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Calculus IV Unit 14 Review

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14.1 Cylindrical coordinate system and transformation

14.1 Cylindrical coordinate system and transformation

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
Calculus IV
Unit & Topic Study Guides

Cylindrical Coordinate System

Defining Cylindrical Coordinates

Cylindrical coordinates describe points in 3D space using three values: (r,θ,z)(r, \theta, z). Think of it as polar coordinates in the xy-plane with a height coordinate tacked on.

  • rr is the radial distance from the z-axis to the point's projection in the xy-plane.
    • Always non-negative: r0r \geq 0
    • Computed as r=x2+y2r = \sqrt{x^2 + y^2}
  • θ\theta is the angle in the xy-plane, measured counterclockwise from the positive x-axis.
    • Range: 0θ<2π0 \leq \theta < 2\pi
    • Computed as θ=arctan ⁣(yx)\theta = \arctan\!\left(\frac{y}{x}\right), with the usual quadrant adjustments (use atan2(y,x)\text{atan2}(y, x) to get the correct quadrant automatically)
  • zz is the height along the z-axis, exactly the same as in Cartesian coordinates. It can be positive, negative, or zero.

This system is ideal whenever the region or integrand has circular symmetry about the z-axis (cylinders, cones, paraboloids, etc.), because the geometry lines up naturally with rr and θ\theta.

Notation note: Many textbooks use (r,θ,z)(r, \theta, z) while others use (ρ,ϕ,z)(\rho, \phi, z). They mean the same thing. In this guide we use (r,θ,z)(r, \theta, z) to avoid confusion with spherical coordinates, where ρ\rho typically denotes the distance from the origin.

Defining Cylindrical Coordinates, Vectors and the Geometry of Space | Boundless Calculus

Relationship to Cartesian Coordinates

Cylindrical → Cartesian:

x=rcosθ,y=rsinθ,z=zx = r\cos\theta, \qquad y = r\sin\theta, \qquad z = z

Cartesian → Cylindrical:

r=x2+y2,θ=arctan ⁣(yx),z=zr = \sqrt{x^2 + y^2}, \qquad \theta = \arctan\!\left(\frac{y}{x}\right), \qquad z = z

The zz-coordinate is unchanged in both directions. The first two equations are just the polar-coordinate conversions you already know from Calculus II/III, applied to the xy-plane.

Quick example: Convert the Cartesian point (1,3,5)(1, \sqrt{3}, 5) to cylindrical.

  • r=12+(3)2=4=2r = \sqrt{1^2 + (\sqrt{3})^2} = \sqrt{4} = 2
  • θ=arctan ⁣(31)=π3\theta = \arctan\!\left(\frac{\sqrt{3}}{1}\right) = \frac{\pi}{3}
  • z=5z = 5

So the cylindrical form is (2,π3,5)(2,\, \frac{\pi}{3},\, 5).

Defining Cylindrical Coordinates, HartleyMath - Rectangular, Cylindrical, and Spherical Coordinates

Coordinate Transformation

Cartesian to Cylindrical Transformation

When you convert a triple integral from Cartesian to cylindrical coordinates, you need to do three things:

  1. Substitute the coordinate expressions into the integrand:

    • Replace every xx with rcosθr\cos\theta
    • Replace every yy with rsinθr\sin\theta
    • Leave zz alone
  2. Replace the volume element dxdydzdx\,dy\,dz with rdrdθdzr\,dr\,d\theta\,dz (the extra factor of rr comes from the Jacobian; see below).

  3. Transform the limits of integration to describe the same region in (r,θ,z)(r, \theta, z) variables. This is often the trickiest step: sketch the region and express its boundaries in terms of rr, θ\theta, and zz.

Example: Consider the integral over the upper half of a unit cylinder:

01 ⁣01x2 ⁣01dzdydx\int_{0}^{1}\!\int_{0}^{\sqrt{1-x^2}}\!\int_{0}^{1} dz\,dy\,dx

The xy-limits describe the upper half of the unit disk (xx from 0 to 1, yy from 0 to 1x2\sqrt{1-x^2}). In cylindrical coordinates that region is 0r10 \leq r \leq 1, 0θπ20 \leq \theta \leq \frac{\pi}{2}. The zz-limits stay the same. So the integral becomes:

0π/2 ⁣01 ⁣01rdzdrdθ\int_{0}^{\pi/2}\!\int_{0}^{1}\!\int_{0}^{1} r\,dz\,dr\,d\theta

Notice the limits changed to θ[0,π/2]\theta \in [0, \pi/2] (first quadrant only), not [0,2π][0, 2\pi], because the original Cartesian region only covers the first quadrant.

Jacobian Determinant and Volume Element

Why does that extra rr appear? It comes from the Jacobian determinant of the coordinate transformation. The Jacobian matrix is:

J=(xrxθxz$4pt]yryθyz$4pt]zrzθzz)=(cosθrsinθ0sinθrcosθ0001)J = \begin{pmatrix} \frac{\partial x}{\partial r} & \frac{\partial x}{\partial \theta} & \frac{\partial x}{\partial z} \$4pt] \frac{\partial y}{\partial r} & \frac{\partial y}{\partial \theta} & \frac{\partial y}{\partial z} \$4pt] \frac{\partial z}{\partial r} & \frac{\partial z}{\partial \theta} & \frac{\partial z}{\partial z} \end{pmatrix} = \begin{pmatrix} \cos\theta & -r\sin\theta & 0 \\ \sin\theta & r\cos\theta & 0 \\ 0 & 0 & 1 \end{pmatrix}

Computing the determinant gives:

J=cosθ(rcosθ)(rsinθ)(sinθ)=rcos2θ+rsin2θ=r|J| = \cos\theta \cdot (r\cos\theta) - (-r\sin\theta)\cdot(\sin\theta) = r\cos^2\theta + r\sin^2\theta = r

So J=r|J| = r, and the volume element transforms as:

dV=dxdydz=rdrdθdzdV = dx\,dy\,dz = r\,dr\,d\theta\,dz

Geometrically, this makes sense: a small "box" in cylindrical coordinates is a wedge-shaped piece. Its radial side has length drdr, its height is dzdz, but its arc-length side is rdθr\,d\theta (not just dθd\theta). The product of these three gives rdrdθdzr\,dr\,d\theta\,dz.

The general transformation formula for a triple integral is:

Df(x,y,z)dxdydz=Df(rcosθ,rsinθ,z)  rdrdθdz\iiint_D f(x,y,z)\,dx\,dy\,dz = \iiint_{D'} f(r\cos\theta,\, r\sin\theta,\, z)\; r\,dr\,d\theta\,dz

where DD' is the region DD described in cylindrical coordinates. Don't forget the rr factor; dropping it is one of the most common mistakes on exams.