Primary electron and positron fluxes measured by the PAMELA experiment

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

doi:10.3103/S1062873811030300

Primary electron and positron fluxes measured by the PAMELA experiment

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

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Abstract

The PAMELA experiment is being conducted on board the RESURS DK1 satellite, launched into a near-Earth, near-polar orbit with an altitude of 350-610 km and an inclination of 70° on June 15, 2006. The apparatus comprises a magnetic spectrometer, an electromagnetic calorimeter (16X ₀), a time-of-flight system, a neutron detector, an anticoincidence system, and a shower tail scintillator. It allows measurements of electron and positron fluxes in cosmic rays over a wide energy range of ∼100 MeV to several hundreds of GeVs. In this work, we present data on the electron and positron energy spectra in primary cosmic rays, obtained between June 2006 and December 2008.

Original language	English
Pages (from-to)	316-318
Number of pages	3
Journal	Bulletin of the Russian Academy of Sciences: Physics
Volume	75
Issue number	3
DOIs	https://doi.org/10.3103/S1062873811030300
State	Published - Mar 2011
Externally published	Yes

Bibliographical note

Funding Information:
The authors are grateful to the RF Space Agency ROSKOSMOS, the Research Center for Earth Oper ative Monitoring, the Samara Space Center “TsSKB Progress,” the INFN, and the Russian Foundation for Basic Research (grant nos. 10 02 01301a and 09 02 00394a) for their support and assistance in performing the experiment.

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Mikhailov, V. V., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Belotti, R., Boezio, M., Bogomolov, E. A., Bonvicini, V., Bongi, M., Bonechi, L., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Crishantseva, L. A., ... Zverev, V. G. (2011). Primary electron and positron fluxes measured by the PAMELA experiment. Bulletin of the Russian Academy of Sciences: Physics, 75(3), 316-318. https://doi.org/10.3103/S1062873811030300

@article{981c66235980432eb0e4a938cb89e7ca,

title = "Primary electron and positron fluxes measured by the PAMELA experiment",

abstract = "The PAMELA experiment is being conducted on board the RESURS DK1 satellite, launched into a near-Earth, near-polar orbit with an altitude of 350-610 km and an inclination of 70° on June 15, 2006. The apparatus comprises a magnetic spectrometer, an electromagnetic calorimeter (16X 0), a time-of-flight system, a neutron detector, an anticoincidence system, and a shower tail scintillator. It allows measurements of electron and positron fluxes in cosmic rays over a wide energy range of ∼100 MeV to several hundreds of GeVs. In this work, we present data on the electron and positron energy spectra in primary cosmic rays, obtained between June 2006 and December 2008.",

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

note = "Funding Information: The authors are grateful to the RF Space Agency ROSKOSMOS, the Research Center for Earth Oper ative Monitoring, the Samara Space Center “TsSKB Progress,” the INFN, and the Russian Foundation for Basic Research (grant nos. 10 02 01301a and 09 02 00394a) for their support and assistance in performing the experiment.",

year = "2011",

month = mar,

doi = "10.3103/S1062873811030300",

language = "אנגלית",

volume = "75",

pages = "316--318",

journal = "Bulletin of the Russian Academy of Sciences: Physics",

issn = "1062-8738",

publisher = "Pleiades Publishing",

number = "3",

}

Mikhailov, VV, Adriani, O, Bazilevskaya, GA, Barbarino, GC, Belotti, R, Boezio, M, Bogomolov, EA, Bonvicini, V, Bongi, M, Bonechi, L, Borisov, SV, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Crishantseva, LA, Danilchenko, IA, De Pascale, MP, Di Felice, V, Galper, AM, Gastellini, G, Gillard, W, Jerse, G, Karelin, AV, Koldashov, SV, Koldobsky, SA, Krutkov, SY, Kvashnin, AN, Leonov, AA, Malakhov, VV, Malvezzi, V, Marcelli, L, Mayorov, AG, Menn, W, Mocchiutti, E, Mori, N, Nikonov, NV, Osteria, G, Papini, P, Pearce, M, Picozza, P, Pizzolotto, P, Ricci, M, Ricciarini, S, Runtso, MF, Simon, M, De Simone, N, Sparvoli, R, Spillantini, P, Stozhkov, YI, Vacchi, A, Vannuccini, E, Vasilyev, GI, Voronov, SA, Wu, Y, Yurkin, YT, Zampa, G, Zampa, N & Zverev, VG 2011, 'Primary electron and positron fluxes measured by the PAMELA experiment', Bulletin of the Russian Academy of Sciences: Physics, vol. 75, no. 3, pp. 316-318. https://doi.org/10.3103/S1062873811030300

TY - JOUR

T1 - Primary electron and positron fluxes measured by the PAMELA experiment

AU - Mikhailov, V. V.

