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or **palaeomagnetism** or **remanent magnetism**

Permanent magnetism in rocks, resulting from the orientation of the Earth's magnetic field at the time of rock formation in a past geologic age. It is a source of information for the paleomagnetic studies of polar wandering and plate tectonics.

Learn more about paleomagnetism with a free trial on Britannica.com.

Encyclopedia Britannica, 2008. Encyclopedia Britannica Online.

Magnetization is defined as the quantity of magnetic moment per unit volume. The origin of the magnetic moments responsible for magnetization can be either microscopic electric currents resulting from the motion of electrons in atoms, or the spin of the electrons. Net magnetization results from the response of a material to an external magnetic field, together with any unbalanced magnetic dipole moments that may be inherent in the material itself, for example, in ferromagnets. Magnetization is not always homogeneous within a body, but rather a function of position.
## Magnetization in Maxwell's equations

#### Relations between B, H and M

#### Magnetization current

#### Magnetostatics

## Types of magnetism

### Diamagnetism

### Paramagnetism

### Superparamagnetism

Superparamagnetic materials are paramagnetic materials whose magnetization saturates at very large fields. They are obtained using magnetic nanoparticle aggregates with large net magnetic moments. Each particle is a single magnetic domain. Consequently, the alignment of spins under applied field is no longer impeded by domain walls. Above the blocking temperature, thermal vibrations randomly fluctuate the net spins, cancelling one another and the net moment of the collective particles is zero at zero field (no coercive field). If a magnetic field is applied, the particles will align producing a net moment. This behavior is characteristic of paramagnetic materials, but the difference is that each nanoparticle has a large net moment, so the saturation of magnetization occurs at very large fields of several teslas.
### Ferromagnetism

## See also

## Sources

The behavior of magnetic fields ($mathbf\{B\}$, $mathbf\{H\}$), electric fields ($mathbf\{E\}$, $mathbf\{D\}$), charge density ($rho,$), and current density ($mathbf\{J\}$) is described by Maxwell's equations. The role of the magnetization is described below.

The magnetization defines the auxiliary magnetic field $mathbf\{H\}$ as

- $mathbf\{B\}\; =\; mu\_0mathbf\{(H\; +\; M)\}$

which is convenient for various calculations.

A relation between $mathbf\{M\}$ and $mathbf\{H\}$ exists in many materials. In diamagnets and paramagnets, the relation is usually linear:

- $mathbf\{M\}\; =\; chi\_mmathbf\{H\}$

where $chi\_m,$ is called the volume magnetic susceptibility.

In ferromagnets there is no one-to-one correspondence between $mathbf\{M\}$ and $mathbf\{H\}$ because of hysteresis.

The magnetization $mathbf\{M\}$ makes a contribution to the current density $mathbf\{J\}$, known as the magnetization current or bound current:

- $mathbf\{J\_m\}\; =\; nablatimesmathbf\{M\}$

so that the total current density that enters Maxwell's equations is given by

- $mathbf\{J\}\; =\; mathbf\{J\_f\}\; +\; nablatimesmathbf\{M\}\; +\; frac\{partialmathbf\{P\}\}\{partial\; t\}$

where $mathbf\{J\_f\}$ is the electric current density of free charges (also called the free current), the second term is the contribution from the magnetization, and the last term is related to the electric polarization $mathbf\{P\}$.

In the absence of free electric currents and time-dependent effects, Maxwell's equations describing the magnetic quantities reduce to

- $mathbf\{nablacdot\; H\}\; =\; -\; nablacdotmathbf\{M\}\; qquad\; mathbf\{nablatimes\; H\}\; =\; 0$

These equations can be easily solved in analogy with electrostatic problems where

- $mathbf\{nablacdot\; E\}\; =\; frac\{rho\}epsilon\_0\; qquad\; qquad\; qquad\; mathbf\{nablatimes\; E\}\; =\; 0$

In this sense $-epsilon\_0nablacdotmathbf\{M\}$ plays the role of a "magnetic charge density" analogous to the electric charge density $rho,$.

Magnetization is volume density of magnetic moment. That is: if a certain volume has magnetization $mathbf\{M\}$ then volume element $dV$ has magnetic moment of $d\; mathbf\{m\}\; =\; mathbf\{M\}\; dV$.

This is the most common magnetic behavior. The diamagnetic magnetization is proportional and opposing to the applied magnetic field. All materials present a diamagnetic response, although it may be shadowed by stronger magnetic behaviors. Diamagnetism can be explained by the normal response of the orbiting electrons considering Lenz's law. This is a weak form of magnetism that is non permanent and persists only while external field is applied. The magnitude of induced magnetic moment is very small and in a direction opposite to that of applied field. Therefore, relative permeability is less than 1 and magnetic susceptibility is negative. When placed between the poles of a strong electromagnet, diamagnetic materials are pushed out towards the region where the field is weaker.

Paramagnetic materials present a magnetization that is proportional to the applied field and reinforces it. This arises from the existence of magnetic dipoles in the material. Paramagnetism varies inversely with temperature and is characterized by the material's saturation magnetization. When placed between the poles of a strong electromagnet, paramagnetic materials are pulled towards the region where the field is stronger.

Ferromagnetic materials present a magnetization much larger than other materials. Ferromagnetism arises from the strong coupling between the neighboring magnetic dipoles in the material. Ferromagnetic materials can present spontaneous magnetization, and this gives rise to the hysteresis loops. Ferromagnetic materials can be characterized by their permeability, Curie temperature (temperature of the phase change to paramagnetic behavior), coercive field (field strength needed to demagnetize the material), and remnant magnetization (magnetization at zero external field).

- Permeability (electromagnetism)
- Magnetic susceptibility
- Earth's magnetic field
- Geomagnetic reversal
- Geomagnetic excursion

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Last updated on Monday October 06, 2008 at 10:26:26 PDT (GMT -0700)

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This article is licensed under the GNU Free Documentation License.

Last updated on Monday October 06, 2008 at 10:26:26 PDT (GMT -0700)

View this article at Wikipedia.org - Edit this article at Wikipedia.org - Donate to the Wikimedia Foundation

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