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Glossary of Terms

 

 

 

 

MAGNETIC FIELDS BASICS Glossary of Terms

 

Air gap

A low permeability gap in the flux path of a magnetic circuit. Often air, but inclusive of other materials such as paint, aluminum, etc.

 

Amplification (of a magnetic field)

The process by which fluid motions in a conducting fluid can make a weak magnetic field become stronger. On the Sun, stretching of the field lines of a magnetic field, coupled with field line preservation, will amplify the field.

 

Angstrom
A unit of length equal to 0.00000001 centimeters. This may also be written as 1 x 10-8 cm

 

Anisotropic magnet

A magnet having a preferred direction of magnetic orientation, so that the magnetic characteristics are optimum in one preferred direction

 

Aurora, polar (also known north of the equator as northern lights or aurora borealis ["northern dawn"], and south of it as aurora australis)

A glow seen in the sky, usually in the auroral zone, caused by electrons hitting atmospheric atoms and causing them to emit light. The typical aurora is produced at altitudes around 100 km (60 miles), by electrons of 3-15,000 electron volts. Most aurora is greenish, caused by light emitted from oxygen, or red, also from oxygen. Electrons producing auroral arcs seen from the ground have usually undergone acceleration in the magnetosphere by electric currents that connect Earth to space. Electrons observed by satellite imagers, often as rings around the auroral oval, are usually escaping from the Earth's magnetotail. Their glow is too dim to be seen by eye from the ground.

 

Closed circuit

This exists when the flux path external to a permanent magnet is confined within high permeability materials that compose the magnet circuit.

 

Coercive force, Hc

The demagnetizing force, measured in Oersteds, necessary to reduce observed induction, B, to zero after the magnet has previously been brought to saturation.

 

Curie temperature, Tc

The temperature at which the parallel alignment of elementary magnetic moments completely disappears, and the material is no longer able to hold magnetization.

declination (magnetic). The difference between magnetic north, given by the compass needle, and true north, the horizontal projection of the direction of the Earth axis.

demagnetization curve: The second quadrant of the hysteresis loop, generally describing the behavior of magnetic characteristics in actual use. Also known as the B-H Curve.

 

Dip angle

The local angle between the horizontal and the direction of the magnetic force. Indicated by a freely-floating magnetic needle, free to turn to any direction in space, or by a "dip circle" instrument, which has a needle pivoted around a horizontal axis aligned in the magnetic east-west direction.

 

Dipole

a compact source of magnetic force, with two magnetic poles. A bar magnet, coil or current loop, if their size is small, create a dipole field. The Earth's field, as a crude approximation, also resembles that of a dipole, located near the Earth's center.

 

Dynamo

Also known as "generator," a machine creating electric currents by relative motions between the conductors that carry them and magnets of electromagnets. In geomagnetism the term is also used for naturally occurring fluid flows through a magnetic field, generating electric currents. A self-excited dynamo (of either kind) is one in which the generated current creates the magnetic field by which the dynamo operates.

 

Dynamo process

The generation of magnetic field by motions of a fluid that conducts electricity, motions driven by some source of energy (e.g. heat convection).

 

Dynamo theory

The theory of fluid dynamos. Initially, "kinematic dynamo theory" asked whether dynamo processes were at all possible, and after some decades of study, the answer was "yes." "MHD (magneto-hydrodynamic) dynamo theory" searches for dynamos which also satisfy consistent pressure and force structures.

 

Dynamo, fluid

A dynamo process occurring in a fluid that conducts electricity.

 

Eddy currents

Circulating electrical currents that are induced in electrically conductive elements when exposed to changing magnetic fields, creating an opposing force to the magnetic flux. Eddy currents can be harnessed to perform useful work (such as damping of movement), or may be unwanted consequences of certain designs, which should be accounted for or minimized.

 

Electric charge

A property of electrons and ions, causing them to attract each other, and to repel particles of the same kind. The electric charge of electrons is called "negative" (-) and that of ions "positive" (+). Materials such as glass, fur and cloth acquire an electric charge by rubbing against each other, a process which tears electrons off one substance and attaches it to the other. Electric charges (+) and (-) may also be separated by a chemical process, as in an electric battery.

 

Electric current

a continuous flow of electric charge through a material which conducts electricity, carried by ions and/or electrons. Currents usually flow in a closed circuit, without beginning or end. In daily life a current is generally driven through wires by a voltage ("electric pressure") produced by batteries or generators. Some currents in space plasmas are also produced this way, but many are inherent to the way ions and electrons move through magnetic fields, e.g. their drifts.

