Measurement of Paα line from pellet ablation cloud in Heliotron J.

A Iwata, S Kado, M Murakumo, T Shikama, G Motojima, A Mori, C Feng, H Okada, T Minami, S Ohshima, S Kobayashi, A Ishizawa, Y Nakamura, S Konoshima, T Mizuuchi, K Nagasaki
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Abstract

The Paα line (1875.13 nm) in the near-infrared (NIR) region was evaluated to apply Stark broadening of the line spectrum to the electron density measurement of the small-pellet ablation cloud in Heliotron J, a medium-sized helical-axis heliotron device. Paα is three-to-four times broader than the visible Hβ line (486.13 nm) for the same electron density. Using a portable NIR spectrometer, preliminary proof-of-concept experiments determined the marginal density, below which the broadening was undetectable. The lower detection density limit can be decreased using a narrower entrance slit or a denser grating.

Heliotron J中球团烧蚀云Paα谱线的测量。
利用Stark展宽谱线测量了中型螺旋轴Heliotron J中小颗粒烧蚀云的电子密度,对近红外(NIR)区1875.13 nm的Paα谱线进行了评价。在相同的电子密度下,Paα比可见的Hβ线(486.13 nm)宽3 - 4倍。使用便携式近红外光谱仪,初步的概念验证实验确定了边际密度,低于此密度,则无法检测到加宽。可以使用更窄的入口狭缝或更密集的光栅来降低较低的检测密度限制。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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