Scales and modes

The page is read by an eye

A sight-reader's eye sits a fixed number of notes ahead of the sounding one and a fixation takes in a fixed number of millimetres, and the spacing rule converts between them. Two bounds follow, from the reader rather than from the music — and the one everybody would expect to bind does not. The saccade rate has enormous headroom at any playable tempo, and what decides is acuity.

Assumes: How much music a page holds · The axis that is not a time axis

How much music a page holds multiplied the two axes — the horizontal spacing rule and the vertical capacity — and got the one design constraint on notation that is not about legibility. Its last paragraph named what every quantity in the ladder leaves out.

Every quantity here is a property of the page, and a page exists to be read by somebody whose eyes move across it in saccades of a measurable size at a measurable rate.

Two facts about that reader are well measured, they are in different units, and the spacing rule is what converts between them.

Every standard rastral size against the two bounds a reader imposes. Print the notes larger and the eye-hand span stops fitting inside one fixation, so the reader has to saccade ahead faster than the eye can move. Print them smaller and a notehead stops subtending enough angle to be identified. Both bounds come from the reader and neither from the music. At 100 beats a minute with 2 notes to the beat, the acuity bound sits at 1.63 millimetres and the saccade bound at 7.5 — so the saccade rate is nowhere near binding and acuity is doing all the work, which is the opposite of what the eye-hand span suggests. 5 of the 9 standard rastrals clear the acuity bound: rastral 4 and larger. Those are exactly the sizes used for parts, and the ones below are used for study scores — which are read at a desk rather than played from at a stand, and a shorter viewing distance moves the bound with them.
Fig. 1 Every standard rastral size against the bound a reader’s acuity imposes. Five of the nine clear it, and they are exactly the five used for parts rather than for scores.

Two facts in different units

The eye–hand span is measured in notes. A sight-reader’s eye sits ahead of the note being played, and how far ahead is one of the better-studied quantities in music psychology. It is about four notes for a competent reader and rather more for an expert, and it is a note count rather than a distance — a reader confronted with wider spacing does not read fewer notes ahead, they look further along the page.

A fixation is measured in millimetres. The useful field of one fixation is a couple of degrees of visual angle, which at a music stand’s distance of half a metre is about nineteen millimetres. That is a property of the fovea and it does not care what is printed in it.

The spacing rule converts. The axis that is not a time axis is the rung about horizontal spacing: an engraver’s rule gives each note a width, in staff spaces, that is a sublinear function of its duration. Multiply by the rastral size — the physical height of one staff space, which is the one real length notation has — and a note occupies a definite number of millimetres.

At a common orchestral rastral of 1.75 millimetres and the standard spacing rule, a note occupies 5.4 millimetres, so a span of four notes is 21.5 — against a useful field of 19.2.

The span does not fit inside one fixation. Reading music is necessarily a sequence of fixations rather than a single wide view, and that is true at every part-sized rastral.

Which means the eye has to move, and easily can

The next question is whether the eye can move fast enough, and this is the bound everybody expects to bind.

One fixation covers 3.6 notes at this layout. At a hundred beats a minute with two notes to the beat, that is 3.3 notes a second, which needs 0.93 saccades a second.

The eye’s ceiling is around four a second.

So there is a factor of four in hand. This layout runs out of eye movements at 428 beats a minute with two notes to the beat, which is 14 notes a second and is not a tempo anybody plays.

The saccade rate has enormous headroom and never binds. That is the negative result of the rung and it is worth stating plainly, because the eye–hand span is the quantity the literature is about and it turns out to describe the strategy rather than the limit.

The eye-hand span does not fit inside one fixation. A sight-reader's eye sits a roughly fixed number of notes ahead of the sounding one, and a fixation takes in a roughly fixed number of millimetres, because that is what the fovea is. Those are two facts in different units and the spacing rule converts between them. At this layout a note occupies 5.4 millimetres, so a span of 4 notes is 22 millimetres against a useful field of 19 — the span does not fit, and reading is therefore a sequence of fixations rather than one. Each fixation covers 3.6 notes, and at 100 beats a minute with 2 to the beat that is 0.9 saccades a second against a ceiling of about four. There is a great deal of headroom: this layout runs out of eye movements at 428 beats a minute, which nobody plays.
Fig. 2 One note occupies five and a half millimetres and a fixation takes in nineteen, so a four-note span does not fit and the reader saccades — at one movement a second against a ceiling of four.

What does bind is the fovea

The other bound is much simpler and it is the one that matters.

