Chapter 13

Continuity and Navier-Stokes Equations in Different Coordinate Systems

13.1 Cartesian Coordinates

13.1.1 Continuity Equation: Compressible

We derived the continuity equation in section 10.4 for Cartesian coordinates. For compressible fluids, it is given by Eq. 10.16 as

ρt+(ρυ)=0ρt+υxρx+υyρy+υzρz+ρ(υxx+υyy+υzz)=0

si1_e

13.1.2 Continuity Equation: Incompressible

For incompressible fluids, the equation simplifies to Eq. 10.17 given by

υ=0υxx+υyy+υzz=0

si2_e

13.1.3 Navier-Stokes Equation: Incompressible Newtonian Fluids

We derived the Navier-Stokes equation in Cartesian coordinates in section 11.7. It is given by Eq. 11.40 in its general form as

ρ(υt+(υ)υ)=kp+ηΔυ

si3_e

which is written out in Cartesian coordinates

x-axis

ρ(υxt+υxυxx+υyυxy+υzυxz)=kxpx+η(2υxx2+2υxy2+2υxz2)

si4_e

y-axis

ρ(υyt+υxυyx+υyυyy+υzυyz)=kypy+η(2υyx2+2υyy2+2υyz2)

si5_e

z-axis

ρ(υzt+υxυzx+υyυzy+υzυzz)=kzpz+η(2υzx2+2υzy2+2υzz2)

si6_e

Before venturing to convert these equations into different coordinate systems, be aware of the meaning of the individual terms. (υ)υsi7_e is a material derivative (see section 7.1.3.10), whereas psi8_e is a gradient (see section 7.1.3.2), and ηΔυsi9_e is a vector Laplacian (see section 7.1.3.7). We must be sure to pick the correctly converted versions of these operators when transferring the equations into different coordinate systems.

13.2 Cylindrical Coordinates

13.2.1 Continuity Equation: Compressible

In order to express the continuity equation in cylindrical coordinates, we need the divergence in cylindrical coordinates that we derived in section 7.6.1 and noted in Eq. 7.94. Using this equation, the continuity equation for compressible fluids becomes

ρt+(ρυ)=0ρt+1rr(ρrυr)+1r(ρυφ)φ+(ρυz)z=0

si10_e

13.2.2 Continuity Equation: Incompressible

Likewise, the continuity equation for incompressible fluids is given by

υ=01rr(rυr)+1rυφφ+υzz=0r+1rυr+1rυφφ+υzz=0

si11_e  (Eq. 13.1)

13.2.3 Navier-Stokes Equation: Incompressible Newtonian Fluids

Pressure Gradient. In order to express Eq. 11.40 in cylindrical coordinates, we require the gradient of the pressure field given by Eq. 7.90 as

P=prer+1rpφeφ+pzez

si12_e

Material Derivative. For the material derivative, we require Eq. 7.106, using F=G=υsi13_e in which case we find

(υ)υ=(υrυrr+υφrυrφυφ2r+υzυrz)er+(υrυφr+υφrυφr+υrυφr+υzυφz)eφ+(υrυzr+υφrυzφ+υzυrz)ez

si14_e

Vector Laplacian. For the vector Laplacian, we use Eq. 7.103, which yields

Δυ=(2υrr2+1rυrr+1r22υrφ2+2υrz2υrr22r2υφφ)er+(2υφr2+1rυφr+1r22υφφ2+2υφz2υφr2+2r2υrφ)eφ+(2υzz2+1rυzr+1r22υzφ2+2Fzz2)ez

si15_e

We can derive a slightly more compact notation using the fact that

r(1rrυrr)=r(1r(υr+rυrr))=r(υrr+υrr)=1rυrrυrr2+2υrr2r(1rrυφr)=r(1r(υφ+rυφr))=r(υφr+υφr)=1rυφrυφr2+2υφr21rr(rrυzr)=1r(υzr+r2rυzr2)=1rυzr+r2rυzr2

