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Endstations 

 

The Secondary Optical Enclosure
(The Endstations)

Diffractometer

Grazing Incidence X-ray diffraction (GIXRD)
Grazing Incidence Wide Angle X-ray Scattering(GIWAXS)
Diffractive Anomalous Fine structure (DAFS)
Thin Film characterization

  • Huber psi-8 diffractometer
  • ARS closed cycle cryostat (10 - 450 K)
  • X-ray CCD detector
  • Analyser crystals ( HOPG(002), Ge(111), Si(111), and Si(004) )
  • Cyberstar Scintillation detector
  •  For more information click the picture or the link above.

     

    XAFS

    • Conventional Ion chamber detector and Lytle detector
    • 32 element Ge solid state detector
    • Low temperature sample environment
    • Vortex silicon drift detector

    For more information click the picture or the link above.

     

    Microprobe

    • KB mirrors, assembled
    • Vortex silicon drift detector

    For more information click the picture or the link above.

     

     


    In the Front End and Primary Optical Enclosure

    The Superconducting Wiggler

    HXMA was the only one of the 7 phase one beamlines at CLS to choose a wiggler. It provides us with a high flux/brilliance at the higher energy levels (20-40keV) which can not be achieved using Undulators. For more information click the picture or the link above.

     

    The Beamline Optics

    HXMA's Major optical components include a double crystal monochromator, a toroidal focusing mirror, and a vertical collimating mirror. For more information click the picture or the link above.