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- W306747758 abstract "In the last years the possible effect of solar variability on atmospheric physics and chemistry is highly debated. In most of the proposed models the role of ion production in the atmosphere due to cosmic rays is significant. At present, effects on minor constituents and aerosols are observed over polar regions during major solar events. According to recent findings for such a study it is necessary an essential increase of ion production, specifically during the winter season. Therefore, the ground level enhancement on 13th of December 2006 is appropriate for such a study. Here, we compute the ion production on 13th of December 2006 on the basis of a full target model based on Monte Carlo simulations. The ion production is computed on a step ranging from 10 to 30 min throughout the event. The spectral and angular characteristics of the solar protons are explicitly considered as well as their time evolution. The ionization effect is computed at several altitudes above the sea level, namely 25 km, 18 km, 15 km, 12 km and 8 km in a sub-polar a and polar region, where the effect is maximal. Several applications of the obtained results are discussed." @default.
- W306747758 created "2016-06-24" @default.
- W306747758 creator A5035931205 @default.
- W306747758 creator A5079726375 @default.
- W306747758 date "2015-07-01" @default.
- W306747758 modified "2023-09-23" @default.
- W306747758 title "Time evolution of ionization effect due to cosmic rays in terrestrial atmosphere during GLE 70" @default.
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- W306747758 doi "https://doi.org/10.1016/j.jastp.2015.04.016" @default.
- W306747758 hasPublicationYear "2015" @default.
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