Abstract
A low temperature vacuum cell 220 cm in length with windows of quartz, ZnSe, and KBr has been designed for working with the high resolution Bruker IFS 125-M Fourier spectrometer. It provides a threshold sensitivity to absorption on the order of 10–7 cm–1, and allows recording absorption spectra of gases in the temperature range from 200 to 296 K in the region 1000–20 000 cm–1 with an accuracy of 0.9 K.
Similar content being viewed by others
REFERENCES
P. Warneck, Chemistry of the Natural Atmosphere (Academic Press, San Diego, 1988).
E. Sepulveda, M. Schneider, and F. Hase, “Long-term validation of tropospheric column-averaged CH4 mole fractions obtained by mid-infrared ground-based FTIR spectrometry,” Atmos. Meas. Tech. 5, 1425–1441 (2012).
P. J. Crutzen, Geophysiology of Amazonia: Vegetation and Climate Interactions (Wiley, New York, 1987).
R. Goody, “Atmospheres of major planets,” J. Atmos. Sci. 26, 997–1001 (1969).
M. Combes, C. D. Bergh, J. Lecacheus, and J. P. Maillard, “Identification of 13CH4 in atmosphere of Saturn,” Astron. Astrophys. 40, 81–84 (1975).
G. L. Bjoraker and D. E. Jennings, “Detection of 13CH4 in Jupiter atmosphere,” Astrophys. J. 383, 29–32 (1991).
T. Encrenaz, “Remote sensing analysis of solar-system objects,” Phys. Scr. 130, 014037 (2008).
R. M. Goody and Y. L. Yung, Atmospheric Radiation: Theoretical Basis (Oxford University Press, New York, 1995 (University Press Inc, Oxford, 1995).
K. Sung, A. W. Mantz, and M. A. H. Smith, “Cryogenic absorption cells operating inside a Bruker IFS 125HR: First results for 13CH4 at 7 μm,” J. Mol. Spectrosc. 262, 122–134 (2010).
A. W. Mantz, K. Sung, and L. R. Brown, “A cryogenic Herriott cell vacuum-coupled to a Bruker IFS 25HR,” J. Mol. Spectrosc. 304, 12–24 (2014).
D. E. Jennings and J. J. Hillman, “shock isolator for diode-laser operations on a closed-cycle refrigerator,” Rev. Sci. Instrum. 48, 1568–1569 (1977).
A. W. Mantz, D. V. Malathy, D. C. Benner, M. A. H. Smith, A. Predoi-Cross, and M. Dulick, “A multispectrum analysis of widths and shifts in the 2010–2260 cm–1 region of 12C16O broadened by Helium at temperatures between 80–297 K,” J. Mol. Struct. 742, 99–110 (2005).
S. Kassi, B. Gao, D. Romanini, and A. Campargue, “The near infrared (1.30–1.70 mm) absorption spectrum of methane down to 77 K,” Phys. Chem. Chem. Phys. 10, 4410–9 (2008).
A. Campargue, Le. Wang, S. Kassi, M. Masat, and O. Votava, “Temperature dependence of the absorption spectrum of CH4 by high resolution spectroscopy at 81 K: (II) The icosad region (1.49–1.30 μm),” J. Quant. Spectrosc. Radiat. Transfer 111, 1141–1151 (2010).
J. S. Margolis and K. Fox, “Infrared absorption spectrum of CH4 at 9050 cm–1,” J. Chem. Phys. 49, 2451–2452 (1968).
J. P. Maillard, M. Combes, Th. Encrenaz, and J. Lecacheux, “New infrared spectra of the Jovian planets from 12 000 to 4000 cm by Fourier transform spectroscopy,” Astrophys. J. 25, 219–232 (1973).
L. N. Sinitsa, Dissertation in Mathematics and Physics (Institute of Atmospheric Optics, Siberian Branch, Russian Academy of Sciences, 1988).
ACKNOWLEDGMENTS
This work was financially supported by the Russian Science Foundation (grant no. 17-17-01170).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated by S. Ponomareva
Rights and permissions
About this article
Cite this article
Serdyukov, V.I., Sinitsa, L.N., Lugovskoi, A.A. et al. Low-Temperature Cell for Studying Absorption Spectra of Greenhouse Gases. Atmos Ocean Opt 32, 220–226 (2019). https://doi.org/10.1134/S1024856019020106
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1024856019020106