Mathematics – Logic
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24...22i&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, Jan.-Feb. 1984, p. 22-25. In Russian.
Mathematics
Logic
7
Cosmic Plasma, Interplanetary Medium, Magnetohydrodynamic Flow, Solar Flares, Boundary Layers, Interplanetary Magnetic Fields, Mathematical Models, Phenomenology, Propagation Modes, Time Response
Scientific paper
Current ideas on the MHD structure of a typical isolated solar-flare stream are outlined on the basis of satellite measurements of magnetic field and plasma in the interplanetary medium. A new model for this structure is proposed which includes a boundary layer beyond the magnetopause of the magnetic region (cloud) of the flare ejection and a slow magnetoacoustic wave mode in front of the ejection magnetopause. It is concluded that, though this model is phenomenological, its hydrodynamic meaning is evident, so that each structural region and the surface bounding this region have a sufficiently clear MHD interpretation.
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