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Rotation of Solar Magnetic Fields for the Current Solar Cycle 24

  • Authors: X. J. Shi and J. L. Xie

Shi & Xie 2014 The Astronomical Journal 148 101.

  • 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.

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