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CaiiK2Vspectral features and their relation to small-scale photospheric magnetic fields

✍ Scribed by K. R. Sivaraman; W. C. Livingston


Publisher
Springer
Year
1982
Tongue
English
Weight
492 KB
Volume
80
Category
Article
ISSN
0038-0938

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✦ Synopsis


Although the Ca II K232 network is known to be cospatial with magnetic elements there has been doubt as to the magnetic origin of the fainter Kzv points. We demonstrate that weak magnetic elements also lie at the roots of the K2v points, and because the latter are numerous they may contribute sensibly to the integrated light profile of Ca II K.


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