Direct evidence of differences in magnetic rotation rate between Saturn's northern and southern polar regions

Details Direct evidence of differences in magnetic rotation rate between Saturn's northern and southern polar regions Direct evidence of differences in magnetic rotation rate between Saturn's northern and southern polar regions

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jgra..11601201s&link_type=abstract

Journal of Geophysical Research, Volume 116, Issue A1, CiteID A01201

Physics

7

Magnetospheric Physics: Planetary Magnetospheres (5443, 5737, 6033)

Scientific paper

The discovery of a difference in apparent rotation rate between Saturn kilometric radio emission from northern and southern hemispheres leads immediately to the question of whether there is a counterpart detectable in the Saturnian magnetic field. We report direct detection of a difference in the rotating magnetic signal measured by the Cassini spacecraft magnetometer consistent with that seen in the radio signals. Theoretical consequences of the direct detection are discussed.

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