Soho Image Anomalies - Analysis 1

The Evidence IIThe Evidence II
Analysis of SOHO images andAnalysis of SOHO images and
other sourcesother sources
- compiled by „Nobody“ * -- compiled by „Nobody“ * -
2007/05/01(update: 2007/06/04)2007/05/01(update: 2007/06/04)
*Movie: Terence Hill / Henry Fonda*Movie: Terence Hill / Henry Fonda

IntroductionIntroduction
 analysis based on originalanalysis based on original NASANASA data files fromdata files from SOHOSOHO
near real time data archive and science archive:near real time data archive and science archive:
 ~ 15,000+ C2/C3 images visual check~ 15,000+ C2/C3 images visual check
 ~ 1,000+ C2/C3 images filtered (5-10 filters)~ 1,000+ C2/C3 images filtered (5-10 filters)
 random selection & filtering of 2006 C2/C3 archiverandom selection & filtering of 2006 C2/C3 archive
(~ 2,000 – 3,000 images)(~ 2,000 – 3,000 images)
 manual check of ~ 500 – 1,000 FITS filesmanual check of ~ 500 – 1,000 FITS files
 manual check of ~ 1,000+ EIT/EUV imagesmanual check of ~ 1,000+ EIT/EUV images
 image download & analysis from differentimage download & analysis from different
web pagesweb pages
 analysis of the available SOHO & instrument papersanalysis of the available SOHO & instrument papers
 NASA can‘t fake up to 240 LASCO imagesNASA can‘t fake up to 240 LASCO images
per day transmitted by SOHO!per day transmitted by SOHO!

Excursion: Visible spectrumExcursion: Visible spectrum
 Visible spectrumVisible spectrum
 From Wikipedia, the free encyclopediaFrom Wikipedia, the free encyclopedia
 source:source: http://en.wikipedia.org/wiki/Visible_lighthttp://en.wikipedia.org/wiki/Visible_light
 TheThe visible spectrumvisible spectrum (or sometimes(or sometimes optical spectrumoptical spectrum) is the portion of the electromagnetic spectrum that is) is the portion of the electromagnetic spectrum that is
visible to (can be detected by) the human eye. Electromagnetic radiation in this range of wavelengths is calledvisible to (can be detected by) the human eye. Electromagnetic radiation in this range of wavelengths is called
visible lightvisible light or simply light. There are no exact bounds to the visible spectrum; a typical human eye will respondor simply light. There are no exact bounds to the visible spectrum; a typical human eye will respond
to wavelengths in air from 400 to 700 nm, although some people may be able to perceive wavelengths from 380to wavelengths in air from 400 to 700 nm, although some people may be able to perceive wavelengths from 380
to 780 nm. The corresponding wavelengths in water and other media are reduced by a factor equal to theto 780 nm. The corresponding wavelengths in water and other media are reduced by a factor equal to the
refractive index. In terms of frequency, this corresponds to a band in the vicinity of 450-750 terahertz. A light-refractive index. In terms of frequency, this corresponds to a band in the vicinity of 450-750 terahertz. A light-
adapted eye typically has its maximum sensitivity at around 555 nm, in the green region of the optical spectrumadapted eye typically has its maximum sensitivity at around 555 nm, in the green region of the optical spectrum
(see: luminosity function). The spectrum does not, however, contain all the colors that the human eyes and brain(see: luminosity function). The spectrum does not, however, contain all the colors that the human eyes and brain
can distinguish. Brown, pink, and magenta are absent, for example, because they need a mix of multiplecan distinguish. Brown, pink, and magenta are absent, for example, because they need a mix of multiple
wavelengths.wavelengths.
 Wavelengths visible to the eye also pass through the "optical window", the region of the electromagnetic spectrumWavelengths visible to the eye also pass through the "optical window", the region of the electromagnetic spectrum
which passes largely unattenuated through the Earth's atmosphere (although blue light is scattered more than redwhich passes largely unattenuated through the Earth's atmosphere (although blue light is scattered more than red
light, which is the reason the sky is blue). The response of the human eye is defined by subjective testing (seelight, which is the reason the sky is blue). The response of the human eye is defined by subjective testing (see
CIE), but the atmospheric windows are defined by physical measurement. The "visible window" is so calledCIE), but the atmospheric windows are defined by physical measurement. The "visible window" is so called
because it overlaps the human visible response spectrum; the near infrared (NIR) windows lie just out of humanbecause it overlaps the human visible response spectrum; the near infrared (NIR) windows lie just out of human
response window, and the Medium Wavelength IR (MWIR) and Long Wavelength or Far Infrared (LWIR or FIR)response window, and the Medium Wavelength IR (MWIR) and Long Wavelength or Far Infrared (LWIR or FIR)
are far beyond the human response region.are far beyond the human response region.
 The eyes of many species perceive wavelengths different from the spectrum visible to the human eye. ForThe eyes of many species perceive wavelengths different from the spectrum visible to the human eye. For
example, many insects, such as bees, can see light in the ultraviolet, which is useful for finding nectar in flowers.example, many insects, such as bees, can see light in the ultraviolet, which is useful for finding nectar in flowers.
For this reason, plant species whose life cycles are linked to insect pollination may owe their reproductive successFor this reason, plant species whose life cycles are linked to insect pollination may owe their reproductive success
to their appearance in ultraviolet light, rather than how colorful they appear to our eyes.to their appearance in ultraviolet light, rather than how colorful they appear to our eyes.

