-Caveat Lector-

http://www.solarenergy.com/

History of Solar Energy

Revisiting Solar Power's Past
By Charles Smith

Home Location: - Technology Review: July 95: Solar
Power

Inventors unlocked the secrets of turning the sun's
rays into mechanical power more than a century ago,
only to see their dream machines collapse from lack of
public support. Modern solar engineers must not be
doomed to relive their fate.

Charles Smith is an adjunct faculty member in the
Department of Technology at Appalachian State
University, and a doctoral candidate in the Department
of Science and Technology Studies at Virginia
Polytechnic Institute. His primary area of research is
the history of energy.

Many of us assume that the nation's first serious push
to develop renewable fuels was spawned while angry
Americans waited in gas lines during the "energy
crisis" of the 1970s. Held hostage by the OPEC oil
embargo, the country suddenly seemed receptive to
warnings from scientists, environmentalists, and even
a few politicians to end its over-reliance on finite
coal and oil reserves or face severe economic distress
and political upheaval.
But efforts to design and construct devices for
supplying renewable energy actually began some 100
years before that turbulent time--ironically, at the
very height of the Industrial Revolution, which was
largely founded on the promise of seemingly
inexhaustible supplies of fossil fuels. Contrary to
the prevailing opinion of the day, a number of
engineers questioned the practice of an industrial
economy based on nonrenewable energy and worried about
what the world's nations would do after exhausting the
fuel supply.

More important, many of these visionaries did not just
provide futuristic rhetoric but actively explored
almost all the renewable energy options familiar
today. In the end, most decided to focus on solar
power, reasoning that the potential rewards outweighed
the technical barriers. In less than 50 years, these
pioneers developed an impressive array of innovative
techniques for capturing solar radiation and using it
to produce the steam that powered the machines of that
era. In fact, just before World War I, they had
outlined all of the solar thermal conversion methods
now being considered. Unfortunately, despite their
technical successes and innovative designs, their work
was largely forgotten for the next 50 years in the
rush to develop fossil fuels for an energy-hungry
world.

Now, a century later, history is repeating itself.
After following the same path as the early
inventors--in some cases reinventing the same
techniques--contemporary solar engineers have arrived
at the same conclusion: solar power is not only
possible but eminently practical, not to mention more
environmentally friendly. Alas, once again, just as
the technology has proven itself from a practical
standpoint, public support for further development and
implementation is eroding, and solar power could yet
again be eclipsed by conventional energy technologies.

The First Solar Motor
The earliest known record of the direct conversion of
solar radiation into mechanical power belongs to
Auguste Mouchout, a mathematics instructor at the Lyce
de Tours. Mouchout began his solar work in 1860 after
expressing grave concerns about his country's
dependence on coal. "It would be prudent and wise not
to fall asleep regarding this quasi-security," he
wrote. "Eventually industry will no longer find in
Europe the resources to satisfy its prodigious
expansion. Coal will undoubtedly be used up. What will
industry do then?" By the following year he was
granted the first patent for a motor running on solar
power and continued to improve his design until about
1880. During this period the inventor laid the
foundation for our modern understanding of converting
solar radiation into mechanical steam power.

Mouchout's initial experiments involved a
glass-enclosed iron cauldron: incoming solar radiation
passed through the glass cover, and the trapped rays
transmitted heat to the water. While this simple
arrangement boiled water, it was of little practical
value because the quantities and pressures of steam it
produced were minimal. However, Mouchout soon
discovered that by adding a reflector to concentrate
additional radiation onto the cauldron, he could
generate more steam. In late 1865, he succeeded in
using his apparatus to operate a small, conventional
steam engine.

By the following summer, Mouchout displayed his solar
motor to Emperor Napoleon III in Paris. The monarch,
favorably impressed, offered financial assistance for
developing an industrial solar motor for France. With
the newly acquired funds, Mouchout enlarged his
invention's capacity, refined the reflector,
redesigning it as a truncated cone, like a dish with
slanted sides, to more accurately focus the sun's rays
on the boiler. Mouchout also constructed a tracking
mechanism that enabled the entire machine to follow
the sun's altitude and azimuth, providing
uninterrupted solar reception. After six years of
work, Mouchout exhibited his new machine in the
library courtyard of his Tours home in 1872, amazing
spectators. One reporter described the reflector as an
inverted "mammoth lamp shade...coated on the inside
with very thin silver leaf" and the boiler sitting in
the middle as an "enormous thimble" made of blackened
copper and "covered with a glass bell."

