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Astronomy
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Energetic electrons in the tail and transition region of the magnetosphere
Energetic electrons in the tail and transition region of the magnetosphere
Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events
Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events
Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events
Solar Energetic Proton Fluxes in Near-Earth Space on March 13–23, 2023
On the belt of energetic electrons at L = 2.75 in the Earth’s magnetosphere
Relaxation of electron and proton radiation belts of the earth after strong magnetic storms
Relaxation of electron and proton radiation belts of the earth after strong magnetic storms
Catalogs of Solar Proton Events as a Tool for Studying Space Weather
Coronal Propagation of Solar Protons during and after Their Stochastic Acceleration
Solar and Heliospheric Phenomena in October–November 2003: Causes and Effects
Solar and Heliospheric Phenomena in October–November 2003: Causes and Effects
The rigidity dependence of characteristic decay time and mean free path in SCR events
The rigidity dependence of characteristic decay time and mean free path in SCR events
Energy Spectrum of Galactic 10–100 MeV Protons in Quiet Sun Periods
Energy Spectrum of Galactic 10–100 MeV Protons in Quiet Sun Periods
Fluxes of low-energy particles in quiet periods of solar activity and the MgII index
Contribution of solar cosmic rays to the formation of the Earth’s proton radiation belt
On the belt of energetic electrons at L = 2.75 in the Earth’s magnetosphere