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Experimental intensity and lineshape parameters of the oxygen A-band using frequency-stabilized cavity ring-down spectroscopy
Authors:David J Robichaud  Linda R Brown  Daniel Lisak  Piotr Mas?owski  Laurence Y Yeung  Charles E Miller
Institution:a Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA 91125, USA
b Process Measurements Division, National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, MD 20899, USA
c Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
d Instytut Fizyki, Uniwersytet Miko?aja Kopernika, ul. Grudziadzka 5/7, 87-100 Toruń, Poland
Abstract:Line intensities, self- and air-broadened linewidths, pressure-induced shifts, and collisional narrowing coefficients were measured from 2 ? J′ ? 32 in the P branch of the O2A-band (12 975-13110 cm−1) utilizing Galatry line profiles. Spectra were recorded using the frequency-stabilized cavity ring-down spectrometer located at NIST, Gaithersburg, MD with a spectral resolution <0.0001 cm−1 and noise-equivalent absorption coefficient of 6 × 10−8 m−1 Hz−1/2. Line intensities, obtained from calibrated gas samples for 2 ? J′ ? 32, are ∼1% lower than the values in current spectroscopic databases. At higher J (18 ? J′ ? 32), the measured air- and self- broadened half widths are up to 20% lower than the extrapolated values given in HITRAN 2004, while corresponding half-widths for 2 ? J′ ? 15 are in better agreement. Available self-broadened half widths are fitted to empirical expressions with an rms of 0.8%. We discuss the implications of our results for accurate remote sensing of surface pressure and photon path length distributions.
Keywords:Oxygen  A-band  Intensities  Cavity ring-down spectroscopy
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