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Intermittent Electron-Only Reconnection at Lunar Mini-Magnetospheres
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Intermittent Electron-Only Reconnection at Lunar Mini-Magnetospheres

Adam Stanier, Li-Jen Chen, Ari Le, Jasper Halekas and Rhyan Sawyer
arXiv.org
Cornell University
02/02/2024
DOI: 10.48550/arxiv.2402.01859
url
https://doi.org/10.48550/arxiv.2402.01859View
Preprint (Author's original)This preprint has not been evaluated by subject experts through peer review. Preprints may undergo extensive changes and/or become peer-reviewed journal articles. Open Access

Abstract

Lunar crustal magnetic anomalies (LCMA) are sub-ion-gyroradius structures that have been shown to stand off the solar wind (SW) plasma from the Moon's surface, forming shock-like discontinuities and reflecting incident SW protons. In this letter, the results of high-resolution, two-dimensional fully kinetic simulations show a bursty electron-only magnetic reconnection in the SW-LCMA interaction region, characterized by the quasi-periodic formation and ejection of magnetic islands and strong parallel electron flows along the X-point separator lines. The islands are observed to modify the magnetic pressure pile-up and Hall electric field above the LCMA, leading to sharp increases in reflected protons that drive electromagnetic fluctuations downstream and short distances upstream in the SW.
Physics - Plasma Physics Physics - Space Physics

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