Nearly 10 years ago - in October, 2007, to be precise - we (exactly "who" to be mentioned later) successfully managed a 173 mile, Earth-based all-electronic two-way contact between two remote mountain ranges in western Utah.
For many years before this I'd been mulling over in the back of my mind
various ways that optical ("lightbeam") communications could be
accomplished over
long distances. Years ago, I'd observed that even a modest,
2 AA-cell focused-beam flashlight could be easily seen over a distance
of more than 30 miles (50km) and that sighting even the lowest-power
Laser over
similar distances was fairly trivial - even if holding a steady beam
was not. Other than keeping such ideas in the back of my
head, I
never
really did more that this - at least until the summer of 2006, when I
ran across
a web site that intrigued me, the "Modulated
Light DX page"
written by Chris Long (now amateur radio operator VK3AML) and Dr. Mike Groth (VK7MJ). While I'd been following
the history and progress of such things all along, this and similar
pages rekindled the intrigue, causing me to do additional research - and
I
began to build things.
Working up to the distance...
Over the winter of 2006-2007 I spent some time building, refining, and
rebuilding various circuits having to do with optical
communications. Of particular interest to me were circuits used
for
detecting weak optical signals and it was those that I
wanted to see if I could improve. After considerable
experimentation, head-scratching, cogitation, and testing, I was
finally able to
come up with a fairly simple optical
receiver circuit that was at least
10dB more
sensitive than other voice-bandwidth circuits that were out
there. Other experimentation was done on modulating light
sources and the first serious attempt at this was building a PIC-based PWM
(Pulse-Width Modulation) circuit followed, somewhat
later,
by a simpler current-linear
modulator - both being approaches that
seemed to work extremely well.
After this came the hard part: Actually assembling the mechanical parts that made up the optical transceivers. I decided to
follow the field-proven
Australian
approach of using large, plastic,
molded Fresnel
lenses in conjunction with high-power LEDs for the
source of light emissions with a second parallel lens and a photodiode
for reception and the stated reasons for taking this approach
seemed to me to be quite well thought-out and sound - both
technically and practically. This led to the eventual
construction of an optical
transceiver that consisted of a pair of
identical Fresnel lenses, each being 318 x 250mm (12.5" x 9.8")
mounted side-by-side in a rigid, wooden enclosure comprising an optical
transceiver with parallel transmit and
receive "beams." In taking this approach, proper aiming of either
the transmitter or
receiver
would guarantee that the other was already
aimed - or very close to being properly aimed - requiring only a single
piece of
gear to be deployed with precision.
After completing this first transceiver I hastily built a second
transceiver to be used at the "other" end of test path.
Constructed of foam-core
posterboard, picture frames and inexpensive, flexible vinyl "full-page"
magnifier Fresnel
lenses, this transceiver used, for the optical emitter and transmitter
assemblies, my original, roughly-repackaged prototype circuits.
While it was
neither pretty or
capable of particularly high performance, it
filled the need of being the "other" unit with which communications
could be
carried out for testing: After all, what good would a receiver be
if there were no transmitters?
On March
31, 2007 we completed our first 2-way optical QSO
with a path that crossed the Salt Lake Valley, a distance of about 24
km (15 miles.) We were pleased to note that our signals were
extremely strong and, despite the fact that our optical path crossed
directly over downtown Salt Lake City, they seemed to have
30-40dB signal-noise ratio - if you ignored some 120 Hz hum and the
occasional "buzz" from an unseen, failing streetlight. We also
noted a
fair amount of amplitude scintillation, but this wasn't too
surprising
considering that the streetlights visible from our locations also
seemed to shimmer being subject to the turbulence caused by the
ever-present
temperature inversion layer in the valley.
Bolstered by this success we conducted several other experiments over
the next several months, continuing to improve and build more gear,
gain experience, and refine our techniques. Finally, for August
18, 2007, we decided on a more ambitious goal: The
spanning of a
107-mile optical path. By this time, I'd completed a third
optical transceiver using a pair of larger (430mm x 404mm, or 16.9"
x
15.9")
Fresnel lenses, and it significantly out-performed the
"posterboard"
version that had been used earlier. On this occasion we were
dismayed by the amount of haze in the air - the remnants of smoke that
had blown into the area just that day from California wildfires.
