Physics
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..131..239h&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 131, Feb. 1991, p. 239-257.
Physics
9
Magnetic Flux, Magnetic Signatures, Solar Activity, Solar Magnetic Field, Digital Data, Solar Cycles, Solar Observatories
Scientific paper
The Mount Wilson daily magnetogram data set is analyzed to examine the daily growth and decay of active region magnetic fields. Rates of magnetic flux growth and decay, both absolute and in terms of percentage, are studied for various subsets of the data. The daily percentage flux growth of regions is about twice as great as the percentage flux decay. Relationships are found between daily flux change and region size, hemisphere, cycle phase, leading and following polarities, normal and reversed polarity orientation, rotation rate, meridional drift rate and region complexity. In general, growth and decay of flux is faster in more active situations: at cycle maximum or for the more active hemisphere. Leading polarity fields grow and decay more rapidly than following polarity fields. Regions with reversed magnetic polarity orientations have much larger rates of flux growth and decay than do normally oriented regions, but this is an effect of region size. The smallest rates of flux growth and decay are seen for regions rotating nearest the average rate and with the smallest meridional drift rates. These results are discussed in terms of the current understanding of how regions form and decay.
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