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

Related authors

Magnetic reconnection during steady magnetospheric convection and other magnetospheric modes
Benoit Hubert, Jean-Claude Gérard, Steve E. Milan, and Stanley W. H. Cowley
Ann. Geophys., 35, 505–524, https://doi.org/10.5194/angeo-35-505-2017,https://doi.org/10.5194/angeo-35-505-2017, 2017
Short summary
Magnetospheric magnetic field modelling for the 2011 and 2012 HST Saturn aurora campaigns – implications for auroral source regions
E. S. Belenkaya, S. W. H. Cowley, C. J. Meredith, J. D. Nichols, V. V. Kalegaev, I. I. Alexeev, O. G. Barinov, W. O. Barinova, and M. S. Blokhina
Ann. Geophys., 32, 689–704, https://doi.org/10.5194/angeo-32-689-2014,https://doi.org/10.5194/angeo-32-689-2014, 2014
Magnetic interconnection of Saturn's polar regions: comparison of modelling results with Hubble Space Telescope UV auroral images
E. S. Belenkaya, S. W. H. Cowley, V. V. Kalegaev, O. G. Barinov, and W. O. Barinova
Ann. Geophys., 31, 1447–1458, https://doi.org/10.5194/angeo-31-1447-2013,https://doi.org/10.5194/angeo-31-1447-2013, 2013
Download
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.