Radio emission of air showers with extremely high energy measured by the Yakutsk radio array
The Yakutsk Array is designed to study cosmic rays at energy 10$^{15}$-10$^{20}$ eV. It consists several independent arrays that register charged particles, muons with energy E$\geq$1 GeV, Cherenkov light and radio emission. The paper presents a technical description of the Yakutsk Radio Array and s...
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| Online Access: | https://dx.doi.org/10.48550/arxiv.1705.01260 https://arxiv.org/abs/1705.01260 |
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ftdatacite:10.48550/arxiv.1705.01260 2023-05-15T18:45:18+02:00 Radio emission of air showers with extremely high energy measured by the Yakutsk radio array Knurenko, S. P. Petrov, Z. E. Petrov, I. S. 2017 https://dx.doi.org/10.48550/arxiv.1705.01260 https://arxiv.org/abs/1705.01260 unknown arXiv https://dx.doi.org/10.1016/j.nima.2017.04.033 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences article-journal Article ScholarlyArticle Text 2017 ftdatacite https://doi.org/10.48550/arxiv.1705.01260 https://doi.org/10.1016/j.nima.2017.04.033 2022-04-01T10:40:03Z The Yakutsk Array is designed to study cosmic rays at energy 10$^{15}$-10$^{20}$ eV. It consists several independent arrays that register charged particles, muons with energy E$\geq$1 GeV, Cherenkov light and radio emission. The paper presents a technical description of the Yakutsk Radio Array and some preliminary results obtained from measurements of radio emission at 30-35 MHz frequency induced by air shower particles with energy $\varepsilon$ $\geq$ 1$\cdot$10$^{17}$ eV. The data obtained at the Yakutsk array in 1986-1989 (first set of measurements) and 2009-2014 (new set of measurements). Based on the obtained results we determined: Lateral distribution function (LDF) of air showers radio emission with energy $\geq$ 10$^{17}$ eV. Radio emission amplitude empirical connection with air shower energy. Determination of depth of maximum by the ratio of amplitude at different distances from the shower axis. For the first time, at the Yakutsk array, radio emission from the air shower with energy $>$ 10$^{19}$ eV was registered including the shower with the highest energy ever registered at the Yakutsk array with energy $\sim$2 $\cdot$ 10$^{20}$ eV. : 11 pages, 20 figures, 2 tables, accepted for publication in NIM A. arXiv admin note: text overlap with arXiv:1609.03273 Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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Open Polar |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
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unknown |
| topic |
Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
| spellingShingle |
Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences Knurenko, S. P. Petrov, Z. E. Petrov, I. S. Radio emission of air showers with extremely high energy measured by the Yakutsk radio array |
| topic_facet |
Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
| description |
The Yakutsk Array is designed to study cosmic rays at energy 10$^{15}$-10$^{20}$ eV. It consists several independent arrays that register charged particles, muons with energy E$\geq$1 GeV, Cherenkov light and radio emission. The paper presents a technical description of the Yakutsk Radio Array and some preliminary results obtained from measurements of radio emission at 30-35 MHz frequency induced by air shower particles with energy $\varepsilon$ $\geq$ 1$\cdot$10$^{17}$ eV. The data obtained at the Yakutsk array in 1986-1989 (first set of measurements) and 2009-2014 (new set of measurements). Based on the obtained results we determined: Lateral distribution function (LDF) of air showers radio emission with energy $\geq$ 10$^{17}$ eV. Radio emission amplitude empirical connection with air shower energy. Determination of depth of maximum by the ratio of amplitude at different distances from the shower axis. For the first time, at the Yakutsk array, radio emission from the air shower with energy $>$ 10$^{19}$ eV was registered including the shower with the highest energy ever registered at the Yakutsk array with energy $\sim$2 $\cdot$ 10$^{20}$ eV. : 11 pages, 20 figures, 2 tables, accepted for publication in NIM A. arXiv admin note: text overlap with arXiv:1609.03273 |
| format |
Text |
| author |
Knurenko, S. P. Petrov, Z. E. Petrov, I. S. |
| author_facet |
Knurenko, S. P. Petrov, Z. E. Petrov, I. S. |
| author_sort |
Knurenko, S. P. |
| title |
Radio emission of air showers with extremely high energy measured by the Yakutsk radio array |
| title_short |
Radio emission of air showers with extremely high energy measured by the Yakutsk radio array |
| title_full |
Radio emission of air showers with extremely high energy measured by the Yakutsk radio array |
| title_fullStr |
Radio emission of air showers with extremely high energy measured by the Yakutsk radio array |
| title_full_unstemmed |
Radio emission of air showers with extremely high energy measured by the Yakutsk radio array |
| title_sort |
radio emission of air showers with extremely high energy measured by the yakutsk radio array |
| publisher |
arXiv |
| publishDate |
2017 |
| url |
https://dx.doi.org/10.48550/arxiv.1705.01260 https://arxiv.org/abs/1705.01260 |
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Yakutsk |
| geographic_facet |
Yakutsk |
| genre |
Yakutsk |
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Yakutsk |
| op_relation |
https://dx.doi.org/10.1016/j.nima.2017.04.033 |
| op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
| op_doi |
https://doi.org/10.48550/arxiv.1705.01260 https://doi.org/10.1016/j.nima.2017.04.033 |
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1766236344906940416 |