The following is taken in full from
Section IX. Optics, Heat, and Electronics;
Chapter 3. An Inexpensive X-ray Machine
The Scientific American Book of Projects for The Amateur Scientist
Library of Congress Card Catalog Number: 60-14286
© Copyright 1960 by C. L. Strong
An Inexpensive X-ray Machine
From an old radio tube, some copper wire, and other inexpensive
materials — total cost: roughly $20 — you can construct an X-ray
machine that will make good pictures through an inch of wood. SAFETY
MEASURES THAT YOU MUST OBSERVE. Notes on Röntgen's invention. Highlights
of X-ray theory.
Harry Simons of 118 Windsor Street, Kearny, N.J., is a lonely amateur
scientist. “For 23 years,” he writes, “I have been dabbling in the
X-ray portion of the electromagnetic spectrum without once coming across a
fellow amateur. Thousands of enthusiasts can be found in the region of
radio waves, of light and of gamma rays. But none of them come to play in
my back yard. If the prospect of exploring fresh electromagnetic territory
sounds interesting to any of these amateurs, I can promise good hunting in
the
-centimeter region — and for a total investment of less than $20.”
As a lure Simons offers the collection of radiographs reproduced in
Figures 225, 226, 227 and 228. He takes special pride in the one which
shows screws embedded in an inch-thick block of wood. This shot resulted
from his first experiment with X-rays and illustrates what can happen when
a fellow with a sharp eye follows a happy hunch.

