The Solar Wind: A Turbulent Magnetohydrodynamic Medium

Details The Solar Wind: A Turbulent Magnetohydrodynamic Medium The Solar Wind: A Turbulent Magnetohydrodynamic Medium

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ssrv...78...29b&link_type=abstract

Space Science Reviews, Volume 78, Issue 1-2, pp. 29-32

Physics

2

Scientific paper

MHD turbulence properties in the solar wind are briefly reviewed. The evolution of fluctuations of alfvénic type in near-ecliptic regions of the inner heliosphere is described. The role of interplanetary sources and the influence of interactions with structures convected by the solar wind are discussed. Turbulence features at high latitudes and in the outermost regions of the heliosphere are finally highlighted.

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