The pressure mode oscillation spectrum of a rotating gaseous sphere - Application to Jupiter

Details The pressure mode oscillation spectrum of a rotating gaseous sphere - Application to Jupiter The pressure mode oscillation spectrum of a rotating gaseous sphere - Application to Jupiter

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...87..198m&link_type=abstract

Icarus (ISSN 0019-1035), vol. 87, Sept. 1990, p. 198-209. Research supported by INSU and CNRS.

Physics

19

Atmospheric Pressure, Jupiter (Planet), Planetary Meteorology, Planetary Rotation, Degenerate Matter, P Waves, Perturbation Theory, Seismology

Scientific paper

An investigation is conducted of the influence of rotation on the pattern of pressure mode oscillations of a gaseous sphere in rotation, taking the removal of rotation-generated degeneracy from Jupiter as paradigmatic but proceeding to transpose the results thus obtained to the case of a rotating star. A perturbation theory is developed to treat a major effect of Jovian rotation on the oscillation pattern, which is produced by oblateness and involves the removal of eigenperiod degeneracy. While it is possible to measure the oblateness variations in the planet's interior, it remains difficult to identify the rotating oscillation pattern.

Affiliated with

Also associated with

No associations

Rating

The pressure mode oscillation spectrum of a rotating gaseous sphere - Application to Jupiter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The pressure mode oscillation spectrum of a rotating gaseous sphere - Application to Jupiter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The pressure mode oscillation spectrum of a rotating gaseous sphere - Application to Jupiter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1404672