Abstract
Today, at the high-mountain scientific station for the study of the physics of cosmic rays, various, independently operating unique experimental installations are used. The ways and methods of combining these installations into a single system are discussed in the article. A single system includes networks of scintillation detectors of the "carpet" type for registration of the electron-photon component, ground and underground monitors for registration of neutron components, calorimeters, Cherenkov detectors, a scintillation spectrometer and a number of other subsystems. The newly created unified system for registering cosmic rays based on the achievements of modern technology and scientific thought will have a high resolution, with a common databank with synchronization in time of operation of separate, independently operating experimental installations. The solution to this problem will help to perform a detailed analysis of the recorded events from a single position, to carry out complex calculations of the spatial distribution, mass composition, and also the energy structure of cosmic rays with a high degree of accuracy. Significant scientific results, obtained in recent years at the Horizon-T experimental installation, are provided. The presented preliminary significant data obtained during the implementation of the project testify to the high information content of the obtained results.