Convection in the equatorial layers of rotating chemically inhomogeneous stars

Details Convection in the equatorial layers of rotating chemically inhomogeneous stars Convection in the equatorial layers of rotating chemically inhomogeneous stars

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15...33d&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Jan. 1989, p. 33-41. In Russian. In Russian.

Statistics

Computation

Conductive Heat Transfer, Convective Heat Transfer, Cosmochemistry, Stellar Rotation, Computational Astrophysics, Stellar Structure, Traveling Waves

Scientific paper

Spatial structures arising upon transition from the heat conductivity regime to the convection regime in the equatorial layers of rotating chemically inhomogeneous stars is considered. These structures resemble two-dimensional waves (rolls) travelling along or opposite the direction of rotation and extended along the meridian. It is shown that both the subcritical and supercritical appearance of the structures is possible, depending on the rotation rate and the degree of chemical inhomogeneity.

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