Excursion: CCD technologyExcursion: CCD technology
 http://http://en.wikipedia.org/wiki/CCD_cameraen.wikipedia.org/wiki/CCD_camera
 CCDs are typically sensitive to infrared light, which allows infrared photography, night-vision devices, and zero luxCCDs are typically sensitive to infrared light, which allows infrared photography, night-vision devices, and zero lux
(or near zero lux) video-recording/photography. Because of their sensitivity to infrared, CCDs used in astronomy(or near zero lux) video-recording/photography. Because of their sensitivity to infrared, CCDs used in astronomy
are usually cooled to liquid nitrogen temperatures, because infrared black body radiation is emitted from room-are usually cooled to liquid nitrogen temperatures, because infrared black body radiation is emitted from room-
temperature sources. One other consequence of their sensitivity to infrared is that infrared from remote controlstemperature sources. One other consequence of their sensitivity to infrared is that infrared from remote controls
will often appear on CCD-based digital cameras or camcorders if they don't have infrared blockers. Cooling alsowill often appear on CCD-based digital cameras or camcorders if they don't have infrared blockers. Cooling also
reduces the array's dark current, improving the sensitivity of the CCD to low light intensities, even for ultravioletreduces the array's dark current, improving the sensitivity of the CCD to low light intensities, even for ultraviolet
and visible wavelengths.and visible wavelengths.
 Thermal noise, dark current, and cosmic rays may alter the pixels in the CCD array. To counter such effects,Thermal noise, dark current, and cosmic rays may alter the pixels in the CCD array. To counter such effects,
astronomers take an average of several exposures with the CCD shutter closed and opened. The average ofastronomers take an average of several exposures with the CCD shutter closed and opened. The average of
images taken with the shutter closed is necessary to lower the random noise. Once developed, the “dark frame”images taken with the shutter closed is necessary to lower the random noise. Once developed, the “dark frame”
average image is then subtracted from the open-shutter image to remove the dark current and other systematicaverage image is then subtracted from the open-shutter image to remove the dark current and other systematic
defects in the CCD (dead pixels, hot pixels, etc.).defects in the CCD (dead pixels, hot pixels, etc.).
 CCD cameras used in astrophotography often require very sturdy mounts to cope with vibrations and breezes,CCD cameras used in astrophotography often require very sturdy mounts to cope with vibrations and breezes,
along with the tremendous weight of most imaging platforms. To take long exposures of galaxies and nebulae,along with the tremendous weight of most imaging platforms. To take long exposures of galaxies and nebulae,
many astronomers use a technique known as auto-guiding. Most autoguiders use a second CCD chip to monitormany astronomers use a technique known as auto-guiding. Most autoguiders use a second CCD chip to monitor
deviations during imaging. This chip can rapidly detect errors in tracking and command the mount's motors todeviations during imaging. This chip can rapidly detect errors in tracking and command the mount's motors to
correct for them.correct for them.

Excursion: CCD vs. human eyeExcursion: CCD vs. human eye
There are no exact bounds to the visible spectrum;There are no exact bounds to the visible spectrum;
a typical human eye will respond to wavelengthsa typical human eye will respond to wavelengths
in air from 400 to 700 nmin air from 400 to 700 nm
CCD sensors additionally cover IR and
UV/EUV spectrum – range can be extended
with special filters or coatings of the sensor

Excursion: SolarizationExcursion: Solarization
Legend:
γ = Gamma rays
HX = Hard X-rays
SX = Soft X-Rays
EUV = Extreme ultraviolet
NUV = Near ultraviolet
Visible light
NIR = Near infrared
MIR = Moderate infrared
FIR = Far infrared
Radio waves:
EHF = Extremely high frequency (Microwaves)
SHF = Super high frequency (Microwaves)
UHF = Ultrahigh frequency
VHF = Very high frequency
HF = High frequency
MF = Medium frequency
LF = Low frequency
VLF = Very low frequency
VF = Voice frequency
ELF = Extremely low frequency
http://en.wikipedia.org/wiki/Solarisation
- Solarisation is a phenomenon in photography in which the image
recorded on a negative or on a photographic print is wholly or partially
reversed in tone. Dark areas appear light and vice versa
- Solarization refers to a phenomenon in physics where a material
undergoes a temporary change in color after being subjected to high
energy electromagnetic radiation, such as ultraviolet light or X-rays

Excursion: CCD basicsExcursion: CCD basics
“…In order for a continuous-tone or analog image to be processed or displayed by a computer, it must first be converted into
a computer-readable form or digital format. This process applies to all images, regardless the origin and complexity, and
whether they exist as black and white (grayscale) or full color. To convert a continuous-tone image into a digital format,
the analog image is divided into individual brightness values through two operational processes that are termed
sampling and quantization. After sampling in a two-dimensional array, brightness levels at specific locations in the analog
image are recorded and subsequently converted into integers during the process of quantization. The target objective is to
convert the image into an array of discrete points that each contain specific information about brightness or tonal range and
can be described by a specific digital data value in a precise location. The sampling process measures the intensity at
successive locations in the image and forms a two-dimensional array of intensity information. After sampling is completed,
the resulting data is quantized to assign a specific digital brightness value to each sampled data point, ranging from black,
through all of the intermediate gray levels, to white. The result is a numerical representation of the intensity, which is
commonly referred to as a picture element or pixel, for each sampled data point in the array.
array of
intensity values
(digital)
CCD = array of photo elements
brightness
values
(analog)
incoming
photons
1
2
3

Excursion: CCD – how toExcursion: CCD – how to
prevent blooming Iprevent blooming I
„Laterial Overflow Drain to Prevent Blooming“
Keep this in mind…
source: http://micro.magnet.fsu.edu/primer/digitalimaging/concepts/ccdsatandblooming.html
„…Saturation and blooming are related phenomena that occur
in all charge-coupled device (CCD) image sensors under
conditions in which either the finite charge capacity of individual
photodiodes, or the maximum charge transfer capacity of the
CCD, is reached. Once saturation occurs at a charge collection
site, accumulation of additional photo-generated charge results in
overflow, or blooming, of the excess electrons into adjacent
device structures. A number of potentially undesirable effects of
blooming may be reflected in the sensor output, ranging from
white image streaks and erroneous pixel signal values (as
illustrated in Figure 1) to complete breakdown at the output
amplification stage, producing a dark image…“
how can this be?
?

Excursion: CCD – blooming IIExcursion: CCD – blooming II
EIT 304 EUV image (composite).
CCD hit by massive CME and
there is no blooming at all
how can this be?
image copied from web
Filters Unlimited 2.0: gradients filter
IrfanView 4.0: inversion
CCD waffles
?
?
?

