Abstract
The electrodynamic interaction of the dust and gas comae of comet Shoemaker-Levy 9 with the jovian magnetosphere was unique and different from the atmospheric effects. Early theoretical predictions of auroral-type processes on the comet magnetic field line and advanced modeling of the time-varying morphology of these lines allowed dedicated observations with the Hubble Space Telescope Wide Field Planetary Camera 2 and resulted in the detection of a bright auroral spot. In that respect, this observation of the surface signature of an externally triggered auroral process can be considered as a "magnetospheric active experiment" on Jupiter.
Original language | English (US) |
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Pages (from-to) | 1317-1320 |
Number of pages | 4 |
Journal | Science |
Volume | 267 |
Issue number | 5202 |
State | Published - Mar 3 1995 |
Externally published | Yes |
ASJC Scopus subject areas
- General