This paper describes a comparison of winds measured by the meteor echo
detection and collection (MEDAC) system and a collocated spaced anten
na MF radar at the Buckland Park field station near Adelaide, Australi
a (35 degrees S, 138 degrees E). A previous paper has described a deta
iled comparison between the MEDAC and Adelaide meteor radar system whi
ch was also operated during the campaign. In this paper, which uses on
ly hand-classified underdense meteor echoes, the meteor horizontal zon
al wind velocities were compared to the those produced by the MF space
d antenna system. Care was taken when interpreting the comparison resu
lts in light of the varying meteor data rates. A point-to-point compar
ison showed that the excursions seen in the meteor data tended to be l
arger than those in the MF data. Excellent agreement was found between
the two systems and relevant model results across the observed height
s for both the mean winds and tides.