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The thread: Not a projection at all — page 3

Every theorem quoted on this site is a theorem about a map through a centre. Water is not one; a real lens is not one. Rather than mention that and move on, these essays measure what survives and what does not — a cross-ratio 1.2% out where the pinhole is exact to the last bit, a bundle of rays that misses its own centre by ten millimetres, and the two things that survive anyway. Essays 49 to 64 of 64.
undone: near 3e-12 px · far 3e-12 pxturning 1 rad/s The rectangle behind the lens

A turning frame can be straightened; a travelling one cannot

Read a frame row by row while the camera turns at a radian a second and every point is 21 px from where a global shutter would put it, at every depth alike. Turn each row's rays back and every point returns to six trillionths of a pixel, with no depth known. Travel at 3 m/s instead, and the best correction that needs no depth is exact at one distance and 21 px wrong at 2 m.

00.50011.5020123where a pinhole would put the point, in focal lengths from the centrewhere the model puts itwhere the polynomial foldsthe division model's horizonboth at k = -0.42fold 42° · horizon 1.54 The real instrument

A model that inverts has a horizon instead of a fold

The polynomial every calibration fits turns around at a finite radius and stops being a map from direction to picture. The division model, chosen because it inverts in closed form, never turns around — it rises for ever toward a horizon at one over the root of its own coefficient, so the whole hemisphere of directions lands inside a finite disc. Fitted to the four fisheye laws over seventy-five degrees it follows every one of them three to five times more closely, and below sixty the polynomial is still the better model.

78.510.5142142105105078.510.51421421051050where the horizontal slit sits (m)where the vertical slit sits (m)8 with a centre, 17 with a measurenone with both What each system gave up

The exclusion is two conditions, not ten rows

Ten systems have been measured and none has both a centre and a true measure. Ten is not a proof. Swept across the whole two-slit family — eighty-one members, both parameters run out to infinity — a centre appears at exactly the eight members whose slits sit at one finite distance, a measure at exactly the seventeen with a slit at infinity, and at none of them both. The case the two conditions appear to leave open is closed by the rays themselves: one divide is a slit, and eight page points use 6.02 m of it.

-7.50-5-2.5000123how far the projector stands from the eye, log₁₀ mmwhat the seat is left with, log₁₀ pixels1 pxcurved television as a wall, the seat at 3 ma pixel by 50 mm · exact at zero The second projection

A projector in the viewer's eye

A projector paints a wall along its own rays, so from the projector's own position the wall's shape is invisible — exactly, on a cylinder, on a dome and on a plane alike. Move a hand's breadth away and the residual is pixels. The one place a projector can stand and ignore the shape of what it is throwing onto is the eye of the person watching.

eyethe stickcorrect from 18 cm, at 160 mm widerays miss by 3.13 mm Through water and glass

The stick a stereo pair puts back

Two eyes side by side reconstruct a submerged stick exactly as the sagittal image — kinked 14.96° — and two eyes one above the other exactly as the tangential one, kinked 9.59°. Roll the baseline between them and the two rays to a point miss each other by up to 3.13 millimetres, past the 2.85 a pixel covers at that range, and the reconstruction is a third stick that is neither — 551 millimetres of a one-metre stick, with its tip at 0.405 metres against a true 0.866.

toward the designup63 mm apart10 mm14 mm across36 mm along the sight line Where to stand

An anamorph has one eye

From the design point exactly — a camera's single eye — the floor marks give the design back to sixteen decimal places. A head carries two eyes 63 mm apart, and neither of them is the design point. The difference between the disparity the floor gives and the disparity an upright board would give runs to 47 arcminutes, against a stereoacuity of a few tens of arcseconds. This is why pavement paintings are photographed.

0.313100510how far away the subject is, in metreshow far the pupil moves forward, in millimetres0.50 mthe whole walk with field anglea 50 mm lens, focused as one pieceequal at 0.50 m The real instrument

Focusing moves the pivot past its best place

Focusing a fifty-millimetre lens to one metre carries its entrance pupil 2.63 millimetres forward of the camera body, and to half a metre 5.56 — which is more than the whole 5.53 that the pupil walks with field angle, so past a subject at 502 millimetres the focus decides where the pupil is. A panorama head aligned at infinity and used at a metre leaves 7.46 arcminutes along its seam; aligned at four metres it leaves 2.21, better than pivoting at the pupil at all.

the pivottangent circle, 30.0 mmno single viewpoint — the rays miss by 24.98 mm6 frames · pivot 60 mm off Surfaces that are not flat

The pivot that is not the eye

A camera bolted to a tripod turns about the screw under its baseplate, and the light crosses somewhere else. Every ray of the panorama that results passes the pivot by e sin γ — the offset times the sine of how far off its own frame's axis the ray points — so the picture has a radius where a projection would have a point.

