Two‐Spacecraft Observations of Asymmetric Martian Bow Shock: Conjunctions of Tianwen‐1 and MAVEN

Abstract The Martian bow shock has been extensively studied through magnetic field and plasma instrument observations from various Mars space missions. However, prior investigations primarily involve statistical analyses based on single spacecraft crossings, leaving the asymmetry of the Martian bow shock unstudied through simultaneous two‐spacecraft observations. In this study, utilizing simultaneous observations from Tianwen‐1 and MAVEN, we examine the instantaneous asymmetry of the Martian bow shock. We present the asymmetry of the Martian bow shock in the Mars‐Solar‐Electric and Mars‐Solar‐Orbital reference frames, possibly influenced by the solar wind motional electric field and Martian crustal magnetic field, respectively. Moreover, we suggest that the bow shock exhibits increased asymmetry under stronger solar wind motional electric field conditions. This study highlights how a two‐point observation approach offers valuable insights into the dynamic behavior of the Martian induced magnetosphere.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2024-09-01
DOI
https://doi.org/10.1029/2024ja033185
Citations
1
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
0.33

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article

Two‐Spacecraft Observations of Asymmetric Martian Bow Shock: Conjunctions of Tianwen‐1 and MAVEN

D. L. Mitchell, Shannon Curry, J. S. Halekas, Tielong Zhang et al.
1 citations
Journal of Geophysical Research Space Physics
Planetary Science and Exploration
0.33
article

Two‐Spacecraft Observations of Asymmetric Martian Bow Shock: Conjunctions of Tianwen‐1 and MAVEN

D. L. Mitchell, Shannon Curry, J. S. Halekas, Tielong Zhang, R. J. Lillis, B. Langlais, J. Gruesbeck, Yuming Wang, Long Cheng
article en
1 citations

Abstract

Abstract The Martian bow shock has been extensively studied through magnetic field and plasma instrument observations from various Mars space missions. However, prior investigations primarily involve statistical analyses based on single spacecraft crossings, leaving the asymmetry of the Martian bow shock unstudied through simultaneous two‐spacecraft observations. In this study, utilizing simultaneous observations from Tianwen‐1 and MAVEN, we examine the instantaneous asymmetry of the Martian bow shock. We present the asymmetry of the Martian bow shock in the Mars‐Solar‐Electric and Mars‐Solar‐Orbital reference frames, possibly influenced by the solar wind motional electric field and Martian crustal magnetic field, respectively. Moreover, we suggest that the bow shock exhibits increased asymmetry under stronger solar wind motional electric field conditions. This study highlights how a two‐point observation approach offers valuable insights into the dynamic behavior of the Martian induced magnetosphere.

Journal of Geophysical Research Space PhysicsVol. 129(9)
University of Iowa (US), University of Science and Technology of China (CN), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), Austrian Academy of Sciences (AT), University of Colorado Boulder (US), Université Nantes Angers Le Mans (FR), Space Research Institute (AT), Le Mans Université (FR), Laboratory for Atmospheric and Space Physics (US), Laboratoire de Planétologie et Géosciences (FR), University of California, Berkeley (US), Nantes Université (FR)
National Natural Science Foundation of China, University of Science and Technology of China
Affordable and clean energy
Openalex Percentile: Top 34%
Planetary Science and Exploration
0.33
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