Simulation of the ATIC-2 silicon matrix for protons and helium GCR Primaries at 0.3, 10, and 25 TeV/nucleon
Document Type
Conference Proceeding
Publication Date
1-1-2005
Abstract
The energy deposition distribution for protons and helium galactic cosmic ray primaries at 0.3, 10, and 25 TeV/nucleon in the ATIC-2 silicon matrix detector are simulated with GEANT4.
Publication Source (Journal or Book title)
29th International Cosmic Ray Conference, ICRC 2005
First Page
89
Last Page
92
Recommended Citation
Watts, J., Adams, J., Bashindzhagyan, G., Batkov, K., Chang, J., Christl, M., Fazely, A., Ganel, O., Gunasingha, R., Guzik, T., Isbert, J., Kim, K., Kouznetsov, E., Panasyuk, M., Panov, A., Schmidt, W., Seo, E., Sina, R., Sokolskaya, N., Wang, J., Wefel, J., Wu, J., & Zatsepin, V. (2005). Simulation of the ATIC-2 silicon matrix for protons and helium GCR Primaries at 0.3, 10, and 25 TeV/nucleon. 29th International Cosmic Ray Conference, ICRC 2005, 6, 89-92. Retrieved from https://repository.lsu.edu/physics_astronomy_pubs/5506