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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 04754naa a2201141 4500 | |
| 001 | oai:DiVA.org:kth-43742 | |
| 003 | SwePub | |
| 008 | 111018s2004 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-437422 URI |
| 024 | 7 | a https://doi.org/10.1109/TNS.2004.8295042 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 Bongi, M4 aut |
| 245 | 1 0 | a PAMELA :b A satellite experiment for antiparticles measurement in cosmic rays |
| 264 | 1 | c 2004 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20111020 | |
| 520 | a PAMELA is a satellite-borne experiment that will study the antiproton and positron fluxes in cosmic rays in a wide range of energy (from 80 MeV up to 190 GeV for antiprotons and from 50 MeV up to 270 GeV for positrons) and with high statistics, and that will measure the antihelium/helium ratio with a sensitivity of the order of 10(-8). The detector will fly on-board a polar orbiting Resurs DK1 satellite, which will be launched into space by a Soyuz rocket in 2004 from Baikonur cosmodrome in Kazakhstan, for a 3-year-long mission. Particle identification and energy measurements are performed in the PAMELA apparatus using the following subdetectors: a magnetic spectrometer made up of a permanent magnet equipped with double-sided microstrip silicon detectors, an electromagnetic imaging calorimeter composed of layers of tungsten absorber and silicon detectors planes, a transition radiation detector made of straw tubes interleaved with carbon fiber radiators, a plastic scintillator time-of-flight and trigger system, a set of anticounter plastic scintillator detectors, and a neutron detector. The features of the detectors and the main results obtained in beam test sessions are presented. | |
| 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 satellite experiment | |
| 700 | 1 | a Adriani, O4 aut |
| 700 | 1 | a Ambriola, A4 aut |
| 700 | 1 | a Bakaldin, A4 aut |
| 700 | 1 | a Barbarino, G C4 aut |
| 700 | 1 | a Basili, A4 aut |
| 700 | 1 | a Bazilevskaja, G4 aut |
| 700 | 1 | a Bellotti, R4 aut |
| 700 | 1 | a Bencardino, R4 aut |
| 700 | 1 | a Boezio, M4 aut |
| 700 | 1 | a Bogomolov, E A4 aut |
| 700 | 1 | a Bonechi, L4 aut |
| 700 | 1 | a Bongiorno, L4 aut |
| 700 | 1 | a Bonvicini, V4 aut |
| 700 | 1 | a Boscherini, M4 aut |
| 700 | 1 | a Cafagna, F S4 aut |
| 700 | 1 | a Campana, D4 aut |
| 700 | 1 | a Carlson, Peru KTH,Fysik4 aut0 (Swepub:kth)u1ua4u32 |
| 700 | 1 | a Casolino, M4 aut |
| 700 | 1 | a Castellini, G4 aut |
| 700 | 1 | a Circella, M4 aut |
| 700 | 1 | a De Marzo, C N4 aut |
| 700 | 1 | a De Pascale, M P4 aut |
| 700 | 1 | a Furano, G4 aut |
| 700 | 1 | a Galper, A M4 aut |
| 700 | 1 | a Giglietto, N4 aut |
| 700 | 1 | a Grigorjeva, A4 aut |
| 700 | 1 | a Koldashov, S V4 aut |
| 700 | 1 | a Korotkov, M G4 aut |
| 700 | 1 | a Krut'kov, S Y4 aut |
| 700 | 1 | a Lund, Jensu KTH,Fysik4 aut0 (Swepub:kth)u1xt8kw1 |
| 700 | 1 | a Lundquist, J4 aut |
| 700 | 1 | a Menicucci, A4 aut |
| 700 | 1 | a Menn, W4 aut |
| 700 | 1 | a Mikhailov, V V4 aut |
| 700 | 1 | a Minori, M4 aut |
| 700 | 1 | a Mirizzi, N4 aut |
| 700 | 1 | a Mitchell, J W4 aut |
| 700 | 1 | a Mocchiutti, E4 aut |
| 700 | 1 | a Morselli, A4 aut |
| 700 | 1 | a Mukhametshin, R4 aut |
| 700 | 1 | a Orsi, Silviou KTH,Fysik4 aut0 (Swepub:kth)u1mukymv |
| 700 | 1 | a Osteria, G4 aut |
| 700 | 1 | a Papini, P4 aut |
| 700 | 1 | a Pearce, Marku KTH,Fysik4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a Picozza, P4 aut |
| 700 | 1 | a Ricci, M4 aut |
| 700 | 1 | a Ricciarini, S B4 aut |
| 700 | 1 | a Romita, M4 aut |
| 700 | 1 | a Rossi, G4 aut |
| 700 | 1 | a Russo, S4 aut |
| 700 | 1 | a Schiavon, P4 aut |
| 700 | 1 | a Simon, M4 aut |
| 700 | 1 | a Sparvoli, R4 aut |
| 700 | 1 | a Spillantini, P4 aut |
| 700 | 1 | a Spinelli, P4 aut |
| 700 | 1 | a Stochaj, S J4 aut |
| 700 | 1 | a Stozhkov, Y4 aut |
| 700 | 1 | a Straulino, S4 aut |
| 700 | 1 | a Streitmatter, R E4 aut |
| 700 | 1 | a Taccetti, F4 aut |
| 700 | 1 | a Vacchi, A4 aut |
| 700 | 1 | a Vannuccini, E4 aut |
| 700 | 1 | a Vasilyev, G I4 aut |
| 700 | 1 | a Voronov, S A4 aut |
| 700 | 1 | a Wischnewski, R4 aut |
| 700 | 1 | a Yurkin, Y4 aut |
| 700 | 1 | a Zampa, G4 aut |
| 700 | 1 | a Zampa, N4 aut |
| 710 | 2 | a KTHb Fysik4 org |
| 773 | 0 | t IEEE Transactions on Nuclear Scienceg 51:3, s. 854-859q 51:3<854-859x 0018-9499x 1558-1578 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-43742 |
| 856 | 4 8 | u https://doi.org/10.1109/TNS.2004.829504 |
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- Bellotti, R
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- Boezio, M
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- Boscherini, M
- Cafagna, F S
- Campana, D
- Carlson, Per
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- De Marzo, C N
- De Pascale, M P
- Furano, G
- Galper, A M
- Giglietto, N
- Grigorjeva, A
- Koldashov, S V
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- Lund, Jens
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- Menicucci, A
- Menn, W
- Mikhailov, V V
- Minori, M
- Mirizzi, N
- Mitchell, J W
- Mocchiutti, E
- Morselli, A
- Mukhametshin, R
- Orsi, Silvio
- Osteria, G
- Papini, P
- Pearce, Mark
- Picozza, P
- Ricci, M
- Ricciarini, S B
- Romita, M
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- Russo, S
- Schiavon, P
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- Sparvoli, R
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- Vacchi, A
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