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| Main Authors: | , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2410.05913 |
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| _version_ | 1866916427998429184 |
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| author | Miyake, Y. Nakazono, J. Miyoshi, Y. Harada, Y. Nishino, M. N. Kurita, S. Kasahara, S. Usui, H. Nagamatsu, A. Nakamura, S. |
| author_facet | Miyake, Y. Nakazono, J. Miyoshi, Y. Harada, Y. Nishino, M. N. Kurita, S. Kasahara, S. Usui, H. Nagamatsu, A. Nakamura, S. |
| contents | It is widely accepted that the surface potential of the lunar dayside is "on average" several to 10 V positive due to photoelectron emission in addition to the solar wind plasma precipitation. Recent studies, however, have shown that an insulating and rough regolith layer tends to make positive and negative charges separated and irregularly distributed on sub-Debye-length scales. The local charge separation then gives rise to an intense and structured electrostatic field. Such micro-scale electrostatic structures lie in the innermost part of the photoelectron sheath and may contribute to the mobilization of the charged dust particles. Since the electrostatic structures can take different states depending on the topography of the lunar surface, it is necessary to update the research approach. We have launched a research group to develop an integrated assessment framework that includes theoretical and numerical modeling, on-orbit observations, ground-based testing, and the development of charging measurement instruments, with the ultimate goal of comprehensively understanding the surface charging processes on the Moon. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_05913 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Micro-scale Electrostatic Structures formed on the Rough Surfaces of the Moon Miyake, Y. Nakazono, J. Miyoshi, Y. Harada, Y. Nishino, M. N. Kurita, S. Kasahara, S. Usui, H. Nagamatsu, A. Nakamura, S. Space Physics It is widely accepted that the surface potential of the lunar dayside is "on average" several to 10 V positive due to photoelectron emission in addition to the solar wind plasma precipitation. Recent studies, however, have shown that an insulating and rough regolith layer tends to make positive and negative charges separated and irregularly distributed on sub-Debye-length scales. The local charge separation then gives rise to an intense and structured electrostatic field. Such micro-scale electrostatic structures lie in the innermost part of the photoelectron sheath and may contribute to the mobilization of the charged dust particles. Since the electrostatic structures can take different states depending on the topography of the lunar surface, it is necessary to update the research approach. We have launched a research group to develop an integrated assessment framework that includes theoretical and numerical modeling, on-orbit observations, ground-based testing, and the development of charging measurement instruments, with the ultimate goal of comprehensively understanding the surface charging processes on the Moon. |
| title | Micro-scale Electrostatic Structures formed on the Rough Surfaces of the Moon |
| topic | Space Physics |
| url | https://arxiv.org/abs/2410.05913 |