This page drills the PN law until no case can surprise you . We plug numbers, flip every sign, break the inputs (zero range rate, zero LOS rate), push to the limiting range R → 0 , and finish with a word problem and an exam twist. Before each example: Forecast — cover the answer and guess. After: Verify — plug back and check units.
If any symbol below feels unfamiliar, it was built in the parent note and in Line-of-Sight Geometry and Kinematics , Closing Velocity and Range Rate , and Polar Coordinate Kinematics .
Every worked example targets one row. The cell column is the label you'll see in each [!example].
Cell
Case class
What it stress-tests
A
Baseline: V c > 0 , λ ˙ > 0 , N standard
Plain substitution, units, g -conversion
B
Sign flip: λ ˙ < 0 (LOS clockwise)
Direction of a c
C
Sign flip: V c < 0 (opening range)
PN on a receding target — what breaks
D
Degenerate: λ ˙ = 0 exactly
The collision-course fixed point
E
Degenerate: R ˙ = 0 (co-orbiting, V c = 0 )
Zero closing speed — no command, no hit
F
Limiting: R → 0 with λ ˙ ∝ R N − 2
Terminal behaviour, boundary N = 2
G
Word problem: side-window / crossing target
Reading λ ˙ from raw kinematics
H
Exam twist: solve for N (or λ ˙ ) backwards
Inverting the law under an actuator cap
Recall Which cell is the stability boundary?
Cell F ::: at N = 2 the exponent N − 2 = 0 , so λ ˙ ∝ R 0 = constant — the LOS rate never decays. Convergence needs N > 2 .
V c > 0 , λ ˙ > 0 , standard N
A missile closes at V c = 800 m/s , measures LOS rate λ ˙ = 0.015 rad/s , and flies N = 4 . Command a c ? Express in g (g = 9.81 m/s 2 ).
Forecast: guess whether this is a gentle or violent maneuver (under or over 10 g).
Write the law: a c = N V c λ ˙ .
Why this step? PN is a pure product — no calculus needed once you have the three inputs live.
Multiply: a c = 4 × 800 × 0.015 = 48 m/s 2 .
Why this step? Order doesn't matter; the number is the raw lateral demand.
Convert to g : 48/9.81 = 4.89 g .
Why this step? Missile structural and actuator limits are quoted in g , so this is the number an engineer sanity-checks against.
Verify: units are ( dimensionless ) ⋅ ( m/s ) ⋅ ( 1/s ) = m/s 2 ✓. About 4.9 g is a modest, realistic command — well inside a typical ∼ 30 g airframe limit.
λ ˙ < 0 (sightline swinging clockwise)
Same missile: V c = 800 m/s , N = 4 , but now λ ˙ = − 0.015 rad/s . Find a c and say which way the missile turns.
Forecast: guess whether the magnitude changes versus Cell A, and predict the sign.
Substitute: a c = 4 × 800 × ( − 0.015 ) = − 48 m/s 2 .
Why this step? The law is linear in λ ˙ , so flipping its sign flips a c but leaves the magnitude identical to Cell A.
Interpret the sign: a c < 0 means acceleration in the direction of decreasing λ .
Why this step? A negative λ ˙ means the sightline is drifting toward smaller λ ; to null that drift the missile must push the same way the sightline is going — i.e. also toward smaller λ . See Feedback Control — Nulling an Error Signal : the sign always opposes the drift's growth, driving λ ˙ → 0 .
Verify: ∣ a c ∣ = 48 m/s 2 = 4.89 g , identical magnitude to Cell A ✓. The sign is opposite ✓ — PN is symmetric under LOS-direction reversal, exactly what a negative-feedback nuller should be.
growing — is PN still valid?
The target is pulling away: R ˙ = + 300 m/s so V c = − R ˙ = − 300 m/s . LOS rate λ ˙ = 0.02 rad/s , N = 4 . Compute a c and interpret.
Forecast: will the command still null λ ˙ , or make it worse?
Substitute: a c = 4 × ( − 300 ) × 0.02 = − 24 m/s 2 .
Why this step? The formula happily accepts a negative V c ; the sign of the command flips.
Check the stability exponent. From the derivation λ ˙ ∝ R N − 2 , but that assumed R shrinking . With R ˙ > 0 , R grows , so R N − 2 grows for N > 2 .