Excursion: CCD – blooming IIIExcursion: CCD – blooming III
Source: HAMAMATSU – characteristics
and use of back-thinned TDI-CCDSource: EIT instrument paper

Brilliant UFO Over Byron Bay IBrilliant UFO Over Byron Bay I
(auto) image enhancement
using PSP
Scout ship designed
for flights within planets/earth
atmosphere?3D curved shape
force field
hotsho
t
2007
Source: http://www.rense.com/general76/bril.htm
„the evidence“ because of available details:
propulsion, force field, 3D shape, color, etc.
image shows under-exposure and low contrast
caused by camera processor/software.
Camera: Olympus SP350, 8 mpx

Brilliant UFO Over Byron Bay IIBrilliant UFO Over Byron Bay II
color speckles indicate
energy/wave packets released
by propulsion?
filter: solarization
hotsho
t
2007
cut-out: filter: metallic ice
(IrfanView 4.0)

Brilliant UFO Over Byron Bay IIIBrilliant UFO Over Byron Bay III
force field clearly visible
filter: high-pass
hotsho
t
2007

Brilliant UFO Over Byron Bay IVBrilliant UFO Over Byron Bay IV
inversion of the image shows
force field/shape
filter: inversion
hotsho
t
2007

Silver Disc In DaylightSilver Disc In Daylight
Videotaped Over Venice, CAVideotaped Over Venice, CA II
http://www.rense.com/general53/silverff.htm
image copied from rense.com,
controversial discussion on UFO
vs. balloon
I/R filter applied with PSP,
do bright areas indicate high
energy state?

Silver Disc In DaylightSilver Disc In Daylight
Videotaped Over Venice, CAVideotaped Over Venice, CA IIII
solarization filter applied with PSP, color speckles indicate high
energy state/high frequency?
http://www.rense.com/general53/silverff.htm

UFO‘s Over Brisbane/AUSUFO‘s Over Brisbane/AUS
- analysis of video stills -- analysis of video stills -
color speckles may indicate energy/wave packets released
by propulsion?
Step1: images copied from Web (credits to Australia )
Step2: auto image enhancement (PSP)
Step3: filter: solarization (PSP)
Camera: single chip PANASONIC
hotshot
s
2003

Soho Image Anomalies - Analysis 1

SOHO: Useful linksSOHO: Useful links
 SOHO Home:SOHO Home:
http://http://sohowww.nascom.nasa.govsohowww.nascom.nasa.gov//
 SOHO search tool for near real time data:SOHO search tool for near real time data:
http://sohowww.nascom.nasa.gov/cgi-bin/realtime_queryhttp://sohowww.nascom.nasa.gov/cgi-bin/realtime_query
 SOHO archive search (FITS files):SOHO archive search (FITS files):
http://sohodata.nascom.nasa.gov/cgi-bin/guihttp://sohodata.nascom.nasa.gov/cgi-bin/gui
 SOHO instruments explained:SOHO instruments explained:
http://sohowww.nascom.nasa.gov/data/realtime/image-description.htmlhttp://sohowww.nascom.nasa.gov/data/realtime/image-description.html
 LASCO home page:LASCO home page:
http://lasco-www.nrl.navy.milhttp://lasco-www.nrl.navy.mil//
 LASCO “debris list”:LASCO “debris list”:
http://lasco-www.nrl.navy.mil/index.php?phttp://lasco-www.nrl.navy.mil/index.php?p=content/debris=content/debris
http://lasco-www.nrl.navy.mil/debris_gifhttp://lasco-www.nrl.navy.mil/debris_gif//
 SOHO comets – “common mistakes”:SOHO comets – “common mistakes”:
http://http://ares.nrl.navy.mil/sungrazer/index.php?pares.nrl.navy.mil/sungrazer/index.php?p==cometformcometform

Excursion: CCD manufacturerExcursion: CCD manufacturer
“…CCD…fabricated by Scientific Imaging Technologies Inc. (SITe,
formerly a group within Tektronix)…”
LASCO
instruments
= custom
CCD
EIT (EUV)
instruments
= custom
CCD
EIT LASCO

Excursion: EIT: Extreme-UVExcursion: EIT: Extreme-UV
imaging telescopeimaging telescope
2.3 CCD Image Sensor (source: EIT instrument paper)
The CCD used to record the images is a thinned, back-illuminated device fabricated by Scientific Imaging Technologies Inc.
(SITe, formerly a group within Tektronix). The back surface has been processed to provide a high and stable EUV
quantum efficiency (Moses, et al. 1993). The CCD is a 1024 x 1024 array of 21 µm square pixels with gate implants to
provide Multi-Pinned Phase (MPP) operation. This provides lower thermally generated dark current and improves the
radiation hardness of the CCD. There are four readout ports, at the corners of the image array, with only one used at any
time. The full-well capacity of a pixel is about 150,000 electrons and the charge transfer efficiency of the device is about
0.99995. The CCD is mounted in a special ceramic package with provision to position its surface accurately and reproducibly
in the EIT focal plane. The CCD is cooled by passively radiating to deep space and the temperature is regulated at about -80
C by a small heater. This heater may be used with an additional higher wattage heater to warm the CCD above ambient
temperature in order to evaporate any condensates that may have formed on its surface and that could degrade its EUV
quantum efficiency. A temperature sensor is located on the ceramic package and another is present on the CCD itself.

Excursion: C2 coronagraphExcursion: C2 coronagraph
Source: LASCO instrument paper

Excursion: C3 coronagraphExcursion: C3 coronagraph

Excursion: LASCO exposureExcursion: LASCO exposure
timestimes

Excursion: LASCO C2/C3 IExcursion: LASCO C2/C3 I
 (Large Angle Spectrometric Coronagraph) is able to take images of the solar corona by blocking the light coming(Large Angle Spectrometric Coronagraph) is able to take images of the solar corona by blocking the light coming
directly from the Sun with an occulter disk, creating an artificial eclipse within the instrument itself. The position ofdirectly from the Sun with an occulter disk, creating an artificial eclipse within the instrument itself. The position of
the solar disk is indicated in the images by the white circle. The most prominent feature of the corona are usuallythe solar disk is indicated in the images by the white circle. The most prominent feature of the corona are usually
the coronal streamers, those nearly radial bands that can be seen both in C2 and C3. Occasionally, a coronalthe coronal streamers, those nearly radial bands that can be seen both in C2 and C3. Occasionally, a coronal
mass ejection can be seen being expelled away from the Sun and crossing the fields of view of bothmass ejection can be seen being expelled away from the Sun and crossing the fields of view of both
coronagraphs. The shadow crossing from the lower left corner to the center of the image is the support for thecoronagraphs. The shadow crossing from the lower left corner to the center of the image is the support for the
occulter disk.occulter disk.
 C2 imagesC2 images show the inner solar coronashow the inner solar corona up to 8.4 million kilometers (5.25 million miles)up to 8.4 million kilometers (5.25 million miles) away from the Sun.away from the Sun.
 C3 imagesC3 images have a larger field of view: They encompass 32 diameters of the Sun. To put this in perspective, thehave a larger field of view: They encompass 32 diameters of the Sun. To put this in perspective, the
diameter of the images isdiameter of the images is 45 million kilometers (about 30 million miles)45 million kilometers (about 30 million miles) at the distance of the Sun, or half ofat the distance of the Sun, or half of
the diameter of the orbit of Mercury. Many bright stars can be seen behind the Sun.the diameter of the orbit of Mercury. Many bright stars can be seen behind the Sun.

