Horizontal diffusion and resolution are important factors to generate and maintain the super-rotation in the general circulation model (GCM) because waves which transport angular momentum are sensitive to them. Here, we investigated how the super-rotation depends on the magnitude of horizontal hyper diffusion using a Venus atmospheric GCM with medium and high resolutions. In both the runs, we found a parameter range where the structure of fully developed super-rotation is almost independent of the magnitude of horizontal diffusion. Spectral analysis shows that unrealistically strong super-rotation is developed when medium-scale disturbances are dissipated by stronger horizontal diffusion. On the other hand, artificially weak super-rotation is also realized because spurious small-scale disturbances are accumulated when the horizontal diffusion is too weak. Graphical Abstract: [Figure not available: see fulltext.]
CITATION STYLE
Sugimoto, N., Fujisawa, Y., Komori, N., Kashimura, H., Takagi, M., & Matsuda, Y. (2023, December 1). Super-rotation independent of horizontal diffusion reproduced in a Venus GCM. Earth, Planets and Space. Springer Science and Business Media Deutschland GmbH. https://doi.org/10.1186/s40623-023-01806-7
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