Lateral distribution of radio signal measured in showers with energy 5*10^16-10^18 eV at the Yakutsk EAS array
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 f...
| Main Authors: | , |
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| Format: | Report |
| Language: | unknown |
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arXiv
2013
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| Subjects: | |
| Online Access: | https://dx.doi.org/10.48550/arxiv.1309.6698 https://arxiv.org/abs/1309.6698 |
| Summary: | 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. : 33rd International Cosmic Ray Conference, Rio de Janeiro, Brazil, July 2013 |
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