Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment

G. A. Bazilevskaya; A. G. Mayorov; V. V. Malakhov; V. V. Mikhailov; O. Adriani; G. C. Barbarino; R. Belotti; M. Boezio; E. A. Bogomolov; V. Bonvicini; M. Bongi; L. Bonechi; S. V. Borisov; S. Bottai; A. Bruno; A. Vacci; E. Vanuccini; G. I. Vasilyev; S. A. Voronov; J. Wu; A. M. Galper; L. A. Grishantseva; I. A. Danilchenko; W. Gillard; G. Jerse; G. Zampa; N. Zampa; V. G. Zverev; M. Casolino; D. Campana; R. Carbone; A. V. Karelin; P. Carlson; G. Castellini; F. Cafagna; A. N. Kvashnin; S. V. Koldashov; S. A. Koldobskiy; S. Yu Krutkov; L. Consiglio; A. A. Leonov; V. Malvezzi; L. Marcelli; W. Menn; E. Mocchiutti; A. Monaco; N. Mori; N. N. Nikonov; G. Osteria; F. Palma; P. Papini; C. Pizzolotto; M. P. De Pascale; P. Picozza; M. Pearce; M. Ricci; S. B. Ricciarini; L. Rossetto; M. F. Runtso; C. De Santis; R. Sarkar; M. Simon; N. De Simone; R. Sparvoli; P. Spillantini; Yu I. Stozhkov; V. Di Felice; M. D. Kheymits; Yu T. Yurkin

doi:10.3103/s1062873813050109

Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment

G. A. Bazilevskaya, A. G. Mayorov, V. V. Malakhov, V. V. Mikhailov, O. Adriani, G. C. Barbarino, R. Belotti, M. Boezio, E. A. Bogomolov, V. Bonvicini, M. Bongi, L. Bonechi, S. V. Borisov, S. Bottai, A. Bruno, A. Vacci, E. Vanuccini, G. I. Vasilyev, S. A. Voronov, J. WuA. M. Galper, L. A. Grishantseva, I. A. Danilchenko, W. Gillard, G. Jerse, G. Zampa, N. Zampa, V. G. Zverev, M. Casolino, D. Campana, R. Carbone, A. V. Karelin, P. Carlson, G. Castellini, F. Cafagna, A. N. Kvashnin, S. V. Koldashov, S. A. Koldobskiy, S. Yu Krutkov, L. Consiglio, A. A. Leonov, V. Malvezzi, L. Marcelli, W. Menn, E. Mocchiutti, A. Monaco, N. Mori, N. N. Nikonov, G. Osteria, F. Palma, P. Papini, C. Pizzolotto, M. P. De Pascale, P. Picozza, M. Pearce, M. Ricci, S. B. Ricciarini, L. Rossetto, M. F. Runtso, C. De Santis, R. Sarkar, M. Simon, N. De Simone, R. Sparvoli, P. Spillantini, Yu I. Stozhkov, V. Di Felice, M. D. Kheymits, Yu T. Yurkin

Research output: Contribution to journal › Article › peer-review

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Abstract

The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satellite in June 2006; in December 2006, it recorded the last strong solar high-energy particle event of the 23rd solar cycle. A deficit was thereafter observed in solar energetic particle events because of the lengthy solar activity minimum and the weak evolution of the next (24th) solar cycle. As a result, only a few solar events involving protons with energies of more than 100 MeV were recorded between 2010 and 1012. This work presents the preliminary results from measurements of charged particle fluxes in these events, recorded by the Pamela spectrometer.

Original language	English
Pages (from-to)	493-496
Number of pages	4
Journal	Bulletin of the Russian Academy of Sciences: Physics
Volume	77
Issue number	5
DOIs	https://doi.org/10.3103/s1062873813050109
State	Published - May 2013
Externally published	Yes

Bibliographical note

Funding Information:
ACKNOWLEDGMENTS The authors are grateful to the Space Council of the Russian Academy of Sciences, the Roskosmos Federal Space Agency, the TsSKB Progress Federal Space Center, the Research Center for Earth Opera tive Monitoring, the Italian Space Agency (Agenzia Spaziale Italiana), the German Aerospace Center (DLR), the Swedish National Space Board, and the Swedish Research Council.

