Astrophysical Bulletin

, 66:379 | Cite as

RATAN-600 radio telescope in the 24th solar activity cycle. IV. Information system for RATAN-600 solar observations

Article

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/.

Key words

Sun activity—techniques radar astronomy—techniques polarimetric 

References

  1. 1.
    V. M. Bogod, Astrophysical Bulletin 66, 189 (2011).ADSGoogle Scholar
  2. 2.
    V. M. Bogod, A. M. Alesin, and A. A. Pervakov, Astrophysical Bulletin 66, 204 (2011).ADSGoogle Scholar
  3. 3.
    V. M. Bogod, G. N. Zhekanis, M. G. Mingaliev, and S. Kh. Tokhchukova, Izv. Vyssh. Uchebn. Zaved., Radiofiz. 47, 1 (2004) (in Russian) (English translation in: Radiophys. Quantum Electron. (Engl. Transl.) 2004, v. 47, no. 4, p. 227).Google Scholar
  4. 4.
    V. M. Bogod and S. Kh. Tokhchukova, Pis’ma Astronom. Zh. 29, 305 (2003).Google Scholar
  5. 5.
    V. M. Bogod and L. V. Yasnov, Solar Phys. 255, 253 (2009).ADSCrossRefGoogle Scholar
  6. 6.
    T. I. Kal’tman, A. N. Korzhavin, and Yu. P. Tsap, Astronom. Zh. 82, 838 (2005).Google Scholar
  7. 7.
    S. V. Baldin and V. I. Garaimov, Astrophysical Bulletin 66, 371 (2011).ADSCrossRefGoogle Scholar
  8. 8.
    T. I. Kal’tman, Dissertation Cand. Phys.-Math. Sci. (Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnii Arkhyz, 2000).Google Scholar
  9. 9.
    S. L. Freeland and B. N. Handy, Solar Phys. 182, 497 (1998).ADSCrossRefGoogle Scholar
  10. 10.
    V. I. Garaimov, Preprint No. 127T (Nizhnii Arkhyz, Special Astrophysical Observatory of the Russian Academy of Sciences, 1997).Google Scholar
  11. 11.
    V. V. Grechnev, in Proceedings of Int. Symp. Phys. Processes associated with the Sun, (Weihai, China, 2002), http://srg.bao.ac.cn/weihailect/Grechnev//Grechnev01.htm.
  12. 12.
    S. B. Akhmedov, V. M. Bogod, V. N. Borovik et al., Astrof. Issled. (Izv. Spetsialnoi Astrofiz.Obs.) 25, 105 (1987).ADSGoogle Scholar
  13. 13.
    R. A. Sych, V. M. Nakariakov, S. A. Anfinogentov, and L. Ofman, Solar Phys. 266, 349 (2010).ADSCrossRefGoogle Scholar
  14. 14.
    Sh. B. Akhmedov, G. B Gelfreikh, V. M. Bogod, and A. N. Korzhavin, Solar Phys. 79, 41 (1982).ADSCrossRefGoogle Scholar
  15. 15.
    Markus J. Aschwanden, Solar Phys. 262, 235 (2010).ADSCrossRefGoogle Scholar
  16. 16.
    T. I. Kaltman, V. M. Bogod, S. Kh. Tokhchukova, and A. N. Korzhavin, in Electronic proceedings of 12th European Solar Physics Meeting, (Freiburg, Germany, 2008), http://espm.kis.uni-freiburg.de/fileadmin//user_upload/espm/Proceedings-Poster/p_23-28.pdf.

Copyright information

© Pleiades Publishing, Ltd. 2011

Authors and Affiliations

  1. 1.Special Astrophysical ObservatoryRussian Academy of SciencesNizhnii ArkhyzRussia

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