SKR Characteristics and Variability with Cassini/RPWS/HFR data

Details SKR Characteristics and Variability with Cassini/RPWS/HFR data SKR Characteristics and Variability with Cassini/RPWS/HFR data

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..713c&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

Physics

Scientific paper

ABSTRACT We present the state of the art the Saturn Kilometric Radiation (SKR) characteristics and variability as observed with Cassini/RPWS/HFR. Thanks to the goniopolarimetric capabilities of this receiver, it is possible to retrieve the direction of arrival, the polarization of the flux of an incoming electromagnetic wave. It was thus possible to locate the sources of the SKR during close flybys. Statistical properties (source location, polarization and flux density, periodicity) of the SKR were also inferred from 4 years of continuous radio observations. Modelling the visibility of the emission has also been perform and provided constraints on the characteristics of the radio emission.

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