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Evolution of Coronal MHD Shocks into Interplanetary MHD Shocks

Show simple item record Wu, S. T. en_US Guo, W. P. en_US Dryer, M. en_US Tsuratani, B. T. en_US Vaisberg, O. L. en_US 2004-10-04T20:24:34Z 2004-10-04T20:24:34Z 1995 en_US
dc.identifier.citation The Solar Environment [book] published at IKI, Moscow, Russia en_US
dc.identifier.clearanceno 95-1411
dc.description.abstract The energetic particle environment near the Sun, particularly during solar activity, is of major importance to the planning of a solar probe. It is not known if intensive fluxes are generated solely in the impulsive phase of flares or whether they are augmented by, or contained within, the coronal mass ejections and shock waves spatially preceding them. A solar wind model with various ejecta is studied. en_US
dc.format.extent 155474 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other sun coronal shocks interplanetary shocks solar probe MHD en_US
dc.title Evolution of Coronal MHD Shocks into Interplanetary MHD Shocks en_US

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