Part 2 · Chapter 6

Streamer Theory and Paschen's Law

Chapter 5 ended with one equation, \(\gamma(e^{\alpha d}-1)=1\), and two loose ends. Fed with the field's dependence on pressure and gap, that criterion blooms into Paschen's law — a single curve, with a famous minimum, that governs every low-pressure gap. But at atmospheric pressure breakdown is faster than the criterion allows, and indifferent to the cathode it relies on. This chapter ties off both ends: first the law, then the streamer that supersedes it.

High-Voltage Engineering Prof. Mithun Mondal Reading time ≈ 45 min
i What you'll learn
  • How to turn the Townsend criterion into Paschen's law — breakdown voltage as a function of the product \(pd\) alone.
  • The shape of the Paschen curve, why it has a minimum, and the simple formulas for \((pd)_{\min}\) and \(V_{\min}\).
  • The contrasting physics of the left and right branches — too few collisions versus too many.
  • Why, at high \(pd\), a single avalanche grows large enough for its own space charge to distort the applied field.
  • The streamer mechanism: propagation by photoionization ahead of the front, and cathode- versus anode-directed streamers.
  • The Raether–Meek criterion \(\alpha x_c \approx 18\text{–}20\) that marks the avalanche-to-streamer transition.
Section 6-1

From Criterion to a Law

The Townsend criterion of Chapter 5, \(\gamma(e^{\alpha d}-1)=1\), is a statement about a particular gap at a particular voltage. To make it useful we want a law: a formula that predicts the breakdown voltage of any uniform-field gap from the things we control — the gas, the pressure \(p\), and the spacing \(d\). The bridge is the dependence of \(\alpha\) on the reduced field, which we met in Chapter 4. Since \(\gamma\) is small, the criterion is well approximated by demanding that the avalanche reach a fixed size:

The criterion as a fixed avalanche size
\[ \alpha d = \ln\!\left(1+\tfrac{1}{\gamma}\right) \equiv K \quad(\text{a constant for a given gas and cathode}) \]

Everything now hinges on writing \(\alpha\) in terms of \(p\) and the field \(E=V/d\) (uniform field), substituting, and solving for the voltage \(V\). When we do, a small miracle occurs: \(p\) and \(d\) appear only ever as the product \(pd\). The breakdown voltage of a uniform gap is not a function of pressure and spacing separately, but of their product alone. This is Paschen's law, discovered experimentally in 1889 and here recovered from first principles.

Section 6-2

Deriving Paschen's Law

Start from the experimental fit for the first ionization coefficient and put \(E=V/d\):

Ionization coefficient in a uniform gap
\[ \frac{\alpha}{p} = A\,e^{-Bp/E} \;\Longrightarrow\; \alpha = A p\,\exp\!\left(-\frac{Bpd}{V}\right) \]

Multiply by \(d\) and impose the criterion \(\alpha d = K\):

Applying the breakdown criterion
\[ A\,(pd)\,\exp\!\left(-\frac{Bpd}{V}\right) = K = \ln\!\left(1+\tfrac1\gamma\right) \]

Take logarithms and rearrange for \(V\). The result is Paschen's law in closed form — the breakdown voltage as an explicit function of the single variable \(pd\):

Paschen's law
\[ V_{b} = \frac{B\,(pd)}{\ln\!\left[\dfrac{A\,(pd)}{\ln\!\left(1+\tfrac1\gamma\right)}\right]} \]

The constants \(A\) and \(B\) are properties of the gas (for air, roughly \(A\approx 15~(\mathrm{cm\cdot torr})^{-1}\) and \(B\approx 365~\mathrm{V/(cm\cdot torr)}\) over the usual range), and \(\gamma\) carries the cathode. The formula is unwieldy to look at but tells a clean story once plotted, which is the next section.

Why \(pd\), physically. Breakdown needs an electron to make a fixed number of ionizing collisions crossing the gap. The number of collisions available is set by how many molecules lie in its path — and that is proportional to pressure times distance, \(pd\). Squeeze the gas and shorten the gap in inverse proportion, and the electron meets the same molecules and breaks down at the same voltage.
Section 6-3

The Paschen Curve and Its Minimum

Plotted against \(pd\), Paschen's law traces a distinctive U-shape: the breakdown voltage is high at very small \(pd\), falls to a minimum, and rises again at large \(pd\). That a curve with a minimum should exist at all is the law's most striking and useful feature.

