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Fine structure of the thermal emission of the earth's atmosphere
Affiliation:1. Department of Geology, University of Georgia, Athens, GA 30602, USA;2. Georgia Electron Microscopy, University of Georgia, Athens, GA 30602, USA;1. Financial University under the Government of Russian Federation, 49 Leningradsky Prospekt, Moscow, Russia;2. National Research University Higher School of Economics, 20 Myasnitskaya str., Moscow, Russia;3. Lomonosov Moscow State University, 1-2 Leninskiye Gory, Moscow, Russia;1. Intelligent Systems for Medicine Laboratory, School of Mechanical and Chemical Engineering, The University of Western Australia, 35 Stirling Highway, Crawley/Perth, WA 6009, Australia;2. School of Engineering, Cardiff University, UK;1. Dana-Dwek Children''s Hospital, Tel Aviv Sourasky Medical Center, Sackler Faculty of Medicine, Tel Aviv University, Israel;2. Division of Pulmonary Medicine, Cincinnati Children''s Hospital Medical Center, Cincinnati, Ohio;3. Pediatric Pulmonology Unit, Wolfson Medical Center, Holon, Israel;4. Division of Biostatistics and Epidemiology, Cincinnati Children''s Hospital Medical Center, Cincinnati, Ohio;5. Division of Hospital Medicine, Cincinnati Children''s Hospital Medical Center, Cincinnati, Ohio;6. Department of Pediatrics, University of Cincinnati College of Medicine, Cincinnati, Ohio;7. Department of Cardiovascular Diseases, Mayo Clinic, Rochester, Minnesota;8. Department of Pediatrics, University of Colorado School of Medicine, Children''s Hospital Colorado, Aurora, Colorado
Abstract:The difficulties of investigating the composition and structure of the Earth's atmosphere by satellite measurement of the spectral distribution of the outward radiation are discussed. Calculations are made of the contour of isolated emission lines of various intensities at different altitudes in the atmosphere. The change in altitude of the lines' contour under conditions of standard atmospheric stratification is analysed. Line “rotations” and “splitting” phenomena are found. Taking the examples discussed as a basis the importance is shown of investigating the fine structure of the atmosphere's emission spectrum to solve the “converse” problems of atmospheric spectroscopy.
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