We have built and operated a large-scale axion detector, based on a method
originally proposed by Sikivie, to search for halo axions. The apparatus co
nsists of a cylindrical tunable high-Q microwave cavity threaded axially by
a static high magnetic field. This field stimulates axions that enter the
cavity to convert into single microwave photons. The conversion is resonant
ly enhanced when the cavity resonant frequency is near the axion rest mass
energy. The experiment is cooled to 1.5 K and the electromagnetic power spe
ctrum emitted by the cavity is measured by an ultra-low-noise microwave rec
eiver. The axion would be detected as excess power in a narrow line within
the cavity resonance. The apparatus has achieved a power sensitivity better
than 10(-23) W in the mass range 2.9-3.3 mu eV. For the first time the rf
cavity technique has explored plausible axion models, assuming axions make
up a significant fraction of the local halo density. The experiment continu
es to operate and will explore a large part of the mass in the range of 1-1
0 mu eV in the near future. An upgrade of the experiment is planned with dc
superconducting quantum interference device microwave amplifiers operating
at a lower physical temperature. This next generation detector would be se
nsitive to even more weakly coupled axions contributing only fractionally t
o the local halo density.