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A&A 423, 391-395 (2004)
DOI: 10.1051/0004-6361:20034532
Modelling the Lyman
dayglow in the Jovian atmosphere
M. Barthélemy1, C. Parkinson2, 3, J. Lilensten1 and R. Prangé4
1 Laboratoire de Planétologie de Grenoble, CNRS-UJF, BP 53, 38041 Saint Martin d'Hères, Cedex 9, France
e-mail: mathieu.barthelemy@ujf-grenoble.fr
2 MS 150-21, Caltech, Pasadena, California 91125, USA
3 MS 183-501, JPL, Pasadena, California 9110, USA
e-mail: cdp@gps.caltech.edu
4 Observatoire de Paris-Meudon, 5 place Jules Jansen, 92195 Meudon, France
e-mail: renee.prange@obspm.fr
(Received 17 October 2003 / Accepted 15 March 2004 )
Abstract
The Lyman
dayglow of Jupiter provides an important source of
information about its atmosphere. The H Lyman
and the
H
2 6-0 P(1) line of the Lyman system overlap, resulting in a coupling effect between these two lines. In this paper, we evaluate
the effect of this overlapping via radiative transfer modelling and show its
effect both on the integrated intensity and the line profile. The intensity
increases at about 1025 Å at the centre of the disc, tends to slightly
decrease at the limb, and creates an asymmetry in the profile. This
asymmetry is also present in the jovian H-Lyman
bulge
region.
Key words: radiative transfer -- planets and satellites: individual: Jupiter -- ultraviolet: solar system
© ESO 2004
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