Experimental study of galactic cosmic ray fluxes in the solar modulation energy region

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Abstract

Proposals for a new approach to the development of scientific equipment for the study of galactic and solar cosmic ray fluxes in the solar modulation energy range (30–1000 MeV/nucleon) with elementary charge and mass resolution are considered. It is proposed to place the equipment on the Russian space station ROS (project "Modulation") and on the international scientific lunar station MNLS (project "Moon–Modulation"), if it is created. The projects assume the creation of a database of galactic and solar cosmic rays (SCR) for the entire solar activity cycle. Such a database is necessary to improve numerical models of the fluxes of energetic heliospheric particles in interplanetary and near-Earth space.

About the authors

D. M. Podorozhny

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Email: dmpo@bk.ru
Moscow, Russia

A. V. Gorbunov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

V. V. Kalegaev

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

D. E. Karmanov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

I. M. Kovalev

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

A. A. Kurganov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

A. D. Panov

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

M. V. Podzolko

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

A. N. Turundavsky

Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics

Moscow, Russia

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