Limits on Decametric Radiation from the Shoemaker-Levy 9 Impacts on Jupiter

Details Limits on Decametric Radiation from the Shoemaker-Levy 9 Impacts on Jupiter Limits on Decametric Radiation from the Shoemaker-Levy 9 Impacts on Jupiter

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...484..432k&link_type=abstract

Astrophysical Journal v.484, p.432

Astronomy and Astrophysics

Astronomy

Comets: Individual Name: Shoemaker-Levy/9, Planets And Satellites: Individual Jupiter, Radio Continuum: Solar System

Scientific paper

Observations were carried out from South Africa (lat. = -25.dg89, long. = 27.dg69) of the collisions of fragments A, E, H, Q1, Q2, and S with Jupiter. The excellent observing location and winter ionosphere allowed observations at important low frequencies not routinely accessible at other sites. Observations were carried out at 7.06, 8.7, 10.2, and 11.9 MHz, and in the entire band 12.4--34 MHz. No signals which could definitely be attributed to the collisions were seen. Significant upper limits on the emissions, depending on frequency and on the observing conditions during the particular impact, were obtained.

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