Figure 7 from The Multi-slit Approach to Coronal Spectroscopy with the Multi-slit Solar Explorer (MUSE)

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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 7.

Single Gaussian fits to MUSE observables (left column) from the flux emergence simulation in model B (Hansteen et al. 2019) reproduce intensity, velocity, and broadening of the ground truth (middle column) to within the desired uncertainty in almost all locations (with S/N > 10, white contours in intensity).

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