Roy
was Physicist who worked in the Applied Physics division of the Canadian
government's
National Research Council (NRC). (See
a list of the titles and positions that he held.) He began his career
there as on May 18, 1950, and retired in 1979.
When Roy
first began at
NRC in 1950 he joined its
Photometry and Colorimetry section and worked in its laboratories at 100 Sussex Dr.,
Ottawa. (See
image at right.)
Between early 1953 and
late
1955, he took a leave
of absence from NRC to obtain his doctorate
in physics in the Department of
Technical Optics (Colour) at the University of London's Imperial College
in Britain.
(See image below.)
While there, Roy continued to receive his NRC salary (although it was
reduced by 50%).
Roy's Ph.D. thesis, completed in 1955, was called "The colour rendering properties of illuminants,
and their assessment by colour tolerance determinations." At Roy's
memorial service, one of his NRC colleagues,
Dr. Alan Robertson,
spoke about the novel approach to the physics of "colour rendering" which
Roy's thesis promoted. Roy's early research in this technical field
is still being remembered in scientific journals. For instance, his work
was discussed in the journal
Lighting Research & Technology
in a paper called
"Memory and preferred colours and the colour rendition of white light
sources."
Roy's
thesis at Imperial College
was completed under the guidance of
Dr.
W.D.Wright, left, who was a world-renowned physicist in the field of colorimetry.
His work forms the basis of the
international standard for measuring colour.
While living in London, Roy
and Sylvia befriended Professor Wright's other Ph.D. students.
See photo, right, with some of these students, including Nasser (Egypt),
Sanders (Canada), Moreland (UK), De (Pakistan), Coug (Spain). In the
front row are Mrs. Moreland, Sylvia (with Heather) and Mrs De.
(Interestingly, Nasser was closely related to Gamal Abdel Nasser who led
the overthrow the Egypt's monarchy in 1952 and was that country's
president from 1956 to 1970.)
During
his NRC career, Roy produced
technical reports and published over two dozen papers in
leading scientific journals.
(See below.) He
led work in NRC's
photometry and radiometry lab and was responsible for maintaining and
developing Canadian standards for light and radiation. His work
applied physics to practical things from fluorescent lights, car signals
and the flashing lights on emergency vehicles, to colour TV monitors and
standardising the exact shade of red for Canada's flag.
(See some 1960s NRC
reports mentioning his work.)
Through his work, Roy also
deeply involved with the
International Bureau of Weights and
Measures (BIPM) and
International Commission on
Illumination (CIE). In
1962 he began chairing the BIPM's Working Group on the Primary
Standard of Light, a position he held until
1971. In 1963, Roy was also awarded the distinction of being made a Fellow of the Optical Society of
America. That was also the year that he began his four-year term as the president
of the CIE's Canadian National Committee.
Roy remained on this committee until his retirement in 1979 and was its
vice president between 1972 and 1975.
Through
the
CIE,
Roy
met and worked with
scientists from around the world,
including physicists from both western
and
eastern
Europe.
His work at the international
level included chairing the CIE's Subcommittee on Spectroradiometry
between 1967 and 1971. And,
as
a leader in the
field, Roy was appointed to chair the
the CIE's Technical Committee on Photometry
and Radiometry from 1971 until his retirement in 1979. In
that role, he coordinated
the work of international scientists in this field.
During
the 1970s, Roy was in charge of photometric standards and calibrations at
NRC. His work formed an important basis for establishing the
relationship between the world’s fundamental units of light (the candela)
and power (the watt). Read a short summary of
some of this work, which Roy wrote in his late 80s.
Throughout
the 1960s and 1970s, Roy's work for NRC took him
to high-level scientific conferences in many
countries.
These trips were sometimes combined with holidays with his wife Sylvia and
their younger children. Through
his connections with scientists in Britain, France,
Hungary, Czechoslovakia, Poland, the USSR, Japan, India and
South Africa, Roy
and Sylvia developed not only working relationships but
some
long-lasting
friendships. These international work-related friendships
included leading scientists from East and West.
For instance, American friends, like Luke Thorington (the lead engineer at
America's largest light manufacturer, Duro-Test Corp.) visited the Sanders
cottage in Quebec in the early 1970s. On the other side of the Cold
War divide, Roy and Sylvia were treated to the hospitality of Soviet
physicist Dr. Vera E. Kartachevskaia, who headed
the Photometry Lab at the Mendeleev Institute of Métrology. During
a work trip there in the late 1960s she had taken Roy and Sylvia on a tour
of Leningrad.
