Tesla (unit)


The tesla is the unit of magnetic flux density in the International System of Units.
One tesla is equal to one weber per square metre. The unit was announced during the General Conference on Weights and Measures in 1960 and is named in honour of Serbian-American electrical and mechanical engineer Nikola Tesla, upon the proposal of the Slovenian electrical engineer France Avčin.

Definition

A particle, carrying a charge of one coulomb, and moving perpendicularly through a magnetic field of one tesla, at a speed of one metre per second, experiences a force with magnitude one newton, according to the Lorentz force law. That is,
As an SI derived unit, the tesla can also be expressed in terms of other units. For example, a magnetic flux of 1 weber through a surface of one square meter is equal to a magnetic flux density of 1 tesla. That is,
Expressed only in SI base units, 1 tesla is:
where A is ampere, kg is kilogram, and s is second.
Additional equivalences result from the derivation of coulombs from amperes, :
the relationship between newtons and joules, :
and the derivation of the weber from volts, :

Electric vs. magnetic field

In the production of the Lorentz force, the difference between electric fields and magnetic fields is that a force from a magnetic field on a charged particle is generally due to the charged particle's movement, while the force imparted by an electric field on a charged particle is not due to the charged particle's movement. This may be appreciated by looking at the units for each. The unit of electric field in the MKS system of units is newtons per coulomb, N/C, while the magnetic field can be written as N/. The dividing factor between the two types of field is metres per second, which is velocity. This relationship immediately highlights the fact that whether a static electromagnetic field is seen as purely magnetic, or purely electric, or some combination of these, is dependent upon one's reference frame.
In ferromagnets, the movement creating the magnetic field is the electron spin. In a current-carrying wire the movement is due to electrons moving through the wire.

Conversion to non-SI units

One tesla is equivalent to:
For the relation to the units of the magnetising field, see the article on permeability.

Multiples

Examples

The following examples are listed in the ascending order of the magnetic-field strength.
  • – strength of Earth's magnetic field at 0° latitude, 0° longitude
  • – walking under a high-voltage power line
  • – the strength of a typical refrigerator magnet
  • 0.3 T – the strength of solar sunspots
  • 1 T to 2.4 T – coil gap of a typical loudspeaker magnet
  • 1.5 T to 3 T – strength of medical magnetic resonance imaging systems in practice, experimentally up to 17 T
  • 4 T – strength of the superconducting magnet built around the CMS detector at CERN
  • 5.16 T – the strength of a specially designed room temperature Halbach array
  • 8 T – the strength of LHC magnets
  • 11.75 T – the strength of INUMAC magnets, largest MRI scanner
  • 13 T – strength of the superconducting ITER magnet system
  • 14.5 T – highest magnetic field strength ever recorded for an accelerator steering magnet at Fermilab
  • 16 T – magnetic field strength required to levitate a frog according to the 2000 Ig Nobel Prize in Physics
  • 17.6 T – strongest field trapped in a superconductor in a lab as of July 2014
  • 20 T – strength of the large scale high temperature superconducting magnet developed by MIT and Commonwealth Fusion Systems to be used in fusion reactors
  • 27 T – maximal field strengths of superconducting electromagnets at cryogenic temperatures
  • 35.4 T – the current world record for a superconducting electromagnet in a background magnetic field
  • 45 T – the current world record for continuous field magnets
  • 97.4 T – strongest magnetic field produced by a "non-destructive" magnet
  • 100 T – approximate magnetic field strength of a typical white dwarf star
  • 1200 T – the field, lasting for about 100 microseconds, formed using the electromagnetic flux-compression technique
  • 109 T – Schwinger limit above which the electromagnetic field itself is expected to become nonlinear
  • 108 – 1011 T – magnetic strength range of magnetar neutron stars