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...
Main Authors: | , , , , , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2018-09-01
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Series: | Galaxies |
Subjects: | |
Online Access: | http://www.mdpi.com/2075-4434/6/4/104 |