Curvilinear Coordinates Outline: 1. Orthogonal curvilinear coordinate systems 2. Differential operators in orthogonal curvilinear coordinate systems 3. Derivatives of the unit vectors in orthogonal curvilinear coordinate systems 4. Incompressible N-S equations in orthogonal curvilinear coordinate systems 5. Example: Incompressible N-S equations in cylindrical polar systems The governing equations were derived using the most basic coordinate system, i.e, Cartesian coordinates: x xˆi yˆj zkˆ f f f grad f f ˆi ˆj kˆ x y z F F F div F F 1 2 3 x y z ˆi ˆj kˆ curl f F x F1 y F2 z F3 2 f 2 f 2 f Laplacian f 2 2 2 x y z 2 Example: incompressible flow equations V 0 DV p z 2 V Dt V V V p z 2 V t V 1 V V V ω p z V ω t 2 ω V V 0 in the above equation, but retained to keep the complete vector identity for 2 V in equation. However, once the equations are expressed in vector invariant form (as above) they can be transformed into any convenient coordinate system through the use of appropriate definitions for the , , , and 2 . Frequently, alternative coordinate systems are desirable which either exploit certain features of the flow at hand or facilitate numerical procedures. The most general coordinate system for fluid flow problems are nonorthogonal curvilinear coordinates. A special case of these are orthogonal curvilinear coordinates. Here we shall derive the appropriate relations for the latter using vector technique. It should be recognized that the derivation can also be accomplished using tensor analysis 1. Orthogonal curvilinear coordinate systems Suppose that the Cartesian coordinates x, y, z are expressed in terms of the new coordinates x1 , x2 , x3 by the equations x x x1 , x2 , x3 y y x1 , x2 , x3 z z x1 , x2 , x3 where it is assumed that the correspondence is unique and that the inverse mapping exists. For example, circular cylindrical coordinates x r cos y r sin zz i.e., at any point P , x1 curve is a straight line, x2 curve is a circle, and the x3 curve is a straight line. The position vector of a point