On a mechanism of polarization origin at the polar regions of Jupiter

We propose the following mechanism of linear polarization origin at Jupiter’s polar regions: the principal contribution in polarization is made by the light reflected by cloud layer and then scattered by stratospheric aerosol particles. The linear polarization distributions along the central meridia...

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Published in:Кинематика и физика небесных тел
Date:2005
Main Authors: Goryunova, O.S., Korokhin, V.V., Akimov, L.A., Shalygin, E.V., Velikodsky, Yu.I.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79696
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:On a mechanism of polarization origin at the polar regions of Jupiter / O.S. Goryunova, V.V. Korokhin, L.A. Akimov, E.V. Shalygin, Yu.I. Velikodsky // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 443-447. — Бібліогр.: 16 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79696
record_format dspace
spelling Goryunova, O.S.
Korokhin, V.V.
Akimov, L.A.
Shalygin, E.V.
Velikodsky, Yu.I.
2015-04-03T19:34:48Z
2015-04-03T19:34:48Z
2005
On a mechanism of polarization origin at the polar regions of Jupiter / O.S. Goryunova, V.V. Korokhin, L.A. Akimov, E.V. Shalygin, Yu.I. Velikodsky // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 443-447. — Бібліогр.: 16 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79696
We propose the following mechanism of linear polarization origin at Jupiter’s polar regions: the principal contribution in polarization is made by the light reflected by cloud layer and then scattered by stratospheric aerosol particles. The linear polarization distributions along the central meridian for two spectral bands (0.46 μm and 0.70 μm) are calculated. They are in good qualitative agreement with observational data. The mean scattering particle radius is estimated as rmean = 0.5 μm.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS5: Dynamics and Physics of Solar System Bodies
On a mechanism of polarization origin at the polar regions of Jupiter
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title On a mechanism of polarization origin at the polar regions of Jupiter
spellingShingle On a mechanism of polarization origin at the polar regions of Jupiter
Goryunova, O.S.
Korokhin, V.V.
Akimov, L.A.
Shalygin, E.V.
Velikodsky, Yu.I.
MS5: Dynamics and Physics of Solar System Bodies
title_short On a mechanism of polarization origin at the polar regions of Jupiter
title_full On a mechanism of polarization origin at the polar regions of Jupiter
title_fullStr On a mechanism of polarization origin at the polar regions of Jupiter
title_full_unstemmed On a mechanism of polarization origin at the polar regions of Jupiter
title_sort on a mechanism of polarization origin at the polar regions of jupiter
author Goryunova, O.S.
Korokhin, V.V.
Akimov, L.A.
Shalygin, E.V.
Velikodsky, Yu.I.
author_facet Goryunova, O.S.
Korokhin, V.V.
Akimov, L.A.
Shalygin, E.V.
Velikodsky, Yu.I.
topic MS5: Dynamics and Physics of Solar System Bodies
topic_facet MS5: Dynamics and Physics of Solar System Bodies
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description We propose the following mechanism of linear polarization origin at Jupiter’s polar regions: the principal contribution in polarization is made by the light reflected by cloud layer and then scattered by stratospheric aerosol particles. The linear polarization distributions along the central meridian for two spectral bands (0.46 μm and 0.70 μm) are calculated. They are in good qualitative agreement with observational data. The mean scattering particle radius is estimated as rmean = 0.5 μm.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79696
citation_txt On a mechanism of polarization origin at the polar regions of Jupiter / O.S. Goryunova, V.V. Korokhin, L.A. Akimov, E.V. Shalygin, Yu.I. Velikodsky // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 443-447. — Бібліогр.: 16 назв. — англ.
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first_indexed 2025-12-07T15:41:10Z
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