Measurement of the Muon Production Depths at the Pierre Auger Observatory
- INFN, Turin (Italy). et al.
The muon content of extensive air showers is an observable sensitive to the primary composition and to the hadronic interaction properties. The Pierre Auger Observatory uses water-Cherenkov detectors to measure particle densities at the ground and therefore is sensitive to the muon content of air showers. We present here a method which allows us to estimate the muon production depths by exploiting the measurement of the muon arrival times at the ground recorded with the Surface Detector of the Pierre Auger Observatory. The analysis is performed in a large range of zenith angles, thanks to the capability of estimating and subtracting the electromagnetic component, and for energies between $$10^{19.2}$$ and $$10^{20}$$ eV.
- Research Organization:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- Contributing Organization:
- Pierre Auger Collaboration
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1327018
- Report Number(s):
- FERMILAB-PUB--16-356-AD-AE-CD-TD; arXiv:1609.02498; 1485682
- Journal Information:
- European Physical Journal Plus, Journal Name: European Physical Journal Plus Vol. 131; ISSN 2190-5444
- Publisher:
- SpringerCopyright Statement
- Country of Publication:
- United States
- Language:
- English
| Open Questions in Cosmic-Ray Research at Ultrahigh Energies 
 | text | January 2019 | 
| Open Questions in Cosmic-Ray Research at Ultrahigh Energies 
 | journal | June 2019 | 
| Open Questions in Cosmic-Ray Research at Ultrahigh Energies 
 | text | January 2019 | 
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