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              Dielectric Gases                                                                            361





































                     FIGURE 1  Ionization cross section σ i  (ε) for N 2  and SF 6  close to the ionization onset I . Electron-scattering cross
                     section as a function of ε for N 2  and electron-attachment cross section σ a (ε) for SF 6 . Normalized electron energy
                     distribution function ε 1/2 f (ε, E /N) as a function of ε for N 2  at two values of E /N. [From Christophorou, L. G., et al.
                     (1984). IEEE Trans, Elect. Insul. El-19, 550–566.]


              electron produces a successor, the current maintains itself  Thus  (see  Fig.  2)  for  pure  SF 6 , (E /N) lim  = 3.61 ×
                                                                         2
              and becomes independent of γ .                    10 −15  V cm , and it decreases as N 2  is added in the binary
                For an electronegative gas the situation is different be-  mixture.
              cause in this case the free electrons can be effectively pre-  For nonuniform fields,  ¯α is a function of the position
              ventedfrominitiatingbreakdowniftheyattachthemselves  between the electrodes, and the breakdown voltage V s  can
              to gas molecules and form stable negative ions. The total  be calculated from the so-called streamer criterion,
              attachment cross section σ a (ε) for SF 6  is shown in Fig. 1.

                                                                                 x 0
              In general, σ a (ε) is large at very low energies, and thus          ¯ α(x) dx = k ,         (6)
              only electrons with energies at the extreme low-energy            0
              range can be removed efficiently by electron attachment.
                                                                where  x 0  is the length at which the electron avalanche
              The shaded area in Fig. 1 that is designated by η is a mea-                             8
                                                                reaches  the  critical  number  of  electrons  (∼10 )  in  the
              sure of the effective electron attachment coefficient η/N a
                                                                avalanche tip for causing streamer formation. The k is a
              [Eq. (2)]. Knowledge of α/N and η/N a  allows one to pre-
                                                                constant characteristic of the gas. It is generally accepted
              dict (E /N) lim , which for static uniform fields and a unary
                                                                that photoionization processes play a role in the propaga-
              gas is defined as the value of E /N at which α = η, namely,
                                                                tion of the streamer.
                       γ [exp{(α − η)d }− 1] = 1 − η/α.  (4)      For the gas dielectric strength to be optimized, not only
                                                                must σ i (ε) be small and σ a (ε) be large [and extend to high
              Both α/N  and η/N a  are functions of  E /N  (see Figs. 2
                                                                energies to maximize the overlap of σ a (ε) and  f (ε, E /N),
              and 3). Most often, one measures the so-called effective
                                                                as in Eq. (2)], but the electron energies must be as low as
              ionization coefficient (α − η)/N (see Fig. 2), and the static
                                                                possible because a low-lying  f (ε, E /N) minimizes α and
              uniform field breakdown strength (E /N) lim  is defined as
                                                                maximizes η. Many studies, however, clearly show that
              the value of E /N for which
                                                                high breakdown strengths require large σ a (ε). This can be
                           (α − η)/N ≡  ¯α/N = 0.        (5)    seen from the examples in Fig. 3. As the attachment-rate
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