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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


