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Measurement of plasma parameters in the exhaust of a magnetoplasma rocket by gridded energy analyzer and emissive Langmuir probe.

机译:网格能量分析仪和发射朗缪尔探针测量磁等离子体火箭排气中的等离子体参数。

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The 10 kilowatt prototype of the Variable Specific Impulse Magnetoplasma Rocket (VASIMR) engine, abbreviated as VX-10, is designed to eject plasma at exhaust velocities of tens of kilometers per second. In this device, energy is imparted to the plasma ions by two mechanisms: ion cyclotron resonant heating (ICRH), and acceleration in an ambipolar electric field. Measurements from two different electrostatic probes are combined to determine how much each mechanism contributes to the total ion energy. The first probe is a gridded retarding potential analyzer (RPA) that incorporates a multi-channel collimator to obtain precise measurement of the ion and electron parallel energy distributions. The second is an emissive Langmuir probe that measures the DC and RF components of the plasma potential. The plasma potential obtained from the emitting probe allows calculation of the parallel velocity distribution once the parallel energy distribution is obtained from the energy analyzer data.; Biasing the RPA housing is shown to minimize the plasma perturbation, as monitored by an auxiliary probe. When this minimization is done, the RPA measurements become compatible with the emissive probe's measurement of plasma potential.; The collimated RPA and emissive probe have been used to examine the effects of a double dual half-turn (DDHT) antenna encircling the plasma. When power at the ion cyclotron frequency is applied, changes are seen in the saturation current and mean ion energy of the collimated RPA characteristic. The evolution of these changes as the RPA is moved downstream from the antenna is interpreted as firm evidence of ion cyclotron heating, albeit at absorbed energies of less than 1 electronvolt per ion. The emissive probe shows that, within experimental error, all of the increased ion energy is accounted for by an increase in the plasma potential that occurs when the ICRF power is applied. The combined RPA and emissive probe data also show that there is a jet of flowing plasma in the VX-10 when operated with the helicon source alone but that the signal from this jet is overwhelmed by a rapidly growing stationary plasma within the first second of the discharge.
机译:10千瓦的可变比冲激磁浆火箭(VASIMR)发动机原型,缩写为VX-10,旨在以每秒几十公里的排气速度喷射等离子体。在该装置中,能量通过两种机制传递给等离子体离子:离子回旋共振加热(IC​​RH)和双极性电场中的加速。将来自两个不同静电探针的测量值结合起来,以确定每种机制对总离子能量的贡献程度。第一个探针是栅格化延迟电势分析仪(RPA),该分析仪结合了多通道准直仪,可精确测量离子和电子平行能分布。第二个是发射式Langmuir探针,可测量等离子体电势的DC和RF分量。一旦从能量分析仪数据获得平行能量分布,从发射探针获得的等离子体电势就可以计算平行速度分布。如图所示,通过辅助探针监测,对RPA外壳进行偏置可最大程度地减少等离子体扰动。完成此最小化后,RPA测量将与发射探针的血浆电势测量兼容。准直的RPA和发射探针已用于检查环绕等离子体的双双半圈(DDHT)天线的效果。当施加离子回旋加速器频率的功率时,可以看到准直RPA特性的饱和电流和平均离子能量发生变化。 RPA从天线向下游移动时,这些变化的演变被解释为离子回旋加速器加热的确凿证据,尽管吸收的能量小于每个离子1电子伏特。发射探针表明,在实验误差范围内,所有增加的离子能量都由施加ICRF功率时发生的等离子体电势增加引起。组合的RPA和发射探针数据还显示,当单独使用螺线管源进行操作时,VX-10中有一个流动的等离子体射流,但是在该射流的第一秒内,快速增长的固定等离子体使来自该射流的信号不堪重负。排出。

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