Figure 3
IR extraction mirror heat load. (a) A vertical-mounted flat mirror (M1) is illuminated by near 140 W of synchrotron radiation from the B2 bending magnetic. The Au-coated mirror surface reflects low-energy radiation (UV–VIS–IR) and transmits the high-energy portion (mostly X-rays) that is mainly absorbed by the Glidcop substrate. (b) Cross section of the M1 shaft highlighting the water-cooling flow path. (c) Numerical simulation of the thermal load, X-deformation and stress around the illuminated area of the mirror (left to right). (d–g) Optical simulation of the secondary source produced by the M1 flat mirror with a Si substrate at −150 °C (control case) and the Glidcop substrate (actual case with thermal bump) with the heat load and water-cooling system for λ = 15 µm (scale bars 1 mm) and λ = 1.24 µm (scale bars 100 µm). |