Unbalanced infrared radiation and natural laser effect in atmospheres of Venus and Mars

Details Unbalanced infrared radiation and natural laser effect in atmospheres of Venus and Mars Unbalanced infrared radiation and natural laser effect in atmospheres of Venus and Mars

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984rpspr.......81g&link_type=abstract

In its USSR Rept.: Space (JPRS-USP-84-003) p 81-82 (SEE N84-28823 19-12) Transl. into ENGLISH from Kosmich. Issled. (USSR), v

Physics

Atmospheric Models, Atmospheric Temperature, Capture Effect, Carbon Dioxide, Infrared Radiation, Mars Atmosphere, Molecular Excitation, Venus Atmosphere, Lasers, Mars (Planet), Planetary Temperature, Radiation Absorption, Venus (Planet)

Scientific paper

The partical variable temperature and CO2 excitation in the 15 micrometer band and the infrared range below 4.3 micrometers in the atmospheres of Venus and Mars were studied theoretically. In addition an analysis was made of infrared radiation in the 10.6 and 9.4 micrometer bands for CO2 in the context of the features of infrared radiation capture. Studies were done for altitudes of 80 to 130 kilometers for Venus and 35 to 120 kilometers for Mars. The model and analytical method employed in the study were described. It was found that in the near-infrared (4.3 micrometers), there is direct conversion of absorbed radiation into planetary atmospheric radiation at 10.6 and 9.4 micrometers. A layer of unbalanced infrared radiation exists in these fields at an altitude of approximately 108 kilometers on Venus and about 60 kilometers on Mars at intensities of 2300 and 320 ERG/sq cm/sec respectively. Inversion settling occurs at 10.6 micrometers at the 00 deg 1 to 10 deg 0 boundary at altitudes of 110 to 125 kilometers for Venus and 70 to 80 kilometers for Mars. The findings indicate that Venus and Mars are the first known natural laser objects in the infrared range.

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