 

Electricity

Colloquially, electric charge and currents, viewed as a "fluid" which may be attached to matter or flow through it. The word came from "elektron," the Greek name of amber, one of the materials which when dry and lightly rubbed can attract small objects (by "static electricity"). The Greeks and Romans already knew about such attractions, but William Gilbert, who studied them, called such materials "electricks," and from that came the modern term.

 

Electromagnet

A magnet, consisting of a solenoid with an iron core, which has a magnetic field existing only during the time of current flow through the coil.

 

Electromagnetic spectrum
The full range of frequencies, from radio waves to gamma rays, that characterizes light.

 

Electromagnetic waves (radiation)
Another term for light. Light waves are fluctuations of electric and magnetic fields in space.

 

Electron
A negatively charged particle commonly found in the outer layers of atoms. The electron has only 0.0005 the mass of the proton.

 

ELF

Extremely low frequency magnetic field

 

EMF

Electromagnetic field

 

Energy product

Indicates the energy that a magnetic material can supply to an external magnetic circuit when operating at any point on its demagnetization curve. Calculated as Bd x Hd, and measured in Mega Gauss Oersteds, MGOe.

 

Ferromagnetic

A material which like iron ("ferrum" in Latin) can become strongly magnetized, temporarily or permanently. William Gilbert named such materials "magneticks."

 

Ferromagnetic material

A material whose permeability is very much larger than 1 (from 60 to several thousand times 1), and which exhibits hysteresis phenomena.

 

Field

The region in which a particular type of force can be observed; depending on the force, one can thus speak of a gravity field, magnetic field, electric field (or when the two are linked by fast oscillations, electromagnetic field) and nuclear field. The laws of physics suggest that fields represent more than a possibility of force being observed, and that they can also transmit energy and momentum, e.g. a light wave is a phenomenon completely defined by fields. For that reason a field is often viewed as a space which was modified by the sources of the force which the field represents.

 

Field, electric

The region in which electric forces can be observed, e.g. near an electric charge.(see field).

 

Field, electromagnetic(EM field)

The regions of space near electric currents, magnets, broadcasting antennas etc., regions in which electric and magnetic forces may act (see field). Unchanging magnetic or electric phenomena can often be handled by just considering the magnetic or the electric field alone; however wave phenomena such as radio and light involve a tight interplay of time-varying electric and magnetic fields, viewed as manifestations of their electromagnetic fields.

 

Field line, closed

In magnetospheric physics, field lines which are not open, but have both ends attached to Earth. The field lines reaching most locations on Earth are closed and can trap charged particles.

 

Field line, open

In magnetospheric physics, a field line whose one end reaches Earth (specifically, the conducting ionosphere layer in the high atmosphere) but whose other end extends into the solar wind. Presumably, such lines have undergone magnetic reconnection. Because plasma and energy easily flow along magnetic field lines, these lines offer an easy pathway by which energy and plasma can flow from the solar wind to the Earth's magnetosphere.

 

Field line preservation

A predicted property of fluids which are perfect conductors of electricity (including "ideal plasmas"), fairly closely obeyed in much of the space environment. By this property, two particles which initially share the same field line, continue to do so into the future, even if the line is deformed. The opposite also holds for such fluids: two particles which start out on different field lines will always be on different field lines (but see magnetic reconnection).

 

Field lines, magnetic

Imaginary lines in space used for visually representing magnetic fields (just as lines of latitude and longitude are used to represent locations on Earth). At any point in space, the local field line points in the direction an ideal compass needle would assume, if it were free to rotate in 3 dimensions. It is also the direction of the magnetic force--the force which an isolated magnetic pole at that point would experience. In a plasma, magnetic field lines guide the motion of ions and electrons, are sometimes able to trap them and direct the flow of some electric currents.

 

Field, magnetic

The region where magnetic forces can be observed.

 

Flux

The condition existing in a medium subjected to a magnetizing force. This quantity is characterized by the fact that an electromotive force is induced in a conductor surrounding the flux at any time the flux changes in magnitude. The cgs unit of flux is the Maxwell.

 

Fluxmeter

An instrument that measures the change of flux linkage with a search coil.

 

Frequency
A property of a wave that describes how many wave patterns or cycles pass by in a period of time. Frequency is often measured in Hertz (Hz), where a wave with a frequency of 1 Hz will pass by at 1 cycle per second.

 

Fringing fields

Leakage flux particularly associated with edge effects in a magnetic circuit.

