Purpose. For radio astronomy, radio physical and geophysical research, student training, analysis and bearing of radio interference in the range of 10-70 MHz, space programs.
Specifications. Operating frequency range 10-70 MHz, electronic aiming, beam width 30° × 30° at a frequency of 40 MHz, two orthogonal linear polarizations, the possibility of additive negative and correlation reception and modular expansion of the effective area.
Application area. Radio astronomy, radiophysical and geophysical research, student training.
Advantages. Relatively cheap design with high sensitivity and does not require a significant surface area for installation. Can be controlled remotely and used in hard-to-reach areas as a short-baseline interferometer or a stationary or mobile base station of an interferometric network. There is a mode for quickly scanning a place.