Numerical simulation of the current sheet above solar spots

Details Numerical simulation of the current sheet above solar spots Numerical simulation of the current sheet above solar spots

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..156...41p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 156, no. 1, p. 41-64

Physics

18

Current Sheets, Simulation, Solar Magnetic Field, Solar Physics, Sun, Sunspots, Boundary Conditions, Magnetohydrodynamic Flow, Magnetohydrodynamics, Photosphere, Plasmas (Physics), Solar Corona

Scientific paper

Current sheet (CS) creation in a region with a X-type zero magnetic field time in plasma was simulated by numerically solving the 3D MHD equations for conditions which were close to the solar corona: the disturbance propagated from the photosphere boundary under which the magnetic field sources were situated. Some of the values (B, rho, V) were set on the photosphere boundary, while others were determined from the conditions inside the region. Several Alfven times after its creation, the CS motion practically ceased, and the plasma velocity changed its direction above the sheet, so that the plasma flow was directed into the CS from both sides.

Affiliated with

Also associated with

No associations

Rating

Numerical simulation of the current sheet above solar spots 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 Numerical simulation of the current sheet above solar spots, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical simulation of the current sheet above solar spots will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-838386