Sökning: WFRF:(Bogomolov S. L.) > (2010-2014) > PAMELA Measurements...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 04958naa a2201177 4500 | |
001 | oai:DiVA.org:kth-32598 | |
003 | SwePub | |
008 | 110418s2011 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-325982 URI |
024 | 7 | a https://doi.org/10.1126/science.11991722 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 Adriani, O.4 aut |
245 | 1 0 | a PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra |
264 | 1 | b American Association for the Advancement of Science (AAAS),c 2011 |
338 | a print2 rdacarrier | |
500 | a QC 20110420 | |
520 | a Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the acceleration and subsequent propagation of cosmic rays in our Galaxy. We report precision measurements of the proton and helium spectra in the rigidity range 1 gigavolt to 1.2 teravolts performed by the satellite-borne experiment PAMELA (payload for antimatter matter exploration and light-nuclei astrophysics). We find that the spectral shapes of these two species are different and cannot be described well by a single power law. These data challenge the current paradigm of cosmic-ray acceleration in supernova remnants followed by diffusive propagation in the Galaxy. More complex processes of acceleration and propagation of cosmic rays are required to explain the spectral structures observed in our data. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a SOLAR MODULATION | |
653 | a ACCELERATION | |
653 | a PROPAGATION | |
653 | a GALAXY | |
653 | a MATTER | |
653 | a WAVES | |
653 | a BESS | |
653 | a Astronomy and astrophysics | |
653 | a Astronomi och astrofysik | |
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,Partikel- och astropartikelfysik4 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 Menn, W.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 Rossetto, Laurau KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1tv6cqb |
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 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 Yurkin, Y. T.4 aut |
700 | 1 | a Wu, Juanu KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1y0e14w |
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 Scienced : American Association for the Advancement of Science (AAAS)g 332:6025, s. 69-72q 332:6025<69-72x 0036-8075x 1095-9203 |
856 | 4 | u https://art.torvergata.it/bitstream/2108/55474/2/science.1199172.full.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-32598 |
856 | 4 8 | u https://doi.org/10.1126/science.1199172 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
Kopiera och spara länken för att återkomma till aktuell vy