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Energy Spectra of H and He from the ATIC-2 ExperimentThe Advanced Thin Ionization Calorimeter (ATIC) experiment measures the energy spectra of individual elements, from H to Fe, in the energy region from about 100 GeV to tens of TeV. The ATIC instrument was flown twice in long-duration balloon flights around the South Pole in 2000-2001 (ATIC-1) and 2002-2003 (ATIC-2). ATIC-2 gathered about 18 days of data at an altitude of 36 km. In this paper we discuss the separation of protons from helium and present preliminary energy spectrum of each component, including deconvolution of the measured energy deposit spectra. The results are compared to previous data and to different cosmic ray propagation models, including a diffusion model with weak re-acceleration.
Document ID
20050215459
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Wefel, J. P.
(Louisiana State Univ. Baton Rouge, LA, United States)
Adams, J. H.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ahn, H. S.
(Maryland Univ. College Park, MD, United States)
Bashindzhagyan, G. L.
(Moscow State Univ. Russia)
Batkov, K. E.
(Moscow State Univ. Russia)
Chang, J.
(Max-Planck-Inst. for Solar System Research 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.
(Maryland Univ. College Park, MD, United States)
Gunasingha, R. M.
(Southern Univ. Baton Rouge, LA, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2005
Publication Information
Publication: 29th International Cosmic Ray Conference
Subject Category
Nuclear 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
Other

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