VARIATIONS OF THE SOLAR FLARE ENERGY SPECTRUM OVER TWO ACTIVITY CYCLES (1972 - 1995)

V. V. KASINSKY; R. T. SOTNIKOVA

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VARIATIONS OF THE SOLAR FLARE ENERGY SPECTRUM OVER TWO ACTIVITY CYCLES (1972 - 1995) KCI 등재 SCOPUS

V. V. KASINSKY, R. T. SOTNIKOVA

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URLhttps://db.koreascholar.com/Article/Detail/387910

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천문학회지 (Journal of The Korean Astronomical Society)

제29권 제S호 (1996.12)
pp.315-316

한국천문학회 (Korean Astronomical Society)

초록

Based on X-ray (1-8 Å) flux data for 1972-1995 the integral spectra of solar flare energy were computed. It has been shown that the spectral index β of the integral energy spectrum (IES) vanes systematically with the 11-year cycle phase. The interval of $\beta$ 수식 이미지-variations (0.47 <β<1) is characteristic of UV-Cet stars. The maximum energy of the X-ray flares does not exceed 10 32 erg.

저자

V. V. KASINSKY(Department of Physics, Irkutsk State University)
R. T. SOTNIKOVA(Department of Physics, Irkutsk State University)

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