The re-publication of the original directions is given with the view of showing what a clear conception Gillett had of the value of his invention. The careful directions given for centring must be regarded with interest, although nearly superseded by the centring screw arrangement in connection with the sub-stage. The best results, he goes on to say, will be secured by using the plain mirror and focussing the window-bar on the object, while a white-cloud illuminator will afford as much light as may be required. It is a mistake to suppose that direct light is more critical than indirect. As a rule, the student is given to over-illuminate the object. These questions will, however, be discussed further on.

Very many modifications of Gillett’s condenser have, since 1850, become known to microscopists. Ross’s present improved form (Fig. 127) is made to drop into the sub-stage of the microscope, and when adjusted, is an extremely efficient instrument. The optical part is similar to a ⁴⁄₁₀-inch objective. It has two sets of revolving diaphragms, with apertures and stops for showing surface markings in a perfect manner.

Abbe’s Condenser.

The essential feature of this condenser is its short focus, which collects the light reflected by the mirror, so as to form a cone of rays of very large aperture, having its focus in the plane of the object.

The full aperture of the illuminating cone should only be used when finely granular and deeply stained particles (protoplasm, bacteria, &c.) are being examined with objectives of large aperture. In all cases the cone must be suitably reduced, either by an iris, or other form of diaphragm (central illumination). By placing the diaphragm excentrically, by means of rack-work attached to the carrier, the central rays are excluded and a certain extra-axial portion of the illuminating pencil falls upon the object (oblique illumination). When the diaphragm is thus excentrically placed, this oblique pencil can be directed from all sides by rotating the carrier round the optic axis. The central stop diaphragm shuts off all the axial and transmits only the marginal rays, thus producing dark-ground illumination. The iris diaphragm (Fig. 128) is so shaped that the edge of its smallest opening closely approximates the object-slide on the stage.

The Abbe condenser is the most popular form in use, for all purposes. Owing to the large aperture of the cone of light which it projects, it can be employed with the highest powers; by removing the top lens it can also be used with low powers. Dark ground illumination may be obtained with it up to a ¼-inch objective.

The condenser is made in two forms of 1·2 and 1·4 numerical aperture by Messrs. Watson. The lenses are mounted in aluminium. Fig. 130 is in more general use, but by workers with high powers Fig. 131 is preferred, as it ensures the most oblique illumination with objectives of largest aperture. It is preferred for photo-micrographic purposes.

Watson’s Achromatic Condenser (Fig. 132), 1·0 numerical aperture, shown in section, although originally designed for use with the micro-spectroscope, is equally efficient for ordinary purposes. This condenser transmits a larger aplanatic cone of light than Abbe’s. It may therefore be employed with higher power objectives, and by removing the top lens it is just as useful a condenser for lower powers. Being constructed with lenses of an unusually large size, it is well adapted for use with the micro-spectroscope. It is certainly one of the best all-round condensers in use. The new Schott glass enters into the construction of the lenses, and these are mounted in aluminium.

Many microscopists consider on the whole that Powell’s sub-stage apochromatic condenser with collar correction (Fig. 133) surpasses that of Abbe. The mechanical arrangement of Powell’s is very simple: the correction collar is similar to that of an ordinary objective, it has a steeper spiral slot and only half a revolution of movement; a long arc is fixed to the collar so that it may conveniently be reached by the finger. It is so constructed as to turn easily and smoothly at the slightest touch. The collar moves only the back lens of the combination, leaving the mount rigid. The diaphragms are regulated by A and B.

The object of the correctional movement is to increase the maximum aplanatic aperture of the condenser by separating the lenses. If the back of a wide-angled objective be examined when an object is illuminated by the full aperture of the condenser, the edge of the flame being in focus, it will be noticed that the illuminated portion of the back lens will be oval and pointed instead of circular. Also that when the condenser is racked up, although the external shape of the illuminated portion becomes more circular, two dark patches will appear on either side of the centre, showing the operation of the spherical aberration of the condenser. If under these circumstances the lenses are separated by means of the collar adjustment, the black spots will be closed up, and a circular and evenly-illuminated disc of illumination of a larger size will result. The wheel of diaphragms, or a series of graduated diaphragm discs to drop into a holder, is intended for critical work; the diaphragm can always be recorded, and the identical illuminating cone reproduced.