Ron, K7RJ and company (his wife Elaine, N7BDZ and Gordon, K7HFV) who
went to
the northern end of the path (near Willard Peak, north of Ogden, Utah)
experienced even more trials, having had to retreat on three occasions
from their chosen vantage point due to brief, but intense
thunderstorms. Finally, just before midnight, a voice exchange
was completed with some difficulty - despite the fact that they never
could see the distant transmitter with the naked eye due to the
combination of
haze and light pollution - over this path, with the southern end (with
Clint, KA7OEI and Tom, W7ETR) located near Mount Nebo, southeast of
Payson, Utah.
Following the successful 107-mile exchange we decided that it was
time to try an even-greater distance. After staring at maps and
poring
over topographical data we found what we believed to be a 173-mile
line-of-sight shot that seemed to provide reasonable accessibility at
both ends - see figure 1. This path spanned the Great Salt Lake
Desert - some of the flattest, desolate, and most remote land in the
continental U.S. At the south end of this path was Swasey Peak,
the
tallest point in the House range, a series of mountains about 70 miles
west of Delta, in west-central Utah. Because Gordon had hiked
this
peak on more than one occasion we were confident that this goal was
quite attainable.
At the north end of the path was George Peak in the Raft River range,
an obscure line of mountains that run east and west in the extreme
northwest corner of Utah,
just south of the Idaho boarder. None of us had ever been there
before, but our research indicated that it should be possible to drive
there using a high-clearance 4-wheel drive vehicle so, on August 25,
2007, Ron and Gordon piled into my Jeep (along with a 2nd
spare tire
swiped from Ron's Jeep as
recommended by more than one account) and we headed north to
investigate.
Getting there:
Following the Interstate highway nearly to the Idaho border, we turned
west onto a state highway, following it as the road swung north into
Idaho,
passing the Raft River range, and we then turned off onto a gravel road
to
Standrod,
Utah. In this small town (a spread-out collection of
houses,
really) we turned onto a county road that began to take us up canyons
on the northern slope of the range. As we continued to climb, the
road
became rougher and we resorted to peering at maps and using our
intuition to guide us onto the
one road that would take us to the top of the mountain range.
Luckily, our guesses were correct and we soon found ourselves at the
top
of the ridge. Traveling for a short distance, we ran into a
problem: The road stopped at a fence gate that
was
plastered with "No Trespassing" signs. At this point, we simply
began
to follow what looked like road that paralleled the fence only
to discover, after traveling several hundred feet - and past a point at
which we could safely turn around - that this "road" had degenerated
into
a rather precarious dirt path traversing a steep slope. After
driving
several hundred more feet, fighting all the while to keep the Jeep on
the road and moving in a generally forward direction, the path leveled
out once again and
rejoined what appeared to be the main road. After a combination
of
both swearing at and praising deities we vowed that we would never travel on that "road" again and simply stay on what had appeared to
have been the main road,
regardless of what the signs on the gates said!
Looking for Swasey Peak:
Having passed these trials, we drove along the range's ridge top,
looking to the south. On this day, the air was quite hazy -
probably
due to wildfires that were burning in California, and in the
distance we
could vaguely spot, with our naked eyes, the outline of a mountain
range that we thought to be the House range: In comparing
its
outline and position with a computer-simulated view, it "looked" to be
a fairly close match as best as we could guess.
Upon seeing this distant mountain we stopped to get a better look, but
when we looked through binoculars or a telescope the distant outline
seemed to
disappear - only to reappear once again when viewed with the naked
eye. We finally realized what was happening: Our
eyes and brain are "wired" to look at objects, in part, by detecting
their outlines,
but in this case the haze reduced the contrast considerably. With
the naked eye, the distant mountain was quite small but with the
enlarged image in the binoculars and telescope the apparent contrast
gradient around
the object's outline was greatly
diminished. The trick to being able to visualize the distant
mountain turned out be keeping the
binoculars moving as our eyes and brain are much more
sensitive
to slight changes in brightness of moving
objects than stationary
ones. After discovering this fact, we noticed with some amusement
that the distant mountain seemed to vanish from sight once we stopped
wiggling the binoculars only to magically reappear when we moved them
again. For later analysis we also took
pictures
at this same location and noted the GPS coordinates.
