Reconstruction of Ionization Density Distribution in Hall Thruster Channel from Ion Energy Spectrum of Plasma Jet

2006 ◽  
Vol 8 (6) ◽  
pp. 666-669 ◽  
Author(s):  
Li Yuquan ◽  
Yu Daren
Aerospace ◽  
2020 ◽  
Vol 7 (5) ◽  
pp. 58
Author(s):  
Thibault Hallouin ◽  
Stéphane Mazouffre

The 100 W-class ISCT100-v2 Hall Thruster (HT) has been characterized in terms of far-field plume properties. By means of a Faraday Cup and a Retarding Potential Analyzer, both the ion current density and the ion energy distribution function have been measured over a 180 ∘ circular arc for different operating points. Measurements are compared to far-field plume characterizations performed with higher power Hall thrusters. The ion current density profiles remain unchanged whatever the HT input power, although an asymptotic limit is observed in the core of the plume at high discharge voltages and anode mass flow rates. In like manner, the ion energy distribution functions reveal that most of the beam energy is concentrated in the core of the plume [ − 40 ∘ ; 40 ∘ ] . Moreover, the fraction of low energy ion populations increases at large angles, owing to charge exchange and elastic collisions. Distinct plume regions are identified; they remain similar to the one described for high-power HTs. An efficiency analysis is also performed in terms of current utilization, mass utilization, and voltage utilization. The anode efficiency appears to be essentially affected by a low voltage utilization, the latter originating from the large surface-to-volume ratio inherent to low-power HTs. Experimental results also show that the background pressure clearly affects the plume structure and content.


2010 ◽  
Vol 28 (3) ◽  
pp. 429-436 ◽  
Author(s):  
J.P. Xin ◽  
X.P. Zhu ◽  
M.K. Lei

AbstractEnergy deposition by high-intensity pulsed ion beam into a metal target has been studied with time-of-flight (TOF) of ions which can be related to the original ion kinetic energy E0 and the ion mass with $t_{\rm TOF} \propto 1/\sqrt{2E_{0}/m_{i}}$. It is found that the TOF effect has a profound influence on the kinetic energy distribution of implanted ions and subsequent energy deposition process into the target. The HIPIB of mixed H+ and C+ was extracted from a magnetically insulated ion diode at a peak accelerating voltage of 350 kV, leading to an ion current density of 300 A/cm2 at the target. The widespread ion energy spectrum remarkably varied in shape as arriving at the target surface, from the original Gaussian-like of 80-ns duration to a pulse form of a sharp front and a long tail extending to about 140-ns duration. Energy loss of the mixed ions into a Ti target was simulated utilizing a Monte Carlo method. The energy deposition generally showed a shallowing trend and could be divided into two phases proceeded with sequent arrivals of H+ and C+. Note that, the peak value of deposited energy profile appeared at the beginning of mixed ion irradiation phase, other than the phase of firstly arrived H+ with peak kinetic energy and peak ion current. This study indicated that TOF effect of ions greatly affects the HIPIB-matter interaction with a kinetic energy spectrum of impinging ions at the target, noticeably differing from that of original output of the ion source; consequently, the specific energy deposition phenomena of the widespread ion energy can be studied with the TOF correlation of ion energy and ion current, otherwise not obtainable in common cases assuming fixed ion energy distribution in accordance with the original source output.


2010 ◽  
Vol 22 (6) ◽  
pp. 1343-1347
Author(s):  
魏番惠 Wei Fanhui ◽  
吴玉迟 Wu Yuchi ◽  
谷渝秋 Gu Yuqiu ◽  
刘猛 Liu Meng ◽  
刘红杰 Liu Hongjie ◽  
...  

The satellite Ariel I, launched in April 1962, provided a survey of the topside ionosphere over a latitude range of ± 55°. The measurements made by the ion energy spectrometer showed the ions O + and He + to be the major massive components of the ionosphere and enabled a global study of the composition over the northern summer of 1962 to be made. Publication of earlier analyses of parts of the data showed a diurnal and seasonal variation in the composition, a strong geomagnetic control and a suggestion of a departure from hydrostatic equilibrium in the diffusive separation of the ions. This paper provides a definitive presentation of the computer analysis of nearly all of the ion composition data obtained by the energy spectrometer. It confirms and strengthens the earlier conclusions by the inclusion of much more data and by its regression analysis in terms of geomagnetic latitude, altitude and local solar time. The paper also gives results of the total ionization density measurements and of a study of the effect of vehicle aspect on these data.


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