EXFO IQS-5240S-NS1623 CALIBRATION and EXFO IQS-5240S-NS1623 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 IQS-5240S-NS1623 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 IQS-5240S-NS1623   Description / Specification:    
EXFO IQS-5240S-NS1623 950 to 1650 nm Optical Spectrum Analyzer (OSA) Module

The Exfo IQS-5240S-NS1623 Optical Spectrum Analyzer (OSA) has 33 pm (or ~4.5 GHz) resolution bandwidth defined as the FWHM of the OSA filter shape, the instrument can analyze all densely spaced signals, including important 50 GHz ITU-grid WDM signals, high-speed modulated lasers/emitters and DWDM passive components, all critical in today’s networks. Combined with a very sharp rejection ratio (–35 dBc at 0.1 nm), the optical signal-to-noise ratio (OSNR) and modulated band profile can be measured with high accuracy. To ensure accurate noise and broad signal power measurements, the noise equivalent bandwidth (NEB) of the OSA is calibrated at many points from 950 nm to 1650 nm. Specifications. Wavelength range: 1250 to 1650 nm. Wavelength uncertainty (1520 to 1610 nm): ±0.05 nm. Resolution bandwidth (FWHM): 0.065 nm. Wavelength linearity: ±0.01 nm. Dynamic range (per channel): –80 to +18 dBm. Maximum total safe power: +23 dBm. Absolute power uncertainty: ±0.5 dB. Optical rejection ratio at 1550 nm at 0.2 nm (25 GHz): 35 dB (40 typical). Channel spacing: 50 to 200 GHz CWDM. PDL at 1550 nm: ±0.08 dB. Options. 00 = Without polarization controller, P = With polarization controller. 28 = UPC/DIN 47256, 76 = UPC/HMS-10/AG, 89 = UPC/FC narrow key, 90 = UPC/ST, 91 = UPC/SC, 95 = UPC/E-2000, 28 = APC/DIN 47256, 89 = APC/FC narrow key, 91 = APC/SC, 95 = APC/E-2000. 00 = Without software option, InB = With In-Band OSNR software.



 

Standard Calibration $625.00 *
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*This is a Web introductory price for one calibration of the EXFO IQS-5240S-NS1623. 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.

Coherence Time
Average time for the wave train to lose its phase realtionships

Fiber Bragg Grating (FBG)
A fiber Bragg grating (FBG) is a type of distributed Bragg reflector constructed in a short segment of optical fiber that reflects particular wavelengths of light and transmits all others. This is achieved by adding a periodic variation to the refractive index of the fiber core, which generates a wavelength specific dielectric mirror. A fiber Bragg grating can therefore be used as an inline optical filter to block certain wavelengths, or as a wavelength-specific reflector.

Modulation
Modulation is the process by which the characteristic of one wave (the carrier) is modified by another. Adding information into pulses of light.

Power Linearity
When changing the power level and measuring the differences (in dB) between actual and displayed power levels, the power linearity is ± half the span (in dB) between the maximum and the minimum value of all differences.

Stability
Stability is the extent to which a specified property, characteristic, or parameter of a substance, device, or apparatus, such as a fiber optic transmission system, remains fixed with the passage of time or with varying environmental conditions.


Please contact us for your EXFO IQS-5240S-NS1623 CALIBRATION and/or EXFO IQS-5240S-NS1623 950 to 1650 nm Optical Spectrum Analyzer (OSA) Module REPAIR

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