Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.340..539d&link_type=abstract
Nature (ISSN 0028-0836), vol. 340, Aug. 17, 1989, p. 539-541.
Astronomy and Astrophysics
Astronomy
194
Cosmochemistry, Hydrogen Ions, Iue, Jupiter Atmosphere, Molecular Spectra, Ultraviolet Astronomy, Atmospheric Composition, Planetary Magnetospheres, Rotational Spectra, Ultraviolet Spectra, Jupiter, Hydrogen 3, Ions, Auroras, Spectra, Wavelengths, Spectroscopy, Earth-Based Observations, Temperature, Satellite Observations, Ultraviolet, Iue Satellite, Emissions, Data, Chemistry, Thermal Properties
Scientific paper
High-resolution spectra at 2 microns in the southern auroral region of Jupiter are presented which may represent the first astronomical spectroscopic detection of H3(+). The derived rotational temperature of H3(+) is in the range 1000-1200 K. Such strong H3(+) lines could be used in future ground-based monitoring of the Jovian auroral activity and to search for this molecule ion in the interstellar medium.
Atreya Sushil K.
Caldwell J. Jr. J.
Clarke John T.
Drossart Pierre
Kim Jai Sam
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