2002
DOI: 10.1063/1.1426246
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Xenon charge exchange cross sections for electrostatic thruster models

Abstract: Charge exchange between xenon ions and xenon atoms is the source of a detrimental low energy plasma in the vicinity of electrostatic spacecraft thrusters. Proper modeling of charge-exchange induced spacecraft interactions requires knowledge of the respective charge-exchange cross sections. Guided-ion beam measurements and semiclassical calculations are presented for xenon atom charge-exchange collisions with Xe+ and Xe2+ at energies per ion charge ranging from 1 to 300 eV. The present measurements for the symm… Show more

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Cited by 211 publications
(110 citation statements)
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“…Although negative potential wells may be destroyed by the buildup of slow charge exchange ions [31], in this case, the time for charge exchange ions [24] to accumulate in the negative potential well around the filament, (ν i cx ) −1 ∼ n 0 < σ i cx v i > 150µs, was substantially longer than the time for ions to be accelerated to the filament supports. This ion loss time was on the order of the filament length (∼ 10 cm) over the ion velocity gained from the potential gradient along the filament ( 10 V), τ i loss ∼ L/(2eV /m i ) 40µs.…”
Section: Wallsmentioning
confidence: 97%
“…Although negative potential wells may be destroyed by the buildup of slow charge exchange ions [31], in this case, the time for charge exchange ions [24] to accumulate in the negative potential well around the filament, (ν i cx ) −1 ∼ n 0 < σ i cx v i > 150µs, was substantially longer than the time for ions to be accelerated to the filament supports. This ion loss time was on the order of the filament length (∼ 10 cm) over the ion velocity gained from the potential gradient along the filament ( 10 V), τ i loss ∼ L/(2eV /m i ) 40µs.…”
Section: Wallsmentioning
confidence: 97%
“…O þ 2 þ Xe charge exchange is described using Xe þ þ Xe cross section data from Miller et al 41 Xenon 34)), and therefore, the charge exchange cross sections for O þ 2 þ Xe charge exchange should be higher than the reverse reaction. The Xe þ þ Xe charge exchange cross sections are approximately twice as large as the O þ 2 þ O 2 charge exchange cross sections.…”
Section: Gas Phase Reactions In the Xenon Plasmamentioning
confidence: 99%
“…Although negative potential wells may be destroyed by the buildup of slow charge exchange ions [31], in this case, the time for charge exchange ions [24] to accumulate in the negative potential well around the filament, (ν…”
Section: Wallsmentioning
confidence: 99%
“…The mean free path for ion charge exchange on background neutrals [24] was λ in cx = v i /(n a < σ in cx v i >) = 280 cm for 200 eV ions, characteristic of those produced in the thruster. A maximum background pressure of 20 µTorr was chosen so that the probability that a plume ion would undergo charge exchange before it reached the ion flux probe (1 − exp(−l/λ in cx ) ≈ 0.05) was nearly identical to previous experiments in the large thruster facility conducted at a higher flow rate (4 sccm through the anode and 2 sccm through the hollow cathode).…”
Section: Experiments Backgroundmentioning
confidence: 99%