A notehead has to subtend enough visual angle to be identified. Its width is about 1.18 staff spaces, so at a rastral of r millimetres it is 1.18r millimetres wide, and at half a metre it subtends an angle proportional to that. Taking twelve minutes of arc as the angle needed to identify a glyph as complex as a notehead in context gives a minimum rastral of 1.63 millimetres.

The standard rastral sizes are a series that engravers have used for two centuries: rastral 0 at 2.4 millimetres down to rastral 8 at 1.2. Against that bound:

rastral notehead clears acuity use
0 2.83 mm yes a conductor’s score in large print
1 2.60 yes an easy part
2 2.30 yes a solo part
3 2.18 yes the commonest orchestral part
4 2.06 yes an orchestral part
5 1.89 no a dense part
6 1.71 no a study score
7 1.53 no a small study score
8 1.42 no a miniature score

Five of the nine clear the bound, and they are the five used for parts. The four that do not are the ones used for study scores.

That is a division the model did not know about. The rastral series is a printers’ convention with no acoustics in it, and the point at which it crosses the acuity bound is the point at which its own conventional descriptions change from part to score.

Why the score sizes are allowed to fail

The four small rastrals are not unreadable and the model says why they are not.

The bound depends on the viewing distance. Half a metre is a music stand: a player sitting back, arms free, instrument in the way. A study score is read at a desk, at perhaps thirty-five centimetres, which is a factor of one and a half nearer — and the acuity bound scales with the distance, so it falls to about 1.1 millimetres.

At that distance every one of the nine clears.

So the rastral series is not two arbitrary halves; it is one series read at two distances, and where it divides is where the distance changes. A part is read from a stand and a score is read from a desk, and the sizes follow.

There is a second reason the small sizes are allowed to fail, and it is that a study score is generally not being sight-read. A conductor studying a score is reading at their own pace with unlimited time; a player reading a part is reading at the tempo. The saccade bound is irrelevant to both and the acuity bound is much softer when there is no time pressure.

The band a rastral size has to sit in, and where it closes. The upper line is the largest notehead the eye can still saccade past fast enough; the lower is the smallest it can identify. The band between them is where a rastral size has to be, and it narrows with tempo because the saccade bound falls and the acuity bound does not move at all. At 40 beats a minute the band is a factor of 11.5 wide; at 300 it is 1.54. It does not close inside any tempo a player meets, which is the answer to whether a page can be laid out too densely to sight-read: not by the eye's speed. The dots on the lower line are the standard rastrals, and 5 of the nine sit inside the band at every tempo here.
Fig. 3 The two bounds against tempo. The acuity bound is flat, because it has nothing to do with time; the saccade bound falls, because faster music needs more notes a second. They do not meet inside any tempo a player meets.

The band never closes

Plotting the two bounds against tempo says how much of a real constraint this is.

At forty beats a minute the band between them is a factor of eleven — any rastral at all works. At three hundred it is a factor of 1.54, which is still four of the nine standard sizes.

The band does not close at any playable tempo. So the answer to whether a page can be laid out too densely to sight-read is: not by the eye’s speed. The eye is not the bottleneck in music reading, and every difficulty a sight-reader has is somewhere else — in recognising the patterns, in the hands, in the memory.

That is a useful negative and it disposes of an intuition. The impression that a dense page is hard to read is real and it is not about the fovea’s throughput; it is about how much a reader has to decode, which is a different quantity entirely and one this ladder has no measure of.

The vertical axis has its own version of the same bound

Everything above is horizontal, and the eighth and ninth rungs measured two axes rather than one.

The vertical question is not about spacing but about discrimination: a reader has to tell a line from a space, which is a judgement about a position to within half a staff space. Half a staff space at rastral 4 is 0.87 millimetres, which at half a metre subtends about six minutes of arc — comfortably above the limit for judging whether a small object sits on a line or between two, which is a vernier acuity task and one the eye is remarkably good at.

So the vertical axis has more headroom than the horizontal, which is a small vindication of a notation that has five lines rather than more. The clef is an integer and the notations invented for the overflow are the rungs about what happens when a range exceeds what five lines carry, and the answer is always a symbol — a clef change, an octave sign, a ledger line — rather than a finer grid.

That is the right design given these numbers. Making the staff finer would trade a task the eye is very good at, judging a position against a line, for one it is worse at, resolving two nearby marks. Adding a symbol costs nothing visually and costs the reader an inference instead.

The stave is not a ruler is the ladder’s first rung and it makes the same point from the other end: the staff’s vertical axis is not linear in pitch, and it does not need to be, because what it is doing is naming positions rather than measuring distances.

