Here is a direct use of the spherical representation that also avoids estimating separate coordinate derivatives at the poles. Put , , and write for unit-sphere area. Then . Expanding its squared norm with the physical measure gives
On each boundary sphere , so every angular derivative, including and , is zero there. Radial and angular integration by parts consequently give
Indeed the term gives with boundary remainder , while the term is , its boundary remainder also being zero. Thus
where the last step uses the preceding energy estimate and . All unmarked integrals in these two identities are with .
To control every angular second derivative, the spherical Hessian identity is
It follows by integrating the derivative-commutation identity and using on the unit sphere. There is no sphere boundary. Hence the preceding bound controls , , and in their appropriate weighted norms.
In an orthonormal polar frame the Cartesian Hessian matrix has components
and . Since is bounded above and below, these bounds plus the first-order estimate prove
This is the direct spherical-shell H2 estimate. Intrinsic angular integration combines the suggested angular tests, with no spurious boundary at the polar coordinate singularities.

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