225 Simon's radiograph of two screws imbedded in an inch-thick block of
wood

226 Radiograph of the plug from an electric flatiron

227 bones of fish revealed by homemade X-ray machine

228 Effectiveness of Simon's X-ray machine in penetrating the steel leaves
of a thickness ranging from .002 to .010 of an inch thick
During a rainy weekend back in 1933 Simons was fiddling with an Oudin
coil. This almost forgotten gadget, a close relative of the Tesla coil,
can step up low voltages 1,000 times or more. High voltage generated in
this way has an advantage for the amateur experimenter in that it is
relatively harmless. In the course of stepping up the voltage the Oudin
coil also increases the frequency of the current, so that it tends to flow
through the skin and away from vital organs such as the heart.
“My original Oudin coil,” Simons recalls, “was part of an
ultraviolet lamp with which I tested mineral specimens for fluorescence.
For no particular reason I decided to replace the evacuated quartz bulb,
which produced the ultraviolet rays, with an old radio tube of the 01
type. The glass envelope of these tubes is coated inside with a silvery
film of evaporated magnesium — the so-called “getter” which helps
clear the tube of stray gas during the evacuation process and absorbs any
that may be liberated by the glass walls or metal parts after the
seal-off. I simply held the 01 in my hand and touched its prongs to the
high-voltage terminal of the coil.” Instead of filling with a lavender
glow, like the quartz bulb, the inside of the tube remained dark but the
glass in contact with the magnesium lighted with a pale greenish
fluorescence that reminded me of the glow emitted by old style X-ray tubes
of the gas type. Was the radio tube producing X-rays?
“To obtain the answer to this question I put a narrow band of tinfoil
around the top of the tube and grounded it — as a substitute for the
electrode previously represented by my hand. I then fished a small block
of wood, which happened to have two screws in it, from the trash box and
placed it on a sheet of photographic film wrapped in black paper. The
combination was exposed to the energized tube for 15 seconds at a distance
of seven inches. When I had developed the film, I discovered a wonderful
radiograph of the screws — plus a lifetime hobby that should appeal to
anyone interested in physics.”
Why has Simons's hobby failed to catch on? One reason is that
commercial X-ray equipment is costly. Even tubes of relatively low power
are priced at $100 and up. Many other commercial X-ray parts are also
expensive and difficult to procure. The apparatus supplying high voltage
to conventional tubes, while no more complex than the power supply of a
husky radio transmitter, calls for special rectifying devices,
transformers and other components which are not regularly stocked by
dealers in electrical supplies.
Moreover, X-rays have earned a bad reputation as playthings. No
distinction can be drawn between the danger of exposure to a high-powered
X-ray machine and the fallout of an H-bomb. It is a danger that extends
not only to the experimenter but to his potential progeny. Human evolution
is the result of mutations caused by, among other agents, cosmic rays and
the radiations of radioactive elements in the earth's crust. Any radiation
added by man alters the rate of mutation, and is rightly a cause of deep
concern.
Simons has solved the problem of equipment cost. Protection against
exposure to the rays is not difficult to arrange. With these two
considerations out of the way, X-rays open a range of experiments equaled
by few other phenomena of physics. In addition to providing a source of
X-rays for radiographs, a generator of X-rays in combination with
accessories enables you to measure the charge of the electron, to study
the structure of crystals, to observe the wave-particle duality of matter
and radiation, and to probe other microcosmic corners.
Like visible light, X-rays are a form of radiant energy. Their ability
to penetrate substances opaque to visible light, however, is neither
unique nor particularly unusual. Many substances opaque to light are
transparent to other electromagnetic waves. For example, long electrical
waves, as well as the shorter ones of radio, pass freely through dry wood,
plaster and other substances that do not conduct electricity and are
opaque to light. If this were not so, all radio and television receivers
would need outdoor antennas.
On the other hand, a thick sheet of flint glass, which transmits radio
waves and light with no appreciable loss, stops X-rays. The ability of
X-rays to penetrate substances like flesh and bone is merely their most
publicized property. However, this property provides a striking case of
the immediate application of a scientific discovery. Within weeks of the
description of X-rays by Wilhelm Konrad Röntgen in 1895, surgeons
heralded them as a tool of the first importance.
They are characterized chiefly by extremely short wavelength — about
one ten-thousandth the length of visible light waves. Like light waves,
X-rays can be reflected, refracted, diffracted and polarized. The