The staff holds 11 positions and nothing fits in it. Each clef's eleven staff positions — five lines, four spaces and the space either side — as a bar on an axis that counts letters, with eight ranges laid underneath. The clefs step through the axis in thirds and cover fifteen positions of offset between them. Every range drawn is wider than eleven positions: the four voices span 13, 12, 13, 13 and the four instruments 24, 24, 25, 23, so the best clef for each still leaves 1 to 7 positions off the staff. A clef is a choice of which end sticks out.
Fig. 4 The vertical axis the horizontal one is being multiplied by: eleven positions per staff, with everything outside them supplied by a symbol rather than by a finer grid. Its discrimination task is easier than the horizontal axis’s identification task, which is why five lines has been enough for six hundred years.

What a page turn is, in these terms

The tenth rung’s own product was a page turn, and the reader adds one thing to it.

A page holds a number of notes, from the vertical capacity times the horizontal spacing, and at a stated tempo that converts to a number of seconds. Making the rastral smaller puts more notes on a page and lengthens the interval between turns.

The acuity bound is therefore a bound on how far that can be pushed: a part cannot be printed smaller than about 1.6 millimetres to the staff space, so a page cannot hold more than a certain number of notes, so a turn cannot be delayed beyond a certain time.

That is the one place in this ladder where the reader and the page’s arithmetic produce a single number together, and it is what the tenth rung asked for.

How much music each spacing rule fits on a page. The two axes multiplied. Vertically, a system is as tall as the staves the range needs; horizontally, a system holds as many notes as fit once the shortest is wide enough to read. proportional: 3 staves to the system, 4 systems and 27 notes to a system, 108 notes to the page — 32 seconds at 100 beats a minute, so a page turn every 32 seconds; Ross, 1970: 3 staves to the system, 4 systems and 38 notes to a system, 152 notes to the page — 46 seconds at 100 beats a minute, so a page turn every 46 seconds; Gould, 2011: 3 staves to the system, 4 systems and 40 notes to a system, 160 notes to the page — 48 seconds at 100 beats a minute, so a page turn every 48 seconds; one column a note: 3 staves to the system, 4 systems and 50 notes to a system, 200 notes to the page — 60 seconds at 100 beats a minute, so a page turn every 60 seconds. one column a note holds 1.85 times what proportional does, which is a difference of 0.85 page turns a minute — and a page turn is a thing a player with two hands occupied cannot do.
Fig. 5 The earlier product: how much music a page holds under each spacing rule, and how often it turns. The reader’s contribution is a floor under the rastral, and therefore a ceiling on how much can be crammed onto a page.

What the spacing rule is really trading

There is a reading of the horizontal rule that this essay makes available and the ninth rung could not.

The axis that is not a time axis found that every engraving rule puts a note somewhere other than where its moment is: proportional spacing is the only rule that is true to time and it wastes an enormous amount of paper on long notes, so every practical rule compresses the long ones and displaces the short ones from their moments.

That trade was presented as being between fidelity and paper. It is also a trade against the reader, and in a direction the rules get right.

A rule that compresses long notes puts more notes in a fixed number of millimetres, which raises the notes per fixation and lowers the saccade rate. Since the saccade bound has a factor of four in hand, that is buying something the reader does not need — but it also lowers the distance a reader’s span covers, which means a reader looking four notes ahead is looking a shorter way and is more likely to have the span inside a single fixation.

At the tightest practical setting the span does fit. So the rules that engravers arrived at are, among other things, rules that bring the eye–hand span toward the size of one fixation, and the sublinearity is what does it.

That is offered as a consequence rather than as a motive. Nobody was measuring fixations in the eighteenth century, and the rules were arrived at by looking at pages and judging them handsome.

It has one testable corollary. The rules differ from each other in how sublinear they are, so they differ in how many notes a fixation covers — and a reader given the same music under two rules should saccade at measurably different rates. That is a measurement on an eye-tracker rather than an arithmetic, and it is the only prediction in this rung that could distinguish the rules on the reader’s behalf rather than on the engraver’s.

The time signature is a claim is the rung about the other thing a page asserts that is not a measurement, and it is the same shape of argument: a convention that looks like a description of the music and is really an instruction to the reader.

Where a phrase sits on the page, under each rule for spacing it. The same 13 notes under four rules, each drawn at the fraction of the system's width it would occupy. The open marks are where each note falls in TIME, which is the same under every rule and is the top row. proportional puts a note as much as 0.0 per cent of the system away from its moment; Ross, 1970 puts a note as much as 5.9 per cent of the system away from its moment; Gould, 2011 puts a note as much as 6.9 per cent of the system away from its moment; one column a note puts a note as much as 11.5 per cent of the system away from its moment. Only proportional notation has no error, and no engraver uses it, because a system in which a semibreve is thirty-two times a demisemiquaver is a system with almost nothing on most of the page.
Fig. 6 Four spacing rules with the same phrase under each, and how far each one puts a note from its moment. The sublinearity that costs fidelity buys density, and density is what brings a reader’s span toward one fixation.

