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Library for up to 3D resistive MHD simulations in solar atmosphere

Publication at Faculty of Mathematics and Physics |
2020

Abstract

There are several phenomena in the universe that we can look at as magnetohydrodynamic in nature - planets consisting of metals, interplanetary space, stars. As for the stars, these phenomena include spots, solar flares, solar winds, space weather.

To study these phenomena, it is important that we are able to model them at a reasonable scale, in a reasonable detail, but most importantly - model them in a physically correct way.