|
Analysis of a Photograph of a High Speed Ball of
Light
Richard F. Haines
Copyright 2003
Los Altos, California
January 26, 2002
Date of Photograph: July 16, 1988
Time of Photograph: approx. 1400 PST
Location: 33o 49' N; 116o 44' W (West of Palm Springs,
CA)
Duration of Sighting: from 5 to 10 seconds
Number of UAP: one
Number of eye witnesses: one plus others (alleged)
Number of photographic frames: one
Abstract
This pilot sighting report and color photograph
of an unidentified aerial phenomena (UAP) called for a number of
different forensic methods including photo-analysis, aircraft window
study, camera-lens-film analyses, and evaluation of reporter credibility.
The single frame, Kodak color, copy negative was submitted for examination
by one of the several eye-witnesses. This paper describes the results
of these analyses. It is concluded that: (1) whatever the UAP was
it was probably in sub-sonic flight. If the UAP was travelling at
subsonic speed the estimated total sighting duration and/or its
estimated distance from the witness are clearly in error by a factor
of two or more, (2) no evidence of a hoax or double exposure was
found nor were any bolides, meteorites, or other unidentified aerial
phenomena reported for that time and place, (3) the luminance of
the main body of the object and immediately adjacent tail area were
so high they fully saturated (exposed) the relatively ÒslowÓ
film. This may explain why the photograph does not correspond closely
to what was seen, (4) the filmÕs optical density, as measured
along the length of the white tail behind the UAP, changed in a
peculiar fashion and is not characteristic of reflected sunlight
off water droplet vapor, and (5) interesting micro-details were
discovered that suggest the possibility of some type of energy emissions
extending from the UAP but not necessarily in the direction of its
flight. The nature of the UAP and constitution of its atmospheric
trail remains unknown at this time.
Introduction and Flight Background Details
As many writers have said before, the credibility
of a purported ufo photograph rests far more upon the credibility
of the photographer than upon all of the technical characteristics
and details producing the photograph. But when the credibility of
the eye witness is found to be high and no evidence of fraud or
hoax is found it is more reasonable to accept the photograph at
least as what it purports to be, evidence of an interesting, if
unknown, phenomenon of some kind.
An interesting aerial sighting (with 35mm color
slide) was reported by photographer-witness, R. J. Childerhose (1966)
on August 27, 1956. He was flying a Royal Canadian Air Force F-86
jet at the time. As noted by Klass (1968, pg. 146), "The photo
(used on the dust cover of his book) shows an intensely bright,
white, egg-shaped object that seems to be suspended below an intense
thunderstorm" but visible through a hole in the clouds whose
tops were at about 12,000 feet altitude or higher. He told Klass
that the object seemed to have sharply defined edges and looked
"like a shiny silver dollar sitting horizontal." The pilot
also wrote to tell Dr. James McDonald (Maccabee, 1999, pg. 209)
that "Éthe photo of the bright object doesn't represent
quite what appeared to the naked eye. When I first saw the object
it appeared as a very bright, clearly defined discoid, like a silver
dollar lying on its side. The photo makes it look like a blob of
light, the result of light intensity." Both Klass and Altschuler,
a member of the University of Colorado's UFO study panel (Gillmor,
1968, pg. 733), felt that the object seen and photographed by Childerhose
was ball lightning. Later work by Maccabee (1999) suggests that
few of the characteristics of ball lightning match those seen and
photographed by this pilot witness.
Childerhose tried to explain why what he saw did
not correspond to what appeared on his photograph. He stated, "The
light it emitted was very much brighter than the existing sunlight
at that time of day and this over-exposed the film, causing the
blurred edges you see in the picture." (Klass, 1968, pg. 147)
Subsequent assumptions and calculations by Maccabee (1999) suggest
that the object was actually made up of two distinct bright spots/objects
very close to one another whose luminous surrounds merged together
and that its power output would have been more than 109 watts. This
classic photograph has continued to perplex investigators over the
years. Interestingly, the author learned about the existence of
another photograph, described in this paper, that contains a number
of elements similar to the Childerhose event. As will be seen, the
present case is important not only because of the apparent overlap
it has with the earlier event but also because it might shed more
light on why some photographs don't correspond more closely with
what was reportedly seen.
The author received word via e-mail to the National
Aviation Reporting Center on Anomalous Phenomena (NARCAP)1 on January
27, 2001 that a John Williams (pseudonym) had in his possession
an Òoriginal photo and negative as well as the flight logÉÓ.
In this e-mail he also provided a relatively complete narrative
of his flight location when the event occurred, viz., five miles
NE of Mt. San Jacinto which is about eight miles NW of Palm Springs
airport, California.
Basic Sighting Events
Mr. Williams, piloting a Mini-Nimbus/C sailplane2,
towed behind a standard tow plane, took off from Hemet, California's
Ryan airport[1] at 1315 hrs PST on July 16, 1988 and climbed toward
the NE, eventually reaching an altitude of about 12,000 feet above
ground level (AGL). The ground in this area rises from 1,600 feet
above mean sea level (MSL) gradually toward the east where the San
Jacinto mountain range (typically from 7,000 to 10,000 feet high)
runs roughly north and south. Since the primary purpose of this
flight (which lasted just over ninety minutes) was to obtain color
photographs of the sailplane in flight from a chase plane, Mr. Williams
had arranged for a personal friend to ride both as passenger and
photographer in the Mooney M20C
aircraft4 with the pilot (Mr. D. L. S.) sitting in the left seat.
Mr. R. C. sat in the right-front seat and took twenty four photographs
(mainly) through his right-hand window. Mr. Williams provided him
both the camera and film (discussed later) and recovered all items
immediately upon landing5.
