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

  • I. Sattarov (a1), A.A. Pevtsov (a2), N.V. Karachek (a1) and Ch.T. Sherdanov (a1) (a3)

Abstract

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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