 

Gamma ray
The highest energy, shortest wavelength electromagnetic radiations. Usually, they are thought of as any photons having energies greater than about 100 keV. (It's "gamma-ray" when used as an adjective.)

 

Gauss

Lines of magnetic flux per square centimeter, cgs unit of flux density, equivalent to lines per square inch in the English system, and Webers per square meter or Tesla in the SI system.


Gaussmeter

An instrument that measures the instantaneous value of magnetic induction, B. Its principle of operation is usually based on one of the following: the Hall effect, nuclear magnetic resonance (NMR), or the rotating coil principle.

 

Hertz, Heinrich (1857 - 1894)

A German physics professor who did the first experiments with generating and receiving electromagnetic waves, in particular radio waves. In his honor, the units associated with measuring the cycles per second of the waves (or the number of times the tip-tops of the waves pass a fixed point in space in 1 second of time) is called the hertz.

 

Hertz; Hz

The derived SI unit of frequency, defined as a frequency of 1 cycle per second.

 

Hysteresis loop

A closed curve obtained for a material by plotting corresponding values of magnetic induction, B, (on the abscissa) against magnetizing force, H, (on the ordinate).

 

Induction, B

The magnetic flux per unit area of a section normal to the direction of flux. Measured in Gauss, in the cgs system of units.

 

Infrared
Electromagnetic radiation at wavelengths longer than the red end of visible light and shorter than microwaves (roughly between 1 and 100 microns). Almost none of the infrared portion of the electromagnetic spectrum can reach the surface of the Earth, although some portions can be observed by high-altitude aircraft (such as the Kuiper Observatory) or telescopes on high mountaintops (such as the peak of Mauna Kea in Hawaii).

 

Intrinsic coercive force, Hci

Measured in Oersteds in the cgs system, this is a measure of the materialيs inherent ability to resist demagnetization. It is the demagnetization force corresponding to zero intrinsic induction in the magnetic material after saturation. Practical consequences of high Hci values are seen in greater temperature stability for a given class of material, and greater stability in dynamic operating conditions.


Intrinsic induction, Bi

The contribution of the magnetic material to the total magnetic induction, B. It is the vector difference between the magnetic induction in the material and the magnetic induction that would exist in a vacuum under the same field strength, H. This relationship is expressed as: Bi = B-H.

 

Ions
An atom with one or more electrons stripped off, giving it a net positive charge.

 

Irreversible loss

Defined as the partial demagnetization of a magnet caused by external fields or other factors. These losses are only recoverable by re-magnetization. Magnets can be stabilized to prevent the variation of performance caused by irreversible losses.


Isotropic magnet

A magnet material whose magnetic properties are the same in any direction, and which can therefore be magnetized in any direction without loss of magnetic characteristics.


Keeper

A piece of soft iron that is placed on or between the poles of a magnet, decreasing the reluctance of the air gap and thereby reducing the flux leakage from the magnet.

 

Knee of the demagnetization curve

The point at which the B-H curve ceases to be linear. All magnet materials, even if their second quadrant curves are straight line at room temperature, develop a knee at some temperature. Alnico 5 exhibits a knee at room temperature. If the operating point of a magnet falls below the knee, small changes in H produce large changes in B, and the magnet will not be able to recover its original flux output without re-magnetization.

 

Laser
Laser is an acronym for Light Amplification by Stimulated Emission of Radiation. It's a device that produces a coherent beam of optical radiation by stimulating electronic, ionic, or molecular transitions to higher levels so that when they return to lower energy levels they emit energy.

 

Leakage flux

That portion of the magnetic flux that is lost through leakage in the magnetic circuit due to saturation or air-gaps, and is therefore unable to be used.


Length of air-gap, Lg

The length of the path of the central flux line in the air-gap.

 

Light
The common term for electromagnetic radiation, usually referring to that portion visible to the human eye. However, other bands of the e-m spectrum are also often referred to as different forms of light.

 

Line of force

Michael Faraday's original term for what is now known as magnetic field line.

 

Load line

A line drawn from the origin of the Demagnetization Curve with a slope of -B/H, the intersection of which with the B-H curve represents the operating point of the magnet. Also see Permeance Coefficient.

 

Lodestone (also spelled loadstone)

A rare mineral, found to have strong permanent magnetization. For many centuries, lodestones provided humanity with its only known source of magnetism. The mineral is a rare form of fine-grained magnetite and is believed to acquire its magnetic properties when struck by lightning.

