Search: onr:"swepub:oai:DiVA.org:kth-153600" > Two years of flight...
Fältnamn | Indikatorer | Metadata |
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000 | 03916naa a2200973 4500 | |
001 | oai:DiVA.org:kth-153600 | |
003 | SwePub | |
008 | 141006s2009 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1536002 URI |
024 | 7 | a https://doi.org/10.1143/JPSJS.78SA.352 DOI |
040 | a (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Casolino, M.4 aut |
245 | 1 0 | a Two years of flight of the Pamela experiment :b Results and perspectives |
264 | 1 | c 2009 |
338 | a print2 rdacarrier | |
500 | a QC 20141007 | |
520 | a PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons: 80 MeV-700 GeV, electrons 50 MeV-400 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV-190 GeV), positrons (50 MeV-270 GeV) and search for antinuclei with a precision of the order of 10~8). The experiment, housed on board the Russian Resurs-DKl satellite, was launched on June, 15th 2006 in a 350 x 600 km orbit with an inclination of 70 degrees. In this work we describe the scientific objectives and the performance of PAMELA in its first two years of operation. Data on protons of trapped, secondary and galactic nature - as well as measurements of the December 13th 2006 Solar Particle Event - are also provided. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a Antimatter | |
653 | a Cosmic rays | |
653 | a Dark matter | |
653 | a Solar particle events | |
653 | a Trapped cosmic rays | |
700 | 1 | a De Simone, N.4 aut |
700 | 1 | a Bongue, D.4 aut |
700 | 1 | a De Pascale, M. P.4 aut |
700 | 1 | a Felice, V. D.4 aut |
700 | 1 | a Marcelli, L.4 aut |
700 | 1 | a Minori, M.4 aut |
700 | 1 | a Picozza, P.4 aut |
700 | 1 | a Sparvoli, R.4 aut |
700 | 1 | a Castellini, G.4 aut |
700 | 1 | a Adriani, O.4 aut |
700 | 1 | a Bonechi, L.4 aut |
700 | 1 | a Bongi, M.4 aut |
700 | 1 | a Bottai, S.4 aut |
700 | 1 | a Papini, P.4 aut |
700 | 1 | a Ricciarini, S.4 aut |
700 | 1 | a Spillantini, P.4 aut |
700 | 1 | a Taddei, E.4 aut |
700 | 1 | a Vannuccini, E.4 aut |
700 | 1 | a Barbarino, G.4 aut |
700 | 1 | a Campana, D.4 aut |
700 | 1 | a Carbone, R.4 aut |
700 | 1 | a De Rosa, G.4 aut |
700 | 1 | a Osteria, G.4 aut |
700 | 1 | a Boezio, M.4 aut |
700 | 1 | a Bonvicini, V.4 aut |
700 | 1 | a Mocchiutti, E.4 aut |
700 | 1 | a Vacchi, A.4 aut |
700 | 1 | a Zampa, G.4 aut |
700 | 1 | a Zampa, N.4 aut |
700 | 1 | a Bruno, A.4 aut |
700 | 1 | a Cafagna, F. S.4 aut |
700 | 1 | a Ricci, M.4 aut |
700 | 1 | a Hofverberg, Petteru KTH,Fysik4 aut0 (Swepub:kth)u1i33ozx |
700 | 1 | a Pearce, Marku KTH,Fysik4 aut0 (Swepub:kth)u17jptna |
700 | 1 | a Carlson, Peru KTH,Fysik4 aut0 (Swepub:kth)u1ua4u32 |
700 | 1 | a Bogomolov, E.4 aut |
700 | 1 | a Krutkov, S.Yu.4 aut |
700 | 1 | a Nikonov, N. N.4 aut |
700 | 1 | a Menn, W.4 aut |
700 | 1 | a Simon, M.4 aut |
700 | 1 | a Galper, A. M.4 aut |
700 | 1 | a Grishantseva, L.4 aut |
700 | 1 | a Koldashov, S.4 aut |
700 | 1 | a Leonov, A.4 aut |
700 | 1 | a Mikhailov, V. V.4 aut |
700 | 1 | a Voronov, S. A.4 aut |
700 | 1 | a Yurkin, Y. T.4 aut |
700 | 1 | a Zverev, V. G.4 aut |
700 | 1 | a Bazilevskaya, G. A.4 aut |
700 | 1 | a Kvashnin, A. N.4 aut |
700 | 1 | a Maksumov, O.4 aut |
700 | 1 | a Stozhkov, Y.4 aut |
710 | 2 | a KTHb Fysik4 org |
773 | 0 | t Journal of the Physical Society of Japang 78:Suppl. A, s. 35-40q 78:Suppl. A<35-40x 0031-9015x 1347-4073 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-153600 |
856 | 4 8 | u https://doi.org/10.1143/JPSJS.78SA.35 |
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