Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.1869f&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
We present results on the spectra and relative abundances of C, N, and O nuclei in the cosmic radiation as measured from the Advanced Thin Ionization Calorimeter Balloon experiment (ATIC). 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 flight, investigation of the cosmic ray spectra from below 50 GeV to near 100 TeV total energy, using a fully active Bismuth Germanate calorimeter. It is equipp ed 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 ho doscopes were employed, above, in the middle and below a 0.75 nuclear interaction length graphite target.
Adams James H. Jr.
Ahn H. S.
Bashindzhagyan George
Batkov K. E.
Chang Jaewan
No associations
LandOfFree
Relative Abundances and Energy Spectra of C, N, and O as Measured by the Advanced Thin Ionization Calorimeter Balloon Experiment does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Relative Abundances and Energy Spectra of C, N, and O as Measured by the Advanced Thin Ionization Calorimeter Balloon Experiment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relative Abundances and Energy Spectra of C, N, and O as Measured by the Advanced Thin Ionization Calorimeter Balloon Experiment will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1139634