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The science
What is modelled
Three optics experiments on one bench, each with its own station. This is the 3D companion of the 2D page "Light Bench: Refraction, Thin Lens and Diffraction"; both use the same closed-form optics and the same four checks.
Equations
- Refraction (station A). Snell's law
n1 sinθ1 = n2 sinθ2. The reflected power is the mean of the Fresnel s and p terms,Rs = ((n1cosθ1 − n2cosθ2)/(n1cosθ1 + n2cosθ2))²,Rp = ((n2cosθ1 − n1cosθ2)/(n2cosθ1 + n1cosθ2))². Critical angleasin(n2/n1)for n1 > n2; Brewster angleatan(n2/n1). Beam brightness shows the power split. - Thin lens (station B).
1/f = 1/do + 1/di,m = −di/do. Each of the three drawn rays is bent at the lens by the paraxial ruleu' = u − y/f; a virtual image (di < 0) is shown as a blue ghost with dashed back-extensions. - Diffraction (station C). Fraunhofer far field
I = I0 sinc²(π a sinθ/λ), for two slits timescos²(π d sinθ/λ). The pattern on the screen 1.000 m behind the slit plate is painted from this formula; first minimum atsinθ = λ/a, fringe spacingλL/d.
Checks run in the page
- Snell's law by bisection on the angle against the arcsine closed form.
- Energy: R + T = 1, with T built from the amplitude transmission coefficients.
- Lens: two numerically traced rays cross where the lens equation predicts.
- Diffraction: a brute-force sum of phasors over the aperture against the closed form.
- The Blender bench geometry: slit plate to screen distance equals the 1 m used in the formulas, and the object base sits on the lens axis.
Honest simplifications
- Scalar waves, no dispersion (the index does not depend on colour), no absorption, paraxial thin lens with no aberrations; the lens model in the picture only changes its thickness with 1/f.
- The beams in station A stop at the tank wall; the real exit refraction at the glass wall is not drawn. The two liquids and the glass walls are only tinted by their index.
- The slits are micrometres wide, so the glowing slit marks on the plate are drawn 200 times too large; the pattern itself is true to scale at L = 1 m.
- Fresnel reflectance is for unpolarised light and plane interfaces. The colour of a wavelength is an approximate display mapping.
What to try
- Station A: raise the angle beyond the critical angle in "Glass to air" and watch the refracted beam vanish; at Brewster's angle p-polarised reflection is zero, so R is at a minimum, not zero for unpolarised light.
- Station B: move the object inside the focal length to see the virtual, magnified image.
- Station C: shrink the slit width and the central maximum widens; add the second slit to see the fringes.
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