Anxious to put his invention to work, he connected the
apparatus to a steam engine that powered a water pump.
On what was deemed "an exceptionally hot day," the
solar motor produced one-half horsepower. Mouchout
reported the results and findings to the French
Academy of Science. The government, eager to exploit
the new invention to its fullest potential, decided
that the most suitable venue for the new machine would
be the tropical climes of the French protectorate of
Algeria, a region blessed with almost constant
sunshine and entirely dependent on coal, a
prohibitively expensive commodity in the African
region.

Mouchout was quickly deployed to Algeria with ample
funding to construct a large solar steam engine. He
first decided to enlarge his invention's capacity yet
again to 100 liters (70 for water and 30 for steam)
and employ a multi-tubed boiler instead of the single
cauldron. The boiler tubes had a better
surface-area-to-water ratio, yielding more pressure
and improved engine performance.

In 1878, Mouchout exhibited the redesigned invention
at the Paris Exposition. Perhaps to impress the
audience or, more likely, his government backers, he
coupled the steam engine to a refrigeration device.
The steam from the solar motor, after being routed
through a condenser, rapidly cooled the inside of a
separate insulated compartment. He explained the
result: "In spite of the seeming paradox of the
statement, [it was] possible to utilize the rays of
the sun to make ice." Mouchout was awarded a medal for
his accomplishments.

By 1881 the French Ministry of Public Works, intrigued
by Mouchout's machine, appointed two commissioners to
assess its cost efficiency. But after some 900
observations at Montpelier, a city in southern France,
and Constantine, Algeria, the government deemed the
device a technical success but a practical failure.
One reason was that France had recently improved its
system for transporting coal and developed a better
relationship with England, on which it was dependent
for that commodity. The price of coal had thus
dropped, rendering the need for alternatives less
attractive. Unable to procure further financial
assistance, Mouchout returned to his academic
pursuits.

The Tower of Power
During the height of Mouchout's experimentation,
William Adams, the deputy registrar for the English
Crown in Bombay, India, wrote an award-winning book
entitled Solar Heat: A Substitute for Fuel in Tropical
Countries. Adams noted that he was intrigued with
Mouchout's solar steam engine after reading an account
of the Tours demonstration, but that the invention was
impractical, since "it would be impossible to
construct [a dish-shaped reflector] of much greater
dimensions" to generate more than Mouchout's one-half
horsepower. The problem, he felt, was that the
polished metal reflector would tarnish too easily, and
would be too costly to build and too unwieldy to
efficiently track the sun.

Fortunately for the infant solar discipline, the
English registrar did not spend all his time finding
faults in the French inventor's efforts, but offered
some creative solutions. For example, Adams was
convinced that a reflector of flat silvered mirrors
arranged in a semicircle would be cheaper to construct
and easier to maintain. His plan was to build a large
rack of many small mirrors and adjust each one to
reflect sunlight in a specific direction. To track the
sun's movement, the entire rack could be rolled around
a semicircular track, projecting the concentrated
radiation onto a stationary boiler. The rack could be
attended by a laborer and would have to be moved only
"three or four times during the day," Adams noted, or
more frequently to improve performance.

Confident of his innovative arrangement, Adams began
construction in late 1878. By gradually adding
17-by-10-inch flat mirrors and measuring the rising
temperatures, he calculated that to generate the
1,200û F necessary to produce steam pressures high
enough to operate conventional engines, the reflector
would require 72 mirrors. To demonstrate the power of
the concentrated radiation, Adams placed a piece of
wood in the focus of the mirrored panes where, he
noted, "it ignited immediately." He then arranged the
collectors around a boiler, retaining Mouchout's
enclosed cauldron configuration, and connected it to a
2.5-horsepower steam engine that operated during
daylight hours "for a fortnight in the compound of
[his] bungalow."

Eager to display his invention, Adams notified
newspapers and invited his important
friends--including the Army's commander in chief, a
colonel from the Royal Engineers, the secretary of
public works, various justices, and principal mill
owners--to a demonstration. Adams wrote that all were
impressed, even the local engineers who, while
doubtful that solar power could compete directly with
coal and wood, thought it could be a practical
supplemental energy source.

