Predicting GCR fluxes for future space missions
- Authors: Popova E.P.1,2, Kuznetsov N.V.1, Panasyuk M.I.1,3
-
Affiliations:
- Skobeltsyn Institute of Nuclear Physics
- Schmidt Institute of Physics of the Earth
- Faculty of Physics
- Issue: Vol 81, No 2 (2017)
- Pages: 173-176
- Section: Proceedings of the 34th All-Russian Conference on Cosmic Rays
- URL: https://journal-vniispk.ru/1062-8738/article/view/184961
- DOI: https://doi.org/10.3103/S1062873817020332
- ID: 184961
Cite item
Abstract
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.
About the authors
E. P. Popova
Skobeltsyn Institute of Nuclear Physics; Schmidt Institute of Physics of the Earth
Author for correspondence.
Email: popovaelp@mail.ru
Russian Federation, Moscow, 119991; Moscow, 123242
N. V. Kuznetsov
Skobeltsyn Institute of Nuclear Physics
Email: popovaelp@mail.ru
Russian Federation, Moscow, 119991
M. I. Panasyuk
Skobeltsyn Institute of Nuclear Physics; Faculty of Physics
Email: popovaelp@mail.ru
Russian Federation, Moscow, 119991; Moscow, 119991
Supplementary files
