Three Potential Description of the Dynamics of Rotating Fluid Bodies

Details Three Potential Description of the Dynamics of Rotating Fluid Bodies Three Potential Description of the Dynamics of Rotating Fluid Bodies

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agusm.u52a..05s&link_type=abstract

American Geophysical Union, Spring Meeting 2004, abstract #U52A-05

Statistics

Applications

5430 Interiors (8147), 5724 Interiors (8147), 8147 Planetary Interiors (5430, 5724)

Scientific paper

The oscillatory dynamics of a rotating, inviscid, stratified and compressible liquid body is simplified by an exact description in terms of three scalar fields which are constructed from the perturbations in pressure, gravitational potential and the dilatation. We show that this scheme has several advantages over the conventional approach of using the displacement (velocity) vector field, and that it provides a reliable method for computing normal modes of a fluid body. We will also discuss the geophysical and astrophysical applications of this approach.

Affiliated with

Also associated with

No associations

Rating

Three Potential Description of the Dynamics of Rotating Fluid Bodies 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 Three Potential Description of the Dynamics of Rotating Fluid Bodies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three Potential Description of the Dynamics of Rotating Fluid Bodies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1178128