Intuition The one idea behind this whole topic
A hot gas dumps energy onto a wall; an ablative shield survives by letting its own surface be destroyed , because destroying material soaks up energy and the escaping gas blocks more heat from arriving. Every symbol on the parent page is just a way of counting how much heat arrives versus how much material and energy leave — that is the entire bookkeeping.
This page assumes you know nothing . We will not use a single letter from the parent note until it is defined in plain words and pinned to a picture. Read top to bottom; each block earns the next.
Before any symbol, picture the situation.
On the left is very hot gas (thousands of kelvin). On the right is the cold structure we must protect. In between sits our sacrificial material. Heat flows left to right , from hot to cold — that is the only direction heat ever moves on its own.
Definition Heat flux — the star quantity
q ˙
Plain words: how much heat energy crosses one square metre of surface each second .
Picture: count the little orange arrows piercing a 1 m 2 window per second in the figure above.
Units: joules per second per square metre = W/m 2 (a watt is one joule per second).
Why the topic needs it: everything — recession, survival time, cooling — is a comparison of fluxes in versus fluxes away .
The little dot on top, q ˙ , is worth its own line.
Definition The dot ("per second")
A dot over any symbol means "rate of that thing — how fast it changes per second."
q = energy (joules). q ˙ = energy per second (watts).
m = mass (kg). m ˙ = mass per second (kg/s) — how fast material leaves.
s = a distance. s ˙ = d t d s = speed (m/s) — how fast a front moves.
Picture: a stopwatch attached to the letter. No dot = a total; dot = a flow.
Why do we need a rate and not a total? Because a heat shield can absorb a huge total, yet fail if the heat arrives too fast . Rate is the fair way to compare arrival against removal.
T , T g a s , T w a l l
T = temperature (in kelvin, K), a measure of how hot something is.
T g a s = temperature of the hot gas on the left.
T w a l l = temperature of the material's exposed surface.
Picture: a colour-map in the figure — bright orange gas, cooler grey wall.
Why: heat only flows because these two differ. The gap T g a s − T w a l l is the "push" driving heat into the wall.
difference drives heat
Heat is like water finding a lower level. No height difference ⇒ no flow. If T g a s = T w a l l , nothing crosses — the push is zero. The bigger the gap, the harder heat is shoved in.
Before we can read the parent's first equation we must own the letter h that sits inside it — so we define h first , then assemble the law.
h — the convective heat-transfer coefficient
Plain words: how good the flowing gas is at handing heat to the wall, per degree of push.
Units: W/(m²·K) — flux per kelvin of gap.
Picture: a fat pipe (big h , heat pours in easily) vs a thin pipe (small h ). Blowing, later, narrows this pipe .
Why the topic needs it: cooling by "blowing" is nothing but shrinking h . You cannot understand blowing without first owning h .
Now every symbol in the law is defined, so we may write it.
The wall pays for cooling in mass . We need three linked symbols.
m , m ˙ , and the per-area version m ˙ ′′
m = mass, kg.
m ˙ = mass leaving per second, kg/s.
m ˙ ′′ = mass leaving per second per square metre , kg/(m²·s).
The double-prime ′′ means "per unit area." One prime would mean per unit length; two primes mean per area. It lets us compare a big shield and a small sample fairly.
Picture: grams of char-gas puffing off each 1 m 2 tile every second.
ρ (rho) — density
Plain words: how many kilograms are packed into one cubic metre. Greek letter "rho," written ρ .
Units: kg/m³.
ρ v = density of the virgin (unburnt) material. The subscript v = "virgin."
Picture: a solid block; density is the block's heaviness for its size.
Why: to turn "kg lost" into "millimetres eaten away," we divide by density.
Now the front . As the surface burns inward, an imaginary line — the pyrolysis front — creeps deeper into the block.
Intuition Why link mass and depth?
If each square metre loses m ˙ ′′ kg every second, and each cubic metre holds ρ v kg, then the surface must retreat by
s ˙ = ρ v m ˙ ′′ [ kg/m 3 kg/m 2 s = m/s ] .
Cancel the units and you get metres per second — a real speed. This single link converts the whole topic's "energy talk" into "will my 2 cm liner last?"
Ablation is a trade: kilograms out buy joules absorbed . So we need "joules per kilogram" symbols.
Q p — heat of pyrolysis
Plain words: the energy needed to chemically break apart one kilogram of resin (turn solid into gas + char).
Units: J/kg.
Picture: a locked box; Q p is the energy to snap the lock. That energy is stolen from the incoming heat , which is why it cools.
Subscript p = pyrolysis (chemical decomposition by heat).
c p — specific heat capacity (and a warning about two uses)
Plain words: energy to raise one kilogram by one kelvin (at constant pressure — that's the subscript p , "constant pressure," not pyrolysis).
Units: J/(kg·K).
Picture: a bucket; c p is how many joules you must pour to lift its temperature by 1 K.
Which substance's c p ? It depends on whose kilogram we heat:
In the sensible-heating term (§7), c p is the solid material's heat capacity — we are warming the virgin solid.
In the blowing parameter B ′ (§6), c p is the injected gas's heat capacity — because there we compare the gas's ability to carry heat. Same symbol, different substance; always ask "whose c p ?"
Definition Two "totals" you must define before
Q ∗
Q ∗ is built from a net heat flux and a total mass loss , so define both plainly first.
q ˙ n e t = the net heat flux that actually reaches and must be handled by the wall (W/m²): what arrives by convection minus what is re-radiated away and blocked by blowing. It is the heat the material genuinely has to absorb.
m ˙ t o t a l ′′ = the total mass leaving per area per second (kg/m²·s): the sum of all material lost — the pyrolysis gas (from charring) plus any char removed by surface reaction, sublimation or mechanical erosion.
