Modeling of the outer heliosphere with the realistic solar cycle
Modeling of the outer heliosphere with the realistic solar cycle
- New search for: Izmodenov, Vladislav V.
- New search for: Malama, Yuri G.
- New search for: Ruderman, Michael S.
- New search for: Izmodenov, Vladislav V.
- New search for: Malama, Yuri G.
- New search for: Ruderman, Michael S.
AbstractTime-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.
Document information
Modeling of the outer heliosphere with the realistic solar cycle
Advances in Space Research ; 41 , 2 ; 318-324
2007-06-14
7 pages
Article (Journal)
Electronic Resource
English
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