Plume-like structures of extinction clouds at 19 Saturn radii

Details Plume-like structures of extinction clouds at 19 Saturn radii Plume-like structures of extinction clouds at 19 Saturn radii

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986basi...14..232v&link_type=abstract

Astronomical Society of India, Bulletin, vol. 14, Dec. 1986, p. 232-235.

Astronomy and Astrophysics

Astronomy

2

Interstellar Extinction, Magnetospheric Ion Density, Planetary Magnetospheres, Saturn (Planet), Saturn Rings, Stellar Occultation, Cosmic Gases, Light Curve

Scientific paper

Observations of the occultation of the star SAO 158763 by Saturn's magnetospheric region around 19 RS on 1984 May 12 are compared with the observations by Mahra et al. of the same event. Certain disparities between the Naini Tal and Kavalur data suggest that the extinction signatures are more likely to be caused by irregular density enhancements of ions, charged dust grains, or gas rather than regular ring systems confined to the equatorial plane.

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