Hence we have a simple method of graduating apertures between any two contiguous diaphragms; if, for example, we place the lever to the left, so that the lens may be separated as far as possible, and use a No. 6 diaphragm, and if, on examining the object, it is thought that the illuminating cone is not large enough, and if when No. 7 is turned on it is found too much, we can go back to No. 6, and by turning the lever 60° towards the right, closing the lenses and increasing the power a little, we shall obtain an aperture somewhere between Nos. 6 and 7 diaphragm. Thus we can by means of the correction collar graduate the aperture with the facility as with an iris, and we can record any particular aperture with a degree of accuracy foreign to the iris. It must be admitted, however, that the cone of light transmitted by the condenser is a very small one.

Powell also supplies an apochromatic oil-immersion condenser, numerical aperture 1·40, but without collar correction; Fig. 134 shows the sliding tube lowered by arm A and cell B withdrawn for changing stops, which can be done without altering the focus of the condenser. Fig. 134a shows the cell B closed and raised by arm A close to the back lens of optical combination. In Fig. 134b six of the principal stops are shown. Powell’s dry apochromatic condenser, of nearly 0·9 aplanatic cone, is also very good; but the high price of all is a bar to their more general use. The speciality of these is the conversion of axis light into condensed oblique incident light by the refraction of the condenser.

Messrs. R. & J. Beck have various forms of achromatic condensers, some of which partake of a somewhat elaborate arrangement; others are simple and inexpensive, to suit the students’ microscope; as when the light of the concave mirror proves insufficient for any object requiring intense transmitted light, an achromatic condenser must be adapted to even the students’ form of microscope. The latest form of condenser (Fig. 135) is fitted with revolving stops and iris diaphragm, and other appliances for obtaining satisfactory results.

Beck’s Compound Illuminating Apparatus (Fig. 136).—It is useful in working with the microscope to be enabled to rapidly change the illumination, and for this reason this compound form of condenser has been constructed. It consists of an upper portion A, a wide-angle condenser, the aperture of which can be reduced at will by an iris diaphragm, moved by the lever B. This can be used for all other purposes. Below this diaphragm is a plate C, which can be swung back out of position at will, as shown in outline. Into a cell in this plate the stops D can be dropped, and the condenser can be used for dark field illumination, or for high powers as an oblique illuminator. A large-size polarising prism E, fastens to the plate C, and can be removed when not required. In this way any of the various modes of illumination may be separately or conjointly obtained.

Their condenser (Fig. 137) has a large aperture, and facilities for rotating the series of diaphragms. It is available for either dry or immersion objectives up to 1·3 numerical aperture on diatoms, and wet or dry histological objects. The spherical form of the front is worked by a milled-head that rotates a series of lenses and diaphragms. It also avoids the inconvenience of having the connecting fluid drawn away by capillary attraction, as would be the case if mounted on a flat surface. It is also less in the way of the sub-stage movements.

The Parachromatic Condenser of Messrs. Watson (Fig. 138) was made to meet a demand for a condenser giving a large solid cone of illumination free from colour. The optical part of this condenser consists of a full hemispherical front lens, and the middle and back combinations of such forms as to produce the necessary corrections. The Jena phosphate crown and silicate flints are used in its manufacture, and to these are due its special qualities. The total aperture of the condenser is 1·0, and it yields an aplanatic aperture of ·90 numerical aperture. The magnifying power is ²⁄₇ths of an inch. From this it will be seen that it is especially suitable for use with high-power objectives.

It can also be employed without the front lens, when the magnifying power is ⁴⁄₁₀ths of an inch, and the numerical aperture ·35. It is mounted in an exceedingly convenient manner, the iris diaphragm being fitted in such a way as to be absolutely central with the optical system.

The arc through which the handle controlling the iris travels is divided, and indicates the aperture at which the condenser may be working at any time. An important feature in this condenser is that it is almost wholly free from colour. As a rule condensers of the same form are found difficult to work with, because of the small diameter of the field or back lens. This difficulty has been successfully overcome by increasing the size of this lens, and the whole of which is fully utilised.

