On the disappearance of a small sunspot group

Details On the disappearance of a small sunspot group On the disappearance of a small sunspot group

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...81...33w&link_type=abstract

Solar Physics, vol. 81, Nov. 1982, p. 33-46.

Physics

50

Magnetic Flux, Solar Magnetic Field, Sunspots, Astronomical Photography, Magnetic Signatures, Photosphere, Solar Granulation

Scientific paper

The small sunspot group associated with Hale active region 17694 was observed jointly by the Mount Wilson and the Big Bear Solar Observatories, through the time of sunspot disappearance. The magnetic flux from the region was seen to decrease by about 10% per day during the observing interval. This was accompanied by fragmentation of the dominant spot as a supergranule network formed. No evidence for spreading or diffusion of the active region field was found.

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