LWS Measurements of HD in the Giant Planets

Details LWS Measurements of HD in the Giant Planets LWS Measurements of HD in the Giant Planets

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456...29d&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Physics

1

Iso, Lws, Hd, Giant Planets

Scientific paper

The first two rotational lines of HD were measured in all four giant planets using LWS. For Uranus and Neptune, medium-resolution observations of the R(0) line of HD have been analysed using both Mars and Callisto as calibrators. The results for Callisto are promising, but those for Mars are inconsistent for reasons which have not yet been identified. For Jupiter and Saturn, analysis of the high-resolution observations reveals the presence of the R(0) and R(1) lines in both planets.

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