Abstract
Frequency fluctuation data of monochromatic radio waves propagating through the circumsolar plasma in 1975–2002 are systematized and analyzed. The radial dependences of the intensity of the frequency fluctuations are obtained for the decimeter radio waves in the circumsolar plasma from the results of radio sounding using the Ulysses and Galileo spacecrafts. It is demonstrated that the radial profile of the rms frequency fluctuations can be approximated by a power-law function whose exponent is determined by the intensity of the plasma inhomogeneities, the velocity of solar wind, the spectral index of the spatial spectrum of the plasma fluctuations, and the outer scale of turbulence. It is also shown that three different frequency fluctuation regimes are found in the solar wind acceleration region and in the inner and outer regions of the stable solar wind.
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Original Russian Text © A.I. Efimov, L.A. Lukanina, L.N. Samoznaev, I.V. Chashei, M.K. Bird, 2010, published in Radiotekhnika i Elektronika, 2010, Vol. 55, No. 11, pp. 1343–1349.
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Efimov, A.I., Lukanina, L.A., Samoznaev, L.N. et al. Frequency fluctuation of spacecraft radio signals in the circumsolar plasma. J. Commun. Technol. Electron. 55, 1253–1259 (2010). https://doi.org/10.1134/S1064226910110070
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DOI: https://doi.org/10.1134/S1064226910110070