MHD simulations indicate that SKA-Mid Band 5a can detect filamentary polarized emission from ICM magnetic fields at high resolution and sensitivity, allowing inference of turbulence driving scales.
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2 Pith papers cite this work, alongside 64 external citations. Polarity classification is still indexing.
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The radio galaxy RACS 0900-28 7036 is Faraday-complex, requiring two Faraday-dispersive components plus an instrumental slab to explain its ASKAP polarization spectra.
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Unraveling the Imprints of Fluctuation-dynamo on the Intracluster Medium with the SKA
MHD simulations indicate that SKA-Mid Band 5a can detect filamentary polarized emission from ICM magnetic fields at high resolution and sensitivity, allowing inference of turbulence driving scales.
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Faraday Complexity and Depolarisation in a High-Rotation-Measure Radio Galaxy from the Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) DR2
The radio galaxy RACS 0900-28 7036 is Faraday-complex, requiring two Faraday-dispersive components plus an instrumental slab to explain its ASKAP polarization spectra.