Electromagnetic wave

In physics, an electromagnetic wave is a change, periodic in space and time, of an electric field E(r,t) and a magnetic field B(r,t). A stream of electromagnetic waves is referred to as electromagnetic radiation. Because an electric as well as a magnetic field is involved, the term electromagnetic is used, a contamination of electric and magnetic. Examples of electromagnetic waves, in increasing wavelength, are: gamma rays, X-rays, ultraviolet light, visible light, infrared, microwaves, and radio waves. All these waves propagate in vacuum with the same speed c, the speed of light. With regard to propagation of electromagnetic waves, air at standard temperature and pressure is very close to vacuum (its refractive index n = 1.0002926, meaning that the speed of light in air is c/n ≈ c).

Electromagnetic waves were predicted on theoretical grounds by James Clerk Maxwell in 1861 and first emitted and received in the laboratory by Heinrich Hertz a quarter century later. The first to see the applicability for communication purposes was the inventor of radiotelegraphy Guglielmo Marconi (around 1900). Later applications are radio, television, radar, cellular phones, gps, and all kinds of wireless applications, from remote control of television sets to internet access in public places.

Fig. 1. Electromagnetic wave. Electric component (red) in plane of drawing; magnetic component (blue) in orthogonal plane. Wave propagates to the right. The wavelength is λ.

Properties

In figure 1 we see a snapshot (i.e., a picture at a certain point in time) of the magnetic and electric fields in adjacent points of space. In each point, the vector E is perpendicular to the vector B. The wave propagates to the right, along an axis which we conveniently refer to as y-axis. Both E and B are perpendicular to the propagation direction, which is expressed by stating that an electromagnetic wave is a transverse wave, in contrast to sound waves, which are longitudinal waves (i.e., air molecules vibrate parallel to the propagation direction of the sound).

Assume that the snapshot in figure 1 is taken at time t, then at a certain point y we see an arrow of certain length representing E(y,t) and also a vector B(y,t). At a point in time Δt later, the same values of E and B (same arrows) are seen at y + c Δt. The arrows seem to have propagated to the right with a speed c.

The time t is fixed and the position y varies in figure 1. Conversely, we can keep the position fixed and imagine what happens if time changes. Focus on a fixed point y, then in progressing time the two vectors E(y,t) and B(y,t) in the point y, grow to a maximum value, then shrink to zero, become negative, go to a minimum value, and grow again, passing through zero, they grow to the same maximum value again. This cycle is repeated indefinitely. When we now plot E and B in the fixed point y as a function of time t, we see the same type (sine-type) function as in figure 1. The number of times per second that the vectors go through a full cycle is the frequency of the electromagnetic wave.

Periodicity in space means that the electromagnetic (EM) wave is repeated after a certain distance. This distance, the wavelength is traditionally designated by λ, see figure 1. If we go at a fixed time a distance λ to the right or to the left we encounter the very same fields E and B.

Basically, the only property distinguishing different kinds of EM waves, is their wavelength, see figure 2. Note the enormous span in wavelengths, from one trillionth of a millimeter for gamma-rays (radioactive rays) up to the VLF (very low frequency) radio waves of about 100 kilometer.

Frequency of electromagnetic waves

Often EM waves are characterized by their frequency (the number of cycles per unit time), instead of by their wavelength. If the EM field goes through ν full cycles in a second, where ν is a positive integral number, we say that the field has a frequency of ν Hz (hertz). The speed of propagation of the EM waves being c, in 1/ν seconds the wave propagates a distance c×(1/ν) meter (according to the formula: distance covered is speed times traveling time). The distance covered in 1/ν seconds is the wavelength λ:

Fig. 2. Schematic overview of the electromagnetic spectrum. Vertical axis: wavelengths in meter. Examples: infrared extends from 8 ·10⁻⁷ to 10⁻³ m; radio from 10⁻⁴ to about 10⁴ m.

