Magnetic current

Flow of magnetic monopole charge
Magnetic current (flowing magnetic monopoles), M, creates an electric field, E, in accordance with the left-hand rule.
Articles about
Electromagnetism
Solenoid
Electrostatics
  • v
  • t
  • e

Magnetic current is, nominally, a current composed of moving magnetic monopoles. It has the unit volt. The usual symbol for magnetic current is k {\displaystyle k} , which is analogous to i {\displaystyle i} for electric current. Magnetic currents produce an electric field analogously to the production of a magnetic field by electric currents. Magnetic current density, which has the unit V/m2 (volt per square meter), is usually represented by the symbols M t {\displaystyle {\mathfrak {M}}^{\text{t}}} and M i {\displaystyle {\mathfrak {M}}^{\text{i}}} .[a] The superscripts indicate total and impressed magnetic current density.[1] The impressed currents are the energy sources. In many useful cases, a distribution of electric charge can be mathematically replaced by an equivalent distribution of magnetic current. This artifice can be used to simplify some electromagnetic field problems.[b][c] It is possible to use both electric current densities and magnetic current densities in the same analysis.[4]: 138 

The direction of the electric field produced by magnetic currents is determined by the left-hand rule (opposite direction as determined by the right-hand rule) as evidenced by the negative sign in the equation[1] × E = M t . {\displaystyle \nabla \times {\mathcal {E}}=-{\mathfrak {M}}^{\text{t}}.}

Magnetic displacement current

Magnetic displacement current or more properly the magnetic displacement current density is the familiar term B/∂t[d][e][f] It is one component of M t {\displaystyle {\mathfrak {M}}^{\text{t}}} .[1][2] M t = B t + M i . {\displaystyle {\mathfrak {M}}^{\text{t}}={\frac {\partial B}{\partial t}}+{\mathfrak {M}}^{\text{i}}.} where

  • M t {\displaystyle {\mathfrak {M}}^{\text{t}}} is the total magnetic current.
  • M i {\displaystyle {\mathfrak {M}}^{\text{i}}} is the impressed magnetic current (energy source).

Electric vector potential

The electric vector potential, F, is computed from the magnetic current density, M i {\displaystyle {\mathfrak {M}}^{\text{i}}} , in the same way that the magnetic vector potential, A, is computed from the electric current density.[1]: 100  [4]: 138  [3]: 468  Examples of use include finite diameter wire antennas and transformers.[5]

magnetic vector potential: A ( r , t ) = μ 0 4 π Ω J ( r , t ) | r r | d 3 r . {\displaystyle \mathbf {A} (\mathbf {r} ,t)={\frac {\mu _{0}}{4\pi }}\int _{\Omega }{\frac {\mathbf {J} (\mathbf {r} ',t')}{|\mathbf {r} -\mathbf {r} '|}}\,\mathrm {d} ^{3}\mathbf {r} '\,.}

electric vector potential: F ( r , t ) = ε 0 4 π Ω M i ( r , t ) | r r | d 3 r , {\displaystyle \mathbf {F} (\mathbf {r} ,t)={\frac {\varepsilon _{0}}{4\pi }}\int _{\Omega }{\frac {{\mathfrak {M}}^{\text{i}}(\mathbf {r} ',t')}{|\mathbf {r} -\mathbf {r} '|}}\,\mathrm {d} ^{3}\mathbf {r} '\,,} where F at point r {\displaystyle \mathbf {r} } and time t {\displaystyle t} is calculated from magnetic currents at distant position r {\displaystyle \mathbf {r} '} at an earlier time t {\displaystyle t'} . The location r {\displaystyle \mathbf {r} '} is a source point within volume Ω that contains the magnetic current distribution. The integration variable, d 3 r {\displaystyle \mathrm {d} ^{3}\mathbf {r} '} , is a volume element around position r {\displaystyle \mathbf {r} '} . The earlier time t {\displaystyle t'} is called the retarded time, and calculated as t = t | r r | c . {\displaystyle t'=t-{\frac {|\mathbf {r} -\mathbf {r} '|}{c}}.}

Retarded time accounts for the accounts for the time required for electromagnetic effects to propagate from point r {\displaystyle \mathbf {r} '} to point r {\displaystyle \mathbf {r} } .

