Babankova Dagmar, Civis Svatopluk, Juha Libor, Bittner Michal, Cihelka Jaroslav, Pfeifer Miroslav, Skala Jirí, Bartnik Andrzej, Fiedorowicz Henryk, Mikolajczyk Janusz, Ryć Leszek, Sedivcova Tereza
J. Heyrovský Institute of Physical Chemistry, Czech Academy of Sciences, Dolejskova 3, 182 23 Prague 8, Czech Republic.
J Phys Chem A. 2006 Nov 9;110(44):12113-20. doi: 10.1021/jp063689o.
Large-scale plasma was created in molecular gases (CO, CO2, N2, H2O) and their mixtures by high-power laser-induced dielectric breakdown (LIDB). Compositions of the mixtures used are those suggested for the early earth's atmosphere of neutral and/or mildly reducing character. Time-integrated optical spectra emitted from the laser spark have been measured and analyzed. The spectra of the plasma generated in the CO-containing mixtures are dominated by emission of both C2 and CN radicals. A vibrational temperature of approximately 10(4) K was determined according to an intensity distribution in a vibronic structure of the CN (B2Sigma(+)u-X2Sigma(+)g) violet band. For comparison, the NH3-CH4-H2-H2O mixture has been irradiated as a model of the strongly reducing version of the early earth's atmosphere. In this mixture, excited CN seems to be significantly less abundant than C2. The LIDB experiments were in the molecular gases carried out not only in the static cell but also using a large, double stream pulse jet (gas puff target) placed in the vacuum interaction chamber. The obtained soft X-ray emission spectra indicate the presence of highly charged atomic ions in the hot core of high-power laser sparks.
通过高功率激光诱导介电击穿(LIDB)在分子气体(CO、CO₂、N₂、H₂O)及其混合物中产生了大规模等离子体。所使用混合物的成分是针对早期地球具有中性和/或轻度还原性特征的大气所建议的成分。已对激光火花发射的时间积分光谱进行了测量和分析。在含CO混合物中产生的等离子体光谱主要由C₂和CN自由基的发射主导。根据CN(B²Σ⁺u - X²Σ⁺g)紫光带的振动电子结构中的强度分布,确定了约10⁴K的振动温度。作为对比,对NH₃ - CH₄ - H₂ - H₂O混合物进行了辐照,将其作为早期地球大气强还原版本的模型。在这种混合物中,激发态的CN似乎比C₂的丰度明显更低。LIDB实验不仅在静态池中对分子气体进行,还使用了置于真空相互作用室中的大型双流脉冲射流(喷气靶)进行。所获得的软X射线发射光谱表明在高功率激光火花的热核心中存在高电荷的原子离子。