Numerical simulation of subsynoptic-scale cyclogenesis around an idealized antarctic continent

Numerical simulation of subsynoptic-scale cyclogenesis around an idealized antarctic continent

Autores/as

  • Jorge F. Carrasco Universidad de Magallanes

Resumen

A three-dimensional numerical model of 100- km horizontal resolution was used to simulate subsynoptic-scale cyclogenesis around an idealized Antarctic continent. The simulation resolved a series of subsynoptic-scale cyclones around the idealized continent. These cyclones form adjacent to the confluence zones of katabatic winds. Their movements indicate an eastward direction going away from their initial point of formation. Baroclinic instability appears as primary mechanism for the development of these cyclones.

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Publicado

2017-12-29

Cómo citar

Carrasco, J. F. (2017). Numerical simulation of subsynoptic-scale cyclogenesis around an idealized antarctic continent. Anales Del Instituto De La Patagonia, 45(3), 5–17. Recuperado a partir de https://www.analesdelinstitutodelapatagonia.cl/index.php/analespatagonia/article/view/746

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