Adams's experimentation ended soon after the
demonstration, though, perhaps because he had achieved
his goal of proving the feasibility of his basic
design, but more likely because, as some say, he
lacked sufficient entrepreneurial drive. Even so, his
legacy of producing a powerful and versatile way to
harness and convert solar heat survives. Engineers
today know this design as the Power Tower concept,
which is one of the best configurations for large
scale, centralized solar plants. In fact, most of the
modern tower-type solar plants follow Adams's basic
configuration: flat or slightly curved mirrors that
remain stationary or travel on a semicircular track
and either reflect light upward to a boiler in a
receiver tower or downward to a boiler at ground
level, thereby generating steam to drive an
accompanying heat engine.

Collection without Reflection
Even with Mouchout's abandonment and the apparent
disenchantment of England's sole participant, Europe
continued to advance the practical application of
solar heat, as the torch returned to France and
engineer Charles Tellier. Considered by many the
father of refrigeration, Tellier actually began his
work in refrigeration as a result of his solar
experimentation, which led to the design of the first
nonconcentrating, or non-reflecting, solar motor.

In 1885, Tellier installed a solar collector on his
roof similar to the flat-plate collectors placed atop
many homes today for heating domestic water. The
collector was composed of ten plates, each consisting
of two iron sheets riveted together to form a
watertight seal, and connected by tubes to form a
single unit. Instead of filling the plates with water
to produce steam, Tellier chose ammonia as a working
fluid because of its significantly lower boiling
point. After solar exposure, the containers emitted
enough pressurized ammonia gas to power a water pump
he had placed in his well at the rate of some 300
gallons per hour during daylight. Tellier considered
his solar water pump practical for anyone with a
south-facing roof. He also thought that simply adding
plates, thereby increasing the size of the system,
would make industrial applications possible.

By 1889 Tellier had increased the efficiency of the
collectors by enclosing the top with glass and
insulating the bottom. He published the results in The
Elevation of Water with the Solar Atmosphere, which
included details on his intentions to use the sun to
manufacture ice. Like his countryman Mouchout, Tellier
envisioned that the large expanses of the African
plains could become industrially and agriculturally
productive through the implementation of solar power.

In The Peaceful Conquest of West Africa, Tellier
argued that a consistent and readily available supply
of energy would be required to power the machinery of
industry before the French holdings in Africa could be
properly developed. He also pointed out that even
though the price of coal had fallen since Mouchout's
experiments, fuel continued to be a significant
expense in French operations in Africa. He therefore
concluded that the construction costs of his
low-temperature, non-concentrating solar motor were
low enough to justify its implementation. He also
noted that his machine was far less costly than
Mouchout's device, with its dish-shaped reflector and
complicated tracking mechanism.

Yet despite this potential, Tellier evidently decided
to pursue his refrigeration interests instead, and do
so without the aid of solar heat. Most likely the
profits from conventionally operated refrigerators
proved irresistible. Also, much of the demand for the
new cooling technology now stemmed from the desire to
transport beef to Europe from North and South America.
The rolling motion of the ships combined with space
limitations precluded the use of solar power
altogether. And as Tellier redirected his focus,
France saw the last major development of solar
mechanical power on her soil until well into the
twentieth century. Most experimentation in the
fledgling discipline crossed the Atlantic to that new
bastion of mechanical ingenuity, the United States.

The Parabolic Trough
Though Swedish by birth, John Ericsson was one of the
most influential and controversial U.S. engineers of
the nineteenth century. While he spent his most
productive years designing machines of war--his most
celebrated accomplishment was the Civil War battleship
the Monitor--he dedicated the last 20 years of his
life largely to more peaceful pursuits such as solar
power. This work was inspired by a fear shared by
virtually all of his fellow solar inventors that coal
supplies would someday end. In 1868 he wrote, "A
couple of thousand years dropped in the ocean of time
will completely exhaust the coal fields of Europe,
unless, in the meantime, the heat of the sun be
employed."