techniques by which they are manipulated differ from those employed with
light, just as light techniques differ from those of radio. The longest
X-rays are indistinguishable from ultraviolet rays; the shortest are
identical with gamma rays. The distinction between the two is largely a
matter of definition. When the emission accompanies the disintegration of
a radioactive substance such as radium, it is called gamma radiation.
Identical waves generated by electronic means are called X-rays.
All radiant energy, including X-rays, has its origin in a disturbance
of electrical charge. Consider a point charge — an electron —
surrounded by a symmetrical electromagnetic field and moving through space
at constant velocity. What happens to the motion of the field if the
central charge is speeded up or slowed down? Experiments indicate that the
field reacts much like a mass of jelly. When the central charge is
accelerated, the disturbance is communicated radially through the field as
a wave motion — the outside parts of the field requiring an appreciable
time interval to catch up with the center. Work expended in accelerating
the central charge is carried away by the wave as radiant energy, at a
velocity which depends on the nature of the “jelly.”
In a vacuum the wave attains a maximum velocity of slightly more than
186,000 miles per second. The length of the wave depends upon the
abruptness with which the central charge is either disturbed or made to
change direction. Violent disturbances require the investment of more work
than gentle ones, and result in proportionately shorter and more energetic
waves. The waves radiated by electrical power lines, in which a stream of
electrons changes direction only 60 times a second, measure about 3,900
miles from crest to crest.
It is possible to subject electrons to much faster oscillations.
Military radars, for example, are constructed around magnetron
oscillators, small copper chambers that have been called electrical
counterparts of the familiar police whistle. The cavities are electrically
tuned to frequencies on the order of four billion cycles per second, and
streams of electrons forced into the cavities vibrate at this rate. The
resulting electromagnetic waves measure some three inches from crest to
crest.
As the cavities are made progressively smaller, the pitch goes up and
the wavelength goes down in obedience to the principle that the smaller
the whistle, the shriller its note. Where, then, can a “whistle” be
found that will accelerate charges rapidly or abruptly enough to create
electromagnetic waves a mere 25 thousandths of an inch long — the
wavelength of visible light? Nature provides such systems in the form of
molecules and atoms.
The normal, stable atom emits no radiation unless it is acted upon by
an external source of energy. If a fast-moving electron encounters an atom
in its normal state, the interloper may collide with one of the planetary
electrons in the outer orbital shell of the atom. The impact may cause the
electron in the atom to jump to an orbit still more remote from the center
of the atom. A sufficiently energetic electromagnetic wave impinging on
the atom can accomplish the same end, the requirement being that the
frequency of the wave coincide with the period of the outer electron's
orbital motion.
In either case the atom gains energy from the encounter and thus
becomes unstable. The normal state is soon restored when the electron hops
back into its “home” orbit. This represents the shifting of a center
of charge, and the excess energy is radiated into space by the
accompanying electromagnetic wave. The abruptness of the jump, and hence
the length of the wave, depends upon the attraction of the positive
nucleus for the planetary electron. When weakly bound electrons occupying
an orbit remote from the nucleus make such jumps, the length of the
radiated wave measures on the order of 25 thousandths of an inch — the
wavelength of light.
This same mechanism accounts for the origin of one kind of X-ray. When
a free electron, accelerated to a velocity of some 18,000 miles per
second, collides with an electron occupying an inner shell of the atom,
both the interloper and the innershell electron may carom into space, as
shown in the upper diagram of Figure 229. The vacancy thus created is
immediately filled by an electron from a shell more remote from the
nucleus. The attraction of the nucleus for this electron is much greater
and the jump accordingly more violent. The resulting wave measures on the
order of 250 millionths of an inch — an X-ray.
This initial jump does not end the display. A vacancy has been created
in the adjacent orbit by the electron that moved inward. Hence a series of
jumps follow as electrons from orbits still more remote from the nucleus
move in to fill the succession of gaps [see lower diagram, Fig. 229].
In the end the atom must capture a new electron to complete its outermost
orbit. In the meantime the atom has emitted a series of waves at
progressively lower frequencies, beginning with X-rays and extending
through ultraviolet radiation and visible light to heat.

