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The temperature dependence of the afterglow decay of electrons and ions from microwave discharges in nitrogen-neon gas mixtures has been studied using combined microwave and mass-spectrometric techniques. Under conditions where N₂^_⁺ is the only significant afterglow ion species, i.e., at nitrogen pressures less than 10^-2 Torr, and for neon pressures in the range 15 to 40 Torr, the afterglow is controlled by the recombination of N₂^_⁺ ions and electrons. Over the temperature range studied, 205 to 480^∘{}K, the recombination coefficients exhibit no significant temperature dependence and can be represented by the constant value α(N₂^_⁺)=(2.7±0.3)×10^-7 cm³/sec. At any given temperature the results show no systematic dependence on the nitrogen or neon gas pressure over the ranges indicated. Temporal mass analysis indicates similar decay rates for the N₂^_⁺ ions and for the electrons over the major portion of the afterglow.
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W. H. Kasner (1967) studied this question.
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