EXFO FTB-5240 REPAIR and EXFO FTB-5240 CALIBRATION

 
Custom-Cal has a high success rate in the repair of the EXFO FTB-5240. A calibration by Custom-Cal is performed by engineers with extensive OEM experience. We have the expertise and the necessary standards to perform the EXFO FTB-5240 Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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As an alternative New Ridge Technologies offers the NRT-8000, the world’s Smallest Optical Spectrum Analyzer with built in “live wavelength calibration” for C-Band applications.  More
   EXFO FTB-5240 (FTB 5240)   Description / Specification:    
EXFO FTB-5240 1250 to 1650 nm Optical Spectrum Analyzer (OSA) Module

The Exfo FTB-5240 is a powerful optical spectrum analyzer (OSA) designed to meet the challenges of DWDM applications. With the increasing sophistication of communication networks comes the need for equally powerful test and measurement equipment designed to meet the challenges of DWDM. Whether testing involves manufacturing, installing and commissioning network fiber, or managing, maintaining, monitoring and troubleshooting performance elements, EXFO’s FTB-5240 Optical Spectrum Analyzers (OSAs) are ready to handle any situation. In addition, the FTB-5240 OSA gives you the best of two worlds: the impressive specifications of a lab-quality instrument in a state-of-the-art, field-ready modular unit for fast, accurate and efficient fiber characterization. This application note presents in-band OSNR measuring techniques become essential to accurately measure the OSNR in reconfigurable networks. Specifications. Wavelength range (nm): 1250 to 1650. Resolution bandwidth FWHM (nm): 0.065. Wavelength uncertainty (nm): ± 0.05. Wavelength repeatability (nm): ± 0.003. Wavelength linearity (nm): typical ± 0.01. Dynamic range c (dBm). 18 to –75. Power uncertainty (dB): ± 0.4. Optical rejection ratio (dBc) at 25 GHz (± 0.2 nm): typical 40, minimum 35. Optical rejection ratio (dBc) at 50 GHz (± 0.4 nm): typical 50, minimum 45. PDL at 1550 nm (dB): typical ± 0.07, maximum ± 0.15. Scanning time (s): < 1.5 (35 nm span, full resolution, multi-peak analysis). ORL (dB): > 35. Size (H x W x D) (module) 96 mm x 76 mm x 26 mm (3 3/4 in x 3 in x 10 1/4 in). Weight (module) 2.2 kg (4.8 lb).



 

Standard Calibration $540.00 *
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*This is a Web introductory price for one calibration of the EXFO FTB-5240. Price does not in most cases include measurement performance data. Pricing does include NIST traceable calibration and issue of a calibration certificate and calibration label. Pricing may vary slightly due to volume and location of laboratory supporting calibration. Volume pricing may apply. On-site fees may apply depending on logistics, location and volume of work to be completed during the visit.


Related Optical Terms and Definitions. For a complete list go to our  Terms and Definitions Page.

Chromatic Dispersion
Chromatic Dispersion is a broadening of the input signal as it travels down the length of the fiber. Chromatic Dispersion results from a variation in propagation delay with wavelength, and is affected by fiber materials and dimensions.

Detector
A Detector is a signal conversion device that converts power from one form to another, such as from optical power to electrical power

Jitter
Jitter in technical terms is the deviation in or displacement of some aspect of the pulses in a high-frequency digital signal. Jitter is the time variation of a periodic signal in electronics and telecommunications, often in relation to a reference clock source. Jitter may be observed in characteristics such as the frequency of successive pulses, the signal amplitude, or phase of periodic signals. Jitter is a significant, and usually undesired, factor in the design of almost all communications links (e.g., USB, PCI-e, SATA, OC-48). In clock recovery applications it is called timing jitter.

Polarization Mode Dispersion (PMD)
Polarization mode dispersion (PMD) is a form of modal dispersion where two different polarizations of light in a waveguide, which normally travel at the same speed, travel at different speeds due to random imperfections and asymmetries, causing random spreading of optical pulses. It is he difference between the maximum and minimum values of loss typically measured in ps/km^1/2.


Please contact us for your EXFO FTB-5240 REPAIR and/or EXFO FTB-5240 1250 to 1650 nm Optical Spectrum Analyzer (OSA) Module CALIBRATION

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