A. Swindlehurst, M. Viberg
tlooto Summary
It is shown how to decouple the NSF search into a two-step procedure, where the DOAs are estimated separately, and the polarization parameters are obtained by solving a linear system of equations.
Abstract
Diversely polarized antenna arrays are widely used in RF applications. The diversity of response provided by diversely polarized antenna arrays can greatly improve direction-finding performance over arrays sensitive to only one polarization component. For d emitters, directly implementing a multidimensional estimation algorithm would require a search for 3d parameters: d directions of arrival (DOAs), and 2d polarization parameters. A more efficient solution is presented based on the noise subspace fitting (NSF) algorithm. It is shown how to decouple the NSF search into a two-step procedure, where the DOAs are estimated separately. The polarization parameters are then obtained by solving a linear system of equations. The advantage of this approach is that the search dimension is reduced by a factor of three, and no initial polarization estimate is required. The algorithm can be shown to yield asymptotically minimum variance estimates: provided no perfectly coherent signals are present. Simulation examples are included. >
Citation format
SWINDLEHURST, A.; VIBERG, M. Subspace fitting with diversely polarized antenna arrays. ACM Transactions on Applied Perception, 1993.