JDSU MOPM-C1 CALIBRATION and JDSU MOPM-C1 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 JDSU MOPM-C1 Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

Need another Optical Power Meter?
Shop for Comparable Products on our  used Optical Power Meter page or new Optical Power Meter page

 
   JDSU MOPM-C1   Description / Specification:    
JDSU MOPM-C1 750 to 1700 nm Optical Power Meter Module

The JDSU mOPM-C1 (multiple application platform optical power meter module) is a third-generation power meter that brings a range of panel-mount and remote-head configurations to the Viavi Solutions MAP-200 platform. The MAP Optical Power Meter (mOPM-C1) module extends the optical power measurement capability of the MAP series by offering four grades of optical performance in panel-mount or remote-head configurations with 1, 2, or 4 inputs per module. Designed with 4 unique performance ranges, versions are available for all applications. Models with 110dBm dynamic range are complimented by versions that support 26dBm input power. The mOPM can be used for numerous applications such as measuring DUT settling time, cross talk, rise and fall times. It can also be used to measure synchronization and insertion loss stability. Also, allows for performance comparison (for example, comparing sequential switching to random switching).

Features and Benefits.
  Panel-mount or remote-head configuration.
  Single-, dual-, or quad-channel configurations available.
  Compatible with single-mode and multimode fiber.
  Ability to store up to 100,000 data points per channel.
  All four performance grades are based on indium gallium arsenide (InGaAs) detectors and are suitable for applications using singlemode (SM) or multimode (MM) fiber. The response of the detector varies with the wavelength of the incident light.

Specifications.
Maximum Input Power: 27 dBm.
Operating Wavelength Range: 750 to 1700 nm.
Sampling Rate: 250 kHz.
Dynamic Range: 110 dB.
Compliance: CE, CSA/UL/IEC61010-1, and LXI Class C requirements (when installed in a MAP chassis).

Options and Configurations.
The mOPM-C1 is available in four detector types in 1,2 or 4 detectors per cassette. It is also offered in cassette mounted or remote detector option.

Detector type:
2mm InGaAs General Purpose.
  Measures power levels from -70 to +11 dBm over the wavelength range of 800 to 1650 nm.
  Features high accuracy, very linear behavior and low relative uncertainty due to polarization.
3mm InGaAs Premium performance.
  Measures power levels from -80 to +11 dBm over the wavelength range of 750 to 1700 nm.
  Features high accuracy, very linear behavior and extremely low relative uncertainty due to polarization.
3mm InGaAs Ultra performance.
  Measures power levels from -110 to +11 dBm over the wavelength range of 750 to 1700 nm.
  In addition to the features of the Premium Performance detector, the Ultra Performance detector offers excellent stability for long term measurement of extremely low optical power levels.
Filtered 2mm InGaAs High power.
  Measures power levels from -45 to +27 dBm over the wavelength range of 800 to 1650 nm.
  Features high accuracy as well as very linear behavior.



 



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)

Please contact us for your JDSU MOPM-C1 CALIBRATION and/or JDSU MOPM-C1 750 to 1700 nm Optical Power Meter Module REPAIR
I'm interested in: 
Calibration Type (Select one):
Repair Information:
 Serial Number:

 Is there any physical damage?  
 If yes, describe:


What is the description of the problem?

How/when did the problem start?


 (*) Required Fields    For formal quote please fill in all fields.
Company:
From (Email):*
Contact Name:*
Country:*
Address 1:
Address 2:
City:
State/Territory/Province: *
Zip/Postal Code:
Phone:*

Comment: