Part 2 · Chapter 5

Townsend Breakdown Mechanism

Chapter 4 left a single electron multiplying into an avalanche of \(e^{\alpha d}\) — impressive, but not yet a spark. An avalanche crosses the gap once and is gone; for breakdown the gas must learn to replace the electron that started it. This chapter is how it does so: the secondary processes at the cathode that close the loop, the current equation that captures the feedback, and the exact criterion at which a multiplying current turns into a self-feeding discharge.

High-Voltage Engineering Prof. Mithun Mondal Reading time ≈ 40 min
i What you'll learn
  • Why the primary avalanche \(n=n_0 e^{\alpha d}\), on its own, is a one-shot event and not yet a breakdown.
  • The secondary processes that regenerate electrons at the cathode — positive-ion bombardment, photoemission, metastables — all gathered into Townsend's second coefficient \(\gamma\).
  • The complete Townsend current \(i=\dfrac{i_0 e^{\alpha d}}{1-\gamma(e^{\alpha d}-1)}\) and what makes its denominator the whole story.
  • The Townsend breakdown criterion \(\gamma(e^{\alpha d}-1)=1\): the precise moment a gap becomes self-sustaining.
  • The statistical and formative time lags that decide how fast a gap responds to an impulse.
  • Why Townsend breakdown is cathode-dependent, the \(pd\) range over which it holds, and where the streamer takes over.
Section 5-1

From Avalanche to Self-Sustained Discharge

At the close of Chapter 4 we had a single electron leaving the cathode and arriving at the anode as \(e^{\alpha d}\) electrons — a genuine avalanche. It is tempting to call that breakdown, but it is not. The avalanche sweeps across the gap, deposits its electrons on the anode, and is over; if no fresh electron is launched from the cathode, the current simply stops. The gap has conducted a pulse, not struck a spark. To break down, the discharge must become self-sustained — able to keep itself going after the external agent that supplied the first electron is removed.

Townsend's insight was that the avalanche does not only deliver electrons to the anode; it also leaves behind a trail of positive ions and emits a burst of photons, and these can travel back to the cathode and knock loose new electrons. If, on average, each avalanche manages to liberate at least one replacement electron at the cathode, the process becomes a closed loop: avalanche → secondary electron → fresh avalanche → and so on, no longer needing any outside help. That single condition — one avalanche begetting at least one successor — is the Townsend criterion, and the rest of this chapter makes it precise.

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Breakdown is a loop, not a pulse
\[ \text{avalanche} \;\longrightarrow\; \text{secondary electron at cathode} \;\longrightarrow\; \text{new avalanche} \]

The primary coefficient \(\alpha\) builds the avalanche; the secondary coefficient \(\gamma\) closes the loop. Self-sustained breakdown needs both.

Section 5-2

The Primary Avalanche

Recall the multiplication law from Chapter 4. With the cathode supplying \(n_0\) electrons per second by some external means (irradiation, say), each multiplies by collision ionization as it drifts, so the number arriving at the anode of a gap \(d\) wide is \(n_0 e^{\alpha d}\). In terms of measurable current — the current that would flow if there were no secondary effects — this is the primary Townsend relation:

Primary avalanche current (no feedback yet)
\[ i = i_{0}\,e^{\alpha d} \]
cathode (−) anode (+) electron head e^{αd} n₀ slow positive ions left behind
The primary avalanche: electrons race ahead as a growing cloud while the heavy positive ions linger, drifting slowly back toward the cathode

Two things to notice set up everything that follows. First, the electrons reach the anode in nanoseconds, but the positive ions they leave behind are thousands of times heavier and crawl back toward the cathode far more slowly — so the ions are the messengers that carry the avalanche's influence back to where it began. Second, \(i = i_0 e^{\alpha d}\) alone can never run away: switch off \(i_0\) and the current vanishes. Something must regenerate \(i_0\) from within. That something is the secondary emission of the next section.

Section 5-3

Secondary Emission and the Coefficient γ

An avalanche feeds the cathode in several ways at once, and each can liberate a fresh electron there. Townsend lumped them all into a single number, the second ionization coefficient \(\gamma\): the average number of secondary electrons released at the cathode for every primary ionizing collision made in the gap. There are three contributing mechanisms.

Positive-ion bombardment (γi). The slow positive ions left in the avalanche's wake drift back and strike the cathode; if an ion arrives with enough energy it ejects an electron from the metal surface. This is usually the dominant secondary process at the low \(pd\) where Townsend's mechanism reigns.

