Keysight (Agilent) N7714A CALIBRATION and Keysight (Agilent) N7714A 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) N7714A 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) N7714A   Description / Specification:    
Keysight (Agilent) N7714A 1527-1565 or 1570-1608nm opt based 4 Port Tunable Laser Sour

The Agilent N7714A Tunable Laser Source is a four-port source, available with C-band or L-band wavelength coverage. With high output power up to +15 dBm, narrow linewidth of 100 kHz, gridless and grid-defined wavelength setting, and offset fine-tuning capability, the N7714A makes an ideal source for realistic loading of the latest transmission systems. Targeted for high test throughput, lowest cost-per-channel, and narrow footprint, all members of Agilent’s 77-Series optical test instruments are built on a common platform and a common PC-based user interface. A complete set of control interfaces including LAN, USB2.0 and GPIB simplifies integration with manufacturing control systems. Code compatible to Agilent’s Lightwave Measurement System modules, the new instrument generation can serve as plug-in replacements in existing test solutions. Specifications apply to wavelengths on the 50 GHz ITU-T grid, after 1 hour warm-up, in non-condensing conditions, in CW operation. Wavelength (frequency) range: 1527.60 nm to 1565.50 nm (196.25 THz to 191.50 THz) Opt 222 and 240, 1570.01 nm to 1608.76 nm (190.95 THz to 186.35 THz) Opt 222 and 204. Frequency (wavelength) resolution:100 MHz (0.8 pm at 1550 nm). 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 ± 2.5 pm (± 0.3 GHz), 24 hours (Typical ± 0.5 pm, 1 minute). Tuning time: Typical < 30 sec. Max. output power: >= +13.5 dBm (Typical >= +15 dBm). Power stability: Typical ± 0.03 dB over 24 hours. Power flatness: Typical ± 0.2 dB (full wavelength range). Power repeatability: Typical ± 0.08 dB. Linewidth: Typical < 100 kHz (SBS suppression off). Side mode suppression ratio (SMSR): Typical 50 dB. Relative intensity noise (RIN): Typical –145 dB/Hz (10 MHz to 40 GHz). Grid spacing: 100 GHz, 50 GHz, 25 GHz, or arbitrary grid. Fine tuning speed: 15 sec from -6 GHz to +6 GHz. Power attenuation range: 8 dB. Power setting resolution: 0.1 dB. Fiber type: 9/125 µm panda PMF, TE mode in slow axis, in line with connector key. Polarization extinction ratio: 16 dB typical. Output isolation: 30 dB typical. Options. 071, Straight connector interface, PMF. 072, Angled connector interface, PMF. 240, 4 C-band lasers. 204, 4 L-band lasers. 222, 2 C-band lasers and 2 L-band lasers.



 

Standard Calibration $675.00 *
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*This is a Web introductory price for one calibration of the Keysight (Agilent) N7714A. 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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