High resolution observations of linear polarization of the 6818.8 A feature of methane for Uranus and Saturn

Details High resolution observations of linear polarization of the 6818.8 A feature of methane for Uranus and Saturn High resolution observations of linear polarization of the 6818.8 A feature of methane for Uranus and Saturn

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...57..228s&link_type=abstract

Icarus (ISSN 0019-1035), vol. 57, Feb. 1984, p. 228-230.

Computer Science

5

High Resolution, Linear Polarization, Methane, Planetary Composition, Saturn Atmosphere, Uranus Atmosphere, Atmospheric Composition, Line Spectra, Planetology, Rayleigh Scattering, Spectral Resolution, Planets, Uranus, Saturn, Telescopic Observations, Polarization, Methane, Scattering, Origin, Satellites, Titan, Spectra, Imagery, Features, Absorption, Distribution, Techniques, Infrared, Wavelengths, Data

Scientific paper

Observations of the linear polarization in the fully resolved 6818.8 Å feature of CH4 in Saturn and Uranus show dramatic changes of linear polarization across the line profile. The change in position angle of polarization across the line core, especially for Saturn, indicates a likely Rayleigh scattering origin for the observed polarization.

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