1. Performance of new infrared beamline U12IR at the National Synchrotron Light Source
- Author
-
David B. Tanner, J. D. LaVeigne, G. L. Carr, R. P. S. M. Lobo, and D. H. Reitze
- Subjects
Physics ,Infrared ,business.industry ,Astrophysics::High Energy Astrophysical Phenomena ,Synchrotron radiation ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Photon energy ,National Synchrotron Light Source ,Optics ,Beamline ,Far infrared ,High-energy X-rays ,Physics::Accelerator Physics ,Optoelectronics ,Black-body radiation ,business ,Instrumentation ,Astrophysics::Galaxy Astrophysics - Abstract
The instrumentation and performance of the new infrared beamline U12IR at the National Synchrotron Light Source of Brookhaven National Laboratory is described. This beamline utilizes infrared synchrotron radiation from a bending magnet. A combination of beamline design features and spectroscopic instrumentation allows the facility to reach the extremely low frequency limit of ∼2 cm−1 (i.e., 60 GHz or a photon energy of 250 μeV). The infrared light from the synchrotron emission at U12IR is compared to standard thermal sources and reveals substantial benefits for the study of small samples. In particular, the intensity of the synchrotron radiation in the far infrared can be as much as 200 times greater than that from a blackbody when millimeter-sized samples are measured. The effects of diffraction and noise on beamline performance are also discussed.
- Published
- 1999
- Full Text
- View/download PDF