  This is a direct computation of the spectral representation of homogeneous
spin-weighted spherical random fields with arbitrary integer spin. It
generalises known results from Cosmology for the spin-2 Cosmic Microwave
Background polarisation and Cosmic Shear fields, without decomposition into
$E$- and $B$-modes. The derivation uses an instructive representation of
spin-weighted spherical functions over the Spin(3) group, where the
transformation behaviour of spin-weighted fields can be treated more naturally
than over the sphere, and where the group nature of Spin(3) greatly simplifies
calculations for homogeneous spherical fields. It is shown that i) different
modes of spin-weighted spherical random fields are generally uncorrelated, ii)
the usual definition of the power spectrum generalises, iii) there is a simple
relation to recover the correlation function from the power spectrum, and iv)
the spectral representation is a sufficient condition for homogeneity of the
fields.
