Keysight (Agilent) N4375B REPAIR and Keysight (Agilent) N4375B CALIBRATION
 
Custom-Cal has a high success rate in the repair of the Keysight (Agilent) N4375B. 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) N4375B 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) N4375B   Description / Specification:    
Keysight (Agilent) N4375B 20/26.5 GHz Single-Mode Lightwave Component Analyzer

The Agilent N4375B Lightwave Component Analyzer (LCA) tests 10G Ethernet, FCx8, FCx10 and FCx16 electro-optical components, with up to 20 or 26.5 GHz modulation range. It comes in two basic versions. The economic line is based on a PNA-L network-analyzer and is available as a 2 port system. The high end version is based on the new PNA-X and offers true balanced measurements, extended optical modulation index (OMI) and is available with 2 or 4 ports. Both versions have the same specifications up to 20 GHz. The PNA-X based LCA is calibrated up to 26.5 GHz.
Specifications.

Optical test set.
Operation frequency range: 10 MHz to 20 GHz (Opt -322, -382), 10 MHz to 26.5 GHz (Opt -312, -314, -392, -394).

LCA optical input.
Operating input wavelength range: 1250 nm to 1640 nm.
Maximum linear average input power: +4 dBm (Input 1), +14 dBm (Input 2).
Maximum safe average input power: +7 dBm (Input 1), +17 dBm (Input 2).
Optical return loss (typical): > 27 dBo.
Average power measurement range: -25 dBm to +4 dBm (optical input 1), -15 dBm to +14 dBm (optical input 2).
Average power measurement uncertainty (typical): ±0.5 dBo.

LCA optical output.
Optical modulation index (OMI) at 10 GHz (typical): > 27% @ +5dBm RF.
Output wavelength: 1310 ± 20 nm, 1550 ± 20 nm (Opt -100, -102).
Average output power range: -2 dBm to +4 dBm.
Average output power uncertainty (typical): ± 0.5 dBo.
Average output power stability, 15 minutes (typical): ± 0.5 dBo.

External optical source input (-050).
Recommended optical input power: +8 to + 15 dBm.
Optical input power damage level: +20 dBm.
Typical loss at quadrature bias point: 9 dB.
Operating input wavelength range: 1290 nm to 1610 nm.

LCA RF test port input.
Maximum safe input level at port A or B: +15 dBm RF, 7V DC.

Options.
-312; 26.5 GHz, 2 port LCA based on N5242A-200.
-314; 26.5 GHz, 4 port LCA based on N5242A-400.
-322; 20 GHz, 2 port LCA based on N5230C-225.
-382; Integration of customer PNA-L.
-392; Integration of customer PNA-X (N5242A -200).
-394; Integration of customer PNA- X (N5242A -400).
-100; 1310 nm source optical test set.
-101; 1550 nm source optical test set.
-102; 1310 nm and 1550 nm source optical test set.
-010; Time domain.
-050; External optical source input.
-021; Straight connector interface (External 0.5 m patch cord).
-022; Angled connector interface (External 0.5 m patch cord).



 

Standard Calibration $1,485.00 *
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*This is a Web introductory price for one calibration of the Keysight (Agilent) N4375B. 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.

Absolute Wavelength Accuracy
Absolute Wavelength Accuracy is the maximum difference between the actual wavelength and the displayed wavelength of the Optical Source. Wavelength is defined as wavelength in vacuum.

Decibel (dB)
A unit of measurement of optical power which indicates relative power. A -10 dB means a reduction in power by 10 times, -20 dB means another 10 times or 100 times overall, -30 means another 10 times or 1000 times overall and so on.

Nanometer (nm)
A unit of measure used to measure wavelength of light, meaning one one-billionth of a meter

Relative Intensity Noise (RIN)
Relative intensity noise (RIN), describes the instability in the power level of a laser. The noise term is important to describe lasers used in fiber-optic communication and LIDAR remote sensing. It is the square of the (spectrally resolved) RMS optical power amplitude divided by the measurement bandwidth and the square of the average optical power, expressed in dB/Hz.

Total Return loss
In an optical fiber, the loss that takes place at any discontinuity of refractive index, especially at an air-glass interface such as a fiber endface, at which a fraction of the optical signal is reflected back toward the source. RL = - 10log10 (Preflected/Preference)

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