Refraction at Curved Optical Surfaces and Paraxial Optics

Vergence and Wavefront Optics

  • Definition of Wavefront: A wavefront represents the locus of points having the same phase of oscillation. The curvature of a wavefront as it propagates through space defines its vergence.

  • Definition of Vergence: Vergence is the quantitative measure of the extent of convergence or divergence of incident or emergent light rays.

  • Mathematical Formula for Vergence: An inverse relationship exists between vergence and the distance from the wavefront to the point source or point focus:

Vergence=1distance-to-source\text{Vergence} = \frac{1}{\text{distance-to-source}}

  • Determinants of Wavefront Vergence:

    • Distance from the point of interest on the wavefront to the source (or focal point).

    • Refractive index (nn) of the medium in which the light rays are traveling.

  • Units of Vergence:

    • Measured in reciprocal meters (m−1\text{m}^{-1}), universally referred to as Diopters (D\text{D}).

  • Diverging Rays:

    • Light rays originating from a point object spread outward.

    • Represented by negative vergence (−ve-\text{ve} vergence).

Diverging Wavefronts
  • Parallel Rays / Light from Infinity:

    • When light originates from a source at infinity, the wavefronts are flat (plano).

    • Because the distance to the source is infinite, the curvature is zero:

Vergence=1∞=0\text{Vergence} = \frac{1}{\infty} = 0

Parallel Wavefronts
  • Converging Rays:

    • Light rays traveling toward a point focus (F′F') contract inward.

    • Represented by positive vergence (+ve+\text{ve} vergence).

    • The wavefront curvature becomes steeper (higher vergence) as it gets closer to the point focus.

Converging Wavefronts

Cartesian Optical Sign Convention

  • Purpose: Optical sign conventions use positive (+ve+\text{ve}) and negative (−ve-\text{ve}) mathematical signs to establish spatial orientation, indicating whether images are real or virtual, erect or inverted, and positioned to the left or right of refracting elements.

Cartesian Sign Cross
  • Origin / Vertex (AA):

    • The vertex (AA) is the geometric center point of the refracting surface where the principal optical axis intersects the surface.

    • AA coincides directly with the origin (0,0)(0,0) of the Cartesian coordinate system.

  • Direction of Light Propagation:

    • Light rays are drawn traveling strictly from left to right.

    • Objects are located on the left side, and emergent rays/images form toward the right.

Cartesian Coordinates and Center of Curvature
  • Horizontal Axis Rules (xx -axis):

    • Distances measured to the left of vertex AA are negative (−--direction).

    • Distances measured to the right of vertex AA are positive (++-direction).

  • Vertical Axis Rules (yy -axis):

    • Distances measured above the principal optical axis are positive (++-direction).

    • Distances measured below the principal optical axis are negative (−--direction).

  • Angles:

    • Angles are measured relative to the principal horizontal optical axis (xx -axis) or the surface normal.

Refraction Principles at Flat and Curved Surfaces

  • Snell's Law of Refraction:

    • Applies universally to all optical boundaries.

    • When a light ray passes from a medium with refractive index nn into a medium with higher refractive index n′n', the ratio of the sine of the angle of incidence (ii) to the sine of the angle of refraction (i′i' or rr) equals the inverse ratio of the refractive indices:

n′n=sin⁡(i)sin⁡(i′)\frac{n'}{n} = \frac{\sin(i)}{\sin(i')}

Re-expressed as: nsin⁡(i)=n′sin⁡(i′)\text{Re-expressed as: } n \sin(i) = n' \sin(i')

Snell's Law Diagram
  • Refraction at Curved Interfaces:

    • At any point of incidence on a curved surface, a tangent line is defined.

    • The surface normal is drawn perpendicular to the tangent at the point of entry and passes through the center of curvature (CC).

Normal and Tangent at Curved Surface
  • Refraction at Convex Surfaces (n′>nn' > n):

    • Light traveling from a lower index medium (nn) into a higher index medium (n′n') undergoes a reduction in phase velocity.

    • Wavefront spacing/wavelength shortens inside the higher index medium.

    • Rays refract toward the surface normal.

    • Convex refracting surfaces cause light rays to converge.

Refraction at Convex Surface
  • Refraction at Concave Surfaces (n′>nn' > n):

    • Light entering a medium of higher refractive index slows down, shortening wavefronts.

    • Rays bend toward the normal, directed away from the principal axis.

    • Concave refracting surfaces cause light rays to diverge.

Refraction at Concave Surface

Spherical Aberration, Hyperbolic Surfaces, and Paraxial Optics Assumptions

  • Spherical Aberration in Spherical Surfaces:

    • Marginal rays (rays striking the outer edge of a spherical surface) undergo greater refraction than paraxial rays (rays passing near the vertex).

