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Fluid and particle simulations of the interaction of the solar wind with magnetic anomalies on the surface of the Moon and Mars
(2003)
Simulations of the solar wind interacting with the Moon and Mars indicate that the presence of magnetic anomalies on the surface can lead to the formation of mini-magnetospheres around the anomalies. These mini-magnetospheres are not just small scale versions of planetary magnetospheres, but rather their small size leads to ...