Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation method

Details Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation method Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation method

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....92.7269k&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 92, July 1, 1987, p. 7269-7279.

Physics

96

Scintillation Counters, Solar Cycles, Solar Wind Velocity, Velocity Distribution, Solar Activity, Solar Corona, Solar Magnetic Field, Three Dimensional Flow

Scientific paper

The solar cycle evolution of solar wind speed structure was studied for
the years from 1973 to 1985 on the basis of interplanetary scintillation
observations using a new method for mapping solar wind speed to the
source surface.

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