Image Details

Choose export citation format:

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 1.

Total solar eclipse observations from Mitchell, OR, on 2017 August 21. Solar north is vertically up in all images. A: Processed white light image of the solar corona. B: Processed image of the Fe XI 789.2 nm emission at ≈1.1 × 106 K. C: Processed image of the Fe XIV 530.3 nm emission at ≈1.8 × 106 K. D: Composite of B (red) and C (green). E: Same as D overlaid on the white light image (note that the corresponding continuum has been subtracted from the on band Fe XI and Fe XIV images prior to processing to produce the images shown here).

Other Images in This Article

Show More

Copyright and Terms & Conditions