DESCRIPTION |
Instrument Overview
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Coherently related radio signals were transmitted by the spacecraft at
wavelengths of 8 cm and 32 cm. These passed through the ionosphere of
Venus before being received at the Evpatoria station (in the Crimean
region of what is now Ukraine) of the Soviet Deep Space Communication
Center. The standard equipment provided signal amplification,
heterodyning, and filtering. Next, the received transmissions were fed
into a dispersion interferometer, which used a closed-loop system to
perform narrow-band filtering in order to isolate the desired signals.
Amplitude and phase of both signals was recorded. Ionospheric electron
densities were obtained from these data products using standard
techniques for radio occultation experiments. The leader of the radio
occultation experiment was N. A. Savich and one of the experimenters
was A. L. Gavrik.
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