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Direct Observations of Magnetic Reconnection in the Solar Wind Current Sheets near Mars
Journal article   Open access   Peer reviewed

Direct Observations of Magnetic Reconnection in the Solar Wind Current Sheets near Mars

Chi Zhang, Chuanfei Dong, Xinmin Li, Han-Wen Shen, Jasper Halekas, Tai Phan, Christian Mazelle, Yuki Harada, Hongyang Zhou, Jiawei Gao, …
Astrophysical journal. Letters, Vol.1004(2), L45
06/20/2026
DOI: 10.3847/2041-8213/ae78dc
url
https://doi.org/10.3847/2041-8213/ae78dcView
Published (Version of record) Open Access

Abstract

Magnetic reconnection is a fundamental and ubiquitous process in astrophysical plasmas that converts magnetic energy into plasma kinetic and thermal energy. Throughout the heliosphere, the solar wind is permeated with current sheets (CSs), providing a natural laboratory for investigating this process. Using measurements from NASA's Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, we report the first direct observations of magnetic reconnection occurring within the solar wind CSs near Mars. Specifically, MAVEN observed the classic Petschek-type reconnection exhaust regions, evidenced by bifurcated magnetic field signatures and Alfv & eacute;nic ion outflows. Notably, the observed exhaust region appears to be large scale, significantly exceeding the typical thickness of solar wind CSs near Mars. This suggests that magnetic reconnection may significantly broaden the CS. Our results underscore the ubiquity of magnetic reconnection across heliocentric distances and may provide new insights into the large-scale evolution of the solar wind and the development of turbulence within it.
Physical Sciences Astronomy & Astrophysics Science & Technology

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