Download Atmospheric Circulation Dynamics and General Circulation by Masaki Satoh PDF

By Masaki Satoh

General move versions (GCMs), which outline the elemental dynamics of atmospheric circulate, are these days utilized in numerous fields of atmospheric technological know-how comparable to climate forecasting, weather predictions and environmental estimations. the second one variation of this well known paintings has been up-to-date to incorporate contemporary development of excessive answer international modeling. It additionally includes for the 1st time facets of high-resolution international non-hydrostatic types that the writer has been learning because the book of the 1st version. a few highlighted effects from the Non-hydrostatic ICosahedral Atmospheric version (NICAM) also are incorporated. the writer outlines the theoretical innovations, basic versions and numerical equipment for modeling the overall circulate of the ambience. focusing on the actual mechanisms accountable for the advance of large-scale stream of the ambience, the e-book deals entire assurance of an immense and quickly constructing process utilized in the atmospheric technology. Dynamic interpretations of the atmospheric constitution and their facets within the normal move version are defined step by means of step.

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Example text

1. 14 [Ch. 19) where f is the frictional force, whose components are defined by fi 1 ∂ σ . 17) yields f 1 η 2 ∇ v+ ρ ρ = 1 ζ + η ∇(∇ · v). 23) is the kinematic viscosity. This form of the equations of motion is called the NavierStokes equation. We then derive the momentum equation in a rotating frame. We define the angular velocity of the rotating frame by Ω, which is constant irrespective of time. We also designate a quantity in the inertial frame by a subscript a and that in the rotating frame by a subscript r.

59) must satisfy this requirement. 36). The expression of ε is determined so as not to be negative. 17). 37). From the requirement ε ≥ 0, the coefficients of viscosity must be positive: η ≥ 0 and ζ ≥ 0. 44). 45) is used. Since this must be non-negative, it is concluded that the thermal conductivity κT must not be negative. 61), in general. This comes from the fact that local thermodynamic equilibrium is not generally satisfied for the photon gas in the atmosphere. 5 Enthalpy balance and Bernoulli’s theorem From the transformation between enthalpy and kinetic energy, we obtain Bernoulli’s theorem.

The outward normal component of the flux F at one side of V is Fn . 6) (ρa) + ∇ · (ρav + F ) = σ[ρa]. ∂t The conservation of mass is given by setting A = ρ and a = 1. e, the conservation of mass). 9) dt ∂t is the material derivative. Using the conservation of mass, the time dependence of an arbitrary quantity a is written as ∂ da = (ρa) + ∇ · (ρav). 6) is rewritten as da + ∇ · F = σ[ρa]. 11) becomes ρ da = 0. dt This means that a conserves along fluid motion. Sec. 2 Conservation of momentum Let the velocity of the fluid be v and its components in the Cartesian coordinates be vi (i = 1, 2, 3).

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