Radiative damping of trapped gravity waves in the solar atmosphere
✍ Scribed by Patricia André Clark; Alfred Clark
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 383 KB
- Volume
- 30
- Category
- Article
- ISSN
- 0038-0938
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✦ Synopsis
The radiative damping of trapped gravity waves in an optically thin atmosphere is studied for a stratified Boussinesq fluid. The character of the atmospheric eigenmodes depends on the distribution of the Brunt-V~iis~il/i frequency N and the radiative relaxation time r. The calculations for simple layer models show that if Nr is large over some finite fraction of the trapping region, then modes of long lifetime can exist. In order to suppress gravity waves entirely, it is necessary that Nr ~< 1 over the entire trapping region. Qualitative application of the results to the solar atmosphere leads to the conclusion that gravity wave eigenmodes of the solar atmosphere, although damped, are by no means eliminated by radiative effects.
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