Models of solar differential rotation

Details Models of solar differential rotation Models of solar differential rotation

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220...33p&link_type=abstract

In ESA The Hydromagnetics of the Sun p 33-35 (SEE N85-25091 14-92)

Physics

Angular Velocity, Anisotropy, Convective Heat Transfer, Solar Rotation, Stellar Models, Viscosity, Latitude, Mixing Length Flow Theory, Radiative Heat Transfer, Velocity Distribution

Scientific paper

The dependence of the angular velocity in the Sun's convection zone on various parameters is considered. The latitude dependence of the heat transport (or the latitude dependence of the mixing length because of the assumed validity of mixing length theory) caused by the interaction between rotation and convection; and the anisotropy of the viscosity (AV) are examined as the cause of differential rotation. The former leads to meridional circulation which drives differential rotation; the latter drives differential rotation directly.

Affiliated with

Also associated with

No associations

Rating

Models of solar differential rotation 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 Models of solar differential rotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models of solar differential rotation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1753254