The effect of the mutual orientation of the background solar magnetic field and a field in the region of a flare on the propagation velocity of the flare stream

Details The effect of the mutual orientation of the background solar magnetic field and a field in the region of a flare on the propagation velocity of the flare stream The effect of the mutual orientation of the background solar magnetic field and a field in the region of a flare on the propagation velocity of the flare stream

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24....6p&link_type=references

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, Jan.-Feb. 1984, p. 6-10. In Russian.

Physics

1

Solar Flares, Solar Magnetic Field, Solar Wind Velocity, Background Radiation, Differential Equations, Lines Of Force, Magnetic Field Configurations

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