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5 Bad Habits in dark field light microscope

dark field light microscope

RPR/VDRL/MHA-TP (Serologic Tests for Syphilis) Darkfield/FTA-ABS MicroscopyRPR / VDRL / MHA-TP

RPR/VDRL/MHA-TP (Serologic Tests for Syphilis) Darkfield/FTA-ABS Microscopy

A variety of serologic tests for syphilis are available, including:

VDRL (Venereal Disease Research Laboratory)
RPR (Rapid Plasma Reagin)
FTA-ABS (Fluorescent Treponemal Antibody Absorption)
TP-MHA (Treponema Pallidum Microhemagglutination Assay)

Each differs the others in the precise substance being measured, complexity, and specificity. All are satisfactory for use in managing syphilis. Abnormals may be:

Reactive,
Weakly reactive, or
Bordeline

Whenever a screening test (RPR, VDRL) is positive, a more specific test (FTA-ABS, TP-MHA) should be used to confirm the test and rule out a “biologic false positive.”

A negative or “nonreactive” test may indicate:

The patient doesn’t have syphilis
The patient has syphilis, but is so early in the course of the disease that the test has not yet turned positive. In these cases, the test may never turn positive if the patient is effectively treated.
The patient had primary syphilis, had a positive test, was effectively treated, 6 months have passed and the test has now reverted back to negative.
The patient had secondary syphilis, had a positive test, was effectively treated, 12-18 months have passed and the test has now reverted back to negative.
The patient has syphilis, but his/her immune system is impaired.

A positive or “reactive” test may indicate:

The patient has syphilis.
The patient had syphilis, was effectively treated, but the test has not yet returned to negative:
With primarily syphilis, it typically takes about 6 months for the test to turn negative.
With secondary syphilis, it typically takes 12-18 months for the test to turn negative.
The longer syphilis remains untreated, the longer it will take for the test to return to normal, and the less likely it is to ever return to normal.
The patient has a biologic false positive (BFP)

dark field light microscope

How to Make a dark field light microscope?

You don’t need to buy a huge expensive set-up to experiment with dark field illumination.

To create a dark field, an opaque circle called a patchstop is placed in the condenser of the microscope. The patchstop prevents direct light from reaching the objective lens, and the only light that does reach the lens is reflected or refracted by the specimen. Easy enough, right?

If you want to make a dark field microscope you’ll first need a regular light microscope. Below is your full list of “ingredients”:

Dark field microscopeMicroscope
Hole punch
Black construction paper
Transparency film
Glue
Scissors
Pen
Now use the following steps to make your patchstop:

Set up your microscope and choose the lowest-power objective lens.
Set the eyepiece aside somewhere safe.
Open the diaphragm as wide as possible. Then slowly close it until is just encroaches on the circle of visible light.
Now bend over and take a look at the diaphragm from below. See that opening? It’s only slightly smaller than the finished patchstop you’ll create.
Punch a few circles in the black construction paper with the hole punch. Measure one against the diaphragm opening. If it’s more than 10% larger, cut it down to about that size (10% larger than the diaphragm opening). If it’s smaller, cut out a larger circle.
Cut a 5 cm square of transparency paper.
Glue the black circle onto the transparency film, about 2 cm from the corner of the square. In that free 2 cm of paper, write the correct magnification power of your objective.
Mark the patchstop with the correct magnification power.
Repeat the above steps for all the objective powers except the oil immersion lenses.
Now use your patchstop to turn a light field unit into a dark field microscope:

Select the correct patchstop for the objective power to be used.
Slip the patchstop between the filter holder and condenser. If your microscope has no filter, hold it manually below the condenser.
Remove the eyepiece.
Open the diaphragm and move the patchstop until the light is blocked entirely. Use tape to secure it if there is no condenser on your microscope.
Replace the eyepiece and examine the sample.
As you can see, a dark field microscope can let users see specimens in a whole new way, bringing those into focus that don’t stand out under intense light. Using dark field illumination can open up a whole new view of microscopy
The first picture of the plankton was taken by Uwe Kils and is from Wikipedia under the GNU Free Documentation License.

dark field light microscope

what is dark field light microscope?

what is dark field light microscope?

Use scissors or (preferably) a brass cork borer to cut a set of stops matched to all of the objectives, and glue them to a sturdy sheet of clear acetate or glass. The acetate or glass substrate should be easily mountable onto the underside of the substage condenser, either through a filter holder or by other means, such as adhesive tape. Alignment of the stop can be done by observing it through a Bertrand lens or removing the eyepiece and viewing through a phase telescope while adjusting the condenser centering screws.

