Anritsu MS9710C Optical Spectrum Analyzer

The MS9710C is a diffraction grating optical spectrum analyzer for analyzing optical spectra in the wavelength range of 600 to 1750 nm. In addition to uses such as measuring LD and LED spectra, it also has the function of measuring the transmission characteristics of passive components such as optical isolators and the NF/gain of fiber amplifier systems.
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Anritsu MS9710C Optical Spectrum Analyzer

The MS9710C is a diffraction-grating spectrum analyzer for analyzing optical spectra in the 600 to 1750 nm wavelength band. In addition to uses such as measurement of LD and LED spectra, it has functions for measuring the transmission characteristics of passive elements such as optical isolators, as well as NF/Gain of optical fiber amplifier systems. In addition to its basic features, the superior stability and reliability of the diffraction grating (patent pending) offer the severe level and wavelength specifications particularly in the WDM band. This analyzer has the dynamic range, reception sensitivity and sweep speed requested by users, backed by Anritsu’s highlevel technology. The high sensitivity meets the exacting demands placed on today’s measuring instruments. In particular, the excellent wavelength and level specifications fully meet the dense WDM requirements (1520 to 1620 nm). The MS9710C Optical Spectrum Analyzer is the successor to the popular MS9710B but with improved functions and higher performance. The specifications have been upgraded for the important 1.55 µm band for WDM communications and have also been optimised to include the new requirements for the L-band (1570 to 1620 nm) use. In addition to the high reliability and excellent basic performance, this analyzer has a full range of application functions to support accurate measurement in the fastest possible time.

Feature:

  • ·TFT color screen,
  • ·600 to 1750 nm,
  • ·Accuracy: wavelength ±20 pm (1530 to 1570 nm), ±20 to ± 50 pm (1520 to 1620 nm),
  • ·Possibility of optional SD reader,
  • ·Programmable GP-IB.

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