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Radiating plasma species density distribution in EUV-induced plasma in argon: a spatiotemporal experimental study

机译:氩气中EUV诱发等离子体中的辐射等离子体物质密度分布:时空实验研究

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In this contribution we experimentally study temporally and spatially resolved radiating plasma species density distribution in plasma induced by irradiating a low pressure argon gas with high energy photons with a wavelength of 13.5 nm, i.e. extreme ultraviolet (EUV). This is done by recording the optical emission spatially and temporally resolved by an iCCD camera as a function of the argon gas pressure. Our experimental results show that the emission intensity, i.e. density of radiating plasma species, depends quadratically on the gas pressure. The linear term is due to photoionization and simultaneous excitation by EUV photons, the quadratic term due to electron impact excitation by electrons generated by photoionization. The decay of radiating plasma species can be divided into two phases. At time scales shorter than 10 mu s (first phase), the decay is governed by radiative decay of radiating plasma species. At longer time scales (second phase, >10 mu s), the decay is dominated by diffusion and subsequent de-excitation at the wall. The experimental decay and expansion during this phase corresponds well with a simplified diffusion model. In order to gain more insight in this exotic type of plasma, we compare the electron density from previous measurements with the results obtained here.
机译:在这一贡献中,我们实验性地研究了通过在低压氩气中辐照波长为13.5 nm的高能光子(即极紫外(EUV))而在等离子体中产生的时空分辨辐射等离子体物种密度分布。这是通过记录iCCD摄像机根据氩气压力在空间和时间上分辨出的光发射来完成的。我们的实验结果表明,发射强度,即辐射等离子体种类的密度,与气体压力成二次关系。线性项归因于EUV光子的光电离和同时激发,二次项归因于由光电离产生的电子的电子碰撞激发。辐射等离子体物质的衰减可以分为两个阶段。在小于10μs(第一阶段)的时间尺度上,衰减由辐射等离子体物质的辐射衰减控制。在较长的时间尺度上(第二阶段,> 10μs),衰减主要由扩散和随后在壁上的去激励引起。此阶段的实验衰减和扩展与简化的扩散模型非常吻合。为了更深入地了解这种奇异类型的等离子体,我们将先前测量的电子密度与此处获得的结果进行了比较。

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