Thus by 1870 Ericsson had developed what he claimed to
be the first solar-powered steam engine, dismissing
Mouchout's machine as "a mere toy." In truth,
Ericsson's first designs greatly resembled Mouchout's
devices, employing a conical, dish-shaped reflector
that concentrated solar radiation onto a boiler and a
tracking mechanism that kept the reflector directed
toward the sun.

Though unjustified in claiming his design original,
Ericsson soon did invent a novel method for collecting
solar rays--the parabolic trough. Unlike a true
parabola, which focuses solar radiation onto a single,
relatively small area, or focal point, like a
satellite television dish, a parabolic trough is more
akin to an oil drum cut in half lengthwise that
focuses solar rays in a line across the open side of
the reflector. This type of reflector offered many
advantages over its circular (dish-shaped)
counterparts: it was comparatively simple, less
expensive to construct, and, unlike a circular
reflector, had only to track the sun in a single
direction (up and down, if lying horizontal, or east
to west if standing on end), thus eliminating the need
for complex tracking machinery. The downside was that
the device's temperatures and efficiencies were not as
high as with a dish-shaped reflector, since the
configuration spread radiation over a wider area--a
line rather than a point. Still, when Ericsson
constructed a single linear boiler (essentially a
pipe), placed it in the focus of the trough,
positioned the new arrangement toward the sun, and
connected it to a conventional steam engine, he
claimed the machine ran successfully, though he
declined to provide power ratings.

The new collection system became popular with later
experimenters and eventually became a standard for
modern plants. In fact, the largest solar systems in
the last decade have opted for Ericsson's parabolic
trough reflector because it strikes a good engineering
compromise between efficiency and ease of operation.

For the next decade, Ericsson continued to refine his
invention, trying lighter materials for the reflector
and simplifying its construction. By 1888, he was so
confident of his design's practical performance that
he planned to mass-produce and supply the apparatus to
the "owners of the sunburnt lands on the Pacific
coast" for agricultural irrigation.

Unfortunately for the struggling discipline, Ericsson
died the following year. And because he was a
suspicious and, some said, paranoid man who kept his
designs to himself until he filed patent applications,
the detailed plans for his improved sun motor died
with him. Nevertheless, the search for a practical
solar motor was not abandoned. In fact, the
experimentation and development of large-scale solar
technology was just beginning.

The First Commercial Venture
Boston resident Aubrey Eneas began his solar motor
experimentation in 1892, formed the first solar power
company (The Solar Motor Co.) in 1900, and continued
his work until 1905. One of his first efforts resulted
in a reflector much like Ericsson's early parabolic
trough. But Eneas found that it could not attain
sufficiently high temperatures, and, unable to unlock
his predecessor's secrets, decided to scrap the
concept altogether and return to Mouchout's
truncated-cone reflector. Unfortunately, while
Mouchout's approach resulted in higher temperatures,
Eneas was still dissatisfied with the machine's
performance. His solution was to make the bottom of
the reflector's truncated cone-shaped dish larger by
designing its sides to be more upright to focus
radiation onto a boiler that was 50 percent larger.

Finally satisfied with the results, he decided to
advertise his design by exhibiting it in sunny
Pasadena, Calif., at Edwin Cawston's ostrich farm, a
popular tourist attraction. The monstrous machine did
not fail to attract attention. Its reflector, which
spanned 33 feet in diameter, contained 1,788
individual mirrors. And its boiler, which was about 13
feet in length and a foot wide, held 100 gallons of
water. After exposure to the sun, Eneas's device
boiled the water and transferred steam through a
flexible pipe to an engine that pumped 1,400 gallons
of water per minute from a well onto the arid
California landscape.

Not everyone grasped the concept. In fact, one man
thought the solar machine had something to do with the
incubation of ostrich eggs. But Eneas's marketing
savvy eventually paid off. Despite the occasional
misconceptions, thousands who visited the farm left
convinced that the sun machine would soon be a fixture
in the sunny Southwest. Moreover, many regional
newspapers and popular-science journals sent reporters
to the farm to cover the spectacle. To Frank Millard,
a reporter for the brand new magazine World's Work,
the potential of solar motors placed in quantity
across the land inspired futuristic visions of a
region "where oranges may be growing, lemons
yellowing, and grapes purpling, under the glare of the
sun which, while it ripens the fruits it will also
water and nourish them." He also predicted that the
potential for this novel machine was not limited to
irrigation: "If the sun motor will pump water, it will
also grind grain and saw lumber and run electric
cars."

