Lines, where a wire has a length

The mismatch that the cable hides

A lossless line carries a reflection back unchanged, so the standing-wave ratio at the instrument is the standing-wave ratio at the load. A real line does not, and the departure is exact: ten decibels of one-way loss improves any mismatch by twenty. A four-to-one load at the end of twenty metres of ordinary coaxial cable measures 1.13 at the near end, a return loss of 24 decibels, and passes an acceptance test the load could never pass. The boundary is a loss rather than a length, which makes it a frequency: 30.2 metres at 100 megahertz, 9.5 at a gigahertz, 3.0 at ten.

Assumes: The staircase in time · A quarter wave, and the path the current takes back

The lossless transmission line is the model this field is taught in, and it makes one statement about a mismatch that everything downstream depends on: the magnitude of the reflection coefficient is the same everywhere along the line. Only the phase turns. So a load’s standing-wave ratio can be measured from the other end of any length of cable, and the length does not matter.

That statement is exactly true of a line with no loss and exactly wrong of every real one, and the departure is large enough to invert the conclusion of an acceptance test.

A 4.0:1 load reads 1.13:1 through twenty metres of cablecomputed by solving, not by drawing. A 200 Ω load on a 50 Ω line — a standing-wave ratio of 4.00 at the load itself — measured from the other end of a length of cable that attenuates 0.500 dB per metre at 1 GHz. The reading falls as the length grows, exactly as |Γ| times ten to the minus twice the one-way loss over twenty, and reaches 1.5 at 9.5 m and 1.128 at twenty metres, which is 24.4 dB of return loss and would pass any acceptance test. The load is unchanged; the instrument is looking at it through 10.0 dB of attenuator. The length that hides it falls 3.16× per decade of frequency, which is the root of ten and is the attenuation's own law.12345100m110100length of cable between the instrument and the load (metres)standing-wave ratio the instrument reads at its own end4.00 — what the load actually isreads 1.5 past 9.5 m100 MHz10 GHzthe load200 Ω on 50 Ωits own SWR4.000frequency1 GHzattenuation0.500 dB/mSWR through 20 m1.128return loss there24.44 dBone-way loss there10.00 dBreads 1.5 beyond9.54 mper decade of f3.162× shortersolved, then checked — the line solved with its loss inten decibels of loss buys twenty of return loss
Fig. 1 A two-hundred-ohm load on a fifty-ohm line — a standing-wave ratio of four — measured from the far end of a length of ordinary coaxial cable. The reading falls as the length grows. The slider is the frequency, because the same cable changes its mind about how much it attenuates.

The closed form, and the solve that confirms it

A line’s propagation constant is γ=α+jβ\gamma = \alpha + j\beta: an attenuation per metre and a phase shift per metre. A wave travelling to the load and back travels 22\ell, so it comes back attenuated by e2αe^{-2\alpha\ell}. The reflection coefficient measured at the input is therefore

Γin=ΓL102αdB/20|\Gamma_{\text{in}}| = |\Gamma_L| \cdot 10^{-2\alpha_{\text{dB}}\ell/20}

and the phase, which the lossless model also gets, rotates at 2β2\beta\ell.

The figure does not evaluate that expression to draw its curve. It solves the line — the full complex hyperbolic tangent of γ\gamma\ell, which knows nothing about the expression above — and then asserts the two agree. Over six lengths spanning two orders they agree to better than a part in a billion, which is the arithmetic’s own floor.

The consequence is stated most usefully in decibels, and in decibels it is trivial: the return loss measured at the input is the load’s own return loss plus twice the one-way loss. Ten decibels of cable buys twenty decibels of apparent match.

What that does to a measurement

Take a load that is genuinely four to one — two hundred ohms on fifty, a reflection coefficient of 0.6, a return loss of 4.44 dB. It is a bad load by any standard.

