Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-02T23:07:55.745Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  14 March 2005

I. Sattarov
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: [email protected]
A.A. Pevtsov
Affiliation:
National Solar Observatory
Operated by the Association of Universities for Research in Astronomy (AURA, Inc) under cooperative agreement with the National Science Foundation (NSF).
, Sunspot, NM 88349, USA email: [email protected]
N.V. Karachek
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: [email protected]
Ch.T. Sherdanov
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: [email protected] Astronomical Institute AS of Uzbekistan, 33 Astronomicheskaya ul., Tashkent 700052, Uzbekistan email: chori@astrin,uzsci.net
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union