Lateral distribution of radio signal measured in showers with energy 5*10¹6-10¹8 eV at the Yakutsk EAS array

2013/09/26 by С. П. Кнуренко, S. Knurenko, Knurenko, S. +3
Engineering · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Electromagnetic Compatibility and Measurements #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Radio Astronomy Observations and Technology #astro-ph.HE

paper · pdf · doi:10.48550/arxiv.1309.6698

33rd International Cosmic Ray Conference, Rio de Janeiro, Brazil, July 2013

arxiv created 2013/09/26 · openalex publication_date 2013/09/26 · arxiv updated 2013/09/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We present of measurements of radio emission from EAS at the frequency 32 MHz performed in 2008-2012. Showers were selected by zenith and azimuth directions, sampled by energy. A mean lateral distribution function was fitted to the data each interval. The paper presents unied approximation formula for all three energy intervals of lateral distribution, using connection between equation (1) and (2) coefficients with energy and geomagnetic angle. Here we analyze the connection between the shape of lateral distribution and the depth of the maximum shower development Xmax too.

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