Dynamic spectra of interplanetary scintillations

Details Dynamic spectra of interplanetary scintillations Dynamic spectra of interplanetary scintillations

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.312..251c&link_type=abstract

Nature (ISSN 0028-0836), vol. 312, Nov. 15, 1984, p. 251-254.

Computer Science

5

Interplanetary Medium, Scintillation, Solar Wind, Spectrum Analysis, Computerized Simulation, Electron Density (Concentration), Wave Diffraction

Scientific paper

Interplanetary scintillations (IPS) are fluctuations in the apparent intensity of radio sources caused by fluctuations in the electron density of the solar wind. The authors compare the observations with a numerical simulation of the diffraction of plane waves by a two-dimensional random phase screen. The frequency-time structure of the simulated IPS shows good qualitative agreement with the observations when the turbulence spectrum in the phase screen is a simple power law with the Kolmogorov exponent.

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