episciences.org_17084_2026053118342751420260531183427514episciences.orgraphael.tournoy+crossrefapi@ccsd.cnrs.frepisciences.orgJournal of Studies of Earth’s Deep Interior3099-287710.46298/journals/jsedihttps://jsedi.episciences.org05152026Volume 2SouvikNaskarhttps://orcid.org/0000-0003-0445-8417Jonathan E.Moundhttps://orcid.org/0000-0002-1243-6915Christopher J.Davieshttps://orcid.org/0000-0002-1074-3815Andrew T.Clarkehttps://orcid.org/0000-0003-2128-0016Convection in Earth's outer core is driven by the release of heat and light elements at the inner core boundary. A key question is whether these buoyancy sources drive convection throughout the core, or whether a stable layer exists just below the core-mantle boundary (CMB). Recent simulations incorporating CMB heat flux heterogeneities propose locally stable ``regional inversion lenses'' (RILs) rather than a global layer, allowing stable and unstable regions to coexist. However, these simulations combine thermal and compositional anomalies, ignoring differences in diffusivities and boundary conditions. Here we simulate thermal, chemical, and thermochemical convection at Ekman number $E=10^{-5}$, with thermal and chemical flux Rayleigh numbers $\widetilde{Ra}_T=30-4000$ and $\widetilde{Ra}_ξ=30-100000$, and Prandtl numbers $Pr_T=1$ and $Pr_ξ=10$. Purely chemical simulations accumulate light elements below the CMB, forming locally stable regions near the poles or global layers, depending on $\widetilde{Ra}_ξ$. These chemically stratified regions persist in thermochemical simulations even when thermal forcing is destabilising. Introducing heterogeneous CMB heat flux produces thermally stratified RILs even with strongly destabilising compositional buoyancy. Our simulations reveal a diverse range of locations, properties, and morphologies of stable regions depending on $\widetilde{Ra}_T$ and $\widetilde{Ra}_ξ$, they can have a seismically detectable thickness and strength and might also have a signature in geomagnetic observations.Submitted to Journal of Studies of Earths Deep Interior051520260509202617084https://creativecommons.org/licenses/by/4.0https://creativecommons.org/licenses/by/4.0https://creativecommons.org/licenses/by/4.0arXiv:2507.0353810.48550/arXiv.2507.03538https://arxiv.org/abs/2507.03538v4https://arxiv.org/abs/2507.03538v2https://doi.org/10.5285/74c2ed9d-6ab4-4d24-863d-5991afbe84ce10.46298/jsedi.17084https://jsedi.episciences.org/17084https://arxiv.org/pdf/2507.03538v5https://arxiv.org/pdf/2507.03538v5