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Solar Wind and Interplanetary Magnetic Field: A Tutorial

2011; American Geophysical Union; Linguagem: Inglês

10.1029/gm125p0073

2328-8779

C. T. Russell,

Ionosphere and magnetosphere dynamics

Free Access Solar Wind and Interplanetary Magnetic Field: A Tutorial C. T. Russell, C. T. Russell Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angles, CaliforniaSearch for more papers by this author C. T. Russell, C. T. Russell Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angles, CaliforniaSearch for more papers by this author Book Editor(s):Paul Song, Paul SongSearch for more papers by this authorHoward J. Singer, Howard J. SingerSearch for more papers by this authorGeorge L. Siscoe, George L. SiscoeSearch for more papers by this author First published: 01 January 2001 https://doi.org/10.1029/GM125p0073Citations: 21Book Series:Geophysical Monograph Series AboutPDFPDFView & download chapterView & download chapterView & download full book ToolsRequest permissionExport citationAdd to favoritesTrack citation ShareShareShare a linkShare onEmailFacebookTwitterLinkedInRedditWechat Summary This chapter contains sections titled: Introduction The Solar Wind Plasma The Solar Wind Magnetic Field Effects of Solar Rotation Time Variation Concluding Remarks References J. R. Asbridge, S. J. Bame, W. C. Feldman, Abundance differences in solar wind double streams, Solar Phys., 37, 451– 467, 1974. 10.1007/BF00152503 Web of Science®Google Scholar L. F. Burlaga, Magnetic clouds and force-free fields with constant alpha, J. Geophys. Res., 93, 7217, 1988. 10.1029/JA093iA07p07217 Web of Science®Google Scholar R. K. Burton, R. L. McPherron, C. T. 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