About: Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth

Facets (new session)
Description
Metadata
Settings
- owl:sameAs
- Inference Rule:

About: Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth Goto Sponge NotDistinct Permalink

An Entity of Type : http://linked.opendata.cz/ontology/domain/vavai/Vysledek, within Data Space : linked.opendata.cz associated with source document(s)

Attributes	Values
rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
rdfs:seeAlso	http://dx.doi.org/10.1103/PhysRevD.90.012012
Description	The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60 degrees and different energies of the primary particle. From these distributions, we define X-max(mu) as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of X-max(mu) as a useful observable to infer the mass composition of ultrahigh-energy cosmic rays. Likewise, we assess its ability to constrain hadronic interaction models. The surface detector array of the Pierre Auger Observatory provides information about the longitudinal development of the muonic component of extensive air showers. Using the timing information from the flash analog-to-digital converter traces of surface detectors far from the shower core, it is possible to reconstruct a muon production depth distribution. We characterize the goodness of this reconstruction for zenith angles around 60 degrees and different energies of the primary particle. From these distributions, we define X-max(mu) as the depth along the shower axis where the production of muons reaches maximum. We explore the potentiality of X-max(mu) as a useful observable to infer the mass composition of ultrahigh-energy cosmic rays. Likewise, we assess its ability to constrain hadronic interaction models. (en)
Title	Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth (en)
skos:prefLabel	Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth (en)
skos:notation	RIV/00216208:11320/14:10283721!RIV15-MSM-11320___
http://linked.open...avai/riv/aktivita	I P
http://linked.open...avai/riv/aktivity	I, P(7AMB14AR005), P(ED2.1.00/03.0058), P(GA14-17501S), P(LG13007)
http://linked.open...iv/cisloPeriodika	1
http://linked.open...vai/riv/dodaniDat	2015
http://linked.open...aciTvurceVysledku	Novotný, Vladimír Nosek, Dalibor
http://linked.open.../riv/druhVysledku	J - Článek v odborném periodiku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Univerzita Karlova v Praze / Matematicko-fyzikální fakulta
http://linked.open...dnocenehoVysledku	31164
http://linked.open...ai/riv/idVysledku	RIV/00216208:11320/14:10283721
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	system; model; cosmic-rays; surface detector array (en)
http://linked.open.../riv/klicoveSlovo	cosmic-rays surface detector array model system
http://linked.open...odStatuVydavatele	US - Spojené státy americké
http://linked.open...ontrolniKodProRIV	[4F603C9B935D]
http://linked.open...i/riv/nazevZdroje	Physical Review D - Particles, Fields, Gravitation and Cosmology
http://linked.open...in/vavai/riv/obor	BF
http://linked.open...ichTvurcuVysledku	2 (xsd:int)
http://linked.open...cetTvurcuVysledku	487 (xsd:int)
http://linked.open...vavai/riv/projekt	Možnosti využití astronomických celooblohových kamer Participation of the Czech Republic in the Pierre Auger Observatory Regional Centre of Advanced Technologies and Materials Properties of Ultra-High Energy Cosmic Rays
http://linked.open...UplatneniVysledku	2014
http://linked.open...v/svazekPeriodika	90
http://linked.open...iv/tvurceVysledku	Abreu, P. Aglietta, M. Novotný, Vladimír Ave, M. Ahlers, M. Nosek, Dalibor Allekotte, I. Aublin, J. Aab, A. Ahn, EJ Al Samarai, I. Albuquerque, IFM Allen, J. Allison, P. Almela, A. Ambrosio, M. Aminaei, A. Anchordoqui, L. Andringa, S. Aramo, C. Arqueros, F. Asorey, H. Assis, P. Avenier, M. Avila, G. Badescu, A. M. Barber, KB Batista, R. A. Bauml, J. Baus, C. Castillo, J. A. Alvarez-Munniz, J.
http://linked.open...ain/vavai/riv/wos	000339922100001
issn	1550-7998
number of pages	12 (xsd:int)
http://bibframe.org/vocab/doi	10.1103/PhysRevD.90.012012
http://localhost/t...ganizacniJednotka	11320

Faceted Search & Find service v1.16.116 as of Feb 22 2024

Alternative Linked Data Documents: ODE Content Formats:

RDF

ODATA

Microdata

About

OpenLink Virtuoso version 07.20.3239 as of Feb 22 2024, on Linux (x86_64-pc-linux-gnu), Single-Server Edition (126 GB total memory, 80 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software