Research matters - Illuminating Engineering Society
Research matters - Illuminating Engineering Society
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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