    • This uneven focusing forms a envelope of focused rays called a caustic curve or caustic surface, preventing a single sharp focus point.

Spherical Refraction and Caustic CurveCaustic Light Reflection Photo
  • Hyperbolic Surfaces:

    • Hyperbolic optical surfaces refract all incident parallel rays directly into a single sharp point focus, eliminating spherical aberration natively.

  • Paraxial Optics Model:

    • Paraxial optics restricts analysis to light rays traveling very close to the principal optical axis (chief ray) passing through the vertex (AA).

  • Core Paraxial Assumptions:

    1. Spherical wavefronts refracted by spherical surfaces are assumed to emerge as perfect spherical wavefronts focusing at a single, precise point focus (ignoring differences between spherical and hyperbolic shapes).

    2. Refraction is assumed to occur along a single plane perpendicular to the optical axis (the distance between the actual curved surface and a flat reference plane, known as the sagitta, is treated as negligible).

    3. Variations in refractive index due to light frequency/color are neglected (monochromatic light is assumed, ignoring chromatic aberration).

Derivation of the Fundamental Paraxial Equation

  • Small Angle Approximations:

    • For points PP close to the vertex AA, angles of incidence (ii), refraction (i′i'), object slope (α\alpha), surface slope (β\beta), and image slope (γ\gamma) are extremely small.

    • Under the small angle approximation in radians:

sin⁡(i)≈i≈tan⁡(i)\sin(i) \approx i \approx \tan(i)

  • Simplifying Snell's Law:

nsin⁡(i)=n′sin⁡(i′)  ⟹  ni≈n′i′n \sin(i) = n' \sin(i') \implies n i \approx n' i'

Geometric Angle Derivation
  • Geometric Relationships from Triangles:

    • From triangle ΔBPC\Delta BPC (exterior angle theorem):

i=α+βi = \alpha + \beta

*   From triangle ΔB′PC\Delta B'PC:

\beta = i' + \gamma \implies i' = \tbeta - \gamma

  • Substituting into Snell's Law:

n(α+β)=n′(β−γ)n(\alpha + \beta) = n'(\beta - \gamma)

  • Expressing Angles in Terms of Heights and Distances:

    • Let l=ABl = AB be the object distance (measured negatively from vertex AA).

    • Let l′=AB′l' = AB' be the image distance (measured positively from vertex AA).

    • Let r=ACr = AC be the surface radius of curvature.

    • For small angles, arc length APAP approximates a straight vertical segment perpendicular to the axis:

tan⁡(α)≈PA−l\tan(\alpha) \approx \frac{PA}{-l}

tan⁡(β)≈PAr\tan(\beta) \approx \frac{PA}{r}

tan⁡(γ)≈PAl′\tan(\gamma) \approx \frac{PA}{l'}

  • Algebraic Expansion:

n(PA−l+PAr)=n′(PAr−PAl′)n\left(\frac{PA}{-l} + \frac{PA}{r}\right) = n'\left(\frac{PA}{r} - \frac{PA}{l'}\right)

  • Dividing both sides by segment PAPA:

n−l+nr=n′r−n′l′\frac{n}{-l} + \frac{n}{r} = \frac{n'}{r} - \frac{n'}{l'}

  • Rearranging terms puts object and image quantities on the left side and surface curvature on the right side:

n′l′−nl=n′−nr\frac{n'}{l'} - \frac{n}{l} = \frac{n' - n}{r}

Refracting Surface Power and Reduced Vergence

  • Surface Power (FF):

    • Defined as the quantitative change in reduced vergence imparted by a refracting interface:

F=n′−nrF = \frac{n' - n}{r}

*   Where radius of curvature rr is measured in meters (m\text{m}), surface power FF is expressed in Diopters (D\text{D}, or m−1\text{m}^{-1}).
  • Object Vergence (LL):

    • The reduced vergence of incident wavefronts at the vertex:

L=nlL = \frac{n}{l}

  • Image Vergence (L′L'):

    • The reduced vergence of emergent wavefronts at the vertex:

L′=n′l′L' = \frac{n'}{l'}

  • Fundamental Paraxial Equation in Reduced Vergence:

L′−L=F  ⟹  L′=L+FL' - L = F \implies L' = L + F

Linear Magnification at a Single Refracting Surface

  • Definition of Linear Magnification (mm):

    • The ratio of lateral image height (h′h') to lateral object height (hh):

m=h′hm = \frac{h'}{h}

  • Derivation Using Small Angles and Snell's Law:

