Do changes in the photospheric magnetic network cause the 11 year variation of total solar irradiance?

Details Do changes in the photospheric magnetic network cause the 11 year variation of total solar irradiance? Do changes in the photospheric magnetic network cause the 11 year variation of total solar irradiance?

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...383l..89f&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 383, Dec. 20, 1991, p. L89-L92.

Astronomy and Astrophysics

Astrophysics

49

Irradiance, Photosphere, Solar Magnetic Field, Sunspot Cycle, Analysis Of Variance, Astronomical Photometry, Radiant Flux Density

Scientific paper

Changes in the area of the photospheric magnetic network over the sunspot cycle have been put forward as the 'missing component' required to explain the 11-yr variation of total solar irradiance observed by space-borne radiometers. It is shown that this explanation is consistent with recent measurements of the photometric contrast of magnetic faculae and with the present measurement of the network area change during cycle 21.

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