Imaginary part of the refractive index of aerosol in latitudinal belts of Jupiter’s disc
- Авторы: Morozhenko A.V.1, Ovsak A.S.1, Vid’machenko A.P.1, Teifel V.G.2, Lysenko P.G.2
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Учреждения:
- Main Astronomical Observatory
- Fesenkov Astrophysical Institute
- Выпуск: Том 32, № 1 (2016)
- Страницы: 30-37
- Раздел: Dynamics and Physics of Bodies of the Solar System
- URL: https://ogarev-online.ru/0884-5913/article/view/177836
- DOI: https://doi.org/10.3103/S0884591316010062
- ID: 177836
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Аннотация
The values of the imaginary part of the refractive index ni of aerosol in bright (EZ, NTrZ, and STrZ) and dark (NTB, NEB, SEB, and STB) latitudinal bands of Jupiter’s disc have been determined. They are averaged over the effective depth where the intensity of radiation diffusely reflected by the planet is formed. These values turned out to be lower in the zones than in the belts: specifically, 0.00017–0.00041 vs. 0.00063–0.00098, 0.00019–0.00041 vs. 0.00065–0.00097, 0.00017–0.00041 vs. 0.00070–0.00112, and 0.00019–0.00044 vs. 0.00069–0.00111 at λ = 605, 631, 714, and 742 nm, respectively. These results probably indicate the difference in the vertical stratification of the nature of cloud layers, as well as in the sizes of aerosol particles (they are larger in the belts).
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Об авторах
A. Morozhenko
Main Astronomical Observatory
Email: ovsak@mao.kiev.ua
Украина, ul. Akadademika Zabolotnoho 27, Kyiv, 03680
A. Ovsak
Main Astronomical Observatory
Автор, ответственный за переписку.
Email: ovsak@mao.kiev.ua
Украина, ul. Akadademika Zabolotnoho 27, Kyiv, 03680
A. Vid’machenko
Main Astronomical Observatory
Email: ovsak@mao.kiev.ua
Украина, ul. Akadademika Zabolotnoho 27, Kyiv, 03680
V. Teifel
Fesenkov Astrophysical Institute
Email: ovsak@mao.kiev.ua
Казахстан, Almaty, 050020
P. Lysenko
Fesenkov Astrophysical Institute
Email: ovsak@mao.kiev.ua
Казахстан, Almaty, 050020
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