Supersonic solar wind ion flows downstream of the terminationshock explained by a two-fluid shock model

Publisher: Edp Sciences

E-ISSN: 1432-0746|490|3|L35-L38

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.490, Iss.3, 2008-11, pp. : L35-L38

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