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Pumping of Rossby Waves and Vortices at the Base of the Solar Convection Zone
Published online by Cambridge University Press: 08 February 2017
Extract
Rossby vortices excited near the base of the solar convection zone are very appealing objects for interpretation of a number of solar phenomena such as long-lived large-scale magnetic structures, the poleward drift of the axisymmetric components after the polar field reversal, and a peculiar long-term behavior of the nonaxisymmetric components (Tikhomolov and Mordvinov 1996).
- Type
- III. Large-Scale Structure of the Sun
- Information
- Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 177 - 178
- Copyright
- Copyright © Kluwer 1998