Which computation produced the numbers

The horizontal spacing is the engraver’s rule from the ninth rung, giving each note a width in staff spaces as a function of its duration; the vertical capacity is the eighth rung’s, giving a system’s height from the staff’s own positions plus the ledger lines a range needs.

The reader’s constants are all published figures with ranges around them, and every one is named rather than buried: a span of four notes, a useful field of two degrees, a viewing distance of 55 centimetres, a saccade ceiling of four a second, and a notehead 1.18 staff spaces wide.

The acuity criterion is twelve minutes of arc, which is generous compared with the limit for detecting a fine line and appropriate for identifying a glyph in a cluttered field.

Where the model stops

Acuity is one number for one task. Reading a notehead’s position on the staff is a much finer discrimination than detecting the notehead, and reading an accidental or an articulation is finer still. A model with one angle for everything is a caricature, and the true bound is probably set by the fine marks rather than by the noteheads.

The span is a mean. Eye–hand span varies enormously with skill, from about two notes for a beginner to eight or more for an expert sight-reader, and it varies within a performance with how predictable the music is.

Reading is not note by note. A skilled reader takes in a chord, a scale fragment or a familiar figure as one unit, so the note count that matters is a count of chunks. That makes the effective span longer in notes and does not change the millimetres.

And nothing here is about music. The whole model treats a page as a field of glyphs at a spacing, and the actual difficulty of sight-reading is about pattern recognition — which is why a hard piece and an easy piece printed identically are not equally readable. A melody is a walk, not a set is the collection’s account of what makes a sequence of pitches predictable, and predictability is what a chunk is made of.

Nor is the notation the only one. Three notations, one progression and what a tablature keeps are the rungs about systems that encode different things, and a tablature’s glyphs are numerals rather than positions — a different identification task with different acuity demands, which this model has no way to compare.

What the picture cannot show

It cannot show the page turn as an event. A turn is a hand leaving the instrument, and the constraint is about when a hand is free rather than about how much is on the page. How much music a page holds says the same and neither rung has a model of the player’s hands.

Nor can it show the second staff. A pianist reads two staves at once, which is a vertical span as well as a horizontal one, and nothing in a one-dimensional model of fixations addresses it.

And it cannot show the screen. A great deal of music is now read from a tablet at a fixed size and a fixed distance, with no page turns and no rastral series. The bounds still apply and the conventions the series encodes do not.

Whose notation, and when

The rastral series is a European engraving convention, standardised in the nineteenth century and still in use — the numbers and their conventional descriptions are what a publisher’s specification sheet contains. The spacing rules are the same tradition’s.

The reading measurements are twentieth-century experimental work, mostly on Western staff notation and mostly on pianists, and the eye–hand span in particular has been measured many times with fairly consistent results.

The historical claim the figure supports is narrow and rather satisfying. The rastral series was arrived at by printers balancing cost, legibility and the size of a sheet of paper, over a long period, with no measurement of anybody’s eye. It divides exactly where a modern account of visual acuity says it should, and the division is between the sizes read at a stand and the sizes read at a desk. Nobody designed that boundary and everybody has been using it.

Where this ladder goes next

Eleven rungs. The stave is not a ruler; two names for one key; the time signature is a claim; a mark that is not a level; what a tablature keeps; three notations for one progression; the clef is an integer; the notations invented for the overflow; the axis that is not a time axis; the two axes multiplied; and now the eye that has to cross them.

What the ladder owes now is the chunk. Every quantity above counts notes, and a reader does not read notes — they read figures, and a scale fragment of eight notes is one object where eight unrelated pitches are eight. That is the difference between a sight-readable page and an unreadable one, and it is not a property of the layout at all. This collection has an account of what makes a sequence of pitches predictable, on the melody ladder, and applying it to a page would give the first quantity in this anchor that depends on what the music is rather than on how it is printed.

Part 11 of 18

One essay in the series on notation. The essays either side of this one:

What links here

Essays that reach for this one mid-argument — the half of a link its own author cannot write down.

The objects named here

The third way in, after the field and the series: the things themselves, and every essay that touches each one.

AcuityEngravingNotationPage turnReadingSaccadeSight-readingStaff