B. Finite difference equations of the model   a. Atmospheric model up previous next
B.a.iii. Diagnostic equation of the pressure function

Before deriving the finite difference equation, Equation (A.8) is transformed as follows.


(The definition of is described in Appendix B.a.i.). This equation can be solved by using the dimension reduction method. The finite difference form of the pressure equation can be written in matrix form.

(B.19)

where are matrixes whose elements are in finite difference form for the following terms.


and are the eigenvalue and eigenvector of . By using the eigenvalue matrix and the eigenvector matrix of , . Expanding so , Equation (B.19) can be rewritten as follows.


Therefore,

(B.20)

The elements of matrix , which are required to derive eigenvalue and eigenvector , are evaluated in finite form as


Second- and fourth-order centered schemes are used since space differencing in the continuity equation is evaluated by a fourth-order centered scheme while space differencing in the pressure gradient term is evaluated by a second-order centered scheme. Therefore, is a quint-diagonal matrix. , which is element of , is represented as follows.

(B.21)
(B.22)
(B.23)
(B.24)
(B.25)

Boundary conditions are at the lower and upper boundary.

The horizontally-dependent terms are expanded by using an eigenfunction. In this model, we use a Fourier series.

(B.26)
(B.27)
(B.28)


(B.29)


A Numerical Simulation of Thermal Convection in the Martian Lower Atmosphere with a Two-Dimensional Anelastic Model
Odaka, Nakajima, Ishiwatari, Hayashi,   Nagare Multimedia 2001
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