The article describes the project of the large-scale astrophysical complex TAIGA-100, aimed at solving a wide range of fundamental problems in the field of gamma-ray astronomy and cosmic ray physics. The results of the analysis of the astroclimate of potential sites for its placement are presented. The importance of in-situ measurements based on automatic monitoring is emphasized. The prototype of the astroclimatic station deployed on the territory of the current TAIGA-1 complex and the first results obtained using this station are described.
A. L. Ivanova (Wed,) studied this question.