Replication Data for: Dissipation in rapidly rotating fluid spheres caused by weak longitudinal libration

Also includes the linear numerical code used for the results with an example of its use. Summary of publication: Planetary bodies with non-spherical mass distributions are subject to gravitational torques from their orbital companions.

One influence of these torques is a modulation of the rotation rate of the planet, known as longitudinal libration. For a planet with a fluid interior, the solid outer layer undergoes libration independently, and drag forces drive a flow in the fluid. We investigate the dissipation in linear flows driven by small amplitude longitudinal librations in a rapidly rotating fluid sphere.