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11.2 Principlesofdarkeldillumination
Darkeld microscopy is a specialized illumination tech-
nique that capitalizes on oblique illumination to enhance
contrast in specimens that are not imaged well under nor-
mal brighteld illumination conditions.
All of us are quite familiar with the appearance and visibi-
lity of stars on a dark night, this despite their enormous di-
stances from the earth. Stars can be seen because of the
stark contrast between their faint light and the black sky.
This principle is applied in darkeld (also called
darkground) microscopy, a simple and popular method for
making unstained objects clearly visible. Such objects are
often have refractive indices very close in value to that of
their surroundings and are difcult to image in conven-
tional brighteld microscopy. For instance, many small
aquatic organisms have a refractive index ranging from
1.2 to 1.4, resulting in a negligible optical difference from
the surrounding aqueous medium. These are ideal candi-
dates for darkeld illumination.
Darkeld illumination requires blocking out of the central
light which ordinarily passes through and around (sur-
rounding) the specimen, allowing only oblique rays from
every azimuth to “strike” the specimen mounted on the
microscope slide. The top lens of a simple Abbe darkeld
condenser is spherically concave, allowing light rays
emerging from the surface in all azimuths to form an in-
verted hollow cone of light with an apex centered in the
specimen plane. If no specimen is present and the nu-
merical aperture of the condenser is greater than that of
the objective, the oblique rays cross and all such rays will
miss entering the objective because of their obliquity. The
eld of view will appear dark.
The darkeld condenser/objective pair illustrated in Fig. 22 is a high-numerical aperture arrangement that repre-
sents darkeld microscopy in its most sophisticated conguration, which will be discussed in detail below. The
objective contains an internal iris diaphragm that serves to reduce the numerical aperture of the objective to a
value below that of the inverted hollow light cone emitted by the condenser. The cardioid condenser is a reec-
ting darkeld design that relies on internal mirrors to project an aberration-free cone of light onto the specimen
plane.
When a specimen is placed on the slide, especially an unstained, non-light absorbing specimen, the oblique
rays cross the specimen and are diffracted, reected, and/or refracted by optical discontinuities (such as the cell
membrane, nucleus, and internal organelles) allowing these faint rays to enter the objective. The specimen can
then be seen bright on an otherwise black background. In terms of Fourier optics, darkeld illumination removes
the zeroth order (unscattered light) from the diffraction pattern formed at the rear focal plane of the objective.
This results in an image formed exclusively from higher order diffraction intensities scattered by the specimen.
Ideal candidates for darkeld illumination include minute living aquatic organisms, diatoms, small insects, bone,
bers, hair, unstained bacteria, yeast, and protozoa.
Non-biological specimens include mineral and chemical crystals, colloidal particles, dust-count specimens, and
thin sections of polymers and ceramics containing small inclusions, porosity differences, or refractive index
gradients.
Care should be taken when preparing specimens for darkeld microscopy because features that lie above and
below the plane of focus can also scatter light and contribute to image degradation.
Specimen thickness and microscope slide thickness are also very important and, in general, a thin specimen is
desirable to eliminate the possibility of diffraction artifacts that can interfere with image formation.
Cardioid condenser for
darkfield Fig. 22
High
Numerical
Aperture
Objective
ObliqueHollow
Light Cone
Light to
Eyepieces
Iris Diaphragm
Specimen
Slide
Concave
mirror
Cardioid
Condenser
Convex
Mirror
Opaque
Light Stop
Light From
Source