Cosmic ray study with the PAMELA experiment

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

doi:10.1088/1742-6596/409/1/012003

Cosmic ray study with the PAMELA experiment

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

Research output: Contribution to journal › Conference article › peer-review

8 Scopus citations

Abstract

In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.

Original language	English
Article number	012003
Journal	Journal of Physics: Conference Series
Volume	409
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/409/1/012003
State	Published - 2013
Externally published	Yes
Event	23rd European Cosmic Ray Symposium, ECRS 2012 and 32nd Russian Cosmic Ray Conference - Moscow, Russian Federation Duration: 3 Jul 2012 → 7 Jul 2012

Access to Document

10.1088/1742-6596/409/1/012003

Cite this

Picozza, P., Marcelli, L., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., 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. (2013). Cosmic ray study with the PAMELA experiment. Journal of Physics: Conference Series, 409(1), Article 012003. https://doi.org/10.1088/1742-6596/409/1/012003

@article{40ba3c9f60d649aa84516f2a53511b7e,

title = "Cosmic ray study with the PAMELA experiment",

abstract = "In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.",

author = "P. Picozza and L. Marcelli and O. Adriani and Barbarino, {G. C.} and Bazilevskaya, {G. A.} and R. Bellotti and M. Boezio and Bogomolov, {E. A.} 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 {De Pascale}, {M. P.} and {De Santis}, C. and {De Simone}, N. and {Di Felice}, V. and Galper, {A. M.} and L. Grishantseva and G. Jerse and Karelin, {A. V.} and Kheymits, {M. D.} and Koldashov, {S. V.} and Krutkov, {S. Y.} and Kvashnin, {A. N.} and A. Leonov and V. Malakhov and Mayorov, {A. G.} and W. Menn and Mikhailov, {V. V.} and E. Mocchiutti and A. Monaco and N. Mori and N. Nikonov and G. Osteria and F. Palma and P. Papini and M. Pearce and C. Pizzolotto and M. Ricci and Ricciarini, {S. B.} and R. Sarkar and L. Rossetto 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 Yurkin, {Y. T.} and J. Wu and G. Zampa and N. Zampa and Zverev, {V. G.}",

year = "2013",

doi = "10.1088/1742-6596/409/1/012003",

language = "אנגלית",

volume = "409",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

number = "1",

note = "23rd European Cosmic Ray Symposium, ECRS 2012 and 32nd Russian Cosmic Ray Conference ; Conference date: 03-07-2012 Through 07-07-2012",

}

Picozza, P, Marcelli, L, Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Pascale, MP, De Santis, C, De Simone, N, Di Felice, V, Galper, AM, Grishantseva, L, Jerse, G, Karelin, AV, Kheymits, MD, Koldashov, SV, Krutkov, SY, Kvashnin, AN, Leonov, A, Malakhov, V, Mayorov, AG, Menn, W, Mikhailov, VV, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, N, Osteria, G, Palma, F, Papini, P, Pearce, M, Pizzolotto, C, Ricci, M, Ricciarini, SB, Sarkar, R, Rossetto, L, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, YI, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, SA, Yurkin, YT, Wu, J, Zampa, G, Zampa, N & Zverev, VG 2013, 'Cosmic ray study with the PAMELA experiment', Journal of Physics: Conference Series, vol. 409, no. 1, 012003. https://doi.org/10.1088/1742-6596/409/1/012003

TY - JOUR

T1 - Cosmic ray study with the PAMELA experiment

AU - Picozza, P.

AU - Marcelli, L.

AU - Adriani, O.

AU - Barbarino, G. C.

AU - Bazilevskaya, G. A.

AU - Bellotti, R.

AU - Boezio, M.

AU - Bogomolov, E. A.

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 - De Pascale, M. P.

AU - De Santis, C.

AU - De Simone, N.

AU - Di Felice, V.

AU - Galper, A. M.

AU - Grishantseva, L.

AU - Jerse, G.

AU - Karelin, A. V.

AU - Kheymits, M. D.

AU - Koldashov, S. V.

AU - Krutkov, S. Y.

AU - Kvashnin, A. N.

AU - Leonov, A.

AU - Malakhov, V.

AU - Mayorov, A. G.

AU - Menn, W.

AU - Mikhailov, V. V.

AU - Mocchiutti, E.

AU - Monaco, A.

AU - Mori, N.

AU - Nikonov, N.

AU - Osteria, G.

AU - Palma, F.

AU - Papini, P.

AU - Pearce, M.

AU - Pizzolotto, C.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Sarkar, R.

AU - Rossetto, L.

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 - Yurkin, Y. T.

AU - Wu, J.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

PY - 2013

Y1 - 2013

N2 - In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.

AB - In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.

UR - http://www.scopus.com/inward/record.url?scp=84874296905&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/409/1/012003

DO - 10.1088/1742-6596/409/1/012003

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.conferencearticle???

AN - SCOPUS:84874296905

SN - 1742-6588

VL - 409

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012003

T2 - 23rd European Cosmic Ray Symposium, ECRS 2012 and 32nd Russian Cosmic Ray Conference

Y2 - 3 July 2012 through 7 July 2012

ER -

Cosmic ray study with the PAMELA experiment

Abstract

Access to Document

Other files and links

Fingerprint

Cite this