State of the art in the Jovian radio arc modelization

Details State of the art in the Jovian radio arc modelization State of the art in the Jovian radio arc modelization

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsm41b1671p&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SM41B-1671

Astronomy and Astrophysics

Astronomy

2704 Auroral Phenomena (2407), 2732 Magnetosphere Interactions With Satellites And Rings, 6220 Jupiter, 6954 Radio Astronomy, 6969 Remote Sensing

Scientific paper

The Jovian radio arcs are decameter emissions related to the Io-Jupiter interaction. Their arc shape in the time frequency plane is known to be due to geometrical visibility effect on sources spread along an "active" magnetic field line. The state of the art in their modelization will be presented, including some recent results which permit to deduce from their shape the position of the active field line relative to the Io field line and the emitting particle energy. This modeling is permitted by a numerical code, which was also used to model the Cassini observation of Saturn. The interest on such a modelization of the future observations of JUNO will be discussed.

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