Observations of Microwave Continuum Emission from Air Shower Plasmas
P. W. Gorham, N. G. Lehtinen, G. S. Varner, J. J. Beatty, A. Connolly,, P. Chen, M. E. Conde, W. Gai, C. Hast, C. L. Hebert, C. Miki, R. Konecny, J., Kowalski, J. Ng, J. G. Power, K. Reil, D. Saltzberg, B. T. Stokes, and D., Walz

TL;DR
This paper explores a novel microwave detection technique for ultra-high energy cosmic ray air showers, demonstrating initial experimental success and potential advantages over existing optical methods in continuous observation conditions.
Contribution
It presents the first experimental evidence of microwave emission from air shower plasmas and develops a prototype detector using satellite TV technology for cosmic ray detection.
Findings
Microwave emission from air ionized by high-energy particles was observed.
Follow-up experiments confirmed initial results with improved precision.
Prototype detectors show potential for continuous cosmic ray observation.
Abstract
We investigate a possible new technique for microwave measurements of ultra-high energy cosmic ray (UHECR) extensive air showers which relies on detection of expected continuum radiation in the microwave range, caused by free-electron collisions with neutrals in the tenuous plasma left after the passage of the shower. We performed an initial experiment at the AWA (Argonne Wakefield Accelerator) laboratory in 2003 and measured broadband microwave emission from air ionized via high energy electrons and photons. A follow-up experiment at SLAC (Stanford Linear Accelerator Center) in summer of 2004 confirmed the major features of the previous AWA observations with better precision and made additional measurements relevant to the calorimetric capabilities of the method. Prompted by these results we built a prototype detector using satellite television technology, and have made measurements…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Neutrino Physics Research
