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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 fuÈr 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 1995±1998, in the 2.3±180 mm range. Both the grating modes (R = 150±2000) and the Fabry-Pe rot modes (R = 8000±
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