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• W181725612 abstract "With the Akeno Giant Air Shower Array (AGASA), we published the small-scale anisotropy of cosmic rays with energies above 10 eV. Among them, a broad cluster n BC1 around (20 50 , 32 ) n has interesting characteristics: The time distribution of members of the BC1 cluster is burst-like around MJD50000 , and this cluster locates near the famous supernova remnant: the Cygnus Loop. From this BC1 direction, two observations from the Tibet and Milagro experiments have been reported. In this report, we summarize the results from the whole observation time of AGASA and the Akeno 1km array experiment, and the relation with the observations from the Tibet and Milagro experiments is discussed." @default.
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• W181725612 date "2005-01-01" @default.
• W181725612 modified "2023-09-27" @default.
• W181725612 title "A possible cosmic ray source in TeV and EeV from the direction around the Cygnus Loop" @default.
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