Key considerations in choosing an optical power meter

Key considerations in choosing an optical power meter

 

 

Optical power meters for testing fiber optic components use semiconductor photodiodes as detectors to generate electrical current proportional to the incident optical power. This photocurrent is then measured, typically with a transimpedance amplifier and analog-to-digital converter, to determine that power. That requires the conversion factor from mA current to mW power, which depends on the wavelength of the light and combines contributions from the properties of the detector as well as any optics used to collect the light. Calibration of the power meter thus involves tracably measuring and recording the wavelength dependent responsivity and including this data with the instrument.

 

 

This responsivity is one of the key considerations in choosing an optical power meter for a particular application. First, the instrument must be calibrated at the wavelength of the light to accurately determine the absolute power level. If only relative power change will be measured, as for determining the attenuation of a passive optical component, this calibration factor is not actually needed. However it is still necessary that the detector has sufficient responsivity for this wavelength. For measuring light that is distributed over a range of wavelength or for which the wavelength is not accurately known, it is

 

also important that the variation of responsivity over wavelength is not too large.

 

 Example responsivity spectra for optical power meters based on three commonly used semiconductor materials are shown in Fig. 1. These are actual calibration data for individual instruments and the curves can vary somewhat from unit to unit, but the spectral shapes are primarily determined by the detector material. The values displayed on the y-axis correspond approximately to conversion efficiency in mA/mW. For wavelengths supported by standard single-mode fiber from about 1250 nm to 1650 nm, the InGaAs detector (like used here in the fiber-mart.com 81624B optical head) provides the highest performance with high responsivity and relatively low wavelength dependence. InGaAs (atually a shorthand label for the alloy chemical formula InxGa1-xAs) as a direct-gap semiconductor also typically provides the lowest noise level which permits power measurements over the widest dynamic range.

 

The germanium detector is useful over an even wider wavelength range and is less expensive, so these make good general purpose power meters. However the steep wavelength dependence above about 1545 nm makes the measurements more sensitivity to wavelength uncertainty or instability.

 

850 nm optical power measurement

Fiber links for transmission over short distances, like within buildings and data centers, predominantly use multimode fiber and signals at 850 nm. Another less common wavelength used with this fiber is 1300 nm. The wavelength here is a nominal value and the actual wavelength can be offset substantially. For example the IEEE 802.3 standard requires center wavelength to be between 840 nm and 860 nm. Other applications may tolerate wider wavelength variation. If the actual wavelength of such sources is not used to make the optical power measurement, this variation contributes to the measurement uncertainty. With this in consideration, the silicon detector has clear advantages. The responsivity is about five times stronger than for germanium, which itself is stronger than for the InGaAs detector. But more important for measuring moderate signal levels like 1 mW is the dependence on wavelength, as shown expanded for this wavelength.

 

Additional functionality of the optical power meters

fiber-mart.com optical power meters do support a programming command to read out the wavelength responsivity calibration data (like used for the graphs in this document). This can be used for example in post-processing to get calibrated absolute power values without needing to change the wavelength setting of the power meter each time that the wavelength of the signal is changed. That can be especially helpful when the optical power meter logging function is used to record a series of samples, during which the wavelength setting cannot be changed. When used together with a tunable laser, this can provide the input power to a device under test, while the wavelength is swept. That is important for example to measure O/E conversion devices. It can also be used to normalize a reference measurement made on one optical power meter port for use as reference on other power meter ports connected to the device.

 

Besides simple optical power measurements, fiber-mart.com optical power meters provide higher functionality, especially including the logging function just mentioned and flexible internal and external triggering functions for synchronization with other instruments or the DUT itself. The optical head models mentioned above have memory for up to 20k samples with individual averaging times selectable between 100 µs and 10 s duration. Other models support logging of up to 1M samples and averaging times down to 1 µs. The optical heads also provide an analog output signal with a voltage proportional to the input optical power. Especially combined with the large 5 mm diameter detector area, this supports various automated alignment procedures. The heads can be used to measure open beams and have a selection of fiber connector adapters. As external heads connected to the mainframe with a cable, these can be located conveniently on optical tables or workbenches.