Commissioning of the Siberian Solar Radiotelescope and the results of first observations

Physics

Scientific paper

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Angular Resolution, Antenna Arrays, Parabolic Reflectors, Radio Interferometers, Radio Telescopes, Solar Activity, Circular Polarization, Microwave Equipment, Siberia, Waveguide Antennas

Scientific paper

The Siberian Solar Radiotelescope (SSRT) completed at a site in the eastern Sayan mountains in 1984 is described, and some previously published observational results are briefly summarized. The SSRT comprises two mutually orthogonal lines of 128 synchronously tracking 2.5-m parabolic reflector antennas placed 4.9 m apart. The SSRT field of view (70 arcmin) and angular resolution (20 arcsec at wavelength 5.2 cm) permit study of active regions or flare processes and measurement of whole-sun diagnostics to be performed simultaneously.

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