More Kronoseismology with Saturn's rings
M.M. Hedman, P.D. Nicholson

TL;DR
This paper advances Kronoseismology by analyzing additional waves in Saturn's rings, identifying resonances with planetary normal modes, and observing temporal changes in resonant radii, revealing insights into Saturn's internal structure.
Contribution
It applies and extends previous tools to identify new wave resonances with Saturn's internal modes and reports a drifting resonant radius indicating changing planetary oscillation frequencies.
Findings
Identification of a wave generated by an m=10 normal mode.
Detection of five waves with pattern speeds near Saturn's rotation rate.
Observation of a drifting resonant radius over thirty years.
Abstract
In a previous paper (Hedman and Nicholson 2013), we developed tools that allowed us to confirm that several of the waves in Saturn's rings were likely generated by resonances with fundamental sectoral normal modes inside Saturn itself. Here we use these same tools to examine eight additional waves that are probably generated by structures inside the planet. One of these waves appears to be generated by a resonance with a fundamental sectoral normal mode with azimuthal harmonic number m=10. If this attribution is correct, then the m=10 mode must have a larger amplitude than the modes with m=5-9, since the latter do not appear to generate strong waves. We also identify five waves with pattern speeds between 807 degrees/day and 834 degrees/day. Since these pattern speeds are close to the planet's rotation rate, they probably are due to persistent gravitational anomalies within the planet.…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
