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Authors :
Papini, P.
Adriani, O.
Barbarino, G. C.
Bazilevskaya, G. A.
Bellotti, R.
Boezio, M.
Bogomolov, E. A.
Bonechi, L.
Bongi, M.
Bonvicini, V.
Borisov, S.
Bottai, S.
Bruno, A.
Cafagna, F.
Campana, D.
Carbone, R.
Carlson, Per
Casolino, M.
Castellini, G.
De Pascale, M. P.
De Simone, N.
Di Felice, V.
Galper, A. M.
Gillard, William
Grishantseva, L.
Hofverberg, Petter
Jerse, G.
Koldashov, S. V.
Krutkov, S. Y.
Kvashnin, A. N.
Leonov, A.
Malvezzi, V.
Marcelli, L.
Menn, W.
Mikhailov, V. V.
Mocchiutti, E.
Mori, N.
Nikonov, N.
Osteria, G.
Pearce, Mark
Picozza, P.
Pizzolotto, C.
Ricci, M.
Ricciarini, S. B.
Ritabrata, S.
Rossetto, Laura
Simon, M.
Sparvoli, R.
Spillantini, P.
Stozhkov, Y. I.
Vacchi, A.
Vannuccini, E.
Vasilyev, G.
Voronov, S. A.
Wu, Juan
Yurkin, Y. T.
Zampa, G.
Zampa, N.
Zverev, V. G.
Papini, P.
Adriani, O.
Barbarino, G. C.
Bazilevskaya, G. A.
Bellotti, R.
Boezio, M.
Bogomolov, E. A.
Bonechi, L.
Bongi, M.
Bonvicini, V.
Borisov, S.
Bottai, S.
Bruno, A.
Cafagna, F.
Campana, D.
Carbone, R.
Carlson, Per
Casolino, M.
Castellini, G.
De Pascale, M. P.
De Simone, N.
Di Felice, V.
Galper, A. M.
Gillard, William
Grishantseva, L.
Hofverberg, Petter
Jerse, G.
Koldashov, S. V.
Krutkov, S. Y.
Kvashnin, A. N.
Leonov, A.
Malvezzi, V.
Marcelli, L.
Menn, W.
Mikhailov, V. V.
Mocchiutti, E.
Mori, N.
Nikonov, N.
Osteria, G.
Pearce, Mark
Picozza, P.
Pizzolotto, C.
Ricci, M.
Ricciarini, S. B.
Ritabrata, S.
Rossetto, Laura
Simon, M.
Sparvoli, R.
Spillantini, P.
Stozhkov, Y. I.
Vacchi, A.
Vannuccini, E.
Vasilyev, G.
Voronov, S. A.
Wu, Juan
Yurkin, Y. T.
Zampa, G.
Zampa, N.
Zverev, V. G.
Publication Year :
2009

Abstract

The PAMELA experiment is a satellite-borne apparatus designed to study charged particles in the cosmic radiation, with a particular focus on antiparticles. The detector is housed on the Resurs-DK1 satellite and it is taking data since June 2006. The main parts of the apparatus are a magnetic spectrometer, which is equipped with a silicon-microstrip tracking system and which is used to measure the rigidity and the charge of particles, and a silicon/tungsten electromagnetic calorimeter which provides particle identification. The main results about the antiparticles component of cosmic rays obtained during the first 500 days of data taking are summarized here.<br />QC 20110301 Galileo-Galilei-Institute Conference on Dark Matter and Dark Energy, Florence, ITALY, JAN 19-MAR 12, 2009

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1234547612
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1016.j.nuclphysbps.2009.07.011