The special Soviet radio network for Vega balloon data acquisition and interferometry

Details The special Soviet radio network for Vega balloon data acquisition and interferometry The special Soviet radio network for Vega balloon data acquisition and interferometry

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sval...12...52a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Feb. 1986, p. 131-136) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Jan.-Feb

Computer Science

Sound

3

Balloon Sounding, Radio Interferometers, Vega Project, Venus Atmosphere, Data Acquisition, Meteorological Parameters, Real Time Operation, Signal To Noise Ratios, Very Long Base Interferometry

Scientific paper

Special receiving and recording equipment was developed for Project Vega so as to optimize the signal/noise ratio during acquisition of meteorological data from the balloons and to maximize the ratio interferometry accuracy. In the working band, the system has a phase-frequency characteristic curve linear to within 1 deg; four-bit signal coding is used. During the experiment, the balloon and flyby-craft signals were recorded simultaneously; the signal parameters were monitored and the scientific information discriminated in real time.

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