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Coronal Magnetometry with EUV Permitted Lines

  • Authors: Nataliia G. Shchukina, Javier Trujillo Bueno, Supriya Hebbur Dayananda, Rafael Manso Sainz, Andrii V. Sukhorukov

Nataliia G. Shchukina et al 2025 The Astrophysical Journal 988 .

  • Provider: AAS Journals

Caption: Figure 7.

The left and right panels show results for the Fe X and Fe XIII lines, respectively. Top panels: the density matrix elements ﹩{\rho }_{0}^{0}({\alpha }_{\ell }{J}_{\ell })﹩. Bottom panels: the term F(NeTe), the fractional alignment ﹩{\sigma }_{0}^{2}({\alpha }_{\ell }{J}_{\ell })﹩ (lower level) and the fractional alignment ﹩{\sigma }_{0}^{2}({\alpha }_{u}{J}_{u})﹩ (upper level) for the Fe X 174.531 Å and Fe XIII 202.021 Å lines as a function of the radial distance R/RSun in the spherically symmetric 1D quiet-Sun coronal model of Figure 1.

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