Continuing onwards, we drove along the ridge toward George Peak.
When
we got near the GPS coordinates that I had marked for the peak we
were somewhat disappointed - but not surprised: The highest spot
in the neighborhood, the peak, was one of several gentle, nondescript
hills that
rose above the
road only by a few 10's of feet. Stopping, we ate lunch, looked
through binoculars and telescopes, took pictures, recorded GPS
coordinates, and thought apprehensively about the
return trip along the road.
Returning home:
Retracing our path - but not taking the "road" that had
paralleled the fence line - we soon came to the gate that marked the
boundary of the private land. While many of the markings were the
same at this gate, we noticed another sign - one that had been missing
from the
other end of the road - indicating that this was, in fact,
a
public right-of-way plus the admonition that those traveling
through must stay on the road. This sign seemed to
register with what we thought we'd remembered about Utah laws
governing the use of such roads and our initial interpretation of the
county parcel maps: Always leave a gate the way you
found it, and don't go off the road! With relief, we crossed this
parcel with no difficulty and soon found ourselves at the other gate
and in familiar territory.
Retracing our steps down the mountain we found ourselves hurtling
along the state highway a bit more than an hour later - until I heard
the unwelcome sound of a noisy tire. Quickly pulling over I
discovered that a large rock that had embedded itself in
the middle of the
tread of a rear tire. After 45 minutes of changing the tire and
bringing the
spare up to full pressure, we were again underway - but with only one
spare remaining...
Analyzing the path:
Upon returning home I was able to analyze the photographs that I had
taken. Fortunately, my digital SLR camera takes pictures in "Raw"
image
mode, preserving the digital picture without loss caused by converting
it to a lossy format like JPEG. Through considerable contrast
enhancement, the "stacking" of several similar images using an
astronomical photo processing program and making a comparison against
computer-generated view I
discovered that the faint outline that we'd seen
was not Swasey Peak but was, in fact, a range that was
about 25 miles (40km) closer - the Fish Springs mountains - a mere
150 or so
miles (240km) away. Unnoticed (or invisible) at the time of our
mountaintop visit was another
small bump in the distance that was, in fact, Swasey Peak.
Interestingly, the first set of pictures were taken at a location that,
according to the computer analysis, was barely line-of-sight
with Swasey Peak. At the time of the site visit we had assumed
that the just-visible mountain that we'd seen in the distance was
Swasey Peak and that there was some sort of parallax error in the
computer simulation, but analysis revealed that not only was the
computer simulation correct in its positioning of the distant features,
but also that the apparent height of Swasey Peak above the horizon was
being enhanced by atmospheric refraction - a property that the program
did not take into account: Figure 2 shows a comparison
between the computer simulation and an actual photograph taken from
this same location.
Building confidence - A retry of the 107-mile path:
Having verified to our satisfaction that we could not only get to the
top of the Raft River mountains, but also that we also had a
line-of-sight
path to
Swasey Peak, we began to plan for our next adventure. Over the
next several weeks we watched the weather and the air - but before we
did this, we wanted to try our 107-mile path again in clearer weather
to make sure that our gear was working, to gain more experience with
its setup and operation, and to see how well it would work over a long
optical path given reasonably good seeing conditions: If we had
good
success over a 107-mile path we
felt confident that we should be able to manage a 173-mile path.
A few weeks later, on September
3, we got our chance: Taking
advantage of clear weather just after a storm front had moved through
the area
we went back to our respective locations - Ron, Gordon and Elaine at
Inspiration Point while I went (with Dale, WB7FID) back to the location
near Mt. Nebo. This time, signal-to-noise
ratios were 26dB better than before and voice was "armchair"
copy. Over the several hours of experimentation we were able to
transmit not only voice, but SSTV
(Slow-Scan Television) images over the LED link - even
switching over to using a "raw" Laser Pointer for one experiment and a
Laser module collimated by an 8" reflector telescope in another.
With our success on the clear-weather 107-mile path we waited for our
window to attempt the 173-mile path between Swasey and George
Peak but in the following weeks we were dismayed by the appearance
of bad weather and/or frequent haze - some of the latter resulting from
the
still-burning wildfires around the western U.S.
To be continued!
[End]
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