The future, like the machine itself, looked bright and
shiny. In 1903 Eneas, ready to market his solar motor,
moved his Boston-based company to Los Angeles, closer
to potential customers. By early the following year he
had sold his first complete system for $2,160 to Dr.
A. J. Chandler of Mesa, Ariz. Unfortunately, after
less than a week, the rigging supporting the heavy
boiler weakened during a windstorm and collapsed,
sending it tumbling into the reflector and damaging
the machine beyond repair.

But Eneas, accustomed to setbacks, decided to push
onward and constructed another solar pump near Tempe,
Ariz. Seven long months later, in the fall of 1904,
John May, a rancher in Wilcox, Ariz., bought another
machine for $2,500. Unfortunately, shortly afterward,
it was destroyed by a hailstorm. This second
weather-related incident all but proved that the
massive parabolic reflector was too susceptible to the
turbulent climactic conditions of the desert
southwest. And unable to survive on such measly sales,
the company soon folded.

Though the machine did not become a fixture as Eneas
had hoped, the inventor contributed a great deal of
scientific and technical data about solar heat
conversion and initiated more than his share of public
exposure. Despite his business failure, the lure of
limitless fuel was strong, and while Eneas and the
Solar Motor Company were suspending their operations,
another solar pioneer was just beginning his.

Moonlight Operation
Henry E. Willsie began his solar motor construction a
year before Eneas's company folded. In his opinion,
the lessons of Mouchout, Adams, Ericsson, and Eneas
proved the cost inefficiency of high-temperature,
concentrating machines. He was convinced that a
nonreflective, lower-temperature collection system
similar to Tellier's invention was the best method for
directly utilizing solar heat. The inventor also felt
that a solar motor would never be practical unless it
could operate around the clock. Thus thermal storage,
a practice that lent itself to low-temperature
operation, was the focus of his experimentation.

To store the sun's energy, Willsie built large
flat-plate collectors that heated hundreds of gallons
of water, which he kept warm all night in a huge
insulated basin. He then submerged a series of tubes,
or vaporizing pipes, inside the basin to serve as
boilers. When the acting medium--Willsie preferred
sulfur dioxide to Tellier's ammonia--passed through
the pipes, it transformed into a high-pressure vapor,
which passed to the engine, operated it, and exhausted
into a condensing tube, where it cooled, returned to a
liquid state, and was reused.

In 1904, confident that his design would produce
continuous power, he built two plants, a 6-horsepower
facility in St. Louis, Mo., and a 15-horsepower
operation in Needles, Calif. And after several power
trials, Willsie decided to test the storage capacity
of the larger system. After darkness had fallen, he
opened a valve that "allowed the solar-heated water to
flow over the exchanger pipes and thus start up the
engine." Willsie had created the first solar device
that could operate at night using the heat gathered
during the day. He also announced that the
15-horsepower machine was the most powerful
arrangement constructed up to that time. Beside
offering a way to provide continuous solar power
production, Willsie also furnished detailed cost
comparisons to justify his efforts: the solar plant
exacted a two-year payback period, he claimed, an
exceptional value even when compared with today's
standards for alternative energy technology.

Originally, like Ericsson and Eneas before him,
Willsie planned to market his device for desert
irrigation. But in his later patents Willsie wrote
that the invention was "designed for furnishing power
for electric light and power, refrigerating and ice
making, for milling and pumping at mines, and for
other purposes where large amounts of power are
required."

Willsie determined all that was left to do was to
offer his futurist invention for sale. Unfortunately,
no buyers emerged. Despite the favorable long-term
cost analysis, potential customers were suspicious of
the machine's durability, deterred by the high ratio
of machine size to power output, and fearful of the
initial investment cost of Willsie's ingenious solar
power plant. His company, like others before it,
disintegrated.

A Certain Technical Maturity
Despite solar power's dismal commercial failures, some
proponents continued to believe that if they could
only find the right combination of solar technologies,
the vision of a free and unlimited power source would
come true. Frank Shuman was one who shared that dream.
But unlike most dreamers, Shuman did not have his head
in the clouds. In fact, his hardheaded approach to
business and his persistent search for practical solar
power led him and his colleagues to construct the
largest and most cost-effective machine prior to the
space age.

