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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 02796naa a2200517 4500 | |
| 001 | oai:DiVA.org:kth-23896 | |
| 003 | SwePub | |
| 008 | 100810s2004 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-238962 URI |
| 024 | 7 | a https://doi.org/10.1016/j.nuclphysbps.2004.08.0062 DOI |
| 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 space experiment PAMELA |
| 264 | 1 | b Elsevier BV,c 2004 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20100525 QC 20110923 QC20150708 | |
| 520 | a We present in this paper a status report of the space experiment PAMELA. PAMELA is a satellite-borne experiment which primarily aims to measure the antiproton and positron spectra in the cosmic radiation over a large energy range (from 80 MeV up to 190 GeV for antiprotons and from 50 MeV up to 270 GeV for positrons) and to search for antinuclei with a sensitivity of the order of 10(-8) in the antihelium/ helium ratio. In addition, it will measure the light nucleax component of cosmic rays and investigate phenomena connected with Solar and Earth physics. The apparatus will be installed onboard the polar orbiting Resurs DK1 satellite, which will be launched into space by a Soyuz TM2 rocket in 2004 from Baikonur cosmodrome in Kazakhstan, for a 3 year long mission. PAMELA consists of: a time of flight system, a transition radiation detector, a magnetic spectrometer, an anticoincidence detector, an electromagnetic imaging calorimeter, a shower tail catcher scintillator and a neutron detector. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a cosmic-ray electrons | |
| 653 | a solar minimum activity | |
| 653 | a magnetic spectrometer | |
| 653 | a imaging calorimeter | |
| 653 | a antiproton spectrum | |
| 653 | a positrons | |
| 653 | a flux | |
| 653 | a radiation | |
| 653 | a ratio | |
| 653 | a orbit | |
| 700 | 1 | a Bonvicini, V.4 aut |
| 700 | 1 | a Mocchiutti, E.4 aut |
| 700 | 1 | a Schiavon, P.4 aut |
| 700 | 1 | a Vacchi, A.4 aut |
| 700 | 1 | a Carlson, Peru KTH,Fysik4 aut0 (Swepub:kth)u1ua4u32 |
| 700 | 1 | a Lund, Jensu KTH,Fysik4 aut0 (Swepub:kth)u1xt8kw1 |
| 700 | 1 | a Lundquist, Johanu KTH,Fysik4 aut0 (Swepub:kth)u1kmhoav |
| 700 | 1 | a Pearce, Marku KTH,Fysik4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a al, et4 aut |
| 710 | 2 | a KTHb Fysik4 org |
| 773 | 0 | t Nuclear Physics B - Proceedings Supplementsd : Elsevier BVg , s. 39-46q <39-46 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-23896 |
| 856 | 4 8 | u https://doi.org/10.1016/j.nuclphysbps.2004.08.006 |
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