2005
DOI: 10.1063/1.1944328
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Space charge saturated sheath regime and electron temperature saturation in Hall thrusters

Abstract: Secondary electron emission in Hall thrusters is predicted to lead to space charge saturated wall sheaths resulting in enhanced power losses in the thruster channel.Analysis of experimentally obtained electron-wall collision frequency suggests that the electron temperature saturation, which occurs at high discharge voltages, appears to be caused by a decrease of the Joule heating rather than by the enhancement of the electron energy loss at the walls due to a strong secondary electron emission.2

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Cited by 84 publications
(65 citation statements)
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“…This similarity in shape is unexpected since these profiles are expected to be influenced by the length and position of the acceleration zone, which should change with operating condition. 17,19 However, these results are consistent with the similarity in radial profiles seen in Fig. 11, since the axial and radial profiles are connected via the magnetic field topology which shapes isothermal lines.…”
Section: Analysis Of the Very-near-field Plumesupporting
confidence: 81%
See 2 more Smart Citations
“…This similarity in shape is unexpected since these profiles are expected to be influenced by the length and position of the acceleration zone, which should change with operating condition. 17,19 However, these results are consistent with the similarity in radial profiles seen in Fig. 11, since the axial and radial profiles are connected via the magnetic field topology which shapes isothermal lines.…”
Section: Analysis Of the Very-near-field Plumesupporting
confidence: 81%
“…It has been well-established from previous measurements that the electron temperature increases fairly linearly with local plasma potential in Hall thrusters, with typical reported values of 0.07 -0.16 eV/V of potential. 16,17,19 However, the data in this study show that the average value in the near-field plume of the NASA-457Mv2 is 0.52 and 0.46 eV/V at 300 V and 400 V, respectively. An elevated value of 0.24 eV/V was also found for the NASA-300M at 500 V and 20 kW.…”
Section: Analysis Of the Very-near-field Plumementioning
confidence: 65%
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“…The modelisation of this interaction is usually established by models that may not capture all microscopic processes involved, specially in Weakly Ionized Plasmas (WIP) for which the inclusion of a dense heavy cold neutral species hinders the development of models [137][138][139]. Our research group is interested in the use of these probes to analyse the plasma generated in our low temperature laboratory [99,100,152], making this topic of main interest.…”
Section: Plasma-wall Interactionmentioning
confidence: 99%
“…The I-V curves of collecting probes provide information about parameters such as the local plasma potential, the electron or ion temperatures and the charged species density [131][132][133]. These probes are widely used for the diagnostics of fully [134][135][136] and weakly ionized plasmas [137][138][139]. Theoretically, the operation of Langmuir probes does not depend on the shape of the signal used to bias the probe.…”
Section: Analysis Of Certain Discrepancies On the Characterisation Ofmentioning
confidence: 99%