By M. Barone
Court cases of the seventh foreign convention on ICATPP-7, held October 15-19, 2001 in Villa, Olmo, Como, Italy. gains modern know-how purposes to radiation detection.
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To examine the performance of the AC system in-orbit a simulation study has been performed using a proton spectrum 2 for the polar region of the orbit where the flux is largest due to the negligible geomagnetic cut-off. Protons make up the largest part of the cosmic radiation (~90%) and the polar flux will be approximately 8 times larger than the equatorial flux. A first level trigger rate of 24Hz is predicted with 'good' triggers contributing 7Hz and 17Hz coming from 'false' triggers. The dominant part of the 'false' triggers are produced by particles hitting the experiment from above, but a non-neglible amount is also produced due to particles hitting the experiment from the sides and from below.
Pixel size, weight, fast time response and single photoelectron resolution are well adaptable to the EUSO focal surface detector. The organization in "macrocells" of the focal 43 surface (a macrocell is a bi-dimensional array of nxn pixels) offers many advantages as easy planning and implementation, flexibility and redundancy. Moreover, modularity is ideal for space application. The Multi-Anode Photomultipliers represent, in this contest, a workable solution. Trigger and Electronics System. Special attention has been given to the trigger scheme where the implementation of hardware/firmware special functions is foreseen.
Advanced Technology and Particle Physics by M. Barone