About 20 years later,
they visited her there again. (Learn
more in the subsection called "1985 April 25 - May 18.
'Adventure
Peace Tour to
the Soviet Union,'"
in the "Travels"
section.) You can also read more about these friendships in "Mixing
Business and Pleasure, Both East and West" and in the "Travel: For
Work and Pleasure" section on his "Biography"
page. Other details about Roy's many work-related trips can also be found
in the "Travels" section.
Roy's interest in light was diverse. He was for instance eager that
the world move away from fossil fuels and nuclear power to the use of the
sun's power. Roy was ahead of his time in seeing solar radiation as
a major potential source of energy which is safe, reliable and
sustainable. He became a member of the Solar Energy Society of Canada as
early as 1975 and installed an old, now almost antique, solar panel at the
Sanders cottage. He was also involved in researching many other impacts of
light and helped establishe the CIE's Study Group on
the Non-Sensory Effects of Optical
Radiation.
This involved studying effects as
diverse
as the ability of solar radiation to kill moulds and bacteria, as well as
the role of sunlight in causing cancer.
As part of this work, Roy and fellow NRC scientist
David Makow patented an "Ultraviolet Radiation
Dosimeter" in
1976. This invention was "a method and apparatus using liquid
crystals for indicating and measuring the exposure of objects to radiation
especially ultraviolet light radiation." (See NRC photo of Makow,
left, in 1958.)
Although Roy
retired in 1979 from his position as
a Senior
Research Officer at NRC, he did have occasion to
keep in touch with some of his closest colleagues.
For example, in 1994 he attended a retirement party for
Clarence Dodd who
had started work for NRC in 1956 as a technician in the labs run by Roy
and two other physicists at NRC.
In
2013, at age 89,
Roy was still thinking about physics. At that time
he devised a cosmological hypothesis to debunk "Big Bang" theory.
Roy challenged the prevailing scientific narrative
by arguing that the belief in a supposed "Big Bang" is caused by
false assumptions based on a Doppler-like optical illusion. This illusion, he argued, was caused by the journey of light through
dark matter and dark energy.
Read about his antiBig-Bang ideas
here.
Roy's
90th birthday party in 2014, was attended by several of his NRC colleagues
and replacements.
In the following year, when the government was celebrating
the 50th anniversary of Canada's maple-leaf flag, a ceremony was held at
NRC to remember its work in
stabilizing and defining the
flag's colour.
(See photo at left NRC retirees: Ron Burton, Roy and Clarence Dodd.)
At this ceremony, after being honoured for his part in that
scientific process, Roy was asked to say a few words. As
Alan Robertson
recalled at Roy's Memorial Service:
"After
receiving a plaque commemorating the work, Roy was photographed in front
of the flag and asked about his feelings. His main comment in response was
that he hoped that the flag would never be used to march behind into war."
"In conclusion," Alan said, "Roy was a modest man, an
excellent and innovative scientist, an unconventional thinker, and a good
friend."
Scientific papers
authored and co-authored by
C.L. ("Roy")
Sanders
(between 1951-1979)
His papers were published in a variety of scientific
journals
including
Applied Optics, Illuminating Engineering,
Metrologia,
Motion Imaging (Society
of Motion Pictures and TV Engineers),
National Bureau of Standards, Optical Society,
Planetary and Space
Science,
Revue d'Optique,
and Nature.
Some of Roy's pioneering research is still
being cited in scientific journals such as
Lighting Research & Technology (2015).
By
Middleton, W. E.K.;
Sanders, C. L.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 41, No.6; Publication date: June 6, 1951, Pages:
419–424
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-43-1-58_1
Abstract
The published values of the spectral diffuse reflectance of magnesium
oxide indicate that it should reflect more highly in the red than in the
blue. Using a modification of the method described by Preston, we have
measured the absolute value of this quantity between λ=0.24μ and λ=0.85μ.
