A model of the atmospheric convection zone with a large increase of rotation velocity between its bottom and top (Q796383)
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scientific article; zbMATH DE number 3864796
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | A model of the atmospheric convection zone with a large increase of rotation velocity between its bottom and top |
scientific article; zbMATH DE number 3864796 |
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A model of the atmospheric convection zone with a large increase of rotation velocity between its bottom and top (English)
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1982
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A simple model of a slowly rotating stellar or planetary atmospheric convection zone is considered supposing that only growing convective perturbations contribute to the value of nonlinear azimuthal force maintaining the differential rotation of the zone. A hypothesis is put forward that fast rotation of the upper atmosphere of Venus is due to such resonance interaction.
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slowly rotating stellar or planetary atmospheric convection zone
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only growing convective perturbations
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nonlinear azimuthal force
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differential rotation
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fast rotation
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upper atmosphere of Venus
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