Study of decameter-wavelength ionospheric scintillation by astronomical methods using the URAN-1 radiotelescope

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We present and analyze the results of monitoring of ionospheric scintillation at frequencies 16.7 25 MHz in 2002-2002. Extensive experimental evidence allowed us to obtain the laws of the amplitude distribution of signals, temporal variations in scintillation indices, autocorrelation times, and parameters of the temporal spectra of signals and find the frequency dependences of scintillation indices. The influence of scintillation on estimates of the received signal power and refraction angle is studied.

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