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Autor:
Wollmann, Jiří
Solar flare is a process which releases magnetic energy stored in the solar corona due to the effect of magnetic reconnection. Similar activity has been observed on other stellar types, namely type K and M stars, which usually have vast and strong ma
Externí odkaz:
http://www.nusl.cz/ntk/nusl-448260
Autor:
Kára, Jan
The works deals with the study of the flare stars, which is a group of stars for which sudden brightening can be observed. The work focuses on a star GJ 3236, which is a low-mass eclipsing binary and on which numerous flares have been observed. For t
Externí odkaz:
http://www.nusl.cz/ntk/nusl-383145