 

Magnetic circuit

An assembly consisting of some or all of the following: permanent magnets, ferromagnetic conduction elements, air gaps, electrical currents.

 

Magnetic field
A description of the strength of the magnetic force exerted by an object. Bar magnets have "di-polar" fields, as the force is exerted from the two ends of the bar. In simple terms, the earth, the sun, stars, pulsars all have dipolar magnetic fields.

 

Magnetic flux

The total magnetic induction over a given area. When the magnetic induction, B, is uniformly distributed over an area A, Magnetic Flux = BA.

 

Magnetizing force, H

The magnetomotive force per unit length at any point in a magnetic circuit. Measured in Oersteds in the cgs system.


Magnetomotive force, F

Analogous to voltage in electrical circuits, this is the magnetic potential difference between any two points.

 

Magnetic induction

This term may refer to one of two phenomena, either induced magnetism or electromagnetic induction. The latter may be loosely defined as the ability of a substance that conducts electricity to develop a circulating current, if it senses a changing magnetic field. The change might come either from of variation of the strength of the magnetic source, or from the motion of the conductor relative to that source. The dynamo process is based on such currents.

 

Magnetic pole

(1)A magnetic pole of a bar magnet is a compact source of magnetic force near the end of the bar. Magnetic poles always come in matched pairs, north-seeking (N) and south-seeking (S). Magnetic poles are just an observed consequence of the way magnetic field lines are channeled by the bar: actually, the bar's magnetization is evenly spread inside it and is not concentrated at its ends. (2) The magnetic pole of Earth is one of the two points on Earth towards which the compass needle seems to point. At the pole, the magnetic force is vertical. The magnetic poles of Earth are near the geographic poles, the points where the Earth's surface intersects its rotation axis; however the two are not the same, and on Uranus and Neptune are quite widely separated.

 

Magnetic (scalar) potential

The magnetic force at a point in space is a "vector" quantity, one which has both direction and strength. To specify it, three numbers are required--for instance, one specifying its strength and two its direction. However, the magnetic field near the surface of the Earth (and at any other location where electric currents are absent) is of a relatively simple kind, describable by a single varying quantity--an ordinary number or "scalar", as distinct from a vector. A similar simplified representation exists for the force of gravity, even when its sources are complicated. The magnetic scalar potential was introduced for describing the Earth's magnetic field by Gauss and is described in terms of "spherical harmonics." It is still being used.

 

Magnetization, induced

The magnetization of iron and similar "ferromagnetic" materials, when placed near a magnet or lodestone. In magnetically "soft" materials this magnetization is only temporary.

 

Magnetize

Cause to become magnetic. This can happen by placing the material in the strong magnetic field produced by a permanent magnet or by an electric current, or when heated material which can become magnetic (e.g. iron or basaltic lava) cools down in the presence of a magnetic field.

 

Magnetometer

An instrument for measuring the direction and/or intensity of magnetic fields. Spacecraft often carry fluxgate magnetometers, which measure components of the magnetic field (3 of them are combined to provide all three, giving both strength and direction of the field) but they need to be calibrated. Instruments using rubidium vapor measure only the field strength, but their reading is absolute, related to atomic constants.

 

Magnetometer, fluxgate

An electronic magnetometer based on the saturation of certain magnetizable materials. Can be made very sensitive.

 

Magnetometer, proton precession

An electronic magnetometer based on the resonance between protons (hydrogen nuclei) and an oscillating electromagnetic signal. Protons are small magnets, and the magnetic strength of each (like the proton's mass) always has the same value, which is well known. Because of this, the resonance frequency has a simple relation to the strength of the magnetic field. By measuring that frequency, the magnetic field strength can be immediately calculated, and no calibration of the instrument is needed.

 

Magnetometer, Overhauser effect

A greatly improved version of the proton precession magnetometer (preceding item), using an added chemical to enhance performance.

 

Magnetometer, alkali vapor

A magnetometer which, like the proton precession type, is based on an atomic resonance process and therefore requires no calibration. A glass chamber containing the vapor of an alkali metal (e.g. rubidium or caesium) becomes slightly more opaque to a specific light frequency when exposed to a radio signal of resonant frequency. That frequency gives the strength of the surrounding magnetic field.

 

Magnetopause

The boundary of the magnetosphere, separating plasma attached to Earth from that of the flowing solar wind.

 

Magnetosphere
The region of space in which the magnetic field of an object (e.g., a star or planet) dominates the radiation pressure of the stellar wind to which it is exposed.

