Beamline U10B


GENERAL INFORMATION

Research Program - Mid-infrared microspectroscopy of materials
Ring - VUV-IR Port
Status - Fully Operational
Time Dedicated to NSLS General User Program - 50%


PARTICIPATING INSTITUTIONS

National Synchrotron Light Source

Case Western Reserve University


SPOKESPERSON

Lisa Miller: 631.344.2091, lmiller@bnl.gov


LOCAL CONTACT

Randy Smith: 631.344.8033, rsmith@bnl.gov


INSTRUMENT

OPTICAL CONFIGURATION

A two-mirror system (M1 and M2) collects and re-images the synchrotron infrared source at a point just outside 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 an aluminum reflective coating. The ellipsoidal mirror focuses the beam through an 11mm aperture wedged diamond window (~350 microns thick). Delivered spectral range extends from approximately 10 cm-1 to beyond 40,000 cm-1. The infrared is then collimated to a diameter of 14mm or 8mm and transported under rough vacuum through a KBr (or polyethylene) window and into the nitrogen-purged, Bruker endstation.


EXPERIMENTAL APPARATUS

Bruker Vertex 80v Step-Scan FTIR equipped with KBr beamsplitter and an internal DTGS-KBr detector. Bruker Hyperion 3000 IR microscope equipped with 15x, 36x, and 74x transmission/reflection IR objectives. "View-thru" capability allow simultaneous sample viewing and IR data collection. One glass objective (10X plan) for visual inspection. DIC and fluorescence microscopy capabilities. IR and visible polarizers. Automated X-Y scanning stage for spectroscopic mapping. Includes video image capture of sample specimen. Step resolution of 1 micron. 128x128 focal plane array, single-pixel MCT-A detectors.


COMPUTER SYSTEM HARDWARE AND SOFTWARE

Intel Pentium VI, 2.0 GHz computer running Windows XP; 2.0 GB RAM, 200 GB hard disk, 17" flat panel monitor; Bruker OPUS 6.0 software. HP LaserJet 1100 (B&W) printer for hardcopy output. Data can be stored on USB flash drive or external hard drive.


FORMS and MANUALS

This page last updated by Lisa Miller on January 08, 2009. Disclaimers.