A very carefully prepared surface of MgO on silver has a reflectance of
about 0.98 at λ=0.54μ, where there is a very flat maximum. The reflectance
of a fresh surface falls to less than 0.96 at 0.4μ, but exposure to strong
ultraviolet light bleaches it, the final result being a reflectance
increasing continuously from the near-infrared to about 0.4μ, where it
begins to fall sharply, reaching 0.96 at about 0.25μ. A sphere lined with
such a bleached surface raises the color-temperature of Planckian
radiation a little, and the observed color agrees well with that predicted
from the new results. It is believed that these results are reliable to
±0.002 from λ=0.4μ to λ=0.7μ, but different surfaces prepared with equal
care may differ in reflectance by at least 0.005.
The bleaching is presumed to be caused by the decomposition of small
amounts of magnesium nitride.
By
Sanders, C. L.;
Middleton, W. E.K.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 43, Issue: 254; Publication date: January 1, 1953,
Pages: 58
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-43-1-58_1
By
Middleton, W. E.K.;
Sanders, C. L.
Journal of the
Illuminating Engineering
Society, ISSN:
0019-2333, Volume: 48, Issue: May, Publication date: 1953, Pages:
254–256
First paragraph
In 1950 Miescher and Rometschl reported a very high and uniform
reflectance for plates of compressed barium sulphate, either alone or with
gelatine as a binder, and suggested its use as a standard of whiteness. In
this laboratory we attempted to reproduce their results, following their
very clear and detailed instructions with the greatest care, but in
several attempts we were unable to obtain nearly as good a white as they
claim to have produced, even without the gelatine. Our best result, by an
absolute method due to Taylor and confirmed by direct comparison in a
recording spectrophotometer, showed the com-pressed BaSO4 to be somewhat
yellower than magnesium oxide, its absolute reflectance being measured as
0.963 at λ
= μ,
and 0.989 at 0.7μ.
It is, of course, possible that our preparation was in some way at fault,
but at least it can safely be stated that the use of barium sulphate as a
standard white seems too difficult a procedure for ordinary use.
By
Sanders, C. L.;
Stevens, B. A.;
Middleton, W. E.K.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 44, Issue: 88; Publication date: January 1, 1954,
Pages: 88–89
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-44-1-88_1
Read the letter here.
Le Pouvoir emissif d'un corps noir
cylindrique
By
Sanders, C. L.;
Stevens, B. A.
Revue d'Optique,
Volume: 33, Issue: 179, Publication date: 1954
Abstract
A method given by Gouffé,
to calculate the emissive power of a cavity, cannot be used for a long
cylander such as the primary standard for luminous intensity. Yamauti
gives a correct result which is 1
– 2 X 10−8
for a cylinder 25 times longer than its radius.
Errata: The Primary Standard of Luminous Intensity at the National
Intensity at the National Research Council of Canada
C. L. Sanders, B. A.
Stevens, and W. E. K. Middleton
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 45, Issue: 12; Publication date: 1955, Pages:
pp. 1115_1-1115.
By
Sanders, C. L.;
Wyszecki, G. W.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 47, Issue: May 5, Publication date: 1957, Pages:
398–404
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-47-9-840
Abstract
In order to establish a correlate for lightness in terms of CIE-tristimulus
values, a simple experiment was performed using Munsell samples of value
5/. The observers compared each sample with a lightness scale and
estimated the value of the neutral which would appear equally light.
Analysis of the data by the least-squares method showed that a correlate
for lightness may be calculated with good approximation from the
tristimulus values by means of a second-degree equation, which, for
constant lightness, may be interpreted geometrically as an hyperboloid in
the CIE-color space. From this, it is concluded that the CIE method of
calculating luminous reflectance and using it as a lightness index does
not conform with the visual sensation.
It
has been established that although the coefficients of the second-degree
equation vary with field size and depend upon the individual observer,
characteristic features of the results are maintained in each case.
With respect to color vision theory the nature of the results seems to
indicate that the contribution of the violet receptor to the sensation of
lightness decreases with field size.
By
Wyszecki, G. W.;
Sanders, C. L.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 47, Publication date: September 9, 1957, Pages:
840–842
Abstract
A triangulation technique was used to check the definition of lightness as
applied in the previous paper. The results indicate that the procedure of
defining lightness in terms of the luminous reflectance of neutral samples
is satisfactory.
The investigation has been further extended to show a systematic
dependence of lightness index on background color. As might be expected,
the lightness index of colors similar to the background is decreased and
the lightness index of complementary colors is increased relative to the
lightness index obtained using a black background. This effect is due to
the change in chromatic adaptation of the eye.
