Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26at...20..509s&link_type=abstract
Astronomical and Astrophysical Transactions, vol. 20, Issue 3, pp.509-513
Astronomy and Astrophysics
Astronomy
Sun - X-Ray, Sun - Bright Points, Solar Activity
Scientific paper
The relation of the X-ray bright point number to the intensity of X-ray background is studied on the basis of satellite observations. The daily X-ray bright point number for the time interval 1991-1999 was inferred from YOHKOH Soft X-ray telescope data. It was found that the X-ray bright point number is indeed anti-correlated with the solar activity indices as was found from SKYLAB data a little earlier. At the same time the X-ray bright point number is anti-correlated with the intensity of the X-ray background from GOES data. The high degree of anti-correlation of the number of XBPs with the X-ray background data inspires the assumption that the number of XBPs slightly alters during the solar cycle. It was shown that the maximum number of XBPs strongly depends on the X-ray background level: the lower the level, the greater the number.
Hojaev Alisher S.
Ladenkov O. V.
Sattarov Isroil
Sherdonov Ch.T.
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