Excursion: LASCO C2/C3 IIExcursion: LASCO C2/C3 II
LASCO C2 = tele lens
field of view = ~ 8.4 million kilometers,
~ 6 x sun size (1.4 million KM)
LASCO C3 = wide angle lens (+/- 8º)
field of view = ~ 45 million kilometers
object “fires” 3 beams object “fires” 2 beams,
details cut-out
cut-out: 1024 x 1024 / 8 BPP ->
4096 x 4096 / 150 dpi -> zoom ->
filter: metallic ice (IrfanView 4.0)
cut-out: 1024 x 1024 / 8 BPP -> 4096
x 4096 / 150 dpi -> zoom -> filter:
gradients (Filters Unlimited 2.0)

Excursion: EIT IExcursion: EIT I
 EITEIT (Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore,(Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore,
shows solar material at different temperatures. In the images taken at 304 Angstroms the bright material is atshows solar material at different temperatures. In the images taken at 304 Angstroms the bright material is at
60,000 to 80,000 degrees Kelvin. In those taken at 171, at 1 million degrees. 195 Angstrom images correspond to60,000 to 80,000 degrees Kelvin. In those taken at 171, at 1 million degrees. 195 Angstrom images correspond to
about 1.5 million Kelvin. 284 Angstrom, to 2 million degrees. The hotter the temperature, the higher you look inabout 1.5 million Kelvin. 284 Angstrom, to 2 million degrees. The hotter the temperature, the higher you look in
the solar atmosphere.the solar atmosphere.
Source: EIT instrument paper

Excursion: EIT IIExcursion: EIT II
massive ejection of energy flooding
the CCD sensor - no blooming!
massive ejection of energy from the sun –
what happens in the covered (make up)
area?
CCD waffles NASA whistle-blowers
tell us the truth - picture
shown is composite of
EIT & LASCO images!
make-up done
by NASA operator.
We can prove this
because of reduced
GIF file size
typical EIT (EUV) image
LASCO: solid occulter disk & pylon

Excursion: Hints – how to get…Excursion: Hints – how to get…
 Step 1: always download the complete C2/C3 archives from the SOHO WEBStep 1: always download the complete C2/C3 archives from the SOHO WEB
 Step 2: do manual inspection of the images with slideshow tool (Step 2: do manual inspection of the images with slideshow tool (www.irfanview.comwww.irfanview.com). Irfanview allows to go step-). Irfanview allows to go step-
by-step through the unpacked archives using the keyboard (page-up / page-down keys)by-step through the unpacked archives using the keyboard (page-up / page-down keys)
 Step 3: start slideshow manually by holding page-up or page-down key (slow motion forward or reverse)Step 3: start slideshow manually by holding page-up or page-down key (slow motion forward or reverse)
 Step 4: download MPEG videos of the current day from the archive (sometimes they leave breathtaking materialStep 4: download MPEG videos of the current day from the archive (sometimes they leave breathtaking material
inin
the MPEG videos which is sorted out of the standard C2/C3 archives)the MPEG videos which is sorted out of the standard C2/C3 archives)
 Step 5: variable zoom of the individual C2/C3 images to check for details (Paint Shop Pro XI, etc.)Step 5: variable zoom of the individual C2/C3 images to check for details (Paint Shop Pro XI, etc.)
 Step 6: apply different filters to the images and have the truth coming out (do not mix filters):Step 6: apply different filters to the images and have the truth coming out (do not mix filters):
 inversion/negativeinversion/negative
 infraredinfrared
 solarizationsolarization
 edge filtersedge filters
 high-passhigh-pass
 additional steps to gain confidence what you see:additional steps to gain confidence what you see:
 download C2/C3 archives from year 2006 with the near time data search tool. Do random selection of the archivesdownload C2/C3 archives from year 2006 with the near time data search tool. Do random selection of the archives
 check the science archive for older FITS files (original LASCO C2/C3 data files)check the science archive for older FITS files (original LASCO C2/C3 data files)
 ThumbsPlus 7.x can read FITS files used by NASA. FITS file format is common file format used in astronomyThumbsPlus 7.x can read FITS files used by NASA. FITS file format is common file format used in astronomy
 recommendation: make screenshots of SOHO home page/MPEG archive/C2 archive/C3 archive to document therecommendation: make screenshots of SOHO home page/MPEG archive/C2 archive/C3 archive to document the
cover-up activities. C2/C3 archives vary in size nearly every day. Sometimes the archive size growths by intentioncover-up activities. C2/C3 archives vary in size nearly every day. Sometimes the archive size growths by intention

Excursion: Images (size per day)Excursion: Images (size per day)
LASCO: “…high volume
memories and a high-
speed microprocessor
enable extensive on-board
image processing. Image
compression by a factor of
about 10 will result in the
transmission of 10 full
images per hour…”
Source: LASCO instrument
paper.

