Modeling of satellite control of Jovian radio emission

Details Modeling of satellite control of Jovian radio emission Modeling of satellite control of Jovian radio emission

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....4477m&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #4477

Physics

Scientific paper

Observations from the plasma wave instrument on board the Galileo spacecraft have distinguished control of Jovian radio emission not only by Io, but possibly by Ganymede and Callisto. We have developed a simple model of radio emission from sites along the magnetic flux tubes connecting these satellites to Jupiter. The results indicate radio emission at large wave normal angles should produce distinctive features of radio emission displayed in plots of satellite phase vs. Jovian system III longitude. These results are in qualitative agreement with the observations.

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