Darkfield Microscopy at High Magnifications

For more precise work and blacker backgrounds, you may choose a condenser designed especially for darkfield, i.e. to transmit only oblique rays. There are several varieties: “dry” darkfield condensers with air between the top of the condenser and the underside of the slide–and immersion darkfield condensers which require the use of a drop of immersion oil (some are designed to use water instead) establishing contact between the top of the condenser and the underside of the specimen slide. The immersion darkfield condenser has internal mirrored surfaces and passes rays of great obliquity and free of chromatic aberration, producing the best results and blackest background.

Perhaps the most widely used darkfield condenser is the paraboloid, consisting of a solid piece of glass ground very accurately into the shape of a paraboloid, as illustrated in Figure 5(b). Light incident upon the reflecting surface (between the glass and condenser housing in Figure 5(b)) of a paraboloid condenser will be focused at the focal point of the reflector. Most paraboloid condensers are cut to ensure that the focal point is slightly beyond the top of the condenser so that parallel light rays will be focused at a position that maximizes illumination of the specimen. The light stop at the bottom of the glass condenser serves to block central rays from reaching the specimen. Light rays that are reflected by the condenser are angled higher than the critical angle of reflection and converge at the principal focus of the condenser. The combination of a glass slide, mounting medium, and immersion oil (between the condenser and the microscope slide) complete the optical homogeneity of the paraboloid shape.

As discussed above, the dry darkfield condenser is useful for objectives with numerical apertures below 0.75 (Figure 5(a)), while the paraboloid and cardioid immersion condensers (Figures 1 and 5(b)) can be used with objectives of very high numerical aperture (up to 1.4). Objectives with a numerical aperture above 1.2 will require some reduction of their working aperture since their maximum numerical aperture may exceed the numerical aperture of the condenser, thus allowing direct light to enter the objective. For this reason, many high numerical aperture objectives designed for use with darkfield as well as brightfield illumination are made with a built-in adjustable iris diaphragm that acts as an aperture stop. This reduction in numerical aperture also limits the resolving power of the objective as well as the intensity of light in the image. Specialized objectives designed exclusively for darkfield work are produced with a maximum numerical aperture close to the lower limit of the numerical aperture of the darkfield condenser. They do not have internal iris diaphragms, however the lens mount diameters are adjusted so at least one internal lens has the optimum diameter to perform as an aperture stop.

Table 2 lists several properties of the most common reflecting high numerical aperture darkfield condensers. This table should be used as a guide when selecting condenser/objective combinations for use with high numerical aperture darkfield applications.
High Numerical Aperture Darkfield Condenser Specifications
Condenser Type Hollow Cone
Numerical Aperture Objective Maximum
Numerical Aperture Number of Reflecting
Surfaces Optical Corrections
Paraboloid 1.00-1.40 0.85 1 Parabolic Achromatic
Cardioid 1.20-1.30 1.05 1 Spherical
1 Cardioidal Achromatic/
Aplanatic
Bicentric 1.20-1.30 1.05 1 Cardioidal
1 Spherical Aplanatic
Bispheric 1.20-1.30 1.05 2 Spherical Aplanatic
Cassegrain 1.40-1.50 1.30 1 Aspheric
1 Spherical Aplanatic
Spot Ring
(Bicentric) 1.40-1.50 1.30 2 Spherical Aplanatic
Nelson
Cassegrain 1.30-1.45 1.20 1 Aspheric
1 Spherical Aplanatic

The condensers illustrated in Figure 5 are designed specifically to produce oblique hollow light cones of high numerical aperture for darkfield illumination. In both instances, the upper surface of the condenser is planar and perpendicular to the optical axis of the microscope. The condenser on the left (Figure 5(a)) is designed to be used “dry” with no oil between the condenser and the underside of the microscope slide. In contrast, the paraboloid condenser in Figure 5(b) is intended to be “oiled” to the bottom of the microscope slide, directly underneath the specimen. Omission of immersion oil when using this condenser (or any of the other condensers listed in Table 2) will preclude any light from reaching the specimen. The oblique hollow cone of light rays emitted by these condensers cannot emerge from the top lens without oil and will be totally reflected back into the condenser. Light emitted from the illumination source is reflected at the mirrored glass surfaces within the interior of the condensers and exits the top of the condensers at much higher angles of inclination than the critical angle (approximately 41 degrees) at which total reflection occurs for passage of light from glass to air. In the situation of the oiled paraboloid condenser (Figure 5(b) and the condensers in Table 2) where the refractive index of the condenser glass, immersion oil, and glass slide are equal, light emitted from the condenser passes through the specimen unrefracted by glass-air interfaces.
Hollow Light Cone Numerical Aperture

