Predicting GCR fluxes for future space missions


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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

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