The SuperDARN radars are now able to measure the angles of arrival of
the backscattered radiation. We describe the analysis procedure and pr
esent results for meteor scatter from slant ranges below 500 km and gr
ound scatter from either the E region or the F region at greater slant
ranges which can be used to determine peak electron densities and the
ir heights. The angle of arrival measurements can also be used to iden
tify ''unwanted'' backscatter from the backward lobes of the antenna r
adiation pattern. Electron densities can also be measured in the back
lobes.