Excursion: FITS filesExcursion: FITS files
FITS header keywords:
NASA has got all details…
22240839.FTS, 2006/11/26, 00:12:04,
LASCO C2, orange
FTS -> TIF 150 dpi (1024 x 1024 / 8 BPP)
-> 8192 x 8192 / 150 dpi -> zoom ->
filter: gradients (Filters Unlimited 2.0)
LASCO C2, 2006/01/23, 02:06
Corel Photo Paint X3:
8192 x 8192 /150 dpi,
filter: relief

Excursion: NASA at it‘s bestExcursion: NASA at it‘s best
copied from document „LASCO early
results“
LASCO C2: solid
occulter disk
FTS -> TIF 150 dpi (1024 x 1024 / 8 BPP)
-> 8192 x 8192 / 150 dpi -> zoom ->

Excursion: LASCO debris list IExcursion: LASCO debris list I
- Image retrieved from LASCO debris list: http://lasco-www.nrl.navy.mil/debris_gif/
- Why does NASA only provide b/w images in this directory?
- Image on the right side has been re-worked by NASA with distortion filters
- Psychology being used to fool our consciousness (ambiguity) therefore the image
on the right side is used to have the intended effect in place (what I see can’t be true)
massive appearance of “objects”
image re-worked by NASA
with distortion filters!
?
?
?
(NASA) Explanatory note: “…The images….on the right are so-
called "running difference" images, showing the difference in
brightness from one observation to another. This brings out more
contrast, highlighting the coronal mass ejections, but also
introduces some artifacts. Most notably, most of the dark areas
are not really "dark", they have just dimmed since the last image
(or a bright spot may have moved from one place to another)…”
http://sohowww.nascom.nasa.gov/hotshots/2000_02_17/

Excursion: LASCO debris list IIExcursion: LASCO debris list II
GIF taken from debris list -> filter: gradients (Filters Unlimited 2.0)
“the fake” - ©NASA“the truth” - ©Nobody

Excursion: LASCO debris list IIIExcursion: LASCO debris list III
the most beautiful debris seen so far 
gateway into other dimension?
(NASA) Explanatory note: “…The images….on the right are so-
called "running difference" images, showing the difference in
brightness from one observation to another. This brings out more
contrast, highlighting the coronal mass ejections, but also
introduces some artifacts. Most notably, most of the dark areas
are not really "dark", they have just dimmed since the last image
(or a bright spot may have moved from one place to another)…”

Excursion: How to create debrisExcursion: How to create debris
original GIF-image from SOHO web apply any distortion or effect filter you like!
ambiguity: what‘s real? – confusion when these images presented side-by-side
welcome to 22nd ++
century!

NASA: Monkey business 1NASA: Monkey business 1
SOHO 2003 hotshots ISOHO 2003 hotshots I
 NASA‘s attempt to teach us like chimpanzee:
http://sohowww.nascom.nasa.gov/hotshots/2003.html
(extract from SOHO hotshots)
 these pages are designed by special purpose. They help NASA
not to give correct answers to nasty questions they receive
 “How to make your own UFO” = misinformation !
NASA forgot to make-up
this EUV image and people started
to ask the right questions!

SOHO 2003 hotshots IISOHO 2003 hotshots II
 NASA‘s attempt to teach us like chimpanzee:
(extract from SOHO hotshots)
 these pages are designed by special purpose.
They help NASA not to give correct answers to
nasty questions they receive
 “How to make your own UFO” = misinformation!
 Original: Visual inspection of the
highlighted area tells the truth already!
 Step1: why did they modify the color scaling?
 Step2: which interpolation method has been
used out of the zillion possible methods?
 Step3: how did they touch-up the color table?
 conclusion:
- this EUV image has been re-touched by intention
 filters used: softener, interpolation filters

SOHO 2003 hotshots IIISOHO 2003 hotshots III
 (A.D. Johnson) SOHO UFOs Manipulated?
http://www.rense.com/general62/manip.htm
 this gentlemen posted an article to rense.com
discussing the NASA hotshot and the attempt
to make-up the image
 he delivered a proof further down in the same page
but didn‘t analyze the image in detail
 object „firing“ two beams into the sun.
Sun releases G-waves
 image zoomed +300% with PSP
(JPG downloaded from rense.com). Cut-out
done with Screenshot Pilot

SOHO 2000 hotshotsSOHO 2000 hotshots

“riders in the (particle) storm”“riders in the (particle) storm”
22072507.FTS, 2000/07/14, 11:06:05,
LASCO C2, orange, inverted with PSP
22072517.FTS, 2000/07/14, 18:28:24,
LASCO C2, orange, inverted with PSP
cut-outs: FTS (1024 x 1024 / 8 BPP) -> JPG -> 8192 x 8192 / 150 dpi
-> zoom -> filter: metallic ice (IrfanView 4.0)

SOHO comets – known objectsSOHO comets – known objects
http://ares.nrl.navy.mil/sungrazer/index.php?p=cometform
„The majority of these objects are stars“ –> what about the other ones?
„Stars will always move from left-to-right“ –> please define planets/stars…
„at a speed of a few pixels/hour“ –> Venus sampled = ~ 32 pixels/hour…
„have a nearly horizontal motion“ –> perfect horizontal motion lasting days
NASA: „…saturate the CCD“ – no way!, each CCD pixel
has got a drain to prevent overflow. Bleeding = signature
of propulsion? - caused by exposure time of the images.
“The rings…are not real” – what about Saturn?

SOHO comets “left-or-right”SOHO comets “left-or-right”
“…NASA: Occasionally,
planets appear in LASCO
images and they, too, have
a nearly horizontal motion.
However, planets can
move left or right through
the field-of-view and can be
faster or slower than
the background stars…”
Source:
http://ares.nrl.navy.mil/sungrazer/i
ndex.php?p=cometform
Images have been re-touched with SW tools. Proof point
that SOHO images are composites created from different
instruments. Unpack C3 archive of 2006/11/26 and enjoy
the images with slideshow tool!
cut-out/zoom +150%
http://en.wikipedia.org/wiki/Planet
“…All the planets revolve around the Sun in the
same direction — counter-clockwise as seen from
over the Sun's north pole…” -> oops !
Orbit inclination to ecliptic:
Mercury = 7 deg
Venus = 3,39 deg
Earth = 0,00005 deg
Jupiter = 1,305 deg
Saturn = 2,484 deg

SOHO – “planets vs. stars”SOHO – “planets vs. stars”
The Pleiades, an open cluster of stars
in the constellation of Taurus. NASA photo
NASA: “planets” vs. background stars
http://en.wikipedia.org/wiki/Star
A star is a massive, luminous ball of plasma. Stars group together
to form galaxies, and they dominate the visible universe. The
nearest star to Earth is the Sun, which is the source of most of the
energy on Earth, including daylight. Other stars are visible in the
night sky, when they are not outshone by the Sun. A star shines
because nuclear fusion in its core releases energy which
traverses the star's interior and then radiates into outer
space. Almost all elements heavier than hydrogen and helium
were created inside the cores of stars.
http://en.wikipedia.org/wiki/Planets
A planet, as defined by the International Astronomical
Union (IAU), is a celestial body orbiting a star or stellar
remnant that is massive enough to be rounded by its own
gravity, not massive enough to cause thermonuclear
fusion in its core, and has cleared its neighbouring
region of planetesimals. After stars and stellar remnants,
planets are some of the most massive objects known to
man. They play an important part in the structure of
planetary systems, and are also considered, along with
large moons, the most feasible environment for life

