  We present FUV and UV spectroscopic observations of AD Leonis, with the aim
of investigating opacity effects in the transition regions of late-type stars.
The C III lines in FUSE spectra show significant opacity during both the
quiescent and flaring states of AD Leonis, with up to 30% of the expected flux
being lost during the latter. Other FUSE emission lines tested for opacity
include those of O VI, while C IV, Si IV and N V transitions observed with STIS
are also investigated. These lines only reveal modest amounts of opacity with
losses during flaring of up to 20%. Optical depths have been calculated for
homogeneous and inhomogeneous geometries, giving path lengths of ~20-60 km and
\~10-30 km, respectively, under quiescent conditions. However path lengths
derived during flaring are ~2-3 times larger. These values are in excellent
agreement with both estimates of the small-scale structure observed in the
solar transition region, and path lengths derived previously for several other
active late-type stars.