P in space is R xˆi yˆj zkˆ R r cos ˆi r sin ˆj z kˆ for cylindrical coordinates By definition a vector tangent to the x1 curve is given by: R x xx ˆi yx ˆj z x kˆ (Subscript denotes partial differentiation) 1 1 1 1 So that the unit vectors tangent to the xi curve are eˆ1 R x1 h1 , eˆ 2 R x2 h2 , eˆ 3 R x3 h3 Where hi R x are called the metric coefficients or scale factors hr 1, hz 1 for cylindrical coordinates h r , 1 The arc length along a curve in any direction is given by ds 2 dR dR h12 dx12 h22 dx22 h32 dx32 Since dR R xi dxi hi dxi eˆ i and R xi hi eˆ i 0, and since the xi are orthogonal: eˆ i eˆ j 1, i j i j An element of volume is given by the triple product d h1dx1eˆ1 h2 dx2eˆ 2 h3dx3eˆ 3 h1h2 h3dx1dx2dx3 Where since the xi are orthogonal eˆ1 eˆ 2 eˆ 3 Finally, on the surface x1 constant, the vector element of surface area is given by ds1 h2 dx2eˆ 2 h3dx3eˆ 3 eˆ1h2 h3dx2 dx3 With similar results for x2 and x3 constant ds2 eˆ 2 h3h1dx3dx1 ds3 eˆ 3h1h2 dx1dx2 2. Differential operators in orthogonal curvilinear coordinate systems With the above in hand, we now proceed to obtain the desired vector operators 1 f 1 f 1 f eˆ1 eˆ 2 eˆ 3 h1 x1 h2 x2 h3 x3 By definition: df f dR f xi dxi 2.1 Gradient f If we temporarily write f 1eˆ1 2eˆ 2 3eˆ 3 Then by comparison df f xi dxi i hi dxi 1 f hi xi 1 1 1 eˆ1 eˆ 2 eˆ 3 h1 x1 h2 x2 h3 x3 1 eˆ r eˆ eˆ z for cylindrical coordinates r r z i eˆ i hi 1 f i hi xi Note xi So that by definition ( curl grad f 0 ) xi Also eˆ i 0 hi eˆ1 eˆ eˆ 2 3 x2 x3 h2 h3 h2 h3 So that by definition ( f g 0 ) eˆ eˆ eˆ 1 2 3 0 h1h2 h2 h3 h3h1 2.2 Divergence F 1 h1h2 h3 h3h1F2 h1h2 F3 h2 h3 F1 x2 x3 x1 F F1eˆ1 F2eˆ 2 F3eˆ 3 eˆ F1eˆ1 h2 h3 F1 1 using u u u h2 h3 eˆ eˆ eˆ eˆ 1 h2 h3 F1 using 1 2 3 0 h2 h3 h1h2 h2 h3 h3h1 1 h2 h3 F1 h1h2 h3 x1 Treating the other terms in a similar manner results in 1 F h3h1F2 h1h2 F3 h2 h3 F1 h1h2 h3 x1 x2 x3 1 F rF1 F2 rF3 r r z 1 1 rF1 F2 F3 for cylindrical coordinates r r r z h1eˆ1 1 2.3 Curl F h1h2 h3 x1 h2eˆ 2 x2 h3eˆ 3 x3 h1 F1 h2 F2 h3 F3 F F1eˆ1 F2eˆ 