

Dayside Magnetic Reconnection With Outflow Below the Mars' Escape Velocity: MAVEN Observation

Xiaojun Xu, Siqi Yi, Zilu Zhou, Jun Cui et al.
2 citations
Journal of Geophysical Research Planets
Astro and Planetary Science
2.31
article

Dayside Magnetic Reconnection With Outflow Below the Mars' Escape Velocity: MAVEN Observation

Xiaojun Xu, Siqi Yi, Zilu Zhou, Jun Cui, Hengyan Man, Lei Luo, Zhihong Zhong, Jing Wang, Xiaohua Deng, Peishan He, Xing Wang, Pu Yang, Wenjing Zhao
article en
2 citations

Abstract

Abstract Previous studies have demonstrated that magnetic reconnection can cause ionospheric ions to escape from Mars. Using data from the Mars Atmosphere and Volatile Evolution (MAVEN) mission, we observed a dayside magnetic reconnection event with a jet speed of approximately 1.1 km/s, which is below Mars' escape velocity of 5 km/s. This event, characterized by a clear Hall magnetic field between draped interplanetary magnetic fields and open crustal field lines, was detected in the dayside ionosphere of the southern hemisphere. Due to the high density of heavy ions, the inflow Alfvén speed is low, around 2 km/s. Consequently, the reconnection jet, moving approximately at the inflow Alfvén speed, cannot escape Mars despite moving towards space. However, the reconnection significantly heated the ionospheric ions. Our findings may offer valuable insights into the study of similar processes, such as failed eruptions in the solar corona.

Journal of Geophysical Research PlanetsVol. 130(4)
Macau University of Science and Technology (MO), Nanchang University (CN), Sun Yat-sen University (CN), China National Space Administration (CN), Nanchang Institute of Science & Technology (CN)
National Natural Science Foundation of China
Openalex Percentile: Top 12%
Astro and Planetary Science
2.31
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