Articles | Volume 14, issue 11
https://doi.org/10.5194/amt-14-7187-2021
https://doi.org/10.5194/amt-14-7187-2021
Research article
 | 
17 Nov 2021
Research article |  | 17 Nov 2021

A simulation chamber for absorption spectroscopy in planetary atmospheres

Marcel Snels, Stefania Stefani, Angelo Boccaccini, David Biondi, and Giuseppe Piccioni

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Cited articles

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Ballard, J., Strong, K., Remedios, J., Page, M., and Johnston, W.: A coolable long path absorption cell for laboratory spectroscopic studies of gases, J. Quant. Spectrosc. Ra., 52, 677–691, https://doi.org/10.1016/0022-4073(94)90034-5, 1994. a, b
Baranov, Y., Fraser, G., Lafferty, W., and Vigasin, A.: Weakly interacting molecular pairs, in: NATO Science, vol. 27, chap. Collision-induced absorption in the CO2 Fermi triad for temperatures from 211 K to 296 K, NATO Advanced Research Workshop, 25–28 March 2002, Abbaye de Fontevraud, France, Series Nato Science 27, Kluwer Academic, 149–158, 2003. a, b, c, d
Briesmeister, R., Read, G., Kim, K., and Fitzpatrick, J.: Long path length temperature-controlled absorption cell for spectroscopic studies of radioactive compounds, Appl. Spectrosc., 38, 35–38, 1978. a, b
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Short summary
A novel simulation chamber, PASSxS (Planetary Atmosphere Simulation System for Spectroscopy), has been developed for absorption measurements with a Fourier transform spectrometer (FTS) and possibly a cavity ring-down (CRD) spectrometer, with a sample temperature ranging from 100 K up to 550 K, while the pressure of the gas can be varied up to 60 bar. These temperature and pressure ranges cover a significant part of the planetary atmospheres in the solar system and possibly extrasolar planets.