Continuous absorption and depression in the solar spectrum at wavelengths from 650 to 820 nm

Author:

Vavrukh M. V.,Vasil’eva I. E.,Stelmakh O. M.,Tyshko N. L.

Publisher

Allerton Press

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference50 articles.

1. L. H. Aller, Atoms, Stars and Nebulae (Blackiston, Philadelphia, 1943; Mir, Moscow, 1976).

2. I. N. Atroshchenko, A. S. Gadun, S. I. Gopasyuk, et al., Variations in the Global Characteristics of the Sun, Ed. by E. A. Gurtovenko (Nauk. Dumka, Kiev, 1991) [in Russian].

3. K. A. Burlov-Vasil’ev, I. E. Vasil’eva, and Yu. B. Matveev, “New measurements of the absolute spectral energy distribution of solar radiation in the range= 650–1070 nm,” Kinematika Fiz. Nebesnykh Tel 12 (3), 75–91 (1996).

4. M. V. Vavrukh and O. M. Stel’makh, “Photoionization cross-section of negative hydrogen ions,” Visn. L’viv. Univ., Ser. Fiz. 47, 3 (2012).

5. M. V. Vavrukh and O. M. Stel’makh, “The cross-sections of the main processes that forms the continuous absorption coefficient in the photosphere of Sun-like stars,” Zh. Fiz. Dosl. 17, 4902 (2013).

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