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Development of Ultra High-Energy Cosmic Ray Research

  • Karl-Heinz KampertEmail author
  • Alan A. Watson

Abstract

The discovery of extensive air showers by Rossi, Schmeiser, Bothe, Kolhörster and Auger at the end of the 1930s, facilitated by the coincidence technique of Bothe and Rossi, led to fundamental contributions in the field of cosmic ray physics and laid the foundation for high-energy particle physics. Soon after World War II a cosmic ray group at MIT in the USA pioneered detailed investigations of air shower phenomena and their experimental skill laid the foundation for many of the methods and much of the instrumentation used today. Soon interests focused to the highest energies requiring much larger detectors to be operated. The first detection of air fluorescence light by Japanese and US groups in the early 1970s marked an important experimental breakthrough towards this end as it allowed huge volumes of atmosphere to be monitored by optical telescopes. Radio observations of air showers, pioneered in the 1960s, are presently experiencing a renaissance and may revolutionise the field again. In the last 7 decades the research has seen many ups but also a few downs. However, the example of the Cygnus X-3 story demonstrated that even non-confirmable observations can have a huge impact by boosting new instrumentation to make discoveries and shape an entire scientific community.

Keywords

Cloud Chamber Geiger Counter Telescope Array Shower Array Pierre Auger Observatory 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgements

We gratefully acknowledge stimulating discussions and generous support given by Luisa Bonolis, Antonella Castellina, Bruce Dawson, Piera Ghia, Antoine Letessier-Selvon, Maria Concetta Maccarone, Marco Segala, Mike Walter, and many other colleagues for helping us to access to some of the original key papers distributed in various archives around the world. KHK also acknowledges financial support by the German Ministry for Research and Education (BMBF) and by the Helmholtz Alliance for Astroparticle Physics and AAW acknowledges the UK Science and Technology Council and the Leverhalme Foundation.

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Authors and Affiliations

  1. 1.Department of PhysicsUniversity WuppertalWuppertalGermany
  2. 2.School of Physics and AstronomyUniversity of LeedsLeedsUK

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