Magnetic fields interacting with nonlinear compressible convection

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

59

Compressible Flow, Convective Heat Transfer, Magnetohydrodynamic Flow, Solar Magnetic Field, Atmospheric Stratification, Kinematics, Magnetic Flux, Oscillating Flow, Prandtl Number, Velocity Distribution

Scientific paper

Two-dimensional numerical simulations are used to study fully compressible convection in the presence of an imposed magnetic field. Highly nonlinear flows are considered that span multiple density scale heights. The convection tends to sweep the initially uniform vertical magnetic field into concentrated flux sheets with significant magnetic pressures. These flux sheets are partially evacuated, and effects of buoyancy and Lorentz forces there can serve to suppress motions. The flux sheets can be surrounded by a sheath of descending flow. If the imposed magnetic field is sufficiently strong, the convection can become oscillatory. The unstably stratified fluid layer has an initial density ratio (bottom to top of layer) of 11. Surveys of solutions at fixed Rayleigh number sample Chandrasekhar numbers from 1 to 1000 and magnetic Prandtl numbers from 1/16 to 1. These nonlinear simulations utilize a two-dimensional numerical scheme based on a modified two-step Lax-Wendroff method.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Magnetic fields interacting with nonlinear compressible convection 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 Magnetic fields interacting with nonlinear compressible convection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic fields interacting with nonlinear compressible convection will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-848075

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.