Fig. 4 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. 4.

Time variation of the nonaxisymmetric (m ≠ 0) field components at r = 2.5 R_☉. (a) Nonaxisymmetric dipole strength ⟨n₁⟩ (solid line), quadrupole strength ⟨n₂⟩ (dashed line), and octupole strength ⟨n₃⟩ (dotted line), all normalized to the total rms field strength ⟨B_r⟩ at r = 2.5 R_☉. (b) Ratio of the nonaxisymmetric field strength ⟨N⟩ (including all multipoles) to the total field strength ⟨B_r⟩ at r = 2.5 R_☉.

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