arXiv Analytics

Sign in

arXiv:1612.07891 [astro-ph.HE]AbstractReferencesReviewsResources

Radio Emission of Air Showers with Energy E$_0$ $\geq$ 10$^{19}$ eV by Yakutsk Array Data

S. Knurenko, I. Petrov, Z. Petrov

Published 2016-12-23Version 1

In this paper, we present results obtained from the measurements of radio emission at frequency of 32 MHz with energy more than 10$^{19}$ eV. Generalized formula that describe lateral distribution and depends on main characteristic of the air showers: energy E$_0$ and depth of maximum X$_{max}$ was derived. The formula has a good agreement with data at average and large distances from shower axis. Employing the ratio of radio emission amplitude at distances 175 m and 725 m we determined the depth of maximum X$_{max}$ for air shower with energy 3.7$\cdot$10$^{19}$ eV, which in our case is equal to X$_{max}$ = 769$\pm$34g$\cdot$cm$^{-2}$.

Comments: XXV ECRS 2016 Proceedings - eConf C16-09-04.3
Categories: astro-ph.HE
Related articles: Most relevant | Search more
arXiv:1009.1994 [astro-ph.HE] (Published 2010-09-10)
REAS3: A revised implementation of the geosynchrotron model for radio emission from air showers
arXiv:2304.08561 [astro-ph.HE] (Published 2023-04-17)
Zenith-Angular Characteristics of Particles in EASs with $E_0 \simeq 10^{18}$ eV According to the Yakutsk Array Data
arXiv:2211.16970 [astro-ph.HE] (Published 2022-11-30)
Multiplicity of TeV muons in air showers detected with IceTop and IceCube