The strengths of H2O lines in the 8200 A region and their application to high dispersion spectra of Mars.
The improvement in the quality of spectroscopic plates taken in recent years in the search for water vapor in the atmosphere of Mars has dictated the need for improved laboratory data with which to interpret the spectra. This paper presents the results of measurements of the strengths of 41 lines of the 8200 A (211) water vapor band. The measured values show evidence of vibration-rotation interactions on the line intensities, beyond the principal stretching effect.