Everything about Electromagnetic Energy totally explained
Electromagnetic (EM) radiation is a
self-propagating wave in space which is the phenomenon
sensed by the human eye as
light. EM radiation has an
electric and
magnetic field component which
oscillate in phase perpendicular to each other and to the direction of energy
propagation. Electromagnetic radiation is classified into types according to the
frequency of the wave, these types include (in order of increasing frequency):
radio waves,
microwaves,
terahertz radiation,
infrared radiation,
visible light,
ultraviolet radiation,
X-rays and
gamma rays. Of these, radio waves have the longest wavelengths and Gamma rays have the shortest.
EM radiation carries
energy and
momentum, which may be imparted when it interacts with
matter.
Physics
Theory
Electromagnetic waves were first postulated by
James Clerk Maxwell and subsequently confirmed by
Heinrich Hertz. Maxwell derived a
wave form of the electric and magnetic equations, revealing the wave-like nature of electric and magnetic fields, and their symmetry. Because the speed of EM waves predicted by the wave equation coincided with the measured
speed of light, Maxwell concluded that
light itself is an EM wave.
According to
Maxwell's equations, a time-varying
electric field generates a
magnetic field and
vice versa. Therefore, as an oscillating electric field generates an oscillating magnetic field, the magnetic field in turn generates an oscillating electric field, and so on. These oscillating fields together form an electromagnetic wave.
A
quantum theory of the interaction between electromagnetic radiation and matter such as electrons is described by the theory of
quantum electrodynamics.
Properties
Electric and magnetic fields obey the properties of
superposition, so fields due to particular particles or time-varying electric or magnetic fields contribute to the fields due to other causes. (As these fields are vector fields, all magnetic and electric field vectors add together according to
vector addition.) These properties cause various phenomena including
refraction and
diffraction. For instance, a travelling EM wave incident on an atomic structure induces oscillation in the
atoms, thereby causing them to emit their own EM waves. These
emissions then alter the impinging wave through interference.
Since light is an oscillation, it isn't affected by travelling through static electric or magnetic fields in a linear medium such as a vacuum. In nonlinear media such as some
crystals, however, interactions can occur between light and static electric and magnetic fields - these interactions include the
Faraday effect and the
Kerr effect.
In refraction, a wave crossing from one medium to another of different
density alters its speed and direction upon entering the new medium. The ratio of the refractive indices of the media determines the degree of refraction, and is summarized by
Snell's law. Light disperses into a visible
spectrum as light is shone through a prism because of refraction.
The
physics of electromagnetic radiation is
electrodynamics, a subfield of
electromagnetism.
EM radiation exhibits both wave properties and
particle properties at the same time (see
wave-particle duality). The wave characteristics are more apparent when EM radiation is measured over relatively large timescales and over large distances, and the particle characteristics are more evident when measuring small distances and timescales. Both characteristics have been confirmed in a large number of experiments.
There are experiments in which the wave and particle natures of electromagnetic waves appear in the same experiment, such as the diffraction of a single
photon. When a single photon is sent through two slits, it passes through both of them interfering with itself, as waves do, yet is detected by a
photomultiplier or other sensitive detector only once. Similar self-interference is observed when a single photon is sent into a
Michelson interferometer or other
interferometers.
Wave model
An important aspect of the nature of light is
frequency. The frequency of a wave is its rate of oscillation and is measured in
hertz, the
SI unit of frequency, where one hertz is equal to one oscillation per
second. Light usually has a spectrum of frequencies which sum together to form the resultant wave. Different frequencies undergo different angles of refraction.
A wave consists of successive troughs and crests, and the distance between two adjacent crests or troughs is called the
wavelength. Waves of the electromagnetic spectrum vary in size, from very long radio waves the size of buildings to very short gamma rays smaller than atom nuclei. Frequency is inversely proportional to wavelength, according to the equation:
»
where
v is the speed of the wave (
c in a vacuum, or less in other media),
f is the frequency and λ is the wavelength. As waves cross boundaries between different media, their speeds change but their frequencies remain constant.
Interference is the superposition of two or more waves resulting in a new wave pattern. If the fields have components in the same direction, they constructively interfere, while opposite directions cause destructive interference.
The energy in electromagnetic waves is sometimes called
radiant energy.
Particle model
Because energy of an EM wave is quantized, in the particle model of EM radiation, a wave consists of discrete packets of energy, or
quanta, called
photons. The frequency of the wave is proportional to the magnitude of the particle's energy. Moreover, because photons are emitted and absorbed by charged particles, they act as transporters of
energy. The energy per
photon can be calculated by
Planck's equation:
»
where
E is the energy,
h is
Planck's constant, and
f is frequency.
This photon-energy expression
is a particular case of the energy levels of the more general
electromagnetic oscillator
whose average energy, which is used to obtain Planck's radiation law,
can be shown to differ sharply from that predicted by the
equipartition principle
at low temperature, thereby establishes a failure
of equipartition due to quantum effects at low temperature.
As a photon is absorbed by an
atom, it excites an
electron, elevating it to a higher
energy level. If the energy is great enough, so that the electron jumps to a high enough energy level, it may escape the positive pull of the nucleus and be liberated from the atom in a process called
photoionisation. Conversely, an electron that descends to a lower energy level in an atom emits a photon of light equal to the energy difference. Since the energy levels of electrons in atoms are discrete, each element emits and absorbs its own characteristic frequencies.
