  The Astrophysics Directorate of CONIDA has installed two radio spectrometer
stations belonging to the e-CALLISTO network in Lima, Peru. Given their
strategic location near the Equator, it is possible to observe the Sun evenly
throughout the whole year. The receiver located at Pucusana, nearby the capital
city of Lima, took data from October 2014 until August 2016 in the metric and
decimetric bands looking for radio bursts. During this period, this e-CALLISTO
detector was unique in its time-zone coverage. To assess the suitability of the
sites and the performance of the antennas we analyzed the radio ambient
background and measured their radiation pattern and beam-width. To show the
capabilities of the facilities to study solar dynamics in these radio
frequencies we have selected and analyzed type III Solar Radio Bursts. The
study of this kind of bursts helps to understand the electron beams traversing
the solar corona and the solar atmospheric density. We have characterized the
most common radio bursts with the following mean values: a negative drift rate
of -25.8 $\pm$ 3.7 MHz/s, a duration of 2.6 $\pm$ 0.3 s and 35 MHz bandwidth in
the frequency range of 114 to 174 MHz. In addition, for some events, it was
possible to calculate a global frequency drift which on average was 0.4 $\pm$
0.1 MHz/s.
