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We have measured the cosmic ray spectrum at energies above eV 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 $3\times 10^{18}6\times 10^{19}$ eV.

生成讲解博客的中文版本

生成AI智能校验的中文版本