Advanced Photon Source (APS), Argonne National Laboratory

SEES supports the following beamlines and techniques for Earth and Environmental synchrotron science. Techniques include Nuclear Resonant Inelastic X-ray Scattering (NRIXS), Diamond Anvil Cell (DAC), Large Volume Press (LVP), X-ray Diffraction (XRD), Crystal Truncation Rod Scattering ( CTR), Computed X-ray Microtomography (CMT), high PT Brillouin Spectroscopy, X-ray Standing Wave Methods (XSW), Grazing Incidence XRF (GIXRF), X-ray Absorption Spectroscopy (XAS), PE cell, high PT, and X-ray Micro-Probe (XRM).

APS Upgrade and SEES APS beamlines

BeamlineX-ray Source, Energy Range, Beam SizeTechniques
3ID, mono, 14-40 keV, 10 μmNRIXS, DAC
6_BMBM, white, 10 mmLVP
13-BM-CBM, mono, 15 & 29 keV, 15 to 300 μmXRD, DAC, CTR
13-BM-DBM, white, mono, 6-110 keV, 12 μm to 20 mmXRD, DAC, LVP, CMT, high PT Brillouin spectroscopy
13-ID-CMono, 5-80 keV, 30 μm to 1 mm (1 μm after APS-U)XRD, CTR, XSW, GIXRF, XAS, PE cell, coherent scattering
13-ID-DID, white, mono, 14-80 keV, 3 μm to 10 μm (0.3 μm after APS-U)XRD, DAC, LVP, high PT
13-ID-EID, mono, 2.4-28 keV, 1μm (0.3 μm after APS-U)XRM, XAS, XRD