Modeling of the outer heliosphere with the realistic solar cycle |
| |
| Authors: | Vladislav V Izmodenov Yuri G Malama Michael S Ruderman |
| |
| Institution: | 1. Lomonosov Moscow State University, Department of Aeromechanics and Gas Dynamics, School of Mechanics and Mathematics, Leninskie Gory, Glavnoe Zdanie, Moscow 119899, Russia;2. Space Research Institute (IKI), Russian Academy of Sciences, Prosouznaya 84/32, Moscow 117997, Russia;3. Institute for Problems in Mechanics, Russian Academy of Sciences, Prospekt Vernadskogo 101-1, Moscow 119526, Russia;4. University of Sheffield, Department of Applied Mathematics, Hicks Building, Hounsfied Road, Sheffield S3 7RH, UK |
| |
| Abstract: | 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 |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
