The Solar Dynamo and Integrated Irradiance Variations in the Course of the 11-Year Cycle

Details The Solar Dynamo and Integrated Irradiance Variations in the Course of the 11-Year Cycle The Solar Dynamo and Integrated Irradiance Variations in the Course of the 11-Year Cycle

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000arep...44..771p&link_type=abstract

Astronomy Reports, vol. 44, Issue 11, p.771-779

Astronomy and Astrophysics

Astronomy

5

Scientific paper

the effect of the large-scale magnetic fields generated by the solar dynamo on the radiation flux issuing from the convection zone is studied. A governing equation describing convective heat transfer is obtained in the framework of mean-field magnetohydrodynamics, with account for the influence of magnetic fields and differential rotation on the energy budget of the convection zone. The principal effects are illustrated using a one-dimensional numerical model. Calculations indicate that the influence of large-scale magnetic fields can modulate the solar irradiance with a relative amplitude of ˜0.07%.

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