Long-Term cosmic ray experiment in the atmosphere: Energetic electron precipitation events during the 20-23 solar activity cycles.

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More than 400 energetic electron precipitation events (EPEs) were observed in the Earth's Northern polar atmosphere (Murmansk region, 68°57'N, 33°03'E) during a long-term cosmic ray balloon experiment (from 1957 up to now). It is shown that the significant X-ray fluxes, caused by precipitating electrons at the top of the atmosphere, sometimes penetrated down to the atmospheric depth of ~60 g· cm-2 (about 20 km). It means that primary energy of precipitating electrons was more than ~ 6 10 MeV. Here we summarize only the characteristics of the energetic electron precipitation events recorded during solar activity cycles 20 to 23. We dis cuss results from the analyses of the interplanetary and geomagnetic conditions related to these events in the atmosphere.

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