SOHO comets – “archives”SOHO comets – “archives”
why did NASA modify this archive?
CCD data files tell us the truth – watch the
shape of the „objects“. Original FITS file
converted to JPG. Image flipped horizontally.
cut-outs zoomed +500% (1280 x 1024)
“…the brightest planets ever seen…”
@NASA: where does the spotlight
come from?
formation flight of planets , all
“planets” have got rings like Saturn

SOHO comets – “planet biz I”SOHO comets – “planet biz I”
Image converted to JPG, solarization filter,
cut-out/zoom +400%
source: http://www.rense.com/general72/size.htm
Mercury = 7 deg
Venus = 3,39 deg
Earth = 0,00005 deg
Jupiter = 1,305 deg
Saturn = 2,484 deg

SOHO comets – “planet biz II”SOHO comets – “planet biz II”
Celestia 1.4.1: date/time set manually to 2000/05/15, 11:18 UTC - images inverted
LASCO C3 field of view = +/- 8 deg.
Saturn: mean distance from sun =
~1,4 billion km (“out of sight”)
Jupiter: mean distance from sun =
~778 million km (“out of sight”)
Earth: mean distance
from sun = ~150 million km
Venus: mean distance from sun =
~108 million km (“too small”)
Mercury: mean distance from sun =
~58 million km (“too small”)
SOHO maintains an orbit around the Sun, 1.5 million km
(a million miles) from Earth at the Lagrangian point (L1)
Mercury = 7 deg
Venus = 3,39 deg
Earth = 0,00005 deg
Jupiter = 1,305 deg
Saturn = 2,484 deg

SOHO comets – “planet biz III”SOHO comets – “planet biz III”
http://www.jpl.nasa.gov/news/news.cfm?release=2007-055
http://www.nasa.gov/mission_pages/spitzer/multimedia/F-Black-artist.html
NASA: „…This artist's concept illustrates
the hottest planet yet observed in the
universe…” – oops!
?
?
?

SOHO comets – “planet biz IV”SOHO comets – “planet biz IV”
NASA: “…This artist's concept illustrates the hottest planet yet observed in the universe. The scorching ball of gas, a "hot Jupiter" called HD
149026b, is a sweltering 3,700 degrees Fahrenheit (2,040 degrees Celsius) – about 3 times hotter than the rocky surface of Venus,
the hottest planet in our solar system. The planet is so hot that astronomers believe it is absorbing almost all of the heat from its star, and
reflecting very little to no light. Objects that reflect no sunlight are black. Consequently, HD 149026b might be the blackest known planet
in the universe, in addition to the hottest. The temperature of this dark and balmy planet was taken with NASA's Spitzer Space Telescope.
While the planet reflects no visible light, its heat causes it to radiate a little visible and a lot of infrared light. Spitzer, an infrared observatory, was
able to measure this infrared light through a technique called secondary eclipse. HD 149026b is what is known as a transiting planet, which means
that it crosses in front of and passes behind its star – the secondary eclipse – when viewed from Earth. By determining the drop in total infrared
light that occurs when the planet disappears, astronomers can figure out how much infrared light is coming from the planet alone. The Spitzer
observations of HD 149026b also suggest a hot spot in the middle of the side of the planet that always faces its star. Even though the planet is
black, the spot would glow like a black lump of charcoal. HD 149026b is thought to be tidally locked, just as our moon is to Earth, such that one
side of the planet is perpetually baked under the heat of its sun. Astronomers think that HD 149026b is probably blazing hot on its sunlit side, and
much cooler on its dark side. A similar phenomenon was observed previously by Spitzer for the planet Upsilon Andromedae b
(http://www.spitzer.caltech.edu/Media/releases/ssc2006-18/index.shtml). In the case of both planets, heat is not being evenly distributed across
their surfaces. This is the opposite of what happens on Jupiter, where temperature differences are minimal all around…”

SOHO – mission impossible ISOHO – mission impossible I
NASA: „planets…have a nearly horizontal motion“ – how many days?
whistle blowers tell us the truth
1
2
cut-out: GIF (1024 x 1024 / 8 BPP)
-> 8192 x 8192 / 150 dpi -> zoom ->

SOHO – mission impossible IISOHO – mission impossible II
NASA: „planets…have a nearly horizontal motion“ – how many days?
daily business in space,
cover me up!
4
3
cut-out: GIF (1024 x 1024 / 8 BPP)
-> 8192 x 8192 / 150 dpi -> zoom ->

SOHO – “cosmic ray noise”SOHO – “cosmic ray noise”
©NASA: image distorted
with filters…
CCD sensor layout:
1024 x 1024 = ~ 1 million
pixels. “NASA: 3 or 4 hit
the CCD in just the right
places”. Ok, let’s play dart!
NASA: “…completely blind our CCDs with
noise”. CCD’s: Laterial Overflow Drain to
Prevent Blooming…
PSP: FITS b/w image
distorted with filters by
intention to prove how easy
manipulation can be done!

SOHO – “debris streaks”SOHO – “debris streaks”
LASCO C3 = wide angle lens
field of view = ~ 45 million kilometers
NASA image distorted
with filters. Debris streak
~ 26 million kilometers?
FITS image colorized with
IrfanView 4.0 -> filter: metallic ice,
CME and “debris streak” visible!
@NASA: what about the reliability of
your spacecrafts…?
CME
?

