Fig. 12 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. 12.

Simulation illustrating the decay of the active region flux and the flattening of the streamer belt in the hypothetical absence of any new activity after 1996 September. The observed photospheric field for CR 1913 was evolved for 13 rotations including only transport effects.

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