Abstract

Even if on-board mm-wave/THz heterodyne receivers have been developed to measure greenhouse gases (GHGs) atmospheric profiles, rotational spectroscopy rests under-exploited for their monitoring unlike IR rovibrational spectroscopy. The present study deals with the ability of THz spectroscopy using long interaction path-lengths for GHG laboratory investigations. High-resolution THz signatures of non-polar greenhouse molecules may be observed by probing very weak centrifugal distortion induced rotational transitions. To illustrate, new measurements on CH4 and CF4 have been carried out. For CH4, pure rotational transitions, recorded by cw-THz photomixing up to 2.6 THz in a White type cell adjusted to 20 m, have allowed to update the methane line list of atmospheric databases. Concerning CF4, Fabry-Perot THz absorption spectroscopy with a km effective pathlength was required to detect line intensities lower than 10−27 cm−1/(moleccm−2). Contrary to previous synchrotron-based FT-FIR measurements, the tetrahedral splitting of CF4 THz lines is fully resolved. Finally, quantitative measurements of N2O and O3 gas traces have been performed in an atmospheric simulation chamber using a submm-wave amplified multiplier chain coupled to a Chernin type multi-pass cell on a 200 m path-length. The THz monitoring of these two polar GHGs at tropospheric and stratospheric concentrations may be now considered.

Highlights

  • The main discussion on climate change tends to focus on carbon dioxide (CO2 ), the most dominant Greenhouse Gas (GHG) (65% of the global emission) produced by the burning of fossil fuels, industrial processes and changes in land use [1]

  • The present article highlights the best performances reached by rotational submmwave/THz long-path absorption spectroscopy of important atmospheric GHGs

  • The results obtained on CH4 and CF4 demonstrate that the weakly intense centrifugal distortioninduced rotational lines are measurable with a high degree of accuracy thanks to the progress of THz gas phase high-resolution spectroscopy

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Summary

Introduction

The main discussion on climate change tends to focus on carbon dioxide (CO2 ), the most dominant Greenhouse Gas (GHG) (65% of the global emission) produced by the burning of fossil fuels, industrial processes and changes in land use (deforestation, intensification of agriculture, flooding, etc.) [1]. Several currently operating satellite and air-borne missions aim to estimate emissions and absorptions of the main GHGs. By monitoring the column densities in our atmosphere, they accumulate new knowledge of their global distribution and temporal variation. We can mention: (i) the IASI interferometer in the European MetOp satellite which monitors CO2 , O3 , CH4 , N2 O GHG column amounts in several IR channels of detection [5]; (ii) ACE on board the Canadian

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