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Limits on the Density of the Lunar Ionosphere: ARTEMIS Observations
Journal article   Open access   Peer reviewed

Limits on the Density of the Lunar Ionosphere: ARTEMIS Observations

Han-Wen Shen, Jasper Halekas and Andrew Poppe
The Astrophysical journal, Vol.958(2), 165
12/01/2023
DOI: 10.3847/1538-4357/ad054b
url
https://doi.org/10.3847/1538-4357/ad054bView
Published (Version of record) Open Access

Abstract

The Moon of our Earth has a tenuous atmosphere, known as an exosphere. The ionization of this exosphere is speculated to possibly form a weak ionosphere. Some radio occultation (RO) experiments have suggested the presence of a dense ionosphere with an electron density on the order of hundreds of cm−3 near the surface. Using in situ measurements from the ARTEMIS mission during 2012–2021, we conduct statistical analyses and case studies to investigate the plasma density at near-surface altitudes. ARTEMIS measurements reveal no plasma densities at altitudes between 10 and 50 km that exceed 35 cm−3, and therefore they provide no evidence for a steady-state or global lunar ionosphere at the level suggested by some RO observations. Density profiles with local time and altitude show higher density in the sunlit sector than in the shadowed sector. These observations suggest that the natural variation of solar wind plasma flux with solar zenith angle plays a critical role in controlling the plasma population near the surface. This research provides a reference for a comparison with RO observations and a statistical view of the low-altitude plasma environment near the lunar surface.
Ionosphere Altitude Electron density Exosphere In situ measurement Ionization Low altitude Lunar surface Moon Plasma Plasma density Radio occultation Solar wind Space missions Statistical analysis

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