Use this tutorial to visualize how the hollow cone of light changes with numerical aperture in reflecting darkfield condensers.
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Reflecting high numerical aperture condensers listed in Table 2 cover a wide range of designs used to produce the oblique hollow cone of light necessary for high-magnification darkfield microscopy. The paraboloid darkfield condenser has been discussed in detail above. Another very useful design is the cardioid condenser that is illustrated in Figure 1. This condenser design utilizes a mirrored hemisphere in the center of the condenser that serves as both a light stop and a reflector to direct light onto a second reflecting surface shaped to resemble a cardioid of revolution, from which the condenser derives its name. The combination of spherical and cardioid reflecting surfaces produces a condenser that is free from coma and both spherical and chromatic aberration. There are several technical drawbacks to using a condenser of such high numerical aperture. The cardioid condenser is very sensitive to alignment and must be carefully positioned to take advantage of the very sharp cone of illumination, making it the most difficult darkfield condenser to use. In addition, the condenser produces a significant amount of glare, even from the most minute dust particles, and the short focal length may result in poor illumination on objects that exceed a few microns in size or thickness. When choosing microscope slides for quantitative high-magnification darkfield microscopy, make certain to select slides made from a glass mixture that is free of fluorescent impurities.

High numerical aperture reflecting condensers (Figures 1, 5, 6 and Table 2) with darkfield illumination provide the method of choice for observing and photographing collections of very small particles or colloidal suspensions, even when the particle diameter is significantly lower than the limit of resolution for the objective. This is due to light diffracted by the particles, which passes through the objective and becomes visible as bright diffraction disks. Each particle is visible as a minute diffraction disk, provided the lateral distance between adjacent particles is greater than the limit of resolving power of the objective. As illumination intensity is increased, the optical difference between minute diffracting particles and their background increases. Simultaneously, even smaller particles (detectable solely by their ability to scatter light) now diffract enough light to become visible and suspended particles can be seen even when their diameters are smaller than 40 nanometers, which is about one-fifth the 200 nanometer resolution limit with oil immersion objectives of the highest numerical aperture. In biological applications, the movements of living bacterial flagella that average about 20 nanometers in diameter (too small to be seen in brightfield or DIC illumination) can be observed and photographed using high numerical aperture darkfield condensers.

Careful attention should be paid to the details of oiling a high numerical aperture condenser to the bottom of the specimen slide. It is very difficult to avoid introduction of tiny air bubbles into the area between the condenser top lens and the bottom of the microscope slide, and this technique should be practiced to perfection. Air bubbles will cause image flare and distortion, leading to a loss of contrast and overall image degradation. Problems are also encountered when using microscope slides that are either too thick or too thin. Many darkfield condensers contain the range of usable slide thickness inscribed directly on the condenser mount. If the slide is too thick, it is often difficult to focus the condenser without resorting to a higher viscosity immersion oil. On the other hand, slides that are too thin have a tendency to break the oil bond between the condenser and the slide. It is a good idea to purchase precision microscope slides of the correct thickness to avoid any of the problems mentioned above.
Darkfield Condenser Adjustment

Explore how alignment and configuration of a darkfield condenser affects image quality.
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A unique situation arises when specimens immersed in aqueous medium are being imaged using a high numerical aperture darkfield condenser. Under these conditions the refractive index of the aqueous solution limits the angle of inclination under which light can pass from the glass microscope slide (n = 1.515) into the water (n = 1.336) surrounding the specimen. The maximum numerical aperture of light passing from glass to water is given by the following equation:

NA (illumination) = 1.555 × sin(i) = 1.336 × sin(90°)

and because sin(90°) = 1

NA (illumination) = 1.336

Even though reflecting darkfield condensers designed for oil immersion are listed with upper limits of numerical aperture as high as 1.50 (see Table 2), light contributing to the illumination of specimens in aqueous media must have a numerical aperture no greater than 1.336, reducing the effective upper limit of darkfield illumination. In the case of specimens immersed in liquids of higher refractive index, the effective upper limit of the numerical aperture of darkfield illumination can approach a maximum of 1.50, although this is difficult to achieve in practice.

High numerical aperture condensers, whether intended for use dry or with oil, must be accurately centered in the optical path of the microscope to realize optimum performance. To achieve this, many darkfield condensers are built with a small circle engraved onto the upper surface to aid in centering the condenser. Centering is performed with a low power (10x-20x) objective by imaging the engraved circle and using the condenser centering screws to ensure the circle (and condenser) are correctly centered in the optical path. For more detailed information about microscope alignment for darkfield illumination, consult our section on darkfield microscope configuration elsewhere in the microscopy primer.

In general, objects imaged under proper conditions of darkfield illumination are quite spectacular to see (e.g. try a drop of fresh blood in darkfield). Often specimens containing very low inherent contrast in brightfield microscopy shine brilliantly in darkfield. Such illumination is best for revealing outlines, edges, boundaries, and refractive index gradients. Unfortunately, darkfield illumination is less useful in revealing internal details.

