The Main Results and the Perspectives in the Researches at SSRT

被引：0

作者：

G.Y.Smolkov

S.V.Lesovoy

V.G.Zandanov

A.T.Altyntsev

A.V.Gubin

机构：

[1] Radioastrophysical observatory

[2] Institute of Solar-Terrestrial Physics

[3] Siberian Branch

[4] Russian Academy of Sciences

[5] Irkutsk

[6] Russia

[7] 不详

来源：

空间科学学报 | 2005年 / 05期

关键词：

Monitoring; Diagnostic; Space weather; Solar factors; Microwave emission;

D O I：

暂无

中图分类号：

P18 [太阳系];

学科分类号：

070401 ;

摘要：

<正>In this report briefly presented the contemporary state of the experimental base of Radio Astro-physical Observatory (RAO) of the Institute of Solar-Terrestrial Physics (ISTP), the methodology of radioheli-ographic 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.

引用

页码：351 / 355

页数：5

共 9 条

[1] Analysis of a solar eruptive event on November 4, 2001, using CORONAS-F/SPIRIT data[J] . I. M. Chertok,V. A. Slemzin,S. V. Kuzin,V. V. Grechnev,O. I. Bugaenko,I. A. Zhitnik,A. P. Ignat’ev,A. A. Pertsov.Astronomy Reports . 2004 (5)
[2] A method to analyze imaging radio data on solar flares
Grechnev, VV
[J]. SOLAR PHYSICS, 2003, 213 (01) : 103 - 110
[3] The Siberian Solar Radio Telescope: the current state of the instrument, observations, and data[J] . V.V. Grechnev,S.V. Lesovoi,G. Ya. Smolkov,B.B. Krissinel,V.G. Zandanov,A.T. Altyntsev,N.N. Kardapolova,R.Y. Sergeev,A.M. Uralov,V.P. Maksimov,B.I. Lubyshev.Solar Physics . 2003 (1)
[4] A flare of 23 September 1998: relation between temporal and spatial structures[J] . A.T. Altyntsev,R.A. Sych,V.V. Grechnev,N.S. Meshalkina,G.V. Rudenko.Solar Physics . 2002 (1)
[5] Dual-filament initiation of a Coronal Mass Ejection: Observations and Model[J] . A.M. Uralov,S.V. Lesovoi,V.G. Zandanov,V.V. Grechnev.Solar Physics . 2002 (1)
[6] Extrapolation of the solar magnetic field within the potential-field approximation from full-disk magnetograms
Rudenko, GV
[J]. SOLAR PHYSICS, 2001, 198 (01) : 5 - 30
[7] Microwave signatures of solar flare buildup
Smolkov, GY
Maksimov, VP
Uralov, AM
[J]. SPACE WEATHER: PHYSICS AND APPLICATIONS, 2000, 26 (01): : 193 - 196
[8] THE OBSERVATION OF A NEGATIVE BURST WITH HIGH SPATIAL-RESOLUTION
MAKSIMOV, VP
NEFEDYEV, VP
[J]. SOLAR PHYSICS, 1991, 136 (02) : 335 - 342
[9] The Siberian Solar Radio-Telescope: Parameters and principle of operation, objectives and results of first observations of spatio-temporal properties of development of active regions and flares[J] . G. Ya. Smolkov,A. A. Pistolkors,T. A. Treskov,B. B. Krissinel,V. A. Putilov,N. N. Potapov.Astrophysics and Space Science . 1986 (1)

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