2 F3eˆ 3 eˆ F1eˆ1 h1 F1 1 h1 eˆ eˆ1 h1 F1 using u u u and i 0 h1 hi eˆ1 1 h1F1 1 h1F1 1 h1F1 eˆ1 eˆ 2 eˆ 3 h1 h1 x1 h2 x2 h3 x3 eˆ 3 eˆ 2 h1F1 h1F1 h1h2 x2 h3 h1 x3 1 h3eˆ 3 h2eˆ 2 h1F1 h1h2 h3 x3 x2 h1eˆ1 h2eˆ 2 h3eˆ 3 1 F h1h2 h3 x1 x2 x3 h1 F1 h2 F2 h3 F3 eˆ r reˆ eˆ z 1 F for cylindrical coordinates r r z F1 rF2 F3 2.4 Laplacian acting on a scalar 2 f 1 h1h2 h3 h2 h3 h3 h1 h1h2 x1 h1 x1 x2 h2 x2 x3 h3 x3 2 h2 h3 h3h1 h1h2 x1 h1 x1 x2 h2 x2 x3 h3 x3 1 1 2 r r r r r r z z 1 h1h2 h3 1 1 r r r r r 1 r 1 r r z z 2.5 Laplacian acting on a vector 2F F F Using f and F F 1 f 1 f 1 f eˆ1 eˆ 2 eˆ 3 h1 x1 h2 x2 h3 x3 1 h1h2 h3 h3h1F2 h1h2 F3 h2 h3 F1 x2 x3 x1 1 1 h3h1F2 h1h2 F3 eˆ1 h2 h3 F1 h1 x1 h1h2 h3 x1 x2 x3 1 1 h3h1F2 h1h2 F3 eˆ 2 h2 h3 F1 h2 x2 h1h2 h3 x1 x2 x3 1 1 h2 h3 F1 h3h1F2 h1h2 F3 eˆ 3 h3 x3 h1h2 h3 x1 x2 x3 h1eˆ1 1 Using F h1h2 h3 x1 h2eˆ 2 x2 h3eˆ 3 x3 h1 F1 h2 F2 h3 F3 F 1 h2 h3 h3 x2 h1h2 h h1F1 2 h2 F2 x2 x1 x3 h1h3 h1F1 h3 F3 eˆ1 x1 x3 h1 h3 ˆ h F h F h F h F 3 3 2 2 2 2 1 1 e2 x3 x2 x3 h2 h3 x2 x1 h1h2 x1 h 1 h2 h1F1 h3 F3 1 h3 F3 h2 F2 eˆ 3 h1h2 x1 h1h3 x3 x1 x3 x2 h2 h3 x2 1 h1h3 Combining those two terms gives 2F F F 1 1 h2 h3 F1 h3h1F2 h1h2 F3 eˆ1 h1 x1 h1h2 h3 x1 x2 x3 h2 1 h3 ˆ h F h F h F h F 2 2 1 1 1 1 3 3 e1 h2 h3 x2 h1h2 x1 x2 x1 x3 h1h3 x3 1 1 h3h1F2 h1h2 F3 eˆ 2 h2 h3 F1 h2 x2 h1h2 h3 x1 x2 x3 h 1 h1 h3 F3 h2 F2 3 h2 F2 h1F1 eˆ 2 h1h3 x3 h2 h3 x2 x3 x2 x1 h1h2 x1 1 1 h2 h3 F1 h3h1F2 h1h2 F3 eˆ 3 h3 x3 h1h2 h3 x1 x2 x3 h1 1 h2 ˆ h F h F h F h F 1 1 3 3 3 3 2 2 e3 h1h2 x1 h1h3 x3 x1 x3 x2 h2 h3 x2 For cylindrical coordinates r, , z , h1 hr 1, h2 h r , h3 hz 1 , and use the definition of Laplacian operator acting on a scalar 2 f 1 1 2 f r r r r r r z z 1 1 2 2 r r r r r 2 2 z 2 1 2 1 2 2 2 2 r r r r 2 z 2 F 1 2 F 2 F 2 F aeˆ r beˆ ceˆ z 2 F1 2 F1 2 2 eˆ r 2 F2 22 2 1 eˆ 2 F3 eˆ z r r r r a 1 1 h3h1F2 h1h2 F3 h2 h3 F1 h1 x1 h1h2 h3 x1 x2 x3 h3 x2 h1h2 h h1F1 2 h2 F2 x2 x1 x3 h1h3 1 h2 h3 1 rF1 F2 rF3 r r r z h1F1 h3 F3 x1 x3 1 1 rF2 F1 r F1 F3 r r r r z z F F F 1 F1 r 1 2 r 3 r