A numerical simulation of observations of the spatial properties of the five-minute oscillations is carried out, assuming the oscillations are internal gravity waves excited by granular convection according to the theory of Thomas et al. (1971). The simulation includes the effects of seeing and fini
Solar five-minute oscillations of low, intermediate, and high degree
β Scribed by H. M. Antia; S. M. Chitre; D. Narashima
- Publisher
- Springer Netherlands
- Year
- 1986
- Tongue
- English
- Weight
- 219 KB
- Volume
- 118
- Category
- Article
- ISSN
- 0004-640X
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