SOHO – “objects reported”SOHO – “objects reported”
NASA claims:
-> we are inexperienced observers…
-> have a chat in Yahoo newsgroups
-> consult a student in astronomy, he
will tell you the “truth” about comets…
-> avoid the “common mistakes by
using the resources described here…

bureaucracy @NASAbureaucracy @NASA
filling this form is helpful for NASA to clean the science archive!
C2 / C3 archives often vary in size. FITS archives also modified by NASA.
This can be proven because FITS meta-data included in the FTS data files
and the date of the ZIP archives do not correlate on certain days!
source: http://ares.nrl.navy.mil/sungrazer/index.php?p=cometform

# LASCO C2 / C3 images# LASCO C2 / C3 imagesJanuary 2007 February 2007 March 2007 April 2007 May 2007
# C2 images # C3 images # C2 images # C3 images # C2 images # C3 images # C2 images # C3 images # C2 images # C3 images
1 40 42 62 40 7 5 62 41 65 43
2 32 21 67 43 42 17 65 42 66 42
3 41 28 55 37 36 15 67 42 65 42
4 44 24 61 42 117 47 66 42 64 41
5 44 30 62 39 75 30 62 40 56 38
6 41 29 65 43 34 11 66 42 57 40
7 57 41 47 32 118 47 66 41 59 39
8 52 32 65 43 117 47 66 42 60 37
9 50 32 60 40 115 45 65 42 58 36
10 47 30 56 38 117 47 66 42 49 32
11 51 32 57 39 118 47 66 42 65 43
12 48 29 58 39 97 45 65 41 37 25
13 43 24 42 29 47 41 65 39 38 26
14 43 24 117 46 48 42 57 38 61 39
15 42 23 68 27 48 41 63 41 56 34
16 50 32 42 15 48 42 66 42 41 29
17 40 31 118 46 42 36 63 40 46 29
18 35 31 115 48 31 28 67 42 36 23
19 36 21 30 12 30 27 56 35 105 39
20 7 7 44 18 47 42 65 40 112 45
21 45 30 38 16 48 42 57 38 116 45
22 66 43 36 16 44 39 63 41 110 44
23 41 26 32 12 47 41 62 39 52 19
24 40 25 36 16 44 38 63 42 30 13
25 67 43 16 7 31 27 63 39 29 13
26 50 34 n/a n/a 47 33 65 42 26 18
27 27 17 n/a n/a 64 41 65 41 27 18
28 27 16 n/a n/a 67 42 58 38 22 12
29 67 42 66 42 63 39 n/a n/a
30 50 32 66 41 65 41 n/a n/a
31 34 21 54 35 28 18
# images 1357 892 1449 783 1912 1123 1908 1216 1636 922
archive has been updated by NASA !
LASCO: “…high volume memories and a high-speed microprocessor enable extensive on-board image processing.
Image compression by a factor of about 10 will result in the transmission of 10 full images per hour…”
Source: LASCO instrument paper…

Excursion: AdvancedExcursion: Advanced
ET communication IET communication I
LASCO C3 flooded with codes – blue squares = NASA make-up,
whistle blowers leave the truth in! Zoomed area prove the appearance of codes
-> no image processing errors (otherwise NASA would use scrap software)
DNA helix?
?

ET communication IIET communication II
GIF (1024 x 1024 / 8 BPP) ->
8192 x 8192 / 150 dpi -> zoom ->
LASCO C3 flooded with codes – blue squares = NASA make-up. What do we get
here? Layout of LASCO’s integrated circuits housed in the LEB (LASCO electronic
box) or the layout of LASCO CCD sensor. Decide yourself…

ET communication IIIET communication III
?
?
GIF (1024 x 1024 / 8 BPP) ->
8192 x 8192 / 150 dpi -> zoom ->
Source: KODAK CCD Primer – MTD/PS-0218
LASCO CCD’s = Frame-Transfer (FT) !

ET communication IVET communication IV
GIF (1024 x 1024 / 8 BPP) ->
16384 x 16384 / 150 dpi -> zoom ->
chip mounting holes?
To convert a continuous-tone image into a digital format, the analog image is
divided into individual brightness values through two operational processes
that are termed sampling and quantization… The result is a numerical
representation of the intensity… for each sampled data point in the array
image array or
storage array?

Excursion: Special feature IExcursion: Special feature I
solar activity affects all life on Earth!

Excursion: Special feature IIExcursion: Special feature II

Excursion: Special feature IIIExcursion: Special feature III

Excursion: Special feature IVExcursion: Special feature IV
 conclusionconclusion::
 sun‘s activity is partly controlled by higher intelligence we do not understand yetsun‘s activity is partly controlled by higher intelligence we do not understand yet
 NASA composes the EIT / C2 / C3 images from different instrumentsNASA composes the EIT / C2 / C3 images from different instruments
 sun ejects massive amounts of energy partly triggered by higher intelligencesun ejects massive amounts of energy partly triggered by higher intelligence
 NASA does massive cover-up / make-up with the images to hide the truthNASA does massive cover-up / make-up with the images to hide the truth
 NASA is using image processing software to rework the imagesNASA is using image processing software to rework the images
 coronal mass ejections might be the cause for the global climate changes we are currently faced withcoronal mass ejections might be the cause for the global climate changes we are currently faced with
 the one who controls the sun controls life on planet Earththe one who controls the sun controls life on planet Earth
 22nd ++ century technology seems to be in action to control solar activities22nd ++ century technology seems to be in action to control solar activities
 some of the effects shown can‘t be explained at allsome of the effects shown can‘t be explained at all
 CME‘s seem to cause shock waves hitting SOHO satellite (2007/03/25 20:42 C3 image can proof this – rememberCME‘s seem to cause shock waves hitting SOHO satellite (2007/03/25 20:42 C3 image can proof this – remember
LASCO exposure times)LASCO exposure times)
SOHO hit by shock
wave – causing blurred
image?
most advanced technology
in action

Excursion: C2 sample analysis IExcursion: C2 sample analysis I
Step 1: always use the original GIF files for visual inspection
Step 2: zoom the image to
identify the objects – PSP
zoom +500%

Excursion: C2 sampleExcursion: C2 sample
analysis IIanalysis II
Step 3: image inversion
Step 4: hold your breath! – propulsion
becomes visible

analysis IIIanalysis III
Step 5: apply solarization filter
Step 6: energy / wave packets
ejected by propulsion! – compare
to sun CMEs (high energy /
high frequency state

analysis IVanalysis IV
Step 7: apply I/R filter
Step 8: force fields / high frequency

analysis Vanalysis V
Step 9: apply high-pass filter
Step 10: yet another proof for
advanced propulsion

analysis VIanalysis VI
Step 11: GIF (1024 x 1024 / 8BPP) -> 8192 x 8192 / 150 dpi -> zoom ->
Step 12: fasten seat belt
and take-off 
true object size? The
“planet” shape might be
caused by a strong energy
field generated by the
propulsion system –
means also perfect stealth!
Corel Photo Paint X3:
8192 x 8192 /150 dpi,
filter: relief

Samples ISamples I
why do planets „fire“ a beam?
space ship „fires“ a beam into sun
G-waves
shield?