By
Sanders, C. L.;
Wyszecki, G. W.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 48, Publication date: June 6, 1958, Pages: 389–392
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-48-6-389
Abstract
In
previous papers a correlate for lightness (L) was found in terms of
CIE-tristimulus values for colors of approximately constant luminous
reflectance (Y). L could be expressed by a second degree
equation with X, Y, Z as variables. In the present
study about 100 samples were selected to cover the gamut of existing
surface colors. The lightness-equivalent neutrals were estimated by three
observers for these colors under the same conditions as described in a
previous paper. The original type of equation could not be used to fit the
observational data because of the large differences in luminous
reflectance among the samples. However, the L/Y ratios could
be expressed by a second degree equation with chromaticity coordinates
x, y as variables. This type of equation appears to be valid
for all reflecting surface colors.
The assessment of color rendition under an illuminant using color tolerances for natural objects
By Sanders,
C.L.
Journal of the
Illuminating Engineering
Society, Volume: 54 (10)
Publication date: 1959.
Pages: 640-646.
Abstract
Consideration of the color
rendering properties of illuminants and of
the methods previously suggested for
assessing them indicates the desirability of a more subjective assessment.
This paper suggests a proceedure which uses the color tolerance ellipses
obtained by subjective judgements of the color rendition of several
natural objects.
Color Preferences for Natural Objects
By Sanders,
C.L.
Journal of the
Illuminating Engineering
Society,
Volume: 54,
Publication date: 1959.
Pages:
452-456
First
paragraph
Since the advent of artificial sources of light, and in particular the
fluorescent lamp, certain difficulties have been experienced in selecting
illuminants with energy distributions which make the color of objects
appear normal, that is, as they appear in daylight. Although the colors of
many objects may be rendered poorly by fluorescent lamps, common natural
objects are generally the subjects of complaint. it was thought that these
objects might have peculiar spectral reflectance curves or fluorescence
which could cause the difficulty. These properties were investigated for
tea, butter, the human complexion, potato chips and raw beefsteak, because
these objects are known to evoke complaints of bad color rendition.
The Primary Standard of Light
By Sanders,
C.L.
Read before the meeting of the
Illuminating Engineering
Society on June 12, 1959.
By
Jones, O. C.;
Sanders, C. L.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 51, Issue: 105; Publication date: January 1, 1961,
Pages: 105–108
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-51-1-105
Abstract
During work on the primary standard of light a photometer has been
developed which possesses desirable qualities. The detector used is a
Gillod-Boutry vacuum photocell with cesium-bismuth cathode surface having
a basic sensitivity of 25 μA/lu. The photocurrent is measured by a simple
circuit, using balanced electrometer tubes, similar to circuits which have
been described frequently over a long period of time in the literature
[e.g., C. H. Sharp and H. A. Smith, Trans. IES 23, 434 (1928), and O. C.
Jones, R. S. Maddever, and J. H. Sanders, J. Sci. Instr. 36, 24 (1959)]
except in one rather important respect which is described fully. The
photometer is compact and portable. Battery replacement is only necessary
every three months. Differences between successive readings and zeros
repeat to ±2/104 when measuring a steady incidence of 10−4
lu. Zero drift is small, necessitating readings only every 15 min. Circuit
stability is good, so that the simple balance adjustment need not be used
more than twice daily, provided that the triodes are suitably matched. Due
to undetermined causes day-to-day variations in sensitivity of 0.5%
sometimes occur.
By
Sanders, C. L.
Applied Optics, ISSN:
0003-6935, Volume: 1, Issue: 207; Publication date: May 3, 1962, Pages:
207–211
https://www.osapublishing.org/ao/abstract.cfm?uri=ao-1-3-207
Abstract
Illumination provided by an apparatus with nine pairs of apertures may be
used conveniently to test the linearity of photometers. The apertures
increase in area from one pair to the next by a factor of two. Thus the
range covered is 512 to 1. The apertures are selected individually or in
pairs by holes in a rotatable disk. The photometer reading on each
illumination level in a pair is determined, and the numerical sum of these
is compared with the reading on the two together. The ratio can be used to
correct the photometric scale of the receiver. The advantage of this
apparatus is the straightforward method of selecting illumination levels,
the wide range of illumination, and the easily arranged equipment.
By
Sanders, C. L.;
Jones, O. C.
