  The Auger Engineering Radio Array (AERA) aims to detect extensive air showers
caused by the interactions of ultra-high energy cosmic rays with the Earth's
atmosphere, providing complementary information to the Auger surface,
fluorescence and muon detectors. AERA, currently consisting of 124 radio
stations, comprises an area of about 6 km$^{2}$. The main objective for
exploiting a radio detector is to measure the fundamental air-shower
parameters, such as the direction, energy and composition. We have developed
reconstruction strategies and algorithms to precisely measure the air-shower
parameters with high efficiency. In addition, we will present the results
obtained by applying the reconstruction strategies on the experimental data
taken by AERA.
