The Stationary Phase Point Method for Transitional Scattering: Diffractive Radio Scintillation

Details The Stationary Phase Point Method for Transitional Scattering: Diffractive Radio Scintillation The Stationary Phase Point Method for Transitional Scattering: Diffractive Radio Scintillation

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjas...6b.223z&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Supplement, Volume 6, Issue S2, Proceedings of the 2005 Lake Hanas International

Astronomy and Astrophysics

Astrophysics

Radio Scintillations, Pulsar General, Interstellar Medium

Scientific paper

The stationary phase point (SPP) method is introduced to treat the diffractive scintillation. From weak scattering, where the SPP number N=1, to strong scattering (N≫1), via transitional scattering regime (N˜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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