229 Classical representation of X-ray origin in excited atom
The pattern of forces acting between. the nucleus and orbital electrons
responsible for the radiation is unique for each kind of atom. Measure the
radiation emitted at each frequency and you have an identifying tag for
the atom. This is the basis of spectroscopy. The fundamental particles of
the atom move in their orbits at rates fixed by these same forces. In
effect the atom is “tuned,” much as a group of radio receiving sets
might be pretuned for a group of broadcasting stations.
Atoms low on the periodic table, such as carbon, hydrogen, oxygen and
nitrogen — the stuff of living matter — are far out of tune with
X-rays of extremely high, frequency. When such waves impinge on
protoplasm, they ignore the barrier and sail right through.
X-rays of the highest frequency, those used for making most radiographs
and for the treatment of disease, are liberated when the bombarding
electron crashes into the massive nucleus of a target atom. The precise
nature of such encounters is not fully understood, but it appears that
when the bombarding electron collides with the nucleus head-on, and is
stopped dead in its track, the onrushing field may consume the entire mass
of the arrested particle and, in effect, transform the electron into an
X-ray of very high energy and frequency.
Other electrons strike the nucleus glancing blows, and are thus
decelerated. The deceleration is accompanied by the emission of an X-ray
of proportionate wavelength and energy. Hence when a stream of bombarding
electrons plays on a target composed of massive atoms, the emission of
radiant energy includes: (1) X-rays liberated by the acceleration of
planetary electrons, characteristic of the kind of atoms comprising the
target, and (2) X-rays that span a continuous band of frequencies from the
ultraviolet range to those of almost infinitesimal wavelength.
It was this continuous or “white” X-radiation, arising from the
bombardment of silicon nuclei in the glass of a Crookes tube, that led Röntgen
to his discovery. While studying the green fluorescence that appears at
one stage in the evacuation of the energized tube, Röntgen observed a
bright fluorescence among some nearby crystals of platinocyanide. The
crystals continued to glow even after he covered the energized tube with
black paper. He concluded that the tube was emitting a previously
unobserved form of radiation.
The Crookes tube consists of a pear-shaped glass bulb that is partially
evacuated and fitted with a cathode at the small end and an anode at the
large end. When a direct-current potential of about 20,000 volts is
connected across the electrodes, positive ions, accelerated by the
electric field, bombard the cathode and dislodge electrons from the metal.
Most of these are attracted to the anode, but some overshoot the mark. The
latter electrons continue to the end of the tube, where they collide with
the glass target.
Soon after Röntgen's discovery, the mechanism of white X-ray
production was explained by experimental investigation that paved the way
for improvements in the tube. By shaping the cathode in the form of a
paraboloid, for example, the electron stream could be focused sharply on
the metallic target composed of atoms more massive than silicon. X-rays
liberated at the spot were more energetic and cast sharper shadows than
those from the broad expanse of glass.
Electrostatic machines for the production of accelerating voltages grew
in size until some featured a spinning disk of plate glass seven feet
across, capable of generating 200,000 volts and currents up to five
milliamperes. All the early tubes contained some gas, the atoms of which
were needed as a source of electrons. The gas imposed an upper limit on
the accelerating voltage.
The limitation was removed in 1913 when W. D. Coolidge of the General
Electric Company succeeded in making ductile filaments of tungsten, which
he substituted for the cold cathode of the gas tubes. With this
independent source of electrons, tubes could be evacuated to the limit of
pumping techniques. Accelerating potentials of 300,000 volts and more
became practical. Such power levels created another problem; the heating
of the anode or target. This problem was first tackled by using tungsten,
with its high melting temperature, at both ends of the tube, then by
cooling the target with water, and finally by focusing the bombarding
electrons in a small spot near the edge of a motor-driven disk made of
tungsten.
Although Simons's tube is not in the class with large X-ray tubes of
the modern Coolidge type, it performs impressively well. A number of years
ago Simons shipped his first machine to George L. Clark at the University
of Illinois who, after testing it, reported to the journal Radiology:
“Simons's apparatus proves that X-rays can be produced for experimental
purposes by a unit which can be built for a very small fraction of the
cost of an installation of standard commercial equipment. The machine,
when in operation, will produce a beam of X-rays easily detected for a
distance of several feet in all directions. With ‘r’ meter
measurements we determined the intensity of the rays to be three fourths
of a Röntgen unit per minute at a distance of three feet.”
The explanation of this copious radiation, compared with that of a
Crookes tube, appears to lie in the magnesium coating.
Unfortunately the old 01 and tubes of similar construction are
currently in short supply because magnesium is no longer favored as a
material to remove gases, except in certain types of mercury-vapor
rectifying tubes which are unsuitable for X-ray production. For this
reason (plus the fact that he is an inveterate experimenter) Simons now
designs his own tubes and has them manufactured by a local glass blower.
They cost about $15 each. He rarely makes two alike, for the same reason
that amateur telescope makers seldom build two identical instruments. Each
design is a new and exciting experience.
One of Simons's latest designs is illustrated in Figure 230. This tube
is equipped with a disk-shaped cathode of molybdenum and a magnesium
target. It is evacuated to a barometric pressure of .0001 millimeters of
mercury. The over-all length of the tube is about seven inches. Its
emission is substantially greater than that of the 01 tube. Simons's
radiographs, with the exception of the one showing the screws in a block
of wood, were made with it. Such tubes can be made with a wide variety of
target materials and cathode shapes.