Samples IIISamples IIIEIT image merged with
LASCO C3 image!

Samples VSamples V
cut-outs taken from GIF files (1024 x 1024 / 8BPP) -> 4096 x 4096 / 150 dpi -> zoom ->
LASCO C3, 2007/05/18, 09:18LASCO C2, 2007/05/16, 20:06LASCO C3, 2007/05/16, 03:18LASCO C3, 2007/05/15, 03:18

Samples VISamples VI
cut-outs taken from GIF files (1024 x 1024 / 8BPP) -> 4096 x 4096 / 150 dpi -> zoom ->
LASCO C3, 2007/04/30, 23:18
http://en.wikipedia.org/wiki/Sombrero_Galaxy
A mid-infrared image of the Sombrero Galaxy as seen by
the Spitzer Space Telescope (SST). The white colors represent
3.6 and 5.8 micrometre emission from starlight. The red colors
represent 8.0 micrometre emission from polycyclic aromatic
hydrocarbons (PAHs) within the dust ring.
credit: http://gallery.spitzer.caltech.edu/

@NASA@NASA: Please answer our: Please answer our
nasty questions…nasty questions…
 why do we miss most of the FITS files in the science archive?why do we miss most of the FITS files in the science archive?
 why does NASA use software tools to cover-up / make-up the images?why does NASA use software tools to cover-up / make-up the images?
 why does NASA supply C2/C3 archives with different file size?why does NASA supply C2/C3 archives with different file size?
 why does NASA make-up often EIT / EUV images?why does NASA make-up often EIT / EUV images?
 why not supply a process chart explaining the whole imaging procedure?why not supply a process chart explaining the whole imaging procedure?
 why does NASA mix older images with actual images?why does NASA mix older images with actual images?
 why supply only fragments of SOHO papers / instrument papers in the SOHO web?why supply only fragments of SOHO papers / instrument papers in the SOHO web?
 why supply a LASCO debris list with b/w GIF files only?why supply a LASCO debris list with b/w GIF files only?
 why supply GIF images varying in size?why supply GIF images varying in size?
 why does NASA explain „common errors“ in „sungrazer“ web page?why does NASA explain „common errors“ in „sungrazer“ web page?
 why does NASA supply „hotshots“ page having explanations „how to make your own UFO“?why does NASA supply „hotshots“ page having explanations „how to make your own UFO“?
 why does NASA sometimes supply C2/C3 archives only after a 2-3 day break?why does NASA sometimes supply C2/C3 archives only after a 2-3 day break?
 why does NASA brush-up older C2/C3 archives – they simply grow in size?why does NASA brush-up older C2/C3 archives – they simply grow in size?
 why does NASA report from time to time CCD BAKEOUT on EUV instruments?why does NASA report from time to time CCD BAKEOUT on EUV instruments?

Recommended LinksRecommended Links
 Google Video: “The Case for Antigravity” (hosted by Andrew Johnson)Google Video: “The Case for Antigravity” (hosted by Andrew Johnson)
 explanation of Anti-G (Townsend Brown, John Hutchison, NASA black projects, etc.)explanation of Anti-G (Townsend Brown, John Hutchison, NASA black projects, etc.)
http://http://video.google.de/url?docidvideo.google.de/url?docid=-286184459501486399&esrc=sr3&ev==-286184459501486399&esrc=sr3&ev=v&qv&q==anti+gravity&vidurlanti+gravity&vidurl
=http://video.google.de/videoplay%3Fdocid%3D-286184459501486399%26q%3Danti%2Bgravity&usg=AL29H23I=http://video.google.de/videoplay%3Fdocid%3D-286184459501486399%26q%3Danti%2Bgravity&usg=AL29H23I
 Google Video: “Mars, Pyramids and Changes in the Solar System” (hosted by Andrew Johnson)Google Video: “Mars, Pyramids and Changes in the Solar System” (hosted by Andrew Johnson)
 explanation of Earth/Mars relation (hyperD energy, changes in the solar system, pyramids,explanation of Earth/Mars relation (hyperD energy, changes in the solar system, pyramids,
interview with Dr. Eugene Mallove)interview with Dr. Eugene Mallove)
http://http://video.google.de/url?vidurlvideo.google.de/url?vidurl
=http%3A%2F%2Fvideo.google.de%2Fvideoplay%3Fdocid%3D-3835552873482653680%26q%3Dmars%252C%2=http%3A%2F%2Fvideo.google.de%2Fvideoplay%3Fdocid%3D-3835552873482653680%26q%3Dmars%252C%2
v&esrcv&esrc=sr1&usg=AL29H22iwktvJvD-vrQX1sPIJcAOCFQWQA=sr1&usg=AL29H22iwktvJvD-vrQX1sPIJcAOCFQWQA
 Google Video: „NASA UFOs STS-115 (Full Version)“Google Video: „NASA UFOs STS-115 (Full Version)“
http://http://video.google.de/videoplay?docidvideo.google.de/videoplay?docid=7478848621447936646=7478848621447936646
 UFO technology / Turkish web (refers also to Paul Potter: http://homepage.ntlworld.com/ufophysics/)UFO technology / Turkish web (refers also to Paul Potter: http://homepage.ntlworld.com/ufophysics/)
 most of the content available in English language, deals with advanced propulsion systems onmost of the content available in English language, deals with advanced propulsion systems on
technical leveltechnical level
http://http://www.zamandayolculuk.com/cetinbal/UFOTEKNOLOJII.HTMwww.zamandayolculuk.com/cetinbal/UFOTEKNOLOJII.HTM

Whistle blowersWhistle blowers @NASA@NASA……
EIT 304 EUV image (composite)
EIT 304 EUV image
LASCO occulter disk
& pylon
EIT 171 EUV image
shock waves?

Real life answers from NASAReal life answers from NASA
NASA: “controlled” shutdown
sequence of EIT (EUV) instruments
(2007/05/18):
17:00 -> EIT 171
17:10 -> EIT 284
17:20 -> EIT 195
17:30 -> EIT 304

peace and love…peace and love…

Soho Image Anomalies - Analysis 1

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