Some new aspects in analyzing photopolarimetric observations of planets
Some new difficulties appearing in analyzing polarimetric observations of planets with optically thick and optically thin atmospheres are discussed. Using the atmosphere of Jupiter as an example, it is demonstrated that specific choice of particle shape in model computations can affect significantly...
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| Опубліковано в: : | Кинематика и физика небесных тел |
|---|---|
| Дата: | 2005 |
| Автори: | , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2005
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| Теми: | |
| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/79695 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | Some new aspects in analyzing photopolarimetric observations of planets / J.M. Dlugach, M.I. Mishchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 437-442. — Бібліогр.: 13 назв. — англ. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-79695 |
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dspace |
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Dlugach, J.M. Mishchenko, M.I. 2015-04-03T19:32:16Z 2015-04-03T19:32:16Z 2005 Some new aspects in analyzing photopolarimetric observations of planets / J.M. Dlugach, M.I. Mishchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 437-442. — Бібліогр.: 13 назв. — англ. 0233-7665 https://nasplib.isofts.kiev.ua/handle/123456789/79695 Some new difficulties appearing in analyzing polarimetric observations of planets with optically thick and optically thin atmospheres are discussed. Using the atmosphere of Jupiter as an example, it is demonstrated that specific choice of particle shape in model computations can affect significantly the values of cloud particle parameters retrieved from photopolarimetric data. Besides, we consider the influence of various factors on the interpretation of ptotopolarimetric observations of Mars performed during periods of high transparency of its atmosphere. The re-analysis of the polarization phase curves obtained in such periods shows the impossibility to derive reliable estimates of the properties of Martian dust particles. en Головна астрономічна обсерваторія НАН України Кинематика и физика небесных тел MS5: Dynamics and Physics of Solar System Bodies Some new aspects in analyzing photopolarimetric observations of planets Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Some new aspects in analyzing photopolarimetric observations of planets |
| spellingShingle |
Some new aspects in analyzing photopolarimetric observations of planets Dlugach, J.M. Mishchenko, M.I. MS5: Dynamics and Physics of Solar System Bodies |
| title_short |
Some new aspects in analyzing photopolarimetric observations of planets |
| title_full |
Some new aspects in analyzing photopolarimetric observations of planets |
| title_fullStr |
Some new aspects in analyzing photopolarimetric observations of planets |
| title_full_unstemmed |
Some new aspects in analyzing photopolarimetric observations of planets |
| title_sort |
some new aspects in analyzing photopolarimetric observations of planets |
| author |
Dlugach, J.M. Mishchenko, M.I. |
| author_facet |
Dlugach, J.M. Mishchenko, M.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 |
Some new difficulties appearing in analyzing polarimetric observations of planets with optically thick and optically thin atmospheres are discussed. Using the atmosphere of Jupiter as an example, it is demonstrated that specific choice of particle shape in model computations can affect significantly the values of cloud particle parameters retrieved from photopolarimetric data. Besides, we consider the influence of various factors on the interpretation of ptotopolarimetric observations of Mars performed during periods of high transparency of its atmosphere. The re-analysis of the polarization phase curves obtained in such periods shows the impossibility to derive reliable estimates of the properties of Martian dust particles.
|
| issn |
0233-7665 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/79695 |
| citation_txt |
Some new aspects in analyzing photopolarimetric observations of planets / J.M. Dlugach, M.I. Mishchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 437-442. — Бібліогр.: 13 назв. — англ. |
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AT dlugachjm somenewaspectsinanalyzingphotopolarimetricobservationsofplanets AT mishchenkomi somenewaspectsinanalyzingphotopolarimetricobservationsofplanets |
| first_indexed |
2025-12-07T16:38:25Z |
| last_indexed |
2025-12-07T16:38:25Z |
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