@inproceedings{c59e4790141547dfa9b043217fc6b051,
title = "HIGH-ENERGY COSMIC RAYS: GALACTIC OR EXTRAGALACTIC?",
abstract = "The bulk of cosmic rays is assumed to be accelerated in our Milky Way, while the highest-energy particles in the Universe are attributed to extra-galactic sources. A transition is expected at energies around 1017 to 1018 eV. A new method is presented to measure the properties of cosmic rays in this energy region: the radio detection of air showers. And a comprehensive model is discussed to describe consistently the Galactic and extra-galactic components of cosmic rays from GeV energies up to ∼ 1020 eV.",
author = "H{\"o}randel, \{J{\"o}rg R.\} and A. Achterberg and S. Buitink and A. Corstanje and H. Falcke and A. Nelles and Rachen, \{J. P.\} and L. Rossetto and P. Schellart and O. Scholten and \{ter Veen\}, S. and S. Thoudam and Trinh, \{T. N.G.\} and \{van Vliet\}, A.",
note = "Funding Information: JRH is grateful to the organizers of the Vulcano workshop for their kind invitation and the great hospitality on the Vulcano island. Publisher Copyright: {\textcopyright} 2017 Istituto Nazionale di Fisica Nucleare. All rights reserved.; 16th Vulcano Workshop on Frontier objects in Astrophysics and Particle Physics, Vulcano 2016 ; Conference date: 22-05-2016 Through 28-05-2016",
year = "2017",
language = "British English",
series = "Frascati Physics Series",
pages = "95--102",
editor = "Roberto Fusco-Femiano and Giampaolo Mannocchi and Aldo Morselli and Trinchero, \{Gian Carlo\}",
booktitle = "Vulcano 2016 - Frontier Objects in Astrophysics and Particle Physics",
}