Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-20T07:32:12.931Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Published online by Cambridge University Press:  14 March 2005

I. Sattarov ,
A.A. Pevtsov ,
N.V. Karachek  and
A.M. Tillaboev
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]
A.M. Tillaboev
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: [email protected]
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 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

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 665 - 666
Copyright
© 2004 International Astronomical Union