High-speed solar-wind plasma fluxes and solar active regions

Details High-speed solar-wind plasma fluxes and solar active regions High-speed solar-wind plasma fluxes and solar active regions

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976kosis..14..248z&link_type=abstract

Kosmicheskie Issledovaniia, vol. 14, Mar.-Apr. 1976, p. 248-256. In Russian.

Physics

Interplanetary Magnetic Fields, Solar Activity Effects, Solar Wind Velocity, Explorer 34 Satellite, Shock Fronts, Time Dependence, Velocity Distribution

Scientific paper

A possible connection between increases in solar-wind velocity and solar active regions is investigated using IMP-6 data on solar-wind speed for a three-month period. The velocity of the shock front caused by interactions between solar-wind fluxes with different speeds is estimated, and it is shown that active regions play a substantial part in forming the sector structure of the interplanetary magnetic field. It is found that active regions are the sources of the high-speed solar wind in about 95% of the cases examined.

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