Dependence of the Martian radiation environment on atmospheric depth: Modeling and measurement
Jingnan Guo, Tony C. Slaba, Cary Zeitlin, Robert F., Wimmer-Schweingruber, Francis F. Badavi, Eckart B\"ohm, Stephan B\"ottcher,, David E. Brinza, Bent Ehresmann, Donald M. Hassler, Daniel Matthi\"a, and, Scot Rafkin

TL;DR
This study models and measures how Martian atmospheric depth influences surface radiation levels, showing that atmospheric shielding varies with solar activity, which is crucial for planning human missions to Mars.
Contribution
It introduces an updated modeling approach using HZETRN2015 and compares it with recent measurements, enhancing understanding of Martian radiation environment dependence.
Findings
Model and measurements agree well on atmospheric shielding effects.
Shielding decreases as solar modulation increases.
Results inform risk assessments for human Mars exploration.
Abstract
The energetic particle environment on the Martian surface is influenced by solar and heliospheric modulation and changes in the local atmospheric pressure (or column depth). The Radiation Assessment Detector (RAD) on board the Mars Science Laboratory rover Curiosity on the surface of Mars has been measuring this effect for over four Earth years (about two Martian years). The anticorrelation between the recorded surface Galactic Cosmic Ray-induced dose rates and pressure changes has been investigated by Rafkin et al. (2014) and the long-term solar modulation has also been empirically analyzed and modeled by Guo et al. (2015). This paper employs the newly updated HZETRN2015 code to model the Martian atmospheric shielding effect on the accumulated dose rates and the change of this effect under different solar modulation and atmospheric conditions. The modeled results are compared with the…
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Taxonomy
TopicsPlanetary Science and Exploration · Space Science and Extraterrestrial Life · Space exploration and regulation
