Abstract
Actively bent X-ray mirrors are important components of many synchrotron and X-ray free-electron laser beamlines. A high-quality optical surface and good bending performance are essential to ensure that the X-ray beam is accurately focused. Two elliptically bent X-ray mirror systems from FMB Oxford were characterized in the optical metrology laboratory at Diamond Light Source. A comparison of Diamond-NOM slope profilometry and finite-element analysis is presented to investigate how the 900 mm-long mirrors sag under gravity, and how this deformation can be adequately compensated using a single, springloaded compensator. It is shown that to independent mechanical actuators can accurately bend the trapezoidal substrates to a range of elliptical profiles. Stateof- the-art residual slope errors of <200 nrad r.m.s. are achieved over the entire elliptical bending range. High levels of bending repeatability (ΔR/R = 0.085% and 0.156%r.m.s. for the two bending directions) and stability over 24 h (ΔR/R = 0.07% r.m.s.) provide reliable beamline performance.
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Nistea, I. T., Alcock, S. G., Kristiansen, P., & Young, A. (2017). Long, elliptically bent, active X-ray mirrors with slope errors <200 nrad. Journal of Synchrotron Radiation, 24(3), 615–621. https://doi.org/10.1107/S1600577517005422
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