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Conductance Writing Fourier's law can also be stated as: where U is the conductance. The reciprocal of conductance is resistance, equal to: and it is resistance which is additive when several conducting layers lie between the hot and cool regions, because A and Q are the same for all layers. In a multilayer partition, the total conductance is related to the conductance of its layers by: So, when dealing with a multilayer partition, the following formula is usually used: When heat is being conducted from one fluid to another through a barrier, it is sometimes important to consider the conductance of the thin film of fluid which remains stationary next to the barrier. This thin film of fluid is difficult to quantify, its characteristics depending upon complex conditions of turbulence and viscosity, but when dealing with thin high-conductance barriers it can sometimes be quite significant. Newtons law of cooling A related principle, Newton's law of cooling, states that the rate of heat loss of a body is proportional to the difference in temperatures between the body and its surroundings. This form of heat loss principle, however, is not very precise; a more accurate formulation requires an analysis of heat flow based on the heat equation in an inhomogeneous medium. This simplification can be applied so long as it is permitted by the Biot number. Nevertheless, it is easy to derive from this principle the exponential decay of temperature of a body. If T is the temperature of the body, then where r is some positive constant. From which, it follows that For example, simplified climate models may use Newtonian cooling instead of a full (and computationally expensive) radiation code to maintain atmospheric temperatures. Fouriers Law of Conduction abla T : heat flux vector J·Metre|m−2·Second|s−1 T: temperature K : thermal conductivity tensor W·Metre|m−1·Kelvin|K−1 See also | ||||||||||
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