Photoemission (γp). Excited molecules in the avalanche relax by emitting photons; those that strike the cathode can liberate electrons by the photoelectric effect.

Metastable and other surface effects (γm). Long-lived excited atoms reaching the cathode, and the neutralisation of ions at the surface, contribute further electrons.

cathode anode electrons → anode (α) positive ions → cathode photons → cathode γ : secondary electron released → new avalanche
The Townsend loop closes at the cathode: ions and photons returning from a primary avalanche eject the secondary electron that starts the next one

The single most important consequence of \(\gamma\) is that breakdown becomes cathode-dependent. Because the secondary electrons come from the metal surface, the breakdown voltage of a gap depends on what the cathode is made of and how clean it is — a feature that sharply distinguishes the Townsend mechanism from the streamer mechanism of Chapter 6, which needs no cathode help at all. Typical values of \(\gamma\) are small, from about \(10^{-2}\) down to \(10^{-4}\), which is exactly why the primary avalanche must grow enormously before so feeble a feedback can sustain it.

Section 5-4

The Complete Townsend Current

Now assemble the loop into an equation. Suppose the cathode emits \(n_0\) primary electrons per second. Each grows by \(e^{\alpha d}\), so \(n_0(e^{\alpha d}-1)\) new ion pairs are created in the gap. A fraction \(\gamma\) of these returns to liberate further electrons at the cathode, which themselves multiply, and so on. Summing the geometric series of successive generations gives the steady-state current:

The complete Townsend current equation
\[ i = \frac{i_{0}\,e^{\alpha d}}{1 - \gamma\!\left(e^{\alpha d} - 1\right)} \]

Read this carefully, because the whole physics hides in the denominator. When \(\gamma(e^{\alpha d}-1)\) is small, the denominator is close to one and the current is essentially the primary avalanche \(i_0 e^{\alpha d}\) — a non-self-sustained discharge that still needs \(i_0\). But as the voltage rises, \(\alpha\) grows, the term \(\gamma(e^{\alpha d}-1)\) climbs toward unity, and the denominator collapses toward zero. The current then grows without bound, limited in reality only by the external circuit. That run-away is breakdown.

current i voltage V → Vₛ i = i₀e^{αd} / [1 − γ(e^{αd}−1)] denominator → 0
As the denominator \(1-\gamma(e^{\alpha d}-1)\) approaches zero, the current runs away — the gap breaks down at \(V_s\)
Section 5-5

The Townsend Breakdown Criterion

The threshold of run-away is the value of voltage at which the denominator first reaches zero. Setting it to zero gives the celebrated Townsend breakdown criterion:

Self-sustaining condition
\[ \gamma\!\left(e^{\alpha d} - 1\right) = 1 \qquad\Longleftrightarrow\qquad \alpha d = \ln\!\left(1 + \tfrac{1}{\gamma}\right) \]

Its meaning is beautifully physical. The quantity \(e^{\alpha d}-1\) is the number of new ion pairs one avalanche creates; multiplying by \(\gamma\) gives the number of replacement electrons it produces at the cathode. The criterion says simply: each avalanche must produce exactly one successor. Below this, every generation is weaker than the last and the discharge dies; above it, every generation is stronger and the current explodes. Because \(\gamma\) is small, \(1/\gamma\) is large and the criterion is often written in the approximate form \(\gamma e^{\alpha d}\approx 1\), i.e. \(\alpha d \approx \ln(1/\gamma)\) — telling us the avalanche must reach a size of order \(1/\gamma\), typically \(10^{2}\)–\(10^{4}\), before it can sustain itself.

One number, two readings. The criterion fixes the breakdown voltage: since \(\alpha\) depends on \(E/p\) (Chapter 4), demanding \(\alpha d = \ln(1+1/\gamma)\) for a gap \(d\) at pressure \(p\) determines the field, and hence the voltage, at which the gap goes. Feeding the \(\alpha/p = A e^{-Bp/E}\) law into it produces Paschen's curve — the subject of Chapter 6.
Section 5-6

Time Lags of Breakdown

The criterion tells us whether a gap will break down, but not when. Under a slowly rising voltage the distinction hardly matters; under an impulse — a lightning or switching surge lasting microseconds — it is everything, because a gap that needs longer to break down than the surge lasts will simply survive a voltage well above its static threshold. The delay between applying an over-voltage and the collapse of the gap is the time lag, and it has two distinct parts.

