Infrared spectroscopy of Jovian aurorae

Details Infrared spectroscopy of Jovian aurorae Infrared spectroscopy of Jovian aurorae

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005basi...33..233g&link_type=abstract

Bulletin of the Astronomical Society of India, Vol. 33, Issue 2, p.233

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Scientific paper

We report on the detection at Mt.Abu of H+ 3 molecular ion emissions in the near infrared spectra of the northern auroral zone of Jupiter. These H+3 transitions are of rotational-vibrational origin and are due to the dynamics of Jovian auroral ionosphere located mainly at high Jovian latitudes, which confirms their magnetospheric origin. The main overtone transition at 2.093 m and several other transitions including that of H2 have been detected. Details are presented.

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