电邮这篇文章 Predicting GCR fluxes for future space missions
- 作者: Popova E.P.1,2, Kuznetsov N.V.1, Panasyuk M.I.1,3
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隶属关系:
- Skobeltsyn Institute of Nuclear Physics
- Schmidt Institute of Physics of the Earth
- Faculty of Physics
- 期: 卷 81, 编号 2 (2017)
- 页面: 173-176
- 栏目: Proceedings of the 34th All-Russian Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/184961
- DOI: https://doi.org/10.3103/S1062873817020332
- ID: 184961
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详细
An empirical model of galactic cosmic ray (GCR) fluxes is developed using a wide range of experimental data obtained during solar cycles 21–24. Forecasts of GCR fluxes for cycles 25 and 26 are given.
作者简介
E. Popova
Skobeltsyn Institute of Nuclear Physics; Schmidt Institute of Physics of the Earth
编辑信件的主要联系方式.
Email: popovaelp@mail.ru
俄罗斯联邦, Moscow, 119991; Moscow, 123242
N. Kuznetsov
Skobeltsyn Institute of Nuclear Physics
Email: popovaelp@mail.ru
俄罗斯联邦, Moscow, 119991
M. Panasyuk
Skobeltsyn Institute of Nuclear Physics; Faculty of Physics
Email: popovaelp@mail.ru
俄罗斯联邦, Moscow, 119991; Moscow, 119991
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