Radio Morphing - towards a fast computation of the radio signal from air-showers
Over the last decades, radio detection of air showers has been established as a promising detection technique for ultrahigh-energy cosmic rays and neutrinos. Very large or dense antenna arrays are necessary to be proficient at collecting information about these particles and understanding their prop...
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2019-01-01
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doaj-fa62cbf9136741d0bf0d1286672015f22021-08-02T04:56:09ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-012160301210.1051/epjconf/201921603012epjconf_arena2018_03012Radio Morphing - towards a fast computation of the radio signal from air-showersZilles AnneMartineau-Huynh OlivierKotera KumikoTueros Matiasde Vries KrijnCarvalho WashingtonNiess ValentinOver the last decades, radio detection of air showers has been established as a promising detection technique for ultrahigh-energy cosmic rays and neutrinos. Very large or dense antenna arrays are necessary to be proficient at collecting information about these particles and understanding their properties accurately. The exploitation of such arrays requires to run massive air-shower simulations to evaluate the radio signal at each antenna position, taking into account features such as the ground topology. In order to reduce computational costs, we have developed a fast computation of the emitted radio signal on the basis of generic shower simulations, called Radio Morphing. The method consists in the calculation of the radio signal of any air-shower by i) a scaling of the electric-field amplitude of a reference air shower to the target shower, ii) an isometry on the simulated positions and iii) an interpolation of the radio pulse at the desired position. This technique enables one to gain many orders of magnitude in CPU time compared to a standard computation. In this contribution, we present this novel tool and explain its methodology. In particular, Radio Morphing will be a key element for the simulation chain of the Giant Radio Array for Neutrino Detection (GRAND) project, that aims at detecting ultra-high-energy neutrinos with an array of 200 000 radio antennas in mountainous regions.https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_03012.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Zilles Anne Martineau-Huynh Olivier Kotera Kumiko Tueros Matias de Vries Krijn Carvalho Washington Niess Valentin |
spellingShingle |
Zilles Anne Martineau-Huynh Olivier Kotera Kumiko Tueros Matias de Vries Krijn Carvalho Washington Niess Valentin Radio Morphing - towards a fast computation of the radio signal from air-showers EPJ Web of Conferences |
author_facet |
Zilles Anne Martineau-Huynh Olivier Kotera Kumiko Tueros Matias de Vries Krijn Carvalho Washington Niess Valentin |
author_sort |
Zilles Anne |
title |
Radio Morphing - towards a fast computation of the radio signal from air-showers |
title_short |
Radio Morphing - towards a fast computation of the radio signal from air-showers |
title_full |
Radio Morphing - towards a fast computation of the radio signal from air-showers |
title_fullStr |
Radio Morphing - towards a fast computation of the radio signal from air-showers |
title_full_unstemmed |
Radio Morphing - towards a fast computation of the radio signal from air-showers |
title_sort |
radio morphing - towards a fast computation of the radio signal from air-showers |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2019-01-01 |
description |
Over the last decades, radio detection of air showers has been established as a promising detection technique for ultrahigh-energy cosmic rays and neutrinos. Very large or dense antenna arrays are necessary to be proficient at collecting information about these particles and understanding their properties accurately. The exploitation of such arrays requires to run massive air-shower simulations to evaluate the radio signal at each antenna position, taking into account features such as the ground topology. In order to reduce computational costs, we have developed a fast computation of the emitted radio signal on the basis of generic shower simulations, called Radio Morphing. The method consists in the calculation of the radio signal of any air-shower by i) a scaling of the electric-field amplitude of a reference air shower to the target shower, ii) an isometry on the simulated positions and iii) an interpolation of the radio pulse at the desired position. This technique enables one to gain many orders of magnitude in CPU time compared to a standard computation. In this contribution, we present this novel tool and explain its methodology. In particular, Radio Morphing will be a key element for the simulation chain of the Giant Radio Array for Neutrino Detection (GRAND) project, that aims at detecting ultra-high-energy neutrinos with an array of 200 000 radio antennas in mountainous regions. |
url |
https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_03012.pdf |
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