Perspectives of advance of RATAN-600 solar observations

Details Perspectives of advance of RATAN-600 solar observations Perspectives of advance of RATAN-600 solar observations

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992an....313...97b&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 313, no. 2, 1992, p. 97-100.

Astronomy and Astrophysics

Astronomy

2

Radio Telescopes, Reflector Antennas, Solar Activity, Solar Observatories, Solar Spectra, Radio Astronomy, Solar Cycles, Spectrum Analysis

Scientific paper

The RATAN-600 telescope for solar radio-astronomical research is evaluated to optimize the use of the device during maximum solar activity. Improvements of the characteristics of the antenna receiver are assessed for: (1) radioheliographic observations; (2) full spectral coverage of the radio telescope at 1.5-18 GHz with frequency resolutions of near 1-2 MHz; and/or (3) solar tracking with msec temporal resolution. A self-adapting receiver complex is set forth which can optimally match observational tasks with instrumental capabilities.

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