A detailed FLUKA-2005 Monte-Carlo simulation for the ATIC detector

• Published in: Advances in Space Research
• Main Authors: Gunasingha, R. M., Fazely, A. R., Adams, J. H., Ahn, H. S., Bashindzhagyan, G. L., Batkov, K. E., Chang, J., Christl, M., Ganel, O., Guzik, T. G., Isbert, J., Kim, K. C., Kouznetsov, E. N., Panasyuk, M. I., Panov, A. D., Schmidt, W. K.H., Seo, E. S., Sokolskaya, N. V., Watts, J. W., Wefel, J. P., Wu, J., Zatsepin, V. I., Lin, Z. W.
• Format: Text
• Language: unknown
• Published: LSU Digital Commons 2008
• Subjects: ATIC long duration balloon project; Scientific ballooning; Fluka; Antarc*; Antarctica
• Online Access: https://digitalcommons.lsu.edu/physics_astronomy_pubs/2219; https://doi.org/10.1016/j.asr.2007.03.079; https://digitalcommons.lsu.edu/context/physics_astronomy_pubs/article/3299/viewcontent/2219.pdf

We have performed a detailed Monte-Carlo (MC) simulation for the Advanced Thin Ionization Calorimeter (ATIC) detector using the MC code FLUKA-2005 which is capable of simulating particles up to 10 PeV. The ATIC detector has completed two successful balloon flights from McMurdo, Antarctica lasting a total of more than 35 days. ATIC is designed as a multiple, long duration balloon flight, investigation of the cosmic ray spectra from below 50 GeV to near 100 TeV total energy; using a fully active Bismuth Germanate (BGO) calorimeter. It is equipped with a large mosaic of silicon detector pixels capable of charge identification, and, for particle tracking, three projective layers of x-y scintillator hodoscopes, located above, in the middle and below a 0.75 nuclear interaction length graphite target. Our simulations are part of an analysis package of both nuclear (A) and energy dependences for different nuclei interacting in the ATIC detector. The MC simulates the response of different components of the detector such as the Si-matrix, the scintillator hodoscopes and the BGO calorimeter to various nuclei. We present comparisons of the FLUKA-2005 MC calculations with GEANT calculations and with the ATIC CERN data. © 2008.