Episode 21 1:37 Quality EN · العربية

Flicker, the invisible quality you only notice when it's gone

A rectified mains supply ripples at twice the line frequency, so on the Saudi 60 Hz grid an LED's output pulses at 120 Hz. Done well you never notice. Done badly it bands on camera, and it is measurable: IEEE 1789 grades depth against frequency, CIE TN 006 defines the modern metrics, and IEC TR 61547-1 and IEC TR 63158 give the methods for measuring Pst LM and SVM.

A television studio lit by overhead LED panels, with a broadcast camera on a pedestal
Animated explainer, press play to watch the concepts now; the filmed cut publishes once production wraps.

What you'll walk away with

Four ideas to carry into the next specification conversation you have.

01

Depth means nothing without frequency.

IEEE 1789 grades the pair, not either alone. On the Saudi 120 Hz ripple the low-risk ceiling is 9.6% modulation and the no-effect ceiling is 4.0%. At 60 Hz the same two lines allow only 1.5% and 0.6%.

02

Percent flicker and flicker index are the old metrics.

Percent flicker = 100 × (max − min) / (max + min). Flicker index = the area of one cycle above the average light level, over the total area. Neither carries any frequency information at all, which is exactly why neither is enough on its own.

03

SVM measures stroboscopic effect on moving objects.

Stroboscopic Visibility Measure, defined in CIE TN 006. SVM = 1 is the visibility threshold, where an average observer detects the effect half the time. The EU's SVM ≤ 0.4 is a legal ceiling well below that, not a "no effect" line.

04

PstLM measures perceptible flicker for static viewers.

Measured by the light flickermeter method in IEC TR 61547-1, which sets no limit itself. Pst LM = 1.0 does not mean imperceptible: it means the source is as flickery as a 60 W incandescent lamp, which about half of viewers notice.

WHERE IT COMES FROM
On a 60 Hz grid, mains-related LED ripple commonly appears at 120 Hz
1 mains cycle = 2 light pulses
120 Hz is common, not inevitable. A well-filtered driver can reduce this modulation substantially.
THE TWO OLD NUMBERS
What percent flicker and flicker index actually measure
maxmeanmin0percent flicker = 100 x (max - min) / (max + min) = 50%flicker index = area 1 / (area 1 + area 2) = 0.16
Neither metric includes frequency. Both are read from a single cycle, so they cannot tell you how fast it repeats.
A lit LED softbox at the left of a dark studio, a cinema camera on a fluid head facing it from the right

Flicker metrics × thresholds × who cares

The Saudi grid runs at 60 Hz, so the ripple to design against is 120 Hz, not the 100 Hz behind most published rules of thumb. IEEE 1789 supplies the depth-against-frequency lines; the Pst LM and SVM ceilings are EU law, not measurement standards.

Metric Threshold Affected scenario
Modulation depth at 120 Hz< 9.6%IEEE 1789 low risk, 0.08 × f, on the Saudi ripple
Modulation depth at 120 Hz< 4.0%IEEE 1789 no observable effect, 0.0333 × f
Modulation depth below 90 Hz< 5%IEEE 1789 Recommended Practice 3, the only unconditional one
Pst LM≤ 1.0 at full loadEU ecodesign limit. Pst LM = 1 is the 50% detection point, not silence
SVM≤ 0.4 at full loadEU ecodesign since 1 Sep 2024. Visibility threshold is SVM = 1
Percent amplitude modulation< 30% below 200 HzCalifornia Title 24 JA8, required at full output and at 20%
WHY ONE NUMBER IS NOT ENOUGH
Same modulation depth. Different waveform. Different index.
percent flicker 50%flicker index 0.16percent flicker 50%flicker index 0.26
Both waveforms modulate 50%. The pulse scores a flicker index of 0.26 against the sine's 0.16, because the index reads the shape between the extremes.
THE RISK PLANE
IEEE 1789 is a plane, not a number
0.1%1%10%100%10 Hz100 Hz1 kHz3 kHzRP3 5%120 Hzdepth (y) against frequency (x), both log
IEEE 1789 gives frequency-dependent recommended practices, not one universal percentage. Its 8% and 9.6% both come from the low-risk line, Mod% < 0.08 x f, at 100 Hz and 120 Hz.
An oscilloscope showing a rippling waveform beside a photodiode probe aimed at a lit LED panel

Why flicker finally made it onto spec sheets

Five points the lighting industry only agreed on after 2015.

Fluorescent flickered too; we just accepted it.

Magnetic-ballast fluorescent measured roughly 30% to 49% modulation, not the 100% often quoted. A 1989 double-blind cross-over study in occupied offices more than halved headaches and eyestrain by moving from switch-start choke ballasts at 43% to 49% modulation to 32 kHz electronic ballasts under 7%. LEDs reopened the conversation because some drivers are worse than the fluorescent they replaced, and cameras finally exposed it.

IEEE 1789 is a risk plot, not a single number.

The 2015 standard plots modulation depth against modulation frequency and shades two regions: the no-observable-effect region and the low-risk region. It names no third zone, and it says outright that operating outside them "does not necessarily imply high risk". The word NIOSH appears nowhere in it. Above 1250 Hz, 100% modulation becomes low risk; it only becomes no-observable-effect above 3000 Hz. And 1250 Hz is not a rule in its own right, it is simply where the line 0.08 × f reaches 100%, which is why it attaches to PWM dimming.

Phone cameras are the modern flicker meter.

