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Warm up the laser and detectorWarming up is an essential part of getting the best results when measuring laser power because it can vary with time, particularly just after turning on the laser system. This is due to temperature and material changes within the laser as it reaches a balance with its environment. It is therefore recommended that laser power not be measured during the first few minutes after it’s turned on.It is equally important to warm up the power detector. Making sure it reaches equilibrium with its environment helps acquire the most accurate measurements possible; otherwise, further heat transfer can interfere with the measurement process.A laser power detector should remove heat efficiently—some systems come with fan or water cooling for this purpose. If the power meter does not, it is important to provide sufficient space around it.Precautions for low power measurementsKeep room temperature as constant as possible to avoid positioning thermal detectors near fans, or any sources of heat or air convection. This will help null the effects of thermal drift and thus reduce thermal noise and measurement uncertainty.Users should also avoid touching the casing of the detector or putting it in contact with a heat source, as this can create an offset in the measurements.Isolating the detector from undesired radiation sources is important. Photodetectors can be affected by ambient lighting, and very sensitive broadband detectors can even react to people moving around the room. Optical filters and enclosures can block unwanted interferences and isolate the detector from heat and air currents.One thing to keep in mind is to check if the chosen environment is suitable for power measurements, which allows characterization of the ambient noise by an acquisition (with laser turned off).Zero the power meterA laser power meter will feature a function that will allow the user to “zero” the device, eliminating the offset coming from the environment. It is important to use this after warming everything up appropriately and blocking the laser beam. It is also important to use a proper tool—not a hand—to block the beam.If there is uncertainty about a measurement or a systematic error is suspected, it may be worth repeating the zeroing process as a check. For longer tests, it is recommended that zeroing be repeatedly carried out once every four hours, especially when there are changes in room temperature or lighting conditions.Measuring laser powerThe beam can now be unblocked and the laser power measured. Leave the beam unblocked for at least a minute ahead of time to ensure that everything is stable.If the laser power meter has an anticipation or speed-up function, a full minute is not required, as the meter is able to work out what the measurement value should be. This may be useful in certain situations where a quicker measurement is needed.Potential challengesLaser power meters are very stable and should yield highly repeatable results. There shouldn’t be more than about half of a percent variation in power measurement; if it is larger than that, try re-zeroing. This may be required as a result of changes in the environment. Re-zeroing should help to identify whether or not this is the problem. Alternatively, the issue may be a result of the stability of the laser itself.Double-check the following factors:Is the laser beam properly aligned and fully contained in the detector’s aperture?Is the correct wavelength entered in the power meter or software controls?Is the detector’s surface scratched or damaged?Was the detector recalibrated recently? How often this should be done depends on multiple factors, but the general recommendation is every 12 to 18 months.And that’s it! Measuring laser power like an expert is in fact possible in just a few simple steps.
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Laser power meters are very stable and should yield highly repeatable results. There shouldn’t be more than about half of a percent variation in power measurement; if it is larger than that, try re-zeroing. This may be required as a result of changes in the environment. Re-zeroing should help to identify whether or not this is the problem. Alternatively, the issue may be a result of the stability of the laser itself.
According to corresponding author Andrew Forbes, SPIE Fellow and Distinguished Professor at University of the Witwatersrand in Johannesburg, “What is exciting about the work is that it opens up a new approach to studying complex light in complex systems — for instance, in transporting classical and quantum light through optical fiber, underwater channels, living tissue, and other highly aberrated systems.” He adds, “Because of the nature of eigenmodes, it doesn’t matter how long this medium is, nor how strong the perturbation, so that it should work well even in regimes where traditional corrective procedures, such as adaptive optics, fail.” Maintaining the integrity of structured light in complex media will pave the way to future work in imaging and communicating through noisy channels, which is particularly relevant when the structured forms of light are fragile quantum states.
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It is equally important to warm up the power detector. Making sure it reaches equilibrium with its environment helps acquire the most accurate measurements possible; otherwise, further heat transfer can interfere with the measurement process.
Do you need to measure laser power more accurately? With a laser power detector, the process is relatively straightforward. However, there are some important steps needed to ensure an accurate measurement.
If there is uncertainty about a measurement or a systematic error is suspected, it may be worth repeating the zeroing process as a check. For longer tests, it is recommended that zeroing be repeatedly carried out once every four hours, especially when there are changes in room temperature or lighting conditions.
Users should also avoid touching the casing of the detector or putting it in contact with a heat source, as this can create an offset in the measurements.
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A laser power meter will feature a function that will allow the user to “zero” the device, eliminating the offset coming from the environment. It is important to use this after warming everything up appropriately and blocking the laser beam. It is also important to use a proper tool—not a hand—to block the beam.
