Variation of the solar constant during 1978-79 and 1981

Details Variation of the solar constant during 1978-79 and 1981 Variation of the solar constant during 1978-79 and 1981

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986baicz..37..202p&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 37, July 1986, p. 202-210.

Astronomy and Astrophysics

Astronomy

2

Periodic Variations, Solar Activity Effects, Solar Constant, Sunspots, Convective Heat Transfer, Magnetohydrodynamic Waves, Nimbus 7 Satellite, Solar Magnetic Field, Solar Maximum Mission

Scientific paper

The measurements of the Nimbus-7 and the SMM satellites indicate decreases of the solar constant in the order of a few hundredths and tenths of a percent on a time scale from days to weeks. It seems that the largest decreases of the solar constant occurred when quickly developing sunspot groups with complex structure were on the solar disk. It seems that the magnetic fields of the 'active' sunspot groups could stop the convection, and that the MHD waves originating during this process could transport one part of the radiation deficit due to the sunspots.

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