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               360                                                                                    Dielectric Gases


               (reaction 12) or positive and negative ions (reaction 13);  η     E        2    1/2  −1     ∞     E     1/2
               can collisionally detach electrons from negative ions (re-  =        w       f ε,   ε  σ a (ε) d ε,
                                                                   N a  N     m         0       N
               actions 14 and 15) or convert one ionic species to another
               (reaction 16) (and thus change its stability); or can change                                  (2)
               the ion’s size (and thus its mobility) by clustering (reac-  where  I  is the ionization onset energy,  N  the total gas
               tion 17). While the role of these processes may be less ob-  number density, and N a  the attaching gas number density;
               viousthantherolesofgroupsAandB,itcan,dependingon  for a unary electronegative gas dielectric N = N a , but for
               the prevailing conditions, be most significant. For exam-  mixtures containing electronegative and nonelectronega-
               ple, the gas dielectric behavior under steep-fronted voltage  tive components N a  < N.
               pulses is affected by the availability of “initiating” elec-
               trons produced by reactions 14 and 15. Similarly, corona
                                                                 B.  Dielectric Properties
               stabilization (Section III.B) is influenced by the electron–
               ion (12) and ion–ion (13) recombination processes.  Having elaborated briefly on the basic physical processes
                 Understanding of the phenomena preceding the tran-  occurring in electrically stressed dielectric gases, we can
               sition of the gas from an insulator to a conductor (pre-  appropriately  ask  the  question:  How  can  the  dielectric
               breakdown phenomena) and the mechanisms involved in  properties of a gaseous medium be optimized based on
               discharge initiation and development invariably requires  knowledge of such processes? To illustrate the type of
               basic knowledge on at least a fraction of the processes in  answer one can get to this question let us see how knowl-
               Table I. This knowledge comes from two sources: low-  edge  of  the  electron-attaching,  electron  slowing-down,
               pressure beam experiments and high-pressure swarm ex-  and electron impact-ionization properties of gases allows
               periments.Inhigh-pressureswarmexperiments,asinelec-  one to choose and to tailor gaseous dielectrics. This can be
               trically stressed gas dielectrics, the free electrons attain an  seen by referring to Fig. 1. When the value of E /N is low
               equilibrium energy distribution  f (ε, E/N), and the mea-  (e.g., 1.24 × 10 −16  V cm in Fig. 1 for N 2 ), f (ε, E /N) lies
                                                                                     2
               sured electron trasport coefficients (the electron drift ve-  at low energies, and the number of electrons capable of
               locity w and the ratio  D T  /µ of the transverse diffusion  ionizing the gas is negligible (i.e., the gas is an insulator).
               coefficient  D T  to the electron mobility µ) are related to  As the voltage is increased, however,  f (ε, E /N) shifts to
               the cross sections for the microscopic electron–molecule  higher energies, and for sufficiently high E /N values the
               interactions through  f (ε, E/N). In principle, from a mea-  number of electrons capable of ionizing the gas is such that
               surement of w(E/N) and  D T  /µ(E/N) and a knowledge  the gas makes the transition from an insulator to a conduc-
               of the electron scattering cross section,  f (ε, E/N) can be  tor. In Fig. 1,  f (ε, E /N) is shown for N 2  at the limiting
                                                                                                      2
               calculated through the Boltzmann transport equation or by  value of E /N , (E /N) lim  (
1.3 × 10 −15   V cm ) (i.e., the
               Monte Carlo methods. If, then, for a given gas dielectric  value of E /N  at which breakdown occurs). Even at this
               the various cross sections are known, they can be inte-  high E /N value only a small fraction of electrons possess
               grated over  f (ε, E/N) and used along with the appropri-  sufficient energy to induce ionization, which, nonetheless,
               ate charge conservation equations to determine the current  for a non-electron-attaching gas such as N 2 , is sufficient
               growth in the gas and predict its breakdown voltage. In  to promote gas breakdown. This is designated in Fig. 1 by
               practice this is difficult because neither the cross sections  the shaded area α, which is a measure of the ionization
               nor  f (ε, E /N) is known for the majority of the dielectric  coefficient α/N [Eq. (1)].
               gases or gas mixtures, so one resorts to the more easily  For a non-electron-attaching gas and a uniform field,
               accessible swarm coefficients to predict the discharge de-  knowledge of α provides a measure of (E/N) lim through
               velopment and behavior.                           the so-called Townsend breakdown criterion,
                 From high-pressure swarm studies, the coefficients for               αd
                                                                                  γ (e  − 1) = 1.            (3)
               excitation,  detachment,  and  ion–molecule  reactions  are
               obtained as functions of E /N, as well as the primary ion-  In Eq. (3), αd is the number of electrons generated by an
               ization coefficient α and the effective electron attachment  electron leaving the cathode and arriving as an electron
               coefficient η. Most of the data are on the latter two coeffi-  avalanche at the anode (at a distance d from the cath-
               cients.Thecoefficients α and η aremostsignificantandare  ode), and γ is the so-called secondary ionization coeffi-
               related to the respective ionization, σ i (ε), and attachment,  cient, defined as the number of secondary electrons pro-
               σ a (ε), cross sections and  f (ε, E /N) by       duced perprimary ionization. These secondary-electron
                                                                 processes include (1) electron emission from the cathode
                               1/2

                  α E       2      −1  ∞      E   1/2            as it is struck and photons, positive ions, and metastable



                        =        w       f ε,    ε  σ i (ε) d ε,
                 N N        m         I       N                  molecules and (2) gas processes such as photoionization
                                                          (1)    of the gas. Physically, Eq. (3) states that when each initial
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