Put twenty metres of ordinary small coaxial cable in front of it, at a gigahertz, where its attenuation is half a decibel a metre. The one-way loss is ten decibels. The instrument at the near end reads

  • Γin=0.060|\Gamma_{\text{in}}| = 0.060
  • standing-wave ratio 1.128
  • return loss 24.44 dB

That would pass essentially any specification written for a connector, an antenna or a filter. Nothing about the load has changed. The instrument is looking at it through ten decibels of attenuator, twice.

The length at which it happens is the number worth carrying: the figure bisects the length at which the reading falls to 1.5, and at a gigahertz it is 9.5 metres. Nine and a half metres of cable between an instrument and a load turns a four-to-one mismatch into something a specification would accept.

A 4.0:1 load reads 1.82:1 through twenty metres of cable. computed by solving, not by drawing. A 200 Ω load on a 50 Ω line — a standing-wave ratio of 4.00 at the load itself — measured from the other end of a length of cable that attenuates 0.158 dB per metre at 0.1 GHz. The reading falls as the length grows, exactly as |Γ| times ten to the minus twice the one-way loss over twenty, and reaches 1.5 at 30.2 m and 1.816 at twenty metres, which is 10.8 dB of return loss and would pass any acceptance test. The load is unchanged; the instrument is looking at it through 3.2 dB of attenuator. The length that hides it falls 3.16× per decade of frequency, which is the root of ten and is the attenuation's own law.
Fig. 2 The same load and the same cable at a hundred megahertz, where the attenuation is 0.158 dB per metre and the reading reaches 1.5 only past thirty metres. At low frequency the lossless model is nearly right and the measurement is nearly honest.
A 4.0:1 load reads 1.00:1 through twenty metres of cable. computed by solving, not by drawing. A 200 Ω load on a 50 Ω line — a standing-wave ratio of 4.00 at the load itself — measured from the other end of a length of cable that attenuates 1.581 dB per metre at 10 GHz. The reading falls as the length grows, exactly as |Γ| times ten to the minus twice the one-way loss over twenty, and reaches 1.5 at 3.0 m and 1.001 at twenty metres, which is 67.7 dB of return loss and would pass any acceptance test. The load is unchanged; the instrument is looking at it through 31.6 dB of attenuator. The length that hides it falls 3.16× per decade of frequency, which is the root of ten and is the attenuation's own law.
Fig. 3 And at ten gigahertz, where 1.58 dB per metre reduces it to three metres. Three metres of cable is a bench setup rather than an installation, which is what makes this a laboratory problem and not only a field one.

The boundary is a loss, so it is also a frequency

The three panels have the same shape and different scales, and the scaling is the second measurement.

The attenuation of a coaxial cable in the regime that matters here is set by the skin effect: the conductor’s resistance per metre goes as f\sqrt f, and so does the attenuation in decibels per metre. So the length that hides a mismatch, being a fixed number of decibels divided by the decibels per metre, goes as 1/f1/\sqrt f.

Measured: the length at which the reading falls to 1.5 is 30.18 m at 100 MHz and 9.54 m at 1 GHz — a ratio of 3.164 against 10=3.162\sqrt{10} = 3.162, which the figure asserts to two parts in a thousand.

That is a more useful statement than the length itself, because it says which measurements are safe. An audio-frequency or a low-radio-frequency measurement through a laboratory cable is not affected at all: at ten megahertz the same cable is 0.05 dB per metre, and thirty metres of it costs 1.5 dB one way, which moves a return loss by three decibels. A microwave measurement through the same physical cable is affected severely. The cable did not change; the frequency did.

