Beamline 7.0.1.1
COSMIC Scattering
Current status | Operational; open to general users |
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ALS-U Status | This COSMIC Scattering branch will close at the start of the ALS-U dark time. The capability will migrate to the new planned FLEXON beamline at 10.0.1. For more information, see ALS-U Beamline Impacts and other ALS-U web pages. |
Source | EPU3.8 |
Minimum energy (eV) | 250 |
Maximum energy (eV) | 1,600 |
Research areas |
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Technique category |
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Access modes |
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Additional notes | Currently accepting general user proposals . Please contact Beamline Scientists Sujoy Roy and Sophie Morley to discuss if your experiment is suitable. |
Primary contact(s) | Sujoy Roy Sophie Morley |
Beamline phone number | 510-495-8831 |
Endstation
Status | Operational; open to general users |
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Research areas |
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Technique category |
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Spot size | Focused to 7um without pinhole; pinhole diameters available (on request): 2 - 20 um |
Sample information | Vacuum compatible (p < 1e-7), sample heating (400 K) and cooling (20 K). Transmission geometry samples: need soft x-ray transparent substrates e.g. Si3N4 membranes - can estimate x-ray transparency for transmission substrates here. Reflection geometry samples: need <8mm lateral dimensions, < 3mm in height/thickness. |
Additional Notes | Twotheta scannable from -10 - 150deg with 50 mm translation perpendicular to the beam. Polarization is user selectable; linear (variable from horizontal to vertical) & circular (left and right-handed). Detectors: Flange mounted ANDOR CCD iKon L 936. Twotheta arm Princeton Instruments MTE3 CCD & Si Photodiode. Vector plane magnet (x-z) up to 0.1T without cooling, 0.65T with LN2 cooling. |
Primary contact(s) | Sujoy Roy Sophie Morley |