Picture: q ˙ n e t = heat left on the wall's plate after two helpers (radiation, blowing) took their share; m ˙ t o t a l ′′ = every gram that walked out the door, gas and solid alike.
Q ∗ — effective heat of ablation (the figure of merit)
Plain words: total heat handled per kilogram of material sacrificed — the master score of an ablator.
Q ∗ ≡ m ˙ t o t a l ′′ q ˙ n e t [ J/kg ]
Reading it: (net heat handled per second per m²) ÷ (total kg lost per second per m²) = joules handled per kg lost.
Picture: kilometres-per-litre for a car, but "joules-per-kilogram" for a heat shield. Big Q ∗ = miserly, efficient, good.
The star ∗ is just a name-tag , distinguishing this special "effective" quantity from a plain Q .
Q p (one channel) with Q ∗ (the total)
Why it feels right: both are "Q, joules per kg." The fix: Q p is only the chemistry sink. Q ∗ adds up all channels — chemistry + sensible heating + blowing. Q ∗ is always the bigger, headline number.
H — enthalpy
Plain words: the total heat content of the gas per kilogram, including energy hidden in its chemical bonds — not just its temperature.
Units: J/kg.
H g a s = enthalpy of the hot gas; H w a l l (or H w ) = enthalpy at wall conditions.
Picture: temperature is the visible tip of an iceberg; enthalpy is the whole iceberg (bonds included).
Why the topic needs it: super-hot gas breaks its own molecules apart (dissociation). That stored bond energy is invisible to a thermometer but very real to the wall. Using H g a s − H w a l l instead of T g a s − T w a l l counts it correctly.
T lies and H tells the truth
At 300 K, T and H carry the same information. At 6000 K on re-entry, molecules split and later recombine on your wall, dumping extra energy a thermometer never saw. So high-temperature work switches from T to H .
B ′ — blowing parameter
Plain words: a pure number comparing how fast gas is injected to how fast the flow can carry heat . No units — it is a ratio.
B ′ = h 0 m ˙ ′′ c p , gas
m ˙ ′′ = injected gas per area per second (kg/m²·s).
c p , gas = specific heat of the injected gas (see the warning in §4 — not the solid's c p ).
h 0 = the heat-transfer coefficient with no blowing (subscript 0 = "the baseline, un-blown case").
Picture: a tug-of-war — outward puff (m ˙ ′′ ) versus the gas's inward heat delivery (h 0 ).
ln — the natural logarithm
Plain words: ln x answers "to what power must the special number e ≈ 2.718 be raised to give x ? "
Picture: a curve that rises fast at first then flattens — it saturates . That flattening is exactly why "more blowing" stops helping.
Why here: the cooling gain from blowing is B ′ ln ( 1 + B ′ ) , a fraction that starts at 1 (no help removed) and slides toward 0 (heating shut off). The log's flattening shape is the physics of diminishing returns.
Definition Sensible-heating term
c p ( T w − T i )
Plain words: the energy stored just by warming one kilogram of the solid material from its cold start T i up to the hot surface T w , before it ever leaves.
c p here = the solid material's heat capacity, J/(kg·K).
T i = initial (cold) temperature; T w = wall (hot surface) temperature, K.
Picture: the bucket from §4 being filled as the solid heats up on its journey to the surface.
Why: this is one of the three channels summed inside Q ∗ — chemistry (Q p ) + sensible (c p Δ T ) + blowing.
convection law q = h times gap
mass per area m-double-prime
blowing parameter B-prime
energy per kg Q-p and c-p
Ablative Cooling charring and blowing
Every arrow says "you need the left box to make sense of the right box." Follow any path and you reach the parent topic: Ablative cooling — charring, blowing (index 3.3.30) .
The convection law and h deepen in Convective Heat Transfer (Stanton number) and Boundary Layer Theory .
Q p and pyrolysis chemistry are unpacked in Heat of Reaction and Pyrolysis .
The rival cooling schemes: Regenerative Cooling and Radiative Cooling .
The extreme heating environment: Re-entry Aerothermodynamics .
Recall Self-test — can you say each in one plain sentence?
What does a dot over a symbol mean? ::: a rate — that quantity per second.
What does the double-prime ′′ add to a symbol? ::: "per unit area" (per square metre).
q ˙ in words and units? ::: heat crossing one m² each second; W/m².
Why does heat flow at all in this problem? ::: because T g a s > T w a l l ; a temperature gap is the push.
What is h and what happens to it during blowing? ::: the conductance from gas to wall; blowing shrinks it.
How do you turn m ˙ ′′ into a recession speed s ˙ ? ::: divide by density, s ˙ = m ˙ ′′ / ρ v .
What does q ˙ n e t include? ::: convective heat in, minus radiation and blowing losses — the heat the wall must actually handle.
What does m ˙ t o t a l ′′ comprise? ::: all mass lost per area per second — pyrolysis gas plus char removed by reaction/erosion.
Difference between Q p and Q ∗ ? ::: Q p is only the chemistry sink; Q ∗ sums all cooling channels per kg lost.
Whose c p appears in B ′ versus in the sensible term? ::: in B ′ the injected gas's c p ; in the sensible term the solid material's c p .
Why use enthalpy H not temperature T at high heat? ::: H counts bond energy from dissociation that a thermometer misses.
What does B ′ compare? ::: injected gas rate vs the gas's heat-delivery ability; it is dimensionless.
Why does ln ( 1 + B ′ ) / B ′ mean "diminishing returns"? ::: the logarithm flattens, so extra blowing buys ever less cooling.