r r z F F F F 1 1 F2 r 2 1 r 1 r 3 r r r z z r F 1 F2 F3 1 F1 1 r r r r z 2 F3 F 1 F1 2 F1 1 1 F2 2 r r r r r r z 2 zr 2 2 2 1 1 F1 F1 1 F2 1 F2 F3 2 F1 2 2 r r r r r r r rz 2 F3 2 F1 1 1 F2 2 F2 1 2 F1 r r r r r r 2 z 2 zr 2 F3 1 1 F1 2 F1 1 F2 1 2 F2 F 1 r2 r r r 2 r 2 r r rz 1 F 1 2 F 1 2 F1 2 F1 2 F3 2 2 2 2 2 2 z zr r r r r 2 2 2 1 1 F1 F1 2 F2 1 F1 F1 2 F1 r r r r 2 r 2 r 2 2 z 2 1 F1 2 F1 1 2 F1 2 F1 1 2 F 2 2 2 2 F1 2 2 2 r z r r r r r 1 F1 1 2 F1 2 F1 1 2 F 2 2 F1 2 2 2 2 z r r r r r r 1 2 F 2 F1 2 F1 2 2 r r b 1 1 h3h1F2 h1h2 F3 h2 h3 F1 h2 x2 h1h2 h3 x1 x2 x3 h 1 h1 h3 F3 h2 F2 3 h2 F2 h1F1 h1h3 x3 h2 h3 x2 x3 x2 x1 h1h2 x1 1 1 rF1 F2 rF3 r r r z 1 1 F3 rF2 rF2 F1 z r r r z r F F F 1 1 F1 r 1 2 r 3 r r r z 1 F3 F2 1 F2 F1 F2 r r z r z r r F 1 F2 F3 1 1 F1 1 r r r r z 1 2 F3 2 F2 1 F 1 F1 2 F2 2 r r r r r z z 1 1 F1 2 F1 1 2 F2 2 F3 r r r r 2 z 1 2 F3 2 F2 F2 1 F2 2 F2 1 F1 1 2 F1 2 2 2 2 r r r r r r r r z z 1 F1 1 2 F1 1 2 F2 1 2 F3 r 2 r r r 2 2 r z 1 2 F3 2 F2 F2 1 F2 2 F2 1 F1 1 2 F1 2 2 2 2 z r r r r r r r r z 1 F2 2 F2 1 2 F2 2 F2 F2 2 F1 2 2 2 2 2 r r 2 z r r r r 1 F2 1 2 F2 2 F2 F2 2 F1 2 2 2 r 2 2 z r r r r r r F 2 F 2 F2 22 2 1 r r c 1 1 h2 h3 F1 h3h1F2 h1h2 F3 h3 x3 h1h2 h3 x1 x2 x3 h 1 h2 h1F1 h3 F3 1 h3 F3 h2 F2 h1h2 x1 h1h3 x3 x1 x3 x2 h2 h3 x2 1 rF1 F2 rF3 z r r z 1 1 r F1 F3 F3 rF2 r r z r z r F F F 1 F1 r 1 2 r 3 z r r z F 1 F3 F2 1 F r 1 r 3 r r z r r z F F 1 F2 F3 1 1 z r r r z 2 F 1 2 F3 2 F2 2 F1 F3 1 F 1 r r 23 r z r z r r r 2 z 1 F1 2 F1 1 2 F2 2 F3 2 r z zr r z z 1 F1 2 F1 1 F3 2 F3 1 2 F3 1 2 F2 2 2 rz r r r r 2 r z r z 1 F3 2 F3 1 2 F3 2 F3 2 2 r r r r 2 z 2 1 F3 2 F3 1 2 F3 2 F3 r r r r r 2 r 2 2 z 2 2 F3 3. Derivatives of the unit vectors in orthogonal curvilinear coordinate systems The last topic to be discussed concerning curvilinear coordinates is the procedure to obtain the derivatives of the unit vectors, i.e. eˆ i eˆ ij x j Such quantities are required, for example, in obtaining the rate-of-strain and rotation tensor eij V 1 1 eij eijT V V 2 2 1 1 ij eij eijT