In 1967, the Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy developed a global survey method that allowed application of the global network of neutron monitors as a single device, simultaneously oriented to various directions and providing information on distribution of cosmic rays per each measured moment. By analogy with this approach, a method for calculation of anisotropy parameters of high-energy cosmic rays has been proposed, involving measurement data from the Global Muon Detector Network and Yakutsk stations. To implement the method, receiving vectors of the stations have been calculated, making it possible to consider associations between cosmic ray variations in the interplanetary medium and those observed at Earth. The paper also discusses some methodological issues related to correct determination of angular distribution of cosmic rays in the interplanetary space. Based on the modified method of global survey, parameters of the first two moments of the angular distribution of cosmic rays for 2012–2018 have been calculated.

1967年，Yu.G。Shafer宇宙物理研究与航空研究所开发了一种全球调查方法，该方法允许将中子监测器全球网络作为单个设备应用，同时面向各个方向，并提供每个测量时刻的宇宙射线分布信息。类似于这种方法，已经提出了一种计算高能宇宙射线各向异性参数的方法，其中涉及来自全球Muon检测器网络和雅库茨克站的测量数据。为了实现该方法，已经计算了站点的接收矢量，从而可以考虑行星际介质中的宇宙射线变化与地球观测到的射线之间的关联。本文还讨论了与正确确定行星际空间中宇宙射线的角度分布有关的一些方法学问题。根据修改后的全球调查方法，计算了2012-2018年宇宙射线角分布的前两个矩的参数。