Sökning: WFRF:(Carbone F.) > North-south asymmet...
Fältnamn | Indikatorer | Metadata |
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000 | 04141naa a2201009 4500 | |
001 | oai:DiVA.org:kth-131731 | |
003 | SwePub | |
008 | 131017s2013 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1317312 URI |
024 | 7 | a https://doi.org/10.1134/S10637761131001292 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 Karelin, A. V.4 aut |
245 | 1 0 | a North-south asymmetry for high-energy cosmic-ray electrons measured with the PAMELA experiment |
264 | 1 | c 2013 |
338 | a print2 rdacarrier | |
500 | a QC 20131017 | |
520 | a The north-south asymmetry for cosmic-ray particles was measured with one instrument of the PAMELA satellite-borne experiment in the period June 2006-May 2009. The analysis has been performed by two independent methods: by comparing the count rates in regions with identical geomagnetic conditions and by comparing the experimental distribution of particle directions with the simulated distribution that would be in the case of an isotropic particle flux. The dependences of the asymmetry on energy release in the PAMELA calorimeter and on time have been constructed. The asymmetry (N (n) - N (s) )/(N (n) + N (s) ) is 0.06 +/- 0.004 at the threshold energy release in the calorimeter and gradually decreases with increasing energy release. The observed effect is shown to be produced by electrons in the energy range 10-100 GeV. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
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 Bottai, S.4 aut |
700 | 1 | a Bruno, A.4 aut |
700 | 1 | a Vacchi, A.4 aut |
700 | 1 | a Vannuccini, E.4 aut |
700 | 1 | a Vasilyev, G. I.4 aut |
700 | 1 | a Voronov, S. A.4 aut |
700 | 1 | a Galper, A. M.4 aut |
700 | 1 | a Danilchenko, I. A.4 aut |
700 | 1 | a De Donato, C.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 Zverev, V. G.4 aut |
700 | 1 | a Zampa, G.4 aut |
700 | 1 | a Zampa, N.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 Kvashnin, A. N.4 aut |
700 | 1 | a Koldashov, S. V.4 aut |
700 | 1 | a Koldobskiy, S. A.4 aut |
700 | 1 | a Krutkov, S. Y.4 aut |
700 | 1 | a Leonov, A. A.4 aut |
700 | 1 | a Malvezzi, V.4 aut |
700 | 1 | a Marcelli, L.4 aut |
700 | 1 | a Martucci, M.4 aut |
700 | 1 | a Mayorov, A. G.4 aut |
700 | 1 | a Malakhov, V. V.4 aut |
700 | 1 | a Menn, W.4 aut |
700 | 1 | a Merge, M.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 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 Runtso, M. F.4 aut |
700 | 1 | a Sarkar, R.4 aut |
700 | 1 | a Simon, M.4 aut |
700 | 1 | a Sparvoli, R.4 aut |
700 | 1 | a Spillantini, P.4 aut |
700 | 1 | a Yurkin, Y. T.4 aut |
710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
773 | 0 | t Journal of Experimental and Theoretical Physicsg 117:2, s. 268-273q 117:2<268-273x 1063-7761x 1090-6509 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-131731 |
856 | 4 8 | u https://doi.org/10.1134/S1063776113100129 |
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