Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included

Details Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004chjaa...4..490l&link_type=abstract

Chinese J. Astron. Astrophys., Vol. 4, 490-498 (2004)

Astronomy and Astrophysics

Astrophysics

1

Solar Convection, Mhd: Thermodynamics Variables, Sun: Hydrostatic Equilibrium Equation

Scientific paper

Correction of non-ideal effect due to a magnetic fluctuating tensor is derived from the ideal MHD equations. The inclusion of a magnetic turbulent field leads to modifications of the hydrostatic equilibrium equation and thermodynamical variables such as the temperature T, the adiabatic exponent γ, the adiabatic temperature gradient nablaad and the temperature gradient nabla. In particular, the modifications in the adiabatic and radiative temperature gradients will result in a change in the Schwarzchild criterion, hence in the location of the base of the convective zone. Incorporating the modifications, we construct a modified thermodynamical equilibrium structure of the Sun.

Affiliated with

Also associated with

No associations

Rating

Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included 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 Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-901351