Dark field emphasizes borders and isolated, single structures, flagella of protozoa and tiny particles. The comparison of a diatom sample in bright field and dark field clearly shows this:
How such an image is achieved? We need to eliminate the direct light which ordinarily passes the specimen and which is responsible for the bright background in bright field illumination. For objectives with a Numerical Aperture ≤ 0.65 this
can be done by inserting a simple “central stop” into the ray path at the height of the condenser. Higher Numerical Apertures require a more sophisticated condenser setup and special objectives with iris diaphragm.
The central stop is a round piece of black metal, mounted into an attachment, a slider or the disc of a turret condenser. The stop has to be aligned so that it is exactly placed in the middle of the ray path. The procedure of alignment is quite similar to phase contrast, where the illumination rings also have to be positioned precisely.
Once done, the sample is illuminated only by light that passes through the slot around the central stop in the form of a hollow cone. Thanks to the front lens of the condenser, this light will miss the front lens of the objective. In case there is no sample placed on the x/y stage, the user will observe a dark field of view.
First prepare the respective microscope for optimal bright field use, best start with a 10X objective. If necessary, perform the KOEHLER setup (focus the sample, center the image of the field diaphragm, adjust the height of the condenser, open the field diaphragm). For dark field now open the condenser (= aperture) diaphragm completely. This allows the condenser to operate at its maximum numerical aperture.
Insert the central stop into the optical path of the microscope. Depending on the microscope model, plug-in the DF attachment, push in the DF slider, or rotate the condenser disc to the respective DF position.
Pull-out one eyepiece and insert a centering telescope (CT) instead. Loosen the fixing screw and focus the back focal plane of the objective by pulling out the inner part of the centering telescope. A bright disk of light that is partially obscured by the central stop will be visible at the objective rear focal plane. If not, use the centering screws and move the central stop so that the bright disk is completely covered.
Now watch the image of the sample. In case the background is not perfectly dark, carefully raise/lower the condenser until the background becomes dark. Have a closer look on single particles within the sample. They all should have a symmetric brightness all around their periphery. If not, center the DF stop more precisely. The periphery of each single particle should display a symmetric brightness.
If there is no centering telescope at hand, use a sheet of paper as a sample. While slowly raising and lowering the condenser, a bright spot will appear on the paper (a). Below or above this condenser position, a dark spot appears. This spot has to be in central position (b).
If not (c, d), the DF stop has to be centered. The microscope is now ready for dark field observation. Take care that the glass slide is perfectly clean on both sides. Each finger print, each dust particle will cause stray light and will destroy the aesthetic impression of the dark field image. This is why some people regard dark field as a “dust-detecting method”.