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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
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: isattar@astin.uzsci.net
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: apevtsov@nso.edu
N.V. Karachek
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: isattar@astin.uzsci.net
A.M. Tillaboev
Affiliation:
Tashkent State Pedagogical University, 103 Usif Xos-Hojib St., Tashkent 700100, Uzbekistan, email: isattar@astin.uzsci.net
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Abstract

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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
Copyright
© 2004 International Astronomical Union