Computer Science
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ssrv...53..173k&link_type=abstract
Space Science Reviews (ISSN 0038-6308), vol. 53, Aug. 1990, p. 173-222.
Computer Science
85
Solar Wind Velocity, Sunspot Cycle, Velocity Distribution, Interplanetary Medium, Scintillation, Solar Activity, Spatial Distribution
Scientific paper
A review is given of observational results concerning the solar cycle dependence of the global structure of solar wind speed distribution during the years from 1973 to 1987. Since observations of solar wind speed in three-dimensional space can only be made by the interplanetary scintillation method which has been carried out over one sunspot activity cycle since the early 1970's, the review is based on IPS observations. The low-speed regions tend to be distributed along neutral lines which are derived on the source surface, so comparisons between speed distribution and the neutral line are discussed.
Kakinuma Takakiyo
Kojima Masayoshi
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