2002/07/30 by Tim Huege, Heino Falcke
Physics and Astronomy · #astro-ph
published as in: Proceedings of the 6th European VLBI Network Symposium, Ros E., Porcas R.W., Lobanov, A.P., & Zensus, J.A. (eds.), MPIfR, Bonn, Germany (2002), p. 25 · enhanced version with respect to original conference proceedings (additional data points in figure 1, updated references), 3 pages, 3 figures, original conference proceedings can be found at http://www.mpifr-bonn.mpg.de/staff/hfalcke/LOPES
arxiv created 2002/07/30 · arxiv updated 2009/12/01
High-energy cosmic ray air-showers have been known for over 30 years to emit strong radio pulses in the regime between a few and several 100 MHz (Allan 1971). To date, however, a thorough analysis of the emission mechanisms has not yet been conducted. Adopting a simplified shower geometry and electron-positron energy distribution, we calculate theoretical pulse spectra in the scheme of synchrotron emission from highly relativistic electron-positron pairs gyrating in the Earth's magnetic field. These calculations will play an important role for the calibration of observational data of radio-emission from cosmic ray air-showers acquired with LOPES and later LOFAR and SKA.