Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results
The Viking infrared thermal mapper measures the thermal emission of the martian surface and atmosphere and the total reflected sunlight. With the high resolution and dense coverage being achieved, planetwide thermal structure is apparent at large and small scales. The thermal behavior of the best-ob...
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American Association for the Advancement of Science
1976
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ftcaltechauth:oai:authors.library.caltech.edu:74568 2023-05-15T18:02:14+02:00 Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results Kieffer, Hugh H. Chase, Stillman C., Jr. Miner, Ellis D. Palluconi, Frank Don Münch, Guido Neugebauer, Gerry Martin, Terry Z. 1976-08-27 https://authors.library.caltech.edu/74568/ https://resolver.caltech.edu/CaltechAUTHORS:20170227-162205245 unknown American Association for the Advancement of Science Kieffer, Hugh H. and Chase, Stillman C., Jr. and Miner, Ellis D. and Palluconi, Frank Don and Münch, Guido and Neugebauer, Gerry and Martin, Terry Z. (1976) Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results. Science, 193 (4255). pp. 780-786. ISSN 0036-8075. doi:10.1126/science.193.4255.780. https://resolver.caltech.edu/CaltechAUTHORS:20170227-162205245 <https://resolver.caltech.edu/CaltechAUTHORS:20170227-162205245> Article PeerReviewed 1976 ftcaltechauth https://doi.org/10.1126/science.193.4255.780 2021-11-18T18:40:55Z The Viking infrared thermal mapper measures the thermal emission of the martian surface and atmosphere and the total reflected sunlight. With the high resolution and dense coverage being achieved, planetwide thermal structure is apparent at large and small scales. The thermal behavior of the best-observed areas, the landing sites, cannot be explained by simple homogeneous models. The data contain clear indications for the relevance of additional factors such as detailed surface texture and the occurrence of clouds. Areas in the polar night have temperatures distinctly lower than the CO_2 condensation point at the surface pressure. This observation implies that the annual atmospheric condensation is less than previously assumed and that either thick CO_2 clouds exist at the 20-kilometer level or that the polar atmosphere is locally enriched by noncondensable gases. Article in Journal/Newspaper polar night Caltech Authors (California Institute of Technology) The Landing ENVELOPE(-45.689,-45.689,-60.733,-60.733) Science 193 4255 780 786 |
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Caltech Authors (California Institute of Technology) |
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ftcaltechauth |
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description |
The Viking infrared thermal mapper measures the thermal emission of the martian surface and atmosphere and the total reflected sunlight. With the high resolution and dense coverage being achieved, planetwide thermal structure is apparent at large and small scales. The thermal behavior of the best-observed areas, the landing sites, cannot be explained by simple homogeneous models. The data contain clear indications for the relevance of additional factors such as detailed surface texture and the occurrence of clouds. Areas in the polar night have temperatures distinctly lower than the CO_2 condensation point at the surface pressure. This observation implies that the annual atmospheric condensation is less than previously assumed and that either thick CO_2 clouds exist at the 20-kilometer level or that the polar atmosphere is locally enriched by noncondensable gases. |
format |
Article in Journal/Newspaper |
author |
Kieffer, Hugh H. Chase, Stillman C., Jr. Miner, Ellis D. Palluconi, Frank Don Münch, Guido Neugebauer, Gerry Martin, Terry Z. |
spellingShingle |
Kieffer, Hugh H. Chase, Stillman C., Jr. Miner, Ellis D. Palluconi, Frank Don Münch, Guido Neugebauer, Gerry Martin, Terry Z. Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results |
author_facet |
Kieffer, Hugh H. Chase, Stillman C., Jr. Miner, Ellis D. Palluconi, Frank Don Münch, Guido Neugebauer, Gerry Martin, Terry Z. |
author_sort |
Kieffer, Hugh H. |
title |
Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results |
title_short |
Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results |
title_full |
Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results |
title_fullStr |
Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results |
title_full_unstemmed |
Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results |
title_sort |
infrared thermal mapping of the martian surface and atmosphere: first results |
publisher |
American Association for the Advancement of Science |
publishDate |
1976 |
url |
https://authors.library.caltech.edu/74568/ https://resolver.caltech.edu/CaltechAUTHORS:20170227-162205245 |
long_lat |
ENVELOPE(-45.689,-45.689,-60.733,-60.733) |
geographic |
The Landing |
geographic_facet |
The Landing |
genre |
polar night |
genre_facet |
polar night |
op_relation |
Kieffer, Hugh H. and Chase, Stillman C., Jr. and Miner, Ellis D. and Palluconi, Frank Don and Münch, Guido and Neugebauer, Gerry and Martin, Terry Z. (1976) Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results. Science, 193 (4255). pp. 780-786. ISSN 0036-8075. doi:10.1126/science.193.4255.780. https://resolver.caltech.edu/CaltechAUTHORS:20170227-162205245 <https://resolver.caltech.edu/CaltechAUTHORS:20170227-162205245> |
op_doi |
https://doi.org/10.1126/science.193.4255.780 |
container_title |
Science |
container_volume |
193 |
container_issue |
4255 |
container_start_page |
780 |
op_container_end_page |
786 |
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1766172025292849152 |