$\lambda ={\frac {c}{\nu }}\quad \Longrightarrow \quad \nu ={\frac {c}{\lambda }}$

If we express c in m/s then λ is obtained in m. To convert quickly from wavelength to frequency we can approximate c by 3·10⁸ m/s.

The wavelengths of the various parts of the EM spectrum are very different in magnitude, the sources of the radiations, the interactions with matter, and the detectors employed differ widely, too, and, so it is not surprising that in the past different parts of the spectrum were discovered at different times. This is why electromagnetic radiation of different wavelengths is called by different names. In the table and in figure 2 some illustrative values are given for several kinds of EM waves.

TABLE

Some typical values of:  wavelength (λ), frequency (ν = c/λ), photon energy (hν), cycle time (T = 1/ν), and inverse wavelength [1/(100⋅λ)].
EM wave	λ  (m)	ν  (1/s)	hν  (J)	T  (s)	1/λ  (cm−1)
γ-rays	1.00⋅10−14	3.00⋅1022	1.98⋅10−11	3.33⋅10−23	1.00⋅1012
X-rays	5.00⋅10−10	6.00⋅1017	3.96⋅10−16	1.67⋅10−18	2.00⋅107
Ultraviolet	2.00⋅10−7	1.50⋅1015	9.90⋅10−19	6.67⋅10−16	5.00⋅104
Visible	6.00⋅10−7	5.00⋅1014	3.30⋅10−19	2.00⋅10−15	1.67⋅104
Infrared	5.00⋅10−6	6.00⋅1013	3.96⋅10−20	1.67⋅10−14	2.00⋅103
Microwave	1.00⋅10−2	3.00⋅1010	1.98⋅10−23	3.33⋅10−11	1.00
Radio	1.00⋅102	3.00⋅106	1.98⋅10−27	3.33⋅10−7	1.00⋅10−4

Monochromatic linearly polarized waves

It is known that EM waves can be linearly superimposed, which is due to the fact that they are solutions of a linear partial differential equation, the wave equation (see next section). A linear superposition of waves is a solution of the same wave equation as the waves themselves. Such a superposition is also an electromagnetic wave (a propagating periodic disturbance of the EM field). If waves of different wavelengths are superimposed, then a non-monochromatic wave is obtained (the term multi-chromatic wave would be apt, but is hardly ever used). By means of Fourier analysis a non-monochromatic wave can be decomposed into monochromatic components. The wave in figure 1 has one wavelength, it is a monochromatic wave.

The electric field vectors in figure 1 are all in one plane, this is the plane of polarization, and a wave with one fixed polarization plane, is called linearly polarized.

The radiation of many lasers is monochromatic and linearly polarized (at least to a very good approximation).

Relation to Maxwell's equations

In this section it will be shown that the electromagnetic wave depicted in figure 1 is a solution of the Maxwell equations in the vacuum.

We assume that at some distance away from the source of EM waves (a radio transmitter, a laser, gamma radiating nuclei, etc.), there is no charge density ρ and no current density J. For that region of space, the microscopic (vacuum) Maxwell equations become (in SI units):

${\boldsymbol {\nabla }}\cdot \mathbf {B} =0,\qquad {\boldsymbol {\nabla }}\cdot \mathbf {E} =0,$

and

${\boldsymbol {\nabla }}\times \mathbf {B} ={\frac {1}{c^{2}}}{\frac {\partial \mathbf {E} }{\partial t}},\qquad {\boldsymbol {\nabla }}\times \mathbf {E} =-{\frac {\partial \mathbf {B} }{\partial t}}.$

Apply to the last Maxwell equation the following relation, known from vector analysis and valid for any (differentiable) vector field,

${\boldsymbol {\nabla }}\times ({\boldsymbol {\nabla }}\times \mathbf {E} )={\boldsymbol {\nabla }}({\boldsymbol {\nabla }}\cdot \mathbf {E} )-{\boldsymbol {\nabla }}^{2}\mathbf {E}$

and use that ∇ · E = 0, then E satisfies the wave equation,

${\boldsymbol {\nabla }}^{2}\mathbf {E} ={\frac {\partial ({\boldsymbol {\nabla }}\times \mathbf {B} )}{\partial t}}={\frac {1}{c^{2}}}{\frac {\partial ^{2}\mathbf {E} }{\partial t^{2}}}.$

Note that the displacement current (time derivative of E) is essential in this equation, if it were absent (zero), the field E would be a static, time-independent, electric field, and there would be no waves.

