Optics Flashcards
Prentice’s Rule
Prismatic power of lens is:
Delta = hD, where h is distance from optical axis in cm (not mm) and D is power of lens
Prismatic effect of glasses on deviations
2.5 x D = % difference
Minus measures more
Plus measures less
Basic lens formula
U + D = V
U = vergence entering lens D = power of lens V = vergence exiting lens
Power of a spherical surface in a fluid
Ds = (n-n’)/r
n-n' = diff in refractive indices R = radius of curvature
Power of a thin lens immersed in fluid
Dair/Dfluid = [n(lens) - n(air)]/[n(lens) - n(fluid)]
Transverse/linear magnification
M(L) = I/O
Image height over object height
Axial magnification
Mag of depth
Max = [M(L)]^2
ie square of linear mag
Angular magnification
Ma = D/4
Vertex distance and magnification
1 mm increase of vertex distance
- increases mag by 0.1% x D for plus lens
- decreases mag by 0.1% x D for minus lens
Aniseikonia
Every 1 D anisometropia between the two eyes produces 2% aniseikonia
Unilateral aphakes have 25% with spectacles, 7% c CTL, 2.5% c IOL.
Can usually tolerate ~6-7% (3 D).
Astronomical telescope
Aka keplerian
2 plus lenses; distance apart is sum of FL
Higher power is eyepiece; inverted image
Galilean telescope
Strong minus lens (eyepiece) and weak plus lens (obj). Distance btwn is sum of focal lengths
Erect image (ie loupes)
Telescope formulas
Angular Mag: Ma = -De/Do
Accommodation thru telescope: At = An (Ma)^2, where An = normal accommodation
SRK formula
P = A - 2.5AL - 0.9K (emmetropia)
For other target RE: Diol = P - (R/1.5), where R is desired RE
Define:
Apical alignment
Apical bearing
Apical clearance
Apical alignment: RGP has same BC as K
Apical bearing: RGP has rests on K BC too flat
Apical clearance: RGP is steeper (smaller BC) than K