Field‐Aligned Proton Beams Upstream of the Martian Bow Shock: First Observations

Abstract We report fast sunward‐propagating energetic proton field‐aligned beams (FABs) observed about one Mars radius upstream of the Martian bow shock, recorded by the Solar Wind Ion Analyzer instrument on the MAVEN spacecraft. The velocity distributions show that all the beams have a bulk parallel speed , exceeding the shock speed . Several FABs are observed in the field‐aligned region, linked to the quasi‐parallel shock. The nearly synchronous variations of shock values and beam speeds rule out specular reflection, suggesting a non‐specular reflection mechanism. However, the slower Martian foreshock beam speeds remain unexplained compared to their terrestrial counterparts.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-05-30
DOI
https://doi.org/10.1029/2025gl115483
Citations
1
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
1.15

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article

Field‐Aligned Proton Beams Upstream of the Martian Bow Shock: First Observations

D. L. Mitchell, J. S. Halekas, C. Bertucci, J. R. Espley et al.
1 citations
Geophysical Research Letters
Planetary Science and Exploration
1.15
article

Field‐Aligned Proton Beams Upstream of the Martian Bow Shock: First Observations

D. L. Mitchell, J. S. Halekas, C. Bertucci, J. R. Espley, K. Meziane, A. M. Hamza, C. Mazelle
article en
1 citations

Abstract

Abstract We report fast sunward‐propagating energetic proton field‐aligned beams (FABs) observed about one Mars radius upstream of the Martian bow shock, recorded by the Solar Wind Ion Analyzer instrument on the MAVEN spacecraft. The velocity distributions show that all the beams have a bulk parallel speed , exceeding the shock speed . Several FABs are observed in the field‐aligned region, linked to the quasi‐parallel shock. The nearly synchronous variations of shock values and beam speeds rule out specular reflection, suggesting a non‐specular reflection mechanism. However, the slower Martian foreshock beam speeds remain unexplained compared to their terrestrial counterparts.

Geophysical Research LettersVol. 52(11)
University of New Brunswick (CA), University of Iowa (US), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), Université Toulouse III - Paul Sabatier (FR), Austrian Academy of Sciences (AT), Université Fédérale de Toulouse Midi-Pyrénées (FR), Space Research Institute (AT), Institute of Astronomy and Space Physics (AR), University of California, Berkeley (US)
Centre National d’Etudes Spatiales
Openalex Percentile: Top 19%
Planetary Science and Exploration
1.15
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