Computer Science – Numerical Analysis
Scientific paper
Dec 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202..439l&link_type=abstract
Astrophysical Journal, vol. 202, Dec. 1, 1975, pt. 1, p. 439-453.
Computer Science
Numerical Analysis
25
Astrophysics, Interstellar Matter, Radiative Transfer, Scintillation, Turbulence Effects, Wave Propagation, Numerical Analysis, Plasma Turbulence, Radiant Flux Density, Solar Wind
Scientific paper
Fluctuations in intensity due to wave propagation in a wide range of turbulent media, are discussed on the basis of a previously developed theory of strong scintillations. An asymptotic analytic solution to the fourth-moment equation is presented, and its range of validity is discussed. Various parameters characterizing the intensity fluctuations, such as scintillation index and correlation scale, are expressed in terms of turbulence parameters for both Gaussian and power-law irregularity spectra as well as for thick and thin turbulent media.
Jokipii Randy J.
Lee Clarence L.
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