Nanosecond-level Time Synchronization Of Autonomous Radio Detector Stations For Extensive Air Showers

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dc.creatorE. J.; Al Samarai
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dc.creatorI. F. M.; Allekotte
dc.creatorI.; Allison
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dc.creatorR. Alves; Ambrosio
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dc.date2016
dc.datejan
dc.date2017-11-13T13:24:22Z
dc.date2017-11-13T13:24:22Z
dc.date.accessioned2018-03-29T05:56:53Z
dc.date.available2018-03-29T05:56:53Z
dc.identifierJournal Of Instrumentation. Iop Publishing Ltd, v. 11, p. , 2016.
dc.identifier1748-0221
dc.identifierWOS:000371469800106
dc.identifier10.1088/1748-0221/11/01/P01018
dc.identifierhttp://iopscience.iop.org/article/10.1088/1748-0221/11/01/P01018/meta
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/328281
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1365306
dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.descriptionTo exploit the full potential of radio measurements of cosmic-ray air showers at MHz frequencies, a detector timing synchronization within 1 ns is needed. Large distributed radio detector arrays such as the Auger Engineering Radio Array (AERA) rely on timing via the Global Positioning System (GPS) for the synchronization of individual detector station clocks. Unfortunately, GPS timing is expected to have an accuracy no better than about 5 ns. In practice, in particular in AERA, the GPS clocks exhibit drifts on the order of tens of ns. We developed a technique to correct for the GPS drifts, and an independent method is used to cross-check that indeed we reach a nanosecond-scale timing accuracy by this correction. First, we operate a "beacon transmitter" which emits defined sine waves detected by AERA antennas recorded within the physics data. The relative phasing of these sine waves can be used to correct for GPS clock drifts. In addition to this, we observe radio pulses emitted by commercial airplanes, the position of which we determine in real time from Automatic Dependent Surveillance Broadcasts intercepted with a software-defined radio. From the known source location and the measured arrival times of the pulses we determine relative timing offsets between radio detector stations. We demonstrate with a combined analysis that the two methods give a consistent timing calibration with an accuracy of 2 ns or better. Consequently, the beacon method alone can be used in the future to continuously determine and correct for GPS clock drifts in each individual event measured by AERA.
dc.description11
dc.descriptionComision Nacional de Energia Atomica, Argentina
dc.descriptionAgencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Argentina
dc.descriptionConsejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Argentina
dc.descriptionGobierno de la Provincia de Mendoza, Argentina
dc.descriptionMunicipalidad de Malargue, Argentina
dc.descriptionNDM Holdings, Argentina
dc.descriptionValle Las Lenas, Argentina
dc.descriptionAustralian Research Council [DP150101622]
dc.descriptionConselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Brazil
dc.descriptionFinanciadora de Estudos e Projetos (FINEP), Brazil
dc.descriptionFundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Brazil
dc.descriptionSao Paulo Research Foundation (FAPESP), Brazil [2010/07359-6, 1999/05404-3]
dc.descriptionMinisterio de Ciencia e Tecnologia (MCT), Brazil
dc.descriptionCzech Science Foundation, Czech Republic [14-17501S]
dc.descriptionCentre de Calcul IN2P3/CNRS, France
dc.descriptionCentre National de la Recherche Scientifique (CNRS), France
dc.descriptionConseil Regional Ile-de-France, France
dc.descriptionDepartement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), France
dc.descriptionDepartement Sciences de l'Univers (SDU-INSU/CNRS), France
dc.descriptionInstitut Lagrange de Paris (ILP) within the Investissements d'Avenir Programme, France [LABEX ANR-10-LABX-63, ANR-11-IDEX-0004-02]
dc.descriptionBundesministerium fur Bildung und Forschung (BMBF), Germany
dc.descriptionDeutsche Forschungsgemeinschaft (DFG), Germany
dc.descriptionFinanzministerium Baden-Wurttemberg, Germany
dc.descriptionHelmholtz Alliance for Astroparticle Physics (HAP), Germany
dc.descriptionHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Germany
dc.descriptionMinisterium fur Wissenschaft und Forschung, Nordrhein Westfalen, Germany
dc.descriptionMinisterium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany
dc.descriptionIstituto Nazionale di Fisica Nucleare (INFN), Italy
dc.descriptionIstituto Nazionale di Astrofisica (INAF), Italy
dc.descriptionMinistero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy
dc.descriptionGran Sasso Center for Astroparticle Physics (CFA), Italy
dc.descriptionCETEMPS Center of Excellence, Ministero degli Affari Esteri (MAE), Italy
dc.descriptionConsejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico
dc.descriptionMinisterie van Onderwijs, Cultuur en Wetenschap, Netherlands
dc.descriptionNederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands
dc.descriptionStichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands
dc.descriptionNational Centre for Research and Development, Poland [ERA-NET-ASPERA/01/11, ERA-NET-ASPERA/02/11]
dc.descriptionNational Science Centre, Poland [2013/08/M/ST9/00322, 2013/08/M/ST9/00728, HARMONIA 5 - 2013/10/M/ST9/00062]
dc.descriptionPortuguese national funds, Portugal
dc.descriptionFEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE), Portugal
dc.descriptionRomanian Authority for Scientific Research ANCS, CNDI-UEFISCDI partnership projects, Romania [20/2012, 194/2012, 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, PN-II-RU-PD-2011-3-0062]
dc.descriptionMinister of National Education, Programme Space Technology and Advanced Research (STAR), Romania [83/2013]
dc.descriptionSlovenian Research Agency, Slovenia
dc.descriptionComunidad de Madrid, Spain
dc.descriptionFEDER funds, Spain
dc.descriptionMinisterio de Educacion y Ciencia, Spain
dc.descriptionXunta de Galicia, Spain
dc.descriptionEuropean Community 7th Framework Program, Spain [FP7-PEOPLE-2012-IEF-328826]
dc.descriptionScience and Technology Facilities Council, United Kingdom
dc.descriptionDepartment of Energy, U.S.A. [DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107, DE-SC0011689]
dc.descriptionNational Science Foundation, U.S.A. [0450696]
dc.descriptionGrainger Foundation, U.S.A.
dc.descriptionNAFOSTED, Vietnam
dc.descriptionMarie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program [PIRSES-2009-GA-246806]
dc.descriptionUNESCO
dc.description[MSMT-CR LG13007]
dc.description[7AMB14AR005]
dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.languageEnglish
dc.publisherIOP Publishing Ltd
dc.publisherBristol
dc.relationJournal of Instrumentation
dc.rightsfechado
dc.sourceWOS
dc.subjectPattern Recognition, Cluster Finding, Calibration And Fitting Methods
dc.subjectTiming Detectors
dc.subjectDetector Alignment And Calibration Methods (lasers, Sources, Particle-beams)
dc.titleNanosecond-level Time Synchronization Of Autonomous Radio Detector Stations For Extensive Air Showers
dc.typeArtículos de revistas


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