Upon reaching 12,000 feet altitude the (commercial)
tow-plane released the sailplane and immediately banked away to
return to Hemet airport. The pilot of the chase plane, Mr. D.L.S.,
followed behind and generally to the left hand side of the sailplane
which permitted the photographer to take his photos from the right
hand window. All three individuals were in constant radio communication
throughout the flight on 123.3 MHz. Figure 1 is a photograph of
the Mooney M20C chase plane taken by Williams with his calibrated
cockpit camera during the flight.

Figure 1 - Mooney M20C Aircraft
(Registration: N1985Y)
Figure 2 was prepared to help understand the relative
instantaneous locations of the sailplane (S), chase plane (A) and
the unidentified aerial phenomenon (UAP) of interest, and other
geometry. The heavy black line (V - V') indicates the approximate
flight path of the sailplane during the five to ten second-long
visual sighting. The straight dashed line (Y - Z) is the assumed
linear path of motion of the UAP. The angle (X-A-X'; not drawn to
scale) represents the camera lens' angular diameter subtending an
arc (Th) of approximately 57 degrees (discussed later).

Figure 2 - Sketch of Relative Aircraft Locations
and UAP During the Visual Sighting
Note in Figure 2 that during the sighting the sailplane
was on a heading of about 45 degrees (magnetic); it was approximately
Òfive miles North East of Mt. San JacintoÓ at the
time. In the primary witnessÕ own words, ÒÉa
shallow descent was established to 11,000 ft. to build air speed
for (the) photo run. A number of photos were taken without anything
unusual (happening), then a bank and turn to the right, away from
the chase plane was made (V Ð VÕ). During this turn observers
in both aircraft observed, and the photographer in the chase plane
photographed the UAP seen in Figure 3. Williams said that the fast-moving
object looked like "Éa large reflecting sphereÉ
almost like a large ball bearing with a tail."
Initially, the UAP came from the 7:00 position
relative to the sailplane (point Y) and passed in front of him at
an estimated distance (d) of about 1 Ð 2 miles. According to
Williams, "It (the UAP) exited (my) vision at the 1:00 position
relative to the sailplane.Ó (point Z). Perhaps the single
most critical question is how large was distance (d)?
Mr. Williams indicated that they landed between
1445 and 1500 hrs at Hemet, Ryan Field. This amounted to a total
flight duration of from 90 to 105 minutes.
; Chase Plane Details. With a propeller tip-to-tip
length of 6Õ 2Ó located less than ten feet ahead of
the cameraman it would be unwise to photograph another aircraft
looking through it directly ahead of the chase plane. A fast shutter
speed could almost ÒstopÓ a blade making it become
visible during its rotation or at least produce a darkened blur
region that could reduce the clarity of the image. So Mr. R. C.
took all photos through the right side cabin window. These photographs
would likely have been taken somewhat oblique to the window plane
as suggested in Figure 1.
The UAP Photograph
Figure 3 shows the Mini-Nimbus/C sailplane against
a clear blue-sky background with the unidentified aerial phenomena
(UAP) (white streaked region) seen just above it. The local time
was about 1400 hrs. If the photograph is rotated thirty degrees
CW to place the sailplane in a right-hand bank the UAPÕs
trajectory is seen in a slight climb just as Williams recalled it.
If the UAP was at a higher altitude than the witness
and in straight and level flight, perceptu- ally speaking, it would
have appeared to be rising as it passed him.

Figure 3 - Photograph of Sailplane and UAP Other
Potential Eye Witnesses
This event allegedly involved as many as five eye
witnesses in four different aircraft: (1) the sailplane in which
Mr. Williams visually sighted the UAP, (2) a Mooney model M20C chase
plane with a pilot (D. S. now deceased) and Mr. R. C. the photographer
and friend of Mr. Williams, (3) a second sailplane in the vicinity
whose pilot (Capt. Leo; first name) was the first to see the approaching
UAP, and (4) the tow plane pilot.6 It was learned that Mr. R. C.,
was an engineer who had worked previously for the Hewlett-Packard
Company. He is a "very private person" according to Williams.
In 1988 both he and Williams were employed in law enforcement and
were very concerned that their careers would be affected by seeing
and reporting this phenomenon. They maintained only infrequent contact
after he (Williams) moved from southern California to the state
of Washington. Williams did not know the identity of Capt. Leo other
than his first name and that he was a commercial pilot. Although
over thirteen years had passed since this incident took place the
author attempted to locate the other alleged witnesses but without
success. When asked why he waited so long to report his sighting
Williams answered that he had no particular interest in ufo nor
did he even place his photograph in that category. He simply forgot
about the incident and the photograph until many years later (January
10, 2000) when he came across the National UFO Reporting Center's
web site and decided to submit a report to them "in case someone
might be interested in it." As mentioned above, he subsequently
learned of NARCAP's existence and contacted us because of our interest
in UAP and flight safety.
Camera-Lens-Film
Camera. A Minolta Maxxum Model 7000, 35mm, single
lens reflex camera body was used with motorized film advance capability
(permitting up to two frames/second in the continuous exposure mode).
The camera was allegedly set to AE (automatic exposure) mode such
that all the photographer had to do was aim, zoom, and shoot.
Lens. A Rokor zoom lens was used with focal length
range from 28 to 80 mm. The f-stop range for this lens is from 3.5
to 4.5 for these limiting focal lengths, respectively.
