Fig. 10 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. 10.

Effect of reversing the east‐west polarity of the active region complex in CR 1909 (left). Because the equatorial dipole components of the bipoles and the background field are now in phase with each other, the streamer belt shows a greater latitudinal excursion than in the original case (right).

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