Books by Mahon, Basil
- Mahon, Basil.
The Forgotten Genius of Oliver Heaviside.
Amherst, NY: Prometheus Books, 2017.
ISBN 978-1-63388-331-4.
-
At age eleven, in 1861, young Oliver Heaviside's family,
supported by his father's irregular income as an engraver of
woodblock illustrations for publications (an art beginning to be
threatened by the advent of photography) and a day school for
girls operated by his mother in the family's house, received a
small legacy which allowed them to move to a better part of
London and enroll Oliver in the prestigious Camden House School,
where he ranked among the top of his class, taking thirteen
subjects including Latin, English, mathematics, French, physics,
and chemistry. His independent nature and iconoclastic views
had already begun to manifest themselves: despite being an
excellent student he dismissed the teaching of Euclid's geometry
in mathematics and English rules of grammar as worthless. He
believed that both mathematics and language were best learned,
as he wrote decades later, “observationally,
descriptively, and experimentally.” These principles
would guide his career throughout his life.
At age fifteen he took the College of Perceptors examination,
the equivalent of today's A Levels. He was the
youngest of the 538 candidates to take the examination and
scored fifth overall and first in the natural sciences. This
would easily have qualified him for admission to university,
but family finances ruled that out. He decided to
study on his own at home for two years and then seek a job,
perhaps in the burgeoning telegraph industry. He would receive
no further formal education after the age of fifteen.
His mother's elder sister had married
Charles
Wheatstone, a successful and wealthy scientist, inventor,
and entrepreneur whose inventions include the concertina,
the stereoscope, and the Playfair encryption cipher, and who
made major contributions to the development of telegraphy.
Wheatstone took an interest in his bright nephew, and guided
his self-studies after leaving school, encouraging him
to master the Morse code and the German and Danish languages.
Oliver's favourite destination was the library, which he later
described as “a journey into strange lands to go a
book-tasting”. He read the original works of
Newton, Laplace, and other “stupendous names”
and discovered that with sufficient diligence he could
figure them out on his own.
At age eighteen, he took a job as an assistant to his older
brother Arthur, well-established as a telegraph engineer in
Newcastle. Shortly thereafter, probably on the recommendation
of Wheatstone, he was hired by the just-formed
Danish-Norwegian-English Telegraph Company as a telegraph
operator at a salary of £150 per year (around £12000
in today's money). The company was about to inaugurate a cable
under the North Sea between England and Denmark, and Oliver set
off to Jutland to take up his new post. Long distance telegraphy
via undersea cables was the technological frontier at the time—the
first successful transatlantic cable had only gone into
service two years earlier, and connecting the continents into
a world-wide web of rapid information transfer was the
booming high-technology industry of the age. While the job
of telegraph operator might seem a routine clerical task,
the élite who operated the undersea cables worked in
an environment akin to an electrical research laboratory,
trying to wring the best performance (words per minute) from
the finicky and unreliable technology.
Heaviside prospered in the new job, and after a merger
was promoted to chief operator at a salary of £175
per year and transferred back to England, at Newcastle.
At the time, undersea cables were unreliable. It was not
uncommon for the signal on a cable to fade and then die
completely, most often due to a short circuit caused by failure
of the
gutta-percha
insulation between the copper conductor and the iron sheath
surrounding it. When a cable failed, there was no alternative
but to send out a ship which would find the cable with a
grappling hook, haul it up to the surface, cut it, and test
whether the short was to the east or west of the ship's
position (the cable would work in the good direction but
fail in that containing the short. Then the cable would be
re-spliced, dropped back to the bottom, and the ship would
set off in the direction of the short to repeat the exercise
over and over until, by a process similar to
binary
search, the location of the fault was narrowed down and
that section of the cable replaced. This was time consuming
and potentially hazardous given the North Sea's propensity
for storms, and while the cable remained out of service it
made no money for the telegraph company.
Heaviside, who continued his self-study and frequented the
library when not at work, realised that knowing the resistance
and length of the functioning cable, which could be easily
measured, it would be possible to estimate the location of
the short simply by measuring the resistance of the cable
from each end after the short appeared. He was able to
cancel out the resistance of the fault, creating a quadratic
equation which could be solved for its location. The first
time he applied this technique his bosses were sceptical,
but when the ship was sent out to the location he
predicted, 114 miles from the English coast, they quickly
found the short circuit.
