W.J. Baggaley*, R.G.T. Bennetta, S.H. Marsha, G.E. Planka and D.P. Galligana aDepartment of Physics and Astronomy, University of Canterbury, Private Bag 4800, New Zealand.
AMOR is a continuously operating radar facility for measuring the heliocentric orbits of Earth-impacting grains down to sizes of about 40 /im. Recent developments including additional extensive antenna arrays and multi-antenna independent phase measurements are providing an expanded sky coverage and increased meteoroid velocity resolution yielding an enhanced system capability.
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