Auroral Signature of Comet Shoemaker-Levy 9 in the Jovian Magnetosphere
R. Prangé, Irene M. Engle, J. T. Clarke, Malcolm Wray Dunlop, Gilda E. Ballester, W.‐H. Ip, S. Maurice, John T. Trauger
Abstract
R. Prangé, Irene M. Engle, J. T. Clarke, Malcolm Wray Dunlop, Gilda E. Ballester, W.‐H. Ip, S. Maurice, John T. Trauger
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.
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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.
Key concepts: Jovian, Magnetosphere, Jupiter (rocket family), Physics, Comet, Astronomy, Astrobiology, Atmosphere of Jupiter