At the time, most workers in electricity had little use for
mathematics: their trade journal, The Electrician
(which would later publish much of Heaviside's work) wrote in
1861, “In electricity there is seldom any need of
mathematical or other abstractions; and although the use of
formulæ may in some instances be a convenience, they may
for all practical purpose be dispensed with.” Heaviside
demurred: while sharing disdain for abstraction for its own
sake, he valued mathematics as a powerful tool to understand
the behaviour of electricity and attack problems of
great practical importance, such as the ability to send
multiple messages at once on the same telegraphic line and
increase the transmission speed on long undersea cable links
(while a skilled telegraph operator could send traffic
at thirty words per minute on intercity land lines,
the transatlantic cable could run no faster than eight words
per minute). He plunged into calculus and differential
equations, adding them to his intellectual armamentarium.
He began his own investigations and experiments and began
to publish his results, first in English Mechanic,
and then, in 1873, the prestigious Philosophical
Magazine, where his work drew the attention of two of
the most eminent workers in electricity:
William Thomson (later Lord Kelvin) and
James Clerk Maxwell. Maxwell would go on
to cite Heaviside's paper on the Wheatstone Bridge in
the second edition of his Treatise on Electricity
and Magnetism, the foundation of the classical
theory of electromagnetism, considered by many the greatest
work of science since Newton's Principia,
and still in print today. Heady stuff, indeed, for a
twenty-two year old telegraph operator who had never set
foot inside an institution of higher education.
Heaviside regarded Maxwell's Treatise as the
path to understanding the mysteries of electricity he
encountered in his practical work and vowed to master it.
It would take him nine years and change his life. He
would become one of the first and foremost of the
“Maxwellians”, a small group including
Heaviside, George FitzGerald, Heinrich Hertz, and Oliver
Lodge, who fully grasped Maxwell's abstract and highly
mathematical theory (which, like many subsequent milestones
in theoretical physics, predicted the results of experiments
without providing a mechanism to explain them, such as
earlier concepts like an “electric fluid” or
William Thomson's intricate mechanical models of the
“luminiferous ether”) and built upon its
foundations to discover and explain phenomena unknown
to Maxwell (who would die in 1879 at the age of just 48).
While pursuing his theoretical explorations and publishing
papers, Heaviside tackled some of the main practical problems
in telegraphy. Foremost among these was “duplex
telegraphy”: sending messages in each direction
simultaneously on a single telegraph wire. He invented a
new technique and was even able to send two
messages at the same time in both directions as fast as
the operators could send them. This had the potential
to boost the revenue from a single installed line by
a factor of four. Oliver published his invention, and in
doing so made an enemy of William Preece, a senior engineer
at the Post Office telegraph department, who had invented
and previously published his own duplex system (which would
not work), that was not acknowledged in Heaviside's paper.
This would start a feud between Heaviside and Preece
which would last the rest of their lives and, on several
occasions, thwart Heaviside's ambition to have his work
accepted by mainstream researchers. When he applied to
join the Society of Telegraph Engineers, he was rejected
on the grounds that membership was not open to “clerks”.
He saw the hand of Preece and his cronies at the Post Office
behind this and eventually turned to William Thomson to
back his membership, which was finally granted.
By 1874, telegraphy had become a big business and the work
was increasingly routine. In 1870, the Post Office had
taken over all domestic telegraph service in Britain and,
as government is wont to do, largely stifled innovation and
experimentation. Even at privately-owned international
carriers like Oliver's employer, operators were no longer
concerned with the technical aspects of the work but rather
tending automated sending and receiving equipment. There
was little interest in the kind of work Oliver wanted to do:
exploring the new horizons opened up by Maxwell's work. He
decided it was time to move on. So, he quit his job, moved
back in with his parents in London, and opted for a life
as an independent, unaffiliated researcher, supporting himself
purely by payments for his publications.
With the duplex problem solved, the largest problem that
remained for telegraphy was the slow transmission speed on long
lines, especially submarine cables. The advent of the telephone
in the 1870s would increase the need to address this problem.
