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Enhancement of Optically Thick to Thin Line Intensities in Solar and Stellar Coronal Plasmas through Radiative Transfer Effects: An Angularly Resolved Study

  • Authors: F. M. Kerr, S. J. Rose, J. S. Wark, and F. P. Keenan

Kerr et al. 2004 The Astrophysical Journal Letters 613 L181.

  • Provider: AAS Journals

Caption: Fig. 3.

Angular dependence of the f factor in the 3–1 and 5–1 lines at a column density of ~﹩2\times 10^{16}﹩ cm−2.

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