C. Cecchi-pestellini et F. Scappini, Modeling water emission induced by the Shoemaker-Levy 9/Jupiter catastrophic impact, CAN J PHYS, 79(2-3), 2001, pp. 123-129
We reconsider the water emission observed at 22.2 GHz by Cosmovici et al. (
1996) during the Shoemaker-Levy 9/Jupiter impact. In contrast to the maser
effect proposed by the authors, we discuss the detection in terms of therma
l emission. A statistical equilibrium and radiative transfer model is const
ructed and the results that can be obtained depending on different input pa
rameters are evaluated in the light of literature data.