While telegraphic transmission on a long line slowed down the
speed at which a message could be sent, with the telephone voice
became increasingly distorted the longer the line, to the point
where, after around 100 miles, it was incomprehensible. Until
this was understood and a solution found, telephone service
would be restricted to local areas.
Many of the early workers in electricity thought of it as
something like a fluid, where current flowed through a wire like
water through a pipe. This approximation is more or less
correct when current flow is constant, as in a direct current
generator powering electric lights, but when current is varying
a much more complex set of phenomena become manifest which
require Maxwell's theory to fully describe. Pioneers of
telegraphy thought of their wires as sending direct
current which was simply switched off and on by the sender's
key, but of course the transmission as a whole was a varying
current, jumping back and forth between zero and full current at
each make or break of the key contacts. When these transitions
are modelled in Maxwell's theory, one finds that, depending upon
the physical properties of the transmission line (its
resistance, inductance, capacitance, and leakage between the
conductors) different frequencies propagate
along the line at different speeds. The sharp on/off
transitions in telegraphy can be thought of,
by Fourier
transform, as the sum of a wide band of frequencies,
with the result that, when each propagates at a different
speed, a short, sharp pulse sent by the key will, at
the other end of the long line, be “smeared out”
into an extended bump with a slow rise to a peak and then
decay back to zero. Above a certain speed, adjacent dots and dashes
will run into one another and the message will be undecipherable
at the receiving end. This is why operators on the transatlantic
cables had to send at the painfully slow speed of eight words
per minute.
In telephony, it's much worse because human speech is composed
of a broad band of frequencies, and the frequencies involved
(typically up to around 3400 cycles per second) are much
higher than the off/on speeds in telegraphy. The smearing
out or dispersion as frequencies are transmitted at
different speeds results in distortion which renders the voice
signal incomprehensible beyond a certain distance.
In the mid-1850s, during development of the first transatlantic
cable, William Thomson had developed a theory called the
“KR law” which predicted the transmission speed
along a cable based upon its resistance and capacitance.
Thomson was aware that other effects existed, but without
Maxwell's theory (which would not be published in its
final form until 1873), he lacked the mathematical tools
to analyse them. The KR theory, which produced results
that predicted the behaviour of the transatlantic cable
reasonably well, held out little hope for improvement:
decreasing the resistance and capacitance of the cable would
dramatically increase its cost per unit length.
Heaviside undertook to analyse what is now called the
transmission line
problem using the full Maxwell theory and, in 1878, published
the general theory of propagation of alternating current through
transmission lines, what are now called the
telegrapher's
equations. Because he took resistance, capacitance,
inductance, and leakage all into account and thus modelled both
the electric and magnetic field created around the wire by the
changing current, he showed that by balancing these four
properties it was possible to design a transmission
line which would transmit all frequencies at the same speed. In
other words, this balanced transmission line would behave for
alternating current (including the range of frequencies in a
voice signal) just like a simple wire did for direct current:
the signal would be attenuated (reduced in amplitude) with
distance but not distorted.
In an 1887 paper, he further showed that existing telegraph
and telephone lines could be made nearly distortionless by
adding
loading coils
to increase the inductance at points along the line (as long as
the distance between adjacent coils is small compared to the
wavelength of the highest frequency carried by the line). This
got him into another battle with William Preece, whose incorrect
theory attributed distortion to inductance and advocated
minimising self-inductance in long lines. Preece moved to block
publication of Heaviside's work, with the result that the paper
on distortionless telephony, published in The
Electrician, was largely ignored. It was not until 1897
that AT&T in the United States commissioned a study of
Heaviside's work, leading to patents eventually worth millions.
The credit, and financial reward, went to Professor Michael
Pupin of Columbia University, who became another of Heaviside's
life-long enemies.
You might wonder why what seems such a simple result (which can
be written in modern notation as the equation
L/R = C/G)
which had such immediate technological utlilty eluded
so many people for so long (recall that the problem with
slow transmission on the transatlantic cable had been observed
since the 1850s). The reason is the complexity of Maxwell's
theory and the formidably difficult notation in which it
was expressed. Oliver Heaviside spent nine years
fully internalising the theory and its implications, and
he was one of only a handful of people who had done so and,
perhaps, the only one grounded in practical applications such
as telegraphy and telephony. Concurrent with his work on
transmission line theory, he invented the mathematical
field of
vector
calculus and, in 1884, reformulated Maxwell's original
theory which, written in modern notation less
cumbersome than that employed by Maxwell, looks like:
into the four famous vector equations we today think of
as Maxwell's.
