spherical coordinates

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spherical coordinates

pl n
(Mathematics) three coordinates that define the location of a point in three-dimensional space in terms of the length r of its radius vector, the angle, θ, which this vector makes with one axis, and the angle, φ, made by a second axis, perpendicular to the first, with the plane containing the first axis and the point. Usually written (r, θ, φ)
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The components of the general solutions are particular solutions of the Helmholtz equation in Cartesian, cylindrical, and spherical coordinates. (Ringgold, Inc., Portland, OR)
For the dyadic representation of integral equations in spherical coordinates, when all incoming waves are collected in a certain finest box, due to the discontinuities in the spherical vector components, the Gibbs phenomenon will arise if the integral operation of the spherical harmonics representation is also evaluated in spherical coordinates [6].
Attempts to solve similar equations in spherical coordinates in the presence of an electric dipole have been made.
Gouesbet, "T-matrix formulation and generalized Lorenz-Mie theories in spherical coordinates," Optics Communications, vol.
where u = sin [theta] cos [phi] and v = sin [theta] sin [phi] are the usual spherical coordinates. Eq.
The last integral using spherical coordinates gives the estimate [N.sup.m+2([alpha]-[beta]) which tends to 0 under n [right arrow] [delta] if [beta] > [alpha] + m/2.
It is well known that the associated Legendre polynomials play an important role in the central fields when one solves the physical problems in the spherical coordinates. However, in the case of the noncentral fields we have to introduce the universal associated Legendre polynomials [P.sup.m'.sub.l'] (x) when one studies the modified Poschl-Teller [1], the single and double ring-shaped potentials, and time-dependent potential [2-4].
Therefore, the point on the unit sphere that corresponds to our texture point (x, y) is given in spherical coordinates as:
Spherical harmonics (SH) represent a complete set of angular functions in spherical coordinates, where the position of a point is defined by the polar radius r and two polar and azimuthal spherical angles, [theta] and [phi], respectively.
We consider an infinitesimal mass dM of the sphere represented by its spherical coordinates (r, [theta], [phi]), where r is the radial distance, [theta] the polar angle, and [phi] the azimuthal angle (see Figure 4).
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