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 monitori...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.展开更多
基金Supported by Siberian Branch of RASEducation and Science Ministry of Russian Federation(No.01-27-SSRT,FSTP"Astron-omy",Leading scientific school 00-15-96710/SS-477.2003.2)RFBR(02-02-39030,03-02-16591,03-02-16229,03-07-90087,03-02-3102)+2 种基金RFBR-SFNS(02-02-39030)Integration with the Universities:state contract(No.10208/1173)the China-Russia Joint Research Center on Space Weather,Chinese Academy of Sciences
文摘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.
