Results from PAMELA

E. Mocchiutti; O. Adriani; G. C. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. Boezio; E. A. Bogomolov; L. Bonechi; M. Bongi; V. Bonvicini; S. Borisov; S. Bottai; A. Bruno; F. Cafagna; D. Campana; R. Carbone; P. Carlson; M. Casolino; G. Castellini; L. Consiglio; M. P. De Pascale; C. De Santis; N. De Simone; V. Di Felice; A. M. Galper; W. Gillard; L. Grishantseva; G. Jerse; A. V. Karelin; S. V. Koldashov; S. Y. Krutkov; A. N. Kvashnin; A. Leonov; O. Maksumov; V. Malakhov; V. Malvezzi; L. Marcelli; A. G. Mayorov; W. Menn; A. Monaco; V. V. Mikhailov; N. Mori; N. N. Nikonov; G. Osteria; F. Palma; P. Papini; M. Pearce; P. Picozza; C. Pizzolotto; M. Ricci; S. B. Ricciarini; L. Rossetto; M. Runtso; R. Sarkar; M. Simon; R. Sparvoli; P. Spillantini; Y. I. Stozhkov; A. Vacchi; E. Vannuccini; G. Vasilyev; S. A. Voronov; J. Wu; Y. T. Yurkin; G. Zampa; N. Zampa; V. G. Zverev

doi:10.1016/j.nuclphysbps.2011.04.111

Results from PAMELA

E. Mocchiutti, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, L. ConsiglioM. P. De Pascale, C. De Santis, N. De Simone, V. Di Felice, A. M. Galper, W. Gillard, L. Grishantseva, G. Jerse, A. V. Karelin, S. V. Koldashov, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, O. Maksumov, V. Malakhov, V. Malvezzi, L. Marcelli, A. G. Mayorov, W. Menn, A. Monaco, V. V. Mikhailov, N. Mori, N. N. Nikonov, G. Osteria, F. Palma, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, M. Runtso, R. Sarkar, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, J. Wu, Y. T. Yurkin, G. Zampa, N. Zampa, V. G. Zverev

Research output: Contribution to journal › Article › peer-review

2 Scopus citations

Abstract

The PAMELA satellite experiment was launched into low earth orbit on June 15^th 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - several hundred GeV). A primary scientific goal is to search for dark matter particle annihilation by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment are presented with a particular focus on cosmic ray antiprotons and positrons.

Original language	English
Pages (from-to)	243-248
Number of pages	6
Journal	Nuclear Physics B - Proceedings Supplements
Volume	217
Issue number	1
DOIs	https://doi.org/10.1016/j.nuclphysbps.2011.04.111
State	Published - Aug 2011
Externally published	Yes

Bibliographical note

Funding Information:
We would like to acknowledge contributions and support from: Italian Space Agency (ASI), Deutsches Zentrum für Luft– und Raumfahrt (DLR), The Swedish National Space Board, Swedish Research Council, Russian Space Agency (Roskosmos, RKA). R. S. wishes to thank the TRIL program of the International Center of Theoretical Physics, Trieste, Italy that partly sponsored his activity.

Access to Document

10.1016/j.nuclphysbps.2011.04.111

Cite this

Mocchiutti, E., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., ... Zverev, V. G. (2011). Results from PAMELA. Nuclear Physics B - Proceedings Supplements, 217(1), 243-248. https://doi.org/10.1016/j.nuclphysbps.2011.04.111

@article{7aaa7da66c5c412aa4fa07116941bbe3,

title = "Results from PAMELA",

abstract = "The PAMELA satellite experiment was launched into low earth orbit on June 15th 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - several hundred GeV). A primary scientific goal is to search for dark matter particle annihilation by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment are presented with a particular focus on cosmic ray antiprotons and positrons.",

author = "E. Mocchiutti and O. Adriani and Barbarino, {G. C.} and Bazilevskaya, {G. A.} and R. Bellotti and M. Boezio and Bogomolov, {E. A.} and L. Bonechi and M. Bongi and V. Bonvicini and S. Borisov and S. Bottai and A. Bruno and F. Cafagna and D. Campana and R. Carbone and P. Carlson and M. Casolino and G. Castellini and L. Consiglio and {De Pascale}, {M. P.} and {De Santis}, C. and {De Simone}, N. and {Di Felice}, V. and Galper, {A. M.} and W. Gillard and L. Grishantseva and G. Jerse and Karelin, {A. V.} and Koldashov, {S. V.} and Krutkov, {S. Y.} and Kvashnin, {A. N.} and A. Leonov and O. Maksumov and V. Malakhov and V. Malvezzi and L. Marcelli and Mayorov, {A. G.} and W. Menn and A. Monaco and Mikhailov, {V. V.} and N. Mori and Nikonov, {N. N.} and G. Osteria and F. Palma and P. Papini and M. Pearce and P. Picozza and C. Pizzolotto and M. Ricci and Ricciarini, {S. B.} and L. Rossetto and M. Runtso and R. Sarkar and M. Simon and R. Sparvoli and P. Spillantini and Stozhkov, {Y. I.} and A. Vacchi and E. Vannuccini and G. Vasilyev and Voronov, {S. A.} and J. Wu and Yurkin, {Y. T.} and G. Zampa and N. Zampa and Zverev, {V. G.}",

