A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector

We have performed a detailed Monte Carlo (MC) calculation 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...

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Main Authors: Ahn, H. S., Guzik, T. G., Gunasingha, R. M., Batkov, K. E., Christl, M., Adams, J. H., Ganel, O., Chang, J., Fazely, A. R., Bashindzhagyan, G. L.
Format: Other/Unknown Material
Language:unknown
Published: 2006
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Online Access:http://hdl.handle.net/2060/20060047793
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:20060047793 2023-05-15T13:30:43+02:00 A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector Ahn, H. S. Guzik, T. G. Gunasingha, R. M. Batkov, K. E. Christl, M. Adams, J. H. Ganel, O. Chang, J. Fazely, A. R. Bashindzhagyan, G. L. Unclassified, Unlimited, Publicly available [2006] application/pdf http://hdl.handle.net/2060/20060047793 unknown Document ID: 20060047793 http://hdl.handle.net/2060/20060047793 Copyright, Distribution under U.S. Government purpose rights CASI Astrophysics 36th COSPAR Scientific Assembly; 16-23 Jul. 2006; Beijing; China 2006 ftnasantrs 2019-07-21T01:44:31Z We have performed a detailed Monte Carlo (MC) calculation 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 Bight, investigation of the cosmic ray spectra from below 50 GeV to near 100 TeV total energy; using a fully active Bismuth Germanate @GO) calorimeter. It is equipped with a large mosaic of silicon detector pixels capable of charge identification and as a particle tracking system, three projective layers of x-y scintillator hodoscopes were employed, above, in the middle and below a 0.75 nuclear interaction length graphite target. Our calculations are part of an analysis package of both A- and energy-dependences of different nuclei interacting with the ATIC detector. The MC simulates the responses of different components of the detector such as the Simatrix, the scintillator hodoscopes and the BGO calorimeter to various nuclei. We also show comparisons of the FLUKA-2005 MC calculations with a GEANT calculation and data for protons, He and CNO. Other/Unknown Material Antarc* Antarctica NASA Technical Reports Server (NTRS) Fluka ENVELOPE(17.567,17.567,66.017,66.017)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic Astrophysics
spellingShingle Astrophysics
Ahn, H. S.
Guzik, T. G.
Gunasingha, R. M.
Batkov, K. E.
Christl, M.
Adams, J. H.
Ganel, O.
Chang, J.
Fazely, A. R.
Bashindzhagyan, G. L.
A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector
topic_facet Astrophysics
description We have performed a detailed Monte Carlo (MC) calculation 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 Bight, investigation of the cosmic ray spectra from below 50 GeV to near 100 TeV total energy; using a fully active Bismuth Germanate @GO) calorimeter. It is equipped with a large mosaic of silicon detector pixels capable of charge identification and as a particle tracking system, three projective layers of x-y scintillator hodoscopes were employed, above, in the middle and below a 0.75 nuclear interaction length graphite target. Our calculations are part of an analysis package of both A- and energy-dependences of different nuclei interacting with the ATIC detector. The MC simulates the responses of different components of the detector such as the Simatrix, the scintillator hodoscopes and the BGO calorimeter to various nuclei. We also show comparisons of the FLUKA-2005 MC calculations with a GEANT calculation and data for protons, He and CNO.
format Other/Unknown Material
author Ahn, H. S.
Guzik, T. G.
Gunasingha, R. M.
Batkov, K. E.
Christl, M.
Adams, J. H.
Ganel, O.
Chang, J.
Fazely, A. R.
Bashindzhagyan, G. L.
author_facet Ahn, H. S.
Guzik, T. G.
Gunasingha, R. M.
Batkov, K. E.
Christl, M.
Adams, J. H.
Ganel, O.
Chang, J.
Fazely, A. R.
Bashindzhagyan, G. L.
author_sort Ahn, H. S.
title A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector
title_short A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector
title_full A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector
title_fullStr A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector
title_full_unstemmed A Detailed FLUKA-2005 Monte Carlo Simulation for the ATIC Detector
title_sort detailed fluka-2005 monte carlo simulation for the atic detector
publishDate 2006
url http://hdl.handle.net/2060/20060047793
op_coverage Unclassified, Unlimited, Publicly available
long_lat ENVELOPE(17.567,17.567,66.017,66.017)
geographic Fluka
geographic_facet Fluka
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source CASI
op_relation Document ID: 20060047793
http://hdl.handle.net/2060/20060047793
op_rights Copyright, Distribution under U.S. Government purpose rights
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