SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
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2 Pith papers cite this work, alongside 10 external citations. Polarity classification is still indexing.
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GRMHD simulations of MAD and SANE black-hole accretion can be tested and refined with SKA high-resolution imaging, polarization, and VLBI of jets from stellar-mass to supermassive systems.
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Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect
SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.
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Probing magnetized accretion disk-jet systems: stellar mass to supermassive black holes
GRMHD simulations of MAD and SANE black-hole accretion can be tested and refined with SKA high-resolution imaging, polarization, and VLBI of jets from stellar-mass to supermassive systems.