Fornax cluster magnetic field follows a power-law spectrum of slope ~2.7 with central strength ~5 μG scaling as n^1.6, consistent with recent central re-amplification and trends across 17 clusters.
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MHD simulations forecast polarized synchrotron emission in clusters and filaments to assess SKA detection capabilities.
Predictions show the SKA-mid RM grid will deliver higher precision and accuracy for intra-cluster and intra-group magnetic field studies than POSSUM.
citing papers explorer
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The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems
Fornax cluster magnetic field follows a power-law spectrum of slope ~2.7 with central strength ~5 μG scaling as n^1.6, consistent with recent central re-amplification and trends across 17 clusters.
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Study of Polarized Emission in Radio Halos and Filaments in the SKA Telescopes Era
MHD simulations forecast polarized synchrotron emission in clusters and filaments to assess SKA detection capabilities.
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The Impact of Dense RM Grids on the Study of Intra-cluster and Intra-group Magnetic Fields
Predictions show the SKA-mid RM grid will deliver higher precision and accuracy for intra-cluster and intra-group magnetic field studies than POSSUM.