Correlation between the Jovian Polar cusps FUV emissions and low frequency radio emissions of Jupiter measured by the Cassini spacecraft.

Details Correlation between the Jovian Polar cusps FUV emissions and low frequency radio emissions of Jupiter measured by the Cassini spacecraft. Correlation between the Jovian Polar cusps FUV emissions and low frequency radio emissions of Jupiter measured by the Cassini spacecraft.

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....11498p&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #11498

Physics

Scientific paper

During its flyby of Jupiter at the end of 2000, the Cassini spacecraft have recorded strong LF radio emissions with the RPWS instrument. This radio bursts have been preceded by the arrival of a strong interplanetary schock at Jupiter. We have examined the FUV emissions associated to the Jovian polar cusps in the images archive taken at the same period with the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope. The variations of these emissions have been previously correlated to the conditions of the solar wind, but only with measurements extrapolated from the Earth orbit. We study here the correlation of the polar cusps emissions with the LF radio emissions and the solar wind measurements at Jupiter with the Cassini spacecraft.

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