...
首页> 外文期刊>The Astrophysical journal >POLARIZED LINE TRANSFER WITH F-STATE INTERFERENCE IN A NON-MAGNETIC MEDIUM: PARTIAL FREQUENCY REDISTRIBUTION EFFECTS IN THE COLLISIONLESS REGIME
【24h】

POLARIZED LINE TRANSFER WITH F-STATE INTERFERENCE IN A NON-MAGNETIC MEDIUM: PARTIAL FREQUENCY REDISTRIBUTION EFFECTS IN THE COLLISIONLESS REGIME

机译:非磁性介质中具有F态干扰的极化线传输:无蠕变系统中的部分频率重分配效应

获取原文

摘要

Quantum interference phenomena manifest themselves in several ways in the polarized solar spectrum formed due to coherent scattering processes. One such effect arises due to interference between the fine structure (J) states giving rise to multiplets. Another effect is that which arises due to interference between the hyperfine structure (F) states. We extend the redistribution matrix derived for the J-state interference to the case of F-state interference. We then incorporate it into the polarized radiative transfer equation and solve it for isothermal constant property slab atmospheres. The relevant transfer equation is solved using a polarized approximate lambda iteration (PALI) technique based on operator perturbation. An alternative method derived from the Neumann series expansion is also proposed and is found to be relatively more efficient than the PALI method. The effects of partial frequency redistribution and the F-state interference on the shapes of the linearly polarized Stokes profiles are discussed. The emergent Stokes profiles are computed for hypothetical line transitions arising due to hyperfine structure splitting of the upper J = 3/2 and lower J = 1/2 levels of a two-level atom model with nuclear spin Is = 3/2. We confine our attention to the non-magnetic scattering in the collisionless regime.
机译:在由于相干散射过程而形成的极化太阳光谱中,量子干涉现象以多种方式表现出来。由于精细结构(J)状态之间的干扰导致多重峰,因此产生了一种这样的效果。另一个效果是由于超精细结构(F)状态之间的干扰而产生的。我们将针对J状态干扰得出的重新分配矩阵扩展到F状态干扰的情况。然后,我们将其合并到极化辐射传递方程中,并针对等温恒定特性的平板气氛进行求解。使用基于算子扰动的极化近似λ迭代(PALI)技术求解相关的传递方程。还提出了从Neumann级数展开得到的另一种方法,并且发现该方法比PALI方法相对更有效。讨论了部分频率重新分布和F状态干扰对线性极化Stokes轮廓形状的影响。针对由于原子自旋Is = 3/2的两级原子模型的上层J = 3/2和下层J = 1/2的超精细结构分裂而产生的假设的线跃迁,计算了出现的斯托克斯轮廓。我们将注意力集中在无碰撞状态下的非磁性散射上。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号