These are not only simpler, condensing twenty equations to
just four, but provide (once you learn the notation and
meanings of the variables) an intuitive sense for what is
going on. This made, for the first time, Maxwell's theory
accessible to working physicists and engineers interested
in getting the answer out rather than spending years
studying an arcane theory. (Vector calculus was
independently invented at the same time by the American
J. Willard Gibbs. Heaviside and Gibbs both acknowledged
the work of the other and there was no priority dispute.
The notation we use today is that of Gibbs, but the
mathematical content of the two formulations is
essentially identical.)
And, during the same decade of the 1880s, Heaviside
invented the
operational
calculus, a method of calculation which reduces the solution
of complicated problems involving differential equations to
simple algebra. Heaviside was able to solve so many problems
which others couldn't because he was using powerful computational
tools they had not yet adopted. The situation was similar to
that of Isaac Newton who was effortlessly solving problems
such as the
brachistochrone
using the calculus he'd invented while his contemporaries
struggled with more cumbersome methods. Some of the things
Heaviside did in the operational calculus, such as cancel
derivative signs in equations and take the square root of a
derivative sign made rigorous mathematicians shudder but, hey,
it worked and that was good enough for Heaviside and the many
engineers and applied mathematicians who adopted his methods.
(In the 1920s, pure mathematicians used the theory of
Laplace transforms
to reformulate the operational calculus in a rigorous manner,
but this was decades after Heaviside's work and long after
engineers were routinely using it in their calculations.)
Heaviside's intuitive grasp of electromagnetism and powerful
computational techniques placed him in the forefront of
exploration of the field. He calculated the electric field of
a moving charged particle and found it contracted in the
direction of motion, foreshadowing the Lorentz-FitzGerald contraction
which would figure in Einstein's
special relativity. In 1889
he computed the force on a point charge moving in an electromagnetic
field, which is now called the
Lorentz force
after Hendrik Lorentz who independently discovered it six years
later. He predicted that a charge moving faster than the speed
of light in a medium (for example, glass or water) would emit
a shock wave of electromagnetic radiation; in 1934 Pavel
Cherenkov experimentally discovered the phenomenon, now
called Cherenkov
radiation, for which he won the Nobel Prize in 1958. In
1902, Heaviside applied his theory of transmission lines to the
Earth as a whole and explained the propagation of
radio waves over intercontinental distances as due to a
transmission line formed by conductive seawater and a hypothetical
conductive layer in the upper atmosphere dubbed the
Heaviside
layer. In 1924 Edward V. Appleton confirmed the existence
of such a layer, the ionosphere, and won the Nobel prize in 1947
for the discovery.
Oliver Heaviside never won a Nobel Price, although he was
nominated for the physics prize in 1912. He shouldn't
have felt too bad, though, as other nominees passed over for the
prize that year included Hendrik Lorentz, Ernst Mach,
Max Planck, and Albert Einstein. (The winner that year was
Gustaf Dalén,
“for his invention of automatic regulators for use in
conjunction with gas accumulators for illuminating lighthouses
and buoys”—oh well.) He did receive Britain's
highest recognition for scientific achievement, being named a
Fellow of the Royal Society in 1891. In 1921 he was the first
recipient of the Faraday Medal from the Institution of
Electrical Engineers.
Having never held a job between 1874 and his death in 1925,
Heaviside lived on his irregular income from writing, the
generosity of his family, and, from 1896 onward a pension
of £120 per year (less than his starting salary as a
telegraph operator in 1868) from the Royal Society. He was
a proud man and refused several other offers of money which
he perceived as charity. He turned down an offer of compensation
for his invention of loading coils from AT&T when they
refused to acknowledge his sole responsibility for the invention.
He never married, and in his elder years became somewhat of a
recluse and, although he welcomed visits from other scientists,
hardly ever left his home in Torquay in Devon.