Funding

ACKNOWLEDGMENTS The authors are grateful to the Space Council of the Russian Academy of Sciences, the Roskosmos Federal Space Agency, the TsSKB Progress Federal Space Center, the Research Center for Earth Opera tive Monitoring, the Italian Space Agency (Agenzia Spaziale Italiana), the German Aerospace Center (DLR), the Swedish National Space Board, and the Swedish Research Council.

Funders	Funder number
Roskosmos Federal Space Agency
Space Council of the Russian Academy of Sciences
Swedish National Space Agency
Deutsches Zentrum für Luft- und Raumfahrt
Agenzia Spaziale Italiana
Vetenskapsrådet

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Bazilevskaya, G. A., Mayorov, A. G., Malakhov, V. V., Mikhailov, V. V., Adriani, O., Barbarino, G. C., Belotti, R., Boezio, M., Bogomolov, E. A., Bonvicini, V., Bongi, M., Bonechi, L., Borisov, S. V., Bottai, S., Bruno, A., Vacci, A., Vanuccini, E., Vasilyev, G. I., Voronov, S. A., ... Yurkin, Y. T. (2013). Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment. Bulletin of the Russian Academy of Sciences: Physics, 77(5), 493-496. https://doi.org/10.3103/s1062873813050109

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title = "Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment",

abstract = "The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satellite in June 2006; in December 2006, it recorded the last strong solar high-energy particle event of the 23rd solar cycle. A deficit was thereafter observed in solar energetic particle events because of the lengthy solar activity minimum and the weak evolution of the next (24th) solar cycle. As a result, only a few solar events involving protons with energies of more than 100 MeV were recorded between 2010 and 1012. This work presents the preliminary results from measurements of charged particle fluxes in these events, recorded by the Pamela spectrometer.",

author = "Bazilevskaya, {G. A.} and Mayorov, {A. G.} and Malakhov, {V. V.} and Mikhailov, {V. V.} and O. Adriani 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 A. Vacci and E. Vanuccini and Vasilyev, {G. I.} and Voronov, {S. A.} and J. Wu and Galper, {A. M.} and Grishantseva, {L. A.} and Danilchenko, {I. A.} and W. Gillard and G. Jerse and G. Zampa and N. Zampa and Zverev, {V. G.} and M. Casolino and D. Campana and R. Carbone and Karelin, {A. V.} and P. Carlson and G. Castellini and F. Cafagna and Kvashnin, {A. N.} and Koldashov, {S. V.} and Koldobskiy, {S. A.} and Krutkov, {S. Yu} and L. Consiglio and Leonov, {A. A.} and V. Malvezzi and L. Marcelli and W. Menn and E. Mocchiutti and A. Monaco and N. Mori and Nikonov, {N. N.} and G. Osteria and F. Palma and P. Papini and C. Pizzolotto and {De Pascale}, {M. P.} and P. Picozza and M. Pearce and M. Ricci and Ricciarini, {S. B.} and L. Rossetto and Runtso, {M. F.} and {De Santis}, C. and R. Sarkar and M. Simon and {De Simone}, N. and R. Sparvoli and P. Spillantini and Stozhkov, {Yu I.} and {Di Felice}, V. and Kheymits, {M. D.} and Yurkin, {Yu T.}",

note = "Funding Information: ACKNOWLEDGMENTS The authors are grateful to the Space Council of the Russian Academy of Sciences, the Roskosmos Federal Space Agency, the TsSKB Progress Federal Space Center, the Research Center for Earth Opera tive Monitoring, the Italian Space Agency (Agenzia Spaziale Italiana), the German Aerospace Center (DLR), the Swedish National Space Board, and the Swedish Research Council.",

