Cosmic ray electron and positron spectra measured with PAMELA

Vladimir Mikhailov; O. Adriani; G. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. Boezio; E. A. Bogomolov; L. Bonechi; M. Bongi; V. Bonvicini; S. V. Borisov; S. Bottai; A. Bruno; F. S. 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; G. Jerse; A. V. Karelin; S. V. Koldashov; S. Koldobsky; S. Yu Krutkov; A. N. Kvashnin; A. A. Leonov; V. V. Malakhov; V. Malvezzi; L. Marcelli; A. G. Mayorov; W. Menn; E. Mocchiutti; A. Monaco; N. Mori; G. Osteria; P. Papini; F. Palma; M. Pearce; P. Picozza; C. Pizzolotto; M. Ricci; S. B. Ricciarini; L. Rossetto; R. Sarkar; M. Simon; R. Sparvoli; P. Spillantini; Yu I. Stozhkov; A. Vacchi; E. Vannuccini; G. I. Vasiliev; S. A. Voronov; J. Wu; Yu T. Yurkin; G. Zampa; N. Zampa; V. G. Zverev

doi:10.1088/1742-6596/409/1/012035

Cosmic ray electron and positron spectra measured with PAMELA

Vladimir Mikhailov, O. Adriani, G. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. V. Borisov, S. Bottai, A. Bruno, F. S. 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, G. Jerse, A. V. Karelin, S. V. Koldashov, S. Koldobsky, S. Yu Krutkov, A. N. Kvashnin, A. A. Leonov, V. V. Malakhov, V. Malvezzi, L. Marcelli, A. G. Mayorov, W. Menn, E. Mocchiutti, A. Monaco, N. Mori, G. Osteria, P. Papini, F. Palma, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, R. Sarkar, M. Simon, R. Sparvoli, P. Spillantini, Yu I. Stozhkov, A. Vacchi, E. Vannuccini, G. I. Vasiliev, S. A. Voronov, J. Wu, Yu T. Yurkin, G. Zampa, N. Zampa, V. G. Zverev

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

1 Scopus citations

Abstract

The PAMELA experiment is carried out on board of the satellite Resurs DK1 launched on June 15th 2006 on polar orbit (the inclination is 70, the altitude is 350-600 km). The instrument which consists of magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter gives a possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Measurements made in June 2006- January 2010 are presented and compared with other results and models. Positron spectrum appears to be harder than standard diffusive propagation models predict.

Original language	English
Article number	012035
Journal	Journal of Physics: Conference Series
Volume	409
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/409/1/012035
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

10.1088/1742-6596/409/1/012035

Cite this

Mikhailov, V., Adriani, O., Barbarino, G., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F. S., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., ... Zverev, V. G. (2013). Cosmic ray electron and positron spectra measured with PAMELA. Journal of Physics: Conference Series, 409(1), Article 012035. https://doi.org/10.1088/1742-6596/409/1/012035

@article{b4dbc50bd8cb4e67990551e62deac7fd,

title = "Cosmic ray electron and positron spectra measured with PAMELA",

abstract = "The PAMELA experiment is carried out on board of the satellite Resurs DK1 launched on June 15th 2006 on polar orbit (the inclination is 70, the altitude is 350-600 km). The instrument which consists of magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter gives a possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Measurements made in June 2006- January 2010 are presented and compared with other results and models. Positron spectrum appears to be harder than standard diffusive propagation models predict.",

author = "Vladimir Mikhailov and O. Adriani and G. Barbarino and Bazilevskaya, \{G. A.\} and R. Bellotti and M. Boezio and Bogomolov, \{E. A.\} and L. Bonechi and M. Bongi and V. Bonvicini and Borisov, \{S. V.\} and S. Bottai and A. Bruno and Cafagna, \{F. S.\} 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 G. Jerse and Karelin, \{A. V.\} and Koldashov, \{S. V.\} and S. Koldobsky and \{Yu Krutkov\}, S. 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 A. Monaco and N. Mori and G. Osteria and P. Papini and F. Palma 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, \{Yu I.\} and A. Vacchi and E. Vannuccini and Vasiliev, \{G. I.\} and Voronov, \{S. A.\} and J. Wu and Yurkin, \{Yu T.\} and G. Zampa and N. Zampa and Zverev, \{V. G.\}",

year = "2013",

doi = "10.1088/1742-6596/409/1/012035",

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",

}

Mikhailov, V, Adriani, O, Barbarino, G, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, SV, Bottai, S, Bruno, A, Cafagna, FS, 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, Jerse, G, Karelin, AV, Koldashov, SV, Koldobsky, S, Yu Krutkov, S, Kvashnin, AN, Leonov, AA, Malakhov, VV, Malvezzi, V, Marcelli, L, Mayorov, AG, Menn, W, Mocchiutti, E, Monaco, A, Mori, N, Osteria, G, Papini, P, Palma, F, 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, Vasiliev, GI, Voronov, SA, Wu, J, Yurkin, YT, Zampa, G, Zampa, N & Zverev, VG 2013, 'Cosmic ray electron and positron spectra measured with PAMELA', Journal of Physics: Conference Series, vol. 409, no. 1, 012035. https://doi.org/10.1088/1742-6596/409/1/012035

TY - JOUR

T1 - Cosmic ray electron and positron spectra measured with PAMELA

AU - Mikhailov, Vladimir

AU - Adriani, O.

AU - Barbarino, G.

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. V.

AU - Bottai, S.

AU - Bruno, A.

AU - Cafagna, F. 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 - Jerse, G.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Koldobsky, S.

AU - Yu Krutkov, S.

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 - Monaco, A.

AU - Mori, N.

AU - Osteria, G.

AU - Papini, P.

AU - Palma, F.

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, Yu I.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasiliev, G. I.

AU - Voronov, S. A.

AU - Wu, J.

AU - Yurkin, Yu T.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

PY - 2013

Y1 - 2013

N2 - The PAMELA experiment is carried out on board of the satellite Resurs DK1 launched on June 15th 2006 on polar orbit (the inclination is 70, the altitude is 350-600 km). The instrument which consists of magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter gives a possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Measurements made in June 2006- January 2010 are presented and compared with other results and models. Positron spectrum appears to be harder than standard diffusive propagation models predict.

AB - The PAMELA experiment is carried out on board of the satellite Resurs DK1 launched on June 15th 2006 on polar orbit (the inclination is 70, the altitude is 350-600 km). The instrument which consists of magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter gives a possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Measurements made in June 2006- January 2010 are presented and compared with other results and models. Positron spectrum appears to be harder than standard diffusive propagation models predict.

UR - https://www.scopus.com/pages/publications/84874303962

U2 - 10.1088/1742-6596/409/1/012035

DO - 10.1088/1742-6596/409/1/012035

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

AN - SCOPUS:84874303962

SN - 1742-6588

VL - 409

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012035

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 electron and positron spectra measured with PAMELA

Abstract

Access to Document

Other files and links

Fingerprint

Cite this