WFRF:(Bogomolov S. L.)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05007naa a2201129 4500 | |
| 001 | oai:DiVA.org:kth-118199 | |
| 003 | SwePub | |
| 008 | 130213s2013 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1181992 URI |
| 024 | 7 | a https://doi.org/10.1016/j.asr.2011.06.0302 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 Menn, W.4 aut |
| 245 | 1 0 | a The PAMELA space experiment |
| 264 | 1 | b Elsevier BV,c 2013 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20130215 | |
| 520 | a On the 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus is comprised of a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV to 100's GeV) with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectra in order to search for exotic sources, such as dark matter particle annihilations. PAMELA is also searching for primordial antinuclei (anti-helium), and testing cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and precision studies of light nuclei and their isotopes. Moreover, PAMELA is investigating phenomena connected with solar and earth physics. After 4 years of operation in flight, PAMELA is now delivering coherent results about spectra and chemical composition of the charged cosmic radiation, allowing scenarios of production and propagation of cosmic rays to be fully established and understood. | |
| 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-borne experiment | |
| 700 | 1 | a Adriani, O.4 aut |
| 700 | 1 | a Barbarino, G. C.4 aut |
| 700 | 1 | a Bazilevskaya, G. A.4 aut |
| 700 | 1 | a Bellotti, R.4 aut |
| 700 | 1 | a Boezio, M.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 Bonvicini, V.4 aut |
| 700 | 1 | a Borisov, S.4 aut |
| 700 | 1 | a Bottai, S.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 Carbone, R.4 aut |
| 700 | 1 | a Carlson, Peru KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1ua4u32 |
| 700 | 1 | a Casolino, M.4 aut |
| 700 | 1 | a Castellini, G.4 aut |
| 700 | 1 | a Consiglio, L.4 aut |
| 700 | 1 | a De Pascale, M. P.4 aut |
| 700 | 1 | a De Santis, C.4 aut |
| 700 | 1 | a De Simone, N.4 aut |
| 700 | 1 | a Di Felice, V.4 aut |
| 700 | 1 | a Galper, A. M.4 aut |
| 700 | 1 | a Gillard, Williamu KTH,Fysik4 aut0 (Swepub:kth)u171jmfw |
| 700 | 1 | a Grishantseva, L.4 aut |
| 700 | 1 | a Jerse, G.4 aut |
| 700 | 1 | a Karelin, A. V.4 aut |
| 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 Leonov, A.4 aut |
| 700 | 1 | a Malakhov, V.4 aut |
| 700 | 1 | a Malvezzi, V.4 aut |
| 700 | 1 | a Marcelli, L.4 aut |
| 700 | 1 | a Mayorov, A. G.4 aut |
| 700 | 1 | a Mikhailov, V. V.4 aut |
| 700 | 1 | a Mocchiutti, E.4 aut |
| 700 | 1 | a Monaco, A.4 aut |
| 700 | 1 | a Mori, N.4 aut |
| 700 | 1 | a Nikonov, N.4 aut |
| 700 | 1 | a Osteria, G.4 aut |
| 700 | 1 | a Palma, F.4 aut |
| 700 | 1 | a Papini, P.4 aut |
| 700 | 1 | a Pearce, Marku KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u17jptna |
| 700 | 1 | a Picozza, P.4 aut |
| 700 | 1 | a Pizzolotto, C.4 aut |
| 700 | 1 | a Ricci, M.4 aut |
| 700 | 1 | a Ricciarini, S. B.4 aut |
| 700 | 1 | a Sarkar, R.4 aut |
| 700 | 1 | a Rossetto, Laurau KTH,Fysik4 aut0 (Swepub:kth)u1tv6cqb |
| 700 | 1 | a Simon, M.4 aut |
| 700 | 1 | a Sparvoli, R.4 aut |
| 700 | 1 | a Spillantini, P.4 aut |
| 700 | 1 | a Stochaj, S. J.4 aut |
| 700 | 1 | a Stockton, J. C.4 aut |
| 700 | 1 | a Stozhkov, Y. I.4 aut |
| 700 | 1 | a Vacchi, A.4 aut |
| 700 | 1 | a Vannuccini, E.4 aut |
| 700 | 1 | a Vasilyev, G.4 aut |
| 700 | 1 | a Voronov, S. A.4 aut |
| 700 | 1 | a Wu, Juanu KTH,Fysik4 aut0 (Swepub:kth)u1y0e14w |
| 700 | 1 | a Yurkin, Y. T.4 aut |
| 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 Partikel- och astropartikelfysik4 org |
| 773 | 0 | t Advances in Space Researchd : Elsevier BVg 51:2, s. 209-218q 51:2<209-218x 0273-1177x 1879-1948 |
| 856 | 4 | u http://arxiv.org/pdf/0905.2551 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-118199 |
| 856 | 4 8 | u https://doi.org/10.1016/j.asr.2011.06.030 |
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- Consiglio, L.
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- Di Felice, V.
- Galper, A. M.
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- Karelin, A. V.
- Koldashov, S. V.
- Krutkov, S. Y.
- Kvashnin, A. N.
- Leonov, A.
- Malakhov, V.
- Malvezzi, V.
- Marcelli, L.
- Mayorov, A. G.
- Mikhailov, V. V.
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- Vacchi, A.
- Vannuccini, E.
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