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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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| Main Authors: | , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2005
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| Series: | Кинематика и физика небесных тел |
| Subjects: | |
| Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/79695 |
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