One thing to keep in mind is to check if the chosen environment is suitable for power measurements, which allows characterization of the ambient noise by an acquisition (with laser turned off).
On the other hand, a beam that is too large can lead to wasted power not being transferred to the detector. Ideally, beam diameter should be between 40% and 60% of the optical aperture area. This is the best way to optimize the absorption of heat by the power detector.
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Read the Gold Open Access article by A. Kug, C. Peters, and A. Forbes, “Robust structured light in atmospheric turbulence,” Adv. Photon. 5(1) 016006 (2023) doi 10.1117/1.AP.5.1.016006.
The beam can now be unblocked and the laser power measured. Leave the beam unblocked for at least a minute ahead of time to ensure that everything is stable.
If the laser power meter has an anticipation or speed-up function, a full minute is not required, as the meter is able to work out what the measurement value should be. This may be useful in certain situations where a quicker measurement is needed.
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An exciting prospect in modern optics is to exploit patterns of light — how the light looks in its many degrees of freedom — often referred to as “structured light.” Each distinct pattern could form an encoding alphabet for optical communication, or might be used in manufacturing to enhance performance and productivity. Unfortunately, patterns of light get distorted when they pass through noisy channels, for instance, stressed optical fiber, aberrated optics, turbid living tissue, and perhaps a very severe example, atmospheric turbulence in air. In all these examples, the distorted pattern can deteriorate to the point that the output pattern looks nothing like the input, negating the benefit. As reported in Advanced Photonics, researchers in South Africa have shown how it is possible to find distortion-free forms of light that come out of a noisy channel exactly the same as they were put in. Using atmospheric turbulence as an example, they showed that these special forms of light, called eigenmodes, can be found for even very complex channels, emerging undistorted, while other forms of structured light would be unrecognizable.
Warming up is an essential part of getting the best results when measuring laser power because it can vary with time, particularly just after turning on the laser system. This is due to temperature and material changes within the laser as it reaches a balance with its environment. It is therefore recommended that laser power not be measured during the first few minutes after it’s turned on.
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Isolating the detector from undesired radiation sources is important. Photodetectors can be affected by ambient lighting, and very sensitive broadband detectors can even react to people moving around the room. Optical filters and enclosures can block unwanted interferences and isolate the detector from heat and air currents.
Selecting the power meter’s correct wavelength makes a difference as well, because the response of optical detectors is not the same for every wavelength. Detector manufacturers encode the spectral response inside a chip in the detector, and power meters use this correction factor to display the correct value at a specific wavelength. This is especially crucial for photodiodes, as their sensitivity varies greatly over the spectrum.
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The first thing to do is choose a laser power meter. There are a large range of specialty power meters available and determining exactly which one will work best can be tricky. However, choosing the correct one is critical to getting an accurate and reliable power measurement for a given application (see Fig. 1). The main factors influencing the choice in detector technology include the laser’s power, beam size, and wavelength. For pulsed lasers, energy per pulse, repetition rate, and pulse width could also influence the choice. To find a durable product, it is important to check that the laser power detector will be able to handle both the energy and power densities.
When selecting a power meter, think about what beam diameter is required for measurements. This is crucial for accuracy and using a beam diameter that is too small can damage the power detector, given the high-power density of a smaller beam.
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A laser power detector should remove heat efficiently—some systems come with fan or water cooling for this purpose. If the power meter does not, it is important to provide sufficient space around it.
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Keep room temperature as constant as possible to avoid positioning thermal detectors near fans, or any sources of heat or air convection. This will help null the effects of thermal drift and thus reduce thermal noise and measurement uncertainty.
Passing light through the atmosphere is crucial in many applications, such as free-space optics, sensing, and energy delivery, but finding how best to do this has proved challenging. Traditionally a trial-and-error approach has been used to find the most robust forms of light in some particular noisy channel, but to date all forms of familiar structured light have shown to be distorted as the medium becomes progressively noisier. The reason is that light can “see” the distortion. But is it possible to create light that doesn’t see the distortion, passing through as if it wasn’t there? To make this advance, the researchers treated the noisy channel as a mathematical operator and asked a simple question: what forms of light would be invariant to this operator? In other words, light waves that are in the natural modes of the channel behave as if they don’t see the distortion: the true eigenmodes of the channel. The example tackled was the severe case of distortions due to atmospheric turbulence. The answer to the problem revealed previously unrecognized forms of light, i.e., not in any well-known structured light family, but nevertheless completely robust to the medium. This fact was confirmed experimentally and theoretically for weak and strong turbulence conditions.