Towards Exascale Simulations of the ICM Dynamo with WENO-Wombat

In galaxy clusters, modern radio interferometers observe non-thermal radio sources with unprecedented spatial and spectral resolution. For the first time, the new data allows to infer the structure of the intra-cluster magnetic fields on small scales via Faraday tomography. This leap forward demands...

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Bibliografiska uppgifter
Huvudupphovsmän: Julius Donnert, Hanbyul Jang, Peter Mendygral, Gianfranco Brunetti, Dongsu Ryu, Thomas Jones
Materialtyp: Artigo
Språk:Inglês
Publicerad: MDPI AG 2018-09-01
Serie:Galaxies
Ämnen:
galaxy clusters
magnetic fields
numerical methods
magneto-hydrodynamics
Länkar:http://www.mdpi.com/2075-4434/6/4/104
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