Energy Transport in the Climate System and Its Parameterisation

0Citations
Citations of this article
1Readers
Mendeley users who have this article in their library.
Get full text

Abstract

In the annual mean, the Earth takes up energy between 30∘ S and 30∘ N, while it has a negative energy balance towards the poles (Fig. 4.1). Since neither a continuous warming in the lower latitudes nor a cooling in the high latitudes are observed, a strong poleward transport of energy is required. The integration of the meridional radiation balance from the South Pole to the North Pole, as it is given in Fig. 4.1, yields the heat transport, required by the radiation balance (Fig. 4.2). In each hemisphere, about (Petawatt) are transported polewards. This flux is split about evenly between ocean and atmosphere. The maximum heat transport in the northern hemisphere occurs around 45∘ N in the atmosphere and around 20∘ N in the ocean. This fact points to the different mechanisms and boundary conditions (continents) responsible for the meridional heat transport. The atmosphere transports heat in a way fundamentally different from that of the ocean. The most important mechanisms are briefly explained in the following sections.

Cite

CITATION STYLE

APA

Stocker, T. (2011). Energy Transport in the Climate System and Its Parameterisation. In Advances in Geophysical and Environmental Mechanics and Mathematics (pp. 79–89). Springer Science+Business Media B.V. https://doi.org/10.1007/978-3-642-00773-6_4

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free