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,, and A. E. Tsvetkova

TL;DR
This paper presents a comprehensive analysis of solar flare observations from 1994 to 2013 using Konus-Wind and Helicon-Coronas-F instruments, including spectral evolution studies of specific flares.
Contribution
It provides detailed data and analysis techniques for solar flare observations over nearly two decades, highlighting spectral evolution and instrument capabilities.
Findings
Detection of 834 solar flares by Konus-Wind
Over 300 solar flares detected by Helicon-Coronas-F
Spectral analysis of specific notable flares
Abstract
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.
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