How to Solve a PDE in Spherical Coordinates Using Vector Spherical Harmonics?

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The discussion focuses on solving a partial differential equation (PDE) in spherical coordinates using vector spherical harmonics. The approach involves expanding the unknown function f and the known functions g and vector field B into spherical harmonic bases. By integrating the equation over the unit sphere, an ordinary differential equation (ODE) for the coefficients f_{lm}(r) is derived, which can be solved numerically. The main concern is whether the solutions for f_{lm} will satisfy the original equation after integration. The spherical harmonic method is preferred for its elegance, despite the complexities of numerical solutions in a 3D spherical grid.
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I am trying to solve the following equation in spherical coordinates:
<br /> \left( \nabla f \right) \cdot \vec{B} = g<br />
where g is a known scalar function, \vec{B} is a known vector field, and f is the unknown function.

I think the best way to approach this is to expand everything into a spherical harmonic basis:
<br /> f(r,\theta,\phi) = \sum_{lm} f_{lm}(r) Y_{lm}(\theta,\phi)<br />
<br /> g(r,\theta,\phi) = \sum_{lm} g_{lm}(r) Y_{lm}(\theta,\phi)<br />
<br /> \vec{B}(r,\theta,\phi) = \sum_{lm} \left[ B_{lm}^r(r) \vec{Y}_{lm} + B_{lm}^{(1)} \vec{\Psi}_{lm} + B_{lm}^{(2)} \vec{\Phi}_{lm} \right]<br />
where \vec{Y}_{lm}, \vec{\Psi}_{lm}, \vec{\Phi}_{lm} are the vector spherical harmonics (VSH) defined here:
http://en.wikipedia.org/wiki/Vector_spherical_harmonics
Then, to evaluate the dot product between \nabla f and \vec{B}, it is necessary to integrate over the unit sphere since the VSH orthogonality relations are defined in terms of integrals over d\Omega.

So, integrating the original equation over d\Omega will yield the following ODE equation for the unknown f_{lm}(r):
<br /> B_{lm}^r(r) \frac{d}{dr} f_{lm}(r) + \frac{l(l+1)}{r} B_{lm}^{(1)}(r) f_{lm}(r) = c_{lm} g_{lm}(r)<br />
with
<br /> c_{lm} = \int d\Omega Y_{lm} e^{-im\phi}<br />

This ODE should be straightforward to solve numerically. However, my question is the ODE equation will determine f_{lm} values which satisfy the equation:
<br /> \int d\Omega \left( \nabla f \right) \cdot \vec{B} = \int d\Omega g<br />

Is it true that these f_{lm} will also satisfy the original equation?
 
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My first choice of solution method would be method of characteristics, take a 2D case and you can easily see how this works and you can generalise to 3D case.
 
Yes its true that the method of characteristics could work, however I am solving this equation numerically on a 3D grid in spherical coordinates. Integrating along characteristic curves would add complexity in that I'd have to pick lots of different starting points for the integration to get a decent grid of solutions, and then interpolate those solutions back to a spherical grid.

I think the spherical harmonic approach is more elegant and natural for this problem...if only the method I've described above is sound.
 
Every time you separate your variables, the resulting functions satisfy the original equations on their own only under special conditions (the obvious one being the other function being equal to 1). As far as I know, it is not something you can generalise.
 

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