Large-scale and solar cycle variations of the solar wind

Details Large-scale and solar cycle variations of the solar wind Large-scale and solar cycle variations of the solar wind

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ssrv...17..221n&link_type=abstract

(IAU, IUGG, URSI, IUPAP, COSPAR, and SCOSTEP, International Solar-Terrestrial Physics Symposium, Sao Paulo, Brazil, June 17-24,

Physics

7

Interplanetary Magnetic Fields, Solar Cycles, Solar Wind Velocity, Spatial Dependencies, Latitude, Long Term Effects, Magnetic Field Configurations, Mass Flow Rate, Radial Distribution, Spatial Distribution

Scientific paper

Space probe observations relevant to the determination of the large-scale, three-dimensional structure of the solar wind and its solar cycle variations are summarized. There is a pronounced decrease in the velocity spread about the average as distance from the sun increases (from 0.6 to 5 AU). A latitude variation is found for several plasma parameters, and a dependence on the phase of the solar activity cycle is demonstrated by some of the data.

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