Abstract
The development of observational equipment and software for processing and efficient representation of spectral and polarization solar microwave observations on the RATAN-600 contributes to obtaining new information about the parameters of plasma at the chromospheric and coronal levels. Current status of information system for RATAN-600 solar observations is described, which is devoted to automatically capturing, storing, transmitting and processing the data and near-real-time publishing them on the Internet. The user web interface for interactive search, visualization, and on-line analysis of the data is available at http://www.spbf.sao.ru/prognoz/.
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Original Russian Text © S.Kh. Tokhchukova, 2011, published in Astrofizicheskii Byulleten, 2011, Vol. 66, No. 3, pp. 409–419.
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Tokhchukova, S.K. RATAN-600 radio telescope in the 24th solar activity cycle. IV. Information system for RATAN-600 solar observations. Astrophys. Bull. 66, 379–388 (2011). https://doi.org/10.1134/S1990341311030102
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DOI: https://doi.org/10.1134/S1990341311030102