Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory
Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detec...
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Published in | Journal of instrumentation Vol. 15; no. 10; p. P10021 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Bristol
IOP Publishing
01.10.2020
Institute of Physics (IOP) |
Subjects | |
Online Access | Get full text |
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Summary: | Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60ˆ using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers. |
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Bibliography: | arXiv:2007.09035; FERMILAB-PUB-20-487-AD-E-TD USDOE Office of Science (SC), High Energy Physics (HEP) National Science Foundation (NSF) The Grainger Foundation AC02-07CH11359; FG02-04ER41300; FG02-99ER41107; SC0011689; 0450696 |
ISSN: | 1748-0221 1748-0221 |
DOI: | 10.1088/1748-0221/15/10/P10021 |