Published February 6, 2025 | Published
Journal Article Open

Direct Frequency Comb Cavity Ring-Down Spectroscopy Using Vernier Filtering

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon National Chiao Tung University
  • 3. ROR icon Jet Propulsion Lab
  • 4. ROR icon Wrocław University of Science and Technology
  • 5. ROR icon United States Naval Research Laboratory

Abstract

We present direct frequency comb cavity ring-down spectroscopy with Vernier filtering as a straightforward approach to sensitive and multiplexed trace gas detection. The high finesse cavity acts both to extend the interaction length with the sample and as a spectral filter, alleviating the need for dispersive elements or an interferometer. In this demonstration, a free running interband cascade laser was used to generate a comb centered at 3.3 μm covering ∼10 cm–1 (300 GHz), which was coupled into a high-finesse cavity, providing 0.9 km of effective path length. The Vernier configuration transmitted the comb modes in sequence, and ring-down decays could be initiated either with an acousto-optic modulator or by scanning the cavity length beyond the adiabatic limit, with trade-offs between duty cycle and sensitivity. This implementation achieved a figure of merit of 4.3 × 10–8 cm–1 Hz–1/2 per spectral element, and measurements of toluene demonstrated its ability to observe trace concentrations of a continuum absorber. This method does not require anything beyond a conventional single-mode cavity ring-down instrument other than an optical frequency comb, making it readily accessible to a wide range of applications.

Copyright and License

© 2025 The Authors. Published by American Chemical Society. This publication is licensed under CC-BY-NC-ND 4.0 .

Featured In

Published as part of The Journal of Physical Chemistry A special issue “Richard J. Saykally Festschrift”.

Acknowledgement

C.R.M. is grateful for support from the Arnold and Mabel Beckman Foundation through the A.O. Beckman Postdoctoral Fellowship. T.-L. C. acknowledges support from the Ministry of Education in Taiwan under the Yushan Young Scholar Program. This work was supported under the grants: National Aeronautics and Space Agency’s (NASA) PICASSO Program (106822/811073.02.24.01.85), PDRDF Program; Universities Space Research Association (USRA), NASA Postdoctoral Program (NPP); Office of Naval Research through the U.S. Naval Research Laboratory; National Science and Technology Council NSTC111-2628-M-A49-009, NSTC112-2628-M-A49-002, NSTC113-2628-M-A49-002.

Supplemental Material

Comparison between the comb spectrum measured with Vernier and FTIR spectroscopy; discussion on the intermode beat note width and coupling efficiency; and a description of the procedure to eliminate outliers (PDF)

Files

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Additional details

Created:
May 14, 2025
Modified:
May 14, 2025