  We present far ultraviolet (FUV: 912 - 1750AA) spectral imaging observations
recorded with the SPEAR satellite of the interstellar OVI (1032AA), CIV
(1550AA), SiIV (1394AA), SiII* (1533AA) and AlII (1671AA) emission lines
originating in a 60 x 30 degree rectangular region lying close to the North
Galactic Pole. These data represent the first large area, moderate spatial
resolution maps of the distribution of UV spectral-line emission originating
the both the highly ionized medium (HIM) and the warm ionized medium (WIM)
recorded at high galactic latitudes.