Set to the full zoom position (28mm focal length),
the angular width of the resulting photograph is approximately 57
degrees arc. At the manufactureÕs ÔstandardÕ
setting the photoÕs angular width would have been about 40
degrees arc which value is used for calculations made in the present
paper. Since the zoom setting was not recorded this value could
be in error. Nevertheless, the overall conclusions of the analyses
are not changed materially if a different angular width were used.
In the A-E mode, this camera possesses a fixed
exposure Òprogram,Ó i.e., the relationship between
aperture and shutter speed at a given zoom setting is pre-established.
Figure 4 presents the A-E program factors for this model camera.
It shows that mid-way between f3.5 and f4.5 and its ÒTELEÓ
lens setting, the resultant shutter speed would have been approximately
1/500 second. Likewise, if the zoom lens had been set at its mid-point
the corresponding shutter speed would have been approximately 1/250th
second. Finally, if the zoom lens had been set at its widest setting
the corresponding shutter speed would have been about 1/30th second.
In order to obtain a shot with the sailplane almost filling the
entire frame the zoom setting would have had to be at least at its
mid point or more; an assumed shutter speed of 1/250th second is
used here which is consistent with the sharpness of the sailplane's
image.

Figure 4 - Automatic Exposure Relationships
Shutter speed is important because the longer the
shutter is open the greater is the chance for image blur to occur
due to chase plane/camera motion. Conversely, a sharply defined
target object indicates a relatively stable camera and target during
an exposure. This clearly was the case here. The upper and front
edge of the UAP that appears to have a double boundary must be due
to some other cause than camera motion.
Film. The negative stock was Kodak VPS 5026 which
is also known as Vericolor III Professional Film. This 35mm, medium
speed, color negative film possesses a nominal ASA rating of 100.
ÒThis film is designed for exposure with daylight or electronic
flash at exposure times of 1/10,000 second to 1/10 second.Ó
(Kodak, Pg. 2, 1997) The grain size and image structure on the enlargement
received by the author appears to be consistent with statements
made in the Kodak specification sheet; their print grain index sets
a value of 25 as the Òapproximate visual threshold for graininessÓ
(given various standardized viewing conditions). A higher number
represents an increase in the amount of observed graininess. KodakÕs
published print grain index for a 35mm negative of Vericolor III
film enlarged to 8Ó x 10Ó is 61. If further enlarged
to 16Ó x 20Ó this value increases to 91. Inspection
of the present 8Ó x 11Ó color positive print reveals
obvious graininess, as expected. The yellow forming dye layer peaks
in sensitivity at 425 nm and ends at a maximum wavelength of 525
nm. The magenta layer peaks at 558 nm and ends at 620 nm and the
cyan-forming layer peaks at 660 nm and ends at 690 nm. Its modulation-transfer
function curve is relatively flat at between 2.5 and 12 cycles/minute
arc and then smoothly falls off to 32% response at about 75 cycles/minute
arc. In short, this professional film supports relatively high resolution
photography over a wide range of contrasts. Consult the following
web site for more information:
http://www.kodak.com/global/en/professional/techPubs/e26/f002_0475ac.gif
On March 9, 2001 the author received a 4.25Ó
long, color negative strip containing one exposed frame (no. 3A)
connected to frames 4A and 5A that were unexposed for some unexplained
reason.Ó The single exposed UAP frame was in very good condition
with no scratches at all; it did contain a lighter density, linear
border measuring 2.05 mm wide on the vertical dimension and a 0.9
mm wide border on its lower edge. A positive print made by the author
from this negative showed these two black borders which was absent
on the 8Ó x 11Ó enlargement received from Williams
(i.e., either they had been cropped out or his photo had been made
from another negative). The total frame width was 36 mm as expected.
The presence of these two visible borders that could not have been
produced within the camera during exposure, coupled with the absence
of any exposed frames after the UAP frame, strongly suggest that
this was not the original negative but a copy negative. Where could
this copy negative have originated if not from Mr. Williams?
Film Processing. Mr. Williams said that upon
receiving his camera from his friend (R. C.) immediately after landing
he placed the camera (with film still inside) into his nylon camera
bag. He said he took the exposed film to a one-hour photo processor
on Convoy Street in San Diego Òthat afternoon or the following
day on his way to workÓ and, about a week later, picked up
the processed film and standard size positive color prints. ÒI
didnÕt even look at them then,Ó he explained. ÒI
was going flying again that weekend and took them with me to show
the guys how they had come out. We flew almost every weekend.Ó
When they all noticed the frame of interest (UAP) the chase plane
pilot said almost nothing while Mr. R. C. simply remarked, ÒLook
what we got on that photo!Ó ÒHe is a very stoic person,Ó
observed Mr. Williams, who then ordered two (2) each eight by eleven
inch color enlargements of the frame showing the UAP, one of which
he submitted with the negative.7
Details of the Photo-Analysis
The author made a number of digital scans of
this UAP frame as described below. The objective of these scans
was to better understand the nature of various image details. The
initial scan emphasized the left wing of the sailplane where the
white (vapor?) trail passed through it. If this was a double exposure
the (positive print) luminance of the wing in the region of the
trail should be somewhat higher than in regions where the trail
did not intersect it because of exposure additivity. Figure 5 shows
the seven equally spaced lines (each normal to the wingÕs
surface) along which density measurements were obtained as well
as ten locations along the white tail (see below).

Figure 5 - Sailplane Left Wing and Vapor Trail Image
(250 dpi scan, B=-10, C=+5%)
Happily, no evidence was found that would support
the contention that a double exposure had been carried out (within
a margin of error of +/- 2%). The luminance of the left wing was
not measurably greater where the vapor trail intersected it as compared
with the area where the wing was imaged against the clear blue sky.
