To do this, it is necessary to equip the SSRT antenna elements with multiwave convertor modules (MCM). Each MCM will comprise the polarization switch, the low-noise amplifier, the frequency converter with the synthesizer as the heterodyne, the attenuator, the phase shifter, and the microprocessor. It is admissible to use six wavelengths in the frequency range from 2 GHz  to 10 GHz  (2340, 3100, 4340, 5730, 7815 and 0300 MHz).  MCM converts signals of all waves received by the antenna, to an intermediate frequency. Synthesizers at all antennas are synchronized by the phase-stable reference signal. Signals at the intermediate frequency are fed to the working room for a correlation processing.      An important characteristic of MWRH would be the simultaneous obtaining of the spatial spectrum at different wavelengths. To accomplish this, it is possible to use the redundancy of the SSRT antenna system. Based on the objective of flare and coronal mass ejection observation, the changes in spatial structures of our interest are occurring in the region of high spatial frequencies. To record them simultaneously, it is sufficient to fill the edges of the SSRT array with antennas operating at different frequencies (Fig. 6). For measuring coronal magnetic fields, the instrument will operate in the mode of sequential use of working wavelengths (100...500 ms for each of the six working wavelengths). For observing a quiet Sun, active regions, filaments, and coronal holes, use will be made of the redundancy of the SSRT antenna system to simultaneously obtaining spatial spectra at different wavelengths. Thus we expect to obtain a flexible instrument for performing different tasks simultaneously.