When referring to the Spectral Atlas, please cite our publication:
Keller-Rudek, H., Moortgat, G. K., Sander, R., and Sörensen,
R.: The MPI-Mainz UV/VIS spectral atlas of gaseous molecules of
atmospheric interest, Earth Syst. Sci. Data, 5, 365–373, (2013),
DOI: 10.5194/essd-5-365-2013
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DATAFILE: | CH4_Karkoschka(1994)_125-128K_406-1000nm.txt |
NAME: | methane |
FORMULA: | CH4 |
AUTHOR(YEAR): | Karkoschka(1994) |
T: | 125-128K |
λ: | 406-1000nm |
BIBLIOGRAPHY: |
E. Karkoschka, "Spectrophotometry of the Jovian planets and Titan 300- to 1000-nm wavelengths: The methane spectrum",
Icarus 111, 174-192 (1994);
DOI: 10.1006/icar.1994.1139
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COMMENTS: | The cold-temperature absorption spectrum (presumably 125-128 K) of methane was infered from planetary (jovian planets and Titan) albedo spectra
Absorption coefficients in km-1 amagat-1 (base e) at the temperature of the jovian planets listed in Table VIII have been converted to absorption cross sections (conversion factor 3.72×10-25) |
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