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Books I. and II, L Books III. and ÏV., Is. 6d. Books I.-IV., in one ELEMENTARY TREATISE O' PLANE TRIGONOMETRY. By E. W. HORS M.A., Fellow of Christ's College, Cambridg University Lecturer in Mathematics, and C. M. JESS M.A., Fellow of Clare College, and Assistant Ma Reading School. 4s. 6d. AN and inestimably valuable theory itself. The" elementary" character of this is at least questionable. Beyond this that most important factor in the diffraction theory in its practical application, Numerical Aperture, is wholly without explanation, save such as arises from its technical introduction and employment; but there are few points on which it is more important that an elementary student should be more clearly instructed, and there are few that lend themselves more to efficient diagrammatic presentation. In the same relation it may be noted that the very essential formula n sin u-expressing the general relation discovered by Abbe between the pencil of light admitted into the front of the objective, and that emerging from the back lens of the same, which is such that the ratio of the semi-diameter of the emergent pencil to the focal length of the objective could be expressed by the sine of half the angle of aperture (u) multiplied by the refractive index of the medium (#) in front of the objective or n sin. u—but this is a German mathematical formula; and its English equivalent is μ sin. 4, and although the German form of symbol is employed in England, and thoroughly understood by mathematicians, those who are entering for the first time upon a study of this difficult subject, and therefore unaccustomed to the mathematical formulæ em 66 'elementary" source of their information leaves them without a hint on the subject. Sele Its author has aimed apparently at an elementary treatise on the microscope, which is nevertheless intended to cover almost the entire field involved in its history, production, and use. The difficulties of such a task are not a few. To be elementary and thoroughly popular upployed, might readily fall into confusion, seeing that the to a limit, very sharply defined, and then to lead on those who choose to follow into the deeper aspects of this manysided subject, is at once practical and natural. The optics of the modern microscope are the possession of the specialist. Abbe himself has failed to make them accessible to and understanded by any but those educationally equipped. Hence the constant misunderstanding of the fundamental principles of the Diffraction Theory and its related applications so frequently manifest even where the subject is supposed to be more or less familiar. As might have been readily supposed, the author of this treatise has given evidence of skill in the presentation of the main points of elementary optics; it is, however, clearness and conciseness, not originality, that is to be noticed. The illustrations are those familiar to English text-books for the last quarter of a century, and the diffraction theory has in no way been simplified to the reader of an elementary treatise by that most efficient of all elementary modes of imparting ideas on more or less abstruse subjects, viz. carefully devised and well-explained diagrams. Considering the object of this treatise, viz. the impartation of knowledge to those not mathematically prepared to follow it in that direction, by giving a concise, clear, and comprehensive view of the meaning and application of the diffraction theory of microscopic vision, the transition from the first to the second chapter will be so abrupt and unlinked as to leave the elementary reader practically in the dark. The chapter on "The Theory of Microscopic Vision" is unexceptional so far as it goes. It cannot be other, it is Prof. Abbe's; but in a treatise claiming to maintain its elementary character more completely than any other similar work which covers so wide a range this is surely not enough. The diffraction theory of vision is introduced to the tyro with no explanation of what diffraction is, and with no illustration of its action until he is plunged in medias res in Abbe's application of it to the profoundly important Another serious defect, as we believe, in this mentary presentation of the diffraction theory of microscopic vision is the absence of an easy explanation of the photometrical equivalent of different apertures. Certainly it is not of the essence of the problem, but it is just one of those points which in a very marked and instructive manner illustrate the meaning and value of numerical aperture as such; and for elementary exposition this must be of importance. Thus, if two circles be taken to represent the backs of two objectives of the same power but of different apertures, and the radius of one be twice that of the other, then each radius will represent the angle n sin. u. But because the areas of these circles are to each other in the proportion of the squares of their radii, it follows that if each radius be designated by n sin. u, the area of the lesser circle will be to the area of the greater circle as the square of the radius of the former is to the square of the radius of the latter. Hence the area of the greater circle will be four times as great as that of the lesser, which teaches that since the numerical aperture of one objective is twice as great as that of another its illuminating power will be four times as great-a most important incidental and explanatory raison d'être for great N. A. In this connection we notice what is certainly not easily explicable as an exposition of the details of Abbe's great theory. On page 56 of "The Microscope" Dr. Van Heurck almost incidentally states the very important fact that "Prof. Abbe has satisfactorily established the fact that a certain relation inust exist between magnification and angular (?) aperture." This is undoubtedly one of the most important demonstrations of the theory. Great numerical apertures have proved of untold value to the competent student of minute details, by opening up structures that mere amplification must have left for ever impenetrable. But that does not annul the import ance