year = "2013",

month = may,

doi = "10.3103/s1062873813050109",

language = "אנגלית",

volume = "77",

pages = "493--496",

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

issn = "1062-8738",

publisher = "Pleiades Publishing",

number = "5",

}

Bazilevskaya, GA, Mayorov, AG, Malakhov, VV, Mikhailov, VV, Adriani, O, Barbarino, GC, Belotti, R, Boezio, M, Bogomolov, EA, Bonvicini, V, Bongi, M, Bonechi, L, Borisov, SV, Bottai, S, Bruno, A, Vacci, A, Vanuccini, E, Vasilyev, GI, Voronov, SA, Wu, J, Galper, AM, Grishantseva, LA, Danilchenko, IA, Gillard, W, Jerse, G, Zampa, G, Zampa, N, Zverev, VG, Casolino, M, Campana, D, Carbone, R, Karelin, AV, Carlson, P, Castellini, G, Cafagna, F, Kvashnin, AN, Koldashov, SV, Koldobskiy, SA, Krutkov, SY, Consiglio, L, Leonov, AA, Malvezzi, V, Marcelli, L, Menn, W, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, NN, Osteria, G, Palma, F, Papini, P, Pizzolotto, C, De Pascale, MP, Picozza, P, Pearce, M, Ricci, M, Ricciarini, SB, Rossetto, L, Runtso, MF, De Santis, C, Sarkar, R, Simon, M, De Simone, N, Sparvoli, R, Spillantini, P, Stozhkov, YI, Di Felice, V, Kheymits, MD & Yurkin, YT 2013, 'Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment', Bulletin of the Russian Academy of Sciences: Physics, vol. 77, no. 5, pp. 493-496. https://doi.org/10.3103/s1062873813050109

TY - JOUR

T1 - Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment

AU - Bazilevskaya, G. A.

AU - Mayorov, A. G.

AU - Malakhov, V. V.

AU - Mikhailov, V. V.

AU - Adriani, O.

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 - Vacci, A.

AU - Vanuccini, E.

AU - Vasilyev, G. I.

AU - Voronov, S. A.

AU - Wu, J.

AU - Galper, A. M.

AU - Grishantseva, L. A.

AU - Danilchenko, I. A.

AU - Gillard, W.

AU - Jerse, G.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

AU - Casolino, M.

AU - Campana, D.

AU - Carbone, R.

AU - Karelin, A. V.

AU - Carlson, P.

AU - Castellini, G.

AU - Cafagna, F.

AU - Kvashnin, A. N.

AU - Koldashov, S. V.

AU - Koldobskiy, S. A.

AU - Krutkov, S. Yu

AU - Consiglio, L.

AU - Leonov, A. A.

AU - Malvezzi, V.

AU - Marcelli, L.

AU - Menn, W.

AU - Mocchiutti, E.

AU - Monaco, A.

AU - Mori, N.

AU - Nikonov, N. N.

AU - Osteria, G.

AU - Palma, F.

AU - Papini, P.

AU - Pizzolotto, C.

AU - De Pascale, M. P.

AU - Picozza, P.

AU - Pearce, M.

AU - Ricci, M.

AU - Ricciarini, S. B.

AU - Rossetto, L.

AU - Runtso, M. F.

AU - De Santis, C.

AU - Sarkar, R.

AU - Simon, M.

AU - De Simone, N.

AU - Sparvoli, R.

AU - Spillantini, P.

AU - Stozhkov, Yu I.

AU - Di Felice, V.

AU - Kheymits, M. D.

AU - Yurkin, Yu T.

N1 - Funding Information: ACKNOWLEDGMENTS The authors are grateful to the Space Council of the Russian Academy of Sciences, the Roskosmos Federal Space Agency, the TsSKB Progress Federal Space Center, the Research Center for Earth Opera tive Monitoring, the Italian Space Agency (Agenzia Spaziale Italiana), the German Aerospace Center (DLR), the Swedish National Space Board, and the Swedish Research Council.

PY - 2013/5

Y1 - 2013/5

N2 - The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satellite in June 2006; in December 2006, it recorded the last strong solar high-energy particle event of the 23rd solar cycle. A deficit was thereafter observed in solar energetic particle events because of the lengthy solar activity minimum and the weak evolution of the next (24th) solar cycle. As a result, only a few solar events involving protons with energies of more than 100 MeV were recorded between 2010 and 1012. This work presents the preliminary results from measurements of charged particle fluxes in these events, recorded by the Pamela spectrometer.

AB - The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satellite in June 2006; in December 2006, it recorded the last strong solar high-energy particle event of the 23rd solar cycle. A deficit was thereafter observed in solar energetic particle events because of the lengthy solar activity minimum and the weak evolution of the next (24th) solar cycle. As a result, only a few solar events involving protons with energies of more than 100 MeV were recorded between 2010 and 1012. This work presents the preliminary results from measurements of charged particle fluxes in these events, recorded by the Pamela spectrometer.

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SN - 1062-8738

VL - 77

SP - 493

EP - 496

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

IS - 5

ER -

Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment

Abstract

Bibliographical note

Funding

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