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The study on fine structures in solar prominences

✍ Scribed by A. Adjabshirizadeh; H. Ebadi


Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
290 KB
Volume
95
Category
Article
ISSN
0022-4073

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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