Key points are not available for this paper at this time.
A number of unusual electromagnetic scattering effects for magnetic spheres are described. When ∊ = μ, the backscatter gain is zero; the scattered radiation is polarized in the same sense as the incident radiation. In the small-particle (or long-wavelength) limit, conditions are described for zero forward scatter, for complete polarization of scattered radiation in other directions, and for asymmetry of forward scatter to backscatter. The special case in the small-particle limit of m = 1, i.e., μ = 1/∊, provides interesting special instances of complete polarization and forward-scatter-to-backscatter asymmetry.
Building similarity graph...
Analyzing shared references across papers
Loading...
Milton Kerker
RWTH Aachen University
D.-S. Wang
Clarkson College
C. Lee Giles
Texas Tech University
Journal of the Optical Society of America
Clarkson College
Building similarity graph...
Analyzing shared references across papers
Loading...
Kerker et al. (Wed,) studied this question.
synapsesocial.com/papers/69f48be370d05fdca4d40103 — DOI: https://doi.org/10.1364/josa.73.000765