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Multi-wavelength Observations of Coronal Structure and Dynamics, Yohkoh 10th Anniversary Meeting, p. 97-98

DOI: 10.1016/s0964-2749(02)80026-9

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Solar cycle dependency of X-ray bright points and photospheric bipoles

Journal article published in 2002 by I. Sattarov, A. A. Pevtsov ORCID, A. S. Hojaev, C. T. Sherdonov
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

We employ daily Yohkoh SXT full disk images and National Solar Observatory/Kitt Peak (NSO/KP) photospheric magnetograms from 1993–1999 to study the solar cycle variation of X-ray bright points (XBP) and magnetic bipoles (BP). The XBP number follows a well-known anti-cycle variation, but the BP number does not. We see this as a clear indication that the anti-cycle variation of XBP number is an apparent, not a real effect.