作者: K. R. Flammer
DOI: 10.1017/S0252921100012859
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摘要: The global interaction of the solar wind with a comet as it orbits Sun is reviewed. After brief survey flow transition regions observed at Halley presented, theoretical models are given for cometocentric distance bow shock, cometopause, and ionopause. In addition, predictions made to what heliocentric these boundaries should form at. results compared in situ observations Halley.