The development of a system to detect the radio-frequency (RF) pulse associated with extensive air showers of cosmic rays is described. This work was performed at the CASA/MIA array in Utah, with the intention of designing equipment that can be used in conjunction with the Auger Giant Array. A small subset of data (less than 40 out of a total of 600 hours of running time), taken under low-noise conditions, permitted upper limits to be placed on the rate for pulses accompanying showers of energies around $10^{17}$ eV
The Pierre Auger Observatory is exploring the potential of the radio detection technique to study ex...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
A project to detect the radio-frequency pulse associated with extensive air showers of cosmic rays i...
A prototype system for detecting radio pulses associated with extensive cosmic ray air showers is de...
International audienceThe radio detection technique has successfully been applied to the measurement...
Due to the very low flux, cosmic ray air shower studies at ultra high energy necessitate equipping v...
The Pierre Auger Observatory detects ultra-high energy cosmic rays by measuring extensive air shower...
AbstractThe measurement of microwave emission from air showers initiated by ultra-high energy cosmic...
Abstract: The southern Auger Observatory provides an excellent test bed to study the radio detection...
Abstract—Cosmic rays are energetic particles from outside the earth’s atmosphere. When a high energy...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
The Pierre Auger Observatory is exploring the potential of the radio detection technique to study ex...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
A project to detect the radio-frequency pulse associated with extensive air showers of cosmic rays i...
A prototype system for detecting radio pulses associated with extensive cosmic ray air showers is de...
International audienceThe radio detection technique has successfully been applied to the measurement...
Due to the very low flux, cosmic ray air shower studies at ultra high energy necessitate equipping v...
The Pierre Auger Observatory detects ultra-high energy cosmic rays by measuring extensive air shower...
AbstractThe measurement of microwave emission from air showers initiated by ultra-high energy cosmic...
Abstract: The southern Auger Observatory provides an excellent test bed to study the radio detection...
Abstract—Cosmic rays are energetic particles from outside the earth’s atmosphere. When a high energy...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
The Pierre Auger Observatory is exploring the potential of the radio detection technique to study ex...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...
Accepted for publication in JINST, 50 pages, 25 figuresInternational audienceThe Pierre Auger Observ...