Power-law models of totally anisotropic scattering

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Power-law models of totally anisotropic scattering

The interstellar scattering responsible for pulsar parabolic arcs, and for intraday variability of compact radio quasars, is highly anisotropic in some cases. We numerically simulate these observed phenomena using totally anisotropic, power-law models for the electron density fluctuations which caus...

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Bibliographic Details
Main Authors:	Tuntsov, A., Bignall, Hayley, Walker, M.
Format:	Journal Article
Published:	Oxford University Press 2013
Subjects:	pulsars: individual: B0834+06 ISM: structure ISM: general scattering turbulence BL Lacertae objects: individual: PKS?1257-326
Online Access:	http://hdl.handle.net/20.500.11937/8456

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