@article {5004,
	title = {A numerical model approximating extreme energetic electron events involved in the physical and chemical processes of the middle atmosphere},
	journal = {Advances in Space Research},
	volume = {43},
	year = {2009},
	note = {Export Date: 2 November 2015CODEN: ASRSDCorrespondence Address: Tritakis, V.P.; Research Center for Astronomy and Applied Mathematics, Academy of Athens, Soranou Efesiou 4, 11527 Athens, Greece; email: vas@academyofathens.grReferences: Burns, A.G., Killeen, T.L., Crowley, G., Emery, B.A., Roble, R.G., On the mechanisms responsible for high latitude thermospheric composition variations during the recovery phase of a geomagnetic storm (1989) J. Geophys. Res., 94 (A12), pp. 16961-16968;Butko, A.S., Ivanova, I.N., Kokin, G.A., Some peculiarities of thermal and circulation regime of the atmosphere (1974) Solar-Atmospheric Relationships, pp. 125-144. , Hydrometeoizdat, Leningrad (in Russian); 
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},
	month = {2009},
	pages = {665 - 672},
	abstract = {Relativistic electrons (with energies >150 keV) which originate in the outer radiation belt and detected by the Russian {\textquoteright}Meteor{\textquoteright} series of satellites have been correlated with the atmospheric total ozone data compiled by almost 90 stations located around the world within the latitude zone 40{\textdegree}-70{\textdegree}N. In more than 60\% of the stations examined we have detected a clear decrease of the ozone 3-5 days after the electron flux excess. A numerical model has been applied to approximate this effect based on relativistic electron initiated nitric oxides creation in the upper mesosphere with subsequent atmospheric transport (both vertical and horizontal) towards the upper stratosphere. A first attempt of local and temporal prediction of ozone depletion because of energetic electrons impact in the middle atmosphere has been illustrated. {\textcopyright} 2008 COSPAR.},
	keywords = {Atmospheric chemistry, Atmospheric ozone, Atoms, Chemical engineering, Electron scattering, Electrons, Energetic electrons, Gases, Magnetosphere, Meteor satellites, Middle atmosphere, Modelling, Nitric oxide, Nuclear energy, Numerical methods, Ozone, Ozone layer, Radiation belts, Relativistic electron precipitation, Satellites, Sulfur compounds, Upper atmosphere},
	isbn = {02731177 (ISSN)},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-59749106380\&partnerID=40\&md5=6edbad3b45321a96f5f9ec632d081e5a},
	author = {Tritakis, V. P. and Pisanko, Yu.V. and Paliatsos, A. G. and Korbakis, G. K. and Nastos, P.Th.}
}
