On Jupiter's inertial mode oscillations
Nordic Institute for Theoretical Physics, Blegdamsvej 17, 2100 Copenhagen, Denmark
2 Laboratoire d'Astrophysique de Toulouse, Observatoire Midi-Pyrénées, 14 avenue É. Belin, 31400 Toulouse, France
Corresponding author: B. Dintrans, firstname.lastname@example.org
Accepted: 8 July 2001
Properties of inertial modes of Jupiter are investigated for an polytropic description of the planet interior. We use the anelastic approximation to overcome the usual handicap of a severe spherical harmonics truncation. A powerful iterative solver then allows us to compute the frequencies of the most promising low-order modes using as many spherical harmonics as necessary. The induced errors of our model are now within observational limits. A plausible seismological model of Jupiter might thus be at hand provided the use of a more realistic description of the planet interior.
Key words: planets and satellites: individual: Jupiter
© ESO, 2001