Phasor form

When all the functions of time are sinusoids of the same frequency, the time domain equation can be replaced with a frequency domain equation. Retarded time is replaced with a phase term. F ( r ) = ε 0 4 π Ω M i ( r ) e j k | r r | | r r | d 3 r , {\displaystyle \mathbf {F} (\mathbf {r} )={\frac {\varepsilon _{0}}{4\pi }}\int _{\Omega }{\frac {{\mathfrak {M}}^{\text{i}}(\mathbf {r} )e^{-jk|\mathbf {r} -\mathbf {r} '|}}{|\mathbf {r} -\mathbf {r} '|}}\,\mathrm {d} ^{3}\mathbf {r} '\,,} where F {\displaystyle \mathbf {F} } and M i {\displaystyle {\mathfrak {M}}^{\text{i}}} are phasor quantities and k {\displaystyle k} is the wave number.

Magnetic frill generator

A dipole antenna driven by a hypothetical annular ring of magnetic current. b is chosen so that 377 Ω × ln(b/a) is equal to the impedance of the driving transmission line (not shown).

A distribution of magnetic current, commonly called a magnetic frill generator, may be used to replace the driving source and feed line in the analysis of a finite diameter dipole antenna.[4]: 447–450  The voltage source and feed line impedance are subsumed into the magnetic current density. In this case, the magnetic current density is concentrated in a two dimensional surface so the units of M i {\displaystyle {\mathfrak {M}}^{\text{i}}} are volts per meter.

The inner radius of the frill is the same as the radius of the dipole. The outer radius is chosen so that Z L = Z 0 ln ( b a ) , {\displaystyle Z_{\text{L}}=Z_{0}\ln \left({\frac {b}{a}}\right),} where

  • Z L {\displaystyle Z_{\text{L}}} = impedance of the feed transmission line (not shown).
  • Z 0 {\displaystyle Z_{0}} = impedance of free space.

The equation is the same as the equation for the impedance of a coaxial cable. However, a coaxial cable feed line is not assumed and not required.

The amplitude of the magnetic current density phasor is given by: M i = k ρ {\displaystyle {\mathfrak {M}}^{\text{i}}={\frac {k}{\rho }}} with a ρ b . {\displaystyle a\leq \rho \leq b.} where

  • ρ {\displaystyle \rho } = radial distance from the axis.
  • k = V s ln ( b a ) {\displaystyle k={\frac {V_{\text{s}}}{\ln \left({\frac {b}{a}}\right)}}} .
  • V s {\displaystyle V_{\text{s}}} = magnitude of the source voltage phasor driving the feed line.

See also

Surface equivalence principle

Notes

  1. ^ Not to be confused with magnetization M
  2. ^ "For some electromagnetic problems, their solution can often be aided by the introduction of equivalent impressed electric and magnetic current densities."[2]
  3. ^ "there are many other problems where the use of fictitious magnetic currents and charges is very helpful."[3]
  4. ^ "Because of the symmetry of Maxwell's equations, the ∂B/∂t term ... has been designated as a magnetic displacement current density."[2]
  5. ^ "interpreted as ... magnetic displacement current ..."[3]
  6. ^ "it also is convenient to consider the term ∂B/∂t as a magnetic displacement current density."[1]

References

  1. ^ a b c d e Harrington, Roger F. (1961), Time-Harmonic Electromagnetic Fields, McGraw-Hill, pp. 7–8, hdl:2027/mdp.39015002091489, ISBN 0-07-026745-6
  2. ^ a b c Balanis, Constantine A. (2012), Advanced Engineering Electromagnetics, John Wiley, pp. 2–3, ISBN 978-0-470-58948-9
  3. ^ a b c Jordan, Edward; Balmain, Keith G. (1968), Electromagnetic Waves and Radiating Systems (2nd ed.), Prentice-Hall, p. 466, LCCN 68-16319
  4. ^ a b c Balanis, Constantine A. (2005), Antenna Theory (third ed.), John Wiley, ISBN 047166782X
  5. ^ Kulkarni, S. V.; Khaparde, S. A. (2004), Transformer Engineering: Design and Practice (third ed.), CRC Press, pp. 179–180, ISBN 0824756533