Physics
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..203l&link_type=abstract
Solar Physics, vol. 79, Aug. 1982, p. 203-230.
Physics
49
Magnetic Flux, Photosphere, Solar Cycles, Solar Magnetic Field, Stellar Models, Coronal Holes, Solar Activity, Solar Rotation, Stellar Evolution
Scientific paper
Models of open solar magnetic structures for periods near solar maximum and minimum, together with previous models of open magnetic structures during the declining phase, provide clues to the relations between open structures, coronal holes, and active regions at different times of the solar cycle. It is suggested that near solar minimum, the emergence of new flux with the polarity imblance required to maintain open magnetic structures may occur primarily at very small spatial scales, while near solar maximum the active regions role in maintaining open structures and coronal holes is prominent. The rotation properties of calculated open structures near solar maximum strongly suggest two classes of features: one that rotates differentially, as do sunspots and active regions, and a separate class that rotates more rigidly, as was the case for single large coronal holes during Skylab.
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