Let be probability density per unit solid angle, with and isotropic initial condition . In still fluid, bottom-heavy spherical-cell orientation dynamics gives . Adding isotropic rotational diffusion gives the gyrotactic orientation Fokker-Planck equation
The derivatives are tangential to the unit sphere. Rotational symmetry about is preserved by both the equation and the initial condition, so depends only on . Since , the polar probability flux is . Expanding yields
Regular solutions have no probability flux through the poles. The mean swimming velocity is , with only a vertical component by symmetry.
Use the rotation convention of part (a), so the orientation drift is . The steady gyrotactic orientation Fokker-Planck equation on the unit sphere is
Let , , and introduce the rotation generator . Dividing by gives
The leading isotropic density is . At first order, writing , rotational diffusion makes no contribution because . The tangential drift is the spherical gradient of , whose divergence is . Therefore
In the polar convention of the paper, , and . Thus, in the specified first-harmonic form,
The correction integrates to zero, preserving normalization. The first correction has no dependence on because the isotropic leading density has zero spherical Laplacian; enters the next-order equations.
Spherical symmetry gives . Consequently the rapid-rotation mean gyrotactic orientation is
It is this small horizontal swimming bias, rather than a mean vertical orientation at leading order, that enters the concentration equation of part (c).