Beamlines

Advanced Light Source (ALS), Lawrence Berkeley National Laboratory

SEES supports the following beamlines and techniques for Earth and Environmental synchrotron science. Techniques include X-ray Diffraction and X-ray Diffraction Imaging (XRD), Diamond Anvil Cell (DAC), high PT, Computed X-ray Microtomography (CMT), high PT, and Scanning Transmission X-ray Microscopy (STXM).

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Beamline X-ray Source, Energy Range, Beam Size Techniques
12.2.2 Superbend, mono, 30keV XRD, DAC, high PT
8.3.2 Superbend, mono, white, 8-45 keV CMT
12.3.2 Superbend, mono, white XRD, XRD imaging
5.3.2.1, 5.3.2.2, 7.0.1.2, 11.0.2.2 Various, mono, 0.6-2.6 keV STXM

In situ X-ray and IR probes relevant to Earth science at the Advanced Light Source at Lawrence Berkeley Laboratory
https://link.springer.com/article/10.1007/s00269-024-01278-5

 

National Synchrotron Light Source II (NSLS II), Brookhaven National Laboratory

SEES supports the following beamlines and techniques for Earth and Environmental synchrotron science. Techniques include Infrared Spectroscopy and nanoIR (IR), Diamond Anvil Cell (DAC), X-ray Microprobe (XRM), X-ray Absorption Spectroscopy (XAS), X-ray Diffraction (XRD), Large Volume Press (LVP), and imaging at high PT.

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Shipping Information 2024

Beamline X-ray Source, Energy Range, Beam Size Techniques
FIS, MET IR, 4 meV to 3 eV IR, DAC, nano IR
XFM BM, mono 2.3-20 keV, 5 μm XRM, XAS, XRD
XPD ID, mono, 60 keV XRD, LVP, imaging at high PT

 

 

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).

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Beamline X-ray Source, Energy Range, Beam Size Techniques
3, 30 ID, mono, 14-40 keV, 10 μm NRIXS, DAC
6-BM BM, white, 10 mm LVP
13-BM-C BM, mono, 15 & 29 keV, 15 to 300 μm XRD, DAC, CTR
13-BM-D BM, white, mono, 6-110 keV, 12 μm to 20 mm XRD, DAC, LVP, CMT, high PT Brillouin spectroscopy
13-ID-C Mono, 5-80 keV, 30 μm to 1 mm (1 μm after APS-U) XRD, CTR, XSW, GIXRF, XAS, PE cell, coherent scattering
13-ID-D ID, white, mono, 14-80 keV, 3 μm to 10 μm (0.3 μm after APS-U) XRD, DAC, LVP, high PT
13-ID-E ID, mono, 2.4-28 keV, 1μm (0.3 μm after APS-U) XRM, XAS, XRD

 

 

Stanford Synchrotron Radiation Lightsource (SSRL), SLAC National Accelerator Laboratory

SEES supports the following beamlines and techniques for Earth and Environmental synchrotron science. Techniques include X-ray Microprobe (XRM), X-ray Absorption Spectroscopy (XAS) and X-ray Diffraction (XRD).

 Apply for Beamtime

Beamline X-ray Source, Energy Range, Beam Size Techniques
10 beamlines Various, mono, 2-20 keV, 1μm to 10mm XRM, XAS, XRD