Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/110180
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dc.contributor.authorAab, A.-
dc.contributor.authorAbreu, P.-
dc.contributor.authorAglietta, M.-
dc.contributor.authorAl Samarai, I.-
dc.contributor.authorAlbuquerque, I.-
dc.contributor.authorAllekotte, I.-
dc.contributor.authorAlmela, A.-
dc.contributor.authorCastillo, J.-
dc.contributor.authorAlvarez-Muiniz, J.-
dc.contributor.authorAnastasi, G.-
dc.contributor.authorAnchordoqui, L.-
dc.contributor.authorAndrada, B.-
dc.contributor.authorAndringa, S.-
dc.contributor.authorAramo, C.-
dc.contributor.authorArqueros, F.-
dc.contributor.authorArsene, N.-
dc.contributor.authorAsorey, H.-
dc.contributor.authorAssis, P.-
dc.contributor.authorAvila, G.-
dc.contributor.authorBadescu, A.-
dc.contributor.authoret al.-
dc.date.issued2017-
dc.identifier.citationJournal of Instrumentation, 2017; 12(10):T10005-1-T10005-37-
dc.identifier.issn1748-0221-
dc.identifier.issn1748-0221-
dc.identifier.urihttp://hdl.handle.net/2440/110180-
dc.description.abstractAn in-situ calibration of a logarithmic periodic dipole antenna with a frequency coverage of 30MHz to 80MHz is performed. Such antennas are part of a radio station system used for detection of cosmic ray induced air showers at the Engineering Radio Array of the Pierre Auger Observatory, the so-called Auger Engineering Radio Array (AERA). The directional and frequency characteristics of the broadband antenna are investigated using a remotely piloted aircraft carrying a small transmitting antenna. The antenna sensitivity is described by the vector effective length relating the measured voltage with the electric-field components perpendicular to the incoming signal direction. The horizontal and meridional components are determined with an overall uncertainty of 7.4⁺⁰·⁹ˍ₀ꓸ₃% and 10.3⁺²·⁸ˍ₁ꓸ₇% respectively. The measurement is used to correct a simulated response of the frequency and directional response of the antenna. In addition, the influence of the ground conductivity and permittivity on the antenna response is simulated. Both have a negligible influence given the ground conditions measured at the detector site. The overall uncertainties of the vector effective length components result in an uncertainty of 8.8⁺²·¹ˍ₁ꓸ₃% in the square root of the energy fluence for incoming signal directions with zenith angles smaller than 60.-
dc.description.statementofresponsibilityA. Aab … J.A. Bellido … S.G. Blaess … R.W. Clay … M.J. Cooper … B.R. Dawson … T.D. Grubb … T.A. Harrison … G.C. Hill … P.H. Nguyen … S.J. Saffi … J. Sorokin ... T. Sudholz … P. van Bodegom … [et al.] (The Pierre Auger Collaboration)-
dc.language.isoen-
dc.publisherInstitute of Physics-
dc.rights© 2017 IOP Publishing Ltd and Sissa Medialab-
dc.source.urihttp://dx.doi.org/10.1088/1748-0221/12/10/t10005-
dc.subjectAntennas; detector alignment and calibration methods (lasers, sources, particle-beams); large detector systems for particle and astroparticle physics; particle detectors-
dc.titleCalibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter-
dc.typeJournal article-
dc.identifier.doi10.1088/1748-0221/12/10/T10005-
dc.relation.grantARC-
pubs.publication-statusPublished-
dc.identifier.orcidBellido, J. [0000-0002-0833-9194]-
dc.identifier.orcidClay, R. [0000-0002-9040-9648]-
dc.identifier.orcidDawson, B. [0000-0002-4271-3055]-
Appears in Collections:Aurora harvest 3
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