
We propose a technique for analyzing radiooccultation data that allows the effects of the noise, ionosphere, and atmosphere on the radiooccultation resu lts to be reliably separated. This enables a more accurate investigation into the ionosphere formation mechanisms. Ionized layers are shown to exist in the dayside ionosphere of Venus at altitudes from 80 to 120 km. The position of the lower boundary of this ionized region can vary over the range of 80-100 km and the electron density gradients can change several times sev� eral.
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