White Trail. Two separate tests were performed
within the same region as Figure 5 to better understand details
of the vapor(?) trail. In the first test the 'Posterize' filter
(Adobe Photoshop) was set to five (5) levels to see if discrete
edges could be extracted from the otherwise diffuse white trail
behind the head of the object. As expected, several non-parallel,
tapering gradients could be discriminated as shown in Figure 6.

Figure 6 - UAP Vapor Trail Luminance Gradients (650
dpi scan, B=5, C=5%, posterize=5)
The second test performed used the 'Emboss'
Filter that significantly accentuates low-contrast, micro-image
grain details as a function of pseudo-illumination angle and pseudo-depth
of the pixel luminance. Figure 7 presents the results of this test
where areas of the image that are nearly 100% exposed areas (i.e.,
diffuse, very luminous white portion of the UAP tail) appear here
as an oval shaped, smooth, gray region. Note the enhanced 'granularity'
within the tail of the UAP (between lines X and Y) as compared with
the clear sky (outside lines X and Y). This large granularity is
probably due to sunlight scattered from greater turbulence within
the tail. One possibility may be that the UAP's white tail represents
ionized or otherwise excited air by emitted microwave energy from
the UAP (cf. McCampbell, Pp. 23-37, 1973), a possibility that is
further supported by Figures 8 and 9 related to the head or leading
edge of the effect.

Figure 7 - UAP Vapor Trail Grain Micro Structure
(1300 dpi scan, B=0, C=0, Angle= -66deg, Ht. = 10 pixels, Amt.=420%)
The final test conducted was on the variation
in luminance of the white tail streaming behind the UAP. It was
scanned at equal distances along its entire length (equivalent to
approximately 27.3 degrees arc) at the positions shown in Figure
5. Due to luminance variations at each location an upper and lower
value was recorded (Cols. 2 and 3). These relative luminance values
are given in Table 1.
| Table 1 Relative Luminance Distribution
Measured on Each Side of a Central Line Along Entire Length
of the Tail (See Figure 5 for Exact Measurement Locations) |
| |
Measurement
Location |
Lower
Value + |
Upper
Value + |
Angle (deg.)
behind head |
Cos A |
| (End of Tail) |
1.0 |
60 |
62 |
27.3 |
.518 |
| |
1.5 |
56 |
62 |
|
|
| |
2.0 |
58 |
62 |
23.9 |
.443 |
| |
2.5 |
56 |
64 |
|
|
| |
3.0 |
57 |
60 |
20.5 |
.374 |
| |
3.5 |
62 |
64 |
|
|
| |
4.0 |
58 |
68 |
|
|
| |
4.5 |
63 |
76 |
17.0 |
.306 |
| |
5.0 |
60 |
70 |
|
|
| |
5.5 |
58 |
67 |
13.6 |
.242 |
| |
6.0 |
67 |
75 |
|
|
| |
6.5 |
70 |
80 |
10.2 |
.178 |
| |
7.0 |
77 |
85 |
|
|
| |
7.5 |
95 |
98 |
6.8 |
.119 |
| |
8.0 |
100 |
100 |
|
|
| |
8.5 |
100 |
100 |
3.4 |
.059 |
| |
9.0 |
100 |
100 |
|
|
| (Head of UAP) |
9.5 |
100 |
100 |
0 |
0 |
* Approximately 0.5Ó apart along entire length of white tail
on enlarged image.
+ 100 % on this scale represents fully exposed film, i.e., highest
luminance.
It may be noted that, progressing away from
the "forward" end of the UAP, the luminance of the tail
decreases very rapidly beyond measurement location 5.5 (just below
and left of the sailplaneÕs wing in Figure 5) which suggests
an almost exponential decay rate. If the tail was composed only
of water vapor one would expect its reflectance (in the direction
of the camera) to be approximated by the cosine of the angle (sun
- UAP - camera) (cf. Col. 5 in Table 1) which it clearly does not.
Is the tail the by-product of a totally different process? Perhaps
it is made up of a substance with a rapid luminous half-life on
the order of a second or two or is composed of particles possessing
directional reflectivity, or some other explanation?
Head of UAP. Another set of tests was performed
on the region of the head of the UAP. This region is greatly overexposed
- virtually to the point of making any discrimination of object
edge or surface detail impossible. The ÔembossÕ filter
was used first. The homogeneous gray, flat-appearing region in Figure
8 depicts the 100% over exposed area of the film and is very likely
the actual UAP itself and part of its high luminance trail.

Figure 8 - UAP Head Area Emphasizing Coronal Micro-Structure
(450 dpi scan, B=10, C=15, emboss filter)
The left tip of the tail can be seen here.
The areas lying outside of this central, gray region are of more
interest, however. Thin, parallel fingers are seen protruding from
the rounded front of this image. It is interesting that most of
these fingers diverge from ten to fifteen degrees arc from the UAP's
flight path. What these short protrusions are is not known but may
represent energy projections of some sort.

Figure 9 - UAP Head Area Emphasizing Corona Macro-Structure
(450 dpi scan, B=10, C=15, RGB curves filter as described in text)
These protrusions also appear in Figure 9 where
the same part of the image was subjected to a sinusoidal filtering
(RGB Curves function) using seven (7) equally spaced cycles across
the 255 bits of exposure depth. This yields artificially enhanced
profiles of equal luminance. The luminance boundaries nearest the
head of the UAP tend to include the projections that characterize
the head itself while boundaries more distant do not. This effect
seems consistent with a radiation effect that decreases in intensity
with distance from the energy source.
The appearance of separated striations within
the white tail behind the UAP appear
to be consistent with condensation trails of a blunt-nose body in
sub-sonic flight through EarthÕs atmosphere (Smith, 2001).
