Author/Authors :
Straulino، نويسنده , , S. and Adriani، نويسنده , , O. and Bonechi، نويسنده , , L. and Bongi، نويسنده , , M. and Bottai، نويسنده , , S. and Castellini، نويسنده , , G. and Fedele، نويسنده , , D. and Grandi، نويسنده , , M. Petrangeli Papini، نويسنده , , P. and Ricciarini، نويسنده , , S.B. and Spillantini، نويسنده , , P. and Taccetti، نويسنده , , F. and Taddei، نويسنده , , E. and Vannuccini، نويسنده , , E.، نويسنده ,
Abstract :
The PAMELA apparatus has been assembled and it is ready to be launched in a satellite mission to study mainly the antiparticle component of cosmic rays. In this paper, the performances obtained for the silicon microstrip detectors used in the magnetic spectrometer are presented. This subdetector reconstructs the curvature of a charged particle in the magnetic field produced by a permanent magnet and consequently determines momentum and charge sign, thanks to a very good accuracy in the position measurements (better than 3 μ m in the bending coordinate). A complete simulation of the silicon microstrip detectors has been developed in order to investigate in great detail the sensorʹs characteristics. Simulated events have been then compared with data gathered from minimum ionizing particle (MIP) beams during the last years in order to tune free parameters of the simulation. Finally some either widely used or original position finding algorithms, designed for such kind of detectors, have been applied to events with different incidence angles. As a result of the analysis, a method of impact point reconstruction can be chosen, depending on both the particleʹs incidence angle and the cluster multiplicity, so as to maximize the capability of the spectrometer in antiparticle tagging.
