Volume 25 Issue 5
Sep.  2005
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G. Y. Smolkov, S. V. Lesovoy, V. G. Z,anov, A. T. Altyntsev, A.V. Gubin. The Main Results and the Perspectives in the Researches at SSRT[J]. Journal of Space Science, 2005, 25(5): 351-355. doi: 10.11728/cjss2005.05.351
Citation: G. Y. Smolkov, S. V. Lesovoy, V. G. Z,anov, A. T. Altyntsev, A.V. Gubin. The Main Results and the Perspectives in the Researches at SSRT[J]. Journal of Space Science, 2005, 25(5): 351-355. doi: 10.11728/cjss2005.05.351

The Main Results and the Perspectives in the Researches at SSRT

doi: 10.11728/cjss2005.05.351
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2005-09-15
  • In this report briefly presented the contemporary state of the experimental base of Radio Astrophysical Observatory (RAO) of the Institute of Solar-Terrestrial Physics (ISTP), the methodology of radioheliographic monitoring of the solar corona, the SSRT database, the RAO Web-pages, factors limiting the effective use of SSRT. Here are formulated the original results of the basic directions of the solar activity researches and the problems solutions on SSRT: (1) active regions at various development stages, morphology, modeling,signs of energy accumulation and flares buildup, forecast of powerful flares; (2) scenario, topology and the fine temporal picture of flares development, signs of primary energy release, radio emission mechanisms, scatter effects of radio emission in turbulent corona, energetic particles fluxes; (3) filaments; (4) CME with the localization of their initiation at the solar disk background, development scenario of filament activation + CME +flare; (5) coronal holes, and (6) bright coronal points.

     

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