High-energy gamma radiation of solar flares as an indicator of acceleration of energetic protons

被引:0
作者
Viktoriya G. Kurt
B. Yu. Yushkov
K. Kudela
V. I. Galkin
机构
[1] Moscow State University,Skobeltsyn Institute of Nuclear Physics
[2] Slovak Academy of Sciences,Institute of Experimental Physics
来源
Cosmic Research | 2010年 / 48卷
关键词
Flare; Solar Flare; Cosmic Research; Neutral Pion; Ground Level Enhancement;
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学科分类号
摘要
Using the SONG detector onboard the CORONAS-F satellite, gamma-ray emission of high energies (>100 MeV) was recorded during four solar flares. In the sequential spectra of gamma rays the peculiarity caused by generation and decay of neutral pions was isolated, which made it possible to determine with a high accuracy the moments of appearance in the solar atmosphere of protons accelerated up to energies above 300 MeV.
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页码:70 / 79
页数:9
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  • [1] Ramaty R.(1975)Solar Gamma Rays Space Sci. Rev. 18 341-388
  • [2] Kozlovsky B.(1987)Nuclear Processes and Accelerated Particles in Solar Flares Space Sci. Rev. 45 213-268
  • [3] Lingenfelter R.E.(1987)High-Energy Processes in Solar Flares Astrophys. J. Suppl. 63 721-748
  • [4] Ramaty R.(2006)Gamma-Rays and Neutrons from Solar Flares Detected by the SONG Instrument in 2001-2004 Astron. Vestn. 40 120-126
  • [5] Murphy R.J.(1995)Preliminary Results of an Experiment Carried out with SCR Instrumentation onboard the Izv. Akad. Nauk, Ser. Fiz. 59 2-6
  • [6] Murphy R.J.(1968) Satellite Astrophys. J. 153 L59-L64
  • [7] Dermer C.D.(2005)Comparison of Solar X-Ray Line Emission with Microwave Emission during Flares Astrophys. J. 621 482-497
  • [8] Ramaty R.(2004)Physics of the Neupert Effect: Estimates of the Effects of Source Energy, Mass Transport, and Geometry Using RHESSI and GOES Data Kosm. Issled. 42 453-508
  • [9] Kuznetsov S.N.(2005)Solar and Heliospheric Phenomena in October-November 2003: Causes and Effects Int. J. Modern Phys. A 20 6705-6707
  • [10] Kurt V.G.(2008)28 October 2003 Flare: High-Energy Gamma Emission, Type II Radio Emission and Solar Particle Observations Astrophys. J. 678 509-514