Extended channel Hall thruster for air-breathing electric propulsion

2021 ◽  
Vol 130 (5) ◽  
pp. 053306
Author(s):  
Francesco Marchioni ◽  
Mark A. Cappelli
Author(s):  
Jason D. Frieman ◽  
Hani Kamhawi ◽  
Wensheng Huang ◽  
Jon Mackey ◽  
Drew M. Ahern ◽  
...  

2012 ◽  
Vol 2012 ◽  
pp. 1-16 ◽  
Author(s):  
Li Yan ◽  
Ping-Yang Wang ◽  
Yang-Hua Ou ◽  
Xiao-Lu Kang

Potential sputtering erosion caused by the interactions between spacecraft and plasma plume of Hall thrusters is a concern for electric propulsion. In this study, calculation model of Hall thruster’s plume and sputtering erosion is presented. The model is based on three dimensional hybrid particle-in-cell and direct simulation Monte Carlo method (PIC/DSMC method) which is integrated with plume-wall sputtering yield model. For low-energy heavy-ion sputtering in Hall thruster plume, the Matsunami formula for the normal incidence sputtering yield and the Yamamura angular dependence of sputtering yield are used. The validation of the simulation model is realized through comparing plume results with the measured data. Then, SPT-70’s sputtering erosion on satellite surfaces is assessed and effect of mass flow rate on sputtering erosion is analyzed.


Vacuum ◽  
2015 ◽  
Vol 120 ◽  
pp. 89-95 ◽  
Author(s):  
Yanwu Li ◽  
X. Chen ◽  
Danming Li ◽  
Yuhua Xiao ◽  
Peng Dai ◽  
...  

2021 ◽  
Author(s):  
Sukhmander Singh ◽  
Bhavna Vidhani ◽  
Ashish Tyagi

The first part of the contributed chapter discuss the overview of electric propulsion technology and its requirement in different space missions. The technical terms specific impulse and thrust are explained with their relation to exhaust velocity. The shortcoming of the Hall thrusters and its erosion problems of the channel walls are also conveyed. The second part of the chapter discuss the various waves and electromagnetic instabilities propagating in a Hall thruster magnetized plasma. The dispersion relation for the azimuthal growing waves is derived analytically with the help of magnetohydrodynamics theory. It is depicted that the growth rate of the instability increases with magnetic field, electron drift velocity and collisional frequency, whereas it is decreases with the initial drift of the ions.


Author(s):  
Matthew T. Domonkos ◽  
Michael J. Patterson ◽  
Robert S. Jankovsky

NASA’s Glenn Research Center has been selected to lead development of NASA’s Evolutionary Xenon Thruster (NEXT) system. The central feature of the NEXT system is an electric propulsion thruster (EPT) that inherits the knowledge gained through the NSTAR thruster that successfully propelled Deep Space 1 to asteroid Braille and comet Borrelly, while significantly increasing the thruster power level and making improvements in performance parameters associated with NSTAR. The EPT concept under development has a 40 cm beam diameter, twice the effective area of the Deep-Space 1 thruster, while maintaining a relatively-small volume. It incorporates mechanical features and operating conditions to maximize the design heritage established by the flight NSTAR 30 cm engine, while incorporating new technology where warranted to extend the power and throughput capability. The NASA Hall thruster program currently supports a number of tasks related to high power thruster development for a number of customers including the Energetics Program (formerly called the Space-based Program), the Space Solar Power Program, and the In-space Propulsion Program. In program year 2002, two tasks were central to the NASA Hall thruster program: 1.) the development of a laboratory Hall thruster capable of providing high thrust at high power; 2.) investigations into operation of Hall thrusters at high specific impulse. In addition to these two primary thruster development activities, there are a number of other on-going activities supported by the NASA Hall thruster program. These additional activities are related to issues such as thruster lifetime and spacecraft integration.


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