Spatial and temporal variations of Ca II K line profile shapes in different structures of solar chromosphere. I. Features of individual profiles

We have studied Ca II K line profiles, using two time series of spectrograms taken in two regions near the solar disk center. In each of the regions, the spectrograph slit cut out several areas of the quiet region and a plage. For the selected chromospheric structures, we have derived K line profile...

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Bibliographic Details
Main Authors: Turova I.P., Grigoryeva S.A., Ozhogina O.A.
Format: Article
Language:English
Published: INFRA-M 2018-12-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/ru/nauka/article/24423/view