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Time dependence of the proton flux measured by PAMELA during the July 2006 - December 2009 solar minimum

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arxiv 1301.4108 v2 pith:NQ2SO5GU submitted 2013-01-17 astro-ph.HE astro-ph.SR

Time dependence of the proton flux measured by PAMELA during the July 2006 - December 2009 solar minimum

O. Adriani , G. C. Barbarino , G. A. Bazilevskaya , R. Bellotti , M. Boezio , E. A. Bogomolov , M. Bongi , V. Bonvicini
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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
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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 July 2006 to December 2009 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.

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