Ill-posed formulation of the emission source localization in the radio-detection experiments of extensive air showers
arXiv:1208.3539
Abstract
Reconstruction of the curvatures of radio wavefronts of air showers initiated by ultra high energy cosmic rays is discussed based on minimization algorithms commonly used. We emphasize the importance of the convergence process induced by the minimization of a non-linear least squares function that affects the results in terms of degeneration of the solutions and bias. We derive a simple method to obtain a satisfactory estimate of the location of the main point of emission source, which mitigates the problems previously encountered.
References in corpus (7)
- Detection and imaging of atmospheric radio flashes from cosmic ray air showers
- Radio-Detection Signature of High Energy Cosmic Rays by the CODALEMA Experiment
- Geomagnetic origin of the radio emission from cosmic ray induced air showers observed by CODALEMA
- Lateral Distribution of the Radio Signal in Extensive Air Showers Measured with LOPES
- Simulation of radio emission from cosmic ray air shower with SELFAS2
- The TIANSHAN Radio Experiment for Neutrino Detection
- Prospects for determining air shower characteristics through geosynchrotron emission arrival times