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Research matters - Illuminating Engineering Society

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RESEARCH MATTERS Nothing New Under the Sun?<br />

John D. Bullough,<br />

Lighting <strong>Research</strong><br />

Center, Rensselaer<br />

Polytechnic Institute<br />

IS THERE NOTHING NEW<br />

under the sun? Fifty years ago, the<br />

IESNA published a paper in its journal,<br />

then titled <strong>Illuminating</strong> <strong>Engineering</strong>,<br />

that simply amazes me.It is a paper by<br />

the eminent vision scientist W. S.<br />

Stiles, and it bears the inconspicuous<br />

title “Visual factors in lighting.” 1 The<br />

paper was one of a series of papers<br />

given at what appears to have been a<br />

special session of the IESNA’s annual<br />

technical conference, “A Symposium<br />

on Light and Vision,” along with other<br />

authors such as Weston, 2 Helson, 3<br />

Blackwell 4 and Fry. 5<br />

The paper by Stiles is remarkable<br />

for several reasons: it succinctly summarizes<br />

a series of issues pertaining<br />

to color, spectral distribution, brightness<br />

and glare, all areas of research I<br />

personally find particularly interesting.<br />

Further, I believe this information<br />

is pertinent to many of today’s vigorous<br />

discussions taking place at venues<br />

like LIGHTFAIR International, the<br />

IESNA Annual Conference and in the<br />

letters pages of LD+A on these very<br />

topics.<br />

In this column, I hope to touch on<br />

just a few of the “new” ideas in lighting<br />

that Stiles discussed all those<br />

years ago.<br />

Luminance Or Brightness?<br />

The photopic luminous efficiency<br />

function, V(λ ), provides a universallyapplied<br />

weighting for radiant power<br />

making up the portion of the electro-<br />

FIGURE 1<br />

magnetic spectrum known as light.<br />

V(λ ) was derived largely from flicker<br />

photometry studies that seem to do<br />

a decent job at capturing our spectral<br />

sensitivity for visual performance.The<br />

IESNA uses lighting quantities based<br />

on V(λ ) in all of its lighting recommendations,<br />

6 and we often use these<br />

quantities as stand-ins for responses<br />

The paper by Stiles<br />

is remarkable for<br />

several reasons:<br />

it succinctly<br />

summarizes a<br />

series of issues<br />

pertaining to color,<br />

spectral distribution,<br />

brightness and<br />

glare<br />

other than visual performance, such<br />

as brightness perception, but as Stiles<br />

points out, doing so can lead to serious<br />

errors.<br />

Brightness is a complex perception<br />

that depends upon many factors,<br />

including color saturation. Stiles<br />

shows a graph in his paper (Figure<br />

1) 7 that shows the relative brightness<br />

of colored objects of various dominant<br />

wavelengths and saturations.<br />

Relative brightness-to-luminance (B/L) ratios as a function of wavelength<br />

and saturation (λ ).<br />

Higher saturation results in higher<br />

brightness, as do dominant wavelengths<br />

that are both longer and<br />

shorter than about 580 to 590 nm<br />

(“yellow” light). In fact, the spectral<br />

power distribution of neodymiumcoated<br />

incandescent lamps, with a<br />

“notch” in spectral content near 580<br />

nm, may increase brightness by taking<br />

advantage of this phenomenon.<br />

Similar brightness correction factors<br />

have been published since 8,9 but it is<br />

interesting to see that this phenomenon<br />

has been known since V(λ ) was<br />

relatively young!<br />

Awash In LED Light?<br />

Another very interesting graph<br />

published in the paper by Stiles shows<br />

spectral sensitivity for the brightness<br />

perception of an object as it moves<br />

from the line of sight to the far<br />

periphery of the field of view, out to<br />

70 deg off axis. 10 As the object moves<br />

further from the line of sight, the<br />

spectral sensitivity changes dramatically.<br />

Close to the line of sight, brightness<br />

seems to be determined by a<br />

function that is not terribly different<br />

from V(λ ), but at angles from 25 deg<br />

to 70 deg off-axis, the spectral sensitivity<br />

is completely different.<br />

Figure 2 10 shows the large<br />

increases in short-wavelength<br />

(“blue”) sensitivity for off-axis<br />

objects. These increases happen at<br />

both high luminances (about 300 cd<br />

per sq m) and relatively low luminances<br />

(about five cd per sq m).<br />

Interestingly, the resulting spectral<br />

sensitivity is not all that dissimilar in<br />

shape from the spectral power distribution<br />

of a white light emitting diode<br />

(LED). When LEDs reach the light<br />

output required for interior lighting,<br />

perhaps LED “wall washers” can be<br />

effective tools for dramatically<br />

increasing the brightness of a space,<br />

filling our field of view with shortwavelength-rich,<br />

white light?<br />

A Glaring Case of<br />

Foresight?<br />

In previous “<strong>Research</strong> Matters”<br />

columns 11,12 we’ve read about how<br />

recently introduced high intensity discharge<br />

(HID) headlamps have been<br />

singled out, justly or unjustly, to<br />

receive the wrath of the American<br />

driving public. (European and<br />

. . . . . . . . . . . . . . . . . . . . . June . . . 2004 . . . LD+A . . . 18 . . www.iesna.org<br />

. . . . . . . . . . . . . . . . . . . . . . . . . . . .

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