Of course, the tail may be produced by a totally different mechanism.
In addition, if the UAP was travelling at a supersonic velocity
there would be a significantly different appearance of the bow shock
wave than is seen in the photograph. Further, the sailplane pilot
did not hear a sonic boom nor feel any sudden air buffeting during
or soon after the UAP passed him which would be consistent with
a vehicle travelling at sub-sonic velocity.
The last test performed on the head of the
UAP consisted of ÒstretchingÓ the exposure so that
only thirty [about 12%] of the 255 total (245 minus 215) bits of
input (exposure) ÒdepthÓ were stretched over two hundred
(200) bits of output Òdepth.Ó This was done to see
if very low contrast detail might lie buried within the greatly
overexposed region of the UAPÕs head. Figure 10 shows what
was found.

Figure 10 IAP Head Area With Luminance Stretching
(450 dpi scan, B=-5, C=0,Ê Stretched Exposure)
The magnification and image centering of Figure
10 are similar to that of Figures 8 and 9 for sake of comparison.
The luminance stretching was performed only within the smaller inset
square to permit comparison of its diameter with the unstretched
image (seen in the remainder of the figure. It may be noted that
the front edge of the head is relatively circular and (again) includes
several short protrusions located near the top of the head. The
spherical shaped object that Mr. Williams perceived likely corresponded
to part of this rounded region.
Sun's Location, Sky Luminance, and Weather Analysis
On July 16st 1988 at 1400 PST the sun was at 56
deg. 37.8 min. arc elevation and 244 deg. 33.6 min. azimuth at this
location. These values are useful in studying illumination and shadows
on the UAP, sailplane, and chase plane windows. The reported heading
of the sailplane (approx. 45 deg.) at the moment of the photograph
is consistent with the location of the sun's shadow on its fuselage.
In addition, a rather significant amount of sunlight is also reflected
from the earthÕs surface upon the underside of the sailplane
as seen in Figure 3.
No clouds are visible in the photograph which
supports Mr. Williams' statement that clouds had not yet developed
at this hour of the day.
The entire frame was scanned at 175 dpi and
a brightness filter applied to emphasize the range of luminance
along lines A and B (i.e., upper right to lower left). Figure 11
presents the resultant image. When the image is rotated about thirty
degrees CW these measurement lines represent the sky's horizontal
luminance gradient. Individual luminance values (3 x 3 pixel cursor)
are shown at their measurement location. It may be noted that the
sky in the upper right-hand corner of this image is visibly darker
than it is in the lower left-hand corner. A luminance difference
of about x 2.4 was found along line A which is larger than would
be expected from usual atmospheric particle light scattering across
this narrow an angle of sky (Allard, 1876).

Figure 11 - Sky Luminance Distribution (175 DPI
scan, B=+22; c=+76)
Windshield and Side Window Optical Analysis
In order to better understand the possible
cause of this large luminance gradient several hypotheses were formulated.
The first is that sunlight struck the Mooney's right-hand window
to create the veiling luminance seen in Figure 11. An attempt was
made to obtain geometric details of the side windowÕs rate
of curvature and other geometry. A rough estimate of these parameters
was made based upon inspection of a front-view photograph of this
aircraft (cf. Figure 12). The passenger's side window possesses
a large radius (approx. 24) horizontal curve over its upper half
progressing to a nearly flat plane over its bottom half.

Figure 12 - Nose View Photograph of Mooney M20S
Assuming that the chase plane was beginning
a left-hand bank away from the sailplane when the photograph was
taken the camera's line of sight would probably have been through
the lower, planar part of the window. With the Mooney's heading
of approximately 360 deg. and sunlight azimuth at about 244 deg,
sunlight could not have struck the tinted plexiglass side window.
In short, the lighting conditions were perfect for this photograph
with the sun illuminating the top and left-hand side of both the
Mooney and the sailplane; the window and camera both were in shadow.
The gradient of the sky's luminance seen in Figure 11 is not likely
caused by sunlight falling on the Mooney's side window if the aircraft
headings are those assumed here.
A second working hypothesis is that this large
luminance gradient across the film plane may have resulted during
its processing if a typical darkroom environment has been used.
The Kodak film specifications state: "Do not use a safelight.
Handle unprocessed film in total darkness." (Kodak, pg. 2,
1997) Fortunately, Mr. Williams was able to locate five other frames
taken from the chase plane during the same flight. He indicated
that the photograph shown in Figure 13 is very likely the frame
obtained just prior to the UAP photograph (Fig. 3; cf. footnote
7. This frame allowed a comparison to be made of the sky's luminance
gradient with that of the UAP frame; approximately the same range
of luminance was found in each which argues against the second hypothesis
as well as a third.
; The third hypothesis is that the UAP had somehow
caused additional exposure of the film perhaps due to emitted radiation
of some sort. Figure 13, taken many minutes before the appearance
of the UAP, suggests that this possibility is very unlikely because
of a similar amount of luminance gradient present here as well.

Figure 13 Photograph of Sailplane Taken Several
Minutes Before the UAP Photo
The fourth hypothesis is that this luminance
gradient is merely that of the natural daylight sky under these
conditions. Inspection of all photos provided by Mr. Williams tends
to support this hypothesis even though the range is higher than
would be expected (Allard, 1876, Koschmieder, 1924).
Calculations of Possible UAP Velocity
If the UAP (1) travelled in a straight line,
(2) travelled at a constant velocity, (3) was seen for five or ten
seconds (t) total, (4) travelled through the horizontal angles (Col.
A - see below), and (5) was either one or two miles away from Mr.
