Sökning: WFRF:(Bongiorno G) > The first year in o...
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000 | 04410naa a2201117 4500 | |
001 | oai:DiVA.org:kth-164373 | |
003 | SwePub | |
008 | 150416s2007 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1643732 URI |
040 | a (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a kon2 swepub-publicationtype |
100 | 1 | a Boezio, M.4 aut |
245 | 1 0 | a The first year in orbit of the pamela experiment |
264 | 1 | b Universidad Nacional Autonoma de Mexico,c 2007 |
338 | a print2 rdacarrier | |
500 | a QC 20150416 | |
520 | a On the 15th of June 2006, the PAMELA experiment mounted on the Resurs DK1 satellite, was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. PAMELA is a satellite-borne apparatus designed to study charged particles in the cosmic radiation, to investigate the nature of dark matter, measuring the cosmic-ray antiproton and positron spectra over the largest energy range ever achieved, and to search for antinuclei with unprecedented sensitivity. The PAMELA apparatus comprises a time-of-flight system, a magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. We will present the status of the apparatus after one year in orbit. Furthermore, we will discuss the PAMELA in-flight performances. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a Experiments | |
653 | a High energy physics | |
653 | a Anticoincidence systems | |
653 | a Dark matter | |
653 | a Electromagnetic calorimeter | |
653 | a Energy ranges | |
653 | a First year | |
653 | a In-flight performance | |
653 | a Magnetic spectrometers | |
653 | a Time-of-flight system | |
700 | 1 | a Adriani, O.4 aut |
700 | 1 | a Ambriola, M.4 aut |
700 | 1 | a Barbarino, G. C.4 aut |
700 | 1 | a Basili, A.4 aut |
700 | 1 | a Bazilevskaja, G. A.4 aut |
700 | 1 | a Bellotti, R.4 aut |
700 | 1 | a Bogomolov, E. A.4 aut |
700 | 1 | a Bonechi, L.4 aut |
700 | 1 | a Bongi, M.4 aut |
700 | 1 | a Bongiorno, L.4 aut |
700 | 1 | a Bonvicini, V.4 aut |
700 | 1 | a Bruno, A.4 aut |
700 | 1 | a Cafagna, F.4 aut |
700 | 1 | a Campana, D.4 aut |
700 | 1 | a Carlson, Peru KTH,Fysik4 aut0 (Swepub:kth)u1ua4u32 |
700 | 1 | a Casolino, M.4 aut |
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700 | 1 | a Di Felice, V.4 aut |
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700 | 1 | a Hofverberg, Petteru KTH,Fysik4 aut0 (Swepub:kth)u1i33ozx |
700 | 1 | a Koldashov, S. V.4 aut |
700 | 1 | a Krutkov, S. Y.4 aut |
700 | 1 | a Kvashnin, A. N.4 aut |
700 | 1 | a Lundquist, J.4 aut |
700 | 1 | a Maksumov, O.4 aut |
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700 | 1 | a Mocchiutti, E.4 aut |
700 | 1 | a Morselli, A.4 aut |
700 | 1 | a Nikonov, N. N.4 aut |
700 | 1 | a Orsi, S.4 aut |
700 | 1 | a Osteria, G.4 aut |
700 | 1 | a Papini, P.4 aut |
700 | 1 | a Pearce, Mark,d 1970-u KTH,Fysik4 aut0 (Swepub:kth)u17jptna |
700 | 1 | a Picozza, P.4 aut |
700 | 1 | a Ricci, M.4 aut |
700 | 1 | a Ricciarini, S. B.4 aut |
700 | 1 | a Runtso, M. F.4 aut |
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700 | 1 | a Zampa, G.4 aut |
700 | 1 | a Zampa, N.4 aut |
700 | 1 | a Zverev, V. G.4 aut |
710 | 2 | a KTHb Fysik4 org |
773 | 0 | t Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007d : Universidad Nacional Autonoma de Mexicog , s. 99-102q <99-102 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-164373 |
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