| Issue |
EPJ Web Conf.
Volume 208, 2019
ISVHECRI 2018 - XX International Symposium on Very High Energy Cosmic Ray Interactions
|
|
|---|---|---|
| Article Number | 08005 | |
| Number of page(s) | 6 | |
| Section | Cosmic Ray Experiments (Extensive Air Showers) | |
| DOI | https://doi.org/10.1051/epjconf/201920808005 | |
| Published online | 10 May 2019 | |
https://doi.org/10.1051/epjconf/201920808005
Some results from the Yakutsk array experiment and the status of the modernization program
Shafer Institute for Cosmophysical Research & Aeronomy, Yakutsk 677980, Russia
★ e-mail: ivanov@ikfia.ysn.ru
Published online: 10 May 2019
The Yakutsk array has been used to study cosmic rays since 1974. Charged particles such as electrons, positrons and muons are detected, as well as radio signals emitted by air showers. However, the characteristic shower component detected by the array is Cherenkov light. This article briefly reviews recent results from the Yakutsk array group.
© The Authors, published by EDP Sciences, 2019
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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