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

被引：21

作者：

Pal'shin, V. D. ^{[1
,2
]}

Charikov, Yu E. ^{[1
,2
,3
]}

Aptekar, R. L. ^{[1
]}

Golenetskii, S. V. ^{[1
]}

Kokomov, A. A. ^{[1
]}

Svinkin, D. S. ^{[1
]}

Sokolova, Z. Ya ^{[1
]}

Ulanov, M. V. ^{[1
,2
]}

Frederiks, D. D. ^{[1
]}

Tsvetkova, A. E. ^{[1
]}

机构：

[1] AF Ioffe Phys Tech Inst, St Petersburg 194021, Russia

[2] St Petersburg State Polytech Univ, St Petersburg, Russia

[3] Russian Acad Sci, Cent Pulkovo Astron Observ, St Petersburg 196140, Russia

来源：

GEOMAGNETISM AND AERONOMY | 2014年 / 54卷 / 07期

关键词：

RHESSI;

D O I：

10.1134/S0016793214070093

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

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.

引用

页码：943 / 948

页数：6

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