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Solenoidal vector field
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In a solenoidal vector field (also known as an incompressible vector field, a divergence-free vector field, or a transverse vector field) is a v with zero at all points in the field: \nabla \cdot \mathbf{v} = 0. A common way of expressing this property is to say that the field has no sources or sinks.This statement does not mean that the field lines of a solenoidal field must be closed, neither that they cannot begin or end. For a detailed discussion of the subject, see J. Slepian: "Lines of Force in Electric and Magnetic Fields", American Journal of Physics, vol. 19, pp. 87-90, 1951, and L. Zilberti: "The Misconception of Closed Magnetic Flux Lines", IEEE Magnetics Letters, vol. 8, art. 1306005, 2017.


Properties
The divergence theorem gives an equivalent integral definition of a solenoidal field; namely that for any closed surface, the net total flux through the surface must be zero:

where d\mathbf{S} is the outward normal to each surface element.

The fundamental theorem of vector calculus states that any vector field can be expressed as the sum of an and a solenoidal field. The condition of zero divergence is satisfied whenever a vector field v has only a component, because the definition of the vector potential A as: \mathbf{v} = \nabla \times \mathbf{A} automatically results in the identity (as can be shown, for example, using Cartesian coordinates): \nabla \cdot \mathbf{v} = \nabla \cdot (\nabla \times \mathbf{A}) = 0. The converse also holds: for any solenoidal v there exists a vector potential A such that \mathbf{v} = \nabla \times \mathbf{A}. (Strictly speaking, this holds subject to certain technical conditions on v, see Helmholtz decomposition.)


Etymology
Solenoidal has its origin in the Greek word for , which is σωληνοειδές (sōlēnoeidēs) meaning pipe-shaped, from σωλην (sōlēn) or pipe.


Examples
  • The B (see Gauss's law for magnetism)
  • The velocity field of an incompressible fluid flow
  • The field
  • The E in neutral regions (\rho_e = 0);
  • The J where the charge density is unvarying, \frac{\partial \rho_e}{\partial t} = 0.
  • The magnetic vector potential A in Coulomb gauge


See also
  • Longitudinal and transverse vector fields
  • Conservative vector field


Notes
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