Izmodenov, VV., Malama, Y.G. and Ruderman, M.S. (2008) Modeling of the outer heliosphere with the realistic solar cycle. Advances in Space Research , 41 (2). pp. 318-324. ISSN 0273-1177Full text not available from this repository. (Request a copy)
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 1 data obtained at and after the crossing of the termination shock and to predict the time of the TS crossing by Voyager 2.
|Keywords:||Heliospheric termination shock; Heliospheric interface; Solar wind; Solar cycle; Interstellar H atoms|
|Academic Units:||The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
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|Depositing User:||Mrs Megan Hobbs|
|Date Deposited:||17 Mar 2010 16:21|
|Last Modified:||07 Jun 2010 11:10|
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