A 10 kΩ resistor, and the 19.3 MHz it is one below. computed by solving, not by drawing. The dashed line is R, which is what the symbol means. The solid line is the same part with 8.0 nH of lead inductance in series and 0.40 pF across the body, solved as a three-element network and checked against the closed form for the same three elements to 3.3e-16. It is ten per cent below its own value by 19.3 MHz, and which of the two parasitics does that depends on the resistance: the shunt capacitance wins above 91.02 Ω and the lead inductance below it. The slider is the resistance, and the departure frequency it moves is not monotonic — it rises a decade per decade of resistance, peaks near 91.02 Ω at 2.00 GHz, and falls a decade per decade after that.
Fig. 4 Where the frequency dependence comes from. A conductor’s resistance is not a constant, and this is the field in which that stops being a refinement and becomes the whole argument.
A 0.5 mm conductor's resistance against frequency, exact and asymptotic. computed by solving, not by drawing. The exact ratio is computed from the Kelvin functions by their series; the dashed curve is the asymptote everybody quotes, which treats the current as flowing in one skin depth of the rim and is drawn only where that annulus is inside the wire. At 17.4 kHz, where the skin depth equals the radius and the rule of thumb says the effect "starts", the asymptote says 1.0000 — no effect at all — and the exact answer is already 1.0208. The rule of thumb names a frequency the effect has passed, which is the same shape as the tenth-of-a-wavelength criterion marking a point at which the lumped model is already 30% wrong. Two decades above, the two agree to 0.00%, which is what makes it an asymptote rather than a formula.
Fig. 5 The same f\sqrt f measured directly, in the magnetics field. A wire’s resistance rises as the root of frequency once the current has left its middle, and the attenuation of a coaxial cable is that resistance divided by its characteristic impedance.

What it costs, which is the other half

An engineer told that a long cable improves a match might reasonably ask what the problem is. The problem is that the improvement is entirely in the measurement and the loss is entirely real.

At twenty metres and a gigahertz the input accepts 99.6% of the power available from a matched source — which is what a return loss of 24 dB means — and delivers ten decibels less of it to the load, because ten decibels went into the cable. So the arrangement is superbly matched and delivers a tenth of the power. A shorter cable is badly matched and delivers far more.

The two quantities point in opposite directions and only one of them is what anybody wanted. That is worth stating as a rule, because match is so often used as a proxy for efficiency: a reflection coefficient measured at the wrong end of a lossy line is not a statement about power delivered. It is a statement about power accepted, and the difference between accepted and delivered is the loss.

A 4.0:1 load reads 1.41:1 through twenty metres of cable. computed by solving, not by drawing. A 200 Ω load on a 50 Ω line — a standing-wave ratio of 4.00 at the load itself — measured from the other end of a length of cable that attenuates 0.274 dB per metre at 0.3 GHz. The reading falls as the length grows, exactly as |Γ| times ten to the minus twice the one-way loss over twenty, and reaches 1.5 at 17.4 m and 1.410 at twenty metres, which is 15.4 dB of return loss and would pass any acceptance test. The load is unchanged; the instrument is looking at it through 5.5 dB of attenuator. The length that hides it falls 3.16× per decade of frequency, which is the root of ten and is the attenuation's own law.
Fig. 6 Three hundred megahertz: 0.274 dB/m, and a 4.0:1 load reads 1.41:1 through twenty metres. What it costs, which is the other half, is that the same loss attenuates the signal — the reflection is hidden because the round trip through the cable is attenuated twice, and the forward path is attenuated once.
A 4.0:1 load reads 1.02:1 through twenty metres of cable. computed by solving, not by drawing. A 200 Ω load on a 50 Ω line — a standing-wave ratio of 4.00 at the load itself — measured from the other end of a length of cable that attenuates 0.866 dB per metre at 3 GHz. The reading falls as the length grows, exactly as |Γ| times ten to the minus twice the one-way loss over twenty, and reaches 1.5 at 5.5 m and 1.022 at twenty metres, which is 39.1 dB of return loss and would pass any acceptance test. The load is unchanged; the instrument is looking at it through 17.3 dB of attenuator. The length that hides it falls 3.16× per decade of frequency, which is the root of ten and is the attenuation's own law.
Fig. 7 Three gigahertz: 0.866 dB/m, and the same 4.0:1 load reads 1.02:1. A mismatch that would return a third of the power is measured at the near end as two per cent — the cable has not fixed anything, it has made the measurement unable to see it.

