Here we present a laboratory study of CO2 absorption spectra, obtained at high temperatures and pressures, similar to those encountered in the Venusian atmosphere. These spectra have been recorded using a Fourier Transform InfraRed (FT-IR) spectrometer, which is equipped to operate from 800 to 30,000 cm(-1) (0.33-12.5 mu m) with a resolution from 0.06 to 10 cm(-1). A dedicated gas cell, designed to support pressures up to 200 bar and temperatures up to 350 degrees C, has been coupled to the FT-IR. Starting from a realistic vertical pressure-temperature profile of the Venus' atmosphere, based on measurements performed with atmospheric probes, we have recorded a series of absorption spectra of CO2, varying the pressure and temperature from 1 to 50 bar and from 294 to 650 K.

Experimental CO2 absorption coefficients at high pressure and high temperature

Snels M;
2013

Abstract

Here we present a laboratory study of CO2 absorption spectra, obtained at high temperatures and pressures, similar to those encountered in the Venusian atmosphere. These spectra have been recorded using a Fourier Transform InfraRed (FT-IR) spectrometer, which is equipped to operate from 800 to 30,000 cm(-1) (0.33-12.5 mu m) with a resolution from 0.06 to 10 cm(-1). A dedicated gas cell, designed to support pressures up to 200 bar and temperatures up to 350 degrees C, has been coupled to the FT-IR. Starting from a realistic vertical pressure-temperature profile of the Venus' atmosphere, based on measurements performed with atmospheric probes, we have recorded a series of absorption spectra of CO2, varying the pressure and temperature from 1 to 50 bar and from 294 to 650 K.
2013
Istituto di Scienze dell'Atmosfera e del Clima - ISAC
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/173277
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