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Angular velocity distribution in convective regions and the origin of solar differential rotation

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Abstract

The observed differential rotation of the Sun is explained as a result of interaction between global rotation and convective eddies.

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Authors and Affiliations

  1. Space Research Institute, Moscow, U.S.S.R.

    G. S. Bisnovatyi-Kogan

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  1. G. S. Bisnovatyi-Kogan
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Bisnovatyi-Kogan, G.S. Angular velocity distribution in convective regions and the origin of solar differential rotation. Sol Phys 128, 299–304 (1990). https://doi.org/10.1007/BF00154166

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  • DOI: https://doi.org/10.1007/BF00154166

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