Large-scale inhomogeneities in the solar wind of solar origin

Details Large-scale inhomogeneities in the solar wind of solar origin Large-scale inhomogeneities in the solar wind of solar origin

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rvgsp..13.1053g&link_type=abstract

Reviews of Geophysics and Space Physics, vol. 13, July 1975, p. 1053-1058, 1072-1076.

Physics

Space Physics

15

Interplanetary Magnetic Fields, Nonuniform Plasmas, Solar Activity Effects, Solar Wind, Astronomical Models, Plasma Diagnostics, Plasma Interactions, Shock Wave Interaction, Solar Corona, Solar Wind Velocity

Scientific paper

Recent developments in the study of large-scale inhomogeneities of solar origin in the solar wind are discussed. On-site measurements of solar-wind streams are reviewed together with studies and models of stream interactions and their effects. Long- and short-term variations in the solar-wind flow are described as well as the effects of solar latitude on solar-wind speed, the dominant polarity of the interplanetary field, and the latter's polar component. Probable coronal origins are considered for streams and shock disturbances in the solar wind.

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