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 ...
Ultra-high-energy cosmic rays can be measured by short radio pulses in the MHz regime emitted by ext...
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to det...
Submitted to Phys. Rev. D ; see paper for full list of authorsInternational audienceThe Auger Engine...
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
Ultra-high-energy cosmic rays can be measured by short radio pulses in the MHz regime emitted by ext...
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to det...
Submitted to Phys. Rev. D ; see paper for full list of authorsInternational audienceThe Auger Engine...
We measure the energy emitted by extensive air showers in the form of radio emission in the frequenc...
Ultra-high-energy cosmic rays can be measured by short radio pulses in the MHz regime emitted by ext...
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to det...
Submitted to Phys. Rev. D ; see paper for full list of authorsInternational audienceThe Auger Engine...