Journal ArticleThe Utah Fly's Eye detector has revealed a change in the cosmic ray composition which is correlated with structure in the all-particle energy spectrum. The data can be fitted by a simple model of a steep power law spectrum of heavy nuclei which is overtaken at high energies by a flatter spectrum of protons. The transition occurs near 10^18.5 eV. Anisotropy is not detected, so the high-rigidity particles above the transition energy do not originate in the disk of the Galaxy. An outstanding event of 3x10^20 eV implies that the highest energy particles originate in the contemporary era of the Universe
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...
Journal ArticleThe Utah Fly's Eye detector has revealed a change in the cosmic ray composition which...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
Journal ArticleWe report a measurement of the ultrahigh-energy cosmic-ray spectrum using an atmosphe...
Journal ArticleWe describe the current status of the High Resolution Fly's Eye detector. Event recon...
Journal ArticleWe have measured the cosmic ray spectrum above 1017.2 eV using the two air-fluorescen...
An erratum exists for this article. Please see the description link below for details.The average ma...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
We report recently analyzed results on the energy spectrum, and composition of cosmic rays above 0.3...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...
Journal ArticleThe Utah Fly's Eye detector has revealed a change in the cosmic ray composition which...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...
Journal ArticleWe report a measurement of the ultrahigh-energy cosmic-ray spectrum using an atmosphe...
Journal ArticleWe describe the current status of the High Resolution Fly's Eye detector. Event recon...
Journal ArticleWe have measured the cosmic ray spectrum above 1017.2 eV using the two air-fluorescen...
An erratum exists for this article. Please see the description link below for details.The average ma...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
We report recently analyzed results on the energy spectrum, and composition of cosmic rays above 0.3...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A brief review of the energy spectrum of primary cosmic rays above $10^{10}$ eV and the measurement ...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...