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Emission of Fast Non-Maxwellian Hydrogen Atoms in Low-Density Laboratory Plasma

机译:低密度实验室等离子体中快速非最大世界氢原子的排放

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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:在金属表面前面的混合等离子体(或氘)和惰性气体中的BALMER-α线的强度和广泛排放的源是许多等离子体类型的争议讨论的主题。在这项工作中,通过等离子体器件PSI-2中的光学发射光谱来研究BA1MER线的激发源。通过将氢离子加速朝向浸入等离子体中的电极加速来制备中性快的非最大威斯韦氢原子。通过电极电位的变化,离子的能量和反射的快速原子的能量可以在40-300eV的范围内变化。电极前面的快速原子通过梯度光谱仪(0.001nm /沟道)同时观察,并通过等离子体中的成像光谱仪(0.01nm /沟道)同时观察到高达较少的厘米。当氢气与氩气或氪混合时,观察到BALMER线的强烈激励通道。特别是在AR-H和AR-D混合等离子体中,快速氢原子的排放非常强。与其他惰性气体(HE,NE或XE)相同的氢气同时观察到相同的效果然而,与KR-H或KR-D等离子体相比,发射少于一个数量级。结果显示,影响该发射的关键过程是快速中性氢原子和贵瓦族气原子之间的二元碰撞。详细讨论了两个可能的激发源:一种是通过地面状态的氩原子激发氢原子,第二个是惰性气体和氢气的亚稳态之间所谓的激发转移的过程。在后一种情况下,仍然没有在文献中获得BALMER线路的原子数据。需要进一步的实验调查来结束快速原子排放的源过程。

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