Low Vision Formulas Flashcards

1
Q

Moderate Low Vision

A

20/70 - 20/160

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2
Q

Severe Low Vision

A

20/200 - 20/400

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3
Q

M units

A

Metric distance at which lower case letter would subtend 5 min of arc.
20/50 = 1.00M = 8N = 1.45mm ht = 0.40 logMAR

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4
Q

Feq

A

Equivalent power, total dioptric strength needed by patient to achieve their near visual goal

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5
Q

Kestenbaum rule

A

BCVA: denom/numerator for 1M (reciprocal of vision), and then do Kest/goal if their goal is something other than 1M.
Ex. Kest/0.5M would be twice as much power needed than for 1M goal

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6
Q

Effective Mag

A

D/4

Ex. +20/4 = 5X

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7
Q

Conventional Mag

A

(D/4)+1

Ex. +20/4 +1 = 6X

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8
Q

F1

A

Lens held away from spec plane

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9
Q

F2

A

Lens at spec plane (the ADD)

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10
Q

c

A

Separation of the lenses

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11
Q

JND

A

Denom when numerator is 20 of BCVA (better eye), show the lenses +/- half of the JND

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12
Q

How to find Feq for a near goal with near VA given

A

(Working distance D) near VA / goal VA
Ex. Patient with 0.4/3.2M VA wants to see 0.6M —> (3.2/0.6)(+2.50) = +13.33D Feq

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13
Q

Microscopes (spec-mounted convex lenses)

A

Feq = F2
- largest FOV, but poor working distance, RDM, focal length is of the prescribed microscope, but remember to include pt’s eye’s inherent power in the calculation (myopes require less plus, hyperopes require more plus), remember convergence demand issue

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14
Q

Convergence demand for microscope lenses

A

Need to add BI if between +4 and +12 lenses, BI = D + 2 for each lens

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15
Q

Hand-held magnifiers

A

Feq = F1, RDM and angular mag.
For spot reading mostly, held at focal length from reading material. Use long formula if using it with an ADD. Feq = F1 + F2 - cF1F2 where c is the distance bw HHM and ADD

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16
Q

Break-even point

A

1 focal length of magnifier from spectacle plane

17
Q

FOV and HHM

A

FOV decreases as HHM is moved away from the eye. FOV = d*f/h where d is the lens diameter, f is focal length, and h is the lens to eye distance

18
Q

Stand magnifiers

A

Feq = ER x F2, RDM and angular mag. Requires an add. Object to lens distance is fixed, with an upright virtual magnified image.

Enlargement ratio ER = U/V
V=U+P
Wd=1/F2= [z+v]
z is distance between specs/add and the F1 magnifier

19
Q

Electronic magnification

A

Feq = TM x F2
TM = image height/object height
F2 is the add (1/wd)
Good for large Feqs and poor VAs, but expensive

20
Q

Telemicroscopes

A

Feq=TS x F2
RDM and angular mag, F2 is the reading cap (on objective lens)

21
Q

Mag

A

Does not provide clarification, but produces a large enough retinal image for identification

22
Q

Relative distance magnification

A

Original object to eye distance / new object to eye distance
Most common form of mag in low vision devices, like bringing something closer to the eye

23
Q

Relative size magnification

A

new object size / original object size , or final object height / original object
Large print books, increasing font size

24
Q

Angular magnification

A

Ratio of angular size of the image to the angular size of the object at whatever distance the object is located, without changing object size or viewing distance. Ex. Telescopes, HHM, SM

25
Q

Transverse magnification aka lateral or linear mag

A

Final height of image / original height of image
Ex. Overhead projector

26
Q

Telescope mag formulas

A

M= -Doc/Dobj
M= ent pupil diameter / exit pupil diameter

27
Q

Distance of lenses in a telescope formula

A

d= fobj+foc

28
Q

Tube length and power of telescope

A

Increasing tube length, decreases power

29
Q

Keplerian

A

(+) ocular, (+) objective, longer tube length, larger FOV, better image quality. Exit pupil floats outside system. REAL and INVERTED image.
More expensive, higher powers. Uncorrected myope will increase the mag

30
Q

Galilean

A

(-)ocular, (+)objective, shorter tube length, <4X powers, exit pupil fills ocular lens diameter,lower cost, easier use. VIRTUAL and UPRIGHT image. Uncorrected hyperope will increase mag

31
Q

Reverse telescopes

A

Expands FOV by minifying