In the very same way we derive a wave equation for B,

${\boldsymbol {\nabla }}^{2}\mathbf {B} ={\frac {1}{c^{2}}}{\frac {\partial ^{2}\mathbf {B} }{\partial t^{2}}}.$

Observe that E and B are related by the third and fourth Maxwell equation, which express the fact that a displacement current causes a magnetic field, and a changing magnetic field causes an electric field (Faraday's law of induction), respectively. So a time-dependent electric field that is not associated with a time-dependent magnetic field cannot exist, and conversely. Indeed, in special relativity E and c B can be transformed into one another by a Lorentz transformation of the electromagnetic field tensor, which shows their close relationship.

The wave equation is without doubt the most widely studied differential equation in mathematical physics. In figure 1 the electric field depicts a particular solution, with special initial and boundary conditions. The snapshot that is depicted has the analytic form

$\mathbf {E} (\mathbf {r} ,t)=\mathbf {e} _{z}E_{0}\sin {\big [}k(y-ct){\big ]}\quad {\hbox{with}}\quad k\equiv {\frac {2\pi }{\lambda }}.$

The snapshot is taken at $\scriptstyle t=2\pi n/(ck)$ for some arbitrary integer n. We assumed here that the direction of E defines the direction of the z-axis with unit vector e_z along this axis. The quantity E₀ is the amplitude of the wave. Insertion of this expression in in the left hand side of the wave equation for E gives

${\boldsymbol {\nabla }}^{2}\mathbf {E} =\mathbf {e} _{z}E_{0}{\frac {\partial ^{2}\sin {\big [}k(y-ct){\big ]}}{\partial y^{2}}}=-k^{2}\mathbf {e} _{z}E_{0}\sin {\big [}k(y-ct){\big ]}.$

Insertion of this expression in in the right hand side of the wave equation for E gives

${\frac {\mathbf {e} _{z}E_{0}}{c^{2}}}{\frac {\partial ^{2}\sin {\big [}k(y-ct){\big ]}}{\partial t^{2}}}=-{\frac {c^{2}\,k^{2}}{c^{2}}}\mathbf {e} _{z}E_{0}\sin {\big [}k(y-ct){\big ]}=-k^{2}\mathbf {e} _{z}E_{0}\sin {\big [}k(y-ct){\big ]},$

so that it follows that the special solution, depicted in figure 1, is indeed a solution of the wave equation for E.

We could now proceed in the very same way and solve the wave equation for B, but then we could easily overlook the relation between the two fields. So we rather substitute the solution for E into the fourth Maxwell equation and use the definition of curl as a determinant,

${\begin{vmatrix}\mathbf {e} _{x}&\quad \mathbf {e} _{y}&\mathbf {e} _{z}\\{\frac {\partial }{\partial x}}&\quad {\frac {\partial }{\partial y}}&{\frac {\partial }{\partial z}}\\0&\quad 0&E_{0}\sin {\big [}k(y-ct){\big ]}\\\end{vmatrix}}=k\mathbf {e} _{x}E_{0}\cos {\big [}k(y-ct){\big ]}=-{\frac {\partial \mathbf {B} }{\partial t}}.$

It is easy to see that

$\mathbf {B} (\mathbf {r} ,t)=\mathbf {e} _{x}B_{0}\sin {\big [}k(y-ct){\big ]}\quad {\hbox{with}}\quad B_{0}\equiv {\frac {E_{0}}{c}}$

is a solution of this equation. It follows that E and B are perpendicular (along the z-axis and x-axis, respectively) and are in phase. That is, E and B are simultaneously zero and attain simultaneously their maximum and minimum. The fact that (in vacuum) the amplitude of B is a factor c smaller than of E is due to the use of SI units, in which the amplitudes have different dimensions. In Gaussian units this is not the case and E₀ = B₀.

