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Morselli, A.; Picozza, P.; Barbiellini, G.; Golden, R.L.; Paradis, P.J.; Stochaj, S.J.; Badwhar, G.D.; Daniel, R.R.
WIZARD collaboration : Papers presented at the 24. International Cosmic Ray Conference, August 28-September 8, Rome 19951995
WIZARD collaboration : Papers presented at the 24. International Cosmic Ray Conference, August 28-September 8, Rome 19951995
AbstractAbstract
[en] Hydrogen and helium cosmic ray nuclei spectra gathered from 1976 to 1993 have been corrected to the top of the atmosphere and normalized at high rigidities. The variation of these primary cosmic ray fluxes above 400 MeV/nucleon has been examined as a function of the phase of the solar cycle with the force-field approximation model. The intensity of the normalized fluxes between solar maximum and minimum conditions varies by a factor of 6 for hydrogen and a factor of 4.3 for helium at the lowest rigidities considered
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Istituto Nazionale di Fisica Nucleare, Frascati (Italy). Lab. Nazionale di Frascati; 86 p; Sep 1995; p. 59-62; 24. international cosmic ray conference; Rome (Italy); 28 Aug - 8 Sep 1995
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