Turbulence, Vorticity Generation, and Angular Momentum Transport via the Baroclinic Instability in Accretion Disks

Details Turbulence, Vorticity Generation, and Angular Momentum Transport via the Baroclinic Instability in Accretion Disks Turbulence, Vorticity Generation, and Angular Momentum Transport via the Baroclinic Instability in Accretion Disks

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000astu.proge..13k&link_type=multimedia

Presented at the KITP Program: Astrophysical Turbulence, Apr 13, 2000, Kavli Institute for Theoretical Physics, University of Ca

Physics

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

Turbulence, Vorticity Generation, and Angular Momentum Transport via the Baroclinic Instability in Accretion Disks 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 Turbulence, Vorticity Generation, and Angular Momentum Transport via the Baroclinic Instability in Accretion Disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbulence, Vorticity Generation, and Angular Momentum Transport via the Baroclinic Instability in Accretion Disks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-752395