For many applications, the semiclassical, theoretical calculations of Stark broadening parameters of isolated non-hydrogenic ion lines proved useful and reasonably accurate for plasma electron density determination. Several attempts were carried out to improve the calculation procedure of Stark broadening parameters and, in this way, to increase the accuracy of laboratory and astrophysical plasmas and opacity calculations. In this work for the test ions, we selected singly and doubly ionized argon lines. These ions are chosen for several reasons. First, among several studies, there are detailed Ar II calculations by Griem and coworkers, Hamdi et al., and by Blagojević and Konjević for singly and Hamdi et al.for doubly ionized argon lines. These large sets of data facilitate the extension of our work on improving semiclassical calculations. Second, argon gas applications as a plasma matrix are numerous, and reliable plasma diagnostics are of utmost importance for determining electron density, one of the essential plasma parameters for plasma modeling.

对于许多应用，孤立的非氢离子线的斯塔克展宽参数的半经典理论计算证明对于等离子体电子密度测定是有用且相当准确的。进行了多次尝试以改进斯塔克展宽参数的计算程序，并以此方式提高实验室和天体物理等离子体和不透明度计算的准确性。在测试离子的这项工作中，我们选择了单电离和双电离的氩气线。选择这些离子有几个原因。首先，在几项研究中，Griem 及其同事 Hamdi 等人以及 Blagojević 和 Konjević 对单独的 Ar II 和 Hamdi 等人对双电离氩线进行了详细的 Ar II 计算。这些大型数据集有助于扩展我们改进半经典计算的工作。第二，