Behaviour of solar active prominence

Title:

Behaviour of solar active prominence

Creator:

Kučera, A., Rybák, J., and Saniga, M.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:7fd921bf-7065-47ad-b19e-5e1b47c546e4
uuid:7fd921bf-7065-47ad-b19e-5e1b47c546e4

Subject:

solar prominence and spectral analysis

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

Introduction: Prominences are well suited for investigating the energy balance, radiative transfer, and complex interchange of mass between the solar photosphere, chromosphere and corona. They are still a subject of interest in solar physics. The spectral analysis and morphological properties of prominences usually provide us with an important information on the dynamics, radiative transfer, and stability of the prominences. Of a great interest are the prominences with centrál reversal in their Hα profile since they may display appreciable variations in activity. Such observations have also been included in our scientific programme with the Stará Lesná spectrograph because a long series of Hα profiles of prominences can be recorded.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

232-235

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1998 Volume:87-88 | Number:88

Harvested from:

CDK

Metadata only:

false