Articles | Volume 33, issue 7
https://doi.org/10.5194/angeo-33-901-2015
https://doi.org/10.5194/angeo-33-901-2015
Regular paper
 | 
24 Jul 2015
Regular paper |  | 24 Jul 2015

Planetary period oscillations in Saturn's magnetosphere: comments on the relation between post-equinox periods determined from magnetic field and SKR emission data

S. W. H. Cowley and G. Provan

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Latest update: 27 Mar 2024
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Short summary
We compare the reported properties of oscillations in Saturn's outer plasma environment near the ~10.6 hour planetary rotation period, as observed in magnetic field and radio emission data obtained by the Cassini spacecraft. We highlight similarities and differences, and suggest possible reasons for the latter.