    • For small angles of incidence and refraction at the surface:

tan⁡(i)=h−l\tan(i) = \frac{h}{-l}

tan⁡(i′)=−h′l′\tan(i') = \frac{-h'}{l'}

*   Applying Snell's Law in tangent form:

n′n=tan⁡(i)tan⁡(i′)=h−l−h′l′=h×l′h′×l\frac{n'}{n} = \frac{\tan(i)}{\tan(i')} = \frac{\frac{h}{-l}}{\frac{-h'}{l'}} = \frac{h \times l'}{h' \times l}

  • Rearranged Linear Magnification Equation:

m=h′h=l′×nn′×lm = \frac{h'}{h} = \frac{l' \times n}{n' \times l}

  • Magnification expressed via Reduced Vergence:

    • Recognizing that reduced vergence L=nlL = \frac{n}{l} and L′=n′l′L' = \frac{n'}{l'}, the formula simplifies directly to:

m=h′h=LL′m = \frac{h'}{h} = \frac{L}{L'}

First and Second Focal Lengths of Refracting Surfaces

  • Second Principal Focus (F′F') and Second Focal Length (f′f'):

    • The point where incident parallel light rays (L=0L = 0, object at infinity l=−∞l = -\infty) focus after refraction.

    • Given L=0L = 0, reduced image vergence becomes L′=FL' = F:

L′=n′f′=F  ⟹  f′=n′FL' = \frac{n'}{f'} = F \implies f' = \frac{n'}{F}

*   f′f' is the second focal length measured from the surface vertex.
  • First Principal Focus (FF) and First Focal Length (ff):

    • The object position that produces emergent parallel rays (L′=0L' = 0, image at infinity l′=+∞l' = +\infty).

    • Given L′=0L' = 0, reduced object vergence becomes −L=F-L = F:

−L=−nf=F  ⟹  f=−nF-L = -\frac{n}{f} = F \implies f = -\frac{n}{F}

*   ff is the first focal length measured from the surface vertex.
  • Relationship Between Focal Lengths and Refractive Indices:

ff′=−nn′  ⟹  f=−nn′×f′\frac{f}{f'} = -\frac{n}{n'} \implies f = -\frac{n}{n'} \times f'

*   The first and second focal lengths are unequal in magnitude whenever the media on either side of the surface differ in refractive index (n≠n′n \neq n').
  • Sign Conventions for Focal Lengths:

    • Convex Surface (F>0F > 0):

      • Second focal length f′f' is positive (real focus inside medium n′n').

      • First focal length ff is negative (located in front of vertex in medium nn).

    • Concave Surface (F<0F < 0):

      • Second focal length f′f' is negative (virtual focus in front of vertex in medium nn).

      • First focal length ff is positive (virtual object focus inside medium n′n').

Ray Tracing and Graphical Construction of Images

  • Three Principal Rays for Refracting Surfaces:

    1. Parallel Ray: Departs top of object parallel to principal axis, refracts through second focal point F′F'.

    2. Undeviated Ray: Passes through center of curvature CC, striking surface normal to local curvature (i=0∘i = 0^{\circ}, i′=0∘i' = 0^{\circ}), passing straight through without bending.

    3. Focal Ray: Passes through (or directs toward) first focal point FF, emerging from refractive interface parallel to principal axis.

Graphical Construction for Concave Surface
  • Image Properties:

    • Convex Surfaces: Produce real inverted images or virtual erect images depending on whether object distance is greater or less than focal length.

    • Concave Surfaces: Consistently form virtual, upright, and diminished images (m>0m > 0, ∣m∣<1|m| < 1) located in front of the refracting interface.

Newton's Extrafocal Equations

  • Extrafocal Distances:

    • xx: Extrafocal object distance, measured from first focal point FF to object point (x=l−fx = l - f).

    • x′x': Extrafocal image distance, measured from second focal point F′F' to image point (x′=l′−f′x' = l' - f').

Newtonian Diagram with Extrafocal Distances
  • Derivation via Similar Triangles:

    • Comparing similar triangles formed by object, image, and focal points:

h−h′=xfandh−h′=−f′x′\frac{h}{-h'} = \frac{x}{f} \quad \text{and} \quad \frac{h}{-h'} = \frac{-f'}{x'}

  • Newton's Product Formula:

x×x′=f×f′x \times x' = f \times f'

  • Newton's Magnification Equations:

m=h′h=−fx=−x′f′m = \frac{h'}{h} = -\frac{f}{x} = -\frac{x'}{f'}

Step-by-Step Worked Problems and Calculations

  • Sample Calculation 1: Convex Glass Interface

    • Problem: An object of height h=5 cmh = 5\,\text{cm} in air (n=1.0n = 1.0) is placed l=−0.75 ml = -0.75\,\text{m} from a glass block (n′=1.5n' = 1.5) having a convex spherical surface with radius of curvature r=+0.10 mr = +0.10\,\text{m}. Calculate surface power, focal lengths, image distance, image vergence, magnification, and image height.

