The work proposes GRMHD jet simulations to generate synthetic synchrotron maps and polarization signatures for testing physical models of observed magnetic filaments.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
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The chapter summarizes gaps in AGN jet research and projects how SKA standalone and combined observations will address jet-host galaxy co-evolution across scales.
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Exploring the physics behind the observed magnetic filaments in large scale radio galaxies
The work proposes GRMHD jet simulations to generate synthetic synchrotron maps and polarization signatures for testing physical models of observed magnetic filaments.
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AGN Jets from Formation to Dissipation
The chapter summarizes gaps in AGN jet research and projects how SKA standalone and combined observations will address jet-host galaxy co-evolution across scales.