EXFO IQS-1613 CALIBRATION and EXFO IQS-1613 REPAIR

The EXFO IQS-1613 is currently in stock and available for purchase on our  Sales Page
It is also available for immediate rental.
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-1613 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-1613   Description / Specification:    
EXFO IQS-1613 800 to 1700 nm InGaAs Single Optical Power Meter Module

The EXFO IQS-1613 Power meter module features automatic gain range, power fluctuations of up to 95 dB stabilize within 15 ms, and a continuous sampling rate of up to 256 samples per second can be achieved. You can also manually select the gain range for individual channels. In this case, dynamic range is limited to the selection; but in return, stabilization times are shorter (as little as 1 ms), with sampling rates as high as 4096 samples per second. The synchronization capability of the IQS-1613 High-Speed Power Meter complements the high sampling rates. This high-speed power meter provides two types of synchronization triggers, a power level trigger and a TTL voltage (electrical) trigger. The IQS-1613 comes with front panel InGaAs detectors, with an impressive -85 dBm sensitivity. Specifications. Number of detectors: 1. Detector type: InGaAs. Detector size: 1 mm. Wavelength range: 800 to 1700 nm. Power range: 9 to -85 dBm. Uncertainty: ±5% (0 dBm to -55 dBm). Linearity: ±0.015 (0 dBm to -55 dBm). Power resolution: 0.001 dB (9 dBm to -40 dBm). Wavelength resolution: 0.01 nm. Stabilization time automatic range: < 12 ms (9 dBm to -85 dBm). Sampling rate (sample/s/channel) fast acquisition mode: up to 4096. Fiber type: 5/125 to 62.5/125 µm. External trigger input voltage: 0 to 5 V (TTL).



 

Standard Calibration $190.00 *
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*This is a Web introductory price for one calibration of the EXFO IQS-1613. 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 IQS-1613 CALIBRATION and/or EXFO IQS-1613 800 to 1700 nm InGaAs Single Optical Power Meter Module REPAIR

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