Why this step? Convergence relied on R → 0 . If range opens, the same algebra predicts λ ˙ increasing — PN diverges on a receding target.
Verify: ∣ a c ∣ = 24 m/s 2 = 2.45 g (finite, so the law computes) but the physics warns you: PN is a terminal, closing-geometry law. If V c < 0 you cannot intercept — see Closing Velocity and Range Rate . Units: ( − m/s ) ( 1/s ) = m/s 2 ✓.
Worked example D · Zero LOS rate — the fixed point
V c = 1000 m/s , N = 5 , λ ˙ = 0 . Command?
Forecast: zero, or something residual?
Substitute: a c = 5 × 1000 × 0 = 0 m/s 2 .
Why this step? λ ˙ multiplies everything; when it is exactly zero the whole product vanishes.
Interpret: no command needed. The sightline holds constant bearing while R shrinks — the collision-course condition from Step 2 of the derivation.
Why this step? λ ˙ = 0 is the goal state of the whole loop; once reached, PN correctly asks for nothing , which is exactly stable.
Verify: a c = 0 ✓. This is the equilibrium: a missile already on a collision course coasts straight in, burning no lateral effort. Any perturbation reintroduces λ ˙ = 0 and the command reappears — a self-correcting fixed point.
Worked example E · Co-orbiting target, range frozen
A missile and target circle a common point so that R ˙ = 0 , hence V c = 0 , yet λ ˙ = 0.05 rad/s (sightline sweeping fast). N = 4 . Command?
Forecast: big command (fast LOS!) or zero?
Substitute: a c = 4 × 0 × 0.05 = 0 m/s 2 .
Why this step? V c is a factor; zero closing speed zeroes the command regardless of how fast the sightline spins.
Interpret: PN commands nothing because there is no closing geometry to exploit. With V c = 0 the range never collapses, so no intercept exists to steer toward.
Why this step? It shows λ ˙ = 0 alone is not a call to maneuver — PN weights LOS rate by how fast the gap is actually closing. A large λ ˙ with V c = 0 is a miss you cannot fix with PN.
Verify: a c = 0 ✓. The concrete justification comes straight from the PN law: a c = N V c λ ˙ = − N R ˙ λ ˙ , so R ˙ (equivalently V c ) is a multiplicative factor of the command. Set R ˙ = 0 and the whole product is zero — the loop gain − N R ˙ vanishes exactly. It is not "some vague physical need"; it is that literal factor in the boxed formula going to zero. This is why practical seekers combine PN with a range-rate gate.
Worked example F · Residual LOS rate as
R → 0
Two missiles begin with the same λ ˙ 0 = 0.04 rad/s at R 0 = 5000 m . Missile P uses N = 3 , missile Q uses N = 6 . Find each λ ˙ at R = 500 m (one-tenth range). Then state what N = 2 would give.
Forecast: which missile ends nearer to λ ˙ = 0 , and by how many orders of magnitude?
Use the derived scaling λ ˙ = λ ˙ 0 ( R / R 0 ) N − 2 .
Why this step? Step 4 of the derivation integrated λ ¨ / λ ˙ = ( N − 2 ) R ˙ / R to λ ˙ ∝ R N − 2 .
Ratio R / R 0 = 500/5000 = 0.1 .
Why this step? Only the ratio enters, so absolute units cancel.
Missile P (N = 3 ): λ ˙ = 0.04 × 0. 1 1 = 0.004 rad/s .
Missile Q (N = 6 ): λ ˙ = 0.04 × 0. 1 4 = 4 × 1 0 − 6 rad/s .
Why this step? Bigger N ⇒ bigger positive exponent ⇒ far steeper collapse of λ ˙ as R shrinks.
Boundary N = 2 : exponent = 0 , so λ ˙ = 0.04 × 0. 1 0 = 0.04 rad/s — unchanged.
Why this step? This is the stability edge: at N = 2 the LOS rate never decays, guaranteeing a miss.
Read the figure below as you check these numbers: the horizontal axis is range R running right-to-left (intercept approaches as R → 0 ), the vertical axis is λ ˙ . Trace the magenta (N = 3 ) and violet (N = 6 ) curves down to the dotted line at R = 500 m — the violet curve has already plunged three decades lower than magenta, exactly the 1 0 3 gap you computed. Watch the orange dashed line (N = 2 ): it stays flat at 0.04 , never decaying — that is the failure the boundary warns about.
