论文标题
中等物理条件和原子常数对太阳光谱中吸收系的stokes曲线的影响
The influence of the medium physical conditions and atomic constants on the Stokes profiles of absorption lines in the solar spectrum
论文作者
论文摘要
太阳光球中的fe i线的斯托克斯曲线是在unono-beckers-landi-dagl`Innocenti理论中计算的。获得了线的磁强化估计值。 Stokes曲线的变化取决于激发电位，波长，等效宽度，地面因子，微扰动速度，径向速度，阻尼速度，常数，大气模型，磁场强度和方向。 stokes曲线的图形呈现的变化使得通过反演方法确定用于求解磁场矢量重建问题的输入参数的初始值。磁强化对线参数的提出的依赖关系将有助于正确选择磁性敏感的线，以研究黑子，通量管，容器和其他磁性特征。
The Stokes profiles of Fe I lines in the photosphere of the Sun are calculated within the Unno-Beckers-Landi-Dagl`Innocenti theory. Estimates of the magnetic strengthening of the lines were obtained. The changes in the Stokes profiles depending on the excitation potential, wavelength, equivalent width, Lande factor, micro-macroturbulent velocities, radial velocity, damping constant, atmospheric model, magnetic field strength and direction are considered. The graphically presented variations of the Stokes profiles make it possible to determine the initial values of the input parameters for solving the problems of magnetic field vector reconstruction by the inversion method. The presented dependencies of the magnetic strengthening on the line parameters will help to correctly select magnetically sensitive lines for the investigation of sunspots, flux tubes, plages, and other magnetic features.
