Influence of the interstellar magnetic field direction on the shape of the global heliopause

Journal of Geophysical Research: Space Physics

Volumn 103, Issue A1, 1998, Pages 237-245

  Pogorelov, Nikolai V ^a,b   Matsuda, Takuya ^b  

^a INSTITUTE FOR PROBLEMS IN MECHANICS   (Russian Federation)

^b KOBE UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 19844382405     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (18)

1. Alfvén, H., Cosmic Electrodynamics, Clarendon, Oxford, England, 1950.
2. Axford, W. I., The interaction of the solar wind with the interstellar medium, in Solar Wind, NASA Spec. Publ., NASA SP-308, 609-658, 1972.
3. Baranov, V. B., and K. V. Krasnobaev, Hydrodynamic Theory of Cosmic Plasma (in Russian), 336 pp., Nauka, Moscow, 1977.
4. 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, 15,157-15,163, 1993.
5. Baranov, V. B., and N. A. Zaitsev, On the problem of the solar wind interaction with magnetized interstellar plasma, Astron. Astrophys., 304, 631-637, 1995.
6. Baranov, V. B., K. V. Krasnobaev, and A. G. Kulikovskiy, A model of the interaction of the solar wind with the interstellar medium, Sov. Phys. Dokl., Engl. Transl., 15, 791-793, 1971.
7. Baranov, V. B., M. G. Lebedev, and M. S. Ruderman, Structure of the region of the solar wind-interstellar medium interaction and its influence on H-atoms penetrating the solar wind, Astrophys. Space Sci., 66, 441-451, 1979.
8. Baranov, V. B., M. K. Ermakov, and M. G. Lebedev, Three-component gasdynamic model of the interaction of the solar wind with the interstellar medium, Sov. Astron. Lett., Engl. Transl., 7, 206-210, 1981.
9. Barmin, A. A., A. G. Kulikovskiy, and N. V. Pogorelov, Shock-capturing approach and nonevolutionary solutions in magnetohydrodynamics, J. Comput. Phys., 126, 77-90, 1996.
10. Blum, P. W., and H. J. Fahr, Solar wind tail and the anisotropic production of fast hydrogen atoms, Nature, 223, 936-937, 1969.
11. Brandt, J. C., Introduction to the Solar Wind, W. H. Freeman, New York, 1970.
12. Davis, L. E., Jr., Interplanetary magnetic fields and cosmic rays, Phys. Rev., 100, 1440-1444, 1955.
13. Fahr, H. J., Is the heliospheric interface submagnetosonic? Consequences for the LISM presence in the heliosphere, Adv. Space Res., 6, No. 2, 13-25, 1986.
14. Fahr, H. J., S. Grzedzielski, and R. Ratkiewicz, Magnetohydrodynamic modeling of the 3-dimensional heliopause using the Newtonian approximation, Ann. Geophys., 6, 337-354, 1988.
15. Gombosi, T. I., D. L. De Zeeuw, R. M. Häberli, and K. G. Powell, Three-dimensional multiscale MHD model of cometary plasma environments, J. Geophys. Res., 101, 15,233-15,253, 1996.
16. Hirsch, C., Numerical Computation of Internal and External Flows, John Wiley, New York, 1990.
17. Khabibrakhmanov, I. K., and D. Summers, A new model of interaction between the solar wind and the local interstellar medium, J. Geophys. Res., 101, 7609-7618, 1996.
18. Kulikovskiy, A. G., and G. A. Lyubimov, Magnetohydrodynamics, Addison-Wesley, Reading, MA, 1965.