EXFO FPM-302X CALIBRATION and EXFO FPM-302X 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 FPM-302X 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 FPM-302X   Description / Specification:    
EXFO FPM-302X Optical Power Meter

The Exfo FPM-302X Optical Power Meter automatically uses the proper calibration parameters when combined with the FLS-300 or FOT-300 source units. With a high-power option and 10 calibrated wavelengths, the FPM-302X is the most complete, yet simple power meter available. Combined with the FLS-300 or FOT-300 source units, which can transmit with a wavelength-identification digital encrypted protocol, the FPM-300 automatically uses the proper calibration parameters. This auto-wavelength recognition feature reduces the need for communication between the two technicians and decreases the potential for error. This product is part of EXFO's series of FTTx optical test products. It allows for the testing of passive optical networks (PONs) at the three main wavelengths (1310, 1490 and 1550 nm) used in fiber-to-the-home (FTTH) and fiber-to-the-premises (FTTP) networks and complies with the ITU-T G.983 and G.984 Recommendation series and the IEEE 802.3ah standard. Signal encrypting can also give the receiving end information on the power to be used as reference, helping ensure efficient referencing, even when the two units are far apart. Thanks to its unique design, the FPM-302X power meter reduces measurement time in typical measurement situations, as the need for an offset nulling is eliminated.Power meter port GeX. Power range (dBm) 26 to –50. Range displayed (dBm) Down to –50. Number of calibrated wavelengths: 10, (830 nm, 850 nm, 980 nm, 1300 nm, 1310 nm, 1450 nm, 1490 nm, 1550 nm, 1590 nm and 1625 nm.). Power uncertainty ± 5 % ± 10 nW (FPM-302). Resolution (dB) 0.01. Automatic offset nulling Yes. Warmup time (s) 0. Display units dB/dBm/W. Automatic wavelength recognition Yes. Screen refresh rate (Hz) 3. Tone detection (Hz) 270, 1 k, 2 k. Battery life (hours) (typical) > 300. Size (H x W x D) 18.5 cm x 10.0 cm x 5.5 cm (71/4 in x 4 in x 21/8 in). Weight 0.4 kg (0.9 lb).



 

Standard Calibration $160.00 *
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*This is a Web introductory price for one calibration of the EXFO FPM-302X. 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.


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