Spectra of Fe ions in powerful SCR events


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Large solar cosmic ray (SCR) events are registered by PLATAN equipment in September–October 1989 aboard the MIR orbital station and in October–November 2003 aboard the International Space Station (ISS). The energy spectra of Fe ions in the energy intervals of 5–200 MeV/nucleon (1989) and 25–90 MeV/nucleon (2003) are measured. Spectra for SCR events of 1989 and 2003 are approximated with high accuracy by the power law function of energy. The SCR events of 1989 greatly exceed those of 2003 in the fluence of Fe particles. High enrichment of the elemental composition of the SCR events 2003 with Fe ions is observed.

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D. Baranov

Ioffe Institute

编辑信件的主要联系方式.
Email: d.baranov@bk.ru
俄罗斯联邦, St. Petersburg, 194021

V. Dergachev

Ioffe Institute

Email: d.baranov@bk.ru
俄罗斯联邦, St. Petersburg, 194021

R. Nymmik

Skobeltsyn Institute of Nuclear Physics

Email: d.baranov@bk.ru
俄罗斯联邦, Moscow, 119991

M. Panasyuk

Skobeltsyn Institute of Nuclear Physics

Email: d.baranov@bk.ru
俄罗斯联邦, Moscow, 119991

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