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Cylindrical multipole moments : ウィキペディア英語版
Cylindrical multipole moments

Cylindrical multipole moments are the coefficients in a series expansion of a potential that varies logarithmically with the distance to a source, i.e., as \ln \ R. Such potentials arise in the electric potential of long line charges, and the analogous sources for the magnetic potential and gravitational potential.
For clarity, we illustrate the expansion for a single line charge, then generalize to an arbitrary distribution of line charges. Through this article, the primed coordinates such
as (\rho^, \theta^) refer to the position of the line charge(s), whereas the unprimed coordinates such as (\rho, \theta) refer to the point at which the potential is being observed. We use cylindrical coordinates throughout, e.g., an arbitrary vector \mathbf has coordinates ( \rho, \theta, z)
where \rho is the radius from the z axis, \theta is the azimuthal angle and z is the normal Cartesian coordinate. By assumption, the line charges are infinitely long and aligned with the z axis.
==Cylindrical multipole moments of a line charge==

The electric potential of a line charge \lambda located at (\rho^, \theta^) is given by
:
\Phi(\rho, \theta) = \frac \ln R
= \frac \ln \left| \rho^ +
\left( \rho^ \right)^ - 2\rho\rho^\cos (\theta-\theta^ ) \right|

where R is the shortest distance between the line charge and the observation point.
By symmetry, the electric potential of an infinite linecharge has no z-dependence. The line charge \lambda is the charge per unit length in the
z-direction, and has units of (charge/length). If the radius \rho of the observation point is greater than the radius \rho^ of the line charge, we may factor out \rho^
:
\Phi(\rho, \theta) =
\frac \left\ e^ \right) \left( 1 - \frac e^ \right) \right\}

and expand the logarithms in powers of (\rho^/\rho)<1
:
\Phi(\rho, \theta) =
\frac \left\ \left( \frac \right) \left( \frac \right)^
\left(\cos k\theta \cos k\theta^ + \sin k\theta \sin k\theta^ \right ) \right\}

which may be written as
:
\Phi(\rho, \theta) =
\frac \ln \rho +
\left( \frac \right) \sum_^
\frac \sin k\theta} = \frac \left( \rho^ \right)^ \cos k\theta^ ,
and
S_ = \frac \left( \rho^ \right)^ \sin k\theta^ .
Conversely, if the radius \rho of the observation point is less than the radius \rho^ of the line charge, we may factor out \left( \rho^ \right)^ and expand the logarithms in powers of (\rho/\rho^)<1
:
\Phi(\rho, \theta) =
\frac \left\^ \left( \frac \right) \left( \frac
\left(\cos k\theta \cos k\theta^ + \sin k\theta \sin k\theta^ \right ) \right\}

which may be written as
:
\Phi(\rho, \theta) =
\frac \ln \rho^ +
\left( \frac \right) \sum_^
\rho^ \left(I_ \cos k\theta + J_ \sin k\theta \right )

where the interior multipole moments are defined as
Q = \lambda ,
I_ = \frac
\frac \right)^},
and
J_ = \frac \frac \right)^}.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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