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Observation of the Shadowing of Cosmic Rays by the Moon using a Deep Underground Detector by The MACRO Collaboration; al, M. Ambrosio et is a scholarly article available to read on EtoBox.

What is Observation of the Shadowing of Cosmic Rays by the Moon using a Deep Underground Detector about?

Using data collected by the MACRO experiment during the years 1989-1996, we show evidence for the shadow of the moon in the underground cosmic ray flux with a significance of 3.6 sigma. This detection of the shadowing effect is the first by an underground detector. A maximum-likelihood analysis is used to determine that the angular resolution of the apparatus is 0.9+/-0.3 degrees. These results demonstrate MACRO's capabilities as a muon telescope by confirming its absolute pointing ability and quantifying its angular resolution.

Author
The MACRO Collaboration; al, M. Ambrosio et
Published
1998
Language
EN

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