Rotation of Solar Magnetic Fields for the Current Solar Cycle 24
Authors: X. J. Shi and J. L. Xie
Shi & Xie
2014 The Astronomical Journal148101.
Provider: AAS Journals
Caption: Figure 2.
Time variation of smoothed rotation rates of positive (solid line) and negative (dashed line) magnetic fields during CR numbers 2076–2146. Panels (g)–(l) correspond to the higher latitudes of −40°, 40°, −50°, 50°, −60°, and 60°, respectively.