Solar cycle variation of sunspot intensity and X-ray bright points

Details Solar cycle variation of sunspot intensity and X-ray bright points Solar cycle variation of sunspot intensity and X-ray bright points

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234l.147m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 234, Dec. 1, 1979, p. L147-L149. Research supported by the Norges Al

Astronomy and Astrophysics

Astronomy

6

Infrared Astronomy, Solar Cycles, Solar X-Rays, Sunspots, Correlation, Dynamo Theory, Penumbras, Photosphere, Umbras

Scientific paper

Evidence is presented for a possible link between the physical conditions in individual large sunspots and the occurrence of X-ray bright points. For the period 1970-1978 a close correlation is reported between the infrared intensity of large sunspots and the number of X-ray bright points. It is pointed out that the well-known dynamo theory for sunspots, in its present form, is unable to explain the observations.

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