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Collisional Induced Absorption (CIA) bands measured in the IR spectral range

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2016

Publication Year

2020-12-16T10:39:06Z

Acceptance in OA@INAF

Collisional Induced Absorption (CIA) bands measured in the IR spectral range

Title

STEFANI, STEFANIA; PICCIONI, GIUSEPPE; Snels, M.; Adriani, A.; Grassi, D.

Authors

http://hdl.handle.net/20.500.12386/28878

Handle

MEMORIE DELLA SOCIETA ASTRONOMICA ITALIANA

Journal

87

Number

(2)

Mem. S.A.It. Vol. 87, 208

c

SAIt 2016 Memoriedella

Collisional Induced Absorption (CIA) bands

measured in the IR spectral range

S. Stefani1, G. Piccioni1, M. Snels2, A. Adriani1, and D. Grassi1

1 IAPS-INAF, via Fosso del cavaliere 100, Rome (Italy)

e-mail: Stefania.Stefani@iaps.inaf.it

2 ISAC-CNR, via Fosso del cavaliere 100, Rome (Italy)

Abstract.

In this work we present two experimental setup able to characterize the optical properties of gases, in particular CO2and H2, at typically planetary conditions. The apparatus consists of a

Fourier Transform InfraRed (FT-IT) interferometer able to work in a wide spectral range, from 350 to 25000 cm−1(0.4 to 29 µm ) with a relatively high spectral resolution, from 10 to 0.07 cm−1. Two dedicated gas cells have been integrated with the FT-IR. The first, called High Pressure High Temperature (HP-HT), can support pressures up to 300 bar, temperatures up to 300oC and is

char-acterized by an optical path of 2 cm. The second one, a Multi Pass (MP) absorption gas cell, is designed to have a variable optical path, from 2.5 to 30 m, can be heated up to 200oand operate at

pressures up to 10 bar. In this paper, measurements of Collision-Induced Absorption (CIA) bands in carbon dioxide and hydrogen recorded in the InfraRed spectral range will be presented. In principle, linear symmetric molecules such as CO2and H2possess no dipole moment, but, even

when the pressure is only a few bar, we have observed the Collisional Induced Absorption (CIA) bands. This absorption results from a short-time collisional interaction between molecules. The band integrated intensity shows a quadratic dependence versus density opposed to the absorption by isolated molecules, which follows Beer’s law (Frommhold 1993). This behaviour suggests an absorption by pairs rather than by individual molecules. The bands integrated intensities show a linear dependence vs square density according to (Baranov and Vigasin 1999) and (Vigasin 1996). For what concerns the H2CIA bands, a preliminary comparison between simulated data

obtained with the model described in (Borysow et al. 1985)and measured, shows a good agree-ment. These processes are very relevant in the dense atmospheres of planets, such as those of Venus and Jupiter and also in extrasolar planets. A detailed knowledge of these contributions is very important to include this effect in the radiative transfer calculations.

Acknowledgements. We acknowledge the ASI support of this research in the framework of the JUICE (2013-056-R.O.) and Venus Express (I/050/10/0) contracts.

References

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Stefani et al.: CIA bands measured in the IR spectral range 209

Borysow, J., Trafton, L., Frommhold, L., Birnbaum, G. 1985, ApJ, 296, 644

Frommhold, L. 1993, Collision-Induced Absorption in Gases, Cambridge monographs on atomic, molecular and chemical Physics

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