Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Parks Road, Oxford OX1 3PU, UKOxford Martin Programme on Modelling and Predicting Climate
Philos Trans A Math Phys Eng Sci. 2014 Jun 28;372(2018):20130391. doi: 10.1098/rsta.2013.0391.
This paper sets out a new methodological approach to solving the equations for simulating and predicting weather and climate. In this approach, the conventionally hard boundary between the dynamical core and the sub-grid parametrizations is blurred. This approach is motivated by the relatively shallow power-law spectrum for atmospheric energy on scales of hundreds of kilometres and less. It is first argued that, because of this, the closure schemes for weather and climate simulators should be based on stochastic-dynamic systems rather than deterministic formulae. Second, as high-wavenumber elements of the dynamical core will necessarily inherit this stochasticity during time integration, it is argued that the dynamical core will be significantly over-engineered if all computations, regardless of scale, are performed completely deterministically and if all variables are represented with maximum numerical precision (in practice using double-precision floating-point numbers). As the era of exascale computing is approached, an energy- and computationally efficient approach to cloud-resolved weather and climate simulation is described where determinism and numerical precision are focused on the largest scales only.
本文提出了一种新的方法学方法,用于解决模拟和预测天气和气候的方程。在这种方法中,传统上动力核心和次网格参数化之间的硬边界变得模糊。这种方法的动机是大气能量在数百公里及以下尺度上具有相对较浅的幂律谱。首先,由于这个原因,天气和气候模拟器的闭合方案应该基于随机动力系统,而不是确定性公式。其次,由于动力核心的高波数元素在时间积分过程中必然会继承这种随机性,因此,如果所有计算,无论规模如何,都完全确定性地执行,并且所有变量都以最大数值精度表示(实际上使用双精度浮点数),则动力核心的设计将过于复杂。随着 exascale 计算时代的到来,本文描述了一种能量和计算效率高的云分辨天气和气候模拟方法,其中确定性和数值精度仅集中在最大尺度上。