Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1764550 | Advances in Space Research | 2013 | 8 Pages |
Abstract
We present a new measurement of the cosmic ray proton and helium spectra by the PAMELA experiment performed using the “thin” (in terms of nuclei interactions) sampling electromagnetic calorimeter. The described method, optimized by using Monte Carlo simulation, beam test and experimental data, allows the spectra to be measured up to 10 TeV, thus extending the PAMELA observational range based on the magnetic spectrometer measurement.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
O. Adriani, G.C. Barbarino, G.A. Bazilevskaya, M. Boezio, E.A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S.V. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, M.P. De Pascale, C. De Santis,