Letters & Lettering: A Treatise with 200 Examples. Frank Chouteau Brown

Letters & Lettering: A Treatise with 200 Examples - Frank Chouteau Brown


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      An excellent model for constructing the Roman capitals in a standard form will be found in the beautiful adaptation by Mr. A. R. Ross, 1 and 2, from an alphabet of capitals drawn by Sebastian Serlio, an Italian architect, engraver and painter of the sixteenth century, who devised some of the most refined variants of the classic Roman letter. Serlio's original forms, which are shown in 39 and 40, were intended for pen or printed use; but in altering Serlio's scheme of proportions it will be observed that Mr. Ross has partially adapted the letter for use in stone, and has further varied it in details, notably in serif treatment. In most modern stone-cut letters, however, the thin strokes would be made even wider than in this example, as in 14. Mr. Ross's adaptation shows excellently how far the classic letters do or do not fill out the theoretical square.

      Width proportions, which may be found useful in laying out lettering for lines of a given length, are shown in 3 in a more modern style of the Roman capital. In the classic Roman letter the cross-bar is usually in the exact center of the letter height, but in 3 the center line has been used as the bottom of the cross-bar in B, E, H, P, and R, and as the top of the cross-bar in A; and in letters like K, Y and X the "waist lines," as the meeting points of the sloping lines are sometimes called, have been slightly raised to obtain a more pleasant effect.

      The Roman alphabet, although the one most in use, is unfortunately the most difficult to compose into words artistically, as the spacing between the letters plays a great share in the result. The effect of even color over a whole panel is obtained by keeping as nearly as possible the same area of white between each letter and its neighbor; but the shape of this area will be determined in every case by the letters which happen to be juxtaposed. Individual letters may, however, be widened or condensed to help fill an awkward "hole" in a line of lettering;—the lower lobe of the B may be extended, the center bar of the E pulled out (in which case the F should be made to correspond), the lower slant stroke of the K may be used as a swash tail, and the R may have its tail extended or drawn closely back against the upright line, and so on. Indeed, each and every letter of the alphabet is susceptible to such similar modifications in shape as may make it best suit the space left for it by its neighbors. Observe, for example, the spacing of the word MERITAE in 34, and notice how the tail of the R is lengthened to hold off the I because the T on the other side is perforce held away by its top. In the page of capitals, 124, by Mr. Bridwell, see also how the different spacing of the word FRENCH in the first and second lines is managed. In the advertisement, 123, also by Mr. Bridwell, note how the letters are spaced close or wide in order to produce a definite effect. The whole problem of spacing is, however, one of such subtle interrelation and composition, that it can only be satisfactorily solved by the artistic sense of the designer. Any rules which might be here formulated would prove more often a drawback than a help.

      Certain optical illusions of some of the Roman letter forms should be briefly mentioned. These illusions are caused by the failure of certain letters to impinge squarely with determining serifs against the demarking top and bottom guide lines. The round letters C, G, O and Q often seem to be shorter and smaller than the other characters in a word unless the outsides of their curves run both above and below the guide lines. For the same reason S should be sometimes slightly increased in height, though in this case the narrowness of the letter makes less increase necessary; and J, on account of its kern, is governed by the same conditions as S, save when letters with distinct serifs come closely against it at the bottom. Theoretically the right side of D would require similar treatment, but actually this is seldom found necessary. The pointed ends of the letters V and W should, for similar optical reasons, be extended slightly below the bottom guide lines, the amount of this extension being determined by the letters on each side of them. In the A, the Roman letterer at first got over the optical difficulty caused by its pointed top by running this letter also higher than its neighbors; but he later solved the problem by shaping its apex as shown in I, thus apparently getting the letter into line with its companions while still obtaining a sufficient width of top to satisfy the eye. Because of its narrowness, I should generally be allowed more proportionate white space on either side of it than the wider letters.

      Some idea of the proportionate variations required to counteract the optical illusions of the letters above named may be obtained from the practice of type-founders. In making the designs for a fount of type, it has been customary to first draw each letter at a very large size. Taking an arbitrary height of twelve inches as a standard, the points of A and V were made to extend about three-quarters of an inch above or below the guides, the letter O was run over about half an inch at both top and bottom, and the points of the w were made to project about the same distance. In pen lettering, however, it is possible and preferable to adapt each letter more perfectly to its individual surroundings by judgment of the eye than to rely upon any hard and fast rules.

      Certain variations between the stone-cut forms of the Roman letters and their forms as drawn or printed should be understood before an intelligent adaptation of stone forms to drawn forms, or the opposite, is possible. When drawn or printed a character is seen in black against a white ground with no illusory alterations of its line widths caused by varying shadows. In stone-cut letters, on the other hand, where the shadows rather than the outlines themselves reveal the forms, different limitations govern the problem. The thin lines of a letter to be V-sunk should generally be made slightly thicker in proportion to the wide lines than is the case with the pen-drawn letter, especially as the section is likely to be less deeply and sharply cut nowadays than in the ancient examples, for the workmanship of to-day seems to be less perfect and the materials used more friable. A slight direct sinkage before beginning to cut the V-sunk section is a useful method of partially atoning for modern shallow cutting, as shadows more directly defining the outlines are thus obtained. The student should, however, be warned at the outset that all reproductions or tracings from rubbings of ancient stone-cut letters are apt to be more or less deceptive, as all the accidental variations of the outlines are exaggerated, and where the stone of the original has been chipped or worn away it appears in the reproduction as though the letter had been actually so cut.

      

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      The photograph of a panel of lettering from the upper part of the Arch of Constantine, Rome, shown in 6, well indicates the effect of shadows in defining the classic Roman letters; and the effect of shadows on an incised letter may be clearly observed by comparing 4 and 5, the former showing a drawing for an inscription in which the Serlio-Ross alphabet was used as a basis for the letter forms, and the latter being a photograph of the same inscription, as cut in granite. It will be noted how much narrower the thin lines appear when defined only by shadow than in the drawing. The model used for the lettering on the frieze of the Boston Public Library, Скачать книгу