作者: I.S. Veselovsky , A.N. Zhukov , A.V. Dmitriev , M.V. Tarsina , F. Clette
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摘要: We report on observations of the solar luminosity variations in Fe xii line (195 A) over period 1996–1999, which corresponds to minimum and rising phase current 23rd cycle. The relatively or rather high temporal cadence spatial resolution Extreme-ultraviolet Imaging Telescope (EIT) board Solar Heliospheric Observatory (SOHO) allowed a nearly continuous measurement intensity different structures Sun. find that significant contribution longitudinal asymmetry, thus 27-day variability EUV radiation, is produced by numerous intermediate brightness elements are globally distributed large areas (up about \( \sim \frac{2}{3} \) whole surface Sun). When activity low, this component even becomes dominant from localized active regions bright points. This suggests weak magnetic field outside constitute an important factor through modulates luminosity.