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Electron avalanche

Equations 2.7 and 2.11 can be combined into a more general expression which can be solved to determine the change in electron density due to both $\nu_i$ and $\nu_a$:


\begin{displaymath}
\frac{dn_e}{dt} = (\nu_i-\nu_{a})n_e
\end{displaymath} (2.13)


\begin{displaymath}
n_{e}(t) = n_{o}e^{(\nu_i-\nu_{a})t}
\end{displaymath} (2.14)

It is clear from Equation 2.14 that the electron density will increase exponentially if $\nu_i\!>\!\nu_a$. This occurs when $E/N
\gtrsim 123$ Td in Figure 2.1. An exponential increase of electrons from one or more seed electrons is an electron avalanche.

An electron avalanche will develop at the electron drift velocity, $\vec{v}_e$. As it develops, the avalanche will expand due to diffusion and mutual electrostatic repulsion. The diffusion expansion dominates during the initial stages while electrostatic repulsion dominates in the latter stages as a result of the growing number of electrons (Bazelyan and Raizer, 1997, p. 80). An electron avalanche will also leave behind a trail of relatively immobile positively charged ions. A schematic illustration of an electron avalanche is shown in Figure 2.2a.

Figure 2.2: a) A schematic diagram of an electron avalanche. The electrons leave behind a trail of positive ions as they propagate towards the positively charged anode. b) An actual photograph of individual electron avalanches. (From Raether (1964)).
\begin{figure}\begin{center}
\par\epsfig{file=eps/avalanche.eps,height=3.5in}\par\par\par\end{center}\end{figure}

In a laboratory experiment where $n_o$ is sufficiently small, electron avalanches starting from a single electron can be clearly distinguished on a photograph. Figure 2.2b shows a photograph from Raether (1964) of electron avalanches which began in this fashion. Electron avalanches can transition into streamers and are also a fundamental component of streamers, as will be discussed in Section 2.6. The relevance of electron avalanches and streamers to sprites will be shown in Chapter 5.


next up previous contents
Next: Atmospheric Models Up: Breakdown basics Previous: Ionization, Recombination, and Attachment   Contents
Mark Stanley 2000-10-22