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The Main Results and the Perspectives in the Researches at SSRT

G. Y. Smolkov S. V. Lesovoy V. G. Zandanov A. T. Altyntsev A.V. Gubin

G. Y. Smolkov, S. V. Lesovoy, V. G. Zandanov, A. T. Altyntsev, A.V. Gubin. The Main Results and the Perspectives in the Researches at SSRT[J]. 空间科学学报, 2005, 25(5): 351-355. doi: 10.11728/cjss2005.05.351
引用本文: G. Y. Smolkov, S. V. Lesovoy, V. G. Zandanov, A. T. Altyntsev, A.V. Gubin. The Main Results and the Perspectives in the Researches at SSRT[J]. 空间科学学报, 2005, 25(5): 351-355. doi: 10.11728/cjss2005.05.351
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

The Main Results and the Perspectives in the Researches at SSRT

  • 摘要: 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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出版历程
  • 收稿日期:  1900-01-01
  • 修回日期:  1900-01-01
  • 刊出日期:  2005-09-15

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