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Latitudinal Distribution of the Coronal Bright Points at Solar Minimum and the Rising Phase of Solar Activity Cycle 23

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, UzbekistanAzlarxon TillaboevTashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan

Proceedings of the International Astronomical Unionjournal2004en

ABI

Annotatsiya

We show that the latitudinal distribution of the coronal bright points (BPs) changes between the solar minimum and the rising phase of solar cycle 23. In 1996, the number of BPs peaks near the disk center. In 1998, the distribution shows bands of increased BPs' number at the ARs' latitudes.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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Solar and Space Plasma Dynamics Stellar, planetary, and galactic studies Geophysics and Gravity Measurements

Identifikatorlar

DOI: 10.1017/s1743921304007264

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