A search for the H2 /3, 0/ S1 line in the spectrum of Titan

• 1 September 1977
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 216, 963-966
• https://doi.org/10.1086/155540

Abstract

Keywords

• ATMOSPHERIC COMPOSITION
• HYDROGEN
• INFRARED SPECTROMETERS
• LINE SPECTRA
• TITAN
• OPTICAL THICKNESS
• SPECTRAL RESOLUTION