Scintillations due to a concentrated layer with a power-law turbulence spectrum

Details Scintillations due to a concentrated layer with a power-law turbulence spectrum Scintillations due to a concentrated layer with a power-law turbulence spectrum

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rasc...10..107r&link_type=abstract

Radio Science, vol. 10, Jan. 1975, p. 107-114. NSF-supported research.

Physics

Optics

45

Atmospheric Radiation, Atmospheric Turbulence, Luminous Intensity, Scintillation, Spectrum Analysis, Atmospheric Optics, Born Approximation, Interplanetary Medium, Plane Waves, Refractivity, Stellar Radiation, Turbulence Effects

Scientific paper

The parabolic wave equation is used to derive the spatial spectrum of intensity fluctuations due to a concentrated layer of turbulence. The spectrum of refractive-index fluctuations is taken to be an unmodified power law of arbitrary strength, with an exponent between 2 and 6. The results obtained are confirmed by exact calculations for an exponent equal to 3 and by observations of interplanetary scintillations.

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