Maqola

Two types of coronal bright points their characteristics, and evolution

I. SattarovTashkent State Pedagogical University, 103 Yusif Kxos Kxojib str., Tashkent 100070, UzbekistanNina KarachikNational Solar Observatory, Sunspot, NM 88349, USAChori T. SherdanovAstronomical Institute of the Academy of Sciences of UzbekistanAzlarxon TillaboevTashkent State Pedagogical University, 103 Yusif Kxos Kxojib str., Tashkent 100070, UzbekistanAlexei PevtsovNational Solar Observatory, Sunspot, NM 88349, USA

Proceedings of the International Astronomical Unionjournal2010en

ABI

Annotatsiya

Abstract 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.

Mavzular

Solar and Space Plasma Dynamics Stellar, planetary, and galactic studies Astro and Planetary Science

Identifikatorlar

DOI: 10.1017/s1743921311015511

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