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THE RADIO SIGNAL FROM EXTENSIVE AIR SHOWERS
"... The field of ultra-high energy cosmic rays made a lot of progresses last years with large area experiments such as the Pierre Auger Observatory, HiRes and the Telescope Array. A suppression of the cosmic ray flux at energies above 5.5 × 1019 eV is observed at a very high level of significance but th ..."
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V on primary photons and neutrinos and primary cosmic rays are expected to be hadrons. Identifying the precise composition (light or heavy nuclei) will permit to solve the puzzle. It has been proven that the radio signal emitted by the extensive air showers initiated by ultra-high energy cosmic rays reflects
The LOPES Collaboration , Lateral distribution of the radio signal in extensive air showers measured with
, 2010
"... a b s t r a c t The antenna array LOPES is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and aims to measure and investigate radio pulses from extensive air showers. The coincident measurements allow us to reconstruct the electric field strength ..."
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Cited by 7 (1 self)
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a b s t r a c t The antenna array LOPES is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and aims to measure and investigate radio pulses from extensive air showers. The coincident measurements allow us to reconstruct the electric field strength
Radio Emission in Atmospheric Air Showers: First Measurements with LOPES-30
"... Abstract. When Ultra High Energy Cosmic Rays (UHECR) interact with particles in the Earth’s atmosphere, they produce a shower of secondary particles propagating towards the ground. LOPES-30 is an absolute calibrated array of dipole antennas investigating the radio emission from these showers in deta ..."
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in detail and clarifying if the technique is useful for large-scale applications. LOPES-30 is co-located and measure in coincidence with the air shower experiment KASCADE-Grande. Status and first measurements with LOPES-30 are presented. 1.
New measurements of cosmic ray air showers with the digital radio interferometer LOPES
, 2011
"... Abstract. LOPES is a digital radio interferometer which measures the radio emission of extensive cosmic ray air showers. It mainly consists of 30 dipole antennas installed in co-location with KASCADE-Grande at the Karlsruhe Institute of Technology (KIT) in Germany. KASCADE-Grande measures the secon ..."
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Abstract. LOPES is a digital radio interferometer which measures the radio emission of extensive cosmic ray air showers. It mainly consists of 30 dipole antennas installed in co-location with KASCADE-Grande at the Karlsruhe Institute of Technology (KIT) in Germany. KASCADE-Grande measures
Coll.): On noise treatment in radio measurements of cosmic ray air showers
- Nucl. Instr. Meth. A - ARENA proc. in press
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Precision measurements of cosmic ray air showers
, 2014
"... Supplemented with suitable buffering techniques, the low-frequency part of the SKA can be used as an ultra-precise detector for cosmic-ray air showers at very high energies. This would enable a wealth of scientific applications: the physics of the transition from Galactic to extragalactic cosmic ray ..."
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rays could be probed with very high precision mass measurements, hadronic interactions could be studied up to energies well beyond the reach of man-made particle accelerators, air shower tomography could be performed with very high spatial resolution exploiting the large instantaneous bandwith and very
Radio detection of cosmic ray air showers with the LOPES experiment
"... Abstract. In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance. In particular, the LOPES project has successfully implemented modern interferometric methods to measure radio emission from air showers. LOPES has confirmed that the emission is coherent a ..."
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Abstract. In the last few years, radio detection of cosmic ray air showers has experienced a true renaissance. In particular, the LOPES project has successfully implemented modern interferometric methods to measure radio emission from air showers. LOPES has confirmed that the emission is coherent
LOPES Detecting Radio Emission from Cosmic Ray Air Showers
"... Radio pulses emitted in the atmosphere during the air shower development of high-energy primary cosmic rays were measured during the late 1960ies in the frequency range from 2 MHz to 520 MHz. Mainly due to difficulties with radio interference these measurements ceased in the late 1970ies. LOFAR (Low ..."
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Radio pulses emitted in the atmosphere during the air shower development of high-energy primary cosmic rays were measured during the late 1960ies in the frequency range from 2 MHz to 520 MHz. Mainly due to difficulties with radio interference these measurements ceased in the late 1970ies. LOFAR
Results 11 - 20
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