The same mechanism used on purpose

The effect is not only a nuisance. It is one of the standard tools of the trade, and recognising it as the same arithmetic is worth doing because it fixes the sign.

An amplifier that is conditionally stable will oscillate if it sees the wrong impedance at its input or output. A cable of unknown length with an unknown thing on the end of it can present any impedance at all, so the standard defence is a small attenuator between the amplifier and the outside world. Three decibels of attenuator improves the worst-case reflection the amplifier can see by six, and six decibels of margin on a reflection is the difference between “any load” and “any load that is not absurd”.

The same construction appears as the isolation between two ports of a splitter, as the pad on a mixer’s local-oscillator port, and as the reason a directional coupler’s directivity is quoted as a number rather than assumed infinite. In every case it is Γ|\Gamma| multiplied by ten to the minus twice the loss over twenty, and the only difference from this essay’s cable is that somebody chose the loss.

What it costs is also always the same and always in the same place. Every decibel of attenuation ahead of a stage is a decibel on the noise figure of everything after it, exactly, by the cascade formula. So the trade is completely specified: buy two decibels of match with one decibel of noise, and the exchange rate is fixed by physics rather than by the component.

Getting the load back out again

If the loss is known, the load’s own reflection is recoverable — the expression is invertible — and it is worth being explicit about how well, because the answer decides whether the measurement was worth making.

Multiply the measured Γin|\Gamma_{\text{in}}| by 10+2α/2010^{+2\alpha\ell/20} and the load’s magnitude comes back exactly. The difficulty is not the arithmetic; it is that the correction amplifies the instrument’s own errors by the same factor. Through twenty decibels of round-trip loss, a directivity error of −35 dB in the instrument becomes an effective −15 dB at the load’s plane, which is a reflection uncertainty of 0.18 on a load whose true reflection might be 0.06. The correction has taken a precise measurement of the wrong thing and produced an imprecise measurement of the right one.

That is the general shape of every de-embedding problem and the reason a return-loss specification is written at a stated reference plane. Two rules follow and both are worth stating flatly.

Measure at the plane the specification is written at, or move the specification. A number measured at the bottom of a feeder is a statement about the bottom of the feeder, and is a perfectly good specification if that is what it is called.

The correction is bounded by the instrument’s directivity, not by its dynamic range. An instrument that can measure 60 dB of return loss cannot recover a load through 20 dB of round-trip loss to better than its directivity plus 20 dB, and directivity is the number that gets left off a data sheet summary.

The Smith chart becomes a spiral

There is a graphical consequence that is the clearest single picture of the difference.

On a lossless line, moving away from the load traces a circle of constant Γ|\Gamma| on the reflection plane, one full turn per half wavelength. That circle is the whole content of the lossless model: the mismatch is a radius and the length is an angle.

On a lossy line the radius shrinks as the angle turns, so the locus is a logarithmic spiral into the origin. Long enough, and every load looks matched, because the spiral has reached the middle.

That also explains a measurement artefact worth naming. Sweeping frequency on a mismatched lossy cable gives a reflection whose magnitude wobbles — the ripple of the standing wave — riding on a curve falling as the attenuation grows. Reading the average of that as the load’s mismatch is wrong by the attenuation, and reading the ripple is a much better estimate, because the ripple depends on the mismatch at the far end and comparatively little on the loss in between.

0.5 m smears a 59 ps edge to 659 and delivers it exactly on time. computed by solving, not by drawing. A raised-cosine edge sent down 0.5 m of ordinary trace, synthesised by multiplying its spectrum by exp(−γℓ) and transforming back, with the same edge down a lossless line of the same length drawn beside it. The two arrive together — 3.496 ns against the lossless 3.498 — so nothing about the loss has moved the arrival. What it has done is turn a 59 ps edge into a 659 ps one and take 2.9 per cent off the level it reaches. The delay and the rise time are two different quantities and only the first of them is what this field has been calling "the delay of the line".
Fig. 8 And the same trace read in time rather than in frequency: half a metre turns a 59 ps edge into 659 ps, arriving at 3.496 ns. The Smith chart becomes a spiral for the same reason — every reflection coefficient measured through a lossy line is pulled towards the centre by the round-trip attenuation, and the amount it is pulled by depends on the frequency.

