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The time decay of electron density in pulsed helium afterglow discharges is studied experimentally employing both conventional and modified microwave-cavity techniques. The two methods permit density measurements from nₑ10¹¹ cm^-3 to as low as nₑ2×10⁴ cm^-3 in helium at pressures of 0.4 and 4.0 Torr. For Debye lengths less than {~}1% of the characteristic diffusion length Λ, the electron loss rate is through ambipolar diffusion controlled by the atomic ion He⁺ at 0.4 Torr and by the molecular ion He₂^_⁺ at 4.0 Torr. At lower electron densities, the electrons diffuse more rapidly than ambipolar diffusion, and in the limit of Debye lengths much greater than the characteristic diffusion length, the electrons diffuse freely to the walls. The experimentally observed effective diffusion coefficient Dₛ in the transition region is compared with a mathematical expression proposed by Phelps relating Dₛ to nₑ. Satisfactory agreement is obtained at 4.0 Torr where the electron mean free path λΛ. By using this expression to calculate theoretically expected decays of electron density, a computer optimization procedure produced an even better fit to experimental data by slightly altering a numerical parameter in the formula. At 0.4 Torr, where λ≈Λ and the theoretical treatment is not expected to be valid, diffusion in the transition region is observed to occur at a rate substantially less than that predicted theoretically.
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Freiberg et al. (1968) studied this question.
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