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.
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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.