Statistical analysis of the space-time structure of the solar wind

Details Statistical analysis of the space-time structure of the solar wind Statistical analysis of the space-time structure of the solar wind

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18..998e&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 18, Nov.-Dec. 1978, p. 998-1002. In Russian.

Physics

1

Photosphere, Solar Magnetic Field, Solar Wind Velocity, Spatial Distribution, Latitude, Solar Cycles, Statistical Analysis, Time Dependence

Scientific paper

The characteristic features of the space-time picture of the solar wind at large distances from the sun is studied on the basis of solar wind velocity data for 1972-1976. The spatial structure of the solar wind was found to be significantly dependent on solar latitude. The solar-latitude-dependent structure of solar wind velocities is related to large-scale characteristics of the distribution of mass fluxes and magnetic fields in the photosphere and corona. The evolution of these features in different periods of the solar activity cycle is examined.

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