The A.I. Kuz’min cosmic ray spectrograph: New scintillation muon telescopes
- 作者: Starodubtsev S.A.1, Grigoryev V.G.1, Gololobov P.Y.1
-
隶属关系:
- Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- 期: 卷 81, 编号 4 (2017)
- 页面: 538-541
- 栏目: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185066
- DOI: https://doi.org/10.3103/S1062873817020393
- ID: 185066
如何引用文章
详细
The state-of-the-art Yakutsk cosmic ray spectrograph consists of the 24-NM-64 neutron monitor, four muon telescopes of the same type, and SGM-14 gas-discharge counters that detect particles coming from five directions and are installed at levels of 0, 7, 20, and 40 meters of water equivalent. A new complex of four muon telescopes of the same type based on SC-301 scintillation counters that record particles from 13 destinations has now been added to the spectrograph. Acceptance vectors that consider the geometry, geographical position, and energy spectra of the observed cosmic ray variations have been developed for these instruments. Analysis of the data from the new scintillation detectors shows that the count rate is as expected in all directions. The parameters of the acceptance characteristics of the new scintillation telescopes and current detection data are available on the Institute’s website at http://www.ysn.ru/smt.
作者简介
S. Starodubtsev
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: grig@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
V. Grigoryev
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
编辑信件的主要联系方式.
Email: grig@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
P. Gololobov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: grig@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
补充文件