Where this changes what a measurement means

Three places, and they are not exotic.

Acceptance testing through an installed feeder. An antenna at the top of a mast is tested from the bottom, through the feeder that goes up. The feeder’s loss is the whole reason the test is generous, and the correction is arithmetic — add twice the one-way loss back — but it requires knowing the loss, which is itself frequency dependent and degrades with age and water ingress. A feeder that has got worse makes its antenna look better.

Cascaded stages inside an instrument. An attenuator in front of a mixer improves the match seen by everything upstream by twice its attenuation, which is the standard reason for putting one there. That is a legitimate use of exactly this effect, and it costs exactly its attenuation in noise figure.

A time-domain reflectometer. The reflection from a fault at the far end of a long cable is attenuated twice on its way back, so a distant fault reads as a smaller discontinuity than an identical near one. Correcting for that is what the instrument’s “cable loss” setting is, and getting it wrong misjudges the fault rather than its position.

Copper smears an edge as the 1.94 power of the length and the laminate as the 1.00. computed by solving, not by drawing. The rise time a trace adds to a 59 ps edge, against its length, for a trace whose only loss is the conductor's skin effect, one whose only loss is the laminate, and one with both. The exponents are 1.937, 0.997 and 1.624: a loss rising as √f smears as the square of the length and a loss rising as f smears linearly, so the measured exponent is a diagnosis rather than a number. The edge's own rise time is taken out in quadrature, because otherwise the shortest trace is measuring the source. The arrival, on every curve and at every length, stays exactly linear.
Fig. 9 The laminate’s own contribution alone, against length: the 0.997 power of the length, adding 426 ps at a metre. Where this changes what a measurement means is exactly here — the exponent separates the two mechanisms, and a measurement taken through an unknown length of cable cannot separate them at all.

Where the model itself stops

This essay has been about a model failing — the lossless line’s claim that a mismatch travels unchanged — and it is worth saying where the replacement stops, because it does.

The expression ΓL102α/20|\Gamma_L|\,10^{-2\alpha\ell/20} assumes the attenuation is the only thing the line does to the wave’s amplitude, which requires the line to be uniform and its characteristic impedance to be real. Neither is exactly true. A real cable’s characteristic impedance has a small negative imaginary part wherever its loss is resistive rather than dielectric, so it is not fifty ohms but fifty ohms with an angle of a fraction of a degree, and a load that is exactly fifty resistive ohms is therefore not exactly matched to it. At the loss levels drawn here that correction is a few parts in a thousand of the reflection and is buried under everything else; at the very low frequencies where α\alpha is dominated by the conductor and β\beta is small it is not, which is the regime a telephone line lives in and the reason its characteristic impedance is quoted with a phase angle.

The second assumption is uniformity. A cable with a periodic imperfection — a regular variation in diameter from the manufacturing process, or a repeated bend — has a reflection that adds coherently at the frequency whose half wavelength matches the period, and the result is a narrow spike of reflection that no amount of loss between it and the load can hide, because it is not at the load. That is a structural return loss, it is specified separately, and it is the one fault in this field that gets worse with length rather than better.

What the loss changes about the rest of the field

Nine essays in this field quote a delay and a reflection coefficient, and a lossy line makes both of them frequency-dependent. The delay that is not one number is where that is measured directly, with two exponents separating the two mechanisms. The staircase in time is the lossless picture every reflection argument in the field is drawn on, and A ladder is not a line is the other approximation to the same object, converging far more slowly. Several sections, and the band they buy is a design whose whole merit is a reflection coefficient, measured through cable that would hide it. And The resistor that is only a resistor is the component version of the same argument: an instrument sees the far end through everything in between.

What is checked

Two assertions, and the second is the one that makes the first mean something.

