Advanced flow-polishing and surface metrology of the SO56 X Ray Telescope

Physics – Optics

Scientific paper

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Geometrical Optics, Grazing Incidence, Metrology, Mirrors, Surface Finishing, X Ray Telescopes, Asphericity, Curvature, Layouts, Optimization, Substrates, Wave Fronts

Scientific paper

The surface finishing of X ray grazing incidence optics is a most demanding area of optical processing, both in terms of metrology and application of optical finishing techniques. An existing optical mirror was processed using a new removal technique that uses a jet of finely dispersed and extremely small particles that impact a surface, which under the correct conditions, produces an ultrasmooth surface, especially on aspheric curvatures. The surfaces of the SO56 mirror are tapered conical shapes that have a continuously changing radius with the primary mirror having a parabolic shape and the secondary mirror a hyperbolic shape. An optical ray trace that was conducted of a telescope used the measured parameters from the existing substrates to set up the prescription for the optical layout. The optimization indicated a wavefront performance of 0.10 A at 0.633 micron.

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