The formation and migration of the extrema in the angular distribution of t
he scattered light intensity with varying size, ellipticity, and refractive
index of a homogeneous spheroid oriented with the axis of revolution along
the incident light direction are studied analytically and numerically. The
Wentzel-Kramers-Brillouin (WKB), Rayleigh-Gans-Debye, Fraunhofer diffracti
on, and anomalous diffraction approximations are used for relative refracti
ve indices ranging from 1.025 to 1.200. Equations relating the locations of
the extrema to the particle parameters are derived. The analysis of the ex
trema predicted by the WKB approximation shows that the locations of differ
ent minima migrate monotonously when the size of the spheroid is varied. We
also discuss the disappearance of the extrema with increasing relative ref
ractive index and particle size. (C) 1999 Elsevier Science Ltd. All rights
reserved.