theoretical astrophysics laboratory 3  

The computational projects will be realized with the aid of the magnetohydrodynamical code PIERNIK. Students perform and analyze a series of numerical experiments including: supernova explosions, accretion disks, astrophysical jets and selected hydrodynamical instabilities (gravitational instability, thermal instability, Kelvin-Helmholtz instability) of astrophysical relevance.
Presential
English
theoretical astrophysics laboratory 3
English

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