A rolling-shutter sensor writes the light's waveform down the frame, so a phone can reveal modulation a viewer cannot see. It is a one-way test: a phone can reveal temporal light modulation but cannot certify its absence, because the anti-banding control defaults to automatic and its documented job is to choose an exposure that hides the bands. A clean image is not a compliance test. To screen a fixture, lock the phone to manual exposure at a speed that does not divide the modulation period, such as 1/250 on the Saudi grid, and look for bands.

Dimming is where cheap drivers betray themselves.

PWM dimming produces 100% percent flicker by construction; reducing the drive current instead holds it near zero. When California tested 25 LED A-lamps against its own filtered limit, 13 passed at both full output and 25% output, and 12 failed at 100%, at 25%, or at both. Dimming can expose modulation that a full-output test alone does not show. On a separate set of PAR38 lamps, simply installing a phase-cut dimmer and leaving it at full output raised measured flicker index by as much as 0.15, and by a ratio of at least three to one the products that moved got worse rather than better. Specify the requirement at 100%, 50%, 20% and minimum output.

Hospitals and schools have new specs.

Only one major scheme has a real gate: WELL v2 Feature L08. LEED v4.1 has no flicker requirement at all, in either the BD+C or the ID+C guides. BREEAM's only flicker criterion is a legacy high-frequency-ballast one for fluorescent lamps. Mostadam has no flicker credit, and its indoor lighting credit awards its point to fluorescent with high-frequency ballasts. The SASO lighting energy-efficiency standards reviewed, 2870, 2902 and 2927, set no Pst LM, SVM or modulation-depth limit. In Saudi projects, flicker performance therefore often rests on the project specification: write a limit and it can be tested and enforced.

READ THE STANDARD, NOT THE BLOG
Three recommended practices. Only one is unconditional.
RP2 0.6%RP3 5.0% · unconditionalRP1 1.5%0%at 60 Hz the only unconditional line is the loosest
Full-depth PWM is low risk only above 1250 Hz, where 0.08 x f reaches 100%. A driver under 9.6% at 120 Hz needs no kilohertz switching.
WHAT THE MODERN NUMBERS MEAN
Two thresholds that are routinely read backwards
equivalent modulation depth, pure 120 Hz sinusoid onlyIEEE no effect4.0%IEEE low risk9.6%EU law, SVM 0.411.0%SVM 1, detected27.6%the EU limit is looser than IEEE low risk, not stricter
Pure 120 Hz sinusoid only: SVM = 1 corresponds to about 27.6% modulation and SVM = 0.4 to about 11.0%.
HISTORICAL CALIFORNIA TEST DATA, 2014
Dimming can expose what a full-output test misses
reduced currentPWM at full heightboth reach the same average output
PWM dimming creates high modulation depth by design, while reducing the drive current adds little modulation of its own. On PAR38 lamps, adding a phase-cut dimmer at full output raised the measured flicker index by up to 0.15, and dimmed lamps usually got worse.

Why flicker carves dark bands into your footage

Your eye averages the pulse away. A camera sensor samples it in milliseconds, so the strobe your eye misses lands straight on the frame.

1

The light pulses with the mains, hundreds of times a second. Here it is slowed right down so you can watch it dim and brighten.

2

Many rolling-shutter sensors expose one row at a time, top to bottom, rather than the whole frame at once.

3

Rows caught on a dim pulse record dark, so the frame fills with the rolling dark bands you see on camera.

The rolling shutter reads the frame line by line.

Most CMOS sensors, in phones and cinema cameras alike, expose the image one row of pixels at a time, top to bottom, rather than all at once. While the sensor scans down, a flickering light keeps pulsing bright then dim. Rows captured on a bright pulse come out light; rows captured on a dim pulse come out dark. The result is a stack of horizontal dark bands rolling through the frame.

Banding in stills, pulsing in video.

In a single photo the bands freeze in place and ruin a product shot or a portrait under the wrong panel. In video they drift frame to frame and the clip breathes between bright and dark. High frame rates force short exposures, and a short exposure is precisely the case where almost none of the modulation is averaged away, so slow motion under a flickering source strobes hard. Frame rate and shutter speed fix different problems: frame-rate divisibility settles frame-to-frame pulsing, only exposure-time divisibility removes the bands.

It is shutter speed against the light's pulse.

The exposure has to contain a whole number of modulation periods. Integrating the light over a window of length T attenuates its modulation by |sinc(f × T)|, which is exactly zero when T is a whole multiple of 1/f, and because every harmonic is nulled at the same moment the rule works on any periodic waveform. Saudi mains runs at 60 Hz, so the light pulses at 120 Hz and the safe shutter speeds are 1/120, 1/60, 1/40, 1/30 and 1/24. 1/240 is not one of them: it is half a period, and it leaves about 64% of the modulation in the frame for a sinusoidal source and up to all of it for a PWM driver. 1/100 leaves about 16%, 1/250 about 66%, and 1/1000 about 98%.

High-frequency drivers fix it at the source.

Shutter tricks only patch one camera at one setting, so the fix belongs in the fixture. Raising the modulation frequency buys headroom rather than immunity: what survives an exposure is still |sinc(f × T)|, so a 1.25 kHz driver reads clean at ordinary shutter speeds, where the exposure spans many pulses, and still writes about 96% of its depth into a 1/8000 s frame. The depth is what makes it invisible: a driver held under the no-observable-effect line has little left to record at any shutter speed. Specify the depth and the frequency together at the fixture, and stop chasing either one in the camera.

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Sources & further reading

The standards, regulations and test reports behind every number on this page. Where a document defines a measurement method but sets no limit, that is stated.

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