SIMETRIUM SIMETRIUM .COM 1 D = 1 m⁻¹
optics of the eye
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Z(2.2) 0.42 µm Ø 6.0 mm · 41×41 L 24.0 mm −6−4−20+2 SYMBOL PLATE SE −2.50 D n′ 1.336 ISO 24157 · λ 840 nm
Letter case
Capital Latin D. Prescriptions also use dpt. In essence it is m⁻¹.
Do not confuse
Not to be confused with the prism dioptre Δ, the debye D and the day d.

On the plate is a cross-section of the eye. The crystalline lens thickens, then relaxes. A beacon beam leaves the macula, and the wavefront exits the eye towards the sensor. The sensor is the letter D itself: inside it you can see the grid of microlenses, the astigmatism map turns, and the scan line runs from top to bottom. The mark on the scale moves from zero to −2.50 D.

Unit passport · non-SI · optical power

Dioptre

Unit of optical power equal to the reciprocal metre · quantity: optical power and vergence

In half a minute a laser removes a layer thinner than a hair from the cornea, and the eye starts to see without glasses. The surgeon works out how much to remove in dioptres. With a 6 mm optical zone, one dioptre of myopia is about 12 µm of tissue. The whole eye refracts light with a power of about 60 D, and an error of one sixtieth is already enough to blur the letters on the chart.

Symbol
D · dpt
In SI terms
1 D = 1 m⁻¹
Definition
F = n / f — the power of a lens with a focal length of 1 m in air
Standard
ISO 13666 · ISO 24157 (aberrations)
Prescription step
0.25 D; cylinder axis in 1° steps from 1 to 180
Typical values
−2.50 D — glasses for myopia · 43 D — cornea · 60 D — whole eye
To the conversion → To the history →
01 · Definition

Lens power is the reciprocal of focal length

A lens with a focal length of one metre has a power of 1 D. A focal length of half a metre gives 2 D, ten centimetres gives 10 D. A diverging lens gets a minus sign. Glasses for myopia have minus lenses, glasses for hyperopia have plus lenses.

The beauty of dioptres is that they add up. Light from a point 0.5 m away reaches the eye with a vergence of −2 D: that is what opticians call the curvature of the wavefront. The cornea adds its 43 D, the crystalline lens about 20 D more. If the sum brings the front to a focus exactly on the retina, the image is sharp. If not, the difference in dioptres is the prescription.

Inside the eye, light travels in a medium with an index of 1.336, so there vergence is divided not by the distance but by the distance divided by n. The cornea and the optical centre of the lens are almost 6 mm apart, and this gap also changes the sum. The lab below works through all of this step by step.

f — focal length, n — refractive index of the medium, d — gap, S — optical zone, mm
m⁻¹
in SI units
L⁻¹
dimension
± 0.25
prescription step, D
Interactive · vergences add up
Where a lens focuses the light of a lamp
On the left is a point source; its wavefront spreads out. The blue arcs are the front before the lens, the violet ones after it. The number above each arc is its vergence. If the sum is positive, the front converges to a point on the right.
left: source V′ = V + F
before the lens
after
image
The eye as a stack of lenses
Cornea, front surface+48.8 D Cornea, back surface−5.9 D Crystalline lens, relaxed — accommodating+19 … +33 D Whole eye, Gullstrand model+58.6 D
The total is less than a simple sum, because the lenses are separated by a gap. Two thirds of the eye's power comes not from the crystalline lens but from the cornea. That is why a laser can change vision by working on the cornea alone.
Interactive · refraction lab

Measure the eye, correct it and see the world as it does

On the left is a cross-section of the eye at true size: cornea, crystalline lens, length from cornea to retina. Blue rays come from the object, violet ones are the two principal meridians in astigmatism, and the coral dot is where they meet. Top right is the patient's view: the picture is blurred by the eye's point spread function. Bottom right is the screen of the selected instrument. Below the scene is the visual acuity scale, logMAR.

left: eye, scale 1 mm = 11 pxD · logMAR · µm
Patient
Instrument
Looking at
Correction
Refraction
—
—
Focus error
—
—
Acuity
—
—
Accommodation
—
—
Cornea
—
—
Visual acuity, logMAR—
normal · ≤ 0.0
0.1—0.3
0.3—0.5
worse than 0.5
−0.20.00.30.51.0
—
02 · Conversion

Dioptres, focal length and old lens numbers

Optical power
Strong glasses and a contact lens with the same effect carry different numbers. Glasses sit 12 mm in front of the cornea, so for −8 D glasses the contact lens needs only −7.30 D.
Until the 1870s lenses were numbered by their focal length in inches. Lens No. 40 has a focal length of 40 inches, about 0.9 D. Inches differed from country to country, so the numbers did not match.
03 · Orders of magnitude
Optical power from the prescription step to a ball lens, D

04 · Measuring instruments
−2.50 D · ISO 8598
lensmeter
Power of a finished lens
Light from a target passes through the spectacle lens. The instrument moves the target until the cross is sharp and converts the shift into dioptres.
IR S −2.25 C −0.50 × 178
autorefractor
A prescription in three seconds
An infrared band sweeps across the pupil. From where and how fast the reflection from the retina moves, the instrument finds the sphere, cylinder and axis.
Δx ∝ ∂W/∂x
Hartmann–Shack aberrometer
A map of the whole wavefront
A grid of microlenses splits the wavefront leaving the eye into hundreds of beams. The shift of each spot is the slope of the front. Zernike coefficients are built from these shifts.
CL₁L₂R24.02 mm
OCT biometer
Eye length to the micron
An interferometer finds the reflections from the cornea, the crystalline lens and the retina. A length error of 0.1 mm gives a prescription error of about 0.27 D, which is why the eye is measured with light before lens replacement.
05 · Writing rules
Correct
−2.50 D — a sign and two decimal places
sph −1.25 cyl −0.75 ax 180 — sphere, cylinder, axis
Add +2.00 — the addition for near vision
1 D = 1 m⁻¹
Incorrect
2.5 — without a sign it is unclear whether it is plus or minus
ax 0° — the axis is written from 1 to 180; zero is written as 180
−2.5 dptr. — symbol without a full stop, power in hundredths
D = 1 / f (cm) — the focal length is taken in metres
06 · Neighbouring units
07 · Historical section
1619 · 2 holes
Scheiner disc
Metrological note
Two holes from 1619 inside a machine

The Jesuit Christoph Scheiner pricked two holes in a card and looked at a needle through them. If the eye is in focus, there is one needle. If not, there are two, and the way they split shows which way the error goes. Almost all autorefractors still work on this principle: the instrument finds the power at which the two beams meet at one point on the retina.

the two beams meet
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