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Emission of fast non-Maxwellian hydrogen atoms in low-density laboratory plasma

机译:低密度实验室血浆中快速非麦克斯韦氢原子的发射

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摘要

The source of strong and broad emission of the Balmer-α line in mixed plasmas of hydrogen (or deuterium) and noble gases in front of metallic surfaces is a subject of controversial discussion of many plasma types. In this work the excitation source of the Balmer lines is investigated by means of optical emission spectroscopy in the plasma device PSI-2. Neutral fast non-Maxwellian hydrogen atoms are produced by acceleration of hydrogen ions towards an electrode immersed into the plasma. By variation of the electrode potential the energy of ions and in turn of reflected fast atoms can be varied in the range of 40−300 eV. The fast atoms in front of the electrode are observed simultaneously by an Echelle spectrometer (0.001 nm/channel) and by an imaging spectrometer (0.01 nm/channel) up to few cm in the plasma. Intense excitation channels of the Balmer lines are observed when hydrogen is mixed with argon or with krypton. Especially in Ar-H and Ar-D mixed plasmas the emission of fast hydrogen atoms is very strong. Intermixing hydrogen with other noble gases (He, Ne or Xe) one observes the same effect however the emission is one order of magnitude less compared to Kr-H or Kr-D plasmas. It is shown, that the key process, impacting this emission, is the binary collision between the fast neutral hydrogen atom and the noble gas atom. Two possible sources of excitation are discussed in details: one is the excitation of hydrogen atoms by argon atoms in the ground state and the second one is the process of the so-called excitation transfer between the metastable states of noble gases and hydrogen. In the latter case the atomic data for excitation of Balmer lines are still not available in literature. Further experimental investigations are required to conclude on the source process of fast atom emission.
机译:在金属表面前的氢(或氘)和稀有气体的混合等离子体中,Balmer-α线的强而宽的发射源是许多等离子体类型的有争议讨论的主题。在这项工作中,借助于等离子体装置PSI-2中的光发射光谱法研究了巴尔默线的激发源。中性快速非麦克斯韦氢原子是通过氢离子向浸入等离子体的电极加速而产生的。通过改变电极电势,离子的能量以及反射的快速原子的能量可以在40-300 eV的范围内变化。同时通过Echelle光谱仪(0.001meternm /通道)和成像光谱仪(0.01 nm /通道)同时观察等离子体中长达几厘米的电极前快速原子。当氢气与氩气或k气混合时,会观察到Balmer谱线的强烈激发通道。特别是在Ar-H和Ar-D混合等离子体中,快速氢原子的发射非常强。将氢与其他稀有气体(He,Ne或Xe)混合会观察到相同的效果,但是与Kr-H或Kr-D等离子体相比,其发射少一个数量级。结果表明,影响这种排放的关键过程是快速中性氢原子与稀有气体原子之间的二元碰撞。详细讨论了两种可能的激发源:一种是基态的氩原子对氢原子的激发,第二种是稀有气体与氢的亚稳态之间所谓的激发转移的过程。在后一种情况下,巴尔默线激发的原子数据在文献中仍然不可用。需要进一步的实验研究以得出快速原子发射的源过程。

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