Decametric observations of Jupiter were made at frequencies from 16.7
to 32 MHz from the Maipu Radio Astronomy Observatory in Chile, the Uni
versity of Florida Radio Observatory, and the Owens Valley Radio Obser
vatory in California before, during, and after the collision of comet
Shoemaker-Levy 9 with the planet. No significant change in the general
level of Jovian decametric activity that might be attributed to the c
omet was observed. However, single bursts of possibly Jovian origin ap
peared at two of the 12 fragment impact times during which we were obs
erving. We are attempting to establish more definitely whether these t
wo bursts really were Jovian, and assuming that they were, we are tent
atively modeling the circumstances of their emission.