A Cluster of Ultrahigh Energy Cosmic Rays
نویسنده
چکیده
Five ultrahigh energy cosmic rays in the combined AGASA and HiRes stereo data are analyzed to test whether they come from a single source. The quad above 37 EeV in the 94-event high energy dataset can be analyzed without considering magnetic dispersion. The probability that it is a chance association is 10. Assuming the source is continuous, the random magnetic deflections these UHECRs accumulated en route from their source can be used to estimate
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تاریخ انتشار 2005