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000618851 1001_ $$0P:(DE-HGF)0$$aScholten, O.$$b0$$eCorresponding author
000618851 245__ $$aAperture correction for beamforming in the radiometric detection of ultrahigh energy cosmic rays
000618851 260__ $$aRidge, NY$$bAmerican Physical Society$$c2024
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000618851 500__ $$aAccepted for publication in Phys. Rev. D
000618851 520__ $$aFor high-energy cosmic-ray physics, it is imperative to determine the mass and energy of the cosmic ray that initiated the air shower in the atmosphere. This information can be extracted from the longitudinal profile of the air shower. In radio-metric observations, this profile is customarily determined through an extensive fitting procedure where calculated radio intensity is fitted to data. Beamforming the measured signals offers a promising alternative to bypass the cumbersome fitting procedure and to determine the longitudinal profile directly. Finite aperture effects in beamforming hamper the resolution with which this profile can be determined. We present a comprehensive investigation of the beamforming resolution in radiometric observations of air showers. There are two, principally different, approaches possible in air-shower beamforming, one where the total beamforming intensity is determined and an alternative where the beamforming trace is cross-correlated with a known response function. The effects due to a finite aperture (size of antenna array and bandwidth) are large for both approaches. We argue that it is possible to correct for the aperture corrections using an unfolding procedure. We give an explicit expression for the folding function, the kernel. Being able to calculate the folding function allows for unfolding the finite aperture effects from the data. We show that, in a model-to-model comparison, this allows for an accurate reconstruction of the current profile as the shower develops in the atmosphere. We present also an example where we reconstruct the longitudinal current profile of a shower developing under thunderstorm conditions where the atmospheric electric fields greatly alter the orientation of the transverse current in the shower front.
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000618851 536__ $$0G:(EU-Grant)805486$$aRadNu - Radio detection of the PeV - EeV cosmic-neutrino flux (805486)$$c805486$$fERC-2018-STG$$x2
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000618851 693__ $$0EXP:(DE-H253)RNO-G-20230101$$5EXP:(DE-H253)RNO-G-20230101$$eThe Radio Neutrino Observatory in Greenland$$x0
000618851 7001_ $$0P:(DE-HGF)0$$aTrinh, T. N. G.$$b1$$eCorresponding author
000618851 7001_ $$aBuitink, S.$$b2
000618851 7001_ $$00000-0001-5992-6228$$aCorstanje, A.$$b3
000618851 7001_ $$00000-0001-5138-1235$$aHare, B. M.$$b4
000618851 7001_ $$00000-0002-2783-4772$$aHuege, T.$$b5
000618851 7001_ $$00000-0002-2639-0049$$aJhansi, B. V.$$b6
000618851 7001_ $$aMulrey, K.$$b7
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000618851 7001_ $$00000-0002-8999-9249$$aSchoorlemmer, H.$$b9
000618851 7001_ $$00000-0002-7066-3614$$aThoudam, S.$$b10
000618851 7001_ $$00009-0006-1262-7507$$aTurekova, P.$$b11
000618851 7001_ $$ade Vries, K.$$b12
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000618851 7870_ $$0PUBDB-2025-00510$$aScholten, Celine Xenia Rosinda et.al.$$d2024$$iIsParent$$rarXiv:2411.12324$$tAperture correction for beamforming in the radiometric detection of ultrahigh energy cosmic rays
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000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.physrep.2016.02.001
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1038/nature16976
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2007.11.012
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.90.082003
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1063/1.4807534
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2011.10.005
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.22323/1.444.0425
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevLett.132.021001
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.109.022002
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.97.023005
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.108.083041
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1029/2019JD031433
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.105.063027
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1051/0004-6361:20079218
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1140/epjc/s10052-021-08912-4
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1140/epjc/s10052-021-09925-9
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.22323/1.444.0380
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1029/2019JD032273
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1029/2020JD034309
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.104.063022
000618851 999C5 $$1J. A. Högbom$$2Crossref$$oJ. A. Högbom 1974$$y1974
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2012.07.007
000618851 999C5 $$1G. Askaryan$$2Crossref$$oG. Askaryan 1962$$y1962
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2008.04.004
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.22323/1.444.0380
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1051/0004-6361/201220873
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.22323/1.215.0174
000618851 999C5 $$1T. K. Gaisser$$2Crossref$$oT. K. Gaisser International Cosmic Ray Conference 1977$$tInternational Cosmic Ray Conference$$y1977
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2010.10.002
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1088/1475-7516/2019/03/018
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.95.083004
000618851 999C5 $$1D. S. Briggs$$2Crossref$$oD. S. Briggs Synthesis Imaging in Radio Astronomy II 1999$$tSynthesis Imaging in Radio Astronomy II$$y1999
000618851 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1093/mnras/stu1494