arXiv · astro-ph/0701605
The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar
Abstract
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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C. M. Zhang. 2007-01-22. The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar. https://doi.org/10.1088/1009-9271%2F6%2Fs2%2F41
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