Near-Infrared Spectroscopy and Spectral Mapping of Jupiter and the Galilean Satellites: Results from Galileo's Initial Orbit-Reference-Cited by-同舟云学术

Near-Infrared Spectroscopy and Spectral Mapping of Jupiter and the Galilean Satellites: Results from Galileo's Initial Orbit

Published:1996-10-18 Issue:5286 Volume:274 Page:385-388
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Carlson R.¹,Smythe W.¹,Baines K.¹,Barbinis E.²,Becker K.³,Burns R.¹,Calcutt S.⁴,Calvin W.³,Clark R.⁵,Danielson G.⁶,Davies A.¹,Drossart P.⁷,Encrenaz T.⁷,Fanale F.⁸,Granahan J.⁸,Hansen G.⁸,Herrera P.¹,Hibbitts C.⁸,Hui J.¹,Irwin P.⁴,Johnson T.¹,Kamp L.¹,Kieffer H.³,Leader F.²,Lellouch E.⁷,Lopes-Gautier R.¹,Matson D.¹,McCord T.⁸,Mehlman R.²,Ocampo A.¹,Orton G.¹,Roos-Serote M.⁷,Segura M.¹,Shirley J.¹,Soderblom L.³,Stevenson A.¹,Taylor F.⁴,Torson J.³,Weir A.⁴,Weissman P.¹

Affiliation:

1. R. Carlson, W. Smythe, K. Baines, R. Burns, A. Davies, P. Herrera, J. Hui, T. Johnson, L. Kamp, R. Lopes-Gautier, D. Matson, A. Ocampo, G. Orton, M. Segura, J. Shirley, A. Stevenson, P. Weissman, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

2. E. Barbinis, F. Leader, R. Mehlman, Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA.

3. K. Becker, W. Calvin, H. Kieffer, L. Soderblom, J. Torson, U.S. Geological Survey, Flagstaff, AZ 86001, USA.

4. S. Calcutt, P. Irwin, F. Taylor, A. Weir, Department of Atmospheric, Oceanic, and Planetary Physics, Oxford University, Oxford OX1 3PU, UK.

5. R. Clark, U.S. Geological Survey, Denver, CO 80225, USA.

6. G. Danielson, Division of Geological and Planetary Science, California Institute of Technology, Pasadena, CA 91125, USA.

7. P. Drossart, T. Encrenaz, E. Lellouch, M. Roos-Serote, Observatoire de Paris, Meudon 92150, France.

8. F. Fanale, J. Granahan, G. Hansen, C. Hibbitts, T. McCord, Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, HI 96822, USA.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference22 articles.

1. Carlson R., Weissman P. R., Smythe W.D., Mahoney J. C., Space Sci. Rev. 60, 457 (1990).

2. The ammonia ice reflectance spectrum of Fig. 2 is from Fink U., Sill G., in Comets, , Wilkening L., Ed. (Univ. of Arizona Press, Tucson, 1982), pp. 164–202. The ammonia gas spectrum was computed for a vertical path starting at the 1 bar level and an ammonia mixing ratio of 14 ppmv, using absorption coefficients from I. Kleiner, G. Tarrago, Q-L. Kou, G. Guelachvili, L. Brown, 14th International Conference on High Resolution Molecular Spectroscopy, Prague, September 1996. Both spectra are evaluated for the NIMS spectral resolution

3. We used two independent line-by-line radiative transfer models [after Drossart P., Encrenaz T., Icarus 52, 483 (1982);

4. also Lellouch E., Drossart P., Encrenaz T., ibid. 77, 457 (1989);

5. and Irwin P. et al. Adv. Space Sci. in press]

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