Scientific Program | ISCRA-2017

Multi-component (nuclei, protons, gammas, neutrons, muons, neutrinos) research of PeV-energy cosmic rays.

1.1. Experimental data and their interpretation.

1.2. Search for PeVatrons.

1.3. Models of CR acceleration and their limiting energies.
Cosmic Rays in heliosphere, magnetosphere and atmosphere of the Earth.

2.1. Unsolved problems of CR modulation in the heliosphere.

2.2. Penetration of CR into dynamic magnetosphere and their influence on the atmosphere.

2.3. Solar activity and radiation safety of space flights.