note = "Funding Information: We would like to acknowledge contributions and support from: Italian Space Agency (ASI), Deutsches Zentrum f{\"u}r Luft– und Raumfahrt (DLR), The Swedish National Space Board, Swedish Research Council, Russian Space Agency (Roskosmos, RKA). R. S. wishes to thank the TRIL program of the International Center of Theoretical Physics, Trieste, Italy that partly sponsored his activity.",

year = "2011",

month = aug,

doi = "10.1016/j.nuclphysbps.2011.04.111",

language = "אנגלית",

volume = "217",

pages = "243--248",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier B.V.",

number = "1",

}

Mocchiutti, E, Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Consiglio, L, De Pascale, MP, De Santis, C, De Simone, N, Di Felice, V, Galper, AM, Gillard, W, Grishantseva, L, Jerse, G, Karelin, AV, Koldashov, SV, Krutkov, SY, Kvashnin, AN, Leonov, A, Maksumov, O, Malakhov, V, Malvezzi, V, Marcelli, L, Mayorov, AG, Menn, W, Monaco, A, Mikhailov, VV, Mori, N, Nikonov, NN, Osteria, G, Palma, F, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, SB, Rossetto, L, Runtso, M, Sarkar, R, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, YI, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, SA, Wu, J, Yurkin, YT, Zampa, G, Zampa, N & Zverev, VG 2011, 'Results from PAMELA', Nuclear Physics B - Proceedings Supplements, vol. 217, no. 1, pp. 243-248. https://doi.org/10.1016/j.nuclphysbps.2011.04.111

TY - JOUR

T1 - Results from PAMELA

AU - Mocchiutti, E.

AU - Adriani, O.

AU - Barbarino, G. C.

AU - Bazilevskaya, G. A.

AU - Bellotti, R.

AU - Boezio, M.

AU - Bogomolov, E. A.

AU - Bonechi, L.

AU - Bongi, M.

AU - Bonvicini, V.

AU - Borisov, S.

AU - Bottai, S.

AU - Bruno, A.

AU - Cafagna, F.

AU - Campana, D.

AU - Carbone, R.

AU - Carlson, P.

AU - Casolino, M.

AU - Castellini, G.

AU - Consiglio, L.

AU - De Pascale, M. P.

AU - De Santis, C.

AU - De Simone, N.

AU - Di Felice, V.

AU - Galper, A. M.

AU - Gillard, W.

AU - Grishantseva, L.

AU - Jerse, G.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Krutkov, S. Y.

AU - Kvashnin, A. N.

AU - Leonov, A.

AU - Maksumov, O.

AU - Malakhov, V.

AU - Malvezzi, V.

AU - Marcelli, L.

AU - Mayorov, A. G.

AU - Menn, W.

AU - Monaco, A.

AU - Mikhailov, V. V.

AU - Mori, N.

AU - Nikonov, N. N.

AU - Osteria, G.

AU - Palma, F.

AU - Papini, P.

AU - Pearce, M.

AU - Picozza, P.

AU - Pizzolotto, C.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Rossetto, L.

AU - Runtso, M.

AU - Sarkar, R.

AU - Simon, M.

AU - Sparvoli, R.

AU - Spillantini, P.

AU - Stozhkov, Y. I.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasilyev, G.

AU - Voronov, S. A.

AU - Wu, J.

AU - Yurkin, Y. T.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

N1 - Funding Information: We would like to acknowledge contributions and support from: Italian Space Agency (ASI), Deutsches Zentrum für Luft– und Raumfahrt (DLR), The Swedish National Space Board, Swedish Research Council, Russian Space Agency (Roskosmos, RKA). R. S. wishes to thank the TRIL program of the International Center of Theoretical Physics, Trieste, Italy that partly sponsored his activity.

PY - 2011/8

Y1 - 2011/8

N2 - The PAMELA satellite experiment was launched into low earth orbit on June 15th 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - several hundred GeV). A primary scientific goal is to search for dark matter particle annihilation by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment are presented with a particular focus on cosmic ray antiprotons and positrons.

AB - The PAMELA satellite experiment was launched into low earth orbit on June 15th 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - several hundred GeV). A primary scientific goal is to search for dark matter particle annihilation by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment are presented with a particular focus on cosmic ray antiprotons and positrons.

UR - http://www.scopus.com/inward/record.url?scp=80051626170&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2011.04.111

DO - 10.1016/j.nuclphysbps.2011.04.111

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:80051626170

SN - 0920-5632

VL - 217

SP - 243

EP - 248

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - 1

ER -

Results from PAMELA

Abstract

Bibliographical note

Access to Document

Other files and links

Fingerprint

Cite this