Image Details

Choose export citation format:

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 6.

Fractional alignment ﹩{\sigma }_{0}^{2}({\alpha }_{\ell }{J}_{\ell })﹩ of the first ﹩{}^{2}{P}_{3/2}^{0}﹩ J1-level of the Fe X ground term (left panel) and of the second ﹩{}^{3}{P}_{1}^{e}﹩ J2-level of the Fe XIII ground term (right panel) as a function of the radial distance R/RSun in the spherically symmetric 1D quiet-Sun coronal model of Figure 1. Solid lines: ﹩{\sigma }_{0}^{2}({\alpha }_{\ell }{J}_{\ell })﹩ values calculated taking into account electron collisions. Dashed lines: ﹩{\sigma }_{0}^{2}({\alpha }_{\ell }{J}_{\ell })﹩ values obtained in the absence of collisions. Red circles: anisotropy of the continuum radiation at 6376 Å (for Fe X) and at 10747 Å (for Fe XIII). The results shown are for the case of a vertical magnetic field (θB = 0°).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse