The divergence of the position vector field is . At height , the horizontal cross-section is a disk of area . By the divergence theorem, the outward flux integral is three times the enclosed volume:
Therefore
A direct check separates the two pieces of the surface integral. On the unit sphere, the outward unit normal is , so and the curved contribution is . On the top disk, , giving . Their sum is the same flux.
Differentiate the flux:
On , is strictly increasing. Its limiting endpoint values are and , and . It has horizontal limiting tangents at the endpoints, curves upward for , curves downward for , and has an inflection point at zero.
The derivative graph is a downward-opening parabola, approaching zero at both endpoints and attaining its maximum at .
Figure 1.
Flux through the truncated unit sphere and its derivative
. Both curves are scaled by . Endpoint circles show limiting values because the prescribed truncation parameter lies in . The flux increases from zero to , while its derivative is largest at the equator. Details.
Use the two pieces of the surface integral directly; this avoids introducing an unnecessary second derivative of . On the unit sphere, and . A spherical band between heights and has area , so the curved flux is
by the fundamental theorem of calculus. On the horizontal top disk, and the area is . Thus
As usual for these surface integrals, the first derivative is assumed sufficiently integrable for the displayed fundamental theorem of calculus evaluation; a continuous first derivative suffices. Mere pointwise differentiability without such an integrability assumption need not make an ordinary flux integral exist.
Choose
or add any constant. Then , so the vector field is exactly and necessarily has the same flux as in part (a). The formula from part (b)(i) confirms this:

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