Observation of filamentary structure in sunspot umbrae
β Scribed by D. Papathanasoglou
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 585 KB
- Volume
- 21
- Category
- Article
- ISSN
- 0038-0938
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π SIMILAR VOLUMES
Our theory of a resonator for slow magneto-atmospheric waves in the chromosphere of a sunspot umbra has been used to check different models of the structure of the chromosphere and transition region. Oscillations of velocity and intensity in CIV, SiIv, and OIv lines observed by Gurman et al. (1982)
Zentralinstitut fiir Astrophysik der Akadcmic der Wissenschaftcn der DDR Sonneiiol~servatoriuin Einsteintnrni IVitli 5 f i p r e s (Rcceivctl 1984 Sovembrr 30) Multiple wavelength observations of sunspot umbrae can only be expalined by an inhomogeneous, two-component model for the structure of the u