Journal of the Optical Society of America, ISSN:
0030-3941, Volume: 52, Issue: 731; Publication date: July 7, 1962,
Pages: 731–746
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-52-7-731
Abstract
Although the accuracy required of a primary standard of light is of the
order of 0.1%, there is a spread of 1% in the size of the candelas derived
from the primary standards constructed at several national laboratories.
In this paper, the standard has been critically appraised: Some of the
suspected weaknesses have been studied experimentally, others are
discussed at length.
A
tantalum susceptor, used around the crucible containing the platinum to
absorb the induced currents and heat the platinum indirectly, increased
the photometric precision by an order of magnitude. The technique
unfortunately introduced excessive contamination of the platinum.
Since none of the modifications has created the desired improvement in
accuracy, other types of light standard may need to be reconsidered.
Correlate for
brightness in terms of CIE Color matching data
By
Sanders,
C.L.;
Wyszecki, G. W.
International Commission on Illumination
(CIE) Proceedings, 15 Session Vienna, Austria, 1963, Paper no. P.63.6
Summary
Twenty observers with normal color vision made heterochromatic
brightness matches on 96 test colors. A 10° bipartite photometric field
with a white surround was used. All test colors and the surround has a
luminance of 20 cd/m2. Each observer adjusted the luminance of the
achromatic comparison field until it matched the test color in
brightness. The luminance (B) of the equally bright achromatic field was
compared with the luminance (Y) of the colored test field. Values of
log10 (B/Y) generally showed a linear increase with saturation. The data
have been used to establish an average observer for heterochromatic
luminance matching.
Use
of a radioactivated light source for the absolute calibration of
two-colour night airglow photometer
Abstract
An experimental procedure is
described for the absolute calibration of a low intensity
radioactivated light source against a standard lamp. This light
source then could be used periodically to check and calibrate the
night airglow photometer which uses two filters to isolate a line
emission from the continuum in the night airglow spectrum.
The two filter problem is treated
analytically and an expression is derived for calculating the
spectral line intensity. Then it is shown that with certain
assumptions a simple formula can be evolved and used with the
experiment observations obtained with the two colour photometer to
obtain the emission rate of photons for a certain wavelength (i.e.
in a spectral line).
By
Sanders, C. L.;
Gaw, W.
Applied Optics, ISSN:
0003-6935, Volume: 6, Issue: October 10, Publication date: 1967,
Pages: 1639–1647
https://www.osapublishing.org/ao/abstract.cfm?uri=ao-6-10-1639
Abstract
A spectroradiometer is described which is designed to make measurements of
spectral radiance, irradiance, transmittance, and reflectance. In one
minute the Hilger D300 monochromator is set to the next wavelength to be
measured and a measurement is made of (a) the dark current of the
photomultiplier, (b) the photocurrent produced by the reference source,
(c) a voltage indicating the wavelength, and (d) the photocurrent produced
by a test source. An integrating digital voltmeter with a 10-sec gate is
used. The data are recorded on punched cards and analyzed by a digital
computer. Experimental results are given to illustrate the performance.
The applications described include calibration of standards of spectral
radiance and irradiance from a blackbody at the freezing point of platinum
and the developmet of a color temperature scale.
By
Sanders, C. L.
Metrologia, ISSN:
0026-1394, Volume: 3, Publication date: October 4, 1967, Pages:
119–129
Abstract
The thermal and spectral radiation characteristics of the cylindrical
enclosures used in the primary standard of light are studied in detail.
The temperatures at the walls and base of the cylindrical ceramic
sight-tubes are calculated on the basis of thermo-dynamic equilibrium. The
effect of the spectral emissivity of the ceramic on the apparent spectral
emissivity of the base is studied. Changes of about one percent in the
luminance of the base can occur with the sight-tubes that have commonly
been used. The effect of a temperature gradient in the surrounding ingot
is also considered. A practical design is suggested which should permit
realization of the primary standard of light with a luminance error,
caused by the sight-tube, of not more than 0.1%.
Sanders,
C. L. Gaw,
W
Wyszecki, G.
SMPTE Motion Imaging Journal,
Volume: 77,
Issue: 6,
Publication date: June 1968,
Page: 622
- 623
Abstract
The color calibrator permits an observer to compare the color
of the peak-white video level on a TV monitor with the standard white
provided by filtered light from a lamp in the calibrator. The standard
white chromaticity is equal to that from CIE Illuminant D6500. The
design, construction, calibration and application of the instrument
are discussed. Control of the chromaticity of the peak white from
various studios and stations using such an instrument should improve
the quality of color television.