    • Step 1: Surface Power (FF):

F=n′−nr=1.5−1.0+0.10 m=+5.00 DF = \frac{n' - n}{r} = \frac{1.5 - 1.0}{+0.10\,\text{m}} = +5.00\,\text{D}

*   *Step 2: Focal Lengths (ff and f′f')*:

f=−nF=−1.0+5.00 D=−0.20 mf = -\frac{n}{F} = -\frac{1.0}{+5.00\,\text{D}} = -0.20\,\text{m}

f′=n′F=1.5+5.00 D=+0.30 mf' = \frac{n'}{F} = \frac{1.5}{+5.00\,\text{D}} = +0.30\,\text{m}

*   *Step 3: Object Vergence (LL)*:

L=nl=1.0−0.75 m=−1.333 DL = \frac{n}{l} = \frac{1.0}{-0.75\,\text{m}} = -1.333\,\text{D}

*   *Step 4: Image Vergence (L′L')*:

L′=L+F=−1.333 D+5.00 D=+3.667 DL' = L + F = -1.333\,\text{D} + 5.00\,\text{D} = +3.667\,\text{D}

*   *Step 5: Image Distance (l′l')*:

l′=n′L′=1.5+3.667 D=+0.408 m=+40.8 cml' = \frac{n'}{L'} = \frac{1.5}{+3.667\,\text{D}} = +0.408\,\text{m} = +40.8\,\text{cm}

*   *Step 6: Linear Magnification (mm)*:

m=LL′=−1.333 D+3.667 D=−0.3635m = \frac{L}{L'} = \frac{-1.333\,\text{D}}{+3.667\,\text{D}} = -0.3635

*   *Step 7: Image Height (h′h')*:

h′=h×m=5 cm×(−0.3635)=−1.82 cmh' = h \times m = 5\,\text{cm} \times (-0.3635) = -1.82\,\text{cm}

*   *Interpretation*: The image forms 40.8 cm40.8\,\text{cm} inside the glass block to the right of the vertex; it is real, inverted, and reduced in height to 1.82 cm1.82\,\text{cm}.
  • Sample Calculation 2: Determining Radius of Curvature

    • Problem: An object of height h=5 cmh = 5\,\text{cm} in air (n=1.0n = 1.0) is located 50 cm50\,\text{cm} (l=−0.50 ml = -0.50\,\text{m}) in front of a glass block (n′=1.5n' = 1.5). If a real image forms inside the glass at 80 cm80\,\text{cm} (l′=+0.80 ml' = +0.80\,\text{m}) behind the surface, find the surface radius of curvature (rr), magnification (mm), and image height (h′h').

    • Step 1: Calculate Object Vergence (LL):

L=nl=1.0−0.50 m=−2.00 DL = \frac{n}{l} = \frac{1.0}{-0.50\,\text{m}} = -2.00\,\text{D}

*   *Step 2: Calculate Image Vergence (L′L')*:

L′=n′l′=1.5+0.80 m=+1.875 DL' = \frac{n'}{l'} = \frac{1.5}{+0.80\,\text{m}} = +1.875\,\text{D}

*   *Step 3: Calculate Surface Power (FF)*:

F=L′−L=+1.875 D−(−2.00 D)=+3.875 D≈+3.88 DF = L' - L = +1.875\,\text{D} - (-2.00\,\text{D}) = +3.875\,\text{D} \approx +3.88\,\text{D}

*   *Step 4: Calculate Radius of Curvature (rr)*:

F=n′−nr  ⟹  +3.875 D=1.5−1.0rF = \frac{n' - n}{r} \implies +3.875\,\text{D} = \frac{1.5 - 1.0}{r}

r=0.5+3.875 D=+0.129 m=+12.9 cmr = \frac{0.5}{+3.875\,\text{D}} = +0.129\,\text{m} = +12.9\,\text{cm}

*   *Step 5: Calculate Magnification (mm)*:

m=LL′=−2.00 D+1.875 D=−1.0667m = \frac{L}{L'} = \frac{-2.00\,\text{D}}{+1.875\,\text{D}} = -1.0667

*   *Step 6: Calculate Image Height (h′h')*:

h′=h×m=5 cm×(−1.0667)=−5.33 cmh' = h \times m = 5\,\text{cm} \times (-1.0667) = -5.33\,\text{cm}

*   *Interpretation*: The surface is convex with a radius of curvature r=+12.9 cmr = +12.9\,\text{cm}, creating an inverted real image of height −5.33 cm-5.33\,\text{cm}.