AU - Adriani, O.

AU - Bazilevskaya, G. A.

AU - Barbarino, G. C.

AU - Belotti, R.

AU - Boezio, M.

AU - Bogomolov, E. A.

AU - Bonvicini, V.

AU - Bongi, M.

AU - Bonechi, L.

AU - Borisov, S. V.

AU - Bottai, S.

AU - Bruno, A.

AU - Cafagna, F.

AU - Campana, D.

AU - Carbone, R.

AU - Carlson, P.

AU - Casolino, M.

AU - Crishantseva, L. A.

AU - Danilchenko, I. A.

AU - De Pascale, M. P.

AU - Di Felice, V.

AU - Galper, A. M.

AU - Gastellini, G.

AU - Gillard, W.

AU - Jerse, G.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Koldobsky, S. A.

AU - Krutkov, S. Yu

AU - Kvashnin, A. N.

AU - Leonov, A. A.

AU - Malakhov, V. V.

AU - Malvezzi, V.

AU - Marcelli, L.

AU - Mayorov, A. G.

AU - Menn, W.

AU - Mocchiutti, E.

AU - Mori, N.

AU - Nikonov, N. V.

AU - Osteria, G.

AU - Papini, P.

AU - Pearce, M.

AU - Picozza, P.

AU - Pizzolotto, P.

AU - Ricci, M.

AU - Ricciarini, S.

AU - Runtso, M. F.

AU - Simon, M.

AU - De Simone, N.

AU - Sparvoli, R.

AU - Spillantini, P.

AU - Stozhkov, Yu I.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasilyev, G. I.

AU - Voronov, S. A.

AU - Wu, Y.

AU - Yurkin, Yu T.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

N1 - Funding Information: The authors are grateful to the RF Space Agency ROSKOSMOS, the Research Center for Earth Oper ative Monitoring, the Samara Space Center “TsSKB Progress,” the INFN, and the Russian Foundation for Basic Research (grant nos. 10 02 01301a and 09 02 00394a) for their support and assistance in performing the experiment.

PY - 2011/3

Y1 - 2011/3

N2 - The PAMELA experiment is being conducted on board the RESURS DK1 satellite, launched into a near-Earth, near-polar orbit with an altitude of 350-610 km and an inclination of 70° on June 15, 2006. The apparatus comprises a magnetic spectrometer, an electromagnetic calorimeter (16X 0), a time-of-flight system, a neutron detector, an anticoincidence system, and a shower tail scintillator. It allows measurements of electron and positron fluxes in cosmic rays over a wide energy range of ∼100 MeV to several hundreds of GeVs. In this work, we present data on the electron and positron energy spectra in primary cosmic rays, obtained between June 2006 and December 2008.

AB - The PAMELA experiment is being conducted on board the RESURS DK1 satellite, launched into a near-Earth, near-polar orbit with an altitude of 350-610 km and an inclination of 70° on June 15, 2006. The apparatus comprises a magnetic spectrometer, an electromagnetic calorimeter (16X 0), a time-of-flight system, a neutron detector, an anticoincidence system, and a shower tail scintillator. It allows measurements of electron and positron fluxes in cosmic rays over a wide energy range of ∼100 MeV to several hundreds of GeVs. In this work, we present data on the electron and positron energy spectra in primary cosmic rays, obtained between June 2006 and December 2008.

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DO - 10.3103/S1062873811030300

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AN - SCOPUS:79955849231

SN - 1062-8738

VL - 75

SP - 316

EP - 318

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

IS - 3

ER -

Primary electron and positron fluxes measured by the PAMELA experiment

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Bibliographical note

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