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http://hdl.handle.net/20.500.12386/30355
Titolo: | Preliminary JIRAM results from Juno polar observations: 2. Analysis of the Jupiter southern H3+ emissions and comparison with the north aurora | Autori: | ADRIANI, Alberto MURA, Alessandro Moriconi, M. L. Dinelli, B. M. Fabiano, F. ALTIERI, FRANCESCA Sindoni, G. Bolton, S. J. Connerney, J. E. P. Atreya, S. K. Bagenal, F. Gérard, J. -C. M. C. FILACCHIONE, GIANRICO TOSI, Federico MIGLIORINI, Alessandra GRASSI, Davide PICCIONI, GIUSEPPE NOSCHESE, RAFFAELLA CICCHETTI, ANDREA Gladstone, G. R. Hansen, C. Kurth, W. S. Levin, S. M. Mauk, B. H. McComas, D. J. Olivieri, A. TURRINI, Diego STEFANI, STEFANIA Amoroso, M. |
Data pubblicazione: | 2017 | Rivista: | GEOPHYSICAL RESEARCH LETTERS | Numero: | 44 | Fascicolo: | 10 | Da pagina:: | 4633 | Abstract: | The Jupiter InfraRed Auroral Mapper (JIRAM) aboard Juno observed the Jovian South Pole aurora during the first orbit of the mission. H<SUB>3</SUB><SUP>+</SUP> (trihydrogen cation) and CH<SUB>4</SUB> (methane) emissions have been identified and measured. The observations have been carried out in nadir and slant viewing both by a L-filtered imager and a 2-5 μm spectrometer. Results from the spectral analysis of the all observations taken over the South Pole by the instrument are reported. The coverage of the southern aurora during these measurements has been partial, but sufficient to determine different regions of temperature and abundance of the H<SUB>3</SUB><SUP>+</SUP> ion from its emission lines in the 3-4 μm wavelength range. Finally, the results from the southern aurora are also compared with those from the northern ones from the data taken during the same perijove pass and reported by Dinelli et al. (2017). | URI: | http://hdl.handle.net/20.500.12386/30355 | URL: | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017GL072905 | ISSN: | 0094-8276 | DOI: | 10.1002/2017GL072905 | Bibcode ADS: | 2017GeoRL..44.4633A | Fulltext: | open |
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GRL2017GL072905.pdf | Pdf editoriale | 2.12 MB | Adobe PDF | Visualizza/apri |
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