By
Wright, H.;
Sanders, C. L.;
Gignac, D. S.
Applied Optics, ISSN:
0003-6935, Volume: 8, Issue: December 12, Publication date: 1969,
Pages: 2449–2455
https://www.osapublishing.org/ao/abstract.cfm?uri=ao-8-12-2449
Abstract
Two nonlinear curve-fitting computer programs have been developed for
designing subtractive glass filter combinations for use in photoelectric
photometers. One program adjusts the filter thicknesses to minimize the
sum of squares of errors at each wavelength and is thus useful in
designing a general purpose instrument. The second program minimizes the
errors in the photometric measurements of preselected light sources.
Filters for correcting various photoelectric detectors to the CIE luminous
efficiency function are specified. Several spectral response functions
have been utilized including S-4, S-10, S-11, S-20 types, and those of
typical silicon diodes, and selenium cells. Practical photometer designs
with predicted measurement errors of less than 0.1% are presented.
By
Sanders, C. L.
Applied Optics, ISSN:
0003-6935, Volume: 10, Issue: December 12, Publication date: 1971,
Pages: 2589–2591
https://www.osapublishing.org/ao/abstract.cfm?uri=ao-10-12-2589
Abstract
This paper discusses some of the tasks and problems of photometry. It
describes some of the international and national committees,
organizations, and laboratories that carry out these tasks and define and
resolve these problems.
Introduction
The purpose of this
editorial is to acquaint nonphotometrists with some of the problems of
photometrists and with some of the organizations that are involved in
defining and solving these problems. Of course some of these problems go
back a very long time as you will find from reading Middleton's' article
in this issue. Still I cannot help feeling that if vision had been
discovered at the same time as the hologram or the laser, vision would
have rightly attracted much more public attention and financial support
than either of the others. Therefore, the use of a little space in Applied
Optics on the mundane subject of photometry can be justified.
Light may be defined as
radiant energy which is capable of stimulating the eye, and photometry is
concerned with the measurement of such radiations in respect of their
ability to stimulate the eye. Following this definition given by Wright in
an excellent extensive treatment of the problem of photometry and knowing
the visual phenomena involved, the photometrist must decide which
radiometric quantities are important, measure them, and convert them to
visual quantities using appropriate factors. If the photometrist must also
decide the weighting factors and the acceptable limits of the results, he
will need to have knowledge of psychology, statistics, and physiology.
Many of the factors for converting radiometric quantities have been
accepted by international committees, and it is only necessary that the
photometrist know which to use in the case at hand.
The visual phenomena to
be considered will include brightness or lightness, glare, resolution or
acuity, the functions of photopic, scotopic, and mesopic vision, effect of
field size, position, color, movement, duration, shape, observer
differences, effect of adjacent and distant sources, additivity (or
nonadditivity), and adaptation. Some knowledge is required about the
required accuracy and precision of measurement. The extent of observer
differences give some indication of required accuracy.
Since radiant energy in
the visible region of the spectrum also affects processes other than the
human visual mechanism, these radiant quantities may be measured and
reported by some scientists for other than photometric use. (In some
cases, such as in photographic sensitometry, one finds photometric
quantities used because of the absence of more appropriate spectral
weighting functions.) These scientists, serving a wider purpose than the
production of visual quantities, may be called radiometrists or
spectroradiometrists.
Photometric measurements
are made at the International Bureau of Weights and Measures (BIPM) in
Svres, France, national standards laboratories, commercial standardizing
laboratories, industrial laboratories, and universities and by
illuminating engineers. The end result of all these measurements is to
ensure that in the living environment people are able to see adequately
and comfortably.
Read the full text of
this paper here
Accuracy
of Luminous Flux Measurements of Flourescent Lamps
By
Sanders, C. L.; J. Bak; W. Gaw
This article (found in Roy's papers) matches
a similarly titled paper by the same three authors which was made at the
International Conference on Photometry and Colorimetry. It was organised
by the Bulgarian Academy of Sciences and held in Varna, Bulgaria, on
25-30 June 1973. The paper presented at that conference was called:
Corrections of Luminous Flux of Fluorescent Lamps for Sphere
Selectivity and Imperfect Receivers. It was published in the
Proceedings of the Conference on Photometry and Colorimetry, Varna,
Bulgaria, 1973, pp. 81-86.
