Authors

A. Aab, Universität SiegenFollow
P. Abreu, Instituto Superior TécnicoFollow
M. Aglietta, Università degli Studi di TorinoFollow
E. J. Ahn, Fermi National Accelerator LaboratoryFollow
I. Al Samarai, Institut de Physique Nucléaire d’OrsayFollow
I. F.M. Albuquerque, Universidade de São PauloFollow
I. Allekotte, Instituto BalseiroFollow
P. Allison, The Ohio State UniversityFollow
A. Almela, Universidad Tecnologica Nacional
J. Alvarez Castillo, Universidad Nacional Autónoma de MéxicoFollow
J. Alvarez-Muñiz, Universidad de Santiago de CompostelaFollow
R. Alves Batista, Universität HamburgFollow
M. Ambrosio, Università degli Studi di Napoli Federico IIFollow
A. Aminaei, Radboud UniversiteitFollow
G. A. Anastasi, Università degli Studi di CataniaFollow
L. Anchordoqui, Lehman CollegeFollow
S. Andringa, Instituto Superior TécnicoFollow
C. Aramo, Università degli Studi di Napoli Federico II
F. Arqueros, Universidad Complutense de Madrid
N. Arsene, Universitatea din Bucuresti
H. Asorey, Instituto Balseiro
P. Assis, Instituto Superior Técnico
J. Aublin, Laboratoire de Physique Nucléaire et de Hautes Energies
G. Avila, Comision Nacional de Energia Atomica Argentina
N. Awal, New York University
A. M. Badescu, University Politehnica of Bucharest
C. Baus, Karlsruher Institut für Technologie
J. J. Beatty, The Ohio State University
K. H. Becker, Bergische Universität Wuppertal
J. A. Bellido, The University of Adelaide
C. Berat, Universite Grenoble Alpes
M. E. Bertaina, Università degli Studi di Torino
X. Bertou, Instituto Balseiro

Document Type

Article

Publication Date

6-14-2016

Abstract

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.

Publication Source (Journal or Book title)

Physical Review Letters

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