作者: G.G. Karapetyan
DOI: 10.1016/J.ASTROPARTPHYS.2012.09.006
关键词: Electron avalanche 、 Atomic physics 、 Cosmic ray 、 Physics 、 Bremsstrahlung 、 Radiation 、 Gamma ray 、 Electric field 、 Thunderstorm 、 Electron
摘要: Abstract We conducted theoretical investigation of long lasting pulses cosmic-ray electrons and gamma-ray radiation, which are often observed during thunderstorms by particle detectors at high altitude stations. These thunderstorm ground enhancements (TGEs) last several minutes, the flux gamma-quants can surpass a few hundred percent over background level. developed model derived energetic spectrums given value electric field. The considers two following mechanisms, change in field: (i) transformation spectrum (ii) formation electron avalanche. Due to number low (few MeV) energy decreases small abundance ( 10 MeV emerges. spectral fluxes components – avalanche derived, shows that contribution total is small. Consequently, gamma ray produced as well. exact equations for these radiation showed curve be approximated simple function exp(− E / 0 )/E up ∼40 MeV. At higher energies it has approximately power-law spectrum.