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Number of Coronal Bright Points in Different Phases of the Solar Activity Cycle

I. SattarovTashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, UzbekistanAlexei PevtsovNational Solar ObservatoryN.V. KarachekTashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, UzbekistanCh.T. SherdanovAstronomical Institute AS of Uzbekistan, 33 Astronomicheskaya ul., Tashkent 700052, Uzbekistan

Proceedings of the International Astronomical Unionjournal2004en

ABI

Annotatsiya

We present the preliminary results of study of the coronal bright points (BPs) using the SoHO/EIT data. We show that the number of BPs in quiet Sun areas does not vary between 1996 and 1997. In 1998 the BPs number (full disk) increases by about 20%.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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Mavzular

Solar and Space Plasma Dynamics Solar Radiation and Photovoltaics Stellar, planetary, and galactic studies

Identifikatorlar

DOI: 10.1017/s1743921304007276

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