 

Magnetotail
The portion of a planetary magnetosphere which is pushed in the direction of the solar wind.

 

Main field (of Earth)

A term frequently used by scientists for the internal magnetic field of the Earth, in distinction from fields originating outside its surface.

 

Maximum energy product, BHmax

The point on the Demagnetization Curve where the product of B and H is a maximum and the required volume of magnet material required to project a given energy into its surroundings is a minimum. Measured in Mega Gauss Oersteds, MGOe.

 

Meter; m
The fundamental SI unit of length, defined as the length of the path traveled by light in vacuum during a period of 1/299 792 458 s. A unit of length equal to about 39 inches. A kilometer is equal to 1000 meters.

 

MF

Magnetic field

 

Microwave
Electromagnetic radiation which has a longer wavelength (between 1 mm and 30 cm) than visible light. Microwaves can be used to study the Universe, communicate with satellites in Earth orbit, and cook popcorn.

 

MHD

Short for "magneto-hydrodynamics, " the theory of fluids which conduct electricity. MHD is applicable to the Earth's fluid core and also to many plasmas.

 

MHD dynamo theory

The theory of dynamo action in conducting fluids, including force balance and other physical effects.

 

MRI

Magnetic resonance imaging

 

Noise
The random fluctuations that are always associated with a measurement that is repeated many times over.

 

North pole

That pole of a magnet which, when freely suspended, would point to the north magnetic pole of the earth. The definition of polarity can be a confusing issue, and it is often best to clarify by using "north seeking pole" instead of "north pole" in specifications.

 

North seeking pole

The pole of a bar magnet which, if the magnet is freely suspended (or is placed on a "boat" floating on water) tends to point northward. Also known as the "north pole" (or "N pole") of the bar magnet. However, it should be noted that if a bar magnet at the center of the Earth were the source of the Earth's field, the N-pole of that bar would be directed southward, because it tends to repel another N-pole, not attract it.

 

Oersted, Oe

A cgs unit of measure used to describe magnetizing force. The English system equivalent is Ampere Turns per Inch, and the SI systemيs is Ampere Turns per Meter.


Orientation direction

The direction in which an anisotropic magnet should be magnetized in order to achieve optimum magnetic properties. Also known as the "axis", "easy axis", or "angle of inclination".

 

Paramagnetic material

A material having a permeability slightly greater than 1.

 

PEMF

Pulsed electromagnetic field


permeance

The inverse of reluctance, analogous to conductance in electrical circuits.


Permeance coefficient, Pc

Ratio of the magnetic induction, Bd, to its self demagnetizing force, Hd. Pc = Bd / Hd. This is also known as the "load line", "slope of the operating line", or operating point of the magnet, and is useful in estimating the flux output of the magnet in various conditions. As a first order approximation, Bd / Hd = Lm/Lg, where Lm is the length of the magnet, and Lg is the length of an air gap that the magnet is subjected to. Pc is therefore a function of the geometry of the magnetic circuit.

 

Photon
The smallest (quantum) unit of light/electromagnetic energy. Photons are generally regarded as particles with zero mass and no electric charge.

 

Plasma

A gas containing free ions and electrons, and therefore capable of conducting electric currents. A "partially ionized plasma" such as the Earth's ionosphere or the gas inside a fluorescent lamp is one that also contains neutral atoms.

 

Plasma sheet

The region in the magnetotail of relatively denser plasma and rather weak magnetic field, stretching tailwards from the Earth's magnetic equator. It separates the two tail lobes and is the site of substorms and the source region of most of the polar aurora.

 

Polarization
A special property of light; light has three properties, brightness, color and polarization. Polarization is a condition in which the planes of vibration of the various rays in a light beam are at least partially aligned.

 

Pole pieces

Ferromagnetic materials placed on magnetic poles used to shape and alter the effect of lines of flux.

 

Positron
The antiparticle to the electron. The positron has most of the same characteristics as an electron except it is positively charged.

 

Proton
A particle with a positive charge commonly found in the nucleus of atoms.

 

Radiation belt
Regions of charged particles in a magnetosphere.

 

Radio
Electromagnetic radiation which has the lowest frequency, the longest wavelength, and is produced by charged particles moving back and forth; the atmosphere of the Earth is transparent to radio waves with wavelengths from a few millimeters to about twenty meters.

 

Relative permeability

The ratio of permeability of a medium to that of a vacuum. In the cgs system, the permeability is equal to 1 in a vacuum by definition. The permeability of air is also for all practical purposes equal to 1 in the cgs system.

