Possibilities of the spectroscopic detection of oxygen in the lower atmosphere of Venus

Details Possibilities of the spectroscopic detection of oxygen in the lower atmosphere of Venus Possibilities of the spectroscopic detection of oxygen in the lower atmosphere of Venus

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..812k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, Sept.-Oct. 1984, p. 812-815. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Lower Atmosphere, Oxygen Spectra, Planetary Composition, Venus Atmosphere, Absorption Spectra, Atmospheric Chemistry, Fabry-Perot Spectrometers, Spectral Line Width, Spectral Resolution, Vertical Distribution

Scientific paper

It is shown that a diffraction spectrometer with a resolution of 1 A can ensure a detection threshold of molecular oxygen of 1 ppb for a constant relative concentration of O2 in the entire atmosphere, 3 ppb when O2 is present only above 25 km, and 30 ppb when O2 is present only in the cloud layer. If these thresholds are raised, the diffraction spectrometer will make it possible to acquire data on the vertical profile of O2 concentration in the lower atmosphere of Venus.

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