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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, IAUS223(2004)

DOI: 10.1017/s1743921304007264

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

Journal article published in 2004 by I. Sattarov, A. A. Pevtsov ORCID, N. V. Karachek, A. M. Tillaboev
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

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.