Seismic anisotropy arises from the structural or mineralogical fabric and is thus a useful proxy for mapping deformation. In the upper mantle, it is commonly explained by crystallographic preferred orientation of the olivine crystals (e.g., Karato et al., 2008). Earth's zero-order anisotropy component is its radial anisotropy (RA), also called vertical transverse isotropy. It is present in particular in the upper mantle of the PREM model (Dziewonski & Anderson, 1981), where the horizontally polarized S waves (SH) down to 200 km depth have a velocity higher than the vertically polarized S waves (SV) by 2.5% on average. The conventional explanation for this so-called positive RA is the dominantly horizontal direction of the flow in the upper part of the mantle, leading to horizontal preferred orientation of the olivine crystal a-axis, which, if averaged in azimuth, results in SH waves faster than SV waves (see review in Maupin & Park, 2015). The sparser regions with negative RA (and thus vertical a-axis