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15 Jun 2011 1IEKP, Karlsruher Institut für Technologie, KIT, Germany 2Observatorio Pierre Auger, Av. San Martin Norte 304, 5613 Malargüe, Argentina *A full author list and affiliations can be found at http://www.auger.org/archive/authors_2010_10.html As an introduction, in this article we will summarize the main results from the first generation of radio detection experiments: LOPES and CODALEMA. Then, we will show which questions concerning the radio emission mechanisms can be answered from larger-scale experiments like the Auger Engineering Radio Array (AERA), which is a 20 km2 antenna array under construction close to other enhancement devices at the Pierre Auger Observatory. Citation: Maximilien Melissas1 for the Pierre AUGER Collaboration2,*: Overview of radio detection of cosmic ray air showers in the MHz range, and prospects for a large scale experiment, Astrophys. Space Sci. Trans., 7, 207-210, doi:10.5194/astra-7-207-2011, 2011.
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