Наукова електронна бібліотека
періодичних видань НАН України
періодичних видань НАН України
On a mechanism of polarization origin at the polar regions of Jupiter
Репозиторій DSpace/Manakin
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| dc.contributor.author | Goryunova, O.S. | |
| dc.contributor.author | Korokhin, V.V. | |
| dc.contributor.author | Akimov, L.A. | |
| dc.contributor.author | Shalygin, E.V. | |
| dc.contributor.author | Velikodsky, Yu.I. | |
| dc.date.accessioned | 2015-04-03T19:34:48Z | |
| dc.date.available | 2015-04-03T19:34:48Z | |
| dc.date.issued | 2005 | |
| dc.identifier.citation | 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. | uk_UA |
| dc.identifier.issn | 0233-7665 | |
| dc.identifier.uri | http://dspace.nbuv.gov.ua/handle/123456789/79696 | |
| dc.description.abstract | 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. | uk_UA |
| dc.language.iso | en | uk_UA |
| dc.publisher | Головна астрономічна обсерваторія НАН України | uk_UA |
| dc.relation.ispartof | Кинематика и физика небесных тел | |
| dc.subject | MS5: Dynamics and Physics of Solar System Bodies | uk_UA |
| dc.title | On a mechanism of polarization origin at the polar regions of Jupiter | uk_UA |
| dc.type | Article | uk_UA |
| dc.status | published earlier | uk_UA |
