Macroscopic Transport Large-scale advection, turbulent diffusion, wave transport

Details Macroscopic Transport Large-scale advection, turbulent diffusion, wave transport Macroscopic Transport Large-scale advection, turbulent diffusion, wave transport

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ssrv...85...79z&link_type=abstract

Space Science Reviews, v. 85, Issue 1/2, p. 79-90 (1998).

Computer Science

4

Stellar Interiors, Stellar Rotation, Turbulent Transport

Scientific paper

While the solar convection zone is very well mixed by its turbulent motions, chemical composition gradients build up in the radiative interior due to microscopic diffusion and settling, and to nuclear burning. Standard models, which ignore any type of macroscopic transport, cannot explain the depletion of lithium in solar-type stars, as they evolve; neither do they account for the observed profile of molecular weight at the base of the solar convection zone.

Affiliated with

Also associated with

No associations

Rating

Macroscopic Transport Large-scale advection, turbulent diffusion, wave transport 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 Macroscopic Transport Large-scale advection, turbulent diffusion, wave transport, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Macroscopic Transport Large-scale advection, turbulent diffusion, wave transport will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1047427