Fig. 3 from A Model for Solar Coronal Mass Ejections

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A Model for Solar Coronal Mass Ejections

Authors: S. K. Antiochos, C. R. DeVore, and J. A. Klimchuk

Antiochos, DeVore, & Klimchuk 1999 The Astrophysical Journal 510 485.

Provider: AAS Journals

Caption: Fig. 3.

Magnetic‐free energy as a function of shear for the force‐free field solution (lower line) and the MHD solution (upper line). The shear is in units of π and the free energy is expressed as percentage of the initial potential field energy.

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