Let v = 8zk be the velocity field (in meters per second) of a fluid in R3. Calculate the flow rate (in cubic meters per second) through the upper hemisphere (z ≥ 0) of the sphere x2 + y2 + z2 = 1.
Recall how to find flow rate through a surface, S, for a fluid with velocity vector field v. Choose the correct integral below to calculate the flow rate across the S (volume per unit time).
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To calculate the integral, you will also need to recall how to find a vector surface integral. Let F be a vector field. Let G(u, v) be an oriented parametrization of an oriented surface S with parameter domain D. Assume that G is one-to-one, and regular, except possibly at points on the boundary of D. Then we can calculate the vector surface integral as follows.
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If the orientation of S is reversed, the surface integral changes sign.
Before we can make any calculations, we must find an appropriate parametrization for the upper hemisphere of the sphere x2 + y2 + z2 = 1 since that is the surface through which the fluid is moving. Since this is part of a sphere, it will be easiest to convert the surface to spherical coordinates.
State the standard conversions.
x = R cos θ
y = R sin θ
z = R
Because the surface through which the fluid is moving is only the upper hemisphere, we have the following bounds on the parameters θ and φ.
0 ≤ θ <
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0 ≤φ ≤
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Since the radius of the sphere is 1, we have the following parametrization.
G(θ, φ) = (cos θ sin φ, sin θ sin φ, cos φ)
Find Tφ and Tθ for G(θ, φ). Then use these vectors to compute n(φ, θ), the outward normal vector through the upper hemisphere.
Tφ = (∂G / ∂φ) =
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Tθ = (∂G / ∂θ) =
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n(φ, θ) = Tφ × Tθ =
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Express the velocity field v = 8zk in terms of the parameters φ and θ. In other words, calculate v(G(θ, φ)).
v = 8zk
= <0, 0, 8z>
Therefore v(G(θ, φ)) = <, , cosφ>
Compute the dot product v(G(θ, φ)) ·n(φ, θ).
v(G(θ, φ)) · n(φ, θ) = <0, 0, 8 cos φ> · sin φ <cos θ sin φ, sin θ sin φ, cos φ>
= sin φ cos2φ
Integrate to calculate the flow rate through the upper hemisphere.
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