CHEP Particle Astrophysics Seminar
TRACER (Transition Radiation Array for Cosmic Energetic
Radiation)
Patrick (Jojo) Boyle
Kavli Institute for Cosmological Physics University of
Chicago
The individual energy spectra of heavy cosmic rays are poorly known above
a TeV/nucleon. At these energies cosmic rays carry an important imprint of
the acceleration and propagation mechanisms allowing one to probe possible
sources of these cosmic rays. Extending the energy range will also enable
overlap with measurements from the ground, allowing for a more definitive
understanding of air-shower development.
TRACER is currently the largest detector system for direct measurements
of cosmic-ray nuclei on balloons. In a 14 day Antarctic balloon flight
TRACER has extended the energy spectra of heavy cosmic ray nuclei to beyond
1014 eV per particle.
In this talk I will discuss TRACER in terms of design and performance
and will compare our results with previous measurements in space and on
balloons, with interpretations of air shower data and also constraints on
models of cosmic-ray propagation through the Galaxy. TRACER is currently
being readied for an additional flight around the Arctic Circle in 2006.
Wednesday, November 23rd 2005, 15:30
Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
|