Abstract

A scheme to generate wide-bandwidth radiation using a step-wise tapered undulator with a segmented structure is proposed. This magnetic field configuration allows to broaden the undulator harmonic spectrum by two orders of magnitude, providing 1 keV bandwidth with spectral flux density exceeding 1016 photons s-1 mm-2 (0.1% bandwidth)-1 at 5 keV on the sample. Such a magnetic setup is applicable to superconducting devices where magnetic tapering cannot be arranged mechanically. The resulting radiation with broadband spectrum and flat-top shape may be exploited at a multipurpose beamline for scanning over the spectrum at time scales of 10-100 ms. The radiation from a segmented undulator is described analytically and derivations with numerical simulations are verified. In addition, a start-to-end simulation ofan optical beamline is performed and issues related to the longitudinally distributed radiation source and its image upon focusing on the sample are addressed.

Highlights

  • Synchrotron radiation (SR) serves as a powerful tool for investigating materials with X-rays

  • Fast monochromators allow to speed up data acquisition, for example for extended X-ray absorption fine structure (EXAFS) spectroscopy resulting in quick-EXAFS (Frahm, 1988)

  • We found that to effectively generate a wide-bandwidth flat-top spectrum the individual resonances of each segment should be shifted by their full width at half-maximum (FWHM)

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Summary

Introduction

Synchrotron radiation (SR) serves as a powerful tool for investigating materials with X-rays. Fast monochromators allow to speed up data acquisition, for example for extended X-ray absorption fine structure (EXAFS) spectroscopy resulting in quick-EXAFS (Frahm, 1988). This requires fast scanning over 1 keV bandwidth at a sub-second time scale with a sufficient photon flux on the sample. We propose an advanced superconducting undulator scheme for the experiments where fast scanning over the spectrum along with micrometre-scale focusing is required We suggest that this source may be installed for future beamlines specialized in micro- and nano-probing, e.g. I18 at DIAMOND (Mosselmans et al, 2009), P06 and P11 at PETRA III (Schroer et al, 2010; Burkhardt et al, 2016) and ID13 at ESRF (Flot et al, 2010)

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