of small apertures. Low amplifications are as useful in their own department as high ones; and to put great apertures to lower magnifying powers than such magnifying power warrants is to sin against the elementary principles of the Abbe theory of vision. And on the other hand, wide apertures can never be utilised unless there is a concurrent and suitable linear amplification of the image which is competent to exhibit to the eye the smallest dimensions which are by optical law within the reach of such apertures. Thus it follows that great amplification will be useless with small apertures. If the power be deficient the aperture will not avail; if the aperture be wanting nothing is gained by high power. The law is, "Employ the full aperture suitable to the power used." In Abbe's words, "A proper economy of aperture is of equal importance with economy of power." "1 Taking these facts, then, which are apparently recognised by Dr. Van Heurck, it is very remarkable to find on page 49, in a discussion of the "screw threads" or gauges employed by the makers of microscopes,that the general value of the English gauge is admitted, but it is added, "The English thread is not, however, all that we have to say on this matter. In America the American thread is also employed, which is considerably greater, and admits the use of lenses with a much larger diameter, and thus offers certain advantages. In the first place, the larger the lens the easier it is to make, and consequently the real curvatures approach closer to the calculated curvatures; then the larger the lens the more luminous rays it admits, and this in photography is not to be despised." To our judgment this statement is a contradiction of apochromatic, object glasses, by which we can get larger the admission made on page 49, quoted above. 2 The enlargement of the screw for the purpose of putting in larger back lenses to objective combinations was first mooted in America in 1879, when "Mr. Bullock urged the desirability of adopting a uniform objective screw of larger size than the Society screw now in use (1879), as being essential to the efficacy of low power lenses of high angle." 66 This American gauge" was subsequently introduced and known as the "Butterfield gauge of screw for objectives." 3 "3 really were. They in fact made a jrds a ; ala aths a; aa; and so on. Since Butterfield's gauge was introduced, long le .:! the days of apochromatism, that is when our ignora”! allowed us to over-aperture our low magnifying powers it was tolerable, because it was evidence of exper mental effort to improve the capacity of our les But to day with the society screw we are easily provice with a series beginning with a 1 inch objective of 3. as: a inch objective of 65 N. A., and we may venture i think that these are the highest ratios of aperture power that will be accomplished for many a day; ar therefore the highest ratios allowable by the Abbe thes of vision, which we now know, at least in this point, " be an enunciation of the established laws of optics Moreover, these lenses are really difficult to make, wri their back lenses easily placed within the diameter of the Society screw. A high ratio of aperture to power alway involves great expense in production; and therefore wr find that the low-priced oil immersions of this inme diate time areths and ths, not objectives of low ma nifying power, and for this reason only. Since then the Society screw is sufficient for more than double the apertures shown by Abbe to be in sa able ratio to the lower powers, we find it more than dăcult to account for the teaching in a treatise intended te be essentially elementary, that the Butterfield screw gauge for objectives provides conditions which offer certain advantages," when the supreme object of this part of the book is to enunciate fully the nature asi qualities of oil immersion achromatic, and especiall Now, we must remember the date of the introduction of this large gauge for objectives, and its relation to the introduction of the apochromatic system of lenses. We must further remember that the purpose of its adoption was to permit the introduction of larger back lenses than the Society gauge would suffer into an objective combination. This meant giving relatively great apertures to lower powers. But this, carried beyond a certain limit, violated a fundamental law of Abbe's theory. Now it is said that these larger lenses are easier to make (!) and approach more nearly to the calculated curves But in truth objectives with wide apertures which are low powers, and must therefore have large backs, are most difficult lenses to produce. It was, in fact, to escape the difficulty of giving lower powers larger angles that opticians of the first rank always designated their objectives as of lower magnifying power than they 1 J. R. M. S., ser. ii. vol. ii. p. 304. apertures with the society screw than in the old days o In a treatise purporting to be essentially for the beginner we confess to disappointment concerning the instructions as to the "choice of a microscope." What is needed is that the tyro should know the essentials of the instrument; the points in it that are of indispensable importance, and a clear account of the manner in which these may-by the uninitiated-be seen to be of inferior or acceptable workmanship. The reader is not even in formed that in so important a matter as the adjustment there is a different value to be attached to several entirely different methods by which this function of the microscope is performed. The bar and lever movement, essentially the best in principle and practice. is only referred to as existing, in the index, which is thus made to serve as a kind of glossary; and even more remarkable is the fact that the patent lever fine adjustment of Swift and Son, the only fine adjustment which, in our judgment, makes the "Jackson Model" microscope (which Dr. Van Heurck evidently affects) at all a practicable instrument, is treated in the same way. So indeed is Campbell's differential screw; and the highest commendation is given to the form adopted in the author's own model. No doubt in its present form it is relieved of many defects