1.6.13 · D2Oscillations & Waves

Visual walkthrough — Mechanical waves — transverse and longitudinal

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Before line one, a promise: every symbol below is introduced in plain words and pinned to a picture before it is ever used in an equation.


Step 1 — One dot that just bobs (the source)

WHAT. Picture a single particle sitting at the very start of a long rope, at the place we call . We grab it and move it smoothly up and down — the same gentle back-and-forth a mass on a spring makes. That special motion is Simple Harmonic Motion (see Simple Harmonic Motion).

WHY this and not some random jiggle. We choose SHM because it is the simplest repeating motion, and because almost any real vibration (a plucked string, a tuning fork) is built out of SHM pieces. If we can describe one SHM dot, we can describe the whole wave by copying it.

PICTURE. In the figure, the amber dot rides up and down a vertical dashed line. Its height above the middle line is what we call .

Two words earn their symbols here:

  • = the dot's displacement — how far up (positive) or down (negative) it is from its resting middle.
  • = time, ticking forward.

The height as time passes traces a sine curve, so we write:


Step 2 — The neighbour copies, but late

WHAT. The dot at is tied by the rope to the dot just to its right. When our dot goes up, it tugs its neighbour up too — but the neighbour needs a moment to respond. So the neighbour does the exact same dance, started a little later. The next dot copies the neighbour, later still, and so on down the rope.

WHY. This "copy-but-delayed" idea is the whole secret of a travelling wave. Nothing moves along the rope except the timing of the dance. Each dot stays over its own spot (matter stays put); only the pattern of who-is-up-now marches forward.

PICTURE. The figure shows a row of dots. The leftmost is at the top of its bounce; each one to the right is a little further "behind" in its cycle, so the tops-and-bottoms line up into a frozen sine shape in space.

Now we need to say how much later each dot starts. Two new plain-word symbols:

  • = position along the rope, distance to the right of the source.
  • = the wave speed, how fast the "start signal" travels along the rope (metres per second). This is fixed by the rope itself — see Step 5.

The disturbance travels a distance at speed , so it arrives after a time


Step 3 — Write the delay into the formula

WHAT. The dot at position does now whatever the source did a time ago. So wherever the source formula had , the far dot uses (a smaller, earlier time).

WHY. Subtracting the delay is exactly what "does the same thing, later" means in maths. If you rewind the far dot's clock by , it matches the source.

PICTURE. Two clocks: the source clock reads , the far-away clock is set back by . Feed the rewound clock into the same sine and you get the far dot's height.

Multiply the inside:

That messy deserves its own name. Call it :

Substituting gives the star of the show:


Step 4 — Why the minus sign points the wave to the right (and to the left)

WHAT. We test the sign. To "ride a crest," you must keep the phase at a fixed value (say the value where sine peaks). As time grows, what must do to keep the phase constant?

WHY. A crest is just "a spot where the phase equals a peak value." Following that spot tells us which way — and how fast — the pattern moves.

PICTURE. Two snapshots a tiny bit apart in time. The amber crest has slid to the right; the dashed vertical line tracks it.

Keep the phase fixed: A tiny time step later, the phase mustn't change, so . Solve for the crest's speed:


Step 5 — Where do and come from? (Naming the medium and the source)

WHAT. We tie and back to things you can measure with a ruler and a stopwatch.

WHY. Symbols are only useful if you can point at them in the real world. and are "per second" and "per metre" versions of two everyday quantities.

PICTURE. A snapshot of the rope frozen in space (top): the repeat-distance between two crests is , the wavelength. A single dot watched over time (bottom): the repeat-time of its bounce is , the period.

  • One full cycle in time is radians of phase and takes a time :
  • One full cycle in space is radians of phase and takes a distance :

Step 6 — The universal payoff:

WHAT. Combine the two definitions. Since , plug in and :

WHY it's the same as "one wavelength per period." In exactly one period , the pattern slides forward exactly one whole repeat-distance . Speed = distance ÷ time = . It falls out two ways because both say the same geometric truth.

PICTURE. Over one tick of , the whole sine pattern is shown shifting right by precisely one — the amber crest lands exactly where the next crest used to be.

This same runs everything downstream: Sound waves, Standing waves & resonance, the Doppler effect, and it is the engine inside the full Wave equation.


Step 7 — Edge and degenerate cases (never leave the reader stranded)

WHAT & WHY. A formula you trust must survive its extreme settings. We push the knobs to their limits and check the picture still makes sense.

PICTURE. Four mini-panels, one per case, each showing the rope's shape.

  • (no shake). everywhere for all time — a flat, dead rope. Correct: no disturbance, no wave.
  • (source held still forever). , so frozen in time — a static shape, not a travelling wave. A wave needs the source to actually move.
  • i.e. . The whole rope moves up and down together, in step — pure SHM with no spatial pattern. This is the bridge back to Simple Harmonic Motion: a wave of infinite wavelength is just synchronised bobbing.
  • Left-mover, . Same shape, crest slides the other way (from Step 4). Both signs are legitimate waves; adding a left-mover and a right-mover is how Standing waves & resonance and Superposition and Interference are born.

The one-picture summary

Everything above, on one canvas: a source dot doing SHM (left), each neighbour copying it with delay , freezing into a sine in space whose repeat-distance is ; the pattern marches right at , while each dot only bobs with height .

Recall Feynman retelling — the whole walkthrough in plain words

A single kid at the front of a line wiggles up and down in a smooth, spring-like way (that's the sine, with as how high and as how fast). The kid next to her can't move instantly — she copies the wiggle a heartbeat later, because the tug takes time to arrive. Everyone down the line copies their neighbour a heartbeat later still. Freeze the picture and the "who's up now" pattern looks like a sine drawn along the line, repeating every metres. Let time run and that whole pattern slides forward — one full repeat-distance every period — so it travels at . The kids never leave their spots (matter stays); only the wiggle-pattern travels (energy moves). Shake faster and the crests crowd closer, because the rope only lets the pattern travel at one speed. Turn the source off and the pattern freezes; make the wavelength infinite and the whole line just bobs together — which is exactly where we started, plain SHM.

Recall Fast self-check

What does the term do physically? ::: It delays each point's phase by how far the wave had to travel, and its minus sign sends the wave in . Why is a sine used at all? ::: Because each particle does SHM, whose displacement-vs-time is a sine. If you triple in a fixed medium, what happens to ? ::: It becomes one third, since and is fixed. What is the limit? ::: Infinite wavelength — every point oscillates in unison, i.e. pure SHM.