Before you can read the parent note de Laval nozzle, you must own every letter it throws at you. This page builds each one from nothing — plain words, then a picture, then the reason the topic needs it.
Why the topic needs this: it lets us describe the whole flow with quantities that depend only on position along the tube, so a single number like "area here" or "speed here" is meaningful. Look at the s01 figure — each vertical slice is one "state" of the gas.
Converging = A shrinking as you move downstream (tube pinches in).
Throat = the spot where A is smallest.
Diverging = A growing again (tube flares out).
Why needed: the entire topic is about shapingA along the tube. The master equation is literally a statement about how a change in A forces a change in speed.
Why needed: gases are compressible — squeeze them and ρ rises; let them expand and ρ falls. Liquids barely change ρ, which is exactly why nozzle physics differs from water pipes. The counter-intuitive supersonic behaviour comes entirely from ρ dropping faster than A grows.
Combine the three quantities above: in one second the gas at a slice sweeps forward a distance V, filling a tube-chunk of volume A×V; multiply by density to get mass:
m˙=ρAV
Why needed: this single conserved product ties A, V, ρ together — it is Step 1 of the parent's derivation.
Here the letter d in front of a quantity means "a tiny change in it" — dp is a small pressure change over a small step down the tube. We use tiny changes because area, speed and pressure all vary smoothly and continuously along the nozzle; small steps let us relate their slopes.
Why needed: a is the referee. It sets the magic speed at which the nozzle's rule flips. It also connects pressure and density changes: for a gentle isentropic disturbance, a2=dp/dρ (Step 3 of the parent).
M<1subsonic — slower than sound; pressure news can travel upstream.
M=1sonic — exactly the sound barrier.
M>1supersonic — faster than sound; the gas outruns its own pressure news.
Why needed: M is the single knob that decides the sign of (M2−1), and therefore whether narrowing or widening accelerates the gas. It is the star of the master equation.
Why needed: this assumption is what lets pressure, density and temperature all lock together in tidy formulas (the T0/T, p0/p, A/A∗ ratios). Drop it and the algebra explodes.
Why needed: every isentropic ratio compares a local quantity to a stagnation or starred one. Choking, and the whole Choked Flow & Mass Flow Limit story, are stated in these symbols.
AdA = the fractional change in area (a 2% widening, say). Dividing the tiny change dA by A itself makes it a percentage, so tubes of any size compare fairly.
VdV = the fractional change in speed.
(M2−1) = the sign-flipping gatekeeper: negative when M<1, zero at M=1, positive when M>1.
Why needed: once you read every symbol, the equation says in words — "to speed the gas up, change the area in the direction the gatekeeper allows; at exactly Mach 1 the gatekeeper is zero, so speed can only be sonic where area stops changing (the throat)."
Two more devices the parent mentions in passing:
Normal shock — a paper-thin jump where supersonic flow snaps back to subsonic, raising p and T abruptly (Normal Shock Waves).
These foundations later power Rocket Propulsion & Thrust and Steam Turbine Nozzles.