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CME-induced Thermodynamic Changes in the Corona as Inferred from Fe XI and Fe XIV Emission Observations during the 2017 August 21 Total Solar Eclipse

  • Authors: Benjamin Boe, Shadia Habbal, Miloslav Druckmüller, Adalbert Ding, Jana Hodérova, and Pavel Štarha

2020 The Astrophysical Journal 888 100.

  • Provider: AAS Journals

Caption: Figure 12.

Top left: Excess of emission at 786 nm compared to 527 nm at Mitchell. Top right: Doppler shifted (≈530 km s−1) line to continuum ratio of Fe XIV measured at Alliance. Bottom left: Doppler shifted line to continuum ratio of Fe XI from Mackay. Bottom right: Same as left but for Alliance. The line and continuum data were calibrated using the technique outlined in Section 2.2. The white ring in the middle panels indicates the location of a ghost image in the raw data produced by internal reflections in the optics (see Appendix B).

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