Keysight (Agilent) 81940A REPAIR and Keysight (Agilent) 81940A CALIBRATION

The Keysight (Agilent) 81940A is currently in stock and available for purchase on our  Sales Page
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Custom-Cal has a high success rate in the repair of the Keysight (Agilent) 81940A. A calibration by Custom-Cal is performed by engineers with extensive OEM experience. We have the expertise and the necessary standards to perform the Keysight (Agilent) 81940A Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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   Keysight (Agilent) 81940A   Description / Specification:   Spec Sheet 
Keysight (Agilent) 81940A 1520 to 1630 nm Compact Tunable Laser Source Module

The Agilent 81940A high power compact tunable laser enables optical device characterization at high power levels and measurement of nonlinear effects. It improves the testing of all types of optical amplifiers and other active components as well as broadband passive optical components. As single slot plug-in modules for Agilent's 8163A/B, 8164A/B and 8166A/B mainframes, they are a flexible and cost effective stimulus for single channel and DWDM test applications. Each module covers a total wavelength range of 110 nm in the C+L-band.
Specifications.

Wavelength range: 1520 nm to 1630 nm.
Wavelength (frequency) resolution: 1 pm, 125 MHz at 1550 nm
Mode-hop free tenability: Full wavelength range.
Maximum sweep speed: 50 nm/s.
Absolute wavelength accuracy: ± 20 pm, typical ± 5 pm.
Relative wavelength accuracy: ± 10 pm, typical ± 5 pm.
Wavelength repeatability: ± 2.5 pm, typical ± 1 pm.
Wavelength stability (typical, over 24 hours): ± 2.5 pm.
Linewidth (typical), coherence control off: 100 kHz.
Effective linewidth (typical), coherence control on: > 50 MHz (1570 nm to 1620 nm).
Maximum output power (continuous power during tuning):
  ≥ +14.5 dBm peak (typical),
  ≥ +13 dBm (1570 nm to 1620 nm),
  ≥ +10 dBm (1520 nm to 1630 nm).
Power linearity: ± 0.1 dB.
Power stability: ± 0.01 dB over 1 hour.
Power flatness versus wavelength: ± 0.2 dB, typical ± 0.1 dB (1570 nm to 1620 nm), ± 0.3 dB, typical ± 0.15 dB (full range).
Power repeatability (typical): ± 0.01 dB.
Side-mode suppression ratio (typical): ≥ 50 dB.

Options.
071, PMF, straight contact output connector.
072, PMF, angled contact output connector.



 

Standard Calibration $780.00 *
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*This is a Web introductory price for one calibration of the Keysight (Agilent) 81940A. 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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