The Extreme Ultraviolet Explorer (EUVE) satellite conducted extensive
observations of the jovian system before, during, and after the impact
of the fragments of comet Shoemaker-Levy 9 in July 1 994. About 2 to
4 hours after the impacts of several of the larger fragments, the brig
htness of the neutral helium (He I) resonance line at 58.4 nanometers
temporarily increased by a factor of about 10. The transient 58.4-nano
meter brightenings are most simply explained by resonant scattering of
sunlight from the widespread high-altitude remnants of the larger imp
act plumes. Other possible sources of emission, such as electron impac
t excitation of He or radiative recombination of He+, may contribute t
o the observed signal.