Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9861107 | Physics Letters B | 2005 | 10 Pages |
Abstract
We have measured the cosmic ray spectrum at energies above 1017eV using the two air fluorescence detectors of the High Resolution Fly's Eye experiment operating in monocular mode. We describe the detector, PMT and atmospheric calibrations, and the analysis techniques for the two detectors. We fit the spectrum to models describing galactic and extragalactic sources. Our measured spectrum gives an observation of a feature known as the “ankle” near 3Ã1018eV, and strong evidence for a suppression near 6Ã1019eV.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
High Resolution Fly's Eye Collaboration High Resolution Fly's Eye Collaboration, R.U. Abbasi, T. Abu-Zayyad, J.F. Amman, G. Archbold, R. Atkins, J.A. Bellido, K. Belov, J.W. Belz, S.Y. Ben Zvi, D.R. Bergman, G.W. Burt, Z. Cao, R.W. Clay, B.C. Connolly,