Williams (Col. D) it would have had to travel at the velocities
(Col. V) shown in Table 2.
Table 2 Calculated UAP Parameters for These Assumed
Parameters
__________________________________________________________________________
| Total Horizontal Angular
rate Duration Distance (st.mi.) |
Total
Distance |
Velocity |
Angle (deg arc.) of UAP (sec.) from Sailplane
|
Traveled (st. mi.) (mph) |
UAP Travelled (deg./sec.) t D Vin Time "t" |
| 100 |
20 |
5 |
1 |
2.38 |
1,714 |
| 100 |
20 |
5 |
2 |
4.77 |
3,434 |
| 100 |
10 |
10 |
1 |
2.38 |
857 |
| 100 |
10 |
10 |
2 |
4.77 |
1,717 |
| 100 |
10 |
10 |
3 |
7.15 |
2,574 |
| 110 |
22 |
5 |
1 |
2.86 |
2,059 |
| 110 |
22 |
5 |
2 |
5.71 |
4,111 |
| 110 |
11 |
10 |
1 |
2.86 |
1,030 |
| 110 |
11 |
10 |
2 |
5.71 |
2,056 |
| 110 |
11 |
10 |
3 |
8.57 |
3,085 |
It appears that all of these velocities
are too large in view of the likelihood that the UAP was travelling
at sub-sonic speed for reasons given above. Either the sighting
duration estimate was too short, the distance to the UAP was too
large, the angle through which the UAP appeared to pass was in error,
or some combination of these factors. Even the 857 mph (bold faced)
value given above is supersonic. Clearly, a rather large error exists
in these estimated parameters. Such perceptual errors are not at
all uncommon when there are few if any stable, visual landmarks
and/or time references available within the visual field (Haines,
1980). Even if the distance to the UAP was reduced to only one-half
mile it would have had to travel at 428 mph over ten seconds and
100 deg arc; at 0.75 mile distance it would have had to travel at
644 mph over ten seconds and 100 deg arc given the other estimates.
The change in azimuth angle through which the
sailplane traveled at 110 kts in a coordinated 20 deg banked turn
(no side slip assumed) to the right over five seconds equals about
14 degrees and 27 degrees over ten seconds.8 The sailplane would
have traversed about 700 and 1,400 feet during these two durations,
respectively. Since the UAP was seen initially on the left-hand
side of the sailplane, i.e., on the outside of his right-hand turn,
Williams would be turning in a direction to keep it in sight slightly
longer than if he were in straight flight by about 2.7 seconds.
A UAP subtending a visual angle of 2 deg. 35
min arc at one and two miles distance would measure 238 and 475
feet across, respectively. At 0.25 mile distance it would measure
59.4 feet across.
Evaluation of Reporter Credibility
Mr. John Williams was confirmed to be a licensed
pilot (S.E.L. and "Diamond" level soaring pilot with 18
years flying experience) at the time of the event. He did not possess
any waivers or limitations. He claimed to have had 400 logged hours
with 350 hrs. in high performance sailplanes "Éin multiple
flight envelopes and conditions." His reported directorship
on a prominent California aerospace museum in the 1980s also was
confirmed. His clear and detailed knowledge of aeronautics and flight
details was found to be accurate in every respect. No evidence of
any kind could be found that he ever attempted to capitalize on
this photograph in any way.
Discussion
Two primary subjects will be discussed: (1)
the differences (and possible causes) between what was reportedly
seen and what was recorded on the photograph and, (2) the ambiguity
of whether or not the negative submitted was original or a copy
negative and reasons for accepting it for study.
(1) Differences Between What was Seen and Photographed.
Mr. Williams remarked that the UAP looked to him like a Òlarge
reflective sphere É almost like a large ball bearing."
But this is not what his photo looked like. A quite similar situation
exists with the 1956 report by Childerhose discussed earlier. And,
when asked to comment on whether or not he remembered seeing a parallel
upper edge to the vapor trail that is visible in his photograph
he remarked, "The UAP looked more distinct and spherical than
it does in the photo, with an area to the rear, several times its
diameter that had a vapor quality." This perceptually-based
description clearly implies the presence of an object with a polished
metal surface and not a diffuse white ball with a vapor trail that
is seen on the film. He did recall seeing a "tail" behind
it.
Several possible explanations exist for these
appearance differences: (a) Williams' memory may have been modified
somewhat over the intervening years. Such examples of memory modification
are well documented (e.g., Shepard, 1979). (b) Williams changed
the visual description of the UAP for some unknown reason. The likelihood
of this seems small in view of the fact that his description of
the UAP didn't correspond at all to the photograph he submitted.
This argues in support of his honesty and self-assurance in this
sighting detail. (c) The radiation reflected or emitted by the "spherical"
UAP affected this film differently than it affected his retina and
visual system. This last possibility deserves further comment related
to both the geometric and the spectral sensitivity aspects of the
case.
Geometric Aspects. The author has conducted
laboratory research on both the perceptual and photographic effects
of using ultra-high luminance targets in support of the space program
(Haines, 1965, 1966, 1968, 1969, 1971) and has photographed highly
polished metal spheres and other surface shapes under full sunlight
conditions (e.g., Haines, Fig. 39, 40; 1980). These studies clearly
demonstrate that the normal human eye perceives very bright targets
differently than they will appear on film that has been exposed
under so-called "normal" conditions. Let us first consider
the visual appearance of a polished metal sphere. For prolonged,
light adapted viewing of a sunlit sphere one will see its entire
outline and "metallic" surface (reflecting sky and other
background) with a smaller diameter, reflected, virtual image of
the sun that is extremely bright. But the entire surface of the
sphere will not appear homogeneously bright. Recall that Mr. Williams'
perceptually based statement was that the UAP looked like "a
large reflective sphereÉ a large ball bearing."
