In vector calculus, Helmholtz’s decomposition theorem states that any vector field in three dimensions can be decomposed into the superposition of a curl-free field and a divergence-free field (called the Helmholtz decomposition or the Helmholtz representation). Formally:

The flux field () is called the irrotational or conservative field, where is the scalar potential. The circulation field () is called the source-free or solenoidal field.

I think it’s good to think about the flux field like an electric field, just like how the field lines radiate out from a positive point charge towards a negative point charge. Similarly for the divergence field like a magnetic field, where the field lines rotate. This is in fact the set-up for Maxwell’s equations.

Computations

If we take the curl of the field, then:

where is some flux density. If we take the divergence of the field:

where is the scalar density.