Spectra of Fe ions in powerful SCR events
- 作者: Baranov D.G.1, Dergachev V.A.1, Nymmik R.A.2, Panasyuk M.I.2
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隶属关系:
- Ioffe Institute
- Skobeltsyn Institute of Nuclear Physics
- 期: 卷 81, 编号 2 (2017)
- 页面: 128-131
- 栏目: Proceedings of the 34th All-Russian Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/184948
- DOI: https://doi.org/10.3103/S1062873817020058
- ID: 184948
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详细
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.
作者简介
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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