作者: D. Winterhalter , K. Sauer , T.E. Cravens , S. Brecht , C. Mazelle
DOI: 10.1023/B:SPAC.0000032718.47512.92
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摘要: When the supersonic solar wind reaches the neighborhood of a planetary obstacle it decelerates. The nature of this interaction can be very different, depending upon whether …