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Phet. Spwe Sd.. Vol. 43. No. 12, pp. 1485--1516.1995 Copyright ic, 1995 Elsevier Science Ltd
 

Summary: Pergamon
Phet. Spwe Sd.. Vol. 43. No. 12, pp. 1485-- 1516.1995
Copyright ic, 1995 Elsevier Science Ltd
Printed in Great Britain. All rights reserved
0032p0633:95 $9.50+ 0.00
0032-0633(95)00064-X
Detectability of molecular species in planetary and satellite atmospheres
from their rotational transitions
Th. Encrenaz,' B. BCzard,' J. Crovisier,' A. Coustenis,' E. Lellouch,' S. Gulkis' and S. K. Atreyaj
' Observatoire de Paris, F-92195 Meudon, France
`Jet Propulsion Laboratory, California Institute of Technology, Pasadena. CA 91109. U.S.A.
`The University of Michigan. Ann Arbor. MI 48109-2143. U.S.A.
Received 26 June 1994; revised 28 March 1995 ; accepted 29 March 1995
Abstract. High-resolution spectroscopy in the milli-
meter and submilIimeter range has made significant
contributions to the study of chemical composition and
thermal structure of planetary and satellite atmo-
spheres. This field of research is expected to make con-
siderable progress in the future, from both ground-
based and space experiments, with the availability of

  

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

 

Collections: Physics