Remote sensing of planetary atmospheres: Venus
More than any other planet except the Earth, Venus has been the subject of a variety of remote sensing investigations over a wide range of wavelengths. Since Venus has complete cloud cover, with a complex composition and layering, the retrieval of the information from these measurements is particula...
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| Format: | Conference item |
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1998
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| _version_ | 1826267137864368128 |
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| author | Taylor, F |
| author_facet | Taylor, F |
| author_sort | Taylor, F |
| collection | OXFORD |
| description | More than any other planet except the Earth, Venus has been the subject of a variety of remote sensing investigations over a wide range of wavelengths. Since Venus has complete cloud cover, with a complex composition and layering, the retrieval of the information from these measurements is particularly challenging. The problem is further complicated by the high temperatures and pressures found in the deep atmosphere, resulting in a novel and interesting radiative transfer problem even before scattering and absorption by cloud particles is taken into account. This paper reviews the achievements so far of remote sensing of Venus and future challenges and opportunities. (C) 1998 COSPAR. Published by Elsevier Science Ltd. |
| first_indexed | 2024-03-06T20:49:36Z |
| format | Conference item |
| id | oxford-uuid:371f86e3-7e3e-43f6-98be-31c502962820 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T20:49:36Z |
| publishDate | 1998 |
| record_format | dspace |
| spelling | oxford-uuid:371f86e3-7e3e-43f6-98be-31c5029628202022-03-26T13:42:03ZRemote sensing of planetary atmospheres: VenusConference itemhttp://purl.org/coar/resource_type/c_5794uuid:371f86e3-7e3e-43f6-98be-31c502962820Symplectic Elements at Oxford1998Taylor, FMore than any other planet except the Earth, Venus has been the subject of a variety of remote sensing investigations over a wide range of wavelengths. Since Venus has complete cloud cover, with a complex composition and layering, the retrieval of the information from these measurements is particularly challenging. The problem is further complicated by the high temperatures and pressures found in the deep atmosphere, resulting in a novel and interesting radiative transfer problem even before scattering and absorption by cloud particles is taken into account. This paper reviews the achievements so far of remote sensing of Venus and future challenges and opportunities. (C) 1998 COSPAR. Published by Elsevier Science Ltd. |
| spellingShingle | Taylor, F Remote sensing of planetary atmospheres: Venus |
| title | Remote sensing of planetary atmospheres: Venus |
| title_full | Remote sensing of planetary atmospheres: Venus |
| title_fullStr | Remote sensing of planetary atmospheres: Venus |
| title_full_unstemmed | Remote sensing of planetary atmospheres: Venus |
| title_short | Remote sensing of planetary atmospheres: Venus |
| title_sort | remote sensing of planetary atmospheres venus |
| work_keys_str_mv | AT taylorf remotesensingofplanetaryatmospheresvenus |