2008/01/03 by M. Ave, P. J. Boyle, F. Gahbauer +9
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Chemical composition #Composition (language) #Dark Matter and Cosmic Phenomena #Primary (astronomy) #Primary component #Radioactive Decay and Measurement Techniques #Spectral line #astro-ph
paper · pdf · doi:10.1086/529424
published as The Astrophysical Journal, 678:262-273, 2008 May 1 · Accepted for publication in the Astrophysical Journal (3-Jan-08), 37 pages, 15 figures
arxiv created 2008/01/03 · openalex publication_date 2008/04/28 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The TRACER instrument (Transition Radiation Array for Cosmic Energetic Radiation) has been developed for direct measurements of the heavier primary cosmic-ray nuclei at high energies. The instrument had a successful long-duration balloon flight in Antarctica in 2003. The detector system and measurement process are described, details of the data analysis are discussed, and the individual energy spectra of the elements O, Ne, Mg, Si, S, Ar, Ca, and Fe (nuclear charge Z = 8-26) are presented. The large geometric factor of TRACER and the use of a transition radiation detector make it possible to determine the spectra up to energies in excess of 10 14 eV per particle. A power-law fit to the individual energy spectra above 20 GeV amu −1 exhibits nearly the same spectral index (2.65 ± 0.05) for all elements, without noticeable dependence on the elemental charge Z .