Sub-cutoff electrons and positrons spectra measured with PAMELA

Vladimir Mikhailov; L. A. Grishantseva; 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; P. Hofverberg; 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; N. N. Nikonov; G. Osteria; P. Papini; 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:10.7529/ICRC2011/V06/0558

Sub-cutoff electrons and positrons spectra measured with PAMELA

Vladimir Mikhailov, L. A. Grishantseva, 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. CastelliniL. Consiglio, M. P. De Pascale, C. De Santis, N. De Simone, V. Di Felice, A. M. Galper, G. Jerse, P. Hofverberg, 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, N. N. Nikonov, G. Osteria, P. Papini, 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 conference › Paper › peer-review

Abstract

Precise spectra of electron and positron fluxes in energy range from 80 MeV to several GeV below the geomagnetic cutoff rigidity were obtained using data of the PAMELA magnetic spectrometer. It was launched on June 15th 2006 onboard the Resurs-DK satellite on an elliptical orbit (the inclination is 70, the altitude is 350-610km). The work presents measurements of spatial distributions of secondaries produced in interactions of cosmic ray protons with the residual atmosphere in the near Earth space. Altitude , latitudinal and longitudinal dependences are discussed. These results are particularly interesting for more accurate definition of flux model in the Earth magnetosphere.

Original language	English
Pages	25-28
Number of pages	4
DOIs	https://doi.org/10.7529/ICRC2011/V06/0558
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

Funding

Funders	Funder number
Swedish National Space Board

Keywords

Electrons
Magnetic spectrometer
Magnetosphere
Positrons

Access to Document

10.7529/ICRC2011/V06/0558

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Mikhailov, V., Grishantseva, L. A., 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., ... Zverev, V. G. (2011). Sub-cutoff electrons and positrons spectra measured with PAMELA. 25-28. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China. https://doi.org/10.7529/ICRC2011/V06/0558

@conference{88e8170f8d834284a9d88e4394493983,

title = "Sub-cutoff electrons and positrons spectra measured with PAMELA",

abstract = "Precise spectra of electron and positron fluxes in energy range from 80 MeV to several GeV below the geomagnetic cutoff rigidity were obtained using data of the PAMELA magnetic spectrometer. It was launched on June 15th 2006 onboard the Resurs-DK satellite on an elliptical orbit (the inclination is 70, the altitude is 350-610km). The work presents measurements of spatial distributions of secondaries produced in interactions of cosmic ray protons with the residual atmosphere in the near Earth space. Altitude , latitudinal and longitudinal dependences are discussed. These results are particularly interesting for more accurate definition of flux model in the Earth magnetosphere.",

keywords = "Electrons, Magnetic spectrometer, Magnetosphere, Positrons",

author = "Vladimir Mikhailov and Grishantseva, {L. A.} 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 P. Hofverberg and Karelin, {A. V.} and Koldashov, {S. V.} and S. Koldobsky 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 A. Monaco and N. Mori and Nikonov, {N. N.} and G. Osteria 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, {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 = "2011",

doi = "10.7529/ICRC2011/V06/0558",

language = "אנגלית",

pages = "25--28",

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

}

Mikhailov, V, Grishantseva, LA, 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, Hofverberg, P, Karelin, AV, Koldashov, SV, Koldobsky, S, Krutkov, SY, Kvashnin, AN, Leonov, AA, Malakhov, VV, Malvezzi, V, Marcelli, L, Mayorov, AG, Menn, W, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, NN, Osteria, G, 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, Vasiliev, GI, Voronov, SA, Wu, J, Yurkin, YT, Zampa, G, Zampa, N & Zverev, VG 2011, 'Sub-cutoff electrons and positrons spectra measured with PAMELA', Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China, 11/08/11 - 18/08/11 pp. 25-28. https://doi.org/10.7529/ICRC2011/V06/0558

TY - CONF

T1 - Sub-cutoff electrons and positrons spectra measured with PAMELA

AU - Mikhailov, Vladimir

AU - Grishantseva, L. A.

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 - Hofverberg, P.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Koldobsky, S.

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 - Monaco, A.

AU - Mori, N.

AU - Nikonov, N. N.

AU - Osteria, G.

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, 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 - 2011

Y1 - 2011

N2 - Precise spectra of electron and positron fluxes in energy range from 80 MeV to several GeV below the geomagnetic cutoff rigidity were obtained using data of the PAMELA magnetic spectrometer. It was launched on June 15th 2006 onboard the Resurs-DK satellite on an elliptical orbit (the inclination is 70, the altitude is 350-610km). The work presents measurements of spatial distributions of secondaries produced in interactions of cosmic ray protons with the residual atmosphere in the near Earth space. Altitude , latitudinal and longitudinal dependences are discussed. These results are particularly interesting for more accurate definition of flux model in the Earth magnetosphere.

AB - Precise spectra of electron and positron fluxes in energy range from 80 MeV to several GeV below the geomagnetic cutoff rigidity were obtained using data of the PAMELA magnetic spectrometer. It was launched on June 15th 2006 onboard the Resurs-DK satellite on an elliptical orbit (the inclination is 70, the altitude is 350-610km). The work presents measurements of spatial distributions of secondaries produced in interactions of cosmic ray protons with the residual atmosphere in the near Earth space. Altitude , latitudinal and longitudinal dependences are discussed. These results are particularly interesting for more accurate definition of flux model in the Earth magnetosphere.

KW - Electrons

KW - Magnetic spectrometer

KW - Magnetosphere

KW - Positrons

UR - http://www.scopus.com/inward/record.url?scp=84899568239&partnerID=8YFLogxK

U2 - 10.7529/ICRC2011/V06/0558

DO - 10.7529/ICRC2011/V06/0558

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

AN - SCOPUS:84899568239

SP - 25

EP - 28

T2 - 32nd International Cosmic Ray Conference, ICRC 2011

Y2 - 11 August 2011 through 18 August 2011

ER -

Sub-cutoff electrons and positrons spectra measured with PAMELA

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Keywords

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