“…It has been suggested that iron from Earth's outer core may be responsible for their presence, either driven to the mantle by diffusion (e.g., Lesher et al., 2020) or via morphological instabilities (Otsuka & Karato, 2012). Alternatively, enrichment of iron in ferropericlase could explain the ultralow velocities (e.g., Finkelstein et al., 2018; Lai et al., 2022). The presence of partial melt has also been suggested as an explanation for ULVZs (e.g., Ferrick & Korenaga, 2023; Lay et al., 2004; Yuan & Romanowicz, 2017), although it is imperfectly understood how melt pockets just above the CMB can stay stable over geological time scales (e.g., Dannberg et al., 2021; Hernlund & Jellinek, 2010).…”