Astrophysics

    

Magnetic Activity of Solar-Type Stars

Authors: Sylwester Kornowski

Here we described the origin of the magnetic-activity cycles of solar-like cool stars. On the basis of the atom-like structure of baryons, we calculated the ratios of the activity-cycle period to rotation period for the Sun and for the active and inactive branches. We also solved the coronal heating problem.

Comments: 10 Pages.

Download: PDF

Submission history

[v1] 2020-12-15 09:51:15
[v2] 2020-12-17 05:37:35

Unique-IP document downloads: 248 times

Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.

Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.

comments powered by Disqus