ADITYA-U托卡马克中子等离子体硬x射线谱的时间演化研究

IF 0.8 Q4 PHYSICS, FLUIDS & PLASMAS
Shishir PUROHIT, Manoj K. GUPTA, Malay B. CHOWDHURI, Umesh NAGORA, Yashika TAUNK, Abhishek KUMAR, Kajal GARG, Surya K. PATHAK, Kumarpalsinh A. JADEJA, Rohit KUMAR, Kumudni TAHILIANI, Sameer KUMAR, Kaushal M. PATEL, Rakesh L. TANNA, Supriya A. NAIR, Joydeep GHOSH
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引用次数: 0

摘要

与失控电子(RE)相关的不利影响需要对RE产生的硬x射线(HX)光谱进行时间监测,这使我们能够知道在时间空间中对应于特定能量的HX的光子通量。在ADITYA-U托卡马克上常规运行了一个基于溴化镧(LaBr3)的HX光谱仪系统(80 keV ~ 5 MeV),用于监测HX光谱的时间演变。分析了氖(Ne)杂质注入等离子体的最大计数HX能量和平均RE温度(RE平均能量)的时间演化。研究发现,在Ne气体抽吸后,峰值能量和平均失控能量显著降低,这种降低发生在Ne气体抽吸后电子密度上升的时候。注入Ne前后的RE温度分别为~ 620 KeV和230 KeV。光谱形状,在计数和能量上,都急剧缩小,表明在Ne气体膨胀后HX的排放减少了。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Investigation of Temporal Evolution of Hard X-Ray Spectrum from Neon-Seeded Plasma of ADITYA-U Tokamak
The adverse effect associated with runaway electrons (RE) requires the temporal monitoring of the Hard X-ray (HX) spectrum produced by RE. This enables us to know the photon flux corresponding to a particular energy of HX in temporal space. A Lanthanum Bromide (LaBr3)-based HX spectrometer system (80 keV ∼ 5 MeV) is routinely operated on the ADITYA-U tokamak for monitoring the temporal evolution of the HX spectrum. The temporal evolutions of the HX energy having maximum count and the average RE temperature (RE average energy) have been analyzed for the plasmas injected with neon (Ne) impurity. It has been found that peak energy and average runaway energy reduces significantly after the Ne gas puffand this reduction happens when the electron density rises after the Ne gas puff. The RE temperature values were ∼ 620 KeV and 230 KeV before and after the Ne injection, respectively. The spectral shape, in both counts and energy, shrunk drastically, suggesting the reduction of the HX emission after the Ne gas puffing.
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来源期刊
Plasma and Fusion Research
Plasma and Fusion Research PHYSICS, FLUIDS & PLASMAS-
CiteScore
1.00
自引率
25.00%
发文量
100
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