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.
, author Parthasarathy , A
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Scintillation study of PSR B1257+12 finds distant scattering screens at 166-354 pc and a relatively clean immediate pulsar environment.
FAST observations of three pulsars detect scintillation arcs whose curvatures scale as ν^{-2} with frequency, locating scattering screens at 30-420 pc.
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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Scintillation of the first-known pulsar planetary system
Scintillation study of PSR B1257+12 finds distant scattering screens at 166-354 pc and a relatively clean immediate pulsar environment.
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Interstellar Scintillation of Three Nearby Pulsars with FAST
FAST observations of three pulsars detect scintillation arcs whose curvatures scale as ν^{-2} with frequency, locating scattering screens at 30-420 pc.