Spectrophotometry and upper limit of gaseous CH4 for Triton

Details Spectrophotometry and upper limit of gaseous CH4 for Triton Spectrophotometry and upper limit of gaseous CH4 for Triton

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...46..288j&link_type=abstract

Icarus, vol. 46, May 1981, p. 288-291.

Computer Science

11

Methane, Satellite Atmospheres, Spectral Reflectance, Spectrophotometry, Triton, Albedo, Atmospheric Composition, Spectrum Analysis, Neptune, Triton, Satellites, Spectrophotometry, Methane, Spectrum, Data, Reflectivity, Comparisons, Pluto, Atmosphere, Wavelengths, Absorption, Analysis

Scientific paper

Spectra of Triton with a CCD spectrometer yielded a relative spectral
reflectivity curve from 0.56 to 1.05 micron at a resolution of 25 A.
Using low-temperature band model parameters from Fink et al. (1980), an
upper limit for the one-way path gaseous CH4 abundance of 1 m-am was
derived.

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