Saturn's Magnetic Field Periodicity: Spectral Sidebands, their Origin and Significance
Abstract
Magnetic field measurements during the first 15 Cassini orbits inside 10 Saturn radii yield spectra containing a central peak, Saturn's periodicity, and sidebands with difference frequencies corresponding to the orbital period. The sidebands are interpreted as a phase modulation of the periodicity caused by the periodic changes in longitude and distance from Saturn. The sideband amplitudes are used to determine a single parameter characterizing the modulation. This interpretation is consistent with outward propagation of a wave from an inner source rotating differentially with respect to the magnetosphere as proposed in the 'Cam' model. The modulation parameter coincides with a wave speed of 30 km/sec. This speed agrees with that derived by Cowley et al. (2006) who used the Cam model to reproduce the observed phase shift during a single orbit. Future studies of the periodicity and the wave properties should benefit from analyses based on this phase modulation.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2008
- Bibcode:
- 2008AGUFM.P11B1259S
- Keywords:
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- 5734 Magnetic fields and magnetism;
- 5737 Magnetospheres (2756);
- 5794 Instruments and techniques;
- 6275 Saturn