Near-infrared CVF spectrophotometry of Saturn in 1992.

Details Near-infrared CVF spectrophotometry of Saturn in 1992. Near-infrared CVF spectrophotometry of Saturn in 1992.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...298..624m&link_type=abstract

Astronomy and Astrophysics, v.298, p.624

Astronomy and Astrophysics

Astrophysics

2

Planets And Satellites: Saturn, Infrared: Solar Systems

Scientific paper

Absolutely calibrated measurements of the reflectivity of Saturn in 1992 are presented. The observations were carried out using a Circular Variable Filter in combination with a photometer with a single element InSb detector at the 1.54m Carlos Sanchez infrared telescope of the Observatorio del Teide in the Canary Islands (Spain). The spectral ranges covered were 1.4-2.4μm and 2.6-4.5μm. Besides the measurements at the disk, values of the reflectance of the Saturn's rings in the West Ansa were obtained. A comparison with the few related published works is made, and the significant spectral features in this wavelength region are discussed. A spectrum of Jupiter obtained in 1993 is also presented and compared with spectra obtained by us in 1991 using the same instrumental configuration.

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