Physics
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..660o&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, July-Aug. 1987, p. 660-662. In Russian.
Physics
3
Coronal Holes, Interplanetary Magnetic Fields, Solar Magnetic Field, Space-Time Functions, Histograms, Solar Atmosphere, Statistical Analysis
Scientific paper
The statistical correlation between the large-scale solar magnetic field and the IMF sector structure is examined. It is shown that, despite a close interrelationship, there can be slight divergences between the two, connected with the inadequacy of their determination and the presence of short-term perturbations. A refined determination is made of the boundary-zone width between the beginning of the coronal hole and the boundary of the large-scale solar magnetic field; a value of 40-50 heliographic degrees is obtained.
Obridko Vladimir N.
Shel'Ting B. D.
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