ANRITSU MS9740A REPAIR and ANRITSU MS9740A CALIBRATION

 
Custom-Cal has a high success rate in the repair of the ANRITSU MS9740A. A calibration by Custom-Cal is performed by engineers with extensive OEM experience. We have the expertise and the necessary standards to perform the ANRITSU MS9740A Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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   ANRITSU MS9740A   Description / Specification:    
ANRITSU MS9740A 600 to 1750 nm Optical Spectrum Analyzer

The Anritsu MS9740A supports the performance and functions for evaluating all active optical devices, including SFP, XFP, and SFP+ modules, as well as optical transceivers and DFB optical sources. It has seven application modes (DFB-LD, FP-LD, LED, PMD, Opt. Amp, WDM, LD Module) matching the measurement target. For example, at evaluation of LD characteristics, analysis items and methods can be tailored to the spectrum, such as a single DFB-LD spectrum, multiple discrete-wavelength FP-LD, wideband LED, etc. Specifications. Wavelength measurement range: 600 nm to 1750 nm. Wavelength accuracy: ±20 pm (1520 nm to 1620 nm, Resolution: 0.03 nm to 0.2 nm), ±100 pm (1520 nm to 1620 nm, Resolution: 0.5 nm, 1.0 nm). Wavelength stability: <= ±5 pm. Wavelength linearity: ±20 pm (1520 nm to 1620 nm). Setting resolution: 0.03, 0.05, 0.07, 0.1, 0.2, 0.5, 1.0 nm; (RBW: 3 dB optical filter: transmission bandwidth). Level accuracy: ±0.4 dB (Wavelength: 1310 nm/1550 nm, Input: –10 dBm, Resolution: >=0.1 nm). Level stability: ±0.02 dB (1 min, Resolution: >= 0.1 nm, Input: -23 dBm, 1550 nm, no polarization fluctuation). High dynamic range: 70 dB (1 nm from peak wavelength), 60 dB (0.4 nm from peak wavelength), 42 dB (0.2 nm from peak wavelength). Normal dynamic range: 62 dB (1 nm from peak wavelength), 58 dB (0.4 nm from peak wavelength), 42 dB (0.2 nm from peak wavelength). Optical return loss: >= 35 dB (1300 nm/1550 nm). Sampling point: 51, 101, 251, 501, 1001, 2001, 5001, 10001, 20001, 50001. Supported optical fiber: 10 µm/125 µm SM fiber (ITU-T G.652), 50 µm/125 µm GI fiber. Optical connector: User replaceable; FC, SC, ST, DIN, LC. Display: 800 × 600 dots, 8.4 inch SVGA color LCD



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Standard Calibration $890.00 *
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*This is a Web introductory price for one calibration of the ANRITSU MS9740A. 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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