Abstract
Reply to the comment by Cowley et al. on “Magnetic phase structure of Saturn's 10.7 h oscillations”
Highlights
CPA conclude that the analysis and discussions in YSD are flawed and YSD’s comments on the post-equinox magnetic oscillations determined by Andrews et al [2012]
We should emphasise that our intention is to build on the results of AP and to examine how one may exploit them further
A correction due to spacecraft local time (LT) was not applied to the magnetic phases determined by AP
Summary
CPA conclude that the analysis and discussions in YSD are flawed and YSD’s comments on the post-equinox magnetic oscillations determined by Andrews et al [2012]. The revision means the first three passes in interval C are in phase and consistent with the strong southern dominance in this interval [Provan et al, 2013]. During interval B, P determines that the amplitude ratio between the northern and southern oscillations is ∼1 suggesting that the magnetic field in the low latitude region chosen for study might be expected to be governed by the mean phase/period.
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