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Dynamics of solar wind protons reflected by the Moon

Dynamics of solar wind protons reflected by the Moon

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Proton fluxes in <strong>the</strong> wake<br />

E SW<br />

Wake entry<br />

possible for<br />

<strong>reflected</strong><br />

<strong>protons</strong><br />

Depending<br />

on IMF<br />

u SW<br />

(Nishino et al.,<br />

GRL 2009,<br />

Type-II entry)<br />

B SW

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