星球核心中的流对流长度尺度
Céline Guervilly1, Philippe Cardin2, Nathanaël Schaeffer2
1School of Mathematics, Statistics and Physics, Newcastle University, Newcastle upon Tyne, UK. celine.guervilly@ncl.ac.uk.
Nature
|June 21, 2019
概括
行星核心对流对于磁场至关重要,通过新的模型可以更好地理解. 动荡的对流长度尺度变得独立于粘度,简化了地球和月球的模拟.
科学领域:
- 地质学
- 流体动力学
- 星球科学
背景情况:
- 在行星流体核心中的对流会运输热量和化学物质,驱动行星磁场.
- 由于对旋转,浮力和磁场的依赖性,对核心对流的准确建模具有挑战性.
- 在非磁性核心中快速旋转的流对流是一个鲜为人知的模式.
研究的目的:
- 探索行星核心中快速旋转的流对流.
- 确定控制行星核心对流长度尺度的关键因素.
- 为小型非磁性行星核心开发更现实的模型,并推断到更大的模型.
主要方法:
- 使用非磁性数值模型模拟快速旋转的流对流.
- 研究了对流长度尺度对粘度,流速和行星旋转的依赖.
- 应用这些发现来建模小型非磁性核心的动态,并推断到更大的行星体.
主要成果:
- 在现实的行星核心条件下,对流长度尺度变得独立于粘度.
- 长度尺度主要由流速和行星旋转决定.
- 对于地球的核心,流对流长度尺度大约为30公里,远大于粘性尺度.
结论:
- 流对流长度尺度为核心流中的能量载体尺度提供了下限.
- 这一发现简化了地力学模拟,可能减轻了解决粘度尺度的需要.
- 这项研究提供了一种更现实的方法来模拟像月球这样的小型非磁性核心的对流,并允许将其推断到更大的核心.
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