Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS

Since 2003, significant eﬀorts have been devoted to the understanding of the radio emission of extensive air shower in the range [20-200] MHz. Despite some studies led until the early nineties, the [1-10] MHz band has remained unused for 20 years. However, it has been measured by some pioneering exp...
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Autor*in:	Escudie Antony [verfasserIn] Charrier Didier [verfasserIn] Dallier Richard [verfasserIn] García-Fernández Daniel [verfasserIn] Lecacheux Alain [verfasserIn] Martin Lilian [verfasserIn] Revenu Benoît [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2019

Übergeordnetes Werk:	In: EPJ Web of Conferences - EDP Sciences, 2010, 210, p 05003(2019)
Übergeordnetes Werk:	volume:210, p 05003 ; year:2019

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.1051/epjconf/201921005003

Katalog-ID:	DOAJ055131832

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author	Escudie Antony
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topic_title	QC1-999 Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS
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title	Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS
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title_full	Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS
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title_sort	multi-wavelength observation of cosmic-ray air-showers with codalema/extasis
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title_auth	Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS
abstract	Since 2003, significant eﬀorts have been devoted to the understanding of the radio emission of extensive air shower in the range [20-200] MHz. Despite some studies led until the early nineties, the [1-10] MHz band has remained unused for 20 years. However, it has been measured by some pioneering experiments that extensive air shower emit a strong electric field in this band and that there is evidence of a large increase in the amplitude of the radio pulse at lower frequencies. The EXTASIS experiment, located within the Nançay Radioastronomy Observatory and supported by the CODALEMA experiment, aims to reinvestigate the [1-10] MHz band, and especially to study the so-called “Sudden Death” contribution, the expected electric field emitted by shower front when hitting the ground level. Currently, EXTASIS has confirmed some results obtained by the pioneering experiments, and tends to bring explanations to the other ones, for instance the role of the underlying atmospheric electric field. Moreover, CODALEMA has demonstrated that in the most commonly used frequency band ([20-80] MHz) the electric field profile of EAS can be well sampled, and contains all the information needed for the reconstruction of EAS: an automatic comparison between the SELFAS3 simulations and data has been developed, allowing us to reconstruct in an almost real time the primary cosmic ray characteristics.
abstractGer	Since 2003, significant eﬀorts have been devoted to the understanding of the radio emission of extensive air shower in the range [20-200] MHz. Despite some studies led until the early nineties, the [1-10] MHz band has remained unused for 20 years. However, it has been measured by some pioneering experiments that extensive air shower emit a strong electric field in this band and that there is evidence of a large increase in the amplitude of the radio pulse at lower frequencies. The EXTASIS experiment, located within the Nançay Radioastronomy Observatory and supported by the CODALEMA experiment, aims to reinvestigate the [1-10] MHz band, and especially to study the so-called “Sudden Death” contribution, the expected electric field emitted by shower front when hitting the ground level. Currently, EXTASIS has confirmed some results obtained by the pioneering experiments, and tends to bring explanations to the other ones, for instance the role of the underlying atmospheric electric field. Moreover, CODALEMA has demonstrated that in the most commonly used frequency band ([20-80] MHz) the electric field profile of EAS can be well sampled, and contains all the information needed for the reconstruction of EAS: an automatic comparison between the SELFAS3 simulations and data has been developed, allowing us to reconstruct in an almost real time the primary cosmic ray characteristics.
abstract_unstemmed	Since 2003, significant eﬀorts have been devoted to the understanding of the radio emission of extensive air shower in the range [20-200] MHz. Despite some studies led until the early nineties, the [1-10] MHz band has remained unused for 20 years. However, it has been measured by some pioneering experiments that extensive air shower emit a strong electric field in this band and that there is evidence of a large increase in the amplitude of the radio pulse at lower frequencies. The EXTASIS experiment, located within the Nançay Radioastronomy Observatory and supported by the CODALEMA experiment, aims to reinvestigate the [1-10] MHz band, and especially to study the so-called “Sudden Death” contribution, the expected electric field emitted by shower front when hitting the ground level. Currently, EXTASIS has confirmed some results obtained by the pioneering experiments, and tends to bring explanations to the other ones, for instance the role of the underlying atmospheric electric field. Moreover, CODALEMA has demonstrated that in the most commonly used frequency band ([20-80] MHz) the electric field profile of EAS can be well sampled, and contains all the information needed for the reconstruction of EAS: an automatic comparison between the SELFAS3 simulations and data has been developed, allowing us to reconstruct in an almost real time the primary cosmic ray characteristics.
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title_short	Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS
url	https://doi.org/10.1051/epjconf/201921005003 https://doaj.org/article/4dfd56f80f2543eaa0eb097a24b01db2 https://www.epj-conferences.org/articles/epjconf/pdf/2019/15/epjconf_uhecr18_05003.pdf https://doaj.org/toc/2100-014X
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author2	Charrier Didier Dallier Richard García-Fernández Daniel Lecacheux Alain Martin Lilian Revenu Benoît
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up_date	2024-07-04T01:55:04.676Z
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Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS

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