Thunderstorm observations by air-shower radio antenna arrays

@article{Apel2011ThunderstormOB,
  title={Thunderstorm observations by air-shower radio antenna arrays},
  author={W-D. Apel and Juan Carlos Arteaga and L. Bahren and K. Bekk and Mario Edoardo Bertaina and Peter L. Biermann and Johannes Blumer and H. Bozdog and I. Brancus and Peter Buchholz and Stijn Buitink and Elena Cantoni and Andrea Chiavassa and Kai Daumiller and Vitor de Souza and P. Doll and Moses Ender and Ralph Engel and Heino Falcke and Marcelo Finger and Daniel R. Fuhrmann and Hartmut Gemmeke and Claus Grupen and Andreas Haungs and D. Heck and Jorg R. Horandel and Andreas Horneffer and Daniel Huber and T. Huege and Paula Gina Isar and K-H. Kampert and D. Kang and Oliver Kromer and Jan Kuijpers and Katrin Link and P. Luczak and Marianne Ludwig and H. J. Mathes and Maximilien Melissas and Carlo Morello and S. Nehls and J. Oehlschlager and N. Palmieri and Tanguy Pierog and Julian Rautenberg and Heinigerd Rebel and Markus Roth and Christoph Ruhle and A. Saftoiu and Harald Schieler and Adrian Schmidt and Frank G. Schroder and Octavian Sima and G. Toma and G. C. Trinchero and Andreas Weindl and J{\"u}rgen Wochele and Michael Wommer and Janusz Zabierowski and J. Anton Zensus},
  journal={Advances in Space Research},
  year={2011},
  volume={48},
  pages={1295-1303}
}

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References

SHOWING 1-10 OF 36 REFERENCES
Amplified radio emission from cosmic ray air showers in thunderstorms
Context. The detection of radio pulses from cosmic ray air showers is a potentially powerful new detection mechanism for studying spectrum and composition of ultra high energy cosmic rays that needs
Measuring the radio emission of cosmic ray air showers with LOPES
Detection and imaging of atmospheric radio flashes from cosmic ray air showers
TLDR
The results show that it should be possible to determine the nature and composition of UHECRs with combined radio and particle detectors, and to detect the ultrahigh-energy neutrinos expected from flavour mixing.
High energy cosmic ray particles and the most powerful discharges in thunderstorm atmosphere
Observations of lightning phenomena using radio interferometry
A radio interferometer system is described which utilizes multiple baselines to determine the direction of lightning radiation sources with an angular resolution of a few degrees and with microsecond
Energy spectrum and mass composition of high-energy cosmic rays
Primary cosmic rays above energies of about 100 TeV are investigated by observations of extensive air showers (EAS) using large area ground based detector installations for registering various
Diffusion of relativistic runaway electrons and implications for lightning initiation
[1] Using detailed Monte Carlo simulations, the diffusion coefficients for relativistic runaway electron avalanches in air are found for the range of electric field strengths applicable to
...
...