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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. 5.

Left: Measured ratios of the principal satellite feature at 5.82 Å (marked D) to the Si XIII ﹩w_{3}+y_{3}﹩ line at 5.681 Å during the four flares of Table 1, plotted against ﹩T_{e}﹩ measured from GOES data. Filled circles denote line fluxes from Gaussian fits; open circles denote line fluxes from total flux above continuum level. The solid line is the calculated ratio. Right: Measured ratios plotted against ﹩T_{0}﹩ for ﹩\mathrm{DEM}\,=\mathrm{exp}\,( -T_{e}/ T_{0}) ﹩. The solid line is the calculated curve.

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