期刊
ADVANCES IN SPACE RESEARCH
卷 41, 期 2, 页码 318-324出版社
ELSEVIER SCI LTD
DOI: 10.1016/j.asr.2007.06.033
关键词
heliospheric termination shock; heliospheric interface; solar wind; solar cycle; interstellar H atoms
Time-dependent kinetic-continuum model of the solar wind interaction with the two-component local interstellar cloud (LIC) has been developed recently [Izmodenov, V., Malama, Y.G., Ruderman, M.S. Solar cycle influence on the interaction of the solar wind with local interstellar cloud. Astron. Astrophys. 429, 1069-1080, 2005a.]. Here, we adopted this model to the realistic solar cycle, when the solar wind parameters at the Earth's orbit are taken from space data. This paper focuses on the results related to the termination shock (TS) excursion with the solar cycle that may help to understand Voyager I data obtained at and after the crossing of the termination shock and to predict the time of the TS crossing by Voyager 2. (C) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.
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