Study of mutual occultation phenomena of the Galilean satellites at radio wavelengths

Details Study of mutual occultation phenomena of the Galilean satellites at radio wavelengths Study of mutual occultation phenomena of the Galilean satellites at radio wavelengths

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..269..245p&link_type=abstract

Galileo's Medicean Moons: their impact on 400 years of discovery, Proceedings of the International Astronomical Union, IAU Sympo

Astronomy and Astrophysics

Astronomy

1

Occultations, Planets And Satellites: Individual (Europa, Ganymede, Io, Jupiter), Radio Continuum: Solar System

Scientific paper

We present preliminary results for our study of mutual phenomena of the Galilean satellites performed at radio wavelengths with the Medicina and Noto antennas of the Istituto di Radioastronomia - INAF, and with the Effelsberg 100-m radio telescope of the Max-Planck-Institute for Radioastronomy, Bonn. Measurements of the radio flux density variation during the mutual occultations of Io by Europa and Ganymede were carried out during the PHEMU09 campaign at 22 GHz and 43 GHz. Flux density variations observed at radio wavelengths are consistent with the typical optical patterns measured when partial occultations occur.

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