 

Reluctance, R

Analogous to resistance in an electrical circuit, reluctance is related to the magnetomotive force, F, and the magnetic flux by the equation R = F/(Magnetic Flux), paralleling Ohm's Law where F is the magnetomotive force (in cgs units).


Remanence, Bd

The magnetic induction that remains in a magnetic circuit after the removal of an applied magnetizing force. If there is an air gap in the circuit, the remanence will be less than the residual induction, Br.


Residual induction, Br

This is the point at which the hysteresis loop crosses the B axis at zero magnetizing force, and represents the maximum flux output from the given magnet material. By definition, this point occurs at zero air gap, and therefore cannot be seen in practical use of magnet materials.


Return path

Conduction elements in a magnetic circuit which provide a low reluctance path for the magnetic flux.

 

Reversals, magnetic

Episodes of changes in the Earth's magnetic field which result in the polarity of the north and south magnetic poles being interchanged. Reversals have occurred in the geological history of the Earth at typical intervals of 500,000 years. The Sun's global magnetic polarity seems to reverse every 11-year sunspot cycle.

 

Reversible temperature coefficient

A measure of the reversible changes in flux caused by temperature variations.

 

Saturation

The condition under which all elementary magnetic moments have become oriented in one direction. A ferromagnetic material is saturated when an increase in the applied magnetizing force produces no increase in induction. Saturation flux densities for steels are in the range of 16,000 to 20,000 Gauss.

 

Scientific notation
A compact format for writing very large or very small numbers, most often used in scientific fields. The notation separates a number into two parts: a decimal fraction, usually between 1 and 10, and a power of ten. Thus 1.23 x 104 means 1.23 times 10 to the fourth power or 12,300; 5.67 x 10-8 means 5.67 divided by 10 to the eighth power or 0.0000000567.

 

Search coil

A coil conductor, usually of known area and number of turns that is used with a fluxmeter to measure the change of flux linkage with the coil.


SMF

Static magnetic field

 

Soft materials (magnetically)

Materials such as soft iron which become temporary magnets when placed near permanent magnets or electric currents, but lose their magnetization when taken away again.

 

South seeking pole

The magnetic pole (for example, on a bar magnet) which, when freely suspended in space, tends to point south. See north-seeking pole.

 

Stabilization

Exposure of a magnet to demagnetizing influences expected to be encountered in use in order to prevent irreversible losses during actual operation. Demagnetizing influences can be caused by high or low temperatures, or by external magnetic fields.

 

Synchrotron radiation
Electromagnetic radiation given off when very high energy electrons encounter magnetic fields.

 

TMF

Time-varied magnetic field

 

Toroidal field

One of two modes of magnetic fields (particularly in spherical configurations), the other being the poloidal field. A typical toroidal field is the one created by a current in a long straight wire, with ring-shaped ("torus shaped") field lines around the wire. A general magnetic field has a toroidal part and a poloidal part. On the Sun, the uneven solar rotation (faster near the equator) amplifies only the toroidal part, though the poloidal field is essential to the process.

 

TVF

Time-varied magnetic field

 

Temperature coefficient

A factor, which describes the change in a magnetic property with change in temperature. Expressed as percent change per unit of temperature.

 

Ultraviolet
Electromagnetic radiation at wavelengths shorter than the violet end of visible light; the atmosphere of the Earth effectively blocks the transmission of most ultraviolet light.

 

Visible
Electromagnetic radiation at wavelengths which the human eye can see. We perceive this radiation as colors ranging from red (longer wavelengths; ~ 700 nanometers) to violet (shorter wavelengths; ~400 nanometers.)

 

Wave-particle duality
The principle of quantum mechanics which implies that light (and, indeed, all other subatomic particles) sometimes act like a wave, and sometimes act like a particle, depending on the experiment you are performing. For instance, low frequency electromagnetic radiation tends to act more like a wave than a particle; high frequency electromagnetic radiation tends to act more like a particle than a wave.

 

Wavelength
The distance between adjacent peaks in a series of periodic waves. Also see electromagnetic spectrum.

 

Weber

The practical unit of magnetic flux. It is the amount of magnetic flux which, when linked at a uniform rate with a single-turn electric circuit during an interval of 1 second, will induce in this circuit an electromotive force of 1 volt.

 

X-ray
Electromagnetic radiation of very short wavelength and very high-energy; X-rays have shorter wavelengths than ultraviolet light but longer wavelengths than gamma rays.

 

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