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