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The Main Results and the Perspectives in the Researches at SSRT

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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.

MonitoringDiagnosticSpace weatherSolar factorsMicrowave emission

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

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Radioastrophysical observatory, Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, Irkutsk 664033, Russia

Siberian Branch of RAS, Education and Science Ministry of Russian FederationFSTP "Astronomy", Leading scientific schoolRFBRRFBRRFBRRFBRRFBRRFBRRFBR-SFNS中-俄合作基金China-Russia Joint Research Center on Space WeatherChinese Academy of Sciences

01-27-SSRT00-15-96 710/SS-477.2003.202-02-39 03003-02-16 59103-02-16 22903-07-90 08703-02-310202-02-39030I0208/1173

2005

空间科学学报
中国科学院空间科学与应用研究中心 中国空间科学学会

空间科学学报

CSCD北大核心
影响因子：0.328
ISSN：0254-6124
年,卷(期)：2005.25(5)
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