Abstract
The identification of the magnetic dipole rotation spectrum of oxygen in atmospheric studies has been confirmed by laboratory measurements in the spectral range 12 to 65 cm
-1
, using interferometric techniques combined with long absorption paths and pressures of 2 to 3 atmospheres. A quantitative comparison has also been made between the laboratory observations and the theoretical predictions, giving agreement in the frequencies to within +0∙026 cm
-1
and that of the integrated line-strengths within experimental error, as defined by the signal/noise ratio of the observed spectra.
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