230 X-ray tube designed and constructed by Simons
Almost any source of high voltage can be used for energizing X-ray
tubes, including Van de Graaff electrostatic generators of the type
described in this section. Simons prefers to stick with Oudin coil. It is
easily constructed with hand tools. The job is simplified if you can lay
hands on a vibrator of the type used in the spark coil of a Model-T Ford.
As shown by Roger Hayward's diagram, Figure 231, and the general view in
Figure 232, the vibrator consists of a core of soft magnetic iron equipped
with an armature of soft magnetic iron and a set of breaker points.

231 Circuit diagram of Simon's X-ray apparatus

232 The source of high voltage for Simon's X-ray machine
The core of the vibrator is wound with 3,800 turns of No. 24 magnet
wire and connected in series with the breaker points as shown. When
bridged with the one-microfarad capacitor and connected to the power line,
the self-inductance of the coil is sufficient to charge the capacitor to a
potential of several hundred volts when the breaker points are adjusted to
open at the peak of the current cycle. The capacitor discharges through
the five-turn primary winding of the Oudin coil. The primary is wound with
five turns of ¼-inch copper tubing on a 2¼-inch plastic form three
inches in diameter.
The secondary winding consists of 5,000 turns of No. 32 enameled magnet
wire wound on a ½-inch rod of clear plastic. Each layer of wire must be
carefully insulated with a layer of varnished cambric that extends well
beyond the end of the coil. When the winding is completed, the secondary
coil must be thoroughly doped with high-grade insulating varnish. Both
ends of the coil are insulated with a tube of varnished cambric.
The assembly is then slipped inside the plastic form on which the
primary was wound. The outside end of the secondary is brought out through
a small hole in the form and soldered to one end of the primary winding.
The inner end of the secondary is threaded through a four-inch length of
½-inch plastic tubing and soldered to the inner face of a chromium-plated
chair glide, which serves as the high-voltage terminal. The ends of the
primary form are then closed with disks of ¼-inch plastic and secured in
place with screws at the edge. A ½-inch hole in the center of one disk
admits the tube support for the high-voltage terminal.
The chair glide is lifted temporarily and enough transformer oil or
potting compound poured through the ½-inch tube to fill the interior.
When wired according to the diagram [Fig. 231] and connected to the
power line, the coil will produce some 50,000 to 75,000 volts
continuously. The power consumption at 110 volts and 60 cycles is 35
watts.
As shown in Figure 233, all this apparatus must be housed in a
well-grounded metal container. The X-ray tube must be enclosed in an inner
compartment of lead sheet at least 1/8-inch thick. An opening in the end
of the double housings opposite the tube provides a window for the X-rays.

233 X-ray machine built by Harry Simons of Kearny, N.J.
WARNING! You must take these precautions
First, Oudin Coils are notorious emitters of radio waves that take the
form of ragged noise. They can black out radio and television reception
for miles around. Federal regulations prohibit the operation of such
devices unless they are thoroughly shielded. If any stray radiation can be
detected on a nearby radio or TV receiver after the apparatus is assembled
as described, it will be necessary to insert a low-pass filter at the
point where the power cord enters the housing. The design of such filters
is available in standard radio reference texts.
Whenever the machine is in operation, the experimenter must wear a
lead apron and stand well behind the orifice through which the rays are
emitted. Never turn your back to the machine so that you are between
it and the apron! It is also advisable to place a few exploratory samples
of film around the room while the apparatus is in operation. When
developed, these will show the pattern of radiation and protective lead
shielding can be installed accordingly. Finally, resist the temptation to
make X-ray examinations of the bones in your hands or other body parts. A
frozen fish makes a much safer test object.
The preceding was taken in full from
Section IX. Optics, Heat, and Electronics;
Chapter 3. An Inexpensive X-ray Machine
The Scientific American Book of Projects for The Amateur Scientist
Library of Congress Card Catalog Number: 60-14286
© Copyright 1960 by C. L. Strong
mailto:noah@noah.org
Shortcut to Noah's homepage
(http://www.noah.org)
November 27, 1995
April 1, 1997
|