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Structure of Saturn's Mesosphere from the 28 Sgr Occultations

โœ Scribed by W.B. Hubbard; C.C. Porco; D.M. Hunten; G.H. Rieke; M.J. Rieke; D.W. McCarthy; V. Haemmerle; J. Haller; B. McLeod; L.A. Lebofsky; R. Marcialis; J.B. Holberg; R. Landau; L. Carrasco; J. Elias; M.W. Buie; E.W. Dunham; S.E. Persson; T. Boroson; S. West; R.G. French; J. Harrington; J.L. Elliot; W.J. Forrest; J.L. Pipher; R.J. Stover; A. Brahic; I. Grenier

Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
863 KB
Volume
130
Category
Article
ISSN
0019-1035

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โœฆ Synopsis

We analyze an extensive data set of immersion and emersion

2 Visiting Astronomer, Cerro Tololo Inter-American Observatory, lightcurves of the occultation of 28 Sgr by Saturn's atmosphere National Optical Astronomy Observatories, operated by the Association on 3 July 1989. The data give profiles of number density as a of Universities for Research in Astronomy, Inc., under cooperative function of altitude at a variety of latitudes, at pressures ranging agreement with the National Science Foundation. from about 0.5 to about 20 bar. The atmosphere is essentially 3 Steward Observatory.

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