On the diffusion of light in turbulent shearing media

Details On the diffusion of light in turbulent shearing media On the diffusion of light in turbulent shearing media

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199..734l&link_type=abstract

Astrophysical Journal, vol. 199, Aug. 1, 1975, pt. 1, p. 734-740.

Astronomy and Astrophysics

Astrophysics

1

Atmospheric Turbulence, Light Scattering, Pulsar Magnetospheres, Pulsars, Radiative Transfer, Stellar Atmospheres, Astronomical Models, Laminar Flow, Ray Tracing, Shear Flow, Turbulence Effects

Scientific paper

Some simple calculations are presented to show that a beam of light is, in general, severely distorted and dispersed from the straight-line path that would obtain in vacuum when passing through a medium possessing a turbulent velocity of the order of the speed of light in vacuum. The motivation underlying these calculations is the problem of radiative transport through the magnetospheres of pulsars where particle energies in excess of about 100 million times mc-squared are believed to obtain.

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