A mode-coupling model reproduces the qualitative frequency-dependent circular polarization of selected FAST single pulses, but its Bayesian parameter constraints are undermined by the model's poor fits to most pulses.
and LHAASO observations
2 Pith papers cite this work, alongside 4 external citations. Polarity classification is still indexing.
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SKA will enable spatially resolved radio studies of pulsar wind nebulae to probe particle acceleration and propagation in ultra-relativistic outflows.
citing papers explorer
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Pulsar electrodynamics inferred from frequency-dependent circular polarization diversity
A mode-coupling model reproduces the qualitative frequency-dependent circular polarization of selected FAST single pulses, but its Bayesian parameter constraints are undermined by the model's poor fits to most pulses.
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Understanding Pulsar Wind Nebulae with the SKA
SKA will enable spatially resolved radio studies of pulsar wind nebulae to probe particle acceleration and propagation in ultra-relativistic outflows.