Together, these effects explain the absorption spectra of
light. The dark bands in the spectrum are due to the atoms in the intervening medium absorbing different frequencies of the light. The composition of the medium through which the light travels determines the nature of the absorption spectrum. For instance, dark bands in the light emitted by a distant star are due to the atoms in the star's atmosphere. These bands correspond to the allowed energy levels in the atoms. A similar phenomenon occurs for
emission. As the electrons descend to lower energy levels, a spectrum is emitted that represents the jumps between the energy levels of the electrons. This is manifested in the
emission spectrum of
nebulae. Today, scientists use this phenomenon to observe what elements a certain star is composed of. It is also used in the determination of the distance of a star, using the so-called
red shift.
Speed of propagation
Any electric charge which accelerates, or any changing magnetic field, produces electromagnetic radiation. Electromagnetic information about the charge travels at the speed of light. Accurate treatment thus incorporates a concept known as
retarded time (as opposed to advanced time, which is unphysical in light of
causality), which adds to the expressions for the electrodynamic
electric field and
magnetic field. These extra terms are responsible for electromagnetic radiation. When any wire (or other conducting object such as an
antenna) conducts
alternating current, electromagnetic radiation is propagated at the same frequency as the electric current. Depending on the circumstances, it may behave as a
wave or as
particles. As a wave, it's characterized by a velocity (the
speed of light),
wavelength, and
frequency. When considered as particles, they're known as
photons, and each has an energy related to the frequency of the wave given by
Planck's relation
E = hν, where
E is the energy of the photon,
h = 6.626 × 10
-34 J·s is
Planck's constant, and
ν is the frequency of the wave.
One rule is always obeyed regardless of the circumstances: EM radiation in a vacuum always travels at the
speed of light,
relative to the observer, regardless of the observer's velocity. (This observation led to
Albert Einstein's development of the theory of
special relativity.)
In a medium (other than vacuum),
velocity of propagation or
refractive index are considered, depending on frequency and application. Both of these are ratios of the speed in a medium to speed in a vacuum.
Electromagnetic spectrum
Generally, EM radiation is classified by wavelength into
electrical energy,
radio,
microwave,
infrared, the
visible region we perceive as light,
ultraviolet,
X-rays and
gamma rays.
The behavior of EM radiation depends on its wavelength. Higher frequencies have shorter wavelengths, and lower frequencies have longer wavelengths. When EM radiation interacts with single atoms and molecules, its behavior depends on the amount of energy per quantum it carries. Electromagnetic radiation can be divided into
octaves — as sound waves are — winding up with eighty-one octaves.
Spectroscopy can detect a much wider region of the EM spectrum than the visible range of 400 nm to 700 nm. A common laboratory spectroscope can detect wavelengths from 2 nm to 2500 nm. Detailed information about the physical properties of objects, gases, or even stars can be obtained from this type of device. It is widely used in
astrophysics. For example,
hydrogen atoms
emit radio waves of
wavelength 21.12
cm.
Light
EM radiation with a
wavelength between approximately 400
nm and 700 nm is detected by the
human eye and perceived as visible
light. Other wavelengths, especially nearby infrared (longer than 700 nm) and ultraviolet (shorter than 400 nm) are also sometimes referred to as light, especially when the visibility to humans isn't relevant.
If radiation having a frequency in the visible region of the EM spectrum reflects off of an object, say, a bowl of fruit, and then strikes our eyes, this results in our
visual perception of the scene. Our brain's visual system processes the multitude of reflected frequencies into different shades and hues, and through this not-entirely-understood psychophysical phenomenon, most people perceive a bowl of fruit.
At most wavelengths, however, the information carried by electromagnetic radiation isn't directly detected by human senses. Natural sources produce EM radiation across the spectrum, and our technology can also manipulate a broad range of wavelengths.
Optical fiber transmits light which, although not suitable for direct viewing, can carry data that can be translated into sound or an image. The coding used in such data is similar to that used with radio waves.
Radio waves
Radio waves can be made to carry information by varying a combination of the amplitude, frequency and phase of the wave within a frequency band.
When EM radiation impinges upon a
conductor, it couples to the conductor, travels along it, and
induces an electric current on the surface of that conductor by exciting the electrons of the conducting material. This effect (the
skin effect) is used in antennas. EM radiation may also cause certain molecules to absorb energy and thus to heat up; this is exploited in
microwave ovens.
Derivation
Electromagnetic waves as a general phenomenon were predicted by the classical laws of
electricity and magnetism, known as
Maxwell's equations. If you inspect Maxwell's equations without sources (charges or currents) then you'll find that, along with the possibility of nothing happening, the theory will also admit nontrivial solutions of changing electric and magnetic fields. Beginning with Maxwell's equations for
free space:
» :
.
From the viewpoint of an electromagnetic wave traveling forward, the electric field might be oscillating up and down, while the magnetic field oscillates right and left; but this picture can be rotated with the electric field oscillating right and left and the magnetic field oscillating down and up. This is a different solution that's traveling in the same direction. This arbitrariness in the orientation with respect to propagation direction is known as
polarization.
Further Information
Get more info on 'Electromagnetic Energy'.
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