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

Publikace na Matematicko-fyzikální fakulta |
2020

Tento text není v aktuálním jazyce dostupný. Zobrazuje se verze "en".Abstrakt

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.