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Is a Rikitake Dynamo in Saturn's Interior at the Origin of the Variability of the Radio Rotation Periods?
Bibcode: 2011pre7.conf...65G

Galopeau, P. H. M.

Recent observations performed by the radio and plasma wave science (RPWS) experiment on board the Cassini spacecraft have revealed the presence of two distinct and variable spin modulation periods (10.6 hours and 10.8 hours) in Saturn's radio emissions emanating from the northern and southern hemispheres respectively. The main time modulation of p…

2011 Planetary, Solar and Heliospheric Radio Emissions (PRE VII)
Cassini 0
AKR Sources Positions - Interball 2 vs CLUSTER Observations
Bibcode: 2011pre7.conf..261S

Panchenko, M.; Schreiber, R.; Hanasz, J.

Interball-2 (Auroral Probe) Polrad triaxial spectropolarimeter was used to determine positions of AKR source footprints on the auroral oval. Our findings are consistent with AKR beams narrowly confined to a plane tangent to the source magnetic latitude circle and containing the local magnetic field vector, in agreement with Mutel et al. [2008]. Ou…

2011 Planetary, Solar and Heliospheric Radio Emissions (PRE VII)
Cluster 0