  SECIS observations of the June 2001 total solar eclipse were taken using an
Fe xiv 5303 A filter. Existing software was modified and new code was developed
for the reduction and analysis of these data. The observations, data reduction,
study of the atmospheric and instrumental effects, together with some
preliminary results are discussed. Emphasis is given to the techniques used for
the automated alignment of the 8000 images, the application of the a Trous
algorithm for noise filtering and the software developed for the automated
detection of intensity oscillations using wavelet analysis. In line with
findings from the 1999 SECIS total eclipse observations, intensity oscillations
with periods in the range of 20-30 s, both inside and just outside coronal
loops are also presented.
