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<p><strong>Abstract.</strong> Periodic signatures present in the magnetospheres of both Jupiter and Saturn have yet to be fully explained. At Jupiter the unexplained signatures are related to emissions from the Io torus ("System IV"); at Saturn they are observed in emissions of kilometric radiation (SKR) and in magnetometer data. These signatures are often interpreted in terms of magnetic field anomalies. This paper describes an alternative mechanism by which the neutral atmosphere may imposedoi:10.5194/angeo-24-2709-2006 fatcat:45wilmcyxfg2tlz4kl2b5kd3uy