Back-Tracing and Flux Reconstruction for Solar Events with PAMELA
A. Bruno,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,R. Bellotti,M. Boezio,E. A. Bogomolov,M. Bongi,V. Bonvicini,S. Bottai,U. Bravar,F. Cafagna,D. Campana,R. Carbone,P. Carlson,M. Casolino,G. Castellini,E. C. Christian,C. De Donato,G. A. de Nolfo,C. De Santis,N. De Simone,V. Di Felice,V. Formato,A. M. Galper,A. V. Karelin,S. V. Koldashov,S. Koldobskiy,S. Y. Krutkov,A. N. Kvashnin,M. Lee,A. Leonov,V. Malakhov,L. Marcelli,M. Martucci,A. G. Mayorov,W. Menn,M. Mergé,V. V. Mikhailov,E. Mocchiutti,A. Monaco,N. Mori,R. Munini,G. Osteria,F. Palma,B. Panico,P. Papini,M. Pearce,P. Picozza,M. Ricci,S. B. Ricciarini,J. M. Ryan,R. Sarkar,V. Scotti,M. Simon,R. Sparvoli,P. Spillantini,S. Stochaj,Y. I. Stozhkov,A. Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev arXiv (Cornell University)（2014）
Key words
Environmental Magnetism
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