Fig. 3 from Origin and Evolution of Coronal Streamer Structure During the 1996 Minimum Activity Phase

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution

Export to PDF PPT Format

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. 3.

Time variation of the Sun's lowest order, rms multipole strengths, evaluated (a) at the photosphere, (b) at r = 2.5 R_☉. The dipole strength ⟨b₁⟩ is indicated by the solid line, the quadrupole strength ⟨b₂⟩ by the dashed line, and the octupole strength ⟨b₃⟩ by the dotted line. The curves were derived using WSO photospheric field data for CR 1835–1913.

Other Images in This Article

Copyright and Terms & Conditions