Unraveling the Cosmic-ray Spectrum: Measurements with high altitude Balloons
Patrick (Jojo) Boyle
McGill University

The balloon-borne cosmic-ray detector TRACER ("Transition Radiation for Cosmic Radiation") was designed to measure cosmic-ray nuclei with single element resolution up to high energies, and to facilitate a large geometric aperture by utilizing a transition radiation detector. TRACER was launched in two long-duration balloon flights, in Antarctica (2003), and subsequently, after significant upgrades, from Kiruna, Sweden (2006). The data cover the elements from boron (Z=5) to iron (Z=26), and reach energies in excess of 1014 eV/ particle. The results provide constraints on the elemental abundance and spectral slope at the cosmic-ray source and on the propagation of cosmic rays through the interstellar medium. Here, I will discuss what it takes to fly the largest and heaviest cosmic-ray detector ever flown on a high-altitude balloon. I will present new results on the abundance of secondary elements such as boron, and will discuss our results with an eye on the recent gamma-ray measurements of supernova remnants by FERMI and VERITAS. Finally, I will briefly discuss the potential of the TRACER technique for future investigations.

Date:	Mardi, 30 mars 2010
Time:	16:00
Where:	McGill University
	Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
Contact:	Robert Rutledge