V_b pd (log scale) → (pd)ₘᵢₙ Vₘᵢₙ left branch too few collisions right branch too many collisions
The Paschen curve: breakdown voltage is minimum at an optimum \(pd\), and rises on either side for opposite reasons

The minimum is found by differentiating \(V_b\) with respect to \(pd\) and setting the derivative to zero. The algebra yields compact expressions for the optimum product and the minimum sparking voltage:

The Paschen minimum
\[ (pd)_{\min} = \frac{e}{A}\,\ln\!\left(1+\tfrac1\gamma\right), \qquad V_{\min} = \frac{e\,B}{A}\,\ln\!\left(1+\tfrac1\gamma\right) \]

Here \(e=2.718\) is Euler's number. For air the minimum sits at a few hundred volts — about \(327~\mathrm{V}\) near \(pd \approx 0.57~\mathrm{torr\cdot cm}\) — and remarkably, no uniform air gap, at any pressure or spacing, can be broken down by less than this. It is a hard floor on sparking voltage, and it explains why vacuum and very small gaps can hold off surprisingly little voltage: you cannot get below the Paschen minimum.

Section 6-4

Reading the Two Branches

The two arms of the curve climb for opposite physical reasons, and understanding them is more valuable than memorising the formula.

The right branch (large \(pd\)). At high pressure or wide gaps there are too many molecules. An electron collides so often that it cannot gather the ionization energy between impacts; each free path is short, so a higher field — and hence a higher voltage — is needed to make each collision count. As \(pd\) grows, \(V_b\) rises roughly in proportion. This is the everyday branch of atmospheric, centimetre-scale gaps.

The left branch (small \(pd\)). At very low pressure or tiny gaps there are too few molecules. Now an electron may cross the whole gap making only a handful of collisions — sometimes none — so even though each electron is highly energetic, there are simply not enough ionizing events to build an avalanche. A higher voltage is required to ensure that the rare collisions that do occur are all ionizing. This is the branch of vacuum gaps and micro-gaps, and its rising trend is why a near-perfect vacuum is an excellent insulator.

low pd — few molecules crosses, barely ionizes → V↑ high pd — dense gas collides often, gains little → V↑
Both branches need a higher voltage, for opposite reasons: too few collisions on the left, too little energy per collision on the right
Section 6-5

When a Single Avalanche Wins

Paschen's law and the Townsend mechanism behind it work beautifully at low \(pd\). But at atmospheric pressure across a centimetre gap — \(pd\) of several hundred torr·cm — careful measurement contradicts the theory on three counts, all flagged at the end of Chapter 5: breakdown is far too fast for ion feedback, it ignores the cathode material, and it carves a thin luminous channel rather than a uniform glow. The resolution lies in something Townsend's accounting quietly ignored: the avalanche's own charge.

By the time an avalanche has grown to perhaps \(10^{8}\) electrons, the fast electrons crowd at its head and the slow positive ions trail behind, forming a compact dipole of space charge. The field this dipole produces is no longer negligible — it becomes comparable to the applied field itself. In front of and behind the avalanche head the two fields add; on its flanks they oppose. The applied field is locally distorted, intensely strengthened just ahead of the advancing tip, and the orderly Townsend picture of independent electrons drifting in a uniform field collapses.

applied field E₀ → + + ion tail − electron head field intensified ahead
A critical-size avalanche is a space-charge dipole; its own field reinforces the applied field just ahead of the electron head, setting the stage for a streamer
Section 6-6

The Streamer Mechanism

The intensified field at the avalanche head does two things. It accelerates ionization locally, and — crucially — the excited and recombining molecules there emit a copious flood of ultraviolet photons. These photons fly out into the gas ahead of the head and, by the photoionization of Chapter 4, liberate fresh electrons in the region of already-enhanced field. Each such electron immediately launches its own secondary avalanche, which is drawn straight back into the head, lengthening and brightening it. The discharge no longer waits for slow ions to crawl to the cathode; it advances by photons at nearly the speed of light, growing a thin, branching, self-propagating filament — a streamer.

cathode anode head photons (hν) secondary avalanches → merge into front streamer →
The streamer propagates by photoionization: photons from the head seed avalanches ahead, which merge in and carry the filament forward at near light speed

Two kinds of streamer are distinguished by the direction of advance. A cathode-directed (positive) streamer develops once the primary avalanche has reached the anode: its positive-ion trail, reinforced by photoelectrons from the gas, extends back toward the cathode, and is the common form in long gaps. An anode-directed (negative) streamer can form before the avalanche reaches the anode, when the head's field is already critical, and advances forward toward the anode. In either case, once a streamer bridges the gap it provides a conducting channel and the spark follows at once. Because the whole process is driven by photons in the gas volume, it needs no help from the cathode — exactly the cathode-independence that the measurements demanded.

