Visual walkthrough — Huygens' principle — wavefront propagation
Step 1 — What is even moving? Draw the wavefront
WHAT. Before any bending, we need the thing that bends. A wavefront is a line (in 2D) joining all points of the wave that are "doing the same thing at the same moment" — all cresting together. Picture a straight rank of soldiers marching in step: the rank is the wavefront.
WHY. We track this equal-phase line, not individual light "particles", because the whole trick of Huygens is: every point on this line is a tiny new source. If we know where the line is now, we can build where it is next.
PICTURE. The blue line is our wavefront. The pale-yellow arrow, drawn perpendicular to it, is the ray — the direction the whole rank marches. Remember: ray and wavefront are always at right angles (never parallel).
Step 2 — Let it march: distance = speed × time
WHAT. Give the wave a stopwatch. In a time the rank advances a distance. If the wave moves at speed (metres per second in medium 1), then in seconds it covers
WHY. Speed literally means "distance per unit time", so distance is just speed times time. This is the only physics input — everything after is geometry.
PICTURE. Two blue lines: the old wavefront and, a distance ahead, the new one. They stay parallel because every point marched the same . This is the parent's "plane stays plane".
Step 3 — Tilt the wavefront onto a boundary
WHAT. Now let the marching rank hit a slanted line — the surface between medium 1 (top, speed ) and medium 2 (bottom, slower, speed ). Because the wavefront is slanted, one end — call it — reaches the surface first, while the other end is still up in medium 1 at a point we call .
WHY. If the wavefront hit the surface perfectly flat-on, both ends would cross together and nothing interesting would happen. The tilt is what makes one end wait while the other crosses — and waiting is what makes light bend.
PICTURE. sits on the boundary. still hangs above it. The angle between the incoming wavefront and the surface (equivalently, between the incoming ray and the normal, the dashed perpendicular to ) is the angle of incidence .
Step 4 — The race: end finishes in medium 1 while end starts in medium 2
WHAT. Two things happen in the same time interval :
- End , still in medium 1, races down to meet the surface at a point . It travels
- End , having already crossed, sends its Huygens wavelet forward into medium 2. In the same it spreads only
WHY. This is the heart of the whole thing. and get the same clock time , but is in the slow medium and in the fast one. Same time, different speeds ⟹ different distances. That mismatch is the bend.
PICTURE. is a long blue segment (fast). is a short pink arc of radius — the secondary wavelet from (Huygens: every point is a source). Because , the arc is smaller than .
Step 5 — Draw the new wavefront: the common tangent
WHAT. By time , end has just arrived at (so its wavelet has radius zero there), while 's wavelet has grown to radius . Every point between and crossed at some in-between moment, so its wavelet has an in-between radius. The new wavefront in medium 2 is the straight line from that is tangent to all these wavelets — it touches 's circle exactly at .
WHY. Huygens' rule: the next wavefront is the common tangent (envelope) of all the secondary wavelets. Off the tangent, wavelets are out of step and cancel; along it they reinforce.
PICTURE. The refracted wavefront (blue) leans against the pink wavelet at , with a right angle at (, because a tangent is perpendicular to the radius at the touch point).
Recall Why is
perpendicular to ? A tangent line touches a circle at exactly one point, and the radius to that point always meets the tangent at . Here is tangent to 's wavelet at , so . ::: This right angle is what makes triangle a right triangle in Step 6. Which point is the refracted wavefront pinned to on the surface? ::: Point , where end has just arrived.
Step 6 — Two right triangles that share a hypotenuse
WHAT. Look at the two triangles that meet along the surface segment :
- : right angle at , hypotenuse , and the side sits opposite the angle at , which equals .
- : right angle at , hypotenuse (the same segment), and side sits opposite the angle at , which equals the angle of refraction .
Now use the definition of sine — "opposite over hypotenuse":
WHY sine, and why these two angles? Sine turns an angle into a ratio of sides, which is exactly the language a triangle speaks. We pick and because both angles ride on the same hypotenuse — so when we divide, cancels and the messy geometry disappears.
PICTURE. Both triangles drawn on the shared base : yellow highlights the two "opposite" sides and ; the angle lives at , the angle lives at .
Step 7 — Divide, and Snell's law falls out
WHAT. Divide the two sine expressions. The common time and the common hypotenuse both cancel:
WHY. Everything that depended on how far or how long the wave travelled (, ) has vanished. What survives is only the ratio of the two speeds — a fixed property of the two media. A constant ratio is exactly what a "law" is.
Using (refractive index = light speed in vacuum ÷ speed in the medium):
PICTURE. The final annotated diagram: incident ray, bent refracted ray, and the boxed result — see Snell's Law and Refractive Index and Phase and Path Difference for where this feeds forward.
Step 8 — The edge cases (never leave the reader stranded)
WHAT & WHY & PICTURE, all three at once, for the situations the clean derivation glossed over:
- Straight-on incidence (). Wavefront parallel to surface, both ends cross together, no tilt develops. Then . Light passes straight through, un-bent — but still slower inside.
- Same medium (). The ratio is , so , : no bending. There was never a boundary worth bending at.
- Slow → fast (). Now : the wavelet outruns end . So , : the ray bends away from the normal.
- Critical angle & total internal reflection. Going slow→fast, keep increasing . The required climbs toward . At the critical angle where , we get — the refracted wavefront skims along the surface. Beyond , is impossible: no tangent wavefront can be drawn in medium 2, so all the light reflects back. (See Laws of Reflection.)
The one-picture summary
Everything on one slate: the tilted incident wavefront , the race ( long, short), the two right triangles sharing hypotenuse , and the bent wavefront — with the boxed law underneath.
Recall Feynman: the whole walkthrough in plain words
A line of friends marches in step (the wavefront). They reach a muddy field cut on a slant. The friend nearest the mud steps in first and slows down; his neighbours in mud slow too, but the friends still on firm ground keep sprinting. In the same few seconds, the sprinters cover a long stretch while the mud-walkers only shuffle a little. So the whole line pivots — it's now aimed more steeply into the mud. That pivot is the bend. Write "sprinter distance = " and "mud distance = " on the same slanted baseline; the two right triangles they form share the baseline, so dividing their sines cancels the baseline and the time, leaving just . Speed things up instead of slowing them (mud → firm ground) and the line pivots the other way. Slow them so hard that no forward line can even form, and the whole rank bounces back — total internal reflection.
Connections
- Huygens' principle — wavefront propagation (parent)
- Snell's Law and Refractive Index
- Laws of Reflection
- Phase and Path Difference
- Wave Optics — Interference
- Young's Double Slit Experiment
- Diffraction