incident to the form of fine adjustment to which it belongs; but it must be remembered that we are told that each of the divisions of the milled head of this fine adjustment corresponds to the 13th of a millimetre. Yet the screw which gives this fine result has to lift the whole "body" of the instrument. In the lever fine adjustments only a nose-piece is lifted, having an inconsiderable weight, and producing in practice no friction, and to this the objective is attached; it certainly appears but reasonable, as it has proved in practice to workers who have employed the several methods for continuous years, that the "wear and tear" upon so fine a screw to which such heavy work is given does not contribute to permanent steadiness, or in constant work, to continued accuracy. In fact, after careful study of the microscope specialised in this treatise, it is difficult to discover anything really new or distinctive in it save the bringing of the fine adjustment pinion of the sub-stage above the level of the principal stage. The value of this may be variously assessed, but it has the plain disadvantage of preventing the complete rotation of the principal stage; and it may be doubted if it has any advantage which will compensate for this. There is little, if anything, to enable the reader to distinguish as to the practical value of one form of stand as compared with another, and yet there can be no greater divergence in form than that between the Continental stand on the one hand with its dead weight to produce steadiness, and the two English models known as the Ross and Jackson models respectively on the other. What distinguishes them, in what either of them has superiority over the other, and wherein in any of them what is essential to a first-rate working microscope, is nowhere discussed. It is true that the models of many makers are presented and beautifully printed; but many of these are not printed in these pages as revealing essential differences important for the reader to observe, but they are placed amongst others simply as the productions, with slight variations, of the same instruments by different makers. We cannot but believe that if some plain directions had been given as to the essentials of a good microscope, and the principal models passed in review showing their conformity or otherwise to these requirements, the "elementary" object of the book would have been more fully accomplished, and the tyro more fully aided in the "choice of a microscope." Dr. Van Heurck has shown his practical knowledge of the microscope as a manipulator in many ways, in this book, but perhaps this is nowhere more fully seen than in his full appreciation of the condenser as an indispensable instrument in bringing out the finest optical possibilities of the most perfectly constructed object glasses. His book may be said to be alone amongst continental treatises on the microscope in this respect. It has been by very tardy steps that the continental makers, or the continental microscopists, have learned to appreciate the immense importance of a condenser in causing optical combinations to give their highest results. It is but recently that so leading a firm as Zeiss has yielded on this point and produced condensers. The first was chromatic, and, as a consequence, proportionately unsatisfactory. Then came the most useful achromatic form of Abbe. But we are glad to observe that Van Heurck recognises that the apochromatic immersion condenser of Powell "is the most perfect condenser which exists at present" (p. 85). It is inevitable that with apochromatic objectives it should be. We cannot possibly see how the splendid objectives on apochromatic principles can give their finest results unless they are illuminated by an apparatus which is not only as perfect in workmanship, but of as great a numerical aperture, and with as complete corrections as the objective which is collecting the light and forming the image of the object the condenser is illuminating. And for this reason, while we admit fully that the plate of photo-micrographs produced in this and other volumes by the very exceptional skill of Dr. Van Heurck with the most remarkable object glass which the manipulative skill of man has yet produced, viz. the 25 mm. with N.A. 163, is a monument to his manipulative ability, we still contend that he worked under difficulties of no small importance. The only condenser provided for this lens by the great firm which produce it, is one which of necessity has a flint front, but is as wholly uncorrected as the glasses used by Hooke or Bonanni! Now if it be important to use an apochromatic condenser at all, how much more important to use it on such a lens, with such an aperture and such exquisitely refined corrections. This objective has never yet had its best power revealed, because its illumination has been always a counteraction of its own refinements. We are surprised that in manipulation the tyro is recommended in this treatise to focus down upon the object first, of course with great care, and then to find the actual focal point by withdrawing the tube by either coarse or fine adjustment. A far more elegant and safe method is certainly adopted, and we doubt the preference expressed for daylight as the best constant source of illumination. It is uncertain and always variable and more refractory than the edge of a good lamp-flame, unless we need a monochromatic ray from a sunbeam. At the close of the book there is a communication which had appeared before in the Journ. Roy. Micro. Soc., from Dr. S. Czapski, which gives a suggestion for the possible enlargement of the practical N.A. of homogeneous object-glasses, which makes an advance to 2'0 possible without the employment of the dense flint and highly refractive media needed by the lens spoken of above. In fact it is plain that true monochromatic light may increase a N.A. of 140 to 175. There is a chapter on photomicrography which has the value that is inevitable, coming as it does from one of the most practised and efficient workers; still it can hardly be expected to be exhaustive, and every practical photomicrographer has, and adopts as most perfect, his |