Section 6-7

The Raether–Meek Criterion

The transition from a harmless avalanche to a self-propagating streamer happens when the avalanche's space-charge field grows to roughly the size of the applied field. Raether and, independently, Meek quantified this. The space-charge field at the head depends on how many electrons it carries, \(e^{\alpha x}\), so the condition for transition is reached when the avalanche has travelled a critical distance \(x_c\) such that this number reaches about \(10^{8}\). In its most-used form the criterion is simply:

Raether–Meek streamer criterion
\[ \alpha\,x_{c} \approx 18\text{–}20 \qquad\Longleftrightarrow\qquad e^{\alpha x_c} \approx 10^{8} \]

Meek's fuller statement equates the radial space-charge field of the avalanche head to the applied field \(E\), giving a relation of the form \(E_{r}\approx 5.3\times10^{-7}\,\dfrac{\alpha\,e^{\alpha x}}{\sqrt{x/p}} = E\), but the round number \(\alpha x_c \approx 20\) captures the essential idea for design: breakdown by streamer requires an avalanche to reach a critical multiplication before it crosses the gap. Where \(\alpha d < 18\) the gap tends to break down in the slow, cathode-dependent Townsend way; where \(\alpha d\) comfortably exceeds 20, the fast streamer dominates. The two mechanisms are not rivals so much as the same physics at different \(pd\), and the table below sets the boundary in context.

QuantityTownsend regimeStreamer regime
Governing lawPaschen's law (criterion \(\alpha d = \ln(1+1/\gamma)\))Raether–Meek (\(\alpha x_c \approx 18\text{–}20\))
Typical \(pd\)Low (below ~200 torr·cm)High (atmospheric, long gaps)
Sustained byCathode secondary emission \(\gamma\)Photoionization in the gas
Critical avalanche\(e^{\alpha d}\sim 1/\gamma\) (\(10^2\)–\(10^4\))\(e^{\alpha x_c}\sim 10^{8}\)
Cathode materialDecisiveIrrelevant
Section 6-8

Worked Examples

1 Paschen's law depends on pd alone

Problem. A uniform gap breaks down at \(V_b\) at pressure \(p\) and spacing \(d\). The pressure is then doubled and the spacing halved. What happens to the breakdown voltage, and why?

Solution. The product is unchanged:

Working
\[ (2p)\!\left(\tfrac{d}{2}\right) = pd \;\Rightarrow\; V_b\;\text{unchanged} \]

Because \(V_b\) is a function of \(pd\) only, halving the gap while doubling the pressure leaves the breakdown voltage exactly the same. The electron meets the same number of molecules along its path.

2 The Paschen minimum

Problem. For a gas with \(A = 15~(\mathrm{cm\cdot torr})^{-1}\), \(B = 365~\mathrm{V/(cm\cdot torr)}\) and a cathode giving \(\gamma = 10^{-2}\), find \((pd)_{\min}\) and \(V_{\min}\).

Solution. First \(\ln(1+1/\gamma) = \ln(101) = 4.615\). Then use the minimum formulas with \(e = 2.718\):

Working
\[ (pd)_{\min} = \frac{2.718}{15}(4.615) = 0.836~\mathrm{torr\cdot cm}, \quad V_{\min} = \frac{2.718\times365}{15}(4.615) \approx 305~\mathrm{V} \]

The minimum sparking voltage is about 305 V near \(pd \approx 0.84~\mathrm{torr\cdot cm}\) — close to the measured air value (~327 V), and a hard floor: no such gap breaks down at less.

3 Streamer-onset gap (Raether–Meek)

Problem. In atmospheric air at a certain field the ionization coefficient is \(\alpha = 50~\mathrm{cm^{-1}}\). Estimate the avalanche length \(x_c\) at which it converts to a streamer, and the number of electrons in the head.

Solution. Use \(\alpha x_c \approx 20\):

Working
\[ x_c = \frac{20}{\alpha} = \frac{20}{50} = 0.4~\mathrm{cm} = 4~\mathrm{mm}, \qquad e^{\alpha x_c} = e^{20} \approx 4.85\times10^{8} \]

Within about 4 mm the avalanche reaches the critical \(\sim 5\times10^{8}\) electrons and turns into a streamer. A gap wider than this in such a field will break down by the fast streamer route.