Energy

In this section the following balance of power (energy per unit time) densities will be derived:

${\boldsymbol {\nabla }}\cdot \mathbf {S} +{\frac {\partial {\mathcal {E}}_{\textrm {Field}}}{\partial t}}=-{\mathcal {E}}_{\textrm {Joule}}$

where

${\begin{aligned}\mathbf {S} &=\mathbf {E} \times \mathbf {H} \equiv \mathbf {E} \times {\frac {1}{\mu _{0}}}\mathbf {B} \\{\mathcal {E}}_{\textrm {Field}}&={\frac {1}{2}}(\mathbf {E} \cdot \mathbf {D} +\mathbf {B} \cdot \mathbf {H} )\equiv {\frac {1}{2}}(\epsilon _{0}\mathbf {E} \cdot \mathbf {E} +{\frac {1}{\mu _{0}}}\mathbf {B} \cdot \mathbf {B} )\\{\mathcal {E}}_{\textrm {Joule}}&=\mathbf {E} \cdot \mathbf {J} \\\end{aligned}}$

The terms in this equation have dimension W/m³ (power per volume). The quantity $\scriptstyle -{\mathcal {E}}_{\textrm {Joule}}>0$ represents the rate at which energy is produced per unit volume by ordinary Joulean (resistance) heating. The quantity $\scriptstyle {\mathcal {E}}_{\textrm {Field}}$ is the energy density of the EM field and the time derivative is the rate of increase (power density). The vector S, Poynting's vector, is the power flux, the amount of energy crossing unit area perpendicular to the vector, per unit time.

Multiplying the terms by a volume ΔV and a time span Δt, both small enough that the terms in the equation may assumed to be constant, the equation represents the conservation of energy: the energy generated in ΔVΔt (the right hand side) is equal to the increase in energy in ΔV plus the net flow of energy leaving ΔV. Hence, when this equation is multiplied by ΔVΔt it is an equation of continuity for energy.

Derivation

Recall from elementary electricity theory the laws of Joule and Ohm . They state that the amount of energy W per unit time, produced by a conduction current I, is equal to

$W=I^{2}\,R=I\,V,\quad {\hbox{with}}\quad R,\,W>0,$

where R is the resistance and V a voltage difference.

Assuming that the current flows along z, we introduce the current density J_z, and using

$V=-E_{z}\Delta z\quad {\hbox{and}}\quad I=J_{z}\Delta x\Delta y$

we obtain

$W=-E_{z}J_{z}\,\Delta x\Delta y\Delta z.$

We could continue discussing the system with the small volume $\Delta x\Delta y\Delta z$. However, because all terms in the equations would be multiplied by the same volume, it is more convenient to consider densities and to divide out the volume. Nevertheless, we still refer to the system. Thus, we define

${\mathcal {E}}_{\textrm {Joule}}\equiv -{\frac {W}{\Delta x\Delta y\Delta z}}=\mathbf {E} \cdot \mathbf {J} <0.$

The negative quantity $\scriptstyle {\mathcal {E}}_{\textrm {Joule}}$ is the loss of energy of the system per unit time and per unit volume (according to Joule's and Ohm's laws). One may look upon the quantity $\scriptstyle -{\mathcal {E}}_{\textrm {Joule}}$ as the work (per unit time and unit volume) done by the Lorentz force $\scriptstyle q(\mathbf {v} \times \mathbf {B} +\mathbf {E} )$ on the moving particles constituting the current density J. Since $\scriptstyle \mathbf {v} \cdot (\mathbf {v} \times \mathbf {B} )=0$, this work depends only on the electric field E.

