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Si XII X‐Ray Satellite Lines in Solar Flare Spectra

  • Authors: K. J. H. Phillips, J. Dubau, J. Sylwester, and B. Sylwester

Phillips et al. 2006 The Astrophysical Journal 638 1154.

  • Provider: AAS Journals

Caption: Fig. 4.

Synthesized spectra (5.76–5.83 Å) showing the Si XII satellite features A, B, C, and D (notation of Boiko et al. [1978] and Audebert et al. [1985]; see Table 2) for ﹩T_{e}=13﹩ and 6 MK. The spectra (solid line) show the total of dielectronic and inner‐shell satellites; the dielectronic satellites alone (dotted line; most evident for feature C) are also shown. The line widths are for thermal Doppler broadening at 13 MK (FWHM 2.8 mÅ) and 6 MK (1.9 mÅ). At the resolution of RESIK (15.7 mÅ FWHM), the contribution of inner‐shell satellites would be negligible.

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