  We present an extended analysis of the high dispersion IUE spectra of SN
1993J in M81, based on the improved data in the IUE final archive. Eight
interstellar absorption components can be identified in the velocity range from
-200 km/s to +200 km/s. Column densities are determined for Fe II, Mg I, Mg II,
O I, S II, Si II, and Zn II. From the ion ratios, we estimate electron
densities and temperatures of the gas in these components. In addition, we
rederive column density profiles for the higher ionisation stages Al III, Si
IV, and C IV for the entire line of sight.
  Of special interest are the absorption components at positive velocities,
which are associated with the intergalactic medium (IGM) in the foreground of
M81. The medium has many gas components, as known from radio measurements,
probably released in dynamical interactions by galaxies in the M81 group. The
IUE spectra contain the only UV absorption information on such gas. We find
neutral and ionised gas absorption at the same velocity, having a metal content
similar to a galactic disk.
  We combine the spectra towards SN 1993J in M81 with those towards SN 1987A in
the LMC, the directions being essentially antipodes on the celestical sphere.
Comparing the total profile with QSO spectra, we conclude that most absorption
in QSO spectra occurs in diffuse clouds on those sight lines and is not similar
to absorption by galactic disk gas. However, one absorption component towards
SN 1993J is clearly very similar to some of the absorption components in QSO
spectra.
