It seems
like ‘black’ was an important topic of much of my early technical career. It
all began with a story told us by Dr. Seibert Quimby Duntley during my second
job out of college as a research engineer at the Scripps Institute of Oceanography, Visibility Lab, in San
Diego. Doc Duntley, the director of the lab, had been a research scientist at
MIT during WWII doing military camouflage studies. This work continued after
the war in California at what came to be known as “The Vis Lab.”
Duntley
described the development of the “Black Widow” paint used on night fighter
aircraft during the forties. Before the days of radar antiaircraft defense by
the Germans consisted of sonic detection with big horns and search lights to
spot the overhead aircraft. When pinned by the lights the planes, as Duntley
described them, appeared as easily seen bright grey silhouettes – even though
painted black. It turned out that the best black paints diffusely reflect at least
5 or 6 percent of the light that illuminates them. That’s enough to make them
easily seen and identified. Take the moon for example. We are used to seeing it
as a brilliant white object in the night sky. It’s not at all white. The Moon’s
average albedo (reflectance) is only 12% and the mare, flat areas, are probably
closer to 5 or 6% - like black paint.
To achieve a
reflectance of less than one percent a priority wartime project was undertaken.
A pharmaceutical firm came up with the solution to the problem – a paint that
consisted of tiny exploded carbon particles similar to popcorn suspended in a
glossy transparent durable binder. This top secret material was sent to England
in a container locked to a courier’s wrist for trials as a coating on the North
American P-61 night fighter, the Black Widow. It was highly successful. Even though
the glossy binder gave a substantial specular reflectance there was practically
no diffuse reflectance. As seen from the ground. Only a few sparkles might
appear and identification as an aircraft was exceedingly difficult.
Cmdr. Dayton
R. E. Brown, a mentor of mine and the Navy’s camouflage expert during the war,
tells the story of designing the paint for aircraft in the pacific. The Navy
had already rejected the idea of black – to much like a coffin – and had opted
for a deep blue. Admiral John Sidney McCain, ComNavAirPac, was paying a quick visit
to an island base in the Pacific during a period that coincided with Brown’s
presence at the base. Brown wanted to sell his idea for painting Navy planes more effectively
and tried to get the Admiral to give him some time. The Admiral was in a hurry
so Dayton volunteered to paint a plane at the side of the runway with a fire
hose while the Admiral’s plane was waiting to depart. McCain agreed and Dayton
Brown succeeded in selling his paint scheme to the Navy. It wasn’t black but it
was a good camouflage story.
Eliminating
stray light inside of optical instruments is always a prime concern in the
design process. Various techniques have been used in cameras, telescopes and
the like. Usually it’s just black paint which in most cases serves well. One
technique for absorbing light that is little used but is very effective is a stack of razor blades
seen edge on. If they are brand new and have never been handled the edges are
very sharp and the incident light vanishes down the interstitial cavities
between the individual blades. It's an interesting technique but hardly suitable for coating the entire inside of an instrument. One needs a hundred or more to make a small
black trap. Over the years we came to
use a 3M product called Velvet Black. It may no longer be available but it
had a diffuse reflectance of about 2 or 3 percent. It produced a very matte surface
and was fairly delicate so it would not weather well if used on the exterior
surfaces.
Our major efforts at instrument design were directed to the measurement of "meteorological range." Roughly, this is defined as the maximum distance at which one could detect a small dark object seen against the horizon sky. There are exact mathematical formulas for this distance and any reader who wishes to pursue it can look up the article referenced at the end of this blog.
In particular it found a good home inside the Meteorological Range Meter we installed on the aircraft pictured below which required a phototube to measure the scattering of light by particles and air molecules of a one meter column of air at an altitude of 35,000 feet. The photo below shows the MR Meter installed on the upper fuselage of the B-29 that the Air Force assigned to the Vis Lab for research purposes.
Our major efforts at instrument design were directed to the measurement of "meteorological range." Roughly, this is defined as the maximum distance at which one could detect a small dark object seen against the horizon sky. There are exact mathematical formulas for this distance and any reader who wishes to pursue it can look up the article referenced at the end of this blog.
In particular it found a good home inside the Meteorological Range Meter we installed on the aircraft pictured below which required a phototube to measure the scattering of light by particles and air molecules of a one meter column of air at an altitude of 35,000 feet. The photo below shows the MR Meter installed on the upper fuselage of the B-29 that the Air Force assigned to the Vis Lab for research purposes.
The most
interesting and “colorful” use of black surfaces, however, was the employment of a very
large amount of heavy black velvet cloth in our research station at Point
Barrow, Alaska. The station consisted of a well-insulated cubicle facility
containing all the electronic and mechanical machinery along with a stool, a
desk, and a coffee pot for the attending scientist. This facility was located
on a low platform well out on the tundra away from the base and village itself.
The MR Meter machinery, optics, and recording devices were safely enclosed in
the cubical. Out on the distant tundra were two black cavities – the more
distant a ten foot cube –and the
nearer one a three foot cube. They were arranged so that they both appeared the
same size to the meter’s optics. During recording the telescope was
electrically driven to view one after the other of these cavities and then the
horizon just above them. If the reader is interested in the details of these experiments and the theory behind the
measurements see the reference below.
The scale of
the distant black cavity is evident in this shot of the construction process.
The large
cavity, complete, and braced for bad weather.
This view below is
similar to what the MR Meter saw except for alignment and actual distances.
Many Inuit
helped with this project, all under the direction of Chester, the village
chief. When all was complete Chester instituted the penultimate use of our
wonderful black fabric by asking if he could have some of the scraps to
decorate his best parka. We, of course, gave him all he wanted. One of my
prized possessions is a photo of him leading his people in some of their
ceremonial dancing at the village hall.
John M. Hood Jr., "A Two
Cavity Long-Base Mode Meteorological Range Meter”, Applied
Optics, Vol. 3, P. 603-8, May 1964.