Magnetic field

In physics, a magnetic field (commonly denoted by H and sometimes referred to as magnetic intensity) describes a magnetic force (a vector) on a magnetic probe (for instance a piece of iron) at every point in space; it is a vector field. In non-relativistic physics, the space in question is the three-dimensional Euclidean space &#x1D53C;3&mdash;the infinite world that we live in.

In general H is seen as an auxiliary field useful when a magnetizable medium is present. The magnetic flux density B is usually seen as the fundamental magnetic field, see the article about B for more details about magnetism.

The SI unit of magnetic field strength is ampere&sdot;turn/meter; a unit that is based on the magnetic field of a solenoid. In the Gaussian system of units |H| has the unit oersted, with one oersted being equivalent to (1000/4π)&sdot;A&sdot;turn/m.

Relation between H and B
The magnetic field H is closely related to the magnetic induction B (also a vector field). It is the vector B that gives the magnetic force on moving charges (Lorentz force). Historically, the theory of magnetism developed from Coulomb's law, where H played a pivotal role and B was an auxiliary field, which explains its historic name "magnetic induction". At present the roles have swapped and some authors give B the name magnetic field (and do not give a name to H other than "auxiliary field").

The relation between B and H is for the most common case of linear materials in SI units,
 * $$ \mathbf{B} = \mu_0(\mathbf{1} + \boldsymbol{\chi}) \mathbf{H}, $$

where 1 is the 3&times;3 unit matrix, &chi; the magnetic susceptibility tensor of the magnetizable medium, and &mu;0 the magnetic permeability of the vacuum (also known as magnetic constant). In Gaussian units the relation is
 * $$ \mathbf{B} = (\mathbf{1} + 4\pi \boldsymbol{\chi}) \mathbf{H}, $$

Most non-ferromagnetic materials are linear and isotropic; in the isotropic case the susceptibility tensor is equal to &chi;m1, and H can easily be solved (in SI units)
 * $$ \mathbf{H} = \frac{\mathbf{B}}{\mu_0 (1+\chi_m)} \equiv \frac{\mathbf{B}}{\mu_0 \mu_r}, $$

with the relative magnetic permeability &mu;r = 1 + &chi;m.

For example, at standard temperature and pressure (STP) air, a mixture of paramagnetic oxygen and diamagnetic nitrogen,  is paramagnetic (i.e., has positive &chi;m), the &chi;m of air is 4&sdot;10&minus;7. Argon at STP is diamagnetic with &chi;m = &minus;1&sdot;10&minus;8. For most ferromagnetic materials &chi;m depends on H, with a non-linear relation between H and B and is large (depending on the material) from, say, 50 to 10000 and strongly varying as a function of H.

Both magnetic fields, H and B, are solenoidal (divergence-free, transverse) vector fields because of one of Maxwell's equations
 * $$ \boldsymbol{\nabla}\cdot\mathbf{H} = \boldsymbol{\nabla}\cdot\mathbf{B} = 0. $$

This equation denies the existence of magnetic monopoles (magnetic charges) and hence also of magnetic currents.