The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar

Details The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar

2007-01-22

arxiv.org/abs/astro-ph/0701605v1

Chin.J.Astron.Astrophys.6:223,2007

Astronomy and Astrophysics

Astrophysics

Hanas Meeting paper, appear in ChJAA, 2006, 6, Sup

Scientific paper

The stationary phase point (SPP) method in one-dimensional case is introduced to treat the diffractive scintillation. From weak scattering, where the SPP number N=1, to strong scattering (N$\gg$1), via transitional scattering regime (N$\sim$2,3), we find that the modulation index of intensity experiences the monotonically increasing from 0 to 1 with the scattering strength, characterized by the ratio of Fresnel scale $\rf$ to diffractive scale $\rdiff$.

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