Abstract
The 200-600 cm-1 continuum opacity in the troposphere and lower stratosphere of Titan is inferred from thermal emission spectra from the Voyager 1 IR spectrometer (IRIS). The surface temperature and mean molecular weight are 94 K < TG < 97K and 28.3
Cite
CITATION STYLE
APA
Samuelson, R. E., Hanel, R. A., Kunde, V. G., & Maguire, W. C. (1981). Mean molecular weight and hydrogen abundance of Titan’s atmosphere. Nature, 292(5825), 688–693. https://doi.org/10.1038/292688a0
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