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Back-Tracing and Flux Reconstruction for Solar Events with PAMELA
A. Bruno, O. Adriani, G. C. Barbarino +64
The PAMELA satellite-borne experiment is providing first direct measurements of Solar Energetic Particles (SEPs) with energies from 80 MeV to several GeV in near-Earth space.…
Temporal and energy behavior of cosmic ray fluxes in the periods of low solar activity
G. A. Bazilevskaya, M. S. Kalinin, M. B. Krainev +3
Modulation of galactic cosmic ray intensity is governed by several mechanisms including diffusion, convection, adiabatic energy losses and drift. Relative roles of these factors ch…
Modeling the time and energy behavior of the GCR intensity in the periods of low activity around the last three solar minima
M. B. Krainev, G. A. Bazilevskaya, M. S. Kalinin +2
Using the simple model for the description of the GCR modulation in the heliosphere and the sets of parameters discussed in the accompanying paper we model some features of the tim…
On the description of the GCR intensity in the last three solar minima
M. S. Kalinin, G. A. Bazilevskaya, M. B. Krainev +2
We discuss the main characteristic features in the heliospheric parameters important for the GCR intensity modulation for the last three solar minima (1986--1987, 1996--1997 and 20…
Measurement of boron and carbon fluxes in cosmic rays with the PAMELA experiment
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya +61
The propagation of cosmic rays inside our galaxy plays a fundamental role in shaping their injection spectra into those observed at Earth. One of the best tools to investigate this…