Geomagnetic secular acceleration is a unique window on the dynamics taking place in Earth's core. In this study, the behaviours of the secular acceleration and underlying core dynamics are examined in new numerical simulations of the geodynamo that reside on a theoretical path in parameter space connecting the region where most classical models are found to the natural conditions. The typical time scale for geomagnetic acceleration is found to be invariant along this path, at a value close to 10 years that matches Earth's core estimates. Despite this invariance, the spatio-temporal properties of secular acceleration show significant variability along the path, with an asymptotic regime of rapid rotation reached after 30% of this path (corresponding to a model Ekman number $E=3~10^{-7}$). In this regime, the energy of secular acceleration is entirely found at periods longer than that of planetary rotation, and the underlying flow acceleration patterns acquire a two-dimensional columnar structure representative of the rapid rotation limit. The spatial pattern of the secular acceleration at the core-mantle boundary shows significant localisation of energy within an equatorial belt. Rapid hydromagnetic wave dynamics is absent at the start of the path but can be clearly exhibited in the asymptotic regime. This study reports on ubiquitous axisymmetric geostrophic torsional waves of weak amplitude relatively to convective transport, and also stronger, laterally limited, quasi-geostrophic Alfvén waves propagating in the cylindrical radial direction from the tip of convective plumes towards the core-mantle boundary. Quasi-geostrophic Alfvén waves are shown to be an important carrier of flow acceleration to the core surface that links with the generation of strong, short-lived and intermittent equatorial pulses in the secular acceleration energy.
Stochastic Resonance in a Thermally Driven Low-Dimensional Geodynamo Model
Università degli Studi di Roma Tor Vergata（罗马托尔维加塔大学）；Ca’ Foscari University of Venice（威尼斯卡福斯卡里大学）；INAF-Istituto di Astrofisica e Planetologia Spaziali（意大利国家天体物理研究所）
Joint Bayesian inference of Earth's magnetic field and core surface flow on millennial timescales
Lund University（隆德大学）；Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, IRD, Univ. Gustave Eiffel（格勒诺布尔阿尔卑斯大学、萨瓦-蒙布朗大学、法国国家科学研究中心、法国国家科研所、古斯塔夫·埃菲尔大学）；Institut de Physique du Globe de Paris, CNRS, Université Paris Cite（巴黎地球物理研究所、法国国家科学研究中心、巴黎 Cité 大学）
