Image Details

Choose export citation format:

The Multi-slit Approach to Coronal Spectroscopy with the Multi-slit Solar Explorer (MUSE)

  • Authors: Bart De Pontieu, Juan Martínez-Sykora, Paola Testa, Amy R. Winebarger, Adrian Daw, Viggo Hansteen, Mark C.M. Cheung, and Patrick Antolin

2020 The Astrophysical Journal 888 3.

  • Provider: AAS Journals

Caption: Figure 9.

Same as Figure 8 but the response functions used in the inversion have different abundances than the ones used to calculate the MUSE intensities. The only difference between this result and the one shown in Figure 8 is the somewhat broader distribution of intensities in the main lines.

Other Images in This Article

Show More

Copyright and Terms & Conditions