The structure and parameters of flare streams

Details The structure and parameters of flare streams The structure and parameters of flare streams

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.6649p&link_type=abstract

Journal of Geophysical Research, vol. 84, Nov. 1, 1979, p. 6649-6652.

Physics

15

Plasma Jets, Solar Flares, Transition Layers, Shock Fronts, Solar Magnetic Field, Solar Wind

Scientific paper

The structure and parameters of flare streams in relation to the location of the flare and to the configuration of the large-scale magnetic field on the sun are considered. The following results are obtained: (1) the flare streams spread in a rather wide angle (approximately + or - 60 deg); (2) the velocity of the streams ejected by the flares in the sun's western hemisphere is 1.5 times higher than that of the streams ejected by eastern flares; (3) the sign of Bz being fixed, the sign of Bx within the stream is determined by the location of the flare with respect to the solar equator; and (4) the polytropic index for the solar-wind plasma (1.4-1.7) is close to or less than the adiabatic value.

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