si16_e

which allows us to write

Δυ=(r(1r2υrr)+1r22υrφ22r2υφφ+2υrz2)er+(r(1r(rυφ)r)+1r22υφφ2+2r2υrφ+2υφz2)eφ+(1rr(r(rυz)r)+1r22υzφ2+2Fzr2)ez

si17_e

Navier-Stokes Equation. We can now write the Navier-Stokes equation for incompressible Newtonian fluids in cylindrical coordinates as

r-axis

ρ(υrt+υrυrr+υφrυrφυφ2r+υzυrz)=krpr+η(r(1r(rυr)r)+1r22υrφ22r2υφφ+2υrz2)

si18_e

ϕ-axis

ρ(υφt+υrυφr+υφrυφφ+υrυφr+υzυφz)=kφ1rpφ+η(r(1r(rυφ)r)+1r22υφφ22r2υrφ+2υφz2)

si19_e

z-axis

ρ(υzt+υrυzr+υφrυzφ+υzυzz)=kzpz+η(1rr(r(rυz)r)+1r22υzφ2+2Fzz2)

si20_e  (Eq. 13.2)

13.3 Polar Coordinates

We noted in section 7.3 that polar coordinates are a special case of cylindrical coordinates that can be derived by merely ignoring the z-axis of the cylindrical equations.

13.3.1 Continuity Equation: Compressible

For the continuity equation for compressible fluids, we therefore find

ρt+(ρυ)=0ρt+1rr(ρrυr)+1r(ρυφ)φ=0

si21_e

13.3.2 Continuity Equation: Incompressible

In comparison, the continuity equation for incompressible fluids is given by

υ=01rr(rυr)+1rυφφ=0υrr+1rυr+1rυφφ=0

si22_e

13.3.3 Navier-Stokes Equation: Incompressible Newtonian Fluids

The Navier-Stokes equation for incompressible Newtonian fluids in polar coordinates can simply be copied from the equation for cylindrical coordinates by ignoring all contributions in z-direction. We thus find

r-axis

ρ(υrt+υrυrr+υφrυrφυφ2r)=krpr+η(r(1r(rυr)r))+1r22υrφ22r2υφφ

si23_e

ϕ-axis

ρ(υφt+υrυφr+υφrυφφυrυφr)=kφ1rpφ+η(r(1r(rυφ)r)+1r22υφφ2+2r2υrφ)

si24_e  (Eq. 13.3)

13.4 Spherical Coordinates

13.4.1 Continuity Equation: Compressible

For spherical coordinates,1 we derived the divergence in Eq. 7.122, which allows us to express the continuity equation for compressible fluids as

ρt+(ρυ)=0ρt+1r2r(r2ρFr)+1rsinθ(θ(pF0sinθ+ρFφφ))=0

si25_e

13.4.2 Continuity Equation: Incompressible

For incompressible fluids, the continuity equation simplifies to

(ρυ)=01r2r(r2Fr)+1rsinθ(θ(F0sinθ)+Fφφ)=0

si26_e

13.4.3 Navier-Stokes Equation: Incompressible Newtonian Fluids

Pressure Gradient. The pressure gradient in spherical coordinates is given by Eq. 7.118 as

p=prer+1rpθeθ+1rsinθpφeφ

si27_e

Material Derivative. For the material derivative, we use Eq. 7.143 and set F=G=υsi13_e, in which case we find

(υ)υ=(υrυrr+υθrυrθ+υφrsinθυrφυθυθ+υφυφr)er+(υrυθr+υθrυθθ+υφrsinθυθφ+υθυrrυφυφrcosθsinθ)eθ+(υrυφr+υθrυφθ+υφrsinθυθφ+υφυrr+υφυθrcosθsinθ)eφ