Now consider the visual appearance of a correctly
exposed photograph of the same mirror surface target as above. Given
the proper shutter speed and aperture much the same object detail
will be seen as described above. On the other hand, if the shutter
speed and/or aperture are not adequate to reduce the ultra high
optical power coming from the spherical target what is produced
is a much larger diffuse white area perhaps the same angular size
of the entire sphere itself as is seen in the present photograph.
Yet in the present photograph the sailplane was properly exposed
so the shutter speed and aperture had to be approximately correct
for these nominal conditions. The over-exposed UAP had to result
only from its excessive output of optical power. It is likely that
this is what occurred in the present case as well as in the earlier
Childerhose case.
Now consider a sunlit sphere in the sky whose
surface is not mirror but diffusely reflecting, like white chalk.
It will appear both to the naked eye and on a photograph as an almost
flat surfaced object, i.e., its third dimension will be significantly
reduced. Its round edge will correspond with its angular diameter.
Each point on its surface will radiate light toward the eye and
camera. The difference between sunlit a mirror surface and a diffuse
surface sphere is immediately discernable and will not be confused.
Another possibility in one or both aerial sightings
is that the film may have undergone some poorly understood type
of direct irradiation effect,9 perhaps due to non-visible (near
infra-red?) wavelengths from the source. Further research is called
for to find out if this is possible.
Spectral Sensitivity Aspects. Another issue
is the degree to which Kodak ASA100 color film faithfully captures
the same target wavelengths as does the normal human visual system.
In fact, there has been shown to be a relatively good correspondence
in this regard (cf. Kodak, 1997). Indeed, if this were not the case
such film would not be sold as consistently as it is. People would
not continue to purchase film that did not capture the same hues
and contrasts as exist the perceived scene. At the shorter wavelength
end of the spectrum of Kodak 5026 the yellow-forming layer's spectral
sensitivity curve extends down to 400 nm while the normal visual
sensitivity falls off to virtually nothing at 395 nm. (Prince, 1962).
Much the same correspondence is found at the longer wavelength end
of the spectrum as well where the (cyan -forming layer) of the emulsion
is sensitive out to 690 nm which is just under the 730 nm cut-off
of the normal eye. Thus, the eye can see slightly farther into the
near infrared than can this particular film stock.
What is the possibility that this UAP emitted
non-visible radiation that affected the film?
There is no known published research on this
important matter. Further research should be conducted to evaluate
such a possibility, particularly microwave wavelengths in the 1mm
to 1cm wavelength range.
(2) The Issue of Negative Originality. Of course
it is important to study the original negative of an alleged UAP
or other claimed anomaly whenever possible (Louange, 1999) unless
it has been lost and a high quality copy, unaltered negative has
been made. As mentioned earlier, it appears that the negative that
the author received was not original but a copy. In addition, of
the three frame negative strip received, the UAP was imaged on frame
3A with no exposures on frame 4A or 5A. When Williams was asked
about this discrepancy (on March 9, 2001) he said he thought it
was original "as far as I know." Whether or not this fact
seriously impacts the value of the entire case rests on the personal
motives and credibility of the primary witness. The only other two
people who handled the film were the photographer and the technician
at the one-hour film developing shop on Convoy Street in San Diego.
Since the photographer did not remove the film from the witness's
camera but simply handed it all to Williams upon landing it removes
him from suspicion. It isn't known whether the copy negative was
made by the technician. He had it for a full week according to Williams
who further recalls that he did receive a full roll of negatives
back but can't be sure if they were his originals.
Consider the following: (1) Mr. Williams did
nothing with the negative for 11.5 years as far as can be determined
other than having two enlargements made - one of which he submitted
to the author for study and the other for his office wall, (2) It
is possible that the photographer had loaded a second roll of film
and then stopped taking photos immediately after the UAP passed
by. Williams though that they all headed back to land very soon
after the sighting. (3) When the author visited him in his home-office
located NW of Seattle, Washington it was noticed that (a) he was
a former Naval officer, (b) There was no indication that he had
any kind of an interest in ufo or anything occult, (c) At no time
did he become defensive or belligerent about the apparent discrepancy
surrounding the copy negative; he merely shrugged it off as something
of no great importance. At no time did he contradict himself or
give facts that were later found to be in error, and (d) He is well
educated, a respected member of the community, and now a salesman
of high technology, non-destructive testing hardware and is very
precise in his vocabulary and knowledge of flying. All of these
facts tend to support the contention that Williams is a trustworthy
individual despite the fact that the negative analyzed probably
was not original. Of course, theoretically, overall case reliability
is lessened because of this fact.
(3) Other Issues. A check was made to determine
whether other UAP reports had been made at this time, date, and
location. No reports to the National UFO Reporting Center (Seattle,
Washington) were found other than Mr. Williams' own abbreviated
report submitted on January 10, 2000. It may be important to note
that Mr. Williams did not include the day of the month of the incident
in his report to NUFORC. He had to locate this date in his flight
log book for them later. There also were no sighting reports found
in the national data base maintained by Hatch (2001). A check was
also made with an international astronomical clearing house in Czechoslovakia
regarding meteorite and bolide sightings; none were reported by
astronomers for this time and location.
