  We present maps of the 22MHz radio emission between declinations -28d and
+80d, covering ~73% of the sky, derived from observations with the 22MHz
radiotelescope at the Dominion Radio Astrophysical Observatory (DRAO). The
resolution of the telescopt (EWxNS) is 1.1d x 1.7d secant(zenith angle). The
maps show the large scale features of the emission from the Galaxy including
the thick non-thermal disk, the North Polar Spur (NPS) and absorption due to
discrete HII regions and to an extended band of thermal electrons within 40d of
the Galactic centre. We give the flux densities of nine extended supernova
remnants shown on the maps.
