SUMMARY 1 An important characteristic of MWRH would be the simultaneous obtaining of the spatial spectrum at different wavelengths. Obtaining radio images of the solar corona during the daytime by recording all spatial scales is possible through the implementation of adaptive multiwave approach. The essence of the method is as follows. All SSRT antennas will be equipped with multiwave modules. The adaptive multiwave mode make sit possible to realize a redundancy of the SSRT antenna array. For calibrations and for observations of slowly varying structures, it is intended to obtain solar radio images consecutively at different wavelengths. Specifically, either all SSRT antennas or one and the same optimum configuration will be used for each wavelength. Thus it is intended to obtain a quality image of all Sun at six frequencies. The only limitation will be the overlay of noon images at frequencies higher than the SSRT design frequency, 5.7 GHz.  This will be caused by the mismatch of the lowest spatial frequency to the angular size of the Sun for these frequencies. The use of all SSRT antennas in synthesizing the image make sit possible to obtain a highest-quality image but increases substantially (several times) the amount of information. Therefore, the selection of the particular configuration in this case will be influenced not only by the physical expediency but also by the overall performance of the system.