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Theoretical calculations of atmospheric emission and absorption spectra in the far-infrared
Affiliation:1. Harvard-Smithsonian Center for Astrophysics, Atomic and Molecular Physics Division, Cambridge, MA, USA;2. Tomsk State University, Laboratory of Quantum Mechanics of Molecules and Radiative Processes, Tomsk State University, Tomsk, Russia;3. University of Reading, Dept. of Meteorology, Reading, UK;4. Battelle Pacific Northwest National Laboratory, Richland, WA, USA;5. Ford Motor Company, Research & Advanced Engineering, Dearborn, MI, USA;6. Department of Physics and Astronomy, University of Leicester, Leicester, UK;7. National Centre for Earth Observation, University of Leicester, Leicester, UK;8. Leicester Institute for Space and Earth Observation, University of Leicester, Leicester, UK;9. Old Dominion University, Dept. of Chemistry & Biochemistry, Norfolk, VA, USA;10. DLR, Institute for Remote Sensing Technology, Wessling, Germany;11. St. Francis Xavier University, Department of Physics, Antigonish, NS, Canada;12. University of Castilla-La Mancha, Dept. of Physical Chemistry, Faculty of Pharmacy, Albacete, Spain;13. International Atomic Energy Agency (IAEA), Vienna, Austria;1. Physical and Life Sciences, Lawrence Livermore National Laboratory, Livermore, CA, 94550, USA;2. Mechanical and Aerospace Engineering, Center for Advanced Turbomachinery and Energy Research (CATER), University of Central Florida, Orlando, FL 32816, USA;3. Department of Physics, University of Central Florida, Orlando FL, 32816 USA
Abstract:Over the past decade the National Physical Laboratory has been using the method of far-infrared Fourier transform spectroscopy to determine the composition of the upper atmosphere(1,2) In support of this work we have developed a computer program(3) which enables us to calculate theoretical atmospheric spectra using as input data the spectral line positions, strengths and half-widths and appropriate atmospheric profiles of temperature and mixing ratio. This paper presents the results of some recent calculations using this program.
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