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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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Volume 11, issue 5 | Copyright
Atmos. Chem. Phys., 11, 1979-1988, 2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.

Research article 03 Mar 2011

Research article | 03 Mar 2011

Ionization effect of solar particle GLE events in low and middle atmosphere

I. G. Usoskin1, G. A. Kovaltsov2, I. A. Mironova3, A. J. Tylka4, and W. F. Dietrich5 I. G. Usoskin et al.
  • 1Sodankylä Geophysical Observatory (Oulu unit), University of Oulu, Finland
  • 2Ioffe Physical-Technical Institute, St. Petersburg, Russia
  • 3Institute of Physics, St.Petersburg State University, St. Petersburg, Russia
  • 4Space Science Division, Naval Research Laboratory, Washington, DC, USA
  • 5Praxis, Inc., Alexandria, VA, USA

Abstract. Using a new reconstruction of the solar proton energy spectra for Ground Level Enhancement (GLE) events, based on fits to measurements from ground-based and satellite-borne instruments covering a wide energy range, we quantitatively evaluate the possible ionization effects in the low and middle atmosphere for 58 out of the 66 GLE events recorded by the world-wide neutron monitor network since 1956. The ionization computations are based on the numerical 3D CRAC:CRII model. A table of the ionization effect caused by the GLE events at different atmospheric heights is provided. It is shown that the direct ionization effect is negligible or even negative, due to the accompanying Forbush decreases, in all low- and mid-latitude regions. The ionization effect is important only in the polar atmosphere, where it can be dramatic in the middle and upper atmosphere (above 30 km) during major GLE events.

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