Gain variation
effects and correction in CCD cameras for TEM
By Bill
Mollon, Gatan
As technology evolves, more and more people
are taking the course towards replacing conventional film
with the newer CCD cameras created for TEM applications. With
this progression towards CCD camera use on TEM’s, is
the need to fully understand all the parameters that can affect
the final image quality. Gain normalization is a common procedure
to correct for any artificial defects from the CCD camera
and has greatly improved the image quality. However, little
attention has been paid to the dependence of the gain reference
image on TEM magnification.
The purpose of this article is to first demonstrate
such dependence and show how it can affect the image quality.
Then we show a new patented procedure to make gain reference
image TEM magnification dependent.
Digital Image components
A digital image acquired from a microscope,
camera, or other optical device is often described as the
raw image prior to any processing or adjustment of critical
pixel values (see Figure 1). In many cases, this raw image
is unsuitable for use in target applications (printing, web
display, reports, etc.), due to it exhibiting a significant
level of noise and other artifacts from the capture system.
Typical examples are detector irregularities (pixel non-uniformity
and fixed-pattern contrast from the scintillator), dust, scratches,
etc.. These “errors” in the raw image are manifested
as dark shadows, excessively bright highlights, specks, and
mottles that alter the true pixel values. Applying the gain
normalization technique to raw digital images can often ensure
photometric accuracy and remove common image defects to restore
the fidelity of features and achieve a more visual balance
(Figure 2).
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| Figure 1 Raw image
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Figure 2 Corrected
image (gain normalized) |
Gain Variations Due to TEM Magnification
(Beam Profile)
Successful gain normalization assumes that
uniform illumination condition exist on the CCD scintillator
and the gain reference image is recorded under such condition.
If there is a deviation from the uniform illumination as a
result of changing TEM magnification, gain normalization will
certainly fail.
For bottom mounted CCD cameras, since the
field of view is small compared to that of film, the variation
of illumination with TEM magnification is found to be very
small and can be ignored. However, for CCD cameras mounted
in the 35mm port (wide angle position), such variation can
not be ignored. The reason is simply that the field of view
of the CCD camera is now larger than that of film. As a result,
distortions in the TEM electron-optical system can significantly
degrade the image quality since we can not assume the uniform
illumination remains when TEM magnification is changed.
Figure 3 shows a perfect gain normalized image
(no sample) just after gain reference image is recorded at
8500x using parallel illumination. The image is flat and free
from any artifacts.

Figure 3 Gain normalized image of the parallel electron
beam (8500x)
Using the line profile tool on this image you can see that
it shows a uniform “flat” intensity response after
gain normalization (Figure 4)

Figure 4 Line profile of Figure 3
Now we can show the variation of the TEM beam profile as TEM
magnification changes. This variation is most pronounced when
the camera is mounted in the 35mm port of the TEM due to large
field of view.
The problem is noticeable if only one gain
reference series is collected and is attempted to be used
for all magnifications. To demonstrate this phenomenon we
will change the TEM magnification and re-acquire the gain
normalized image to see if there are noticeable affects on
the image quality.
Magnification Affects on TEM Beam
Profile
So far we have only collected on set of reference
images at a magnification of 8500x. After the TEM magnification
was raised from 8500x to 38,000x. A gain normalized image
of the beam (using gain reference image recorded at 8500x)
was then acquired. As you can see in Figure 5, the gain reference
images recorded at 8500x have failed to reproduce a uniform
image at this higher magnification.
Remember that we only changed the TEM magnification
and nothing else. So the unevenness in the image must come
from change in illumination pattern and nothing else! This
has clearly demonstrated that the illumination pattern changes
with TEM magnification and hence we must consider this fact
when preparing gain reference images.

Figure 5 Gain normalized image of electron beam (38,000x)
If we continue our investigation and go to an even higher
magnification (105,000x) you will see that the TEM beam profile
has changed again resulting in another example of the reference
images unable to correct properly.

