modules

This module is designed to give you an overview of the key physical processes determining the behaviour of the Earth's ocean and atmosphere, exploring both some of the major processes involved and the fundamental theory behind them. An informative subtitle might be climate physics for the mathematically literate. The module builds upon basic principles and key equations (such as hydrostatic balance, ideal gas law, adiabatic fluid motion etc) to bring to life an application of the content from MTH3007 - Fluid Dynamics. Topics covered will include radiative energy transfer, the structure, motion and thermodynamics of the atmosphere, the surface energy balance, and the main components of the general circulation (Hadley cells, Walker cells, jet streams etc.). The emphasis, where possible, will be on simple analytical models (such as shallow water equations and Ekman layers) for commonly observed phenomena and on the development of physical intuition. The material is developed further in modules such as MTHM019 Fluid Dynamics of Atmospheres and Oceans.

Prerequisite module: MTH3007 or equivalent

_{Please note that all modules are subject to change, please get in touch if you have any questions about this module.}