  The Siberian Solar Radio Telescope (SSRT) is a solar-dedicated
directly-imaging interferometer observing the Sun at 5.7 GHz. The SSRT operates
in the two-dimensional mode since 1996. The imaging principle of the SSRT
restricts its opportunities in observations of very bright flare sources, while
it is possible to use `dirty' images in studies of low brightness features,
which do not overlap with side lobes from bright sources. The interactive CLEAN
technique routinely used for the SSRT data provides imaging of active regions
but consumes much time and efforts and does not reveal low-brightness features
below the CLEAN threshold. The newly developed technique combines the CLEAN
routine with the directly imaging capability of the SSRT and provides clean
images with an enhanced dynamic range automatically. These elaborations
considerably extend the range of tasks, which can be solved with the SSRT. We
show some examples of the present opportunities of the SSRT and compare its
data with the images produced by the Nobeyama Radioheliograph at 17 GHz as well
as observations in different spectral ranges.
