The University of Florida Radio Observatory (UFRO) has generated a listing of the prediction of the configurations of CML, Io Phase, the active sources, and the probabilities of emission at 18.0 and 26.3 MHz. 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. If these tables prove useful in your research please acknowledge us in your paper.
For further information, see Description of Tables.
Questions or comments regarding the predictions can be sent to F. Reyes at reyes@astro.ufl.edu.
Prof. Kazumas a Imai has developed an interactive Jupiter ephemeris for observation.