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Receiving vectors of muon telescope of cosmic ray station Novosibirsk

机译：宇宙射线站新西伯利亚的μ子望远镜的接收向量

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The method of receiving vectors allows us to determine cosmic ray anisotropy at every moment of time. Also, the method makes it possible to study fast anisotropy fluctuations related to the interplanetary medium dynamics. Receiving vectors have been calculated earlier for neutron monitors and muon telescopes. However, most muon telescopes of the network of cosmic ray stations for which calculations were made does not operate now. In recent years, new, improved detectors have been developed. Unfortunately, the use of them is limited because of the absence of receiving coefficients. These detectors include a matrix telescope in Novosibirsk. Therefore, receiving vector components for muon telescopes of observation cosmic ray station Novosibirsk have been defined. Besides, design features of the facility, its orientation, and directional diagram depending on zenith and azimuth angles were taken into account. Also, for the system of telescopes, we allowed for coupling coefficients found experimentally by the test detector.
机译：接收向量的方法使我们能够确定每个时刻的宇宙射线各向异性。同样，该方法使得研究与行星际介质动力学有关的快速各向异性波动成为可能。接收矢量是较早为中子监测仪和μ子望远镜计算的。但是，大多数进行了计算的宇宙射线站网络的μ子望远镜现在不工作。近年来，已经开发了新的，改进的探测器。不幸的是，由于缺少接收系数，它们的使用受到限制。这些探测器包括新西伯利亚的矩阵望远镜。因此，已经定义了宇宙射线观测站新西伯利亚的μ子望远镜的接收矢量分量。此外，还考虑了设施的设计特点，设施的方位以及取决于天顶和方位角的方向图。同样，对于望远镜系统，我们允许测试探测器通过实验找到耦合系数。

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