Volume 532, August 2011
|Number of page(s)||12|
|Published online||08 August 2011|
Rossby waves and polar spots in rapidly rotating stars: implications for stellar wind evolution
Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, 8042 Graz, Austria
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2 Departament de Física, Universitat de les Illes Balears, 07122 Palma de Mallorca, Spain
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3 Departament de Matemàtiques i Informàtica, Universitat de les Illes Balears, 07122 Palma de Mallorca, Spain
4 Institut für Physik, IGAM, Karl-Franzens Universität Graz, Universitätsplatz 5, 8010 Graz, Austria
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5 Abastumani Astrophysical Observatory at Ilia State University, University St. 2, Tbilisi, Georgia
Received: 21 April 2011
Accepted: 23 June 2011
Context. Rapidly rotating stars show short-period oscillations in magnetic activity and polar appearance of starspots.
Aims. The aim of this paper is to study large-scale shallow water waves in the tachoclines of rapidly rotating stars and their connection to the periodicity and the formation of starspots at high latitudes.
Methods. Shallow-water magnetohydrodynamic equations were used to study the dynamics of large-scale waves at the rapidly rotating stellar tachoclines in the presence of toroidal magnetic field. Dispersion relations and latitudinal distribution of wave modes were derived.
Results. We found that low-frequency magnetic Rossby waves tend to be located at poles, but high-frequency magnetic Poincaré waves are concentrated near the equator in rapidly rotating stars. These results have important implications for the evolution of the stellar wind in young Sun-like stars.
Conclusions. Unstable magnetic Rossby waves may lead to the local enhancement of magnetic flux at high latitudes of tachoclines in rapidly rotating stars. The enhanced magnetic flux may rise upwards owing to the magnetic buoyancy in the form of tubes and appear as starspots at polar regions. Magnetic Rossby waves may also cause observed short-term periodicity in the stellar magnetic activity.
Key words: stars: magnetic field / stars: activity / starspots / stars: oscillations / magnetohydrodynamics (MHD)
© ESO, 2011
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