Fig. 2 from Enhancement of Optically Thick to Thin Line Intensities in Solar and Stellar Coronal Plasmas through Radiative Transfer Effects: An Angularly Resolved Study

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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. 2.

Comparison of CRETIN and KB01 results for rays exiting normally from an Fe XV slab plasma at differing column densities. The CRETIN results denoted in the key as "7–4 thin" take the reference line to be optically thin, while the values "7–4 thick" use CRETIN output for all values of intensity.

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