Most London opticians have their own especial form of achromatic condenser, designed for and fitted to their several stands and objectives, varying from a small price to the more expensively-fitted accessories.

Messrs. Swift’s illuminating apparatus (Fig. 139) is conveniently supplied with numerous useful appliances. The optical combination A is computed to be used as an effective spot lens from a 3-inch objective up to a sixth. C C are two small milled heads by means of which the optical combination A is centred to the axis of the objective. The revolving diaphragm E has four apertures for the purpose of receiving central stops, oblique light discs, and selenite films. D is a frame carrying two revolving cells, into one of which a mica film is placed, which can be revolved with ease over either of the selenites below, whereby changes of colour can be obtained in experimenting with polarised light. The darts and P A’s indicate the position of the positive axis of the mica and selenite films, and by this means results can be recorded, etc. Either of the revolving cells can be thrown into the centre of the condenser, and there stopped by means of a spring catch; when so arranged the mica film, &c., may be revolved in its place by turning the cell D, as both cells are geared together with fine racked teeth. F is a polarising prism mounted on an eccentric arm, rendered central when in use, or thrown out, as seen, when out of use. G is the rack dove-tail slide for indicating and focussing the condenser on the object. The advantages associated with this condenser consist in having the polarising prism, selenite films, dark-ground, and oblique light stops, so that they may be brought close under the optical combination.

Baker’s Nelson Condenser, shown in Fig. 140, is intended for use with their medium instruments. It has, however, many pieces of apparatus essential to those of a higher class. It is applicable, indeed, to all instruments having sufficient depth beneath the stage to receive it. It comprises an achromatic combination of 90° aperture, available with all powers up to ¹⁄₈-inch tinted glass for neutralising the yellow rays of artificial light, focussing adjustment, dark-ground illuminator, large diaphragm with rotating tube to carry oblique light stops, small wheel of apertures, polarising prism with two selenite films, clear aperture, and oblique light-shutter for low powers.

Baker’s Students’ Condenser (Fig. 141) is designed to take the place of Abbe’s, and costs much less. It transmits a larger aplanatic cone of light, and can be used either with high or low powers by removing the front lens. It is equally useful for photo-micrographic work.

Mr. J. Mayall’s semi-cylinder or prism for oblique illumination (Fig. 142) is a convenient form, as it permits of the semi-cylinder being tilted and placed excentrically; in this manner, without immersion contact, and by suitable adjustment, a dry object can be viewed with any colour of monochromatic light. If placed in immersion contact with the slide, the utmost obliquity of incident light can be obtained. Objects in fluid may be placed on the plane-surface of the semi-cylinder, and illuminated by ordinary transmitted light, or rendered “self-luminous” in a dark field, as with the hemispherical illuminator or Wenham’s immersion paraboloid. A concave mirror with a double arm is quite sufficient to direct the illuminating pencil. This semi-cylinder was originally made by Tolles, of Boston, for measuring apertures, but, at Mr. Mayall’s suggestion, Messrs. Ross mounted it as an illuminator.

The spiral slot should be fixed close beneath the larger lens of the condenser, and when properly arranged will be found a convenient mode of obtaining oblique light.

The Webster-Collins Universal Condenser (Fig. 143) is so well known that it scarcely calls for any lengthy description. It is an inexpensive form of condenser, designed in the first instance for use with the students’ microscope. It is fitted into the sub-stage; has an iris diaphragm as well as a series of revolving diaphragms moved by a milled head screw arrangement.

Oblique Illumination.

Wenham’s Parabolic Condenser.—Mr. Wenham’s many useful additions to the microscope and its accessories demand especial notice. When mention is made of the various immersion condensers (illuminators, as he preferred to call them), his original right-angled prism, his truncated hemispherical lens, his immersion paraboloid, and his reflex illuminator, in which rays beyond the angle of total reflexion are utilised by reflex action from cover-glass on to the surface of the object, every one of these well-devised inventions will always be spoken of in terms of praise. All in their turn conferred a great service upon the microscope, and enabled the student to clear up difficulties that stood in the way of developing structure when achromatic lenses and dry-objectives were considered perfect. The superior illumination of the object was wholly due to, and effected by, reflected rays from the object to the aperture of the objective, and obviously, reflex action could only take place with dry-objectives. This reflex action must be regarded as Mr. Wenham’s special discovery. It must be observed, however, that it is not the same as the more modern achromatic appliances used for throwing direct rays upon the object, and which proved the existence of apertures capable of direct transmission up to 27° measured in the body of the front lens.

