TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum

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

doi:10.1088/0004-637X/765/2/91

TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum

O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, M. P. De Pascale, C. De Santis, N. De SimoneV. Di Felice, V. Formato, A. M. Galper, L. Grishantseva, A. V. Karelin, S. V. Koldashov, S. Koldobskiy, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, A. G. Mayorov, W. Menn, V. V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, N. Nikonov, G. Osteria, F. Palma, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, R. Sarkar, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, Y. T. Yurkin, J. Wu, G. Zampa, N. Zampa, V. G. Zverev, M. S. Potgieter, E. E. Vos

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Abstract

The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation.

Original language	English
Article number	91
Journal	Astrophysical Journal
Volume	765
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/765/2/91
State	Published - 10 Mar 2013
Externally published	Yes

Keywords

Sun: heliosphere
cosmic rays
solar wind

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10.1088/0004-637X/765/2/91

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Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Pascale, M. P., De Santis, C., ... Vos, E. E. (2013). TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum. Astrophysical Journal, 765(2), Article 91. https://doi.org/10.1088/0004-637X/765/2/91

@article{90cb5f4b04284fe69ebee84381e9cbd6,

title = "TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum",

abstract = "The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation.",

keywords = "Sun: heliosphere, cosmic rays, solar wind",

author = "O. Adriani and Barbarino, {G. C.} and Bazilevskaya, {G. A.} and R. Bellotti and M. Boezio and Bogomolov, {E. A.} and M. Bongi and V. Bonvicini and S. Borisov 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 {De Pascale}, {M. P.} and {De Santis}, C. and {De Simone}, N. and {Di Felice}, V. and V. Formato and Galper, {A. M.} and L. Grishantseva and Karelin, {A. V.} and Koldashov, {S. V.} and S. Koldobskiy and Krutkov, {S. Y.} and Kvashnin, {A. N.} and A. Leonov and V. Malakhov and L. Marcelli and Mayorov, {A. G.} and W. Menn and Mikhailov, {V. V.} and E. Mocchiutti and A. Monaco and N. Mori and N. Nikonov and G. Osteria and F. Palma 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, {Y. I.} and A. Vacchi and E. Vannuccini and G. Vasilyev and Voronov, {S. A.} and Yurkin, {Y. T.} and J. Wu and G. Zampa and N. Zampa and Zverev, {V. G.} and Potgieter, {M. S.} and Vos, {E. E.}",

year = "2013",

month = mar,

day = "10",

doi = "10.1088/0004-637X/765/2/91",

language = "אנגלית",

volume = "765",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

}

Adriani, O, Barbarino, GC, Bazilevskaya, GA, Bellotti, R, Boezio, M, Bogomolov, EA, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Pascale, MP, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, AM, Grishantseva, L, Karelin, AV, Koldashov, SV, Koldobskiy, S, Krutkov, SY, Kvashnin, AN, Leonov, A, Malakhov, V, Marcelli, L, Mayorov, AG, Menn, W, Mikhailov, VV, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, N, Osteria, G, Palma, F, 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, Vasilyev, G, Voronov, SA, Yurkin, YT, Wu, J, Zampa, G, Zampa, N, Zverev, VG, Potgieter, MS & Vos, EE 2013, 'TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum', Astrophysical Journal, vol. 765, no. 2, 91. https://doi.org/10.1088/0004-637X/765/2/91

TY - JOUR

T1 - TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum

AU - Adriani, O.

AU - Barbarino, G. C.

AU - Bazilevskaya, G. A.

AU - Bellotti, R.

AU - Boezio, M.

AU - Bogomolov, E. A.

AU - Bongi, M.

AU - Bonvicini, V.

AU - Borisov, S.

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 - De Pascale, M. P.

AU - De Santis, C.

AU - De Simone, N.

AU - Di Felice, V.

AU - Formato, V.

AU - Galper, A. M.

AU - Grishantseva, L.

AU - Karelin, A. V.

AU - Koldashov, S. V.

AU - Koldobskiy, S.

AU - Krutkov, S. Y.

AU - Kvashnin, A. N.

AU - Leonov, A.

AU - Malakhov, V.

AU - Marcelli, L.

AU - Mayorov, A. G.

AU - Menn, W.

AU - Mikhailov, V. V.

AU - Mocchiutti, E.

AU - Monaco, A.

AU - Mori, N.

AU - Nikonov, N.

AU - Osteria, G.

AU - Palma, F.

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, Y. I.

AU - Vacchi, A.

AU - Vannuccini, E.

AU - Vasilyev, G.

AU - Voronov, S. A.

AU - Yurkin, Y. T.

AU - Wu, J.

AU - Zampa, G.

AU - Zampa, N.

AU - Zverev, V. G.

AU - Potgieter, M. S.

AU - Vos, E. E.

PY - 2013/3/10

Y1 - 2013/3/10

N2 - The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation.

AB - The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation.

KW - Sun: heliosphere

KW - cosmic rays

KW - solar wind

UR - http://www.scopus.com/inward/record.url?scp=84874460278&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/765/2/91

DO - 10.1088/0004-637X/765/2/91

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:84874460278

SN - 0004-637X

VL - 765

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 91

ER -

TIme dependence of the proton flux measured by pamela during the 2006 july-2009 december solar minimum

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Keywords

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