EXFO FTB-5230 CALIBRATION and EXFO FTB-5230 REPAIR

 
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-5230 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-5230 (FTB 5230)   Description / Specification:    
EXFO FTB-5230 1250 to 1650 nm Optical Spectrum Analyzer (OSA) Module

The Exfo FTB-5230 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-5230 Optical Spectrum Analyzers (OSAs) are ready to handle any situation. Since CWDM systems generally use uncooled lasers, whose typical wavelength drift is 0.1 nm per degree Celsius, it is critical to track the evolution and drift of the lasers’ central wavelength. And since path attenuation can significantly vary within a single channel, passband drift also creates power drift. This is why it becomes extremely important to monitor—simultaneously for all CWDM channels—the evolution of peak power and wavelength over time. The FTB-5230 Optical Spectrum Analyzer’s Drift mode functionalities makes this an easy task. Specifications. Wavelength range (nm): 1250 to 1650. Resolution bandwidth FWHM (nm): <= 0.1. Wavelength uncertainty (nm): ± 0.1. Dynamic range (dBm). 10 to –60. Power uncertainty (dB): ± 0.4. Optical rejection ratio (dBc) at 50 GHz (± 0.4 nm): typical 55. Optical rejection ratio (dBc) at 100 GHz (± 0.8 nm) typical 45. PDL at 1550 nm (dB): typical ± 0.1. Scanning time (s): 4 (35 nm span,multiple-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 $625.00 *
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*This is a Web introductory price for one calibration of the EXFO FTB-5230. 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.

Absolute Wavelength Accuracy
Absolute Wavelength Accuracy is the maximum difference between the actual wavelength and the displayed wavelength of the Optical Source. Wavelength is defined as wavelength in vacuum.

Decibel (dB)
A unit of measurement of optical power which indicates relative power. A -10 dB means a reduction in power by 10 times, -20 dB means another 10 times or 100 times overall, -30 means another 10 times or 1000 times overall and so on.

Nanometer (nm)
A unit of measure used to measure wavelength of light, meaning one one-billionth of a meter

Relative Intensity Noise (RIN)
Relative intensity noise (RIN), describes the instability in the power level of a laser. The noise term is important to describe lasers used in fiber-optic communication and LIDAR remote sensing. It is the square of the (spectrally resolved) RMS optical power amplitude divided by the measurement bandwidth and the square of the average optical power, expressed in dB/Hz.

Total Return loss
In an optical fiber, the loss that takes place at any discontinuity of refractive index, especially at an air-glass interface such as a fiber endface, at which a fraction of the optical signal is reflected back toward the source. RL = - 10log10 (Preflected/Preference)


Please contact us for your EXFO FTB-5230 CALIBRATION and/or EXFO FTB-5230 1250 to 1650 nm Optical Spectrum Analyzer (OSA) Module REPAIR

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