Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment

A. G. Maiorov; O. Adriani; G. Barbarino; G. A. Bazilevskaia; R. Bellotti; M. Boezio; E. A. Bogomolov; L. Bonechi; M. Bongi; V. Bonvicini; S. V. Borisov; S. Bottai; A. Bruno; F. Cafagna; D. Campana; R. Carbone; P. Carlson; M. Casolino; G. Castellini; I. A. Danil'Chenko; M. P. De Pascale; V. Di Felice; A. M. Gal'Per; V. Gillard; L. A. Grishantseva; G. Jerse; A. V. Karelin; S. V. Koldashov; S. A. Koldobskii; S. Yu Krutkov; A. N. Kvashnin; A. A. Leonov; V. V. Malakhov; V. Malvezzi; L. Marcelli; W. Menn; V. V. Mikhailov; E. Mocchiutti; N. Mori; N. V. Nikonov; G. Osteria; P. Papini; M. Pearce; P. Picozza; C. 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. Vasil'Ev; S. A. Voronov; Y. Wu; Yu T. Yurkin; G. Zampa; N. Zampa; V. G. Zverev

doi:10.3103/S1062873811060293

Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment

A. G. Maiorov, O. Adriani, G. Barbarino, G. A. Bazilevskaia, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. V. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, I. A. Danil'ChenkoM. P. De Pascale, V. Di Felice, A. M. Gal'Per, V. Gillard, L. A. Grishantseva, G. Jerse, A. V. Karelin, S. V. Koldashov, S. A. Koldobskii, S. Yu Krutkov, A. N. Kvashnin, A. A. Leonov, V. V. Malakhov, V. Malvezzi, L. Marcelli, W. Menn, V. V. Mikhailov, E. Mocchiutti, N. Mori, N. V. Nikonov, G. Osteria, P. Papini, M. Pearce, P. Picozza, C. 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. Vasil'Ev, S. A. Voronov, Y. Wu, Yu T. Yurkin, G. Zampa, N. Zampa, V. G. Zverev

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Abstract

We present the energy spectra of protons and helium nuclei of cosmic rays obtained in the PAMELA experiment on board the satellite RESURS-DK1 for the period from August 2006 to December 2009. The spectra were measured in the energy range of 100 MeV/nucleon to 100 GeV/nucleon using a magnetic spectrometer within the apparatus. Variations in the solar modulation potential for protons and helium nuclei were calculated on the basis of the monthly mean particle fluxes. A force field model was used to compare the modulation with measurements from balloon experiments, and with measurements from a network of neutron monitors.

Original language	English
Pages (from-to)	779-781
Number of pages	3
Journal	Bulletin of the Russian Academy of Sciences: Physics
Volume	75
Issue number	6
DOIs	https://doi.org/10.3103/S1062873811060293
State	Published - Jun 2011
Externally published	Yes

Bibliographical note

Funding Information:
ACKNOWLEDGMENTS The authors are grateful to the Russian Academy of Sciences’ Council on Outer Space; the Roskosmos Federal Space Agency; the TsSKB Progress State Research and Production Space Rocket Center; the Research Center for Real Time Earth Monitoring; the Italian Space Agency; the German Aerospace Center; the Swedish National Space Board; the Swedish Research Council; and the Russian Foundation for Basic Research, project nos. 10 02 01301a and 09 02 00394a.

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Maiorov, A. G., Adriani, O., Barbarino, G., Bazilevskaia, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., ... Zverev, V. G. (2011). Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment. Bulletin of the Russian Academy of Sciences: Physics, 75(6), 779-781. https://doi.org/10.3103/S1062873811060293

@article{b552691e432f44d4beaa38538041f0bd,

title = "Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment",

abstract = "We present the energy spectra of protons and helium nuclei of cosmic rays obtained in the PAMELA experiment on board the satellite RESURS-DK1 for the period from August 2006 to December 2009. The spectra were measured in the energy range of 100 MeV/nucleon to 100 GeV/nucleon using a magnetic spectrometer within the apparatus. Variations in the solar modulation potential for protons and helium nuclei were calculated on the basis of the monthly mean particle fluxes. A force field model was used to compare the modulation with measurements from balloon experiments, and with measurements from a network of neutron monitors.",