The most practical of Mr. Wenham’s inventions is probably the hemispherical lens, since adopted by Messrs. Ross in connection with their excellent Zentmayer stand, and which has proved eminently serviceable. But the fact is that devices of the kind for obtaining direct oblique light require a thin stage, and therefore most of those who possess the earlier-made microscope stand would doubtless hail the appearance of any appliance which will convert axial light into oblique light; as by so doing the possessors of such instruments, in which the stage is generally of considerable thickness, would enjoy the pleasure of seeing the best resolution it is possible to get with their dry-objectives.27

Wenham’s Parabolic Reflector.—This will be better understood by reference to Fig. 145, which represents it in section A B C, and shows that the rays of light r r′ r′′, entering perpendicularly at its surface C, and then reflected by its parabolic surface A B to a focus at F, can form no part of the largest pencil of light admitted by the object-glass and represented by G F H; but an object placed at F will interrupt the rays and be strongly illuminated. A stop at S prevents any light from passing through direct from the mirror.

In the microscope the parabolic reflector fits into the cylindrical fitting under the stage, and the adjustment of its focus upon the object is made by giving it a spiral motion when fitted in—that is, carefully pushing it up or down at the same time that it is turned round by the milled edge B B. It must then be focussed by the rack and pinion motion. As the rays of light must be parallel when they enter it, a flat mirror, which in this case should be added to the instrument, is generally used; daylight will then require only direct reflection, but the rays from an artificial source will have to be made parallel by placing a side condenser between the light and the mirror, about 1¾ inch from the former and 4½ inches from the latter. Nearly the whole surface of the mirror should be equally illuminated; this may be tested by temporarily placing upon it a card or piece of white paper. Parallel rays can also be obtained from the concave mirror, if the light is placed about 2½ inches from it. Dark-ground illumination is not suitable for very transparent objects—that is, unless there is a considerable difference in their index of refraction, or they are pervaded by air-cells.

One very remarkable example of this may be seen in the tracheal system of insects. If any of the transparent larvæ of the various kinds of gnat be mounted in gelatine and glycerine jelly, slightly warmed but not enough to kill the insect outright, about the third day the fluids circulating in the body will be absorbed and replaced by air. Illuminated by the parabolic condenser, and viewed with a binocular microscope, and a low power, the gnat-larva becomes a superb object. The body of the insect is but faintly visible, and in its place is displayed a marvellous tracheal skeleton, with the tubes standing out in perspective, shining brilliantly, like a structure of burnished silver. Unfortunately, such objects are not permanent, for when the whole of the water dries up, the tracheal tubes either collapse or become refilled with fluid.

As to the blackness of field, and luminosity of the object, this depends upon excess of light from the paraboloid received beyond the angle of aperture of the object-glass. It is found in practice that more and more of the inner annulus of rays from the paraboloid has to be stopped off, until at last, with high-angled objectives, it is scarcely possible to obtain a black field.

The light, on the whole, most suitable for this method of illumination is lamp, the rays of which should in all cases be rendered more parallel by means of a large plano-convex lens, or condenser.

Wenham’s Immersion Condenser.—Mr. Wenham, in the year 1856, described various forms of oblique illuminators, one of which was an immersion; a simple right-angled prism, connected by a fluid medium of oil of cloves. This, however, was abandoned for a nearly hemispherical lens connected with the slide, and although an improvement, did not touch the point of excellence Mr. Wenham was looking for. Ultimately he adopted a semi-circular disc of glass of the exact form and size represented in the drawing, Fig. 146, having a quarter-inch radius, with a well-polished rounded edge, the sides being grasped by a simple kind of open clip attached to the sub-stage, the fluid medium used for connecting the upper surface with the slide being either water, glycerine, or oil; an increase of oblique illumination being obtained by swinging the ordinary mirror sideways. By means of an illuminator of the kind difficult objects mounted in balsam are resolved. This simple piece of glass collects and concentrates light in a marvellous manner, and is by no means a bad substitute for some of the more costly forms of achromatic condenser. It can be used either in fluid contact with the slide, or dry, as an ordinary condenser.

