| Issue |
Section |
Title |
File |
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Spectra of solar neutrons with energies of ~10–1000 MeV in the PAMELA experiment in the flare events of 2006–2015 |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Solar modulation of cosmic deuteron fluxes in the PAMELA experiment |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Modulation of electrons and positrons in 2006–2015 in the PAMELA experiment |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Crossovers of the energy spectra of galactic cosmic rays in the activity minima of consecutive solar cycles |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Secondary positrons and electrons in near-Earth space in the PAMELA experiment |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Precipitation of magnetospheric electrons into the Earth’s atmosphere and the electrons of the outer radiation belt |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Variations in cosmic rays and the surface electric field in January 2016 |
|
| Vol 81, No 2 (2017) |
Proceedings of the 34th All-Russian Conference on Cosmic Rays |
Cosmic rays, solar activity, and changes in the Earth’s climate |
|
| Vol 83, No 5 (2019) |
Article |
Solar Activity and Cosmic Ray Variations in September 2017 |
|
| Vol 83, No 5 (2019) |
Article |
Solar Modulation of the Galactic Electron and Proton Intensity near the Activity Minimum of 2009 |
|
| Vol 83, No 5 (2019) |
Article |
Minimum Value of the Heliospheric Magnetic Field in 2008–2010, According to WIND and ACE Data |
|
| Vol 83, No 5 (2019) |
Article |
Long-Term Evolution of the Occurrence Rate of Magnetospheric Electron Precipitation into the Earth’s Atmosphere |
|
| Vol 83, No 8 (2019) |
Article |
Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment |
|
