"Evidence of differential rotation inside Saturn from waves of its rings"
The rotation rate of Saturn is not well constrained. This rate has been
estimated based on several investigations of its shape (Anderson and
Schubert 2007, Read et al., 2009 and Helled et al., 2015), its cloud top
winds (Garcia Melendo et al., 2011, Sanchez-Lavega et al., 2014) and its
magnetic field (Ye et al., 2010, Lamy et al., 2011, Andrews et al.,
2012, Provan et al., 2013). The reason why the interior rotation rate
is not well known is that its magnetic field seems to be closely...
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