Our theory ofumbral oscillations as resonant modes of magneto-atmospheric waves is extended and confirmed by calculating the resonant modes in a much more detailed model of the umbral atmosphere. The depths of forcing required to produce observed oscillation periods (roughly 140 to 185 s) are in go
A simple two cavity model for umbral oscillations
โ Scribed by H.S. Yun; J.W. Lee
- Book ID
- 107880595
- Publisher
- Elsevier Science
- Year
- 1988
- Tongue
- English
- Weight
- 237 KB
- Volume
- 31
- Category
- Article
- ISSN
- 0083-6656
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