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Determination of Differential Emission Measure from Solar Extreme Ultraviolet Images

  • Authors: Yang Su, Astrid M. Veronig, Iain G. Hannah, Mark C. M. Cheung, Brian R. Dennis, Gordon D. Holman, Weiqun Gan, and Youping Li

2018 The Astrophysical Journal Letters 856 L17.

  • Provider: AAS Journals

Caption: Figure 3.

Tests of three DEM codes with Gaussian DEM models. The models include: a single Gaussian model with (a) σ = 0.06, (b) σ = 0.2 , and (c) double-Gaussian DEM model with σ = 0.06. The peak temperatures vary from log10 T = 5.6 to 7.6 (in model c, one Gaussian peaks at a fixed log10 T = 6.3). Top row: DEM solutions for Gaussian models (black) peak at log10 T = 6.2 (7.0 in panel c). The solutions from the regularized inversion are shown in green, the original sparse inversion code in red crosses (the code did not find solutions for all the tests), and the sparse inversion code with new settings in blue. Middle row is the same as top row, but for Gaussian models peak at log10 T = 7.6. Bottom row: comparison of the TEM derived from the solutions and the models. The dashed lines show the expected relation between peak temperatures and TEM. The area in gray shows the range of expected values ±σ.

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