Literature DB >> 21766933

Design and evaluation of a pulsed-jet chirped-pulse millimeter-wave spectrometer for the 70-102 GHz region.

G Barratt Park1, Adam H Steeves, Kirill Kuyanov-Prozument, Justin L Neill, Robert W Field.   

Abstract

Chirped-pulse millimeter-wave (CPmmW) spectroscopy is the first broadband (multi-GHz in each shot) Fourier-transform technique for high-resolution survey spectroscopy in the millimeter-wave region. The design is based on chirped-pulse Fourier-transform microwave (CP-FTMW) spectroscopy [G. G. Brown, B. C. Dian, K. O. Douglass, S. M. Geyer, S. T. Shipman, and B. H. Pate, Rev. Sci. Instrum. 79, 053103 (2008)], which is described for frequencies up to 20 GHz. We have built an instrument that covers the 70-102 GHz frequency region and can acquire up to 12 GHz of spectrum in a single shot. Challenges to using chirped-pulse Fourier-transform spectroscopy in the millimeter-wave region include lower achievable sample polarization, shorter Doppler dephasing times, and problems with signal phase stability. However, these challenges have been partially overcome and preliminary tests indicate a significant advantage over existing millimeter-wave spectrometers in the time required to record survey spectra. Further improvement to the sensitivity is expected as more powerful broadband millimeter-wave amplifiers become affordable. The ability to acquire broadband Fourier-transform millimeter-wave spectra enables rapid measurement of survey spectra at sufficiently high resolution to measure diagnostically important electronic properties such as electric and magnetic dipole moments and hyperfine coupling constants. It should also yield accurate relative line strengths across a broadband region. Several example spectra are presented to demonstrate initial applications of the spectrometer.

Year:  2011        PMID: 21766933     DOI: 10.1063/1.3597774

Source DB:  PubMed          Journal:  J Chem Phys        ISSN: 0021-9606            Impact factor:   3.488


  6 in total

1.  Nonlinear two-dimensional terahertz photon echo and rotational spectroscopy in the gas phase.

Authors:  Jian Lu; Yaqing Zhang; Harold Y Hwang; Benjamin K Ofori-Okai; Sharly Fleischer; Keith A Nelson
Journal:  Proc Natl Acad Sci U S A       Date:  2016-10-04       Impact factor: 11.205

2.  Continuous probing of cold complex molecules with infrared frequency comb spectroscopy.

Authors:  Ben Spaun; P Bryan Changala; David Patterson; Bryce J Bjork; Oliver H Heckl; John M Doyle; Jun Ye
Journal:  Nature       Date:  2016-05-04       Impact factor: 49.962

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.  Collisional excitation of HNC by He found to be stronger than for structural isomer HCN in experiments at the low temperatures of interstellar space.

Authors:  Brian M Hays; Divita Gupta; Théo Guillaume; Omar Abdelkader Khedaoui; Ilsa R Cooke; Franck Thibault; François Lique; Ian R Sims
Journal:  Nat Chem       Date:  2022-05-05       Impact factor: 24.427

5.  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

6.  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

  6 in total

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