The azimuthal currents in the ion-driven magnetic nozzle

IF 5.4 2区 工程技术 Q1 ENGINEERING, AEROSPACE
Zhiyuan Chen , Yibai Wang , Haibin Tang , Junxue Ren , Min Li , Peng Wu , Jinbin Cao
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引用次数: 1

Abstract

Ion-driven magnetic nozzles (Ti > Te) are designed as intrinsic parts of cutting-edge propulsive technologies such as variable specific impulse magnetoplasma rockets (VASIMRs) and applied-field magnetoplasmadynamic thrusters. Employing a two-dimensional axisymmetric particle-in-cell (PIC) code, in the ion-driven magnetic nozzle, the compositions and distributions of azimuthal currents in different axial regions are investigated under various inlet ion temperatures Ti0 and found to differ dramatically from that in the electron-driven magnetic nozzles. Previously reported to be all paramagnetic and vanishing under a high magnetic field, the azimuthal currents resulting from the E × B drift are shown to turn diamagnetic and sustain a considerable magnitude when Ti0 is considered. The previously reported profile of diamagnetic drift current is altered by the introduction of inlet ion temperature, and the paramagnetic part is significantly suppressed. Moreover, a wide range of paramagnetic currents appear downstream due to the inward detachment of ions, which can also be reduced by increasing inlet ion temperature. Albeit considered in this paper, the azimuthal currents resulting from grad-B and curvature drift are still negligible in all cases of interest. The magnitude of diamagnetic azimuthal currents increases with amplifying Ti0, indicating a clear physical image of energy transformation from ion thermal energy to the directed kinetic energy through electromagnetic processes in the magnetic nozzle. Additionally, the magnetic inductive strength also has noticeable impacts on the azimuthal currents, the current magnitude tends to decrease as the magnetic field increases, and over-increment of it may result in larger divergence angles and lower nozzle efficiency.

离子驱动磁喷嘴的方位电流
离子驱动磁喷嘴(Ti >它们被设计为尖端推进技术的固有部分,如可变比脉冲磁等离子体火箭(VASIMRs)和应用磁场磁等离子体动力推进器。采用二维轴对称粒子池(PIC)代码,研究了离子驱动磁喷嘴中不同入口离子温度下不同轴向区域的方位电流组成和分布,发现其与电子驱动磁喷嘴中的方位电流组成和分布存在显著差异。以前的报道都是顺磁性的,在高磁场下消失,当考虑到Ti0时,由E × B漂移产生的方位电流显示为反磁性的,并保持相当大的幅度。引入入口离子温度后,以往报道的反磁漂移电流分布发生了改变,顺磁漂移部分明显受到抑制。此外,由于离子向内分离,下游出现了大范围的顺磁电流,这也可以通过提高入口离子温度来降低。尽管本文考虑了梯度b和曲率漂移引起的方位电流,但在所有感兴趣的情况下仍然可以忽略不计。反磁方位电流的大小随着Ti0的增大而增大,表明能量在磁喷嘴内通过电磁过程从离子热能转变为定向动能的物理图像清晰。此外,磁感应强度对方位电流的影响也很明显,电流大小随着磁场的增大而减小,过大的磁场会导致发散角增大,降低喷嘴效率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
7.50
自引率
5.70%
发文量
30
期刊介绍: Propulsion and Power Research is a peer reviewed scientific journal in English established in 2012. The Journals publishes high quality original research articles and general reviews in fundamental research aspects of aeronautics/astronautics propulsion and power engineering, including, but not limited to, system, fluid mechanics, heat transfer, combustion, vibration and acoustics, solid mechanics and dynamics, control and so on. The journal serves as a platform for academic exchange by experts, scholars and researchers in these fields.
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