Literature cited
V. B. Baranov and K. V. Krasnobaey, Hydrodynamic Theory of the Cosmic Plasma [in Russian], Nauka, Moscow (1977), p. 335.
V. B. Baranov, K. V. Krasnobaev, and A. G. Kulikovskii, “Model of the interaction of the solar wind with the interstellar medium,” Dokl. Akad. Nauk SSSR,194, 41 (1970).
G. G. Chernyi, Gas Flows at High Supersonic Velocities [in Russian], Fizmatgiz, Moscow (1959), p. 220.
V. B. Baranov, M. G. Lebedev, and M. S. Ruderman, “Structure of the region of solar wind-interstellar medium interaction and its influence on H atoms penetrating the solar wind,” Astrophys. Space Sci.,66, 441 (1979).
K. I. Babenko and V. V. Rusanov, “Difference methods of solution of three-dimensional problems of gas dynamics,” in: Proc. Second All-Union Symposium on Theoretical and Applied Mechanics, No. 2 [in Russian], Nauka, Moscow (1965), pp. 247–262.
M. K. Wallis, “Local interstellar medium,” Nature,254, 202 (1975).
V. B. Baranov, M. K. Ermakov, and M. G. Lebedev, “Some results of calculation of a three-dimensional model of the interaction of the solar wind with the interstellar medium,” Pis'ma Astron. Zh.,7, 372 (1981).
S. Grzedzielski and R. Ratkiewicz, “Asymmetric distant solar wind,” Acta Astron.,25, 177 (1975).
M. G. Lebedev and I. D. Sandomirskaya, “The interaction of colliding supersonic inviscid gas flows,” in: Computational Methods and Programming, No. 34 [in Russian], Izd. MGU, Moscow (1981).
M. M. Gilinskii and M. G. Lebedev, “Calculation of strong blowing on a blunt body and a profile,” Izv. Akad. Nauk SSSR, Mekh. Zhidk. Gaza, No. 1, 117 (1977).
V. B. Baranov, “The interaction of solar and interstellar winds: observational tests,” Comments Astrophys.,9, 75 (1981).
Author information
Authors and Affiliations
Additional information
Translated from Izvestiya Akademii Nauk SSSR, Mekhanika Zhidkosti i Gaza, No. 5, pp. 122–128, September–October, 1982.
Rights and permissions
About this article
Cite this article
Baranov, V.B., Ermakov, M.K. & Lebedev, M.G. Three-component gas-dynamic model of the interaction of the solar wind with the interstellar medium. Fluid Dyn 17, 754–759 (1982). https://doi.org/10.1007/BF01090158
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF01090158