Mr. Wenham subsequently contrived a small truncated glass paraboloid, for use in fluid contact with the slide; water, glycerine, oil, or other substance being employed as a contact medium. The rays of light in this illuminator, being internally reflected from a convex surface of glass, impinge obliquely on the under surface of the slide, and are transmitted by the fluid uniting medium, and internally reflected from the upper surface of the cover-glass to the objective. To use the reflex illuminator efficiently it must be racked up to a level with the stage. The centre of rotation is then set true by a dot on the fitting, seen with a low power, a drop of water is then placed on the top, and upon this the slide is laid. Minute objects on the slide must be found either by the aid of a low power, by their greater brilliancy, or by rotating the illuminator; the effect on the podura scale is superb, the whole scale appearing dotted with bright blue spots in a zig-zag direction. Objects for this illuminator should be especially selected and mounted.

The Amici Prism, originally designed for oblique illumination, consists of a flattened triangular glass prism, the two narrower sides of which are slightly convex, while the third or broadest side forms the reflecting surface. When properly used, it is capable of transmitting a very oblique pencil of light. The prism is either mounted, as in Fig. 147, for slipping into the fitting of the sub-stage, or on an independent stand, as arranged for Powell’s microscope, page 85, Fig. 56.

Method of Employing the Achromatic Condenser to the Greatest Advantage.

Its Illumination.—Good daylight is the best for general work. The microscope should be placed near a window with a northern aspect. Direct sunlight should never be utilised; the best light is that reflected from a white cloud. A good paraffin lamp is the most serviceable artificial source of light, and it is quite under control. As an illuminant more often brought into requisition in the smoky atmosphere of towns, the paraffin lamp is on the whole the handiest and the most useful. If gas-light can be brought into use as suggested for micro-photography, with the incandescent mantle, it will be found to be the purest and best form of artificial illumination for the microscope. Among paraffin lamps those constructed by Baker and Swift are all that can be desired.28

As the chimneys of these lamps are made of metal, and blackened, no reflected light disturbs the eye. Care must be taken to have the wick evenly trimmed; the metal chimney has a glazed front, giving exit to the rays of light, the flat of the flame being used with low powers, and the image of the flame being reflected by a plane mirror to give equal illumination of the whole field. In working with high powers, the lamp is turned with the flame edge-wise, and at the same time the mirror must be dispensed with. By working, as it is termed, directly on the edge of the flame, the illumination is greatly increased, and a band of light can be concentrated on any part of the preparation it is desired to make a careful study of.

To obtain the best results, time and care must be given to the illumination of the object. The lamp and microscope having been placed in position, a low power is first used and the smallest diaphragm. On looking through the microscope it will probably be observed that the image of the diaphragm is not in the centre of the field; by moving the centring screw of the condenser this may be adjusted. The low power is then replaced by a high power, the largest diaphragm used, and the bacteria or diatom brought into focus. The diaphragm must now be replaced by one of medium size, and by racking the condenser up and down, a point will be arrived at when the image of the edge of the flame appears as an intensely bright band of light. If this is not exactly in the centre of the field the centring screw of the condenser must again be adjusted. With regard to the use of diaphragms, various sizes should be tried while focussing with the fine adjustment, at the same time using the correction colour; in this way we obtain the sharpest possible image. When the condenser has been accurately centred, it will still be necessary to focus it for each individual specimen, so as to correct for difference in the thickness of slides and the layers of mounting medium. Correction for different thickness of cover-glasses must be made by the aid of the collar adjustment in the following way: a high-power eye-piece is substituted for the ordinary eye-piece, and the faults in the image will thereby be intensified. By moving the collar completely round, first in one direction and then in the other, while carefully observing the effect of the image, it will be seen to become obviously worse whichever way the collar is turned. The collar must then be turned through gradually diminishing distances until an intermediate point is reached at which the best image results with the high-power eye-piece, and on replacing this by the low-power eye-piece the sharpest possible image will be obtained.

