Intensity distribution of interplanetary scintillation at 408 MHz

Details Intensity distribution of interplanetary scintillation at 408 MHz Intensity distribution of interplanetary scintillation at 408 MHz

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975aujph..28..621m&link_type=abstract

Australian Journal of Physics, vol. 28, Oct. 1975, p. 621-632.

Mathematics

Probability

3

Interplanetary Medium, Probability Distribution Functions, Radio Sources (Astronomy), Scintillation, Electron Density (Concentration), Histograms, Point Sources, Radiation Distribution, Solar Electrons, Solar Wind

Scientific paper

It is shown that interplanetary scintillation of small-diameter radio sources at 408 MHz produces intensity fluctuations which are well-fitted by a Rice-squared distribution, better so than is usually claimed. The observed distribution can be used to estimate the proportion of flux density in the core of 'core-halo' sources without the need for calibration against known point sources.

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