On the relative locations of the bow shocks of the terrestrial planets

作者: C. T. Russell

DOI: 10.1029/GL004I010P00387

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摘要: The observed bow shock encounters at Mercury, Venus and Mars are least square fit using the same technique so that their sizes shapes can be intercompared. front of Mercury most resembles terrestrial in shape, stand off distance is consistent with moment. fronts more resemble each other than earth's distances direct interaction solar wind ionosphere on dayside. closer to planet suggesting absorption Venus.

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