Plasma lensing models show that outer and inner caustics plus arclet brightness patterns in pulsar scintillation can constrain substructure column density gradients, sizes, and amplitudes.
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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
UNVERDICTED 2representative citing papers
The thin-screen approximation for pulsar scintillation arcs has key limitations; 3D volume propagation produces variable curvature and features linked to branched flow from correlated weak scatterings.
citing papers explorer
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Plasma lensing modeling of substructures on pulsar scintillation screens
Plasma lensing models show that outer and inner caustics plus arclet brightness patterns in pulsar scintillation can constrain substructure column density gradients, sizes, and amplitudes.
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Pulsar scintillation arcs formed from branched flow
The thin-screen approximation for pulsar scintillation arcs has key limitations; 3D volume propagation produces variable curvature and features linked to branched flow from correlated weak scatterings.