Figure 2
Top: instrumentation shown in Fig. 1 (top view, without the vacuum chamber) in situations that dispersive optics could make the beam pass or not through the QWP. In the case of this instrumentation, S ≫ d. So as the slit scans across the dispersive beam, there is a condition when the beam does not hit the QWP. This alignment limitation causes the short spectral energy bandwidth, requiring a relative slit translation to maintain the QWP centered at the beam through an entire energy scan. Middle: representation of the elements used to elaborate the correction for the QWP positioning. An X-ray beam with energy E selected by the slit at a distance S from focus, positioned at an XS with respect to the translation axis X. The QWP ideal position is then Xd, at a distance d from the focal point. Then, equation (1) is obtained using the relation for energy resolution in space: = , and substituting L = SX/M (because the energy bandwidth ΔL is selected at S), where X and M are variables in directions X and M. Bottom: DXAS beamline energy bandwidth (black line) at a fixed energy of 7243 eV, p = 9.75 m and q = 1.5 m; and theoretical calculation for the bandwidth available for the XMCD experiment (red line), as a function of the distance from the QWP (∼5 mm × 5 mm) to the slit. The blue line is the bandwidth calculation as a function of the QWP size, for the same energy of 7243 eV, at a fixed distance of 100 cm between the QWP and the slit. |