Introduction and Motivation
Inner Core AnisotropyThe Earth's inner core (IC) is a solid ball with a radius of about 1,220 km (e.g., Kennett et al., 1995) located in the center of our planet. As the Earth cools, the IC grows over time through solidification of the liquid outer core (Buffett et al., 1992;Jacobs, 1953). The release of latent heat and light elements during solidification drives convection in the outer core, providing energy for the geodynamo and generating Earth's magnetic field (e.g., Gubbins et al., 2003;Labrosse & Macouin, 2003;Loper, 1984). In addition to the decay of radioactive isotopes and the Earth's long-term secular cooling, the heat loss from the Earth's core is one of the largest energy sources driving the mantle convection-the primary mechanism responsible for plate tectonics. Therefore, studies on the IC have the potential to unravel the history of the internal dynamic processes of our planet. Unfortunately, progress on seismic imaging of the Earth's IC is limited by the poor worldwide distribution of large sources and