18 MHz interferometry of Non-Io-C L-bursts

Statistics – Computation

Scientific paper

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Decametric Waves, Jupiter (Planet), Planetary Radiation, Radio Bursts, Radio Interferometers, Circular Polarization, Computational Astrophysics, Correlation, Very Long Base Interferometry

Scientific paper

In order to investigate previous discrepancies in source size measurements, 18-MHz interferometric data of L-bursts from a Non-Io-C storm have been collected during the summer of 1986. Variations noted in the fringe visibility of the Jovian L-bursts indicate that the source size changes in time and that the emission region can sometimes be resolved with a relatively modest baseline. The results suggest that all Jovian source sizes are smaller than 10 arcsec (and are possibly smaller than 0.1 arcmin) and that it is more probable that L-burst emission during a Jovian storm will evolve into S-bursts than that S-bursts will become L-bursts.

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