Influence of the Earthward and Tailward Ion Flows on the Lunar Surface Water in the Magnetotail

Abstract Earth wind, namely the particles from the Earth's magnetotail, is an important source of lunar water. Besides tailward flow incident on the lunar nearside when the Moon is in the magnetotail, there exists earthward flow bombarding the farside, affecting the distribution and preservation of lunar water. In this study, we determine the incident fluxes of both the tailward and earthward flows on the lunar surface with the ARTEMIS observations and examine their influences on the concentration and migration of lunar surface water and its reservation in the polar regions using Monte Carlo modeling. It is found that water molecules produced by the earthward flow can stay longer on the surface than those produced by the tailward flow. Our results suggest that the evolution of the Earth's magnetosphere can be inferred from Earth wind particles implanted in the soils of both the lunar nearside and farside.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-11-27
DOI
https://doi.org/10.1029/2024je008621
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
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article

Influence of the Earthward and Tailward Ion Flows on the Lunar Surface Water in the Magnetotail

Anmin Tian, T. Pitkänen, Chao Yue, Qiugang Zong et al.
Journal of Geophysical Research Planets
Planetary Science and Exploration
article

Influence of the Earthward and Tailward Ion Flows on the Lunar Surface Water in the Magnetotail

Anmin Tian, T. Pitkänen, Chao Yue, Qiugang Zong, Chao Xiao, Wenlong Liu, S. Y. Fu, Jong‐Sun Park, Huizi Wang, Alexander William Degeling, Yue Fu, Wensai Shang, Siqi Zhao, Ruilong Guo, Kevin X. Li, J. Zhang, Quanqi Shi, T. L. Chen, Jian Chen, Yao Chen, Ji Liu, Lianghai Xie
article en

Abstract

Abstract Earth wind, namely the particles from the Earth's magnetotail, is an important source of lunar water. Besides tailward flow incident on the lunar nearside when the Moon is in the magnetotail, there exists earthward flow bombarding the farside, affecting the distribution and preservation of lunar water. In this study, we determine the incident fluxes of both the tailward and earthward flows on the lunar surface with the ARTEMIS observations and examine their influences on the concentration and migration of lunar surface water and its reservation in the polar regions using Monte Carlo modeling. It is found that water molecules produced by the earthward flow can stay longer on the surface than those produced by the tailward flow. Our results suggest that the evolution of the Earth's magnetosphere can be inferred from Earth wind particles implanted in the soils of both the lunar nearside and farside.

Journal of Geophysical Research PlanetsVol. 130(12)
Macau University of Science and Technology (MO), Tibet University (CN), University of Alberta (CA), National University of Defense Technology (CN), Chinese Academy of Sciences (CN), Peking University (CN), Deutsches Elektronen-Synchrotron DESY (DE), Institute of Space Sciences (ES), National Space Science Center (CN), Space Engineering University (CN), Beihang University (CN), Umeå University (SE)
National Natural Science Foundation of China, Natural Science Foundation of Shandong Province
Openalex Percentile: Top 75%
Planetary Science and Exploration
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