Supplementary Files
Keywords
MHD
computer simulation
plasmas
MHD
simulaciones por computadora
How to Cite
Abstract
In this contribution, we present the simulations of convective plasma cells of the Sun in two dimensions. With a simple stream function, it is possible to visualize multiple n × n convective cells. To obtain the simulation, we solve the magnetic diffusion equation with a fourth order scheme. Some applications for this simulations are also presented.
References
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