4 Which mechanism?

Problem. Decide whether breakdown is Townsend or streamer for (a) a discharge tube at \(p = 2~\mathrm{torr}\), \(d = 5~\mathrm{cm}\); (b) a sphere gap in air at \(760~\mathrm{torr}\), \(d = 1~\mathrm{cm}\).

Solution. Compare the product \(pd\):

Working
\[ \text{(a)}\; pd = 2\times5 = 10~\mathrm{torr\cdot cm}\;(\text{low}); \qquad \text{(b)}\; pd = 760\times1 = 760~\mathrm{torr\cdot cm}\;(\text{high}) \]

Case (a), at low \(pd\), is the home of the Townsend mechanism and Paschen's law. Case (b), at high \(pd\), breaks down fast and cathode-independently by a streamer — the everyday case for high-voltage apparatus in air.

Review

Chapter Summary

Criterion → law

Putting \(\alpha = Ap\,e^{-Bpd/V}\) into \(\alpha d = \ln(1+1/\gamma)\) makes \(p\) and \(d\) appear only as \(pd\) — that is Paschen's law.

Paschen's law

\(V_b = \dfrac{B(pd)}{\ln[A(pd)/\ln(1+1/\gamma)]}\): breakdown voltage of a uniform gap is a function of \(pd\) alone.

The minimum

\(V_{\min} = \dfrac{eB}{A}\ln(1+1/\gamma)\) — about 327 V for air. A hard floor on sparking voltage no gap can beat.

Two branches

Right branch: too many collisions, too little energy each. Left branch: too few collisions to build an avalanche. Both raise \(V_b\).

Streamer

At high \(pd\) a single avalanche's space charge distorts the field; photoionization ahead drives a fast, cathode-independent filament.

Raether–Meek

The avalanche becomes a streamer when \(\alpha x_c \approx 18\text{–}20\), i.e. the head reaches about \(10^8\) electrons.

Practice

Problems

For each item, first name the idea it tests — the derivation, Paschen's law, the minimum, the branches, space charge, the streamer, or the Raether–Meek criterion — then work it through. Difficulty rises down the list.

  1. State Paschen's law in words, and explain why pressure and gap appear only through their product \(pd\).
  2. A gap breaks down at \(30~\mathrm{kV}\) at \(1~\mathrm{bar}\) over \(10~\mathrm{mm}\). Estimate the breakdown voltage at \(2~\mathrm{bar}\) over \(5~\mathrm{mm}\), and justify your answer.
  3. Sketch the Paschen curve, label the minimum and both branches, and say which branch describes an ordinary atmospheric air gap.
  4. For \(A = 15~(\mathrm{cm\cdot torr})^{-1}\), \(B = 365~\mathrm{V/(cm\cdot torr)}\), \(\gamma = 10^{-3}\), compute \((pd)_{\min}\) and \(V_{\min}\).
  5. Explain physically why the breakdown voltage rises as \(pd\) is reduced below the Paschen minimum.
  6. Why is the breakdown voltage of the streamer mechanism essentially independent of the cathode material, whereas the Townsend voltage is not?
  7. In air \(\alpha = 40~\mathrm{cm^{-1}}\). Find the critical avalanche length for streamer onset and the number of electrons at the head.
  8. Describe how a cathode-directed (positive) streamer differs from an anode-directed (negative) one in its direction of growth and the moment it forms.
  9. A \(d = 6~\mathrm{mm}\) air gap has \(\alpha = 28~\mathrm{cm^{-1}}\). Compute \(\alpha d\), and decide whether the gap is likely to break down by the Townsend or the streamer mechanism.
  10. Using \(V_b = B(pd)/\ln[A(pd)/K]\) with \(K = \ln(1+1/\gamma)\), explain why \(V_b\) tends to rise almost linearly with \(pd\) far out on the right branch.
Tip: the chapter has one hinge — the size an avalanche must reach to provoke breakdown. In the Townsend world that size is modest, \(\sim 1/\gamma\), and the bookkeeping gives Paschen's \(pd\) law and its minimum. In the streamer world the size is enormous, \(\sim 10^{8}\), set instead by when the avalanche's own space charge rivals the applied field. Same avalanche, same coefficient \(\alpha\), two thresholds — and which one a gap meets first is decided almost entirely by \(pd\). Hold that and the next chapter's non-uniform fields and corona follow naturally.