Shuman's first effort in 1906 was similar to Willsie's
flat-plate collector design except that it employed
ether as a working fluid instead of sulfur dioxide.
The machine performed poorly, however, because even at
respectable pressures, the steam--or more accurately,
the vapor--exerted comparatively little force to drive
a motor because of its low specific gravity.

Shuman knew he needed more heat to produce steam, but
felt that using complicated reflectors and tracking
devices would be too costly and prone to mechanical
failure. He decided that rather than trying to
generate more heat, the answer was to better conserve
the heat already being absorbed.

In 1910, to improve the collector's insulation
properties, Shuman enclosed the absorption plates not
with a single sheet of glass but with dual panes
separated by a one-inch air space. He also replaced
the boiler pipes with a thin, flat metal container
similar to Tellier's original greenhouse design. The
apparatus could now consistently boil water rather
than ether. Unfortunately, however, the pressure was
still insufficient to drive industrial-size steam
engines, which were designed to operate under
pressures produced by hotter-burning coal or wood.

After determining that the cost of building a larger
absorber would be prohibitive, Shuman reluctantly
conceded that the additional heat would have to be
provided through some form of concentration. He thus
devised a low-cost reflector stringing together two
rows of ordinary mirrors to double the amount of
radiation intercepted. And in 1911, after forming the
Sun Power Co., he constructed the largest solar
conversion system ever built. In fact, the new plant,
located near his home in Talcony, Penn., intercepted
more than 10,000 square feet of solar radiation. The
new arrangement increased the amount of steam
produced, but still did not provide the pressure he
expected.

Not easily defeated, Shuman figured that if he
couldn't raise the pressure of the steam to run a
conventional steam engine, he would have to redesign
the engine to operate at lower pressures. So he teamed
up with E.P. Haines, an engineer who suggested that
more precise milling, closer tolerances in the moving
components, and lighter-weight materials would do the
trick. Haines was right. When the reworked engine was
connected to the solar collectors, it developed 33
horsepower and drove a water pump that gushed 3,000
gallons per minute onto the Talcony soil.

Shuman calculated that the Talcony plant cost $200 per
horsepower compared with the $80 of a conventionally
operated coal system--a respectable figure, he pointed
out, considering that the additional investment would
be recouped in a few years because the fuel was free.
Moreover, the fact that this figure was not initially
competitive with coal or oil-fired engines in the
industrial Northeast did not concern him because, like
the French entrepreneurs before him, he was planning
to ship the machine to the vast sunburnt regions in
North Africa.

To buy property and move the machine there, new
investors were solicited from England and the Sun
Power Co. Ltd. was created. But with the additional
financial support came stipulations. Shuman was
required to let British physicist C. V. Boys review
the workings of the machine and suggest possible
improvements. In fact, the physicist recommended a
radical change. Instead of flat mirrors reflecting the
sun onto a flat-plate configuration, Boys thought that
a parabolic trough focusing on a glass-encased tube
would perform much better. Shuman's technical
consultant A.S.E. Ackermann agreed, but added that to
be effective, the trough would need to track the sun
continuously. Shuman felt that his conception of a
simple system was rapidly disintegrating.

Fortunately, when the machine was completed just
outside of Cairo, Egypt, in 1912, Shuman's fears that
the increased complexity would render the device
impractical proved unfounded. The Cairo plant
outperformed the Talcony model by a large margin--the
machine produced 33 percent more steam and generated
more than 55 horsepower--which more than offset the
higher costs. Sun Power Co.'s solar pumping station
offered an excellent value of $150 per horsepower,
significantly reducing the payback period for
solar-driven irrigation in the region. It looked as if
solar mechanical power had finally developed the
technical sophistication it needed to compete with
coal and oil.

Unfortunately, the beginning was also the end. Two
months after the final Cairo trials, Archduke
Ferdinand was assassinated in the Balkans, igniting
the Great War. The fighting quickly spread to Europe's
colonial holdings, and the upper regions of Africa
were soon engulfed. Shuman's solar irrigation plant
was destroyed, the engineers associated with the
project returned to their respective countries to
perform war-related tasks, and Frank Shuman died
before the armistice was signed.

