Artigo Revisado por pares

Flow of plasma around the Earth

1962; American Geophysical Union; Volume: 67; Issue: 10 Linguagem: Inglês

10.1029/jz067i010p03805

ISSN

2156-2202

Autores

P. J. Kellogg,

Tópico(s)

Solar and Space Plasma Dynamics

Resumo

Journal of Geophysical Research (1896-1977)Volume 67, Issue 10 p. 3805-3811 Flow of plasma around the Earth P. J. Kellogg, P. J. KelloggSearch for more papers by this author P. J. Kellogg, P. J. KelloggSearch for more papers by this author First published: September 1962 https://doi.org/10.1029/JZ067i010p03805Citations: 160AboutPDF ToolsRequest permissionExport citationAdd to favoritesTrack citation ShareShare Give accessShare full text accessShare full-text accessPlease review our Terms and Conditions of Use and check box below to share full-text version of article.I have read and accept the Wiley Online Library Terms and Conditions of UseShareable LinkUse the link below to share a full-text version of this article with your friends and colleagues. Learn more.Copy URL Share a linkShare onEmailFacebookTwitterLinkedInRedditWechat Abstract The interplanetary plasma flow measured by means of Explorer 10 is supersonic in the sense that the flow speed is greater than the Alfvén speed. It is shown that this has some of the same implications as supersonic flow does in ordinary fluid flow theory, and possible consequences are discussed. The position of the shock that would develop if the interplanetary plasma were a perfect gas with a short mean free path is calculated and is shown to be well outside the orbit of Explorer 10, so that it would not have been seen. Speculations on the possible structure of the shock in collisionless plasma are given, and it is shown that this structure may account for the turbulent character of the distant magnetic field. References Adlam, J. H., J. E. Allen, The structure of strong collision-free hydromagnetic waves, Phil., Mag., 3, 448–455, 1958. Åstrom, E., On waves in an ionized gas, Arkiv. Fysik, 2, 443–457, 1951. Auer, P. L., H. Hurwitz Jr., R. W. Kilb, Large-amplitude magnetic compression of a collision-free plasma, 2, Development of a thermalized plasma, Phys. Fluids, 5, 298–316, 1962. Beard, D. B., The interaction of the terrestrial magnetic field with the solar corpuscular radiation, J. Geophys. Research, 65, 3559–3568, 1960. Bridge, H. S., C. Dilworth, A. J. Lazarus, E. F. Lyon, B. Rossi, F. Scherb, Direct observations of the interplanetary plasma, Phys. Soc. Japan, Suppl., 17, 553–560, 1962. De Hoffmann, F., E. Teller, Magneto-hydrodynamic shocks, Phys. Rev., 80, 692–703, 1950. Dungey, J. W., Cosmic Electrodynamics, 139, Cambridge University Press, 1958. Gringauz, K. I., V. V. Bezrukikh, V. D. Ozerov, R. E. Rybchinskii, A study of the interplanetary ionized gas, high-energy electrons, and corpuscular radiation from the sun by means of the three-electrode trap for charged particles on the second Soviet Cosmic Rocket, Soviet Phys., Doklady, 5, 361, 1960. Heppner, J. P., N. F. Ness, T. L. Skillman, C. S. Scearce, Magnetic field measurements with the Explorer 10 satellite, J. Phys. Soc. Japan, Suppl., 17, 546–552, 1962. Hida, K., An approximate study on the detached shock wave in front of a circular cylinder and a sphere, J. Phys. Soc. Japan, 8, 740–747, 1953. Montgomery, D., Development of hydromagnetic shocks from large amplitude Alfvén waves, Phys. Rev. Letters, 2, 36–37, 1959. Morawetz, C. S., Magnetohydrodynamic shock structure without collisions, Phys. Fluids, 4, 998–1006, 1961. Parker, E. N., Suprathermal particle generation on the solar corona, Astrophys. J., 128, 677–685, 1958. Zhigulev, V. N., E. A. Romishevskii, Concerning the interaction of currents flowing in a conduction medium with the earth's magnetic field, Soviet Phys., Doklady, 4, 859, 1960. Citing Literature Volume67, Issue10September 1962Pages 3805-3811 ReferencesRelatedInformation

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