Literature DB >> 21643150

Chirped-pulse terahertz spectroscopy for broadband trace gas sensing.

Eyal Gerecht1, Kevin O Douglass, David F Plusquellic.   

Abstract

We report the first demonstration of a broadband trace gas sensor based on chirp-pulse terahertz spectroscopy. The advent of newly developed solid state sources and sensitive heterodyne detectors for the terahertz frequency range have made it possible to generate and detect precise arbitrary waveforms at THz frequencies with ultra-low phase noise. In order to maximize sensitivity, the sample gas is first polarized using sub-μs chirped THz pulses and the free inductive decays (FIDs) are then detected using a heterodyne receiver. This approach allows for a rapid broadband multi-component sensing with low parts in 10(9) (ppb) sensitivities and spectral frequency accuracy of <20 kHz in real-time. Such a system can be configured into a portable, easy to use, and relatively inexpensive sensing platform.

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Year:  2011        PMID: 21643150     DOI: 10.1364/OE.19.008973

Source DB:  PubMed          Journal:  Opt Express        ISSN: 1094-4087            Impact factor:   3.894


  9 in total

1.  Electromagnetically induced transparency in vacuum and buffer gas potassium cells probed via electro-optic frequency combs.

Authors:  D A Long; A J Fleisher; D F Plusquellic; J T Hodges
Journal:  Opt Lett       Date:  2017-11-01       Impact factor: 3.776

2.  Arbitrary waveform modulated pulse EPR at 200GHz.

Authors:  Ilia Kaminker; Ryan Barnes; Songi Han
Journal:  J Magn Reson       Date:  2017-04-27       Impact factor: 2.229

3.  Photodissociation transition states characterized by chirped pulse millimeter wave spectroscopy.

Authors:  Kirill Prozument; Joshua H Baraban; P Bryan Changala; G Barratt Park; Rachel G Shaver; John S Muenter; Stephen J Klippenstein; Vladimir Y Chernyak; Robert W Field
Journal:  Proc Natl Acad Sci U S A       Date:  2019-12-18       Impact factor: 11.205

4.  Electro-optic frequency combs generated via direct digital synthesis applied to sub-Doppler spectroscopy.

Authors:  David A Long; Benjamin J Reschovsky
Journal:  OSA Contin       Date:  2019

5.  Broad band high resolution rotational spectroscopy for Laboratory Astrophysics.

Authors:  J Cernicharo; J D Gallego; J A López-Pérez; F Tercero; I Tanarro; F Beltrán; P de Vicente; K Lauwaet; B Alemán; E Moreno; V J Herrero; J L Doménech; S I Ramírez; C Bermúdez; R J Peláez; M Patino-Esteban; I López-Fernández; S García-Álvaro; P García-Carreño; C Cabezas; I Malo; R Amils; J Sobrado; C Diez-González; J M Hernandéz; B Tercero; G Santoro; L Martínez; M Castellanos; B Vaquero Jiménez; J R Pardo; L Barbas; J A López-Fernández; B Aja; A Leuther; J A Martín-Gago
Journal:  Astron Astrophys       Date:  2019-06-07       Impact factor: 5.802

6.  Evolution of Microwave Spectroscopy at the National Bureau of Standards (NBS) and the National Institute of Standards and Technology (NIST).

Authors:  F J Lovas; D R Lide; R D Suenram; D R Johnson
Journal:  J Res Natl Inst Stand Technol       Date:  2012-09-28

7.  Long-Wavelength Beam Steerer Based on a Micro-Electromechanical Mirror.

Authors:  Anthony B Kos; Eyal Gerecht
Journal:  J Res Natl Inst Stand Technol       Date:  2013-03-01

8.  Characterization of the Observed Electric Field and Molecular Relaxation Times for Millimeter-Wave Chirped Pulse Instrumentation.

Authors:  G Dhont; D Fontanari; C Bray; G Mouret; A Cuisset; F Hindle; K M Hickson; R Bocquet
Journal:  J Infrared Millim Terahertz Waves       Date:  2020-07-01       Impact factor: 2.647

9.  Using radio astronomical receivers for molecular spectroscopic characterization in astrochemical laboratory simulations: A proof of concept.

Authors:  I Tanarro; B Alemán; P de Vicente; J D Gallego; J R Pardo; G Santoro; K Lauwaet; F Tercero; A Díaz-Pulido; E Moreno; M Agúndez; J R Goicoechea; J M Sobrado; J A López; L Martínez; J L Doménech; V J Herrero; J M Hernández; R J Peláez; J A López-Pérez; J Gómez-González; J L Alonso; E Jiménez; D Teyssier; K Makasheva; M Castellanos; C Joblin; J A Martín-Gago; J Cernicharo
Journal:  Astron Astrophys       Date:  2017-12-22       Impact factor: 5.802

  9 in total

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