Trapped protons in SAA measured by the PAMELA experiment

A. Bruno; F. Cafagna; O. Adriani; G. C. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. Boezio; E. A. Bogomolov; M. Bongi; V. Bonvicini; S. Borisov; S. Bottai; 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; M. D. Kheymits; S. V. Koldashov; S. Y. Krutkov; A. N. Kvashnin; A. Leonov; V. Malakhov; L. Marcelli; A. G. Mayorov; W. Menn; V. V. Mikhailov; E. Mocchiutti; A. Monaco; N. Mori; N. Nikonov; G. Osteria; F. Palma; P. Papini; M. Pearce; P. Picozza; C. Pizzolotto; M. Ricci; S. B. Ricciarini; L. Rossetto; R. Sarkar; 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:10.7529/ICRC2011/V06/0963

Trapped protons in SAA measured by the PAMELA experiment

A. Bruno, F. Cafagna, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, L. Consiglio, M. P. De Pascale, C. De SantisN. De Simone, V. Di Felice, A. M. Galper, W. Gillard, L. Grishantseva, G. Jerse, A. V. Karelin, M. D. Kheymits, S. V. Koldashov, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, A. G. Mayorov, W. Menn, V. V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, N. Nikonov, G. Osteria, F. Palma, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, R. Sarkar, 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 conference › Paper › peer-review

1 Scopus citations

Abstract

An accurate measurement of under cutoff proton fluxes in the energy range 60 MeV ÷ 3 GeV has been performed by the PAMELA satellite-borne experiment. Thanks to the high identification performances and to the semipolar and elliptic satellite orbit, PAMELA is able to provide information about spectra and composition of particles in different regions of the magnetosphere. Here we present the measurement of the geomagnetically trapped protons from the inner radiation belt (SAA). The fluxes as a function of equatorial pitch angle and McIlwain L-shell are reported.

Original language	English
Pages	82-85
Number of pages	4
DOIs	https://doi.org/10.7529/ICRC2011/V06/0963
State	Published - 2011
Externally published	Yes
Event	32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China Duration: 11 Aug 2011 → 18 Aug 2011

Conference

Conference	32nd International Cosmic Ray Conference, ICRC 2011
Country/Territory	China
City	Beijing
Period	11/08/11 → 18/08/11

Keywords

Cosmic rays
Magnetosphere
Radiation belt
Saa
Trapped protons

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10.7529/ICRC2011/V06/0963

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Bruno, A., Cafagna, F., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Consiglio, L., De Pascale, M. P., ... Zverev, V. G. (2011). Trapped protons in SAA measured by the PAMELA experiment. 82-85. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China. https://doi.org/10.7529/ICRC2011/V06/0963

@conference{f1c0faf7d4824d3db758d591f94499da,

title = "Trapped protons in SAA measured by the PAMELA experiment",

abstract = "An accurate measurement of under cutoff proton fluxes in the energy range 60 MeV ÷ 3 GeV has been performed by the PAMELA satellite-borne experiment. Thanks to the high identification performances and to the semipolar and elliptic satellite orbit, PAMELA is able to provide information about spectra and composition of particles in different regions of the magnetosphere. Here we present the measurement of the geomagnetically trapped protons from the inner radiation belt (SAA). The fluxes as a function of equatorial pitch angle and McIlwain L-shell are reported.",

keywords = "Cosmic rays, Magnetosphere, Radiation belt, Saa, Trapped protons",

author = "A. Bruno and F. Cafagna 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 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 Kheymits, {M. D.} and Koldashov, {S. V.} and Krutkov, {S. Y.} and Kvashnin, {A. N.} and A. Leonov and V. Malakhov and L. Marcelli 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 P. Picozza and C. Pizzolotto and M. Ricci and Ricciarini, {S. B.} and L. Rossetto 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 Yurkin, {Y. T.} and J. Wu and G. Zampa and N. Zampa and Zverev, {V. G.}",

year = "2011",

doi = "10.7529/ICRC2011/V06/0963",

language = "אנגלית",

pages = "82--85",

note = "32nd International Cosmic Ray Conference, ICRC 2011 ; Conference date: 11-08-2011 Through 18-08-2011",

}

Bruno, A, Cafagna, F, Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, 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, Kheymits, MD, Koldashov, SV, Krutkov, SY, Kvashnin, AN, Leonov, A, Malakhov, V, Marcelli, L, Mayorov, AG, Menn, W, Mikhailov, VV, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, N, Osteria, G, Palma, F, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, SB, Rossetto, L, Sarkar, R, 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 2011, 'Trapped protons in SAA measured by the PAMELA experiment', Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China, 11/08/11 - 18/08/11 pp. 82-85. https://doi.org/10.7529/ICRC2011/V06/0963

TY - CONF

T1 - Trapped protons in SAA measured by the PAMELA experiment

AU - Bruno, A.

AU - Cafagna, F.

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 - 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 - Kheymits, M. D.

AU - Koldashov, S. V.

AU - Krutkov, S. Y.

AU - Kvashnin, A. N.

AU - Leonov, A.

AU - Malakhov, V.

AU - Marcelli, L.

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 - Picozza, P.

AU - Pizzolotto, C.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Rossetto, L.

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 - Yurkin, Y. T.

AU - Wu, J.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

PY - 2011

Y1 - 2011

N2 - An accurate measurement of under cutoff proton fluxes in the energy range 60 MeV ÷ 3 GeV has been performed by the PAMELA satellite-borne experiment. Thanks to the high identification performances and to the semipolar and elliptic satellite orbit, PAMELA is able to provide information about spectra and composition of particles in different regions of the magnetosphere. Here we present the measurement of the geomagnetically trapped protons from the inner radiation belt (SAA). The fluxes as a function of equatorial pitch angle and McIlwain L-shell are reported.

AB - An accurate measurement of under cutoff proton fluxes in the energy range 60 MeV ÷ 3 GeV has been performed by the PAMELA satellite-borne experiment. Thanks to the high identification performances and to the semipolar and elliptic satellite orbit, PAMELA is able to provide information about spectra and composition of particles in different regions of the magnetosphere. Here we present the measurement of the geomagnetically trapped protons from the inner radiation belt (SAA). The fluxes as a function of equatorial pitch angle and McIlwain L-shell are reported.

KW - Cosmic rays

KW - Magnetosphere

KW - Radiation belt

KW - Saa

KW - Trapped protons

UR - http://www.scopus.com/inward/record.url?scp=84899543007&partnerID=8YFLogxK

U2 - 10.7529/ICRC2011/V06/0963

DO - 10.7529/ICRC2011/V06/0963

M3 - ???researchoutput.researchoutputtypes.contributiontoconference.paper???

AN - SCOPUS:84899543007

SP - 82

EP - 85

T2 - 32nd International Cosmic Ray Conference, ICRC 2011

Y2 - 11 August 2011 through 18 August 2011

ER -

Trapped protons in SAA measured by the PAMELA experiment

Abstract

Conference

Keywords

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