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利用纳秒激光诱导等离子体检测分子氧。

Detection of molecular oxygen using nanosecond-laser-induced plasma.

作者信息

Kim Seon Woong, Choi Jongwun, Byun Hosung, Yoon Taekeun, Carter Campbell D, Do Hyungrok

出版信息

Opt Express. 2023 Sep 25;31(20):32504-32515. doi: 10.1364/OE.499782.

DOI:10.1364/OE.499782
PMID:37859052
Abstract

Molecular oxygen (O) concentration is measured by employing nanosecond laser-induced plasmas (ns-LIP) over a broad temperature spectrum ranging from 300 K to 1000 K, in the presence of an additional oxygen-containing molecule, CO. Typically, emission spectra emanating from ns-LIP are devoid of molecular information, as the ns-LIP causes the dissociation of molecular species within the plasma. However, atomic oxygen absorption lines that momentarily appear at 777 nm in the broadband emission from the early-stage plasma are determined to be highly sensitive to the O mole fraction but negligibly affected by the CO mole fraction. The atomic O absorbing the plasma emission originates from the O adjacent to the plasma: robust UV radiation from the early-stage plasma selectively dissociates adjacent O, exhibiting a relatively low photodissociation threshold, thus generating the specific meta-stable oxygen capable of absorbing photons at 777 nm. A theoretical model is introduced, explicating the formation of the meta-stable O atom from adjacent O. To sustain the UV radiation from the plasma under high-temperature and low-density ambient conditions, a preceding breakdown is triggered by a split laser pulse (532 nm). This breakdown acts as a precursor, seeding electrons to intensify the inverse-Bremsstrahlung photon absorption of the subsequent laser pulse (1064 nm). Techniques such as proper orthogonal decomposition (POD) and support vector regression (SVR) are employed to precisely evaluate the O mole fraction (<1% uncertainty), by analyzing the short-lived (<10 ns) O-indicator depicted in the early-stage plasma.

摘要

在300 K至1000 K的宽温度范围内,在存在额外含氧化合物CO的情况下,通过使用纳秒激光诱导等离子体(ns-LIP)来测量分子氧(O)浓度。通常,ns-LIP发出的发射光谱缺乏分子信息,因为ns-LIP会导致等离子体内分子物种的解离。然而,早期等离子体宽带发射中在777 nm瞬间出现的原子氧吸收线被确定对O摩尔分数高度敏感,但受CO摩尔分数的影响可忽略不计。吸收等离子体发射的原子O源自等离子体附近的O:早期等离子体发出的强烈紫外线辐射选择性地解离相邻的O,其光解离阈值相对较低,从而产生能够吸收777 nm光子的特定亚稳氧。引入了一个理论模型,解释了相邻O形成亚稳O原子的过程。为了在高温和低密度环境条件下维持等离子体的紫外线辐射,由一个分离的激光脉冲(532 nm)触发前体击穿。这种击穿作为前体,注入电子以增强后续激光脉冲(1064 nm)的逆轫致辐射光子吸收。通过分析早期等离子体中描绘的短寿命(<10 ns)O指示物,采用诸如适当正交分解(POD)和支持向量回归(SVR)等技术来精确评估O摩尔分数(不确定度<1%)。

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