si29_e

Vector Laplacian. For the vector Laplacian, we use Eq. 7.135, which yields

Δυ=(2rυrr+2υrr2+1r2cosθsinθυrθ+1r22υrθ2+1r2sin2θ2υrφ22r2υr2r2sin2θ2υφφ2r2υθθ2r2cosθsinθυθ)er+(2rυθr+2υθr2+1r2cosθsinθυθθ+1r22υθθ2+1r2sin2θ2υθφ2υθr2sin2θ+2r2υrθ2r2cosθsin2θυφφ)eθ+(2rυφr+2υφr2+1r2cosθsinθυφθ+1r22υφθ2+1r2sin2θ2υφφ2υφr2sin2θ+2r2sin2θυrφ+2r2cosθsinθυθφ)eφ

si30_e

You may come across a slightly more compact notation that uses the fact that

r(1r2r2υrr)=r(2rυr+υrr)=2r2υr+2rυrr+2υrr21r2sinθθ((υrsinθ)θ)=1r2sinθ(cosθυrθ+sinθ2υrθ2)=1r2cosθsinθυrθ+1r22υrθ22r2sinθθ(υrsinθ)=2r2sinθ(cosθυθ+sinθ2υθθ)=2r2cosθsinθυθ2r2υθθ1r2r(r2υθr)=1r2(2rυθr+r22υθr2)=2rυθr+2υθr21r2θ(1sinθθ(υθsinθ))=1r2θ(cosθsinθυθ+υθθ)=1r2sin2θυθ+1r2cosθsinθυθθ+1r22υθθ21r2r(r2υφr)=1r2(2rυφr+r22υφr2)=2rυφr+2υφr21r2r(1sinθθ(υφsinθ))=1r2r(cosθsinθυφ+υφθ)=1r2sin2θυφ+1r2cosθsinθυφθ+1r22υθθ2

si31_e

which allows us to write

Δυ=(r(1r2(r2υr)r)+1r2sinθθ(υrθsinθ)+1r2sin2θ2υrφ21r2sinθθ(υθsinθ)2r2sinθυφφ)er+

si32_e

(1r2r(r2(υθ)r)+1r2θ(r2υθθ)+2r2υθ+1r2sin2θ2υθφ22r2cosθsin2θυφφ)eθ+(1r2r(r2(υφ)r)+1r2θ(1sinθυθθ(υφsinθ))+1r2sin2θ2υφφ2+2r2sinθυrφ+2r2cosθsin2θυθφ)eφ

si33_e

Navier-Stokes Equation. We can now write the Navier-Stokes equation for incompressible Newtonian fluids in spherical coordinates as

r-axis

ρ(υrt+υrυrr+υθrυrθ+υφrsinθυrφυθ2+υφ2r)=krpr+η(r(1r2(r2υr)r)+1r2sinθθ(sinθυrθ)+1r2sin2θ2υrφ22r2sinθ(υθsinθ)θ2r2sinθυφφ)

si34_e

θ-axis

ρ(υφt+υrυθr+υθrυθθ+υφrsinθυθφ+υrυθrυφ2rcosθsinθ)=kθ1rpθ+η(1r2r(r2υθr)+1r2θ(r2υθθ)+2r2υrθ+1r2sin2θ2υθφ22r2cosθsinθυφφ)

si35_e

ϕ-axis

ρ(υφt+υrυφr+υθrυφθ+υφrsinθυφφ+υrυφr+υθυφrcosθsinθ)=kφ1rsinθpφ+η(1r2r(r2υφr)+1r2θ(1rsinθθ(υφsinθ))+1r2sinθ2υφφ2+2r2sinθυrφ+2r2cosθsinθυθφ)

si36_e  (Eq. 13.4)

13.5 Summary

In this section, we derived the continuity and the Navier-Stokes equations in different coordinate systems. Deriving these equations as functions of the respective operators allowed us to simply use the versions of the respective operators in the different coordinate systems, which we did in section 7.6. As we will see, these different versions of the fundamental equations will come in very handy when discussing flow problems in specific geometries, e.g., cylindrical tubes.


1 In the following, we replace the axis symbol ρ commonly used in spherical coordinates with the symbol r in order to avoid confusion with the density ρ.

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