DETERMINATION OF THE SECOND TWILIGHT BRIGHTNESS BY THE METHOD OF THE TWILIGHT PROBING OF THE EARTH’S ATMOSPHERE

Автор(и)

  • Yu. I. Zaginailo Odessa National University, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.1993.6.104692

Ключові слова:

brightness of the sky’s nightglow, secondary twilight

Анотація

A new method of ’gradients’ for determination of the secondary twilight brightness is proposed, which allows to determine the brightness of secondary twilight directly from the observations.

 

Посилання

Divari N.B., Zaginailo Yu.I: 1971, Doklady AN SSSR. 198, 1323.

Divari N.B.:1968. Atmosfernaia optika (Optics of the Atmosphere). M: Nauka, p.105.

Divari N.B.:1970, Atmosfernaia optika (Optics of the Atmosphere). M: Nauka.p.158.

Divari N.B.:1972, Bulletin Abastumanskoj astrofizitcheskoj observatorii. 41, 87.

Fesenkov V.G.:1955, Astron.Jhurn. 32. 265.

Fesenkov V.G.:1962, Trudy astrofizitcheskogo instituta AN Kaz.SSR. 3, 214

Fesenkov V.G.:1972, Bulletin Abastumanskoj astrofizitcheskoj observatorii. 41, 7.

Staude N.M.:1936, Trudy komisii po izutcheniyu stratosfery pri AN SSSR. 1, 1.

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Опубліковано

2017-06-20

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