V V 2 2 To simplify the notation we define: R xi ri , R xi hi eˆ i ri ij R xi rij and hi hij x j x j Note that rij is symmetric, i.e. rij r ji r1 h1eˆ1 r2 h2eˆ 2 r3 h3eˆ 3 r11 aeˆ1 beˆ 2 ceˆ 3 h11eˆ1 h1eˆ11 r12 h12eˆ1 h1eˆ12 r13 h13eˆ1 h1eˆ13 h h 3.1 Derivation of eˆ11 12 eˆ 2 13 eˆ 3 h2 r1 r1 h 2 1 r1 r11 h1h11 r1 r12 h1h12 r1 r13 h1h13 r1 r2 0 r1 r2 0 x1 r11 r2 r1 r21 0 r11 r2 r1 r12 h3 r11 r2 h1h12 r1 r3 0 r1 r3 0 x1 r11 r3 r1 r31 0 r11 r3 r1 r13 r11 r3 h1h13 hh h1h12 eˆ 2 1 13 eˆ 3 h11eˆ1 h1eˆ11 h2 h3 h h eˆ11 12 eˆ 2 13 eˆ 3 h2 h3 r11 h11eˆ1 3.2 Derivation of eˆ 22 h h21 eˆ1 23 eˆ 3 h1 h3 r2 r2 h22 r2 r22 h2 h22 r2 r21 h2 h21 r2 r23 h2 h23 r1 r2 0 r1 r2 0 x2 r12 r2 r1 r22 0 r22 r1 r2 r21 r22 r1 h2 h21 r2 r3 0 r2 r3 0 x2 r22 r3 r2 r32 0 r22 r3 r2 r23 r22 r3 h2 h23 r22 hh h2 h21 eˆ1 h22eˆ 2 2 23 eˆ 3 h22eˆ 2 h2eˆ 22 h1 h3 eˆ 22 h h21 eˆ1 23 eˆ 3 h1 h3 3.3 Derivation of eˆ 33 h31 h eˆ1 32 eˆ 2 h1 h2 r3 r3 h32 r3 r31 h3h31 r3 r32 h3h32 r3 r33 h3h33 r1 r3 0 r1 r3 0 x3 r13 r3 r1 r33 0 r33 r1 r3 r31 r33 r1 h3h31 r2 r3 0 r2 r3 0 x3 r23 r3 r2 r33 0 r33 r2 r3 r32 r33 r2 h3h32 h3 h31 hh eˆ1 3 32 eˆ 2 h33eˆ 3 h33eˆ 3 h3eˆ 33 h1 h2 h h eˆ 33 31 eˆ1 32 eˆ 2 h1 h2 r33 3.4 Derivation of eˆ 32 h23 h eˆ 2 , eˆ 23 32 eˆ 3 h3 h2 r1 r2 r13 r2 r1 r23 0 x3 r2 r3 0 r2 r3 r21 r3 r2 r31 0 x1 r3 r1 0 r3 r1 r32 r1 r3 r12 0 x2 r1 r2 0 1 2 3 3 2 0 r32 r1 r2 r31 0 r32 r1 r2 r31 r32 r1 r1 r23 r32 r1 0 r32 aeˆ1 beˆ 2 ceˆ 3 h32eˆ 3 h3eˆ 32 r32 aeˆ1 beˆ 2 ceˆ 3 h23eˆ 2 h32eˆ 3 h eˆ 32 23 eˆ 2 h3 r23 h23eˆ 2 h2eˆ 23 r23 r32 aeˆ1 beˆ 2 ceˆ 3 h23eˆ 2 h32eˆ 3 h eˆ 23 32 eˆ 3 h2 h h 3.5 Derivation of eˆ 21 12 eˆ1 , eˆ12 21 eˆ 2 h2 2 1 0 h1 r21 r3 r1 r23 0 r21 r3 r1 r23 r21 r3 r3 r12 r21 r3 0 r21 h21eˆ 2 h2eˆ 21 r21 h12eˆ1 h21eˆ 2 h eˆ 21 12 eˆ1 h2 r12 h12eˆ1 h1eˆ12 r12 r21 h12eˆ1 h21eˆ 2 h eˆ12 21 eˆ 2 h1 3.6 Derivation of eˆ13 3 1 0 h31 h eˆ 3 , eˆ 31 13 eˆ1 h1 h3 r3 r12 r13 r2 0 r2 r13 r3 r12 r2 r13 r2 r31 r2 r13 0 r13 h13eˆ1 h1eˆ13 r13 h13eˆ1 h31eˆ 3 h eˆ13 31 eˆ 3 h1 r31 h31eˆ 3 h3eˆ 31 r31 r13 h13eˆ1 h31eˆ 3 h eˆ 31 13 eˆ1 h3 