Investigate Indian Costus Plasma Parameters using Q-Switched Laser Nd: YAG

Alyaa Hussein, Hadder M. Abdullah
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Abstract

The Indian costus plasma properties are investigated including electron temperature (Te), "electron density (ne)", "plasma frequency (fp)", " Debye sphere length", and amount of Debye(Nd),  using the spectrum of optical emission technique. There are several energies used, with ranging from 300 to 600 mJ. The Boltzmann Plot is used to calculate the temperature; where as Stark's Line Broadening is used to calculate the electron density. The Indian costus was spectroscopically examined in the air with the laser  at 10 cm away from the target and the optical fiber  at 0.5 cm away. The results were obtained for an electron temperature range of (1.8-2.2) electron volts (ev) and a wavelength range of (300-600) nm. The XRF analysis reveals that the Indian costus contains a variety of minerals, each with a different percentage, which explains why the optical emission spectrum has so many peaks. When the laser energy is  (between 300 and 600 mJ) the  "optical emission spectroscopy (OES) "has been  used to analyze the plasma spectrum of the Indian costus in the air. The results shows that as the laser energy grew, the amount of Debye will be greater i-e (Nd) >>>1,  which is one of the plasma properties.
用调q激光Nd: YAG研究印度Costus等离子体参数
利用光谱发射技术研究了印度costus等离子体的电子温度(Te)、电子密度(ne)、等离子体频率(fp)、德拜球长度(Debye)和德拜量(Nd)等特性。有几种能量被使用,范围从300到600兆焦耳。用玻尔兹曼图计算温度;其中斯塔克线展宽法用于计算电子密度。在空气中,激光距离目标10厘米,光纤距离目标0.5厘米,对印度服装进行光谱检测。结果表明,电子温度范围为1.8 ~ 2.2电子伏特(ev),波长范围为300 ~ 600 nm。XRF分析显示,印度古斯特含有多种矿物质,每种矿物质的百分比都不同,这就解释了为什么光学发射光谱有这么多峰。当激光能量在300 ~ 600 mJ之间时,光学发射光谱(OES)已被用于分析空气中印度古斯特的等离子体光谱。结果表明,随着激光能量的增大,Debye的量会增大i-e (Nd) >>>1,这是等离子体的性质之一。
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