A.L. Mishev, P.I.Y. Velinov, Ion production and ionization effect in the atmosphere during the Bastille day GLE 59 due to high energy SEPs, Advances in Space Research, Volume 61, Issue 1, 2018, Pages 316-325, ISSN 0273-1177, https://doi.org/10.1016/j.asr.2017.10.023
Ion production and ionization effect in the atmosphere during the Bastille day GLE 59 due to high energy SEPs
|Author:||Mishev, A.L.1,2; Velinov, P.I.Y.3|
1Space Climate Research Unit, University of Oulu, Finland
2Sodankylä Geophysical Observatory (Oulu unit), University of Oulu, Finland
3Institute for Space Research and Technology, Bulgarian Academy of Sciences, Bl. 1 Acad. G. Bonchev str., 1113 Sofia, Bulgaria
|Online Access:||PDF Full Text (PDF, 1 MB)|
|Persistent link:|| http://urn.fi/urn:nbn:fi-fe2019100431162
|Publish Date:|| 2019-11-02
The influence of high energy particles, specifically cosmic rays, on atmospheric physics and chemistry is highly discussed. In most of the proposed models the role of ionization in the atmosphere due to cosmic rays is not negligible. Moreover, effect(s) on minor constituents and aerosols are recently observed, specifically over the polar regions during strong solar particle events. According to the recent findings for such effects it is necessary an essential increase of ion production, specifically during the winter period. The galactic cosmic rays are the main source of ionization in the Earth’s stratosphere and troposphere. Occasionally, the atmospheric ionization is significantly enhanced during strong solar energetic particles events, specifically over the polar caps. During the solar cycle 23 several strong ground level enhancements were observed. One of the strongest was the Bastille day event occurred on 14 July 2000. Using a full Monte Carlo 3-D model, we compute the atmospheric ionization, considering explicitly the contribution of cosmic rays with galactic and solar origin, focusing on high energy particles. The model is based on atmospheric cascade simulation with the PLANETOCOSMICS code. The ion production rate is computed as a function of the altitude above the sea level. The ion production rate is computed on a step ranging from 10 to 30 min throughout the event, considering explicitly the spectral and angular characteristics of the high energy part of solar protons as well as their time evolution. The corresponding event averaged ionization effect relative to the average due to galactic cosmic rays is computed in lower stratosphere and upper troposphere at various altitudes, namely 20 km, 15 km, 12 km and 8 km above the sea level in a sub-polar and polar regions. The 24h and the weekly ionization effects are also computed in the troposphere and low stratosphere. Several applications are discussed.
Advances in space research
|Pages:||316 - 325|
|Type of Publication:||
A1 Journal article – refereed
|Field of Science:||
115 Astronomy and space science
This work was supported by the Academy of Finland (project 272157, Center of Excellence ReSoLVE).
|Academy of Finland Grant Number:||
272157 (Academy of Finland Funding decision)
© 2017. This manuscript version is made available under the CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/.