Absolute spectrophotometry of Titan, Uranus, and Neptune 3500-10,500 A

Details Absolute spectrophotometry of Titan, Uranus, and Neptune 3500-10,500 A Absolute spectrophotometry of Titan, Uranus, and Neptune 3500-10,500 A

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...60..221n&link_type=abstract

Icarus (ISSN 0019-1035), vol. 60, Nov. 1984, p. 221-235.

Astronomy and Astrophysics

Astronomy

69

Astronomical Photometry, Neptune (Planet), Spectrophotometry, Titan, Uranus (Planet), Albedo, Atmospheric Scattering, Fraunhofer Lines, Raman Spectra, Solar Flux, Tables (Data)

Scientific paper

Absolute measurements of the geometric albedo spectra of Titan, Uranus, and Neptune from 3500 to 10,500 Å are reported. The measurements have spectral resolution of about 7 Å and high signal-to-noise ratio owing to the superb efficiency of the spectrograph and Reticon detector used to acquire them. Agreement is excellent with albedo measurements of Uranus by G. W. Lockwood et al. (1983). The high precision and spectral resolution of the data make possible quantitative measurements of the effects of Raman scattering by H2 in the atmospheres of Uranus and Neptune.

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