Prediction tables.

   The University of Florida Radio Observatory (UFRO) generates a tabular listing of the prediction of the configurations of CML, Io Phase, the active sources, and the probabilities of detecting the emission at 18 and 26.3 MHz for the months of January to December. The probabilities at 18 MHz were obtained with a Yagi antenna (gain around 8 dB) and can be used as reference when observing with low gain antennas. The probabilities at 26.3 MHz are valid for an antenna of large collecting area (These probabilities were obtained with the 640 dipoles of the UFRO 26.3 MHz Large Array), and are included as reference only.  Professor Kazumasa Imai has created an interactive Jupiter ephemeris for observations of the decametric emission.