Imaging Formulae for Lenses in Arbitrary Media
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These formulae allow for the possibility of distinct and completely
arbitrary refractive indices for the object space medium (refractive
index n), lens (refractive
index n'), and image space medium
(refractive index n"). In this situation,
the effective focal length assumes two distinct values,
namely f in object space
and f " in image space, as shown in the
figure below. It is also necessary to distinguish the principal points
from the nodal points. The lens serves both as a lens and as a window
separating the object space and image space media. |
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| Symmetric lens with disparate object and image space indices |
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The nodal points are indicated by N and N". A ray directed at the primary nodal point
N of a lens appears to emerge from the secondary nodal
point N" without change of direction. Conversely, a ray
directed at N" appears to emerge from
N without change of direction. At the infinite
conjugate ratio, if a lens is rotated about a rotational axis orthogonal to the
optical axis at the secondary nodal point (i.e., if N"
is the center of rotation), the image remains stationary during the rotation.
This fact is the basis for the nodal slide method for measuring nodal-point location.
The nodal points coincide with their corresponding principal points when the image
space and object space refractive indices are equal ( n
= n"). This makes the nodal slide method the most
precise method of principal-point location. The situation of a lens immersed in a homogenous fluid is included as a special case ( n = n" ). This case is of considerable practical importance. The two values f and f " are again equal, so that the lens-combination formulas are applicable to systems immersed in a common fluid. The general case (two different fluids) is more difficult, and it must be approached by ray tracing on a surface-by-surface basis. |
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Lens Constant (k) |
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This number appears frequently in the following formulas. It is an explicit function of
the complete lens prescription (both radii, tc
and n' ) and both media indices (n and
n" ). This dependence is implicit anywhere that
k appears. |
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Effective Focal Lengths |
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Lens Formula (Gaussian form) |
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Lens Formula (Newtonian form) |
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where x = s
- f and x" =
s" - f " |
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Principal-Point Locations |
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Object-to-First-Principal-Point distance |
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Second-Principal-Point-to-Image |
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Magnification |
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Lens Maker's Formula |
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Nodal-Point Locations |
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Separation of Nodal Point from Corresponding Principal Point |
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Back Focal Length |
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Front Focal Length |
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Focal Ratios The focal ratios are f /f and f /f, where f is the diameter of the clear aperture of the lens. |
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Numerical Apertures |
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| where | |
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Solid Angles |
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| where | |
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| and | |
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| where | |
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To convert from steradians to spheres, simply divide by 4p |
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| Optics Guide Copyright 2002 Melles Griot Inc. |






















