Turbulization of shear flows in astrophysics

Details Turbulization of shear flows in astrophysics Turbulization of shear flows in astrophysics

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..335c&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 335-340 (SEE N90-25711 19-89)

Statistics

Computation

Accretion Disks, Computational Astrophysics, Incompressible Flow, Shear Flow, Turbulence Models, Dynamical Systems, Galactic Structure, Nonlinear Systems, Planetary Rings, Turbulence, Vortices

Scientific paper

A general approach is used to explain the turbulization of incompressible free shear fluid flows. The determination of a universal criterion for the dynamic instability in a rotating fluid and the nature and nonlinear effects during the evolution of vertical perturbations in free shear flows are discussed. An attempt at understanding the physical causes of turbulization of such flows is made. The theory of turbulization can be applied to accretion disks, galactic disks, planetary rings and protostellar nebulae.

Affiliated with

Also associated with

No associations

Rating

Turbulization of shear flows in astrophysics 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 Turbulization of shear flows in astrophysics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbulization of shear flows in astrophysics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1614547