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Emission measures and heating mechanisms for stellar transition regions and coronae
Published online by Cambridge University Press: 04 August 2017
Abstract
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In order to determine the heating mechanisms for stellar transition regions and coronae we try to determine the damping lengths for the mechanical flux(es) responsible for the heating. For the lower part of the transition regions (30,000 < T≤100,000 K) the damping lengths are consistent with Shockwave damping. This appears to be also true for the upper part of the transition region in Procyon, while for the upper part of the solar transition region the damping length is much larger.
- Type
- Stellar Coronae: Chromospheres of Cool Stars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 359 - 360
- Copyright
- Copyright © Reidel 1987
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