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COMPARISON OF CORONAL EXTRAPOLATION METHODS FOR CYCLE 24 USING HMI DATA

  • Authors: William M. Arden, Aimee A. Norton, Xudong Sun, and Xuepu Zhao

2016 The Astrophysical Journal 823 21.

  • Provider: AAS Journals

Caption: Figure 1.

Diagram representations of coronal field extrapolation models. (a) The PFSS model assumes a “source surface” at which all magnetic field lines are open and radial. Moving the PFSS source surface to a lower height increases the open flux because it forces more higher-order structures to become open. (b) The HCCSSS model includes a “cusp surface,” which we explain in the text. Moving this cusp surface in or out also affects the open flux calculated by this model.

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