Complexes of activity and coronal holes.

Details Complexes of activity and coronal holes. Complexes of activity and coronal holes.

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991bsold...2...78b&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 2/91, p. 78 - 83

Statistics

2

Solar Coronal Holes: Solar Active Regions, Statistics: Solar Activity

Scientific paper

Complexes of activity (CA), after their active phase, transform into extensive unipolar magnetic regions (UMR), which, in principle, create the necessary conditions for the production of coronal holes (CH). The intercomparison of CA and CH synoptic maps for the declining branch of cycle No. 21 shows that there does, indeed, exist a number of signature indicating a relationship between these features. It is concluded that there appears to be a causal association of CH with CA.

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