Keysight (Agilent) 81950A CALIBRATION and Keysight (Agilent) 81950A 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 Keysight (Agilent) 81950A 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) 81950A   Description / Specification:   Spec Sheet 
Keysight (Agilent) 81950A 1527-1565 or 1570-1608 nm opt based Tunable Laser Module

The Agilent 81950A compact tunable laser source is step-tunable for setting channel frequencies within any grid in the C- or L-band. With high output power up to +15 dBm, narrow linewidth of 100 kHz, and offset grid fine-tuning capability, the 81950A is a universal source for realistic loading of the latest transmission systems. It is available with C-band or L-band wavelength coverage. It can reach any wavelength point within its specified wavelength range just like all other Agilent tunable lasers. In system loading applications, it may be preferable to grid-tune the laser like system transmitters, simply by changing the channel index. The channel grid is adjustable to standard ITU-T grid spacing like 50 GHz, and to arbitrary grids. Likewise, the zero frequency (base channel) of the chosen grid is adjustable. A 12 GHz fine-tuning range allows de-tuning the frequency. Specifications. Wavelength (frequency) range: 1527.6 nm to 1565.50 nm (Option 210), 1570.01 nm to 1608.76 nm (Option 201). Frequency resolution: 100 MHz, 0.8 pm at 1550 nm. Tuning time: Typical < 30 sec. Fine tuning range: Typical ± 6 GHz. Fine tuning resolution: Typical 1 MHz. Absolute wavelength (frequency) accuracy: ± 22 pm (± 2.5 GHz). Relative wavelength (frequency) accuracy: ± 12 pm (± 1.5 GHz). Wavelength (frequency) repeatability: Typical ± 2.5 pm (± 0.3 GHz). Wavelength (frequency) stability (typical, over 24 hours): Typical ± 2.5 pm (± 0.3 GHz), 24 hours. Linewidth (typical), SBS suppression off: < 100 kHz. Maximum output power: = +13.5 dBm (typical = +15 dBm). Power stability Typical: ± 0.03 dB over 1 hour. Power flatness: Typical ± 0.2 dB (full wavelength range). Power repeatability: Typical ± 0.08 dB. Side-mode suppression ratio: Typical 50 dB. Relative intensity noise (RIN): Typical -145 dB/Hz (10 MHz to 40 GHz).



 

Standard Calibration $455.00 *
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*This is a Web introductory price for one calibration of the Keysight (Agilent) 81950A. 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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