Whether or not Shuman's device would have initiated
the commercial success that solar power desperately
needed, we will never know. However, the Sun Power Co.
can boast a certain technical maturity by effectively
synthesizing the ideas of its predecessors from the
previous 50 years. The company used an absorber
(though in linear form) of Tellier and Willsie, a
reflector similar to Ericsson's, simple tracking
mechanisms first used by Mouchout and later employed
by Eneas, and combined them to operate an engine
specially designed to run with solar-generated steam.
In effect, Shuman and his colleagues set the standard
for many of the most popular modern solar systems 50
to 60 years before the fact.

The Most Rational Source
The aforementioned solar pioneers were only the most
notable inventors involved in the development of solar
thermal power from 1860 to 1914. Many others
contributed to the more than 50 patents and the scores
of books and articles on the subject. With all this
sophistication, why couldn't solar mechanical
technology blossom into a viable industry? Why did the
discipline take a 50-year dive before again gaining a
measure of popular interest and technical attention?

First, despite the rapid advances in solar mechanical
technology, the industry's future was rendered
problematic by a revolution in the use and transport
of fossil fuels. Oil and coal companies had
established a massive infrastructure, stable markets,
and ample supplies. Also, besides trying to perfect
the technology, solar pioneers had the difficult task
of convincing skeptics to see solar energy as
something more than a curiosity. Visionary rhetoric
without readily tangible results was not well received
by a population accustomed to immediate gratification.
Improving and adapting existing power technology,
deemed less risky and more controlled, seemed to make
far more sense.

Finally, the ability to implement radically new
hardware requires either massive commitment or the
failure of existing technology to get the job done.
Solar mechanical power production in the late
nineteenth and early twentieth centuries did not meet
either criterion. Despite warnings from noted
scientists and engineers, alternatives to what seemed
like an inexhaustible fuel supply did not fit into the
U.S. agenda. Unfortunately, in many ways, these
antiquated sentiments remain with us today. During the
1970s, while the OPEC nations exercised their economic
power and as the environmental and "no-nuke" movements
gained momentum, Americans plotted an industrial coup
whose slogans were energy efficiency and renewable
resources. Consequently, mechanical solar power--along
with its space-age, electricity-producing sibling
photovoltaics, as well as other renewable sources such
as wind power--underwent a revival. And during the
next two decades, solar engineers tried myriad
techniques to satisfy society's need for power.

They discovered that dish-shaped reflectors akin to
Mouchout's and Eneas's designs were the most efficient
but also the most expensive and difficult to maintain.
Low-temperature, nonconcentrating systems like
Willsie's and Tellier's, though simple and less
sensitive to climatic conditions, were among the least
powerful and therefore suited only to small, specific
tasks. Stationary reflectors like those used in
Adams's device, now called Power Tower systems,
offered a better solution but were still pricey and
damage prone.

By the mid-1980s, contemporary solar engineers, like
their industrial-revolution counterparts Ericsson and
Shuman, determined that for sunny areas, tracking
parabolic troughs were the best compromise because
they exhibited superior cost-to-power ratios in most
locations. Such efforts led engineers at the Los
Angeles-based Luz Co. to construct an 80-megawatt
electric power plant using parabolic trough collectors
to drive steam-powered turbines. The company had
already used similar designs to build nine other solar
electric generation facilities, providing a total of
275 megawatts of power. In the process, Luz engineers
steadily lowered the initial costs by optimizing
construction techniques and taking advantage of
economies of buying material in bulk to build
ever-larger plants until the price dropped from 24 to
12 cents per kilowatt hour. The next, even larger
plant--a 300-megawatt facility--scheduled for
completion last year, promised to provide 6 to 7 cents
per kilowatt hour, near the price of electricity
produced by coal, oil, or nuclear technology.

Once again, as with Shuman and his team, the gap was
closing. But once again these facilities would not be
built. Luz, producer of more than 95 percent of the
world's solar-based electricity, filed for bankruptcy
in 1991. According to Newton Becker, Luz's chairman of
the board, and other investors, the demise of the
already meager tax credits, declining fossil fuel
prices, and the bleak prospects for future assistance
from both federal and state governments drove
investors to withdraw from the project. As Becker
concluded, "The failure of the world's largest solar
electric company was not due to technological or
business judgment failures but rather to failures of
government regulatory bodies to recognize the economic
and environmental benefits of solar thermal generating
plants."

