The linear response function of an idealized atmosphere. Part 2: Implications for the practical use of the Fluctuation-Dissipation Theorem and the role of operator's non-normality
Pedram Hassanzadeh, Zhiming Kuang

TL;DR
This paper investigates why the Fluctuation-Dissipation Theorem often performs poorly in climate models by analyzing the impact of operator non-normality and dimension-reduction techniques on the accuracy of linear response functions.
Contribution
It demonstrates that dimension-reduction by EOFs and operator non-normality are key factors causing errors in FDT-based LRF calculations in climate models.
Findings
FDT-based LRFs perform poorly for some test cases.
Dimension-reduction via EOFs introduces significant errors.
Operator non-normality is a primary source of these errors.
Abstract
A linear response function (LRF) relates the mean-response of a nonlinear system to weak external forcings and vice versa. Even for simple models of the general circulation, such as the dry dynamical core, the LRF cannot be calculated from first principles due to the lack of a complete theory for eddy-mean flow feedbacks. According to the Fluctuation-Dissipation Theorem (FDT), the LRF can be calculated using only the covariance and lag-covariance matrices of the unforced system. However, efforts in calculating the LRFs for GCMs using FDT have produced mixed results, and the reason(s) behind the poor performance of the FDT remains unclear. In Part 1 of this study, the LRF of an idealized GCM, the dry dynamical core with Held-Suarez physics, is accurately calculated using Green's functions. In this paper (Part 2), the LRF of the same model is computed using FDT, which is found to perform…
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