Radiative transfer in fine structures of solar prominences
β Scribed by A. Ajabshirizadeh; A.G. Nikoghossian; H. Ebadi
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 191 KB
- Volume
- 103
- Category
- Article
- ISSN
- 0022-4073
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π SIMILAR VOLUMES
Faint, Doppler shifted, emission features are detected in high resolution spectra of limb prominences. Their average line-of-sight velocity is about 3 x 106 cm s i, their average life time is 300 s, and their angular sizes are ~<10 s cm in our spectrograms. The emission line width of the spectral fe
The Ca Β§ K line of the quiescent prominence of 15 October 1969 observed at the Abastumani Astrophysical Observatory of the Academy of Sciences of Georgia, U.S.S.R. is studied in detail. The behaviour of various fragments of the prominence with the line-of-sight Doppler velocities is investigated for