4. Incompressible N-S equations in orthogonal curvilinear coordinate systems 4.1 Continuity equation V 0 1 h3h1F2 h1h2 F3 h2 h3 F1 h1h2 h3 x1 x2 x3 and V v1eˆ1 v2eˆ 2 v3eˆ 3 Since F V 1 h1h2 h3 h3h1v2 h1h2v3 0 h2 h3v1 x2 x3 x1 V 1 V V p 2 V , (where p piezometric pressure) t Since V v1eˆ1 v2eˆ 2 v3eˆ 3 , we can expand the momentum equation term by term 4.2 Momentum equation Local derivative v v V v1 eˆ1 2 eˆ 2 3 eˆ 3 t t t t Convective derivative V V Since V v1eˆ1 v2eˆ 2 v3eˆ 3 and V v1 v2 v3 h1 x1 h2 x2 h3 x3 V V V v1eˆ1 V v2eˆ 2 V v3eˆ3 V v1eˆ1 v1 v1eˆ1 v2 v1eˆ1 v3 v1eˆ1 h1 x1 h2 x2 h3 x3 v v eˆ v v v v eˆ v v v v eˆ v v 1 1 eˆ1 1 1 1 2 1 eˆ1 2 1 1 3 1 eˆ1 3 1 1 h1 x1 h1 x1 h2 x2 h2 x2 h3 x3 h3 x3 v 1 h1 v 1 h1 v1v1 vv v1 v2 v1 v3 v1 vv eˆ11 2 1 eˆ12 3 1 eˆ13 eˆ1 x1 h2 x2 h3 x3 h2 h3 h1 h13 v1 v2 v1 v3 v1 v1v1 h12 eˆ1 eˆ 2 eˆ 3 x1 h2 x2 h3 x3 h1 h2 h3 v2v1 h21 v3v1 h31 eˆ 2 eˆ 3 h2 h1 h3 h1 v v v v v v v vh v vh vvh vvh 1 1 2 1 3 1 eˆ1 2 1 21 1 1 12 eˆ 2 3 1 31 1 1 13 eˆ 3 h1h2 h3h1 h1h2 h1 x1 h2 x2 h3 x3 h3h1 V v2eˆ 2 v v2eˆ 2 v2 v2eˆ 2 v3 v2eˆ 2 1 h1 x1 h2 x2 h3 x3 v v v v eˆ v v v v eˆ v v v v eˆ 1 2 eˆ 2 1 2 2 2 2 eˆ 2 2 2 2 3 2 eˆ 2 3 2 2 h1 x1 h1 x1 h2 x2 h2 x2 h3 x3 h3 x3 v 1 h1 v 1 h1 vv v2 v2 v2 v3 v2 v1v2 vv eˆ 21 2 2 eˆ 22 3 2 eˆ 23 eˆ 2 x1 h2 x2 h3 x3 h1 h2 h3 v2 v2 v2 v3 v2 v1v2 h12 eˆ 2 eˆ1 x1 h2 x2 h3 x3 h1 h2 h23 v3v2 h32 v2v2 h21 eˆ 3 eˆ1 eˆ 3 h2 h1 h3 h3 h2 v v v v v v v v h vv h vvh vvh 1 2 12 2 2 21 eˆ1 1 2 2 2 3 2 eˆ 2 3 2 32 2 2 23 eˆ 3 h2 h1 h2 h3 h1h2 h1 x1 h2 x2 h3 x3 h2 h3 V v3eˆ 3 v v3eˆ 3 v2 v3eˆ 3 v3 v3eˆ 3 1 h1 x1 h2 x2 h3 x3 v v eˆ v v eˆ v v v v eˆ v v v v 1 3 eˆ 3 1 3 3 2 3 eˆ 3 2 3 3 3 3 eˆ 3 3 3 3 h1 x1 h1 x1 h2 x2 h2 x2 h3 x3 h3 x3 v v v v v v vv vv vv 1 3 2 3 3 3 eˆ 3 1 3 eˆ 31 2 3 eˆ 32 3 3 eˆ 33 h1 h2 h3 h1 x1 h2 x2 h3 x3 v v v v v v v v h vv h 1 3 2 3 3 3 eˆ 3 1 3 13 eˆ1 2 3 23 eˆ 2 h1 h3 h2 h3 h1 x1 h2 x2 h3 x3 vv h h 3 3 31 eˆ1 32 eˆ 2 h3 h1 h2 vv h v v h v v v v v v vvh vvh 1 3 13 3 3 31 eˆ1 2 3 23 3 3 32 eˆ 2 1 3 2 3 3 3 eˆ 3 h3h1 h3h2 h1h3 h2 h3 h1 x1 h2 x2 h3 