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Noah D. Brenowitz, Tom Beucler, Michael Pritchard, and Christopher S. Bretherton

in the GCRM budget residuals and training method. The LRF-wave analysis can also identify spurious wave-like modes that could contribute to numerical instability in coupled simulations. Figure 9 shows a mode of the unablated model that has planetary-scale wavelength of 6283 km, phase speed of 44 m s −1 and fast growth rate of 1.29 day −1 . This mode is stable for shorter waves, so we have chosen a longer wavelength. The moisture, humidity, moistening, and drying tendencies are in phase with

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