A compressed matrix propagator method simulates solar dipole evolution 80-1000 times faster than full surface flux transport models with equivalent accuracy.
The explicit form of the governing equation is ∂Br ∂t =− 1 R⊙ sinθ ∂ ∂θ (sinθu θBr) −Ω(θ) ∂Br ∂ϕ + η R2 ⊙ sinθ ∂ ∂θ sinθ ∂Br ∂θ ! + η R2 ⊙ sin2 θ ∂2Br ∂ϕ2 +S
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Ultra-fast simulations of the solar dipole and open flux
A compressed matrix propagator method simulates solar dipole evolution 80-1000 times faster than full surface flux transport models with equivalent accuracy.