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. Author manuscript; available in PMC: 2009 Oct 7.
Published in final edited form as: J Theor Biol. 2008 Jul 4;254(3):674–690. doi: 10.1016/j.jtbi.2008.06.030

Figure 10.

Figure 10

Spiral wave trajectories during windows of stability during the quasi-stable dynamics of the CM, CM-N, and CM-X. Two trajectories are shown for the CM and CM-N, while only one trajectory is shown for the CM-X, which was particularly prone to breakup. All the models produce meandering linear core trajectories approximately 4–6 cm in length.