CALCULATE METHOD OF THE TWILIGHT SKY BRIGHTNESS IN THE SOLAR VERTICAL, STIPULATED BY A MULTIPLE SCATTERING OF A SUNLIGHT

Autor:	Shakun, L. S., Motrich, V. D., Melykjants, S. M.
Jazyk:	angličtina
Rok vydání:	2017
Předmět:	lcsh:QB1-991 lcsh:Astronomy Astrophysics::Solar and Stellar Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Quantitative Biology::Genomics Astrophysics::Galaxy Astrophysics remote sounding atmospheric sounding twilight sounding multiple scattering Physics::Geophysics
Zdroj:	Odessa Astronomical Publications, Vol 17, Iss 0, Pp 78-81 (2017) Odessa Astronomical Publications; Том 17 (2004); 78-81
ISSN:	1810-4215
Popis:	Use of a twilight sounding method of the Earth's atmosphere with the aim to reveal aerosols inflow to the upper and medial atmosphere needs a method of separation twilight sky brightness to the brightness of primary and secondary twilight. Method of secondary twilight brightness calculation on a declination of the logarithm of twilight sky brightness caused by a multiple scattering of sunlight is discussed. The calculation procedure of a declination of the logarithm of secondary twilight brightness on observations in solar vertical is given. The use equal declination of the logarithm of secondary twilight brightness for all viewing directions in solar vertical is proved.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c1e832a9d7bd1ec11ebbe30d11b1a430 http://oap.onu.edu.ua/article/view/93260 Zobrazit plný text záznamu