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Martian Atmospheric Loss Through Foreshock Transient Events
Journal article   Open access   Peer reviewed

Martian Atmospheric Loss Through Foreshock Transient Events

Alexandros C. Cooke-Politikos, Sergey Shuvalov, Yaxue Dong, Yi Qi, David A. Brain and Jasper S. Halekas
Geophysical research letters, Vol.53(4), e2025GL120618
02/28/2026
DOI: 10.1029/2025GL120618
url
https://doi.org/10.1029/2025GL120618View
Published (Version of record) Open Access

Abstract

At Mars, the MAVEN spacecraft has made observations of Hot Flow Anomalies (HFAs) in the foreshock. Due to the bow shock's proximity to the planet, it is theorized that HFAs contribute to atmospheric escape at Mars through the excavation of ionospheric ions. A case study investigates one HFA observation, with parameters suggesting a novel mechanism for planetary ion extraction. The event is further characterized by elevated number densities of O+ and O+ 2 ions observed prior to the current sheet crossing. Statistical study is conducted on a set of 91 events, facilitating the estimation of HFA frequency at Mars to be 1/day. The estimated ion escape of the event is approximately 9% of the typical ion escape rate under nominal conditions at Mars. Calculation of further events reveals escape rates between 1 and 9% of the nominal conditions. This represents a modest contribution to the overall escape, highlighting a potentially underexplored pathway.
atmospheric escape foreshock transient hot flow anomaly Mars MAVEN

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