Figure 10 from Global Coronal Seismology in the Extended Solar Corona through Fast Magnetosonic Waves Observed by STEREO SECCHI COR1

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Global Coronal Seismology in the Extended Solar Corona through Fast Magnetosonic Waves Observed by STEREO SECCHI COR1

Authors: Ryun-Young Kwon, Maxim Kramar, Tongjiang Wang, Leon Ofman, Joseph M. Davila, Jongchul Chae, and Jie Zhang

Kwon et al. 2013 The Astrophysical Journal 776 55.

Provider: AAS Journals

Caption: Figure 10.

Scatter plots of magnetic field strengths. The left panel shows difference of magnetic field strengths determined from the two different image planes taken from Ahead and Behind. The difference between magnetic field strengths determined through the SSI and tomography methods is shown in the right panel.

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