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Animations |
The solution of
the wave equation, written in spherical coordinates (r,,)
,
can be written,
for the solutions with separated variables of the form ,
with
where the
functions jn and nn
are respectively the spherical Bessel functions of the 1st kind and the
spherical Neumann functions, nth-order, and where the functions Pnm(cos) are the
associated Legendre functions, which can be expressed as a
function of Legendre
polynomials of degree n, denoted Pn,
as following (do not confuse functions Pnm and
polynomials Pn):
The functions and are called "spherical harmonics".
Hence, for any given n and m, any given solution coming from the separation of variable methods has a structure which is well determined on the unit sphere (parameters and ). This structure is given by the spherical harmonics, which are orthonormal functions and which form a basis of the considered space (,). These solutions express a complex directivity of the fields which are emitted in an infinite space, by a set of "localised" sources with complex properties. |
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The
animations below present the variations as a fucntion of time, of the
first spherical harmonics
multiplied by the function cos( t),
and visualized on the unit sphere, with
color levels (red = maximum, blue = minimum). |
"Zonal"
harmonics: m=0 "Sectoral" harmonics: n=m |
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"Tesseral"
harmonics: 0<m<n |