Bulletin of the American Physical Society
2018 Annual Meeting of the APS Mid-Atlantic Section
Volume 63, Number 20
Friday–Sunday, November 9–11, 2018; College Park, Maryland
Session G01: Chemical Physics III
4:00 PM–5:48 PM,
Saturday, November 10, 2018
Edward St. John
Room: 1215
Chair: Amy Mullin, University of Maryland, College Park
Abstract ID: BAPS.2018.MAS.G01.3
Abstract: G01.00003 : Multi-Harmonic Wavelength Modulation Spectroscopy for the Detection of Atmospheric Methane and Nitrous Oxide in mid-IR region*
4:48 PM–5:00 PM
Presenter:
May H Hlaing
(Department of Physics and Engineering, Optical Science Center for Applied Research, Delaware State University, Dover, DE, 19901)
Authors:
May H Hlaing
(Department of Physics and Engineering, Optical Science Center for Applied Research, Delaware State University, Dover, DE, 19901)
Caio Azevedo
(Department of Physics and Engineering, Optical Science Center for Applied Research, Delaware State University, Dover, DE, 19901)
Amir Khan
(Department of Physics and Engineering, Optical Science Center for Applied Research, Delaware State University, Dover, DE, 19901)
A high precision and sensitive wavelength modulation spectroscopy (WMS) multi-harmonic detection technique has been utilized in various fields including chemical sensing for environment, defense and industrial applications. The multi-harmonic WMS is an important tool to probe weak molecular rotational-vibrational transitions of overlapping atmospheric line transitions to determine atmospheric broadening, density etc. In this paper, we present quantum cascade laser based multi-harmonic WMS detection to simultaneously probe atmospheric broadened transitions of methane (CH4) and nitrous oxide (N2O) in the mid-infrared region (7.8 μm) of the spectrum. We show that for a given experimental SNR, the spectral line resolution of disparate line transitions can be improved by higher harmonic WMS detection. We also show that Rayleigh resolution criterion can be extended to quantify spectral resolution and the structures of WMS signals.
*This work was sponsored in part by the National Science Foundation’s CREST (Grant no. HRD-1242067), NASA MIRO (Grant no. NNX15AP84A) and NIH DE-INBRE (Grant no. NIGMS (5P20 GM103446-16)).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.MAS.G01.3
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