Preliminary Conclusions
A number of tentative conclusions are offered
as a result of this investigation: (1) There is no firm evidence
of a double exposure or other deliberate hoax despite the fact that
the pilot probably did not submit the original negative. (2) Whatever
the UAP was it was most likely in sub-sonic flight, as suggested
by visual characteristics of turbulence within the tail behind the
UAP's head, the lack of a visible bow-wave effect, and the fact
that no sonic boom was heard. (3) If the UAP was moving at sub-sonic
speed then either the estimated sighting duration was too short,
the distance to the UAP too great, the angle that the UAP appeared
to travel through was in error, or some combination of them all.
It isn't possible to determine which of these estimate(s) are in
error. (4) The UAP's visual appearance did not match the appearance
of the photograph, a finding that parallels an earlier aerial photographic
case. This difference may be because the total optical power of
the UAP was so great as to completely saturate the relatively "slow"
film. Indeed, even with extreme computer "stretching"
of the highly exposed area it wasnÕt possible to locate any
significant detail within the central core of the 'white' head.
(5) The diminution of the albedo of the UAPÕs tail with increased
distance behind its leading edge is not consistent with sunlight
reflected off of water vapor at these angles. It is as if the particles
possessed directional reflectivity or some other non-mundane characteristic.
(6) Very fine micro-structure details were discovered that extended
outward from the "head" of the UAP. The nature of the
UAP has not been identified as of this date.
References
Allard, E., Memoire sur l'Intensite' et la Portee
des Phares. Dunod, Paris, 1876.
Childerhose, R. J., Montreal Star, November
13, 1966.
Gillmor, D. S., (Ed.), Scientific Study of Unidentified
Flying Objects. Bantam Books, New York, 1968.
Haines, R. F., The effects of high luminance
sources upon the visibility of point sources. Adv.
in the Astronautical Sciences, vol. 20, Pp. 887-896, 1965.
Haines, R. F., and S. H. Bartley, A study of
certain visual effects occasioned by factors of so-called glare.
J. of Psychology, vol. 62, Pp. 255-266, 1966.
Haines, R. F., and W. H. Allen, Irradiation
and manual navigation. Navigation, vol. 15, no. 4, Pp. 355-365,
1968.
Haines, R. F., Changes in perceived size of
high luminance targets. Aerospace Medicine, vol. 40, Pp. 754-758,
1969.
Haines, R. F., The retinal threshold gradient
in the presence of a high luminance target and in total darkness.
Perception and Psychophysics, vol. 9, no. 2B, Pp. 197-202, 1971.
Haines, R. F., Observing UFOs. Nelson-Hall,
Chicago, 1980.
Hatch, L., "U", http://www.larryhatch.net,
2001.
Klass, P. J., UFOs Identified. Random House,
New York, 1968.
Koschmieder, H., Theorie der Horizontalen Sichtweite.
Beitraege zur Physik der Atmos - phare, vol. 12, Pp. 33-53, 171-181,
1924.
Kodak, Professional Video Analyzing Computer
PVAC XL CCD Series 6 with Modification 2. Report CCPR10e, Technical
Information Data Sheet, Rev. 11-97 http://www.Kodak.com/global/en/professional/support/techPubs/e26.shtml
Louange, F., Procedures for analysis of photographic
evidence, Chpt. 21 In Sturrock, P. A., The UFO Enigma. Warner Books,
Inc., New York, 1999.
Maccabee, B., Optical power output of an unidentified
high altitude light source. J. Sci. Exploration, vol. 13, no. 2,
Pp. 199-211, 1999.
McCampbell, J. M., Ufology: New insights from
science and common sense. Jaymac Co., Belmont, Calif., 1973.
Prince, J. H., Spectral absorption of the retina
and choroid. The Ohio State University Institute for Research in
Vision, Columbus, Ohio, Publ. No. 14, March 1962. (Also cf. Haines,
1980, Pg. 119)
Shepard, R. N., Reconstruction of witnessesÕ
experiences of anomalous phenomena. Chpt. 10
In Haines, R.F., (Ed.), UFO Phenomena and the Behavioral Scientist.
The Scarecrow
Press, 1979.
Smith, B. E., Ames Research Center-NASA, Personal
communication, April 4, 2001.
1 Since this case did not involve aviation safety
the author investigated it independently from his duties as
Chief Scientist for NARCAP. Nevertheless, it is included as a NARCAP
Topical Report for the benefit
of those who may be interested in it.
2 The Mini-Nimbus/C sail plane has a gross weight
of 480 pounds and a glide ratio of about 44:1.
3 Ryan airport, Hemet, California, is 1,512
feet MSL with a runway length of 4,300 feet and right-hand
pattern. It is used extensively by soaring pilots and hosted almost
a hundred such aircraft at the time.
4 The Mooney M20C was FAA certified in September
1976 and is all metal construction. It holds four
passengers and boasts a 200 hp, flat four cylinder engine. Its high
maneuverability and (low wing) visibility
makes it an ideal candidate as a photographic chase plane. During
this flight its flaps were fully extended in
order to slow to the same speed as the sail plane (approx. 120 kts.).
5 Mr. Williams claims to possess these other
frames although he could not find all of them as of September 1,
2001.
He landed at between 1445 and 1500 hrs.
6 It isn't known if the tow plane pilot saw
the UAP. No effort was made to find out at the time.
7 Is it likely that a copy negative was made
at this point? If so, for what purpose? The author received the
additional five frames from this roll on August 12, 2001. Since
Williams did not take the photos he wasn't sure of their order on
the film.
8 The radius of turn for these conditions =
2,944 feet given by R = v2/(tan theta x g) where: R = turn radius,
theta = bank angle (deg.), and g = 32.2 deg/sec2. Mr. Williams estimated
(later, March 9, 2001) his bank
angle to be from ten to fifteen degrees.
9 Irradiation refers to a lateral spread of
light exposure on the film beyond the edge of the brighter target.
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