The statistical time lag \(t_s\) is the wait for a suitably placed initiating electron to appear in the gap. Until one does, no avalanche can start, however high the field; \(t_s\) is random and is shortened by irradiating the gap or otherwise supplying seed electrons. The formative time lag \(t_f\) is the time the sequence of avalanches and secondary emissions then takes to build up to the full breakdown current once that first electron exists. The total time lag is their sum:

Total time lag
\[ t_{L} = t_{s} + t_{f} \]
V time → static Vₛ applied impulse V=Vₛ tₛ t_f collapse
An impulse can exceed the static level and still not break down until a seed electron appears (statistical lag) and the avalanche sequence develops (formative lag)

This is why a gap withstands a brief impulse of greater amplitude than it could endure as a steady voltage — the basis of the impulse ratio and of the volt–time curves used in insulation coordination later in the course.

Section 5-7

Where Townsend Holds — and Where It Fails

The Townsend picture is not universal. It rests on the assumption that many successive avalanches, linked through slow ion feedback at the cathode, are needed to build the discharge — and that assumption holds only at modest values of the product \(pd\), roughly up to a few hundred \(\mathrm{torr\cdot cm}\) (low pressures, short gaps). In this range the measured breakdown voltage depends on the cathode material, the time lags are relatively long, and everything the equations predict is borne out.

At large \(pd\) — atmospheric pressure across centimetre gaps, the everyday case of a power-system spark — three observations break the Townsend story. Breakdown is far faster than the ion-transit time the mechanism requires; it is essentially independent of the cathode; and it often follows a thin, branched, luminous channel rather than a diffuse glow. The reason is that a single avalanche has by then grown so large that the space charge of its own ions distorts the applied field, and the discharge propagates by photoionization in the gas ahead of it, with no need to wait for the cathode. That is the streamer mechanism, and together with Paschen's law it is the subject of the next chapter.

FeatureTownsend mechanismStreamer mechanism
Typical regimeLow \(pd\), short gapsHigh \(pd\), atmospheric gaps
Sustained byMany avalanches + cathode feedback (\(\gamma\))A single avalanche + photoionization ahead
Cathode materialMatters (cathode-dependent)Largely irrelevant
SpeedSlow (ion transit)Very fast
AppearanceDiffuse glowThin branched filament
Section 5-8

Worked Examples

1 Size of a primary avalanche

Problem. In a gap of \(d = 4~\mathrm{mm}\) the first ionization coefficient is \(\alpha = 5~\mathrm{mm^{-1}}\). How many electrons does one seed electron deliver to the anode, ignoring secondary effects?

Solution. The primary multiplication is \(e^{\alpha d}\):

Working
\[ e^{\alpha d} = e^{(5)(4)} = e^{20} \approx 4.85\times10^{8} \]

A single electron becomes nearly half a billion by the anode — yet this is still only a one-shot pulse. Whether it sustains depends entirely on \(\gamma\).

2 Current with feedback

Problem. A gap has \(\alpha d = 6\), a secondary coefficient \(\gamma = 1.5\times10^{-3}\), and a primary current \(i_0 = 10~\mathrm{pA}\). Find the actual current and compare it with the primary avalanche alone.

Solution. Use the complete Townsend equation. First \(e^{\alpha d}=e^{6}=403.4\):

Working
\[ i = \frac{i_0 e^{\alpha d}}{1-\gamma(e^{\alpha d}-1)} = \frac{10\times403.4}{1-1.5\times10^{-3}(402.4)} = \frac{4034}{0.396}\approx 1.0\times10^{4}~\mathrm{pA} \]

The primary avalanche alone gives \(i_0 e^{\alpha d}\approx 4034~\mathrm{pA}\); the feedback inflates it to about 10 200 pA, a factor of \(1/0.396\approx 2.5\). The denominator (0.396) is already well below one — the gap is approaching breakdown.

3 The breakdown criterion

Problem. For a cathode with \(\gamma = 10^{-2}\), what value of \(\alpha d\) just makes the gap self-sustaining?

Solution. Breakdown requires \(\gamma(e^{\alpha d}-1)=1\), so \(\alpha d=\ln(1+1/\gamma)\):

Working
\[ \alpha d = \ln\!\left(1+\tfrac{1}{10^{-2}}\right) = \ln(101) \approx 4.62 \]

The avalanche must reach \(e^{4.62}\approx 101\) electrons — exactly \(1/\gamma\), as expected — before one successor is guaranteed and the gap goes. A cleaner cathode (smaller \(\gamma\)) would demand a larger \(\alpha d\), hence a higher breakdown voltage.

