Origin of quasi-stationary high-velocity solar wind fluxes /Review/

Details Origin of quasi-stationary high-velocity solar wind fluxes /Review/ Origin of quasi-stationary high-velocity solar wind fluxes /Review/

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18..769k&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 18, Sept.-Oct. 1978, p. 769-797. In Russian.

Physics

Magnetohydrodynamic Flow, Solar Activity Effects, Solar Cycles, Solar Physics, Solar Wind, Coronal Holes, Magnetic Field Configurations, Particle Energy, Radiant Flux Density, Solar Corona, Solar Corpuscular Radiation, Solar Magnetic Field, Solar Terrestrial Interactions, Solar Wind Velocity

Scientific paper

The present paper deals with some aspects of high-velocity solar wind fluxes at heliocentric distances on the order of 1 AU near the plane of the ecliptic. The variation of the flux characteristics over a solar activity cycle is examined, along with the problem of localizing regions which give rise to high-velocity solar wind fluxes on the solar disk. The energy balance of the solar corona and solar wind is studied.

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