Hostname: page-component-f554764f5-c4bhq Total loading time: 0 Render date: 2025-04-11T01:53:03.121Z Has data issue: false hasContentIssue false
  • English
  • Français

TD1A Satellite Spectroscopic Observations of Jupiter in the Ultraviolet

Published online by Cambridge University Press:  14 August 2015

R. Duysinx  and
M. Henrist
R. Duysinx
Affiliation:
Institut d'Astrophysique, Université de Liège, Belgium
M. Henrist
Affiliation:
Institut d'Astrophysique, Université de Liège, Belgium

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Three spectra of Jupiter were recorded by TD1A satellite between 1350 and 2600 Å. From these data, the geometrical albedo of the planet was computed.

From 2600 to 2100 Å, the value of the albedo matches the simple diffusing models of Jupiter's atmosphere (Greenspan and Owen, 1967).

From 2100 to 1800 Å, a broad absorption can be assigned to NH3 molecule (2168 Å transition).

Another absorption commences below 1800 Å. The absorbing molecule involved will be determined at a later date.

Type
Part III Outer Planets and Their Satellites
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 351 - 355
Copyright
Copyright © Reidel 1974 

References

Anderson, R. C., Pipes, J. G., Broadfoot, A. L., and Wallace, L.: 1969, J. Atmospheric Sci. 26, 874.Google Scholar
Beeckmans, F., Macau, D., and Malaise, D.: 1973, Bolometric Corrections for B Stars, COSPAR 1973.Google Scholar
Broadfoot, A. L.: 1972, Astrophys. J. 173, 681.Google Scholar
Detwiler, C. R., Garret, D. L., Purcell, J. D., and Tousey, R.: 1961, Ann. Geophys. 17, 265.Google Scholar
Evans, D. C.: 1966, NASA Goddard Space Flight Center Report Nr X-613-66-172.Google Scholar
Gardier, S., Jamar, C., and Malaise, D.: 1973, Rev. Universelle des Mines 1, 19.Google Scholar
Greenspan, J. A. and Owen, T.: 1967, Science 156, 1489.Google Scholar
Jamar, C., Malaise, D., and Monfils, A.: 1971, ELDO-CECLES/ESRO-CERS Scient. and Tech. Rev. 3, 427.Google Scholar
Jenkins, E. B.: 1969, Icarus 10, 379.Google Scholar
Jenkins, E. B., Morton, D. C., and Sweigart, A.: 1969, Astrophys. J. 157, 913.Google Scholar
Kondo, Y.: 1971, Icarus 14, 269.Google Scholar
Kuiper, G. P. (ed.): 1952, in Atmospheres of the Earth and Planets, University of Chicago Press, Chicago, pp. 304–345.Google Scholar
Malaise, D., Macau, J. P., and Jamar, C.: 1972, ‘Description, but scientifique, premiers résultats de S2/68 de TD1’, Colloque d'Aussois.Google Scholar
Marette, G.: 1973, Optics Communications, in press.Google Scholar
Mason, H. P.: 1969, , University of Illinois.Google Scholar
Moos, H. W., Fastie, W. G., and Bottema, M.: 1969, Astrophys. J. 155, 887.Google Scholar
Newburn, R. L. and Gulkis, S.: 1973, Space Sci. Rev. 3, 179.CrossRefGoogle Scholar
Owen, T.: 1970, Science 167, 1675.Google Scholar
Stecher, T. P.: 1965, Astrophys. J. 142, 1186.CrossRefGoogle Scholar
Tilgner, B.: 1971, ELDO-CECLES/ESRO-CERS Scient. and Techn. Rev. 3, 567.Google Scholar
Wallace, L., Caldwell, J. J., and Savage, B. D.: 1972, Astrophys. J. 172, 755.Google Scholar
Watanabe, K.: 1954, J. Chem. Phys. 22, 1564.Google Scholar