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Simulation of the ATIC-2 Silicon Matrix for Protons and Helium GCR Primaries at 0.3, 10, and 25 TeV/NucleonThe 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. The GEANT3 geometrical model of ATIC developed by the University of Maryland was combined with a GEANT4 application developed for the Deep Space Test Bed (DSTB) detector package. The new code included relatively minor modifications to completely describe the ATIC materials and a more detailed model of the Silicon Matrix detector. For this analysis all particles were started as a unidirectional beam at a single point near the center of the Silicon Matrix front surface. The point was selected such that each primary passed through at least two of the overlapping silicon pixels.
Document ID
20050215608
Acquisition Source
Marshall Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Watts, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Adams, J. H.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Bashindzhagyan, G.
(Louisiana State Univ. Baton Rouge, LA, United States)
Batkov, K. E.
(Moscow State Univ. Russia)
Chang, J.
(Max-Planck-Inst. fuer Aeronomie Lindau, Germany)
Christl, M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Fazely, A. R.
(Southern Univ. Baton Rouge, LA, United States)
Ganel, O.
(Southern Univ. Baton Rouge, LA, United States)
Gunasingha R. M.
(Southern Univ. Baton Rouge, LA, United States)
Guzik, T. G.
(Louisiana State Univ. Baton Rouge, LA, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2005
Subject Category
Solar Physics
Meeting Information
Meeting: 29th International Cosmic Ray Conference
Location: Pune
Country: India
Start Date: August 3, 2005
End Date: August 10, 2005
Distribution Limits
Public
Copyright
Public Use Permitted.
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