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Ionization of the earth's atmosphere by solar and galactic cosmic rays

Wybrane pełne teksty z tego czasopisma
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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
A brief review of the research of atmospheric effects of cosmic rays is presented. Numerical models are discussed, that are capable to compute the cosmic ray induced ionization at a given location and time. Intercomparison of the models, as well as comparison with fragmentary direct measurements of the atmospheric ionization, validates their applicability for the entire atmosphere and the whole range of the solar activity level variations. The effect of sporadic solar energetic particle events is shown to be limited on the global scale, even for the most severe event, but can be very strong locally in polar regions, affecting the physical-chemical properties of the upper atmosphere, especially at high altitudes. Thus, a new methodology is presented to study cosmic ray induced ionization of the atmosphere in full detail using realistic numerical models calibrated to direct observations.
Słowa kluczowe
Czasopismo
Rocznik
Strony
88--101
Opis fizyczny
Bibliogr. 36 poz.
Twórcy
autor
autor
autor
Bibliografia
  • Bazilevskaya, G.A., I.G. Usoskin, E.O. Flückiger, R.G. Harrison, L. Desorgher, R. Bütikofer, M.B. Krainev, V.S. Makhmutov, Y.I. Stozhkov, A.K. Svirzhevskaya, N.S. Svirzhevsky, and G.A. Kovaltsov (2008), Cosmic ray induced ion production in the atmosphere, Space Sci. Rev. 137, 1-4, 149-173,
  • Butikofer, R., E.O. Flückiger, L. Desorgher, and M.R. Moser (2006), Analysis of the GLE on January 20, 2005: an update, Proc. 20th Europ. Cosmic Ray Symp., Lisbon, Portugal, http://www.lip.pt/events/2006/ecrs/proc.
  • Damiani, A., M. Storini, M. Laurenza, C. Rafanelli, E. Piervitali, and E.G. Cordaro (2006), Southern ozone variations induced by solar particle events during 15 January - 5 February 2005, J. Atmos. Solar-Terr. Phys. 68, 2042-2052 [errata corrige: 69, 628-630, 2007],
  • Damiani, A., M. Storini, M. Laurenza, and C. Rafanelli (2008a), Solar particle effects on minor components of the Polar atmosphere, Ann. Geophys. 26, 2, 361-370.
  • Damiani, A., P. Diego, M. Laurenza, M. Storini, and C. Rafanelli (2008b), Ozone variability related to several SEP events occurring during solar cycle no 23, Adv. Space Res., DOI: 10.1016/j.asr.2008.06.006 (in press).
  • Desorgher, L., E.O. Flückiger, M. Gurtner, M.R. Moser, and R. Bütikofer (2005), ATMOCOSMICS: a GEANT4 code for computing the interaction of cosmic rays with the Earth's atmosphere, Int. J. Modern Phys. A 20, 6802- 6804,
  • Dorman, L. (2004), Cosmic Rays in the Earth's Atmosphere and Underground, Kluwer Academic Publishers, Dordrecht.
  • Ermakov, V.I., G.A. Bazilevskaya, P.E. Pokrevsky, and Yu.I. Stozhkov (1997), Ion balance equation in the atmosphere, J. Geophys. Res. 102, D19, 23413-23419,
  • Jackman, C.H., R.G. Roble, and E.L. Fleming (2007), Mesospheric dynamical changes induced by the solar proton events in October-November 2003, Geophys. Res. Lett. 34, L04812,
  • Krivolutsky, A.A., A.V. Klyuchnikova, G.R. Zakharov, T.Yu. Vyushkova, and A.A. Kuminov (2006), Dynamical response of the middle atmosphere to solar proton event of July 2000: Three-dimensional model simulations, Adv.Space Res. 37, 8, 1602-1613,
  • Lowder, W.M., P.D. Raft, and H.L. Beck (1972), Experimental determination of cosmic-ray charged particle intensity profiles in the atmosphere. In:E.A. Warman (ed.), Proc. Nat. Symp. on Natural and Manmade Radiation in Space, Las Vegas, 1971, NASA, 908-913.
  • Mateev, L. (1997), An improved model of the cosmic ray ionization in the high latitude ionosphere considering the anomalous cosmic rays component, Bulg. Geophys. J. 23, 1-2, 87-95.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-BSL8-0025-0027
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