Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1765344 | Advances in Space Research | 2010 | 5 Pages |
Abstract
Alfvén waves have been invoked as an important mechanism of particle acceleration in stellar winds of cool stars. After their identification in the solar wind they started to be studied in winds of stars located in different regions of the HR diagram. We discuss here some characteristics of these waves and we present a direct application in the acceleration of late-type stellar winds.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
A.A. Vidotto, V. Jatenco-Pereira,