NSLS BEAMLINE DESCRIPTION: Beamline U10A
GENERAL INFORMATION
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RING: VUV
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STATUS: Under Construction - commissioning in early 1998.
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RESEARCH PROGRAM: Wide range, high brightness IR spectroscopy of solids
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TIME DEDICATED TO NSLS GENERAL USER PROGRAM: ~25% of operations, following
a commissioning period.
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BEAMLINE SCHEDULE (TBD)
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PARTICIPATING INSTITUTIONS
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BNL-NSLS, BNL-Physics, SUNY @ Stony Brook
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LOCAL CONTACT: Chris Homes
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(516) 344-7579, homes@solids.phy.bnl.gov
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SPOKESPERSON: Larry Carr
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(516) 344-2237, carr@bnl.gov
INSTRUMENTS
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INSTRUMENT #1: BRUKER IFS 66v INTERFEROMETER
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Frequency Range (cm-1): 20- >25,000
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Resolution (cm-1): 0.3
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Brightness (relative to 1000K black body source): 100-1000
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Spot Size (f/4, cm) : 0.1H x 0.05V
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Total Angular Acceptance: (milliradians): 40H x 40V
OPTICAL CONFIGURATION
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Beamline Optical System
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A two-mirror system (M1 and M2) collect and re-image the synchrotron infrared
source at a point just ourside of the storage ring's UHV. M1 is a
water cooled plane mirror made from silicon with a gold reflective coating.
M2 is a glass ellipsoid with a bare aluminum reflective coating.
The ellipsoidal mirror focuses the beam through a 10mm aperture wedged
diamond window (~350 microns thick). Delivered spectral range extends
from approximately 10 cm-1 to beyond 40,000 cm-1.
Beam is then collimated (aluminized off-axis paraboloid) to the IR spectrometer.
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Experimental Apparatus
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Bruker IFS 66v vacuum interferometer with step-scan. Beamsplitters and
detectors for far IR (bolometer, 20 to 700 cm-1), mid &
near IR (Si:B and InSb, 350 cm-1to 11,000 cm-1) and
visible (Si, up to 25,000 cm-1).
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Computer System Hardware and Software
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Bruker's OPUS running under OS/2 on Intel Pentium based PC.
For additional information please contact Larry
Carr or Chris Homes
Revised Date : 16-April-98
DISCLAIMERS
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