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Modelling of spatial plasma by using neural network

机译:利用神经网络对空间等离子体进行建模

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A prediction model of spatial plasma was constructed by combining a radial basis function network and genetic algorithm. Multiparameterised widths were adopted and their effects on the model prediction were optimised by genetic algorithm. Spatial plasma data were collected by using a Langmuir probe in a Cl_2 inductively coupled plasma. For systematic modelling, plasma discharge process was characterised by a face centred Box Wilson experiment. Compared with statistical regression models, optimised radial basis function network model yielded an improved prediction of more than 45% for electron temperature. Electron density model revealed a noticeable increase in plasma density with increasing Cl_2 flow rate only at higher source powers or lower pressures as well as with decreasing the pressure only at higher Cl_2 flow rate. Also, electron temperature model showed a strong dependence on Cl_2 flow rate. Maintaining a higher Cl_2 flow rate was needed to make pressure (or source power) effect on plasma density (or electron temperature) significant.
机译:结合径向基函数网络和遗传算法,构建了空间等离子体预测模型。采用多参数宽度,并通过遗传算法优化了它们对模型预测的影响。通过使用Cl_2感应耦合等离子体中的Langmuir探针收集空间等离子体数据。为了进行系统建模,以面心为中心的Box Wilson实验表征了等离子体放电过程。与统计回归模型相比,优化的径向基函数网络模型对电子温度的预测提高了45%以上。电子密度模型显示,仅在较高的源功率或较低的压力下,随着Cl_2流量的增加,血浆密度显着增加,而仅在较高的Cl_2流量下,压力降低。而且,电子温度模型显示出对Cl_2流速的强烈依赖性。需要保持较高的Cl_2流速,以使压力(或源功率)对等离子体密度(或电子温度)的影响显着。

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