Statistics – Computation
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.228...77g&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 228, Sept. 1, 1987, p. 77-100.
Statistics
Computation
48
Accretion Disks, Compressible Fluids, Motion Stability, Rotating Cylinders, Rotating Fluids, Stellar Rotation, Boundary Value Problems, Computational Astrophysics, Coupled Modes, Sound Waves, Surface Waves
Scientific paper
The stability of differentially rotating fluid cylinders is re-examined. One kind of instability occurring is shown to be due to resonant interaction of modes belonging to different boundaries. A detailed description of the mode interaction is given applicable both to surface and sound waves. The author classifies the modes due to their physical origin and provides a general scheme of their order. The second kind of instability is due to energy loss from the system, in particular due to acoustic radiation. A physical interpretation is given for both of the instabilities in terms of the energy of a mode.
No associations
LandOfFree
On the stability of compressible differentially rotating cylinders. II 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 On the stability of compressible differentially rotating cylinders. II, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the stability of compressible differentially rotating cylinders. II will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1676465