First Page
In 1967 we investigated a number of methods of measuring the luminous
flux from fluorescent lamps in an integrating sphere using incandescent
lamps as standards. The theory behind these methods was given by Bak.
The measurements were not reported at that time because it was not
possible to achieve the desired reproducibility or the desired agreement
between the methods. Since then further measurements indicate the source
of some of the problems and it now seems worthwhiIe to report the
results and our conclusions.
In
the earlier measurements a selenium (barrier layer cell) made by Weston
with a Viscor filter was used as the physical photometer.
Spectroradiometric measurements on the same lamps were made with the
same integrating sphere during separate lightings of the lamps. Four
types of 20-W fluorescent lamps were used, i.e., warm white, white, cool
white and daylite. The incandescent standard lamp was a flux standard at
a colour temperature of 2788 K for all methods. Its spectral
distribution was assumed to be Planckian. The methods used were
corrected for the spectral transmittance of the sphere and of the sphere
window as measured by the NRC spectroradiometer.
By
Sanders, C. L.
Journal of Research of the National Bureau of Standards (NBS). Section A.
Physics and Chemistry, ISSN:
0022-4332, Volume: 76A, Issue: 5, Publication date: June 7, 1972, Pages:
437–453
Abstract
The
methods described in the literature for accurately measuring photocell
linearity are surveyed and assessed. The effect of not measuring photocell
linearity under the conditions used in the final apparatus are considered.
Some of the conditions necessary for accurate assessment of the
nonlinearity under working conditions are specified. The use of the NRC
″Photocell Linearity Tester″ to measure and correct for the nonlinearity
of various receivers is described.
Read the full text of this paper here
The above paper was
presented
at a conference held at the NBS on March 22-24, 1972, in Gaithersburg,
Maryland, USA. The paper was therefore also published in the
proceedings of this conference in a book called Accuracy in spectrophotometry and luminescence measurements,
NBS Special Publication 378 NBS Special Publication 378.
His paper appears on pages
63-79.
Required and Achieved Accuracy in Photometry
and Radiometry
By
Sanders, C. L.
Proceedings of the Conference on
Photometry and Colorimetry, Varna, 1973. Pages: 1-12.
This paper was presented to the
International Conference on Photometry and Colorimetry organised by the
Bulgarian Academy of Sciences and held in Varna, Bulgaria, on 25-30 June
1973.
Abstract
Accuracy is distinguished from short and long term standard deviation
since a small standard deviation may be obtained in measurements
containing a large error. A block diagram is given indicating the kinds
of quantities to be measured in photometry and radiometry. The
quantities include total (and spectral) irradiance, radiance and radiant
flux, luminous fluxes luminous intensity and luminance. Lists are given
of the methods, auxiliary standards and relationships which are required
to compare one kind of quantity to another. Lists are given of the
information require about sources, methods, auxiliary standards and
relationships if an enlightened choice is to be made regarding the
optimum procedures and sources to be used. The accuracy achieved in
various intercomparisons is given. Reasons for limited achieved accuracy
are suggested. Suggestions are given for improving the accuracy,
particularly in measurements outside the national laboratories.
By
Budde, W.;
Sanders, C. L.
Applied Optics, ISSN:
0003-6935, Volume: 12, Publication date: September 9, 1973, Pages:
2099–2107
https://www.osapublishing.org/ao/abstract.cfm?uri=ao-12-9-2099
Abstract
The results of an interlaboratory comparison of measurements of relative
spectral sensitivity of vacuum photocells are summarized. The comparison
was part of the work of the CIE Photometry and Radiometry Committee
(TC-1.2). Nine laboratories measured two cells each. The results were
corrected for the drifting of relative spectral sensitivity of each cell.
The standard deviation of an individual measurement on a cell without
filter was less than 2% from 450 nm to 620 nm, increasing to 5% at 390 nm
and 690 nm. The standard deviation was larger for a V(lambda) corrected
cell, being less than 2% in the range 490-600 nm and increasing to 5% at
475 nm and 660 nm. The largest errors were probably caused by wavelength
and bandwidth errors.
By
Sanders, C. L.;
Jerome, C. W.
