Series Solution to Quasi-Geostrophic (QG) Equation
Xiaoyun Liu
Table of Contents
QG Equation
Luu≡(∇h2+∂p2∂2)u=fx∈Ω=gx∈∂Ω
where Laplacian in spherical coordinates (θ,ϕ) (polar (colatitudinal), azimuthal (longitudinal)) is defined as:
∇h2=r2sin2ϕ1∂θ2∂2+r2sinϕ1∂ϕ∂(sinϕ∂ϕ∂)
Note that θ=π/2−Φ and ϕ=λ, where (Φ,λ) = (latitude, longitude).
Spherical Harmonic
The operator ∇h2 has eigenfunctions (Spherical Harmonic) satisfying:
∇h2Yl=−λlYl
Assuming Y=Θ(θ)Φ(ϕ) with 2π periodicity, we find λl=l(l+1) for l=0,1,⋯. For each l:
dθ2d2ΘΘ1and Φ(ϕ)=−m2,m=−l,⋯,l satisfies the associated Legendre differential equation
The normalized solutions are:
Ylm(θ,ϕ)=4π2l+1(l+m)!(l−m)!Plm(cosθ)eimϕ
with orthonormality:
⟨Ylm,Yl′m′⟩w=δm,m′δl,l′
where the weighted inner product is:
⟨f,g⟩w≡∫[0,2π]×[0,π]fgˉsin(θ)dθdϕ
Spectral Method
Expanding solutions:
ufwhere Flm(p)=l=0∑∞m=−l∑lAlm(p)Ylm(θ,ϕ)=l=0∑∞m=−l∑lFlm(p)Ylm(θ,ϕ)=⟨Ylm,Ylm⟩w⟨f,Ylm⟩w
Substituting into QG equation yields ODE system:
dp2d2Alm(p)−l(l+1)Alm(p)=Flm(p)
with boundary conditions:
u=g=l=0∑∞m=−l∑lGlm(p)Ylm(θ,ϕ)x∈∂Ω
- Numerical implementation requires careful handling of inner product integrals
- Real-world QG equations involve scale factors in L and discrete spherical harmonic transforms
- This spectral approach converts PDEs into solvable ODE systems