Fig. 11 from Origin and Evolution of Coronal Streamer Structure During the 1996 Minimum Activity Phase

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Origin and Evolution of Coronal Streamer Structure During the 1996 Minimum Activity Phase

Authors: Y.-M. Wang, N. R. Sheeley, Jr., R. A. Howard, J. R. Kraemer, N. B. Rich, M. D. Andrews, G. E. Brueckner, K. P. Dere, M. J. Koomen, C. M. Korendyke, D. J. Michels, J. D. Moses, S. E. Paswaters, D. G. Socker, D. Wang, P. L. Lamy, A. Llebaria, D. Vibert, R. Schwenn, and G. M. Simnett

Wang et al. 1997 The Astrophysical Journal 485 875.

Provider: AAS Journals

Caption: Fig. 11.

Left panels illustrate how the photospheric field, equatorial dipole, and streamer structure would have appeared during CR 1913 if no new flux had erupted over the previous two rotations. The WSO photospheric field map for CR 1911 was evolved in time including only transport effects (differential rotation, supergranular diffusion, and meridional flow). Right panels show the corresponding maps based on the observed photospheric field for CR 1913.

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