Vertical cloud distribution in the Uranian atmosphere

In this work, the vertical cloud distribution in the Uranian atmosphere is investigated. We used the method of determinination of the deviation scope of the real atmosphere from homogeneity conditions. The idea of this methods is that the diffusely reffected radiations form at different effective de...

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Дата:2011
Автор: Kostogryz, N.M.
Формат: Стаття
Мова:English
Опубліковано: Advances in astronomy and space physics 2011
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119086
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Vertical cloud distribution in the Uranian atmosphere / N.M. Kostogryz // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 77-80. — Бібліогр.: 22 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-1190862017-06-04T03:03:10Z Vertical cloud distribution in the Uranian atmosphere Kostogryz, N.M. In this work, the vertical cloud distribution in the Uranian atmosphere is investigated. We used the method of determinination of the deviation scope of the real atmosphere from homogeneity conditions. The idea of this methods is that the diffusely reffected radiations form at different effective depths in the atmosphere, namely: the strong absorption bands form higher in the atmosphere than weak ones. The same is for separate absorption bands: their centres form in higher atmospheric layers than other points of bands or lines contours. The relative methane concentration for all points of the contours of absorption bands will be the same only for a homogeneous atmosphere and will show the systematic deviation in the center and near the edge of the absorption bands in the case of an inhomogeneous atmosphere. It was obtained that Uranus' atmosphere has two cloud layers: the first one in the region with pressure within the range 1.5 − 1.8 bar, and the second one in the region with the pressure 3.5 − 5.5 bar. We also can conclude that aerosol was more abundant in 1981 compared to 1993 and 1995 which was found in our previous work. 2011 Article Vertical cloud distribution in the Uranian atmosphere / N.M. Kostogryz // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 77-80. — Бібліогр.: 22 назв. — англ. 987-966-439-367-3 http://dspace.nbuv.gov.ua/handle/123456789/119086 en Advances in Astronomy and Space Physics Advances in astronomy and space physics
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description In this work, the vertical cloud distribution in the Uranian atmosphere is investigated. We used the method of determinination of the deviation scope of the real atmosphere from homogeneity conditions. The idea of this methods is that the diffusely reffected radiations form at different effective depths in the atmosphere, namely: the strong absorption bands form higher in the atmosphere than weak ones. The same is for separate absorption bands: their centres form in higher atmospheric layers than other points of bands or lines contours. The relative methane concentration for all points of the contours of absorption bands will be the same only for a homogeneous atmosphere and will show the systematic deviation in the center and near the edge of the absorption bands in the case of an inhomogeneous atmosphere. It was obtained that Uranus' atmosphere has two cloud layers: the first one in the region with pressure within the range 1.5 − 1.8 bar, and the second one in the region with the pressure 3.5 − 5.5 bar. We also can conclude that aerosol was more abundant in 1981 compared to 1993 and 1995 which was found in our previous work.
format Article
author Kostogryz, N.M.
spellingShingle Kostogryz, N.M.
Vertical cloud distribution in the Uranian atmosphere
Advances in Astronomy and Space Physics
author_facet Kostogryz, N.M.
author_sort Kostogryz, N.M.
title Vertical cloud distribution in the Uranian atmosphere
title_short Vertical cloud distribution in the Uranian atmosphere
title_full Vertical cloud distribution in the Uranian atmosphere
title_fullStr Vertical cloud distribution in the Uranian atmosphere
title_full_unstemmed Vertical cloud distribution in the Uranian atmosphere
title_sort vertical cloud distribution in the uranian atmosphere
publisher Advances in astronomy and space physics
publishDate 2011
url http://dspace.nbuv.gov.ua/handle/123456789/119086
citation_txt Vertical cloud distribution in the Uranian atmosphere / N.M. Kostogryz // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 77-80. — Бібліогр.: 22 назв. — англ.
series Advances in Astronomy and Space Physics
work_keys_str_mv AT kostogryznm verticalclouddistributionintheuranianatmosphere
first_indexed 2023-10-18T20:33:45Z
last_indexed 2023-10-18T20:33:45Z
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