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© 2012 Rensselaer Polytechnic Institute. All rights reserved. Quantifying Stroboscopic Effects from Flickering Light Sources John D. Bullough, Ph.D. N. Narendran, Ph.D. Lighting Research Center, Rensselaer Polytechnic Institute Council for Optical Radiation Measurements Conference Ottawa, ON May 29-June 1, 2012

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Page 1: Quantifying Stroboscopic Effects from Flickering …cormusa.org/wp-content/uploads/2018/11/2012_2.10...© 2012 Rensselaer Polytechnic Institute. All rights reserved. Quantifying Stroboscopic

© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Quantifying Stroboscopic Effects from Flickering Light Sources

John D. Bullough, Ph.D. N. Narendran, Ph.D.

Lighting Research Center, Rensselaer Polytechnic Institute

Council for Optical Radiation Measurements Conference

Ottawa, ON May 29-June 1, 2012

Page 2: Quantifying Stroboscopic Effects from Flickering …cormusa.org/wp-content/uploads/2018/11/2012_2.10...© 2012 Rensselaer Polytechnic Institute. All rights reserved. Quantifying Stroboscopic

© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Introduction

All electric light sources produce flicker › 120 Hz flicker is common in North America because of

60 Hz alternating current (AC) power

New light sources such as light-emitting diodes (LEDs) can use a wide variety of driving methods

Quantifying the effects of flicker from light sources can be important in specifying light source performance in many lighting applications

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Perception of Flicker

Visual sensitivity to flicker can be characterized in two ways: › Direct perception of light modulation (at ~80 Hz and lower frequency)

› Indirect perception of stroboscopic effects (phantom array, wagon-wheel effect)

Characteristics of flicker that might influence perception include: › Frequency*

› Modulation depth*

› Duty cycle

› Waveform shape

› Correlated color temperature

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

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Flicker Terminology Frequency (cycles

per second)

Modulation depth

(Percent flicker:

[max-min]/ [max+min])

Modulation depth

(Flicker index: area

above average/ total area

flicker index: 0.5

flicker index: 0.9

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Detection of Stroboscopic Effects

5

100% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

54% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

25% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

5% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

Bullough et al. (2012)

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Acceptability of Stroboscopic Effects

6

100% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

54% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

25% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

5% flicker

0%

20%

40%

60%

80%

100%

0 1 2 3 4 5 6

rel. time

rel.

light

out

put

Bullough et al. (2012)

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Quantitative Modeling

Detection (d, from 0%-100%):

Acceptability (a, from -2 to +2):

f: frequency in Hz (from 100-10,000 Hz) p: percent flicker (from 5%-100%)

Bullough et al. (2012)

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Model Application Example

A 60 W incandescent lamp, operated on 50 Hz AC power, produces 10% flicker at 100 Hz (IES 2000)

What combinations of frequency and percent flicker will produce stroboscopic effects no more detectable than 100 Hz/10% flicker?

At 120 Hz, pmax = 14% flicker

At 250 Hz, pmax = 34% flicker

At 1000 Hz, pmax = 100% flicker

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Comparison of Light Source Temporal Waveforms

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• Equipment: Oscilloscope

Photocell/resistor pair

• Photocell was affixed to a stand within the beam of the light source

• Light source was powered up and allowed to warm up/stabilize

• Waveform showing the temporal modulation of the source was captured from the oscilloscope

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Comparison of Light Source Temporal Waveforms (cont’d.)

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Fluorescent lamp on magnetic ballast

Frequency: 120 Hz

Percent flicker: 36%

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Comparison of Light Source Temporal Waveforms (cont’d.)

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Metal halide lamp

Frequency: 120 Hz

Percent flicker: 52%

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Comparison of Light Source Temporal Waveforms (cont’d.)

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High pressure sodium lamp

Frequency: 120 Hz

Percent flicker: 95%

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Comparison of Light Source Temporal Waveforms (cont’d.)

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Light-emitting diode

Frequency: 120 Hz

Percent flicker: 18%

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Comparison of Light Source Temporal Waveforms (cont’d.)

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Light-emitting diode

Frequency: 120 Hz

Percent flicker: 100%

-1

-0.5

0

0.5

1

1.5

0 10 20

rela

tive

light

out

put (

arb.

uni

ts)

time (ms)

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

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Comparison of Light Source Temporal Waveforms (cont’d.)

LED2 HPS

MH

WWF

LED1 INC

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Comparison of Light Source Temporal Waveforms (cont’d.)

LED2 HPS

MH

WWF

LED1 INC

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© 2012 Rensselaer Polytechnic Institute. All rights reserved.

Summary

All electric light sources produce some flicker

A model of the detection and acceptability of stroboscopic effects from flicker has been developed (Bullough et al. 2012)

Even when stroboscopic effects can be detected they are not necessarily unacceptable

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Acknowledgments

Alliance for Solid-State Illumination Systems and Technologies (ASSIST) members › www.lrc.rpi.edu/programs/solidstate/assist

Nicholas Skinner, Kathryn Sweater Hickcox (LRC)