Clinical Optics Made Easy: Vergence, Prisms and Magnification
Last updated: October 2026
Optics frightens residents because it is taught as a page of formulas. In practice almost every clinical optics question comes back to a handful of ideas: vergence, the far point, prisms, accommodation and magnification. Learn these and the formulas become common sense.
Five ideas
1. Everything is vergence: U + P = VVergence is 1 ÷ distance in metres (dioptres). Light from a real object diverges (negative), a lens adds its power, and the result tells you where the image forms. An object at 25 cm has a vergence of −4 D.
2. Correct the far pointA myope sees clearly only out to the far point, 1/D metres in front (−2 D → 50 cm). The correct lens has its focal point at the far point. Moving a lens changes this: a plus lens moved away from the eye becomes stronger, a minus lens becomes weaker.
3. Prisms bend light to the base, images to the apexOne prism dioptre moves the image 1 cm at 1 m. Prentice's rule: prism (Δ) = decentration (cm) × lens power (D). 1° is about 1.75 Δ.
4. Accommodation shrinks with age; keep half in reserveA comfortable near add = the near demand minus half the amplitude of accommodation.
5. Magnification depends on where the lens sitsSpectacles magnify (plus) or minify (minus) by about 1.5–2% per dioptre; contact lenses hardly change image size. Simple magnifier: M = F ÷ 4.
Two pictures to keep in your head: the far point, and how a prism moves an image.
Numbers worth knowing
Fact
Value
Use
Power of the reduced eye
About 60 D (cornea ≈ 43 D, lens ≈ 17–20 D)
Basis of most calculations
Axial length error
1 mm ≈ 3 D of refraction; ≈ 2.5–3 D of IOL power
Why biometry must be accurate
Keratometry error
1 D of K ≈ 1 D of IOL power
SRK formula
P = A − 2.5 L − 0.9 K
Historical; modern formulas are more accurate
Retinoscopy working distance
67 cm → subtract 1.50 D; 50 cm → subtract 2.00 D
Neutralisation point → refraction
Indirect ophthalmoscope magnification
60 ÷ lens power (20 D lens ≈ 3×; 28 D ≈ 2.2×)
Lower power lens = more magnification, smaller field
Direct ophthalmoscope magnification
About 15× (60 ÷ 4)
Mirror power
F = 2 ÷ r (r in metres)
Keratometry uses the cornea as a convex mirror
Prism dioptre to degrees
1° ≈ 1.75 Δ
Converting strabismus measurements
Effective power and vertex distance
When a lens moves towards the eye by d metres, its new power is F ÷ (1 − dF). If it moves away, use + d. It matters above about ±4 D: a −10.00 D spectacle lens at 12 mm becomes about −8.90 D at the cornea, so the contact lens is weaker for a myope and stronger for a hyperope.
Memory hook: Contact lens for a myope: minus less. Contact lens for a hyperope: higher plus.
Astigmatism in three sentences
A cylinder has no power along its axis and full power at 90° to it. Light through an astigmatic system forms two focal lines (the conoid of Sturm) with the circle of least confusion at the spherical equivalent.
With-the-rule: the vertical meridian is steepest (plus cyl at 90 or minus cyl at 180), common in the young. Against-the-rule is common in older people.
Transposition: add the cylinder to the sphere, change the cylinder's sign, rotate the axis by 90°. −1.00/+2.00 × 90 = +1.00/−2.00 × 180.
Memory hook: The plus-cylinder axis lies along the steep meridian. Jackson cross-cylinder: refine the axis first, then the power; keep the spherical equivalent constant by changing the sphere half as much in the opposite direction.
Accommodation by age
Approximate averages; published tables (Donders, Duane) differ by a dioptre or so.
Age (years)
Amplitude (D, approx.)
Near point
10
14
7 cm
20
10
10 cm
30
7
14 cm
40
5
20 cm
45
3.5
29 cm
50
2.5
40 cm
60 and over
1 or less
1 m or more
Worked example: a 50-year-old emmetrope (amplitude 2.5 D) wants to read at 40 cm (demand 2.5 D). Keep half (1.25 D) in reserve, so the add is 2.5 − 1.25 = +1.25 D. A higher add brings the reading distance closer and narrows the range.
Prisms in practice
Prentice's rule: 5 mm decentration of a +6 D lens gives 0.5 × 6 = 3 Δ.
Base direction for a decentred lens: plus lenses act like two prisms base to base, so decentring a plus lens in gives base-in prism; minus lenses give the opposite.
Correcting a deviation: the apex points the way the eye turns: esotropia → base-out, exotropia → base-in, right hypertropia → base-down over the right eye.
Vertical imbalance in anisometropic bifocal wearers when reading: fix with slab-off (bicentric grinding) on the more minus lens.
Magnification and aniseikonia
Knapp's law: in axial ametropia, a spectacle lens at the anterior focal point of the eye (about 15 mm) gives a retinal image the same size as an emmetrope's. So axial anisometropia tolerates glasses; refractive anisometropia (aphakia, post-keratoplasty) does better with contact lenses.
Most people tolerate about 5% aniseikonia (roughly 2–3 D of spectacle anisometropia).
Low vision: magnification needed = target acuity ÷ current acuity, as decimals (from 6/60 to 6/12 is 0.5 ÷ 0.1 = 5×). A +20 D magnifier gives 5×.
Telescopes: M = − eyepiece power ÷ objective power. Galilean (plus objective, minus eyepiece) is short with an upright image; Keplerian (two plus lenses) is longer and needs a prism to turn the image upright.
Purkinje images
Image
Surface
Type
I
Front of the cornea
Upright, virtual, brightest (used in keratometry and Hirschberg test)
II
Back of the cornea
Upright, virtual, faint
III
Front of the lens
Upright, virtual, largest; moves with accommodation
IV
Back of the lens
Inverted, real (the back of the lens acts as a concave mirror)
Where residents slip
Forgetting the working distance in retinoscopy: subtract 1.50 D at 67 cm.
Mixing up which way the image moves through a prism: the light bends to the base, the image shifts to the apex.
Using the full amplitude of accommodation to calculate a reading add: keep half in reserve.
Ignoring vertex distance above ±4 D when converting glasses to contact lenses.
Giving glasses to a high refractive anisometrope (unilateral aphakia): the aniseikonia is too large; use a contact lens or IOL.