A Comparison of Values of the Imaginary Part of Aerosol Refractive Index in the Latitudinal Belts of Saturn’s Northern Hemisphere
- Autores: Ovsak A.S.1, Tejfel V.G.2, Karimov A.M.2, Lysenko P.G.2
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Afiliações:
- Main Astronomical Observatory
- Fesenkov Astrophysical Institute
- Edição: Volume 34, Nº 3 (2018)
- Páginas: 161-165
- Seção: Dynamics and Physics of Bodies of the Solar System
- URL: https://ogarev-online.ru/0884-5913/article/view/178059
- DOI: https://doi.org/10.3103/S0884591318030066
- ID: 178059
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Resumo
Using the spectrophotometric measurements data of 2015, the relation of values of the imaginary part ni of aerosol refractive index was determined for latitudinal belts 17° N, 33° N, 49° N, and 66° N of Saturn’s disc. A steadily decreasing tendency in the relative ni values when moving northward from the equatorial region of the disk to the latitude 49° N, inclusive, was revealed. The ni values in the 17° N and 49° N belts were found to differ significantly from other latitudinal regions of the giant planet’s disk.
Sobre autores
A. Ovsak
Main Astronomical Observatory
Autor responsável pela correspondência
Email: ovsak@mao.kiev.ua
Ucrânia, Kyiv, 03143
V. Tejfel
Fesenkov Astrophysical Institute
Email: ovsak@mao.kiev.ua
Cazaquistão, Almaty, 050020
A. Karimov
Fesenkov Astrophysical Institute
Email: ovsak@mao.kiev.ua
Cazaquistão, Almaty, 050020
P. Lysenko
Fesenkov Astrophysical Institute
Email: ovsak@mao.kiev.ua
Cazaquistão, Almaty, 050020
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