Figure 6 Image of electron beam at higher magnification (105Kx)
When this phenomenon occurs and if we can
store only one set of gain reference images, the end user
would have to take time to properly acquire a new gain reference
image in order to continue on with collecting artifact free
images. This could be time consuming or even worse, overlooked
until later when closely working with the acquired images.
We have noticed an increase in people reporting this problem
as more people enter the digital world in electron microscopy.
Usually it is the Life Science applications that are most
sensitive to this variance due to image acquisitions covering
wide ranges in magnification and the use of wide angle CCD
cameras.
For illustration purposes the examples shown
here used large changes in magnification. There are cases
in which a single set of reference images are adequate if
the magnification step change is very small and close to the
original starting magnification. As can be expected, the variance
due to beam profile changes will be different for each TEM
and operating condition used.
Multiple Gain Reference
Now that you have a better understanding
of gain reference processing, it would be ideal if we could
collect multiple sets of reference images and assign them
to magnification ranges or even individual magnification steps.
As the user changes magnifications the correct gain reference
assigned to that magnification would be used for the acquisition.
In the new Gatan Microscopy Suite, GMS 1.6 we have implemented
exactly this behavior. The user now has the ability to prepare
more than one set of gain reference images and assign them
to individual magnification steps or even ranges. This gives
the user total freedom in changing from one magnification
to another without having to stop and reacquire reference
images. Productivity, ease of use and controlled high quality
image collection becomes the new standard in the digital acquisition
session. Let’s go through the steps and use this new
feature:
Assuming that GMS 1.6 has been installed the
steps to prepare gain reference images has not changed that
much from previous versions. The noticeable difference is
the assigning of magnification ranges to the reference set.
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| 1 |
If your camera requires it, prepare for collecting
dark reference images first. Make sure the electron
beam is off or blanked and the TEM viewing chamber
is covered to prevent stray room light. Pull down
the Camera menu and select “prepare dark reference”.
The software will begin the process of collecting
the dark reference images. |
| 2 |
Next are the gain reference images. Turn the electron
beam back on and make sure the specimen is removed
from the beam path. Select the magnification desired
for final image acquisition. |
| 3 |
With the specimen removed, spread the illumination
so that it is uniformly spread across the CCD and
the proper number of counts per pixel is seen. Use
the Intensity bar as shown in DigitalMicrograph
to assist you with this (Figure 12) |
| 4 |
Pull down the Camera menu and select “prepare
gain reference”. You will be prompted to enter
your camera’s target intensity and the magnification
range you want this to be applied to (Figure 13).
If you want to apply this to a single magnification,
enter the same number in both boxes. |
| 5 |
A dialog window will appear reminding you to
make sure the illumination is uniform and that the
specimen is removed. |
| 6 |
During the reference image acquisition, if the
software finds the illumination to the CCD is too
high or too low, you will be prompted to adjust
the intensity. |
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Figure
12 |
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| 7 |
Upon completion of the gain reference collection
click the OK button to close the dialog window |
| 8 |
The new set of gain reference images have now
been saved in the reference folder and named appropriately
according to the magnification range you specified.
You can continue and collect another set of gain
reference images by changing the TEM magnification
and repeating steps 2 -7 above. There is no need
to collect another set of dark reference images. |
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Figure 13
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Summary
Depending on your TEM model you may find that several successive
magnification steps do not change the beam profile that much.
Most TEM’s have at least 3 basic operating magnification
ranges: low (1000x – 10,000x), medium (11,000x –
40,000x) and high (50,000x – 300,000x). In order to
find out how changing the magnification affects the gain reference
images in these ranges you can start at the low end and collect
the first set. Then with gain normalization processing turned
on, collect an image of the beam after increasing the magnification.
Look for affects shown in Figures 10 and 11. When you notice
an appreciable change, record the magnification step and collect
a new gain reference set there. This should help you “see”
the magnification ranges on your TEM where a gain reference
set should be collected and be used later in correcting your
final image.
Once this is completed you should not have
to recollect gain reference images unless you have changed
other illumination or optical parameters on your TEM such
as condenser aperture size, objective aperture size, accelerating
voltage and in some cases spot size. Overall illumination
intensity delivered to the CCD camera by the TEM optics will
have an affect on the gain reference images collected. Keep
in mind that gain reference images are actually a series of
snapshots of your current beam operating conditions that you
have set on the microscope. Dark reference images should be
re-acquired periodically as a maintenance check or if instructed
by the Gatan Service engineer as part of troubleshooting.
As mentioned earlier the dark reference images correct for
components of the CCD and camera electronics and are independent
of TEM beam illumination.
The development and investigation of this
technique came from valuable input that we receive from our
customers. This is a perfect example of the commitment that
we take to help improve our products based on the needs of
our customers. We hope you find this information and new software
feature gives you assurance in collecting quality, consistent,
easy to use and reliable digital images from our cameras.
Allowing you to spend more time on your application and letting
our systems deliver a solution is our goal.
We
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Gatan
Inc. Corporate Headquarters, 5933 Coronado Lane, Pleasanton,
CA 94588
Tel. (925) 463 0200 Fax. (925) 463 0204
Contact: info@gatan.com
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