A system is intended for equipping radio telescopes with antennas of small (12-13 m) diameters, used in the very long baseline interferometers (VLBIs), including universal time on line monitoring interfer ometers. The system operates in S and X wavelength ranges and process up to 8 signals with spectrum widths of up to 512 MHz, converts them into digital sequences with a 1024 MHz clock frequency, and forms data streams in the VLBI Data Interchange Format (VDIF) with a 2048 Mbit/s rate per channel. Data from each channel of the system via the 10G Ethernet interface are transmitted to the data buffering unit for their send ing to the correlation processing center.