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
It is also available for immediate rental.
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 $675.00 *
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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.

dBm
Optical power referenced to 1 millimatt

Multimode Fiber
Multimode Fiber has a large core (almost always 62.5 microns - a micron is one one millionth of a meter - but sometimes 50 microns) and is used with LED sources at wavelengths of 850 and 1300 nm for short distance, lower speed networks like LANs. Both multimode and singlemode fiber have an outside diameter of 125 microns - about 5 thousandths of an inch - just slightly larger than a human hair.

Power Repeatability
Power Repeatability is the random uncertainty in reproducing the power level after changing and re-setting the power level. The power repeatability is ± half the span (in dB) between the highest and lowest actual power. Note: - The long-term power repeatability can be obtained by taken the power repeatability and power stability into account.

Refractive Index
The refractive index or index of refraction of a substance is a measure of the speed of light in that substance. It is expressed as a ratio of the speed of light in vacuum relative to that in the considered medium. The velocity at which light travels in vacuum is a physical constant, and the fastest speed at which energy or information can be transferred. However, light travels slower through any given material, or medium, that is not vacuum.

Total insertion loss
A measure of the loss of light within an optical component


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