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Evolution of Coronal MHD Shocks into Interplanetary MHD Shocks

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dc.contributor.author Wu, S. T. en_US
dc.contributor.author Guo, W. P. en_US
dc.contributor.author Dryer, M. en_US
dc.contributor.author Tsuratani, B. T. en_US
dc.contributor.author Vaisberg, O. L. en_US
dc.date.accessioned 2004-10-04T20:24:34Z
dc.date.available 2004-10-04T20:24:34Z
dc.date.issued 1995 en_US
dc.identifier.citation The Solar Environment [book] published at IKI, Moscow, Russia en_US
dc.identifier.clearanceno 95-1411
dc.identifier.uri http://hdl.handle.net/2014/32029
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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