Fig. 9 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. 9.

Equatorial dipole field b₁₁ at r = 2.5 R_☉, derived from the WSO photospheric field maps for CR 1908–1913 (Fig. 6). Black denotes b₁₁ < −0.04 G, white denotes b₁₁ > 0.04 G, while intermediate shades indicate fields in the range −0.04 G < b₁₁ < 0.04 G.

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