OBSERVATION OF THE SOLAR PARTICLE EVENT OF DECEMBER 13 2006 WITH PAMELA EXPERIMENT

摘要

PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons: 80 MeV-700 GeV, electrons 50 MeV-400 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV-190 GeV), positrons (50 MeV-270 GeV) and search for antinuclei with a precision of the order of 10~(?8)). In this work we present the measurements of the December 13~(th) 2006 Solar Particle Event.