Effect of the Sub-stage Condenser.—The sub-stage condenser gives the most powerful illumination when it has been racked up until it almost touches the specimen. It produces a cone of rays of very short focus, and the apex of the cone should correspond with the particular bacterium or group of bacterias under observation. The effect of the condenser without a diaphragm is to obliterate what Koch has termed a structure picture. If the component parts of a tissue section were colourless and of the same refractive power as the medium in which the section is mounted, nothing would be visible under the microscope. As, however, the cells and their nuclei and the tissues do not differ in this respect, the rays which pass through them are diffracted, and an image of lines and shadows is developed. If in such a tissue there were minute coloured objects, and if it were possible to mount the tissue in a medium of exactly the same refractive power, the tissue being then invisible, the detection of the coloured objects would be much facilitated. This is exactly what is required in dealing with bacteria which has been stained with aniline dyes, and the desired result can be obtained by the use of the sub-stage condenser.

If we use the full aperture of the condenser the greatly converged rays play on the component parts of the tissue, light enters from all sides, the shadows disappear, and the structure picture is lost. If now a diaphragm is inserted, so that we are practically only dealing with parallel rays, the structure picture reappears. As the diaphragm is gradually increased in size the structure picture gradually becomes less and less distinct, while the colour picture, the image of the stained bacteria, becomes more and more intense. When, therefore, bacteria in the living condition and unstained tissues are examined, a diaphragm must be used, and when the attention is to be concentrated upon the stained bacteria in a section or in a cover-glass preparation the diaphragm must be removed and the field flooded with light—(Crookshank).

The wide-angle condenser, it will be understood, consists of a combination of lenses, which concentrate all the light entering them to a small point, and the condenser must be so accurately focussed that this brilliant cone of light, when it emerges from the upper lens of the condenser, falls upon the object from all directions, forming a wide-angle cone of light, at the apex of which the object must be placed (see Fig. 149). That is to say, the object is illuminated by a cone of rays passing through it in all directions.

There are, however, objects which require a fully illuminated field, when the lamp should be turned round and the Herschel lens condenser (shown in section, Fig. 148) should be used to collect the light and throw it upon the mirror. For moderate powers, as a four-tenth or one-fifth, the condenser should be used a little below the focus to give an even illumination over the whole field. Moreover, as to the use of the condenser for defining general objects, it must be borne in mind that to show different kinds of structure different apertures in the iris diaphragm are necessary, and that whereas some objects show their structure better with a large angle of light cut down in intensity by the use of blue glass, others show better with a small pencil of direct rays. For the resolution of diatoms it is often necessary to use oblique light only, and for this purpose diaphragms with central patches are used, the iris diaphragm being opened to its full extent. An annular ring of oblique light emerges from the condenser upon the object, and it is in this manner also that dark-ground illumination is obtained with moderate and low powers.

THE DIAPHRAGM.

The early form of diaphragm in use was that shown in Fig. 150.

It consists simply of a circular brass plate with a series of circular openings of different sizes, arranged to revolve upon another plate by a central pin or axis, the last being also provided with an opening as large as the largest in the diaphragm-plate, and corresponding in situation to the axis of the microscope body. The holes in the diaphragm-plate are centred and retained in place by a bent spring in the second plate, which rubs against the edge of the diaphragm-plate and catches in a notch. The blank space shuts off the light from the mirror when condensed light is about to be used. It is usually made to fit in under the stage of the microscope. This has been almost superseded by the iris diaphragm, originally designed by Wales, of America. It was made by this optician for his working students’ microscope. An early form of the iris diaphragm is seen in Fig. 151. By pressing upon the lever handle at the side the aperture gradually closes up, and without for a moment losing sight of the object under examination.

The Mirror.

The mode in which an object is illuminated is, in the words of the late Andrew Ross, “second only in importance to the excellence of the glass through which it is seen.” To ensure good illumination the mirror should be in direct co-ordination with the objective and eye-piece; it must be regarded as a part of the same system, and tending by a combined series of acts to a perfect result. Illumination of the object is recognised as of three kinds or qualities—reflected, transmitted, and refracted light. For the illumination of transparent objects, transmitted light is brought into use; for opaque objects, reflected light is needed.

