The electrodynamic interaction of the dust and gas comae of comet Shoe
maker-Levy 9 with the jovian magnetosphere was unique and different fr
om the atmospheric effects. Early theoretical predictions of auroral-t
ype processes on the comet magnetic field line and advanced modeling o
f the time-varying morphology of these lines allowed dedicated observa
tions with the Hubble Space Telescope Wide Field Planetary Camera 2 an
d 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 experim
ent'' on Jupiter.