Modeling of the 10-micron natural laser emission from the mesospheres of Mars and Venus

Details Modeling of the 10-micron natural laser emission from the mesospheres of Mars and Venus Modeling of the 10-micron natural laser emission from the mesospheres of Mars and Venus

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...55..356d&link_type=abstract

Icarus (ISSN 0019-1035), vol. 55, Sept. 1983, p. 356-368.

Astronomy and Astrophysics

Astronomy

36

Laser Outputs, Mesosphere, Radiative Transfer, Astronomical Models, Prediction Analysis Techniques, Solar Heating, Planets, Mesosphere, Mars, Venus, Observations, Emissions, Laser, Flux, Source, Formation, Absorption, Infrared, Wavelengths, Models, Collisions, Carbon Dioxide, Comparisons, Theoretical Studies, Kinetics, Temperature, Analysis, Altitude, Rotation

Scientific paper

Nonthermal emission which occurs in the cores of the 9.4- and 10.4-μm CO2 bands on Mars has been recently identified as a natural atmospheric laser. The emission is believed to be excited by absorption of near-ir solar flux, followed by collisional transfer to the 00°1 state of CO2. A numerical model based on this mechanism is developed which includes the solar pumping contributed by ≡2×104 near-ir CO2 lines.

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