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Characteristics
These fiber configurations are based on the latest wide-band synthetic fused silica materials. They are designed for applications such as astronomical spectroscopy, where stable, broadband spectral coverage from the UV to the near IR is required. The Focal Ratio Degradation (FRD) characteristics are excellent. Polymicro Technologies manufactures these fibers with various core sizes, buffers and jackets. Core sizes range from 50µm to over 1000µm, with tight dimensional tolerances and excellent concentricity. The fiber type STU has low -OH (~5-20ppm) for UV use while the type STU-D has ultra low -OH (~1ppm) for improved NIR at the expense of reduced UV transmission1. The type STU fiber is noticeably improved in the 280nm to 380nm range compared to our standard low -OH (type FI) optical fiber. Typical Characteristics
These fibers can also be assembled into custom configurations as required. Contact Polymicro to assist you with your needs in optical fiber as well as custom micro-optical components, capillary tubing and assemblies.
1 G. Lu, G.F. Schotz, J. Vydra, D. Fabricant, “Optical Fiber for UV-IR Broadband Spectroscopy,” SPIE Proceedings, Optical Astronomical Instrumentation, V3355, pp884-891, Mar 1998 |
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