Abstract
In this paper, we present the results of two series of experiments on radio sounding of near-solarplasma by the signals of the Mars Express and Venus Express spacecraft in 2006 and Mars Express in 2008.The radio sounding data are compared with measurements of the proton concentration near the Earth’s orbiton the Wind satellite. This analysis shows that the general nature of the temporal dynamics of disturbancesobserved in two series of measurements is qualitatively similar. The sequence of amplifications of fluctuationsin the frequency and density of protons indicates that the observed disturbances are associated with co-rotatingregions of interaction of solar wind flows of various velocities
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