4 Cathode dependence of breakdown

Problem. The same gas and gap are tested with two cathodes: one with \(\gamma_1 = 10^{-2}\), one with \(\gamma_2 = 10^{-4}\). By how much does the required avalanche size \(\alpha d\) differ?

Solution. Apply \(\alpha d=\ln(1+1/\gamma)\) to each:

Working
\[ \alpha d_1=\ln(101)=4.62,\qquad \alpha d_2=\ln(10001)=9.21,\qquad \Delta(\alpha d)\approx 4.6 \]

The cleaner cathode needs roughly twice the avalanche growth, and therefore a markedly higher field and breakdown voltage. This measurable cathode-dependence is the experimental fingerprint of the Townsend mechanism — and its absence at high \(pd\) is what reveals the streamer.

Review

Chapter Summary

Avalanche ≠ breakdown

The primary avalanche \(i=i_0 e^{\alpha d}\) is a one-shot pulse. Breakdown needs the gap to regenerate its own seed electrons.

The coefficient γ

Secondary electrons at the cathode — from ion bombardment, photoemission and metastables — are gathered into \(\gamma\), making breakdown cathode-dependent.

Complete current

\(i=\dfrac{i_0 e^{\alpha d}}{1-\gamma(e^{\alpha d}-1)}\); all the physics sits in the denominator, which collapses toward zero at breakdown.

The criterion

\(\gamma(e^{\alpha d}-1)=1\): each avalanche must beget exactly one successor. It fixes the breakdown voltage and leads to Paschen's law.

Time lags

\(t_L=t_s+t_f\): the wait for a seed electron plus the avalanche build-up. They let a gap survive a brief impulse above its static level.

Its limits

Townsend holds at low \(pd\). At high \(pd\) breakdown is faster, cathode-independent and filamentary — the streamer takes over.

Practice

Problems

For each item, first name the idea it tests — the primary avalanche, the coefficient \(\gamma\), the complete current, the breakdown criterion, the time lags, or the limits of the mechanism — then work it through. Difficulty rises down the list.

  1. Explain in one or two sentences why \(i=i_0 e^{\alpha d}\), by itself, cannot describe a self-sustained discharge.
  2. Name the three secondary processes folded into \(\gamma\), and state which usually dominates at the low \(pd\) where Townsend's mechanism applies.
  3. A gap has \(\alpha = 3~\mathrm{mm^{-1}}\) and \(d = 5~\mathrm{mm}\). Find the primary multiplication \(e^{\alpha d}\).
  4. Why does the Townsend breakdown voltage depend on the cathode material, while the streamer breakdown voltage does not?
  5. For \(\gamma = 5\times10^{-3}\), find the value of \(\alpha d\) at which the gap just becomes self-sustaining.
  6. A gap has \(\alpha d = 7\), \(\gamma = 8\times10^{-4}\) and \(i_0 = 5~\mathrm{pA}\). Compute the actual current from the complete Townsend equation, and the value of the denominator.
  7. Distinguish the statistical time lag from the formative time lag, and state one practical way to shorten the statistical lag.
  8. Using the criterion \(\alpha d=\ln(1+1/\gamma)\), find the percentage increase in required \(\alpha d\) when \(\gamma\) falls from \(10^{-2}\) to \(10^{-3}\).
  9. A measurement gives a denominator \(1-\gamma(e^{\alpha d}-1)=0.05\) just below breakdown. If \(\gamma = 2\times10^{-3}\), find \(e^{\alpha d}\) and \(\alpha d\), and state how far the gap is from the self-sustaining point.
  10. List three experimental observations at atmospheric pressure that the Townsend mechanism fails to explain, and name the mechanism that does.
Tip: the entire chapter lives in one fraction. The numerator \(i_0 e^{\alpha d}\) is the primary avalanche from Chapter 4; the denominator \(1-\gamma(e^{\alpha d}-1)\) is the cathode feedback that Chapter 4 lacked. Track that denominator and everything follows — it near one means a harmless multiplying current, it near zero means run-away, and it exactly zero is the breakdown criterion. Carry that single fraction forward and Paschen's curve in Chapter 6 is just this criterion plotted against \(pd\).