Proposal for SKA-Low survey to perform 3D tomography of the Local Bubble's magnetized gas using polarized emission and rotation measure synthesis.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 3verdicts
UNVERDICTED 3representative citing papers
A CPRT formalism is presented as a common platform to link cosmological MHD simulations, theory, and SKA polarized sky data for interpreting magnetic fields across cosmic time.
The paper describes the expected capabilities of the SKA-Mid survey to produce a complete map of the Milky Way's magnetic field in the southern hemisphere using rotation measures and polarized emission.
citing papers explorer
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A 3D tomography of the Local Bubble with SKA-Low
Proposal for SKA-Low survey to perform 3D tomography of the Local Bubble's magnetized gas using polarized emission and rotation measure synthesis.
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The magnetic field in the Milky Way Galaxy: from large to small scales
The paper describes the expected capabilities of the SKA-Mid survey to produce a complete map of the Milky Way's magnetic field in the southern hemisphere using rotation measures and polarized emission.