The mirror should be about 2½ or 3 inches in diameter, and it must not be fixed, but made to slide up and down the stem under the stage, so that the rays of light emanating from it may be brought to a focus. The utility of the mirror is so obvious that it is occasionally passed over in silence by writers. To myself it appears to be an important accessory of the microscope, and I shall therefore proceed to combine theory with practice in what I have to say with regard to the mirror.

The microscope mirror should be the segment of a true sphere, and its centre that of a true curvature. If the mirror has a true circular boundary, the central point on line A (Fig. 152) of the reflecting surface, is the pole of the same. The line A C is known as its principal axis, and any other straight line through C, which meets the mirror, is its secondary axis. When the incident axis is perfectly parallel to the principal axis, the reflected rays converge to a point F, its principal focus. So much for the theory of the mirror. Now we come to its practical use.

Simple as the mirror of the microscope may appear to be, if the curve of the surface is not perfect, it will yield a secondary reflection or double pencil of rays. The plane mirror will occasionally be found to emit more than one reflection of the lamp-flame; this we find may be corrected by rotating the mirror in its cell. Many years ago I proposed to meet a difficulty of the kind by arranging a rectangular prism on a separate stand, shown in Fig. 153, consisting of a prism A B, mounted in gimbal C, D, and E, secured to a brass tube G, fitted to the stem, and thus made to take the place of the mirror.

The direct method of employing the mirror, that more generally resorted to, is by reflecting rays from the concave surface; the plane surface is preferred when the condenser is used. Whichever is employed, it should not be forgotten that the optic axis must be preserved throughout, and so brought to the centre of the open tube of the microscope. Another method is to interpose a bull’s-eye lens, and in this way supply the mirror with a beam of parallel rays of light. The plane side of the bull’s-eye lens should be turned towards the lamp, so that lamp, bull’s-eye, sub-stage condenser, and objective, are brought into an exact line, the bull’s-eye being set at right-angles to the line. A piece of thin white paper held across the bottom of the sub-stage will serve to show whether the rays of light are fairly parallel. The next care is to focus the object on the stage, and then the sub-stage condenser on the slide; further correction should be made by means of the centring screws of the sub-stage, or by moving the bull’s-eye lens or lamp slightly, thus perfecting the arrangements for working with parallel rays of light.

Accessories of the Microscope.

The accessories and appliances of the microscope have become so very numerous, that any attempt to describe them and explain the uses to which they are put would demand more space than I find myself in a position to bestow upon them. I must therefore confine my remarks to those accessories in more general use.

Having described the method of employing transmitted light, I have a few words to add with regard to the illumination of opaque objects by reflected light. A very early and efficient form of opaque illumination is the well-known Lieberkühn. This has not been entirely surpassed by more recent inventions. The concave speculum termed a Lieberkühn, so named after its celebrated inventor, directly reflects down upon the object the light received either from the mirror or bull’s-eye lens. It consists of a silver cap, which slides over the objective (Fig. 154), a indicating the lower part of the compound body, and b the objective over which slides the Lieberkühn, c; the rays of light are collected to a focus upon the object at d. The object may either be mounted on a slip of glass, or held by the stage-forceps, f; if very small, or transparent, it may be gummed to the dark well, e, or mounted on a Beck’s opaque disc-revolver.

This holder will be found useful for the examination of opaque or other objects that cannot be conveniently held by the stage forceps, the specimen being temporarily attached to it by gum or gold size. The holder is intended to rotate, so that every portion of the object can be brought into view. In this way it will be found useful in the study of insects, foraminifera, &c.

With the Lieberkühn, however, the illumination of opaque objects must be more or less one-sided, and therefore, the silver side-reflector has superseded it for general use (Fig. 157). To ensure a more perfect illumination of the object, the bull’s-eye lens should also be used. Mr. Sorby devised a reflector to fit over the objective. It consists of a semi-circular cap; is, in short, a modification of the parabolic reflector. The light from the mirror can, by slightly varying its inclination, be brought into use with this reflector.

The silver side-reflector is usually made with a ball-and-socket joint, so that it can be turned in any direction. It is secured to the stage of the microscope by the pin, which drops into a hole purposely drilled to receive it, and facility given for turning up and down, or in any position. If daylight is used the microscope should be placed in such a position that the light from a white cloud falls upon the speculum, but the light of the lamp is far more manageable for use with the reflector.