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Calibration of the Whipple atmospheric Čerenkov telescope

✍ Scribed by A.C. Rovero; J.H. Buckle; P. Fleury; Y. Jiang; E. Pare; X. Sarazin; M. Urban; T.C. Weekes

Book ID
108029367
Publisher
Elsevier Science
Year
1996
Tongue
English
Weight
618 KB
Volume
5
Category
Article
ISSN
0927-6505

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High energy muons generated by air showers can be detected with atmospheric Cerenkov imaging telescopes via their ring signature. The distribution of (~erenkov light along the ring is a function only of the muon's distance of impact from the telescope: this property makes possible the calibration of