Other solar projects met with similar financial
failure. For example, two plants that employed the
tower power concept, Edison's 10-megawatt plant in
Daggett, Calif., and a 30-megawatt facility built in
Jordan performed well despite operating on a much
smaller scale and without Luz's advantages of heavy
initial capital investment and a lengthy
trial-and-error process to improve efficiency. Still
they were assessed as too costly to compete in the
intense conventional fuel market.

Although some of our brightest engineers have produced
some exemplary solar power designs during the past 25
years, their work reflects a disjointed solar energy
policy. Had the findings of the early solar pioneers
and the evolution of their machinery been more closely
scrutinized, perhaps by Department of Energy officials
or some other oversight committee, contemporary
efforts might have focused on building a new
infrastructure when social and political attitudes
were more receptive to solar technology. Rather than
rediscovering the technical merits of the various
systems, we might have been better served by reviewing
history, selecting a relatively small number of
promising systems, and combining them with
contemporary materials and construction techniques.
Reinventing the wheel when only the direction of the
cart seems suspect is certainly not the best way to
reach one's destination.

While the best period to make our energy transition
may have passed and though our energy future appears
stable, the problems that initiated the energy crisis
of the 1970s have not disappeared. Indeed, the
instability of OPEC and the recent success in the Gulf
War merely created an artificial sense of security
about petroleum supplies. While we should continue to
develop clean, efficient petroleum and coal technology
while our present supplies are plentiful, this
approach should not dominate our efforts. Alternative,
renewable energy technologies must eventually be
implemented in tandem with their fossil-fuel
counterparts. Not doing so would simply provide an
excuse for maintaining the status quo and beg for
economic disruption when reserves run low or political
instability again erupts in oil-rich regions.

Toward that end, we must change the prevailing
attitude that solar power is an infant field born out
of the oil shocks and the environmental movement of
the past 25 years. Such misconceptions lead many to
assert that before solar power can become a viable
alternative, the industry must first pay its dues with
a fair share of technological evolution.

Solar technology already boasts a century of R&D,
requires no toxic fuel and relatively little
maintenance, is inexhaustible, and, with adequate
financial support, is capable of becoming directly
competitive with conventional technologies in many
locations. These attributes make solar energy one of
the most promising sources for many current and future
energy needs. As Frank Shuman declared more than 80
years ago, it is "the most rational source of power."





=====
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
http://www.infiltration.org
http://www.darkpassage.com
http://www.mattoledefense.org/alerts/08192001_video.html
http://sf.indymedia.org/display.php?id=100562#100565

__________________________________________________
Do You Yahoo!?
Yahoo! GeoCities - quick and easy web site hosting, just $8.95/month.
http://geocities.yahoo.com/ps/info1

<A HREF="http://www.ctrl.org/";>www.ctrl.org</A>
DECLARATION & DISCLAIMER
==========
CTRL is a discussion & informational exchange list. Proselytizing propagandic
screeds are unwelcomed. Substance—not soap-boxing—please!  These are
sordid matters and 'conspiracy theory'—with its many half-truths, mis-
directions and outright frauds—is used politically by different groups with
major and minor effects spread throughout the spectrum of time and thought.
That being said, CTRLgives no endorsement to the validity of posts, and
always suggests to readers; be wary of what you read. CTRL gives no
credence to Holocaust denial and nazi's need not apply.

Let us please be civil and as always, Caveat Lector.
========================================================================
Archives Available at:
http://peach.ease.lsoft.com/archives/ctrl.html
 <A HREF="http://peach.ease.lsoft.com/archives/ctrl.html";>Archives of
[EMAIL PROTECTED]</A>

http:[EMAIL PROTECTED]/
 <A HREF="http:[EMAIL PROTECTED]/";>ctrl</A>
========================================================================
To subscribe to Conspiracy Theory Research List[CTRL] send email:
SUBSCRIBE CTRL [to:] [EMAIL PROTECTED]

To UNsubscribe to Conspiracy Theory Research List[CTRL] send email:
SIGNOFF CTRL [to:] [EMAIL PROTECTED]

Om

Reply via email to