Verify: P gives 0.004 , Q gives 4 × 1 0 − 6 — Q is 1 0 3 smaller ✓ (exponent difference 6 − 3 = 3 ). N = 2 stays at 0.04 ✓. Terminal λ ˙ → 0 demands N > 2 ; see Navigation Constant Selection and Actuator Limits for why we don't just pick huge N .
Worked example G · Reading
λ ˙ from raw kinematics
A missile flies straight. A target crosses its path with transverse (across-LOS) relative speed V ⊥ = 120 m/s at the instant range is R = 3000 m , closing at V c = 850 m/s . With N = 4 , what lateral acceleration does PN command right now?
Forecast: the LOS rate isn't given directly — guess whether a c lands near a few g or tens of g .
Recover λ ˙ from the transverse speed: V ⊥ = R λ ˙ ⇒ λ ˙ = V ⊥ / R = 120/3000 = 0.04 rad/s .
Why this step? From Step 1 of the derivation the across-LOS relative speed is exactly R λ ˙ ; a seeker often measures V ⊥ (or λ ˙ ) rather than handing you λ ˙ on a plate. See Polar Coordinate Kinematics .
Now the law: a c = N V c λ ˙ = 4 × 850 × 0.04 = 136 m/s 2 .
Why this step? Convert the geometry into a command via the same product.
In g : 136/9.81 = 13.9 g .
Why this step? This is the number checked against the airframe.
Read the figure below to see where each number lives geometrically: the navy line is the LOS of length R = 3000 m at angle λ ; the magenta arrow at the target is the across-LOS speed V ⊥ = 120 m/s — its length over R is λ ˙ (Step 1); the orange arrow along the sightline is the closing speed V c = 850 m/s (Step 2's second factor). The two arrows are perpendicular because one is "along LOS" and the other "across LOS" — that decomposition is the whole point of working in the LOS frame.
Verify: λ ˙ = 0.04 rad/s ✓, a c = 136 m/s 2 = 13.9 g ✓. Cross-check the "constant bearing" intuition: a fast side-drift (120 m/s across a 3 km line) is a real miss threat, so PN correctly demands a stiff ∼ 14 g lead. A pure-pursuit missile would ask for even more later, too late.
Worked example H · Solve for the largest usable
N
A missile's airframe caps lateral acceleration at a c , m a x = 200 m/s 2 . Early in flight V c = 1000 m/s and λ ˙ = 0.05 rad/s . What is the largest integer N that stays within the cap at this instant? What residual λ ˙ -collapse exponent does that N give?
Forecast: guess whether the standard N = 4 survives, or gets clipped.
Set the command to the cap and solve: N m a x = V c λ ˙ a c , m a x = 1000 × 0.05 200 = 4.0 .
Why this step? The law is linear in N , so inverting it isolates the gain the actuator can afford at this operating point .
Largest integer ≤ 4.0 is N = 4 .
Why this step? You cannot exceed the cap, so round down . N = 5 would demand 250 m/s 2 > 200 — clipped, which corrupts the guarantee λ ˙ ∝ R N − 2 (a saturated actuator breaks the linear ODE).
Convergence exponent: N − 2 = 4 − 2 = 2 , so λ ˙ ∝ R 2 terminally.
Why this step? Confirms N = 4 is safely above the N = 2 boundary from Cell F — it converges.
Verify: N = 4 gives a c = 4 × 1000 × 0.05 = 200 m/s 2 , exactly the cap ✓. N = 5 gives 250 m/s 2 > 200 ✓ clipped. Exponent N − 2 = 2 > 0 ✓ converges. This is the real design tension in Navigation Constant Selection and Actuator Limits : bigger N nulls λ ˙ faster but saturates the fins; the augmented forms in Zero-Effort-Miss and Augmented Proportional Navigation address the same limit against maneuvering targets.
Recall Cell E result and its lesson
With V c = 0 , a c = ? and why ::: a c = 0 ; because a c = N V c λ ˙ has V c as a literal multiplicative factor, zero closing speed forces zero command no matter how fast the sightline spins.
Recall Cell F:
λ ˙ ratio for N = 6 at one-tenth range
λ ˙ / λ ˙ 0 = ? ::: ( 0.1 ) 6 − 2 = 1 0 − 4 .