Applied Optics, ISSN:
0003-6935, Volume: 12, Publication date: September 9, 1973, Pages:
2088–2098
https://www.osapublishing.org/ao/abstract.cfm?uri=ao-12-9-2088
Abstract
A comparison of spectroradiometric measurements has been completed for the
wavelength region from 300 nm to 800 nm. The measurement procedures and
results obtained in eighteen laboratories are described. The results are
considerably better than those in earlier comparisons. Conclusions
regarding procedures to be avoided are given. Without special precautions
45° illumination on the diffuse receiver may cause serious errors. Normal
illumination on a plane or a spherical receiver is better. The power in
the spectral lines was inaccurately measured by Rossler’s method.
Suggestions sur le partage des responsabilités entre le CCPR, le BIPM et
la CIE
By
Sanders, C. L.
Introduction
Afin d'assurer l'accomplissement de toutes les tâches nécessaires et
afin de prévenir le chevauchement des programmes de travail du CCPR, du
BIPM et de la CIE, on doit préciser le partage des responsabilités. Les
suggestions ci-dessous, après discussion , pourraient éventuellement
mener un règle de conduite adoptée mutuellement par le CIE
(TC-1.2) et le CCPR et suivie dans l'avenir.
May 1975. Pages: 35-37. Presented to the
Comité Consultatif de Photométrie et
Radiométrie at the BIPM, 8th Session, September 3-5, 1975.
Read
it in the preceedings here
Possible
comparisons arising from survey of calibration facilities
By
Sanders, C. L.
May 1975. Pages:
35-37. Presented to the Comité
Consultatif de Photométrie et Radiométrie at the BIPM, 8th Session,
September 3-5, 1975.
Read
it in the preceedings here
Discussion
By Heller, J.W., Low,
R.M., Mertz, D.C., Sanders, C.L., Schaefer, A.R., Subotlch, Z.S.
Journal of the Illuminating Engineering Society,
Volume: 5, Issue 3,
Publication date: April 1976
By
Sanders, C. L.
Technical Report,
National Research Council, 1977. 125
pages. Information on 26 laboratories in 16 countries. Published on behalf
on the CIE's Technical Committee on Photometry and Radiometry.
Abstract
The directory was compiled by the
Optics Section, Division of Physics, National Research Council of Canada,
at the request of the International Commission on Illumination, Technical
Committee on Photometry and Radiometry (CIE TC-1.2). It is published as
NRC Physics Division Report No. PO-121.
The directory gives
information on the calibration services available from 26 laboratories in
16 countries. It is divided into three parts: the calibration of sources,
the calibration of receivers or measuring devices and the calibration of
reflecting or transmitting materials.
It is hoped that this
information will improve the dissemination of photometric and radiometric
calibrations throughout the world.
A "Technical Note" describing the directory was published in the journal
Metrologia,
Volume: 13, Issue: 55, Publication date: 1977.
By
Makow, D. M.;
Sanders, C. L.
Nature, ISSN:
0028-0836, Volume: 276, Issue: November 2, 5683, Publication date:
1978, Pages: 48–50
Abstract
Liquid crystals are organic
compounds in a state of matter intermediate between the isotropic liquid
and crystaline solid. They are fluid but at the same time they exhibit
molecular order. Depending on the ordering one distinguishes the smectic,
the nematic and the cholesteric liquid crystals (CLC). In the latter, the
rod-like molecules are arranged in layers with their long axes parallel to
each other. In each successive layer the direction of the long axis is
rotated by an angle of 10-20 arc min; the molecules then form a helical
structure. The spacing between layers differing by an angle of 360° is
called the pitch, p. Due to the periodicity of molecular orientation,
reflections from all layers separated by p/2 interfere constructively, if
the reflected wavelengths equal the product of the pitch and the
refractive indices seen by the wave. This condition is met for a band of
wavelength that is relatively narrow and steep and appears as a highly
saturated colour. The width of the band equals the product of the pitch
and the difference of the two refractive indices of birefringence. Colours
produced by such constructive interference, sometimes described as irridescent colours, have also been observed in certain beetles, birds and
butterflies4. We report here results of experiments showing that colours
of superimposed CLC coatings add like coloured lights and produce a colour
gamut greater than that obtained with inks, dyes and pigments.
By
Sanders, C. L.;
Gignac, D. S.
Technical Report, National Research Council, February 1979
Article, date unknown
Have something to add?
If you have any further information or
photos that you could share for this page of the Roy Sanders memorial website, please let me know.
Many thanks!
Richard Sanders <overcoat@rogers.com> |