Hostname: page-component-7bb8b95d7b-5mhkq Total loading time: 0 Render date: 2024-09-13T09:22:55.226Z Has data issue: false hasContentIssue false
  • English
  • Français

Pumping of Rossby Waves and Vortices at the Base of the Solar Convection Zone

Published online by Cambridge University Press:  08 February 2017

Evgeniy Tikhomolov
Evgeniy Tikhomolov*
Affiliation:
Institute of Solar-Terrestrial Physics SD RAS, Irkutsk, 664033, P.O. Box 4026, Russia

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 

References

Tikhomolov, E.M. (1994) Sustenance of vortex structures in a rotating fluid layer heated from below, JETP Letters 59, pp. 163–167.Google Scholar
Tikhomolov, E. (1996) Short-scale convection and long-scale deformationally-unstable Rossby wave in a rotating fluid layer heated from below, Phys. of Fluids 8(12), pp. 3329–3337.Google Scholar
Tikhomolov, E.M. and Mordvinov, V.I. (1996) The peculiar behavior of the large-scale components of the solar magnetic field as a result of Rossby vortex excitation beneath the convection zone, Astrophys. J. 472, pp. 389–398.Google Scholar