High power, pulsed microwaves are beamed forward of a model in a Mach 6 flo
w using an on-board, Ku-band horn. A thin "precursor" plasma is generated j
ust ahead of the bow shock in the low density free stream. Temporal and spa
tial analysis of the microwave E-field and plasma conductivity in the super
sonic flow field indicate that the plasma reflects a large proportion of th
e microwave power in an individual pulse as soon as the plasma frequency ex
ceeds the wave frequency. Possible methods for more efficient deposition of
power in the free stream are discussed which could lead to increased inter
action with the shock. (C) 2001 American Institute of Physics.