0204060204060frames in the panoramadistance from the pivot (mm)π/β = 9.5across the seamup the framepivot 60 mm · frame 38° tallfloor 19.53 mm Surfaces that are not flat

The parallax you cannot shoot away

A stitched panorama's parallax has two halves and they do not behave alike. The one across the seam falls as the sine of half a frame spacing, so more frames buy it off; the one up the frame is the sine of half the frame's own height, and no quantity of shooting touches it. They cross at π over β, which has no pivot error in it at all.

25102050131030how far away the object really is, in metreshow far away it appears, in metresa flat mirrortwo metres of radiusboth axes logarithmic · the eye 0.8 m from the glassceiling 1.30 m Mirrors that are not cameras

Closer than they appear, by a factor with a number in it

A wing mirror of one metre radius held eighty centimetres from the eye reports 1.30 metres for an object at sixty-four, because the image of anything distant sits half a radius behind the glass. The size such an object subtends reads as a distance 2.60 times the true one, and the factor is exactly one plus twice the eye's distance over the radius — so the warning is a number, and it is larger for the mirror that is further away.

-500500.5001distance to the thing being stitched (log₁₀ metres)what the stitch leaves behind (px)2.86 m80 mm baselinezero at one depth each Surfaces that are not flat

A rig is right on one surface

Several cameras looking outward have several centres, and no warp registers all of a scene. The residual is a disparity, so the depth the stitch is computed for has an exact optimum — the harmonic midpoint of the depth range, not the middle of it — and the arithmetic middle costs a factor of 2 z_far over the sum, which tends to two.

rule A — ordinaryrule B — blendedmix = 0.0207.80 px Systems that kept the measure

Two stations in one picture

A parallel floor under a perspective room found one map absorbing two centres into one sheet. Split a two-rule picture down the middle instead and each half hands back its own horizon — 7.80 px apart at a rule-mix of 0.02 — and no eye's position has anything to do with the gap, because an ordinary pinhole picture's recovered horizon does not depend on where the eye stood at all.

drawn along a fixed direction, not from a pointelevation 52°centre-fit refused Systems that kept the measure

What a removed wall costs that a removed roof does not

Fitting a single centre to a building with its near wall deleted lands at 3.0e-15 m — the arithmetic floor — because deleting a wall does not touch the projection, only which surfaces are drawn. Fitting the identical routine to the same building with its roof removed does not return a number at all: handed a bundle of genuinely parallel rays, it refuses outright.

five points · worst 2.10 px5 straight lines, drawn as arcs between their vanishing pointsworst 2.10 px at 40° of tilt Surfaces that are not flat

The arcs the five-point construction actually draws

The taught five-point construction draws circular arcs between five vanishing points and instructs a draughtsman to graduate the radius evenly. Read that way, the arcs miss a straight line's true image by up to 3.75 pixels on a 300-pixel disc. Read at the stereographic scale instead, the same arcs are exact to 4.3e-13 pixels — the construction was always drawing one projection, and the taught scale was never it.

column 62 mmcorrect from 19 cm, at 160 mm wide0.966% hidden, to 15.3° from the nadir Surfaces that are not flat

The hole a rig cannot fill

A two-lens spherical rig covers every direction between its two lenses and still cannot see 0.470 per cent of the sphere directly beneath it, reaching 12.8 degrees from straight down — its own tripod, standing exactly where neither lens can look. No arrangement of lenses removes it, because it is not a gap in coverage; it is the rig occluding itself.

0.050.10.20.5125105101520braccia in the pavement, drawn to one page widthpixelsthe diagonal, by straightedgethe transversals, by fittingboth read on one pavement47× at eight braccia Drawn confidently

The rule is exact for a floor that lengthens

The constant-ratio rule for spacing receding boards is an exact perspective — to the last digit, on the panel's own horizon — of a floor whose boards grow by the inverse of the ratio, 0.74 braccia deep at the front and 1.31 at the back on an eight-braccio pavement. The orthogonals agree with that floor. What says the tiles were meant to be square is a diagonal, which bends 8.1 pixels off straight where the reader's fitting test finds a sixth of one.

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