Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....9215139c&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 92, Dec. 30, 1987, p. 15139-15147.
Astronomy and Astrophysics
Astronomy
31
Atmospheric Models, Far Ultraviolet Radiation, Gas Giant Planets, Glow Discharges, Planetary Ionospheres, Ultraviolet Astronomy, Dayglow, F Region, Field Aligned Currents, Hydrogen, Ultraviolet Spectrometers, Upper Atmosphere
Scientific paper
The authors propose that the diffuse FUV emissions of H and H2 in excess of photoelectron excitation observed from the sunlit atmospheres of Uranus, Saturn, and Jupiter are produced by electric field acceleration of photoelectrons and ions locally in the upper atmospheres. This in situ acceleration is required to satisfy the many observational constraints on the altitude distribution, exciting particle energy, and total input energy requirements of the electroglow mechanism. The authors further suggest that a primary mechanism leading to this acceleration is an ionospheric dynamo, which is created in the same manner as the Earth's dynamo.
Clarke John T.
Hudson Mary K.
Yung Yuk L.
No associations
LandOfFree
The excitation of the far ultraviolet electroglow emissions on Uranus, Saturn, and Jupiter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The excitation of the far ultraviolet electroglow emissions on Uranus, Saturn, and Jupiter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The excitation of the far ultraviolet electroglow emissions on Uranus, Saturn, and Jupiter will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-904044