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| Application Notes |
Lens TheorySinglet Lenses - NomenclatureBelow is a common diagram used to define quantities for the analysis of a singlet lens. The quantities defined can also be extended to multi-element systems by procedures outlined in optical design textbooks. |
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| The optical axis (O-O) of the lens is a line passing through the
centres of curvature
of the two spherical lens surfaces (centres of curvature not shown). Ray A is incident from left to right and parallel to the optical axis. Ray A is refracted to point F2 on axis, the back, second, or secondary focal point. Ray B is incident from right to left and parallel to the optical axis. Ray B is refracted to point F1 on axis, the front, first, or primary focal point. Suppose the lens is "well-corrected" That means all rays A parallel to the axis are focused to a single point F2, regardless of their distance from the axis. It is clear then that the family of rays refracted to F2 intersect the family of progenitor rays A in a sphere centred at F2. This sphere, or, in general, surface of intersection of progenitor and refracted rays is called the back, second, or secondary principal surface. The intersection H2 of this surface with the optical axis is called the back, second, or secondary principal point. Similarly, rays B incident from the right, and their refracted rays impinging on F1, intersect to form a front, first, or primary principal surface, which intersects the optical axis at H1, the front, first, or primary principal point. In the paraxial approximation, all ray angles are small. This approximation permits the modelling of the principal surfaces as principal planes. The distances from the front and back principal points to their respective focal points are equal and given by f , the focal length or effective focal length. The front and back focal distances FFD and BFD, respectively, are measured from the surface intersections V1 and V2 to the respective focii. V1 and V2 are called the front and back vertices. To calculate these quantities above we need sign conventions.
The formulas below now permit the calculation of the effective focal length, front and back focal distances, and positions of the principal points of a singlet lens in the paraxial approximation. The distance tc below is the centre thickness of the lens V1V2. |
| Important Quantities for Singlet Lenses Immersed in Air |
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| For plano convex, plano concave, equiconvex and equiconcave lenses, we give the focal lengths in the table found on the following page. (Principal plane data may be calculated using the tables above.) |
| Focal Length Formulas for Simple Singlet Lenses in Air The Radii are considered positive in the formulas below. |
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In the singlet lens tables in this catalogue, focal lengths at a few key wavelengths are
given. We also give very accurate radii of curvature and centre thickness data for each
lens. Use the formulas in the above table and the values for n given in the index of
refraction tables at the end of this chapter.Performance and Proper Orientation of Singlet Lenses for Minimum Spot SizeHigh quality singlet lenses are of particular interest in laser focusing and beam handling applications because of their low cost, high damage threshold, and availability of a large variety of standard parts. We offer a large selection of BK7, UV grade fused silica, and SF11 singlets that can satisfy most monochromatic focusing requirements. Can singlet lenses provide diffraction limited performance in the focusing of collimated beams? Examine the figure below. |
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This figure is a geometrical ray trace of 25 rays in the focal region of a 100 mm
focal length BK7 plano convex lens(n = 1.515). The lens is oriented with the plano
surface towards the focus and the origin (0 mm) is at the back vertex (V2) of the lens.
The rays were launched parallel to the axis and equally spaced in a region 16 mm above and
below the axis in a plane containing the axis (meridinal plane). Therefore, the
lens is operating at the rather "fast" aperture of f/3.125. The marginal rays
reach the axis first, in plane MP. The paraxial rays reach the axis last, at
the paraxial focal plane PP. The distance from V2 to PP is the back
focal distance (BFD) of the 100 mm focal length lens. This can be verified using
the formulas previously defined. The distance from PP to MP, here negative,
is the longitudinal spherical aberration LAm of the
marginal rays. The beam width in the paraxial focal plane PP is the transverse
spherical aberration TSAm,determined by the heights of the
marginal rays. Notice that the smallest geometrical spot size can be found at plane MS,
approximately 3/4 LAm back toward the lens from the paraxial focal
plane.Shape FactorFor singlet lenses, the smallest beam diameter dMS at plane MS can be computed from third order aberration theory. The result is: dMS = f where
where d0 is the input beam diameter and K is the shape factor of the lens given by: K = R2 / ( R2 -R1) Note that the lens orientation is contained in K. The angular blur is plotted on the next page as a function of shape factor for three typical glasses used in our singlets. |
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| Geometrical optics angular spot size for spherical singlet lens for indices of refraction typical of fused silica, n = 1.4942 at 280.0 nm, BK7, n = 1.5205 at 514.5 nm, and SF11, n = 1.7648 at 800.0 nm. A collimated beam is assumed incident on R1. To use this graph, find the shape factor of the lens using the proper sign conventions for R1 and R2. Read the angular blur, in units where d is the beam diameter and f is the focal length. Now calculate the actual angular blur in radians by multiplying by (d0/f)³. Finally, multiply by the focal length to obtain the spot size in units of length. If the value is much less than the diffraction limit, performance of the lens will be limited by diffraction rather than spherical aberration. |
| Three important points should be noted: |
For this example,
(K = 1), we compute a geometrical optics minimum beam size LAm = -4f² The minimum spot size occurs at a distance s2 = BFD - 3 / 4 LAm from the rear vertex of the lens. In this example, LAm = -2.82 mm and s2 = 93.92 mm. A 226 µm spot size obtained by focusing a 32 mm diameter collimated beam is hardly diffraction limited. We have purposely chosen a highly aberrated situation as an example. The diffraction limited full angle angular blur with aperture limited by the beam diameter d0 is: |
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| implying a diffraction limited spot size of: |
ddiff = f |
| This is the diameter of the first dark ring of the Airy pattern in the focal plane.
For the above example, ddiff = 4.8 µm at a wavelength of 632.8 nm.
Comparing the aberration limited geometrical optic spot size f If f
If f |
Additional Notes
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| ©2006 | Last update: January 2006 |