scholarly journals Radio detection of Cosmic Rays with LOFAR

2016 ◽  
Author(s):  
Jörg Hörandel
Keyword(s):  
Cosmic Rays ◽  
Radio Detection

scholarly journals Radio detection of cosmic rays in [1.7–3.7] MHz: The EXTASIS experiment

2019 ◽  
Vol 113 ◽  
pp. 6-21
Author(s):  
D. Charrier ◽  
R. Dallier ◽  
Antony Escudie ◽  
D. García-Fernández ◽  
A. Lecacheux ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Radio Detection

scholarly journals Radio detection of cosmic rays with the Auger Engineering Radio Array

2019 ◽  
Vol 210 ◽  
pp. 05011 ◽  
Author(s):  
Tim Huege ◽  
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Cosmic Ray ◽  
Energy Scale ◽  
Pierre Auger Observatory ◽  
Mass Composition ◽  
Frequency Range ◽  
Radio Detection ◽  
Composition Measurements

The Auger Engineering Radio Array (AERA) complements the Pierre Auger Observatory with 150 radio-antenna stations measuring in the frequency range from 30 to 80 MHz. With an instrumented area of 17 km2, the array constitutes the largest cosmic-ray radio detector built to date, allowing us to do multi-hybrid measurements of cosmic rays in the energy range of 1017 eV up to several 1018 eV. We give an overview of AERA results and discuss the significance of radio detection for the validation of the energy scale of cosmicray detectors as well as for mass-composition measurements.

ARENA 2005 CONFERENCE SUMMARY

2006 ◽  
Vol 21 (supp01) ◽  
pp. 269-280
Author(s):  
JOHN G. LEARNED
Keyword(s):  
Neutrino Physics ◽  
Cosmic Rays ◽  
Cosmic Ray ◽  
High Energy ◽  
Communications Technology ◽  
Detection Techniques ◽  
Conference Summary ◽  
Radio Detection ◽  
Real Progress ◽  
Basic Ideas

This meeting, as the reader sees in the preceding written contributions, represented an exciting new step in a budding revolution in extremely high energy cosmic ray and neutrino physics. The focus upon acoustic and radio detection techniques, reveals a rapidly expanding interest and real progress. Most of the basic ideas have been known for many years, but it is only now that they are at last beginning to be exploited. The reasons for this are several, ranging from the advance of technology to scientific focus of the community. The former comes largely from electronics and communications technology progress. The latter comes about due to the "neutrino revolution" and the campaign to understand the highest energy (GZK) cosmic rays. At least 25 projects are in various stages of dreaming through construction. Positive detections would seem not far in the future.

scholarly journals Prospects for radio detection of ultra-high energy cosmic rays and neutrinos

2004 ◽  
Vol 48 (11-12) ◽  
pp. 1487-1510 ◽  
Author(s):  
H. Falcke ◽  
P. Gorham ◽  
R.J. Protheroe
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Ultra High Energy ◽  
High Energy Cosmic Rays ◽  
Radio Detection
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