To implement the tracking modes of the RATAN-600 radio telescope, it is necessary to introduce new automation tools that provide a new quality of monitoring and control of the antenna system geometry [1, 2].In this work, the ACS is considered by the movement of the type 3 feed and the carriage, its structure is shown, new capabilities of the complex, previously unavailable on the RATAN-600 radio telescope, are considered.

Radio astronomy studies of the solar atmosphere possess a very important, not duplicated by other methods, place in the study of solar activity at all stages—from the birth of an active region until its collapse. A significant progress in these studies can be achieved in the implementation of new technical possibilities, such as an increase in the sensitivity of radio telescopes, a detailed spectral analysis over a wide frequency range, high temporal resolution and a broad coverage range in time. We report about the implementation of regular observations with a new spectral and polarization high-resolution system SPHRS, installed at the radio telescope RATAN-600.We describe the concept of the new system and the methods of its implementation.

Radio astronomy studies of the solar atmosphere possess a very important, not duplicated by othermethods, place in the study of solar activity at all stages-from the birth of an active region until its collapse. A significant progress in these studies can be achieved in the implementation of new technical possibilities, such as an increase in the sensitivity of radio telescopes, a detailed spectral analysis over a wide frequency range, high temporal resolution and a broad coverage range in time. We report about the implementation of regular observations with a new spectral and polarization high-resolution system SPHRS, installed at the radio telescope RATAN-600. We describe the concept of the new system and the methods of its implementation.