Turbulent heat transfer and latitudinal temperature variations in a rotating convective envelope

Details Turbulent heat transfer and latitudinal temperature variations in a rotating convective envelope Turbulent heat transfer and latitudinal temperature variations in a rotating convective envelope

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..723k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Aug. 1987, p. 723-729. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Convection Currents, Periodic Variations, Rotating Plasmas, Solar Atmosphere, Stellar Envelopes, Turbulent Heat Transfer, Photosphere, Temperature Distribution

Scientific paper

It is shown that allowance for nonlinear effects in the problem of turbulent heat transfer in a rotating convective envelope significantly decreases the dependence of temperature on latitude. Reasons for the appearance of this nonlinearity are given. The calculated equator-to-pole temperature difference in the solar photosphere is about 1 K, which does not contradict observational data.

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