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arXiv 1412.2015astro-ph.SR
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太阳耀斑的Konus风和Helicon-Coronas-F观测

Konus-Wind and Helicon-Coronas-F Observations of Solar Flares

V. D. Pal'shin, Yu. E. Charikov, R. L. Aptekar, S. V. Golenetskii, A. A. Kokomov, D. S. Svinkin, Z. Ya. Sokolova, M. V. Ulanov, D. D. Frederiks, A. E. Tsvetkova

摘要:

介绍了1994年11月至2013年12月Konus-Wind实验和2001年至2005年Helicon Coronas-F实验运行期间获得的太阳耀斑观测结果。对于所指示的期间,Konus-Wind在触发模式下检测到834个太阳耀斑,Helicon-Coronas-F检测到超过300个太阳耀斑。文中介绍了仪器和数据处理技术。作为例子,利用Konus-Wind数据分析了耀斑SOL 2012 -11- 08 T02:19(M1.7)和SOL 2002 -03- 10 T01:34(C5.1)的光谱演化,利用Helicon-Coronas-F数据分析了耀斑SOL 2003 -10- 26 T06:11(X1.2)在2.223MeV氘线上的光谱演化。

英文摘要:

Results of solar flare observations obtained in the Konus-Wind experiment from November, 1994 to December, 2013 and in the Helicon Coronas-F experiment during its operation from 2001 to 2005, are presented. For the periods indicated Konus-Wind detected in the trigger mode 834 solar flares, and Helicon-Coronas-F detected more than 300 solar flares. A description of the instruments and data processing techniques are given. As an example, the analysis of the spectral evolution of the flares SOL2012-11-08T02:19 (M 1.7) and SOL2002-03-10T01:34 (C5.1) is made with the Konus-Wind data and the flare SOL2003-10-26T06:11 (X1.2) is analyzed in the 2.223 MeV deuterium line with the Helicon-Coronas-F data.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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