His impact on the physics of electromagnetism and the craft
of electrical engineering can be seen in the list of terms he
coined which are in everyday use: “admittance”,
“conductance”, “electret”,
“impedance”, “inductance”,
“permeability”, “permittance”,
“reluctance”, and “susceptance”. His
work has never been out of print, and sparkles with his
intuition, mathematical prowess, and wicked wit directed at
those he considered pompous or lost in needless abstraction and
rigor. He never sought the limelight and among those upon whose
work much of our present-day technology is founded, he is among
the least known. But as long as electronic technology persists,
it is a monument to the life and work of Oliver Heaviside.
November 2018
- Mahon, Basil.
The Man Who Changed Everything.
Chichester, UK: John Wiley & Sons, 2003.
ISBN 978-0-470-86171-4.
-
In the 19th century, science in general and physics in particular grew up,
assuming their modern form which is still recognisable today. At the start
of the century, the word “scientist” was not yet in use, and
the natural philosophers of the time were often amateurs. University
research in the sciences, particularly in Britain, was rare. Those
working in the sciences were often occupied by cataloguing natural
phenomena, and apart from Newton's monumental achievements, few people
focussed on discovering mathematical laws to explain the new physical
phenomena which were being discovered such as electricity and magnetism.
One person, James Clerk Maxwell, was largely responsible for creating the
way modern science is done and the way we think about theories of physics,
while simultaneously restoring Britain's standing in physics compared to
work on the Continent, and he created an institution which would continue
to do important work from the time of his early death until the present day.
While every physicist and electrical engineer knows of Maxwell and his
work, he is largely unknown to the general public, and even those who are
aware of his seminal work in electromagnetism may be unaware of the extent
his footprints are found all over the edifice of 19th century physics.
Maxwell was born in 1831 to a Scottish lawyer, John Clerk, and his wife Frances Cay.
Clerk subsequently inherited a country estate, and added “Maxwell”
to his name in honour of the noble relatives from whom he inherited it. His
son's first name, then was “James” and his surname “Clerk Maxwell”:
this is why his full name is always used instead of “James Maxwell”.
From childhood, James was curious about everything he encountered, and instead
of asking “Why?” over and over like many children, he drove his
parents to distraction with “What's the go o' that?”. His father
did not consider science a suitable occupation for his son and tried to direct
him toward the law, but James's curiosity did not extend to legal tomes and
he concentrated on topics that interested him. He published his first
scientific paper, on curves with more than two foci, at the age of 14.
He pursued his scientific education first at the University of Edinburgh
and later at Cambridge, where he graduated in 1854 with a degree in mathematics.
He came in second in the prestigious Tripos examination, earning the title of
Second Wrangler.
Maxwell was now free to begin his independent research, and he turned
to the problem of human colour vision. It had been established that
colour vision worked by detecting the mixture of three primary colours,
but Maxwell was the first to discover that these primaries were red,
green, and blue, and that by mixing them in the correct proportion,
white would be produced. This was a matter to which Maxwell would
return repeatedly during his life.
In 1856 he accepted an appointment as a full professor and department head
at Marischal College, in Aberdeen Scotland. In 1857, the topic for the
prestigious Adams Prize was the nature of the rings of Saturn. Maxwell's
submission was a tour de force which
proved that the rings could not be either solid nor a liquid, and hence
had to be made of an enormous number of individually orbiting bodies.
Maxwell was awarded the prize, the significance of which was magnified
by the fact that his was the only submission: all of the others who
aspired to solve the problem had abandoned it as too difficult.
Maxwell's next post was at King's College London, where he investigated
the properties of gases and strengthened the evidence for the molecular
theory of gases. It was here that he first undertook to explain the
relationship between electricity and magnetism which had been discovered
by Michael Faraday. Working in the old style of physics, he constructed
an intricate mechanical thought experiment model which might explain the
lines of force that Faraday had introduced but which many scientists
thought were mystical mumbo-jumbo. Maxwell believed the alternative
of action at a distance without any intermediate mechanism was
wrong, and was able, with his model, to explain the phenomenon of
rotation of the plane of polarisation of light by a magnetic field,
which had been discovered by Faraday. While at King's College, to
demonstrate his theory of colour vision, he took and displayed the
first colour photograph.
