Radiative transfer models for Galileo NIMS studies of the atmosphere of Jupiter

Advances in Space Research

Volumn 19, Issue 8, 1997, Pages 1149-1158

  Irwin, P G J ^a   Calcutt, S B ^a   Taylor, F W ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0038050237     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)00266-4     Document Type: Article

References (7)

1. Carlson, R.W., P.R. Weissman, W.D. Smythe, C.R. Mahoney, and the NIMS Science and Engineering Teams. Near Infrared Mapping Spectrometer Experiment on Galileo. Space Sci. Rev., 60, 457, (1992).
2. Goody, R.M. and Y.L. Yung. Atmospheric Radiation. Theoretical Basis 2nd Ed. Oxford University Press, (1989).
3. Goody, R.M., R.West, L.Chen and D.Crisp. The Correlated-k Method for Radiation Calculations in Nonhomogeneous Atmospheres, J. Quant. Spectrosc. Radiat. Trans. 42, 539-550 (1989).
4. Hansen, J.E. and L.D. Travis. Light Scattering in Planetary Atmospheres, Space Sci. Rev. 16, 527-610, (1974).
5. Kamp, L.W. and F.W. Taylor. Radiative transfer models of the night side of Venus. Icarus, 86, 510-529, (1990).
6. Lacis, A.A. and V. Oinas. A Description of the Correlated k Distribution Method for Modelling Nongray Gaseous Absorption, Thermal Emission, and Multiple Scattering in Vertically Inhomogeneous Atmospheres, J.G.R. 96, 9027-9063 (1991).
7. -1 for remote sounding of the atmosphere of Jupiter. J. Quant. Spect. Rad. Trans., 50, 4, 363-429, 1993.