When estimating an integral using spherical coordinates we divide up a solid into small pieces of dimension Δρ by Δθ by Δφ.
The shaded portion has volume Δθ((ρ+Δρ)3-ρ3)(cosφ-cos(φ+Δφ))/3 = Δθ(3ρ2Δρ+3ρ(Δρ)2+(Δρ)3)(cosφ-cosφcos(Δφ)+sinφsin(Δφ))/3 since cos(a+b)=cos(a)cos(b)-sin(a)sin(b). When Δρ, Δθ, and Δφ are small, the volume is approximately ρ2 sinφ Δρ Δθ Δφ since cos(Δφ) is approximately 1 and sin(Δφ) is approximately Δφ. This is a visual aid for why adding an extra ρ2 sinφ is necessary when using spherical coordinates. However, the precise reason is that the absolute value of the Jacobian of the transformation x = ρ sinφ cosθ, y = ρ sinφ sinθ, z = ρ cosφ, is ρ2 sinφ. Therefore, when we integrate a function f(ρ,θ,φ) over a solid T in spherical coodinates, we use
We can also change the order of integration if T is a basic solid (the boundary is a finite number of continuous surfaces--see Calculus One and Several Variables 8th Ed. Salas/Hille/Etgen pg 999.) Thus the following integrals are all equivalent:
To determine the limits of integration, we take the outermost variable and work inward. Sketching the graph of the solid T is extremely helpful.
Here are the basic step for integrating in the order dρ dθ dφ. Other orders are similar.
The integral will have the general form
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