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Two types of coronal bright points their characteristics, and evolution

Published online by Cambridge University Press:  26 August 2011

Isroil Sattarov ,
Nina V. Karachik ,
Chori T. Sherdanov ,
Azlarxon M. Tillaboev  and
Alexei A. Pevtsov
Isroil Sattarov
Affiliation:
Tashkent State Pedagogical University, 103 Yusif Kxos Kxojib str., Tashkent 100070, Uzbekistan email: isattar@astrin.uz
Nina V. Karachik
Affiliation:
National Solar Observatory, Sunspot, NM 88349, USA email: apevtsov@nso.edu
Chori T. Sherdanov
Affiliation:
Astronomical Institute of the Academy of Sciences of Uzbekistan email: chori@astrin.uz
Azlarxon M. Tillaboev
Affiliation:
Tashkent State Pedagogical University, 103 Yusif Kxos Kxojib str., Tashkent 100070, Uzbekistan email: isattar@astrin.uz
Alexei A. Pevtsov
Affiliation:
National Solar Observatory, Sunspot, NM 88349, USA email: apevtsov@nso.edu
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Abstract

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Using maximum brightness of coronal bright point's (CBP) as a criterion, we separate them on two categories: dim CBPs, associated with areas of a quiet Sun, and bright CBPs, associated with an active Sun. This study reports on characteristics of two types of CBPs and their evolution.

Keywords

Solar coronacoronal bright points
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S273: The Physics of Sun and Star Spots , August 2010 , pp. 343 - 346
Copyright
Copyright © International Astronomical Union 2011

References

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