Development and produce of ground-based reflecting coronagraph for solar applications

The ground-based 0.36m mirror coronagraph with super-polished off-axis parabolic primary mirror for solar applications has developed and build now. Optical system design, technology of scattering level measurement of primary mirror surface and the method of adjustment are described. Also presents the constructions of heat-stop, Lyot-stop assemblies and truss. The kit of spectral equipment and detectors for actual solar astrophysics tasks is discussed.