Two sources of recurrent high-speed solar wind streams.

Details Two sources of recurrent high-speed solar wind streams. Two sources of recurrent high-speed solar wind streams.

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..256p&link_type=abstract

Geomagn. Aeron., Vol. 30, No. 2, p. 256 - 257

Physics

Solar Wind

Scientific paper

Variations of the mean diurnal values of the solar-wind velocity at the Earth's orbit during January - September 1979 are discussed. It has been shown that the value of the velocity in solar-wind streams formed near sector boundaries depends on the solar-radiation flux at a wavelength λ = 10.7 cm (r = 0.59); in streams generated within sectors, the velocity depends on the magnetic field intensity (r = 0.38) and does not depend on the radio emission power in the region of the source.

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