Figure 8 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 8.

Azimuthal profiles of plasma β determined from the image planes taken from the COR1 Ahead (top) and Behind (bottom). The closed circles with solid lines denote the values determined at a heliocentric distance of 2.0 R _☉ and the open circles with dashed lines refer to the values at 2.5 R _☉.

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