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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| Опубліковано в: : | Кинематика и физика небесных тел |
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| Дата: | 2005 |
| Автори: | , , , , |
| Формат: | Стаття |
| Мова: | Англійська |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2005
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| Теми: | |
| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/79696 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| Резюме: | 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.
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| ISSN: | 0233-7665 |