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Fig. 5

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Rate coefficients for total ionization through the processes He(23S)+H→He(11S)+H++e, →HeH++e. We calculated these from the (scanned) cross sections reported in the quoted references over a range of temperatures commensurate with the range of energies at which they were reported. The calculations were performed by means of standard expressions and assumed a Maxwellian distribution for the relative velocities between the colliders. Occasionally, we extrapolated the cross sections toward low energies with a ∝E−0.2 law (E is the center-of-mass kinetic energy) and toward high energies with a ∝E−1 law. (References: MI72, Miller et al. (1972); CL73, Cohen & Lane (1973); HM77, Hickman & Morgner (1977); FO78, Fort et al. (1978); MN79, Morgner & Niehaus (1979); WA88, Waibel et al. (1988); MM97, Movre & Meyer (1997)). Also included is the value quoted by Roberge & Dalgarno (1982) and the temperature-dependent expression utilized by Fassia et al. (1998). The expression k [cm3s−1]=10−9 exp(c/T + d1 ln T + d2(ln T)2 + d3(ln T)3) (c=−8.64804E+01; d1=−2.86766E−01; d2=+8.68445E−02; d3=−5.73001E−03) fits the rate coefficient based on the Movre & Meyer (1997) cross sections with errors of <2% from 200 to 10 000 K.

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