x3 Pressure gradient p 1 p 1 p 1 p eˆ1 eˆ 2 eˆ 3 h1 x1 h2 x2 h3 x3 Viscous term 2 V 2V 1 1 h2 h3v1 h3h1v2 h1h2v3 eˆ1 h1 x1 h1h2 h3 x1 x2 x3 h 1 h3 h1v1 2 h1v1 h3v3 eˆ1 h2v2 h2 h3 x2 h1h2 x1 x2 x1 x3 h1h3 x3 1 1 h2 h3v1 h3h1v2 h1h2v3 eˆ 2 h2 x2 h1h2 h3 x1 x2 x3 h3 1 h1 ˆ h v h v h v h v 3 3 2 2 2 2 1 1 e2 h1h3 x3 h2 h3 x2 x3 x2 x1 h1h2 x1 1 1 h3h1v2 h1h2v3 eˆ 3 h2 h3v1 h3 x3 h1h2 h3 x1 x2 x3 1 h1h2 h2 x1 h1h3 h h1v1 h3v3 1 x1 x3 x2 h2 h3 h3v3 h2v2 eˆ 3 x3 x2 4.2.1 Combine terms in ê1 direction to get momentum equation in ê1 direction v1 v1 v1 v2 v1 v3 v1 v1v2 h12 v2v2 h21 v1v3h13 v3v3h31 t h1 x1 h2 x2 h3 x3 h1h2 h2 h1 h1h3 h3h1 1 1 p h1 x1 1 1 h2 h3v1 h3h1v2 h1h2v3 h1 x1 h1h2 h3 x1 x2 x3 h 1 h3 h1v1 2 h1v1 h3v3 h2v2 h2 h3 x2 h1h2 x1 x2 x1 x3 h1h3 x3 4.2.2 Combine terms in ê2 direction to get momentum equation in ê2 direction v2 v2 v1h21 v1v1h12 v1 v2 v2 v2 v3 v2 v2 v3h23 v3v3h32 t h1h2 h1h2 h1 x1 h2 x2 h3 x3 h2 h3 h3h2 1 1 p h2 x2 1 1 h3h1v2 h1h2v3 h2 h3v1 h2 x2 h1h2 h3 x1 x2 x3 h3 1 h1 h v h v h v h v 3 3 2 2 2 2 1 1 h1h3 x3 h2 h3 x2 x3 x2 x1 h1h2 x1 4.2.3 Combine terms in ê3 direction to get momentum equation in ê3 direction v3 v3v1h31 v1v1h13 v3v2 h32 v2v2 h23 v1 v3 v2 v3 v3 v3 t h3h1 h3h1 h2 h3 h2 h3 h1 x1 h2 x2 h3 x3 1 1 p h3 x3 1 1 h2 h3v1 h3h1v2 h1h2v3 h3 x3 h1h2 h3 x1 x2 x3 h 1 h2 h1v1 h3v3 1 h3v3 h2v2 h1h2 x1 h1h3 x3 x1 x3 x2 h2 h3 x2 5. Example: Incompressible N-S equations in cylindrical polar systems 5.1 Continuity equation V 0 in cylindrical coordinates r, , z For cylindrical coordinates r, , z , h1 hr 1, h2 h r , h3 hz 1 1 V rvr v rvz 0 r r z 1 1 rvr v vz 0 r r r z V 1 V V p 2 V in cylindrical coordinates r, , z t For cylindrical coordinates r, , z , h1 hr 1, h2 h r , h3 hz 1 and only h21 h r 1 , all 5.2 Momentum equation others are zero. 5.2.1 The r-momentum equation: vr v v v v v 2 1 p 1 2 v vr r r vz r 2vr 2 vr 2 t r r z r r r r 5.2.2 The -momentum equation: v 1 v v v v F 1 p 2 F vr v vr vz 2 F2 22 2 1 t r r r z r r r 5.2.3 The z-momentum equation: vz v v v v 1 p vr z z vz z 2vz t r r z z