| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9827685 | Journal of Atmospheric and Solar-Terrestrial Physics | 2005 | 6 Pages |
Abstract
Computer simulations of plasmas are relevant nowadays, because they help us understand physical processes taking place in the sun and other stellar objects. We have developed a program called PCell which is intended for displaying the evolution of the magnetic field in a 2D convective plasma cell, with perfectly conducting walls, for different stationary plasma velocity fields. Applications of this program are presented.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Rodrigo Carboni, Francisco Frutos-Alfaro,