Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998dps....30.3705a&link_type=abstract
American Astronomical Society, DPS meeting #30, #37.05; Bulletin of the American Astronomical Society, Vol. 30, p.1083
Astronomy and Astrophysics
Astronomy
Scientific paper
We have made use of the dynamic component of JIM (Jovian global Ionospheric Model) to produce several models of Jupiter's auroral electrojet. We have produced each model by varying the electric potential drop across the auroral oval width between 10(4) V and 10(6) V. We show the resulting profiles of ion density and velocity as a function of altitude, as well as the velocity of neutral species in the model thermosphere. The ions move at speeds of up to several hundred meters per second, with the neutral speeds being approximately 20 percent of this figure. We use the velocity profiles to distinguish the altitudes of transition between flow which is dominated by electrodynamic forces and gas dynamic / Coriolis forces.
Achilleos Nicholas
Miller Samantha
Tennyson Jonathan
UCL Jupiter Group Team
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