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Hesser and T. Spies, Proc. ), ISBN 3-7739-5995-8, 261 (2004). R A D I O SIGNALS F R O M P H O T O N B E A M S IN S A N D A N D SALT D. GORHAM, E. GUILLIAN, R. C. FIELD, R. IVERSON, A. WALZ§ G. RESCH1 P. SCHOESSOW11 In this paper I describe the setup and results of two beamtests which demonstrated the existence and properties of the Askar'yan effect in sand and salt. We observed coherence, 100% linear polarization, and field strength in agreement with simulations. We also demonstrated the possibility of tracking the shower direction with polarization information.

Wong, DESY 05-165. E. Waxman and J. N. Bahcall, Phys. Rev. D 59 (1999) 023002. M. , J. Phys. G 18 (1992) 423. M. Takeda et al. ], Phys. Rev. Lett. 81 (1998) 1163; Astropart. Phys. jp/AGASA/ 20. D. J. Bird et al. [Fly's Eye Collaboration], Phys. Rev. Lett. 71 3401 (1993); Astrophys. J. 424, 491 (1994); Astrophys. J. 441, 144 (1995). 21. T. Abu-Zayyad et al. [HiRes Collaboration], Astropart. Phys. 23 (2005) 157. 22. V. Berezinsky, A. Z. Gazizov and S. I. Grigorieva, arXiv:hep-ph/0204357. 23. Z. Fodor, S.

Therefore, we conclude that the detection possibilities for acoustic and radio methods are very promising. Lower and upper errors are given by the YT(2,2) resp. YT(4,5) parametrization. 5 l°g(Emin/GeV) Figure 3. Threshold energy dependence of the total rate for an acoustic array and for various flux models. Acknowledgments T h e authors would like to t h a n k Shigeru Yoshida for helpful discussions. We would also like to thank Justin Vandenbroucke, David Besson, Sebastian Boser, Rolf Nahnauer and Buford Price for their help with this work.

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Accurately measure flammable gases by Holkom B.

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