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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 2.

Azimuthal profiles of electron density along three circular paths at heliocentric distances of 2.0 (bottom), 2.5 (middle), and 3.0  R (top) on the image planes of Ahead (left) and Behind (right). The electron densities are determined with the SSI (solid curve) and tomography (dashed) methods, within a position angle range from 0° to 120°. The dotted horizontal lines refer to the electron densities determined in polar coronal holes by Saito et al. (1977). The line segments represent the sections that correspond to the solid curves in Figure 1.

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