EXFO FOT-90A REPAIR and EXFO FOT-90A CALIBRATION

 
Custom-Cal has a high success rate in the repair of the EXFO FOT-90A. 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 FOT-90A Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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   EXFO FOT-90A (FOT 90A)   Description / Specification:    
EXFO FOT-90A Optical Power Meter

The Exfo FOT-90A Optical Power Meter series is a high-performance unit for power/loss testing of fiber-optic links and components. It features an automated wavelength-recognition system. Paired with a compatible light source (FLS-210A), the FOT-90A automatically recognize the operating wavelength, then evaluates and stores loss data with easy one-touch operation. The new Ultra-High-Power option allows measurements of up to +35 dBm. The FOT-90A Power Meter, one of the most complete fiber-optic power meters available, just got better. EXFO is leading the industry again by being the first to offer +35 dBm capability in a handheld instrument. This sturdy unit has received worldwide acceptance in the fiber-optic industry. In a world where technology seems to change every second, the FOT-90A continues to demonstrate its superiority by providing reliable performance and accurate measurements. The FOT-90A is a high-performance unit for power/loss testing of fiber-optic links and components. It features an automated wavelength-recognition system with intelligent testing options. Paired with a compatible light source (FLS-210A or FLS-210B), the FOT-90A automatically recognizes operating calibration wavelength parameters, then averages, validates and stores loss data with easy one-button operation. Specifications (based on configuration). Detector type Ge (2 mm) or InGaAs (2 mm). Measurement range (dBm) 35 to -73. Uncertainty (%) ±5 to ±6.5. Resolution (dB) 0.01. Linearity (dB) ±0.01 to ±0.02. Wavelength range (nm) 780 to 1625. Size (H x W x D) 22 cm x 11 cm x 5 cm (8 3/4in x 4 ½in x 2 in). Common configurations include; FOT-92A = Ge detector, FOT-92AX = GeX detector, FOT-93A = InGaAs detector, FOT-93AX-P1 = Ultra High-Power detector InGaAs 28 dBm, FOT-93AX-P2 = Ultra High-Power detector InGaAs 35 dBm.



 

Standard Calibration $185.00 *
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*This is a Web introductory price for one calibration of the EXFO FOT-90A. 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 FOT-90A REPAIR and/or EXFO FOT-90A Optical Power Meter CALIBRATION

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