The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar
Astrophysics
2014-10-13 v1
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 (N1), via transitional scattering regime (N2,3), 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 to diffractive scale .
Keywords
Cite
@article{arxiv.astro-ph/0701605,
title = {The stationary phase point method for transitional scattering: diffractive radio scintillation for pulsar},
author = {C. M. Zhang},
journal= {arXiv preprint arXiv:astro-ph/0701605},
year = {2014}
}
Comments
Hanas Meeting paper, appear in ChJAA, 2006, 6, Sup