Spatially resolved spectra in four 50-Γ FUV spectral windows were obtained across the jovian aurora with the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope. Nearly simultaneous ultraviolet imaging makes it possible to correlate the intensity variations along the STIS
Time-Resolved Observations of Jupiter's Far-Ultraviolet Aurora
β Scribed by Ballester, G. E.; Clarke, J. T.; Trauger, J. T.; Harris, W. M.; Stapelfeldt, K. R.; Crisp, D.; Evans, R. W.; Burgh, E. B.; Burrows, C. J.; Casertano, S.; Gallagher, J. S.; Griffiths, R. E.; Hester, J. J.; Hoessel, J. G.; Holtzman, J. A.; Krist, J. E.; Meadows, V.; Mould, J. R.; Sahai, R.; Scowen, P. A.; Watson, A. M.; Westphal, J. A.
- Book ID
- 121156889
- Publisher
- American Association for the Advancement of Science
- Year
- 1996
- Tongue
- English
- Weight
- 1000 KB
- Volume
- 274
- Category
- Article
- ISSN
- 0036-8075
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π SIMILAR VOLUMES
temperatures derived are in the range 400-850 K with a possible tendency toward lower temperatures for higher methane col-We observed the jovian UV auroral regions with the Goddard umn densities. This tendency and the uncertainty in the temperhigh resolution spectrograph (GHRS) on board the Hubble a