Apply one of Maxwell's equations:

$\mathbf {E} \cdot \mathbf {J} =\mathbf {E} \cdot \left(-\epsilon _{0}{\frac {\partial \mathbf {E} }{\partial t}}+{\frac {1}{\mu _{0}}}{\boldsymbol {\nabla }}\times \mathbf {B} \right)$

Use a rule known from vector analysis and apply another one of Maxwell's equations,

${\begin{aligned}\mathbf {E} \cdot ({\boldsymbol {\nabla }}\times \mathbf {B} )=&\mathbf {B} \cdot ({\boldsymbol {\nabla }}\times \mathbf {E} )-{\boldsymbol {\nabla }}\cdot (\mathbf {E} \times \mathbf {B} )\\=&-\mathbf {B} \cdot \left({\frac {\partial \mathbf {B} }{\partial t}}\right)-{\boldsymbol {\nabla }}\cdot (\mathbf {E} \times \mathbf {B} )\end{aligned}}$

Define

${\mathcal {E}}_{\textrm {Field}}\equiv {\frac {1}{2}}\left(\epsilon _{0}E^{2}+{\frac {1}{\mu _{0}}}B^{2}\right)={\frac {1}{2}}\left(\mathbf {E} \cdot \mathbf {D} +\mathbf {B} \cdot \mathbf {H} \right)$

with

$\mathbf {D} \equiv \epsilon _{0}\mathbf {E} \quad {\hbox{and}}\quad \mathbf {B} \equiv \mu _{0}\mathbf {H} ,$

where ε₀ is the electric constant and μ₀ the magnetic constant of the vacuum. Define also

$\mathbf {S} \equiv {\frac {1}{\mu _{0}}}\mathbf {E} \times \mathbf {B} =\mathbf {E} \times \mathbf {H}$

where S is the Poynting vector called after John Henry Poynting. This vector is perpendicular to the plane of E and B and by the right-hand rule, it points in the direction of propagation of the EM wave. The divergence of the Poynting vector is the energy flow associated with the electromagnetic wave, i.e., with the pair E(r,t) and B(r,t). By definition ∇·S gives the flow leaving the system and − ∇·S gives the flow entering the system. The total energy balance becomes

$-{\mathcal {E}}_{\textrm {Joule}}={\frac {\partial {\mathcal {E}}_{\textrm {Field}}}{\partial t}}+{\boldsymbol {\nabla }}\cdot \mathbf {S} .$

Here we have found an example of the conservation of energy, known as Poynting's theorem: The energy produced per unit time according to Joule's law $\scriptstyle -{\mathcal {E}}_{\textrm {Joule}}$ is equal to the rate in increase of the electromagnetic energy of the system $\scriptstyle {\mathcal {E}}_{\textrm {Field}}$, plus the flow of EM radiation ∇·S leaving the system.

If there is no current, J = 0, then

${\frac {\partial {\mathcal {E}}_{\textrm {Field}}}{\partial t}}=-{\boldsymbol {\nabla }}\cdot \mathbf {S} ,$

which is the continuity equation. The increase of field energy per unit time is the flow of radiation energy into the system.

Example

Consider a radio station with a signal of strength P kW. We wonder what the energy density is at a distance R m from the station. To that end we must assume what shape of source the antenna has, is it a point on the 2D surface of the earth, a point in 3D space, or is it cylindrically shaped? We choose the latter and assume a cylinder height z m. Further it is assumed that power density is homogeneous and that all power crosses the cylindrical walls, that is, power crossing the top and bottom of the cylinder is neglected. Also no absorption by the atmosphere will occur. When a steady state is reached (some time after the beginning of the transmission), the two terms on the left hand side vanish. The energy density at a distance R becomes stationary,

${\mathcal {E}}_{\mathrm {Field} }={\frac {P}{2\pi Rzc}}\quad \mathrm {J/m^{3}} ,$

where c is the speed of propagation of the radio signal (is speed of ligth ≈ 3·10⁸  m/s). To give a numerical example: P = 100 kW, R = 5000 m, z = 50 m, then $\scriptstyle {\mathcal {E}}_{\mathrm {Field} }$ = 2.1·10⁻¹⁰ J/m³.

(To be continued)

External link

ISO 21348 Definitions of Solar Irradiance Spectral Categories