That the reflection at the near end is the load’s own, attenuated by twice the one-way loss, over six lengths from half a metre to fifty. The line is solved with its loss in — a complex hyperbolic tangent that shares no arithmetic with the expression — and the two agree to better than a part in a billion. A closed form checked against the route that produced it would prove nothing; this one is checked against a route that never saw it.

And that the length that hides a mismatch falls as one over the root of frequency, measured as 3.164 times shorter per decade against 10\sqrt{10}. That is the claim that turns a fact about a length into a fact about a frequency, and it is what makes the boundary a boundary of this collection’s usual kind rather than an observation about one cable.

The square root, and the model it belongs to

The one over root frequency is not an empirical fit; it is the skin effect, and it carries a condition that this essay’s loss model does not state. The delay that is not one number is where that condition is measured, and it puts a second boundary underneath this one: below the frequency at which a trace’s reactance overtakes its series resistance — 910 kilohertz for ordinary copper — the line is a diffusion rather than a wave, with a velocity proportional to f\sqrt f rather than constant. Above it the arrival is still exactly linear in the length and the rise time grows as the square of it.

So the loss whose decibels per metre hide a mismatch here has three regimes and this essay is drawn in the middle one. Below 910 kilohertz the line is not carrying a wave at all and the standing-wave argument has nothing to describe. Between there and wherever the dielectric’s own loss overtakes the conductor’s, the loss goes as f\sqrt f and the hiding length falls as 1/f1/\sqrt f, which is the measurement made here. Above that the dielectric loss goes as ff and the hiding length falls faster than the square root — so the numbers in the table are, at the gigahertz end, an underestimate of how short a cable has to be before it stops flattering its load.

That last point is the one worth carrying to an acceptance test. A quarter wave, and the path the current takes back is the other essay in this field where a good measured number conceals a design that is only correct at one frequency — a section reflecting 5×10175\times10^{-17} of what arrives, at one frequency, with seventeen per cent either side of it back to a tenth. The two failures pair: one hides a bad load behind a lossy cable, the other hides a narrow match behind a single-frequency measurement, and both are discovered by sweeping.

An instrument that flatters, which is the rarer kind

Most of the instrument errors this collection measures make a reading worse than the truth — a probe loads a node, a lead adds its own resistance, a shared return adds somebody else’s current. This one does the opposite, and that is what makes it dangerous rather than merely inconvenient.

A four-to-one load at the end of twenty metres of ordinary coaxial cable measures 1.13 at the near end, a return loss of twenty-four decibels, and passes an acceptance test the load could never pass. Nothing has gone wrong with the instrument, the cable or the measurement: the reflection really is that small where it was read, because the reflected wave made the journey twice and lost twice the one-way loss doing it. The reading is correct about the node it was taken at and wrong about the question it was asked.

That is the same distinction the probe is part of the circuit draws — a reading is two solves, the circuit and the circuit-with-the-instrument, and the quantity drawn is the difference — with the sign reversed. There the instrument’s presence degrades the thing being measured and the reading tracks the degraded circuit honestly. Here the instrument’s distance improves the number and the reading tracks a quantity nobody wanted.

The practical consequence is a rule about where to stand rather than about what to buy. A return-loss measurement is a measurement of a plane, and the plane is wherever the instrument’s reference is — so a specification that names a return loss without naming the plane it is measured at has left out the term this essay computes, which at ten decibels of intervening loss is a factor of a hundred in reflected power.

Part 1 on line loss

One argument about Line loss, and one of 2 essays on it so far, each part numbered by how much of the idea it assumes. What sits either side of it:

What links here

Essays that reach for this one mid-argument — the half of a link its own author cannot write down, the 8 sharing most with it of 9.

What this makes readable

Essays that name this one as a prerequisite.

The objects named here

The third axis, after the field and the idea: the things themselves, and every essay that touches each one.

Characteristic impedanceImpedance matchingInsertion lossModel rangeReflection coefficientSkin effectTerminationTransmission line