Other types of specimens, including many that are stained, also respond well to illumination under darkfield conditions. Figure 7 illustrates darkfield photomicrographs of three types of specimen, all of which produce good contrast in both brightfield and darkfield illumination. Details in the body of the deer tick (Ixodes demmini) shown in Figure 7(a) can be washed out in brightfield, unless the condenser aperture is stopped down to maximize contrast. However, in darkfield, most of the specimen detail in the tick becomes visible and can be easily captured on film. The heavily stained helminth trematode (Echinostoma revolutum, Figure 7(b)) also reveals considerably more detail when illuminated under darkfield conditions, as does the silkworm trachea and spiracle illustrated in Figure 7(c). In addition to the examples presented above, a number of other specimens can also be viewed and photographed under both brightfield and darkfield illumination to achieve the desired effects.

During the first half of the Twentieth Century, darkfield microscopy had a very strong following and much effort was expended in optimizing darkfield condensers and illuminators. This intense interest slowly began to fade with the emergence of more advanced contrasting-enhancing techniques such as phase contrast, differential interference contrast, and Hoffman modulation contrast. Recently, a renewed interest in transmitted darkfield microscopy has arisen due to its advantages when used in combination with fluorescence microscopy.

Darkfield microscopy is still an excellent tool for both biological and medical investigations. It can be effectively used at high magnifications to photograph living bacteria, or at low magnifications to view and photograph cells, tissues, and whole mounts. Marine biologists continue to use darkfield illumination at low powers to observe and record data about fresh and salt water organisms such as algae and plankton.

dark field light microscope

Difference between Dark and Bright Field Illumination

Difference between Dark and Bright Field Illumination

-When you view a particular specimen under a bright field microscope, you will observe that the specimen is dark while its background is bright; hence the name bright field microscope.
On the other hand, when you view a particular specimen under a dark field microscope, you will observe that the specimen is bright while its background is dark; hence the name dark field microscope.
-Since little light actually falls on the specimen, dark-field illumination shows less detail overall than bright-field illumination.

Bright Field Illumination.
A way of illuminating a specimen in a microscope by lighting it from behind, making the specimen appear dark against a bright background. It is considered the most basic type of microscope

The Dark field illumination requires blocking out the central light waves along the optical axis of the light waves. Blocking the light waves allows you to see the specimine when only the oblique rays hit the specimen at an angle.
Parts of the Microscope.
Monitor: To display the picture of the specimen your CMO objective lens is focused on.

CMO Objective lens: To magnify on the part of a specimen you wish to observe.

Stage: To hold your specimen.

Lamp Voltage: Controls how bright the light is.

Zoom Body: To zoom in on the specimen.

Illumination section: Illuminates the specimen.

Brightfield/Darkfield Diascopic Stand. Holds the inner pieces of the microscope inside.

Camera Control: Controls where the CMO Objective lens focuses on.

Economic observation tube: Allows you to see the specimen without the monitor.

Digital camera: Transfers the pixels onto the moniter so you can see the specimen.

Stage: Holds the microscope together and supports the microsope.

dark field light microscope

How to Bringing Light to the dark field light microscope

Have you ever heard of a dark field microscope? While such a name may sound like a sci-fi gadget used to measure black holes, in reality it’s just a handy tool used to view certain types of translucent samples. The average microscope user may not know about the concept of dark field microscopy, yet it can shed new light on the old way of viewing specimens.

Most people who have survived a biology class know what a light field microscope is. This type of scope uses bright field illumination, meaning it floods the specimen with white light from the condenser without any interference. Thus the specimen shows up as a dark image on a light background (or white field if you will).

This type of unit works best with specimens that have natural color pigments. The samples need to be thick enough to absorb the incoming light; so staining is usually paired with this type of microscope.

Plankton illuminated with a dark field microscopeYet what if the specimen is light colored or translucent, like the plankton on the right? It certainly won’t stand out against a strong white background. Additionally, some specimens are just too thin. They cannot absorb any of the light that passes through them, so they appear invisible to the user. This is where the concept of dark field illumination comes in!

Rather than using direct light from the condenser, one uses an opaque disk to block the light into just a few scattered beams. Now the background is dark, and the sample reflects the light of the beams only. This results in a light colored specimen against a dark background (dark field), perfect for viewing clear or translucent details.

On a grand scale, the same thing happens every day when you look up at the sky. Do the stars disappear when it’s light out? Of course not! They’re still there, their brilliance blotted out by the mid-day sun.

If you’re still having a hard time visualizing this concept, think of a dusty room with the light on and the door open. You may feel the dust affecting your breathing, but you probably won’t see it flying through the air.

Now turn off the light and close the door to just a sliver, while leaving the light on in the adjacent room. If you look at that sliver of light coming through the door, you’ll see all sorts of dust motes suspended in it. You’re employing a similar principle when you use dark field illumination!

dark field light microscope

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