Abstract
Spectral transmittance measurements have been performed on N 2-broadened lines of 12C 2H 2 and 12C 13CH 2 in the 13.7 μm region at 153,200, and 296 K. From line-by-line comparison of observed and computed spectral transmittance, line strengths, half-widths, and their dependence on temperature have been deduced for conditions relevant to the atmospheres of Jupiter, Saturn, Titan, and Earth.
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