Infrared remote sensing of planetary atmospheres |
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| Institution: | 1. Department of Bioengineering, University of Washington, Seattle, WA 98195, USA;2. School of Engineering, The University of British Columbia, Kelowna, BC V1V 1V7, Canada;1. Department of Earth and Environmental Sciences, University of Pavia, Pavia, Italy;2. Laboratoire de Géologie, ENS–CNRS UMR 8538, Université PSL, Paris, France;3. Department of Earth Science, University of Hamburg, Hamburg, Germany;4. Department of Earth Science, Environment & Life, University of Genoa, Genoa, Italy;1. Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, Peking University, Beijing 100871, China;2. Frontiers Science Center for Deep Ocean Multispheres and Earth System, Key Lab of Submarine Geoscience and Prospecting Techniques, College of Marine Geosciences, Ocean University of China, Qingdao 266100, China;3. The State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences and Resources, China University of Geosciences, Beijing 100083, China;4. School of Geoscience and Technology, Southwest Petroleum University, Chengdu, Sichuan 610500, China;5. Key Laboratory of Ministry of Education on Safe Mining of Deep Metal Mines, Department of Geology, School of Resources and Civil Engineering, Northeastern University, Shenyang 110819, China;6. Development Research Center, China Geological Survey, Beijing 100037, China;1. Maximizing Health Outcomes Research Lab, Sapir College, Sderot, Israel;2. Community Medical Services Division, Clalit Health Services, Tel-Aviv, Israel;3. Faculty of Health Sciences, Ben-Gurion University of the Negev, Beer-Sheva, Israel;4. Department of Health Policy and Management and Department of Industrial Engineering and Management, Ben-Gurion University of the Negev, Beer-Sheva, Israel;5. Department of Health Policy and Management, Harvard T. H. Chan School of Public Health, Boston, MA, USA;1. State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences (Beijing), Beijing 100083, China;2. School of Earth Sciences and Resources, China University of Geosciences (Beijing), Beijing 100083, China;3. State Key Laboratory of Ore Deposit Geochemistry, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang 550002, China;4. Geological Survey of Canada, Calgary Natural Resources Canada, 3303 33rd Street NW, Calgary, AB T2L 2A7, Canada |
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| Abstract: | Infrared remote sensing is a powerful tool for studying the chemical composition and the thermal structure of planetary atmospheres. Infrared spectra, in particular, are used to derive molecular abundances and to infer elemental and isotopic ratios, which allow to constrain theoretical models of the formation and early evolution of the solar system, as well as the history of planetary atmospheres. Infrared imaging and spectroscopy have been performed from the ground but also from space planetary missions (Mariner 9 on Mars, Voyager on the giant planets, Galileo on Jupiter), and from the ISO Earth-orbiting infrared satellite. In the forthcoming decade, the Cassini mission will explore the Saturn system. Planetary exploration from Earth orbit will be performed by the FIRST and NGST space observatories. |
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