Maxwell's greatest scientific achievement was done while living the life
of a country gentleman at his estate, Glenair. In his textbook,
A Treatise on Electricity and Magnetism, he presented
his
famous equations
which showed that electricity and magnetism were
two aspects of the same phenomenon. This was the first of the great unifications
of physical laws which have continued to the present day. But that isn't
all they showed. The speed of light appeared as a conversion factor between
the units of electricity and magnetism, and the equations allowed solutions
of waves oscillating between an electric and magnetic field which could
propagate through empty space at the speed of light. It was compelling
to deduce that light was just such an electromagnetic wave, and that
waves of other frequencies outside the visual range must exist. Thus
was laid the foundation of wireless communication, X-rays, and gamma rays.
The speed of light is a constant in Maxwell's equations, not depending upon
the motion of the observer. This appears to conflict with Newton's laws
of mechanics, and it was not until Einstein's 1905 paper on
special relativity
that the mystery would be resolved. In essence, faced with a dispute between
Newton and Maxwell, Einstein decided to bet on Maxwell, and he chose wisely.
Finally, when you look at Maxwell's equations (in their modern form, using
the notation of vector calculus), they appear lopsided. While they unify
electricity and magnetism, the symmetry is imperfect in that while a moving
electric charge generates a magnetic field, there is no magnetic charge which,
when moved, generates an electric field. Such a charge would be a
magnetic monopole,
and despite extensive experimental searches, none has ever been found. The
existence of monopoles would make Maxwell's equations even more beautiful, but
sometimes nature doesn't care about that. By all evidence to date, Maxwell got it
right.
In 1871 Maxwell came out of retirement to accept a professorship at Cambridge
and found the
Cavendish Laboratory,
which would focus on experimental science and elevate Cambridge to world-class
status in the field. To date, 29 Nobel Prizes have been awarded for work done
at the Cavendish.
Maxwell's theoretical and experimental work on heat and gases revealed
discrepancies which were not explained until the development of quantum
theory in the 20th century. His suggestion of
Maxwell's demon
posed a deep puzzle in the foundations of thermodynamics which eventually,
a century later, showed the deep connections between information theory
and statistical mechanics. His practical work on automatic governors for
steam engines foreshadowed what we now call control theory. He played a key
part in the development of the units we use for electrical quantities.
By all accounts Maxwell was a modest, generous, and well-mannered man. He
wrote whimsical poetry, discussed a multitude of topics (although he had little
interest in politics), was an enthusiastic horseman and athlete (he would swim
in the sea off Scotland in the winter), and was happily married, with his wife
Katherine an active participant in his experiments. All his life, he supported
general education in science, founding a working men's college in Cambridge and
lecturing at such colleges throughout his career.
Maxwell lived only 48 years—he died in 1879 of the same cancer which had
killed his mother when he was only eight years old. When he fell ill, he was
engaged in a variety of research while presiding at the Cavendish Laboratory.
We shall never know what he might have done had he been granted another two
decades.
Apart from the significant achievements Maxwell made in a wide variety of
fields, he changed the way physicists look at, describe, and think about
natural phenomena. After using a mental model to explore electromagnetism,
he discarded it in favour of a mathematical description of its behaviour.
There is no theory behind Maxwell's equations: the equations are
the theory. To the extent they produce the correct results when
experimental conditions are plugged in, and predict new phenomena which
are subsequently confirmed by experiment, they are valuable. If they
err, they should be supplanted by something more precise. But they say
nothing about what is really going on—they only seek to
model what happens when you do experiments. Today, we are so accustomed
to working with theories of this kind: quantum mechanics, special and general
relativity, and the standard model of particle physics, that we don't think
much about it, but it was revolutionary in Maxwell's time. His mathematical
approach, like Newton's, eschewed explanation in favour of prediction: “We
have no idea how it works, but here's what will happen if you do this experiment.”
This is perhaps Maxwell's greatest legacy.
This is an excellent scientific biography of Maxwell which also gives the reader
a sense of the man. He was such a quintessentially normal person there aren't
a lot of amusing anecdotes to relate. He loved life, loved his work, cherished his
friends, and discovered the scientific foundations of the technologies which
allow you to read this. In the
Kindle edition, at least as read on an iPad, the text
appears in a curious, spidery, almost vintage, font in which periods are difficult to
distinguish from commas. Numbers sometimes have spurious spaces embedded within them,
and the index cites pages in the print edition which are useless since the Kindle
edition does not include real page numbers.
August 2014