Fabio Riva, Gioele Janett, Luca Belluzzi, Tanausú del Pino Alemán, Ernest Alsina Ballester, Javier Trujillo Bueno, Pietro Benedusi, Simone Riva, Rolf Krause
{"title":"具有部分频率重分布的强共振线极化信号的数值模拟方法","authors":"Fabio Riva, Gioele Janett, Luca Belluzzi, Tanausú del Pino Alemán, Ernest Alsina Ballester, Javier Trujillo Bueno, Pietro Benedusi, Simone Riva, Rolf Krause","doi":"10.1051/0004-6361/202453107","DOIUrl":null,"url":null,"abstract":"<i>Aims<i/>. The main goal of this paper is to present an accurate and efficient numerical strategy for solving the radiative transfer problem for polarised radiation in strong resonance lines forming out of local thermodynamic equilibrium while taking angle-dependent partial frequency redistribution (PRD) effects and <i>J<i/>-state interference into account. We considered the polarisation produced both by the Zeeman effect and by the scattering of anisotropic radiation along with its sensitivity to the Hanle and magneto-optical effects.<i>Methods<i/>. We introduce a formalism that allows for treating both a two-level and a two-term atom in the presence of arbitrary magnetic and bulk velocity fields. The problem is formulated by treating the population of the lower level or term as a fixed input parameter. This approach makes the problem linear with respect to the radiation field, enabling the application of efficient matrix-free preconditioned iterative methods for its solution. Additionally, the computation of the scattering emissivity in the co-moving frame, together with a careful choice of the angular and spectral quadrature nodes, allowed us to speed up the calculations by reducing the number of evaluations of the redistribution functions.<i>Results<i/>. We applied the proposed solution strategy in order to synthesise the Stokes profiles of the Mg II h&k doublet and the H I Ly-<i>α<i/> line in 1D semi-empirical models. The results demonstrate that the method is both fast and accurate. A comparison with calculations from HanleRT-TIC displayed an overall good agreement, thereby validating our solution strategy. Moreover, for the wavelength-integrated polarisation profiles of the H I Ly-<i>α<i/> line, we found an excellent agreement between the results obtained including PRD effects in their general angle-dependent description and those obtained considering the angle-averaged simplifying approximation.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"19 1","pages":""},"PeriodicalIF":5.8000,"publicationDate":"2025-07-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A numerical approach for modelling the polarisation signals of strong resonance lines with partial frequency redistribution\",\"authors\":\"Fabio Riva, Gioele Janett, Luca Belluzzi, Tanausú del Pino Alemán, Ernest Alsina Ballester, Javier Trujillo Bueno, Pietro Benedusi, Simone Riva, Rolf Krause\",\"doi\":\"10.1051/0004-6361/202453107\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<i>Aims<i/>. The main goal of this paper is to present an accurate and efficient numerical strategy for solving the radiative transfer problem for polarised radiation in strong resonance lines forming out of local thermodynamic equilibrium while taking angle-dependent partial frequency redistribution (PRD) effects and <i>J<i/>-state interference into account. We considered the polarisation produced both by the Zeeman effect and by the scattering of anisotropic radiation along with its sensitivity to the Hanle and magneto-optical effects.<i>Methods<i/>. We introduce a formalism that allows for treating both a two-level and a two-term atom in the presence of arbitrary magnetic and bulk velocity fields. The problem is formulated by treating the population of the lower level or term as a fixed input parameter. This approach makes the problem linear with respect to the radiation field, enabling the application of efficient matrix-free preconditioned iterative methods for its solution. Additionally, the computation of the scattering emissivity in the co-moving frame, together with a careful choice of the angular and spectral quadrature nodes, allowed us to speed up the calculations by reducing the number of evaluations of the redistribution functions.<i>Results<i/>. We applied the proposed solution strategy in order to synthesise the Stokes profiles of the Mg II h&k doublet and the H I Ly-<i>α<i/> line in 1D semi-empirical models. The results demonstrate that the method is both fast and accurate. A comparison with calculations from HanleRT-TIC displayed an overall good agreement, thereby validating our solution strategy. Moreover, for the wavelength-integrated polarisation profiles of the H I Ly-<i>α<i/> line, we found an excellent agreement between the results obtained including PRD effects in their general angle-dependent description and those obtained considering the angle-averaged simplifying approximation.\",\"PeriodicalId\":8571,\"journal\":{\"name\":\"Astronomy & Astrophysics\",\"volume\":\"19 1\",\"pages\":\"\"},\"PeriodicalIF\":5.8000,\"publicationDate\":\"2025-07-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomy & Astrophysics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1051/0004-6361/202453107\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1051/0004-6361/202453107","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
目标。本文的主要目标是在考虑角度相关的部分频率重分布(PRD)效应和j态干涉的情况下,提出一种精确而有效的数值策略来求解局部热力学平衡外形成的强共振线中的极化辐射传输问题。我们考虑了由塞曼效应和各向异性辐射散射产生的极化及其对汉勒效应和磁光效应的敏感性。我们引入了一种形式,允许在任意磁场和体速度场的存在下处理两能级和两项原子。该问题是通过将较低水平或项的总体视为固定输入参数来制定的。该方法使问题与辐射场呈线性关系,从而可以应用有效的无矩阵预条件迭代方法求解问题。此外,在共动坐标系中散射发射率的计算,以及角和谱正交节点的仔细选择,使我们能够通过减少重分配函数的计算次数来加快计算速度。为了在一维半经验模型中综合Mg II h&k重态和H I Ly-α线的Stokes剖面,我们应用了所提出的求解策略。结果表明,该方法快速、准确。与HanleRT-TIC的计算结果进行了比较,显示出总体上良好的一致性,从而验证了我们的解决方案策略。此外,对于H I Ly-α线的波长积分偏振谱,我们发现在一般角度相关描述中包含PRD效应的结果与考虑角度平均简化近似的结果非常吻合。
A numerical approach for modelling the polarisation signals of strong resonance lines with partial frequency redistribution
Aims. The main goal of this paper is to present an accurate and efficient numerical strategy for solving the radiative transfer problem for polarised radiation in strong resonance lines forming out of local thermodynamic equilibrium while taking angle-dependent partial frequency redistribution (PRD) effects and J-state interference into account. We considered the polarisation produced both by the Zeeman effect and by the scattering of anisotropic radiation along with its sensitivity to the Hanle and magneto-optical effects.Methods. We introduce a formalism that allows for treating both a two-level and a two-term atom in the presence of arbitrary magnetic and bulk velocity fields. The problem is formulated by treating the population of the lower level or term as a fixed input parameter. This approach makes the problem linear with respect to the radiation field, enabling the application of efficient matrix-free preconditioned iterative methods for its solution. Additionally, the computation of the scattering emissivity in the co-moving frame, together with a careful choice of the angular and spectral quadrature nodes, allowed us to speed up the calculations by reducing the number of evaluations of the redistribution functions.Results. We applied the proposed solution strategy in order to synthesise the Stokes profiles of the Mg II h&k doublet and the H I Ly-α line in 1D semi-empirical models. The results demonstrate that the method is both fast and accurate. A comparison with calculations from HanleRT-TIC displayed an overall good agreement, thereby validating our solution strategy. Moreover, for the wavelength-integrated polarisation profiles of the H I Ly-α line, we found an excellent agreement between the results obtained including PRD effects in their general angle-dependent description and those obtained considering the angle-averaged simplifying approximation.
期刊介绍:
Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.