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Results of decametric monitoring of the comet collision with Jupiter
Author(s) -
Carr T. D.,
Reyes F.,
Phillips J. A.,
May J.,
Wang L.,
Aparici J.,
Alvarez H.,
Olmos F.,
Garcia L.,
De Buizer J. M.,
Greenman W. B.,
Clark T.,
Levy J.,
Padin S.,
Higgins C. A.
Publication year - 1995
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/95gl00388
Subject(s) - jovian , observatory , comet , jupiter (rocket family) , physics , astronomy , astrobiology , collision , planet , astrophysics , spacecraft , saturn , computer security , computer science
Decametric observations of Jupiter were made at frequencies from 16.7 to 32 MHz from the Maipu Radio Astronomy Observatory in Chile, the University of Florida Radio Observatory, and the Owens Valley Radio Observatory 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 comet was observed. However, single bursts of possibly Jovian origin appeared at two of the 12 fragment impact times during which we were observing. We are attempting to establish more definitely whether these two bursts really were Jovian, and assuming that they were, we are tentatively modeling the circumstances of their emission.