Radio-Emission from Cosmic Ray Air-Showers - A Theoretical Perspective for LOPES

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dc.creatorHuege, Tim
dc.creatorFalcke, Heino
dc.date2002-07-30
dc.date.accessioned2026-07-07T02:04:29Z
dc.date.available2026-07-07T02:04:29Z
dc.descriptionHigh-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.
dc.descriptionenhanced 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0207647
dc.identifierhttp://arxiv.org/abs/astro-ph/0207647
dc.identifierin: 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
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4777
dc.subjectAstrophysics
dc.titleRadio-Emission from Cosmic Ray Air-Showers - A Theoretical Perspective for LOPES
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