author = "Maiorov, {A. G.} and O. Adriani and G. Barbarino and Bazilevskaia, {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 F. Cafagna and D. Campana and R. Carbone and P. Carlson and M. Casolino and G. Castellini and Danil'Chenko, {I. A.} and {De Pascale}, {M. P.} and {Di Felice}, V. and Gal'Per, {A. M.} and V. Gillard and Grishantseva, {L. A.} and G. Jerse and Karelin, {A. V.} and Koldashov, {S. V.} and Koldobskii, {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 W. Menn and Mikhailov, {V. V.} and E. Mocchiutti and N. Mori and Nikonov, {N. V.} and G. Osteria and P. Papini and M. Pearce and P. Picozza and C. 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 Vasil'Ev, {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: ACKNOWLEDGMENTS The authors are grateful to the Russian Academy of Sciences{\textquoteright} Council on Outer Space; the Roskosmos Federal Space Agency; the TsSKB Progress State Research and Production Space Rocket Center; the Research Center for Real Time Earth Monitoring; the Italian Space Agency; the German Aerospace Center; the Swedish National Space Board; the Swedish Research Council; and the Russian Foundation for Basic Research, project nos. 10 02 01301a and 09 02 00394a.",

year = "2011",

month = jun,

doi = "10.3103/S1062873811060293",

language = "אנגלית",

volume = "75",

pages = "779--781",

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

issn = "1062-8738",

publisher = "Pleiades Publishing",

number = "6",

}

Maiorov, AG, Adriani, O, Barbarino, G, Bazilevskaia, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, SV, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Danil'Chenko, IA, De Pascale, MP, Di Felice, V, Gal'Per, AM, Gillard, V, Grishantseva, LA, Jerse, G, Karelin, AV, Koldashov, SV, Koldobskii, SA, Krutkov, SY, Kvashnin, AN, Leonov, AA, Malakhov, VV, Malvezzi, V, Marcelli, L, Menn, W, Mikhailov, VV, Mocchiutti, E, Mori, N, Nikonov, NV, Osteria, G, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, S, Runtso, MF, Simon, M, De Simone, N, Sparvoli, R, Spillantini, P, Stozhkov, YI, Vacchi, A, Vannuccini, E, Vasil'Ev, GI, Voronov, SA, Wu, Y, Yurkin, YT, Zampa, G, Zampa, N & Zverev, VG 2011, 'Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment', Bulletin of the Russian Academy of Sciences: Physics, vol. 75, no. 6, pp. 779-781. https://doi.org/10.3103/S1062873811060293

TY - JOUR

T1 - Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment

AU - Maiorov, A. G.

AU - Adriani, O.

AU - Barbarino, G.

AU - Bazilevskaia, 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.

AU - Campana, D.

AU - Carbone, R.

AU - Carlson, P.

AU - Casolino, M.

AU - Castellini, G.

AU - Danil'Chenko, I. A.

AU - De Pascale, M. P.

AU - Di Felice, V.

AU - Gal'Per, A. M.

AU - Gillard, V.

AU - Grishantseva, L. A.

AU - Jerse, G.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Koldobskii, 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 - Menn, W.

AU - Mikhailov, V. V.

AU - Mocchiutti, E.

AU - Mori, N.

AU - Nikonov, N. V.

AU - Osteria, G.

AU - Papini, P.

AU - Pearce, M.

AU - Picozza, P.

AU - Pizzolotto, C.

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 - Vasil'Ev, 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: ACKNOWLEDGMENTS The authors are grateful to the Russian Academy of Sciences’ Council on Outer Space; the Roskosmos Federal Space Agency; the TsSKB Progress State Research and Production Space Rocket Center; the Research Center for Real Time Earth Monitoring; the Italian Space Agency; the German Aerospace Center; the Swedish National Space Board; the Swedish Research Council; and the Russian Foundation for Basic Research, project nos. 10 02 01301a and 09 02 00394a.

PY - 2011/6

Y1 - 2011/6

N2 - We present the energy spectra of protons and helium nuclei of cosmic rays obtained in the PAMELA experiment on board the satellite RESURS-DK1 for the period from August 2006 to December 2009. The spectra were measured in the energy range of 100 MeV/nucleon to 100 GeV/nucleon using a magnetic spectrometer within the apparatus. Variations in the solar modulation potential for protons and helium nuclei were calculated on the basis of the monthly mean particle fluxes. A force field model was used to compare the modulation with measurements from balloon experiments, and with measurements from a network of neutron monitors.

AB - We present the energy spectra of protons and helium nuclei of cosmic rays obtained in the PAMELA experiment on board the satellite RESURS-DK1 for the period from August 2006 to December 2009. The spectra were measured in the energy range of 100 MeV/nucleon to 100 GeV/nucleon using a magnetic spectrometer within the apparatus. Variations in the solar modulation potential for protons and helium nuclei were calculated on the basis of the monthly mean particle fluxes. A force field model was used to compare the modulation with measurements from balloon experiments, and with measurements from a network of neutron monitors.

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U2 - 10.3103/S1062873811060293

DO - 10.3103/S1062873811060293

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AN - SCOPUS:79960531173

SN - 1062-8738

VL - 75

SP - 779

EP - 781

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

IS - 6

ER -

Solar modulation of the spectra of protons and helium nuclei in the PAMELA experiment

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Bibliographical note

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