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On peculiarities of the H and K Caiilines of quiescent prominences

โœ Scribed by N. N. Morozhenko

Publisher
Springer
Year
1974
Tongue
English
Weight
240 KB
Volume
35
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

A study of the metallic lines in bright quiescent prominences indicates that the optical thickness in the K line of Ca II may reach values as high as 103. This is about 10 times larger than the optical thickness in the Hc~ line and may explain some peculiarities of the H and K lines in solar prominences.

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