Physics
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..197o&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Mar.-Apr. 1987, p. 197-200. In Russian.
Physics
7
Coronal Holes, Interplanetary Magnetic Fields, Magnetic Disturbances, Magnetohydrodynamic Flow, Solar Wind, High Speed, Histograms, Statistical Analysis
Scientific paper
A statistical analysis of a large volume of data shows that most high-speed streams of the solar wind are generated right after passage through the sector structure (SS) of the IMF and just before passage through the coronal-hole (CH) boundary. About 74 to 87 percent of the CH is located within sectors of the same polarity, and the width of the boundary zone between the SS and CH commencement amounts to 20-40 heliographic degrees. About 38-57 percent of all high-speed streams connected with CHs commence in this zone.
Obridko Vladimir N.
Shel'Ting B. D.
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