NOTICE: Due to a lapse in annual appropriations, most of this website is not being updated. Learn more.
Form submissions will still be accepted but will not receive responses at this time. Sections of this site for programs using non-appropriated funds (such as NVLAP) or those that are excepted from the shutdown (such as CHIPS and NVD) will continue to be updated.
An official website of the United States government
Here’s how you know
Official websites use .gov
A .gov website belongs to an official government organization in the United States.
Secure .gov websites use HTTPS
A lock (
) or https:// means you’ve safely connected to the .gov website. Share sensitive information only on official, secure websites.
Experimental Line Parameters of the Oxygen A-Band Using Frequency-Stabilized Cavity Ring-Down Spectroscopy
Published
Author(s)
D J. Robichaud, Joseph T. Hodges, Linda R. Brown, D Lisak, Piotr Maslowski, Charles E. Miller
Abstract
Line intensities, self- and air-broadened linewidths, pressure-induced shifts, and collisional narrowing coefficients were measured from 18 <= J' <= 32 in the P branch of the O2 A-band (12,975 13,055 cm^(-1)). 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^(-10) cm^(-1) Hz^(-1/2). The line intensities determined in the present work are 1% lower than the values in current spectroscopic databases. However, we measure broadening coefficients that are up to 20% lower than the extrapolated values given in HITRAN 2004. We discuss the implications of our results for accurate remote sensing of surface pressure and photon pathlength distributions.
Robichaud, D.
, Hodges, J.
, Brown, L.
, Lisak, D.
, Maslowski, P.
and Miller, C.
(2008),
Experimental Line Parameters of the Oxygen A-Band Using Frequency-Stabilized Cavity Ring-Down Spectroscopy, Journal of Molecular Spectroscopy
(Accessed October 22, 2025)