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The atmospheric composition and structure of Jupiter and Saturn from ISO observations: a preliminary review
 

Summary: The atmospheric composition and structure of Jupiter and Saturn
from ISO observations: a preliminary review
Th. Encrenaza,
*, P. Drossarta
, H. Feuchtgruberb
, E. Lelloucha
, B. Be zarda
,
T. Foucheta
, S.K. Atreyac
a
DESPA, Observatoire de Paris, F-92195, Meudon, France
b
Max-Planck-Institut fur Extraterrestrische Physik, D-85748, Garching, Germany
c
The University of Michigan, Ann Arbor, MI, 48109-2143, USA
Received 29 October 1998; accepted 30 December 1998
Abstract
Infrared spectra of Jupiter and Saturn have been recorded with the two spectrometers of the Infrared Space Observatory
(ISO) in 19951998, in the 2.3180 mm range. Both the grating modes (R = 1502000) and the Fabry-Pe rot modes (R = 8000

  

Source: Atreya, Sushil - Department of Atmospheric, Oceanic and Space Science, University of Michigan

 

Collections: Physics