Predicting the solar and galactic cosmic ray fluxes influencing the upper atmosphere: Dependence on solar activity level

Advances in Space Research

Volumn 22, Issue 1, 1998, Pages 143-146

  Nymmik, R A ^a  

^a MOSCOW STATE UNIVERSITY   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0039394499     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)01115-0     Document Type: Article

References (8)

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3. Nymmik R.A., Behavioural features of energy spectra of particle fluences and peak flux in solar cosmic rays. Proceedings 24th ICRC (Roma), 3, 66 (1995).
4. Nymmik R.A., Radiation environment inducted by cosmic ray particle fluxes in the ALPHA station orbit in terms of the present-day galactic and solar cosmic rays, accepted to Adv. Space Res. (1996).
5. Nymmik R.A., On the dependence of solar cosmic ray occurrence frequency on solar activity level. Kosmicheskiye Issledovaniya 35 (2), 213 (1997a).
6. Nymmik R.A. Statistical and functional analysis of the characteristics of energy spectra of solar cosmic ray particles (1 ≤ Z ≤ 28). Izv. Ross. Akad. Nauk. ser. fiz. 61, (4), (1997b).
7. Nymmik R.A., Panasyuk M.I. and Suslov A.A., Galactic cosmic ray flux simulation and prediction. Adv. Space Res. 17, (2), 19 (1995).
8. Tsyganenko, N.A., Magnetospheric magnetic field model with a warped tail current sheet. Planetary and Space Science 37, 5 (1989).