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SeDDaRA
Image Gallery
Quarktet's
blind deconvolution algorithm, SeDDaRA, has been named as one of
Advanced
Imaging Magazine's Solution of the Year by unanimous decision! The
winning
solution is the removal of blur from an image of the background
radiation
of the universe. A portion of the image and its restoration appear
below.
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Fig1:
Image of the background radiation of the universe as taken by the NASA
Wilkinson Microwave Anistropy Probe (WMAP)
satellite. The image has been false-colored to highlight the contrast.
This
image, together with four images in four other spectral bands, allowed
NASA/WMAP scientists
to more accurately define the age of the universe and the rate of
expansion.
Run your mouse over the image to reveal the restored figure.
Fig 2: Using a fractal image as a model, a
blur function, resembling
a clover-leaf, was extracted from the image. A pseudo-inverse filter
removed the blur to sharpen the image. The image is cleaner and reveals
greater resolution. We hope the use of this processing technique will
enable scientists to achieve even greater accuracy in their
calculations.
Image Courtesy of the
NASA/WMAP Science Team.
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About the Gallery....
Here
and on the following pages, you will see more examples of blind deconvolutions performed using the
SeDDaRA process. A great advantage of this technique
is that it can be applied to any data type, such as consumer
photographs,
medical images, one dimensional signals, microscopy, and astronomy
images.
For most, the improvement is obvious. In some cases, the
improvement more subtle. SeDDaRA removes the blur that is present
in the image (or signal) by extracting the point spread function (or
impulse
function). Thus, the method returns only the physical aspects of the
image, and does not create any new information. This is how the process
differs from a standard edge-enhancing filters.
If you have viewed other deconvolution websites, you may have noticed
that the images displayed here are significantly larger. When we apply
SeDDaRA, we do not hesitate at processing larger images, and have had
to
crop many of the images on display here. This is a testament to the
efficiency
of the process. We do, however, apologize for the longer download
times.
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Fig1: Image of Saturn, taken by the
Hubble Space Telescope before the optical correction was applied in
December
1993. This image has become a standard image deconvolution example.
Run your mouse over the image to reveal the restored figure.
Fig 2: Restored Image. Not only is the planet
much cleaner, but if you look close enough you will see stars behind
the planet that were not apparent before.
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Fig1:
A microscope image of fission yeast that already undergone some
processing. This image was displayed on several websites
as an example of good deconvolution.
Run your mouse over the
image to reveal the restored figure.
Fig 2: Restoration of the microscope
image. Even though the image has already been processed by more
conventional means, the image is significantly enhanced using SeDDaRA.
This
occurs because it is very difficult to measure or calculate the exact
blur
function of a system. Many times, a little help is needed to see
clearly.
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Quarktet
has contacted the producer of the fission yeast image about retrieving
the
original data. To date, no reply has been received.
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Gallery Index
1 Gallery Into
2 Home Pics
3 X-rays
4 1-D Signals
5 Astronomy
6 Microscope
7 Misc.
8 Ultrasound
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