Infrared heterodyne spectroscopy

Details Infrared heterodyne spectroscopy Infrared heterodyne spectroscopy

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982opten..21..313m&link_type=abstract

Optical Engineering, vol. 21, Mar.-Apr. 1982, p. 313-319.

Astronomy and Astrophysics

Astrophysics

17

Astrophysics, Infrared Spectroscopy, Optical Heterodyning, Thermal Emission, Thermodynamic Equilibrium, Atomic Structure, Carbon Dioxide, Doppler Effect, Line Spectra, Mesosphere, Molecular Structure, Planetary Atmospheres

Scientific paper

Infrared heterodyne spectroscopy is an extremely useful tool for Doppler-limited studies of atomic and molecular lines in diverse astrophysical regions. The current state of the art is reviewed, and the analysis of CO2 lines in the atmosphere of Mars is outlined. Doppler-limited observations have enabled the discovery of natural laser emission in the mesosphere of Mars and the discovery of failure of local thermodynamic equilibrium near the surface of Mars.

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