  SECIS observations of the June 2001 total solar eclipse were taken using an
Fe {\sc xiv} 5303 {\AA} filter. Automated tools based on wavelet analysis was
used to detect intensity oscillations on various areas of the images.
Statistical analysis of the detections found in the areas covered by the moon
and the upper corona allowed us to estimate the atmospheric and instrumental
effects on the detection of intensity oscillations. An area of the lower
corona, close to Active Region 9513, was found with a statistically significant
amount of intensity oscillations with periodicity of $\sim7.5s$. The shape of
the wavelet transformation of those detections matches theoretical predictions
of sausage-mode perturbations and for the first time in the SECIS project,
second order oscillations were also detected.
