School of Earth and Environment, University of Leeds, Leeds, LS2 9JT, UK.
Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California at San Diego, La Jolla, CA, 92093-0225, USA.
Nat Commun. 2020 Jul 6;11(1):3371. doi: 10.1038/s41467-020-16888-0.
Extreme variations in the direction of Earth's magnetic field contain important information regarding the operation of the geodynamo. Paleomagnetic studies have reported rapid directional changes reaching 1° yr, although the observations are controversial and their relation to physical processes in Earth's core unknown. Here we show excellent agreement between amplitudes and latitude ranges of extreme directional changes in a suite of geodynamo simulations and a recent observational field model spanning the past 100 kyrs. Remarkably, maximum rates of directional change reach ~10° yr, typically during times of decreasing field strength, almost 100 times faster than current changes. Detailed analysis of the simulations and a simple analogue model indicate that extreme directional changes are associated with movement of reversed flux across the core surface. Our results demonstrate that such rapid variations are compatible with the physics of the dynamo process and suggest that future searches for rapid directional changes should focus on low latitudes.
地球磁场方向的极端变化包含有关地磁场发电机运行的重要信息。古地磁研究报告称,磁场方向快速变化达到 1°/年,尽管这些观测结果存在争议,且其与地球核心内物理过程的关系尚不明确。在这里,我们展示了一套地磁场发电机模拟结果与最近跨越过去 10 万年的观测磁场模型之间在极端方向变化幅度和纬度范围上的极好一致性。值得注意的是,最大的方向变化速率达到~10°/年,通常发生在磁场强度减弱期间,比当前变化快近 100 倍。对模拟结果和简单的模拟模型的详细分析表明,极端方向变化与反向通量在核心表面的运动有关。我们的结果表明,这种快速变化与发电机过程的物理性质是兼容的,并表明未来对快速方向变化的搜索应该集中在低纬度地区。