Solar cycle dependence of the heliospheric shape deduced from a global MHD simulation of the interaction process between a nonuniform time-dependent solar wind and the local interstellar medium

Journal of Geophysical Research: Space Physics

Volumn 104, Issue A6, 1999, Pages 12605-12616

  Tanaka, T ^a  

^a NATIONAL INSTITUTE OF INFORMATION AND COMMUNICATIONS TECHNOLOGY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001056272     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (3)

1. Baranov, V. B., and Y. G. Malama, Model of the solar wind interaction with the local interstellar medium: Numerical solution of self-consistent problem, J. Geophys. Res., 98, 15,157, 1993.
2. Barnes, A., Shape of the heliospheric termination shock: Effects of latitude variations of solar wind dynamic pressure, J. Geophys. Res., 103, 2015, 1998.
3. Gurnett, D. A., and W. S. Kurth, Radio emission from the outer heliosphere, Space Sci. Rev., 78, 53, 1996.